To analyze data from space and ground-based telescopes, scientists rely on computers, not only to do calculations, but also to change numbers into images. Scientists and programmers go through painstaking calibration and validation processes to ensure that computers produce technically correct images. Visual representation of X-ray data, and radio, infrared, ultraviolet, visible, and gamma, involves the use of representative color techniques where colors in the image represent intensity, energy, temperature, or another property of the radiation. This activity creates models from numerical data. Each model will be unique, depending upon how the photon intensity and energy data was processed – binned and assigned color values – and then analyzed. Artistic representations of this data will be made "by hand" and also by using web-based js9 imaging and analysis software. This is one step in allowing students to do their own astronomy research using real data sets.

TAKEAWAYS:
Scientists learn about astronomical objects from the light they produce. Colors in images are based on data from this light and are used to highlight different features.

SPEAKERS:
Pamela Perry (Lewiston High School: Lewiston, ME)

An extension of our previous NASA/JWST ambassador and NSTA workshops, this session empowers educators with deeper understanding of orbiting observatories and provides an inherently engaging hands-on activity which works from pure STEM/STEAM fun to serious exploration of multi-wavelength astronomy. We provide gel filters that participants use with their phones to capture monochrome images at three wavelengths (630nm, 530nm & 470nm for red, green and blue). Participants then open their images in a free, browser-based image processing app to combine them into a "color" picture. This locks in an understanding of how "color" results from image processing. Then, participants choose NASA image files from an archive and repeat the process -- only now, they are assigning RG&B to wavelengths that are not actually visible to the eye. The tool we use includes both presets to make this fun as an introductory activity, and an array of math-driven functionality for deep dives into image processing.

TAKEAWAYS:
Teachers will learn to process multi-wavelength image sets to create color images from space telescopes and your own devices. This leads to a deeper understanding of space-based astronomy and how space telescope images are made – and provides a classroom activity that is fun, rich, and economical.

SPEAKERS:
Donna Kaiser (Stamford High School: Stamford, CT), Vincent Urbanowski (Academy of Information Technology & Engineering: Stamford, CT)

This lesson focuses on radio astronomy data collected with a $50 student-built telescope. The telescope is not needed to do the lesson. Students collect information on the locations of neutral hydrogen. Easy to do and a primary focus of radio astronomy. The data collected can be used in the classroom to teach lessons on the Doppler Effect, Wave behavior, galactic velocity curves, and effects of gravity as well as other science topics. Many physics concepts can be taught in a highly engaging way by studying the concepts found in astronomy. Doppler effect, rotational motion, wave behavior, the EM spectrum are examples. The challenges to doing such lessons is the high cost of the telescopes and the challenges of collecting astronomy data during daylight hours. Plans for building and operating the radio telescope will be provided. Lesson plans for teaching the Doppler Effect via Red Shift/Blue Shift and for teaching how to work with galactic velocity curves will be included.

TAKEAWAYS:
Radio astronomy is done during class time as radio wave detection is not affected by daylight. Students will learn about the unique nature of galactic rotational behavior as compared to circular motion and planetary motion under Kepler’s Laws.

SPEAKERS:
John Clark (Volusia Online Learning: Port Orange, FL)

Participants will use light curve graphs and image analysis software tools located on the web to investigate stellar objects at the centers of supernova remnants, and determine if the objects are white dwarfs or neutron stars. Two sets of data from the Chandra X-Ray public archive will be used to plot brightness versus time to determine the rate of rotation of the object. Centripetal acceleration and Newton's Universal Law of gravitation calculations will then be applied. This activity is designed for physics and/or astronomy classes and integrates STEM analysis tools with the crosscutting concepts, physical science core disciplinary content and engineering concepts embodied by NGSS. Students may also use tools learned in this activity to use js9 to do further research projects using publicly available astronomy data sets.

TAKEAWAYS:
Light curves generated from web-based js9 image analysis software can be used to determine the period of rotation and identify objects as white dwarfs or pulsars using Newton’s Universal Law of gravitation and centripetal acceleration calculations.

