Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Hercules |
A [1] | |
Right ascension | 17h 53m 13.0490s [2] |
Declination | +37° 12′ 42.586″ [2] |
Apparent magnitude (V) | 11.592 [3] |
C a | |
Right ascension | ~17h 53m 13.0496s [4] |
Declination | ~+37° 12′ 44.139″ [4] |
Apparent magnitude (V) | 13.85 [1] |
Characteristics | |
Spectral type | F8 [1]/K or M [1] |
Apparent magnitude (B) | 12.1120005 ±0.007 [5] |
Apparent magnitude (V) | 11.592 ±0.004 [5] |
Apparent magnitude (J) | 10.583 ±0.018 [3] |
Apparent magnitude (H) | 10.350 ±0.015 [3] |
Apparent magnitude (K) | 10.330 ±0.019 [3] |
Astrometry | |
A | |
Proper motion (μ) |
RA: −6.382
[2]
mas/
yr Dec.: −20.891 [2] mas/ yr |
Parallax (π) | 1.9686 ± 0.0124 mas [2] |
Distance | 1,660 ± 10
ly (508 ± 3 pc) |
C | |
Proper motion (μ) |
RA: −6.307
[4]
mas/
yr Dec.: −20.387 [4] mas/ yr |
Parallax (π) | 1.9657 ± 0.1076 mas [4] |
Distance | 1,660 ± 90
ly (510 ± 30 pc) |
Details | |
A | |
Mass | 1.18 [1] M☉ |
Radius | 1.9 [2] R☉ |
Luminosity | 4.6 [2] L☉ |
Surface gravity (log g) | 3.98 [2] cgs |
Temperature | 6,200±75[ citation needed] K |
Metallicity [Fe/H] | +0.14±0.09[ citation needed] dex |
Rotational velocity (v sin i) | 8.3 [6] km/s |
Age | 4.7±2[ citation needed] Gyr |
B | |
Mass | 0.59 [1] M☉ |
Other designations | |
Database references | |
SIMBAD | data |
GSC 02620-00648 is a double star in the constellation Hercules. The brighter of the pair is a magnitude 12 star located approximately 1,660 light-years away. This star is about 1.18 times as massive as the Sun. [1]
In 2006 the TrES program discovered exoplanet TrES-4b using the transit method. [5] This planet orbits the primary star. [1]
Companion (in order from star) |
Mass |
Semimajor axis ( AU) |
Orbital period ( days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 0.919 ± 0.073 [1] MJ | 0.05091 ± 0.00071 [1] | 3.553945 ± 7.5e-05 | 0 | — | 1.799 [7] RJ |
In 2008 a study was undertaken of 14 stars with exoplanets that were originally discovered using the transit method through relatively small telescopes. These systems were re-examined with the 2.2M reflector telescope at the Calar Alto Observatory in Spain. This star system, along with two others, was determined to be a previously unknown binary star system. The previously unknown secondary star is a dim magnitude 14 K or M-type star separated by about 755 AU from the primary, appearing offset from the primary by about one arc second in the images. This discovery resulted in a recalculation of parameters for both the planet and the primary star. [1]