Chapter 42: Q. 8 (page 1236)
Calculate (in ) the total binding energy and the binding energy per nucleon for and for .
Short Answer
For atom, Binding energy =
Binding energy per nucleon =
For atom, Binding energy =
Binding energy per nucleon =
Chapter 42: Q. 8 (page 1236)
Calculate (in ) the total binding energy and the binding energy per nucleon for and for .
For atom, Binding energy =
Binding energy per nucleon =
For atom, Binding energy =
Binding energy per nucleon =
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Get started for freeThe technique known as potassium-argon dating is used to date old lava flows. The potassium isotope 40 K has a 1.28-billionyear half-life and is naturally present at very low levels. 40 K decays by two routes: 89% undergo beta-minus decay into 40 Ca while 11% undergo electron capture to become 40 Ar. Argon is a gas, and there is no argon in flowing lava because the gas escapes. Once the lava solidifies, any argon produced in the decay of 40 K is trapped inside and cannot escape. A geologist brings you a piece of solidified lava in which you find the 40 Ar/ 40 K ratio to be 0.013. What is the age of the rock?
137 Cs is a common product of nuclear fission. Suppose an accident spills 550 mCi of 137 Cs in a lab room.
a. What mass of 137 Cs is spilled?
b. If the spill is not cleaned up, how long will it take until the radiation level drops to an acceptable level, for a room this size, of 25 mCi?
Stars are powered by nuclear reactions that fuse hydrogen into helium. The fate of many stars, once most of the hydrogen is used up, is to collapse, under gravitational pull, into a neutron star. The force of gravity becomes so large that protons and electrons are fused into neutrons in the reaction . The entire star is then a tightly packed ball of neutrons with the density of nuclear matter.
a. Suppose the sun collapses into a neutron star. What will its radius be? Give your answer in .
b. The sun's rotation period is now 27 days. What will its rotation period be after it collapses?
Rapidly rotating neutron stars emit pulses of radio waves at the rotation frequency and are known as pulsars.
Calculate the mass, radius, and density of the nucleus of .
Give all answers in SI units.
a. Draw energy-level diagrams, similar to Figure 42.11, for all nuclei listed in Appendix C. Show all the occupied neutron and proton levels.
b. Which of these nuclei is stable? What is the decay mode of any that are radioactive?
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