V538 Carinae is a
variable star in the constellation of
Carina, and a possible
red supergiant. If this star replaced the Sun in the
Solar System, its photosphere would at least engulf the orbit of Mars.
Properties
V538 Carinae has a measured angular diameter of 3.4
mas.[7] Its distance is uncertain. At the
Hipparcos distance of 1.33+5.81 −0.59kpc, this corresponds to a radius of 580 R☉,[6] but at the distance implied by its
Gaia Data Release 2 parallax, the radius would be around 1,900 R☉.[7] Calculations based on the Gaia DR2 parallax with temperatures and bolometric corrections inferred from Gaia colours give an even larger radius above 2,200 R☉.[8]
Some studies suggest that this star is a luminous
AGB star and a
long-period variable, instead of a supergiant.[9] It is classified in the
General Catalogue of Variable Stars as a
semiregular variable star of type SRb, indicating a cool pulsating giant star, with a possible period of 655 days. Its brightness varies between extremes of magnitude 7.7 and 9.2.[3]
^
abcSamus, 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.
^Pickles, A.; Depagne, É. (2010). "All-Sky Spectrally Matched UBVRI - ZY and u′ g′ r′ i′ z′ Magnitudes for Stars in the Tycho2 Catalog". Publications of the Astronomical Society of the Pacific. 122 (898): 1437.
arXiv:1011.2020.
Bibcode:
2010PASP..122.1437P.
doi:
10.1086/657947.
S2CID54678796.
^Skiff, B. A. (2014). "VizieR Online Data Catalog: Catalogue of Stellar Spectral Classifications (Skiff, 2009-2016)". VizieR On-line Data Catalog: B/Mk. Originally Published in: Lowell Observatory (October 2014). 1.
Bibcode:
2014yCat....1.2023S.