NGC 6851 is a Elliptical Galaxy in the Telescopium constellation. NGC 6851 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its visual magnitude of 11.67, NGC 6851 is visible with the help of a telescope having an aperture of 8 inches (200mm) or more.

The Carnegie-Irvine Galaxy Survey (CGS) Data Products . Images • summary from image atlas • original FITS images (B, V, R, I) • color-composite image (original) • color-composite image (star-cleaned) • stacked image • structure maps (B, V, R, I) • color index maps (B-R, R-I) Radial Profiles

2023年10月31日 · Historical Identification: Per Dreyer, NGC 6851 (= GC 4531 = JH 3807, 1860 RA 19 53 19, NPD 138 39.2) is "pretty faint, small, very little extended, pretty suddenly brighter middle."

NGC 6851 . NGC 6851 is a elliptical galaxy located in the constellation Telescopium. Some key stats include:

NGC 6851 este o galaxie situată în constelația Telescopul. [3] [4] [5] A fost descoperită în 5 septembrie 1836 de către John Herschel. [6] Se află la o distanță de 35,32 de megaparseci de Pământ. [7]

NGC 6851 est une galaxie elliptique située dans la constellation du Télescope. Sa vitesse par rapport au fond diffus cosmologique est de 2 903 ± 18 km/s, ce qui correspond à une distance de Hubble de 42,8 ± 3,0 Mpc (∼140 millions d' al) 1. NGC 6851 a été découverte par l'astronome britannique John Herschel en 1836 3.

NGC 6851A is a Spiral Galaxy in the Telescopium constellation. NGC 6851A is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its B magnitude of 14.88, NGC 6851A is visible with the help of a telescope having an aperture of 20 inches (500mm) or more.

NGC 6851 — Yeni Ümumi Kataloqda qeydə alınmış qalaktikadır. Göy üzündə Teleskop bürcü istiqamətində yerləşir. E3 tipli qalaktikadır. İngilis astronomu Con Herşel tərəfindən 1836-cı …

NGC 6751 是在 天鷹座 的一個 行星狀星雲，又稱為 亮眼星雲。 估計它距離 地球 約6,500 光年，直徑是0.8光年，在這個星雲中心的恆星表面溫度大約是140,000K。 這是一顆在數千年塌縮的 恆星，拋出外層氣體形成的。 這個星雲是澳大利亞高級中學的學生參加 雙子星天文台 舉辦的影像競賽中獲選的畫面，並贏得2009年雙子學校天文競賽的主題。 本條目中NGC 6751的圖片是在2000年4月被選出做為哈伯太空望遠鏡發射十週年紀念的假色合成影像。 ^ 1.0 1.1 SIMBAD …

NGC 6851B is a Barred Spiral Galaxy in the Telescopium constellation. NGC 6851B is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its visual magnitude of 14.81, NGC 6851B is visible with the help of a telescope having an aperture of 20 inches (500mm) or more.