Kepler-452b
| Exoplanet | List of exoplanets | |
|---|---|---|
 |
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| Parent star | ||
| Star | Kepler-452 | |
| Constellation | Cygnus | |
| Right ascension | (α) | 19h 44m 00.89s |
| Declination | (δ) | +44° 16′ 39.2″ |
| Apparent magnitude | (mV) | 13.426 |
| Distance | 1400 ly (430 pc) |
|
| Spectral type | G2V | |
| Mass | (m) | 1.037+0.054 −0.047 M☉ |
| Radius | (r) | 1.11+0.15 −0.09 R☉ |
| Temperature | (T) | 5757 (± 85) K |
| Metallicity | [Fe/H] | 0.21 (± 0.09) |
| Age | 6 (± 2) Gyr | |
| Physical characteristics | ||
| Mass | (m) | 5 (± 2)M⊕ |
| Radius | (r) | 1.5+0.32 −0.22R⊕ |
| Stellar flux | (F⊙) | 1.11⊕ |
| Surface gravity | (g) | 1.9+1.5 −1.0 (est.) g |
| Temperature | (T) | 265 K (−8 °C; 17 °F) K |
| Orbital elements | ||
| Semi-major axis | (a) | 1.046+0.019 −0.015AU |
| Orbital period | (P) | 384.843+0.007 −0.012d |
| Inclination | (i) | 89.806+0.134 −0.049° |
| Discovery information | ||
| Discovery date | 23 July 2015 (announced) | |
| Discoverer(s) | Kepler Science Team | |
| Discovery method | Transit | |
| Discovery site | Kepler | |
| Discovery status | Published | |
| Other designations | ||
|
KOI-7016.01
|
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| Database references | ||
| Extrasolar Planets Encyclopaedia |
data | |
| SIMBAD | data | |
| Exoplanet Archive | data | |
| Open Exoplanet Catalogue | data | |
Kepler-452b (sometimes nicknamed Earth 2.0 or Earth's Cousin based on its characteristics; known sometimes as Coruscant by NASA, also known by its Kepler Object of Interest designation KOI-7016.01) is an exoplanet orbiting the Sun-like star Kepler-452 about 1,400 light-years (430 pc) from Earth in the constellation Cygnus. It was identified by the Kepler space telescope, and its discovery was announced by NASA on 23 July 2015. It is the first potentially rocky super-Earth planet discovered orbiting within the habitable zone of a star very similar to the Sun.
The planet is about 1,400 light-years away from the Solar System. At the speed of the New Horizons spacecraft, about 59,000 km/h (37,000 mph), it would take approximately 26 million years to get there.
Kepler-452b has a probable mass five times that of Earth, and its surface gravity is twice Earth's, though calculations of mass for exoplanets are only rough estimates. If it is a terrestrial planet, it is most likely a super-Earth with many active volcanoes due to its higher mass and density. The clouds on the planet would be thick and misty, covering much of the surface as viewed from space.
The planet takes 385 Earth days to orbit its star. Its radius is 50% bigger than Earth's, and lies within the conservative habitable zone of its parent star. It has an equilibrium temperature of 265 K (−8 °C; 17 °F), a little warmer than Earth.
The host star, Kepler-452, is a G-type star that is about the same mass of the Sun, only 3.7% more massive and 11% larger. It has a surface temperature of 5757 K, nearly the same as the Sun, which has a surface temperature of 5778 K. The star's age is estimated to be about 6 billion years old, about 1.4 billion years older than the Sun, which is 4.6 billion years old. From the surface of Kepler-452b, its star would look almost identical to the Sun as viewed from the Earth.
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