|
G446 / G546 Meteorites
Winter Term 2008
MWF 11:30 - 12:35 am, CH 69
A. Ruzicka (+ iron meteorites + muffin)
e-mail: ruzickaa@pdx.edu
Images of two very different meteorites, the Murchison (CM2) chondrite
at left, and the Henbury (IIIAB) iron at right.
Murchison was derived from an asteroid that never melted,
and which was rich in water and organic
materials. These organic materials provide evidence for pre-biotic
synthesis of organic molecules,
which appear to have formed originally in the interstellar medium.
Bright spots in the meteorite are chondrules and refractory inclusions;
fusion crust is the
brown coating at left.
In contrast, Henbury was derived from the core of a melted
asteroid.
The core cooled very slowly (roughly 1 degree C per million years!)
owing to its deep burial in the
parent body. This slow cooling enabled the low-nickel metal
alloy mineral kamacite to exsolve from the
high-nickel metal alloy mineral taenite, producing the intergrowth
pattern (Widmanstatten texture) obvious
in the image.
Course information
-
I have placed a copy of the readings
on 2-hour Reserve in my mailbox in CH17, in case you want to photocopy
this rather going to the library. Please have consideration for your fellow
students and put this packet back in my mailbox when you are done with
it. I'll leave the packet in my mailbox for the next week or so.
(posted 1-8-07)
-
What to focus on in the Bell et
al. (1989) paper: Read but skim the following sections-- Compositional
Meaning of Tholen Space, Collisonal and Dynamical History, Shapes. (posted
1-16-08)
-
The MacPherson et al. (1988) paper
has a lot of detail, with the risk that you will not see the forest for
all of the trees. For example, the authors describe details about
refractory inclusions in different chondrite groups, with the most important
aspect of this being what is similar rather than different. Use the
problem
set as a guide to what you should understand. (posted 1-25-08)
-
Grades have been submitted (see
final scores and grades link below). I will be leaving a box outside
my door that has your graded final exams and the remaining homeworks.
Each person's materials will be contained in a separate packet, so you
need only look for your name to pick up your work. I hope you
had fun in the class (even though you probably were cursing me more than
once while working on the many homeworks) and learned a lot. I hope
to see you in other upcoming classes I teach (e.g., Astrogeology, Geochemistry).
(posted 3-22-08)
Glossary and concepts
Other reference materials
Homework assignments
-
Homework
10 (posted 2-10-08; revised due date 2-13-08).
Due
2/13/08. Due 2/15/08.
-
Homework
11 (posted 2-10-08; revised due date 2-13-08).
Due
2/15/08. Due 2/18/08.
-
Homework
14 (we will be skipping homework 13; posted 2-18-08). Due 2/22.
Score distributions and answer
keys
Last Updated: March 22 2008
|