Until recently, high-resolution global modeling of tides has been done separately from high-
resolution global modeling of the atmospherically-forced oceanic general circulation. Here …

The long-term history of the Earth–Moon system as reconstructed from the geological record
remains unclear when based on fossil growth bands and tidal laminations. A possibly more …

Due to tidal interactions in the Earth-Moon system, the spin of the Earth slows down and the
Moon drifts away. This recession of the Moon can now be measured with great precision, but …

After the initial suggestion by Zahnle and Walker (1987) that the torque accelerating the spin
rate of the Earth and produced by the heating of the atmosphere by the Sun could counteract …

The melting of ice sheets and global glaciers results in sea-level rise, a pole-to-equator
mass transport increasing Earth's oblateness and resulting in an increase in the length of …

The chaotic behavior of the Solar System prevents the prediction of the precise evolution of
the planetary secular frequencies. Here we use four cyclostratigraphic sequences,∼ 259 Ma …

In the leading theory of lunar formation, known as the giant impact hypothesis, a collision
between two planet-size objects resulted in a young Earth surrounded by a circumplanetary …

The Earth's rotation has been decelerating throughout its history due to tidal dissipation, but
the variation of the rate of this deceleration through time has not been established. We …

Astronomical insolation forcing plays an important role in pacing Earth's climate history,
including paleoclimate dynamics, and its imprint can be seen in various geoarchives. Its …

The angular momentum of the Earth‐Moon system was initially dominated by Earth's rotation
with a short solar day of around 5 hr duration. Since then, Earth gradually transferred …