View source for Orders of magnitude (energy)

{{Short description|Comparison of energies in joules}}
{{Use dmy dates|date=October 2019}}
This list compares various [[energy|energies]] in [[joule]]s (J), organized by '''order of magnitude'''.
{{clear}}

==Below 1 J==
{| class="wikitable"
|+ List of orders of magnitude for [[energy]]
! Factor (joules)
! [[International System of Units|SI]] [[SI prefix|prefix]]
! Value
! Item
|-
|10<sup>−34</sup>||&nbsp;||6.626×10<sup>−34</sup>{{nbsp}}J || [[Photon energy]] of a [[photon]] with a [[frequency]] of 1 [[hertz]].<ref name="britannica">{{cite web|url=http://www.britannica.com/EBchecked/topic/462917/Plancks-constant|publisher=britannica.com|title=Planck's constant {{pipe}} physics {{pipe}} Britannica.com|access-date=26 December 2016}}</ref>
|-
|10<sup>−33</sup>||&nbsp;||2×10<sup>−33</sup>{{nbsp}}J || [[Thermodynamic temperature#The relationship of temperature, motions, Heat, and thermal energy|Average kinetic energy of translational motion]] of a [[molecule]] at the lowest temperature reached, [[Absolute zero#Very low temperatures|100 picokelvins]] {{As of|1999|lc=on}}<ref>Calculated:  KE{{sub|avg}} ≈ (3/2) × T × 1.38{{e|-23}} = (3/2) × 1{{e|-10}} × 1.38{{e|-23}} ≈ 2.07{{e|-33}}{{nbsp}}J</ref>
|-
|10<sup>−30</sup>{{Anchor|10-30}}|| [[quecto-]] (qJ) ||
|-
|10<sup>−28</sup>
| &nbsp;
| 6.6×10<sup>−28</sup>{{nbsp}}J
| Energy of a typical [[AM radio]] photon (1&nbsp;MHz) (4×10<sup>−9</sup> [[electronvolt|eV]])<ref>Calculated:  E{{sub|photon}} = hν = 6.626{{e|-34}}{{nbsp}}J-s × 1{{e|6}} Hz = 6.6{{e|-28}}{{nbsp}}J.  In eV:  6.6{{e|-28}}{{nbsp}}J / 1.6{{e|-19}}{{nbsp}}J/eV = 4.1{{e|-9}} eV.</ref>
|-
|10<sup>−27</sup>{{Anchor|10-27}}|| [[ronto-]] (rJ) ||
|-
|10<sup>−24</sup>{{Anchor|10-24}}|| [[yocto-]] (yJ)
| 1.6×10<sup>−24</sup>{{nbsp}}J
| Energy of a typical [[microwave oven]] photon (2.45&nbsp;GHz) (1×10<sup>−5</sup> [[electronvolt|eV]])<ref>{{cite web
| url=https://hypertextbook.com/facts/1998/HowardCheung.shtml
| title=Frequency of a microwave oven
| first=Howard
| last=Cheung
| year=1998
| website=The Physics Factbook
| editor-last=Elert
| editor-first=Glenn
| accessdate=2022-01-25
}}</ref><ref>Calculated:  E{{sub|photon}} = hν = 6.626{{e|-34}}{{nbsp}}J-s × 2.45{{e|8}} Hz = 1.62{{e|-24}}{{nbsp}}J.  In eV:  1.62{{e|-24}}{{nbsp}}J / 1.6{{e|-19}}{{nbsp}}J/eV = 1.0{{e|-5}} eV.</ref>
|-
|10<sup>−23</sup>||&nbsp;||2×10<sup>−23</sup>{{nbsp}}J || [[Thermodynamic temperature#The relationship of temperature, motions, Heat, and thermal energy|Average kinetic energy of translational motion]] of a molecule in the [[Boomerang Nebula]], the coldest place known outside of a laboratory, at a temperature of 1 [[kelvin]]<ref>{{cite web|title=Boomerang Nebula boasts the coolest spot in the Universe|url=http://www.jpl.nasa.gov/news/releases/97/coldspot.html|publisher=JPL|access-date=13 November 2011|archive-date=27 August 2009|archive-url=https://web.archive.org/web/20090827115717/http://jpl.nasa.gov/news/releases/97/coldspot.html|url-status=dead}}</ref><ref>Calculated:  KE{{sub|avg}} ≈ (3/2) × T × 1.38{{e|-23}} = (3/2) × 1 × 1.38{{e|-23}} ≈ 2.07{{e|-23}}{{nbsp}}J</ref>
|-
| 10<sup>−22</sup>
| &nbsp;
| 2–3000×10<sup>−22</sup>{{nbsp}}J
| Energy of [[infrared]] light photons<ref name="NASA_spectrum"/>
|-
|rowspan=6|10<sup>−21</sup>{{Anchor|10-21}}
|rowspan=6| [[zepto-]] (zJ)
|1.7×10<sup>−21</sup>{{nbsp}}J
| 1{{nbsp}}kJ/mol, converted to energy per molecule<ref>Calculated:  1{{e|3}}{{nbsp}}J / 6.022{{e|23}} entities per mole = 1.7{{e|-21}}{{nbsp}}J per entity</ref>
|-
|2.1×10<sup>−21</sup>{{nbsp}}J
| [[Thermal energy]] in each [[Degrees of freedom (physics and chemistry)|degree of freedom]] of a molecule at 25&nbsp;°C ([[Boltzmann constant|k]]T/2) (0.01 [[electronvolt|eV]])<ref>Calculated:  1.381{{e|-23}}{{nbsp}}J/K × 298.15 K / 2 = 2.1{{e|-21}}{{nbsp}}J</ref>
|-
|2.856×10<sup>−21</sup>{{nbsp}}J
| By [[Landauer's principle]], the minimum amount of energy required at 25&nbsp;°C to change one bit of information
|-
|3–7×10<sup>−21</sup>{{nbsp}}J
| Energy of a [[van der Waals force|van der Waals interaction]] between atoms (0.02–0.04 eV)<ref name=ucla_chem125>{{cite web|title=Bond Lengths and Energies|url=http://www.doe-mbi.ucla.edu/CHEM125/bonds.html|work=Chem 125 notes|publisher=UCLA|access-date=13 November 2011|archive-url=https://web.archive.org/web/20110823121639/http://www.doe-mbi.ucla.edu/CHEM125/bonds.html|archive-date=23 August 2011|url-status=dead}}</ref><ref>Calculated: 2 to 4{{nbsp}}kJ/mol =  2{{e|3}}{{nbsp}}J / 6.022{{e|23}} molecules/mol = 3.3{{e|-21}}{{nbsp}}J.  In eV: 3.3{{e|-21}}{{nbsp}}J / 1.6{{e|-19}}{{nbsp}}J/eV = 0.02 eV.  4{{e|3}}{{nbsp}}J / 6.022{{e|23}} molecules/mol = 6.7{{e|-21}}{{nbsp}}J.  In eV:  6.7{{e|-21}}{{nbsp}}J / 1.6{{e|-19}}{{nbsp}}J/eV = 0.04 eV.</ref>
|-
|4.1×10<sup>−21</sup>{{nbsp}}J
| The "[[Boltzmann constant|k]]T" constant at 25&nbsp;°C, a common rough approximation for the total [[thermal energy]] of each molecule in a system (0.03 eV)<ref>{{cite web|last=Ansari|first=Anjum|title=Basic Physical Scales Relevant to Cells and Molecules|url=http://www.uic.edu/classes/phys/phys450/MARKO/N003.html|work=Physics 450|access-date=13 November 2011}}</ref>
|-
|7–22×10<sup>−21</sup>{{nbsp}}J
| Energy of a [[hydrogen bond]] (0.04 to 0.13 eV)<ref name=ucla_chem125/><ref>Calculated: 4 to 13{{nbsp}}kJ/mol.  4{{nbsp}}kJ/mol = 4{{e|3}}{{nbsp}}J / 6.022{{e|23}} molecules/mol = 6.7{{e|-21}}{{nbsp}}J.  In eV:  6.7{{e|-21}}{{nbsp}}J / 1.6{{e|-19}} eV/J = 0.042 eV. 13{{nbsp}}kJ/mol = 13{{e|3}}{{nbsp}}J / 6.022{{e|23}} molecules/mol = 2.2{{e|-20}}{{nbsp}}J.  In eV:  13{{e|3}}{{nbsp}}J / 6.022{{e|23}} molecules/mol / 1.6{{e|-19}} eV/J = 0.13 eV.</ref>
|-
| 10<sup>−20</sup>
| &nbsp;
| 4.5×10<sup>−20</sup>{{nbsp}}J
| Upper bound of the [[mass–energy equivalence|mass–energy]] of a [[neutrino]] in [[particle physics]] (0.28 eV)<ref>{{Cite journal | last1 = Thomas | first1 = S. | last2 = Abdalla | first2 = F. | last3 = Lahav | first3 = O. | title = Upper Bound of 0.28 eV on Neutrino Masses from the Largest Photometric Redshift Survey | doi = 10.1103/PhysRevLett.105.031301 | journal = Physical Review Letters | volume = 105 | issue = 3 | year = 2010 | pmid =  20867754|arxiv = 0911.5291 |bibcode = 2010PhRvL.105c1301T | pages=031301| s2cid = 23349570 }}</ref><ref>Calculated:  0.28 eV × 1.6{{e|-19}}{{nbsp}}J/eV = 4.5{{e|-20}}{{nbsp}}J</ref>
|-
|rowspan=4|10<sup>−19</sup>
|rowspan=4|&nbsp;
|1.6×10<sup>−19</sup>{{nbsp}}J || ≈1 [[electronvolt]] (eV)<ref>{{cite web|title=CODATA Value: electron volt|url=http://physics.nist.gov/cgi-bin/cuu/Value?tevj|publisher=NIST|access-date=4 November 2011}}</ref>
|-
|3–5×10<sup>−19</sup>{{nbsp}}J || Energy range of [[photon]]s in [[visible light]] (≈1.6–3.1 eV)<ref>{{cite web|title=BASIC LAB KNOWLEDGE AND SKILLS|url=http://www.sci.sdsu.edu/classes/chemistry/chem467l/mardahl/basic.html|quote=Visible wavelengths are roughly from 390 nm to 780 nm|access-date=5 November 2011|archive-url=https://web.archive.org/web/20130515121940/http://www.sci.sdsu.edu/classes/chemistry/chem467l/mardahl/basic.html|archive-date=15 May 2013|url-status=dead}}</ref><ref>Calculated:  E = hc/λ.  E{{sub|780 nm}} = 6.6{{e|-34}} kg-m{{sup|2}}/s × 3{{e|8}} m/s / (780{{e|-9}} m) = 2.5{{e|-19}}{{nbsp}}J.  E_390 _nm = 6.6{{e|-34}} kg-m{{sup|2}}/s × 3{{e|8}} m/s / (390{{e|-9}} m) = 5.1{{e|-19}}{{nbsp}}J</ref>
|-
|3–14×10<sup>−19</sup>{{nbsp}}J
| Energy of a [[covalent bond]] (2–9 eV)<ref name=ucla_chem125/><ref>Calculated:  50 kcal/mol × 4.184{{nbsp}}J/calorie / 6.0{{e|22}}e23 molecules/mol = 3.47{{e|-19}}{{nbsp}}J.  (3.47{{e|-19}}{{nbsp}}J / 1.60{{e|-19}} eV/J = 2.2 eV.) and 200 kcal/mol × 4.184{{nbsp}}J/calorie / 6.0{{e|22}}e23 molecules/mol = 1.389{{e|-18}}{{nbsp}}J.  (7.64{{e|-19}}{{nbsp}}J / 1.60{{e|-19}} eV/J = 8.68 eV.)</ref>
|-
| 5–200×10<sup>−19</sup>{{nbsp}}J
| Energy of [[ultraviolet]] light photons<ref name="NASA_spectrum"/>
|-
|10<sup>−18</sup>{{Anchor|10-18}} || [[atto-]] (aJ) || 2.18×10<sup>−18</sup>{{nbsp}}J || Ground state [[ionization energy]] of [[hydrogen]] (13.6 eV)
|-
| 10<sup>−17</sup>
| &nbsp;
| 2–2000×10<sup>−17</sup>{{nbsp}}J
| Energy range of [[X-ray]] photons<ref name="NASA_spectrum">{{cite web|title=Wavelength, Frequency, and Energy|url=http://imagine.gsfc.nasa.gov/docs/science/know_l1/spectrum_chart.html|archive-url=https://web.archive.org/web/20011118152730/http://imagine.gsfc.nasa.gov/docs/science/know_l1/spectrum_chart.html|url-status=dead|archive-date=18 November 2001|work=Imagine the Universe|publisher=NASA|access-date=15 November 2011}}</ref>
|-
| 10<sup>−16</sup> || &nbsp; || &nbsp; || &nbsp;
|-
| 10<sup>−15</sup>{{Anchor|10-15}} || [[femto-]] (fJ) || 3 × 10<sup>−15</sup>{{nbsp}}J || Average kinetic energy of one human [[red blood cell]].<ref>{{cite journal| last1 = Phillips | first1 = Kevin | last2 = Jacques | first2 = Steven | last3 = McCarty | first3 = Owen | title=How much does a cell weigh?| journal = Physical Review Letters | volume = 109 | issue = 11 | pages = 118105 | year = 2012 | doi = 10.1103/PhysRevLett.109.118105 | pmid = 23005682 |quote = Roughly 27 picograms | bibcode=2012PhRvL.109k8105P| pmc=3621783 }}</ref><ref>{{cite web|title=Our Bodies' Velocities, By the Numbers|author=Bob Berman|access-date=19 August 2016|url = http://discovermagazine.com/2014/julyaug/18-body-of-work | quote = The [...] blood [...] flow[s] at an average speed of 3 to 4 mph}}</ref><ref>Calculated: 1/2 × 27{{e|-12}} g × (3.5 miles per hour){{sup|2}} = 3{{e|-15}}{{nbsp}}J</ref>
|-
|rowspan=4|10<sup>−14</sup>
|rowspan=4|&nbsp;
| 1×10<sup>−14</sup>{{nbsp}}J
| [[Sound energy]] (vibration) transmitted to the [[eardrums]] by listening to a [[whisper]] for one second.<ref>{{cite web|title=Physics of the Body|url=https://www3.nd.edu/~nsl/Lectures/mphysics/Medical%20Physics/Part%20I.%20Physics%20of%20the%20Body/Chapter%204.%20Acoustics%20of%20the%20Body/4.3%20Physics%20of%20the%20ear/Physics%20of%20the%20ear.pdf|publisher=Notre Dame|access-date=19 August 2016|archive-date=6 November 2016|archive-url=https://web.archive.org/web/20161106160152/https://www3.nd.edu/~nsl/Lectures/mphysics/Medical%20Physics/Part%20I.%20Physics%20of%20the%20Body/Chapter%204.%20Acoustics%20of%20the%20Body/4.3%20Physics%20of%20the%20ear/Physics%20of%20the%20ear.pdf|url-status=dead}}. "The eardrum is a [...] membran[e] with an area of 65 mm<sup>2</sup>."</ref><ref>{{cite web|title=Intensity and the Decibel Scale|url=http://www.physicsclassroom.com/class/sound/Lesson-2/Intensity-and-the-Decibel-Scale|publisher=Physics Classroom|access-date=19 August 2016}}</ref><ref>Calculated: two eardrums ≈ 1&nbsp;cm<sup>2</sup>.  1{{e|-6}} W/m<sup>2</sup> × 1{{e|-4}} m<sup>2</sup> × 1 s = 1{{e|-14}}{{nbsp}}J</ref>
|-
| > 2×10<sup>−14</sup>{{nbsp}}J
| Energy of [[gamma ray]] photons<ref name="NASA_spectrum"/>
|-
|2.7×10<sup>−14</sup>{{nbsp}}J || Upper bound of the [[mass–energy equivalence|mass–energy]] of a [[muon neutrino]]<ref>{{cite book|title=Neutrinos in physics and astrophysics: from 10–33 to 1028 cm: TASI 98 : Boulder, Colorado, USA, 1–26 June 1998|year=2000|publisher=World Scientific|isbn=978-981-02-3887-2|url=https://books.google.com/books?id=QC5zi1N-1KMC&q=muon+neutrino+mass+170kev&pg=PA354|author=Thomas J Bowles|author-link=The Experimental Search for Finite Neutrino Mass|editor=P. Langacker|access-date=11 November 2011|page=354|quote=an upper limit ov m_v_u < 170 keV}}</ref><ref>Calculated:  170{{e|3}} eV × 1.6{{e|-19}}{{nbsp}}J/eV = 2.7{{e|-14}}{{nbsp}}J</ref>
|-
|8.2×10<sup>−14</sup>{{nbsp}}J || Rest [[mass–energy]] of an [[electron]]<ref>{{cite web|title=electron mass energy equivalent|url=http://physics.nist.gov/cgi-bin/cuu/Value?mec2|publisher=NIST|access-date=4 November 2011}}</ref> (0.511 MeV)<ref>{{Cite web |title=CODATA Value: electron mass energy equivalent in MeV |url=https://physics.nist.gov/cgi-bin/cuu/Value?mec2mev |access-date=2023-08-13 |website=physics.nist.gov}}</ref>
|-
|rowspan=2|10<sup>−13</sup>
|rowspan=2| &nbsp;
| 1.6×10<sup>−13</sup>{{nbsp}}J || 1 [[megaelectronvolt]] (MeV)<ref>{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=6&num=1&From=ev&To=j&Action=Convert+value+and+show+factor|publisher=NIST|access-date=4 November 2011}}</ref>
|-
| 2.3×10<sup>−13</sup>{{nbsp}}J || Energy released by a single event of two [[proton]]s fusing into [[deuterium]] (1.44 megaelectronvolt MeV)<ref>{{cite web|title=How much energy is released when hydrogen is fused to produce one kilo of helium?|date=11 November 2017|url=https://hbergeronx.medium.com/how-much-energy-is-released-when-hydrogen-is-fused-to-produce-one-kilo-of-helium-64e74b03b13e|access-date=21 July 2021}}</ref>
|-
|10<sup>−12</sup>{{Anchor|10-12}} || [[pico-]] (pJ) || 2.3×10<sup>−12</sup>{{nbsp}}J || Kinetic energy of [[neutron]]s produced by [[DT fusion]], used to trigger fission (14.1 MeV)<ref>{{cite web|last=Muller|first=Richard A.|title=The Sun, Hydrogen Bombs, and the physics of fusion|url=http://muller.lbl.gov/teaching/physics10/old%20physics%2010/chapters%20%28old%29/7-fusion.htm|access-date=5 November 2011|year=2002|quote=The neutron comes out with high energy of 14.1 MeV|archive-url=https://web.archive.org/web/20120402214226/http://muller.lbl.gov/teaching/physics10/old%20physics%2010/chapters%20(old)/7-fusion.htm|archive-date=2 April 2012|url-status=dead}}</ref><ref>{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=7&num=1.41&From=ev&To=j&Action=Convert+value+and+show+factor|publisher=NIST|access-date=4 November 2011}}</ref>
|-
|rowspan=1|10<sup>−11</sup>
|rowspan=1|&nbsp;
|3.4×10<sup>−11</sup>{{nbsp}}J || Average total energy [[nuclear explosions|released]] in the [[nuclear fission]] of one [[uranium-235]] [[atom]] (215 MeV)<ref name="Energy From Uranium Fission">{{cite web|title=Energy From Uranium Fission|url=http://hyperphysics.phy-astr.gsu.edu/hbase/nucene/u235chn.html#c3|work=HyperPhysics|access-date=8 November 2011}}</ref><ref name="Conversion from eV to J">{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=8&num=2.15&From=ev&To=j&Action=Convert+value+and+show+factor|publisher=NIST|access-date=4 November 2011}}</ref>
|-
| rowspan="7" |10<sup>−10</sup>
| rowspan="7" |&nbsp;
|1.492×10<sup>−10</sup>{{nbsp}}J
|[[Mass–energy equivalence|Mass-energy]] equivalent of 1 [[Unified atomic mass unit|u]]<ref>{{Cite web |title=CODATA Value: atomic mass constant energy equivalent |url=https://physics.nist.gov/cgi-bin/cuu/Value?uj |access-date=2023-08-13 |website=physics.nist.gov}}</ref> (931.5 MeV)<ref>{{Cite web |title=CODATA Value: atomic mass constant energy equivalent in MeV |url=https://physics.nist.gov/cgi-bin/cuu/Value?muc2mev |access-date=2023-08-13 |website=physics.nist.gov}}</ref>
|-
|1.503×10<sup>−10</sup>{{nbsp}}J || Rest [[mass–energy]] of a [[proton]]<ref>{{cite web|title=proton mass energy equivalent|url=http://physics.nist.gov/cgi-bin/cuu/Value?mpc2|publisher=NIST|access-date=4 November 2011}}</ref> (938.3 MeV)<ref>{{Cite web |title=CODATA Value: proton mass energy equivalent in MeV |url=https://physics.nist.gov/cgi-bin/cuu/Value?mpc2mev |access-date=2023-08-13 |website=physics.nist.gov}}</ref>
|-
|1.505×10<sup>−10</sup>{{nbsp}}J || Rest [[mass–energy]] of a [[neutron]]<ref>{{cite web|title=neutron mass energy equivalent|url=http://physics.nist.gov/cgi-bin/cuu/Value?mnc2|publisher=NIST|access-date=4 November 2011}}</ref> (939.6 MeV)<ref>{{Cite web |title=CODATA Value: neutron mass energy equivalent in MeV |url=https://physics.nist.gov/cgi-bin/cuu/Value?mnc2mev |access-date=2023-08-13 |website=physics.nist.gov}}</ref>
|-
|1.6×10<sup>−10</sup>{{nbsp}}J || 1 [[gigaelectronvolt]] (GeV)<ref>{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=9&num=1&From=ev&To=j&Action=Convert+value+and+show+factor|publisher=NIST|access-date=4 November 2011}}</ref>
|-
|3×10<sup>−10</sup>{{nbsp}}J || Rest [[mass–energy]] of a [[deuteron]]<ref>{{cite web|title=deuteron mass energy equivalent|url=http://physics.nist.gov/cgi-bin/cuu/Value?mdc2|publisher=NIST|access-date=4 November 2011}}</ref>
|-
|6×10<sup>−10</sup>{{nbsp}}J || Rest [[mass–energy]] of an [[alpha particle]]<ref>{{cite web|title=alpha particle mass energy equivalent|url=http://physics.nist.gov/cgi-bin/cuu/Value?malc2|publisher=NIST|access-date=4 November 2011}}</ref>
|-
|7×10<sup>−10</sup>{{nbsp}}J || Energy required to raise a grain of [[sand]] by 0.1mm (the thickness of a piece of paper).<ref>Calculated: 7{{e|-4}} g × 9.8 m/s<sup>2</sup> × 1{{e|-4}} m</ref>
|-
|rowspan=2|10<sup>−9</sup>{{Anchor|10-9
}}
|rowspan=2| [[nano-]] (nJ)
| 1.6×10<sup>−9</sup>{{nbsp}}J || 10 GeV<ref>{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=10&num=1&From=ev&To=j&Action=Convert+value+and+show+factor|publisher=NIST|access-date=4 November 2011}}</ref>
|-
| 8×10<sup>−9</sup>{{nbsp}}J || Initial operating energy per beam of the [[CERN]] [[Large Electron Positron Collider]] in 1989 (50 GeV)<ref>{{cite web|last=Myers|first=Stephen|title=The LEP Collider|url=http://sl-div.web.cern.ch/sl-div/history/lep_doc.html|publisher=CERN|access-date=14 November 2011|quote=the LEP machine energy is about 50 GeV per beam}}</ref><ref>Calculated:  50{{e|9}} eV × 1.6{{e|-19}}{{nbsp}}J/eV = 8{{e|-9}}{{nbsp}}J</ref>
|-
|rowspan=5|10<sup>−8</sup>
|rowspan=5|&nbsp;
| 1.3×10<sup>−8</sup>{{nbsp}}J || [[Mass–energy]] of a [[W boson]] (80.4 GeV)<ref>{{cite web|title=W|url=http://pdglive.lbl.gov/Rsummary.brl?nodein=S043|archive-url=https://archive.today/20120717002128/http://pdglive.lbl.gov/Rsummary.brl?nodein=S043|url-status=dead|archive-date=17 July 2012|work=PDG Live|publisher=Particle Data Group|access-date=4 November 2011}}</ref><ref>{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=9&num=80.4&From=ev&To=j&Action=Convert+value+and+show+factor&Action=Convert+value+and+show+factor|publisher=NIST|access-date=4 November 2011}}</ref>
|-
| 1.5×10<sup>−8</sup>{{nbsp}}J || [[Mass–energy]] of a [[Z boson]] (91.2 GeV)<ref name="Amsler2008">{{Cite journal | last1 = Amsler | first1 = C. | last2 = Doser | first2 = M. | last3 = Antonelli | first3 = M. | last4 = Asner | first4 = D. | last5 = Babu | first5 = K. | last6 = Baer | first6 = H. | last7 = Band | first7 = H. | last8 = Barnett | first8 = R. | last9 = Bergren | first9 = E. | last10 = Beringer | first10 = J. | last11 = Bernardi | first11 = G. | last12 = Bertl | first12 = W. | last13 = Bichsel | first13 = H. | last14 = Biebel | first14 = O. | last15 = Bloch | first15 = P. | last16 = Blucher | first16 = E. | last17 = Blusk | first17 = S. | last18 = Cahn | first18 = R. N. | last19 = Carena | first19 = M. | last20 = Caso | first20 = C. | last21 = Ceccucci | first21 = A. | last22 = Chakraborty | first22 = D. | last23 = Chen | first23 = M. -C. | last24 = Chivukula | first24 = R. S. | last25 = Cowan | first25 = G. | last26 = Dahl | first26 = O. | last27 = d'Ambrosio | first27 = G. | last28 = Damour | first28 = T. | last29 = De Gouvêa | first29 = A. | last30 = Degrand | first30 = T. | title = Review of Particle Physics⁎ | doi = 10.1016/j.physletb.2008.07.018 | journal = Physics Letters B | volume = 667 | issue = 1 | pages = 1–6 | year = 2008 | url = http://pdglive.lbl.gov/Rsummary.brl?nodein=S044&fsizein=1 | archive-url = https://archive.today/20120712165412/http://pdglive.lbl.gov/Rsummary.brl?nodein=S044&fsizein=1 | url-status = dead | archive-date = 12 July 2012 | bibcode = 2008PhLB..667....1A | display-authors = 29 | hdl = 1854/LU-685594 | s2cid = 227119789 | hdl-access = free }}</ref><ref>{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=9&num=91.2&From=ev&To=j&Action=Convert+value+and+show+factor|publisher=NIST|access-date=4 November 2011}}</ref>
|-
| 1.6×10<sup>−8</sup>{{nbsp}}J || 100 GeV<ref>{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=11&num=1&From=ev&To=j&Action=Convert+value+and+show+factor|publisher=NIST|access-date=4 November 2011}}</ref>
|-
| 2×10<sup>−8</sup>{{nbsp}}J || [[Mass–energy]] of the [[Higgs Boson]] (125.1 GeV)<ref>{{cite journal|last1=ATLAS |last2=CMS |author-link1=ATLAS experiment|author-link2=Compact Muon Solenoid|arxiv=1503.07589 |title= Combined Measurement of the Higgs Boson Mass in pp Collisions at √s=7 and 8 TeV with the ATLAS and CMS Experiments|date=26 March 2015 |doi=10.1103/PhysRevLett.114.191803 |pmid=26024162 |bibcode=2015PhRvL.114s1803A |volume=114 |issue=19 |pages=191803 |journal=Physical Review Letters|s2cid=1353272 }}</ref>
|-
| 6.4×10<sup>−8</sup>{{nbsp}}J || Operating energy per proton of the [[CERN]] [[Super Proton Synchrotron]] accelerator in 1976<ref>{{cite web|last=Adams|first=John|title=400 GeV Proton Synchrotron|url=http://sl-div.web.cern.ch/sl-div/history/sps_doc.html|work=Excertp from the CERN Annual Report 1976|publisher=CERN|access-date=14 November 2011|quote=A circulating proton beam of 400 GeV energy was first achieved in the SPS on 17 June 1976}}</ref><ref>Calculated:  400{{e|9}} eV × 1.6{{e|-19}}{{nbsp}}J/eV = 6.4{{e|-8}}{{nbsp}}J</ref>
|-
|rowspan=2|10<sup>−7</sup>
|rowspan=2|&nbsp;
| 1×10<sup>−7</sup>{{nbsp}}J   || ≡ 1 [[erg]]<ref name=NIST_SI_units/>
|-
| 1.6×10<sup>−7</sup>{{nbsp}}J || 1 TeV (teraelectronvolt),<ref>{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=12&num=1&From=ev&To=j&Action=Convert+value+and+show+factor|publisher=NIST|access-date=4 November 2011}}</ref> about the kinetic energy of a flying [[mosquito]]<ref>{{cite web|title=Chocolate bar yardstick|url=http://www.cernlove.org/blog/2010/04/chocolate-bar-yardstick/|access-date=24 January 2014|quote=A TeV is actually a very tiny amount of energy. A popular analogy is to a flying mosquito.|archive-url=https://web.archive.org/web/20140226141339/http://www.cernlove.org/blog/2010/04/chocolate-bar-yardstick/|archive-date=26 February 2014|url-status=dead}}</ref>
|-
|10<sup>−6</sup>{{Anchor|10-6}} || [[micro-]] (μJ) || 1.04×10<sup>−6</sup>{{nbsp}}J || Energy per proton in the [[CERN]] [[Large Hadron Collider]] in 2015 (6.5 TeV)<ref>{{cite web|title=First successful beam at record energy of 6.5 TeV|url=http://home.web.cern.ch/about/updates/2015/04/first-successful-beam-record-energy-65-tev|access-date=28 April 2015}}</ref><ref>Calculated:  6.5{{e|12}} eV per beam × 1.6{{e|-19}}{{nbsp}}J/eV = 1.04{{e|-6}}{{nbsp}}J</ref>
|-
| 10<sup>−5</sup> || &nbsp; || &nbsp; || &nbsp;
|-
| 10<sup>−4</sup> || &nbsp; || 1.0×10<sup>−4</sup>{{nbsp}}J || Energy released by a typical [[Radium dial|radioluminescent wristwatch]] in 1 hour<ref>{{Cite web |title=The radioactive series of radium-226 |url=https://indico.cern.ch/event/835006/contributions/3548764/attachments/1924479/3184497/Ra226Decays.pdf |website=CERN}}</ref><ref>{{Cite journal |last1=Terrill |first1=James G. Jr. |last2=Ingraham |first2=Samuel C. II |last3=Moeller |first3=Dade W. |date=1954 |title=Radium in the Healing Arts and in Industry: Radiation Exposure in the United States |journal=Public Health Reports |language=en |volume=69 |issue=3 |pages=255–262 |doi=10.2307/4588736|jstor=4588736 |pmid=13134440 |pmc=2024184 }}</ref> (1 [[Curie (unit)|µCi]] × 4.871 MeV × 1 hr)
|-
| 10<sup>−3</sup>{{Anchor|10-3}} || [[milli-]] (mJ) || 3.0×10<sup>−3</sup>{{nbsp}}J || Energy released by a P100 [[atomic battery]] in 1 hour<ref>{{Cite web |title=NanoTritium™: Next-gen Tritium Battery with Decade-Long Betavoltaic Battery Power {{!}} CityLabs |url=https://citylabs.net/products/ |access-date=2022-04-04 |language=en-US}}</ref> (2.4 V × 350 nA × 1 hr)
|-
| 10<sup>−2</sup>{{Anchor|10-2
}} || [[centi-]] (cJ) || 4.0×10<sup>−2</sup>{{nbsp}}J || Use of a typical LED for 1 second<ref>{{Cite web |title=LED - Basic Red 5mm - COM-09590 - SparkFun Electronics |url=https://www.sparkfun.com/products/9590 |access-date=2022-04-04 |website=www.sparkfun.com}}</ref> (2.0 V × 20 mA × 1 s)
|-
|rowspan=1|10<sup>−1</sup>{{Anchor|10-1}}
|rowspan=1| [[deci-]] (dJ)
| 1.1×10<sup>−1</sup>{{nbsp}}J || Energy of an [[Half dollar (United States coin)|American half-dollar]] falling 1 metre<ref>{{cite web |url=http://www.usmint.gov/about_the_mint/?action=coin_specifications |title=Coin specifications |publisher=United States Mint |access-date=2 November 2011 |quote=11.340 g |archive-date=18 February 2015 |archive-url=https://web.archive.org/web/20150218061037/http://www.usmint.gov/about_the_mint/?action=coin_specifications |url-status=dead }}</ref><ref>Calculated:  m×g×h = 11.34{{e|-3}} kg × 9.8 m/s{{sup|2}} × 1 m = 1.1{{e|-1}}{{nbsp}}J</ref>
|}

