HD 212301
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Observation data Epoch J2000.0 |
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Constellation (pronunciation) |
Octans |
Right ascension | 22h 27m 30.9195s |
Declination | −77º 43' 04.5206″ |
Apparent magnitude (V) | 7.77 |
Absolute magnitude (V) | 4.16 |
Distance | 171.93 ly (52.71 pc) |
Spectral type | F8V |
Other designations | |
HD 212301 is a star in the south circumpolar constellation Octans, located at a distance of 171.93 light years or 52.71 parsecs or 1.626 exameters away from the Sun. The magnitudes are m=7.77 and M=4.16. It is a peach main-sequence star of spectral type F8V. The temperature of the photosphere is 5998 Kelvin and have mass 5% more than our Sun. Its age is older than our local star by 1.3 billion years or by the factor of 1.3 times. It is a metal-rich star with 50% more metals than does the Sun has. This star is also called HIP 110852.
[edit] HD 212301 b
Discovery
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Discovered by | Lo Curto et al. |
Discovery site | Chile |
Discovery date | 2005 |
Detection method | Radial Velocity |
Designations
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Alternative names | HIP 110852 b SAO 258040 b |
Semi-major axis | 0.0341 AU |
Eccentricity | 0 |
Orbital period | 2.24572±28 d |
Average orbital speed | 165.8 km/s |
Angular distance | 0.647 mas |
Longitude of periastron | 0° |
Time of periastron | 2453549.195±0.004 JD |
Semi-amplitude | 59.5±0.7 m/s |
Physical characteristics
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Mass | >0.396 MJ |
HD 212301 b is a low-mass exoplanet with a mass type IIc and an appearance type of L (Alkali metal giant). It has an orbital period of 2.25 Earth days with the angular separation of 0.65 milliarcsecond. The orbital distance is 0.0341 astronomical units or 5.10 gigameters or 0.165 microparsecs. The periastron and apastron distance are identical to average orbital distance, meaning its eccentricity is 0.0%. The longitude of periastron is close to 0° or 360°. The time of periastron is 2,453,549.195 JD. The average orbital speed of this planet is as fast as 165.8 km/s. The semi-amplitude or the speed of the stellar wobble caused by a planet is 59.5 m/s.
In 2005, taking place in ESO La Silla Observatory in Chile, the planet was discovered by Lo Curto who used the HARPS spectrometer.
[edit] References
- Lo Curto et al. (2006). "The HARPS search for southern extra-solar planets. VII. A very hot Jupiter orbiting HD 212301". Astronomy and Astrophysics 451: 345-350.
[edit] External links
- Notes for star HD 212301. The Extrasolar Planets Encyclopaedia. Retrieved on December 16, 2007.
- Notes for planet HD 212301 b. The Extrasolar Planets Encyclopaedia. Retrieved on December 16, 2007.
- HD 212301 -- Star. SIMBAD. Retrieved on December 16, 2007.
- HD 212301 b -- Extra-solar Planet Candidate. SIMBAD. Retrieved on December 16, 2007.