HD 33564 b
From Infogalactic: the planetary knowledge core
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | HD 33564 | |
Constellation | Camelopardalis | |
Right ascension | (α) | 05h 22m 33.5319s |
Declination | (δ) | +79° 13′ 52.135″ |
Apparent magnitude | (mV) | 5.08 |
Distance | 68.43 ly (20.98 pc) |
|
Spectral type | F6V | |
Orbital elements | ||
Semi-major axis | (a) | 1.117 ± 0.027 AU |
Periastron | (q) | 0.737 AU |
Apastron | (Q) | 1.497 AU |
Eccentricity | (e) | 0.34 ± 0.02 |
Orbital period | (P) | 388 ± 3 d (1.06 y) |
Orbital speed | (υ) | 31.5 km/s |
Argument of periastron |
(ω) | 205 ± 4° |
Semi-amplitude | (K) | 232 ± 5 m/s |
Physical characteristics | ||
Minimum mass | (m sin i) | 9.13 ± 0.17 MJ (2900 ± 54 M⊕) |
Discovery information | ||
Discovery date | September 3, 2005 | |
Discoverer(s) | Galland et al. | |
Discovery method | Doppler Spectroscopy | |
Discovery site | ![]() |
|
Discovery status | Published | |
Database references | ||
Extrasolar Planets Encyclopaedia |
data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
HD 33564 b is an extrasolar planet located approximately 68 light-years away in the constellation of Camelopardalis. This planet orbits around F6V star HD 33564. The planet has an eccentric orbit, ranging in distance from 0.737 AU at periastron to 1.497 AU at apastron.
HD 33564 b is a gas giant in a habitable zone of its star. Based on a probable 10−4 fraction of the planet mass as a satellite,[1] it can have a Mars-sized moon with habitable surface.[2] On the other hand, this mass can be distributed into many small satellites as well.
See also
References
- ↑ Canup R.M., Ward W.R. (2006). A common mass scaling for satellite systems of gaseous planets. Nature, 441: 834-839.
- ↑ The Habitable Exoplanets Catalog: Data of Potential Habitable Worlds
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External links
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Coordinates: 05h 22m 33.5319s, +79° 13′ 52.135″
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