Module 5 Flashcards

1
Q

Define temperature

A

How hot an object is

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2
Q

Define thermal equalibrium

A

No net flow of thermal energy

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3
Q

Define internal energy

A

The sum of the randomly distrubuted kinetic and potential energies of atoms or molecules within the substance

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4
Q

What happens during the melting or boiling point of a substance

A

Electrostatic potenial energy increases
Internal energy increases
Temperature stays the same

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5
Q

Define specific heat capacity

A

Energy required per unit mass to change the temparature by 1K

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6
Q

Circuit uncluded in specific heat capacity

A

Power supply
Switch
Variable resistor
Heater (voltmeter in parralel)
Ammeter

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7
Q

Define spacific latent heat

A

The amount of energy required to change the phase per unit mass while at constant tamperature

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8
Q

Solid to liquid energy

A

Specific latent heat of fusion

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9
Q

Liquid to gas energy

A

Spacific latent heat of vapourisation

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10
Q

Boyles law

A

p1V1=p2V2

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11
Q

Combined gas law

A

p1V1/T1 = p2V2/T2

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12
Q

How to find angle in radians

A

Arc length/Radius

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13
Q

Define centripital acceleration

A

Force that acts towards the centre of a circle

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14
Q

Equation for V in circular motion

A

V=2pir/T

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15
Q

EQ for Vmax in oscillations

A

V=2piFA
or V=wA

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16
Q

Define free oscillation

A

Allowed to osciallate without any external forces
Also known as natural frequency

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17
Q

Define forced oscillation

A

Driver force is applied to an oscillator and the object will vibrate at the driving frequency

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18
Q

Define resonance

A

If the driving frequency is equal to the natural frequency the onject will resonate causing a spike in amplitude

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19
Q

Keplars 1st law

A

The orbit of a planet is an ellipse with the sun at one of the 2 foci

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20
Q

Keplars 2nd law

A

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

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21
Q

Keplars 3rd law

A

The square of the orbital period of a planet is directly proportional to the cube of its average distance from the sun

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22
Q

Define gravitational potential

A

Work done per unit mass to move an object from infinity to a point in a gravitational feild

23
Q

How does moving from one point in a gravitational feild to another change gravitational potential

A

Moving away from a point mass increases gravitational potential

24
Q

Eq for GPE in cosmology

A

E=mV (v is gravitational potential)

25
Star sequence for star between 0.5 and 1M0
Nebula main sequence red giant planetary nebula White dwarf
26
Star sequence for star greater than 1M0
Nebula main sequence red supergiant supernova 2M core mass=Neutron star 3M core mass=Black hole
27
What is an excited atom
When an electron moves from a lower to a higher energy level within an atom in a gas This causes a photon to be emitted of the energy required to transition
28
Define emmission line spectra
Each element produces a unique emmision line spectrum because of its unique set of energy levels
29
Define continuous spectra
All visable frequencies or wavelengths are present. The atoms of a heated solid metal will produce this type of spectrum
30
Define absorbtion line spectra
This type of spectrum has series of dark spectral lines against the background of a continuous spectrum. The dark lines have exactly the same wavelengths as the bright emission spectral lines for the same gas atoms.
31
How are elements in stars detected
Absorbtion line spectrum If we know the line spectrum of a particular element
32
What light is used in a diffraction grating
Monochromatic
33
Under what circumstances are minima and maxima found
Minima = n x wavelength Maxima = (n+0.5) wavelength
34
Define 1 AU
Avr distance from earth to sun
35
Define parsec
Distance at which a radius of 1 AU subtends an angle of 1 arcsecond
36
1 arcsecond in degrees
1/3600
37
When is stellar parralax used to measure distance from the earth to an object
distances less than 100pc
38
Doppler effect in starlight
If the galaxy is blue shifted it is moving towards the earth red shifted= moving away
39
Hubbles law
Galaxies are red shifted so moving away from us The further away the galaxy is the faster it is moving away
40
State the cosmological principal
The universe is homogeneous (matter is distributed uniformly) and isotropic (the universe looks the same in all directions / there is no centre or edge to the universe
41
Evidence for the big bang
Microwave background radiation The expanding universe
42
Age of the universe
1/Ho
43
Name a similarity between molecules in a liquid and a solid at room temp
KEs are the same
44
Mass required for a white dwarf to form
Under 1.4 MO
45
Mass required for neutron star to form
2 MO
46
Mass required for black hole to form
>3 MO
47
What happens in red giants
fusion no longer takes place in the core as temp isnt high enough fusion occurs in the shell around the core these layers expand and cool
48
Order of events beginning of the universe
Universe starts to expand quarks and leptons form hadrons form nuclei form atoms form
49
How to find pascals from 1AU and arcseconds(d)
1/d
50
what can be used when answering a Q about root mean square speed or escape velocity
Maxwell boltzmann distribution
51
What is newtons law of gravitation
The force between two point masses is directly proportional to the product of their masses and inversly proportional to the square of their seperation
52
Stellar luminosity graphs in relation to temp
Higher temp = higher and to the left
53
Resonance graph in relation to damping
High damping = lower and to the left
54
Define luminosity
Total radiant power of a star