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HD 33283 is a star in the southern constellation Lepus with one planet and a co-moving stellar companion.[3] With an apparent visual magnitude of 8.05,[2] the star is too faint to be seen with the naked eye. It is located at a distance of 294 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +4.5.[2]

HD 33283
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Lepus
Right ascension 05h 08m 01.0123s[1]
Declination −26° 47′ 50.8941″[1]
Apparent magnitude (V) 8.05[2]
Characteristics
Spectral type G3/5V[2] + M4–5[3]
B−V color index 0.641±0.009[2]
Astrometry
Radial velocity (Rv)+4.51±0.19[2] km/s
Proper motion (μ) RA: 56.184[1] mas/yr
Dec.: −46.058[1] mas/yr
Parallax (π)11.0993 ± 0.0286 mas[1]
Distance293.9 ± 0.8 ly
(90.1 ± 0.2 pc)
Absolute magnitude (MV)3.19[2]
Details
HD 33283
Mass1.39±0.04 M☉[4]
1.24±0.1[5] M☉
Radius1.95±0.04 R☉[4]
1.20±0.1[5] R☉
Luminosity4.37±0.02[4] L☉
Surface gravity (log g)3.99±0.03[4] cgs
Temperature5,985±57[4] K
Metallicity [Fe/H]0.35±0.08[2] dex
Rotational velocity (v sin i)1.09±0.26[6] km/s
Age3.6±0.6[4] Gyr
HD 33283 B
Mass0.17[3] M☉
Other designations
CD–26°2029, FK5 4470, Gaia DR2 2955981936912654592, GC 6286, HD 33283, HIP 23889, SAO 170100, PPM 75021, 2MASS J05080100-2647509[7]
Database references
SIMBADdata

This is an ordinary G-type main-sequence star with a stellar classification of G3/5V.[2] It is about 3.6 billion years old and is chromospherically inactive. The star is spinning slowly with a projected rotational velocity of 1 km/s[6] and an estimated rotation period of about 55.5 days.[5] It is larger and more massive than the Sun. HD 33283 is radiating over four times the luminosity of the Sun from its photosphere at an effective temperature of 5,985 K.[4]

In 2014, a co-moving red dwarf companion star, HD 33283 B, of spectral class M4–M5 was detected at an angular separation of 55.7″, corresponding to a projected separation of 5,244 AU.[3]


Planetary system


In 2006, J. A. Johnson and associates found a jovian planet orbiting HD 33283 with the radial velocity method.[5] It is orbiting at a distance of 0.15 AU (22 Gm) from the host star with a period of 18.2 days and an eccentricity (ovalness) of 0.4.[8]

The HD 33283 planetary system[8]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
b ≥0.329±0.071 MJ 0.1508±0.0087 18.1991±0.0017 0.399±0.056 — —

See also



References


  1. 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. Gaia DR2 record for this source at VizieR.
  2. 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. Mugrauer, M.; et al. (March 2014). "New wide stellar companions of exoplanet host stars". Monthly Notices of the Royal Astronomical Society. 439 (1): 1063–1070. Bibcode:2014MNRAS.439.1063M. doi:10.1093/mnras/stu044.
  4. Bonfanti, A.; et al. (2015). "Revising the ages of planet-hosting stars". Astronomy and Astrophysics. 575. A18. arXiv:1411.4302. Bibcode:2015A&A...575A..18B. doi:10.1051/0004-6361/201424951. S2CID 54555839.
  5. Johnson, John Asher; et al. (2006). "The N2K Consortium. VI. Doppler Shifts without Templates and Three New Short-Period Planets". The Astrophysical Journal. 647 (1): 600–611. arXiv:astro-ph/0604348. Bibcode:2006ApJ...647..600J. doi:10.1086/505173. S2CID 12421834.
  6. Jofré, E.; et al. (2015). "Stellar parameters and chemical abundances of 223 evolved stars with and without planets". Astronomy & Astrophysics. 574: A50. arXiv:1410.6422. Bibcode:2015A&A...574A..50J. doi:10.1051/0004-6361/201424474. S2CID 53666931.
  7. "HD 33283". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-06-25.{{cite web}}: CS1 maint: postscript (link)
  8. Ment, Kristo; et al. (2018). "Radial Velocities from the N2K Project: Six New Cold Gas Giant Planets Orbiting HD 55696, HD 98736, HD 148164, HD 203473, and HD 211810". The Astronomical Journal. 156 (5). 213. arXiv:1809.01228. Bibcode:2018AJ....156..213M. doi:10.3847/1538-3881/aae1f5. S2CID 119243619.



На других языках

[de] HD 33283

HD 33283 ist ein etwa 280 Lichtjahre entfernter Hauptreihenstern der Spektralklasse G im Sternbild Hase (Lepus). Er besitzt eine scheinbare Helligkeit von 8,05 mag.
- [en] HD 33283


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