Discovering NGC 3384: The Lenticular Galaxy in Leo

NGC 3384

NGC 3384 (also known as NGC 3371) is a lenticular galaxy. It is located approximately 35 million light-years away. This galaxy is in the constellation Leo. It is a prominent member of the M 96 Group. This group is also called the Leo I Group. It includes the well-known Messier objects M 95, M 96, and M 105.

NGC 3384 and its neighbor M 105 are surrounded by a massive ring of neutral hydrogen. This ring is 650,000 light-years wide. Sparse star formation still occurs there. In the night sky, NGC 3384 forms a visual trio with the elliptical galaxy M 105. It forms this trio with (NGC 3379) and the spiral galaxy NGC 3389.

While M 105 and NGC 3384 are physical companions, NGC 3389 is a background galaxy located significantly further away. The galaxy hosts a supermassive black hole at its core. It has an estimated mass of 16 million times that of the Sun. This black hole is considered “quiet,” producing very little radio energy.

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Discovering Messier 96

Messier 96

Messier 96 is also known as M96 or NGC 3368. It is an intermediate spiral galaxy. It is located approximately 31 million light-years away in the constellation Leo. It is the brightest member of the M96 Group (or Leo I Group). This group includes other prominent galaxies, such as M95 and M105.

M96 has an asymmetrical structure with unevenly distributed dust and gas and ill-defined spiral arms, likely due to gravitational interactions. Its core is not perfectly centered. It has a diameter of about 100,000 light-years. It contains an estimated 100 billion stars. This makes it comparable in size and mass to the Milky Way.

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