Gliese 876 c
Keck Observatories | |
Discovery date | January 9, 2001 |
---|---|
Doppler spectroscopy | |
Orbital characteristics[3] | |
Epoch 2,450,602.09311 BJD | |
0.136044+0.000021 −0.000022 AU | |
Eccentricity | 0.2571±0.0019 |
30.0972+0.0071 −0.0073 d | |
292.55+1 −0.99 º | |
Inclination | 53.06±0.85 º[note 1] |
51.09+0.77 −0.78 º | |
Semi-amplitude | 87.46+0.3 −0.29 m/s |
Star | Gliese 876 |
Physical characteristics[3] | |
Mass | 265.6±2.7 M🜨[note 2] |
Gliese 876 c is an exoplanet orbiting the red dwarf Gliese 876, taking about 30 days to complete an orbit. The planet was discovered in April 2001 and is the second planet in order of increasing distance from its star.
Discovery
At the time of discovery, Gliese 876 was already known to host an extrasolar planet designated
Host star
The planet orbits a (M-type) star named Gliese 876. The star has a mass of 0.33 M☉ and a radius of around 0.36 R☉. It has a surface temperature of 3350 K and is 2.55 billion years old. In comparison, the Sun is about 4.6 billion years old[4] and has a surface temperature of 5778 K.[5]
Orbit and mass
Gliese 876 c is in a 1:2:4
.The orbital
A limitation of the radial velocity method used to detect Gliese 876 c is that only a lower limit on the planet's
Characteristics
Based on its high mass, Gliese 876 c is likely to be a gas giant with no solid surface. Since it was detected indirectly through its gravitational effects on the star, properties such as its radius, composition, and temperature are unknown. Assuming a composition similar to Jupiter and an environment close to chemical equilibrium, the planet is predicted to have a cloudless upper atmosphere.[10]
Gliese 876 c lies at the inner edge of the system's habitable zone. While the prospects for life on gas giants are unknown, it might be possible for a large moon of the planet to provide a habitable environment. Unfortunately tidal interactions between a hypothetical moon, the planet, and the star could destroy moons massive enough to be habitable over the lifetime of the system.[11] In addition it is unclear whether such moons could form in the first place.[12]
This planet, like b and e, has likely migrated inward.[13]
See also
- Appearance of extrasolar planets
- Eccentric Jupiter
- Gliese 581
- List of nearest stars
Notes
References
- ^ doi:10.1086/321552.
- ^ a b "Two new planetary systems discovered" (Press release). Kamuela, Hawaii: W. M. Keck Observatory. January 9, 2001. Archived from the original on August 13, 2019. Retrieved August 13, 2019.
- ^ .
- ^ Fraser Cain (16 September 2008). "How Old is the Sun?". Universe Today. Archived from the original on 18 August 2010. Retrieved 19 February 2011.
- ^ Fraser Cain (September 15, 2008). "Temperature of the Sun". Universe Today. Archived from the original on 29 August 2010. Retrieved 19 February 2011.
- ^ S2CID 118707953.
- S2CID 122255962.
- S2CID 119067572.
- S2CID 121585653.
- S2CID 16004653.
- S2CID 14508244. (paper incorrectly refers to Gliese 876 b as GJ876c)
- S2CID 4327454.
- S2CID 254381557.
External links
- Nemiroff, R.; Bonnell, J., eds. (1998-06-26). "A planet for Gliese 876". Astronomy Picture of the Day. NASA. Retrieved 2008-06-21.
- "Gliese 876 : THE CLOSEST EXTRASOLAR PLANET". Observatoire de Haute Provence. Archived from the original on 2012-10-24. Retrieved 2008-06-21.