Messier 34
From Wikipedia, the free encyclopedia
For other uses, see M34 (disambiguation).
Messier 34 | |
2MASS image of M34 |
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Observation data (J2000.0 epoch) | |
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Constellation | Perseus |
Right ascension | 02h 42.1m[1] |
Declination | +42° 46′[1] |
Distance | 1.4 kly[citation needed] (0.4 kPc) |
Apparent magnitude (V) | 5.5[citation needed] |
Apparent dimensions (V) | 35.0′[citation needed] |
Other designations | NGC 1039[1] |
See also: Open cluster, List of open clusters |
Messier 34 (also known as M 34 or NGC 1039) is an open cluster in the constellation Perseus. It was discovered by Giovanni Batista Hodierna before 1654 and included by Charles Messier in his catalog of comet-like objects in 1764.
M34 is at a distance of about 1,400 light-years away from Earth and consists of some 100 stars. It spans about 35' on the sky which translates to a true radius of 7 light years. The cluster is just visible to the naked eye in very dark conditions, well away from city lights. It is well seen in binoculars.
[edit] External links
- Messier 34, SEDS Messier pages
- Messier 34 Amateur Image by Waid Observatory
[edit] References
- Membership of Stars in NGC 1039 (M34): NASA Astrophysics Data System link to an article by B. F. Jones and Charles F. Prosser.