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Star in the constellation Indus From Wikipedia, the free encyclopedia
Eta Indi, Latinised from η Indi, is a single, white-hued star in the southern constellation Indus. It is a faint star but visible to the naked eye with an apparent visual magnitude of 4.52.[2]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Indus |
Right ascension | 20h 44m 02.33404s[1] |
Declination | −51° 55′ 15.4970″[1] |
Apparent magnitude (V) | 4.52[2] |
Characteristics | |
Spectral type | A9IV[3] |
B−V color index | +0.26[2] |
Astrometry | |
Radial velocity (Rv) | −1.6±0.8[4] km/s |
Proper motion (μ) | RA: +155.80[1] mas/yr Dec.: −53.86[1] mas/yr |
Parallax (π) | 41.37 ± 0.25 mas[1] |
Distance | 78.8 ± 0.5 ly (24.2 ± 0.1 pc) |
Absolute magnitude (MV) | 2.59[5] |
Details | |
Mass | 1.60[6] M☉ |
Radius | 2.27[7] R☉ |
Luminosity | 7.60[5] L☉ |
Temperature | 7,694[6] K |
Rotational velocity (v sin i) | 75[8] km/s |
Age | 100±50[7] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Measurements with the Hipparcos spacecraft showed the star, which is single,[9] appears to move against the deep sky backdrop by a mean biannual parallax shift of around 41.37 mas,[1] which equates to 79 light-years' distance. Its radial vector to our system's own trajectory (radial velocity) shows it to be in a phase of a narrowing of the gap, at a rounded −2 km/s, net.[4] η Indi appears to be a member of the Octans association, a group of 62 stars that are around 30−50 million years old and have common motion.[10]
The spectrum of this star matches a stellar classification of A9 IV[3] which suggests it is an evolving subgiant star of type A. The star is estimated 1.6 M☉ (masses of the Sun),[6] and 2.27 R☉ (its radius).[7] It is shines with 7.60[5] times the Sun's luminosity, which is radiated from its photosphere at an effective temperature of 7,694 K.[6] The star is spinning with a projected rotational velocity of 75 km/s.[8] It is very likely to be a hybrid Delta Scuti/Gamma Doradus variable.[8]
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