Achtung! Das Lehrangebot ist noch nicht vollständig und wird bis Semesterbeginn laufend ergänzt.
280189 VO+SE Cosmochemistry and meteorites (PI) (2015S)
Prüfungsimmanente Lehrveranstaltung
Labels
An/Abmeldung
Hinweis: Ihr Anmeldezeitpunkt innerhalb der Frist hat keine Auswirkungen auf die Platzvergabe (kein "first come, first served").
- Anmeldung von Di 10.02.2015 00:00 bis Di 24.02.2015 23:59
- Anmeldung von Di 10.03.2015 08:00 bis Fr 20.03.2015 23:59
- Anmeldung von Mi 22.04.2015 08:00 bis Mi 13.05.2015 08:00
- Abmeldung bis Mi 13.05.2015 08:00
Details
max. 20 Teilnehmer*innen
Sprache: Englisch
Lehrende
Termine (iCal) - nächster Termin ist mit N markiert
- Dienstag 14.04. 10:00 - 12:00 Friedrich Becke Seminarraum 2C315 3.OG UZA II
- Mittwoch 15.04. 10:00 - 12:00 Friedrich Becke Seminarraum 2C315 3.OG UZA II
- Donnerstag 16.04. 10:00 - 12:00 Friedrich Becke Seminarraum 2C315 3.OG UZA II
- Dienstag 21.04. 10:00 - 12:00 Friedrich Becke Seminarraum 2C315 3.OG UZA II
- Mittwoch 22.04. 10:00 - 12:00 Friedrich Becke Seminarraum 2C315 3.OG UZA II
- Donnerstag 23.04. 10:00 - 12:00 Friedrich Becke Seminarraum 2C315 3.OG UZA II
- Dienstag 28.04. 10:00 - 12:00 Friedrich Becke Seminarraum 2C315 3.OG UZA II
- Mittwoch 29.04. 10:00 - 12:00 Friedrich Becke Seminarraum 2C315 3.OG UZA II
- Donnerstag 30.04. 10:00 - 12:00 Friedrich Becke Seminarraum 2C315 3.OG UZA II
- Dienstag 05.05. 10:00 - 12:00 Friedrich Becke Seminarraum 2C315 3.OG UZA II
- Mittwoch 06.05. 10:00 - 12:00 Friedrich Becke Seminarraum 2C315 3.OG UZA II
- Donnerstag 07.05. 10:00 - 12:00 Friedrich Becke Seminarraum 2C315 3.OG UZA II
- Dienstag 12.05. 10:00 - 12:00 Friedrich Becke Seminarraum 2C315 3.OG UZA II
- Mittwoch 13.05. 10:00 - 12:00 Friedrich Becke Seminarraum 2C315 3.OG UZA II
Information
Ziele, Inhalte und Methode der Lehrveranstaltung
Art der Leistungskontrolle und erlaubte Hilfsmittel
Mindestanforderungen und Beurteilungsmaßstab
Prüfungsstoff
Literatur
Zuordnung im Vorlesungsverzeichnis
Letzte Änderung: Sa 02.04.2022 00:25
* Overview of Meteorites
* Overview of long and short lived isotope systems. Age of solar system.
* 182Hf-182W system. Key to understanding core segregation?
* Nucleosynthesis and presolar grains
* Early solar system processes
* Oxygen isotopic heterogeneity in the early solar system
* Calcium-aluminum inclusions. Current controversies
* Chemical evolution of asteroidal cores from iron meteorites?
* Late accretion? or not?
* Origin and evolution of the Moon.
* What we may know about Mars from SNC meteorites.
* Meteorite lab.This is a seminar course designed to introduce advanced undergraduate and graduate level students to current theories behind the origin and evolution of our solar system. Many of the topics we will cover are
controversial. Issues we must address include not only the interpretation of chemical and isotopic data, but also the accuracy of data (if two labs measure the same material and get two different answers this may indicate: 1) one or both measurements are wrong, 2) one or both measurements are correct). Students enrolled should have a working knowledge of trace elements and radiogenic isotopes.General topics we will cover include current theories for the origin of the solar system (not the universe), the age of the solar system, and the relative ages of the assemblage of its parts. We will also spend two classes examining extraterrestrial materials (lunar and meteoritic).The structure of the course will normally consist of an introduction of a topic by the instructor, coupled with the assignment of topical readings (historic and recent papers), followed by discussion. Students will also be responsible for keeping up with the readings, and each will periodically be assigned the task of directing discussion the week following the introduction.A review project will be completed by each student by the end of the course. The topic of the project is determined by each student, but must focus on topics germane to cosmochemistry. Both written an oral reports are to be delivered. The purpose of the project is to familiarize the student with some aspect of cosmochemistry not discussed previously in the course, and provide valuable experience in synthesizing, writing and presenting science.