NGC 5885 is an intermediate barred spiral galaxy located in the constellation Libra. Its speed relative to the cosmic microwave background is 2,185 ± 13 km/s, which corresponds to a Hubble distance of 32.3 ± 2.3 Mpc (~105 million ly). [1] NGC 5885 was discovered by German-British astronomer William Herschel in 1784. [2]

NGC 5885 is a Intermediate Spiral Galaxy in the Libra constellation. NGC 5885 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.

NGC 5885 is an Barred Spiral Galaxy located in the constellation of Libra in the southern hemisphere. NGC 5885's distance from Earth is 73,900,512.06 light years. NGC 5885 is called NGC 5885 in the New General Catalogue (NGC).

2020年5月11日 · Historical Identification: Per Dreyer, NGC 5850 (= GC 4047 = JH 1902 = WH II 543, 1860 RA 15 00 02, NPD 87 54.9) is "considerably faint, small, a little extended, pretty suddenly brighter middle". Physical Information: Apparent size 4.5 by 3.9? arcmin.

< NGC List NGC 5885. NGC 5885 is a mixed spiral galaxy located in the constellation of Libra. The NGC is a catalog of 7,840 nebulae, star clusters, and galaxies. Here are the key stats on NGC 5885:

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

NGC 5885 (H2157) NGC 5885 (H2157) is a galaxy located in the constellation of Libra. The Herchel 2500 is a catalog of nebulae, star clusters, and galaxies. Here are the key stats on NGC 5885:

NGC 5885 (također poznat kao IRAS 15123-0954, MCG -2-39-13 i PGC 54429) je prečkasta spiralna galaksija koja je udaljena oko 92 miliona sg od Zemlje i nalazi se u sazviježđu Vaga. Najveći prečnik je 3,50 (94 hiljade sg) a najmanji 3,1 uglovnih minuta (83 hiljade sg).

NGC 5885 este o hi (21cm) source ⁠(d) situată în constelația Balanța. [4] [5] [6] A fost descoperită în 9 mai 1784 de către William Herschel. [7] Se află la o distanță de 30,38 de megaparseci de Pământ. [8]

New high-SNR 21 cm H I line profiles have been obtained for 104 galaxieswith the Green Bank 43 m telescope. The primary sample is composed ofisolated spirals with no known optical companions within a 1 radius anda median ratio of optical diameter to beamwidth of 0.17.