spacer.png, 0 kB
首頁 arrow 會員專區 arrow 星際大廳、哈拉區 arrow 天文新知 arrow MWC 758c_ A Planet has Whipped Up Spiral Arms Around a Young Star
MWC 758c_ A Planet has Whipped Up Spiral Arms Around a Young Star
2024-11-05 13:36:58 *
歡迎光臨, 訪客. 請先 登入註冊一個帳號.
您忘了 啟用您的帳號嗎?

請輸入帳號, 密碼以及預計登入時間
新聞:
 
   首頁   說明 登入 註冊  
頁: [1]
  列印  
作者 主題: MWC 758c_ A Planet has Whipped Up Spiral Arms Around a Young Star  (閱讀 1887 次)
peter
正式會員
星系團
******
文章: 49186



« 於: 2023-07-10 12:47:18 »

原恆星盤 MWC 758 巨大的系外行星MWC 758c
http://www.uux.cn/viewnews-116386.html


https://www.nature.com/articles/s41550-023-02028-3

 MWC 758c_ A Planet has Whipped Up Spiral Arms Around a Young Star 
 https://www.universetoday.com/162323/a-planet-has-whipped-up-spiral-arms-around-a-young-star/#more-162323 

Astronomers have found a Jovian protoplanet orbiting a young star known as MWC 758, which is about 500 light-years from Earth. The planet, called MWC 758c, is about twice the mass of Jupiter and orbits its young star at a distance of about 100 AU, or more than three times the distance of Neptune from the Sun. The spiral disk system has been known for a while, but previous observations showed no evidence of a planet. That’s because MWC 758c is particularly red, meaning either it is very cool or shrouded by lots of dust. Low red wavelengths are difficult for ground-based telescopes to observe due to the thermal noise of Earth’s atmosphere. It took the Large Binocular Telescope Interferometer (LBTI), which specializes in infrared and near-infrared observations, to finally observe the gas giant.

已記錄

請連署支持翠峰天文科技觀星園區

http://campaign.tw-npo.org/campaign//sign.php?id=2009113019034900
頁: [1]
  列印  
 
前往:  

重要聲明:本論壇是以即時上載留言的方式運作,論壇對所有留言的真實性、完整性及立場等,不負任何法律責任。而一切留言之言論只代表留言者個人意見,並非本會之立場,用戶不應信賴內容,並應自行判斷內容之真實性。於有關情形下,用戶應尋求專業意見。由於本論壇受到「即時上載留言」運作方式所規限,故不能完全監察所有留言,若讀者發現有留言出現問題,請聯絡我們。觀星論壇有權刪除任何留言及拒絕任何人士上載留言,同時亦有不刪除留言的權利。切勿撰寫粗言穢語、誹謗、渲染色情暴力或人身攻擊的言論,敬請自律。本網站保留一切法律權利。
Powered by MySQL Powered by PHP Powered by SMF 1.1.17 | SMF © 2011, Simple Machines Valid XHTML 1.0! Valid CSS!
spacer.png, 0 kB