
NGC 247 - Wikipedia
NGC 247 (also known as Caldwell 62 and commonly known as the Claw Galaxy [2]) is an intermediate spiral galaxy about 11.1 Mly away in the constellation Cetus. This distance was …
NGC 247 - 维基百科,自由的百科全书
NGC 247 也稱為 科德韋爾62,但通常暱稱為 爪子星系[2],是位於 鯨魚座 的一個 中間螺旋星系 (然而它有時被歸類為 矮螺旋星系),距離大約1110萬 光年。 這一距離在2011年2月下旬得 …
APOD: 2018 March 30 - NGC 247 and Friends
Explanation: About 70,000 light-years across, NGC 247 is a spiral galaxy smaller than our Milky Way. Measured to be only 11 million light-years distant it is nearby though. Tilted nearly edge …
NGC 247 - 維基百科,自由的百科全書 - zh.wikipedia.org
NGC 247 也稱為 科德韋爾62,但通常暱稱為 爪子星系[2],是位於 鯨魚座 的一個 中間螺旋星系 (然而它有時被歸類為 矮螺旋星系),距離大約1110萬 光年。 這一距離在2011年2月下旬得 …
NGC247和伙伴们 | NASA中文
2020年1月19日 · Explanation: About 70,000 light-years across, NGC 247 is a spiral galaxy smaller than our Milky Way. Measured to be only 11 million light-years distant it is nearby …
The dusty disk of NGC 247 | Astronomy.com - Astronomy Magazine
NGC 247 is about 11 million light-years away in the constellation Cetus the Whale. Through a moderate-sized amateur telescope, this galaxy appears quite large, but dim, and needs a dark …
NGC 247及附近的天体 | NASA中文
2024年9月5日 · Explanation: About 70,000 light-years across, NGC 247 is a spiral galaxy smaller than our Milky Way. Measured to be only 11 million light-years distant it is nearby though. …
针眼之谜,一个矮螺旋星系 | NASA中文
2022年5月24日 · The Needle’s Eye, also known as NGC 247 and Caldwell 62, is located about 11 million light-years away in the Sculptor Group – the closest group of galaxies to our own (the …
NGC 247 - Intermediate Spiral Galaxy in Cetus - TheSkyLive
NGC 247 is a Intermediate Spiral Galaxy in the Cetus constellation. NGC 247 is situated close to the celestial equator and, as such, it is at least partly visible from both hemispheres in certain …
NGC 247 - Experienced Deep Sky Imaging - Cloudy Nights
2023年9月3日 · NGC 247 - posted in Experienced Deep Sky Imaging: NGC 257 (ESO 540-22, PGC 2758, UGCA 11, Caldwell 62 and others) is an intermediate (between barred and …
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