From Wikipedia, the free encyclopedia
HD 29587
Observation data
Epoch J2000       Equinox J2000
Constellation Perseus
Right ascension 04h 41m 36.31645s [1]
Declination +42° 07′ 06.4209″ [1]
Apparent magnitude (V) 7.29 [2]
Characteristics
Spectral type G2 V [3]
B−V color index 0.633 [3]
Astrometry
Radial velocity (Rv)+112.67±0.20 [1] km/s
Proper motion (μ) RA: +534.004 [1]  mas/ yr
Dec.: −414.768 [1]  mas/ yr
Parallax (π)36.3130 ± 0.0697  mas [1]
Distance89.8 ± 0.2  ly
(27.54 ± 0.05  pc)
Absolute magnitude (MV)5.08 [3]
Orbit [4]
Period (P)1,474.9±10.2 d
Eccentricity (e)0.713±0.006 [5]
Periastron epoch (T)JD 2,447,763.5±45.8
Argument of periastron (ω)
(secondary)
80.2±13.3°
Semi-amplitude (K1)
(primary)
1.02±0.16 km/s
Details [3]
Mass1.033±0.010 [5]  M
Luminosity0.798+0.040
−0.038
  L
Surface gravity (log g)4.54±0.22  cgs
Temperature5,709±35  K
Metallicity [Fe/H]−0.51±0.05  dex
Age14.7+3.8
−2.7
  Gyr
Other designations
BD+41° 931, FK5 4419, HD 29587, HIP 21832, SAO 39690, TYC 2901-00064-1, 2MASS J04413631+4207065 [6]
Database references
SIMBAD data
Exoplanet Archive data

HD 29587 is a Sun-like [7] star with a candidate brown dwarf companion [8] in the northern constellation of Perseus. It has an apparent visual magnitude of 7.29, [2] which means it is too faint to be viewed with the naked eye. Based upon an annual parallax shift of 36.3  mas, [1] it is located 89.8  light years away. The star is moving away from the Earth with a heliocentric radial velocity of +113 km/s, [1] having come to within 55.8 ly some 148,000 years ago. [2] It is a hyper-velocity halo [7] star moving at a rate of 170 km/s relative to the local standard of rest. [9]

This ancient star has a stellar classification of G2 V, [3] matching a G-type main-sequence star. It has 78% of the mass of the Sun and is radiating 80% of the Sun's luminosity from its photosphere at an effective temperature of 5,709 K. [3]

Planetary system

Formerly an IAU radial velocity standard, this star was found to have a variable radial velocity due to a suspected orbiting companion. [8] The a sin i value for the unseen object is 0.0957 ± 0.0108  AU (14.31 ± 1.62  Gm), [4] where a is the semimajor axis and i is the orbital inclination – providing a lower bound for the semimajor axis. The secondary object most likely has a mass in the range 41.0–97.8  MJ, making it a probable brown dwarf. [10]

The HD 29587 planetary system [10]
Companion
(in order from star)
Mass Semimajor axis
( AU)
Orbital period
( days)
Eccentricity Inclination Radius
b ≥ 55.2±9.2 [5]  MJ 0.0957±0.0108 1,474.9±10.2 0.356±0.095

