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Ancient Astronomy and Planetary Motion
Ancient Astronomy and Planetary Motion
50 terms
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Astronomy
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1
The law that describes the path of a planet that orbits the sun is called the
Law of ellipses
Law of periods
Law of equal areas.
Law of orbital periods.
2
The more elliptical this ellipse gets… what happens to eccentricity?
it goes to zero
it goes above 1
it goes close to zero
it goes close to 1
3
Who believed that planets moved in epicycles as they revolved in larger circles around Earth?
Copernicus
Newton
Aristotle
Ptolemy
4
The turning or spinning of a body on its axis is known as
Precession
Apogee.
Revolution.
Rotation.
5
A girl pulling a sled is crying because when she stopped the sled kept moving into her leg
Newton's 3rd Law
Newton's 2nd Law
Newton's 1st Law
Kepler's 1st Law
6
An orange might roll off your cafeteria tray when you stop suddenly because of
The orange’s inertia.
The centripetal force acting on the orange.
The balanced forces acting on the orange.
The friction forces acting on the orange.
7
the time required for a body to complete a single orbit
orbital period
gravity
eccentricity
inertia
8
Which laws describes the speed of an object travels at different points in its orbits?
law of ellipses
law of eccentricity
law of periods
law of equal areas
9
A swimmer pushes water back with her arms, but her body moves forward.
Kepler's 1st Law
Newton's 1st Law
Newton's 3rd Law
Newton's 2nd Law
10
As an astronaut travels far away from Earth, her weight
Increases because gravity increases.
Decreases because gravity decreases.
Remains the same because her mass remains the same.
Decreases because her mass decreases.
11
Which scientist determined the nature of the forces that keep the planets in their orbits?
Galileo
Newton
Brahe
Copernicus
12
The tendency of an object to resist change in its motion is known as
inertia
balance
mass
force
13
The geocentric model of the universe stated that
The sun was the center of the universe.
Earth was the center of the universe.
Earth was a “wanderer”.
Earth revolved around the celestial sphere.
14
Gravity on Mars is about 1/3 the gravity on Earth. The weight of you on the surface of Mars is
One third its weight on Earth’s surface.
The same as its weight on Earth’s surface.
Nine times greater than its weight on Earth’s surface.
Three times greater than its weight on Earth’s surface.
15
How do you calculate the eccentricity of this ellipse?
299,000,000 * 5,000,000
5,000,000/ 299,000,000
5,000,000 * 299,000,000
299,000,000/ 5,000,000
16
Which scientist was the first to use the telescope in astronomy?
Galileo
Newton
Copernicus
Kepler
17
The force that gravity exerts on an object changes the objects
Mass.
Volume.
Weight.
Density.
18
Low eccentricity is what shape orbit?
a straight line
very elliptical
a perfect circle
very round
19
Seasons are caused by
Both tilt and revolution
Earth’s tilted axis
Earth’s Revolution.
Earth’s rotation.
20
Summer Solstice
C
B
A
D
21
Law that each planet revolves so that an imaginary line sweeps over equal areas in equal time?
the third law of planetary motion
the second law of planetary motion
the first law of planetary motion
the law of universal gravitation
22
Earth is closest to the sun at a point called
Apogee.
Perihelion.
Aphelion.
precession
23
Newton’s third law of motion describes
Centripetal forces.
Action and reaction forces.
Net force.
Balanced forces.
24
According to the 3rd law of planetary motion, the period of a planet is related to the planet’s
Gravitational attraction.
Orbital speed.
Distance to the sun.
Size.
25
In a diagram depicting the solar system as heliocentric, what is located at the center?
Mars
Earth
the moon
the sun
26
The achievement of lifting a rocket off the ground and into space can be explained by
Newton’s third law.
Newton’s second law.
The law of conservation of momentum.
Newton’s first law.
27
Which of the following helps explain why the planets remain in motion around the sun?
inertia
both gravity and inertia
density
gravity
28
The force that pulls falling objects toward Earth is called
air resistance
gravity
free fall
acceleration
29
the degree of elongation of an elliptical orbit
inertia
eccentricity
orbital period
gravity
30
Winter Solstice
C
A
B
D
31
Relationship between the aver distance of a planet from the sun and the planet’s orbital period
Law of periods.
Law of equal areas.
Law of motion.
Law of ellipses.
32
the force that exists between any two bodies in the universe
inertia
orbital period
gravity
retrograde motion
33
What movement of Earth is responsible for night and day?
precession
revolution
perigee
rotation
34
So if a planet has an average distance of 4 astronomical units (AU) would have a period of
16 years
8 years
4 years
32 years
35
The first early astronomer to propose a sun-centered solar system was
Copernicus.
Brahe.
Galileo.
Newton.
36
In which of the following are action and reaction forces involved?
when stepping from a curb
when rowing a boat
all of the above
when a tennis racket strikes a tennis ball
37
Using Tycho Brahe’s data, which scientist proposed three laws of planetary motion?
Galileo
Newton
Kepler
Copernicus
38
Which is the most likely reason that old observers believed in a geocentric universe?
The Earth seemed to move on its axis.
Objects in the sky appear to circle around Earth.
Ancient observers believed the universe was stationary.
Earth's motion is only known because of telescopes
39
Autumnal Equinox
D
B
C
A
40
a pattern that makes it appear as though planets are moving backward in the sky
inertia
retrograde motion
orbital period
eccentricity
41
The true shape of planetary orbits was discovered by
Brahe.
Kepler
Newton.
Galileo.
42
Which astronomer spent 20 years collecting data and making observations?
Galileo
Kepler
Newton
Brahe
43
Vernal Equinox
A
C
D
B
44
Newton’s 2nd law, says the acceleration of an object=the force acting on the object/by object’s
momentum
mass
velocity
weight
45
One astronomical unit (AU) is
the distance from the sun to the moon
the distance from the earth to the moon
the distance from the earth to the Milky Way
the distance from the sun to the earth
46
In the Ptolemaic model of the universe,
The sun was the center of the solar system.
Earth was much larger than the sun
Earth was the center of the universe.
Earth was flat
47
When a planet is at its perihelion what happens to it velocity?
it increases
it fluctuates
it stays the same
it decreases
48
the tendency of a body to resist a change in motion unless acted upon by an outside force
inertia
retrograde motion
orbital period
gravity
49
After you start up your dirt bike, as you give it more gas, it goes faster
Newton's 3rd Law
Kepler's 1st Law
Newton's 2nd Law
Newton's 1st Law
50
What is the shape of a planet’s orbit?
elliptical
irregular
circular
parabolic