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This quick demonstration (on page 11 of PDF) allows learners to understand why scientists think water ice could remain frozen in always-dark craters at the poles of the Moon. This activity also demonstrates why the Lunar Crater Observation and Sensing Satellite (LCROSS) Mission launched in 2009 is targeting craters at the Moon's north/south pole to search for signs of water ice. This demonstration can be conducted with one or several learners, but requires a dark room or can be done at night. The PDF contains step-by-step instructions, photos and presentation tips. [Activity is publicly available through a web crawler capture on Archive.org.]
- Under 5 minutes
- 5 to 10 minutes
- $1 - $5 per group of students
- Ages 6 - adult
- Activity, Demonstration, Lesson/Lesson Plan, Model
- English
Quick Guide
Materials List (per group of students)
- Foam moon ball
- Skewer stick or toothpick
- Bare light bulb (40-60 watt) or a flashlight with a paper towel or wax paper and secured with a rubber band
Subjects
-
Earth and Space Science
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Astronomy
- Probes, Satellites and Spacecraft
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Solar System
- The Sun
- The Moon
-
Astronomy
-
Engineering and Technology
-
Engineering
- Aerospace Engineering
-
Engineering
-
Physical Sciences
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Heat and Thermodynamics
- Heat and Temperature
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States of Matter
- Solids
- Changes of Phase
-
Heat and Thermodynamics
-
The Nature of Technology
-
Technology and Society
- Impacts of Technology
-
Technology and Society
Informal Categories
- Model Building
Audience
To use this activity, learners need to:
- see
Learning styles supported:
- Involves hands-on or lab activities
Other
This resource is part of:
Access Rights:
- Free access
By:
Rights:
- All rights reserved, Astronomical Society of the Pacific,