Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquarius |
Right ascension | 21h 22m 56.25866s[1] |
Declination | −09° 19′ 09.5823″[1] |
Apparent magnitude (V) | 5.99[2] |
Characteristics | |
Spectral type | K4/5 III[3] |
B−V color index | 1.516±0.008[2] |
Astrometry | |
Radial velocity (Rv) | 18.2±2.9[4] km/s |
Proper motion (μ) | RA: −29.659[1] mas/yr Dec.: −29.022[1] mas/yr |
Parallax (π) | 4.9125 ± 0.1260 mas[1] |
Distance | 660 ± 20 ly (204 ± 5 pc) |
Absolute magnitude (MV) | −0.73[2] |
Orbit[5] | |
Period (P) | 7,290 d |
Eccentricity (e) | 0.4 |
Details | |
17 Aqr A | |
Luminosity | 495.46[2] L☉ |
Surface gravity (log g) | 1.74±0.14[6] cgs |
Temperature | 3,951±14[6] K |
Metallicity [Fe/H] | −0.10±0.06[6] dex |
Other designations | |
Database references | |
SIMBAD | data |
17 Aquarii, abbreviated 17 Aqr, is a spectroscopic binary[5] star system in the constellation of Aquarius. 17 Aquarii is the Flamsteed designation. It appears to the naked eye as a faint sixth magnitude star, having a combined apparent visual magnitude of 5.99.[2] The distance to 17 Aqr can be estimated from its annual parallax shift of 4.9 mas,[1] which yields a separation of around 660 light years. It is moving further away with a heliocentric radial velocity of 18 km/s.[4]
A preliminary orbit for the pair gives a period of 20 years and an eccentricity of 0.4.[5] The primary component is an aging giant star with a stellar classification of K4/5 III.[3] It is radiating 495[2] times the Sun's luminosity from its photosphere at an effective temperature of 3,951 K.[6]
GaiaDR2
was invoked but never defined (see the help page).Anderson2012
was invoked but never defined (see the help page).Houk1999
was invoked but never defined (see the help page).Gontcharov2006
was invoked but never defined (see the help page).Famaey2009
was invoked but never defined (see the help page).Wu2011
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).