SPEAKERS:
Pamela Perry (Lewiston High School: Lewiston, ME)

The National Oceanic and Atmospheric Administration (NOAA) collects hundreds of terabytes of data daily from satellites, buoys, weather stations, animal tags, and more. Though that may sound intimidating, much of this data is readily available to teachers and can be used in the classroom to teach about our natural world. Using scientific data in the classroom can be a great way for teachers to motivate students and for students to learn inquiry-based methods using real-world data. This presentation will highlight many of NOAA’s standards-supported resources, how to access them, and strategies for using them in the classroom. NOAA data spans Earth, life, and physical sciences, and comes in a variety of formats ranging from raw unprocessed real-time measurements and satellite images to processed visualizations, graphs, charts, and animations. Many resources are ready-to-go so you can bring data into your classroom tomorrow!

TAKEAWAYS:
What types of data are available from NOAA and how to find and use NOAA data in your classroom.

SPEAKERS:
Kayla Smith (National Oceanic and Atmospheric Administration: Silver Spring, MD)

Working in teams, students take a short analog message and convert it to binary code for cell phone transmission. Students then send those zero’s and one over a carrier wave using a form of amplitude modulation to another team. At the other end the message is decoded and rewritten in analog form. which message was first? How close was it? A discussion of challenges the students’ faced in acting like a DSP (digital signal processor) lets student see some of the challenges of the original binary code and how subsequent forms of coding came about to address some of those challenges. Students discover the binary code they used was Morse code. Students then code and send a different message using the original 5-digit computer code. After racing to send their messages, students are guided through a follow-up discussion on the pros and cons of the new (Baudot) computer code used.

TAKEAWAYS:
Students will understand some of the challenges faced in digital signal processing as sending digital information evolved by completing a lab activity where they will code and decode messages into a digital format for transmission and receiving, similar to how cell phones work.

SPEAKERS:
John Clark (Volusia Online Learning: Port Orange, FL)

Crosscutting Concepts, the links between different science disciplines, can be challenging to use as an anchoring storyline activity. However, it can be one of the best ways to engage students, as they can make personal connections between different domains. Teachers will begin by becoming familiar with the NGSS Appendix G Systems and System Models progression, identifying essential learning by grade. Then, they will investigate how this CCC has been built into a storyline anchor, extending this concept from the initial activity (involving video games) into a different aspect of science–climate modeling. Teachers leave prepared to utilize this storyline in the classroom. Upon completion, students will be able to identify the factors used in climate models and create a model that depicts the flow of energy/matter in a climate system. They will also be able to express the reliability and validity of climate models. Resources: https://ncse.ngo/supporting-teachers/classroom-resources

TAKEAWAYS:
Participants will walk away with a better understanding of how to use the Systems and Systems Modeling Crosscutting Concept to help students analyze the precision and reliability limitations of past and present climate models, dispelling major misconceptions about climate science along the way.

SPEAKERS:
Blake Touchet (National Center for Science Education: Oakland, CA), Michael Lowry (McCallie School: Chattanooga, TN), Lin Andrews (National Center for Science Education: Oakland, CA)

Since the beginning of the COVID pandemic, teachers have had to restructure how they teach. When schools closed, teachers were given multiple options and had to pick one. Many schools chose the Google Classroom option as it was the easiest for some schools to set up, but didn't allow for inclusivity with every student both in and out of the room. Using examples from my own Chemistry and fully virtual Applied Digital Skills classes, I will show how Microsoft Teams can give both the teachers and students a hub for all their presentations, notes, assignments, and even assessments. It allows teachers the ability to grade assignments and for students and parents to see those grades within the platform. It also allows for teachers to keep track of students' mental health and insights that can be shared with parents or councilors about students' habits on their computer. This may not be a science specific topic, but it works so well for managing a science classroom.

TAKEAWAYS:
Attendees will know how to use Microsoft Teams to host virtual lessons, create postings students can read and interact with, create and grade assignments, and how to check in with the emotional needs of students.