==1 to 10<sup>5</sup> J==
{| class="wikitable"
|-
|rowspan=8|10<sup>0</sup>
|rowspan=8| J
| 1{{nbsp}}J || ≡ 1 N·m ([[newton (unit)|newton]]–[[metre]])
|-
| 1{{nbsp}}J || ≡ 1&nbsp;W·s ([[watt]]-second)
|-
| 1{{nbsp}}J || Kinetic energy produced as an extra small apple (~100 grams<ref>{{cite web|url=http://www.nal.usda.gov/fnic/foodcomp/search/ |title=Apples, raw, with skin (NDB No. 09003) |work=USDA Nutrient Database |publisher=USDA |access-date=8 December 2011 |url-status=dead |archive-url=https://web.archive.org/web/20150303184216/http://www.nal.usda.gov/fnic/foodcomp/search/ |archive-date= 3 March 2015 }}</ref>) falls 1 [[meter]] against Earth's [[gravity]]<ref>Calculated:  m×g×h = 1{{e|-1}} kg × 9.8 m/s{{sup|2}} × 1 m = 1{{nbsp}}J</ref>
|-
| 1{{nbsp}}J || Energy required to heat 1 gram of dry, cool [[Earth's atmosphere|air]] by 1 degree [[Celsius]]<ref>{{cite web|title=Specific Heat of Dry Air|url=http://www.engineeringtoolbox.com/air-specific-heat-capacity-d_705.html|publisher=Engineering Toolbox|access-date=2 November 2011}}</ref>
|-
| 1.4{{nbsp}}J || ≈ 1&nbsp;ft·lbf ([[foot-pound force]])<ref name=NIST_SI_units>{{cite web|title=Appendix B8—Factors for Units Listed Alphabetically|url=http://physics.nist.gov/Pubs/SP811/appenB8.html|work=NIST Guide for the Use of the International System of Units (SI)|publisher=NIST|quote=1.355818|date=2 July 2009}}</ref>
|-
| 4.184{{nbsp}}J || ≡ 1 thermochemical [[calorie]] (small calorie)<ref name=NIST_SI_units/>
|-
| 4.1868{{nbsp}}J || ≡ 1 International (Steam) Table calorie<ref>{{cite web|title=Footnotes|url=http://physics.nist.gov/Pubs/SP811/footnotes.html#f09|work=NIST Guide to the SI|publisher=NIST|date=2 July 2009}}</ref>
|-
| 8{{nbsp}}J || [[Greisen–Zatsepin–Kuzmin limit|Greisen-Zatsepin-Kuzmin]] theoretical upper limit for the energy of a [[cosmic ray]] coming from a distant source<ref>{{cite web|title=Physical Motivations|url=http://www.dfg.unito.it/euso/physical-motivation.html|work=ULTRA Home Page (EUSO project)|publisher=Dipartimento di Fisica di Torino|access-date=12 November 2011}}</ref><ref>Calculated:  5{{e|19}} eV × 1.6{{e|-19}}{{nbsp}}J/ev = 8{{nbsp}}J</ref>
|-
| rowspan="3" |10<sup>1</sup>{{Anchor|101}}
| rowspan="3" | [[deca-]] (daJ)
| 1×10<sup>1</sup>{{nbsp}}J || Flash energy of a typical pocket camera electronic flash [[capacitor]] {{nowrap|(100–400 μF}} @ {{nowrap|330 V)}}<ref>{{cite web|title=Notes on the Troubleshooting and Repair of Electronic Flash Units and Strobe Lights and Design Guidelines, Useful Circuits, and Schematics|url=http://www.repairfaq.org/sam/strbfaq.htm|access-date=8 December 2011|quote=The energy storage capacitor for pocket cameras is typically 100 to 400 uF at 330 V (charged to 300 V) with a typical flash energy of 10 W-s.}}</ref><ref name="ev_pwrsh">{{cite web|title=Teardown: Digital Camera Canon PowerShot {{pipe}}|url=http://electroelvis.com/2012/09/02/teardown-digital-camera-canon-powershot/|date=2 September 2012|access-date=6 June 2013|publisher=electroelvis.com|archive-url=https://web.archive.org/web/20130801014811/http://electroelvis.com/2012/09/02/teardown-digital-camera-canon-powershot/|archive-date=1 August 2013|url-status=dead}}</ref>
|-
|3.7–40×10<sup>1</sup>
|Kinetic energy of a punch.<ref>{{Cite web |last=Pomeroy |first=Ross |date=January 1, 2014 |title=How to Get Punched in the Face |url=https://www.realclearscience.com/blog/2014/01/the_physics_of_getting_punched_in_the_face.html |website=RealClearScience}}</ref>
|-
| 5×10<sup>1</sup>{{nbsp}}J || The [[Oh-My-God particle|most energetic cosmic ray]] ever detected.<ref>{{cite web|title=The Fly's Eye (1981–1993)|url=http://www.cosmic-ray.org/reading/flyseye.html#SEC10|publisher=HiRes|access-date=14 November 2011}}</ref> Most likely a [[Oh-My-God Particle|single proton]] traveling only very slightly slower than the speed of light.<ref>
{{Cite journal
 | author=Bird, D. J.
 | date=March 1995
 | title=Detection of a cosmic ray with measured energy well beyond the expected spectral cutoff due to cosmic microwave radiation
 | journal=Astrophysical Journal, Part 1
 | volume=441 |issue=1 |pages=144–150
 | bibcode=1995ApJ...441..144B
 | arxiv=astro-ph/9410067
 | doi=10.1086/175344
 | s2cid=119092012
 }}</ref>
|-
| rowspan="12" |10<sup>2</sup>{{Anchor|100|102}}
| rowspan="12" |[[hecto-]] (hJ)
|1.25×10<sup>2</sup>{{nbsp}}J
|Kinetic energy of a regulation (standard) baseball (5.1&nbsp;oz / 145&nbsp;g)<ref>{{Cite web |date=2024-01-04 |title=How Much Does a Baseball Weigh? - Baseball Weight Facts |url=https://www.nations-baseball.com/how-much-does-a-baseball-weigh/ |access-date=2024-01-04 |archive-url=https://web.archive.org/web/20240104164703/https://www.nations-baseball.com/how-much-does-a-baseball-weigh/ |archive-date=4 January 2024 }}</ref> thrown at 93&nbsp;mph / 150&nbsp;km/h (MLB average pitch speed).<ref>{{Cite web |date=2024-01-04 |title=How fast does an average MLB pitcher throw? - TopVelocity |url=https://www.topvelocity.net/2023/06/05/how-fast-does-an-average-mlb-pitcher-throw/ |access-date=2024-01-04 |archive-url=https://web.archive.org/web/20240104164625/https://www.topvelocity.net/2023/06/05/how-fast-does-an-average-mlb-pitcher-throw/ |archive-date=4 January 2024 }}</ref>
|-
|1.5×10<sup>2</sup>{{nbsp}}to 3.6×10<sup>2</sup>{{nbsp}}J || Energy delivered by a biphasic external electric shock ([[defibrillation]]), usually during adult [[cardiopulmonary resuscitation]] for [[cardiac arrest]].
|-
|3×10<sup>2</sup>{{nbsp}}J || Energy of a lethal dose of [[X-ray]]s<ref>{{cite web|title=Ionizing Radiation|url=http://chemed.chem.purdue.edu/genchem/topicreview/bp/ch23/radiation.php|work=General Chemistry Topic Review: Nuclear Chemistry|publisher=Bodner Research Web|access-date=5 November 2011}}</ref>
|-
|3×10<sup>2</sup>{{nbsp}}J || Kinetic energy of an average person jumping as high as they can<ref>{{cite web|title=Vertical Jump Test|url=http://www.topendsports.com/testing/tests/vertjump.htm|publisher=Topend Sports|access-date=12 December 2011|quote=41–50 cm (males) 31–40 cm (females)}}</ref><ref>{{cite web|title=Mass of an Adult|url=http://hypertextbook.com/facts/2003/AlexSchlessingerman.shtml|work=The Physics Factbook|access-date=13 December 2011|quote=70 kg}}</ref><ref>Kinetic energy at start of jump = potential energy at high point of jump. Using a mass of 70&nbsp;kg and a high point of 40&nbsp;cm => energy = m×g×h = 70&nbsp;kg × 9.8 m/s{{sup|2}} × 40{{e|-2}} m = 274{{nbsp}}J</ref>
|-
|3.3×10<sup>2</sup>{{nbsp}}J || [[Enthalpy of fusion|Energy to melt]] 1&nbsp;g of [[ice]]<ref>{{cite web|title=Latent Heat of Melting of some common Materials|url=http://www.engineeringtoolbox.com/latent-heat-melting-solids-d_96.html|publisher=Engineering Toolbox|access-date=10 June 2013|quote=334{{nbsp}}kJ/kg}}</ref>
|-
|> 3.6×10<sup>2</sup>{{nbsp}}J || Kinetic energy of 800&nbsp;gram<ref>{{cite web|title=Javelin Throw – Introduction|url=http://www.iaaf.org/community/athletics/trackfield/newsid=9427.html|publisher=IAAF|access-date=12 December 2011}}</ref> [[Javelin Throw|standard men's javelin]] thrown at > 30&nbsp;m/s<ref>{{cite web|last=Young|first=Michael|title=Developing Event Specific Strength for the Javelin Throw|url=http://www.indianathrower.com/documents/javelinthrowbiomechanics.pdf|archive-url=https://web.archive.org/web/20110813094040/http://www.indianathrower.com/documents/javelinthrowbiomechanics.pdf|url-status=dead|archive-date=13 August 2011|access-date=13 December 2011|quote=For elite athletes, the velocity of a javelin release has been measured in excess of 30m/s}}</ref> by elite javelin throwers<ref>Calculated: 1/2 × 0.8&nbsp;kg × (30 m/s){{sup|2}} = 360{{nbsp}}J</ref>
|-
|5–20×10<sup>2</sup>{{nbsp}}J || Energy output of a typical [[photography]] studio [[xenon flash lamp|strobe light]] in a single flash<ref>{{cite web|last=Greenspun|first=Philip|title=Studio Photography|url=http://photo.net/learn/studio/primer|access-date=13 December 2011|quote=Most serious studio photographers start with about 2000 watts-seconds|url-status=dead|archive-url=https://web.archive.org/web/20070929104533/http://photo.net/learn/studio/primer|archive-date=29 September 2007}}</ref>
|-
|6×10<sup>2</sup>{{nbsp}}J || Kinetic energy of 2&nbsp;kg<ref>{{cite web|title=Discus Throw – Introduction|url=http://www.iaaf.org/community/athletics/trackfield/newsid=9437.html|publisher=IAAF|access-date=12 December 2011}}</ref> [[Discus Throw|standard men's discus]] thrown at 24.4&nbsp;m/s{{Citation needed|date=November 2011}} by the world record holder [[Jürgen Schult]]<ref>Calculated: 1/2 × 2&nbsp;kg × (24.4 m/s){{sup|2}} = 595.4{{nbsp}}J</ref>
|-
|6×10<sup>2</sup>{{nbsp}}J || Use of a 10-watt flashlight for 1 minute
|-
|7.5×10<sup>2</sup>{{nbsp}}J || A power of 1 [[horsepower]] applied for 1 second<ref name=NIST_SI_units/>
|-
|7.8×10<sup>2</sup>{{nbsp}}J || Kinetic energy of 7.26&nbsp;kg<ref>{{cite web|title=Shot Put – Introduction|url=http://www.iaaf.org/community/athletics/trackfield/newsid=9444.html|publisher=IAAF|access-date=12 December 2011}}</ref> [[Shot Put|standard men's shot]] thrown at 14.7&nbsp;m/s{{Citation needed|date=November 2011}} by the world record holder [[Randy Barnes]]<ref>Calculated: 1/2 × 7.26&nbsp;kg × (14.7 m/s){{sup|2}} = 784{{nbsp}}J</ref>
|-
|8.01×10<sup>2</sup>{{nbsp}}J
|Amount of work needed to lift a man with an average weight (81.7&nbsp;kg) one meter above Earth (or any planet with Earth gravity)
|-
| rowspan="12" |10<sup>3</sup>{{Anchor|103}}
| rowspan="12" | [[kilo-]] (kJ)
|1.1×10<sup>3</sup>{{nbsp}}J || ≈ 1 [[British thermal unit]] (BTU), depending on the [[temperature]]<ref name=NIST_SI_units/>
|-
|1.4×10<sup>3</sup>{{nbsp}}J || Total [[solar radiation]] received from the [[Sun]] by 1 [[square meter]] at the altitude of Earth's orbit per second ([[solar constant]])<ref>{{Cite journal | last1 = Kopp | first1 = G. | last2 = Lean | first2 = J. L. | author2-link=Judith Lean | doi = 10.1029/2010GL045777 | title = A new, lower value of total solar irradiance: Evidence and climate significance | journal = Geophysical Research Letters | volume = 38 | issue = 1 | pages = n/a | year = 2011 |bibcode = 2011GeoRL..38.1706K | doi-access = free }}</ref>
|-
|1.8×10<sup>3</sup>{{nbsp}}J || Kinetic energy of [[M16 rifle]] [[bullet]] ([[5.56×45mm NATO]] [[M855]], 4.1&nbsp;g fired at 930&nbsp;m/s)<ref>{{cite web|title=Intermediate power ammunition for automatic assault rifles|url=http://world.guns.ru/ammunition/intermediate-cartridges-e.html|work=Modern Firearms|publisher=World Guns|access-date=12 December 2011|url-status=dead|archive-url=https://web.archive.org/web/20130810184827/http://world.guns.ru/ammunition/intermediate-cartridges-e.html|archive-date=10 August 2013}}</ref>
<!-- Don't need so many of these bullet entries:
|-
|~1.4×10<sup>3</sup>{{nbsp}}J || Kinetic energy of a [[5.45x39mm]] [[AK-74]] [[bullet]] (3.6 g fired at 880 m/s)<ref>{{cite web|title=Intermediate power ammunition for automatic assault rifles|url=http://world.guns.ru/ammunition/intermediate-cartridges-e.html|work=Modern Firearms|publisher=World Guns|access-date=12 December 2011}}</ref>
|-
|1.7×10<sup>3</sup>{{nbsp}}J || Kinetic energy of a 3.56 g [[.223 Remington]] M193 [[M16 rifle|M16]] [[bullet]] fired at 975 m/s
|-
|3.3×10<sup>3</sup>{{nbsp}}J || Kinetic energy of a 9.33 g [[7.62×51mm NATO]] [[rifle]] [[Cartridge (firearms)|cartridge]] fired at {{nowrap|838 m/s}}
-->
|-
|2.3×10<sup>3</sup>{{nbsp}}J || [[Enthalpy of vaporization|Energy to vaporize]] 1&nbsp;g of [[water]] into steam<ref>{{cite web|title=Fluids – Latent Heat of Evaporation|url=http://www.engineeringtoolbox.com/fluids-evaporation-latent-heat-d_147.html|publisher=Engineering Toolbox|access-date=10 June 2013|quote=2257 kJ/kg}}</ref>
|-
|3×10<sup>3</sup>{{nbsp}}J   || [[Lorentz force]] [[Pinch (plasma physics)#Crushing cans with the pinch effect|can crusher pinch]]<ref>[http://www.powerlabs.org/pssecc.htm powerlabs.org – The PowerLabs Solid State Can Crusher!], 2002</ref>
|-
|3.4×10<sup>3</sup>{{nbsp}}J || Kinetic energy of world-record men's [[hammer throw]] (7.26&nbsp;kg<ref>{{cite web|title=Hammer Throw – Introduction|url=http://www.iaaf.org/community/athletics/trackfield/newsid=9418.html|publisher=IAAF|access-date=12 December 2011}}</ref> thrown at 30.7&nbsp;m/s<ref>{{cite web|last=Otto|first=Ralf M.|title=HAMMER THROW WR PHOTOSEQUENCE – YURIY SEDYKH|url=http://hammerthrow.org/wp-content/uploads/photosequences/otto_sedykh_wr.pdf|access-date=4 November 2011|quote=The total release velocity is 30.7 m/sec}}</ref> in 1986)<ref>Calculated: 1/2 × 7.26&nbsp;kg × (30.7 m/s){{sup|2}} = 3420{{nbsp}}J</ref>
|-
|3.6×10<sup>3</sup>{{nbsp}}J || ≡ 1&nbsp;W·h ([[watt]]-hour)<ref name=NIST_SI_units/>
|-
|4.2×10<sup>3</sup>{{nbsp}}J || Energy released by explosion of 1 gram of [[trinitrotoluene|TNT]]<ref name=NIST_SI_units/><ref name="ReferenceA">4.2{{e|9}}{{nbsp}}J/ton of TNT-equivalent × (1 ton/1{{e|6}} grams) = 4.2{{e|3}}{{nbsp}}J/gram of TNT-equivalent</ref>
|-
|4.2×10<sup>3</sup>{{nbsp}}J || ≈ 1 food [[Calorie]] (large calorie)
|-
|~7×10<sup>3</sup>{{nbsp}}J || Muzzle energy of an [[elephant gun]], e.g. firing a [[.458 Winchester Magnum]]<ref name="accurate458">{{cite web|title=.458 Winchester Magnum|url=http://www.accuratepowder.com/data/PerCaliber2Guide/Rifle/Standarddata(Rifle)/458Cal(11.63mm)/458%20Winchester%20Magnum%20pages%20339%20and%20340.pdf|work=Accurate Powder|publisher=Western Powders Inc|access-date=7 September 2010|archive-url=https://web.archive.org/web/20070928011847/http://www.accuratepowder.com/data/PerCaliber2Guide/Rifle/Standarddata(Rifle)/458Cal(11.63mm)/458%20Winchester%20Magnum%20pages%20339%20and%20340.pdf|archive-date=28 September 2007|url-status=dead}}</ref>
|-
|8.5×10<sup>3</sup>{{nbsp}}J
|Kinetic energy of a regulation baseball thrown at the speed of sound (343{{nbsp}}m/s = 767{{nbsp}}mph = 1,235{{nbsp}}km/h. Air, 20°C).<ref>{{Cite web |date=2024-01-04 |title=speed of sound - Google Search |url=https://www.google.com/search?q=speed+of+sound#ip=1 |access-date=2024-01-04 |archive-url=https://web.archive.org/web/20240104165125/https://www.google.com/search?q=speed+of+sound#ip=1 |archive-date=4 January 2024 }}</ref>
|-
|9×10<sup>3</sup>{{nbsp}}J || Energy in an alkaline AA battery<ref>{{cite web|title=Battery energy storage in various battery sizes|url=http://www.allaboutbatteries.com/Energy-tables.html|publisher=AllAboutBatteries.com|access-date=15 December 2011|archive-url=https://web.archive.org/web/20111204090808/http://www.allaboutbatteries.com/Energy-tables.html|archive-date=4 December 2011|url-status=dead}}</ref>
|-
|rowspan=4|10<sup>4</sup>
|rowspan=4| &nbsp;
| 1.7×10<sup>4</sup>{{nbsp}}J || Energy released by the [[metabolism]] of 1 gram of [[carbohydrates]]<ref>{{cite web|title=Energy Density of Carbohydrates|url=http://hypertextbook.com/facts/2007/AnuragPanda.shtml|work=The Physics Factbook|access-date=5 November 2011}}</ref> or [[protein]]<ref>{{cite web|title=Energy Density of Protein|url=http://hypertextbook.com/facts/2003/DavidDukhan.shtml|work=The Physics Factbook|access-date=5 November 2011}}</ref>
|-
| 3.8×10<sup>4</sup>{{nbsp}}J || Energy released by the metabolism of 1 gram of [[fat]]<ref>{{cite web|title=Energy Density of Fats|url=http://hypertextbook.com/facts/2004/PingZhang.shtml|work=The Physics Factbook|access-date=5 November 2011}}</ref>
|-
| 4–5×10<sup>4</sup>{{nbsp}}J || Energy released by the [[combustion]] of 1 gram of [[gasoline]]<ref name=gascomb>{{cite web|title=Energy Density of Gasoline|url=http://hypertextbook.com/facts/2003/ArthurGolnik.shtml|work=The Physics Factbook|access-date=5 November 2011}}</ref>
|-
| 5×10<sup>4</sup>{{nbsp}}J || Kinetic energy of 1 gram of matter moving at 10&nbsp;km/s<ref>Calculated:  E = 1/2 m×v{{sup|2}} = 1/2 × (1{{e|-3}} kg) × (1{{e|4}} m/s){{sup|2}} = 5{{e|4}}{{nbsp}}J.</ref>
|-
|rowspan=2|10<sup>5</sup>
|rowspan=2| &nbsp;
| {{nowrap|3×10<sup>5</sup> – 15×10<sup>5</sup>{{nbsp}}J}} || [[Kinetic energy]] of an [[automobile]] at highway speeds (1 to 5 tons<ref name=car_weights>{{cite web|title=List of Car Weights|url=http://cars.lovetoknow.com/List_of_Car_Weights|publisher=LoveToKnow|access-date=13 December 2011|quote=3000 to 12000 pounds}}</ref> at {{nowrap|89 km/h}} or {{nowrap|55 mph}})<ref>Calculated:  Using car weights of 1 ton to 5 tons. E = 1/2 m×v{{sup|2}} = 1/2 × (1{{e|3}} kg) × (55 mph × 1600 m/mi / 3600 s/hr) = 3.0{{e|5}}{{nbsp}}J.  E = 1/2 × (5{{e|3}} kg) × (55 mph × 1600 m/mi / 3600 s/hr) = 15{{e|5}}{{nbsp}}J.</ref>
|-
| 5×10<sup>5</sup>{{nbsp}}J
| Kinetic energy of 1 gram of a [[meteor]] hitting Earth<ref>{{cite web|last=Muller|first=Richard A.|title=Kinetic Energy in a meteor|url=http://muller.lbl.gov/teaching/Physics10/old%20physics%2010/physics%2010%20notes/meteorKE.html|work=Old Physics 10 notes|access-date=13 November 2011|archive-url=https://web.archive.org/web/20120402214238/http://muller.lbl.gov/teaching/Physics10/old%20physics%2010/physics%2010%20notes/meteorKE.html|archive-date=2 April 2012|url-status=dead}}</ref>
|}

