Eta Arietis

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Eta Arietis
Diagram showing star positions and boundaries of the Aries constellation and its surroundings
Cercle rouge 100%.svg

Location of η Arietis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Aries
Right ascension 02h 12m 48.08619s[1]
Declination +21° 12′ 39.5839″[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: +163.49[1] mas/yr
Dec.: +5.22[1] mas/yr
Parallax (π) 34.64 ± 0.33[1] mas
Distance 94.2 ± 0.9 ly
(28.9 ± 0.3 pc)
Absolute magnitude (MV) +2.93[2]
Details
Mass 1.3 M
Radius 0.98[5] R
Surface gravity (log g) 4.01[3] cgs
Temperature 6,380[3] K
Metallicity [Fe/H] –0.35[3] dex
Rotational velocity (v sin i) 9[6] km/s
Age 2.6[2] Gyr
Other designations
17 Arietis, BD+20 348, GJ 1043, HD 13555, HIP 10306, HR 646, SAO 75204.[4]

Eta Arietis (η Ari, 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 34.64 mas,[1] the distance to this star is approximately 94.2 light-years (28.9 parsecs).

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.[7] Nor has an infrared excess been detected using the Spitzer Space Telescope, which might otherwise indicate the presence of circumstellar gas or dust.[8]

References

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External links