SPEAKERS:
Jill Elder (Assumption High School: Louisville, KY)

Presentational content will include a high level overview of NASA’s Great Observatories and other past and present orbiting telescopes, how their missions are coordinated, and how they work in concert to provide full spectrum data from across the sky in bands from gamma down to far infrared – almost all of which are invisible to the human eye. In the workshop portion, participants will access archived astronomical data from orbiting observatories using the same browser based tools used by astronomers. They will process their datasets using a variety of tools and techniques for reducing data, vetting objects, and generating results, such as Spectral Energy Distribution, Color-Color and Color-Magnitude plots. Teachers will bring this experience back to their classrooms adding depth of knowledge to astronomy content they may teach, as well as a deeper understanding of the conduct of science research.

TAKEAWAYS:
Attendees will learn to access astronomical data such as monochrome images at various wavelengths and wavelength magnitude measurements for thousands of stars at a time just as professional astronomers do, and how to process such data for research using techniques of professional astronomy.

SPEAKERS:
Donna Kaiser (Stamford High School: Stamford, CT), Vincent Urbanowski (Academy of Information Technology & Engineering: Stamford, CT)

My first years of teaching Physics at Title 1 schools in Memphis were challenging. Many of my students were very behind, especially in math. However, I developed 5 strategies to make learning physics accessible and they completely transformed my classroom. 1. “Building Block” Method The biggest breakthrough in my classroom was breaking long problems down into building blocks. I will show how to do this with a sample forces unit. 2. Pre-manipulated equations I will share an equation sheet that shows all forms of each equation. It is a game-changer for students who struggle with algebra. 3. Setting-Up for Success I will model a consistent way to help students stay organized on different types of problems. 4. Simplifying Motion I will illustrate how to solve motion problems using simpler notation and simpler equations. 5. Simplifying Circuits I will show how to use the “routes method” so students can solve most circuits in a more conceptual way.

TAKEAWAYS:
Teachers will come away from this session with strategies that they can immediately implement in their classrooms to make physics more accessible and engaging, especially for their lower-level learners.

SPEAKERS:
Jack Replinger (FormerTeacher / Founder: , WA)

Case Studies are stories with an educational message. Learn how case studies engage learners, develop critical thinking, and enhance collaborative and communication skills. You will experience a case and try to solve a real-world mystery of a woman who was told she was not her children’s mother.

TAKEAWAYS:
Participants will experience a case study as learners, reflect on the experience and on the pedagogical potential, and discuss ways to use the technique effectively. They will explore NSTA’s collection of almost 1000 freely accessible case studies in all STEM disciplines.

SPEAKERS:
Annie Prud'homme-Généreux (University of British Columbia: No City, No State)

NEED’s Exploring Marine Hydrokinetics (MHK) is an exploratory unit for secondary students that includes teacher and student guides containing comprehensive background information on energy, the properties of fluids and waves, electricity, hydrokinetic technologies, and careers in the emerging industry of MHK. Participants will have the opportunity to apply the science of the oceans and electricity generation as they learn about the many types of MHK technology, explore case studies, consider siting a project, and build their own sample wave generator model. The curriculum is available for free and includes hands-on, inquiry-based explorations, group presentations, and cooperative learning activities.

TAKEAWAYS:
The energy of moving water can be harnessed and converted into electricity in many ways, including technologies for harnessing the energy in ocean tides, waves, and currents. Participants will learn activities for students that explore these concepts and best practices for implementing.

SPEAKERS:
Don Pruett, Jr. (Washington Science Teachers Association: Everett, WA)

The Next Generation Science Standards promote students doing science. Being able to assess them while they are engaged in the "doing" is essential. Attendees will take a deep dive into the SEPs and learn how to create rubrics that they can use to assess the SEPs while walking around and observing students as they work. The result? Higher student engagement and less papers to grade. This session is led by Dr. Carol Baker, NGSS Writer.

TAKEAWAYS:
Attendees will create a rubric that can be used in their classroom to authentically assess the SEPs.

