What is Canis Majoris Dwarf Galaxy?

Canis mairis dwarf is the closest galaxia of our placement in the Milky Way. With just 25,000 light years since the solar system, it is even a little closer to us than the core of our own galaxy. The Canis Majoris Galaxy Dwarf is about 42,000 light years from the galactic core of the Milky Way. It is the latest of the series of newly discovered small galaxies that are closer and closer to the ground, the latest is the dwarf elliptical galaxy shooter. The galaxy would be discovered much earlier, but it is behind the galactic disc from our point of view, which is full of opaque dust, and the galaxy itself is relatively small, with "only" about one hundred million stars.

Canis Majris Galaxy Dwarf is an irregular galaxy, as is currently in the process of tearing the gravitational force of the galaxy of the Milky Way. In fact, before the discovery of the galaxy, astronomers conducting Sloan Digital Sky found that The Milky Way circles Mik. The Monoceros ring is an example of a star stream created an attachmentIv's forces. It wraps around the Milky Way galaxy three times.

hundreds of millions of years ago, the dwarf Canis Majoris was probably significantly larger than today, and some astronomers thought it could have contributed up to 1% of the contemporary star material of the Milky Way. When our galaxy absorbs canis majoris dwarf gravity, all his stars will eventually integrated into the Milky Way and become indistinguishable from the primary mass

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