astro.wikisort.org - Meteorite

HD 219134 g, also known as HR 8832 g, is an unconfirmed^{[citation needed]} exoplanet orbiting around the K-type star HD 219134 in the constellation of Cassiopeia. It has a minimum mass of 11 Earth Masses, suggesting that it could be a high-mass ocean planet or a Neptune-like ice giant. Unlike HD 219134 b and HD 219134 c it was not observed by the Spitzer Space Telescope and thus its radius and density are unknown. It resides closer to the star than the inner edge of the system's (empirical) habitable zone, defined by the recent Venus limit.[3] If it has an Earth-like composition, it would have a radius 1.9 times that of Earth. However, since it is probably an ocean planet or Mini-Neptune, it is likely larger.

HD 219134 g

Discovery
Discovered by	HARPS-N
Discovery site	La Palma, Canary Islands
Discovery date	2015 November 17
Detection method	radial velocity method
Orbital characteristics
Semi-major axis	0.3753 (± 0.0004)[1] AU
Eccentricity	0[1]
Orbital period (sidereal)	94.2 (± 0.2)[1] d
Inclination	null[1]
Star	HD 219134
Physical characteristics
Mean radius	~2.4 REarth
Mass	>10.81 (± 1.27)[1] MEarth
Temperature	298 K (25 °C; 77 °F)[2]

Characteristics

Mass, Radius, and Temperature

HD 219134 g is a sub-Neptune-mass exoplanet with a minimum mass of 10.81 M_Earth and an unknown radius, as it is not known to transit.[1] However, due to the high metal content of the host star, the planet might not be an ice giant. For a rock-iron composition, HD 219134 g would be about 1.9 R_Earth, which seems unlikely for a planet of this mass. A more plausible rock-water composition would put the planet at about 2.4 R_Earth. In the absence of an atmosphere, and assuming an albedo of 0.3, it has an equilibrium temperature of 298 K (25 °C; 77 °F), but with an atmosphere it is likely to have a surface temperature much higher, that is if it has a rocky surface. So, it is rather unlikely to be habitable.

Orbit

HD 219134 g takes about 94.2 days to orbits its star at a distance of 0.3753 AU. This is comparable to Mercury's orbit of 88 days at about 0.38 AU. However, due to the lower luminosity of the host star, HD 219134 g is closer to Venus' situation. The eccentricity of the planet's orbit is believed to be close to zero, indicating a very circular orbit.[1]

Host Star

The planet HD 219134 g orbits the K3V orange dwarf HD 219134, also known as HR 8832. It is 79% the radius and 80% the mass of the Sun with 26% the luminosity. It has a temperature of 4699 K and is around 11 billion years old.[1] For comparison, the Sun has a temperature of 5778 K and is 4.55 billion years old.

The apparent magnitude of the star, or how bright it appears from Earth, is around 5. Therefore, it is just visible to the unaided eye to most observers.

Habitability

HD 219134 g could be a potentially habitable planet.^{[citation needed]} Based on its relatively low mass (~11 M_Earth) and the high metal content of the parent star (+0.11 [Fe/H]), it has a low chance of being an ocean planet. While these types of worlds have no solid surfaces for life to develop, it is predicted that biology would arise in ways other than that of Earth. The planet also appears to have a fairly similar temperature to Earth, if somewhat hotter than Earth's 255 K (−18 °C; −1 °F) equilibrium temperature. HD 219134 g has an equilibrium temperature of 298 K (25 °C; 77 °F), in fact exactly the same as Venus' equilibrium temperature, that is if Venus like Earth had an albedo of 0.3.[2] However, the planet was not reported in the most recent analysis of the system with the HARPS-N spectrograph, which suggests that the planet may not actually exist.^{[citation needed]} Although, even if the planet did exist, but wasn't tidally locked, it would not fit the understood criteria for being located within the star's habitable zone. For example, the habitable zone for this star, as defined by Kopparapu et al. 2014,[4] for a 5 Earth mass planet, would be between 0.499 AU and 0.947 AU.[note 1][3]

References

Notes

---