Section 9 - Gravitational and Electric Fields Flashcards
What is a force field?
A region where an object will experience a non-contact force.
What do force fields cause?
Interactions between objects or particles.
What is a gravitational field?
A region where objects with mass will experience an attractive force.
How can a force field be represented?
Using field lines (or “lines of force”) that show the direction of the force that would be exerted on an object in a given position.
How are field lines used to show the strength of a field?
The further apart the lines are, the weaker the field.
Describe the gravitational field of the Earth.
- It is radial, so the field lines meet at the centre of the Earth like a spiderweb
- Close to the surface, the field can be considered almost uniform since the field lines are almost parallel and equally spaced
Practice drawing out the Earth’s gravitational field.
See diagram pg 120 of revision guide.
What is Newton’s Law of Gravitation?
- An equation used to calculate the gravitational force between two point masses
- F = Gm₁m₂ / r²
What is the equation for the gravitational force between two point masses (Newton’s Law of Gravitation)?
F = Gm₁m₂ / r²
Where:
• F = Force (N)
• G = Gravitational constant = 6.67 x 10^-11 Nm²/kg²
• m = Mass (kg)
• r = Distance between centres of two point masses (m)
What type of law is Newton’s Law of Gravitation and how can this be symbolised?
- Inverse square law
* F ∝ 1 / r²
If the distance between 2 point masses is doubled, what happens to the magnitude of the gravitational force between them?
It is one quarter of the original.
What has a bigger impact on the size of the gravitational force, the distance between them or the mass?
- The distance
* This can be seen with Newton’s Law of Gravitation
In gravitational calculations, what is G?
- The gravitational constant
- It is used in some equations
- 6.67 x 10^-11 Nm²/kg²
What is gravitational field strength?
• The force per unit mass exerted at a given position in a gravitational field.
OR
• The acceleration of a mass in a gravitational field.
What is the symbol for gravitational field strength?
g
What are the units for gravitational field strength?
N/kg or m/s²
What is the equation that defines gravitational field strength?
g = F / m
Where:
• g = Gravitational field strength (N/kg)
• F = Force (N)
• m = Mass (kg)
Is the value of g constant throughout a field?
No, its value depends on the where you are in the field.
What is the value of g at the Earth’s surface?
9.81 N/kg (or m/s²)
Is g constant around the world?
The gravitational field is almost uniform at the Earth’s surface, so you can assume that g is a constant as long as you don’t go too high above the Earth’s surface.
In a radial field, how does g vary with the radius from the centre of the mass?
g is inversely proportional to r²
Describe the gravitational field around a point mass.
Radial
Give the equation for g around a point mass.
g = GM / r²
OR
g = -ΔV / Δr
Where: • g = Gravitational field strength (N/kg) • G = Gravitational constant (Nm²/kg²) • M = Point mass (kg) • r = Distance from centre (m) • V = Gravitational potential (J/kg)
What kind of law is the equation that gives g relative to the distance from a point mass?
Inverse square law (since g is inversely proportional to r²)
Describe the graph of g against r for a point mass.
- Does not cross y-axis
- Curve starts at its highest point at a certain x-value (RE - radius of the Earth)
- It then curves like a 1/x² graph and never quite reaches the x-axis
(See diagram pg 121 of revision guide)
Remember to practise drawing out the graph of g against r for a point mass.
See diagram of 121 of revision guide.
What is gravitational potential?
The gravitational potential energy that a unit mass would have at that point in a gravitational field.
What is the symbol for gravitational potential?
V
What are the units for gravitational potential?
J/kg
What is the difference between gravitational potential energy and gravitational potential?
- Gravitational potential -> GPE that a unit mass would have at a given point in a gravitational field
- Gravitational potential energy -> The energy that a mass has due to its position in a gravitational field
What is the equation for gravitational potential?
V = -GM / r
Where:
• V = Gravitational potential (J/kg)
• G = Gravitational constant = 6.67 x 10^-11 Nm²/kg²
• M = Mass of point mass (kg)
• r = Distance from centre of point mass (m)
What is unusual about gravitational potential and GPE? Why?
- They are negative, since you can think of it of as negative energy since work has to be done to move an object out of the field
- They becomes less negative with distance from the point mass
- At infinite distance, the gravitational potential is 0J/kg and GPE is 0J
Which quantities in gravitational field questions are always negative?
- Gravitational potential
* Gravitational potential energy (GPE)
Describe how gravitational potential (and GPE) changes with distance from a planet’s surface.
- Most negative on the planet’s surface
- Becomes less negative with distance from the planet
- 0J/kg at infinite distance
At infinite distance from a planet, what is the gravitational potential and GPE?
- Gravitational potential (0J/kg)
* GPE (0J)
Describe a graph of V against r for the Earth.
- Does not cross y-axis
- Curve starts at its most negative point at a certain x-value (RE - radius of the Earth)
- It then curves like a -1/x graph and never quite reaches the x-axis
(See diagram pg 122 of revision guide)
How can you work out the value of g at a certain point using a V-r graph for a point mass?
- Find the gradient at any point
* This is because g = -ΔV / Δr
Describe a graph of g against r for the Earth.
- Does not cross y-axis
- Curve starts at its highest point at a certain x-value (RE - radius of the Earth)
- It then curves like a 1/x graph and never quite reaches the x-axis
(See diagram pg 122 of revision guide)
How do you work out ΔV using a g-r graph?
- Area under the curve between two x-values
* Because -ΔV = g x Δr
Remember to practise drawing out all 3 gravitational field graphs. Also, practise finding different quantities from them.
Pgs 121 + 122 of revision guide
What is escape velocity?
- The velocity at which an object’s kinetic energy is equal to minus its gravitational potential energy
- It is the velocity at which an object must travel in order to escape a gravitational field
What is an object’s total energy when it travels at escape velocity?
- Zero
* Because the kinetic energy and GPE sum to 0 (since GPE is always negative)
What is the equation for escape velocity?
v = √(2GM/r)
Where:
• v = Escape velocity (ms⁻²)
• G = Gravitational constant = 6.67 x 10^-11 Nm²/kg²
• M = Mass of point mass (kg)
• r = Distance from centre of point mass (m)
NOTE: Not given in exam.
Derive the equation for escape velocity.
- KE = 1/2mv²
- GPE = -GMm/r
- 1/2mv² = GMm/r
- 1/2v² = GM/r
- v² = 2GM/r
- v = √(2GM/r)
What is the equation for GPE relative to G, M and r?
GPE = -GMm/r
This is derived from V = -GM/r
Is escape velocity dependent on the mass of the object?
No, it is the same for all masses in a gravitational field.
What is gravitational potential difference?
The energy needed to move a unit mass between two gravity sonar potentials.
What is the equation for the work done when moving an object through a gravitational potential difference?
ΔW = mΔV
Where:
• ΔW = Work fine (J)
• m = Mass (kg)
• ΔV = Gravitational potential difference (J/kg)
What are equipotentials?
Lines (in 2D) or surfaces (in 3D) that join all of the points with the same potential (V).
How much work is done when moving an object along an equipotential?
0J
Describe the equipotentials around a uniform spherical mass.
Spherical surfaces
Describe how equipotentials and field lines are related in gravitational fields.
They are perpendicular.
What force keeps an object undergoing circular motion in orbit?
Centripetal force
In the case of a satellite orbiting the Earth, what is the centripetal force?
Gravitational force