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