The Kepler-1542 system contains 4 exoplanets. It is located 1301.73 light years away from the solar system.
Mass | 0.94 solar masses |
Radius | 0.99 solar radiae |
Temperature | 5564 kelvin |
Stellar Metallicity | 0.06 decimal exponent |
Age | 8.51 billion years |
At less than 1.5 Earth masses, Kepler-1542 b is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
Mass | 0.363 Earth masses |
Density | 4.540 grams per cubic centimeter |
Radius | 0.760 Earth radiae |
Semi-major Axis | 0.0479 AU |
Eccentricity | 0 |
Orbital Period | 3.951 days |
Discovery Method | Transit |
Discovery Facility | Kepler |
Discovery Telescope | 0.95 m Kepler Telescope |
Discovery Instrument | Kepler CCD Array |
Discovery Date | 2016-05 |
Reference | Morton et al. 2016 |
At less than 1.5 Earth masses, Kepler-1542 c is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
Mass | 0.208 Earth masses |
Density | 4.160 grams per cubic centimeter |
Radius | 0.650 Earth radiae |
Semi-major Axis | 0.0389 AU |
Eccentricity | 0 |
Orbital Period | 2.892 days |
Discovery Method | Transit |
Discovery Facility | Kepler |
Discovery Telescope | 0.95 m Kepler Telescope |
Discovery Instrument | Kepler CCD Array |
Discovery Date | 2016-05 |
Reference | Morton et al. 2016 |
At less than 1.5 Earth masses, Kepler-1542 d is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
Mass | 0.590 Earth masses |
Density | 4.920 grams per cubic centimeter |
Radius | 0.870 Earth radiae |
Semi-major Axis | 0.0632 AU |
Eccentricity | 0 |
Orbital Period | 5.993 days |
Discovery Method | Transit |
Discovery Facility | Kepler |
Discovery Telescope | 0.95 m Kepler Telescope |
Discovery Instrument | Kepler CCD Array |
Discovery Date | 2016-05 |
Reference | Morton et al. 2016 |
At less than 1.5 Earth masses, Kepler-1542 e is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
Mass | 0.363 Earth masses |
Density | 4.540 grams per cubic centimeter |
Radius | 0.760 Earth radiae |
Semi-major Axis | 0.0567 AU |
Eccentricity | 0 |
Orbital Period | 5.101 days |
Discovery Method | Transit |
Discovery Facility | Kepler |
Discovery Telescope | 0.95 m Kepler Telescope |
Discovery Instrument | Kepler CCD Array |
Discovery Date | 2016-05 |
Reference | Morton et al. 2016 |