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33 Cards in this Set
- Front
- Back
solar system
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the sun and all of the bodies that orbit the sun |
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heliocentric |
earth and the other planets orbit the sun |
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geocentric |
earth was the center of the solar system, with the sun, moon, and the planets circling it |
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parallax |
the apparent shift in the position of an object when viewed from different locations |
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gravity |
the force of attraction between objects that is due to their masses and the distances between them |
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orbit |
the path that a body follows as it travels around another body in space |
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aphelion |
the farthest earth is away from the sun in its orbit; occurs on about july 4 |
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perihelion |
the closest earth is to the sun in its orbit; occurs on about january 3 |
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kepler's first law kepler's second law kepler's third law |
planetary orbits are ellipses with the sun at one focus planets move faster in their orbits when closer to the sun relates the distance of a planet from the sun to the time it takes to complete one orbit |
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law of universal gravitation |
all objects in the universe attract each other through gravitational force; as the distance between two objects increases, the force of gravity decreases |
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centripetal force |
the inward force that causes an object to move in a circular path |
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solar nebula |
a cloud of dust and gas from which the solar system formed |
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protostellar disk |
where the sun formed; from the solar nebula rotating faster and flattening out into a disk |
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planetesimals |
meter sized objects, formed from dust grains colliding and growing in size, that collided to form kilometer sized objects |
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protoplanetary disk |
the disk in which the planets formed |
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terrestrial planets |
rocky, metallic planets that formed in the hot inner protoplanetary disk (Earth, Venus, Mars, and Mercury) |
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gas giant planets |
planets with ricky or metallic cores and deep atmospheres of gas and ice that formed in the cold outer protoplanetary disk; the gravity was so strong that they captured gas and other matter as they grew (Saturn, Jupiter, Uranus, and Neptune) |
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rotation |
the spinning of a planet on its axis earths rotation is counter clockwise (west to east) |
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day |
the time it takes a planet to complete one full rotation; 24 hours |
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revolution |
the motion of a body/planet that travels around another body in space |
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year |
the amount of time it takes earth to complete a full revolution around the sun 365 1/4 days |
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season |
a pattern of temperature and other weather trends; the tilt of earths axis (23.5°) and earths spherical shape play a roll in earths changing seasons |
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equinox |
means "equal night"; sun shines equally in the northern and southern hemispheres fall equinox/spring equinox |
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solstice |
means "sun stops"; the sunlight is at a maximum in one hemisphere and a minimum in the other hemisphere winter solstice/summer solstice |
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precession |
the wobbling motion of earth as it turns on its axis; caused by the gravitational pull exerted on the earth by the moon, sun, and other planets causes earths axis to move slowly in a circle |
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satellite |
a body that orbits a larger body |
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moons |
natural satellites |
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lunar phases |
the portion of sunlight that the moon reflects to earth changes causing the moons appearance to change |
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eclipse |
an event during which one object in space casts a shadow into another |
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lunar eclipse |
when the moon moves through earth's shadow |
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solar eclipse |
when the moon is directly between the sun and Earth, the shadow of the moon falls on a part of the earth; the suns light is completely blocked by the moon |
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umbra |
the darkest part of a shadow |
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penumbra |
spreading cone of lighter shadow |