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M96, John Bozeman

M96

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M96, John Bozeman

M96

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Description

Messier 96 (also known as M96 or NGC 3368) is an intermediate spiral galaxy about 31 million light-years away in the constellation Leo. t 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 solar masses (M☉). Messier 96 is about the same mass and size as the Milky Way. It is a very asymmetric galaxy; its dust and gas are unevenly spread throughout its weak spiral arms, and its core is just offset from the midpoint of its extremes. Its arms are also asymmetrical, thought to have been influenced by the gravitational pull of other galaxies within its group.

Data from the Hubble Space Telescope MAST Portal. Release date: 2024-03-30

Camera: WFC3
Monochrome - F657N

Processed with FITS Liberator, GraXpert, PixInsight and Photoshop 2024.

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M96, John Bozeman