Abstract
In this paper, we review the current state of knowledge about the acceleration of the Earth's spin, and about the closely related acceleration of the Moon. It is now established at a high confidence level that the acceleration of the Moon, when taken respect to Universal time, has changed by a large amount, and that it has even changed sign, within historic times. This almost certainly means that the acceleration of the Earth's spin has also changed by a large amount. At present we do not have enough information to say whether the changes have been in the contributions from tidal friction, in the contributions that do not arise from tidal friction, or both. Further, we do not know yet whether or not the variations in the Earth's rotation can account for the observed fluctuations in the longitudes of the Sun, the Moon, and the planets.
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Abbreviations
- ET:
-
ephemeris time
- UT:
-
Universal time
- T :
-
ET in centuries from 1900 January 0.5 ET
- τ:
-
UT in centuries from 1900 January 0.5 UT
- Δt :
-
=ET-UT
- n :
-
orbital angular velocity, in ET
- ν:
-
orbital angular velocity, in UT
- \(\dot n_M ,\dot n_S \) :
-
derivatives with respect to ET (Moon and Sun, resp.)
- v ' M ,v ' S :
-
derivatives with respect to UT (Moon and Sun, resp.)
- ω e :
-
spin velocity of Earth with respect to ET
- \(\dot \omega _e \) :
-
spin acceleration of Earth with respect to ET
- y :
-
=109 (\({{\dot \omega _e } \mathord{\left/ {\vphantom {{\dot \omega _e } {\omega _e }}} \right. \kern-\nulldelimiterspace} {\omega _e }}\)); Earth spin acceleration parameter
- y f :
-
portion ofy due to tidal friction (solid Earth and ocean)
- y nf :
-
non-tidal portion ofy
- L :
-
celestial longitude
- <>:
-
symbol forepochal average acceleration.
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Newton, R.R. The historical acceleration of the earth. Geophysical Surveys 1, 123–145 (1973). https://doi.org/10.1007/BF01449760
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DOI: https://doi.org/10.1007/BF01449760