Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquarius |
Right ascension | 22h 54m 45.47009s[1] |
Declination | –16° 16′ 19.0505″[1] |
Apparent magnitude (V) | 5.55[2] |
Characteristics | |
Evolutionary stage | giant |
Spectral type | K1 III[3] |
U−B color index | +1.089[2] |
B−V color index | +1.104[2] |
Variable type | suspected[4] |
Astrometry | |
Radial velocity (Rv) | −34.59±0.16[1] km/s |
Proper motion (μ) | RA: –222.505[1] mas/yr Dec.: –88.355[1] mas/yr |
Parallax (π) | 24.1777 ± 0.1211 mas[1] |
Distance | 134.9 ± 0.7 ly (41.4 ± 0.2 pc) |
Absolute magnitude (MV) | 2.46[5] |
Details | |
Mass | 1.14[6] M☉ |
Radius | 5.79+0.22 −0.21[1] R☉ |
Luminosity | 13.347±0.085[1] L☉ |
Surface gravity (log g) | 2.8[7] cgs |
Temperature | 4,583+86 −83[1] K |
Metallicity [Fe/H] | +0.03[7] dex |
Rotational velocity (v sin i) | 3.9[7] km/s |
Age | 7.61[6] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
77 Aquarii is a single[9] star located 135 light years away from the Sun in the equatorial constellation of Aquarius. 77 Aquarii is its Flamsteed designation. It is visible to the naked eye as a dim star with a baseline apparent visual magnitude of 5.55.[2] The star is moving closer to the Earth with a heliocentric radial velocity of −35 km/s.[1]
At the estimated age of 7.61[6] billion years old, this is an aging giant star with a stellar classification of K1 III.[3] It is a suspected variable star that ranges in brightness from a maximum of magnitude 5.53 down to 5.60.[4] 77 Aquarii has 1.14[6] times the mass of the Sun and, after exhausting the hydrogen at its core, has expanded to six times the Sun's radius. It is radiating 13.3[1] times the Sun's luminosity from its photosphere at an effective temperature of 4,581 K,[7] giving it the orange-hued glow of a K-type star.[10]
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