Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Phoenix[1] |
HD 142 A | |
Right ascension | 00h 06m 19.1754s[2] |
Declination | –49° 04′ 30.6741″[2] |
Apparent magnitude (V) | 5.711±0.003[3] |
HD 142 B | |
Right ascension | 00h 06m 19.1480s[4] |
Declination | –49° 04′ 34.9177″[4] |
Apparent magnitude (V) | +11.5[5] |
Characteristics | |
Evolutionary stage | main sequence |
Spectral type | F7V[6] + K8.5-M1.5[7] |
B−V color index | 0.519±0.011[8] |
Astrometry | |
HD 142 A | |
Radial velocity (Rv) | 5.76±0.12[9] km/s |
Proper motion (μ) | RA: 575.099±0.017[9] mas/yr Dec.: −40.874±0.024[9] mas/yr |
Parallax (π) | 38.1945 ± 0.0355 mas[9] |
Distance | 85.39 ± 0.08 ly (26.18 ± 0.02 pc) |
Absolute magnitude (MV) | 3.66±0.02[10] |
HD 142 B | |
Proper motion (μ) | RA: 566.984±0.023[11] mas/yr Dec.: −17.387±0.027[11] mas/yr |
Parallax (π) | 38.2306 ± 0.0349 mas[11] |
Distance | 85.31 ± 0.08 ly (26.16 ± 0.02 pc) |
Details[12] | |
HD 142 A | |
Mass | 1.25±0.10 M☉ |
Radius | 1.41±0.11 R☉ |
Luminosity | 2.9 L☉ |
Surface gravity (log g) | 4.34±0.14 cgs |
Temperature | 6,338±46 K |
Metallicity [Fe/H] | 0.03±0.04 dex |
Rotational velocity (v sin i) | 9.58±0.74[13] km/s |
Age | 2.5 Gyr |
HD 142 B | |
Mass | 0.54[14] M☉ |
Other designations | |
HD 142A: CD−49°14337, HD 142, HIP 522, HR 6, SAO 214963, WDS J00063-4905A[15] | |
HD 142B: CD−49°14337B, WDS J00063-4905B, NLTT 218, 2MASS J00061919-4904348[16] | |
Database references | |
SIMBAD | data |
HD 142 is a wide binary star[5] system in the southern constellation of Phoenix. The main component has a yellow-white hue and is dimly visible to the naked eye with an apparent visual magnitude of 5.7.[3] The system is located at a distance of 85.5 light years from the Sun based on parallax measurements, and is drifting further away with a radial velocity of +6 km/s.[17]
The primary component is an F-type main-sequence star with a stellar classification of F7V,[6] which indicates it is undergoing core hydrogen fusion. It is an estimated 2.5[12] billion years old and is spinning with a projected rotational velocity of 10 km/s.[13] The star has 1.25 times the mass of the Sun and 1.4 times the Sun's radius. It is radiating 2.9 times the luminosity of the Sun from its photosphere at an effective temperature of 6,338 K.[12]
A magnitude 11.5[5] companion star was detected in 1894 making this a binary star system.[18] The binary companion was confirmed to be gravitationally bound in 2007 and determined to be a red dwarf of spectral type K8.5-M1.5[7] with 54% of the Sun's mass.[14] The pair have a projected separation of 120.6 AU.[14]
Roman1987
was invoked but never defined (see the help page).Gaia DR2 A
was invoked but never defined (see the help page).Olsen1994
was invoked but never defined (see the help page).Gaia DR2 B
was invoked but never defined (see the help page).Eggleton2008
was invoked but never defined (see the help page).Gray2006
was invoked but never defined (see the help page).Eggenberger2007
was invoked but never defined (see the help page).Anderson2012
was invoked but never defined (see the help page).Holmberg
was invoked but never defined (see the help page).apj720_2_1290
was invoked but never defined (see the help page).Soto2018
was invoked but never defined (see the help page).Tokovinin2016
was invoked but never defined (see the help page).Simbad for A
was invoked but never defined (see the help page).Simbad for B
was invoked but never defined (see the help page).Valenti2005
was invoked but never defined (see the help page).Raghavan2006
was invoked but never defined (see the help page).