The Moon's Role in the Habitability of the Earth

When one looks at the conditions which make advanced life on the Earth possible, one of the surprises is the importance of the Moon.

The Formation of the Moon

The compositions of the four inner "rocky" planets are similar with Mercury at density 5.4 g/cm³, Venus at 5.2, Earth at 5.5 and Mars at 3.9 g/cm³. This is interpreted as evidence of a core of iron and nickel, with Mars having a smaller core. Even the largest meteorites often show iron/nickel cores, so that the iron core seems like a signature for the formation of massive objects in the inner part of the solar system.

But Earth's Moon with a density of 3.3 g/cm3 is very different from the Earth and from the other bodies in the inner solar system. This was one of the first clues that the origin of the Moon was not just accretion from the same material from which the Earth was formed. 但月球的密度为3.3 g/cm³，与地球和其他内太阳系天体非常不同。这是最早表明月球起源并非仅仅来自地球形成时相同材料的线索之一。

Using data on the structure of the Earth, a simplified perspective can be constructed of the inner planets and Earth's Moon. The size of Earth's core is shown, and the planet densities above are used to construct similar images of the other inner planets. All except the Moon have sizable iron cores. The moons of Mars are too small to show in this perspective.

By the time the Moon samples and extensive data from the Apollo program were analyzed, it was clear that the Moon had a hot, violent origin which left it without significant iron content. The process of modeling the process could begin.

According to Ward and Brownlee, there is remarkable similarity between the trace element content of the Moon rocks and rocks from Earth's mantle. Also the isotopic content of the Earth and Moon samples was essentially identical.

More than a decade was spent analyzing the rich body of information from the Apollo program, including many detailed studies of the surface rocks collected from the Moon. By the mid 1980's there were a number of advocates for an extraordinary and seemingly unlikely scenario for the formation of the Moon. The proposed formation process involves a collision of the young Earth with a body with the mass of Mars or greater. At right is a series of sketches which qualitatively describe this scenario. These sketches follow Ward and Brownlee, who credit A. Cameron and R. M. Canup with computer simulations of this series of events. 超过十年的时间被用于分析阿波罗计划丰富的信息，包括许多关于从月球表面采集的岩石的详细研究。到20世纪80年代中期，有一些人支持一种非凡且似乎不太可能的月球形成情景。所提出的形成过程涉及年轻地球与一个质量相当于火星或更大的天体碰撞。右侧是一系列草图，这些草图定性地描述了这一情景。这些草图遵循Ward和Brownlee的描述，他们将A. Cameron和R. M. Canup归功于对这一系列事件的计算机模拟。 In view of the facts that the tilt angle of the Earth's spin axis is favorable to life, and that the mass of the large Moon is important in stabilizing that spin axis, this proposal for the Moon's formation is remarkable indeed. "To produce such a massive moon, the impacting body had to be the right size, it had to impact the right point on Earth, and the impact had to have occurred at just the right time in the Earth's growth process."(Ward & Brownlee) 鉴于地球自转轴的倾斜角有利于生命存在，而大月球的质量在稳定该自转轴方面也起着重要作用，这一关于月球形成的假说确实令人印象深刻。‘要产生如此巨大的月球，撞击体必须是适当大小，必须撞击地球的适当位置，且撞击必须发生在地球成长过程中的适当时间。’（Ward & Brownlee） Some history 一些历史

This hypothesis about the origin of the Moon is sometimes called "The Big Whack"

According to Canup's simulations, most of the above series of steps would have been acomplished in a time period on the order of a day! She also projects that the Moon might have then formed from the debris in a period on the order of a hundred years. Since rock samples from the Moon have been dated as old as 4.4 billion years, the projected impact is placed in the first 100 million years or so of the Earth's formation.

This is an artist's conception of the mooon-forming impact from NASA, image credit NASA/JPL-Caltech. There is an accompanying video at the linked NASA site.

Development of Lunar Origin Hypotheses

Before the landing of Apollo 11 on the Moon in 1969, the most popular theory was the the Moon had formed cold and could be a Rosetta Stone for studying the origin of the solar system. The sheer volume of data and samples returned by the Apollo program occupied planetary scientists for over a decade. At a critical meeting on the origin of the Moon held in Kona, Hawaii in 1984 a new picture began to emerge, one involving a massive impact early in the history of the Earth. A collection of papers from that meeting was published in a 1986 book edited by Hartmann, Phillips and Taylor who had been working on the impact hypothesis for some years. Hartmann had worked with Donald R. Davis on earlier models of this hypothesis. Cameron and Canup also worked on the impact hypothesis and did computer simulations of the process. Such modeling was the subject of Dr. Robin Canup's Ph.D. dissertation in the 1990's on the moon's origin and the giant impact hypothesis.