lecture15 fission v2 - university of...
TRANSCRIPT
Nuclear Fission
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Einstein:
(1905) Albert Einstein: He comes up with a little formula you may have heard of:
This equation changes everything.
E = mc2
1 g = 9 x 1013 J (equivalent to burning 1000 tons of coal!!!)
Binding energy of helium nucleus can be calculated:
4 x 1.67x10-27 kg 6.644 x 10-27 kg
Mass of 2 protons and 2 neutrons : Mass of a helium nucleus:
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Einstein:
(1905) Albert Einstein: He comes up with a little formula you may have heard of:
E = mc2
Binding energy of helium nucleus can be calculated:
4 x 1.67x10-27 kg - 6.644 x 10-27 kg = 3.6 x 10-29 kg
Binding Energy
Mass difference:
Ebind = mc2 = (3.6x10-‐29 kg) x (3x108 m/s)2 = 3.2x10-‐12 J = 20.2 MeV
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Fusion vs. Fission Fission is • the breaking apart of a nucleus • what occurs during radioacPve decay • naturally occurring and happens in power plants
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Fusion vs. Fission Fusion is • the combining of two nuclei to form a heavier nucleus • what occurs inside the core of the Sun • the magic bullet for solving human energy problems…
or maybe not
Fission vs. Fusion • If Fusion is the process of obtaining energy by adding things together.
• Then Fission is the process of obtaining energy by Breaking things apart.
• A fissionable element can spontaneously decay into one or more different (lighter) elements, releasing energy as it decays.
• The 238U reaction is SLOW, taking 4.5 billion years!
238U ⇒ 234Th + 4He + (4.2 MeV)
(92P+146N) (90P+144N)
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Fission Power Generation • Stimulated Fission occurs when the interaction with another particle triggers element breakup.
• Fission reactors operate on this principle using a stable isotope of Uranium, 235U. About 0.7% of natural U is 235U.
235U + n ⇒ 140Cs + 93Rb + 3n (+ 200MeV)
(92P+143N) (55P+85N) (37P+56N)
• This reaction is easier to trigger than P-P fusion because both the neutron and 235U are neutral.
• It produces a LOT of energy per reaction, but not as much per mass as 3He fusion.
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The 235U Chain Reaction Did you notice that a byproduct of 235U fission by
neutron collision is MORE neutrons?
The 235U chain reaction is self sustaining when natural uranium is enriched to 5% of 235U.
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n
Need something to slow down reacPon and prevent it going “criPcal”
Fission Power Plant
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The 235U Reactor:
• Nuclear generators work by starting a chain reaction in Uranium that is enriched in 235U.
• 235U reactors produce toxic materials including both ‘depleted’ rods and the containment vessel.
• The rate of the chain reaction rate is managed by;
1. By inserting control rods to block neutrons.
2. By cooling the reactor core to slow neutrons.
• Failure to control the reaction leads to a runaway or meltdown. (Chernobyl + 3 mile Island)
The Down Side:
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Some Basic Reactor Designs:
• PWR/BWR: Regular water (coolant), carbon control rods (moderator) and enriched Uranium (fuel)
• PHWR: Heavy water (coolant/moderator) and natural Uranium (fuel)
• RBMK: Regular water (coolant), graphite moderator, and natural Uranium (fuel) – VERY unstable
• LMFBR: Liquid metal (coolant/moderator), various natural fuel sources (Uranium, Thorium)
• IFR: Like an LMFBR but recycles the fuel • And many, many others….
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Natural Fission Reactor : • Oklo – Gabon, Africa
• Like HWR without the heavy water
• 1.7 billion years ago, the abundance of U235 much higher (3.1%, now 0.7%)
1) Nuclear reactor zone 2) Sandstone 3) Uranium ore layer 4) Granit 5) Water
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RTGs :
Radioisotope thermoelectric generator
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RTGs :
RTGs used on Pioneer 10 & 11, Voyager 1 & 2, Galileo, Ulysses, Cassini, New Horizons, MSL, Viking landers, Apollo 12-‐17 Typically provide a few 100 Waks of power for 50-‐100 years. Because RTGs contain plutonium and other highly radioacPve material, they can be more dangerous to launch that a fission reactor
Nuclear Power
Courtesy of Fox TV
7% of World’s Power Plants
16% of World’s Electricity No new Nuclear Power Plants in the US since the 1970s.
Should we build more plants?
What about coal?
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Power in Space
• No such things as hydro-‐power or wind power in space
• Solar power is possible but increasingly limited pasts Mars’ orbit
• All past or current missions going to Jupiter and beyond used a form of power based on radioacPve decay
• Juno mission will use solar panels: >10 kW at Earth but only 480 W (max) at Jupiter
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Solar Flux in the Solar System
• 1365 W/m2 at the top of the Earth’s atmosphere (about 1000 W/m2 at noon
at equator at the surface) • Decreases with (distance)2 : Flux * R2 is const. • Flux at Mars = (1365 W/m2)*(1.0/1.5)2
= 607 W/m2 • Flux at Jupiter = 55 W/m2
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Solar Flux at Mars • Flux at MarPan surface ~ 590 W/m2 (max) • Solar Panels the size of a football field (ISS)
= 3200 kW intercepted • Solar Panels 10 m x 10 m
= 59 kW • But solar panels not 100% efficient, best ones
today 30% è 960 kW / 18 kW ISS: 14%è 448 kW / 8 kW
• Average person uses 250 kW a month, 9 kW day
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