When worlds collide
Billions of years ago a huge object struck the Earth, and
our Moon was born from the debris. But we still don't know
where it came from.
Marcus Chown reports
17 November 2004
In astronomical circles, it is pretty much official. The Moon
was created when a body about the size of Mars slammed into the
newborn Earth. In the cataclysm, the molten iron core of the
impacting body sank to the Earth's core while its molten mantle
splashed out into space to form a ring of debris. This congealed
into the Moon. The Moon, originally about 20 times closer to the
Earth, gradually moved out to its current location. This
"Big Splash" picture, proposed by William Hartmann, Al
Cameron and their colleagues in 1975, is very well-received. For
instance, it explains why the Moon contains essentially no iron.
Unfortunately, it has a big problem. It concerns the body
that collided with the Earth. "Where did it come
from?" says Richard Gott of Princeton University in New
Jersey. "The clues suggest a seemingly impossible
location." One such clue comes from comparing the
composition of the Earth and Moon. Cosmologists are pretty sure
that the disc of swirling debris from which the planets
congealed had a different composition at different distances
from the newborn Sun. The Mars-mass body would, therefore, not
have had the same make-up as the Earth. In the impact, the Earth
and Moon would have been contaminated by different amounts of
this material, which means, when we examine terrestrial and
lunar rocks, we should see marked differences in composition.
"The bizarre thing is, we don't," says Gott.
Take oxygen. It comes in three types - oxygen-16 and two
heavier and rarer types, oxygen-17 and oxygen-18. The relative
proportions of these are like a chemical
"fingerprint". The prediction of the Big Splash
scenario is that the Earth's oxygen fingerprint will be quite
different from the Moon's. But it isn't. It's pretty much
identical.
The oxygen evidence forces the conclusion that the body that
hit the Earth and created the Moon formed at exactly the same
distance from the Sun as the Earth. This is also indicated by
computer simulations of the birth of the Moon, which show that
the impactor came in at relatively low speed, characteristic of
bodies in the Earth's vicinity. "But if the impactor formed
at the same distance from the Sun as the Earth, there is a big
problem understanding how it ever managed to grow as big as
Mars," says Gott.
The accepted theory of the birth of the planets is that they
gradually "accreted" from debris pulled in by their
gravity. The bigger they got, the stronger was their gravity and
the more matter they pulled in. Since it is a process in which
the rich get richer and the poor poorer, the impactor should
have been gobbled up by the proto-Earth long before it reached
the mass of Mars. So, why wasn't it?
Gott set out to solve the puzzle with Princeton colleague
Edward Belbruno. They began by asking: is there some special
location at the Earth's distance from the Sun where a body could
grow to the mass of Mars? Immediately, they realised there is.
In fact, there are two places. These are the
"Lagrange-4" and "Lagrange-5" points, whose
existence was first suggested by the French mathematician Joseph
Louis Lagrange in 1772. One lags 60 degrees behind the Earth as
it orbits the Sun and the other precedes the Earth in its orbit
by the same amount. At the Lagrange points, all the forces in
the Sun-Earth system miraculously balance each other. What's
more, any slow-moving debris that happens to find its way there
becomes hopelessly trapped in a kind of interplanetary Sargasso
Sea.
Gott and Belbruno say the Lagrange points are places where
matter would naturally have accumulated and where a body could
have grown in peace without being affected by the fast-growing
Earth. Eventually, when it had reached the mass of Mars, the
gravity of other embryonic planets in the Solar System, such as
Jupiter, would have tugged it repeatedly, perhaps over millions
of years, until it was ejected from the Lagrange point.
In computer simulations, Gott and Belbruno have followed the
subsequent course of events. They find nothing can prevent the
inevitable - a titanic collision with the Earth. Everything
appears to fit. The impactor comes in on a low-velocity orbit,
delivering a glancing blow on the Earth. Gott and Belbruno's
simulations show that, in a quarter of encounters, the end
result is a body exactly like the Moon.
If Gott and Belbruno are right, the Earth had once had a
planetary which shared its orbit round the Sun. "It's a
clever idea which would solve some obvious problems," says
Carl Murray of Queen Mary University in London. But he thinks
work still needs to be done to prove it. The most interesting
consequence of Gott and Belbruno's scenario is its implications
for our prospects of finding extraterrestrial life. The Earth
has the biggest moon compared to its size of any planet in the
Solar System (Pluto also has a big moon but is rarely considered
a full-blown planet nowadays). And a giant moon has been
important for the evolution of life.
The Earth, for instance, spins around its axis like a top.
And, in common with all tops, it has a tendency to wobble
wildly. Such wobbles would cause severe changes in the Earth's
climate, with grave consequences for life. But every time the
Earth tips too far over on its axis, the Moon's gravity rights
it. The Moon has, therefore, ensured a relatively stable climate
for the evolution of life over billions of years.
And this is not the only way that the Moon has been important
in the evolution of life. The tides created by the Moon, which
are three times bigger than those created by the Sun, leave
large areas of the ocean margins high and dry twice a day.
Hundreds of millions of years ago, this enabled marine creatures
to gradually adapt to arid conditions - the first step in the
conquest of the land. But the Moon's key importance in the
evolution of life has a depressing consequence for our prospects
of finding ET life. The reason is that the kind of collision
needed to create a big moon has always seemed an extremely
unlikely event.
Gott and Belbruno don't see it like that. They say that the
formation of a large Mars-mass body at one of the Lagrange
points of other planetary systems may not be that uncommon at
all. And, since their simulations show a big moon created in a
quarter of cases, the formation of a big moon may be more likely
than anyone expected. They even speculate that there may exist
planetary systems in the Galaxy, where two or more terrestrial
planets have big moons.
Is there any way of proving Gott and Belbruno's scenario? At
first sight, it would appear to be difficult. After all, the
Moon was formed in a tremendously violent manner and the
impactor was utterly destroyed. It would be highly unlikely that
any unprocessed material from that time could have survived to
the present day. "But perhaps not impossible," says
Gott.
Gott and Belbruno point to an asteroid, or chunk of
interplanetary rubble, discovered in 2002. "2002 AA29"
is barely the size of a football pitch and is currently in a
orbit which periodically brings it within a mere 5.8 million
kilometres of the Earth. The peculiar orbit is very similar to
the one the impactor that created the Moon would have been in
4.55 billion years ago. "You have to ask yourself, how did
2002 AA29 get in that orbit?" says Belbruno.
An intriguing possibility is that it might have been
associated with Lagrange-4 or Lagrange-5 in the distant past and
at some point was kicked out. If so, 2002 AA29 may carry the
imprint of the material from which the impactor and the Earth
were formed. Bizarrely, 2002 AA29 has been picked out by
planetary physicists as an asteroid that would be relatively
easy for a space probe to visit. Gott and Belbruno suggest that
a mission to return a sample would be most interesting. If it
found iron and material with the same oxygen fingerprint as the
Earth and Moon, it would support the Lagrange point scenario. If
it contained no iron, it could be a bit of the splashed out
material from the impact that formed the Moon. "Either way,
we think 2002 AA29 could tell us about the origin of the Earth
and Moon," says Gott. "It may be the most valuable
chunk of rock in the Solar System."
Marcus Chown is the author of 'The Universe Next Door:
Twelve Mind-Blowing Ideas from the Cutting Edge of Science',
published by Headline, £7.99
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