ngc 47是鲸鱼座的一個漩渦星系。 星等 為13.1， 赤經 為14分30.5秒， 赤緯 為-7°10'4"。 在1886年首次被 恩斯特·威廉·勒伯萊希特·坦普爾 發現。

NGC 47 (also known as NGC 58, MCG -1-1-55, IRAS00119-0726 and PGC 967) is a barred spiral galaxy in the constellation Cetus, discovered in 1886 by Ernst Wilhelm Leberecht Tempel. Its alternate name NGC 58 is due to the observation by Lewis Swift, who was unaware that Tempel had already discovered the celestial object earlier. It appears as a ...

47 Tucanae or 47 Tuc (also designated as NGC 104 and Caldwell 106) is a globular cluster located in the constellation Tucana. It is about 4.45 ± 0.01 kpc (15,000 ± 33 ly) from Earth, [10][4] and 120 light years in diameter. [11] 47 Tuc can be seen with the naked eye, with an apparent magnitude of 4.1. [6] .

NGC 47 is a Barred Spiral Galaxy in the Cetus constellation. NGC 47 is situated close to the celestial equator and, as such, it is at least partly visible from both hemispheres in certain times of the year. Given its B magnitude of 13.4, NGC 47 is visible with the help of a telescope having an aperture of 10 inches (250mm) or more.

NGC 47，这是一个棒旋星系，在鲸鱼座，同时亦是NGC 58。

杜鹃座47 ( ngc 104) 是一个位于杜鹃座的球状星团，距离地球约13,000光年，其直径120光年。 因为亮度达到裸眼可以看见的4.1等，所以被以佛兰斯蒂德命名法命名。

2018年5月10日 · English: NGC 47 is a spiral galaxy in the constellation Cetus. It is located at RA 00 h 14 m 30.6 s , dec −07° 10′ 03″ ( J2000 ), and has an apparent magnitude of 13.

NGC 47 is a Galaxy located in the constellation of Cetus in the equatorial region. NGC 47 is called NGC 47 in the New General Catalogue (NGC). This catalogue is a list of deep space objects compiled by John Louis Emil Dreyer in 1888 to update John Herschel's earlier work. NGC 47 is not a Messier Object and doesn't have a Messier Number.

NGC 47 (ook wel NGC 58, PGC 967, MCG -1-1-55 of IRAS00119-0726) is een balkspiraalstelsel in het sterrenbeeld Walvis die op ongeveer 240 miljoen lichtjaar afstand van de Aarde staat. NGC 47 werd in 1886 ontdekt door de Duitse astronoom Ernst Wilhelm Leberecht Tempel.

NGC 47 (also known as NGC 58, MCG -1-1-55, IRAS00119-0726 and PGC 967) is a barred spiral galaxy in the constellation Cetus, discovered in 1886 by Ernst Wilhelm Leberecht Tempel. Its alternate name NGC 58 is due to the observation by Lewis Swift, who was unaware that Tempel had already discovered the object earlier. It appears as a small, faint ...

NGC 47 = NGC 58 ist eine Balken-Spiralgalaxie vom Hubble-Typ SBbc im Sternbild Walfisch südlich der Ekliptik. Die Galaxie erscheint als kleine, schwach ovale Spiralgalaxie mit hellem Kern. Sie ist schätzungsweise 258 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 175.000 Lichtjahren.

NGC 47 は、 くじら座 の方向にある 棒渦巻銀河 で、1886年に エルンスト・テンペル によって発見された。 同年 10月21日 に ルイス・スウィフト が再発見し [2] 、テンペルの発見を知らずに届け出たため、 NGC 58 という名前が重複して与えられた。 楕円の明るい核を持つ小さな渦巻状に見える。 NGC 47 (SDSS 撮影)。 ^ 74.4 × 100万 × 3.26を計算し有効数字3桁で四捨五入。 ^ a b c d e f g h i “ NASA/IPAC Extragalactic Database ”. Results for NGC 47. 2019年9月6日閲覧。

2024年10月1日 · NGC 47 (also known as NGC 58, MCG 1155, IRAS001190726 and PGC 967) is a barred spiral galaxy in the constellation Cetus, discovered in 1886 by Ernst Wilhelm Leberecht Tempel. Its alternate name NGC 58 is due to the observation by Lewis Swift, who was unaware that Tempel had already discovered th

NGC 47 (also known as NGC 58, MCG -1-1-55, IRAS00119-0726 and PGC 967) is a barred spiral galaxy in the constellation Cetus, discovered in 1886 by Ernst Wilhelm Leberecht Tempel. Its alternate name NGC 58 is due to the observation by Lewis Swift, who was unaware that Tempel had already discovered the celestial object earlier. It appears as a ...

2024年9月13日 · As a member of the {{0}}AstroBin Beta Testers{{1}} group, you are currently on the beta version of this app. To learn why a beta version is currently being tested, please see the latest posts on the {{2}}AstroBin Beta Testers forum{{3}}.

NGC 47 est une vaste galaxie spirale barrée située dans la constellation de la Baleine. Sa vitesse par rapport au fond diffus cosmologique est de 5 354 ± 24 km/s, ce qui correspond à une distance de Hubble de 79,0 ± 5,5 Mpc (∼258 millions d'al) [1]. NGC 47 a été découverte par Ernst Wilhelm Tempel en 1886.

2023年11月12日 · 47 Tucanae (NGC 104) is a globular cluster located 14,500 light-years away in the constellation Tucana. With an apparent magnitude of 4.09, it is the second brightest globular cluster in the sky, after Omega Centauri

2022年3月10日 · The second brightest globular cluster (after Omega Centauri) as seen from planet Earth, 47 Tuc lies about 13,000 light-years away. It can be spotted with the naked-eye close on the sky to the Small Magellanic Cloud in the constellation of the Toucan.

This NASA/ESA Hubble Space Telescope image shows a globular cluster known as NGC 104 — or, more commonly, 47 Tucanae, since it is part of the constellation of Tucana (The Toucan) in the southern sky. After Omega Centauri it is the brightest globular cluster in the night sky, hosting tens of thousands of stars.

The second brightest globular cluster (after Omega Centauri) as seen from planet Earth, 47 Tuc lies about 13,000 light-years away. It can be spotted with the naked-eye close on the sky to the Small Magellanic Cloud in the constellation of the Toucan .