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Nuclear Weapons. Units of Radiation Dose. Roentgen – Ability to create a specified electric charge per volume of air Rem (Roentgen equivalent man) –Biological effect of one roentgen of X-rays Rad (Radiation absorbed dose) – Energy absorption: 400,000 rads heat H 2 O 1 deg
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Units of Radiation Dose • Roentgen – Ability to create a specified electric charge per volume of air • Rem (Roentgen equivalent man) –Biological effect of one roentgen of X-rays • Rad (Radiation absorbed dose) – Energy absorption: 400,000 rads heat H2O 1 deg • For general human exposure, these units are roughly equivalent
Background Radiation • Cosmic Rays • Solar Wind • Decay of Natural Radioactivity • Typical Doses • Global Average 0.1 rem/year (80% natural) • Some areas up to 1 rem/year • Ramsar, Iran: up to 26 rem/year
Human Radiation Sources • Nuclear Fallout from Atmospheric Testing (US and Russia, 1963; France, 1974; China, 1980) • Chernobyl 1986 • Uranium Mining • Radon release from construction and earth-moving • Conventional power plants
Human Survival Limits • 200 rem (whole body): few immediate fatalities • 500 rem (whole body): 50% fatalities • 1000 rem (whole body): No survivors
Nuclear Fission • Chain reaction requires a critical mass to proceed • 10 kg U-235 = 2.5 x 1025 atoms • 1,2,4,8 … 2.5 x 1025 = 85 steps • @ 1/1,000,000 sec per step = 1/10,000 sec • After 64 steps, T = 10,000 K (twice as hot as sun) • Have only completed 1/1,000,000 of fission
Nuclear Weapons To get a nuclear explosion, you have to • Assemble a critical mass in millionths of a second • Retain a high percentage of the neutrons • Hold the material together against temperatures hotter than the Sun • Imposes limits on yield of weapon • Unless something is specifically designed to be a nuclear weapon, it will not explode
Yields of Nuclear Weapons • Kiloton = 1000 tons of explosives = 4.2 x 1012 joules = 1012 calories • Texas City, Texas, April 16-17, 1947 • Collapse of World Trade Center • Impact of 10-m asteroid • Megaton = 1,000,000 tons of explosives = 4.2 x 1015 joules = 1015 calories • Magnitude 7 earthquake • Impact of 100-m asteroid
Effects of Nuclear Weapons • Direct ionizing radiation • Heat (Fireball) • Rising fireball sucks dust upward, creates “mushroom cloud” • Any large explosion will create a “mushroom cloud” • Blast (Expansion of Fireball) • Fallout • Volume α Yield: Radius α3√Yield
Weapons Terminology • Warhead: The Actual Explosive Component of a Nuclear Weapon • Warhead Section: The Delivery Casing for a Nuclear Weapon. Includes casing, radars, timers, detonators, etc • When most people say “Warhead,” they actually mean “Warhead Section.” • Tactical = Range < 500 km • Strategic = Range > 500 km
Some Nuclear Factoids • Nuclear weapons are always under armed guard • Nobody Ever Goes Near a Nuke Alone. U.S. Protocols Call for a “Two Man” Rule • There are persistent rumors we allowed designs of our locking mechanisms to be leaked to the Russians • Information on locations of nuclear weapons is classified “Secret” or above • Do not confirm/deny
Nuclear Weapons Systems • All military explosive weapons have had nuclear versions • Artillery Shells • Bombs • Depth Charges • Rockets • Missiles • Anti-Aircraft • Stationary charges
Nuclear Winter • Publicized by Carl Sagan and others in 1980’s • Global nuclear exchange would raise large amounts of dust and soot into upper atmosphere • Would absorb or reflect sunlight, cooling the surface • Would be above most precipitation processes • Did not happen in Gulf War 1991
Fusion • Natural: how stars (and the sun) generate energy • Artificial and uncontrolled: Thermonuclear Weapon (hydrogen bomb) • Fusion Reactor: controlled • “Energy source of the future. Always has been, always will be.”
Core of the Sun • Energy output: 90 billion megatons/second • Energy output = 6 microwatts/kg – less than a candle • Human body outputs 1.2 W/kg – 200,000 times greater • Trying to duplicate sun’s energy output not practical on Earth • Energy takes 10,000 – 100,000 years to reach surface
Uncontrolled Fusion • We cannot achieve T and P necessary to use ordinary hydrogen • Have to use H-2 (deuterium) or H-3 (tritium) • Still need T = 1,000,000 K+ • Initiated by a nuclear (fission) weapon • Fission weapons yield up to 20 kilotons • Fusion (hydrogen or thermonuclear) weapons yield up to 20 megatons
Controlled Fusion • Temperatures too high for any material • Need to contain by magnetic fields, achieve small-scale reactions for short periods • Have not achieved break-even • Apparatus will be incredibly complex and expensive • Reactions give off neutrons: there will still be radioactive waste • No spent fuel or fissionable residue
Detecting Nuclear Explosions • Vela System (US) • Space: X-ray and Gamma Ray pulses • Atmospheric: • Double-humped light pulse • Initial Fireball • Obscured by ionized gas in shock wave • Revealed again as shock wave cools • Vela Incident, September 22, 1979 • Subsurface: Seismic First Motion Analysis