File:HD 189733 X-ray.jpg
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DescriptionHD 189733 X-ray.jpg |
English: In April 2010, the researchers observed a single transit using Hubble's Space Telescope Imaging Spectrograph (STIS), but they detected no trace of the planet's atmosphere. Follow-up STIS observations in September 2011 showed a surprising reversal, with striking evidence that a plume of gas was streaming away from the exoplanet.
The researchers determined that at least 1,000 tons of gas was leaving the planet's atmosphere every second. The hydrogen atoms were racing away at speeds greater than 300,000 mph. The findings will appear in an upcoming issue of the journal Astronomy & Astrophysics. Because X-rays and extreme ultraviolet starlight heat the planet's atmosphere and likely drive its escape, the team also monitored the star with Swift's X-ray Telescope (XRT). On Sept. 7, 2011, just eight hours before Hubble was scheduled to observe the transit, Swift was monitoring the star when it unleashed a powerful flare. It brightened by 3.6 times in X-rays, a spike occurring atop emission levels that already were greater than the sun's. |
Date | |
Source | http://www.nasa.gov/topics/universe/features/exoplanet-atmosphere.html |
Author | NASA/Swift/Stefan Immler |
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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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current | 13:04, 24 September 2012 | 2,250 × 2,246 (210 KB) | Stas1995 (talk | contribs) | User created page with UploadWizard |
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Orientation | Normal |
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Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Software used | Adobe Photoshop CS5 Windows |
File change date and time | 10:32, 25 June 2012 |
Color space | sRGB |
Date and time of digitizing | 10:44, 12 June 2012 |
Date metadata was last modified | 06:32, 25 June 2012 |
Unique ID of original document | xmp.did:6E3D8178D2BEE111944DCFE61BAB018C |