Discovery [1] | |
---|---|
Discovered by | Kepler (K2) |
Discovery date | 2020 |
Transit | |
Orbital characteristics [1] | |
0.02±0.00 AU | |
3.14±0.00 d | |
Inclination | 88.7° ±0.2° |
Physical characteristics | |
Mean radius | 0.95±0.06 R🜨 [1] |
Mass | 0.81 M🜨 [2] |
Temperature | 460 ± 5 K (368.33 ± 9.00 °F; 186.85 ± 5.00 °C) [1] |
K2-315b is an exoplanet located 185.3 light years away from Earth in the southern zodiac constellation Libra. [3] [4] It orbits the red dwarf K2-315.
K2-315b was discovered in 2020 by astronomers in an observatory using the Kepler space telescope. [1] It is also nicknamed the "Pi Earth" because it takes approximately 3.14 days to orbit the host star. [5]
The planet is thought to be a small rocky planet, even though composition is unknown. [5] Since it orbits very close to its star, it is too hot to host life, due to it having a scorching temperature of 450 K. Not much is known about it because it was just discovered, but it is similar to Earth, having a radius 95% that of Earth, [6] very similar to Venus, but has 81% Earth's mass. [2]
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
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Constellation | Libra [7] |
Right ascension | 15h 12m 05.1944s [8] |
Declination | −20° 06′ 30.5428″ [8] |
Apparent magnitude (V) | 17.67 [9] |
Characteristics | |
Evolutionary stage | Red dwarf |
Spectral type | M3.5±0.5 V [10] |
Astrometry | |
Radial velocity (Rv) | 6.25±0.17 [10] km/s |
Proper motion (μ) | RA: −120.013 mas/yr [8] Dec.: +74.471 mas/yr [8] |
Parallax (π) | 17.6353 ± 0.0492 mas [8] |
Distance | 184.9 ± 0.5 ly (56.7 ± 0.2 pc) |
Details [10] | |
Mass | 0.174±0.004 M☉ |
Radius | 0.2±0.01 R☉ |
Luminosity | 0.398% L☉ |
Surface gravity (log g) | 5.094±0.006 cgs |
Temperature | 3,300±30 K |
Metallicity [Fe/H] | −0.24±0.09 dex |
Rotational velocity (v sin i) | <5 km/s |
Age | >1 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
K2-315 is a star in the southern zodiac constellation Libra. [11] It has an apparent magnitude of 17.67, [9] requiring a powerful telescope to be seen. The star is relatively close at a distance of 185 light years [8] but is receding with a radial velocity of 6.25 km/s . [10]
K2-315 has a stellar classification of M3.5±0.5 V, indicating that it is a M-type main-sequence star (with 14% uncertainty). [10] It has 17.4% the mass of the Sun and 20% its radius. [10] Typical for red dwarves, it has a luminosity less than 1% of the Sun, which yields an effective temperature of 3,300 K. [10] Unlike most planetary hosts, K2-315 is metal-deficient, with an iron abundance only 57% that of the Sun. [10] It is estimated to be over a billion years old, and has a projected rotational velocity less than 5 km/s . [10]
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HD 97658 is a star with an exoplanetary companion in the equatorial constellation of Leo. The star is too dim to be seen with the naked eye, having an apparent visual magnitude of 7.76. It is located at a distance of 70 light years based on parallax, but is slowly drifting closer with a radial velocity of −1.6 km/s.
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K2-19 is an early K-type or late G-type main sequence star that is magnetically active, and has a light curve that exhibits variations in brightness of ~1%. It is located approximately 976 light-years away in the constellation Virgo. Three confirmed transiting exoplanets are known to orbit this star.
K2-28 is a metal rich M4-type main sequence star. One confirmed transiting exoplanet is known to orbit this star. There is another star 5.2 arcseconds to the north–east of K2-28 however this star has a different proper motion and is therefore physically unrelated and probably a background star.
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HAT-P-41 is a binary star system. Its primary is a F-type main-sequence star. Its surface temperature is 6390±100 K. compared to the Sun, HAT-P-41 is enriched in heavy elements, with a metallicity Fe/H index of 0.21±0.10, but is much younger at an age of 2.2±0.4 billion years.
Kepler-1638 is a G-type main-sequence star located about 5,000 light years away in the constellation of Cygnus. One known exoplanet has been found orbiting the star: Kepler-1638b.As of January 2021, Kepler-1638 is the farthest star with a known exoplanet orbiting in the habitable zone.
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LHS 3844 is a red dwarf star located 48.5 light-years away from the Solar System in the constellation of Indus. The star has about 15% the mass and 19% the radius of the Sun. It is a relatively inactive red dwarf with a slow rotation period of about 128 days, though UV flares have been observed. LHS 3844 is orbited by one known exoplanet.
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