HD 197037

HD 197037 is a binary star system. Its primary or visible star, HD 197037 A, is a F-type main-sequence star. Its surface temperature is 6150±34 K. HD 197037 A is depleted in heavy elements compared to the Sun, with a metallicity Fe/H index of −0.16±0.03, but is younger at an age of 3.408±0.924 billion years.

HD 197037
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 20h 39m 32.9601s
Declination 42° 14 54.7736
Apparent magnitude (V) 6.813
Characteristics
HD 197037 A
Evolutionary stage main-sequence star
Spectral type F7V
HD 197037 B
Spectral type M
Astrometry
Radial velocity (Rv)9.087±0.199 km/s
Proper motion (μ) RA: -62.745 mas/yr
Dec.: -222.168 mas/yr
Parallax (π)30.2286 ± 0.0143 mas
Distance107.90 ± 0.05 ly
(33.08 ± 0.02 pc)
Position (relative to HD 197037 A)
ComponentHD 197037 B
Epoch of observation2013
Angular distance3.676±0.011
Position angle182.21±0.18°
Projected separation121 AU
Details
HD 197037 A
Mass1.063±0.022 M
Radius1.105±0.023 R
Luminosity1.568±0.074 L
Surface gravity (log g)4.37±0.04 cgs
Temperature6137±20 K
Metallicity [Fe/H]−0.16±0.03 dex
Rotation19.1 d
Age3.408±0.924 Gyr
HD 197037 B
Mass0.3412+0.0098
0.0477
 M
Other designations
BD+41 3845, HIP 101948, LTT 16037, NLTT 49662, TYC 3161-126-1, 2MASS J20393296+4214549
HD 197037 A: Gaia EDR3 2066437688140905600
HD 197037 B: Gaia EDR3 2066437688141580928
Database references
SIMBADdata

A multiplicity survey detected a red dwarf stellar companion HD 197037 B in 2016, at a projected separation of 121 AU. The existence of other stellar companions at projected separations from 1.62 to 45.26 AU was excluded.

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