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Chapter 25: The Solar System

AB
geocentrica description of a model of the solar system in which all of the planets revolve around Earth
heliocentrica description of a model of the solar system in which Earth and other planets revolve around the sun
ecliptic planethe plane in space containing Earth's orbit
moona relatively small natural body in space that revolves around a planet
astronomical unita unit of distance that equals average distance from Earth to the sun; 149,598,000 kilometers
space probean unpiloted vehicle that carries scientific instruments into space and transmits information back to earth
mariateh low, flat plains of basalt on the moon formed by ancient lunar lava flow
cratera round depression in the surface of a planet, moon, asteroid, or comet, caused by the impact of a meteroid
meteoroidschunks of rock that move through the solar system
phasesthe different shapes of the illuminated side of the moon as seen from Earth
eclipseevent that occurs when the shadow of one body in space, such as a planet or moon, falls on another
umbrathe darkest part of a shadow
penumbraa region of the moon's shadow that surrounds the umbra and is less dark than the umbra
tidesthe regular rise and fall of water in the oceans
spring tidea tide at the new or full moon when the change between daily high and low tides is the greatest
neap tidea tide at the first or last quarter moon, when there is the least change between daily high and low tides
terrestial planetsthe four planets closest to the sun (Mercury, Venus, Earth, and Mars), whicha re similar ins tructure to Earth
asteroidssmall, rocky solar-system bodies most of which are found orbiting the sun in a region between Mars and Jupiter
asteroid beltregion between the orbits of Mars and Jupiter where most asteroids in the solar system are found
gas giantsa large, massive planet ( such as Jupiter, Saturn, Uranus, or Neptune) that is composed mainly of hydrogen and helium
ringa disk made of many small particles of rock and ice in orbit around a planet
Kuiper belta wide belt beyond Pluto's orbit where objects mostly made of ice and rock orbit the sun
Oort cloudthought to be a very sparse sphere of comets encircling the solar system out to a distance of about 50,000 AU
solar nebulaa cloud of dust and gas that can eventually collapse to form one or more stars with a planetary system
protoplanetary diska large disk-shaped cloud of dust and gas formed as the solar nebula rotated faster and flattened out
planetesimalsasteroid-sized bodies in the protoplanetary disk from which the planets formed by accretion
accretionthe process of adding mass in the information of the planets by collisions between planetesimals



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