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1 Puppis

From Wikipedia, the free encyclopedia
Star in the constellation Puppis
1 Puppis
Location of 1 Puppis (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationPuppis
Right ascension07h 43m 32.38668s[1]
Declination−28° 24′ 39.1887″[1]
Apparent magnitude (V)4.59[2]
Characteristics
Spectral typeM1III[3]
U−Bcolor index+1.94[2]
B−Vcolor index+1.63[2]
Astrometry
Radial velocity (Rv)+32.40[4] km/s
Proper motion (μ)RA: −13.782[1]mas/yr
Dec.: +29.646[1]mas/yr
Parallax (π)4.1384±0.1143 mas[1]
Distance790 ± 20 ly
(242 ± 7 pc)
Absolute magnitude (MV)−2.24[5]
Details
Radius84[6] R
Luminosity1,585 - 1,644[6] L
Surface gravity (log g)0.32[7] cgs
Temperature3,986±170[6] K
Metallicity [Fe/H]−0.19[7] dex
Rotational velocity (v sin i)1.0[8] km/s
Other designations
1 Pup,NSV 3708,CD−28°4767,GC 10409,HD 62576,HIP 37648,HR 2993,SAO 174391,CCDM J07435-2825A,WDS J07435-2825A,GSC 06552-03227[9]
Database references
SIMBADdata

1 Puppis is a single[10]star in the southernconstellation ofPuppis. It lies in the northern part of the constellation at a distance of about 790 ly, east ofAludra inCanis Major and just north of the white supergiant,3 Puppis. This object is visible to the naked eye as a faint, red-hued star with anapparent visual magnitude of 4.59. It is moving further from the Earth with a heliocentricradial velocity of +32.4 km/s.

Alight curve for 1 Puppis, plotted from Hipparcos data

TheHipparcos data for 1 Puppis shows low amplitude (0.007 magnitude) variability with a period of 1.8094 days.[11] The International Variable Star Index classifies the 1 Puppis as a star withstarspots that cause the brightness to change as it rotates, and which varies invisual magnitude from 4.58 to 4.63.[12]

This is ared giant star with astellar classification of M1 III,[3] having exhausted the hydrogen at itscore andevolved away from themain sequence. The star is radiating 1,509 times theluminosity of the Sun from its enlargedphotosphere at aneffective temperature of 4,111 K.[7] It has several visual companions: component B, of magnitude 13.7 andangular separation of26, C, of magnitude 9.21 and separation 78.8″, and D, of magnitude 10.84 and separation from C of 1.3″.[13] Component B is a background object.[14] Components C and D form the binary star HD 62557 and have a similar parallax andproper motion to 1 Puppis.[15][16]

References

[edit]
  1. ^abcdeVallenari, 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 atVizieR.
  2. ^abcDucati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system".CDS/ADC Collection of Electronic Catalogues.2237.Bibcode:2002yCat.2237....0D.
  3. ^abAbt, Helmut A. (2008)."Visual Multiples. IX. MK Spectral Types".The Astrophysical Journal Supplement Series.176 (1):216–217.Bibcode:2008ApJS..176..216A.doi:10.1086/525529.
  4. ^Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system".Astronomy Letters.32 (11):759–771.arXiv:1606.08053.Bibcode:2006AstL...32..759G.doi:10.1134/S1063773706110065.S2CID 119231169.
  5. ^Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation".Astronomy Letters.38 (5): 331.arXiv:1108.4971.Bibcode:2012AstL...38..331A.doi:10.1134/S1063773712050015.S2CID 119257644.Vizier catalog entry
  6. ^abcMessineo, M.; Brown, A. G. A. (2019)."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.S2CID 148571616.
  7. ^abcEarle Luck, R. (2014)."Parameters and Abundances in Luminous Stars".The Astronomical Journal.147 (6): 137.Bibcode:2014AJ....147..137L.doi:10.1088/0004-6256/147/6/137.
  8. ^Glebocki, R.; Gnacinski, P. (2005). "VizieR Online Data Catalog: Catalog of Stellar Rotational Velocities (Glebocki+ 2005)".VizieR On-line Data Catalog: III/244. Originally Published in: 2005csss...13..571G; 2005yCat.3244....0G.3244.Bibcode:2005yCat.3244....0G.Vizier catalog entry
  9. ^"1 Pup".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-04-13.
  10. ^Eggleton, P. P.; Tokovinin, A. A. (September 2008)."A catalogue of multiplicity among bright stellar systems".Monthly Notices of the Royal Astronomical Society.389 (2):869–879.arXiv:0806.2878.Bibcode:2008MNRAS.389..869E.doi:10.1111/j.1365-2966.2008.13596.x.S2CID 14878976.
  11. ^Koen, Chris; Eyer, Laurent (March 2002)."New periodic variables from the Hipparcos epoch photometry".Monthly Notices of the Royal Astronomical Society.331 (1):45–59.arXiv:astro-ph/0112194.Bibcode:2002MNRAS.331...45K.doi:10.1046/j.1365-8711.2002.05150.x.
  12. ^"NSV 3708".The International Variable Star Index. AAVSO. Retrieved3 October 2022.
  13. ^Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001)."The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog".The Astronomical Journal.122 (6): 3466.Bibcode:2001AJ....122.3466M.doi:10.1086/323920.Vizier catalog entry
  14. ^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 atVizieR.
  15. ^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 atVizieR.
  16. ^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 atVizieR.
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