SPEAKERS:
Carol Baker (NGSS: Orland Park, IL)

The Stan-X network is a world-wide partnership of public and private schools that work together to provide research-based learning experiences for students (https://stan-x.org). Through collaboration with the research group led by Dr. Seung Kim at Stanford University, the schools have adopted a fruit fly-based program that provides opportunities for authentic research that generates high-quality data and resources impacting the community of science. Stan-X program elements can fit flexibly into almost any science curriculum at middle or high school grade levels. In our session, we will detail the development and growth of our program and describe examples of courses that have been developed in schools in the U.S. and abroad. We will also describe how Stan-X works with schools to fund program creation and develop instructor skills for guiding students through authentic, open-ended research, while developing sufficient autonomy to modify or expand research-based science teaching.

TAKEAWAYS:
Through Stan-X, middle school and high school students learn science through authentic, open-ended, publishable research. Coordination between schools, both public and private, across the world can enhance scientific learning and research opportunities for your students and for teachers!

SPEAKERS:
Nicole Lantz (The Lawrenceville School: Lawrenceville, NJ)

Most students in Missouri only take physical and life sciences to graduate leaving the Earth & Space Science strands of NGSS untouched. Most educators, additionally, do not have a strong enough earth & space science background to integrate these strands into their science classes. However, most of these Earth and Science strands can easily be adapted into a high school chemistry class (and biology, although my background is in chemistry) without having to give up core content. In this presentation, educators will be do a wet lab (Cleaning Up an Ocean Oil Spill) and receive access to additional labs (precipitation lab, acid rain lab, and viscosity of volcanoes) that meet the basic general chemistry class standards (PS NGSS strands) and incorporate earth and space sciences. Attendees will also learn of additional resources such as Gizmos and NASA that can be incorporated and hit the ESS science standards. Lastly, attendees will learn of books and resources for them to learn more.

TAKEAWAYS:
Learn how to integrate the Earth & Space standards into a basic chemistry high school class. Resources can be adapted for biology and middle school levels.

SPEAKERS:
Stephanie Coyle (Jefferson Middle School: Columbia, MO)

Case studies are stories with an educational message that capture & hold students’ attention. Cases come in all shapes/sizes for small/large classes. They include intimate debate, clicker, discussion, Problem-Based Learning, and jigsaw. Learn how to pick the most appropriate one for your class.

TAKEAWAYS:
Educators will leave the workshop with a better understanding of several case study formats and will be able to choose the best one for their purpose. They will also discuss strategies for facilitating each one most effectively. The NSTA case collection has almost 1,000 selections.

SPEAKERS:
Annie Prud'homme-Généreux (University of British Columbia: No City, No State)

I will take participants through my process of crafting sets of formative multiple choice questions that each use 2 of the 3 dimensions of NGSS, so that all dimensions are addressed. I will also show my process for refining free response questions to get the exact responses I am looking for and that allow for an ease of grading and seeing students’ understanding. I will provide examples from my own classroom & direct them to where they can find more examples from various storylines. As an iHub Chemistry writer, I learned to write 3-D multiple choice formative questions. An assessment graduate course taught me how to write quality distractors to see limits of student understanding and get useful feedback data. I merge these 2 in my own classroom to create assessments to get to what my students know. I will share my learning from these trainings and more to set teachers on the path to quality 3-D classroom assessments.

TAKEAWAYS:
Learn to craft three-dimensional assessments, multiple choice, and free response. Using quality distractors in multiple choice formatives allows you to pinpoint student misconceptions. Free response questions direct students to the specific response you want so that grading goes quicker.

SPEAKERS:
Sarah Evans (Olathe South High School: Olathe, KS)

Stars form in clouds of gas and dust in star formation regions, and follow sequences that end in their destruction. Plotting their changing physical properties on the H-R diagram shows their evolutionary progress. Plotting light curves on the H-D diagram determines instability regions as stars transition to the next stage. Stellar evolution provides the energy which drives the universe and determines its future. Nucleosynthesis creates the elements which will enrich the next generation of protostars and planets. The resources developed by UoL are a progression from understanding astronomical images to plotting stellar transitions through instability strips on the H-R diagram, to analyzing observational data with the same JS9 tools that scientists use to determine everything from the chemical composition of supernovas to determining whether a stellar core is a white dwarf or a neutron star. The JS9 investigations include links to the original research papers and archived data sets.

