From Surf Wiki (app.surf) — the open knowledge base
Gamma1 Leonis b
Exoplanet or brown dwarf
Exoplanet or brown dwarf
| Field | Value |
|---|---|
| name | Gamma1 Leonis b |
| discoverer | Inwoo Han et al. |
| discovery_site | South Korea |
| discovered | November 6, 2009 |
| discovery_method | Radial velocity |
| apsis | astron |
| aphelion | 1.36 AU |
| perihelion | 1.02 AU |
| semimajor | 1.19 AU |
| eccentricity | 0.14 |
| period | 429 d |
| 1.17 y | |
| avg_speed | 30.3 |
| star | Gamma1 Leonis (Algieba A) |
| mass | 10.7 |
1.17 y Gamma1 Leonis b is an extrasolar planet located 125.5 light years away in the constellation Leo, orbiting the giant star Gamma1 Leonis.
Discovery
On November 6, 2009, a planetary companion around primary star Gamma1 Leonis has been announced. 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 10.7 Jupiter masses. The true mass, as with the majority of other extrasolar planets discovered by the radial velocity method, is unknown. Depending on the planet's inclination relative to Earth, it may be sufficiently massive to be classified as a brown dwarf.
Host star
Main article: Algieba
Gamma Leonis A is the main star of a binary star system in the constellation Leo (the lion). It is a K-type red giant of apparent magnitude 2.37, with around 26 times the size of the Sun and 250 times its luminosity. The secondary component is a fainter G-type giant of apparent magnitude 3.64, eleven times bigger than the Sun with 63 times its luminosity. Together, they shine with apparent magnitude 2.04, making it the second-brightest star in Leo after Regulus. This system shares the traditional name Algieba.
The Algieba system can be easily split by a telescope. Due to the large orbital separation between the stars, only a small fraction of the orbit has been observed since discovery, and the orbital parameters are still poorly known.
References
References
- Takeda, Yoichi. (July 2023). "Spectroscopic comparative study of the red giant binary system gamma Leonis A and B". Astrophysics and Space Science.
- (2010). "Detection of a Planetary Companion around the giant star γ1 Leonis". [[Astronomy and Astrophysics]].
- "The Extrasolar Planet Encyclopaedia — Gamma1 Leonis b". [[Extrasolar Planets Encyclopaedia]].
This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.
Ask Mako anything about Gamma1 Leonis b — get instant answers, deeper analysis, and related topics.
Research with MakoFree with your Surf account
Create a free account to save articles, ask Mako questions, and organize your research.
Sign up freeThis content may have been generated or modified by AI. CloudSurf Software LLC is not responsible for the accuracy, completeness, or reliability of AI-generated content. Always verify important information from primary sources.
Report