Rho Serpentis
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Serpens | 
| Right ascension | 15h 51m 15.90985s [1] | 
| Declination | 20° 58′ 40.5166″ [1] | 
| Apparent magnitude (V) | 4.78 [2] | 
| Characteristics | |
| Spectral type | K5III [3] | 
| U−B color index | +1.88 [2] | 
| B−V color index | +1.54 [2] | 
| Astrometry | |
| Radial velocity (Rv) | -61.96[4] km/s | 
| Proper motion (μ) | RA: -53.32[1] mas/yr Dec.: +18.87[1] mas/yr | 
| Parallax (π) | 8.70 ± 0.30[1] mas | 
| Distance | 370 ± 10 ly (115 ± 4 pc) | 
| Absolute magnitude (MV) | -0.52 [5] | 
| Other designations | |
| Database references | |
| SIMBAD | data | 
Rho Serpentis (ρ Ser, ρ Serpentis) is a star in the constellation Serpens.
Rho Serpentis is an orange K-type giant with an apparent magnitude of +4.78.[2] It is approximately 375 light years from Earth.[1]
References
- 1 2 3 4 5 6 van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. Vizier catalog entry
- 1 2 3 4 Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues 2237: 0. Bibcode:2002yCat.2237....0D.
- 1 2 "Rho Serpentis". SIMBAD Astronomical Database. Retrieved 2015-10-17.
- ↑ Famaey, B.; et al. (January 2005), "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters", Astronomy and Astrophysics 430 (1): 165–186, arXiv:astro-ph/0409579, Bibcode:2005A&A...430..165F, doi:10.1051/0004-6361:20041272
- ↑  Absolute magnitude calculated as  , where , where is the star's absolute magnitude, is the star's absolute magnitude, is the star's apparent magnitude, and is the star's apparent magnitude, and is the star's measured parallax in arcseconds. is the star's measured parallax in arcseconds.
| 
 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
This article is issued from Wikipedia - version of the Thursday, April 21, 2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.