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Knowledge and Skills Statement

Earth and space. The student understands the patterns of movement, organization, and characteristics of components of our solar system.

Planets: The International Astronomical Unit has declared, independently of the formal definition of planet, that there are eight planets in the Solar System. In the geological definition used by most planetologists, a planet is a rounded sub-stellar body, possibly a satellite.

Meteors: When a meteoroid, comet, or asteroid enters Earth's atmosphere, aerodynamic heating of that object produces a streak of light, both from the glowing object and the trail of glowing particles that it leaves in its wake. This phenomenon is called a meteor or shooting star. Most meteors are fragments from comets or asteroids, while others are collision impact debris ejected from bodies such as the Moon or Mars.

Asteroids:  The term asteroid generally refers to the minor planets of the inner Solar System, including those co-orbital with Jupiter. Larger asteroids are often called planetoids.

Comets: Comets originate in the Kuiper Belt or the Oort Cloud. Comet nuclei range from a few hundred meters to tens of kilometers across and are composed of loose collections of ice, dust, and small rocky particles. The coma and tail of a comet are caused by the effects of solar radiation and the solar wind acting upon the nucleus of the comet.

Kuiper Belt: Most Kuiper Belt objects are composed largely of frozen volatiles (termed ices) such as methane, ammonia, and water. The Kuiper Belt is home to most of the objects that astronomers generally accept as dwarf planets: Orcus, Pluto, Haumea, Quaoar, and Makemake. Some of the Solar System's moons, such as Neptune's Triton and Saturn's Phoebe, may have originated in the region.

Oort Cloud: The outer Oort Cloud is only loosely bound to the Solar System and thus is easily affected by the gravitational pull both of passing stars and of the Milky Way itself. These forces occasionally dislodge comets from their orbits within the cloud and send them toward the inner Solar System.

a minor planet of the inner Solar System; any astronomical object orbiting the Sun that did not resolve into a disc and does not have characteristics of an active comet such as a tail

an icy, small solar system body that, when passing close to the Sun, warms and begins to release gases that produce a visible atmosphere, or coma, and sometimes also a tail

a circumstellar disc consisting mainly of small icy objects in the outer Solar System, extending from the orbit of Neptune at 30 astronomical units (AU) to approximately 50 AU from the Sun

a small rocky or metallic body in outer space, also called meteoroids, that are significantly smaller than asteroids and range in size from small grains to one-meter-wide objects

an astronomical body that is a natural satellite orbiting a planet, dwarf planet, or small solar system body

a theoretical concept of a cloud of predominantly icy planetesimals proposed to surround the Sun at distances ranging from 2,000 to 200,000 astronomical units, or AU (0.03 to 3.2 light-years), defining the boundary of the Solar System

observable characteristics of matter that can be used to identify particular materials

a non-stellar body that is massive enough to be rounded by its own gravity, directly orbits a star, and has cleared its orbital zone of competing objects

system consisting of the Sun and a collection of objects of varying sizes and conditions—including planets and their moons—that are held in orbit around the Sun by its gravitational pull on them

Research

Riddle, Bob. “The Icy Fringes.” Science Scope  31, no. 4 (2007): 70–73. http://www.jstor.org/stable/43184366

Summary: "The Icy Fringes" provides detailed information about objects in the solar system, such as the Kuiper Belt and Oort Cloud. Objects further from the sun are colder and have less gravitational pull resulting in their composition and orbital nature.