50 Cassiopeiae
From Wikipedia, the free encyclopedia
 |
This article needs additional citations for verification. Please help improve this article by adding citations to reliable sources. Unsourced material may be challenged and removed. (December 2009) |
| Observation data Epoch J2000.0 Equinox J2000.0 |
|
|---|---|
| Constellation | Cassiopeia |
| Right ascension | 02h03m26.1s |
| Declination | +72°25′17″ |
| Apparent magnitude (V) | +3.95 |
| Distance | 162.1 ± 4.5 ly (49.7 ± 1.4 pc) |
| Spectral type | A2V |
| Other designations | |
50 Cassiopeiae is a star in the constellation Cassiopeia. In the past, it had been misidentified as a suspected nebula, and given the number NGC 771.
50 Cassiopeiae is a white A-type main sequence dwarf with an apparent magnitude of +3.95. It is approximately 162.1 light years from Earth.[1]
[edit] References
|
|||||||||||
| Astronomical catalogs | ||
|---|---|---|
| NGC: | NGC 769 - NGC 770 - NGC 771 - NGC 772 - NGC 773 | |
| HD: | HD 12214 - HD 12215 - HD 12216 - HD 12217 - HD 12218 | |
| HIP: | HIP 9596 - HIP 9597 - HIP 9598 - HIP 9599 - HIP 9600 | |
| SAO: | SAO 4558 - SAO 4559 - SAO 4560 - SAO 4561 - SAO 4562 | |
| GC: | GC 2443 - GC 2444 - GC 2445 - GC 2446 - GC 2447 | |
| HR: | HR 578 - HR 579 - HR 580 - HR 581 - HR 582 | |
 |
This main sequence star-related article is a stub. You can help Wikipedia by expanding it. |
