File:Clear to cloudy hot Jupiters.jpg

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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

描述

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 ~~left~~ (right?) 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.

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.

日期

2015年12月14日, 17:00:00

来源

http://www.spacetelescope.org/images/heic1524a/

作者

ESA/Hubble & NASA

其他版本

本檔案有多個提取出的圖像：

许可协议

署名

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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By reproducing ESA/Hubble material, in part or in full, the user acknowledges the terms on which such use is permitted.

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署名: ESA/Hubble

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文件历史

点击某个日期/时间查看对应时刻的文件。

	日期/时间	大小	用户	备注
当前	2018年3月2日 (五) 15:06	10,000 × 6,105（13.33 MB）	Drbogdan	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	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	User created page with UploadWizard

文件用途

以下页面使用本文件：

WASP-39b

全域文件用途

以下其他wiki使用此文件：

ar.wikipedia.org上的用途
ca.wikipedia.org上的用途
- WASP-17b
cs.wikipedia.org上的用途
- WASP-17b
en.wikipedia.org上的用途
es.wikipedia.org上的用途
fr.wikipedia.org上的用途
- WASP-19 b
- WASP-39 b
id.wikipedia.org上的用途
- WASP-12b
it.wikipedia.org上的用途
- WASP-19 b
ja.wikipedia.org上的用途
lt.wikipedia.org上的用途
- WASP-39b
pt.wikipedia.org上的用途
- HD 209458 b
- Júpiter quente
ro.wikipedia.org上的用途
- WASP-12b
- WASP-6b
- WASP-31b
- WASP-17b
- WASP-19b
- WASP-39b
- HAT-P-12b
- HAT-P-1b
- HD 209458 b
uk.wikipedia.org上的用途
- HD 209458 b
uz.wikipedia.org上的用途
- WASP-17b (ekzosayyora)
- WASP-12b (ekzosayyora)
vi.wikipedia.org上的用途

元数据

此文件中包含有扩展的信息。这些信息可能是由数码相机或扫描仪在创建或数字化过程中所添加。

如果此文件的源文件已经被修改，一些信息在修改后的文件中将不能完全反映出来。

图像标题	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. The colors of the planets are for illustration purposes only. There is little scientific data on color with the exception of HD 189733b, which became known as the "blue planet." The planets are also depicted with a variety of different cloud properties. The wind patterns shown on these 10 planets, which resemble the visible structures on Jupiter, are based on theoretical models. The illustrations are to scale with each other. HAT-P-12b, the smallest of these planets, is approximately the size of Jupiter, while WASP-17b, the largest one in the sample, is almost twice the size. 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.
简短标题	Artist's Impression of"Hot Jupiter"Exoplanets
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	8 8 8
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	-{R\|http://www.spacetelescope.org}- Karl-Schwarzschild-Strasse 2 Garching bei Mnchen, , D-85748 Germany
关键词	HAT-P-12b HAT-P-1b HD 189733b HD 209458b WASP-12b WASP-17b WASP-19b WASP-31b WASP-39b WASP-6b
IIM版本	4

File:Clear to cloudy hot Jupiters.jpg

摘要

许可协议

说明

此文件中描述的项目

描繪內容

HAT-P-12b

著作權狀態

版权所有

许可协议

知识共享署名4.0国际

成立或建立時間

14 12 2015

多媒體型式

image/jpeg

核對和

4b5ccdca19e8e74bf638665b82bb6de60c9c04f4

資料大小

13,974,825 字节

高度

6,105 像素

寬度

10,000 像素

文件历史

文件用途

全域文件用途

元数据