檔案:Rosette Nebula (noao-rosette mulligan).jpg

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English: The appropriately named Rosette nebula is, not unlike a newly bloomed flower, a place of newfound life. Many of the stars within this wreath of gas have just formed. Their energetic winds and emissions of UV radiation are quickly blowing away the surrounding clouds of gas to reveal a new cluster of stars. Many thicker parts of the cloud resist their ultimate demise, and remain in radial structures stubborn to relent to the impressive forces arrayed against them. The initial mass of gas clouds such as this determine how many stars are formed within. A very massive cloud will likely form many stars. Here, the stars in the heart of the Rosette nebula are blowing away the building blocks of more stars and have halted most other star formation. However, there are many globules of gas (Bok Globules) that may contain individual stars still in the process of forming. A high resolution image of one of these regions in Hydrogen-alpha light can be seen by looking at this detail image of the Rosette nebula.This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014.
Ngit-khì 2014年Liuk-ngie̍t12日 (上傳日期)
Lòi-ngièn Rosette Nebula
Chok-chá KPNO/NOIRLab/NSF/AURA/Walter Mulligan/Flynn Haase
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The appropriately named Rosette nebula is, not unlike a newly bloomed flower, a place of newfound life. Many of the stars within this wreath of gas have just formed.

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1,800 像素

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1111099d1307859804e1bc3fc76d7164e92d5f95

斷定方法 繁體中文: SHA-1 中文 (已轉換拼寫)

成立或建立時間 繁體中文

12 6 2014

r96zm74mffrvoos462j8m5q75z5ohj89vrsvw8w94peij45i4

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tông-chhièn2023年10月23日 (Yit) 17:182023年10月23日 (Yit) 17:18 ke pán-pún ke Suk-lio̍k-thù1,800 × 1,299(999 KB)OptimusPrimeBot#Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/large/noao-rosette_mulligan.jpg via Commons:Spacemedia

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