Dwarf Irregular Galaxy

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Large Magellanic Cloud

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The Large Magellanic Cloud (LMC) is a dwarf irregular galaxy located on the border between the constellations Dorado and Mensa.

The galaxy is believed to be a satellite of the Milky Way and a member of the Local Group of galaxies, which includes about 30 galaxies that are loosely bound together by their gravitation.
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Whirlpool Galaxy – Messier 51

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The Whirlpool Galaxy, also known as Messier 51 (M51) and NGC 5194, is a grand-design spiral galaxy in Canes Venatici. The galaxy appears face-on when seen from Earth. Its designation in the New General Catalogue is NGC 5194. The galaxy lies about 23 million light years from Earth. It was named the Whirlpool because of its swirling spiral structure.

The Whirlpool Galaxy is one of the brightest and most famous galaxies in the night sky, notable for its two striking spiral arms that make M51 a grand design galaxy. The spiral arms are really lanes of stars and starburst regions interspersed with dust. They compress hydrogen gas and are responsible for creating new clusters of stars.
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NGC 1569 in Camelopardalis

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NGC 1569 is a dwarf irregular galaxy found in the Camelopardalis constellation. It is one of the best known starburst galaxies in the sky. It was first discovered by William Herschel on November 4, 1788. NGC 1569 has an apparent visual magnitude of 11.9 lies at a distance of 11 million light years.

The galaxy’s spectrum is blueshifted, which means that NGC 1569 is moving toward our solar system, unlike most other galaxies, which have redshifted spectra and are therefore moving away from us (because the universe is expanding).
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