Messier 66: Difference between revisions

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Messier 66 (also known as NGC 3627) is an intermediate spiral galaxy about 36 million light-years away in the constellation [[Leo]]. It was discovered by Charles Messier in 1780. M66 is about 95 thousand light-years across with striking dust lanes and bright star clusters along sweeping spiral arms. M66 is part of the famous Leo Triplet, a smallgroup of galaxies that also includes M65 and NGC 3628.
[[File:375px-Sig05-016.jpg|thumb|Messier 66]]
Messier 66 (also known as NGC 3627) is an intermediate spiral galaxy about 36 million light-years away in the constellation [[Leo]]. It was discovered by Charles Messier in 1780. M66 is about 95 thousand light-years across with striking dust lanes and bright star clusters along sweeping spiral arms. M66 is part of the famous Leo Triplet, a small group of galaxies that also includes M65 and NGC 3628.


Gravitational interaction from its past encounter with neighboring NGC 3628 has resulted in:
Gravitational interaction from its past encounter with neighboring NGC 3628 has resulted in:
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==HGS Session References==  
==HGS Session References==  
HGS Sessions - Clearing [[Sexual Misery, Breeder Programs]] - 3/31/2015 <ref>HGS Session</ref>
HGS Sessions - Clearing [[Sexual Misery, Breeder Programs]] - 3/31/2015 <ref>HGS Session</ref>HGS Sessions - Clearing [[Penn State, Happy Valley]] - 4/24/2015 <ref> HGS Session</ref>
 


==References==
==References==