Kepler-444

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Kepler-444

Observation data
Epoch J2000      Equinox 2000
Constellation Lyra
Right ascension 19:19:01.0
Declination +41:38:05
Apparent magnitude (V) 9.0
Characteristics
Spectral type K0V C ~
Apparent magnitude (U) 10.01 ~
Apparent magnitude (B) 9.67 ~
Apparent magnitude (V) 8.86 ~
Apparent magnitude (R) 8.18 ~
Apparent magnitude (I) 7.66 ~
Apparent magnitude (J) 7.244±0.026
Apparent magnitude (H) 6.772±0.047
Apparent magnitude (K) 6.703±0.020
Astrometry
Radial velocity (Rv) −121.19±0.11 km/s
Proper motion (μ) RA: 98.94 mas/yr
Dec.: -632.49 mas/yr
Parallax (π) 28.03±0.82 mas
Distance 117 ly
(36 pc)
Details
Mass 0.758 (± 0.043) M☉
Radius 0.752 (± 0.014) R☉
Temperature 5040 (± 74.0) K
Metallicity [Fe/H] -0.55 (± 0.07) dex
Age 11.23 (± 0.99) Gyr
Other designations
KOI-3158; 2MASS J19190052+4138043; TYC 3129-00329-1; KIC 6278762; LHS 3450; HIP 94931; BD+41 3306
Database references
SIMBAD data

Kepler-444 (or KOI-3158, KIC 6278762, 2MASS J19190052+4138043, BD+41 3306)[1][2][3][4][5][6] is a star, estimated to be 11.2 billion years old (more than 80% of the age of the universe),[4] approximately 117 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 star.[1][2][3][5] According to NASA, no life as we know it could exist on these hot exoplanets, due to their close orbital distances to the host star.[1]

Discovery

Preliminary results of the planetary system around Kepler-444 were first announced at the second Kepler science conference in 2013. At that conference, the star was known as KOI-3158.[7]

Characteristics

The star, Kepler-444, is approximately 11.2 billion years old, whereas the Sun is only 4.6 billion years old. The age of Kepler-444, an orange main sequence star of spectral type K0,[6] is more than 80% of the age of the universe.[4]

The original research on Kepler-444 was published in The Astrophysical Journal on 27 January 2015 under the title "An ancient extrasolar system with five sub-Earth-size planets"[8] by a team of 40 authors, the abstract reads as follows:

"The chemical composition of stars hosting small exoplanets (with radii less than four Earth radii) appears to be more diverse than that of gas-giant hosts, which tend to be metal-rich. This implies that small, including Earth-size, planets may have readily formed at earlier epochs in the Universe's history when metals were more scarce. We report Kepler spacecraft observations of Kepler-444, a metal-poor Sun-like star from the old population of the Galactic thick disk and the host to a compact system of five transiting planets with sizes between those of Mercury and Venus. We validate this system as a true five-planet system orbiting the target star and provide a detailed characterization of its planetary and orbital parameters based on an analysis of the transit photometry. Kepler-444 is the densest star with detected solar-like oscillations. We use asteroseismology to directly measure a precise age of 11.2+/-1.0 Gyr for the host star, indicating that Kepler-444 formed when the Universe was less than 20% of its current age and making it the oldest known system of terrestrial-size planets. We thus show that Earth-size planets have formed throughout most of the Universe's 13.8-billion-year history, leaving open the possibility for the existence of ancient life in the Galaxy. The age of Kepler-444 not only suggests that thick-disk stars were among the hosts to the first Galactic planets, but may also help to pinpoint the beginning of the era of planet formation."[8] The star is believed to have 2 M dwarfs in orbit around it with the fainter companion 1.8 arc-seconds from the main star.[9]

Planetary system

The Kepler-444 planetary system[5]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
b — 0.04178 3.60001053 0.16 88° 0.4 R⊕
c — 0.04881 4.5458841 0.31 88.2° 0.497 R⊕
d — 0.06 6.189392 0.18 88.16° 0.53 R⊕
e — 0.0696 7.743493 0.1 89.13° 0.546 R⊕
f — 0.0811 9.740486 0.29 87.96° 0.741 R⊕

All five rocky exoplanets (Kepler-444b; Kepler-444c; Kepler-444d; Kepler-444e; Kepler-444f) are confirmed,[5] smaller than the size of Venus (but bigger than Mercury) and each of the exoplanets completes an orbit around the host star in less than 10 days.[1][4] The system is also very compact and Kepler-444b is the smallest at 0.403 earth diameters, and even the furthest planet, Kepler-444f, still orbits closer to the star than Mercury is to the Sun.[6] According to NASA, no life as we know it could exist on these hot exoplanets, due to their close orbital distances to the host star.[1]

See also

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 Lua error in package.lua at line 80: module 'strict' not found.
  2. ↑ 2.0 2.1 Lua error in package.lua at line 80: module 'strict' not found.
  3. ↑ 3.0 3.1 Lua error in package.lua at line 80: module 'strict' not found.
  4. ↑ 4.0 4.1 4.2 4.3 Lua error in package.lua at line 80: module 'strict' not found.
  5. ↑ 5.0 5.1 5.2 5.3 Lua error in package.lua at line 80: module 'strict' not found.
  6. ↑ 6.0 6.1 6.2 Lua error in package.lua at line 80: module 'strict' not found.
  7. ↑ Lua error in package.lua at line 80: module 'strict' not found.
  8. ↑ 8.0 8.1 Lua error in package.lua at line 80: module 'strict' not found.
  9. ↑ Lua error in package.lua at line 80: module 'strict' not found.

External links

Coordinates: Sky map 19h 19m 01.0s, +41° 38′ 05″

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