58 Eridani

58 Eridani is a main-sequence star in the constellation Eridanus. It is a solar analogue,[12] having similar physical properties to the Sun. The star has a relatively high proper motion across the sky, and it is located 43 light years distant. It is a probable member of the IC 2391 moving group of stars that share a common motion through space.[10]

58 Eridani

A light curve for IX Eridani, plotted from Hipparcos data[1]
Observation data
Epoch J2000      Equinox J2000
ConstellationEridanus
Right ascension04h 47m 36.29171s[2]
Declination–16° 56′ 04.04-4″[2]
Apparent magnitude (V)5.47 - 5.51[3]
Characteristics
Evolutionary stagemain sequence[2]
Spectral typeG1.5 V CH-0.5[4]
U−B color index+0.13[5]
B−V color index+0.64[5]
Variable typeBY Dra[3]
Astrometry
Radial velocity (Rv)21.60±0.12[2] km/s
Proper motion (μ) RA: +130.264[2] mas/yr
Dec.: +169.338[2] mas/yr
Parallax (π)75.5289 ± 0.0539 mas[2]
Distance43.18 ± 0.03 ly
(13.240 ± 0.009 pc)
Absolute magnitude (MV)4.87[6]
Details
Mass1.053±0.007[7] M
Radius1.00[2] R
Luminosity0.97±0.05[2] L
Surface gravity (log g)4.50±0.02[8] cgs
Temperature5,820±5.7[9] K
Metallicity [Fe/H]0.030±0.007[8] dex
Rotation7.6 days[10]
Rotational velocity (v sin i)3.37±0.11[8] km/s
Age600[11] Myr
Other designations
58 Eri, IX Eri, BD−17°954, GJ 177, HD 30495, HIP 22263, HR 1532, SAO 149888, LTT 2088
Database references
SIMBADdata

Characteristics

This is a BY Draconis variable with the designation IX Eridani, which ranges in magnitude from 5.47 down to 5.51 with a period of 11.3 days.[3] The X-ray emissions from this star's corona indicate an age of less than a billion (109) years,[13] compared to 4.6 billion for the Sun, so it is still relatively young for a star of its mass. Starspot activity has also been detected, which varies from year to year.

A circumstellar disc of dust particles has been detectedin orbit around 58 Eridani.[14]

See also

References