TAKEAWAYS:
All our knowledge of stars and galaxies is determined by spectroscopy -- the analysis of radiation emissions, including radio, infrared, optical, ultraviolet, gamma, and X-ray. Knowledge of spectroscopy is essential to understanding the processes producing the individual wavelengths.

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

SPIN, a FREE web-based notebook created with funding by NSF, has three customizable lessons for data-focused investigations in Earth Science on Sunspots, Tides, and Hurricanes. Teachers can also input their own lessons into SPIN. One of the teachers who created the lessons in the notebook will be presenting. The first 30 minutes presenters will give teachers accounts in SPIN and show how students can use the notebook and the metacognitive support features such as the Communication Hub, I’m Stuck button, and SPAARC prompts. Experiences of teachers and students who have used SPIN will be discussed. In the final 30 minutes, teachers will customize a lesson in SPIN or input their own lessons with help from the presenters. By the end of the session, teachers will be able to use SPIN effectively with the ability to share the notebook with all of the teachers at their school. Use of SPIN is free and is found at https://spin.cehd.gmu.edu/login. Biology, chemistry, and physics also available.

TAKEAWAYS:
Teachers will learn how to use SPIN to download and edit a lesson from the Global Marketplace or create their own lesson in SPIN. Teachers who have used SPIN note that it has helped their students understand data practices explicitly.

SPEAKERS:
Kevin Cabaniss (Teacher, Science), Erin Peters-Burton (George Mason University: Fairfax, VA)

STEM SAIL Ohio project team members will share how this grant-funded work is supporting science education in Ohio through focused regional partnerships. The discussion will include topics like: The Appalachian STEM Collaborative, a STEM Ecosystem that serves some of Ohio’s neediest students and has demonstrated exceptional growth in the wake of COVID-19. The DreamSTEM Educator Summer Externship Program, where teachers participate in business and industry activities and learn how those roles connect with their own content area. “STEM Stories” of teachers like Mark, a computer science teacher at an Ohio high school whose Game Design students are developing job training simulations for a local factory. Participants will see the immense value of cross-sector collaboration to advance classroom and workforce connections in STEM fields. They will be inspired to seek professional and industry connections to strengthen the classroom-workforce pipeline in their own schools and communities.

TAKEAWAYS:
Participants will learn about the STEM SAIL Ohio project from the perspective of program designers, STEM ecosystem partners, and Ohio educators. They will hear examples of activities designed to support teachers and student success, and will be encouraged to connect with their nearest STEM ecosystem.

SPEAKERS:
Sadie Norwick (TIES: No City, No State), Christa Krohn (Director of Learning Systems: , OH)

Participants will use web-based image and data analysis software and real data sets to compare the Cartwheel Galaxy in optical and X-ray bands to determine the sources of the ultra and hyperluminous X-rays in the galaxy. This investigation can be done on smart phones, laptops, and tablets with an internet connection. The unusual shape of the Cartwheel Galaxy is most probably the result of a collision with one of the smaller nearby galaxies several hundred years ago. The collision produced compression waves within the galaxy which triggered bursts of massive star formation. Participants will use the location of the U/HLXs on the x-ray image and optical image, as well as information about expansion rates and the life cycles of stars to determine what these objects might be. This is a great introduction to the software that astrophysicists use. Participants will also learn about the possibilities for other kinds of investigations and research with the software and the thousands of available data sets.

TAKEAWAYS:
Astrophysicists use light in all bands of the electromagnetic spectrum to determine the nature of an object. Web-based software will be used; the same tools used by scientists. This software can be used by students to do their own investigations in astronomy with real data sets.

