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HD 38529

Coordinates:Sky map05h 46m 34.9120s, +01° 10′ 05.496″
From Wikipedia, the free encyclopedia
Binary star system in the constellation Orion
HD 38529
Location of HD 38529 (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationOrion[1]
HD 38529 A
Right ascension05h 46m 34.91314s[2]
Declination+01° 10′ 05.5029″[2]
Apparent magnitude (V)+5.95[3]
HD 38529 B
Right ascension05h 46m 19.37663s[4]
Declination+01° 12′ 47.2640″[4]
Apparent magnitude (V)+13.35[5]
Characteristics
HD 38529 A
Evolutionary stagesubgiant[2]
Spectral typeG4IV[3]
B−Vcolor index0.773[3]
HD 38529 B
Evolutionary stagemain sequence[6]
Spectral typeM3.0V[5]
Astrometry
HD 38529 A
Radial velocity (Rv)30.19±0.12[2] km/s
Proper motion (μ)RA: −77.806mas/yr[2]
Dec.: −141.363mas/yr[2]
Parallax (π)23.5714±0.0422 mas[2]
Distance138.4 ± 0.2 ly
(42.42 ± 0.08 pc)
Absolute magnitude (MV)+2.81[3]
HD 38529 B
Radial velocity (Rv)30.94±0.43[4] km/s
Proper motion (μ)RA: −78.612mas/yr[4]
Dec.: −142.084mas/yr[4]
Parallax (π)23.7139±0.0168 mas[4]
Distance137.54 ± 0.10 ly
(42.17 ± 0.03 pc)
Absolute magnitude (MV)+10.23[citation needed]
Details
HD 38529 A
Mass1.479±0.037[7] M
Radius2.678±0.026[7] R
Luminosity6.16±0.15[7] L
Surface gravity (log g)3.83±0.06[8] cgs
Temperature5619±44[8] K
Metallicity[Fe/H]0.38±0.03[8] dex
Rotation37.0±0.4 d[8]
Rotational velocity (v sin i)3.20±0.50[8] km/s
Age3.07±0.39[7] Gyr
HD 38529 B
Mass0.494[9] M
Radius0.496[9] R
Luminosity0.033[9] L
Surface gravity (log g)4.74[9] cgs
Temperature3,487[9] K
Metallicity[Fe/H]0.39[6] dex
Rotational velocity (v sin i)17[6] km/s
Other designations
RAG 1,WDS J05466+0110AB[10]
HD 38529 A:BD+01°1126,HIP 27253,HR 1988,WDS J05466+0110A[11]
HD 38529 B:WDS J05466+0110B,LP 598-99,2MASS J05461937+0112471[12]
Database references
SIMBADA
B
Exoplanet Archivedata

HD 38529 (138 G. Orionis)[13] is abinary star system approximately 138light-years away in theconstellation ofOrion.

HD 38529 A

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HD 38529 A is a yellowsubgiantstar of spectral type G4IV,[14] though it has also been classified as amain sequencedwarf of type G4V[5] and a borderlinegiant star of type G8III/IV.[15] It is about 48% more massive than theSun.[7]

Two substellar companions are known in orbit around this star, including one with a mass near the deuterium fusion limit that is often used as the dividing line between giant planets andbrown dwarfs. There is adebris disk located at least 86astronomical units from the star.[16] Its orbit is probably mildly misaligned with the planetary orbits, by 21−45°.[17]

Planetary system

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In 2001, the planetHD 38529 b was discovered orbiting the star HD 38529 A byDebra Fischer and collaborators who detected it using theDoppler spectroscopy technique.[14] It has a mass at least 78% that ofJupiter and orbits very close to the star, just beyond the distance limit forhot Jupiters. It does nottransit the star.[8]

In 2003, a massivesuperjovian HD 38529 c was found orbiting at 3.68AU with aminimum mass of 12.7Jupiter masses.[3] Astrometric measurements from theHipparcos satellite gave a best fit inclination of 160° and atrue mass 37 times that of Jupiter, turning this planet into abrown dwarf.[18]

