| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Carina |
| Right ascension | 09h 32m 14.59964s [2] |
| Declination | −62° 47′ 20.0452″ [2] |
| Apparent magnitude (V) | 3.9 - 10.5 [3] |
| Characteristics | |
| Evolutionary stage | AGB [4] |
| Spectral type | M6/7pe [5] |
| B−V color index | 0.906±0.009 [6] |
| Variable type | Mira [3] |
| Astrometry | |
| Radial velocity (Rv) | +28.1±1.0 [6] km/s |
| Proper motion (μ) |
RA: −37.900
[2]
mas/
yr Dec.: +22.232 [2] mas/ yr |
| Parallax (π) | 2.5813 ± 0.4460 mas [2] |
| Distance | approx. 1,300
ly (approx. 390 pc) |
| Absolute magnitude (MV) | 1.48 [6] (at mv = 7.43) |
| Details | |
| Mass | 0.87+0.47 −0.31 [4] M☉ |
| Radius | 241.0+37.6 −32.6 [4] R☉ |
| Luminosity | 4,571+1,331 −1,031 [4] L☉ |
| Temperature | 2,800 [7] K |
| Other designations | |
| Database references | |
| SIMBAD | data |
R Carinae is a double star in the southern constellation of Carina. The brighter component is a variable star that can be viewed with the naked eye at peak brightness, [9] but is usually too faint to be seen without a telescope, having an apparent visual magnitude that fluctuates around 7.43. [6] This star is located at a distance of approximately 1,300 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +28 km/s. [6]
The main component is an aging red giant star on the asymptotic giant branch [4] with a stellar classification of M6/7pe. [5] It is classified as a pulsating Mira type variable star and its visual brightness varies with an average amplitude of 4.25 magnitudes over a period of 303.99±1.08 d. Its average maximum visual magnitude is 5.05±0.45, [9] but the brightest observed maximum was magnitude 3.9 [3] This star is surrounded by a dusty shell, with properties that are consistent with iron-poor silicates or corundum, extending from around three stellar radii outward. [10]
The companion is a magnitude 11.30 star at an angular separation of 2.10 ″ along a position angle of 132° from the main star, as of 2015. [11]
References
- ^ "Download Data". aavso.org. AAVSO. Retrieved 1 October 2021.
- ^ a b c d e 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.
- ^ a b c Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, 5.1, 61 (1): 80–88, Bibcode: 2017ARep...61...80S, doi: 10.1134/S1063772917010085, S2CID 125853869.
- ^ a b c d e Takeuti, Mine; et al. (2013), "A Method to Estimate the Masses of Asymptotic Giant Branch Variable Stars", Publications of the Astronomical Society of Japan, 65 (3): 60, Bibcode: 2013PASJ...65...60T, doi: 10.1093/pasj/65.3.60.
- ^ a b Houk, Nancy; Cowley, A. P. (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan, Bibcode: 1978mcts.book.....H.
- ^ a b c d e Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID 119257644.
- ^ 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, arXiv: 1208.2037, Bibcode: 2012MNRAS.427..343M, doi: 10.1111/j.1365-2966.2012.21873.x, S2CID 118665352.
- ^ "R Car". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-01-30.
- ^ a b Vogt, N.; et al. (2016), "Determination of Pulsation Periods and Other Parameters of 2875 Stars Classified As Mira in the All Sky Automated Survey (Asas)", The Astrophysical Journal Supplement Series, 227 (1): 6, arXiv: 1609.05246, Bibcode: 2016ApJS..227....6V, doi: 10.3847/0067-0049/227/1/6, S2CID 119295645.
- ^ Ireland, M. J.; et al. (July 2005), "Dust scattering in the Miras R Car and RR Sco resolved by optical interferometric polarimetry", Monthly Notices of the Royal Astronomical Society, 361 (1): 337–344, arXiv: astro-ph/0505112, Bibcode: 2005MNRAS.361..337I, doi: 10.1111/j.1365-2966.2005.09181.x, S2CID 14724805.
- ^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466, Bibcode: 2001AJ....122.3466M, doi: 10.1086/323920.
