HD 290327
From Infogalactic: the planetary knowledge core
| Observation data Epoch J2000.0 Equinox J2000.0 |
|
|---|---|
| Constellation | Orion |
| Right ascension | 05h 23m 21.56s[1] |
| Declination | –02° 16′ 39.4″[1] |
| Apparent magnitude (V) | 8.96 |
| Characteristics | |
| Spectral type | G5IV |
| Apparent magnitude (B) | 9.69 |
| Apparent magnitude (J) | 7.683 |
| Apparent magnitude (H) | 7.404 |
| Apparent magnitude (K) | 7.271 |
| B−V color index | 0.73 |
| Astrometry | |
| Proper motion (μ) | RA: 34.44±1.54[1] mas/yr Dec.: −96.93±0.99[1] mas/yr |
| Parallax (π) | 17.65 ± 1.57[1] mas |
| Distance | 180 ± 20 ly (57 ± 5 pc) |
| Absolute magnitude (MV) | 5.26 |
| Details | |
| Mass | 0.84 M☉ |
| Radius | 1.02±0.13 R☉ |
| Luminosity | 0.734±0.134 L☉ |
| Surface gravity (log g) | 4.24 cgs |
| Temperature | 5310±100 K |
| Metallicity | -0.11 |
| Other designations | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
| Extrasolar Planets Encyclopaedia |
data |
HD 290327 is a 9th magnitude G-type subgiant star located approximately 180 light years away in the constellation Orion. This star is larger, cooler, fainter, and less massive than our Sun. Also its metal content is seven-ninths as much as the Sun. In 2009, a gas giant planet was found in orbit around the star.[2]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | ≥ 2.54+0.17 −0.14 MJ |
3.43+0.20 −0.12 |
2443+205 −117 |
0.08+0.08 −0.03 |
— | — |
See also
References
Coordinates: 
05h 23m 21.5647s, −02° 16′ 39.428″
<templatestyles src="Asbox/styles.css"></templatestyles>
 |
This subgiant-star-related article is a stub. You can help Wikipedia by expanding it. |
<templatestyles src="Asbox/styles.css"></templatestyles>
 |
This extrasolar-planet-related article is a stub. You can help Wikipedia by expanding it. |
