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An elliptic Kepler orbit with an eccentricity of 0.7, a parabolic Kepler orbit and a hyperbolic Kepler orbit with an eccentricity of 1.3. The distance to the focal point is a function of the polar angle relative to the horizontal line as given by the equation ( 13 )
From the original Blue Marble photo shot back in 1972 to the new high-definition Blue Marble images to a screen shot of the very first video image of Earth taken by a weather satellite in 1960 ...
Date/Time Thumbnail Dimensions User Comment; current: 22:22, 5 January 2011: 494 × 600 (12 KB): Stamcose~commonswiki {{Information |Description={{en|1=A hyperbolic Kepler orbit with the eccentricity 1.3, a parabolic Kepler orbit and an elliptic Kepler orbit with the eccentricity 0.7}} |Source=Own work |Author=Stamcose |Date=2011-01-05 |Permission= |oth
Kepler-283 c is an exoplanet orbiting the K-type star Kepler-283 every 93 days in the circumstellar habitable zone, discovered by the Kepler space telescope in 2014. [ 4 ] Characteristics
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Kepler's first law placing the Sun at one of the foci of an elliptical orbit Heliocentric coordinate system (r, θ) for ellipse. Also shown are: semi-major axis a , semi-minor axis b and semi-latus rectum p ; center of ellipse and its two foci marked by large dots.
The second-outermost (shown in grey) is a geostationary orbit, 35,786 kilometres (22,236 miles) above Earth's equator and following the direction of Earth's rotation, with an orbital period matching the planet's rotation period (a geosynchronous orbit). An object in such an orbit will appear to occupy a fixed position in the sky.
K2-72e (also known by its EPIC designation EPIC 206209135.04), is a confirmed exoplanet, likely rocky, orbiting within the habitable zone of the red dwarf star K2-72, the outermost of four such planets discovered in the system by NASA's Kepler spacecraft on its "Second Light" mission.