SP77 46-44
From EverybodyWiki Bios & Wiki
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Dorado[1] |
| Right ascension | 05h 29m 42.2038s[2] |
| Declination | −68° 57′ 17.351″[2] |
| Apparent magnitude (V) | 11.54 (var.)[3] |
| Characteristics | |
| Evolutionary stage | Red supergiant |
| Spectral type | M2.5 Ia-Iab[4] |
| Apparent magnitude (B) | 14.04[5] |
| Apparent magnitude (V) | 12.15[5] |
| Apparent magnitude (R) | 10.99[5] |
| Apparent magnitude (J) | 7.922±0.024[6] |
| Apparent magnitude (H) | 7.192±0.047[6] |
| Apparent magnitude (K) | 6.886±0.029[6] |
| B−V color index | 1.89 |
| V−R color index | 1.16 |
| J−H color index | 0.730 |
| J−K color index | 1.036 |
| Variable type | yes[3] |
| Astrometry | |
| Radial velocity (Rv) | 273.0±0.3[5] km/s |
| Proper motion (μ) | RA: 1.445[2] mas/yr Dec.: 0.463[2] mas/yr |
| Details | |
| Radius | 1,278[lower-alpha 1] R☉ |
| Luminosity | 221,000[7] – 251,000[8] L☉ |
| Surface gravity (log g) | 0.5[7] cgs |
| Temperature | 3,500[7] K |
| Other designations | |
| Database references | |
| SIMBAD | data |
SP77 46-44 (WOH S341) is a red supergiant star found in the Large Magellanic Cloud in the constellation of Dorado. It is one of the largest stars discovered, with a radius over 1,200 solar radii. If placed in the Solar System, its photosphere would engulf the orbit of Jupiter.
The apparent magnitude of SP77 46-44 varies by about 0.8 magnitudes around 11.5.[3] No variable star classification has been assigned.[10]
Notes[edit]
- ↑ Applying the Stefan–Boltzmann law with a nominal solar effective temperature of 5,772 K:
References[edit]
- ↑ Staff (2 August 2008). "Finding the constellation which contains given sky coordinates". DJM.cc. Retrieved 16 July 2020.
- ↑ 2.0 2.1 2.2 2.3 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.
- ↑ 3.0 3.1 3.2 Szczygieł, D. M.; Stanek, K. Z.; Bonanos, A. Z.; Pojmański, G.; Pilecki, B.; Prieto, J. L. (2010). "Variability of Luminous Stars in the Large Magellanic Cloud Using 10 Years of ASAS Data". The Astronomical Journal. 140 (1): 14. arXiv:1001.3410. Bibcode:2010AJ....140...14S. doi:10.1088/0004-6256/140/1/14. Unknown parameter
|s2cid=ignored (help) - ↑ González-Fernández, Carlos; Dorda, Ricardo; Negueruela, Ignacio; Marco, Amparo (2015). "A new survey of cool supergiants in the Magellanic Clouds". Astronomy & Astrophysics. 578: A3. arXiv:1504.00003. Bibcode:2015A&A...578A...3G. doi:10.1051/0004-6361/201425362. Unknown parameter
|s2cid=ignored (help) - ↑ 5.0 5.1 5.2 5.3 Massey, Philip; Olsen, K. A. G. (2003). "The Evolution of Massive Stars. I. Red Supergiants in the Magellanic Clouds". The Astronomical Journal. 126 (6): 2867–2886. arXiv:astro-ph/0309272. Bibcode:2003AJ....126.2867M. doi:10.1086/379558. Unknown parameter
|s2cid=ignored (help) - ↑ 6.0 6.1 6.2 Cutri, Roc M.; Skrutskie, Michael F.; Van Dyk, Schuyler D.; Beichman, Charles A.; Carpenter, John M.; Chester, Thomas; Cambresy, Laurent; Evans, Tracey E.; Fowler, John W.; Gizis, John E.; Howard, Elizabeth V.; Huchra, John P.; Jarrett, Thomas H.; Kopan, Eugene L.; Kirkpatrick, J. Davy; Light, Robert M.; Marsh, Kenneth A.; McCallon, Howard L.; Schneider, Stephen E.; Stiening, Rae; Sykes, Matthew J.; Weinberg, Martin D.; Wheaton, William A.; Wheelock, Sherry L.; Zacarias, N. (2003). "VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)". CDS/ADC Collection of Electronic Catalogues. 2246: II/246. Bibcode:2003yCat.2246....0C.
- ↑ 7.0 7.1 7.2 Groenewegen, Martin A. T.; Sloan, Greg C. (2018). "Luminosities and mass-loss rates of Local Group AGB stars and Red Supergiants". Astronomy & Astrophysics. 609: A114. arXiv:1711.07803. Bibcode:2018A&A...609A.114G. doi:10.1051/0004-6361/201731089. ISSN 0004-6361. Unknown parameter
|s2cid=ignored (help) - ↑ Davies, Ben; Crowther, Paul A.; Beasor, Emma R. (2018). "The luminosities of cool supergiants in the Magellanic Clouds, and the Humphreys–Davidson limit revisited". Monthly Notices of the Royal Astronomical Society. 478 (3): 3138–3148. arXiv:1804.06417. Bibcode:2018MNRAS.478.3138D. doi:10.1093/mnras/sty1302. Unknown parameter
|s2cid=ignored (help) - ↑ "[W60] A27 -- Red supergiant star". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 1 August 2020.
- ↑ 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.
 | This supergiant-related article is a stub. You can help EverybodyWiki by expanding it. |
This article "SP77 46-44" is from Wikipedia. The list of its authors can be seen in its historical and/or the page Edithistory:SP77 46-44. Articles copied from Draft Namespace on Wikipedia could be seen on the Draft Namespace of Wikipedia and not main one.
