Lunar orbital evolution: A synthesis of recent results

@article{Bills1999LunarOE,
  title={Lunar orbital evolution: A synthesis of recent results},
  author={B. Bills and R. Ray},
  journal={Geophysical Research Letters},
  year={1999},
  volume={26},
  pages={3045-3048}
}
The present rate of tidal dissipation in the Earth-Moon system is known to be anomalously high, in the sense that the implied age of the lunar orbit is only 1.5×109 years, though other evidence suggests an age closer to 4×109 years. To assess how long the anomalous dissipation has persisted, we use published estimates of lunar orbital configurations derived from (a) fine grained sediments containing tidal laminations and (b) numerical ocean models averaged over varying ocean geometries. The… Expand
Explicitly modelled deep-time tidal dissipation and its implication for Lunar history
Abstract Dissipation of tidal energy causes the Moon to recede from the Earth. The currently measured rate of recession implies that the age of the Lunar orbit is 1500 My old, but the Moon is knownExpand
On the Tidal History and Future of the Earth–Moon Orbital System
Earth’s rotation rate and the evolution of the Earth–Moon system have been controlled by tidal dissipation in Earth’s ocean. Attempts to model the tidal history have shown incomplete compatibilityExpand
Tidal dissipation in the lunar magma ocean and its effect on the early evolution of the Earth–Moon system
Abstract The present-day inclination of the Moon reflects the entire history of its thermal and orbital evolution. The Moon likely possessed a global magma ocean following the Moon-forming impact. InExpand
Tidal evolution of the Moon from a high-obliquity, high-angular-momentum Earth
TLDR
It is shown that tidal dissipation due to lunar obliquity was an important effect during the Moon’s tidal evolution, and the lunar inclination in the past must have been very large, defying theoretical explanations. Expand
Scaling in global tidal dissipation of the Earth-Moon system
Abstract The Moon migrated to cm over a characteristic time r / v = 10  Gyr by tidal interaction with Earth’s oceans at a present velocity of v = 3.8  cm yr − 1 . We model global dissipation to coverExpand
Effects of orbital evolution on lunar ice stability
[1] Many regions near the lunar poles are currently cold enough that surface water ice would be stable against sublimation losses for billions of years. However, most of these environments areExpand
Consequences of Tidal Dissipation in a Putative Venusian Ocean.
The solar tide in an ancient Venusian ocean is simulated using a dedicated numerical tidal model. Simulations with varying ocean depth and rotational periods ranging from -243 to 64 sidereal EarthExpand
Formation of the Lunar Fossil Bulges and Its Implication for the Early Earth and Moon
First recognized by Laplace over two centuries ago, the Moon’s present tidal-rotational bulges are significantly larger than hydrostatic predictions. They are likely relics of a former hydrostaticExpand
Orbital Periodicities Reflected in Ancient Surfaces of our Solar System and the Implications for a Record of Early Life
Uniformitarian processes, governed by invariant physical laws, remain the most reliable source for reconstructing the past. Driving many of the repetitive, predictable processes are the orbitalExpand
Ocean Tidal Dissipation and its Role in Solar System Satellite Evolution
The history of satellites in the Solar System is quite diverse. For example, satellites like Io and Enceladus exhibit active volcanism currently, while satellites like Ganymede and Tethys show signsExpand
...
1
2
3
4
5
...

References

SHOWING 1-10 OF 35 REFERENCES
Evolution of the lunar orbit with temperature- and frequency-dependent dissipation
The coupled thermal-dynamical evolution of the Earth-Moon system is modeled. The lunar orbit is assumed noncircular and inclined to Earth's equator plane. Solid planet dissipation in the Earth andExpand
Lunar nodal tide and distance to the Moon during the Precambrian
TLDR
The first direct determination of the lunar distance in the Precambrian is presented, interpreting a 23.3±0.3-yr periodicity preserved in a 2,500 Myr BP Australian banded iron formation as reflecting the climatic influence of the Lunar nodal tide, which has been detected with its modern 18.6-yrperiodicity in some modern climate records. Expand
Effects of tidal dissipation in the oceans on the Moon's orbit and the Earth's Rotation
The dissipation of tidal friction in the oceans and atmosphere has been estimated by calculating the secular perturbations of the moon's orbit by the tides using the available tide models for theExpand
A stochastic model of the Earth-Moon tidal evolution accounting for cyclic variations of resonant properties of the ocean: an asymptotic solution
A stochastic model of the Earth-Moon tidal evolution taking into account fluctuating effects of the continental drift is described. The above effects caused by alternation of periods of consolidationExpand
Secular effects of oceanic tidal dissipation on the Moon's orbit and the Earth's rotation
The earth and moon are considered as a two-body system in gravitational isolation from the sun and other planets. The lunar orbit is taken as circular, and the solid earth is assumed to be a rigidExpand
Earth—Moon tidal evolution: model results and observational evidence
Abstract There are five datasets which can be used to verify models of the Earth—Moon tidal evolution. Those are: (1) geological evidence of the age of earth and lunar rocks; (2) paleontological andExpand
Tides and the evolution of the Earth—Moon system
Summary. A model of the tides in a hemispherical ocean is used to investigate the effect of changes in the Earth's rotation rate on the power dissipated by the ocean tides. The results obtained areExpand
Tidal dissipation in the oceans: astronomical, geophysical and oceanographic consequences
  • K. Lambeck
  • Physics
  • Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences
  • 1977
The most precise way of estimating the dissipation of tidal energy in the oceans is by evaluating the rate at which work is done by the tidal forces and this quantity is completely described by theExpand
Evolution of the Earth-Moon System
The tidal evolution of the Earth-Moon system is reexamined. Several models of tidal friction are first compared in an averaged Hamiltonian formulation of the dynamics. With one of these models, fullExpand
The history of the lunar orbit
A method of calculating the past states of the earth-moon system is developed. The method is based on the existence of three distinct time scales for dynamical change. The short time scale isExpand
...
1
2
3
4
...