Phi Aquarii

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Template:Short description

Phi Aquarii
Template:Location mark
Location of φ Aquarii (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Aquarius
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) +4.223[2]
Characteristics
Spectral type M1.5 III[3]
U−B Template:Engvar +1.897[2]
B−V Template:Engvar +1.563[2]
Astrometry
Radial velocity (Rv)+2.48±0.32[4] km/s
Proper motion (μ) RA: +36.575 mas/yr[1]
Dec.: −195.441 mas/yr[1]
Parallax (π)14.3482±0.2594 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)0.30±0.120[5]
Details
A
Mass1.00±0.03[6] Template:Solar mass
Radius34.77Script error: No such module "Su".[6] Template:Solar radius
Luminosity207.7±25.2[6] Template:Solar luminosity
Surface gravity (log g)1.5[4] cgs
Temperature3,715±48[6] K
Rotational velocity (v sin i)6.7[4] km/s
Age10.97±0.83[6] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[7]
Database references
SIMBADdata

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Phi Aquarii is a binary star[8] system in the equatorial constellation of Aquarius. Its name is a Bayer designation that is Latinized from φ Aquarii, and abbreviated Phi Aqr or φ Aqr. This system is visible to the naked eye as a point of light with a combined apparent visual magnitude of +4.223.[2] Parallax measurements indicate its distance from Earth is approximately Script error: No such module "convert"..[1] It is drifting further away with a radial velocity of +2.5 km/s.[4] The system is positioned 1.05 degrees south of the ecliptic so it is subject to lunar occultations.[9]

This is a spectroscopic binary star system with an estimated period of Script error: No such module "convert"..[10] The primary component is an aging red giant star with a stellar classification of M1.5 III.[3] At an estimated age of 11 billion years,[6] it has exhausted the supply of hydrogen at its core and evolved away from the main sequence. The star has the same mass as the Sun,[6] but has expanded to 35 times the Sun's girth.[6] It is radiating 208 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 3,715 K,[6] giving it the reddish hue of an M-type star.[11]

On 6 September 2019, it had a close conjunction (geocentric separation <1') with Neptune.[12] Template:Rp

References

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  7. Template:Cite simbad
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External links

Template:Stars of Aquarius