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'''Kepler-444''' is a star about {{convert|117|ly|pc|abbr=on}} away from Earth in the ] ], estimated to be 11.8 billion years old. On 27 January 2015, the ] is reported to have confirmed the detection of five sub-Earth-sized rocky ] orbiting the star.<ref name="AP-20150127" /><ref name="UT-20150127" /><ref name="EX-20150127" /> '''Kepler-444''' is a star about {{convert|117|ly|pc|abbr=on}} away from Earth in the ] ], estimated to be 11.8 billion years old. On 27 January 2015, the ] is reported to have confirmed the detection of five sub-Earth-sized rocky ] orbiting the star.<ref name="AP-20150127" /><ref name="UT-20150127" /><ref name="EX-20150127" />

==Discovery==

Preliminary results of the planetary system around Kepler-444 were first announced second Kepler science conference in 2013. At that the star was known as KOI-3158. <ref>http://nexsci.caltech.edu/conferences/KeplerII/agenda.shtml</ref>


== Characteristics == == Characteristics ==

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Kepler-444

Observation data
Epoch       Equinox
Constellation Lyra
Right ascension 19:19:01.0
Declination +41:38:05
Apparent magnitude (V) 9.0
Characteristics
Spectral type K0
Astrometry
Distance117 ly
(36 pc)
Details
Mass0.758(± 0.043) M
Radius0.752(± 0.014) R
Temperature5040(± 74.0) K
Metallicity -0.55 (± 0.07) dex
Age11.23 (± 0.99) Gyr
Other designations
KOI-3158, KIC 6278762
Database references

Kepler-444 is a star about 117 ly (36 pc) away from Earth in the constellation Lyra, estimated to be 11.8 billion years old. On 27 January 2015, the Kepler spacecraft is reported to have confirmed the detection of five sub-Earth-sized rocky exoplanets orbiting the star.

Discovery

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

Characteristics

The star is approximately 11.8 billion years old, whereas the sun is only 4.6 billion years old. The star is 80% of the age of the universe. It is an orange main sequence star of spectral type K0.

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" 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."

Planetary system

The Kepler-444 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
Kepler-444b 0.04178 3.60001053 0.16 88° 0.4 R🜨
Kepler-444c 0.04881 4.5458841 0.31 88.2° 0.497 R🜨
Kepler-444d 0.06 6.189392 0.18 88.16° 0.53 R🜨
Kepler-444e 0.0696 7.743493 0.1 89.13° 0.546 R🜨
Kepler-444f 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, smaller than the size of Venus and each of the exoplanets completes an orbit around the host star in less than 10 days. 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.

See also

References

  1. ^ Dunn, Marcia (27 January 2015). "Astronomers find solar system more than double ours in age". AP News. Retrieved 27 January 2015.
  2. ^ Atkinson, Nancy (27 January 2015). "Oldest Planetary System Discovered, Improving the Chances for Intelligent Life Everywhere". Universe Today. Retrieved 27 January 2015.
  3. ^ Wall, Mike (27 January 2015). "Found! 5 Ancient Alien Planets Nearly As Old As the Universe". Space.com. Retrieved 27 January 2015.
  4. ^ Staff (27 January 2015). "Exoplanet Catalog". Extrasolar Planets Encyclopaedia. Retrieved 27 January 2015.
  5. ^ Phil, Plait (28 January 2015). "Astronomers Find Ancient Earth-Sized Planets in Our Galactic Backyard". Slate. Retrieved 28 January 2015.
  6. http://nexsci.caltech.edu/conferences/KeplerII/agenda.shtml
  7. ^ Campante, T.L.; et al. (26 January 2015). "An ancient extrasolar system with five sub-Earth-size planets". Arxiv. doi:10.1088/0004-637X/799/2/170. Retrieved 27 January 2015. {{cite journal}}: Explicit use of et al. in: |author= (help)

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