File:A disc of rocky debris from a disrupted planetesimal (geminiann17003a).jpg
預覽大小：450 × 600 像素。 其他解析度：180 × 240 像素 | 360 × 480 像素 | 576 × 768 像素 | 768 × 1,024 像素 | 1,536 × 2,048 像素 | 4,500 × 6,000 像素。
原始檔案 （4,500 × 6,000 像素，檔案大小：3.01 MB，MIME 類型：image/jpeg）
摘要
| 描述 |
English: A disc of rocky debris from a disrupted planetesimal surrounds white dwarf plus brown dwarf binary star. The white dwarf is the burned-out core of a star that was probably similar to the Sun, the brown dwarf is only ~60 times heavier than Jupiter, and the two stars go around each other in only a bit over two hours. |
| 日期 | 2017年2月23日, 13:58:00 (上傳日期) |
| 來源 | A disc of rocky debris from a disrupted planetesimal |
| 作者 | International Gemini Observatory/NOIRLab/NSF/AURA/UCL/University of Warwick/University of Sheffield//Mark Garlick |
| 其他版本 |
|
.jpg?uselang=zh-hk){kind=link}
.jpg?uselang=zh-hk){kind=link}
.jpg?action=history&uselang=zh-hk){kind=link}
.jpg){kind=link}
授權條款
 |
This media was created by the National Optical-Infrared Astronomy Research Laboratory (NOIRLab).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public NOIRLab website, along with the texts of press releases, announcements, images of the week and captions; are licensed under a Creative Commons Attribution 4.0 International License, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible." To the uploader: You must provide a link (URL) to the original file and the authorship information if available. |
  此檔案採用創用CC 姓名標示 4.0 國際授權條款。
| |
檔案歷史
點選日期/時間以檢視該時間的檔案版本。
| 日期/時間 | 縮圖 | 尺寸 | 用戶 | 備註 | |
|---|---|---|---|---|---|
| 目前 | 2023年10月22日 (日) 23:05 | | 4,500 × 6,000（3.01 MB） | OptimusPrimeBot | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/large/geminiann17003a.jpg via Commons:Spacemedia |
檔案用途
下列頁面有用到此檔案：
全域檔案使用狀況
以下其他 wiki 使用了這個檔案：
- en.wikipedia.org 的使用狀況
.jpg){kind=link}