| 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] |
| 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 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]
| 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
- ^ a b c d e 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.
- ^ a b c d e f g h i 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.
- ^ a b c d 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.
- ^ a b c d e f g 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.
- ^ a b c d 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.
- ^ a b 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.
-
^
"HD 33283".
SIMBAD.
Centre de données astronomiques de Strasbourg. Retrieved 2020-06-25.
{{ cite web}}: CS1 maint: postscript ( link) - ^ a b 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.
External links
- "Notes for star HD 33283". Extrasolar Planets Encyclopaedia. Archived from the original on November 6, 2007.
| 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] |
| 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 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]
| 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
- ^ a b c d e 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.
- ^ a b c d e f g h i 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.
- ^ a b c d 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.
- ^ a b c d e f g 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.
- ^ a b c d 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.
- ^ a b 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.
-
^
"HD 33283".
SIMBAD.
Centre de données astronomiques de Strasbourg. Retrieved 2020-06-25.
{{ cite web}}: CS1 maint: postscript ( link) - ^ a b 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.
External links
- "Notes for star HD 33283". Extrasolar Planets Encyclopaedia. Archived from the original on November 6, 2007.