==10<sup>6</sup> to 10<sup>11</sup> J==
{| class="wikitable"
|-
| rowspan="6" |10<sup>6</sup>{{Anchor|106}}
| rowspan="6" | [[mega-]] (MJ)
|1×10<sup>6</sup>{{nbsp}}J || [[Kinetic energy]] of a 2 [[tonne]]<ref name=car_weights/> vehicle at 32 metres per second (115&nbsp;km/h or 72&nbsp;mph)<ref>Calculated:  KE = 1/2 × 2{{e|3}} kg × (32 m/s){{sup|2}} = 1.0{{e|6}}{{nbsp}}J</ref>
|-
|1.2×10<sup>6</sup>{{nbsp}}J || Approximate [[food energy]] of a snack such as a [[Snickers bar]] (280 food calories)<ref>{{cite web|url=http://www.nal.usda.gov/fnic/foodcomp/search/ |title=Candies, MARS SNACKFOOD US, SNICKERS Bar (NDB No. 19155) |work=USDA Nutrient Database |publisher=USDA |access-date=14 November 2011 |url-status=dead |archive-url=https://web.archive.org/web/20150303184216/http://www.nal.usda.gov/fnic/foodcomp/search/ |archive-date= 3 March 2015 }}</ref>
|-
|3.6×10<sup>6</sup>{{nbsp}}J || = 1 kWh (kilowatt-hour) (used for electricity)<ref name=NIST_SI_units/>
|-
|4.2×10<sup>6</sup>{{nbsp}}J || Energy released by explosion of 1 kilogram of [[trinitrotoluene|TNT]]<ref name=NIST_SI_units/><ref name="ReferenceA"/>
|-
|8.4×10<sup>6</sup>{{nbsp}}J || Recommended food energy intake per day for a moderately active woman (2000 food calories)<ref name=nih_balance>{{cite web|title=How to Balance the Food You Eat and Your Physical Activity and Prevent Obesity|url=http://www.nhlbi.nih.gov/health/public/heart/obesity/wecan/healthy-weight-basics/balance.htm|work=Healthy Weight Basics|publisher=National Heart Lung and Blood Institutde|access-date=14 November 2011}}</ref><ref>Calculated:  2000 food calories = 2.0{{e|6}} cal × 4.184{{nbsp}}J/cal = 8.4{{e|6}}{{nbsp}}J</ref>
|-
|9.1×10<sup>6</sup>{{nbsp}}J
|Kinetic energy of a regulation baseball thrown at Earth's escape velocity (First cosmic velocity ≈ 11.186&nbsp;km/s  = 25,020&nbsp;mph = 40,270&nbsp;km/h).<ref>{{Cite web |date=2024-01-04 |title=What is Earth's Escape Velocity? - Earth How |url=https://earthhow.com/escape-velocity-earth-closed-system/ |access-date=2024-01-04 |archive-url=https://web.archive.org/web/20240104165536/https://earthhow.com/escape-velocity-earth-closed-system/ |archive-date=4 January 2024 }}</ref>
|-
| rowspan="8" |10<sup>7</sup>
| rowspan="8" |&nbsp;
| 1×10<sup>7</sup>{{nbsp}}J
| Kinetic energy of the armor-piercing round fired by the [[ISU-152]] assault gun<ref>Calculated: 1/2 × m × v{{sup|2}} = 1/2 × 48.78&nbsp;kg × (655 m/s){{sup|2}} = 1.0{{e|7}}{{nbsp}}J.</ref><!-- Need a source for the muzzle velocity and round weight -->{{Citation needed|date=January 2012}}
|-
| 1.1×10<sup>7</sup>{{nbsp}}J || Recommended food energy intake per day for a moderately active man (2600 food calories)<ref name=nih_balance/><ref>Calculated:  2600 food calories = 2.6{{e|6}} cal × 4.184{{nbsp}}J/cal = 1.1{{e|7}}{{nbsp}}J</ref>
|-
| 3.3×10<sup>7</sup>{{nbsp}}J || Kinetic energy of a 23 lb projectile fired by the Navy's mach 8 railgun.<ref>Ackerman, Spencer. “Video: Navy’s Mach 8 Railgun Obliterates Record.” WIRED, 10 Dec. 2010, https://www.wired.com/2010/12/video-navys-mach-8-railgun-obliterates-record</ref>
|-
| 3.7×10<sup>7</sup>{{nbsp}}J
| $1 of electricity at a cost of $0.10/kWh (the US average retail cost in 2009)<ref>{{cite web|title=Table 3.3 Consumer Price Estimates for Energy by Source, 1970–2009|url=http://www.eia.gov/totalenergy/data/annual/showtext.cfm?t=ptb0303|work=Annual Energy Review|publisher=US Energy Information Administration|access-date=17 December 2011|date=19 October 2011|quote=$28.90 per million BTU}}</ref><ref>Calculated J per dollar:  1 million BTU/$28.90 = 1{{e|6}} BTU / 28.90 dollars × 1.055{{e|3}}{{nbsp}}J/BTU  = 3.65{{e|7}}{{nbsp}}J/dollar</ref><ref>Calculated cost per kWh:  1 kWh × 3.60{{e|6}}{{nbsp}}J/kWh / 3.65{{e|7}}{{nbsp}}J/dollar = 0.0986 dollar/kWh</ref>
|-
| 4×10<sup>7</sup>{{nbsp}}J
| Energy from the combustion of 1 cubic meter of [[natural gas]]<ref>{{cite web|title=Energy in a Cubic Meter of Natural Gas|url=http://hypertextbook.com/facts/2002/JanyTran.shtml|work=The Physics Factbook|access-date=15 December 2011}}</ref>
|-
| 4.2×10<sup>7</sup>{{nbsp}}J
| Caloric energy consumed by [[Olympic Games|Olympian]] [[Michael Phelps]] on a daily basis during Olympic training<ref>{{cite web|title=The Olympic Diet of Michael Phelps|url=http://www.webmd.com/diet/news/20080813/the-olympic-diet-of-michael-phelps|work=WebMD|access-date=28 December 2011}}</ref>
|-
| 6.3×10<sup>7</sup>{{nbsp}}J
| Theoretical minimum energy required to accelerate 1&nbsp;kg of matter to [[escape velocity]] from Earth's surface (ignoring atmosphere)<ref>{{cite web|last=Cline|first=James E. D.|title=Energy to Space|url=http://home.earthlink.net/~jedcline/ets.html|access-date=13 November 2011|quote=6.27{{e|7}} Joules / Kg}}</ref>
|-
|9×10<sup>7</sup>{{nbsp}}J
|Total [[Mass–energy equivalence|mass-energy]] of 1 microgram of matter (25 kWh)
|-
|rowspan=4|10<sup>8</sup>
|rowspan=4| &nbsp;
| 1×10<sup>8</sup>{{nbsp}}J || Kinetic energy of a 55 tonne aircraft at typical landing speed (59&nbsp;m/s or 115 knots){{Citation needed|date=November 2011}}
|-
|1.1×10<sup>8</sup>{{nbsp}}J || ≈ 1 [[therm]], depending on the temperature<ref name=NIST_SI_units/>
|-
|1.1×10<sup>8</sup>{{nbsp}}J || ≈ 1 [[Tour de France]], or ~90 hours<ref>{{cite web|title=Tour de France Winners, Podium, Times|url=http://bikeraceinfo.com/tdf/tdfindex.html|publisher=Bike Race Info|access-date=10 December 2011}}</ref> ridden at 5&nbsp;W/kg<ref>{{cite web|title=Watts/kg|url=http://www.flammerouge.je/content/3_factsheets/constant/wattkilobench.htm|publisher=Flamme Rouge|access-date=4 November 2011|archive-url=https://web.archive.org/web/20120102133701/http://www.flammerouge.je/content/3_factsheets/constant/wattkilobench.htm|archive-date=2 January 2012|url-status=dead}}</ref> by a 65&nbsp;kg rider<ref>Calculated:  90 hr × 3600 seconds/hr × 5 W/kg × 65&nbsp;kg = 1.1{{e|8}}{{nbsp}}J</ref>
|-
|7.3×10<sup>8</sup>{{nbsp}}J || ≈ Energy from burning 16 kilograms of oil (using 135&nbsp;kg per barrel of light crude){{Citation needed|date=December 2011}}<!-- 6120 MJ is 1 bboe which is 135 kg light crude of about 0.85 density - therefore 16&nbsp;kg produces 725 MJ -->
|-
| rowspan="12" |10<sup>9</sup>{{Anchor|109}}
| rowspan="12" | [[giga-]] (GJ)
|1–10×10<sup>9</sup>{{nbsp}}J  || Energy in an average [[lightning]] bolt<ref>{{cite web|last=Smith|first=Chris|title=How do Thunderstorms Work?|date=6 March 2007|url=http://www.thenakedscientists.com/HTML/articles/article/howdothunderstormswork-2/|publisher=The Naked Scientists|access-date=15 November 2011|quote=It discharges about 1–10 billion joules of energy}}</ref> (thunder)<!--search hint-->
|-
|1.1×10<sup>9</sup>{{nbsp}}J || Magnetic stored energy in the world's largest toroidal [[superconducting magnet]] for the [[ATLAS experiment]] at [[CERN]], Geneva<ref>{{cite web|title=Powering up ATLAS's mega magnet|url=http://user.web.cern.ch/public/en/Spotlight/SpotlightATLAS-en.html|work=Spotlight on...|publisher=CERN|access-date=10 December 2011|quote=magnetic energy of 1.1 Gigajoules|archive-url=https://web.archive.org/web/20111130024727/http://user.web.cern.ch/public/en/Spotlight/SpotlightATLAS-en.html|archive-date=30 November 2011|url-status=dead}}</ref>
|-
|1.2×10<sup>9</sup>{{nbsp}}J || Inflight 100-ton [[Boeing 757|Boeing 757-200]] at 300 [[knot (unit)|knot]]s (154&nbsp;m/s)
|-
|1.4×10<sup>9</sup>{{nbsp}}J || Theoretical minimum amount of energy required to melt a tonne of steel (380 [[kWh]])<ref>{{cite web|title=ITP Metal Casting: Melting Efficiency Improvement |url=http://www1.eere.energy.gov/industry/metalcasting/pdfs/umr22_fs.pdf|work=ITP Metal Casting|publisher=U.S. Department of Energy|access-date=14 November 2011|quote=377 kWh/mt}}</ref><ref>Calculated: 380 kW-h × 3.6{{e|6}}{{nbsp}}J/kW-h = 1.37{{e|9}}{{nbsp}}J</ref>
|-
|2×10<sup>9</sup>{{nbsp}}J || Energy of an ordinary {{nowrap|61 liter}} gasoline tank of a car.<!-- m = p × V ; Q = (J/m) × m ; mass = density × volume ; energy = energy_density × mass ; 4.5×10^7 × 719.7 × 0.061 = 2.0×10{{sup|9}} --><!-- gasoline J/kg --><ref name=gascomb/><!-- gasoline kg/m<sup>3</sup> --><ref>{{cite web | title = Lead-Free Gasoline Material Safety Data Sheet | author = Bell Fuels | publisher = [[NOAA]] | url = http://www.sefsc.noaa.gov/HTMLdocs/Gasoline.htm | access-date = 6 July 2008 | url-status = dead | archive-url = https://web.archive.org/web/20020820074636/http://www.sefsc.noaa.gov/HTMLdocs/Gasoline.htm | archive-date = 20 August 2002 | df = dmy-all }}</ref><!-- tank volume 0.061 m<sup>3</sup> (Volvo 240) --><ref>[http://www.thepartsbin.com/guides/volvo/fuel_tank.html thepartsbin.com – Volvo Fuel Tank: Compare at The Parts Bin]{{Dead link|date=April 2020 |bot=InternetArchiveBot |fix-attempted=yes }}, 6 May 2012</ref>
|-
|2×10<sup>9</sup>{{nbsp}}J || The unit of energy in [[Planck units]]<ref><math>E_\text{P} = \sqrt{\frac{\hbar c^5}{G}} </math></ref>
|-
|3×10<sup>9</sup>{{nbsp}}J || Inflight 125-ton [[Boeing 767|Boeing 767-200]] flying at 373 [[knot (unit)|knot]]s (192&nbsp;m/s)
|-
|3.3×10<sup>9</sup>{{nbsp}}J || Approximate average amount of energy expended by a human heart [[muscle]] over an 80-year lifetime<ref>{{cite web|title=Power of a Human Heart|url=http://hypertextbook.com/facts/2003/IradaMuslumova.shtml|work=The Physics Factbook|access-date=10 December 2011|quote=The mechanical power of the human heart is ~1.3 watts}}</ref><ref>Calculated:  1.3{{nbsp}}J/s × 80 years × 3.16{{e|7}} s/year = 3.3{{e|9}}{{nbsp}}J</ref>
|-
|3.6×10<sup>9</sup>{{nbsp}}J
|= 1 MW·h (megawatt-hour)
|-
|4.2×10<sup>9</sup>{{nbsp}}J || Energy released by explosion of 1 [[TNT equivalent|ton of TNT]].
|-
|4.5×10<sup>9</sup>{{nbsp}}J || Average annual energy usage of a standard [[refrigerator]]<ref>{{cite web|title=U.S. Household Electricity Uses: A/C, Heating, Appliances|url=http://www.eia.gov/emeu/reps/enduse/er01_us.html|work=U.S. HOUSEHOLD ELECTRICITY REPORT|publisher=EIA|access-date=13 December 2011|quote=For refrigerators in 2001, the average UEC was 1,239 kWh}}</ref><ref>Calculated:  1239 kWh × 3.6{{e|6}}{{nbsp}}J/kWh = 4.5{{e|9}}{{nbsp}}J</ref>
|-
|6.1×10<sup>9</sup>{{nbsp}}J || ≈ 1 bboe ([[barrel of oil equivalent]])<ref name="oe">'''[http://www.altenergyaction.org/mambo/index.php?option=com_content&task=view&id=9 Energy Units]''', by Arthur Smith, 21 January 2005</ref>
|-
| rowspan="7" |10<sup>10</sup>
| rowspan="7" | &nbsp;
|1.9×10<sup>10</sup>{{nbsp}}J || Kinetic energy of an [[Airbus A380]] at cruising speed (560 tonnes at 511 knots or 263&nbsp;m/s)
|-
|4.2×10<sup>10</sup>{{nbsp}}J || ≈ 1 toe ([[ton of oil equivalent]])<ref name="oe"/>
|-
|4.6×10<sup>10</sup>{{nbsp}}J || Yield energy of a [[Massive Ordnance Air Blast]] bomb, the second most powerful non-nuclear weapon ever designed<ref>{{cite web|title=Top 10 Biggest Explosions|url=http://listverse.com/2011/11/28/top-10-biggest-explosions/|publisher=Listverse|access-date=10 December 2011|quote=a yield of 11 tons of TNT|date=28 November 2011}}</ref><ref>Calculated:  11 tons of TNT-equivalent × 4.184{{e|9}}{{nbsp}}J/ton of TNT-equivalent = 4.6{{e|10}}{{nbsp}}J</ref>
|-
|7.3×10<sup>10</sup>{{nbsp}}J || Energy consumed by the average U.S. automobile in the year 2000<ref>{{cite web|title=Emission Facts: Average Annual Emissions and Fuel Consumption for Passenger Cars and Light Trucks |url=http://www.epa.gov/otaq/consumer/f00013.htm|publisher=EPA|access-date=12 December 2011|quote=581 gallons of gasoline}}</ref><ref>{{cite web|title=200 Mile-Per-Gallon Cars?|url=http://www.uwgb.edu/dutchs/pseudosc/200mpgcar.htm|access-date=12 December 2011|quote=a gallon of gas ... 125 million joules of energy|archive-url=https://web.archive.org/web/20111219011152/http://www.uwgb.edu/dutchs/pseudosc/200mpgcar.htm|archive-date=19 December 2011|url-status=dead}}</ref><ref>Calculated:  581 gallons × 125{{e|6}}{{nbsp}}J/gal = 7.26{{e|10}}{{nbsp}}J</ref>
|-
|8.6×10<sup>10</sup>{{nbsp}}J || ≈ 1 MW·d ([[megawatt]]-day), used in the context of power plants (24 MW·h)<ref>Calculated:  1{{e|6}} watts × 86400 seconds/day = 8.6{{e|10}}{{nbsp}}J</ref>
|-
|8.8×10<sup>10</sup>{{nbsp}}J || Total energy [[nuclear explosions|released]] in the [[nuclear fission]] of one gram of [[uranium-235]]<ref name="Energy From Uranium Fission"/><ref name="Conversion from eV to J"/><ref>Calculated:  3.44{{e|-10}}{{nbsp}}J/U-235-fission × 1{{e|-3}} kg / (235 amu per U-235-fission × 1.66{{e|-27}} amu/kg) = 8.82{{e|-10}}{{nbsp}}J</ref>
|-
|9×10<sup>10</sup>{{nbsp}}J
|Total mass-energy of 1 milligram of matter (25 MW·h)
|-
| rowspan="2" |10<sup>11</sup>
| rowspan="2" |&nbsp;
|1.1×10<sup>11</sup>{{nbsp}}J
|Kinetic energy of a regulation baseball thrown at lightning speed (120&nbsp;km/s = 270,000&nbsp;mph = 435,000&nbsp;km/h).<ref>{{Cite web |date=2024-01-04 |title=10 striking facts about lightning - Met Office |url=https://www.metoffice.gov.uk/weather/learn-about/weather/types-of-weather/thunder-and-lightning/facts-about-lightning |access-date=2024-01-04 |archive-url=https://web.archive.org/web/20240104170325/https://www.metoffice.gov.uk/weather/learn-about/weather/types-of-weather/thunder-and-lightning/facts-about-lightning |archive-date=4 January 2024 }}</ref>
|-
| 2.4×10<sup>11</sup>{{nbsp}}J || Approximate food energy consumed by an average human in an 80-year lifetime.<ref>Calculated:  2000 kcal/day × 365 days/year × 80 years = 2.4{{e|11}}{{nbsp}}J</ref>
|}

