Astronomy:HD 66428 b
From HandWiki
Short description: Long-period jovian exoplanet in the constellation of Monoceros
| Discovery | |
|---|---|
| Discovered by | Butler et al.[1] |
| Discovery site | |
| Discovery date | July 15, 2006 |
| Radial velocity | |
| Orbital characteristics[2] | |
| 3.395+0.141 −0.157 astronomical unit|AU | |
| Eccentricity | 0.471±0.012 |
| Orbital period | 6.214+0.015 −0.016 yr |
| Inclination | 16.639°+10.121° −2.959° |
| Longitude of ascending node | 299.391°+8.486° −8.219° |
| astron|astron|helion}} | 2450057.763+16.562 −18.431 |
| 185.689°+1.688° −1.596° | |
| Semi-amplitude | 54.441+1.035 −1.167 m/s |
| Star | HD 66428 |
| Physical characteristics[2] | |
| Mass | 10.946+2.442 −3.845 MJ |
HD 66428 b is a long-period jovian exoplanet located approximately 174 light-years away in the constellation of Monoceros. It has a minimum mass of 2.82 |♃|J}}}}}} and takes 1973 days or 5.402 years to orbit around its solar-type star HD 66428. The average distance is 3.18 AU, about half the distance between Mars and Jupiter. This planet is a so-called eccentric Jupiter with an orbital eccentricity of 0.465. At periastron, the distance is 1.70 AU and at apastron, the distance is 4.66 AU.[1] In 2022, the inclination and true mass of HD 66428 b were measured via astrometry.[2]
See also
References
- ↑ 1.0 1.1 Butler, R. P. et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal 646 (1): 505–522. doi:10.1086/504701. Bibcode: 2006ApJ...646..505B.
- ↑ 2.0 2.1 2.2 Feng, Fabo et al. (August 2022). "3D Selection of 167 Substellar Companions to Nearby Stars". The Astrophysical Journal Supplement Series 262 (21): 21. doi:10.3847/1538-4365/ac7e57. Bibcode: 2022ApJS..262...21F.
External links
- "Notes for planet HD 66428 b". Extrasolar Planets Encyclopaedia. https://exoplanet.eu/catalog/hd_66428_b--333/. Retrieved 2008-08-20.
- "HD 66428". Exoplanets. http://media4.obspm.fr/exoplanets/base/etoile.php?nom=HD+66428. Retrieved 2008-08-20.
Coordinates:
08h 03m 28.6652s, −01° 09′ 45.752″
