Rho Aquarii

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Rho Aquarii
Diagram showing star positions and boundaries of the Aquarius constellation and its surroundings
Cercle rouge 100%.svg

Location of ρ Aquarii (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Aquarius
Right ascension 22h 20m 11.91628s[1]
Declination –07° 49′ 15.9649″[1]
Apparent magnitude (V) +5.34[2]
Characteristics
Spectral type B8 IIIp Mn:Hg:[3]
U−B color index –0.358[2]
B−V color index –0.057[2]
Astrometry
Radial velocity (Rv) –9[4] km/s
Proper motion (μ) RA: +14.75[1] mas/yr
Dec.: +1.84[1] mas/yr
Parallax (π) 3.70 ± 0.38[1] mas
Distance approx. 880 ly
(approx. 270 pc)
Details
Mass 5.00 ± 0.22[5] M
Luminosity 1,035[5] L
Temperature 12,593[6] K
Rotational velocity (v sin i) 65[3] km/s
Other designations
46 Aquarii, BD–08 5855, HD 211838, HIP 110273, HR 8512, SAO 146023.[7]
Data sources:
Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.)

Rho Aquarii (ρ Aqr, ρ Aquarii) is the Bayer designation for a binary star in the equatorial constellation of Aquarius. It is visible to the naked eye with an apparent visual magnitude of +5.34.[2] Based upon parallax measurements made during the Hipparcos mission, this star is at a distance of roughly 880 light-years (270 parsecs) from Earth.[1]

This is a single-lined spectroscopic binary, with the presence of a companion being revealed by Doppler shifts in the spectrum.[6] The primary is a giant star with a stellar classification of B8 IIIp Mn:Hg:.[3] It is a Mercury-Manganese star, showing a surfeit of these elements in the spectrum.[6] With five times the Sun's mass, this star is radiating 1,035[5] times as much luminosity from its outer atmosphere at an effective temperature of 12,593 K.[6] This heat gives it the blue-white hue of a B-type star.[8] The companion may be a variable star.[9]

References

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External links