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| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Carina |
| Right ascension | 09h 32m 14.59964s [2] |
| Declination | −62° 47′ 20.0452″ [2] |
| Apparent magnitude (V) | 3.9 - 10.5 [3] |
| Characteristics | |
| Evolutionary stage | AGB [4] |
| Spectral type | M6/7pe [5] |
| B−V color index | 0.906±0.009 [6] |
| Variable type | Mira [3] |
| Astrometry | |
| Radial velocity (Rv) | +28.1±1.0 [6] km/s |
| Proper motion (μ) |
RA: −37.900
[2]
mas/
yr Dec.: +22.232 [2] mas/ yr |
| Parallax (π) | 2.5813 ± 0.4460 mas [2] |
| Distance | approx. 1,300
ly (approx. 390 pc) |
| Absolute magnitude (MV) | 1.48 [6] (at mv = 7.43) |
| Details | |
| Mass | 0.87+0.47 −0.31 [4] M☉ |
| Radius | 241.0+37.6 −32.6 [4] R☉ |
| Luminosity | 4,571+1,331 −1,031 [4] L☉ |
| Temperature | 2,800 [7] K |
| Other designations | |
| Database references | |
| SIMBAD | data |
R Carinae is a double star in the southern constellation of Carina. The brighter component is a variable star that can be viewed with the naked eye at peak brightness, [9] but is usually too faint to be seen without a telescope, having an apparent visual magnitude that fluctuates around 7.43. [6] This star is located at a distance of approximately 1,300 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +28 km/s. [6]
The main component is an aging red giant star on the asymptotic giant branch [4] with a stellar classification of M6/7pe. [5] It is classified as a pulsating Mira type variable star and its visual brightness varies with an average amplitude of 4.25 magnitudes over a period of 303.99±1.08 d. Its average maximum visual magnitude is 5.05±0.45, [9] but the brightest observed maximum was magnitude 3.9 [3] This star is surrounded by a dusty shell, with properties that are consistent with iron-poor silicates or corundum, extending from around three stellar radii outward. [10]
The companion is a magnitude 11.30 star at an angular separation of 2.10 ″ along a position angle of 132° from the main star, as of 2015. [11]
References
- ^ "Download Data". aavso.org. AAVSO. Retrieved 1 October 2021.
- ^ a b c d e 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.
- ^ a b c Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, 5.1, 61 (1): 80–88, Bibcode: 2017ARep...61...80S, doi: 10.1134/S1063772917010085, S2CID 125853869.
- ^ a b c d e Takeuti, Mine; et al. (2013), "A Method to Estimate the Masses of Asymptotic Giant Branch Variable Stars", Publications of the Astronomical Society of Japan, 65 (3): 60, Bibcode: 2013PASJ...65...60T, doi: 10.1093/pasj/65.3.60.
- ^ a b Houk, Nancy; Cowley, A. P. (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan, Bibcode: 1978mcts.book.....H.
- ^ a b c d e Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID 119257644.
- ^ 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, arXiv: 1208.2037, Bibcode: 2012MNRAS.427..343M, doi: 10.1111/j.1365-2966.2012.21873.x, S2CID 118665352.
- ^ "R Car". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-01-30.
- ^ a b Vogt, N.; et al. (2016), "Determination of Pulsation Periods and Other Parameters of 2875 Stars Classified As Mira in the All Sky Automated Survey (Asas)", The Astrophysical Journal Supplement Series, 227 (1): 6, arXiv: 1609.05246, Bibcode: 2016ApJS..227....6V, doi: 10.3847/0067-0049/227/1/6, S2CID 119295645.
- ^ Ireland, M. J.; et al. (July 2005), "Dust scattering in the Miras R Car and RR Sco resolved by optical interferometric polarimetry", Monthly Notices of the Royal Astronomical Society, 361 (1): 337–344, arXiv: astro-ph/0505112, Bibcode: 2005MNRAS.361..337I, doi: 10.1111/j.1365-2966.2005.09181.x, S2CID 14724805.
- ^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466, Bibcode: 2001AJ....122.3466M, doi: 10.1086/323920.
| Stars |
| ||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| |||||||||||
|
Star clusters |
| ||||||||||
| Nebulae |
| ||||||||||
| Galaxies |
| ||||||||||
| |||||||||||
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