Celestial hemisphere:  Northern  ·  Constellation: Andromeda (And)  ·  Contains:  Great Nebula in Andromeda  ·  M 31  ·  M 32  ·  NGC 221  ·  NGC 224
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M 31, The Andromeda Galaxy, Paul Kent
M 31, The Andromeda Galaxy
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M 31, The Andromeda Galaxy

Getting plate-solving status, please wait...
M 31, The Andromeda Galaxy, Paul Kent
M 31, The Andromeda Galaxy
Powered byPixInsight

M 31, The Andromeda Galaxy

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Description

The Andromeda Galaxy (M 31) captured from our observatory in Spain. Around 6 hours of data captured through colour filters used to create this image.

Andromeda itself is our nearest large galaxy, located around 2.5 million light years from our own Milky Way. It is easy seen with the naked eye from a moderately dark location, and spans around 3 degrees, or 6 full moon widths, though only the core is bright enough to see.

The galaxy contains around 1000 billion stars, thus its quite probable that Andromeda is physically larger than our own galaxy, even though we are thought to be very similar. Blue spiral arms indicate recent star formation. These young stars are very hot and emit lots of UV and blue light. Further evidence can be spotted by zooming in and noticing small red/pink patches of ionised Hydrogen gas, characteristic of both star forming regions and supernovae. Whilst on the topic of stars, the core is the complete opposite. In the cores of spiral galaxies, star formation is almost non-existent and the only stars that have long enough life spans are cooler, low mass stars like our sun. These are more yellow in colour, hence the colour of the core. Dark dust lanes permeate the spiral arms, just like in our own milky way. Just below centre and in the upper right are two smaller galaxies that orbit Andromeda. The milky way also has satellite galaxies....the largest are the Magellanic Clouds visible from the southern hemisphere.

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M 31, The Andromeda Galaxy, Paul Kent