Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Virgo |
Right ascension | 13h 12m 43.78556s[1] |
Declination | –02° 15′ 54.1307″[1] |
Apparent magnitude (V) | 7.56[2] |
Characteristics | |
Spectral type | K1V[3] |
B−V color index | 0.930±0.013[2] |
Variable type | Constant[4] |
Astrometry | |
Radial velocity (Rv) | −12.07±0.12[1] km/s |
Proper motion (μ) | RA: −138.362(34) mas/yr[1] Dec.: 10.284(22) mas/yr[1] |
Parallax (π) | 47.5529 ± 0.0291 mas[1] |
Distance | 68.59 ± 0.04 ly (21.03 ± 0.01 pc) |
Absolute magnitude (MV) | 6.00[2] |
Details[5] | |
Mass | 0.883+0.018 −0.028 M☉ |
Radius | 0.810+0.011 −0.009 R☉ |
Luminosity | 0.423±0.001[6] L☉ |
Surface gravity (log g) | 4.42±0.58 cgs |
Temperature | 5,114±12 K |
Metallicity [Fe/H] | 0.08±0.11 dex |
Rotational velocity (v sin i) | 1.9±0.5 km/s |
Age | 2.5+3.0 −1.6 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
ARICNS | data |
HD 114783 is a star with two exoplanetary companions in the equatorial constellation of Virgo. With an apparent visual magnitude of 7.56[2] it is too faint to be visible with the unaided eye, but is an easy target for binoculars. Based on parallax measurements, it is located at a distance of 68.6 light-years (21.0 parsecs) from the Sun, but is drifting closer with a radial velocity of −12 km/s.[1]
This is an orange-hued K-type main-sequence star with a stellar classification of K1V.[3] It is roughly 2.5[5] billion years old and is chromospherically inactive[4] with a low projected rotational velocity of 1.9 km/s.[5] The star has 88% of the mass and 81% of the radius of the Sun.[5] It is radiating 42%[6] of the luminosity of the Sun from its photosphere at an effective temperature of 5,114 K.[5]
In 2001, the California and Carnegie Planet Search team found an exoplanet, HD 114783 b, orbiting the star using the radial velocity method. The discovery was made with the Keck Telescope.[4] A second companion, HD 114783 c, was discovered in 2016,[7] and in 2023 its inclination and true mass were measured via astrometry.[8]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | ≥ 1.034±0.089 MJ | 1.169±0.068 | 496.9±2.3 | 0.085±0.033 | — | — |
c | 1.9+0.5 −0.4 MJ |
5.0±0.1 | 4,352+88 −76 |
0.05+0.04 −0.03 |
21+7 −4 or 159+4 −6° |
— |
GaiaDR3
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was invoked but never defined (see the help page).Houk1999
was invoked but never defined (see the help page).Vogt2002
was invoked but never defined (see the help page).Soto_Jenkins2018
was invoked but never defined (see the help page).GaiaDR2
was invoked but never defined (see the help page).Bryan_et_al_2016
was invoked but never defined (see the help page).Philipot2023
was invoked but never defined (see the help page).Butler2006
was invoked but never defined (see the help page).