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The Moons of Jupiter
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The Moons of Jupiter

Download This Lesson (PDF, 206 KB)

Topic:

Grade Level: 5-8, 9-12

Body: Jupiter

Mission:

Science Education Standards:

Physical science:

  • Structure and properties of matter

Science as inquiry:

  • Abilities necessary to do scientific inquiry

Short Description: Students investigate how the density of Jupiter's moons is related to their diameter and distance from Jupiter.

Source: LASP


Lesson Summary

Students investigate how the density of Jupiter's moons is related to their diameter and their distance from Jupiter.

Prior Knowledge & Skills

  • Plotting data
  • Interpreting data

AAAS Science Benchmarks

The Physical Setting
Structure of matter

NSES Science Standards

  • Physical science: Properties and changes of properties in matter (5-8), Structure and properties of matter (9-12)
  • Science as inquiry: Abilities necessary to do scientific inquiry

NCTM Mathematics Standards

  • Data analysis and probability: Develop and evaluate inferences and predictions that are based on data, Formulate questions that can be addressed with data and collect, organize and display relevant data to answer them

Teaching Time:

One 45-minute period

Materials

Each student needs:

  • Copy of "The Moons of Jupiter" worksheet
  • Density and diameter data for Mercury, Mars, and Earth's moon

Advanced Planning Preparation Time: 30 minutes

  1. Prepare handouts

  2. Gather density and diameter data for Mercury, Mars, and Earth's moon

  3. Review lesson plans

Source: Windows to the Universe, at http://www.windows.ucar.edu/ at the University Corporation for Atmospheric Research (UCAR). c 1995-1999, 2000 The Regents of the University of Michigan; c 2000-05 University Corporation for Atmospheric Research. All Rights Reserved.


The Moons of Jupiter

More than 60 moons have been found at Jupiter. The four largest were discovered by Galileo himself in the year 1610! That's why they're called "The Galilean Satellites." There are four smaller satellites in near-circular orbits that are closer to Jupiter than the innermost Galilean Satellite (Io, see below): Amalthea (discovered in 1892) and 3 others (discovered in 1979). The remaining satellites have elliptical orbits and are found far beyond Callisto. And, if that isn't enough, the Voyager mission also discovered a RING around Jupiter!!

This figure shows a diagram of Io, Europa, Ganymede, and Callisto listed in order of their respective distances from Jupiter with information about their diameters and densities.  Io's diameter is 3,642 km, its density is 3.55 grams per cubic centimeter, and it orbits 422,000 km from Jupiter.  Europa's diameter is 3,130 km, its density is 3.04 grams per cubic centimeter, and it orbits 671,300 km from Jupiter.  Ganymede is 5,268 km in diameter, its density is 1.93 grams per cubic centimeter, and it orbits 1,071,000 km from Jupiter. Callisto is 4,806 km in diameter, its density is 2.83 grams per cubic centimeter, and it orbits 1,833,000 km from Jupiter. Below this diagram is a chart for plotting density versus diameter for these moons using the information above, as well as for Mercury, Mars, and Earth's moon using information given below.

Using the data below and the information on the worksheet, plot the density versus diameter of Mercury, Mars, Earth's moon and the Galilean satellites on the chart provided.

Planet Diameter Density
Mercury 4,879 km 5.42 g/cm3
Mars 6,794 km 3.94 g/cm3
Earth's Moon 3,475 km 5.52 g/cm3

How do the Galilean satellites compare to these bodies in terms of size?

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Based on density, can you guess anything about the composition of Jupiter's moons?

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Based on density, can you guess anything about the other bodies? For example, why is Mercury so much denser than Mars?

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Do you see any trends that correspond to distance from Jupiter?

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The source of this material is Windows to the Universe, at http://www.windows.ucar.edu/ at the University Corporation for Atmospheric Research (UCAR). c 1995-1999, 2000 The Regents of the University of Michigan; c 2000-05 University Corporation for Atmospheric Research. All Rights Reserved.

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Last Updated: 20 Jun 2012