Further study of the system usingHubble Space Telescopeastrometry revised the mass of HD 38529 c downwards to 17.7 Jupiter masses and suggested the presence of an additional planet, orbiting in the gap between HD 38529 b and c.[19] The possible third planet was refuted after additional radial velocity measurements were collected.[8] Subsequent astrometric studies have found masses for HD 38529 c ranging from just10.4 MJ[20] to18 MJ,[17] with the most recent value as of 2025 being12.9 MJ.[21]

The HD 38529 A planetary system[a]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b≥0.8047±0.0139 MJ0.1278±0.000614.30978±0.000330.259±0.016
c12.93+0.70
−0.49
 MJ
3.604+0.043
−0.042
2127.8+3.3
−3.2
0.3507+0.0057
−0.0051
104.2+8.9
−11
°
Debris disk46+38
−27
208±54AU
71+10
−7
°

HD 38529 B

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HD 38529 B is acommon proper motion stellar companion to HD 38529 A at a projected distance of about ~12000astronomical units. The star is ared dwarf of spectral type M3.0V.[5] Wide binary stars such as HD 38529 AB have been shown to be vulnerable to disruption bygalactic tides and perturbations by passing stars.[22]

See also

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Notes

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  1. ^HD 38529 b: Henryet al. (2013)[8]
    HD 38529 c: Fenget al. (2025)[21]
    Debris disk: Xuanet al. (2020)[17]

