Module 5: Newtonian World and Astrophysics Flashcards

1
Q

What are energy levels?

A

The name of the discrete set of energies that electrons of atoms in a gas can exist in

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2
Q

Why are the energy level of gaseous atoms negative?

A

Energy is required to remove an electron.

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3
Q

What does if mean is an electron has an energy of zero?

A

It’s free from the atom.

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4
Q

What is the ground state (Energy levels)?

A

Most negative energy level.

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5
Q

What does it mean when an electron has been “excited”?

A

It has moved from a lower energy level to a higher energy level.

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6
Q

What happens if a photon doesn’t have enough energy to free an electron?

A

If it has just enough energy to move it up an energy level, it excites the electron. This energy is the difference in energy between the two energy levels.

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7
Q

What happens once electrons have been excited?

A

They go back down to the lowest energy level they can and emit a photon, and when this light is diffracted, you get an emission line spectrum.

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8
Q

What is a spectrum?

A

A graph of intensity vs frequency.

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9
Q

What is a line spectrum?

A

A series of lines against a background formed by the diffraction of light emitted from excited electrons.

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10
Q

What are the three types of spectra?

A

Continuous spectra: The diffraction of white light produces this spectrum.

Emission line spectra: The result of the diffraction of photons emitted when electrons move to lower energy levels, the colourful lines indicate different energies and are against a dark background.

Absorption line spectra: Similar to emission line spectra but there are dark lines against a continuous spectrum.

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11
Q

What are the similarities and differences between emission and absorption line spectra?

A

Similarity: Lines appear at the same frequencies / positions

Difference: Emission is coloured lines against a dark background, while absorption is dark lines against a coloured background

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12
Q

What is required for an object to undergo uniform circular motion?

A

There must be a resultant force of constant magnitude that is always directed radially inward. This force is called the centripetal force.

Acceleration must be perpendicular to velocity.

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13
Q

Why is speed constant during uniform circular motion?

A

Resultant force and motion are perpendicular, so no work is done in the direction of motion.

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14
Q

Name some examples of sources of centripetal forces.

A
  • Friction
  • Tension
  • Gravitational force
  • Changes in normal contact force
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15
Q

Define simple harmonic motion.

A

When a system oscillates about its equilibrium position in a periodic manner.

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16
Q

What is the defining equation for simple harmonic motion?

A

a = -ω²𝑥

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17
Q

Describe simple harmonic motion.

A

When displaced from equilibrium, a restoring force acts towards equilibrium, the size of which is directly proportional to displacement but in the opposite direction.

18
Q

What equation can be used to find the time period of a pendulum?

A

T = 2𝛑 √(l/g)

Where l is the length of the pendulum and g is the acceleration due to gravity.

19
Q

What equation can be used to find the time period of a mass on a spring?

A

T = 2𝛑 √(m/k)

Where m is the mass of the masses and k is the spring constant of the spring.

20
Q

How is energy transferred in a pendulum system?

A

At the highest point: Maximum potential energy, zero kinetic energy.

As it swings down: Potential energy turns into kinetic energy.

At the lowest point: Maximum kinetic energy, zero potential energy.

As it swings up: Kinetic energy turns back into potential energy.

Energy continuously shifts between kinetic and potential energy as the pendulum swings, but total energy remains constant.

The graph for this has a sinusoidal shape.

21
Q

How is energy transferred in a horizontal mass-spring system?

A

At maximum displacement: Maximum elastic potential energy, zero kinetic energy.

Moving toward equilibrium: Elastic potential energy turns into kinetic energy.

At equilibrium: Maximum kinetic energy, zero elastic potential energy.

Moving away from equilibrium: Kinetic energy turns back into elastic potential energy.

Energy continuously shifts between kinetic and elastic potential energy as the mass moves but total energy remains constant.

The graph for this has a sinusoidal shape.

22
Q

How is energy transferred in a vertical mass-spring system?

A

At maximum displacement (compression): Maximum elastic potential energy and gravitational potential energy, zero kinetic energy.

Moving toward equilibrium (down): Elastic potential energy and gravitational potential energy turn into kinetic energy.

At equilibrium: Maximum kinetic energy, lower elastic potential energy and lower gravitational potential energy.

Moving away from equilibrium (down): Kinetic energy turns back into elastic potential energy (extension) and lower gravitational potential energy unit at maxium extension (EPE is max, KE is 0).

Energy shifts between elastic potential, gravitational potential, and kinetic energy as the mass moves but total energy remains constant.

23
Q

What is damping?

A

Damping is the process by which a system loses energy over time due to external forces (such as friction or air resistance), causing the amplitude of oscillations to decrease.

24
Q

Describe light damping.

A

The amplitude of oscillations decreases gradually over time.

The system oscillates for a long time before coming to rest.

The frequency of oscillation remains almost the same.

25
Q

Describe critical damping.

A

Amplitude of the oscillations is reduced to zero in the shortest possible time, returning the system to the equilibrium point.

This is the ideal case for stopping oscillations without overshooting the equilibrium

26
Q

Describe heavy damping.

A

When a system returns to equilibrium slowly without oscillating.

27
Q

Describe resonance.

A

Resonance occurs when a system is driven at its natural frequency, resulting in a large increase in amplitude. This happens because the driving force is applied at the frequency at which the system naturally wants to oscillate.

28
Q

What is natural frequency?

A

Every oscillating system has a natural frequency, the frequency at which it oscillates when no external driving or damping force is applied.

29
Q

What is a driving force?

A

An external force applied to the system that keeps it oscillating

30
Q

How are amplitude and frequency related?

A

The amplitude of oscillations depends on the frequency of the driving force (bell shaped graph). At resonance, this amplitude reaches its maximum as the frequency of the driving force matches the natural frequency of the system.

31
Q

What are the advantages of resonance?

A
  • Efficient energy transfer (e.g., radios, microwaves).
  • Enhances performance (e.g., musical instruments, sensors).
  • Key in medical imaging (e.g., MRI).
  • Useful in engineering applications (e.g., clocks, filters).
32
Q

What are the disadvantages of resonance?

A
  • Structural damage risk (e.g., bridges, buildings).
  • Unwanted noise/vibrations in machinery.
  • Safety hazards (e.g., aircraft, earthquakes).
  • Adds complexity to engineering design.
33
Q

What is Newton’s law of universal gravitation?

A

Two 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 distance between their centres.

34
Q

Define gravitational field strength.

A

The force per unit mass

35
Q

Define gravitational potential.

A

The work done per unit mass to move a small test mass from infinity to a point in the field a distance r from the centre of the attracting mass.

36
Q

Define gravitational potential energy.

A

The work done to move a test mass from infinity to a distance r from the centre of the attracting mass.

37
Q

What are equipotential surfaces?

A

Surfaces where the gravitational potential is constant and no work is required to move a mass along an equipotential surface.

38
Q

What is Kepler’s first law?

A

The orbit of a planet is an ellipse with the Sun at one of the two foci.

39
Q

What is Kepler’s second law?

A

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

This is because planets move faster when they are closer to the Sun and slower when they are farther away, ensuring that the area swept out over a given time remains constant.

40
Q

What is Kepler’s third law?

A

The square of the orbital period, T, of a planet of mass M, is directly proportional to the cube of the average radius, r, of its orbit.

T² ∝ r³, where k = 4π²/GM