Messier 96

From Ascension Glossary
Messier 96

Messier 96 (also known as M96 or NGC 3368) is an intermediate spiral galaxy about 31 million light-years away in the constellation Leo. It was discovered by French astronomer Pierre Méchain on March 20, 1781. After communicating his finding, French astronomer Charles Messier confirmed the finding four days later and added it to his catalogue of nebulous objects. Finding this object is extremely difficult with binoculars. With a telescope of 25.4 cm (10.0 in) aperture, the galaxy is visible as a 3 × 5 arcminute halo with a brighter core region.This complex galaxy is inclined by an angle of about 53° to the line of sight from the Earth, which is oriented at a position angle of 172°. It is categorized as a double-barred spiral galaxy with a small inner bulge through the core along with an outer bulge. The nucleus displays a weak level of activity of the LINER2 type. Variations in ultraviolet emission from the core suggest the presence of a supermassive black hole. Estimates for the mass of this object range from 1.5×106 to 4.8×107 times the mass of the Sun. On May 9, 1998 a supernova event was observed in this galaxy.

M96 is the brightest galaxy within the M96 Group, a group of galaxies in the constellation Leo that includes the Messier objects M95 and M105, as well as at least nine other galaxies.The M96 galaxy has asymmetric arms and a displaced core, probably caused by the gravitational pull by the other nearby galaxies.[1]

HGS Session References

HGS Sessions - Clearing Macau Island, China - 3/21/2015 [2]


  1. Messier 96
  2. HGS Session

Found in HGS Manual on Page 108 Found in HGS Manual on Page 115