Model stellar evolution processes using NASA images,
plotting H-R diagram transitions, and determining the chemistry and physics of
supernovas using NASA STEM image analysis tools.
TAKEAWAYS:
1. Knowledge of the process of how stars form and change over time ending in catastrophic events, providing conditions for the formation of planets; 2. Students will understand that all knowledge of celestial events is determined by analyzing the light from these events and provide possibilities—not definitive answers—as the data can be interpreted differently; and 3. Image analysis software tools allow scientists to gain knowledge of the physical and chemical processes involved to create constantly evolving models of stellar evolution.
SPEAKERS:
Donna Young (NASA/NSO/UoL Program Manager: Laughlin, NV)