==10<sup>12</sup> to 10<sup>17</sup> J==
{| class="wikitable"
|-
|rowspan=5|10<sup>12</sup>{{Anchor|1012}}
|rowspan=5| [[tera-]] (TJ)
|3.4×10<sup>12</sup>{{nbsp}}J
| Maximum fuel energy of an [[Airbus A330]]-300 (97,530 liters<ref>{{cite web|title=A330-300 Dimensions & key data|url=http://www.airbus.com/aircraftfamilies/passengeraircraft/a330family/a330-300/specifications/|publisher=Airbus|access-date=12 December 2011|quote=97530 litres|archive-date=16 January 2013|archive-url=https://web.archive.org/web/20130116222250/http://www.airbus.com/aircraftfamilies/passengeraircraft/a330family/a330-300/specifications/|url-status=dead}}</ref> of [[Jet A-1]]<ref name=bp_jet_a1>{{cite web|url=http://www.bp.com/liveassets/bp_internet/aviation/air_bp/STAGING/local_assets/downloads_pdfs/a/air_bp_products_handbook_04004_1.pdf |title=Archived copy |access-date=19 August 2011 |url-status=dead |archive-url=https://web.archive.org/web/20110608075828/http://www.bp.com/liveassets/bp_internet/aviation/air_bp/STAGING/local_assets/downloads_pdfs/a/air_bp_products_handbook_04004_1.pdf |archive-date= 8 June 2011 }}</ref>)<ref>Calculated: 97530 liters × 0.804&nbsp;kg/L × 43.15&nbsp;MJ/kg = 3.38{{e|12}}{{nbsp}}J</ref>
|-
|3.6×10<sup>12</sup>{{nbsp}}J
| 1 GW·h ([[gigawatt]]-hour)<ref>Calculated: 1{{e|9}} watts × 3600 seconds/hour</ref>
|-
|4×10<sup>12</sup>{{nbsp}}J
| Electricity generated by one 20-kg [[CANDU]] fuel bundle assuming ~29%<ref>{{cite web|last=Weston|first=Kenneth|title=Chapter 10. Nuclear Power Plants|url=http://www.personal.utulsa.edu/~kenneth-weston/chapter10.pdf|work=Energy Conversion|access-date=13 December 2011|quote=The thermal efficiency of a CANDU plant is only about 29%|archive-date=5 October 2011|archive-url=https://web.archive.org/web/20111005120238/http://www.personal.utulsa.edu/~kenneth-weston/chapter10.pdf|url-status=dead}}</ref> thermal efficiency of reactor<ref>{{cite web|title=CANDU and Heavy Water Moderated Reactors|url=http://www.nucleartourist.com/type/candu.htm|access-date=12 December 2011|quote=fuel burnup in a CANDU is only 6500 to 7500 MWd per metric ton uranium}}</ref><ref>Calculated:  7500{{e|6}} watt-days/tonne × (0.020 tonnes per bundle) × 86400 seconds/day = 1.3{{e|13}}{{nbsp}}J of burnup energy. Electricity = burnup × ~29% efficiency = 3.8{{e|12}}{{nbsp}}J</ref>
<!--
|-
|3.7×10<sup>12</sup>{{nbsp}}J
| Average orbital kinetic energy of the [[Mir]] space station (124 tonnes{{Citation needed|date=December 2011}} at about 7680 m/s{{Citation needed|date=December 2011}})<ref>Calculated: E = 1/2 m.v<sup>2</sup> = 1/2 × 124000 kg × (7680m/s)<sup>2</sup> = 3.66{{e|12}}{{nbsp}}J</ref>
-->
|-
|4.2×10<sup>12</sup>{{nbsp}}J
| Energy released by explosion of 1 [[TNT equivalent|kiloton of TNT]]<ref name=NIST_SI_units/><ref>Calculated:  4.2{{e|9}}{{nbsp}}J/ton of TNT-equivalent × 1{{e|3}} tons/megaton = 4.2{{e|12}}{{nbsp}}J/megaton of TNT-equivalent</ref>
|-
|6.4×10<sup>12</sup>{{nbsp}}J || Energy contained in jet fuel in a [[Boeing 747]]-100B aircraft at max fuel capacity (183,380 liters<ref>{{cite web|title=747 Classics Technical Specs |url=http://www.boeing.com/commercial/747family/pf/pf_classics.html |publisher=Boeing |access-date=12 December 2011 |quote=183,380 L |url-status=dead |archive-url=https://web.archive.org/web/20071210173616/http://www.boeing.com/commercial/747family/pf/pf_classics.html |archive-date=10 December 2007 }}</ref> of [[Jet A-1]]<ref name=bp_jet_a1/>)<ref>Calculated: 183380 liters × 0.804&nbsp;kg/L × 43.15&nbsp;MJ/kg = 6.36{{e|12}}{{nbsp}}J</ref>
|-
|rowspan=4|10<sup>13</sup>
|rowspan=4| &nbsp;
|1.1×10<sup>13</sup>{{nbsp}}J || Energy of the maximum fuel an [[Airbus A380]] can carry (320,000 liters<ref>{{cite web|title=A380-800 Dimensions & key data|url=http://www.airbus.com/aircraftfamilies/passengeraircraft/a380family/a380-800/specifications/|publisher=Airbus|access-date=12 December 2011|quote=320,000 L|archive-date=8 July 2012|archive-url=https://web.archive.org/web/20120708071501/http://www.airbus.com/aircraftfamilies/passengeraircraft/a380family/a380-800/specifications/|url-status=dead}}</ref> of [[Jet A-1]]<ref name=bp_jet_a1/>)<ref>Calculated: 320,000 L × 0.804 kg/L × 43.15 &nbsp;MJ/kg = 11.1{{e|12}}{{nbsp}}J</ref>
|-
|1.2×10<sup>13</sup>{{nbsp}}J || Orbital kinetic energy of the [[International Space Station]] (417 tonnes<ref>{{cite web |url=http://www.nasa.gov/mission_pages/station/structure/isstodate.html |title=International Space Station: The ISS to Date |publisher=NASA |access-date=23 August 2011 |archive-date=11 June 2015 |archive-url=https://web.archive.org/web/20150611163133/http://www.nasa.gov/mission_pages/station/structure/isstodate.html |url-status=dead }}</ref> at 7.7&nbsp;km/s<ref>{{cite web|title=The wizards of orbits|url=http://www.esa.int/esaCP/ESA104MBAMC_FeatureWeek_0.html|publisher=European Space Agency|access-date=10 December 2011|quote=The International Space Station, for example, flies at 7.7&nbsp;km/s in one of the lowest practicable orbits}}</ref>)<ref>Calculated: E = 1/2 m.v<sup>2</sup> = 1/2 × 417000 kg × (7700m/s)<sup>2</sup> = 1.2{{e|13}}{{nbsp}}J</ref>
|-
|6.3×10<sup>13</sup>{{nbsp}}J || Yield of the [[Little Boy]] atomic bomb dropped on [[Hiroshima]] in [[World War II]] (15 kilotons)<ref>{{cite web|title=What was the yield of the Hiroshima bomb?|url=http://www.warbirdforum.com/hiroshim.htm|publisher=Warbird's Forum|quote=21 kt|access-date=4 November 2011}}</ref><ref>Calculated:  15 kt = 15{{e|9}} grams of TNT-equivalent × 4.2{{e|3}}{{nbsp}}J/gram TNT-equivalent = 6.3{{e|13}}{{nbsp}}J</ref>
|-
|9×10<sup>13</sup>{{nbsp}}J || Theoretical total [[mass–energy]] of 1 gram of matter (25 GW·h) <ref>{{cite web|title=Conversion from kg to{{nbsp}}J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=-3&num=1&From=kg&To=j&Action=Convert+value+and+show+factor|publisher=NIST|access-date=4 November 2011}}</ref>
|-
| rowspan="3" |10<sup>14</sup>
| rowspan="3" |&nbsp;
|1.8×10<sup>14</sup>{{nbsp}}J
|Energy released by annihilation of 1 gram of [[antimatter]] and matter (50 GW·h)
|-
| 3.75×10<sup>14</sup>{{nbsp}}J || Total energy released by the [[Chelyabinsk meteor]].<ref name="chelyabinsk">{{cite web|title=JPL – Fireballs and bolides|url=https://cneos.jpl.nasa.gov/fireballs/|website=Jet Propulsion Laboratory|publisher=NASA|access-date=13 April 2017}}</ref>
|-
| 6×10<sup>14</sup>{{nbsp}}J || Energy released by an average [[hurricane]] in 1 second<ref name="noaa">{{cite web|title=How much energy does a hurricane release?|url=http://www.aoml.noaa.gov/hrd/tcfaq/D7.html|work=FAQ : HURRICANES, TYPHOONS, AND TROPICAL CYCLONES|publisher=NOAA|access-date=12 November 2011}}</ref>
|-
|rowspan=3| 10<sup>15</sup>
|rowspan=3| [[peta-]] (PJ) {{anchor|1015}}
|> 10<sup>15</sup>{{nbsp}}J || Energy released by a severe [[thunderstorm]]<ref>{{cite web|title=The Gathering Storms|url=http://www.cosmosmagazine.com/node/3302/full|publisher=COSMOS|access-date=10 December 2011|archive-url=https://web.archive.org/web/20120404113209/http://www.cosmosmagazine.com/node/3302/full|archive-date=4 April 2012|url-status=dead}}</ref>
|-
|1×10<sup>15</sup>{{nbsp}}J || Yearly [[electricity]] consumption in [[Greenland]] as of 2008<ref name="CIA_electricity_consumption">{{cite web|title=Country Comparison :: Electricity – consumption |url=https://www.cia.gov/library/publications/the-world-factbook/rankorder/2042rank.html |work=The World Factbook |publisher=CIA |access-date=11 December 2011 |url-status=dead |archive-url=https://web.archive.org/web/20120128032332/https://www.cia.gov/library/publications/the-world-factbook/rankorder/2042rank.html |archive-date=28 January 2012 }}</ref><ref>Calculated:  288.6{{e|6}} kWh × 3.60{{e|6}}{{nbsp}}J/kWh = 1.04{{e|15}}{{nbsp}}J</ref>
|-
|4.2×10<sup>15</sup>{{nbsp}}J || Energy released by explosion of 1 [[TNT equivalent|megaton of TNT]]<ref name=NIST_SI_units/><ref>Calculated:  4.2{{e|9}}{{nbsp}}J/ton of TNT-equivalent × 1{{e|6}} tons/megaton = 4.2{{e|15}}{{nbsp}}J/megaton of TNT-equivalent</ref>
|-
| rowspan="5" | 10<sup>16</sup>
| rowspan="5" | &nbsp;
| 1×10<sup>16</sup>{{nbsp}}J || Estimated impact energy released in forming [[Meteor Crater]]{{Citation needed|date=November 2011}}
|-
| 1.1×10<sup>16</sup>{{nbsp}}J || Yearly [[electricity consumption]] in [[Mongolia]] as of 2010<ref name="CIA_electricity_consumption"/><ref>Calculated:  3.02{{e|9}} kWh × 3.60{{e|6}}{{nbsp}}J/kWh = 1.09{{e|16}}{{nbsp}}J</ref>
|-
|6.3×10<sup>16</sup>{{nbsp}}J
|Yield of [[Castle Bravo]], the most powerful nuclear weapon tested by the United States<ref>{{Cite web |date=2024-01-04 |title=Castle Bravo: The Largest U.S. Nuclear Explosion {{!}} Brookings |url=https://www.brookings.edu/articles/castle-bravo-the-largest-u-s-nuclear-explosion/ |access-date=2024-01-04 |archive-url=https://web.archive.org/web/20240104171317/https://www.brookings.edu/articles/castle-bravo-the-largest-u-s-nuclear-explosion/ |archive-date=4 January 2024 }}</ref>
|-
|7.9×10<sup>16</sup>{{nbsp}}J
|Kinetic energy of a regulation baseball thrown at 99% the speed of light (KE = ''m''c^2 × [γ-1], where the Lorentz factor γ ≈ 7.09).<ref>{{Cite web |title=0.145kg*c^2*(1/sqrt(1-0.99^2)-1) - Wolfram{{!}}Alpha |url=https://www.wolframalpha.com/ |access-date=2024-01-04 |website=www.wolframalpha.com |language=en}}</ref>
|-
| 9×10<sup>16</sup>{{nbsp}}J || [[Mass–energy]] of 1 kilogram of [[antimatter]] (or matter)<ref>Calculated:  E = mc{{sup|2}} = 1&nbsp;kg × (2.998{{e|8}} m/s){{sup|2}} = 8.99{{e|16}}{{nbsp}}J</ref>
|-
|rowspan=6| 10<sup>17</sup>
|rowspan=6| &nbsp;
|1×10<sup>17</sup>{{nbsp}}J || Energy released on the Earth's surface by the magnitude 9.1–9.3 [[2004 Indian Ocean earthquake and tsunami|2004 Indian Ocean earthquake]]<ref>{{cite web|url=http://neic.usgs.gov/neis/eq_depot/2004/eq_041226/neic_slav_e.html |title=USGS Energy and Broadband Solution |publisher=National Earthquake Information Center, US Geological Survey |access-date=9 December 2011 |url-status=dead |archive-url=https://web.archive.org/web/20100404013939/http://neic.usgs.gov/neis/eq_depot/2004/eq_041226/neic_slav_e.html |archive-date=4 April 2010 }}</ref>
|-
|1.7×10<sup>17</sup>{{nbsp}}J || Total energy from the [[Sun]] that strikes the face of the [[Earth]] each second<ref name="sun1">The Earth has a [[Cross section (geometry)|cross section]] of 1.274×10<sup>14</sup> [[Square meter|square meters]] and the [[solar constant]] is 1361 [[Watt|watts]] per square meter. Note, however, that because portions of Earth reflect light well, the actual energy absorbed is about 1.2*10^17 watts, from an average albedo of 0.3.</ref>
|-
|2.1×10<sup>17</sup>{{nbsp}}J || Yield of the [[Tsar Bomba]], the most powerful [[nuclear weapon]] ever tested (50 megatons)<ref>{{cite web|title=The Soviet Weapons Program – The Tsar Bomba|url=http://www.nuclearweaponarchive.org/Russia/TsarBomba.html|publisher=The Nuclear Weapon Archive|access-date=4 November 2011}}</ref><ref>Calculated:  50{{e|6}} tons TNT-equivalent × 4.2{{e|9}}{{nbsp}}J/ton TNT-equivalent = 2.1{{e|17}}{{nbsp}}J</ref>
|-
|4.2×10<sup>17</sup>{{nbsp}}J || Yearly [[electricity consumption]] of [[Norway]] as of 2008<ref name="CIA_electricity_consumption"/><ref>Calculated:  115.6{{e|9}} kWh × 3.60{{e|6}}{{nbsp}}J/kWh = 4.16{{e|17}}{{nbsp}}J</ref>
|-
|4.5×10<sup>17</sup>{{nbsp}}J || Approximate energy needed to accelerate one ton to one-tenth of the speed of light<!-- energy = 0.5×mass×speed<sup>2</sup> = 0.5 × 1000 × (c/10){{sup|2}} -->
|-
|8×10<sup>17</sup>{{nbsp}}J || Estimated energy released by the eruption of the [[1883 eruption of Krakatoa|Indonesian volcano, Krakatoa, in 1883]]<ref>{{cite book|last=Alexander|first=R. McNeill|title=Dynamics of Dinosaurs and Other Extinct Giants|year=1989|publisher=Columbia University Press|isbn=978-0-231-06667-9|url=https://books.google.com/books?id=0q_1xk3SVKEC|page=144|quote=the explosion of the island volcano Krakatoa in 1883, had about 200 megatonnes energy.}}</ref><ref>Calculated:  200{{e|6}} tons of TNT equivalent × 4.2{{e|9}}{{nbsp}}J/ton of TNT equivalent = 8.4{{e|17}}{{nbsp}}J</ref><ref>This value appears to be referred only to the third explosion on 27th August, 10.02 a.m.

