Kepler-124b
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | Kepler-124 | |
Constellation | Cygnus | |
Right ascension | (α) | 19h 07m 00s[1] |
Declination | (δ) | +49° 03′ 53″[1] |
Distance | 1,170[1] ly (359[1] pc) | |
Mass | (m) | 0.84 ± 0.03[1] M☉ |
Radius | (r) | 0.64 ± 0.03[1] R☉ |
Orbital elements | ||
Semi-major axis | (a) | 0.039[2] AU |
Orbital period | (P) | 3.4105 ± 0.0000[1] d |
Physical characteristics | ||
Radius | (r) | 0.73 ± 0.05[1] R⊕ |
Discovery information | ||
Discovery date | 2014[1] | |
Discoverer(s) | ||
Discovery method | Primary Transit[2] | |
Discovery status | Confirmed[2] | |
Database references | ||
Extrasolar Planets Encyclopaedia | data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
Kepler-124b is an extrasolar planet discovered in 2014. It is located 359 parsecs (1,170 light-years) from Earth, orbiting the unclassified star Kepler-124 in the constellation Cygnus. Within The Kepler-124 system (KOI-241) there are three known planets, Kepler-124b being both the smallest and closest to its parent star.
Characteristics
Kepler-124b is located 359 parsecs (1,170 light-years) from Earth orbiting the star Kepler-124. Both Kepler-124b and its host star are smaller than our own planet and star, respectively; Kepler-124b is estimated to be 40% smaller than Earth at 0.73±0.05 Earth radii (0.067±0.005 Jupiter radii), and its parent star Kepler-124 is estimated to be 56% smaller than the Sun at 0.64±0.03 solar radii.
It is the smallest discovered planet in the Kepler-124 system, and has the closest orbit of the three known planets. Kepler-124b orbits 96% closer to its star than Earth (approximately 3 Earth days), which in the Kepler-124 system is inside the inner limit of the star's habitable zone.
Discovery
Like many Exoplanets discovered by the Kepler telescope, Kepler-124b was found using the transit method. The transit method utilizes the high magnification and numerous instruments on the Kepler telescope to detect slight fluctuations in brightness of a star being observed. These dips can indicate the presence planet and determine certain parameters of it as well. Kepler-124b was initially only a planet candidate but was later confirmed as an exoplanet; a statistical analysis by a team at NASA Ames Research Center validated the existence of Kepler-124b with 99% assurance, along with Kepler-124c and Kepler-124d. Although scientists are very confident about some of Kepler-124b’s parameters, many are still unknown. [1][3]
Gallery
- Illustration of Kepler Telescope
- Cygnus Constellation
- example of light dip in transit method