P2.6 Nuclear Fission + Fusion Flashcards

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1
Q

Define nuclear fission?

A

The splitting up of a nucleus

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2
Q

Explain the process of a nuclear fission chain reaction.

A
  • Slow moving neutron is absorbed into uranium/plutonium nucleus
  • The nucleus becomes unstable and splits
  • This releases 2/3 neutrons which might hit another nucleus, keeping the reaction going
  • This also splits into 2 smaller nuclei which are radioactive (wrong number of neutrons in them)
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3
Q

What 2 types of fuel are usually used in nuclear fission?

A
  • Plutonium-239

- Uranium-235

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4
Q

Describe the process in a nuclear reactor.

A
  • Atomic nuclei split and release heat energy
  • This heats water to make stream
  • This drives a steam turbine connected to a generator
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5
Q

What is the advantage to nuclear fission?

A

Gives out a high amount of energy compared to a chemical reaction

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6
Q

What is are 3 disadvantages to nuclear fission?

A
  • Waste is very radioactive, hard to dispose of safely
  • High cost of power plant and decommissioning
  • Radiation leaks are dangerous
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7
Q

What happens in nuclear fusion?

A

Two light nuclei (e.g hydrogen) join to create a larger one, releasing energy

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8
Q

Where does nuclear fusion tend to happen?

A

In stars

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9
Q

What are the two advantages of nuclear fusion?

A
  • Gives out far more energy than fission

- No radioactive waste

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10
Q

What are the two disadvantages of nuclear fusion?

A
  • High temperatures and high pressures needed to hild hydrogen
  • You need a strong magnetic field
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11
Q

Name (don’t explain) the steps in the star cycle.

A
  • Protostar
  • Star birth
  • Main sequence star

Bigger than sun:

  • Super red giant
  • Supernova
  • Neutron star
  • Black hole (if star big enough)

Same size/smaller than sun:

  • Red giant
  • Planetary nebula
  • White dwarf
  • Black dwarf
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12
Q

What happens to make a protostar?

A
  • Stars form from dust and gas clouds

- Gravity makes this spiral in together (protostar)

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13
Q

How does the birth of a star occur?

A
  • When the gravitational energy is converted to heat energy so the temperature rises
  • When the temperature is high enough, hydrogen nuclei undergo nuclear fusion to form helium nuclei
  • This gives out massive amounts of heat and light
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14
Q

How does a star stay stable during its main sequence period?

A
  • Heat created by fusion creates outward pressure to balance gravity pulling everything inwards
  • Massive amounts of hydrogen consumption maintains energy output for millions of years
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15
Q

How long does a star stay as a main sequence star?

A

Several billion years

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16
Q

Why do stars become red giants/red super giants?

A
  • Eventually hydrogen begins to run out
  • Heavier elements e.g iron are made from the nuclear fusion of helium
  • Stars become red as the surface cools
  • The star swells
17
Q

What happens during a supernova?

A
  • Big stars glow brightly again
  • They undergo fusion and expand and contract several more times
  • This forms elements heavier than iron and ejects them into the universe - these form new planets and stars
18
Q

How do big stars become neutron stars?

A

The supernova throws out outer layers of dust and gas leaving behind a very dense core

19
Q

What happens during a planetary nebula?

A
  • The star becomes unstable
  • It ejects its outer layer of dust and gas
  • This leaves behind a dense and heavy core (white dwarf) which cools to become a black dwarf