References

  1. ^ a b c d e f g h Brown, 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.
  2. ^ a b c Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv: 1108.4971. Bibcode: 2012AstL...38..331A. doi: 10.1134/S1063773712050015. S2CID  119257644.
  3. ^ a b c d e f Da Silva, Ronaldo; et al. (2015). "Homogeneous abundance analysis of FGK dwarf, subgiant, and giant stars with and without giant planets". Astronomy & Astrophysics. 580: A24. arXiv: 1505.01726. Bibcode: 2015A&A...580A..24D. doi: 10.1051/0004-6361/201525770. S2CID  119216425.
  4. ^ a b Halbwachs, J. L.; et al. (March 2000). "Exploring the brown dwarf desert with Hipparcos". Astronomy and Astrophysics. 355: 581–594. Bibcode: 2000A&A...355..581H.
  5. ^ a b c Kiefer, F.; et al. (2019), "Detection and characterisation of 54 massive companions with the SOPHIE spectrograph", Astronomy & Astrophysics, 631: A125, arXiv: 1909.00739, doi: 10.1051/0004-6361/201935113, S2CID  202538098
  6. ^ "HD 29587". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-08-02.
  7. ^ a b Fossati, L.; et al. (2017). "The effect of ISM absorption on stellar activity measurements and its relevance for exoplanet studies". Astronomy & Astrophysics. 601: 17. arXiv: 1702.02883. Bibcode: 2017A&A...601A.104F. doi: 10.1051/0004-6361/201630339. S2CID  17549819. A104.
  8. ^ a b Mazeh; Latham, David W.; Stefanik, Robert P. (1996). "Spectroscopic Orbits for Three Binaries with Low-Mass Companions and the Distribution of Secondary Masses near the Substellar Limit". Astrophysical Journal. 466: 415–427. Bibcode: 1996ApJ...466..415M. CiteSeerX  10.1.1.30.5905. doi: 10.1086/177521.
  9. ^ Hobbs, L. M.; Duncan, Douglas K. (June 15, 1987). "The lithium abundance in halo stars". Astrophysical Journal, Part 1. 317: 796–809. Bibcode: 1987ApJ...317..796H. doi: 10.1086/165328.
  10. ^ a b Reffert, S.; Quirrenbach, A. (March 2011). "Mass constraints on substellar companion candidates from the re-reduced Hipparcos intermediate astrometric data: nine confirmed planets and two confirmed brown dwarfs". Astronomy & Astrophysics. 527: 22. arXiv: 1101.2227. Bibcode: 2011A&A...527A.140R. doi: 10.1051/0004-6361/201015861. S2CID  54986291. A140.
From Wikipedia, the free encyclopedia
HD 29587
Observation data
Epoch J2000       Equinox J2000
Constellation Perseus
Right ascension 04h 41m 36.31645s [1]
Declination +42° 07′ 06.4209″ [1]
Apparent magnitude (V) 7.29 [2]
Characteristics
Spectral type G2 V [3]
B−V color index 0.633 [3]
Astrometry
Radial velocity (Rv)+112.67±0.20 [1] km/s
Proper motion (μ) RA: +534.004 [1]  mas/ yr
Dec.: −414.768 [1]  mas/ yr
Parallax (π)36.3130 ± 0.0697  mas [1]
Distance89.8 ± 0.2  ly
(27.54 ± 0.05  pc)
Absolute magnitude (MV)5.08 [3]
Orbit [4]
Period (P)1,474.9±10.2 d
Eccentricity (e)0.713±0.006 [5]
Periastron epoch (T)JD 2,447,763.5±45.8
Argument of periastron (ω)
(secondary)
80.2±13.3°
Semi-amplitude (K1)
(primary)
1.02±0.16 km/s
Details [3]
Mass1.033±0.010 [5]  M
Luminosity0.798+0.040
−0.038
  L
Surface gravity (log g)4.54±0.22  cgs
Temperature5,709±35  K
Metallicity [Fe/H]−0.51±0.05  dex
Age14.7+3.8
−2.7
  Gyr
Other designations
BD+41° 931, FK5 4419, HD 29587, HIP 21832, SAO 39690, TYC 2901-00064-1, 2MASS J04413631+4207065 [6]
Database references
SIMBAD data
Exoplanet Archive data

HD 29587 is a Sun-like [7] star with a candidate brown dwarf companion [8] in the northern constellation of Perseus. It has an apparent visual magnitude of 7.29, [2] which means it is too faint to be viewed with the naked eye. Based upon an annual parallax shift of 36.3  mas, [1] it is located 89.8  light years away. The star is moving away from the Earth with a heliocentric radial velocity of +113 km/s, [1] having come to within 55.8 ly some 148,000 years ago. [2] It is a hyper-velocity halo [7] star moving at a rate of 170 km/s relative to the local standard of rest. [9]

