Lesson Plan #:AELP-SPA003
Submitted by: Jan Mader, Great Falls, MT
Endorsed by: These lesson plans are the result of the work of the teachers who have attended the Columbia Education Center’s Summer Workshop. CEC is a consortium of teacher from 14 western states dedicated to improving the quality of education in the rural, western, United States, and particularly the quality of math and science Education. CEC uses Big Sky Telegraph as the hub of their telecommunications network that allows the participating teachers to stay in contact with their trainers and peers that they have met at the Workshops.
Date: May 1994
Grade Level(s): 8, 9, 10, 11, 12
Subject(s):
- Science/Space Sciences
This lesson incorporates the learning cycle format with space science material. The lesson examines some of the benefits of the space program to our life on Earth. This lesson consists of an exploratory lab, concept development questions and STS application lab to reinforce the concept of radar mapping and probes.
TITLE: 20,000 LEAGUES UNDER THE SEA (Exploration)
PURPOSE: How can a surface be described without seeing it?
RESOURCES/MATERIALS
1. Playdough
2. Box template or a video tape box with a cover with 16 holes 1cm apart
3. Straw and millimeter measure
4. Graph paper
5. Tape
ACTIVITIES AND PROCEDURES:
Summary:
TYING IT ALL TOGETHER:
TITLE: IS THERE ANYONE OUT THERE ? (Application)
OBJECTIVES:
How are probes designed to map planets? What precautions do developers take?
RESOURCES/MATERIALS:
You will need to order the Magellan Fact sheets from a NASA resource center, and borrow the NASA video series on MARS or Voyager.he manned space missions may have received more public attention over the years, NASA has also managed many exciting and successful unmanned exploratory flights: the Ranger and Surveyor missions to the Moon; the Mariner missions that explored Mars, Venus, and Mercury; the Viking Mars Orbiters; the Pioneer voyages to Venus, Jupiter, Saturn, and Neptune; and the Voyager missions to Jupiter, Saturn, Uranus, and Neptune. Beginning in 1989, NASA embarked on a new round of planetary missions, including Magellan, a Venus orbiter, and Galileo, a Jupiter orbiter and probe. NASA is also a major participant in an international mission to observe the poles of the Sun (Ulysses). Once the Magellan spacecraft arrives at Venus, in early August 1990, it will be placed in an elliptical orbit whose distance from the planet ranges between 250 kilometers (155 miles) and 8,029 kilometers (4,889 miles). When it is close to Venus, the spacecraft will point its imaging radar at the planet’s surface to collect data. When farther away, the spacecraft will transmit its data to Earth. From 70 to 90 percent of the surface of Venus is expected to be mapped. The Magellan imaging radar will send out several thousand pulses of radio energy each second at the speed of light 300,000,000 meters a second, (186,000 miles a second) across a target swath. Magellan’s swath will range between 17 and 28 kilometers (10 and 17 miles) wide. The signals will bounce off the target and be detected by the spacecraft’s radar antenna. A two-dimensional radar image is constructed from three characteristics of each radar pulse: 1) The time the signal takes to make the round trip between instrument and target; 2) The Doppler shift, a measurement of relative motion that is akin to a change in pitch; and 3) Finally, the brightness, or reflectivity, of each component Your group has just been selected to design a new planetary probe to fly on the next generation of exploratory missions. The following procedure describes your task.
ACTIVITIES AND PROCEDURES:
TYING IT ALL TOGETHER: