NGC 115 is a barred spiral galaxy located in the southern constellation of Sculptor. It was discovered by the British astronomer John Herschel on September 25, 1834. [3] The galaxy is approximately 85 million light-years from the Sun, and is about 50,000 light-years in diameter, [3] nearly half the size of our home galaxy, the Milky Way.

NGC 115 is a Barred Spiral Galaxy in the Sculptor constellation. NGC 115 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its B magnitude of 13.73, NGC 115 is visible with the help of a telescope having an aperture of 14 inches (350mm) or more.

NGC 115 is a barred spiral galaxy located in the southern constellation of Sculptor. It was discovered by the British astronomer John Herschel on September 25, ...

NGC 115 (NGC115) is a galaxy that has a distance from Earth of 97,585,988.21 light years. It can be found in the constellation of Sculptor.

< NGC List NGC 115. NGC 115 is a barred spiral galaxy located in the constellation of Sculptor. The NGC is a catalog of 7,840 nebulae, star clusters, and galaxies. Here are the key stats on NGC 115:

Physical Information: Based on a recessional velocity of 1825 km/sec, NGC 115 is about 85 million light-years away, in good agreement with redshift-independent distance estimates of 75 to 130 million light-years. Given that and its apparent size of 2.05 by 0.7 arcmin, it is about 50 thousand light-years across.

Pictures, altitude charts, data sheet and sky map for NGC 115 - Galaxy in Sculptor Constellation

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NGC 115 est une galaxie spirale barrée située dans la constellation du Sculpteur. Sa vitesse par rapport au fond diffus cosmologique est de 1 566 ± 19 km/s, ce qui correspond à une distance de Hubble de 23,1 ± 1,6 Mpc (∼75,3 millions d'al) [1]. NGC 115 a été découverte par l'astronome britannique John Herschel en 1834.

The latter properties are compared to those of other samples ofgalaxies, of both LSBs and ``classical'' high surface brightness (HSB)objects, which were selected in the optical. The 2MASS LSBs have aBT_c-KT colour which is on average 0.9 mag bluerthan that of HSBs from the NGC.