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Old 05-April-2006, 06:50 PM
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Default Why is Mercury so heavy?

Hardcore Mercury had soft edges smashed away

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A jolting collision between Mercury and a large planetesimal in the solar system's formative years could have left the planet unusually dense, according to a new simulation. And as much as 16 million billion tonnes of the material kicked up by the impact might have rained down on the proto-Earth.

Jonathan Horner and colleagues at the University of Bern, Switzerland, created the model to see whether a collision between an early Mercury – about 2.25 times its current size – and a planetesimal of half Mercury's current size could have produced the first rock from the Sun that we see today.

Mercury is something of a planetary misfit. It is less than 5000 kilometres in diameter, making it slightly smaller than Saturn's giant moon, Titan. Yet it is more than twice as massive as Titan and is thought to have an iron core that accounts for about two-thirds of its mass.

Scientists have suggested several possible explanations, but more direct measurements of the planet are needed to determine how Mercury came to be so dense.
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Old 05-April-2006, 06:56 PM
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"Slightly smaller yet twice as massive"

What? Isn't massive used in context of size? Or did they mean Mass? Or do I just have it backward?
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Old 05-April-2006, 07:06 PM
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They mean "mass". - for example, a cubic meter of feathers has less mass than a cubic meter of lead. They occupy the same volume and maybe have the same dimensions, but their masses are different.

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Old 05-April-2006, 10:35 PM
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An alternative would have been that Mercury formed about where it was, and the lighter elements didn't exist there in any quantity.
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Old 06-April-2006, 01:17 AM
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That's always been my thought. The heat and winds from the sun would have evaporated many of the lighter elements.
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Old 06-April-2006, 07:10 PM
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Does this mean we could possibly strip mine the planet for massive space based construction projects? (yes I know this is very very very long term)
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Old 06-April-2006, 11:44 PM
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Quote:
That's always been my thought. The heat and winds from the sun would have evaporated many of the lighter elements.
If thats true, then why don't we see any effect on Venus? In fact, the uncompressed density of a terrestrial planet (the density it would have if it were not compressed by its own gravity) has a linear dependence of the mass - the compressed density of the Earth is higher than Venus' (by the same amount it is more massive than Venus), higher than Mars (again, linear relationship). The moon is slightly different, but given that it formed out of the Earth's mantle, there's no problem with that. The only planet that does not fit into this scheme is Mercury.

So there is on one hand a dependence of mass, but no dependence of distance. If this is true, the logical conclusion would be that Mercury lost a great part of its mantle.

(If you can read german, look at the following picture I did for another forum: http://www.planeten.ch/images/massedichte.gif, if you can't, here's a short explanation: Masse = mass, Dichte = density, Beziehung = relationship, Unkomprimierte Dichte = uncompressed density, Erde = Earth, Merkur = Mercury, Mond = Moon The dot that is extremely of the line formed by Mars, Earth and Venus, is Mercury, the dot nearer to the line is the Moon)

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Old 07-April-2006, 04:06 AM
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You can't say that Venus is unusual by comparing it to Earth. Earth's density is heavier than it should be because a lot of the lighter stuff ended up in the Moon.
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Old 07-April-2006, 09:18 AM
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Well, the mass of Venus is about 82% of the mass of the Earth. The Moon has only around 1.2% of the mass of the Earth. This doesn't add up, meaning, you need an additional explanation - which may be given by the diagram I posted before.
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