Astronomy:HD 114783
Observation data Equinox J2000.0]] (ICRS) | |
---|---|
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)[1] mas/yr Dec.: 10.284(22)[1] mas/yr |
Parallax (π) | 47.5529 ± 0.0291[1] mas |
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 |
Extrasolar Planets Encyclopaedia | 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° |
— |
See also
- HD 114386
- List of extrasolar planets
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940 Gaia DR3 record for this source at VizieR.
- ↑ 2.0 2.1 2.2 2.3 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A.
- ↑ 3.0 3.1 Houk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars". Michigan Spectral Survey 5. Bibcode: 1999MSS...C05....0H.
- ↑ 4.0 4.1 4.2 Vogt, Steven S. et al. (2002). "Ten Low-Mass Companions from the Keck Precision Velocity Survey". The Astrophysical Journal 568 (1): 352–362. doi:10.1086/338768. Bibcode: 2002ApJ...568..352V.
- ↑ 5.0 5.1 5.2 5.3 5.4 Soto, M. G.; Jenkins, J. S. (2018). "Spectroscopic Parameters and atmosphEric ChemIstriEs of Stars (SPECIES). I. Code description and dwarf stars catalogue". Astronomy and Astrophysics 615: A76. doi:10.1051/0004-6361/201731533. Bibcode: 2018A&A...615A..76S.
- ↑ 6.0 6.1 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
- ↑ Bryan, Marta L. et al. (2016). "Statistics of Long Period Gas Giant Planets in Known Planetary Systems". The Astrophysical Journal 821 (2): 89. doi:10.3847/0004-637X/821/2/89. Bibcode: 2016ApJ...821...89B.
- ↑ 8.0 8.1 Philipot, F. et al. (August 2023). "Multi techniques approach to identify and/or constrain radial velocity sub-stellar companions". Astronomy & Astrophysics. doi:10.1051/0004-6361/202346612.
- ↑ Butler, R. P. et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal 646 (1): 505–522. doi:10.1086/504701. Bibcode: 2006ApJ...646..505B.
Coordinates: 13h 12m 43.7860s, −02° 15′ 54.143″
Original source: https://en.wikipedia.org/wiki/HD 114783.
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