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- From: henry@zoo.toronto.edu (Henry Spencer)
- Subject: Re: Cheap Mars Rocks (was Re: Moon Dust For Sale)
- Message-ID: <C0pI3H.BJ8@zoo.toronto.edu>
- Date: Mon, 11 Jan 1993 20:26:04 GMT
- References: <C0Kq8D.G8F@zoo.toronto.edu> <1993Jan11.070745.23686@mr.med.ge.com>
- Organization: U of Toronto Zoology
- Lines: 29
-
- In article <1993Jan11.070745.23686@mr.med.ge.com> hinz@picard.med.ge.com (David Hinz (hinz@picard.med.ge.com)) writes:
- >By what mechanism do these rocks get here? Volcanic action & random launching?
- >How do they acheive escape velocity?
-
- Probably by complex phenomena associated with large impacts. One of the
- sticking points on declaring the SNC meteorites to be definitely Martian
- has been the difficulty in explaining precisely how they got off the planet.
- Getting shrapnel from a large impact off the Moon is not hard, but Mars's
- escape velocity is rather high for this kind of thing.
-
- >Why do they end up so often in
- >Antarctica? Or are they just more visible there? ...
-
- This one's just a sampling effect. Antarctica is a great place for
- meteorite hunters, because any rock found sitting on the ice *must* be
- a meteorite -- there's no other way it could get there. Elsewhere, it
- is hard to tell whether a random rock belongs where it's sitting or not.
-
- In particular, if memory serves, there are a few areas of Antarctica
- where ice flows just sort of terminate, gradually eroded away by wind
- rather than flowing into the ocean. A meteorite which falls on ice that
- is heading that way will end up on the surface in the termination area.
- This concentrates meteorites from large areas over long periods of time.
-
- A bonus is that the Antarctic environment is very cold and virtually
- sterile, preserving the meteorites in very nearly their pristine state.
- --
- "God willing... we shall return." | Henry Spencer @ U of Toronto Zoology
- -Gene Cernan, the Moon, Dec 1972 | henry@zoo.toronto.edu utzoo!henry
-