RSGC1-F02

RSGC1-F02 is a red supergiant star. It belongs to the open cluster RSGC1. It is located in the constellation of Scutum. Its radius was calculated to be between 1,499[5] to 1,549[6] times that of the Sun. The radius is calculated using the Stefan-Boltzmann law. It is one of the largest stars ever discovered. The star has a volume of 3.37 or 3.72 billion times bigger than the Sun.

RSGC1-F02
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Open cluster RSGC1 in which RSGC-F02 is located.
Credit: Spitzer
Observation data
Epoch J2000      Equinox J2000
Constellation Scutum
Right ascension 18h 37m 55.28s[1]
Declination -6° 52′ 48.4″[1]
Characteristics
Apparent magnitude (J) 9.904[1]
Apparent magnitude (H) 6.695[1]
Details
Radius1,128[2] R
Luminosity215,000[2] - 363,000[1][3][4] L
Temperature3,700[2] K
Other designations
RSGC1-F02, TIC 6841387
Database references
SIMBADdata

If RSGC1-F02 was placed at the center of the Solar System, its photosphere would reach the orbit of Jupiter.

References

  1. 1.0 1.1 1.2 1.3 1.4 Lua error in Module:Citation/CS1/Identifiers at line 630: attempt to index field 'known_free_doi_registrants_t' (a nil value).
  2. 2.0 2.1 2.2 Humphreys, Roberta M.; Helmel, Greta; Jones, Terry J.; Gordon, Michael S. (2020). "Exploring the Mass Loss Histories of the Red Supergiants". The Astronomical Journal. 160 (3): 145. arXiv:2008.01108. Bibcode:2020AJ....160..145H. doi:10.3847/1538-3881/abab15. S2CID 220961677.
  3. Lua error in Module:Citation/CS1/Identifiers at line 630: attempt to index field 'known_free_doi_registrants_t' (a nil value).
  4. Emma Bensor (2020). "A new mass-loss rate prescription for red supergiants". Monthly Notices of the Royal Astronomical Society. 492 (4): 5994–6006. arXiv:2001.07222. Bibcode:2020MNRAS.492.5994B. doi:10.1093/mnras/staa255. S2CID 210839222.
  5. Lua error in Module:Citation/CS1/Identifiers at line 630: attempt to index field 'known_free_doi_registrants_t' (a nil value).
  6. Lua error in Module:Citation/CS1/Identifiers at line 630: attempt to index field 'known_free_doi_registrants_t' (a nil value).