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Day length fluctuations

The length of the day (LOD), which has increased over the long term of Earth's history due to tidal effects, is also subject to fluctuations on a shorter scale of time. Exact measurements of time by atomic clocks and satellite laser ranging have revealed that the LOD is subject to a number of different changes. These subtle variations have periods that range from a few weeks to a few years. They are attributed to interactions between the dynamic atmosphere and Earth itself. The International Earth Rotation and Reference Systems Service monitors the changes.

In the absence of external torques, the total angular momentum of Earth as a whole system must be constant. Internal torques are due to relative movements and mass redistribution of Earth's core, mantle, crust, oceans, atmosphere, and cryosphere. In order to keep the total angular momentum constant, a change of the angular momentum in one region must necessarily be balanced by angular momentum changes in the other regions.

Crustal movements (such as continental drift) or polar cap melting are slow secular (non-periodic) events. The characteristic coupling time between core and mantle has been estimated to be on the order of ten years, and the so-called 'decade fluctuations' of Earth's rotation rate are thought to result from fluctuations within the core, transferred to the mantle.[1] The length of day (LOD) varies significantly even for time scales from a few years down to weeks (Figure), and the observed fluctuations in the LOD - after eliminating the effects of external torques - are a direct consequence of the action of internal torques. These short term fluctuations are very probably generated by the interaction between the solid Earth and the atmosphere.

The length of day of other planets also varies, particularly of the planet Venus, which has such a dynamic and strong atmosphere that its length of day fluctuates by up to 20 minutes.[2]

  1. ^ Hide, R. (1989). "Fluctuations in the Earth's Rotation and the Topography of the Core–Mantle Interface". Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences. 328 (1599): 351–363. Bibcode:1989RSPTA.328..351H. doi:10.1098/rsta.1989.0040. S2CID 119559370.
  2. ^ Whitt, Kelly Kizer (2021-05-05). "The length of a day on Venus is always changing - Space". EarthSky. Retrieved 2023-04-29.

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تقلب طول النهار Arabic Fluctuacions de la durada del dia Catalan Fluctuaciones de la duración del día Spanish 日長波動 Chinese

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