31 Aquilae (abbreviated 31 Aql) is a star in the equatorial constellation of Aquila. 31 Aquilae is its Flamsteed designation though it also bears the Bayer designation b Aquilae. This star has an apparent visual magnitude of 5.16 and is 49.5 light years from Earth. It has no known companions.
Properties 31 Aquilae has an apparent visual magnitude of 5.16, making it bright enough to be seen with the naked eye in dark skies. The annual parallax shift of yields a distance estimate of from Earth. It is a variable star with a magnitude change of less than 0.02.
With a stellar classification of G8 IV, the luminosity class of IV indicates this is a subgiant star. Compared to the Sun, it has 107% of the mass and 135% of the radius. It is radiating 1.64 the luminosity of the Sun from its outer atmosphere at an effective temperature of 5,617 K, giving it the yellow hue of a G-type star. Its age is probably similar to NGC 188, the oldest open cluster known, which was calculated to be over 5 billion years. For its age, it is surprisingly rich in elements other than hydrogen or helium, contrary to common assumptions that the oldest stars should be metal-poor. Asteroseismology suggests an age of nine billion years.
No certain substellar companion has been detected so far around 31 Aquilae. McDonald Observatory team has set limits to the presence of one or more planets around 31 Aquilae with masses between 0.22 and 1.9 Jupiter masses and average separations spanning between 0.05 and 5.2 astronomical units.
Optical companions The following stars are optical companions that are coincidentally aligned near the line of sight to 31 Aquilae.
Companion HD 231345 BD+11 3833C Right ascension Declination Magnitude 8.56 10.6 Spectral type G0 Reference Simbad Simbad
References
External links The Old Disk Metal-Rich Subgiant 31 Aquilae Image 31 Aquilae HR 7373 CCDM 19249+1157 R.A. Wittenmeyer et al., "Detection Limits from the McDonald Observatory Planet Search Program", The Astronomical Journal, Volume 132, Issue 1, pp. 177–188, May 2006.