V762_Cassiopeiae

V762 Cassiopeiae

V762 Cassiopeiae

Star in the constellation Cassiopeia


V762 Cassiopeiae is a K-type red supergiant[3] located about 2,500 light-years away in the Cassiopeia constellation.[2] Its apparent magnitude is 5.86, which makes it visible to the naked eye.[2] It is a relatively cool star with an average surface temperature of 3645 K.[5]

Quick Facts Constellation, Right ascension ...

Characteristics

This is an evolved K-type red supergiant star with a spectral type of K0 I.[3] It has around 16.9 times the Sun's mass, and its age is estimated to be 10 million years.[4] It radiates 12,470 times the solar luminosity[3] from its outer atmosphere at an effective temperature of 3645 K.[5] V762 Cassiopeiae is located 2,480 light-years away, based in a parallax from Gaia DR3, and is moving towards Earth at a velocity of 21.37 km/s.[1][lower-alpha 2]

Distance and titleholding

Some websites claim V762 Cassiopeiae is the "farthest star visible to the naked eye", at a distance of 16,308 light-years.[6][7] This is inconsistent with parallax measurements from both Hipparcos, which found a parallax of 1.18±0.45 mas, corresponding to a distance of about 2,800 light-years,[8] and Gaia DR3, which lists a parallax of 1.3148±0.0693 mas, corresponding to a distance of about 2,500 light-years.[1][lower-alpha 2] The websites claiming that V762 Cassiopeiae is the "farthest star visible to the naked eye" also do not cite any references for the distance of 16,308 light-years, making the origin of this value uncertain.


References

  1. Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  2. Messineo, M.; Brown, A. G. A. (2019-07-01). "A Catalog of Known Galactic K-M Stars of Class I Candidate Red Supergiants in Gaia DR2". The Astronomical Journal. 158 (1): 20. arXiv:1905.03744. Bibcode:2019AJ....158...20M. doi:10.3847/1538-3881/ab1cbd. ISSN 0004-6256. Data can be acessed here at VizieR.
  3. Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (2011-01-01). "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun". Monthly Notices of the Royal Astronomical Society. 410 (1): 190–200. arXiv:1007.4883. Bibcode:2011MNRAS.410..190T. doi:10.1111/j.1365-2966.2010.17434.x. ISSN 0035-8711. Data can be acessed here at VizieR.
  4. McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (2012-11-01). "Fundamental parameters and infrared excesses of Hipparcos stars". Monthly Notices of the Royal Astronomical Society. 427 (1): 343–357. arXiv:1208.2037. Bibcode:2012MNRAS.427..343M. doi:10.1111/j.1365-2966.2012.21873.x. ISSN 0035-8711.
  5. "Farthest Star You Can See With The Unaided Eye". Cosmoknowledge. 2021-03-26. Retrieved 2024-04-11.
  6. "How Far Back In Time Can We See With Our Naked Eye?". Big Think. 2021-05-17. Retrieved 2024-04-11.
  7. "HIP 5926". VizieR. Centre de données astronomiques de Strasbourg. Retrieved 11 April 2024.
  1. Derived from a bolometric magnitude of -5.42.
  2. From the equation 1/(P/1000)=D, where P is the parallax in milliarcseconds and D is the distance in parsecs.

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