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  2. File:Orbits around earth scale diagram.svg - Wikipedia

    en.wikipedia.org/wiki/File:Orbits_around_earth...

    Distance above earth (km) Distance from center of earth (km) Earth Erde Terre భూమి: Blue/brown image: 0: 6370 Low Earth Orbit (LEO) Low Earth Orbit Orbite terrestre basse భూ నిమ్న కక్ష్య: Cyan area: 160 to 2,000: 6,530 to 8,370 Medium Earth Orbit (MEO) Medium Earth Orbit Orbite moyenne de la terre

  3. File:Earths orbit and ecliptic.svg - Wikipedia

    en.wikipedia.org/wiki/File:Earths_orbit_and...

    Printable version; Page information; Get shortened URL ... English: Diagram of Earth's orbit, ... Source: Own work: Author: CielProfond: Based on Earths_orbit_and ...

  4. Earth's orbit - Wikipedia

    en.wikipedia.org/wiki/Earth's_orbit

    By astronomical convention, the four seasons are determined by the solstices (the two points in the Earth's orbit of the maximum tilt of the Earth's axis, toward the Sun or away from the Sun) and the equinoxes (the two points in the Earth's orbit where the Earth's tilted axis and an imaginary line drawn from the Earth to the Sun are exactly ...

  5. File:Earths orbit and ecliptic.PNG - Wikipedia

    en.wikipedia.org/wiki/File:Earths_orbit_and...

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  6. Seasons on planets - Wikipedia

    en.wikipedia.org/wiki/Seasons_on_planets

    Given the different Sun incidence in different positions in the orbit, it is necessary to define a standard point of the orbit of the planet, to define the planet position in the orbit at each moment of the year w.r.t such point; this point is called with several names: vernal equinox, spring equinox, March equinox, all equivalent, and named considering northern hemisphere seasons.

  7. Earth's tilt explains seasons, more - AOL

    www.aol.com/news/earths-tilt-explains-seasons...

    Jun. 26—This week marks the end of June and we are heading rapidly around the sun. Because our planet has that interesting tilt to it, the northern hemisphere is collecting many hours of ...

  8. Milankovitch cycles - Wikipedia

    en.wikipedia.org/wiki/Milankovitch_cycles

    The Earth's orbit approximates an ellipse. Eccentricity measures the departure of this ellipse from circularity. The shape of the Earth's orbit varies between nearly circular (theoretically the eccentricity can hit zero) and mildly elliptical (highest eccentricity was 0.0679 in the last 250 million years). [6] Its geometric or logarithmic mean ...

  9. Earth phase - Wikipedia

    en.wikipedia.org/wiki/Earth_phase

    Earth's angular diameter (1.9°) is four times the Moon's as seen from Earth, although because the Moon's orbit is eccentric, Earth's apparent size in the sky varies by about 5% either way (ranging between 1.8° and 2.0° in diameter). Earth shows phases, just like the Moon does for terrestrial observers. The phases, however, are opposite; when ...