R Octantis
R Octantis is a Mira variable star located in the southern constellation of Octans. It shines with a luminosity 9304 times that of the Sun and has a surface temperature of 2571 K.[5]
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Octans | 
| Right ascension | 05h 26m 06.19562s[2] | 
| Declination | −86° 23′ 17.7741″[2] | 
| Apparent magnitude (V) | 6.4-13.2[3] | 
| Characteristics | |
| Spectral type | M5.5e | 
| Variable type | Mira | 
| Astrometry | |
| Radial velocity (Rv) | 46.00 ± 4.7 km/s | 
| Proper motion (μ) | RA: 1.26 ± 0.61[2] mas/yr Dec.: 28.97 ± 0.94[2] mas/yr | 
| Parallax (π) | 1.9834 ± 0.1669 mas[4] | 
| Distance | 1,600 ± 100 ly (500 ± 40 pc) | 
| Details | |
| Luminosity | 9304[5] L☉ | 
| Temperature | 2571[5] K | 
| Other designations | |
| Database references | |
| SIMBAD | data | 
References
    
- "Download Data". aavso.org. AAVSO. Retrieved 1 October 2021.
- 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. S2CID 18759600. Vizier catalog entry
- Otero, Sebastian (26 April 2011). "R Octantis". AAVSO Website. American Association of Variable Star Observers. Retrieved 21 April 2016.
- Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (2012). "Fundamental Parameters and Infrared Excesses of Hipparcos Stars". Monthly Notices of the Royal Astronomical Society. 427 (1): 343–57. arXiv:1208.2037. Bibcode:2012MNRAS.427..343M. doi:10.1111/j.1365-2966.2012.21873.x. S2CID 118665352.
- "V* R Oct". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 21 April 2016.
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