5.4 - Gravitational fields

0.0(0)
Studied by 0 people
call kaiCall Kai
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
GameKnowt Play
Card Sorting

1/12

encourage image

There's no tags or description

Looks like no tags are added yet.

Last updated 6:21 PM on 9/30/26
Name
Mastery
Learn
Test
Matching
Spaced
Call with Kai
Chat

No analytics yet

Send a link to your students to track their progress

13 Terms

1
New cards

What is gravity?

Gravity is the universal attractive force which acts between all matter.

2
New cards

What can field lines tell you about a field?

Direction of field lines and strength depending on density of lines.

3
New cards

What is g?

g is the force per unit area in a uniform gravitational field

In a radial field the magnitude of g is the proportionality constant at that point between force and mass

I.e g=GM/r²

4
New cards

What is Newton’s law of gravitation

States that 2 point masses attract each other with a force that is directly proportional to the product of their masses, and inversely proportional to the square of the distances between them.

5
New cards

What is Kepler’s first law?

The orbit of a planet is an ellipse, with the sun at one foci.

The eccentricity of the ellipse is very low, so the motion can be modeled as circular.

6
New cards

What is Kepler’s second law?

A line segment joining a planet and the sun sweeps out equal areas during intervals of equal time.

This is because the speed of the planet is not constant - the planet moves faster when closer to the Sun.

7
New cards

What is Kepler’s third law?

T² ∝ r³. (T₁/T₂)² = (r₁/r₂)³


Square of the orbital period (T) of a planet is directly proportional to the cube of its average distance from the sun ( r ).

8
New cards

Derive T² = 4pi²r³/GM

1) Kepler’s third law, equate formula of centripetal force with formula for gravitational force, mv²/r = GMm/r²

2) Rearrange for v² = GM/r

3) Since velocity in circular motion is 2pir/T, substitute into previous equation to get 4pi²r²/T² = GM/r

4) Rearrange for formula

9
New cards

What are geostationary satellites? What are they used for?

  • Orbital period of 24 hours

  • Rotate in same direction as Earth’s rotation

  • Be in orbit above Earth’s equator


10
New cards

What is gravitational potential?

The potential energy per kilogram, at any point in the field.

0 potential is defined at infinity, so at a point close to a mass, the potential of an object would be negative.

11
New cards

What is gravitational potential difference?

Difference in the gravitational potentials of 2 points in a gravitational field.

12
New cards

What is gravitational potential energy at a point in the field?

The work done per unit mass in moving object from infinity to that point in the field

13
New cards

What is escape velocity?

  • The minimum velocity an object requires in order to escape the gravitational field of an object when projected vertically from its surface.

  • Vesc derived from equating kinetic energy and gravitational potential energy required to reach infinity.

  • Vesc = root of 2GM/r