Ptolemaic System of Planetary Motion
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Ptolemaic System of Planetary Motion

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Questions and Answers

The Sun and Moon, however, used no ______ (both have almost uniform motion about the sky).

epicycles

For Mercury and Venus, Ptolemy needed to lock the centers of their ______ to the direction of the Sun.

epicycles

The stars appeared to be fixed on a celestial sphere rotating once each day about an axis through the geographic poles of ______.

Earth

The greatest angular displacements for Mercury and Venus set their orbital sizes relative to Earth’s orbital size by forming right angle ________.

<p>triangles</p> Signup and view all the answers

Earth seems to be unmoving from the perspective of an earthbound observer; it feels solid, stable and ______.

<p>stationary</p> Signup and view all the answers

The observed time for a planet to move from opposition to quadrature yields a right-angle ________.

<p>triangle</p> Signup and view all the answers

Planetary orbital periods correlate with the distance from the ________.

<p>Sun</p> Signup and view all the answers

Galileo Galilei was one of the first people to point the telescope at the sky and made it ________.

<p>famous</p> Signup and view all the answers

The eccentricity of a circle is ____, while a line would have an eccentricity of 1.

<p>0</p> Signup and view all the answers

The closest approach of a planet to the Sun is known as the ____, a distance equal to a (1 - e).

<p>perihelion</p> Signup and view all the answers

Kepler's Second Law of Planetary Motion states that a line connecting the planet with the Sun sweeps over an area at a ____ rate.

<p>constant</p> Signup and view all the answers

In consequence, when a planet moves closer to the Sun, its orbital velocity must ____, and vice versa.

<p>increase</p> Signup and view all the answers

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