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Rho Aquilae

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

Location of ρ Aquilae (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Delphinus
Right ascension 20h 14m 16.61886s
Declination +15° 11′ 51.3923″
Apparent magnitude (V) 4.94
Characteristics
Spectral type A2 V
U−B color index +0.01
B−V color index +0.09
Astrometry
Radial velocity (Rv) –23.0 km/s
Proper motion (μ) RA: +55.03 mas/yr
Dec.: +58.14 mas/yr
Parallax (π) 21.75 ± 0.26mas
Distance 150 ± 2 ly
(46.0 ± 0.5 pc)
Details
Surface gravity (log g) 4.07 ± 0.07 cgs
Temperature 8,804 ± 95 K
Metallicity [Fe/H] –0.48 ± 0.10 dex
Rotational velocity (v sin i) 180 km/s
Age 50 to 120 Myr
Other designations
Tso Ke, 67 Aquilae, BD+14 4227, FK5 1526, HD 192425, HIP 99742, HR 7724, SAO 105878.
Database references
SIMBAD data

Rho Aquilae (ρ Aql, ρ Aquilae) is the Bayer designation for a star in the northern constellation of Delphinus – it moved across the border from Aquila into Delphinus in 1992. It has an apparent visual magnitude of 4.94 and is bright enough to be seen with the naked eye in good conditions. The annual parallax shift of this star is 21.75 milliarcseconds, which corresponds to a physical distance of around 150 light-years (46 parsecs) from Earth.

This star has the traditional name Tso Ke, from the Cantonese 左旗 jo keih meaning "the left flag". In Chinese, 左旗 (Zuǒ Qí in Mandarin), meaning Left Flag, refers to an asterism consisting of ρ Aquilae, α Sagittae, β Sagittae, δ Sagittae, ζ Sagittae, γ Sagittae, 13 Sagittae, 11 Sagittae and 14 Sagittae. Consequently, ρ Aquilae itself is known as 左旗九 (Zuǒ Qí jiǔ, English: the Ninth Star of Left Flag.)

Rho Aquilae is an A-type main sequence star with a stellar classification of A2 V. This star is about 50 to 120 million years old and it displays an excess emission of infrared radiation that may be explained by a circumstellar disk of dust.


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Wikipedia

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