This work involves trying to understand how there could be diatomic hydrogen detected by the Cassini probe in the plumes arising from Saturn’s moon Enceladus.
Research
Research
Understanding Hydrogen Content of the Enceladus Plume
- UT Austin PI: David Goldstein
- CO-PIs: Philip Varghese, A. Mahieux, L. Trafton
- Funding Source: NASA
- Award: $300K
Submit Grant Details
New ASE/EM faculty grants will be posted after this online form has been completed.
