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  2. Season - Wikipedia

    en.wikipedia.org/wiki/Season

    The seasons are not the result of the variation in Earth's distance to the Sun because of its elliptical orbit. [10] In fact, Earth reaches perihelion (the point in its orbit closest to the Sun) in January, and it reaches aphelion (the point farthest from the Sun) in July, so the slight contribution of orbital eccentricity opposes the ...

  3. Five themes of geography - Wikipedia

    en.wikipedia.org/wiki/Five_themes_of_geography

    Map projections are used to represent the three-dimensional Earth on a two-dimensional map. The Earth's position relative to the Sun affects climate, seasons, and time zones. [1] Location as a theme helps teachers to demonstrate to students that observers have to know and be able to explain where something is before it can be examined ...

  4. Seasons on planets - Wikipedia

    en.wikipedia.org/wiki/Seasons_on_planets

    Orbit eccentricity causes the planet/Sun distance to change during the year: The higher is the eccentricity, the higher is the change; Sun rays intensity in various moments of the year changes as the planet/Sun distance changes. Earth eccentricity is very low (0.0167 in a scale from 0 to 1.0000), hence it does not affect so much temperature ...

  5. 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 ...

  6. 10 Fascinating Facts About the Summer Solstice

    www.aol.com/news/10-fascinating-facts-summer...

    Earth has seasons because it’s tilted, so light from the sun changes throughout the year differently for different parts of the world. The 2024 summer solstice is the earliest since 1796.

  7. Milankovitch cycles - Wikipedia

    en.wikipedia.org/wiki/Milankovitch_cycles

    The seasons are quadrants of the Earth's orbit, marked by the two solstices and the two equinoxes. Kepler's second law states that a body in orbit traces equal areas over equal times; its orbital velocity is highest around perihelion and lowest around aphelion. [13] The Earth spends less time near perihelion and more time near aphelion.

  8. On the Sizes and Distances (Aristarchus) - Wikipedia

    en.wikipedia.org/wiki/On_the_Sizes_and_Distances...

    Distance from the Earth to the Moon: S: Distance from the Earth to the Sun: ℓ: Radius of the Moon: s: Radius of the Sun: t: Radius of the Earth: D: Distance from the center of Earth to the vertex of Earth's shadow cone d: Radius of the Earth's shadow at the location of the Moon n: Ratio, d/ℓ (a directly observable quantity during a lunar ...

  9. Trump picks Brooke Rollins to be agriculture secretary

    www.aol.com/news/trump-expected-pick-brooke...

    Trump has said he again plans to institute sweeping tariffs that are likely to affect the farm sector. He was considering offering the role to former U.S. Senator Kelly Loeffler, a staunch ally ...

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