Pi Eridani

Pi Eridani, Latinized from π Eridani, is a star in the constellation Eridanus. It has an apparent visual magnitude of 4.40, which is bright enough to be seen on a dark, clear night. Based upon parallax measurements, it is located roughly 480 light years from the Sun.

π Eridani
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Eridanus
Right ascension 03h 46m 08.53581s
Declination −12° 06 05.7282
Apparent magnitude (V) 4.40 (4.38 - 4.44)
Characteristics
Evolutionary stage asymptotic giant branch
Spectral type M1 III
U−B color index +1.96
B−V color index +1.61
Variable type Lb?
Astrometry
Radial velocity (Rv)45.2±0.1 km/s
Proper motion (μ) RA: +55.98 mas/yr
Dec.: +59.28 mas/yr
Parallax (π)6.78 ± 0.53 mas
Distance480 ± 40 ly
(150 ± 10 pc)
Absolute magnitude (MV)−1.40
Details
Radius77 R
Luminosity1,123 L
Temperature3,841 K
Other designations
π Eridani, π Eri, 26 Eridani, BD-12° 707, HD 23614, HIP 17593, HR 1162, SAO 149158.
Database references
SIMBADdata

This is an evolved red giant star with a stellar classification of M1 III, and is currently on the asymptotic giant branch. It is a slow irregular variable type LB that can increase in magnitude up to 4.38. The measured angular diameter of this star is 4.8±0.5 mas. At the estimated distance of Pi Eridani, this yields a physical size of about 77 times the radius of the Sun. It shines with 1,123 times the luminosity of the Sun from an outer atmosphere at an effective temperature of 3,841 K.

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.