U Aquilae

U Aquilae

A visual band light curve for U Aquilae, adapted from Kiss (1998)
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila
Right ascension 19h 29m 21.3603s
Declination −07° 02 38.710
Apparent magnitude (V) 6.08 - 6.86
Characteristics
Spectral type F5-G1 I-II + B9.8V
U−B color index 0.70
B−V color index 1.10
Variable type δ Cep
Astrometry
Radial velocity (Rv)−6.5 km/s
Proper motion (μ) RA: −0.99 mas/yr
Dec.: −9.14 mas/yr
Parallax (π)3.63±0.96 mas
Distance614 pc
Absolute magnitude (MV)−3.68
Orbit
Period (P)1,856
Semi-major axis (a)1.311"
(6.1 AU)
Eccentricity (e)0.165
Inclination (i)74°
Longitude of the node (Ω)190°
Details
A
Mass5.7 M
Radius55 R
Luminosity2,570 L
Surface gravity (log g)1.3 cgs
Temperature5,440-6,640 K
Metallicity [Fe/H]0.17 dex
B
Mass2.3 M
Radius2.1 R
Temperature9,300 K
Other designations
U Aql, AAVSO 1924-07, BD−07°4968, GC 26905, HD 183344, HIP 95820, HR 7402, SAO 143454, ADS 12503, CCDM J19294-0703
Database references
SIMBADdata

U Aquilae is a binary star system in the constellation Aquila, Located approximately 614 parsecs (2,000 ly) away from Earth.

The primary star (component A) is a yellow supergiant with a radius of 55 R and a luminosity of 2,570 L. The secondary (component B) is a blue main-sequence star, twice the mass of the sun and around thirty times more luminous. It is hotter than the primary star at 9,300 K, but much smaller and fainter. The two stars orbit every five years and their separation varies from five to seven astronomical units in a mildly eccentric orbit.

Discovery of the variability of U Aquilae was announced by Edwin F. Sawyer in 1886. In his announcement, he called the star 50 Aquilae, which is its designation in Uranometria Argentina. Sawyer had begun observing the star in late 1882, and had derived a period of "about one week". It was listed with its variable star designation, U Aquilae, in Annie Jump Cannon's 1907 Second Catalogue of Variable Stars.

U Aquilae A is a classical Cepheid variable star, ranging between magnitudes 6.08 and 6.86 over a period of 7.02 days. It is an evolved star which has exhausted its core hydrogen and is now fusing helium into carbon.