GCIRS 7

GCIRS 7 is a red supergiant located in the Galactic Center. It is very bright and is one of the largest stars currently discovered, with a size about 960 solar radii.[2] If placed in our solar system, its photosphere would nearly engulf the orbit of Jupiter.[2]

GCIRS 7
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Sagittarius
Right ascension  17h 45m 39.987s[1]
Declination −29° 00 22.24[1]
Characteristics
Evolutionary stage Red supergiant
Spectral type M2[1]
Apparent magnitude (J) 14.197±0.137[1]
Apparent magnitude (H) 9.260±0.118[1]
Apparent magnitude (K) 6.503±0.017[1]
J−H color index 4.937
J−K color index 7.694
Details
Radius960±92,[2] 1,000±150[3] R
Luminosity189,000+42,000
−35,000
[2] L
Temperature3,600±195[2], 3,400[3] K
Age6.5 - 10[2] Myr
Other designations
GCIRS 7, 2MASS J17454004-2900225[1]
Database references
SIMBADdata

References

  1. "SIMBAD query result: GCIRS 7 -- Star". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved 5 June 2020.
  2. Paumard, T; Pfuhl, O; Martins, F; Kervella, P; Ott, T; Pott, J-U; Le Bouquin, JB; Breitfelder, J; Gillessen, S; Perrin, G; Burtscher, L; Haubois, X; Brandner, W (2014). "GCIRS 7, a pulsating M1 supergiant at the Galactic centre . Physical properties and age". Astronomy & Astrophysics. 568 (85): A85. arXiv:1406.5320. Bibcode:2014A&A...568A..85P. doi:10.1051/0004-6361/201423991.
  3. Pott, J.-U.; Eckart, A.; Glindemann, A.; Kraus, S.; Schöde, R.; Ghez, A. M.; Woillez, J.; Weigelt, G. (2008). "First VLTI infrared spectro-interferometry on GCIRS 7". Astronomy & Astrophysics. 487: 413–418. arXiv:0805.4408. Bibcode:2008A&A...487..413P. doi:10.1051/0004-6361:200809829.


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