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Radioactivity
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Isotopes Isotopes of an atom contain different numbers of neutrons
The ratio of protons to neutrons is related to the stability of the isotope The Band of Stability displays the ratios of protons to neutrons in a stable nucleus
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Radioisotopes An isotope with an unstable nucleus is known as a Radioisotope A radioisotope will undergo a spontaneous change in the nucleus in order to form a stable nucleus This process is known as Radioactivity or Radioactive Decay
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Radioactivity Radioactive nuclei give off particles and waves of electromagnetic radiation Radioactivity always results in a more stable nucleus Radioactivity also always results in a new element A Transmutation is a change in the identity of an atom after a change of the protons in the nucleus
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Radioactivity The three main types of radiation are: alpha radiation, beta radiation, and gamma radiation
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Alpha Radiation Alpha radiation results in the release of an Alpha Particle An alpha particle is a helium nucleus: two protons and two neutrons The mass of an alpha particle is 4 amu, and the charge is 2+ Alpha particles are low in energy and can be shielded by paper or clothing
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Nuclear Equations Radioactive decay is represented with a Nuclear Equation A nuclear equation must balance the mass numbers on both sides
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Alpha Radiation
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Beta Radiation Beta radiation is the result of the breakdown of a neutron Beta Radiation occurs when a neutron is converted to a proton and an electron The proton remains in the nucleus, and the electron is released from the atom Beta particles are negatively charged Beta radiation is stronger than alpha radiation, but can be blocked by aluminum foil or wood
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Beta Radiation
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Beta Radiation
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Gamma Radiation A high energy photon released by a radioisotope is called a gamma ray Gamma rays are often emitted along with an alpha or beta particle Gamma rays are very high in energy and must be shielded by lead or concrete
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Gamma Radiation
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Other types of Radioactive Decay
Other types of nuclear decay include: Positron Emission and Electron Capture
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Positron Emission If the ratio of protons to neutrons is too high, an atom may emit a Positron A positron is a positively charged particle with the mass of an electron The result of a positron emission is one more neutron and one less proton in the nucleus
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Electron Capture If the ratio of Protons to Neutrons is too high, the atom may undergo Electron Capture In electron capture, an electron is taken into the nucleus from its own atom The result of electron capture is one less proton, one less electron, and one more neutron
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Nuclear Fission When a radioisotope is bombarded with neutrons, it may split into smaller atoms This process is called Fission The fission process releases a high amount of energy Fission often results in a chain reaction Nuclear fission is the process used in nuclear power plants Uncontrolled chain reactions are the basis of atomic bombs
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Nuclear Fusion Nuclear fusion occurs when nuclei combine to create a nucleus of greater mass Nuclear fusion releases more energy than fission reactions Nuclear fusion is responsible for the energy provided by the sun
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Radiation Detection Radiation can be measured by several devices
Film badges use exposure of film to measure radiation exposure Geiger Counters detect radiation through electric pulses in ionized gas Scintillation counters measure radiation from substances that emit visible light when energy is absorbed
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Uses of Radiation Radioactive dating uses radioisotopes to determine the approximate age of an object Nuclear radiation is used to detect and kill cancerous cells
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Rate of Decay No two radioisotopes decay at the same rate
A Half-Life(t1/2) is the time required for half of the atoms of a radioisotope to decay A half-life can be as short as a fraction of a second, or billions of years
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Calculations with Half-Lives
The amount of radioactive isotope remaining can be calculated: Nt = No x (0.5)number of half-lives Where: Nt = amount of radioisotope remaining No = original amount of radioisotope number of half-lives = time ÷ half-life Manganese-56 is a beta emitter with a half-life of 2.6 h. What is the mass of manganese-56 in a 1.0-mg sample of the isotope at the end of 10.4 h?
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Calculating Half-Lives
To Calculate a Half Life: t1/2 = (.301)T log(N0/Nt) Where: Nt = amount of radioisotope remaining No = original amount of radioisotope T = Time of decay t1/2 = half-life
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