Messier 66: Difference between revisions
No edit summary |
|||
| (One intermediate revision by the same user not shown) | |||
| Line 1: | Line 1: | ||
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 | [[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: | ||
| Line 8: | Line 9: | ||
==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== | ||