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  1. The inner Van Allen Belt extends typically from an altitude of 0.2 to 2 Earth radii (L values of 1.2 to 3) or 1,000 km (620 mi) to 12,000 km (7,500 mi) above the Earth. [ 4 ] [ 16 ] In certain cases, when solar activity is stronger or in geographical areas such as the South Atlantic Anomaly , the inner boundary may decline to roughly 200 km [ 17 ] above the Earth's surface.

  2. Earth orbit (yellow) compared to a circle (gray) Earth orbits the Sun at an average distance of 149.60 million km (92.96 million mi), or 8.317 light-minutes, [1] in a counterclockwise direction as viewed from above the Northern Hemisphere. One complete orbit takes 365.256 days (1 sidereal year), during which time Earth has traveled 940 million ...

  3. Feb 27, 2020 · The Milankovitch cycles include: The shape of Earth’s orbit, known as eccentricity; The angle Earth’s axis is tilted with respect to Earth’s orbital plane, known as obliquity; and. The direction Earth’s axis of rotation is pointed, known as precession. Let’s take a look at each (further reading on why Milankovitch cycles can't explain ...

  4. nssdc.gsfc.nasa.gov › planetary › factsheetEarth Fact Sheet - NSSDCA

    Orbital parameters Semimajor axis (10 6 km) 149.598 Sidereal orbit period (days) 365.256 Tropical orbit period (days) 365.242 Perihelion (10 6 km) 147.095 Aphelion (10 6 km) 152.100 Mean orbital velocity (km/s) 29.78 Max. orbital velocity (km/s) 30.29 Min. orbital velocity (km/s) 29.29 Orbit inclination (deg) 0.000 Orbit eccentricity 0.0167 Sidereal rotation period (hrs) 23.9345 Length of day ...

  5. Nov 24, 2023 · The second important feature of Earth’s motion is the tilt of the rotational axis (also known as obliquity) relative to the plane of the orbit around the sun (Figure 3.4.2). At present our axis is tilted at 23.5⁰ from “vertical”, but that varies from 22.1⁰ to 24.5⁰ and back to 22.1⁰ on a time scale of close to 41,000 years.

  6. Over long periods of time, the gravitational pull of other members of our solar system slowly change Earth’s spin, tilt, and orbit. Over approximately 100,000 – 400,000 years, gravitational forces slowly change Earth’s orbit between more circular and elliptical shapes, as indicated by the blue and yellow dashed ovals in the figure to the ...

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  8. Earth revolves around an enormous source of energy: the Sun. It orbits the Sun every 365 and one-quarter days. It spins on an axis that is tilted 23 and a half degrees to the plane of its orbit. This axial tilt remains steady throughout the year. Depending on the time of year, some parts of the Earth are tilted more toward the direct rays of ...

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