[meteorite-list] Characteristics
From: Joseph Hum <jkarlhum_at_meteoritecentral.com>
Date: Thu Apr 22 09:49:02 2004 Message-ID: <412001902317135860_at_earthlink.net> ------=_NextPart_84815C5ABAF209EF376268C8 Content-type: text/plain; charset=US-ASCII Hi Bernd--All, If by characteristics of solar nebula, she is referring to planetary Noble gases Venus has higher levels that avg... in this neighborhood... Martian meteorites have shown varying degrees of shock levels, that actually helped prove their arrival... this doesn't seem problematic for a Venusian model; again maybe helpful... Bernd, I would like to know, what influence the size of a gravitational field has on the development of mineral crystal growth... it seems to me with the size of some of the crystals in Ueilites, if not related to shock pressures, should indicate a larger gravitational for their formation than could not be provided by a asteroidal body.... And, as I stated before, some of these primitive characteristics that remain, could be the remnant of the impactor, that struck Venus... please keep this in mind. There is the probability of influences from both sources...! Best Wishes! J.K. Hum --- Joseph Hum --- jkarlhum_at_earthlink.net --- EarthLink: It's your Internet. ------=_NextPart_84815C5ABAF209EF376268C8 Content-Type: text/html; charset=US-ASCII <HTML><HEAD> <META content="text/html; charset=windows-1251" http-equiv=Content-Type> <META content="MSHTML 5.00.3211.1700" name=GENERATOR></HEAD> <BODY> <P> <DIV></DIV> <DIV>Hi Bernd--All,</DIV> <DIV> </DIV> <DIV>If by characteristics of solar nebula, she is referring to planetary Noble gases></DIV> <DIV>Venus has higher levels that avg... in this neighborhood... Martian meteorites</DIV> <DIV>have shown varying degrees of shock levels, that actually helped prove their</DIV> <DIV>arrival... this doesn't seem problematic for a Venusian model; again maybe helpful...</DIV> <DIV>Bernd, I would like to know, what influence the size of a gravitational field has on the</DIV> <DIV>development of mineral crystal growth... it seems to me with the size of some of the</DIV> <DIV>crystals in Ueilites, if not related to shock pressures, should indicate a larger gravitational</DIV> <DIV>for their formation than could not be provided by a asteroidal body....</DIV> <DIV>And, as I stated before, some of these primitive characteristics that remain, could be the</DIV> <DIV>remnant of the impactor, that struck Venus... please keep this in mind. There is the probability</DIV> <DIV>of influences from both sources...!</DIV> <DIV> </DIV> <DIV> </DIV> <DIV>Best Wishes!</DIV> <DIV> </DIV> <DIV>J.K. Hum</DIV> <DIV> </DIV> <DIV>--- Joseph Hum</DIV> <DIV>--- <A href="mailto:jkarlhum_at_earthlink.net">jkarlhum@earthlink.net</A></DIV> <DIV>--- EarthLink: It's your Internet.</DIV> <DIV> </DIV> <P></P></BODY></HTML> ------=_NextPart_84815C5ABAF209EF376268C8-- Received on Sun 23 Sep 2001 01:01:35 PM PDT |
 StumbleUpon del.icio.us reddit Yahoo MyWeb
|