28 Aquilae

28 Aquilae

A light curve for V1208 Aquilae, plotted from Hipparcos data
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila
Right ascension 19h 19m 39.34802s
Declination +12° 22 28.8457
Apparent magnitude (V) 5.51 - 5.56
Characteristics
Spectral type F0 III
U−B color index +0.182
B−V color index +0.257
Variable type δ Sct
Astrometry
Radial velocity (Rv)+4.36 km/s
Proper motion (μ) RA: +4.249 mas/yr
Dec.: +16.199 mas/yr
Parallax (π)9.5836±0.0768 mas
Distance340 ± 3 ly
(104.3 ± 0.8 pc)
Absolute magnitude (MV)+0.46
Details
Mass2.4 M
Radius4.8 R
Luminosity54.20 L
Surface gravity (log g)3.41 cgs
Temperature7,250 K
Metallicity [Fe/H]−0.16 dex
Rotational velocity (v sin i)57 km/s
Age655 Myr
Other designations
28 Aql, V1208 Aql, BD+12°3879, HD 181333, HIP 94982, HR 7331, SAO 104722
Database references
SIMBADdata

28 Aquilae, abbreviated 28 Aql, is a star in the equatorial constellation of Aquila. 28 Aquilae is its Flamsteed designation though it also bears the Bayer designation A Aquilae, and the variable star designation V1208 Aquilae. It has an apparent visual magnitude is 5.5, making this a faint star that requires dark suburban skies to view (according to the Bortle Dark-Sky Scale). The annual parallax shift of 9.6 mas means this star is located at a distance of approximately 340 light-years (100 parsecs) from Earth.

The spectrum of this star matches a stellar classification of F0 III. Despite consistent spectral classifications as a giant star, models show that it is just reaching the end of its main sequence lifetime at an age of 655 million years.

The variability of 28 Aquilae was discovered by Michel Breger in 1969. It was revealed to be a Delta Scuti-type pulsating variable star with at least two periods of pulsation. The known periods have frequencies of 6.68 and 7.12 cycles per day. The outer atmosphere has an effective temperature of 7,250 K, which lies in the range of a yellow-white hued F-type star.