File:NASA-JPL-Caltech - Double the Rubble (PIA11375) (pd).jpg

页面内容不支持其他语言。
這個文件來自維基共享資源
维基百科,自由的百科全书

原始文件(3,000 × 1,600像素,文件大小:2.15 MB,MIME类型:image/jpeg


摘要

描述
English: This artist's conception shows the closest known planetary system to our own, called Epsilon Eridani. Observations from NASA's Spitzer Space Telescope show that the system hosts two asteroid belts, in addition to previously identified candidate planets and an outer comet ring.

Epsilon Eridani is located about 10 light-years away in the constellation Eridanus. It is visible in the night skies with the naked eye.

The system's inner asteroid belt appears as the yellowish ring around the star, while the outer asteroid belt is in the foreground. The outermost comet ring is too far out to be seen in this view, but comets originating from it are shown in the upper right corner.

Astronomers think that each of Epsilon Eridani's asteroid belts could have a planet orbiting just outside it, shepherding its rocky debris into a ring in the same way that Jupiter helps keep our asteroid belt confined. The planet near the inner belt was previously identified in 2000 via the radial velocity, or "star wobble," technique, while the planet near the outer belt was inferred when Spitzer discovered the belt.

The inner belt orbits at a distance of about 3 astronomical units from its star —or about the same position as the asteroid belt in our own solar system (an astronomical unit is the distance between Earth and our sun). The second asteroid belt lies at about 20 astronomical units from the star, or a position comparable to Uranus in our solar system. The outer comet ring orbits from 35 to 90 astronomical units from the star; our solar system's analogous Kuiper Belt extends from about 30 to 50 astronomical units from the sun.
Français : A traduire...
日期 未知日期
Unknown date
来源 Double the Rubble
作者 NASA/JPL-Caltech
本图像或视频收录于美国国家航空航天局 (NASA)喷气推进实验室(Jet Propulsion Laboratory),其照片编号是: PIA11375

此标签不表示文件的著作权状态。任何文件在附有此标签的同時还需要一个有效的著作权标签请参阅许可协议说明页面以了解更多信息。
其他语言:

许可协议

Public domain 本文件完全由NASA创作,在美国属于公有领域。根据NASA的版权方针,NASA的材料除非另有声明否则不受版权保护。(参见Template:PD-USGov/zhNASA版权方针页面JPL图片使用方针。)
警告:

文件历史

点击某个日期/时间查看对应时刻的文件。

日期/时间缩⁠略⁠图大小用户备注
当前2017年2月13日 (一) 21:492017年2月13日 (一) 21:49版本的缩略图3,000 × 1,600(2.15 MB)David Levyrecompressed TIFF file
2011年11月7日 (一) 05:572011年11月7日 (一) 05:57版本的缩略图3,000 × 1,600(4.11 MB)OgreBot(BOT): Reverting to most recent version before archival
2011年11月7日 (一) 05:572011年11月7日 (一) 05:57版本的缩略图3,000 × 1,600(625 KB)OgreBot(BOT): Uploading old version of file from en.wikipedia; originally uploaded on 2008-10-27 21:14:20 by Cookbutter
2008年11月14日 (五) 18:512008年11月14日 (五) 18:51版本的缩略图3,000 × 1,600(4.11 MB)ComputerHotline{{Information |Description={{en|1=This artist's conception shows the closest known planetary system to our own, called Epsilon Eridani. Observations from NASA's Spitzer Space Telescope show that the system hosts two asteroid belts, in addition to previous

以下3个页面使用本文件:

全域文件用途

以下其他wiki使用此文件: