P8.3 - Beyond Earth Flashcards

1
Q

What is the difference between an absorption spectrum and an emission spectrum?

A

Absorption spectrum - A continuous spectrum with dark lines corresponding to particular frequencies being absorbed by an atom.

Emission spectrum - A set of frequencies of radiation emitted by an atom when excited electrons move to lower energy levels.

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2
Q

What is the Doppler effect?

A

The physical phenomena by which there is a change in the observed frequency/wavelength of wave, due to relative motion between observer and source.

Relative motion - Source moving, OR observer moving, OR both source and observer moving.

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3
Q

What happens, in terms of the Doppler effect, when a sound source moves towards you?

A

When the sound source moves towards you, wave peaks move closer together, the wavelength decreases and the observed frequency/pitch of sound increases.

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4
Q

What happens, in terms of the Doppler effect, when a sound source moves away from you?

A

When the sound source moves away from you, wave peaks move further apart, the wavelength increases and the observed frequency/pitch of sound decreases.

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5
Q

Why is the the Doppler effect with light waves very difficult to observe?

A

The light waves have a much smaller wavelength than sound waves.

The Doppler effect is observed when the relative motion between the observer and the source is very large.

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6
Q

What is red-shift and what does it imply?

A

Red shift - The shift in wavelength of the light emitted from a source to longer wavelengths.

Implies - That the source is moving away from us.

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7
Q

What is blue shift and what does it imply?

A

Blue shift - The shift in wavelength of the light emitted from a source to shorter wavelengths.

Implies - That the source is moving towards us.

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8
Q

Describe how the red-shift of distant galaxies provides some evidence for the The Big Bang Theory.

A

OBSERVATIONS
Light from distant galaxies is red-shifted.
The further away the galaxy, the greater the red-shift.

CONCLUSIONS
Galaxies are moving away from us.
The further away the galaxy, the faster it is moving away.

Thus, if galaxies are moving away from each other, this suggests that at one point, all matter must have existed at a single point in space - One piece of evidence for the big bang.

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9
Q

How do we know light from distant galaxies are red shifted?

A

The absorption spectra of stars contain black lines.

These black lines correspond to very specific wavelengths of light absorbed by certain atoms in the star.

Hence, all spectra from starts contain a series of very specific black lines (distinct pattern of separated lines).

These black lines are seen shifted in the spectra from distant stars towards longer wavelengths.

This implies that light from distant stars have undergone a Doppler shift.

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10
Q

Describe how cosmic microwave background radiation provided evidence for the Big Bang theory.

A

At the beginning of the universe, all the energy of the universe would have manifested as very short wavelength gamma waves.

As the universe expanded, this gamma radiation would have stretched out to longer and longer wavelengthsโ€ฆ and is now microwave radiation.

The fact that the microwaves uniformly/evenly fill the universe suggests they all started off from a single point (filling the universe as the universe expanded).

The steady state theory cannot explain this fact, only the Big Bang Theory can.

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11
Q
What is/are:
The sun
Planets
Moons
Minor planets
Comets
A

The sun - Star at the centre of the solar system.

Planets - Spherical bodies that orbit the sun.

Moons - Spherical bodies that orbit planets.

Minor planets - Small spherical objects that orbit the sun.

Comets - Objects made of dust/ice that orbit the Sun with long period, elliptical orbits.

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12
Q

What are the inner planets and what are they made of?

A

Mercury - Atmosphere very thin, no moon

Venus - Atmosphere is mainly carbon dioxide and it rains sulfuric acid, no moon

Earth - One moon

Mars - Atmosphere very thin, two moons

  • Rocky
  • All have an atmosphere
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13
Q

What are the inner planets and their properties?

A

Gas giants - Jupiter and Saturn
Ice giants - Uranus and Neptune

All have rings and a lot of moons.

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14
Q

What is between Mars and Jupiter?

A

An asteroid belt - A band of dust and larger pieces of rock left over from the formation of the solar system and orbits the sun.

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15
Q

Describe the beginning of the life cycle for all stars.

A
  • Dust and gas gather under gravity to form a protostar.

- Once the protostar has become hot and dense enough, nuclear fusion begins and the star becomes a main sequence star.

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16
Q

Describe the middle stages in the life cycle for all stars.

