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- From: bruce.weaver@nitelog.com (Bruce Weaver)
- Newsgroups: sci.physics
- Subject: HELP Wanted!
- Message-ID: <1788.289.uupcb@nitelog.com>
- Date: 23 Jan 93 19:20:00 GMT
- Reply-To: bruce.weaver@nitelog.com (Bruce Weaver)
- Organization: Nitelog BBS - Monterey, CA - 408-655-1096
- Lines: 43
-
- DTL>From: davidlai@unixg.ubc.ca (David TW Lai)
- DTL>Newsgroups: sci.physics
- DTL>Subject: HELP Wanted!
- DTL>Date: 20 Jan 93 01:33:24 GMT
- DTL>Message-ID: <davidlai.727493604@unixg.ubc.ca>
-
- DTL>Hi netters,
-
- DTL> I'm puzzling around the following questions. If you have some
- DTL>hints to the questions, could you give me some help? Thanks in
- DTL>advance.
-
- DTL>(1) Why are Earth age estimates based on sedmentation and erosion rates
- DTL>so poor?
-
- if you mean total age, because uplift and vulcanism are frequent
- compared to the age of the earth
-
- DTL>(2) A rock specimen contains precisely ten times less potassium-40 than
- DTL>its radioactive decay product (half-life 1.3 billion years) argon-40. How
- DTL>old is this rock and where did it come from?
-
- DTL>(3) Give four reasons, in order of important, why the
- DTL>Earth appears to have fewer huge impact scars than
- DTL>The Moon.
-
- One answer dominates: because uplift and vulcanism are frequent compared
- to the age of the earth. From the geologist's point of view, the
- surface of the earth is like a bubbling cauldron. Finding craters on
- the earth is hard and they are all (relatively) young. The moon, on the
- other hand, is relatively inactive. It did have a major melting event
- (hence, the lunar maria on which are relatively few craters). Also, the
- garbage is swept up with time so that the impact rate will decay with
- time from formation. This accentuates the cratering difference between
- the two planets (pop quiz: is the orbit of the moon ever convex towards
- the sun ? )
-
- DTL> Thanks a lot!
-
- DTL>David.
- ---
- . SLMR 2.1a . Physics is a subset of astronomy
-
-