File:Clear to cloudy hot Jupiters.jpg
原始文件 (10,000 × 6,105像素,文件大小:13.33 MB,MIME类型:image/jpeg)
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摘要
[编辑]描述Clear to cloudy hot Jupiters.jpg |
English: This image shows an artist’s impression of the ten hot Jupiter exoplanets studied by David Sing and his colleagues. From top left to lower The images are to scale with each other. HAT-P-12b, the smallest of them, is approximately the size of Jupiter, while WASP-17b, the largest planet in the sample, is almost twice the size. The planets are also depicted with a variety of different cloud properties. There is almost no information about the colours of the planets available, with the exception of HD 189733b, which became known as the blue planet (heic1312). The hottest planets within the sample are portrayed with a glowing night side. This effect is strongest on WASP-12b, the hottest exoplanet in the sample, but also visible on WASP-19b and WASP-17b. It is also known that several of the planets exhibit strong Rayleigh scattering. This effect causes the blue hue of the daytime sky and the reddening of the Sun at sunset on Earth. It is also visible as a blue edge on the planets WASP-6b, HD 189733b, HAT-P-12b, and HD 209458b. The wind patterns shown on these ten planets, which resemble the visible structures on Jupiter, are based on theoretical models. |
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来源 | http://www.spacetelescope.org/images/heic1524a/ | ||
作者 | ESA/Hubble & NASA | ||
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许可协议
[编辑]ESA/Hubble images, videos and web texts are released by the ESA under the Creative Commons Attribution 4.0 International license and may on a non-exclusive basis be reproduced without fee provided they are clearly and visibly credited. Detailed conditions are below; see the ESA copyright statement for full information. For images created by NASA or on the hubblesite.org website, or for ESA/Hubble images on the esahubble.org site before 2009, use the {{PD-Hubble}} tag.
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日期/时间 | 缩略图 | 大小 | 用户 | 备注 | |
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当前 | 2018年3月2日 (五) 15:06 | 10,000 × 6,105(13.33 MB) | Drbogdan(留言 | 贡献) | added better (larger and annotated) version - per http://www.spitzer.caltech.edu/images/6132-sig15-016-Artist-s-Impression-of-Hot-Jupiter-Exoplanets - and - http://www.spitzer.caltech.edu/uploaded_files/images/0010/6597/sig15-016.jpg | |
2016年4月6日 (三) 07:18 | 6,000 × 3,663(3.11 MB) | Codrinb(留言 | 贡献) | Higher resolution from http://photojournal.jpl.nasa.gov/jpeg/PIA20056.jpg | ||
2015年12月15日 (二) 09:22 | 1,280 × 781(243 KB) | Jmencisom(留言 | 贡献) | User created page with UploadWizard |
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以下10个页面使用本文件:
- Commons:WikiProject Aviation/recent uploads/2015 December 15
- Commons:WikiProject Aviation/recent uploads/2016 April 6
- Commons:WikiProject Aviation/recent uploads/2018 March 2
- File:HAT-P-1 b.jpg
- File:Osiris (HD209458b) planet illustration.jpeg
- File:WASP-12 b.jpg
- File:WASP-17b.jpg
- File:WASP-31 b.jpg
- File:WASP-39 b.jpg
- File:WASP-6 b.jpg
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提供者 | ESA/Hubble&NASA |
图像内容提要 | This image shows an artist's impression of the 10 hot Jupiter exoplanets studied using the Hubble and Spitzer space telescopes. From top left to lower left, these planets are WASP-12b, WASP-6b, WASP-31b, WASP-39b, HD 189733b, HAT-P-12b, WASP-17b, WASP-19b, HAT-P-1b and HD 209458b. |
来源 | ESA/Hubble |
数据生成日期时间 | 2015年12月14日 (星期一) |
宽度 | 10,000 px |
高度 | 6,105 px |
每色彩组分位数 |
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压缩方案 | LZW |
像素构成 | RGB |
方向 | 正常 |
色彩组分数 | 3 |
水平分辨率 | 72 dpi |
垂直分辨率 | 72 dpi |
数据排布 | 大块格式 |
使用软件 | Adobe Photoshop CS6 (Macintosh) |
文件修改日期时间 | 2015年12月14日 (一) 10:52 |
色彩空间 | 未标定 |
联系信息 |
Karl-Schwarzschild-Strasse 2 Garching bei Mnchen, , D-85748 Germany |
关键词 |
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IIM版本 | 4 |