A
  • A star is stable during its main sequence.
  • The radiation pressure outwards from nuclear fusion balances the gravitational attraction inwards (there is equilibrium/stability).
  • Eventually, the hydrogen nuclei will run out.
  • The star will cool, and its radiation pressure drops.
  • The gravitational force collapses the star, causing it to heat up again.
  • The fusion of heavier elements begins.
  • The energy from fusion increases. Therefore, the radiation pressure increases. The star becomes either a red giant or a red super giant.
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17
Q

What is the ending steps for the life cycle of a small star (a red giant)?

A
  • The nuclei for fusion run out.
  • Fusion slows down.
  • Radiation pressure decreases.
  • The gravitational force collapses star.
  • The star heats up becomes a white dwarf.
  • The star eventually cools down to form a black dwarf.
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18
Q

What is the ending steps for the life cycle of a large star (a red super giant)?

A
  • Lots of heavier nuclei fused together to release lots of energy.
  • There is a large increase in radiation pressure outwards. This is much larger than the gravitational pull inwards.
  • The star explodes in a supernova.
  • A very dense neutron star forms.
  • If the neutron star is very dense, it could become a black hole.
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19
Q

What is the life cycle for a low mass star?

A

Protostar - Main sequence star - Red giant - White dwarf - Black dwarf

What is the life cycle for a high mass star?
Protostar - Main sequence star - Red super giant - Supernova - Neutron star - If these is a very high density - Black hole

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20
Q

Explain why the sun started to shine.

A

Once the sun became hot and dense enough under gravity, nuclear fusion of nuclei began, releasing energy, causing the sun to emit EM radiation and shine.

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21
Q

Explain why the sun is not expanding?

A

There is a balance between the force of gravity inwards and the radiation pressure from nuclear fusion outwards, that ensures the sun does not expand or contract.

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22
Q

Suggest why the outer planets have many more moons than the inner planets.

A

Outer planets have more mass than the inner planets.

Thus, their gravitational fields and stronger.

When the solar system was forming, the outer planets attracted more dust/gas towards them.

This dust/gas came together under gravity to form the many moons of the outer planets.

23
Q

What type of star is our sun?

A

A small star.

Currently a main sequence star.

24
Q

What is a satellite?

A

A satellite is any body that orbits a planet or star.

25
Q

What are examples of natural satellites and artificial satellites?

A

Natural satellites - The moon is a satellite of Earth. Earth is a satellite of the sun.

Artificial satellites - Communication satellites in orbit about Earth.

26
Q

What are the two types of orbit that a satellite may orbit the Earth in?

A

Satellites that orbit the Earth do so in one of two types of orbit. Either a geostationary orbit or a polar orbit.

27
Q

Give information about satellites that orbit the Earth in a geostationary orbit.

A

Orbital time period = 24 Hours.

Orbital height = 36,000km.

The satellite is launched above the equator. The satellite remains in a fixed position relative to Earth. This is also why satellite dishes down a road face the same way.

Examples = Communications/GPS, television.

28
Q

Give information about satellites that orbit the Earth in a polar orbit.

A

Orbital time period = 100 minutes.

Orbital height = 2000km.

The satellites are launched about the poles. Therefore, the satellites rotate about the Earth once every 100 minutes, as the Earth rotates under it. The satellite can scan the entire surface of the Earth, very quickly.

Examples = Weather, spy satellites.

29
Q

Why must you get the correct satellite orbit velocity?

A

The velocity you launch a satellite at (in its orbitโ€ฆ not on the way up to space!) will determine the radius the satellite orbits the Earth at, and hence the time period of orbit.

30
Q

What is an elliptical orbit?

A

Almost all planets orbit their star in an elliptical orbit.

An elliptical orbit differs from a circular one in that its radius isnโ€™t fixed.

However, at any given point in the orbit, we can treat the planet as moving in a circular orbit of a given radius.

31
Q

Explain the idea of centripetal force?

A

A body in a circular orbit is constantly accelerating, as the direction of its velocity is constantly changing.

Hence, a resultant force must be acting upon a planet orbiting its star.

A resultant force that causes a body to perform circular motion is known as the centripetal force.

The centripetal force for a planet is provided by the gravitational attraction of its star.

32
Q

Explain how the speed of a satellite never changes.

A

The centripetal force/gravitational attraction always attracts towards the centre of the circular motion/orbit.

The centripetal force on any body always acts perpendicular to the bodyโ€™s velocity.

Therefore, the speed of the body never changes, just the direction.

33
Q

What is a stable orbit?

A

A stable orbit maintains a constant radius about the body its orbiting.

34
Q

What happens if a satellite moves too slow or too fast?