SPEAKERS:
Pamela Perry (Lewiston High School: Lewiston, ME)

Rubin Observatory is a public US observatory funded by the NSF. Educational materials and services are freely available to all. “Coloring the Universe” is one of six free online investigations that offer a complete, classroom ready lesson. Designed to support the NGSS, it comes with a phenomenon, teacher guide, presentation slides, videos, and a variety of three-dimensional formative and summative assessments and scoring guides. Since the entire lesson cannot be completed in 60 minutes, we will adopt a drop in approach at various places of the phenomenon and online app, and role-playing from the student perspective.We will then visit the website to preview additional resources. This workshop will also model how the lesson can be incorporated in Earth-Space or Physics storylines, and will demonstrate formative assessment and inclusive learning techniques.

TAKEAWAYS:
Participants will learn how to use the free interactive Coloring the Universe online investigation and support materials designed for NGSS teaching and learning, as well as active learning and assessment strategies that support inclusive techniques for building student communication skills.

SPEAKERS:
Ardis Herrold (Vera C. Rubin Observatory: Tucson, AZ)

As science educators, we often ask our students to make sense of phenomena that have a direct impact on human life such as hurricanes, floods, or wildfires. During this session, participants will explore free online modules which contain uncertainty-infused argumentation sets and interactive models that allow students to explore these events. Students’ work samples will be examined to see how their capacity for developing scientific arguments grows as they learn more about natural hazards. These samples include making claims from evidence, writing explanations that support their claims, and discussing the uncertainty of their explanations. The uncertainty discussions also include students’ evaluations of the models and data presented. This session is designed to introduce you to the modules and demonstrate how using them can strengthen your teaching and deepen student understanding of natural hazards through modeling and argumentation.

TAKEAWAYS:
Participants will explore a series of simulations designed to deepen students’ understanding of natural hazards. They will create a free account to access these simulations and associated curricula. An emphasis on the practices of modeling and argumentation will be used as part of the sensemaking process.

SPEAKERS:
Stephanie Harmon (PIMSER (KY): No City, No State)

Stars form in giant molecular clouds of gas and dust in massive star formation complexes, and depending on their initial mass, usually follow a sequence that ends in their destruction in catastrophic collapses and explosions. The process of stellar evolution provides the energy which drives the universe, and thereby determines its future. During the last stages of evolution, nucleosynthesis creates the elements which will enrich the next generation of protostars and planets. formation of stars also sets the stage for possible exoplanets forming within the debris disks of young protostars as hydrogen begins to fuse in their cores. This basic sequencing activity is one of a series of activities designed to show how scientists view, study, and examine the process of stellar evolution. The card sets have descriptions and links and can be used as a pretest or a posttest, either individually or as a group. Multiple answers are acceptable. A scoring rubric is included.

TAKEAWAYS:
Stellar evolution is a cosmic cycle from the formation of protostars and stars in cold molecular clouds, through their final collapses into remnants and stellar cores. This process creates heavier elements and sets the stage for the formation of exoplanets and the next generation of star formation.

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

Changing global and local climates have perceptible impacts on communities, so teachers need to be able to develop lessons based on reliable date and research-based reports that their students can access and analyze to inform future decision-making. In this session, I will share some examples of use.

TAKEAWAYS:
Available climate data exists to be used in developing lesson plans to guide student decision-making.

SPEAKERS:
Michael Passow (Dwight Morrow HS (retd): Englewood, NJ)

This is a full tour of an astronomy research project done through NITARP (NASA Infrared Teachers Archive Research Program), which pairs Caltech astronomers with STEM teachers for authentic research using data from various observatories. The project presented here is a search for Young Stellar Objects (YSOs) in IC417 (the “Spider and Fly”) nebula. We’ll share how candidate objects were found, how object lists were generated and downloaded, how objects were identified and confidence values assigned. We’ll share how to make and interpret color-color plots, color-magnitude plots, spectral energy distribution plots and more. Most importantly, we’ll share how the astrophysics of star formation reveals itself in spectral data. And how confounding factors, such as dust in the interstellar medium, also show up in the data and can be compensated for. By attending this presentation, educators will be able to share a truer picture of the work of astronomers with their students.

