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Study mode:
on
1
Intro
2
Stellar system formation
3
Meteoritic building blocks
4
Water as a proxy?
5
Another approach: isotopic anomalies
6
Molybdenum (Mo)
7
Samples & Methods
8
Basaltic achondrites
9
Problem 1: No Molybdenum
10
Neodymium (Nd)
11
Problem 3: Irradiation & neutron capture
12
Results
13
Spatial vs. temporal?
14
Two non-exclusive scenarios
15
Integrated isotope data
Description:
Save Big on Coursera Plus. 7,000+ courses at $160 off. Limited Time Only! Grab it Explore the formation of our solar system in this 52-minute colloquium talk by Dr. Jan Render from Lawrence Livermore National Laboratory. Delve into stellar system formation, meteoritic building blocks, and the role of water as a proxy. Examine innovative approaches using isotopic anomalies, focusing on Molybdenum (Mo) and Neodymium (Nd). Investigate challenges in studying basaltic achondrites, including the absence of Molybdenum and issues with irradiation and neutron capture. Analyze the results to understand spatial versus temporal aspects of early solar system development. Consider two non-exclusive scenarios and integrate isotope data to reconstruct the conditions and processes that shaped our cosmic neighborhood billions of years ago.

Reconstructing the Early Solar System

Rutgers Climate & Energy Institute
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