Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aries |
Right ascension | 02h 12m 48.08568s [1] |
Declination | +21° 12′ 39.5776″ [1] |
Apparent magnitude (V) | 5.231 [2] |
Characteristics | |
Spectral type | F5 V [3] |
U−B color index | –0.04 [4] |
B−V color index | +0.44 [4] |
Astrometry | |
Radial velocity (Rv) | +4.5 [2] km/s |
Proper motion (μ) |
RA: +163.917
[1]
mas/
yr Dec.: +5.000 [1] mas/ yr |
Parallax (π) | 33.3383 ± 0.1196 mas [1] |
Distance | 97.8 ± 0.4
ly (30.0 ± 0.1 pc) |
Absolute magnitude (MV) | +2.93 [2] |
Details | |
Mass | 1.21 [5] M☉ |
Radius | 1.823 [6] R☉ |
Luminosity | 6.0 [6] L☉ |
Surface gravity (log g) | 4.01 [3] cgs |
Temperature | 6,700 [6] K |
Metallicity [Fe/H] | –0.35 [3] dex |
Rotational velocity (v sin i) | 9 [7] km/s |
Age | 2.6 Gyr
[2] 3.98 [5] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Eta Arietis, Latinized from η Arietis, is the Bayer designation for a star in the northern constellation of Aries. It is dimly visible to the naked eye with an apparent visual magnitude of 5.231. [2] With an annual parallax shift of 33.34 mas, [1] the distance to this star is approximately 97.8 light-years (30.0 parsecs). It is drifting further away with a radial velocity of +4.5 km/s. [2]
This is an F-type main sequence star with a stellar classification of F5 V. [3] It is younger than the Sun at an age of about 2.6 billion years. [2] The effective temperature of the outer atmosphere is 6,380 K, [3] giving it the yellow-white-hued glow of an F-type star. Eta Arietis was examined using the HARPS instrument for radial velocity variations that may be caused by an orbiting companion, but no signal was detected. [8] Nor has an infrared excess been detected using the Spitzer Space Telescope, which might otherwise indicate the presence of circumstellar gas or dust. [9]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aries |
Right ascension | 02h 12m 48.08568s [1] |
Declination | +21° 12′ 39.5776″ [1] |
Apparent magnitude (V) | 5.231 [2] |
Characteristics | |
Spectral type | F5 V [3] |
U−B color index | –0.04 [4] |
B−V color index | +0.44 [4] |
Astrometry | |
Radial velocity (Rv) | +4.5 [2] km/s |
Proper motion (μ) |
RA: +163.917
[1]
mas/
yr Dec.: +5.000 [1] mas/ yr |
Parallax (π) | 33.3383 ± 0.1196 mas [1] |
Distance | 97.8 ± 0.4
ly (30.0 ± 0.1 pc) |
Absolute magnitude (MV) | +2.93 [2] |
Details | |
Mass | 1.21 [5] M☉ |
Radius | 1.823 [6] R☉ |
Luminosity | 6.0 [6] L☉ |
Surface gravity (log g) | 4.01 [3] cgs |
Temperature | 6,700 [6] K |
Metallicity [Fe/H] | –0.35 [3] dex |
Rotational velocity (v sin i) | 9 [7] km/s |
Age | 2.6 Gyr
[2] 3.98 [5] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Eta Arietis, Latinized from η Arietis, is the Bayer designation for a star in the northern constellation of Aries. It is dimly visible to the naked eye with an apparent visual magnitude of 5.231. [2] With an annual parallax shift of 33.34 mas, [1] the distance to this star is approximately 97.8 light-years (30.0 parsecs). It is drifting further away with a radial velocity of +4.5 km/s. [2]
This is an F-type main sequence star with a stellar classification of F5 V. [3] It is younger than the Sun at an age of about 2.6 billion years. [2] The effective temperature of the outer atmosphere is 6,380 K, [3] giving it the yellow-white-hued glow of an F-type star. Eta Arietis was examined using the HARPS instrument for radial velocity variations that may be caused by an orbiting companion, but no signal was detected. [8] Nor has an infrared excess been detected using the Spitzer Space Telescope, which might otherwise indicate the presence of circumstellar gas or dust. [9]