Observation data Epoch J2000 Equinox 2000 | |
---|---|
Constellation | Lyra[2] |
Kepler-444 A | |
Right ascension | 19h 19m 00.5489s[3] |
Declination | +41° 38′ 04.582″[3] |
Apparent magnitude (V) | 8.86[4] |
Kepler-444 B/C | |
Right ascension | 19h 19m 00.3922s[5] |
Declination | +41° 38′ 04.013″[5] |
Characteristics | |
Spectral type | K0V[6] |
Astrometry | |
Kepler-444 A | |
Radial velocity (Rv) | −123.05±0.17[7] km/s |
Proper motion (μ) | RA: 94.639(13) mas/yr[3] Dec.: −632.269(14) mas/yr[3] |
Parallax (π) | 27.3578 ± 0.0125 mas[3] |
Distance | 119.22 ± 0.05 ly (36.55 ± 0.02 pc) |
Kepler-444 B/C | |
Proper motion (μ) | RA: 94.508(55) mas/yr[5] Dec.: −630.781(78) mas/yr[5] |
Parallax (π) | 27.6079 ± 0.0545 mas[5] |
Distance | 118.1 ± 0.2 ly (36.22 ± 0.07 pc) |
Orbit[1] | |
Primary | A |
Companion | BC |
Period (P) | 324+31 −25 yr |
Semi-major axis (a) | 52.2+3.3 −2.7 AU |
Eccentricity (e) | 0.55+0.05 −0.05 |
Inclination (i) | 85.4+0.3 −0.4° |
Longitude of the node (Ω) | 250.7+0.2 −0.2° |
Periastron epoch (T) | JD 2537060+10881 −8533 |
Argument of periastron (ω) (secondary) | 227.3+6.5 −5.2° |
Details | |
A | |
Mass | 0.754±0.030[8] M☉ |
Radius | 0.753±0.010[8] R☉ |
Surface gravity (log g) | 4.595±0.060[2] cgs |
Temperature | 5046±74.0[2] K |
Metallicity [Fe/H] | −0.55±0.07[2] dex |
Rotation | 49.40±6.04 d[9] |
Age | 11.00±0.8[8] Gyr |
B | |
Mass | 0.307+0.009 −0.008[1] M☉ |
Surface gravity (log g) | 5.0±0.2[2] cgs |
Temperature | 3,464±200[2] K |
C | |
Mass | 0.296±0.008[1] M☉ |
Surface gravity (log g) | ~5[2] cgs |
Temperature | 3,500 - 4,000[2] K |
Other designations | |
Kepler-444A: Gaia DR2 2101486923385239808, HIP 94931, LHS 3450, TYC 3129-00329-1, 2MASS J19190052+4138043[10] | |
Kepler-444BC: Gaia DR2 2101486923382009472[11] | |
Database references | |
SIMBAD | data |
B/C |
Kepler-444 (or KOI-3158, KIC 6278762, 2MASS J19190052+4138043, BD+41°3306)[10] is a triple star system, estimated to be 11.2 billion years old (more than 80% of the age of the universe),[12] approximately 119 light-years (36 pc) away from Earth in the constellation Lyra. On 27 January 2015, the Kepler spacecraft is reported to have confirmed the detection of five sub-Earth-sized rocky exoplanets orbiting the main star. The star is a K-type main sequence star.[13][14][15][12][16] All of the planets are far too close to their star to harbour life forms.[13]
Zhang2023
was invoked but never defined (see the help page).Campante2015
was invoked but never defined (see the help page).Gaia DR3 for A
was invoked but never defined (see the help page).ducati2002
was invoked but never defined (see the help page).Gaia DR3 for B/C
was invoked but never defined (see the help page).wilson1962
was invoked but never defined (see the help page).Dupuy2016
was invoked but never defined (see the help page).Buldgen2019
was invoked but never defined (see the help page).Mazeh2015
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).SP-20150127
was invoked but never defined (see the help page).NASA-20150128
was invoked but never defined (see the help page).AP-20150127
was invoked but never defined (see the help page).UT-20150127
was invoked but never defined (see the help page).EX-20150127
was invoked but never defined (see the help page).