K2-3d
Exoplanet | List of exoplanets
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Parent star | ||||||
Star | K2-3 | |||||
Right ascension | (α) | 11h29m20.39s [1] | ||||
Declination | (δ) | -01d27m17.2s[1] | ||||
Distance | 137±6.5 ly (42±2[1] pc) | |||||
Mass | (m) | 0.612±0.086[1] M☉ | ||||
Radius | (r) | 0.553±0.041[1] R☉ | ||||
Temperature | (T) | null[1] K | ||||
Metallicity | [Fe/H] | null[1] | ||||
Age | null[1] Gyr | |||||
Physical characteristics | ||||||
Mass | (m) | 11.1±3.5[1] M⊕ | ||||
Radius | (r) | 1.53±0.11[1] R⊕ | ||||
Density | (ρ) | 17.5±6.3[1] g cm−3 | ||||
Orbital elements | ||||||
Semi-major axis | (a) | 0.2086±0.0100[1] AU | ||||
Eccentricity | (e) | 0.045±0.045[1] | ||||
Orbital period | (P) | 44.5705±0.0059[1] d | ||||
Inclination | (i) | 89.79±0.15[1]° | ||||
Discovery information | ||||||
Discovery date | 2015 | |||||
Discoverer(s) | Owen Deffner | |||||
Discovery method | Transit | |||||
Discovery site | Kepler Space Observatory | |||||
Discovery status | Confirmed |
K2-3d also known as EPIC 201367065 d is a massive solid exoplanet orbiting K2-3 a Red dwarf, every 44.5 days 137 ly away.[1][2][1]
Composition
K2-3d has a density of 17.5±6.3g/cm3, far greater that of Iron. Although its density is greater than Iron estimates show that K2-3d would need to have a mass of 14.1 Me to be made purely of Iron, this indicates that the planet probably has some silica "rock" or some water resembling that of a terrestrial planet.[3][1]
Type | Mass (Me) |
---|---|
Iron | 14.1 |
Rocky (Earth Like) | 3.7 |
Water | 1.5 |
K2-3d | 11.1 |
References
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