The student will investigate and understand the organization of the solar system and the interactions among the various bodies that comprise it.
Key concepts include
the sun, moon, Earth, other planets and their moons, dwarf planets, meteors, asteroids, and comets
relative size of and distance between planets;
the role of gravity
revolution and rotation
the mechanics of day and night and the phases of the moon
the unique properties of Earth as a planet
the relationship of Earth’s tilt and the seasons
the cause of tides
the history and technology of space exploration
The Solar System
The solar system consists of the sun, moon, Earth, other planets and
their moons, meteors, asteroids, and comets. Each body has its own
characteristics and features.
The distance between planets and sizes of the planets vary greatly.
The
outer, ―gas planets are very large, and the four inner planets are
comparatively small and rocky.
A dwarf planet revolves around the sun, and can maintain a nearly
round shape as planets do, but it cannot move other objects away from
its orbital neighborhood.
Gravity is a force that keeps the planets in motion around the sun.
Gravity acts everywhere in the universe.
Revolution and Rotation
Planets revolve around the sun, and moons revolve around planets. A
planet rotates upon an axis.
As Earth rotates, different sides of Earth face toward or away from the
sun, thus causing day and night, respectively.
Seasons are caused by a combination of the tilt of Earth on its axis, the
curvature of Earth’s surface and, thus, the angle at which sunlight
strikes the surface of Earth during its annual revolution around the sun.
Planet Earth
Earth is a rocky planet, extensively covered with large oceans of liquid
water and having frozen ice caps in its polar regions.
Earth has a protective atmosphere consisting predominantly of nitrogen and oxygen and has a magnetic field.
The atmosphere and the magnetic field help shield Earth’s surface from harmful solar radiation.
Scientific evidence
indicates that Earth is about 4.5 billion years old.
Moon Phases; Tides
The phases of the moon are caused by its position relative to Earth and
the sun.
Tides are the result of the gravitational pull of the moon and sun on the
surface waters of Earth.
Historical
The ideas of Ptolemy, Aristotle, Copernicus, and Galileo contributed to
the development of our understanding of the solar system.
With the development of new technology over the last half-century, our
knowledge of the solar system has increased substantially.
describe the planets and their relative positions from the sun.
compare the characteristics of Pluto to the planets and explain its
designation as a dwarf planet.
design and interpret a scale model of the solar system. (A scale model
may be a physical representation of an object or concept. It can also
be a mathematical representation that uses factors such as ratios,
proportions, and percentages.)
explain the role of gravity in the solar system.
model and describe how Earth’s axial tilt and its annual orbit around
the sun cause the seasons.
describe the unique characteristics of planet Earth.
discuss the relationship between the gravitational pull of the moon and
the cycle of tides.
compare and contrast the ideas of Ptolemy, Aristotle, Copernicus, and Galileo related to the solar system.
create and interpret a timeline highlighting the advancements in solar
system exploration over the past half century. This should include
information on the first modern rockets, artificial satellites, orbital
missions, missions to the moon, Mars robotic explorers, and
exploration of the outer planets.