NGC 2466 is an unbarred spiral galaxy in the constellation of Volans. Its velocity with respect to the cosmic microwave background is 5428 ± 10 km/s, which corresponds to a Hubble distance of 261.2 ± 18.3 Mly (80.07 ± 5.61 Mpc). [1] The galaxy was discovered by British astronomer John Herschel on 20 February 1835. [2]

NGC 246 (also known as the Skull Nebula [5] or Caldwell 56) is a planetary nebula in the constellation Cetus. It was discovered in 1785 by William Herschel. The nebula and the stars associated with it are listed in several catalogs, as summarized by the SIMBAD database. [1] The nebula is roughly 3,500 +720 −850 light-years away. [2]

NGC 2266 is an open cluster [5] of stars in the constellation of Gemini. It was discovered by German-British astronomer William Herschel on 7 December 1785. [6] This is a relatively dim cluster with an integrated visual magnitude of 9.5 and an angular size of 5.0′. The stellar members can be readily resolved with an amateur telescope. [3]

NGC 2466 este o galaxie spirală situată în constelația Peștele Zburător. [3] [4] [5] A fost descoperită în 20 februarie 1835 de către John Herschel. [6]

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Media in category "NGC 2466" The following 3 files are in this category, out of 3 total.

NGC 2566 is a barred spiral galaxy in the constellation of Puppis. Its velocity with respect to the cosmic microwave background is 1898 ± 19 km/s, which corresponds to a Hubble distance of 91.3 ± 6.5 Mly (28.00 ± 1.98 Mpc). [1]

Početna strana; Istaknuti članci; Portali; Kategorije; Nedavne izmjene; Nasumična stranica; Posebne stranice

NGC 2466 is a Spiral Galaxy in the Volans constellation. NGC 2466 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its B magnitude of 13.42, NGC 2466 is visible with the help of a telescope having an aperture of 10 inches (250mm) or more.

NGC 2466 est une vaste galaxie spirale située dans la constellation du Poisson volant. Sa vitesse par rapport au fond diffus cosmologique est de 5 428 ± 10 km/s, ce qui correspond à une distance de Hubble de 80,1 ± 5,6 Mpc (∼261 millions d'al) [1]. Elle a été découverte par l'astronome britannique John Herschel en 1835 [3].