HD 108874 b | |
Discoverer: | Butler et al. |
Discovery Site: | United States |
Discovered: | June 30, 2003 |
Apsis: | astron |
Semimajor: | 1.053± |
Eccentricity: | 0.128 ± 0.022 |
Period: | 394.48 ± 0.60 d |
Time Periastron: | 2,454,045 ± 49 |
Arg Peri: | 219.4 ± 9.4 |
Semi-Amplitude: | 37.3 ± 1.1 |
Mass: | >1.34 ± 0.11 |
HD 108874 b is a gas giant announced in 2003. The orbit lies in the star's habitable zone.[1] It is expected that any moons orbiting this planet are enriched in carbon, and are thus quite different from the silicate-rich bodies in the Solar System.[2] The planet is possibly in a 4 : 1 orbital resonance with HD 108874 c.
The jovian planet HD 108874 b was discovered by the US-based team led by Paul Butler, Geoffrey Marcy, Steven Vogt, and Debra Fischer. A total of 20 radial velocity observations, obtained at the W. M. Keck Observatory in Hawaii between 1999 and 2002, were used to make the discovery.