astro.wikisort.org - StarR Apodis (R Aps) is a star in the constellation Apus.
Variable star in the constellation Apus
R Apodis
Observation data Epoch J2000 Equinox J2000 |
Constellation |
Apus |
Right ascension |
14h 57m 52.98366s[1] |
Declination |
−76° 39′ 45.5556″[1] |
Apparent magnitude (V) |
5.34[2] |
Characteristics |
Spectral type |
K4 III:[3] |
U−B color index |
1.70[2] |
B−V color index |
1.45[2] |
Variable type |
constant[4] |
Astrometry |
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Radial velocity (Rv) | -31.2[5] km/s |
Proper motion (μ) | RA: −68.997[6] mas/yr Dec.: −16.232[6] mas/yr |
Parallax (π) | 8.4408 ± 0.1632 mas[6] |
Distance | 386 ± 7 ly (118 ± 2 pc) |
Absolute magnitude (MV) | −0.22 ± 0.16[7] |
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Details |
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Mass | 1.10 ± 0.18[5] M☉ |
Radius | 22.94 ± 1.65[5] R☉ |
Luminosity | 229+59 −47[5] L☉ |
Surface gravity (log g) | 1.99 ± 0.05[5] cgs |
Temperature | 4318 ± 38[5] K |
Metallicity [Fe/H] | −0.29 ± 0.05[5] dex |
Rotational velocity (v sin i) | 2.64[5] km/s |
Age | 5.68 ± 2.42[5] Gyr |
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Other designations |
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HR 5540, HD 131109, HIP 73223, SAO 257212, CD-76°688, CPD-76°924, IRAS 14520-7627, GSC 09428-02897, 2MASS J14575300-7639454, TYC 9428-2897-1, AAVSO 1446-76, FK5 3175, PLX 3358, GC 20057, PPM 372479, GCRV 8654 |
Database references |
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SIMBAD | data |
R Apodis is an orange K-type giant with an apparent magnitude of +5.34. It is approximately 386 light years from Earth. It was earlier suspected to be a variable star and given the variable star designation R Apodis. Now it is confirmed as a non-variable.[8]
R Apodis has exhausted its core hydrogen fuel and left the main sequence. It has a mass 10% higher than the Sun's, and it has cooled to 4,318 K and expanded to 23 times the radius of the Sun. Despite being cooler than the sun, its large size means it emits 229 times more electromagnetic radiation.
References
- van Leeuwen, F. (November 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.
- Hoffleit, Dorrit; Jaschek, Carlos (1991). The Bright star catalogue. Bibcode:1991bsc..book.....H.
- Keenan, Philip C; McNeil, Raymond C (1989). "The Perkins catalog of revised MK types for the cooler stars". Astrophysical Journal Supplement Series. 71: 245. Bibcode:1989ApJS...71..245K. doi:10.1086/191373.
- Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1: B/gcvs. Bibcode:2009yCat....102025S.
- Jofré, E; Petrucci, R; Saffe, C; Saker, L; de la Villarmois, E. Artur; Chavero, C; Gómez, M; Mauas, P. J. D (2015). "Stellar parameters and chemical abundances of 223 evolved stars with and without planets". Astronomy & Astrophysics. 574: A50. arXiv:1410.6422. Bibcode:2015A&A...574A..50J. doi:10.1051/0004-6361/201424474. S2CID 53666931.
- 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.
- da Silva, L.; et al. (November 2006). "Basic physical parameters of a selected sample of evolved stars". Astronomy and Astrophysics. 458 (2): 609–623. arXiv:astro-ph/0608160. Bibcode:2006A&A...458..609D. doi:10.1051/0004-6361:20065105. S2CID 9341088.
- "R Aps". The International Variable Star Index. AAVSO – American Association of Variable Star Observers. Retrieved 10 April 2016.
Constellation of Apus |
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Stars | |
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Exoplanets |
- HD 131664 b
- HD 137388 b (Kererū)
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Star clusters | |
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 Category |
На других языках
- [en] R Apodis
[es] R Apodis
R Apodis (R Aps / HD 131109 / HR 5540 / HIP 73223)[1][2] es una estrella de la constelación de Apus, el ave del paraíso, de magnitud aparente +5,38. A pesar de llevar la denominación de estrellas variables «R» —indicando que fue la primera variable descubierta en la constelación—, observaciones posteriores han descartado dicha variabilidad. Se encuentra a 374 años luz de distancia del Sistema Solar.
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