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10 Delphini

From Wikipedia, the free encyclopedia
K-type star in the constellation Delphinus
10 Delphini
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationDelphinus
Right ascension20h 41m 16.2079s[1]
Declination+14° 34′ 58.361″[1]
Apparent magnitude (V)6.00±0.01[2]
Characteristics
Evolutionary stagered giant branch[1]
Spectral typeK4 III[3]
U−Bcolor index+1.44[4]
B−Vcolor index+1.24[5]
Astrometry
Radial velocity (Rv)−32±2[6] km/s
Proper motion (μ)RA: −9.462mas/yr[1]
Dec.: −0.344mas/yr[1]
Parallax (π)6.6178±0.0397 mas[1]
Distance493 ± 3 ly
(151.1 ± 0.9 pc)
Absolute magnitude (MV)+0.06[7]
Details
Mass2.42±0.71[8] M
Radius18.47+1.02
−1.03
[9] R
Luminosity125±2[9] L
Surface gravity (log g)2.27[10] cgs
Temperature4,378[10] K
Metallicity[Fe/H]0.00[10] dex
Age794±33[8] Myr
Other designations
10 Del,AG+14°2269,BD+14°4393,GC 28826,HD 197121,HIP 102080,HR 7918,SAO 106384
Database references
SIMBADdata

10 Delphini (10 Del) is a solitarystar in the equatorialconstellationDelphinus. It has anapparent magnitude of 6.00, allowing it to be faintly seen with thenaked eye.Parallax measurements put the object at a distance of 493light years but is drifting closer with a heliocentricradial velocity of−32 km/s.

10 Delphini has astellar classification of K4 III[3] or K2 III,[11] both indicating that it is ared giant. However, there is some uncertainty behind the first classification. It has twice themass of the Sun[8] but at an age of 794million years[8] — expanded to 18 times theradius of the Sun.[9] It shines at125 L[9] from its enlargedphotosphere at aneffective temperature of 4,378K,[10] giving it an orange glow. 10 Del has a solarmetallicity.[10]

10 Del has been suspected to be a variable star, although it hasn't been catalogued as such in the GCVS.[12]

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. ^Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".Astronomy and Astrophysics.355:L27–L30.Bibcode:2000A&A...355L..27H.ISSN 0004-6361.
  3. ^abAdams, Walter S.; Joy, Alfred H.; Humason, Milton L.; Brayton, Ada Margaret (April 1935)."The Spectroscopic Absolute Magnitudes and Parallaxes of 4179 Stars".The Astrophysical Journal.81: 187.Bibcode:1935ApJ....81..187A.doi:10.1086/143628.ISSN 0004-637X.
  4. ^Paunzen, E. (May 2022)."Catalogue of stars measured in the Geneva seven-colour photometric system".Astronomy & Astrophysics.661: A89.arXiv:2111.04810.Bibcode:2022A&A...661A..89P.doi:10.1051/0004-6361/202142355.eISSN 1432-0746.ISSN 0004-6361.
  5. ^Haggkvist, L.; Oja, T. (1970). "Results of BV photometry 1969-70 (Uppsala refractor)".Private Communication.Bibcode:1970Priv.........0H.
  6. ^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. Revisiting the concept of superclusters".Astronomy and Astrophysics.430: 165.arXiv:astro-ph/0409579.Bibcode:2005A&A...430..165F.doi:10.1051/0004-6361:20041272.S2CID 17804304.
  7. ^Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation".Astronomy Letters.38 (5):331–346.arXiv:1108.4971.Bibcode:2012AstL...38..331A.doi:10.1134/S1063773712050015.ISSN 1063-7737.S2CID 255204555.
  8. ^abcdFeuillet, Diane K.; Bovy, Jo; Holtzman, Jon; Girardi, Léo; MacDonald, Nick; Majewski, Steven R.; Nidever, David L. (20 January 2016)."Determining Ages of Apogee Giants with Known Distances".The Astrophysical Journal.817 (1): 40.arXiv:1511.04088.Bibcode:2016ApJ...817...40F.doi:10.3847/0004-637X/817/1/40.eISSN 1538-4357.
  9. ^abcdBrown, 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 atVizieR.
  10. ^abcdeForsberg, R.; Jönsson, H.; Ryde, N.; Matteucci, F. (November 2019)."Abundances of disk and bulge giants from high-resolution optical spectra".Astronomy & Astrophysics.631: A113.arXiv:1909.10535.Bibcode:2019A&A...631A.113F.doi:10.1051/0004-6361/201936343.eISSN 1432-0746.ISSN 0004-6361.
  11. ^Bartkevicius, A.; Lazauskaite, R. (1 January 1997)."Classification of Population II Stars in the Vilnius Photometric System. II. Results".Open Astronomy.6 (4): 499.Bibcode:1997BaltA...6..499B.doi:10.1515/astro-1997-0402.eISSN 2543-6376.
  12. ^Samus’, N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (January 2017). "General catalogue of variable stars: Version GCVS 5.1".Astronomy Reports.61 (1):80–88.Bibcode:2017ARep...61...80S.doi:10.1134/S1063772917010085.ISSN 1063-7729.S2CID 255195566.
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