S Ursae Minoris

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S Ursae Minoris
File:SUMiLightCurve.png
The visual band light curve of S Ursae Minoris, from AAVSO data[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Ursa Minor
Right ascension 15h 29m 34.5775s[2]
Declination +78° 38′ 00.2742″[2]
Apparent magnitude (V) 7.5-<13.2[3]
Characteristics
Spectral type M6e-M9e[3]
Variable type long period variable[3]
Astrometry
Proper motion (μ) RA: −30.986±0.303[2] mas/yr
Dec.: 7.006±0.309[2] mas/yr
Parallax (π)2.5455 ± 0.1578 mas[2]
Distance1,280 ± 80 ly
(390 ± 20 pc)
Other designations
S UMi, HD 139492, HIP 75847[4]
Database references
SIMBADdata

S Ursae Minoris (S UMi) is a long period variable star in the constellation Ursa Minor, ranging from magnitude 7.5 to fainter than 13.2 over a period of 331 days.[3]

References

  1. "Download Data". aavso.org. AAVSO. Retrieved 1 October 2021.
  2. 2.0 2.1 2.2 2.3 2.4 Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  3. 3.0 3.1 3.2 3.3 Watson, Christopher (4 January 2010). "S Ursae Minoris". AAVSO Website. American Association of Variable Star Observers. Retrieved 10 March 2015.
  4. "S UMi". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-10-10.