Messier 95
Adapted from Wikipedia · Discoverer experience
Messier 95, also known as M95 or NGC 3351, is a barred spiral galaxy located about 33 million light-years away in the constellation Leo. It was discovered by Pierre Méchain in 1781 and later catalogued by Charles Messier. In 2012, astronomers found its most recent supernova.
This galaxy is classified as SB(r)b, meaning it has a bar shape with spiral arms that are neither too tightly wound nor too loose, and it features an inner ring surrounding the bar. This ring is a region where new stars are forming and stretches about 70,000 light-years across.
M95 is part of the M96 Group, a collection of galaxies in Leo that includes other Messier objects such as M96 and M105. The galaxy shows active star formation in several regions, with clusters of young stars that might one day become globular clusters.
Supernova
One bright explosion, called a supernova, was seen in M95. It happened on March 16, 2012, and was named SN 2012aw. This type of supernova happens when a big star runs out of energy and collapses. Scientists studied its light and learned more about how these stars behave.
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