This ancient star has a stellar classification of G2 V, [3] matching a G-type main-sequence star. It has 78% of the mass of the Sun and is radiating 80% of the Sun's luminosity from its photosphere at an effective temperature of 5,709 K. [3]

Planetary system

Formerly an IAU radial velocity standard, this star was found to have a variable radial velocity due to a suspected orbiting companion. [8] The a sin i value for the unseen object is 0.0957 ± 0.0108  AU (14.31 ± 1.62  Gm), [4] where a is the semimajor axis and i is the orbital inclination – providing a lower bound for the semimajor axis. The secondary object most likely has a mass in the range 41.0–97.8  MJ, making it a probable brown dwarf. [10]

The HD 29587 planetary system [10]
Companion
(in order from star)
Mass Semimajor axis
( AU)
Orbital period
( days)
Eccentricity Inclination Radius
b ≥ 55.2±9.2 [5]  MJ 0.0957±0.0108 1,474.9±10.2 0.356±0.095

References

  1. ^ a b c d e f g h Brown, 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.
  2. ^ a b c Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv: 1108.4971. Bibcode: 2012AstL...38..331A. doi: 10.1134/S1063773712050015. S2CID  119257644.
  3. ^ a b c d e f Da Silva, Ronaldo; et al. (2015). "Homogeneous abundance analysis of FGK dwarf, subgiant, and giant stars with and without giant planets". Astronomy & Astrophysics. 580: A24. arXiv: 1505.01726. Bibcode: 2015A&A...580A..24D. doi: 10.1051/0004-6361/201525770. S2CID  119216425.
  4. ^ a b Halbwachs, J. L.; et al. (March 2000). "Exploring the brown dwarf desert with Hipparcos". Astronomy and Astrophysics. 355: 581–594. Bibcode: 2000A&A...355..581H.
  5. ^ a b c Kiefer, F.; et al. (2019), "Detection and characterisation of 54 massive companions with the SOPHIE spectrograph", Astronomy & Astrophysics, 631: A125, arXiv: 1909.00739, doi: 10.1051/0004-6361/201935113, S2CID  202538098
  6. ^ "HD 29587". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-08-02.
  7. ^ a b Fossati, L.; et al. (2017). "The effect of ISM absorption on stellar activity measurements and its relevance for exoplanet studies". Astronomy & Astrophysics. 601: 17. arXiv: 1702.02883. Bibcode: 2017A&A...601A.104F. doi: 10.1051/0004-6361/201630339. S2CID  17549819. A104.
  8. ^ a b Mazeh; Latham, David W.; Stefanik, Robert P. (1996). "Spectroscopic Orbits for Three Binaries with Low-Mass Companions and the Distribution of Secondary Masses near the Substellar Limit". Astrophysical Journal. 466: 415–427. Bibcode: 1996ApJ...466..415M. CiteSeerX  10.1.1.30.5905. doi: 10.1086/177521.
  9. ^ Hobbs, L. M.; Duncan, Douglas K. (June 15, 1987). "The lithium abundance in halo stars". Astrophysical Journal, Part 1. 317: 796–809. Bibcode: 1987ApJ...317..796H. doi: 10.1086/165328.
  10. ^ a b Reffert, S.; Quirrenbach, A. (March 2011). "Mass constraints on substellar companion candidates from the re-reduced Hipparcos intermediate astrometric data: nine confirmed planets and two confirmed brown dwarfs". Astronomy & Astrophysics. 527: 22. arXiv: 1101.2227. Bibcode: 2011A&A...527A.140R. doi: 10.1051/0004-6361/201015861. S2CID  54986291. A140.

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