A

If a satellite moves too slow, gravitational attraction will put it in.

If a satellite moves too fast, gravitational attraction is not great enough to hold onto the body and it flies away.

35
Q

What depends on the velocity for a satellite in order for it to maintain a stable orbit?

A

The distance it is away from the Earth.

The further away a body is from the body it orbits, the slower its velocity needs to be to maintain a stable orbit, the longer its time period.

36
Q

What happens the greater the temperature of a body?

A

The greater the temperature of a body, the faster the particles vibrate. This means that EM waves of greater frequency are emitted. This is why bodies that glow blue are hotter than those that glow red.

37
Q

When will the temperature of a body increase and increase?

A

If a body absorbs more radiation that it emits, its temperature will increase.

If a body emits more radiation that it absorbs, its temperature will decrease.

38
Q

Describe the intensity of radiation at each frequency against

A

A hotter object emits more radiation of a higher frequency and less radiation of a lower frequency.

The graph for a hot star peaks over a higher frequency than the graph for a cool star.

The intensity at each frequency is higher for a hot star than a cold one.

39
Q

How does the Earthโ€™s atmosphere affect the temperature of the Earth?

A

The Earth absorbs radiation from the sun and emits radiation into space.

The Earthโ€™s atmosphere reflects some of the radiation back to Earth.

The Earth absorbs more radiation (via the greenhouse effect) from the sun than it emits back into space.

Hence, the temperature of the Earth is increasing.

40
Q

Describe the structure of the Earth.

A

The centre of the Earth is about 6370km below the Earthโ€™s surface.

The Earth has a solid inner core and a liquid outer core.

The mantle is almost entirely solid, but it can flow.

The crust (which we live on) is solid.

41
Q

What is the study of Earthquakes known as?

A

The study of earthquakes is known as seismology.

42
Q

When do earthquakes occur and what are seismic waves?

A

Earthquakes originate in the Earthโ€™s crust and occurs when forces inside the Earth become large enough to break and move layers of rock.

The energy transferred during an Earthquake creates shockwaves, seismic waves.

Seismic waves travel through the Earth and across the surface of the Earth.

43
Q

What is the focus and epicentre of earthquakes?

A

The point where the seismic wave originates is called the focus.

The nearest point on the surface to the focus, is known as the epicentre of the earthquake.

44
Q

How are earthquakes recorded?

A

Earthquakes are recorded by detectors on the surface of the Earth, known as seismometers.

45
Q

What are the two different types of seismic waves?

A

1 - Primary waves (P Waves)

2 - Secondary waves (S Waves)

46
Q

Describe primary waves (P Waves).

A
  • Cause initial tremors lasting about 10 minutes.
  • Longitudinal waves that push and pull the Earth.
  • Can travel through solids and liquids.
47
Q

Describe secondary waves (S Waves).

A
  • Follows primary waves with more tremors a few minutes after.
  • Transverse waves that shake up and down the Earth.
  • Cannot travel through liquids.
48
Q

What happens to P and S waves as they travel through the Earthโ€™s crust?

A

P and S waves refract/bend slowly as they travel through the solid crust. This is because the density of the crust slowly changes as you travel further into the Earth.

49
Q

What happens to P and S waves at the boundary between the mantle and the outer core?

A

At the boundary between the mantle and the outer core, the P and S waves refract a lot, because their speed suddenly changes a lot. This is because there is a large difference in density between the solid mantle and liquid outer core.

50
Q

Why are S waves not detected on the other side of the Earth?

A

S waves cannot travel through the liquid core, so are not detected on the other side of the Earth, producing S-wave shadow zones.

51
Q

How a P-wave shadow zones created?

A

P waves are refracted a lot as they cross the mantle/outer core boundary, creating regions where they are not detected, producing P-wave shadow zones.

52
Q

Explain how seismic waves detected around the world show that part of the Earth is liquid.

A

P-waves are longitudinal and can travel through solids and liquids.

S-waves are transverse and can only travel through solids.

Following an earthquake, P-waves are detected on the other side of the Earth, but S-waves are not detected.

This implies S-waves were unable to pass through part of the Earth.

Part of the Earth must therefore be liquid.

53
Q

Why do the path of waves in the mantle curve and what does this tell you about the mantle?

A

The waves refract/bend as they travel through the Earth. Since refraction is a wave phenomenon that only occurs when waves cross the boundary between two media, we can tell that the mantle contains layers of different densities, such that boundaries between media exist, giving rise to refraction.