According to reports, the third explosion was by far the largest; it is associated to the biggest sound in the recorded history, the highest tsunami during the eruption and the most powerful shock waves rounded the world several times. 200 Megatons of TNT are often referred as the total energy released by the entire eruption, but it's plausible that are rather the energy released by the single third explosion, considering the effects.[http://www.branchcollective.org/?ps_articles=monique-morgan-the-eruption-of-krakatoa-also-known-as-krakatau-in-1883][https://archive.org/details/eruptionkrakato00whipgoog/page/n12/mode/2up?view=theater]</ref>
|}

==10<sup>18</sup> to 10<sup>23</sup> J==
{| class="wikitable"
|-
|rowspan=1| 10<sup>18</sup>{{Anchor|1018}}
|rowspan=1| [[exa-]] (EJ)
|1.4×10<sup>18</sup>{{nbsp}}J || Yearly [[electricity consumption]] of [[South Korea]] as of 2009<ref name="CIA_electricity_consumption"/><ref>Calculated:  402{{e|9}} kWh × 3.60{{e|6}}{{nbsp}}J/kWh = 1.45{{e|17}}{{nbsp}}J</ref>
|-
| rowspan="6" |10<sup>19</sup>
| rowspan="6" |&nbsp;
|1.2×10<sup>19</sup>{{nbsp}}J
|Explosive yield of global nuclear arsenal<ref>{{Cite web|last=Mizokami|first=Kyle|date=2019-04-01|title=Here's What Would Happen If We Blew Up All the World's Nukes at Once|url=https://www.popularmechanics.com/military/weapons/a27008390/blow-up-every-nuke/|access-date=2021-04-08|website=Popular Mechanics|language=en-US}}</ref> (2.86 Gigatons)
|-
|1.4×10<sup>19</sup>{{nbsp}}J || Yearly [[electricity consumption]] in the [[United States|U.S.]] as of 2009<ref name="CIA_electricity_consumption" /><ref>Calculated:  3.741{{e|12}} kWh × 3.600{{e|6}}{{nbsp}}J/kWh = 1.347{{e|19}}{{nbsp}}J</ref>
|-
|1.4×10<sup>19</sup>J || Yearly [[electricity production]] in the [[United States|U.S.]] as of 2009<ref name=CIA_us>{{cite web|title=United States|url=https://www.cia.gov/the-world-factbook/countries/united-states/|work=The World Factbook|publisher=USA|access-date=11 December 2011}}</ref><ref>Calculated:  3.953{{e|12}} kWh × 3.600{{e|6}}{{nbsp}}J/kWh = 1.423{{e|19}}{{nbsp}}J</ref>
|-
|5×10<sup>19</sup>{{nbsp}}J || Energy released in 1 day by an average [[hurricane]] in producing rain (400 times greater than the wind energy)<ref name="noaa"/>
|-
|6.4×10<sup>19</sup>{{nbsp}}J || Yearly [[electricity consumption]] of the world {{As of|2008|lc=on}}<ref name=CIA_world>{{cite web|title=World|url=https://www.cia.gov/the-world-factbook/countries/world/|work=The World Factbook|publisher=CIA|access-date=11 December 2011}}</ref><ref>Calculated:  17.8{{e|12}} kWh × 3.60{{e|6}}{{nbsp}}J/kWh = 6.41{{e|19}}{{nbsp}}J</ref>
|-
|6.8×10<sup>19</sup>{{nbsp}}J || Yearly electricity generation of the world {{As of|2008|lc=on}}<ref name=CIA_world/><ref>Calculated:  18.95{{e|12}} kWh × 3.60{{e|6}}{{nbsp}}J/kWh = 6.82{{e|19}}{{nbsp}}J</ref>
<!--
|-
|6.7×10<sup>19</sup>{{nbsp}}J || Total energy released by the magnitude 8.8 [[2010 Chile earthquake]]{{Citation needed|date=November 2011}}
-->
|-
|rowspan=2| 10<sup>20</sup>
|rowspan=2| &nbsp;
|5×10<sup>20</sup>{{nbsp}}J || [[World energy resources and consumption|Total world annual energy consumption]] in 2010<ref name=BP_Statistical_Review_2011>{{cite web|title=Statistical Review of World Energy 2011 |url=http://www.bp.com/assets/bp_internet/globalbp/globalbp_uk_english/reports_and_publications/statistical_energy_review_2011/STAGING/local_assets/pdf/statistical_review_of_world_energy_full_report_2011.pdf |publisher=BP |access-date=9 December 2011 |url-status=dead |archive-url=https://web.archive.org/web/20110902033116/http://www.bp.com/assets/bp_internet/globalbp/globalbp_uk_english/reports_and_publications/statistical_energy_review_2011/STAGING/local_assets/pdf/statistical_review_of_world_energy_full_report_2011.pdf |archive-date= 2 September 2011 }}</ref><ref>Calculated:  12002.4{{e|6}} tonnes of oil equivalent × 42{{e|9}}{{nbsp}}J/tonne of oil equivalent = 5.0{{e|20}}{{nbsp}}J</ref>
|-
|8×10<sup>20</sup>{{nbsp}}J || Estimated global [[uranium]] resources for generating electricity 2005<ref name=iaea>{{cite web|url=http://www.iaea.org/NewsCenter/News/2006/uranium_resources.html|publisher=iaea.org|title=Global Uranium Resources to Meet Projected Demand {{pipe}} International Atomic Energy Agency|access-date=26 December 2016|date=June 2006}}</ref><ref>{{cite web|url=http://www.eia.doe.gov/pub/international/iealf/table63.xls|title=U.S. Energy Information Administration, International Energy Generation}}</ref><ref name="doe">{{cite web|url=http://www.eia.doe.gov/oiaf/ieo/electricity.html|publisher=eia.doe.gov|title=U.S. EIA International Energy Outlook 2007. |access-date=26 December 2016}}</ref><ref>Final number is computed. Energy Outlook 2007 shows 15.9% of world energy is nuclear. IAEA estimates conventional uranium stock, at today's prices is sufficient for 85 years. Convert billion kilowatt-hours to joules then:  6.25×10<sup>19</sup>×0.159×85&nbsp;= 8.01×10<sup>20</sup>.</ref>
|-
|rowspan=3| 10<sup>21</sup>
|rowspan=3| [[zetta-]] (ZJ) {{anchor|1021}}
|6.9×10<sup>21</sup>{{nbsp}}J || Estimated energy contained in the world's [[natural gas]] [[Mineral resource classification#Mineral reserves|reserves]] as of 2010<ref name=BP_Statistical_Review_2011 /><ref>Calculated:  "6608.9 trillion cubic feet" => 6608.9{{e|3}} billion cubic feet × 0.025 million tonnes of oil equivalent/billion cubic feet × 1{{e|6}} tonnes of oil equivalent/million tonnes of oil equivalent × 42{{e|9}}{{nbsp}}J/tonne of oil equivalent = 6.9{{e|21}}{{nbsp}}J</ref>
|-
|7.9×10<sup>21</sup>{{nbsp}}J || Estimated energy contained in the world's [[petroleum]] reserves as of 2010<ref name=BP_Statistical_Review_2011 /><ref>Calculated: "188.8 thousand million tonnes" => 188.8{{e|9}} tonnes of oil × 42{{e|9}}{{nbsp}}J/tonne of oil = 7.9{{e|21}}{{nbsp}}J</ref>
|-
|9.3×10<sup>21</sup>{{nbsp}}J || Annual [[ocean heat content|net uptake of thermal energy by the global ocean]] during 2003-2018<ref>{{Cite journal |last1=Cheng |first1=Lijing |last2=Foster |first2=Grant |last3=Hausfather |first3=Zeke |last4=Trenberth |first4=Kevin E. |last5=Abraham |first5=John |date=2022 |title=Improved Quantification of the Rate of Ocean Warming |journal=Journal of Climate |volume=35 |issue=14 |pages=4827–4840 |doi=10.1175/JCLI-D-21-0895.1 |bibcode=2022JCli...35.4827C |doi-access=free}}Calculated per reference: 0.58{{nbsp}}W·m<sup>−2</sup> is 9.3{{e|21}}{{nbsp}}J·yr<sup>−1</sup> in the global domain</ref>
|-
| rowspan="4" | 10<sup>22</sup>
| rowspan="4" | &nbsp;
|1.5×10<sup>22</sup>J || Total energy from the Sun that strikes the face of the Earth each day<ref name="sun1"/><ref>Calculated:  1.27{{e|14}} m{{sup|2}} × 1370 W/m{{sup|2}} × 86400 s/day = 1.5{{e|22}}{{nbsp}}J</ref>
|-
|2.4×10<sup>22</sup>{{nbsp}}J || Estimated energy contained in the world's [[coal]] reserves as of 2010<ref name=BP_Statistical_Review_2011 /><ref>Calculated:  860938 million tonnes of coal => 860938{{e|6}} tonnes of coal × (1/1.5 tonne of oil equivalent / tonne of coal) × 42{{e|9}}{{nbsp}}J/tonne of oil equivalent = 2.4{{e|22}}{{nbsp}}J</ref>
|-
|2.9×10<sup>22</sup>{{nbsp}}J || Identified global [[uranium-238]] resources using [[Fast-neutron reactor|fast reactor]] technology<ref name=iaea/>
|-
|3.9×10<sup>22</sup>{{nbsp}}J || Estimated energy contained in the world's [[fossil fuel]] reserves as of 2010<ref name=BP_Statistical_Review_2011 /><ref>Calculated:  natural gas + petroleum + coal = 6.9{{e|21}}{{nbsp}}J + 7.9{{e|21}}{{nbsp}}J + 2.4{{e|22}}{{nbsp}}J = 3.9{{e|22}}{{nbsp}}J</ref>
|-
| rowspan="2" |10<sup>23</sup>
| rowspan="2" |&nbsp;
|2.2×10<sup>23</sup>{{nbsp}}J || Total global [[uranium-238]] resources using fast reactor technology<ref name="iaea" />
|-
|3×10<sup>23</sup>{{nbsp}}J || The energy released in the formation of the [[Chicxulub Crater]] in the [[Yucatán Peninsula]]<ref name="Richards">{{Cite journal |last1=Richards |first1=Mark A. |last2=Alvarez |first2=Walter |last3=Self |first3=Stephen |last4=Karlstrom |first4=Leif |last5=Renne |first5=Paul R. |last6=Manga |first6=Michael |last7=Sprain |first7=Courtney J. |last8=Smit |first8=Jan |last9=Vanderkluysen |first9=Loÿc |last10=Gibson |first10=Sally A. |date=2015-11-01 |title=Triggering of the largest Deccan eruptions by the Chicxulub impact |url=https://doi.org/10.1130/B31167.1 |journal=[[Geological Society of America Bulletin]] |volume=127 |issue=11–12 |pages=1507–1520 |doi=10.1130/B31167.1 |bibcode=2015GSAB..127.1507R |s2cid=3463018 |issn=0016-7606}}</ref>
|}