TAKEAWAYS:
The participants will step through an entire astronomical research project from inception through data gathering, data vetting and processing, results, and publication. This will deepen the participant’s understanding of research and equip them to bring astronomical research to their school.

SPEAKERS:
Donna Kaiser (Stamford High School: Stamford, CT), Vincent Urbanowski (Academy of Information Technology & Engineering: Stamford, CT)

Participants in this workshop will use a temperature sensor/probe to measure the temperature of a liquid. They will then design and code a program that will display the temperature and also incorporate other multi-sensory devices to indicate if the liquid is safe for drinking. This workshop will allow participants to go through the engineering design process and create a working model by the end of the session. No prior coding knowledge is required, just a willingness to create, learn, and have fun doing it.

TAKEAWAYS:
Create a multi-sensory temperature detector. Implement coding in Python into the STEM/Science/Mathematics classroom. Learn how to give students ownership in their projects.

SPEAKERS:
Jessica Kohout (Educational Consultant: Voorhees, NJ), Brad Posnanski (Comsewogue High School: Port Jefferson Station, NY)

Since the first interplanetary probes were launched, the data that have been returned by these probes have been both fascinating in the insight they have returned, but daunting in their sheer volume, making their use by classroom teachers limited. Yet engagement with planetary phenomena rarely cease to generate “wows” among students. A free software package, JMARS, allows GIS-based imagery and chemical data for planetary bodies to be accessed to address the questions of classroom-based investigations. This presentation will show how JMARS, coupled with the broad range of Mars rover photography (Spirit, Opportunity, Curiosity, and Perseverance) available online, can be used to design virtual field trips on Mars, and mesh with the NSTA Sensemaking framework by generating student questions about another planet, as if they were standing on it themselves. Attendees are encouraged to bring a laptop device and download the software appropriate to their computer at https://jmars.asu.edu/.

TAKEAWAYS:
Space exploration seems to be an abstract concept to many students, so placing them as close as possible to the available data, including not just images but chemical and physical information as well, allows them to gain a deeper understanding of Earth phenomena and processes.

SPEAKERS:
Eric Pyle (James Madison University: Harrisonburg, VA)

Rubin Observatory is a public US observatory funded by the NSF. Educational materials and services are freely available to all. “Expanding Universe” is one of six free online investigations that offer a complete, classroom ready lesson. Designed to support the NGSS, it comes with a phenomenon, teacher guide, presentation slides, videos, and a variety of three-dimensional formative and summative assessments and scoring guides. This workshop will model scaffolded teaching and assessment techniques to help students achieve success in making sense of abstract concepts presented in the lesson. Since the entire lesson cannot be completed in 60 minutes, we will adopt a drop in approach at various points by using portions of the phenomenon and the online app, and role-playing from the student perspective. We will then visit the website to preview additional resources.

TAKEAWAYS:
Participants will learn how to use the free interactive Expanding Universe online investigation and support materials designed for NGSS teaching and learning, as well as scaffolded teaching, and as formative assessment strategies to ensure that all students may achieve a successful learning experience.

SPEAKERS:
Ardis Herrold (Vera C. Rubin Observatory: Tucson, AZ)

Activity – Minerals needed to power an electric vehicle and where they are mined 1. Discussion on some of the critical minerals for the green economy & how/where they are mined and provide resources to teachers to assist them in presenting this information: • Jobs of Tomorrow Video Series (https://media.smenet.org) • Minerals Education Coalition website • Educational activities and MEC Mineral Baby (minerals needed in a lifetime) and MEC Minerals Needed Each Year graphics • USGS listing of where minerals are mined (USGS Commodities Summaries) 2. Discussion on the wide array of exciting work available in the minerals industry and related resources including: a. Minerals Education Coalition website free resources about careers, including handouts, activities, videos and PowerPoints, and b. MEC new career-themed activities and new publication of information about related careers. Careers to be discussed include: • Mining Engineer • Geological Engineer • Metallurgist • Geologist

TAKEAWAYS:
Innovation, artificial intelligence, and technology are all modern mining and minerals industry hallmarks. One of the safest and most lucrative engineering careers today; mining professionals solve problems from project management to meeting mineral demands.

