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  2. Milankovitch cycles - Wikipedia

    en.wikipedia.org/wiki/Milankovitch_cycles

    Milankovitch studied changes in these movements of the Earth, which alter the amount and location of solar radiation reaching the Earth. This is known as solar forcing (an example of radiative forcing). Milankovitch emphasized the changes experienced at 65° north due to the great amount of land at that latitude.

  3. 100,000-year problem - Wikipedia

    en.wikipedia.org/wiki/100,000-year_problem

    δ 18 O, a proxy for temperature, for the last 600,000 years (an average from several deep sea sediment carbonate samples) [a]. The 100,000-year problem (also 100 ky problem or 100 ka problem) of the Milankovitch theory of orbital forcing refers to a discrepancy between the reconstructed geologic temperature record and the reconstructed amount of incoming solar radiation, or insolation over ...

  4. Orbital forcing - Wikipedia

    en.wikipedia.org/wiki/Orbital_forcing

    Orbital forcing is the effect on climate of slow changes in the tilt of the Earth's axis and shape of the Earth's orbit around the Sun (see Milankovitch cycles).These orbital changes modify the total amount of sunlight reaching the Earth by up to 25% at mid-latitudes (from 400 to 500 W/(m 2) at latitudes of 60 degrees).

  5. Axial precession - Wikipedia

    en.wikipedia.org/wiki/Axial_precession

    After about 26 000 years the difference amounts to a full year, so the positions of the seasons relative to the orbit are "back where they started". (Other effects also slowly change the shape and orientation of the Earth's orbit, and these, in combination with precession, create various cycles of differing periods; see also Milankovitch cycles ...

  6. Apsidal precession - Wikipedia

    en.wikipedia.org/wiki/Apsidal_precession

    This interaction between the anomalistic and tropical cycle is important in the long-term climate variations on Earth, called the Milankovitch cycles. Milankovitch cycles are central to understanding the effects of apsidal precession. An equivalent is also known on Mars. Effects of apsidal precession on the seasons with the eccentricity and ap ...

  7. Cyclostratigraphy - Wikipedia

    en.wikipedia.org/wiki/Cyclostratigraphy

    The main orbital cycles are precession with main periods of 19 and 23 kyr, obliquity with main periods of 41 kyr, and 1.2 Myr, and eccentricity with main periods of around 100 kyr, 405 kyr, and 2.4 Myr. [2] Precession influences how much insolation each hemisphere receives. Obliquity controls the intensity of the seasons.

  8. Greenhouse and icehouse Earth - Wikipedia

    en.wikipedia.org/wiki/Greenhouse_and_icehouse_Earth

    The astronomical components, discovered by the Serbian geophysicist Milutin Milanković and now known as Milankovitch cycles, include the axial tilt of Earth, the orbital eccentricity (or shape of the orbit), and the precession (or wobble) of Earth's rotation. The tilt of the axis tends to fluctuate from 21.5° to 24.5° and back every 41,000 ...

  9. Chandler wobble - Wikipedia

    en.wikipedia.org/wiki/Chandler_wobble

    The Chandler wobble is an example of the kind of motion that can occur for a freely ... Milankovitch cycles; United States Naval Observatory ... Free Precession of Earth