Learn how ungrading works in a science classroom as feedback and reflection replace points to increase student autonomy and connection to learning.

TAKEAWAYS:
1. Connect deep 3-D learning with the tenets of ungrading to see how they work together; 2. Explore concrete ways of tracking student progress and feedback while devaluing points and centering learning; and 3. Leave with access to resources that support ungrading in STEM classrooms.

SPEAKERS:
Johanna Brown (Washington State OSPI)

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 detailed information of stellar physical and chemical processes and constantly refine our evolving models of stellar evolution.

SPEAKERS:
Donna Young (NASA/NSO/UoL Program Manager: Laughlin, NV)