Contains:  Other
Messier 82, Stephen Duffy

Messier 82

Messier 82, Stephen Duffy

Messier 82

Description

M82 or the Cigar galaxy is remarkable for its star formation activity. The Cigar galaxy experiences gravitational interactions with its galactic neighbor, M81, causing it to have an extraordinarily high rate of star formation — a starburst.

Around the galaxy’s center, young stars are being born 10 times faster than they are inside our entire Milky Way galaxy. Radiation and energetic particles from these newborn stars carve into the surrounding gas, and the resulting galactic wind compresses enough gas to make millions of more stars. The rapid rate of star formation in this galaxy eventually will be self-limiting. When star formation becomes too vigorous, it will consume or destroy the material needed to make more stars. The starburst will then subside, probably in a few tens of millions of years.

M82 was discovered, along with its neighbor M81, by the German astronomer Johann Elert Bode in 1774. Located 12 million light-years from Earth in the constellation Ursa Major, M82 has an apparent magnitude of 8.4 and is best observed in April.
Text from NASA/Goddard
Scope TEC140, Camera QSI683, Mount MYT
RGB 2 hours each, Luminance 4 hours, Ha 9 hours

Reprocessed January 2023

Comments

Histogram

Messier 82, Stephen Duffy