==Over 10<sup>23</sup> J==
{{Anchor|1024 and above}}
{| class="wikitable"
|-
| 10<sup>24</sup> || [[yotta-]] (YJ) || 5.5×10<sup>24</sup>{{nbsp}}J || Total energy from the [[Sun]] that strikes the face of the [[Earth]] each year<ref name="sun1"/><ref>Calculated:  1.27{{e|14}} m{{sup|2}} × 1370 W/m{{sup|2}} × 86400 s/day = 5.5{{e|24}}{{nbsp}}J</ref>
|-
| 10<sup>25</sup> || &nbsp; || 6×10<sup>25</sup>{{nbsp}}J || Upper limit of energy released by a [[solar flare]]<ref>{{cite book |last1=Carroll |first1=Bradley |last2=Ostlie |first2=Dale |date=2017 |title=An Introduction to Modern Astrophysics |publisher=Cambridge University Press |edition=2 |isbn=978-1-108-42216-1}}</ref>
|-
| rowspan=2 | 10<sup>26</sup>
| rowspan=2 | &nbsp;
| >10<sup>26</sup>J || Estimated energy of early [[Archean]] [[asteroid impact]]s<ref>{{Cite journal|url=https://ntrs.nasa.gov/citations/20180006692|title = Climatic Effect of Impacts on the Ocean|date = 26 August 2018|bibcode = 2018LPICo2065.2056Z|last1 = Zahnle|first1 = K. J.|journal = Comparative Climatology of Terrestrial Planets III: From Stars to Surfaces|volume = 2065|page = 2056}}</ref>
|-
| 3.828×10<sup>26</sup>{{nbsp}}J || Total radiative energy output of the [[Sun]] each second<ref name=sun2>{{cite web|title=Ask Us: Sun: Amount of Energy the Earth Gets from the Sun|url=http://helios.gsfc.nasa.gov/qa_sun.html#sunenergymass|archive-url=https://web.archive.org/web/20000816180724/http://helios.gsfc.nasa.gov/qa_sun.html#sunenergymass|url-status=dead|archive-date=16 August 2000|work=Cosmicopia|publisher=NASA|access-date=4 November 2011}}</ref>
|-
| rowspan="3" | 10<sup>27</sup> || rowspan="3" | [[ronna-]] (RJ) || 1×10<sup>27</sup>{{nbsp}}J ||  Estimated energy released by the impact that created the [[Caloris basin]] on [[Mercury (planet)|Mercury]]<ref>{{cite web|last1=Lii|first1=Jiangning|title=Seismic effects of the Caloris basin impact, Mercury|url=https://dspace.mit.edu/bitstream/handle/1721.1/69472/775585855-MIT.pdf?sequence=2|website=MIT}}</ref>
|-
|~3×10<sup>27</sup>{{nbsp}}J
|Estimated energy required to evaporate all water on the surface of Earth
|-
|4.2×10<sup>27</sup>{{nbsp}}J
|Kinetic energy of a regulation baseball thrown at the speed of the [[Oh-My-God particle]], itself a cosmic ray proton with the kinetic energy of a baseball thrown at 60{{nbsp}}mph (~50{{nbsp}}J).<ref>{{Cite web |title=0.145kg*c^2*(1/sqrt(1-0.9999999999999999999999951^2)-1) - Wolfram{{!}}Alpha |url=https://www.wolframalpha.com/ |access-date=2024-01-04 |website=www.wolframalpha.com |language=en}}</ref>
|-
| 10<sup>28</sup> || &nbsp; || 3.8×10<sup>28</sup>{{nbsp}}J || Kinetic energy of the [[Moon]] in its [[Orbit of the Moon|orbit]] around the Earth (counting only its velocity relative to the Earth)<ref>{{cite web | url= http://nssdc.gsfc.nasa.gov/planetary/factsheet/moonfact.html | title= Moon Fact Sheet | publisher=NASA | access-date=16 December 2011 }}</ref><ref>Calculated:  KE = 1/2 × m × v{{sup|2}}.  v = 1.023{{e|3}} m/s.  m = 7.349{{e|22}} kg.  KE = 1/2 × (7.349{{e|22}} kg) × (1.023{{e|3}} m/s){{sup|2}} = 3.845{{e|28}}{{nbsp}}J.</ref>
|-
| 10<sup>29</sup> || &nbsp; || 2.1×10<sup>29</sup>{{nbsp}}J || [[Rotational energy]] of the [[Earth]]<ref>{{cite web|title=Moment of Inertia—Earth|url=http://scienceworld.wolfram.com/physics/MomentofInertiaEarth.html|work=Eric Weisstein's World of Physics|access-date=5 November 2011}}</ref><ref>{{cite web|last=Allain|first=Rhett|title=Rotational energy of the Earth as an energy source|url=http://scienceblogs.com/dotphysics/2009/06/rotational-energy-of-the-earth-as-an-energy-source.php|work=.dotphysics|publisher=Science Blogs|access-date=5 November 2011|quote=the Earth takes 23.9345 hours to rotate|archive-url=https://web.archive.org/web/20111117014824/http://scienceblogs.com/dotphysics/2009/06/rotational-energy-of-the-earth-as-an-energy-source.php|archive-date=17 November 2011|url-status=dead}}</ref><ref>Calculated:  E_rotational = 1/2 × I × w{{sup|2}} = 1/2 × (8.0{{e|37}} kg m{{sup|2}}) × (2×pi/(23.9345 hour period × 3600 seconds/hour)){{sup|2}} = 2.1{{e|29}}{{nbsp}}J</ref>
|-
| 10<sup>30</sup> || [[quetta-]] (QJ) || 1.8×10<sup>30</sup>{{nbsp}}J || [[Gravitational binding energy]] of [[Mercury (planet)|Mercury]]
|-
| rowspan="2" | 10<sup>31</sup> || rowspan="2" | &nbsp; || ~2×10<sup>31</sup>{{nbsp}}J || |The most energetic [[Superflare|stellar superflare]] to date (S Fornacis)<ref>{{Cite journal |last1=Schaefer |first1=Bradley E. |last2=King |first2=Jeremy R. |last3=Deliyannis |first3=Constantine P. |date=February 2000 |title=Superflares on Ordinary Solar-Type Stars |url=https://iopscience.iop.org/article/10.1086/308325 |journal=The Astrophysical Journal |language=en |volume=529 |issue=2 |pages=1026–1030 |doi=10.1086/308325 |arxiv=astro-ph/9909188 |bibcode=2000ApJ...529.1026S |s2cid=10586370 |issn=0004-637X}}</ref>
|-
| &nbsp;3.3×10<sup>31</sup>J || Total energy output of the [[Sun]] each day<ref name="sun2"/><ref>Calculated:  3.8{{e|26}}{{nbsp}}J/s × 86400 s/day = 3.3{{e|31}}{{nbsp}}J</ref>
|-
| 10<sup>32</sup> || &nbsp; || 1.71×10<sup>32</sup>{{nbsp}}J || [[Gravitational binding energy]] of the Earth<ref>{{Cite web |title= |url=http://typnet.net/Essays/EarthBindGraphics/EarthBind.pdf |access-date=2024-01-04 |archive-url=https://web.archive.org/web/20240104173513/http://typnet.net/Essays/EarthBindGraphics/EarthBind.pdf |archive-date=4 January 2024 }}</ref>
|-
| 10<sup>33</sup> || &nbsp; || 2.7×10<sup>33</sup>{{nbsp}}J || [[Earth|Earth's]] kinetic energy at perihelion in its orbit around the Sun<ref>{{Cite web |date=2023-12-26 |title=Earth Fact Sheet |url=https://nssdc.gsfc.nasa.gov/planetary/factsheet/earthfact.html |access-date=2024-01-04 |archive-url=https://web.archive.org/web/20231226062838/https://nssdc.gsfc.nasa.gov/planetary/factsheet/earthfact.html |archive-date=26 December 2023 }}</ref><ref>KE = 1/2 × 5.9722×10^24 kg × (30.29 km/s)^2 = 2.74×10^33 J</ref>
|-
| 10<sup>34</sup> || &nbsp; || 1.2×10<sup>34</sup>{{nbsp}}J || Total energy output of the [[Sun]] each year<ref name="sun2"/><ref>Calculated:  3.8{{e|26}}{{nbsp}}J/s × 86400 s/day × 365.25 days/year = 1.2{{e|34}}{{nbsp}}J</ref>
|-
| colspan="2" rowspan="2" |10<sup>39 &nbsp;</sup>
|1-5×10<sup>39</sup> J

