17 Cygni

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17 Cygni
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 19h 46m 25.60019s[1]
Declination +33° 43′ 39.3452″[1]
Apparent magnitude (V) 5.00[2]
Characteristics
Spectral type F7 V[2] + M0.4[3]
B−V color index 0.46[2]
Astrometry
Radial velocity (Rv) +4.1[4] km/s
Proper motion (μ) RA: +23.25[1] mas/yr
Dec.: –449.31[1] mas/yr
Parallax (π) 47.10 ± 0.26[1] mas
Distance 69.2 ± 0.4 ly
(21.2 ± 0.1 pc)
Absolute magnitude (MV) 3.40[2]
Details
17 Cyg A
Radius 0.95–1.1[5] R
Luminosity 3.66[6] L
Surface gravity (log g) 4.262[6] cgs
Temperature 6,455[6] K
Metallicity [Fe/H] 0.027[6] dex
Rotational velocity (v sin i) 9[2] km/s
Age 2.8[7] Gyr
Other designations
17 Cyg, BD+33 3587, GJ 9670, HD 187013, HIP 97295, HR 7534, SAO 68827.[8]

17 Cygni is the Flamsteed designation for a binary star system in the northern constellation of Cygnus. It has an apparent visual magnitude of 5.00,[2] so, according to the Bortle scale, it is visible from suburban skies at night. Measurements made with the Hipparcos spacecraft show an annual parallax shift of 0.04710″,[1] which is equivalent to a distance of around 69.2 ly (21.2 pc) from the Sun.

The stellar classification of the primary star is F7 V,[2] which means it is a main sequence star like the Sun. It is some 2.8[7] billion years old and shines with 3.66[6] times the Sun's luminosity. The effective temperature of the stellar atmosphere is 6,455[6] K, giving it the yellow-white hued glow of an F-type star.[9]

At an angular separation of 791.40 arcseconds is a proper motion companion with a classification of M0.4, indicating this is a red dwarf star. At the estimated distance of the pair, this is equal to a projected separation of 16,320 AU.[3] Although the CCDM lists four other companions, these are not associated with the pair.[10]

References

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Coordinates: Sky map 19h 46m 25.60s, +33° 43′ 39.35″