P Eridani
From Wikipedia, the free encyclopedia
Observation data Epoch J2000 |
|
---|---|
Constellation | Eridanus |
Right ascension | 01h 39m 47.2s |
Declination | -56° 11′ 44″ |
Apparent magnitude (V) | 5.80/5.90 |
Spectral Characteristics | |
Spectral type | K2 V/K3 V |
U-B color index | 0.56/0.61 |
B-V color index | 0.85/0.88 |
Variable type | None |
Astrometry | |
Radial velocity (Rv) | +19.5 km/s |
Proper motion (μ) | RA: 286.10 mas/yr Dec.: 16.66 mas/yr |
Parallax (π) | 123.90 ± 1.38 mas |
Distance | 26.3 ± 0.3 ly (8.07 ± 0.09 pc) |
Absolute magnitude (MV) | 6.25/6.35 |
Physical Characteristics | |
Mass | 0.88/0.86 M☉ |
Radius | 0.79/0.6 R☉ |
Luminosity | 0.28/0.25 L☉ |
Temperature | ? K |
Metallicity | ? |
Rotation | ? |
Age | ? years |
Visual binary orbit | |
Companion | p Eridani B |
Period (P) | 483.66 years |
Semimajor axis (a) | 7.817" |
Eccentricity (e) | 0.5344 |
Inclination (i) | 142.824° |
Node (Ω) | 13.116° |
Periastron epoch (T) | 1813.494 |
Other designations | |
p Eridani is a multiple star system in the constellation Eridani.
It one of the nearest star in the constellation and it lies about 26.6 light years from the Sun, and consists of two visible components that orbit each other in a wide orbit with a relatively high eccentricity. The closest that these components approach each other is 29.7 astronomical units (or AUs) and the maximum separation is 97.7 AU. The fainter of the two stars also appears to have a spectroscopic companion.
[edit] References
- William I. Hartkopf & Brian D. Mason, "Sixth Catalog of Orbits of Visual Binary Stars", U.S. Naval Observatory, 2001.
[edit] External links
- p Eridani 3? at SolStation.
- ARICNS for Gl 66 A and Gl 66 B.
- Alcyone ephemeris