[meteorite-list] iron meteorite cooling rates and Meteorite Men
Arlene Schlazer
piebear at cox.net
Wed Dec 15 13:31:26 EST 2010
Thank you Dr. Rubin for that explanation. As a collector of mostly iron
meteorites, I've always been fascinated with the various types of etch
patterns. My question is, how many years does it take to cool per degree in
the vacuum of space? Secondly, what determines the structure from fine to
course.....is it just the nickel content or does the cooling rate have
anything to do with it? Thanks in advance.......Arlene
----- Original Message -----
From: "Alan Rubin" <aerubin at ucla.edu>
To: <meteorite-list at meteoritecentral.com>
Sent: Wednesday, December 15, 2010 9:54 AM
Subject: [meteorite-list] iron meteorite cooling rates and Meteorite Men
On last night's Meteorite Men show, the narrator was attempting to explain
that the Widmanstatten pattern is caused by kamacite and taenite cooling at
different rates. This is incorrect. How could two intergrown metal grains
buried deep inside a core cool at different rates? The Widmanstatten
pattern forms in the following manner:
(1) At high temperatures (but below the solidus), metallic Fe-Ni exists as a
single phase -- taenite. (2) As the metal cools, it eventually reaches the
two-phase field (or solvus) on the phase diagram. For metal containing 90%
iron and 10% nickel, it reaches this boundary when temperatures cool to
about 700ºC.
(3) At this point, small kamacite grains nucleate inside the taenite. With
continued cooling, the kamacite grains grow larger at the expense of
taenite, but both phases become richer in nickel. This is possible because
the low-Ni phase (kamacite) is becoming increasingly abundant.
(4) At low temperatures, say <400ºC or so, diffusion becomes so sluggish
that the reaction essentially stops.
These meteorites are called octohedrites because solids have
three-dimensional structures and the kamacite planes are oriented with
respect to each other in the same way as the faces of a regular octahedron.
Alan Rubin
Institute of Geophysics and Planetary Physics
University of California
3845 Slichter Hall
603 Charles Young Dr. E
Los Angeles, CA 90095-1567
phone: 310-825-3202
e-mail: aerubin at ucla.edu
website: http://cosmochemists.igpp.ucla.edu/Rubin.html
______________________________________________
Visit the Archives at
http://www.meteoritecentral.com/mailing-list-archives.html
Meteorite-list mailing list
Meteorite-list at meteoritecentral.com
http://six.pairlist.net/mailman/listinfo/meteorite-list
More information about the Meteorite-list
mailing list