The Moon: A Museum of Cosmic Catastrophes?

Debussy, Claire de Lune
A Quick Summary...

In many ways the earth-moon system is more like a double planet than a planet and moon. The moon is very large (27%) the size of the earth which is a much larger proportion to the size of a parent planet for any other moon in the solar system. Further more its size is comparable to the largest moons of the Jovian planets.

 The moon is interesting for a number of reasons. It certainly is an object of beauty and has been venerated by all peoples. It also represents a museum of the early history of the solar system.

 

The Lunar Orbit

 The moon travels around the earth with a nearly circular orbit of mean radius 384, 400 km and with a period of 27.321661 days. The orbit is a synchronous one which means that the moon's rotation rate is the same as its orbital rate - this means that we always see the same face of the moon pointing towards us. This phenomenon is called tidal locking and, as the name suggests is due to the tidal force that the earth exerts on the moon. This effect is often "seen" or assumed in the case of close binary stars.

Craters, Maria, Rills and Catastrophes

Galileo angered many when he proclaimed that the moon was not a perfect sphere but poc-marked, rugged - much like the earth. Later generations of astronomers have painstakingly mapped the lunar surface both from the earth as well as from lunar orbiters. The lunar surface reveals a number of significant features: What produced the craters, maria, rilles and rays? Are these distinct phenomena or are they related? Several decades ago the idea was popular that the craters were the result of volcanism on the lunar surface. Since this time, however, the incidence of volcanism on the lunar surface has been shown to be too little to account for the cratering that we observe. Instead the currently favoured view is that the lunar surface was struck numerous times in the early phase of the solar system by large "asteroidal" objects. These numerous collisions throw up blankets of debris that gave rise to the rays that we see around some craters. In the early epoch of the moon's history the impact of numerous asteroids and the hotter lunar environment would have produced massive lava flows and it is believed that the maria were indeed seas at one time - but seas of lava not water . The ejecta produced in the early cratering episodes would not be expected to be visible - these would be obliterated by other impacts and flows. We know realize that the presence of rays tells us the relative ages of craters. Young craters are accompanied by the rays produced by their ejecta - old craters are not. We can put all this together to arrive at a crude lunar chronology:

 

This still leaves un-answered the origin of lunar rills. It is now conceded that lunar rills are evidence of lunar volcanism. This is further supported by the observation of lunar domes - small raised regions that are an indicator of volcanic activity. The two figures below are different views of the famous Hadley Rille. Consult a lunar atlas and try to view this the next time you are using a small telescope.

The phenomenon of cratering has interesting parallels with cratering observed on earth and during the past decade has led us to realize that "quasi-periodic" catastrophic meteor impacts are part of the earth-moon history. This has spawned a number of theories that we will consider in a future lecture.

 

 

 

Lunar Geology

The moon has many similarities and some surprising difference with the earth. The composition of the moon is differentiated and the age of the moon is essentially the same as that of the earth. The moon's composition however is decidedly different than is the earth's composition. The moon's composition favours the refractory elements (solid at high temperature) but is underabundant (wrt earth) in volatile elements. This suggests that the moon was formed at a higher temperature than was the earth.

 Also, the moon does show seismic activity - "moonquakes" which suggests that the lunar core may be partially molten. The lunar crust, on the other hand, is much thicker in relation to the lunar radius than is earth's. This is the result of the rapid cooling one would expect for a small body.

 The structure of rocks on the lunar surface is also distinctly different than on earth. Most significant is the large number basalts (indicating lava flow) and breccias which are basically broken or pulverized rock "glued together". This would suggest that the lunar surface has been pummeled vigorously in its past.

 

The Lunar Atmosphere

Basically - there is none! The moon is a small body gravitationally speaking. At the temperatures the bright side of the moon would be subject to gases would heat and reach velocities comparable to the velocity of gases in the earth's atmosphere. On the moon, however these gases would quickly escape ( diffuse ) into space. The lack of atmosphere, of course means that there is no weather and hence no weathering on the lunar surface.

 

Origin of the Moon

  1. fission hypothesis : spinning semi-molten earth split into two bodies. Problem: why was the earth spinning so fast (10x) and where did the angular momentum go?
  2. co-accretion : moon and earth formed together. Problem: why the very different compositions.
  3. capture hypothesis : moon formed closer to the sun and was capture by the earth. Problem: requires a very unlikely set of interaction between the inner planets (3 - body encounter).
  4. large-impact hypothesis : A larger body hit the earth-moon planetesimal. The moon formed from some of the debris. The ejecta would be primarily crust . So far this looks like the winner.

Web Sites to Visit ...


Seeds: Chp 21;
Kaufmann: Chp 9; pgs162-178