References

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  1. ^Roman, Nancy G. (1987)."Identification of a constellation from a position".Publications of the Astronomical Society of the Pacific.99 (617): 695.Bibcode:1987PASP...99..695R.doi:10.1086/132034. Constellation record for this object atVizieR.
  2. ^abcdefVallenari, 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. ^abcdeFischer, Debra A.; et al. (2003)."A Planetary Companion to HD 40979 and Additional Planets Orbiting HD 12661 and HD 38529".The Astrophysical Journal.586 (2):1394–1408.Bibcode:2003ApJ...586.1394F.doi:10.1086/367889.
  4. ^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.
  5. ^abcdRaghavan, Deepak; et al. (2006)."Two Suns in The Sky: Stellar Multiplicity in Exoplanet Systems".The Astrophysical Journal.646 (1):523–542.arXiv:astro-ph/0603836.Bibcode:2006ApJ...646..523R.doi:10.1086/504823.
  6. ^abcKuznetsov, M. K.; Del Burgo, C.; Pavlenko, Ya. V.; Frith, J. (2019)."Characterization of a Sample of Southern M Dwarfs Using Harps and X-shooter Spectra".The Astrophysical Journal.878 (2): 134.Bibcode:2019ApJ...878..134K.doi:10.3847/1538-4357/ab1fe9.
  7. ^abcdeBall, Warrick H.; Chaplin, William J.; Nielsen, Martin B.; González-Cuesta, Lucia; Mathur, Savita; Santos, Ângela R G.; García, Rafael; Buzasi, Derek; Mosser, Benoît; Deal, Morgan; Stokholm, Amalie; Mosumgaard, Jakob Rørsted; Silva Aguirre, Victor; Nsamba, Benard; Campante, Tiago; Cunha, Margarida S.; Ong, Joel; Basu, Sarbani; Örtel, Sibel; Çelik Orhan, Z.; Yıldız, Mutlu; Stassun, Keivan; Kane, Stephen R.; Huber, Daniel (2020)."Robust asteroseismic properties of the bright planet host HD 38529".Monthly Notices of the Royal Astronomical Society.499 (4):6084–6093.arXiv:2010.07323.Bibcode:2020MNRAS.499.6084B.doi:10.1093/mnras/staa3190.S2CID 222378164.
  8. ^abcdefghHenry, Gregory W.; et al. (2013)."Host Star Properties and Transit Exclusion for the HD 38529 Planetary System".The Astrophysical Journal.768 (2). 155.arXiv:1303.4735.Bibcode:2013ApJ...768..155H.doi:10.1088/0004-637X/768/2/155.
  9. ^abcdeStassun, Keivan G.; et al. (2019)."The Revised TESS Input Catalog and Candidate Target List".The Astronomical Journal.158 (4): 138.arXiv:1905.10694.Bibcode:2019AJ....158..138S.doi:10.3847/1538-3881/ab3467.
  10. ^"WDS J05466+0110AB".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-09-07.
  11. ^"HD 38529".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-09-09.
  12. ^"HD 38529 B".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-09-09.
  13. ^Gould, Benjamin Apthorp (1879)."Uranometria Argentina catalog of bright southern stars".Resultados del Observatorio Nacional Argentino en Cordoba.1. Buenos Aires.Bibcode:1879RNAO....1.....G. Retrieved2012-05-08.
  14. ^abFischer, Debra A.; et al. (2001)."Planetary Companions to HD 12661, HD 92788, and HD 38529 and Variations in Keplerian Residuals of Extrasolar Planets".The Astrophysical Journal.551 (2):1107–1118.Bibcode:2001ApJ...551.1107F.doi:10.1086/320224.
  15. ^Houk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars, Vol. 5".Michigan Spectral Survey.5.Bibcode:1999MSS...C05....0H.
  16. ^Hillenbrand, Lynne A.; et al. (2008)."The Complete Census of 70 μm-bright Debris Disks within "the Formation and Evolution of Planetary Systems" Spitzer Legacy Survey of Sun-like Stars".The Astrophysical Journal.677 (1):630–656.arXiv:0801.0163.Bibcode:2008ApJ...677..630H.doi:10.1086/529027.
  17. ^abcXuan, Jerry W.; Kennedy, Grant M.; Wyatt, Mark C.; Yelverton, Ben (2020)."Mutual inclinations between giant planets and their debris discs in HD 113337 and HD 38529".Monthly Notices of the Royal Astronomical Society.499 (4):5059–5074.arXiv:2010.02961.Bibcode:2020MNRAS.499.5059X.doi:10.1093/mnras/staa3155.S2CID 222177269.
  18. ^Reffert, S.; Quirrenbach, A. (2006)."Hipparcos astrometric orbits for two brown dwarf companions: HD 38529 and HD 168443".Astronomy and Astrophysics.449 (2):699–702.Bibcode:2006A&A...449..699R.doi:10.1051/0004-6361:20054611.hdl:1887/7483.
  19. ^Benedict, G. Fritz; et al. (2010)."The Mass of HD 38529c from Hubble Space Telescope Astrometry and High-precision Radial Velocities".The Astronomical Journal.139 (5):1844–1856.arXiv:1003.0421.Bibcode:2010AJ....139.1844B.doi:10.1088/0004-6256/139/5/1844.
  20. ^Feng, Fabo; Butler, R. Paul; et al. (August 2022)."3D Selection of 167 Substellar Companions to Nearby Stars".The Astrophysical Journal Supplement Series.262 (21): 21.arXiv:2208.12720.Bibcode:2022ApJS..262...21F.doi:10.3847/1538-4365/ac7e57.S2CID 251864022.
  21. ^abFeng, Fabo; Xiao, Guang-Yao; et al. (April 2025)."Lessons learned from the detection of wide companions by radial velocity and astrometry".Monthly Notices of the Royal Astronomical Society.539 (4):3180–3200.arXiv:2412.14542.doi:10.1093/mnras/staf689.
  22. ^Correa-Otto, J. A.; Gil-Hutton, R. A. (2017)."Galactic perturbations on the population of wide binary stars with exoplanets".Astronomy and Astrophysics.608. A116.arXiv:1710.00766.Bibcode:2017A&A...608A.116C.doi:10.1051/0004-6361/201731229.hdl:11336/41265.

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