Eta Sagittae

Eta Sagittae (η Sagittae) is solitary^[9] star in the northern constellation of Sagitta. It is faintly visible to the naked eye, having an apparent visual magnitude of +5.09.^[2] Based upon an annual parallax shift of 20.34 mas,^[1] it is approximately 160 light years distant from the Sun. There is a 61.1% chance that it is a member of the Hyades-Pleiades stream of stars that share a common motion through space.^[10]

η Sagittae

Location of η Sagittae (circled)
Observation data Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation	Sagitta
Right ascension	20h 05m 09.49303s[1]
Declination	+19° 59′ 27.8575″[1]
Apparent magnitude (V)	+5.09[2]
Characteristics
Evolutionary stage	red clump[3]
Spectral type	K2 III[4]
U−B color index	+0.98[2]
B−V color index	+1.06[2]
Astrometry
Radial velocity (Rv)	−40.53[5] km/s
Proper motion (μ)	RA: +29.962±0.173[5] mas/yr Dec.: +80.440±0.173[5] mas/yr
Parallax (π)	20.9262±0.1208 mas[5]
Distance	155.9 ± 0.9 ly (47.8 ± 0.3 pc)
Absolute magnitude (MV)	1.61[6]
Details[7]
Mass	1.73±0.09 M☉
Radius	7.08±0.21 R☉
Luminosity	26 L☉
Surface gravity (log g)	3.03±0.10 cgs
Temperature	4,784±3.03 K
Metallicity [Fe/H]	+0.10 dex
Rotational velocity (v sin i)	1.3[6] km/s
Age	1.69±0.25 Gyr
Other designations
η Sge, 16 Sge, BD+19°4277, FK5 3609, GC 27868, HD 190608, HIP 98920, HR 7679, SAO 105659, PPM 137588[8]
Database references
SIMBAD	data

This is an evolved K-type giant star with a stellar classification of K2 III.^[4] At the age of about 1.7 billion years,^[7] it is now a red clump star that is generating energy through the fusion of helium at its core.^[3] Eta Sagittae has 1.7 times the mass of the Sun and has expanded to seven times the Sun's radius. It is radiating 25.7 times the Sun's luminosity from its photosphere at an effective temperature of 4,784 K.^[7]