SPEAKERS:
C. Dale Elifrits (Northern Kentucky University: Highland Heights, KY)

During our district's "austerity" years (around 2008) our supply budget was slashed and has not returned. Our Biology team developed low-cost wet-lab experiences for students to develop skills in experimental design, long-term data collection, graphing, and writing scientifically. These activities are used in our honors and regular biology courses. Check out one of our experiences- (sample of a whiteboard and a class set of the algae lab in our Biofuel Unit.) https://drive.google.com/file/d/1XMpQ5SsBw0YgU9frO2L4lKwv-L38BkQg/view?usp=sharing Students were tasked with maximizing algae growth over two weeks, measuring with turbidity, and then analyzing their protocol compared to the class. You can see not all were successful which leads to rich conversations.

TAKEAWAYS:
Bring home six low-cost, highly engaging lab experiences that can be supported with a minimal financial cost!

SPEAKERS:
Jacqueline Svetich (Science Teacher: Naperville, IL), Adrianne Toomey (Neuqua Valley High School: Naperville, IL)

We’re all passionate about science, and part of that passion stems from the fact that no other discipline is exploring the entire physical universe and making sense of our world. No other discipline can make predictions as accurately as science can! It’s so powerful and engaging that some misunderstand it and use it for purposes it isn't intended to be used for. Some even manipulate our students’ misunderstandings of what science is, creating enough confusion that our students believe in junk science, disinformation, or even deny science! As science educators, we sometimes get distracted by all the minutia on our plates and do not directly incorporate the NGSS Appendix H: Understanding the Scientific Enterprise in our work. Students find joy in “debunking” bad science and become future citizens who can sniff out scientific misinformation. We'll enhance activities with the scientific thinking that is developed from a deeper understanding of the nature of science.

TAKEAWAYS:
Become familiar with NGSS Appendix H and use it to enhance your classroom activities to develop sensemaking skills that help your students to identify logical fallacies and misinformation that are used in sloppy science, disinformation, and science denial in their everyday experiences.

SPEAKERS:
Ericca Thornhill (Mizzou Academy: Columbia, MO)

The presentation will cover the basics of high-altitude ballooning as done at Fort Hays State University. Attendees will be introduced to the FHSU website that we use with school groups who contact us to help with their launch. These cover physics and chemistry involved in launching a balloon, the FAA rules, where to find materials, tracking and recovery systems, designing an experiment, and processing data. We will also introduce the teachers to the technology that can be flown to collect data which includes cameras, data loggers, and how to make and code data collection devices with Arduinos. The presentation will include information about NASA resources on high altitude ballooning. We will also share the high school curriculum developed by Shepherd-Adams that she uses in her classroom for an aeronautics CTE course. Examples of student projects and presentations will be presented. The project aligns with NGSS standards related to engineering, earth and space science, as well as physi

TAKEAWAYS:
Learn how to prepare and launch a high-altitude balloon that integrates science and engineering.

SPEAKERS:
Cheryl Shepherd-Adams (Teacher: Hays, KS), Paul Adams (Fort Hays State University: Hays, KS)

Goodbye, grading labs and lab reports -- Hello, lab practicals! Come learn how we’ve planned, implemented, and graded lab practical assessments in our SBG AP Physics 1 course. They are quick, individual, hands-on, aligned to science and engineering practices, and appropriate for an AP course.

TAKEAWAYS:
We will share how we’ve developed non-traditional lab assessments related to each unit in our standards-based grading AP Physics 1 curriculum. Presenters will share examples, recommendations, and challenges for teachers to think about as they implement lab practicals.

SPEAKERS:
Kristen One (Adlai E. Stevenson High School: Lincolnshire, IL), Kristy Wrona (Adlai E. Stevenson High School: Lincolnshire, IL)