Topic 8- Planetry Motion And Gravity Flashcards

1
Q

Who put forwards the heliocentric model

A

Copernicus

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2
Q

What book did Copernicus write

A

De revolutionibus orbium coelestium- on the revolutions of heavenly spheres

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3
Q

What types of orbits did the planets have in Copernicus’ book

A

Circular orbits

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4
Q

What type of observations supported his theory

A

Mathematical observations

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5
Q

When was the book published

A

After he died

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6
Q

Why did people find it hard to accept the heliocentric theory

A

It went against what the bible said

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7
Q

What model did Tycho Brahe propose

A

The geo-heliocentric model

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8
Q

What is the geo-heliocentric model

A

The moon and sun orbited the earth but everything else orbited the sun

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9
Q

What did tychos base his model on

A

Both religious and on observations

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10
Q

Who was Kepler

A

Tycho Brahe’s assistant in Prague

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11
Q

Who was Kepler influenced by

A

Copernicus

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12
Q

What did Kepler refine

A

The heliocentric model

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13
Q

What did Kepler notice with tychos observations

A

He noticed that planets did not follow circular orbits but we elliptical

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14
Q

What was Galileo Galilei first to do

A

The first telescopic observer to make published astronomical observations

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15
Q

What did Galileo discover

A

Jupiter has moons
Venus had phases

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16
Q

What happened because of Galileos observations

A

The heliocentric model became widely expected

17
Q

What force is responsible for creating stable elliptical orbits

A

Gravity

18
Q

How does gravity create stable elliptical orbits

A

Due to the constant gravitational force between the object and the sun to keep it in orbit

19
Q

What are the 2 things that control gravity

A

Mass and distance

20
Q

What is keplers first law

A

Planets do not move in circular orbits

21
Q

What is an ellipse

A

An oval shape with 2 foci

22
Q

What are the 2 foci

A

The sun and the other is in space

23
Q

What is keplers second law

A

The sun-planet line sweeps out equal areas in equal times

24
Q

Does a planet move faster or slower when near the sun

A

Faster

25
Q

What is keplers 3rd law

A

The orbital period of a planet squared is equal to its mean distance from sun cubed when different planets are compared

26
Q

How do you work out a constant

A

T2/R3

27
Q

What does the T stand for in the constant equation

A

Period/time takes to orbit/ orbital period

28
Q

What does the R mean in the constant equation

A

Mean radius from the body it’s orbiting

29
Q

Who proposed the inverse square law

A

Newton

30
Q

What is the inverse square law

A

If earth had a 1/2 of its mass then it would produce 1/4

31
Q

What was the relation to keplers law

A

For every action there is an equal action and opposite reaction

32
Q

If an object orbits nearer another in an elliptical orbit there must be an increase or decrease in gravitational force between them at that point

A

Increase

33
Q

What is keplers 3rd law

A

The force is proportional to the sum of the masses of both objects it inversely relies on the mass of the sun essentially

34
Q

What does perihelion mean

A

Body nearer the sun

35
Q

What does aphelion mean

A

Body further away from sun