|Energy of the giant flare ([[Starquake (astrophysics)|starquake]]) released by [[SGR 1806−20|SGR 1806-20]]<ref>{{Cite web |title=NASA - Cosmic Explosion Among the Brightest in Recorded History |url=https://www.nasa.gov/vision/universe/watchtheskies/swift_nsu_0205.html |access-date=2022-03-27 |website=www.nasa.gov |language=en}}</ref><ref>{{Cite journal |last1=Palmer |first1=D. M. |last2=Barthelmy |first2=S. |last3=Gehrels |first3=N. |last4=Kippen |first4=R. M. |last5=Cayton |first5=T. |last6=Kouveliotou |first6=C. |last7=Eichler |first7=D. |last8=Wijers |first8=R. a. M. J. |last9=Woods |first9=P. M. |last10=Granot |first10=J. |last11=Lyubarsky |first11=Y. E. |date=April 2005 |title=A giant γ-ray flare from the magnetar SGR 1806–20 |url=https://www.nature.com/articles/nature03525 |journal=Nature |language=en |volume=434 |issue=7037 |pages=1107–1109 |doi=10.1038/nature03525 |pmid=15858567 |arxiv=astro-ph/0503030 |bibcode=2005Natur.434.1107P |s2cid=16579885 |issn=1476-4687}}</ref><ref>{{Cite journal |last1=Stella |first1=L. |last2=Dall'Osso |first2=S. |last3=Israel |first3=G. L. |last4=Vecchio |first4=A. |date=2005-11-17 |title=Gravitational Radiation from Newborn Magnetars in the Virgo Cluster |url=https://iopscience.iop.org/article/10.1086/498685 |journal=The Astrophysical Journal |language=en |volume=634 |issue=2 |pages=L165–L168 |doi=10.1086/498685 |arxiv=astro-ph/0511068 |bibcode=2005ApJ...634L.165S |s2cid=18172538 |issn=0004-637X}}</ref>
|-
| 6.6×10<sup>39</sup> J{{nbsp}} || Theoretical total [[mass–energy]] of the [[Moon]]
|-
|rowspan=2 | 10<sup>41</sup>
|rowspan=2 | &nbsp;
| 2.276×10<sup>41</sup>{{nbsp}}J || Gravitational binding energy of the [[Sun]]<ref name="U"><math>U = \frac{(3/5)GM^2}{r}</math><br />Chandrasekhar, S. 1939, ''An Introduction to the Study of Stellar Structure'' (Chicago: U. of Chicago; reprinted in New York: Dover), section 9, eqs. 90–92, p. 51 (Dover edition)<br>Lang, K. R. 1980, ''Astrophysical Formulae'' (Berlin: Springer Verlag), p. 272</ref>
|-
| 5.4×10<sup>41</sup>{{nbsp}}J || Theoretical total [[mass–energy]] of the [[Earth]]<ref>{{cite web | url=http://solarsystem.nasa.gov/planets/profile.cfm?Object=Earth&Display=Facts | archive-url=https://archive.today/20120723114418/http://solarsystem.nasa.gov/planets/profile.cfm?Object=Earth&Display=Facts | url-status=dead | archive-date=23 July 2012 | title=Earth: Facts & Figures | work=Solar System Exploration | publisher=NASA | access-date=29 September 2011 }}</ref><ref>{{cite web|title=Conversion from kg to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=24&num=6.0&From=kg&To=j&Action=Convert+value+and+show+factor|publisher=NIST|access-date=4 November 2011}}</ref>
|-
|rowspan=1|10<sup>43</sup>
|rowspan=1| &nbsp;
| 5×10<sup>43</sup>{{nbsp}}J
| Total energy of all gamma rays in a typical [[gamma-ray burst]]<ref>{{Cite journal | last1 = Frail | first1 = D. A. | last2 = Kulkarni | first2 = S. R. | last3 = Sari | first3 = R. | last4 = Djorgovski | first4 = S. G. | last5 = Bloom | first5 = J. S. | last6 = Galama | first6 = T. J. | last7 = Reichart | first7 = D. E. | last8 = Berger | first8 = E. | last9 = Harrison | first9 = F. A. | last10 = Price | first10 = P. A. | last11 = Yost | first11 = S. A. | last12 = Diercks | first12 = A. | last13 = Goodrich | first13 = R. W. | last14 = Chaffee | first14 = F. | title = Beaming in Gamma-Ray Bursts: Evidence for a Standard Energy Reservoir | doi = 10.1086/338119 | journal = The Astrophysical Journal | volume = 562 | issue = 1 | pages = L55 | year = 2001 |arxiv = astro-ph/0102282 |bibcode = 2001ApJ...562L..55F | s2cid = 1047372 }} "the gamma-ray energy release, corrected for geometry, is narrowly clustered around 5 × 10{{sup|50}} erg"</ref><ref>Calculated:  5{{e|50}} erg × 1{{e|-7}}{{nbsp}}J/erg = 5{{e|43}}{{nbsp}}J</ref>
|-
| colspan="2" rowspan="4" |10<sup>44</sup>
|~10<sup>44</sup> J
|Average value of a [[Tidal disruption event|Tidal Disruption Event]] (TDE) in [[Visible spectrum|optical]]/[[Ultraviolet|UV]] [[Electromagnetic spectrum|bands]]<ref>{{Cite journal |last1=Lu |first1=Wenbin |last2=Kumar |first2=Pawan |date=2018-09-28 |title=On the Missing Energy Puzzle of Tidal Disruption Events |journal=The Astrophysical Journal |volume=865 |issue=2 |pages=128 |doi=10.3847/1538-4357/aad54a |arxiv=1802.02151 |bibcode=2018ApJ...865..128L |s2cid=56015417 |issn=1538-4357 |doi-access=free }}</ref>
|-
| 1–2×10<sup>44</sup>{{nbsp}}J || Estimated energy released in a [[supernova]],<ref>{{cite journal | author=Khokhlov, A.; Mueller, E.; Hoeflich, P. | title=Light curves of Type IA supernova models with different explosion mechanisms | journal=[[Astronomy and Astrophysics]] | year=1993 | volume=270 | issue=1–2 | pages=223–248 | bibcode=1993A&A...270..223K | last2=Mueller | last3=Hoeflich }}</ref> sometimes referred to as a ''[[foe (unit)|foe]]''
|-
| {{Val|1.2|e=44|u=J}} || Approximate lifetime energy output of the [[Sun]].<!-- Computation from [[Foe (unit)]] -->
|-
|~10<sup>44-45</sup>
|Estimated kinetic energy released by [[Fast blue optical transient|FBOT]] CSS161010<ref>{{Cite journal |last1=Coppejans |first1=D. L. |last2=Margutti |first2=R. |last3=Terreran |first3=G. |last4=Nayana |first4=A. J. |last5=Coughlin |first5=E. R. |last6=Laskar |first6=T. |last7=Alexander |first7=K. D. |last8=Bietenholz |first8=M. |last9=Caprioli |first9=D. |last10=Chandra |first10=P. |last11=Drout |first11=M. R. |date=2020-05-26 |title=A Mildly Relativistic Outflow from the Energetic, Fast-rising Blue Optical Transient CSS161010 in a Dwarf Galaxy |journal=The Astrophysical Journal |language=en |volume=895 |issue=1 |pages=L23 |doi=10.3847/2041-8213/ab8cc7 |arxiv=2003.10503 |bibcode=2020ApJ...895L..23C |s2cid=214623364 |issn=2041-8213 |doi-access=free }}</ref>
|-
| rowspan="5" |10<sup>45</sup>
| rowspan="5" | &nbsp;
| {{Val|1.1|0.2|e=45|u=J}} || Energy released by [[hypernova]] [[ASASSN-15lh]]<ref>{{cite journal
 |last1=Dong|first1=S.|last2=Shappee|first2=B. J.|last3=Prieto|first3=J. L.|last4=Jha|first4=S. W.
 |last5=Stanek|first5=K. Z.|last6=Holoien|first6=T. W.- S.|last7=Kochanek|first7=C. S.|last8=Thompson|first8=T. A.
 |last9=Morrell|first9=N.|last10=Thompson|first10=I. B.|last11=Basu|first11=U.|last12=Beacom|first12=J. F.
 |last13=Bersier|first13=D.|last14=Brimacombe|first14=J.|last15=Brown|first15=J. S.
 |last16=Bufano|first16=F.|last17=Chen|first17=P.|last18=Conseil|first18=E.|last19=Danilet|first19=A. B. 
 |last20=Falco|first20=E.|last21=Grupe|first21=D.|last22=Kiyota|first22=S.|last23=Masi|first23=G.
 |last24=Nicholls|first24=B.|last25=Olivares E.|first25=F.|last26=Pignata|first26=G.|last27=Pojmanski|first27=G.
 |last28=Simonian|first28=G. V.|last29=Szczygiel|first29=D. M.|last30=Wozniak|first30=P. R.
 |display-authors=10
 |title=ASASSN-15lh: A highly super-luminous supernova
 |journal=[[Science (journal)|Science]]
 |date=15 January 2016
 |volume=351 |issue=6270 |pages=257–260
 |doi=10.1126/science.aac9613
 |arxiv=1507.03010|bibcode = 2016Sci...351..257D |pmid=26816375|s2cid=31444274}}</ref>
|-
|2.3×10<sup>45</sup> J
|Energy released by the very energetic supernova [[PS1-10adi]], about twice the energy of [[ASASSN-15lh]]<ref>{{Cite journal |last1=Kankare |first1=E. |last2=Kotak |first2=R. |last3=Mattila |first3=S. |last4=Lundqvist |first4=P. |last5=Ward |first5=M. J. |last6=Fraser |first6=M. |last7=Lawrence |first7=A. |last8=Smartt |first8=S. J. |last9=Meikle |first9=W. P. S. |last10=Bruce |first10=A. |last11=Harmanen |first11=J. |date=December 2017 |title=A population of highly energetic transient events in the centres of active galaxies |url=https://www.nature.com/articles/s41550-017-0290-2 |journal=Nature Astronomy |language=en |volume=1 |issue=12 |pages=865–871 |doi=10.1038/s41550-017-0290-2 |arxiv=1711.04577 |bibcode=2017NatAs...1..865K |s2cid=119421626 |issn=2397-3366}}</ref><ref>Both ASSASN-15lh and PS1-10adi are indicated as supernovae and probably they are; actually, other mechanisms are proposed to explain them, more or less in accordance to the characteristics of supernovae</ref>
|-
|≳5 × 10<sup>45</sup> J
|Energy released by the most energetic [[supernova]] to date, [[SN 2016aps]]<ref>{{Cite web |author1=Mike Wall |date=2020-04-13 |title=Boom! Distant star explosion is brightest ever seen |url=https://www.space.com/brightest-supernova-ever-discovered-sn2016aps.html |access-date=2022-03-29 |website=Space.com |language=en}}</ref><ref>{{Cite web |last=Starr |first=Michelle |title=Astronomers Detect The Most Powerful Star Explosion We've Ever Observed |url=https://www.sciencealert.com/this-exploding-star-was-the-most-powerful-we-ve-ever-spotted |access-date=2022-03-29 |website=ScienceAlert |date=14 April 2020 |language=en-gb}}</ref><ref>{{Cite web |author=Kristen Rogers |title=Astronomers just discovered the brightest supernova ever seen |url=https://www.cnn.com/2020/04/13/world/brightest-supernova-sn2016aps-scn/index.html |access-date=2022-03-29 |website=CNN|date=13 April 2020 }}</ref><ref>{{Cite journal |last1=Nicholl |first1=Matt |last2=Blanchard |first2=Peter K. |last3=Berger |first3=Edo |last4=Chornock |first4=Ryan |last5=Margutti |first5=Raffaella |last6=Gomez |first6=Sebastian |last7=Lunnan |first7=Ragnhild |last8=Miller |first8=Adam A. |last9=Fong |first9=Wen-fai |last10=Terreran |first10=Giacomo |last11=Vigna-Gómez |first11=Alejandro |date=September 2020 |title=An extremely energetic supernova from a very massive star in a dense medium |url=https://www.nature.com/articles/s41550-020-1066-7 |journal=Nature Astronomy |language=en |volume=4 |issue=9 |pages=893–899 |doi=10.1038/s41550-020-1066-7 |arxiv=2004.05840 |bibcode=2020NatAs...4..893N |s2cid=215744925 |issn=2397-3366}}</ref>
|-
|>10<sup>45</sup> J
|Estimated energy of a magnetorotational hypernova<ref>{{Cite journal |last1=Yong |first1=D. |last2=Kobayashi |first2=C. |last3=Da Costa |first3=G. S. |last4=Bessell |first4=M. S. |last5=Chiti |first5=A. |last6=Frebel |first6=A. |last7=Lind |first7=K. |last8=Mackey |first8=A. D. |last9=Nordlander |first9=T. |last10=Asplund |first10=M. |last11=Casey |first11=A. R. |date=2021-07-08 |title=R-Process elements from magnetorotational hypernovae |journal=Nature |volume=595 |issue=7866 |pages=223–226 |doi=10.1038/s41586-021-03611-2 |pmid=34234332 |arxiv=2107.03010 |bibcode=2021Natur.595..223Y |s2cid=235755170 |issn=0028-0836}}</ref>
|-
| few times×10<sup>45</sup>{{nbsp}}J || Beaming-corrected 'True' total [[energy]] (Energy in gamma rays+relativistic kinetic energy) of hyper-energetic [[gamma-ray burst]]<ref>{{Cite journal|arxiv=1003.3885|last1=McBreen|first1=S|title=Optical and near-infrared follow-up observations of four Fermi/LAT GRBs: Redshifts, afterglows, energetics and host galaxies|journal=Astronomy and Astrophysics|volume=516|issue=71|pages=A71|last2=Krühler|first2=T|last3=Rau|first3=A|last4=Greiner|first4=J|last5=Kann|first5=D. A|last6=Savaglio|first6=S|last7=Afonso|first7=P|last8=Clemens|first8=C|last9=Filgas|first9=R|last10=Klose|first10=S|last11=Küpüc Yoldas|first11=A|last12=Olivares E|first12=F|last13=Rossi|first13=A|last14=Szokoly|first14=G. P|last15=Updike|first15=A|last16=Yoldas|first16=A|year=2010|doi=10.1051/0004-6361/200913734|bibcode=2010A&A...516A..71M|s2cid=119151764}}</ref><ref>{{Cite journal|arxiv=1004.2900|last1=Cenko|first1=S. B|title=Afterglow Observations of Fermi-LAT Gamma-Ray Bursts and the Emerging Class of Hyper-Energetic Events|journal=The Astrophysical Journal|volume=732|issue=1|pages=29|last2=Frail|first2=D. A|last3=Harrison|first3=F. A|last4=Haislip|first4=J. B|last5=Reichart|first5=D. E|last6=Butler|first6=N. R|last7=Cobb|first7=B. E|last8=Cucchiara|first8=A|last9=Berger|first9=E|last10=Bloom|first10=J. S|last11=Chandra|first11=P|last12=Fox|first12=D. B|last13=Perley|first13=D. A|last14=Prochaska|first14=J. X|last15=Filippenko|first15=A. V|last16=Glazebrook|first16=K|last17=Ivarsen|first17=K. M|last18=Kasliwal|first18=M. M|last19=Kulkarni|first19=S. R|last20=LaCluyze|first20=A. P|last21=Lopez|first21=S|last22=Morgan|first22=A. N|last23=Pettini|first23=M|last24=Rana|first24=V. R|year=2010|doi=10.1088/0004-637X/732/1/29|bibcode=2011ApJ...732...29C|s2cid=50964480}}</ref><ref>{{Cite journal|arxiv=0905.0690|last1=Cenko|first1=S. B|title=The Collimation and Energetics of the Brightest Swift Gamma-Ray Bursts|journal=The Astrophysical Journal|volume=711|issue=2|pages=641–654|last2=Frail|first2=D. A|last3=Harrison|first3=F. A|last4=Kulkarni|first4=S. R|last5=Nakar|first5=E|last6=Chandra|first6=P|last7=Butler|first7=N. R|last8=Fox|first8=D. B|last9=Gal-Yam|first9=A|last10=Kasliwal|first10=M. M|last11=Kelemen|first11=J|last12=Moon|first12=D. -S|last13=Price|first13=P. A|last14=Rau|first14=A|last15=Soderberg|first15=A. M|author15-link= Alicia M. Soderberg|last16=Teplitz|first16=H. I|last17=Werner|first17=M. W|last18=Bock|first18=D. C. -J|last19=Bloom|first19=J. S|last20=Starr|first20=D. A|last21=Filippenko|first21=A. V|last22=Chevalier|first22=R. A|last23=Gehrels|first23=N|last24=Nousek|first24=J. N|last25=Piran|first25=T|last26=Piran|first26=T|year=2010|doi=10.1088/0004-637X/711/2/641|bibcode=2010ApJ...711..641C|s2cid=32188849}}</ref><ref>url= http://tsvi.phys.huji.ac.il/presentations/Frail_AstroExtreme.pdf {{Webarchive|url=https://web.archive.org/web/20140801172839/http://tsvi.phys.huji.ac.il/presentations/Frail_AstroExtreme.pdf |date=1 August 2014 }}</ref><ref>url= http://fermi.gsfc.nasa.gov/science/mtgs/grb2010/tue/Dale_Frail.ppt</ref>
|-
| colspan="2" rowspan="3" | 10<sup>46</sup> || >10<sup>46</sup>{{nbsp}}J
| Estimated energy released in a [[hypernova]],<ref>{{cite web|title=A Hypernova: The Super-charged Supernova and its link to Gamma-Ray Bursts|url=http://imagine.gsfc.nasa.gov/docs/science/know_l1/why_hyper.html|work=Imagine the Universe!|publisher=NASA|access-date=9 December 2011|quote=With a power about 100 times that of the already astonishingly powerful "typical" supernova|archive-date=19 October 2011|archive-url=https://web.archive.org/web/20111019233153/http://imagine.gsfc.nasa.gov/docs/science/know_l1/why_hyper.html|url-status=dead}}</ref><ref>it is specified that only the 1% of the total energy (10^44 [[Joule|J]]) is [[kinetic energy]]; so, almost the total energy is carried by [[neutrino]]s</ref> in a [[pair-instability supernova]]<ref>{{Cite journal|url=https://iopscience.iop.org/article/10.1088/0004-637X/734/2/102|doi = 10.1088/0004-637X/734/2/102|title = Pair Instability Supernovae: Light Curves, Spectra, and Shock Breakout|year = 2011|last1 = Kasen|first1 = Daniel|last2 = Woosley|first2 = S. E.|last3 = Heger|first3 = Alexander|journal = The Astrophysical Journal|volume = 734|issue = 2|page = 102|arxiv = 1101.3336|bibcode = 2011ApJ...734..102K|s2cid = 118508934}}</ref> and in theoretical [[quark-nova]]e<ref>{{cite journal |url=https://www.aanda.org/component/article?access=bibcode&bibcode=&bibcode=2002A%2526A...390L..39OFUL |title = Quark-Nova {{!}} Astronomy & Astrophysics (A&A)| journal=Astronomy & Astrophysics | date=August 2002 | volume=390 | issue=3 | pages=L39–L42 | doi=10.1051/0004-6361:20020982 | last1=Ouyed | first1=R. | last2=Dey | first2=J. | last3=Dey | first3=M. }}</ref>
|-
|1.5×10<sup>46</sup>{{nbsp}}J
|Estimated total energy of the most energetic optical non-[[quasar]] transient, [[AT 2021lwx|AT2021lwx]].<ref name="Wiseman2023">{{Cite journal |last1=Wiseman |first1=p. |last2=Wang |first2=Y. |last3=Hönig |first3=S. |last4=Castero-Segura |first4=N. |last5=Clark |first5=P. |last6=Frohmaier |first6=C. |last7=Fulton |first7=M. D. |last8=Leloudas |first8=G. |last9=Middleton |first9=M. |last10=Müller-Bravo |first10=T. E. |last11=Mummery |first11=A. |last12=Pursiainen |first12=M |last13=Smartt |first13=S. J. |last14=Smith |first14=K. |last15=Sullivan |first15=M. |date=July 2023 |title=Multiwavelength observations of the extraordinary accretion event AT 2021lwx |journal=[[Monthly Notices of the Royal Astronomical Society]] |volume=522 |issue=3 |pages=3992–4002 |doi=10.1093/mnras/stad1000 |doi-access=free |arxiv=2303.04412 }}</ref>
|-
|2–5×10<sup>46</sup>{{nbsp}}J
|Beaming-corrected 'True' total [[energy]] of the most powerful gamma-ray burst recorded, [[GRB 221009A]].<ref name=":0" /><ref>{{Cite journal |last1=Kann |first1=D. A. |last2=Agayeva |first2=S. |last3=Aivazyan |first3=V. |last4=Alishov |first4=S. |last5=Andrade |first5=C. M. |last6=Antier |first6=S. |last7=Baransky |first7=A. |last8=Bendjoya |first8=P. |last9=Benkhaldoun |first9=Z. |last10=Beradze |first10=S. |last11=Berezin |first11=D. |last12=Boër |first12=M. |last13=Broens |first13=E. |last14=Brunier |first14=S. |last15=Bulla |first15=M. |date=2023-05-09 |title=GRANDMA and HXMT Observations of GRB 221009A: The Standard Luminosity Afterglow of a Hyperluminous Gamma-Ray Burst—In Gedenken an David Alexander Kann |journal=The Astrophysical Journal Letters |language=en |volume=948 |issue=2 |pages=L12 |doi=10.3847/2041-8213/acc8d0 |issn=2041-8205|doi-access=free |arxiv=2302.06225 |bibcode=2023ApJ...948L..12K }}</ref><ref>{{Cite journal |last1=Frederiks |first1=D. |last2=Svinkin |first2=D. |last3=Lysenko |first3=A. L. |last4=Molkov |first4=S. |last5=Tsvetkova |first5=A. |last6=Ulanov |first6=M. |last7=Ridnaia |first7=A. |last8=Lutovinov |first8=A. A. |last9=Lapshov |first9=I. |last10=Tkachenko |first10=A. |last11=Levin |first11=V. |date=2023-05-18 |title=Properties of the Extremely Energetic GRB 221009A from Konus-WIND and SRG/ART-XC Observations |journal=The Astrophysical Journal Letters |volume=949 |issue=1 |pages=L7 |doi=10.3847/2041-8213/acd1eb |issn=2041-8205|doi-access=free |arxiv=2302.13383 |bibcode=2023ApJ...949L...7F }}</ref>
|-
| colspan="2" rowspan="7" |10<sup>47</sup>
|10<sup>45-47</sup> J
|Estimated energy of stellar mass rotational [[Stellar black hole|black holes]] by [[vacuum polarization]] in a [[electromagnetic field]]<ref>{{Cite journal |last1=Ruffini |first1=R. |last2=Salmonson |first2=J. D. |last3=Wilson |first3=J. R. |last4=Xue |first4=S. -S. |date=1999-10-01 |title=On the pair electromagnetic pulse of a black hole with electromagnetic structure |url=https://ui.adsabs.harvard.edu/abs/1999A&A...350..334R |journal=Astronomy and Astrophysics |volume=350 |pages=334–343 |arxiv=astro-ph/9907030 |bibcode=1999A&A...350..334R |issn=0004-6361}}</ref><ref>{{Cite journal |last1=Ruffini |first1=R. |last2=Salmonson |first2=J. D. |last3=Wilson |first3=J. R. |last4=Xue |first4=S. -S. |date=2000-07-01 |title=On the pair-electromagnetic pulse from an electromagnetic black hole surrounded by a baryonic remnant |url=https://ui.adsabs.harvard.edu/abs/2000A&A...359..855R |journal=Astronomy and Astrophysics |volume=359 |pages=855–864 |arxiv=astro-ph/0004257 |bibcode=2000A&A...359..855R |issn=0004-6361}}</ref>
|-
|>10<sup>47</sup> J
|Total energy of a very energetic and relativistic jetted [[Tidal disruption event|Tidal Disruption Event]] (TDE)<ref>{{Cite journal |last1=De Colle |first1=Fabio |last2=Lu |first2=Wenbin |date=September 2020 |title=Jets from Tidal Disruption Events |journal=New Astronomy Reviews |volume=89 |pages=101538 |doi=10.1016/j.newar.2020.101538|arxiv=1911.01442 |bibcode=2020NewAR..8901538D |s2cid=207870076 }}</ref>
|-
|~10<sup>47</sup> J
|Highest possible beaming-corrected 'True' total [[energy]] of a gamma-ray burst.<ref>{{Cite journal |last1=Misra |first1=Kuntal |last2=Ghosh |first2=Ankur |last3=Resmi |first3=L. |date=2023 |title=The Detection of Very High Energy Photons in Gamma Ray Bursts |url=https://www.tifr.res.in/~ipa1970/news/V53-12/Vol53-12-A11.pdf |journal= |publisher=Tata Institute of Fundamental Research}}</ref><ref>{{Cite journal |last1=Frederiks |first1=D. |last2=Svinkin |first2=D. |last3=Lysenko |first3=A. L. |last4=Molkov |first4=S. |last5=Tsvetkova |first5=A. |last6=Ulanov |first6=M. |last7=Ridnaia |first7=A. |last8=Lutovinov |first8=A. A. |last9=Lapshov |first9=I. |last10=Tkachenko |first10=A. |last11=Levin |first11=V. |date=2023-05-01 |title=Properties of the Extremely Energetic GRB 221009A from Konus-WIND and SRG/ART-XC Observations |journal=The Astrophysical Journal Letters |volume=949 |issue=1 |pages=L7 |doi=10.3847/2041-8213/acd1eb |issn=2041-8205|doi-access=free |arxiv=2302.13383 |bibcode=2023ApJ...949L...7F }}</ref>
|-
|1.8×10<sup>47</sup>{{nbsp}}J || Theoretical total [[mass–energy]] of the [[Sun]]<ref>{{cite web |url= http://nssdc.gsfc.nasa.gov/planetary/factsheet/sunfact.html |title= Sun Fact Sheet |publisher= NASA |access-date=15 October 2011 }}</ref><ref>{{cite web|title=Conversion from kg to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=30&num=2.0&From=kg&To=j&Action=Convert+value+and+show+factor|publisher=NIST|access-date=4 November 2011}}</ref>
|-
|5.4×10<sup>47</sup>{{nbsp}}J || [[Mass–energy]] emitted as [[gravitational waves]] during [[Binary black hole|the merger]] of two [[black holes]], originally about 30 Solar masses each, as observed by [[LIGO]] ([[GW150914]])<ref>{{Cite journal | last1 = Abbott | first1 = B. | last2 = Abbott | first2 = R. | display-authors=1 | title = Observation of Gravitational Waves from a Binary Black Hole Merger | journal = Physical Review Letters | doi = 10.1103/PhysRevLett.116.061102 | volume = 116 | issue = 6 | year = 2016|arxiv = 1602.03837 |bibcode = 2016PhRvL.116f1102A | pmid=26918975 | pages=061102| s2cid = 124959784 }}</ref>
|-
|8.6×10<sup>47</sup>{{nbsp}}J || Mass–energy emitted as gravitational waves during the most energetic black hole merger observed until 2020 (GW170729)<ref>If GW190521 is a [[Boson Star|boson star]] merging, the present one remains the largest. See note [246][247]</ref>
|-
|8.8×10<sup>47</sup>{{nbsp}}J || [[GRB 080916C]] – formerly the most powerful Gamma-Ray Burst (GRB) ever recorded – total 'apparent'/isotropic (not corrected for beaming) energy output estimated at 8.8 × 10<sup>47</sup> joules (8.8 × 10<sup>54</sup> erg), or 4.9 times the Sun's mass turned to energy.<ref>{{Cite arXiv |last=Tajima |first=Hiroyasu |date=2009 |title=Fermi Observations of high-energy gamma-ray emissions from GRB 080916C |class=astro-ph.HE |eprint=0907.0714 }}</ref><ref>{{cite web |url= http://www.astronomynow.com/090220fermisrecordbreakinggrb.html|title=Fermi's record breaking gamma-ray burst}}</ref><ref>It is important to specify that the energetic reduction for beaming (invoked to explain so much energetics and jet breaks) is expected in the "Fireball model", which is the traditional one; other main models explain both '''Long''' and '''Short''' GRBs with binary systems, such as "Induced Gravitational Collapse", "Binary-Driven Hypernovae" which refer to the "Fireshell" one, in which cases the beaming isn't assumpted and the isotropic energy is a real value of energy due to the rotational energy of the stellar black hole and vacuum polarization in a electromagnetic field, which are able to explain energetics up and over 10<sup>47</sup> J</ref>
|-
| rowspan="3" |10<sup>48</sup>
|
|~10<sup>48</sup> J
|Estimated energy of a supermassive [[Population III star]] supernova, denominated "General Relativistic Instability Supernova."<ref>{{Cite journal|last1=Whalen|first1=Daniel J.|last2=Johnson|first2=Jarrett L.|last3=Smidt|first3=Joseph|last4=Meiksin|first4=Avery|last5=Heger|first5=Alexander|last6=Even|first6=Wesley|last7=Fryer|first7=Chris L.|title=The Supernova That Destroyed a Protogalaxy: Prompt Chemical Enrichment and Supermassive Black Hole Growth|date=August 2013|url=https://doi.org/10.1088/0004-637x/774/1/64|journal=The Astrophysical Journal|language=en|volume=774|issue=1|pages=64|doi=10.1088/0004-637X/774/1/64|issn=0004-637X|arxiv=1305.6966|bibcode=2013ApJ...774...64W|s2cid=59289675}}</ref><ref>{{Cite journal|last1=Chen|first1=Ke-Jung|last2=Heger|first2=Alexander|last3=Woosley|first3=Stan|last4=Almgren|first4=Ann|last5=Whalen|first5=Daniel J.|last6=Johnson|first6=Jarrett L.|title=The General Relativistic Instability Supernova of a Supermassive Population III Star|date=July 2014|url=https://doi.org/10.1088/0004-637x/790/2/162|journal=The Astrophysical Journal|language=en|volume=790|issue=2|pages=162|doi=10.1088/0004-637X/790/2/162|issn=0004-637X|arxiv=1402.4777|bibcode=2014ApJ...790..162C|s2cid=119269181}}</ref>
|-
|
|~1.2×10<sup>48</sup> J

