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30 Cards in this Set

  • Front
  • Back

geocentric

view that the Earth is at the center of the solar system

heliocentric

view that the sun is at the center of the solar system

retrograde motion

apparent westward movement of the planets with respect to the stars

Aristotle

determined the earth was spherical bc it casts a curved shadow on the moon

Eratosthenes

first successful calculation of the size of the Earth

Aristarchus

Proposed a heliocentric universe. First calculated distance between Earth and sun. First calculated the size of the sun and moon.

Nicolaus Copernicus

Repurposed a heliocentric universe on his deathbed.

Tycho Brahe

made accurate and key observations to disprove a heliocentric universe that ended up proving it

Johannes Kepler

1. Planet orbits are elliptical, not circular


2. Planets speed up and slow down


3. Planets' distance to the sun is proportional to the length go their years

Galileo Galilei

Venus has phases like the moon, proved a heliocentric universe

inertia

property of matter that resists a change in its motion

Law of universal gravitation

every body in the universe attracts every other body with a force that is proportional to their masses and inversely proportional to the square of the distance between them

constellation

apparent group of stars originally named for mythical characters

equatorial system

method of locating stellar objects much like the coordinate system used on Earth's surface

declination

angular distance north or south of the celestial equator denoting the position of a celestial body

right ascension

angular distance measured eastward along the celestial equator from the vernal equinox

revolution

motion of one body about another, such as Earth about the sun

axial precession

slow motion of Earth's axis that traces out a cone over a period of 26,000 years

mean solar day

average time between two passages of the sun across the local celestial meridian

sidereal day

period of rotation with respect to the stars

perihelion

points the orbit of a plane where it is closest to the sun

aphelion

point in the orbit of a planet where it is farthest from the sun

ecliptic

yearly path of Sun plotted against the background of stars

plane of ecliptic

imaginary plane that connects Earth's orbit with the celestial sphere

axial precession

slow motion of Earth's axis that traces out a cone over a period of 26,000 years

synodic month

time period of revolution of the Moon around Earth with respect to the Sun

sidereal month

time period of revolution of the Moon around Earth with respect to the stars

phases of the moon

progression of changes in the Moon's appearance during the month

solar eclipse

eclipse of the Sun

lunar eclipse

eclipse of the Moon