Join us as we explore how NSTA’s three-dimensional resources can be utilized to enhance your teaching. Walk away with effective strategies for science teaching and learning and hear from educators as they provide tips for using these resources.

TAKEAWAYS:
1. Hear from classroom teachers about how they are using NSTA Press publications; and 2. Leave with top-notch teaching tips and innovative lesson plan ideas that promote imaginative learning and student engagement.

SPEAKERS:
Tricia Shelton (NSTA: Arlington, VA), Wendy Binder (NSTA: Arlington, VA)

Dissect the differences between flashy engagers and phenomena to identify essential components of effective phenomenon-based teaching. Critically consider phenomena with personal relevance for your students.

TAKEAWAYS:
1. Build a deeper understanding of the differences between “hooks” and phenomena, 2. Consider and identify the benefits of using contextual, locally inspired phenomena to support all students, and 3. Identify potential local phenomena for their own classrooms to support more inclusive learning

SPEAKERS:
Martha Inouye (University of Wyoming: Laramie, WY), Ana Houseal (University of Wyoming: Laramie, WY)

Explore how to take advantage of NSTA’s vast resources and pathways, including both asynchronous and synchronous options, to create personalized professional learning.

TAKEAWAYS:
1. Discover the value of being a School or District NSTA Partner; 2. Explore how to maximize online professional learning for all teachers; and 3. Discover how to utilize NSTA's online learning resources to support in-person professional learning.

SPEAKERS:
Tricia Shelton (NSTA: Arlington, VA), Wendy Binder (NSTA: Arlington, VA)

Explore NSTA’s NEWProfessional Learning Units. Discover these bite-sized asynchronous professional learning experiences that support student sensemaking to earn credit to submit to your school or district.

TAKEAWAYS:
1. Discover how NSTA can provide asynchronous and bite-sized continuing education credit options (2 hours per PLU); 2. Explore how each PLU contains reflections or tasks connected to the classroom that are submitted to NSTA for review or feedback; and 3. Explore how we can support professional learning for individuals or schools/districts including the flexible options available for Professional Learning Unit topics, and how these fit into our Professional Learning pathways.

SPEAKERS:
Elizabeth Allan (University of Central Oklahoma: Edmond, OK), Tricia Shelton (NSTA: Arlington, VA)

Learning science means engaging in DCIs, SEPs, and CCCs. Come explore how to generate authentic prompts that integrate all three dimensions to drive student learning.

TAKEAWAYS:
1. Practice creating 3-D prompts that explicitly promote the three dimensions and drive more integrated student learning and assessment; 2. Learn how to adapt your own questions and prompts to better target specific dimensions; and 3. Consider how framing of activities, through questions and prompts, can support specific DCIs, SEPs, and CCCs.

SPEAKERS:
Ana Houseal (University of Wyoming: Laramie, WY), Martha Inouye (University of Wyoming: Laramie, WY), Jessica Stephens (Rock Springs Junior High School: Rock Springs, WY)

Come discover a multidisciplinary, open-ended investigation that incorporates absolute and relative dating, anomalies, historical context, volcanoes, solar proton events, energy cycles, Earth systems, terrestrial events, and supernovas.

TAKEAWAYS:
1. Students will have a better understanding of the process of constructing knowledge; 2. Students will have to analyze and defend their results; and 3. Sometimes there is no answer key, only possible solutions from constructing and analyzing data from several sources that cross traditional disciplines.

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

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 providing 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)

Take home an NGSS unit where students test the wave and particle model against phenomena and engage in scientific argumentation, uncovering the nature of light!

TAKEAWAYS:
1. Teachers will walk away with a multi-lesson unit that has students testing the particle and wave model of light against phenomena and engaging in argumentation (including lesson plans, student handouts, and a summative assessment with rubric); 2. The material allows students to investigate multiple wave-like phenomena (e.g. diffraction, interference, polarization) and particle-like phenomena (e.g. Plank’s Blackbody Radiation solution, the photoelectric effect, the Compton Effect, and the Bohr Model) of light; and 3. Teachers will be provided with research-based student argumentation strategies and support materials that encourage students to go beyond “Claim, Evidence, and Reasoning.”

SPEAKERS:
Justin Fournier (Cypress High School: Cypress, CA)