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R Cancri

From Wikipedia, the free encyclopedia
Variable star in the constellation Cancer
Not to be confused withRho Cancri.
R Cancri

Thevisual bandlight curve of R Cancri, from AAVSO data[1]
Observation data
Epoch J2000      Equinox J2000
ConstellationCancer
Right ascension08h 16m 33.82673s[2]
Declination+11° 43′ 34.4691″[2]
Apparent magnitude (V)6.07 - 12.3[3]
Characteristics
Spectral typeM6e-M9e[3]
U−Bcolor index0.49[4]
B−Vcolor index1.53[4]
Variable typeMira[3]
Astrometry
Radial velocity (Rv)35.42 ± 0.52[5] km/s
Proper motion (μ)RA: 0.635±0.195[2]mas/yr
Dec.: −10.785±0.106[2]mas/yr
Parallax (π)3.9375±0.1792 mas[2]
Distance854+36
−39
 ly
(262+11
−12
 pc)[6]
Details
Mass1.43[7] M
Radius371±37[8] R
Luminosity5,700[8][a] L
Surface gravity (log g)−0.69[7] cgs
Temperature2,604±300[8] K
Metallicity[Fe/H]+0.22[7] dex
Other designations
BD+12°1803,HD 69243,HIP 40534,HR 3248,SAO 97694
Database references
SIMBADdata

R Cancri is aMira variable in the constellationCancer. Located approximately 250 parsecs (830 ly) distant, it varies between magnitudes 6.07 and 12.3 over a period of approximately 357 days.[3] At its brightest, it is very faintly visible to thenaked eye.

Friedrich Magnus Schwerd discovered R Cancri in 1829.[9] It was one of the firstvariable stars to be discovered.[10]

Notes

[edit]
  1. ^Calculated using the given radius and temperature by theStefan-Boltzmann law.

References

[edit]
  1. ^"Download Data".aavso.org. AAVSO. Retrieved1 October 2021.
  2. ^abcdeBrown, A. G. A.; et al. (Gaia collaboration) (2021)."Gaia Early Data Release 3: Summary of the contents and survey properties".Astronomy & Astrophysics.649: A1.arXiv:2012.01533.Bibcode:2021A&A...649A...1G.doi:10.1051/0004-6361/202039657.S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source atVizieR.
  3. ^abcdVSX; Otero, S. A. (7 January 2011)."R Cancri".AAVSO Website.American Association of Variable Star Observers. Retrieved26 Jan 2021.
  4. ^abDucati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system".CDS/ADC Collection of Electronic Catalogues.2237: 0.Bibcode:2002yCat.2237....0D.
  5. ^Famaey, B.; Jorissen, A.; Luri, X.; Mayor, M.; Udry, S.; Dejonghe, H.; Turon, C. (2005). "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data".Astronomy and Astrophysics.430 (165):165–186.arXiv:astro-ph/0409579.Bibcode:2005A&A...430..165F.doi:10.1051/0004-6361:20041272.S2CID 17804304.
  6. ^Bailer-Jones, C. A. L.; Rybizki, J.; Fouesneau, M.; Demleitner, M.; Andrae, R. (2021-03-01)."Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3".The Astronomical Journal.161 (3): 147.arXiv:2012.05220.Bibcode:2021AJ....161..147B.doi:10.3847/1538-3881/abd806.ISSN 0004-6256. Data about this star can be seenhere.
  7. ^abcAnders, F.; Khalatyan, A.; Queiroz, A. B. A.; Chiappini, C.; Ardèvol, J.; Casamiquela, L.; Figueras, F.; Jiménez-Arranz, Ó.; Jordi, C.; Monguió, M.; Romero-Gómez, M.; Altamirano, D.; Antoja, T.; Assaad, R.; Cantat-Gaudin, T. (2022-02-01). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia EDR3 stars brighter than G = 18.5".Astronomy and Astrophysics.658: A91.arXiv:2111.01860.Bibcode:2022A&A...658A..91A.doi:10.1051/0004-6361/202142369.ISSN 0004-6361.Database atVizieR.
  8. ^abcKarovicova, I.; Wittkowski, M.; Ohnaka, K.; Boboltz, D. A.; Fossat, E.; Scholz, M. (2013-12-01)."New insights into the dust formation of oxygen-rich AGB stars".Astronomy & Astrophysics.560: A75.arXiv:1310.1924.Bibcode:2013A&A...560A..75K.doi:10.1051/0004-6361/201322376.ISSN 0004-6361.
  9. ^Cannon, Annie J. (1907)."Second catalogue of variable stars".Annals of Harvard College Observatory.55:1–94.Bibcode:1907AnHar..55....1C. Retrieved20 December 2024.
  10. ^"The First Known Variable Stars". Students for the Exploration and Development of Space. Retrieved1 January 2025.
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