HD 204521
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This infobox, "Template:Starbox begin", is from Wikipedia. The list of its authors can be seen in its edit history page. The data in this infobox may not agree or state what Wikipedia states. |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Cepheus |
| Right ascension | 21h 25m 16.798s[1] |
| Declination | +70° 28′ 39.15″ |
| Apparent magnitude (V) | 7.3[1] (binoculars) |
| Characteristics | |
| Spectral type | G0V[2] |
| Astrometry | |
| Radial velocity (Rv) | -76.6[3] km/s |
| Parallax (π) | 37.87 ± 0.42[3] mas |
| Distance | 86.1 ± 1.0 ly (26.4 ± 0.3 pc) |
| Details | |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 204521 is a potential Sun-like star (G5 spectral class) with an apparent magnitude of 7.3.[1] In the sky it is near the magnitude 3.2 star Beta Cephei (β Cep).
Bobylev's calculations from 2010 suggest that this star will pass about 2.20 parsecs (7.2 light-years) from the Sun in about 341 thousand years.[3]
See also[edit]
References[edit]
- ↑ 1.0 1.1 1.2 1.3 Lua error in Module:Citation/CS1 at line 379: attempt to call method 'match' (a nil value).
- ↑ Gray, R. O.; Corbally, C. J.; Garrison, R. F.; McFadden, M. T.; Robinson, P. E. (2003). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 Parsecs: The Northern Sample. I". The Astronomical Journal 126 (4): 2048. arXiv:astro-ph/0308182. Bibcode 2003AJ....126.2048G. doi:10.1086/378365.
- ↑ 3.0 3.1 3.2 Bobylev, Vadim V. (March 2010). "Searching for Stars Closely Encountering with the Solar System". Astronomy Letters 36 (3): 220–226. arXiv:1003.2160. Bibcode 2010AstL...36..220B. doi:10.1134/S1063773710030060.
Joey (talk), Natalia (talk), 
ynoss (talk), or 
Daniel (older account/talk).
External links[edit]
- Wikisky image of HD 204521 (HIP 105766)
- List of G stars within 100 light-years
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