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38 Geminorum

From Wikipedia, the free encyclopedia
Binary star system in the constellation Gemini
This article is about e Geminorum. Not to be confused withε (epsilon) Geminorum.
38 Geminorum

Alight curve for 38 Geminorum plotted fromTESS data[1]
Observation data
EpochJ2000      EquinoxJ2000
ConstellationGemini
Right ascension06h 54m 38.63478s[2]
Declination+13° 10′ 40.2207″[2]
Apparent magnitude (V)4.75 + 7.80[3]
Characteristics
Spectral typeA8V[4] + G6V[5]
U−Bcolor index+0.07[6]
B−Vcolor index+0.30[6]
Variable typeSuspected δ Sct[7]
Astrometry
A
Radial velocity (Rv)+24±5[8] km/s
Proper motion (μ)RA: 68.745[9]mas/yr
Dec.: −86.832[9]mas/yr
Parallax (π)33.9184±0.8248 mas[9]
Distance96 ± 2 ly
(29.5 ± 0.7 pc)
B
Radial velocity (Rv)+22.6±2[8] km/s
Proper motion (μ)RA: 89.235[10] mas/yr
Dec.: −77.171[10] mas/yr
Parallax (π)33.3308 ± 0.0847 mas[10]
Distance97.9 ± 0.2 ly
(30.00 ± 0.08 pc)
Details
38 Gem A
Mass1.55[11] M
Surface gravity (log g)4.23[12] cgs
Temperature7,410±252[12] K
Metallicity [Fe/H]−0.08±0.06[13] dex
Rotational velocity (v sin i)147.5±10.5[14] km/s
Age1.179[12] Gyr
38 Gem B
Mass0.89[11] M
Radius0.89[10] R
Luminosity0.694[10] L
Temperature5,583[10] K
Other designations
e Gem,38 Gem,NSV 3266,BD+13°1462,GJ 9220,HD 50635,HIP 33202,HR 2564,SAO 96265,WDS J06546+1311
Database references
SIMBADdata
A
B

38 Geminorum is abinary star system in the northernzodiacconstellation ofGemini. It has theBayer designatione Geminorum, while38 Geminorum is theFlamsteed designation. This system is visible to the naked eye as a faint, white-hued point of light with anapparent visual magnitude of 4.71. The primary component is a magnitude 4.75 star, while the secondary is magnitude 7.80.[3] The system is located about 98 light years away from the Sun based onparallax, and is drifting further away with aradial velocity of +16 km/s.[15] It is a potential member of theTucana–Horologium stellar kinematic group.[16]

This is a wide binary system with aprojected separation of184.3 AU.[11] Two sets of low qualityorbital elements have been computed for this system, yieldingperiods of 1,943.8 years and 3,190 years, andeccentricities of 0.150 and 0.485, respectively.[17] As of 2018, the pair had anangular separation of7.4 along aposition angle of 143°.[3]

Abt and Morrell (1995) classified the primary component as anA-type main-sequence star with astellar classification of A8V.[4] It is a suspectedchemically peculiar star of subtype CP1 (anAm star),[14] which Slettebak (1955) classified as kA8mF0Vp.[18] This notation indicates the star displays thecalcium K line of anA8 star and themetal lines of anF0V star. In 1949, J. Hopmann catalogued it as a suspectedDelta Scuti variable.[7] The secondary is aG-type main-sequence star with a class of G6V.[5]

References

[edit]
  1. ^"MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved11 September 2024.
  2. ^abvan 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.
  3. ^abcMason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog",The Astronomical Journal,122 (6): 3466,Bibcode:2001AJ....122.3466M,doi:10.1086/323920
  4. ^abAbt, Helmut A.; Morrell, Nidia I. (1995)."The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars".The Astrophysical Journal Supplement Series.99: 135.Bibcode:1995ApJS...99..135A.doi:10.1086/192182.
  5. ^abAdams, Walter S.; et al. (1935)."The Spectroscopic Absolute Magnitudes and Parallaxes of 4179 Stars".Astrophysical Journal.81: 187.Bibcode:1935ApJ....81..187A.doi:10.1086/143628.
  6. ^abJohnson, H. L. (1966). "UBVRIJKL Photometry of the Bright Stars".Communications of the Lunar and Planetary Laboratory.4: 99.Bibcode:1966CoLPL...4...99J.
  7. ^abStarikova, G. A. (July 1979). "Absolute magnitudes and masses for three types of variable stars".Soviet Astronomy Letters.5:188–192.Bibcode:1979SvAL....5..188S.
  8. ^abEvans, D. S. (1967). "The Revision of the General Catalogue of Radial Velocities".Determination of Radial Velocities and Their Applications.30: 57.Bibcode:1967IAUS...30...57E.
  9. ^abcBrown, 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. ^abcdefBrown, 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.
  11. ^abcTokovinin, A.; Kiyaeva, O. (February 2016)."Eccentricity distribution of wide binaries".Monthly Notices of the Royal Astronomical Society.456 (2):2070–2079.arXiv:1512.00278.Bibcode:2016MNRAS.456.2070T.doi:10.1093/mnras/stv2825.S2CID 1615080.
  12. ^abcDavid, Trevor J.; Hillenbrand, Lynne A. (2015). "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets".The Astrophysical Journal.804 (2): 146.arXiv:1501.03154.Bibcode:2015ApJ...804..146D.doi:10.1088/0004-637X/804/2/146.S2CID 33401607.
  13. ^Gáspár, András; et al. (2016)."The Correlation between Metallicity and Debris Disk Mass".The Astrophysical Journal.826 (2): 171.arXiv:1604.07403.Bibcode:2016ApJ...826..171G.doi:10.3847/0004-637X/826/2/171.S2CID 119241004.
  14. ^abPaunzen, E.; et al. (February 2013)."A photometric study of chemically peculiar stars with the STEREO satellites - II. Non-magnetic chemically peculiar stars".Monthly Notices of the Royal Astronomical Society.429 (1):119–125.arXiv:1211.1535.Bibcode:2013MNRAS.429..119P.doi:10.1093/mnras/sts318.S2CID 119231581.
  15. ^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.
  16. ^Nakajima, Tadashi; Morino, Jun-Ichi (2012)."Potential Members of Stellar Kinematic Groups within 30 pc of the Sun".The Astronomical Journal.143 (1): 2.Bibcode:2012AJ....143....2N.doi:10.1088/0004-6256/143/1/2.
  17. ^Abt, Helmut A. (August 2005)."Observed Orbital Eccentricities".The Astrophysical Journal.629 (1):507–511.Bibcode:2005ApJ...629..507A.doi:10.1086/431207.
  18. ^Slettebak, Arne (May 1955)."The Spectra and Rotational Velocities of the Bright Stars of Draper Types A3-G0".Astrophysical Journal.121: 653.Bibcode:1955ApJ...121..653S.doi:10.1086/146031.
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