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82 Aquarii

Star in the constellation Aquarius From Wikipedia, the free encyclopedia

82 Aquarii is a star in the equatorial constellation of Aquarius. 82 Aquarii is its Flamsteed designation. It has an apparent visual magnitude of 6.15,[2] which, according to the Bortle Dark-Sky Scale, means it is a faint star that requires dark rural skies to view. The annual parallax shift of 82 Aquarii is 3.6764±0.1715 mas, which equates to a distance of roughly 890 light-years (270 parsecs) from Earth.[6] Because this star is positioned near the ecliptic, it is subject to lunar eclipses.[7]

Right ascension23h 02m 32.55694s[1]
Declination−06° 34 26.4458[1]
Quick facts Constellation, Right ascension ...
82 Aquarii
Observation data
Epoch J2000      Equinox ICRS
Constellation Aquarius
Right ascension 23h 02m 32.55694s[1]
Declination −06° 34 26.4458[1]
Apparent magnitude (V) 6.15[2]
Characteristics
Evolutionary stage giant
Spectral type M2 III[3]
U−B color index +1.90[2]
B−V color index +1.58[2]
Variable type suspected[4]
Astrometry
Radial velocity (Rv)−3.59±0.17[1] km/s
Proper motion (μ) RA: −7.224[1] mas/yr
Dec.: −33.786[1] mas/yr
Parallax (π)3.6764±0.1715 mas[1]
Distance890 ± 40 ly
(270 ± 10 pc)
Details
Radius56.33+5.50
−7.78
[1] R
Luminosity692.8±37.1[1] L
Temperature3,946+305
−180
[1] K
Other designations
82 Aqr, NSV 25999, BD−07°5913, HD 217701, HIP 113781, HR 8763, SAO 146465[5]
Database references
SIMBADdata
Close

This object is an aging red giant star currently on the asymptotic giant branch[8] with a stellar classification of M2 III,[3] having exhausted both the hydrogen and helium at its core and expanded to 56 times the Sun's radius.[1] It is a suspected variable star of unknown type that ranges in magnitude between 6.24 and 6.29.[4] The star is radiating 693 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 3,946 K.[1]

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