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HD 60532 is a white (F-type) main sequence star located approximately 84 light-years away in the constellation of Puppis, taking its primary name from its Henry Draper Catalogue designation. It is calculated to be 1.44 times more massive than the Sun. The star is only 59% as old as the Sun (2.7 Gyr) and has metallicity of only 38% that of the Sun. In 2008, two extrasolar planets were discovered in orbit around it.

HD 60532
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Puppis
Right ascension 07h 34m 03.18084s[1]
Declination –22° 17′ 45.8398″[1]
Apparent magnitude (V) 4.450[2]
Characteristics
Spectral type F6 IV-V[3]
U−B color index +0.07[4]
B−V color index +0.51[4]
Astrometry
Radial velocity (Rv)60.2±0.4[5] km/s
Proper motion (μ) RA: –39.87[1] mas/yr
Dec.: 46.84[1] mas/yr
Parallax (π)38.1379 ± 0.1087 mas[5]
Distance85.5 ± 0.2 ly
(26.22 ± 0.07 pc)
Absolute magnitude (MV)2.40[2]
Details
Mass1.44+0.03
−0.1[6] M☉
Radius2.52 R☉
Luminosity8.596 L☉
Surface gravity (log g)4.09[7] cgs
Temperature6,095[6] K
Metallicity [Fe/H]–0.42[6] dex
Rotational velocity (v sin i)8[6] km/s
Age2.7 ± 0.1[6] Gyr
Other designations
108 G. Puppis,[8][9] BD–21° 2007, GC 10134, HIP 36795, HR 2906, Gliese 279, SAO 174009 , 2MASS J07340317-2217457
Database references
SIMBADdata
Exoplanet Archivedata
ARICNSdata
Extrasolar Planets
Encyclopaedia		data

Planetary system


In September 2008, two Jupiter-like planets were found orbiting the star.[6] The orbital periods of these two planets appear to be in 3:1 resonance.[10]

The HD 60532 planetary system[11]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
b ≥1.06±0.08 MJ 0.77±0.02 201.9±0.3 0.26±0.02 — —
c ≥2.51±0.16 MJ 1.60±0.04 600.1±2.4 0.03±0.02 — —

See also



References


  1. van Leeuwen, Floor (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752v1, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600 Note: see VizieR catalogue I/311.
  2. Nordström, B.; et al. (May 2004), "The Geneva-Copenhagen survey of the Solar neighbourhood. Ages, metallicities, and kinematic properties of ˜14 000 F and G dwarfs", Astronomy and Astrophysics, 418: 989–1019, arXiv:astro-ph/0405198, Bibcode:2004A&A...418..989N, doi:10.1051/0004-6361:20035959, S2CID 11027621
  3. Gray, R. O.; et al. (July 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. Johnson, H. L.; Iriarte, B.; Mitchell, R. I.; Wisniewskj, W. Z. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory, 4 (99), Bibcode:1966CoLPL...4...99J
  5. Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  6. Desort, M.; et al. (2008), "Extrasolar planets and brown dwarfs around A-F type stars V. A planetary system found with HARPS around the F6IV-V star HD 60532", Astronomy and Astrophysics, 491 (3): 883–888, arXiv:0809.3862, Bibcode:2008A&A...491..883D, doi:10.1051/0004-6361:200810241, S2CID 14562319web preprint
  7. Edvardsson, B.; et al. (August 1993), "The Chemical Evolution of the Galactic Disk - Part One - Analysis and Results", Astronomy and Astrophysics, 275 (1): 101, Bibcode:1993A&A...275..101E
  8. Gould, Benjamin Apthorp (1879), Uranometria Argentina: brightness and position of every fixed star, down to the seventh magnitude, within one hundred degrees of the South Pole, vol. 1, Observatorio Nacional Argentino, p. 172
  9. Gould, Benjamin Apthorp; Pilcher, Frederick, Uranometria Argentina, Revised, archived from the original on 2012-02-27, retrieved 2011-12-08
  10. Laskar, J.; Correia, A. C. M. (2009), "HD60532, a planetary system in a 3:1 mean motion resonance", Astronomy & Astrophysics Letters, 496 (2): L5–L8, arXiv:0902.0667, Bibcode:2009A&A...496L...5L, doi:10.1051/0004-6361/200911689, S2CID 17793870
  11. Borgniet, S.; et al. (2017). "Extrasolar planets and brown dwarfs around AF-type stars. IX. The HARPS southern sample". Astronomy and Astrophysics. 599. A57. arXiv:1608.08257. Bibcode:2017A&A...599A..57B. doi:10.1051/0004-6361/201628805. S2CID 118723455.


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HD 60532 — звезда, которая находится в созвездии Кормы на расстоянии около 84 световых лет от нас. Вокруг звезды обращаются, как минимум, две планеты.


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