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Eta Leporis

From Wikipedia, the free encyclopedia
Star in the constellation of Lepus
η Leporis
Location of η Leporis (circled in red)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationLepus
Right ascension05h 56m 24.29300s[1]
Declination−14° 10′ 03.7189″[1]
Apparent magnitude (V)3.72[2]
Characteristics
Spectral typeF2 V[3]
U−Bcolor index+0.01[2]
B−Vcolor index+0.33[2]
R−Icolor index+0.16[4]
Astrometry
Radial velocity (Rv)−1.6±0.2[5] km/s
Proper motion (μ)RA: −42.06[1]mas/yr
Dec.: +139.26[1]mas/yr
Parallax (π)67.21±0.25 mas[1]
Distance48.5 ± 0.2 ly
(14.88 ± 0.06 pc)
Absolute magnitude (MV)+2.85[6]
Details
Mass1.42[5] M
Radius1.52[7] R
Luminosity6.03[6] L
Surface gravity (log g)4.13[5] cgs
Temperature6,899±80[5] K
Metallicity[Fe/H]−0.19[5] dex
Rotational velocity (v sin i)26[8] km/s
Age1.80[5] Gyr
Other designations
η Lep,16 Leporis,BD−14°1286,FK5 226,GC 7492,GJ 225,HD 40136,HIP 28103,HR 2085,SAO 150957,PPM 216474[9]
Database references
SIMBADdata

Eta Leporis,Latinised from η Leporis, is a single,[10] yellow-white-huedstar in thesouthernconstellation ofLepus, the hare. It is visible to the naked eye with anapparent visual magnitude of approximately 3.72.[2] The annualparallax shift of 67.21 mas yields a distance estimate of 49 light-years. It is moving closer to theSun with aradial velocity of −1.6 km/s.[5]

This is an ordinaryF-type main-sequence star with astellar classification of F2 V.[3] It is about 1.8[5] billion years old and spinning with aprojected rotational velocity of 26 km/s.[8] The star has 1.4[5] times themass of the Sun and 1.5[7] times theSun's radius. It shines with six[6] times theSun's luminosity, which is being radiated from itsphotosphere at aneffective temperature of around6,899 K.[5] Using the IRS instrument on theSpitzer Space Telescope,excess infrared emission has been observed from the star, which can be modeled by adust disk extending from 1 to 16astronomical units from Eta Leporis.[11]

References

[edit]
  1. ^abcdevan Leeuwen, F. (2007)."Validation of the new Hipparcos reduction".Astronomy and Astrophysics.474 (2):653–664.arXiv:0708.1752.Bibcode:2007A&A...474..653V.doi:10.1051/0004-6361:20078357.S2CID 18759600.Vizier catalog entry
  2. ^abcdJohnson, H. L.; et al. (1966). "UBVRIJKL photometry of the bright stars".Communications of the Lunar and Planetary Laboratory.4 (99): 99.Bibcode:1966CoLPL...4...99J.
  3. ^abGray, R. O.; Corbally, C. J.; Garrison, R. F.; McFadden, M. T.; Bubar, E. J.; McGahee, C. E.; O'Donoghue, A. A.; Knox, E. R. (2006). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 pc-The Southern Sample".The Astronomical Journal.132 (1):161–170.arXiv:astro-ph/0603770.Bibcode:2006AJ....132..161G.doi:10.1086/504637.S2CID 119476992.
  4. ^Hoffleit, D.; Warren, Jr., W. H.The Bright Star Catalogue (5th Revised (Preliminary Version) ed.).HR 2085, database entry,CDS IDV/50. Accessed on line February 3, 2011.
  5. ^abcdefghijCasagrande, L.; et al. (June 2011). "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey".Astronomy and Astrophysics.530: A138.arXiv:1103.4651.Bibcode:2011A&A...530A.138C.doi:10.1051/0004-6361/201016276.S2CID 56118016.
  6. ^abcAnderson, 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.S2CID 119257644.Vizier catalog entry
  7. ^abRhee, Joseph H.; et al. (May 2007), "Characterization of Dusty Debris Disks: The IRAS and Hipparcos Catalogs",The Astrophysical Journal,660 (2):1556–1571,arXiv:astro-ph/0609555,Bibcode:2007ApJ...660.1556R,doi:10.1086/509912,S2CID 11879505
  8. ^abZorec, J.; Royer, F. (2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities".Astronomy & Astrophysics.537: A120.arXiv:1201.2052.Bibcode:2012A&A...537A.120Z.doi:10.1051/0004-6361/201117691.S2CID 55586789.
  9. ^"eta Lep".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2017-12-27.
  10. ^Eggleton, P. P.; Tokovinin, A. A. (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. ^Lawler, S. M.; et al. (November 2009). "Explorations Beyond the Snow Line: Spitzer/IRS Spectra of Debris Disks Around Solar-type Stars".The Astrophysical Journal.705 (1):89–111.arXiv:0909.0058.Bibcode:2009ApJ...705...89L.doi:10.1088/0004-637X/705/1/89.S2CID 1272803. See Table 7.
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