File:The Mysterious Case of the Disappearing Dust.jpg
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Summary
DescriptionThe Mysterious Case of the Disappearing Dust.jpg |
English: An artist's concept illustrates a dusty planet-forming disk, similar to the one that vanished around the star called TYC 8241 2652.
Imagine if the rings of Saturn suddenly disappeared. Astronomers have witnessed the equivalent around a young sun-like star called TYC 8241 2652. Enormous amounts of dust known to circle the star are unexpectedly nowhere to be found. "It's like the classic magician's trick: now you see it, now you don't. Only in this case we're talking about enough dust to fill an inner solar system and it really is gone!" said Carl Melis of the University of California, San Diego, who led the new study appearing in the July 5 issue of the journal Nature. A dusty disk around TYC 8241 2652 was first seen by the NASA Infrared Astronomical Satellite (IRAS) in 1983, and continued to glow brightly for 25 years. The dust was thought to be due to collisions between forming planets, a normal part of planet formation. Like Earth, warm dust absorbs the energy of visible starlight and reradiates that energy as infrared, or heat, radiation. |
Date | |
Source | https://www.jpl.nasa.gov/news/the-mysterious-case-of-the-disappearing-dust |
Author | NASA/JPL-Caltech |
Licensing
Public domainPublic domainfalsefalse |
This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) | ||
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5 July 2012
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 19:56, 25 January 2013 | 3,200 × 2,400 (2.88 MB) | wikimediacommons>Stas1995 | User created page with UploadWizard |
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Metadata
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Image title |
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Author | Spitzer Space Telescope |
Credit/Provider | NASA/JPL-Caltech/R. Hurt (SSC/Caltech) |
Headline | This artist's concept shows a young star surrounded by a dusty protoplanetary disk. This disk contains the raw material that can form planets as the star system matures. |
Source | Spitzer Space Telescope |
Short title |
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Usage terms |
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Date and time of data generation | 29 August 2007 |
Width | 3,200 px |
Height | 2,400 px |
Bits per component |
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Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop CS3 Windows |
File change date and time | 11:58, 5 July 2012 |
Color space | Uncalibrated |
Image width | 3,200 px |
Image height | 2,400 px |
Date and time of digitizing | 04:58, 5 July 2012 |
Date metadata was last modified | 04:58, 5 July 2012 |
Contact information |
http://www.spitzer.caltech.edu 1200 E. California Blvd. Pasadena, CA, 91125 USA |
Keywords | NGC 1333-IRAS 4B |
IIM version | 2 |