Kepler-68c
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | Kepler-68 (KOI-246) | |
Right ascension | (α) | 19h 24m 07.76s |
Declination | (δ) | +49° 02′ 25″ |
Apparent magnitude | (mV) | 8.588 |
Distance | 440 ly (135 pc) | |
Mass | (m) | 1.079±0.051 M☉ |
Radius | (r) | 1.243±0.019 R☉ |
Temperature | (T) | 5793±74 K |
Metallicity | [Fe/H] | 0.12±0.074 |
Age | 6.3 ± 1.7 Gyr | |
Physical characteristics | ||
Maximum mass | (m sin i) | 7.3 M⊕ |
Radius | (r) | 0.953 R⊕ |
Density | (ρ) | 5–40 g cm−3 |
Temperature | (T) | 944 |
Orbital elements | ||
Semi-major axis | (a) | 0.09059 AU |
Orbital period | (P) | 9.605085 d |
Inclination | (i) | 86.93 ± 0.41° |
Discovery information | ||
Discovery date | 12 February 2013 | |
Discoverer(s) | ||
Discovery method | Transit (Kepler Mission) | |
Discovery status | Confirmed | |
Other designations | ||
KOI 246.02
|
Kepler-68c is an Earth-sized planet orbiting the star Kepler-68 in the constellation of Cygnus. It was discovered by planetary-transit methods by the Kepler space telescope in February 2013. It has a mass of 4.8+2.5
−3.6 times that of Earth (0.015 MJ)[1] and a radius of 0.953+0.037
−0.042 Earth radii. It has an orbital period of 9.605085 days at a distance of about 0.09059 AU from its star. Relatively wide constraints on Kepler-68c's mass are the result lack of detection of the planet through radial-velocity and transit-timing-variation methods.[2]
See also
References
- ↑ Gilliland, Ronald L. "Kepler-68: Three Planets, One With a Density Between That of Earth and Ice Giants". arXiv:1302.2596.
- ↑ Nasa. "Kepler Discoveries". Nasa.gov. Retrieved 28 February 2013.
This article is issued from Wikipedia - version of the 7/12/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.