Celestial hemisphere:  Northern  ·  Constellation: Triangulum (Tri)  ·  Contains:  HD9483  ·  HD9686  ·  IC 131  ·  IC 132  ·  IC 133  ·  IC 135  ·  IC 136  ·  IC 137  ·  IC 142  ·  IC 143  ·  M 33  ·  NGC 588  ·  NGC 592  ·  NGC 595  ·  NGC 598  ·  NGC 604  ·  Triangulum Galaxy  ·  Triangulum Pinwheel
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Triangulum galaxy, Steed Yu
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Triangulum galaxy

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Triangulum galaxy, Steed Yu
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Triangulum galaxy

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Description

M33, also known as the Triangulum Galaxy, is a spiral galaxy located 2.73 million light-years away from Earth in the constellation Triangulum. It is a member of the Local Group of galaxies, which also includes the Milky Way and Andromeda galaxies. M33 has a relatively bright apparent magnitude of 5.7, making it one of the most distant objects that can be viewed with the unaided eye, although a telescope is needed to observe its spiral features. 

The Triangulum Galaxy is characterized by its orderly spiral structure and is home to numerous sites of rapid star birth. It is believed to be a suspected gravitational companion to the Andromeda Galaxy, and both galaxies are moving toward our own. Star formation in the Triangulum Galaxy (M33) is an ongoing process, with numerous sites of rapid star birth scattered throughout the galaxy. The star formation rate in M33 is ten times higher than the average found in the Andromeda Galaxy. 

Astrometric data from Gaia in 2019 suggests that M33 and M31 are not in orbit around each other, and if correct, M33 is on its first infall proper into the Andromeda Galaxy (M31). The fate of M33 is uncertain, with possible scenarios including being torn apart and absorbed by the greater companion, exhausting its gas supply, or participating in the collision between the Milky Way and M31.

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Triangulum galaxy, Steed Yu