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11 Lacertae

Coordinates:Sky map22h 40m 30.78s, +44° 16′ 34.6″
From Wikipedia, the free encyclopedia
Star in the constellation Lacerta
11 Lacertae

11 Lacertae in optical light
Observation data
Epoch J2000      Equinox J2000
ConstellationLacerta[1]
Right ascension22h 40m 30.85848s[2]
Declination+44° 16′ 34.7069″[2]
Apparent magnitude (V)4.46[3]
Characteristics
Spectral typeK2.5 III[4]
U−Bcolor index+1.36[3]
B−Vcolor index+1.33[3]
Astrometry
Radial velocity (Rv)−10.91±0.09[5] km/s
Proper motion (μ)RA: +93.728mas/yr[2]
Dec.: +10.946mas/yr[2]
Parallax (π)9.317±0.105 mas[2]
Distance350 ± 4 ly
(107 ± 1 pc)
Absolute magnitude (MV)−0.54[6]
Details
Mass1.38[7] M
Radius29.5±0.5[8] R
Luminosity279±10[9] L
Surface gravity (log g)1.56±0.06[9] cgs
Temperature4,352[10] K
Metallicity [Fe/H]−0.2±0.02[9] dex
Rotational velocity (v sin i)8[11] km/s
Age3.2[7] Gyr
Other designations
11 Lac,BD+43° 4266,HD 214868,HIP 111944,HR 8632,SAO 52251[12]
Database references
SIMBADdata

11 Lacertae is astar in the northernconstellation ofLacerta. It is visible to the naked eye as a faint orange-hued star with anapparent visual magnitude of 4.46.[3] It lies at a distance of about 350[2] light years and has anabsolute magnitude -0.54.[6] The object is moving closer to the Earth with a heliocentricradial velocity of −10.9 km/s.[5]

This is anevolvedgiant star with astellar classification of K2.5 III.[4] It is ared clump giant, meaning it is fusing helium in its core after passing through thered giant branch.[7] The star is 3.2[7] billion years old with 1.38 times themass of the Sun and has expanded to 39 times theSun's radius.[8] It is radiating 280[9] times theSun's luminosity from its enlargedphotosphere at aneffective temperature of 4,352 K.[10]

References

[edit]
  1. ^Roman, N. G. (1987)."Identification of a Constellation from a Position". Retrieved2006-12-26.
  2. ^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.
  3. ^abcdDucati, 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.
  4. ^abKeenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins catalog of revised MK types for the cooler stars".Astrophysical Journal Supplement Series.71: 245.Bibcode:1989ApJS...71..245K.doi:10.1086/191373.
  5. ^abFamaey, B.; et al. (2005). "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters".Astronomy and Astrophysics.430:165–186.arXiv:astro-ph/0409579.Bibcode:2005A&A...430..165F.doi:10.1051/0004-6361:20041272.S2CID 17804304.
  6. ^abAnderson, E.; Francis, Ch.; Niedzielski, A. (2012). "XHIP: An extended hipparcos compilation".Astronomy Letters.38 (5): 331.arXiv:1108.4971.Bibcode:2012AstL...38..331A.doi:10.1134/S1063773712050015.S2CID 119257644.
  7. ^abcdAdamczyk, M.; Deka-Szymankiewicz, B.; Niedzielski, A. (2016). "Masses and luminosities for 342 stars from the PennState-Toruń Centre for Astronomy Planet Search".Astronomy and Astrophysics.587: A119.arXiv:1510.07495.Bibcode:2016A&A...587A.119A.doi:10.1051/0004-6361/201526628.S2CID 119299522.
  8. ^abBaines, Ellyn K.; Thomas Armstrong, J.; Clark, James H.; Gorney, Jim; Hutter, Donald J.; Jorgensen, Anders M.; Kyte, Casey; Mozurkewich, David; Nisley, Ishara; Sanborn, Jason; Schmitt, Henrique R.; Van Belle, Gerard T. (2021)."Angular Diameters and Fundamental Parameters of Forty-four Stars from the Navy Precision Optical Interferometer".The Astronomical Journal.162 (5): 198.arXiv:2211.09030.Bibcode:2021AJ....162..198B.doi:10.3847/1538-3881/ac2431.
  9. ^abcdSoubiran, C.; Creevey, O. L.; Lagarde, N.; Brouillet, N.; Jofré, P.; Casamiquela, L.; Heiter, U.; Aguilera-Gómez, C.; Vitali, S.; Worley, C.; de Brito Silva, D. (2024-02-01). "Gaia FGK benchmark stars: Fundamental Teff and log g of the third version".Astronomy and Astrophysics.682: A145.arXiv:2310.11302.Bibcode:2024A&A...682A.145S.doi:10.1051/0004-6361/202347136.ISSN 0004-6361.11 Lacertae's database entry atVizieR.
  10. ^abMaldonado, J.; Villaver, E.; Niedzielski, A. (2016). "Evolved stars and the origin of abundance trends in planet hosts".Astronomy and Astrophysics.588: A98.arXiv:1602.00835.Bibcode:2016A&A...588A..98M.doi:10.1051/0004-6361/201527883.S2CID 119212009.
  11. ^Bernacca, P. L.; Perinotto, M. (1970). "A catalogue of stellar rotational velocities".Contributi Osservatorio Astronomico di Padova in Asiago.239 (1): 1.Bibcode:1970CoAsi.239....1B.
  12. ^"11 Lac".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-02-01.


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