(meteorobs) Correction to previous Trig.calculation.
Chris Peterson
clp at alumni.caltech.edu
Wed Sep 19 11:49:18 EDT 2007
Larry-
We don't see meteors cooling down all that much. What we see when they
get dimmer is less material ablating (because most has already been
lost). The tail of the light curve in this case isn't at all unusual. In
fact, it is what the majority of meteors look like at the end of their
run. I'll track down a few examples from my database and post links
later today.
Chris
*****************************************
Chris L Peterson
Cloudbait Observatory
http://www.cloudbait.com
----- Original Message -----
From: <stange34 at sbcglobal.net>
To: "Global Meteor Observing Forum" <meteorobs at meteorobs.org>
Sent: Wednesday, September 19, 2007 9:38 AM
Subject: Re: (meteorobs) Correction to previous Trig.calculation.
> If I can chip in here, arguably Chri's substantial background &
> knowledge forming his conclusion is most likely what happened with
> this meteor.
>
> I can only cite the unusual (post-time) persistance of the meteor and
> secondly, without an abrupt velocity change, I cannot envision any way
> to distinguish a meteor cooling down from one that is slowly burning
> up on a camera image.
>
> I am on a weak limb here and acknowlege it, but hope to learn from
> this event.
>
> Larry
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