|Approximate energy released in the most energetic black hole merging to date ([[GW190521]]), which originated the first [[intermediate-mass black hole]] ever detected<ref>Assuming the uncertainties about the masses of the objects, the values of the LIGO Data are taken in consideration; so we have a newborn black hole with about 142 solar masses and the conversion in gravitational waves of about 7 solar masses</ref><ref>{{Cite journal |last1=Abbott |first1=R. |last2=Abbott |first2=T. D. |last3=Abraham |first3=S. |last4=Acernese |first4=F. |last5=Ackley |first5=K. |last6=Adams |first6=C. |last7=Adhikari |first7=R. X. |last8=Adya |first8=V. B. |last9=Affeldt |first9=C. |last10=Agathos |first10=M. |last11=Agatsuma |first11=K. |date=2020-09-02 |title=Properties and Astrophysical Implications of the 150 M ⊙ Binary Black Hole Merger GW190521 |journal=The Astrophysical Journal |language=en |volume=900 |issue=1 |pages=L13 |doi=10.3847/2041-8213/aba493 |arxiv=2009.01190 |bibcode=2020ApJ...900L..13A |s2cid=221447444 |issn=2041-8213 |doi-access=free }}</ref><ref>{{Cite journal |last1=LIGO Scientific Collaboration and Virgo Collaboration |last2=Abbott |first2=R. |last3=Abbott |first3=T. D. |last4=Abraham |first4=S. |last5=Acernese |first5=F. |last6=Ackley |first6=K. |last7=Adams |first7=C. |last8=Adhikari |first8=R. X. |last9=Adya |first9=V. B. |last10=Affeldt |first10=C. |last11=Agathos |first11=M. |date=2020-09-02 |title=<nowiki>GW190521: A Binary Black Hole Merger with a Total Mass of $150\text{ }\text{ }{M}_{\ensuremath{\bigodot}}$</nowiki> |journal=Physical Review Letters |volume=125 |issue=10 |pages=101102 |doi=10.1103/PhysRevLett.125.101102|pmid=32955328 |s2cid=221447506 |doi-access=free |arxiv=2009.01075 }}</ref><ref>A research claims that this is instead a [[boson stars]] merging with approximately 8 times more probability than the black hole case; if so, the existence and the collision of boson stars there would be confirmed together. Furthermore, the energy released and the distance would be reduced.[https://spaceaustralia.com/index.php/feature/black-holes-or-boson-stars-mystery-gw190521]

See the following note for the link of the research</ref><ref>{{Cite journal |last1=Bustillo |first1=Juan Calderón |last2=Sanchis-Gual |first2=Nicolas |last3=Torres-Forné |first3=Alejandro |last4=Font |first4=José A. |last5=Vajpeyi |first5=Avi |last6=Smith |first6=Rory |last7=Herdeiro |first7=Carlos |last8=Radu |first8=Eugen |last9=Leong |first9=Samson H. W. |date=2021-02-24 |title=GW190521 as a Merger of Proca Stars: A Potential New Vector Boson of $8.7\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}13}\text{  }\mathrm{eV}$ |url=https://link.aps.org/doi/10.1103/PhysRevLett.126.081101 |journal=Physical Review Letters |volume=126 |issue=8 |pages=081101 |doi=10.1103/PhysRevLett.126.081101|pmid=33709746 |hdl=10773/31565 |s2cid=231719224 |hdl-access=free }}</ref>
|-
|
|1.2–3×10<sup>48</sup> J
|[[GRB 221009A]] – the most powerful Gamma-Ray Burst (GRB) ever recorded – total 'apparent'/isotropic (not corrected for beaming) energy output estimated at 1.2–3 × 10<sup>48</sup> joules (1.2–3 × 10<sup>55</sup> erg).<ref name=":0">{{Cite journal |last1=Burns |first1=Eric |last2=Svinkin |first2=Dmitry |last3=Fenimore |first3=Edward |last4=Kann |first4=D. Alexander |last5=Agüí Fernández |first5=José Feliciano |last6=Frederiks |first6=Dmitry |last7=Hamburg |first7=Rachel |last8=Lesage |first8=Stephen |last9=Temiraev |first9=Yuri |last10=Tsvetkova |first10=Anastasia |last11=Bissaldi |first11=Elisabetta |last12=Briggs |first12=Michael S. |last13=Dalessi |first13=Sarah |last14=Dunwoody |first14=Rachel |last15=Fletcher |first15=Cori |date=2023-03-01 |title=GRB 221009A: The BOAT |journal=The Astrophysical Journal Letters |volume=946 |issue=1 |pages=L31 |doi=10.3847/2041-8213/acc39c |issn=2041-8205|doi-access=free |arxiv=2302.14037 |bibcode=2023ApJ...946L..31B }}</ref><ref>{{Cite journal |last1=Zhang 张 |first1=B. Theodore 兵 |last2=Murase |first2=Kohta |last3=Ioka |first3=Kunihito |last4=Song |first4=Deheng |last5=Yuan 袁 |first5=Chengchao 成超 |last6=Mészáros |first6=Péter |date=2023-04-01 |title=External Inverse-compton and Proton Synchrotron Emission from the Reverse Shock as the Origin of VHE Gamma Rays from the Hyper-bright GRB 221009A |journal=The Astrophysical Journal Letters |volume=947 |issue=1 |pages=L14 |doi=10.3847/2041-8213/acc79f |doi-access=free |arxiv=2211.05754 |bibcode=2023ApJ...947L..14Z |issn=2041-8205}}</ref>
|-
|10<sup>50</sup>
|
|≳10<sup>50</sup> J
|Upper limit of 'apparent'/isotropic energy ''(Eiso)'' of [[Population III stars]] Gamma-Ray Bursts (GRBs).<ref>{{Cite journal|last1=Toma|first1=Kenji|last2=Sakamoto|first2=Takanori|last3=Mészáros|first3=Peter|title=Population III Gamma-Ray Burst Afterglows: Constraints on Stellar Masses and External Medium Densities|date=April 2011|url=https://doi.org/10.1088/0004-637x/731/2/127|journal=The Astrophysical Journal|language=en|volume=731|issue=2|pages=127|doi=10.1088/0004-637X/731/2/127|issn=0004-637X|arxiv=1008.1269|bibcode=2011ApJ...731..127T|s2cid=119288325}}</ref>
|-
| rowspan="2" |10<sup>53</sup>
|
|>10<sup>53</sup> J
|[[Mechanical energy]] of very energetic so-called "[[quasar]] tsunamis"<ref>{{Cite web |last=Garner |first=Rob |date=2020-03-18 |title=Quasar Tsunamis Rip Across Galaxies |url=http://www.nasa.gov/feature/goddard/2020/quasar-tsunamis-rip-across-galaxies |access-date=2022-03-28 |website=NASA}}</ref><ref>To determinate this value, the maximum energy of 10<sup>47</sup> J for gamma-ray burts is taken in consideration; then six orders of magnitude are added, equivalent to ten million of years, the time frame in which the quasar tsunami will exceed the GRBs energetics over 1 million of times, according to the Nahum Arav's statement in the previous note</ref>
|-
| &nbsp; || 6×10<sup>53</sup>{{nbsp}}J || Total mechanical [[energy]] or [[enthalpy]] in the powerful [[Active galactic nucleus|AGN]] outburst in the RBS 797<ref>{{Cite journal|arxiv=1103.0630|last1=Cavagnolo|first1=K. W|title=A Powerful AGN Outburst in RBS 797|journal=The Astrophysical Journal|volume=732|issue=2|pages=71|last2=McNamara|first2=B. R|last3=Wise|first3=M. W|last4=Nulsen|first4=P. E. J|last5=Brüggen|first5=M|last6=Gitti|first6=M|last7=Rafferty|first7=D. A|year=2011|doi=10.1088/0004-637X/732/2/71|bibcode=2011ApJ...732...71C|s2cid=73653317}}</ref>
|-
|10<sup>54</sup>
| &nbsp;|| 3×10<sup>54</sup>{{nbsp}}J || Total mechanical [[energy]] or [[enthalpy]] in the powerful AGN outburst in the Hercules A (3C 348)<ref>url= http://iopscience.iop.org/1538-4357/625/1/L9/fulltext/19121.text.html</ref>
|-
| 10<sup>55</sup> || &nbsp; || >10<sup>55</sup>{{nbsp}}J || Total mechanical [[energy]] or [[enthalpy]] in the powerful AGN outburst in the [[MS 0735.6+7421]],<ref>{{Cite journal|last1=Li|first1=Shuang-Liang|last2=Cao|first2=Xinwu|date=June 2012|title=CONSTRAINTS ON JET FORMATION MECHANISMS WITH THE MOST ENERGETIC GIANT OUTBURSTS IN MS 0735$\mathplus$7421|url=https://doi.org/10.1088/0004-637x/753/1/24|journal=The Astrophysical Journal|language=en|volume=753|issue=1|pages=24|doi=10.1088/0004-637X/753/1/24|issn=0004-637X|arxiv=1204.2327|s2cid=119236058}}</ref> [[Ophiuchus Supercluster eruption|Ophiucus Supercluster Explosion]]<ref>{{Cite journal|last1=Giacintucci|first1=S.|last2=Markevitch|first2=M.|last3=Johnston-Hollitt|first3=M.|last4=Wik|first4=D. R.|last5=Wang|first5=Q. H. S.|last6=Clarke|first6=T. E.|date=February 2020|title=Discovery of a Giant Radio Fossil in the Ophiuchus Galaxy Cluster|journal=The Astrophysical Journal|language=en|volume=891|issue=1|pages=1|doi=10.3847/1538-4357/ab6a9d|issn=0004-637X|arxiv=2002.01291|bibcode=2020ApJ...891....1G|s2cid=211020555 |doi-access=free }}</ref> and [[supermassive black hole]]s [[Binary black hole|mergings]]<ref>{{Cite web |last=Siegel |first=Ethan |title=Merging Supermassive Black Holes Will Become The Most Energetic Events Of All |url=https://www.forbes.com/sites/startswithabang/2020/03/03/the-most-energetic-event-in-the-universe-hasnt-been-discovered-yet/ |access-date=2022-03-21 |website=Forbes |language=en}}</ref><ref>{{Cite web |last=Siegel |first=Ethan |date=2020-03-10 |title=Merging Supermassive Black Holes Are The Universe's Most Energetic Events Of All |url=https://medium.com/starts-with-a-bang/merging-supermassive-black-holes-are-the-universes-most-energetic-events-of-all-be380cdb2975 |access-date=2022-03-21 |website=Starts With A Bang! |language=en}}</ref>
|-
| rowspan="2" |10<sup>57</sup>
| rowspan="2" |
|~10<sup>57</sup> J
|Estimated rotational energy of [[Messier 87|M87]] [[Supermassive black hole|SMBH]] and total energy of the most luminous [[quasar]]s over [[Billion years|Gyr]] time-scales<ref>{{Cite web |last=Diodati |first=Michele |date=2020-04-11 |title=Rotating Black Holes, the Most Powerful Energy Generators in the Universe |url=https://medium.com/amazing-science/rotating-black-holes-the-most-powerful-energy-generators-in-the-universe-832439add442 |access-date=2022-03-28 |website=Amazing Science |language=en}}</ref><ref>{{Cite journal |last1=Tamburini |first1=Fabrizio |last2=Thidé |first2=Bo |last3=Della Valle |first3=Massimo |date=2020 |title=Measurement of the spin of the M87 black hole from its observed twisted light |journal=Monthly Notices of the Royal Astronomical Society: Letters |volume=492 |pages=L22–L27 |url=https://openaccess.inaf.it/handle/20.500.12386/31845 |language=en |doi=10.1093/mnrasl/slz176 |issn=0035-8711|arxiv=1904.07923 }}</ref>
|-
|~2×10<sup>57</sup> J
|Estimated [[thermal energy]] of the [[Bullet Cluster]] of [[Galaxy cluster|galaxies]]<ref>{{Cite journal|last1=Tucker|first1=W.|last2=Blanco|first2=P.|last3=Rappoport|first3=S.|last4=David|first4=L.|last5=Fabricant|first5=D.|last6=Falco|first6=E. E.|last7=Forman|first7=W.|last8=Dressler|first8=A.|last9=Ramella|first9=M.|date=1998-03-02|title=1E 0657–56: A Contender for the Hottest Known Cluster of Galaxies|url=https://iopscience.iop.org/article/10.1086/311234/meta|journal=The Astrophysical Journal|language=en|volume=496|issue=1|pages=L5|doi=10.1086/311234|issn=0004-637X|arxiv=astro-ph/9801120|bibcode=1998ApJ...496L...5T|s2cid=16140198}}</ref>
|-
| rowspan="2" |10<sup>58</sup>
|
|~10<sup>58</sup> J
|Estimated total energy (in shockwaves, turbulence, gases heating up, gravitational force) of [[galaxy cluster]]s mergings<ref>{{Cite journal |last1=Markevitch |first1=Maxim |last2=Vikhlinin |first2=Alexey |date=May 2007 |title=Shocks and cold fronts in galaxy clusters |journal=Physics Reports |volume=443 |issue=1 |pages=1–53 |doi=10.1016/j.physrep.2007.01.001|arxiv=astro-ph/0701821 |bibcode=2007PhR...443....1M |s2cid=119326224 }}</ref>
|-
| &nbsp; || 4×10<sup>58</sup>{{nbsp}}J || Visible [[mass–energy]] in our [[galaxy]], the [[Milky Way]]<ref>{{cite web |url=http://physics.uoregon.edu/~jimbrau/astr123/Notes/Chapter23.html#mass |title=The Milky Way Galaxy |author=Jim Brau |access-date=4 November 2011 |author-link=James E. Brau }}</ref><ref>{{cite web|title=Conversion from kg to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=41&num=4&From=kg&To=j&Action=Convert+value+and+show+factor|publisher=NIST|access-date=4 November 2011}}</ref>
|-
| 10<sup>59</sup> || &nbsp; || 1×10<sup>59</sup>{{nbsp}}J || Total [[mass–energy]] of our [[galaxy]], the [[Milky Way]], including [[dark matter]] and [[dark energy]]<ref name=Karachentsev2006>{{cite journal | last1 = Karachentsev | first1 = I. D. | last2 = Kashibadze | first2 = O. G. | year = 2006 | title = Masses of the local group and of the M81 group estimated from distortions in the local velocity field | journal = Astrophysics | volume = 49 | issue = 1| pages = 3–18 | doi = 10.1007/s10511-006-0002-6 | bibcode=2006Ap.....49....3K| s2cid = 120973010 }}</ref><ref>{{cite web|title=Conversion from kg to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=42&num=1.2&From=kg&To=j&Action=Convert+value+and+show+factor|publisher=NIST|access-date=4 November 2011}}</ref>
|-
| 10<sup>62</sup> || &nbsp; || 1–2×10<sup>62</sup>{{nbsp}}J || Total [[mass–energy]] of the [[Virgo Supercluster]] including [[dark matter]], the [[Supercluster]] which contains the [[Milky Way]]<ref name="ein07">{{cite journal
 | author  = Einasto, M.
 | title   = The richest superclusters. I. Morphology
 | journal = Astronomy and Astrophysics
 | date    = December 2007
 | volume  = 476
 | issue   = 2
 | pages   = 697–711
 | bibcode     = 2007A&A...476..697E
 | doi     = 10.1051/0004-6361:20078037
 | display-authors  = 1
 | last2  = Saar
 | first2  = E.
 | last3  = Liivamägi
 | first3  = L. J.
 | last4  = Einasto
 | first4  = J.
 | last5  = Tago
 | first5  = E.
 | last6  = Martínez
 | first6  = V. J.
 | last7  = Starck
 | first7  = J.-L.
 | last8  = Müller
 | first8  = V.
 | last9  = Heinämäki
 | first9  = P.
 | arxiv = 0706.1122
| s2cid = 15004251
 }}</ref>
|-
| 10<sup>69</sup> ||  || 4×10<sup>69</sup>{{nbsp}}J || Estimated total [[mass–energy]] of the [[observable universe]]<ref name="nasa">{{cite web|url=http://imagine.gsfc.nasa.gov/docs/ask_astro/answers/980211b.html |title=Big Bang Energy |access-date=26 December 2016 |url-status=bot: unknown |archive-url=https://web.archive.org/web/20140819120709/http://imagine.gsfc.nasa.gov/docs/ask_astro/answers/980211b.html |archive-date=19 August 2014 }}</ref>
|}

==SI multiples==
{{SI multiples|unit=joule|symbol=J}}
{{SI unit lowercase|James Prescott Joule|joule|J}}

==See also==
{{portal|Energy}}

*[[Conversion of units of energy]]
*[[Energy conversion efficiency]]
*[[Energy density]]
*[[Metric system]]
*[[Outline of energy]]
*[[Scientific notation]]
*[[TNT equivalent]]

==Notes==
{{Reflist|30em}}

{{Orders of magnitude}}

{{DEFAULTSORT:Orders of Magnitude (Energy)}}
[[Category:Energy]]
[[Category:Units of energy|*]]
[[Category:Orders of magnitude|Energy]]