Gamma1 Leonis b
![Sky map](http://upload.wikimedia.org/wikipedia/commons/thumb/e/e4/Jupiter_and_moon.png/20px-Jupiter_and_moon.png)
Discovery | |
---|---|
Periastron | 1.02 AU (153,000,000 km) |
1.19 AU (178,000,000 km)[1] | |
Eccentricity | 0.14[1] |
429[1] d 1.17 y | |
Average orbital speed | 30.3 |
Star | Gamma1 Leonis |
Gamma1 Leonis b is an
Discovery
On November 6, 2009, a planetary companion around primary star Gamma1 Leonis has been announced.[1] Moreover, radial velocity variations would also hint two strong signals at 8.5 and 1340 days. The former periodicity is likely due to stellar pulsation, whereas the latter could be indicative of the presence of an additional planetary companion with 2.14 Jupiter masses, moderate eccentricity (e=0.13) and located at 2.6 Astronomical Units away from the giant star. Nevertheless, the nature of such a signal is still unclear and further investigations are needed to confirm or rule out an additional substellar companion.
Characteristics
The planet has a minimum mass of 8.78 Jupiter masses. The true mass, as with the majority of other extrasolar planets discovered by the radial velocity method, is unknown. [2]
References
- ^ S2CID 118962986.
- ^ "The Extrasolar Planet Encyclopaedia — Gamma1 Leonis b". Extrasolar Planets Encyclopaedia. Retrieved 10 September 2023.