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To search for teaching materials that address particular concepts in our conceptual framework, visit the teaching guide for your grade level:
K-2, 3-5 , 6-8, 9-12, or College
Found 8 resources:
Luminous
Grade Level(s):
- 9-12
- College
Source:
- Sam Smartt
Resource type:
- classroom activity
- Science Story
- video
Discipline:
- Space science
Time: 2-8 hours
Overview
The film LUMINOUS (now freely available through many libraries and the Kanopy platform) tells the story of astronomer Larry Molnar as he investigates a distant, double-star system, about which he makes a daring and explosive prediction. Interviews with Dr. Molnar’s diverse set of colleagues, collaborators, and skeptics highlight science as a community and intensely human endeavor, debunking the myth of the lone scientist conducting dispassionate research. The Luminous Science Education Toolkit provides classroom activities to support students' interpretation of the film.
Piecing together fossil puzzles in a mysterious museum cabinet
Grade Level(s):
- 9-12
- College
Source:
- UC Museum of Paleontology
Resource type:
- Science Story
Discipline:
- Earth science
Time: 5 minutes
Overview
This Science Short illustrates how paleontologists visualize, tabulate, and share raw data about fossils. Get tips on using Science Stories in class.
Discovering mass extinctions in the fossil record
Grade Level(s):
- College
Source:
- UC Museum of Paleontology
Resource type:
- lab activity
Discipline:
- Earth science
- Life Science
Time: 2 hours
Overview
This activity (suitable for distance learning) is designed to introduce students to the nature and process of science through the discovery of mass extinctions in the fossil record. Students will explore the fossil record of brachiopods and bivalves using the Paleobiological Database, identify patterns in their data, and generate and evaluate hypotheses. They will also document this process using the Understanding Science flowchart. Clicking the link below will download the Word file for this lesson.
High altitude adaptations: The work of Emilia Huerta-Sánchez
Grade Level(s):
- College
Source:
- UC Museum of Paleontology
Resource type:
- research profile
- Science Story
Discipline:
- Life Science
Time: 1 hour
Overview
This research profile tells the story of Emilia Huerta-Sánchez and how she uses mathematical modeling to answer evolutionary questions. Students examine data visualizations and learn about the process of science while focusing on adaptations, allele frequencies, and natural selection. Get tips on using Science Stories in class.
Heating and cooling of the Earth’s surface
Grade Level(s):
- 6-8
Source:
- UC Museum of Paleontology
Resource type:
- lab activity
Discipline:
- Physical Sciences
Time: Two class periods
Overview
Students conduct experiments on the rate that sand and water heat up and cool down. Based on their observations, they make hypotheses about why materials heat up and cool down at different rates and then test their ideas.
Mystery boxes for grades 3-5
Grade Level(s):
- 3-5
Source:
- Janulaw, Sharon
Resource type:
- classroom activity
Discipline:
- General
Time: One class period
Overview
Working in groups, students pose explanations (hypotheses) for what they are observing and are asked to test their hypotheses. These procedures have been modified from Mystery Boxes: Uncertainty and Collaboration by Jean Beard.
Rutherford’s enlarged: A content embedded NOS activity
Grade Level(s):
- 9-12
Source:
- Abd-El-Khalick, Fouad
Resource type:
- lab activity
Discipline:
- Physical Sciences
Time: One class period
Overview
Students reason about a model of Ernst Rutherford's famous experiment supporting the idea of the atomic nucleus. They differentiate between observation and inference and see the role of creativity in the process of science.
Age dating star clusters
Grade Level(s):
- 9-12
Source:
- Whitfield, Lisé
Resource type:
- lab activity
Discipline:
- Space science
Time: ~ one hour
Overview
Students explore how classification and graphing are used by astronomers to determine the age of star clusters. They will measure the color and brightness of stars, as proxies for temperature and luminosity.