Observation data Epoch J2000.0 Equinox J2000.0 (ICRS)
Constellation
Eridanus
Right ascension
02h 26m 59.12177s[1]
Declination
−47° 42′ 13.8247″[1]
Apparent magnitude (V)
4.25[2]
Characteristics
Spectral type
B7 IV[3]
U−B color index
−0.50[2]
B−V color index
−0.14[2]
Astrometry
Radial velocity (Rv)
+25.5±0.5[4] km/s
Proper motion (μ)
RA: +19.32[1] mas/yr Dec.: −5.54[1] mas/yr
Parallax (π)
6.42 ± 0.15 mas[1]
Distance
510 ± 10 ly (156 ± 4 pc)
Absolute magnitude (MV)
−1.72[5]
Details[3]
Mass
5.0±0.8M☉
Radius
6[6][7]R☉
Luminosity
1,175 L☉
Surface gravity (log g)
3.5±0.1 cgs
Temperature
14,700±400 K
Metallicity [Fe/H]
0.02±0.06[8] dex
Rotational velocity (v sin i)
10±8 km/s
Age
93 Myr
Other designations
κ Eri, CD-48° 637, FK5 86, HD 15371, HIP 11407, HR 721, SAO 215906.[9]
Database references
SIMBAD
data
Kappa Eridani, Latinized from κ Eridani, is a solitary star in the constellation Eridanus. With an apparent visual magnitude of 4.25,[2] it is bright enough to be visible to the naked eye on a dark night. Based upon an annual parallax shift of 0.00642 arc seconds,[1] it is roughly 510 light years distant from the Sun.
This appears to be an evolving B-type subgiant star with a stellar classification of B7 IV.[3] The measured angular diameter is 0.346±0.008 mas.[8] At an estimated distance of Kappa Eridani, this yields a physical size of about six times the radius of the Sun.[6] It has five times the Sun's mass, and radiates 1,175 times the solar luminosity from its outer atmosphere at an effective temperature of 14,700 K. Kappa Eridani is spinning with a projected rotational velocity of 10 km/s and is around 93 million years old.[3]
^ abcdefCite error: The named reference vanLeeuwen2007 was invoked but never defined (see the help page).
^ abcdCite error: The named reference Johnson1966 was invoked but never defined (see the help page).
^ abcdCite error: The named reference Levenhagen2006 was invoked but never defined (see the help page).
^Cite error: The named reference deBruijne2012 was invoked but never defined (see the help page).
^Cite error: The named reference Anderson2012 was invoked but never defined (see the help page).
^ abCite error: The named reference lang2006 was invoked but never defined (see the help page).
^Cite error: The named reference cadars was invoked but never defined (see the help page).
^ abCite error: The named reference Niemczura2003 was invoked but never defined (see the help page).
^Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
KappaEridani, Latinized from κ Eridani, is a solitary star in the constellation Eridanus. With an apparent visual magnitude of 4.25, it is bright enough...
Theta Eridani, Chi Eridani, Phi Eridani, KappaEridani, HD 16754, HD 23319, HD 24072, HD 24160, Upsilon4 Eridani, Upsilon3 Eridani, Upsilon2 Eridani and...
Upsilon2 Eridani, Chi Eridani, Phi Eridani, KappaEridani, HD 16754, HD 23319, Theta Eridani, HD 24072, HD 24160, Upsilon4 Eridani, Upsilon3 Eridani and Upsilon1...
Upsilon3 Eridani, Chi Eridani, Phi Eridani, KappaEridani, HD 16754, HD 23319, Theta Eridani, HD 24072, HD 24160, Upsilon4 Eridani, Upsilon2 Eridani and Upsilon1...
Binary star system 3.55 Kappa Ursae Majoris Binary star system 3.559 Lambda Geminorum Triple star system 3.56 Upsilon4 Eridani Binary star system 3.56...
Cambridge University Press. p. 170. ISBN 0-521-44921-9. Kaler, James B. "Saiph (Kappa Orionis)". Stars. University of Illinois. Archived from the original on...
ٱلْنََهْر Theta Eridani Achernar Ākhiru-n-Nahr the River's or Stream's End / Tail / Edge / Border آخر النهر آخِرُ ٱلْنََهْر Alpha Eridani Acrab ʽAqrab the...
the 25th brightest star in the night sky. Beta Eridani (Cursa) 90±0.9 A3 III var or A3 IV 2.4 2 2.796 Kappa Ophiuchi 91.5±0.5 K2III 11 1.19 ± 0.14 3.20 Eta...
Beta Fornacis marking the shallow southern apex. Originally designated 12 Eridani by John Flamsteed, Alpha Fornacis was named by Lacaille as the brightest...
done by Popper in 1954, measuring a 21 km/s gravitational redshift of 40 Eridani B. The redshift of Sirius B was finally measured by Greenstein et al. in...
"Confirming Fundamental Properties of the Exoplanet Host Star epsilon Eridani Using the Navy Optical Interferometer" (2012, ApJ, 744, 138B)". The Astrophysical...
Torsten; Chavez-Dagostino, Miguel (2023-06-01). "The clumpy structure of ϵ Eridani's debris disc revisited by ALMA". Monthly Notices of the Royal Astronomical...
Spring and Autumn period. The other components are Beta Cassiopeiae (Caph), Kappa Cassiopeiae, Alpha Cassiopeiae (Schedar) and Lambda Cassiopeiae. Consequently...
poor or rejected stars. Six stars, namely Iota Herculis, 53 Piscium, Nu Eridani, Gamma Pegasi, HD 13745 (V354 Persei) and 53 Arietis had been found to...
characterize numerous Jovian planets, including the nearest Jupiter analogues ε Eridani b and ε Indi Ab. In addition, radio astrometry using the VLBA has been...
done by Popper in 1954, measuring a 21 km/s gravitational redshift of 40 Eridani B. The redshift of Sirius B was finally measured by Greenstein et al. in...