Lably
Skip to content

Cyclostratigraphy

Study of astronomically forced climate cycles within sedimentary successions

  • 2 min read
  • 3 chapters

Related on Lably

Through Astronomy, Climate variability and change and Sedimentary rock

Orbital changes

Astronomical cycles (also known as Milankovitch cycles) are variations of the Earth's orbit around the Sun due to the gravitational interaction with other masses within the Solar System. Due to this cyclicity, solar irradiation differs through time on different hemispheres and seasonality is affected. These insolation variations have influence on Earth's climate and on the deposition of sedimentary rocks.

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. Precession influences how much insolation each hemisphere receives. Obliquity controls the intensity of the seasons. Eccentricity influences how much insolation the Earth receives altogether. Varied insolation directly influences Earth's climate, and changes in precipitation and weathering are revealed in the sedimentary record. The 405 kyr eccentricity cycle helps correct chronologies in rocks or sediment cores when variable sedimentation makes them difficult to assign. Indicators of these cycles in sediments include rock magnetism, geochemistry, biological composition, and physical features like color and facies changes.

Sign in to keep reading

2 more chapters are free with a Lably account.

More in Earth science