Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Eridanus |
Right ascension | 02h 40m 40.03501s[1] |
Declination | −39° 51′ 19.3541″[1] |
Apparent magnitude (V) | 4.11[2] |
Characteristics | |
Evolutionary stage | Red clump[3] |
Spectral type | K0 III[4] |
U−B color index | +0.74[2] |
B−V color index | +1.02[2] |
Astrometry | |
Radial velocity (Rv) | −9.30±0.70[5] km/s |
Proper motion (μ) | RA: +135.92[1] mas/yr Dec.: −27.53[1] mas/yr |
Parallax (π) | 21.65 ± 0.18 mas[1] |
Distance | 151 ± 1 ly (46.2 ± 0.4 pc) |
Absolute magnitude (MV) | 0.877[3] |
Details[6] | |
Mass | 1.29±0.01 M☉ |
Radius | 11.17±0.06 R☉ |
Luminosity | 54.7±0.5 L☉ |
Surface gravity (log g) | 2.65±0.10 cgs |
Temperature | 4,700±30 K |
Metallicity [Fe/H] | −0.34±0.02 dex |
Age | 3.55±0.12 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Iota Eridani (ι Eri) is a solitary star in the constellation Eridanus. It is visible to the naked eye with an apparent magnitude of 4.11.[2] With an annual parallax shift of 0.02165 arcseconds,[1] it lies at an estimated distance of about 151 light years.
This is an evolved giant star with a stellar classification of K0 III.[4] The measured angular diameter, after correcting for limb darkening, is 2.248±0.014 mas. This star is 3.55 billion years old, sufficient to have exhausted the hydrogen at its core and reached a red clump stage. It is only around 29% more massive than the Sun, but is eleven times larger. It radiates 54.7 times the solar luminosity from its outer atmosphere at an effective temperature of 4,700 K.[6]
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