http://thescotsman.scotsman.com/index.cfm?id=166052007

Why does the Moon look like this? Here it is in black and white ...

EBEN HARRELL
 ([EMAIL PROTECTED]) 

SCIENTISTS in Edinburgh have recreated Moon rock in a laboratory and simulated 
the 
conditions of an asteroid explosion to learn why the lunar body has its 
distinctive black 
and white colouration. 

The Moon was formed 4.5 billion years ago after the Earth collided with a 
massive comet 
and a large chunk of the debris was trapped in the earth's gravitational pull. 

But the collision released a huge amount of energy, in the form of heat, which 
turned 
much of the Moon's surface into a lunar ocean of magma, or lava. The lava then 
cooled and 
solidified. To investigate the effect this cooling had on the Moon's surface, 
geologists 
at Edinburgh University created artificial pieces of Moon rock based on the 
chemical 
compositions of samples brought back from the Apollo space missions. They then 
used a 
special furnace to heat the artificial rock to 1,500C, turning it to magma, and 
then 
watched it cool. 

White crystals were the first to form in the magma, floating on top of the 
black liquid, 
suggesting that during its original formation, the Moon was covered by a 
perfect white 
sheen. 

But the centre of the scientists' sample - and the Moon - was black. 

This all but proves the long-held theory that some 2.5 billion years ago, an 
asteroid 
shower must have hit the Moon, rupturing its white exterior and causing 
volcanic 
explosions of black lava. The lava - dark in colour because of its high 
concentration of 
iron - was slowly pulled by the Moon's weak gravity into valleys, exposing dark 
craters 
and white "lunar highlands". 

This is why the Moon is white and black. 

Dr Stephan Klemme, the lead researcher, said: "When you look at rocks from the 
Moon and 
from the Earth, they are very similar. The black rock on Arthur's Seat [in 
Edinburgh], 
for example, is not much different from black Moon rock. However, there are 
crucial 
differences that have baffled scientists. 

"Our experiments have shown that the minerals creating the white rock - seen in 
the lunar 
highlands - would have crystallised first, whereas the dark and heavy iron-rich 
minerals 
would have sunk in the magma oceans, creating darker rock that would have been 
buried 
deep inside the Moon. 

"The reason that the darker rocks are now visible on the surface of the Moon is 
proof of 
a later period of intensive meteorite showers. The iron-rich minerals that were 
deep 
inside the Moon proved to be especially high in hafnium and low in tungsten, 
and would 
have erupted to the surface as molten rock, filling the valleys on the Moon and 
leaving a 
darker shade we observe today." 

Dr Klemme, of the university's school of geosciences, said the research was 
carried out 
in Edinburgh because of a specialised furnace that allowed scientists to not 
only heat 
the Moon rock, but do so in atmospheric conditions that mimicked the low-oxygen 
conditions found on the lunar surface. 

The research comes during renewed interest in manned exploration of Earth's 
only 
satellite. Last month, NASA, the US space agency, outlined plans for a 
permanent base on 
the Moon as part of preparation for a voyage to Mars. Construction of the base 
is 
scheduled to take about five years, with the first preliminary missions 
beginning by 
2020. 

The latest findings serve as another confirmation of the giant-impact 
hypothesis for the 
formation of the Earth-Moon system. In this theory, the impact of a Mars-sized 
body, 
which has been referred to as Theia or Orpheus, into the proto-Earth is thought 
to have 
put enough material into the planet's orbit to create the Moon. Computer 
simulations can 
account for the angular momentum of the Earth-Moon system, as well as the small 
size of 
the lunar core.

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