Astronomy:HD 33283
Observation data Equinox J2000.0]] (ICRS) | |
---|---|
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[1] mas |
Distance | 293.9 ± 0.8 ly (90.1 ± 0.2 pc) |
Absolute magnitude (MV) | 3.19[2] |
Details | |
HD 33283 | |
Mass | 1.39±0.04 M☉[4] 1.24±0.1[5] M☉ |
Radius | 1.95±0.04 R☉[4] 1.20±0.1[5] R☉ |
Luminosity | 4.37±0.02[4] L☉ |
Surface gravity (log g) | 3.99±0.03[4] cgs |
Temperature | 5,985±57[4] K |
Metallicity [Fe/H] | 0.35±0.08[2] dex |
Rotational velocity (v sin i) | 1.09±0.26[6] km/s |
Age | 3.6±0.6[4] Gyr |
HD 33283 B | |
Mass | 0.17[3] M☉ |
Other designations | |
Database references | |
SIMBAD | data |
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]
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 astronomical unit|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 astronomical unit|AU (22 Gm) from the host star with a period of 18.2 days and an eccentricity (ovalness) of 0.4.[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
- ↑ 1.0 1.1 1.2 1.3 1.4 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 2.7 2.8 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A.
- ↑ 3.0 3.1 3.2 3.3 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. doi:10.1093/mnras/stu044. Bibcode: 2014MNRAS.439.1063M.
- ↑ 4.0 4.1 4.2 4.3 4.4 4.5 4.6 Bonfanti, A. et al. (2015). "Revising the ages of planet-hosting stars". Astronomy and Astrophysics 575: A18. doi:10.1051/0004-6361/201424951. Bibcode: 2015A&A...575A..18B. http://www.aanda.org/articles/aa/full_html/2015/03/aa24951-14/aa24951-14.html.
- ↑ 5.0 5.1 5.2 5.3 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. doi:10.1086/505173. Bibcode: 2006ApJ...647..600J.
- ↑ 6.0 6.1 Jofré, E. et al. (2015). "Stellar parameters and chemical abundances of 223 evolved stars with and without planets". Astronomy & Astrophysics 574: A50. doi:10.1051/0004-6361/201424474. Bibcode: 2015A&A...574A..50J.
- ↑ "HD 33283". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+33283.
- ↑ 8.0 8.1 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. doi:10.3847/1538-3881/aae1f5. Bibcode: 2018AJ....156..213M.
External links
- "Notes for star HD 33283". Extrasolar Planets Encyclopaedia. http://exoplanet.eu/star.php?st=HD+33283.
Coordinates: 05h 08m 01.0118s, −26° 47′ 50.896″
![]() | Original source: https://en.wikipedia.org/wiki/HD 33283.
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