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P Eridani

p Eridani AB
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Eridanus
Right ascension 01h 39m 47.53953s
Declination −56° 11′ 47.0997″
Apparent magnitude (V) 5.87 + 5.76
Characteristics
Spectral type K2V + K2V
U−B color index +0.59 / +0.53
B−V color index +0.90 / +0.87
Astrometry
Radial velocity (Rv) +19.5 km/s
Proper motion (μ) RA: 282.16 mas/yr
Dec.: 10.56 mas/yr
Parallax (π) 127.84 ± 2.19mas
Distance 25.5 ± 0.4 ly
(7.8 ± 0.1 pc)
Absolute magnitude (MV) 6.25 / 6.35
Orbit
Companion p Eridani B
Period (P) 483.66 yr
Semi-major axis (a) 7.817"
Eccentricity (e) 0.5344
Inclination (i) 142.824°
Longitude of the node (Ω) 13.116°
Periastron epoch (T) 1813.494
Details
Metallicity [Fe/H] –0.23 dex
Rotation 30 days
Age 4.8 Gyr
Other designations
Gliese 66, CD−56°328, GCTP 352.00, SAO 232490, WDS 01398-5612, DUN 5, HIP 7751
6 Eri A: HR 486, HD 10360, LTT 903
6 Eri B: HR 487, HD 10361, LTT 902
Database references
SIMBAD data

p Eridani (6 Eri, DUN 5) is a binary star system in the constellation of Eridanus (the River) whose distance is approximately 26 light-years. It was found to be a double star in December 1825 by James Dunlop in Australia at his home at Paramatta, now spelt Parramatta.

The name "p Eridani", according to Nature, p. 589 (19 April 1883) has been:

"... occasionally miscalled 6 Eridani, which would imply that it was one of Flamsteed's stars. Flamsteed, it is true has a star which he calls 6 Eridani. The designated letter 'p' was attached to a star by Lacaille in the catalogue at the end of his Coelum Australe Stelliferum. The number '6' is merely borrowed from Bode."

The use of Bode numbers was commonly used in the early 19th century, but this antiquated system has now fallen into disuse for more than a century.


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Wikipedia

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