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Organizing Questions
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- What does it mean for a planet to orbit the Sun, or a
moon to orbit a planet, or a solar system to orbit a
galaxy?
- What motions produce a planet's day and year?
- Describe how the phases of the moon are
produced.
- Describe the motions of stars relative to each other
(eg. expansion of the Universe).
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Elaboration
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Most objects in the solar system are in regular and
predictable motion. Those motions explain such phenomena as
the day, the year, phases of the moon, and eclipses.NSES
D3b.
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Specific Ideas
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- The motion of an object is always judged with respect
to some other object or point and so the idea of absolute
motion or rest is misleading. Benchmarks 10A1
- An unbalanced force acting on an object changes its
speed or path of motion, or both. If the force acts
toward a single center, the object's path may curve into
an orbit around the center. Benchmarks 4F3
- The moon's orbit around the earth once in about 28
days changes what part of the moon is lighted by the sun
and how much of that part can be seen from the earth--the
phases of the moon. Benchmarks 4B5
- Large numbers of chunks of rock orbit the sun. Some
of those that the earth meets in its yearly orbit around
the sun glow and disintegrate from friction as they
plunge through the atmosphere--and sometimes impact the
ground. Other chunks of rocks mixed with ice have long,
off-center orbits that carry them close to the sun, where
the sun's radiation (of light and particles) boils off
frozen material from their surfaces and pushes it into a
long, illuminated tail. Benchmark s4A4
- Nine planets of very different size, composition, and
surface features move around the sun in nearly circular
orbits. Some planets have a great variety of moons and
even flat rings of rock and ice particles orbiting around
them. Some of these planets and moons show evidence of
geologic activity. The earth is orbited by one moon, many
artificial satellites, and debris. Benchmarks 4A3
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Developmental & Instructional
Implications
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The dependence of apparent size on distance can be used
to pose the historically important puzzle that star patterns
do not appear any larger from one season to the next,
even though the earth swings a hundred million miles closer
to them. Benchmarks p. 63.
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Examples
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