Re: Two questions
- From: "N:dlzc D:aol T:com \(dlzc\)" <N: dlzc1 D:cox T:net@xxxxxxxxxx>
- Date: Sat, 7 May 2005 14:46:55 -0700
Dear Volker Hetzer:
"Volker Hetzer" <volker.hetzer@xxxxxx> wrote in message
news:d5j0ca$rrs$1@xxxxxxxxxxxxxxxxxxxx
> N:dlzc D:aol T:com (dlzc) wrote:
>
>>
>> The only thing I can add is that the Moon
>> has left a pretty continuous record in
>> "tidal rhythmites" over the last 2 billion years. Not that
>> the lunar recession is
>> entirely (or at all) due to universal
>> expansion. In lunar recession, angular
>> momentum transfer from the spinning
>> Earth to the Earth-Moon system is the major player.
> How does it get transferred?
Pour a little coffee (or tea, or beer) in a cup. Swirl it
around, without using a spoon. How did you transfer angular
momentum to the fluid? You moved the container (hopefully).
Like a miner panning for gold.
The water on the Earth is like a "moving container", in that its
(the water's) contribution to spacetime (sorry Bjoern) is always
a little ahead of the Earth. The water sloshes momentum onto the
Moon, and brakes the Earth with tidal friction. In periods
"known" for high glaciation, the recorded lunar recession rate
was low.
To repair any damage I probably did:
Google Advanced
all the words: Earth Moon
exact phrase: angular momentum
either word: tide tidal
from domains: .edu
only 610 hits, like:
URL:http://csep10.phys.utk.edu/astr161/lect/moon/tidal.html
URL:http://burro.cwru.edu/Academics/Astr221/SolarSys/earthmoon.html
URL:http://www.sunspot.noao.edu/sunspot/pr/answerbook/expl-6.html
> Lots of Greetings!
To you as well.
David A. Smith
.
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