Planetary Origins and Magnetism in the Inner Solar System

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Event Details
  • Date/Time:
    • Thursday January 10, 2019
      11:00 am - 11:50 am
  • Location: Ford Environmental, Science & Technology (ES&T) Building, Rm. L1205, 11am
  • Phone:
  • URL:
  • Email:
  • Fee(s):
    Free
  • Extras:
Contact

Andrew Newman

Summaries

Summary Sentence: A seminar by Dr. Joseph O'Rourke, School of Earth and Atmospheric Sciences

Full Summary: No summary paragraph submitted.

Media
  • Joseph O'Rourke Joseph O'Rourke
    (image/jpeg)

The School of Earth and Atmospheric Sciences Presents Dr. Joseph O'Rourke, Arizona State University

Vigorous fluid motions drive dynamos today in Earth and all major planets except Mars and Venus. Here, I will show how magnetic histories of rock/metal planets directly depend on conditions during their accretion and differentiation. 

In particular, giant impacts and planetary size and water content are always critical to dynamo energetics. Precipitation of magnesium oxide boosts the likelihood of dynamo activity in Earth and Venus, but hydrogenation of the core of Mars destroyed its dynamo. 

My future plans center on comparative planetology to understand fundamental interior processes that affect planetary atmospheres and surfaces. In parallel with computational geodynamics, I aim to develop spacecraft missions that provide ground truth for my models. To illustrate, I will present my proposed SmallSat mission to (2) Pallas—the largest unexplored protoplanet in the main asteroid belt and parent of many near-Earth asteroids.

Additional Information

In Campus Calendar
Yes
Groups

EAS

Invited Audience
Faculty/Staff, Postdoc, Graduate students, Undergraduate students
Categories
Seminar/Lecture/Colloquium
Keywords
EAS Seminar
Status
  • Created By: nlawson3
  • Workflow Status: Published
  • Created On: Dec 13, 2018 - 11:47am
  • Last Updated: Jan 3, 2019 - 9:38am