Introduction to Physical Science Monday Wednesday Thursday Tom
- Slides: 38
Introduction to Physical Science Monday, Wednesday, Thursday Tom Burbine tomburbine@astro. umass. edu
• Fission – Splitting of the nucleus of a heavy atom with the release of energy • Fusion – Combination of the nuclei of light atoms to form heavier nuclei with the release of energy
Energy Source for Sun • Fusing hydrogen into helium – Hydrogen nucleus – 1 proton – Helium nucleus – 2 protons, 2 neutrons • Need high temperatures for this to occur • ~10 to 14 million degrees Kelvin
http: //www. astronomynotes. com/starsun/s 3. htm
http: //www. astronomynotes. com/starsun/s 3. htm
How does Fusion Convert Mass to Energy • What is the most famous formula in the world?
E = mc 2 • • m is mass in kilograms c is speed of light in meters/s E (energy) is in joules very small amounts of mass may be converted into a very large amount of energy
Who came up with it?
http: //msnbcmedia 3. msn. com/j/msnbc/Components/Photos/z_Projects_in_progress/050418_Einstein/050405_einstein_tongue. widec. jpg
Law • Law of Conservation of mass and energy – Sum of all mass and energy (converted into the same units) must always remain constant during any physical process
Reaction • 4 protons → helium-4 + 2 neutrinos + energy Neutrino-virtually massless, chargeless particles Positron-positively charged electron – annihilated immediately by colliding with an electron to produce energy
Antiparticles • Antiparticle – particle with the same mass and opposite electric charge • Antiparticles make up antimatter • Annihilation – when a particle and an antiparticle collide • Antimatter is said to be the most costly substance in existence, with an estimated cost of $62. 5 trillion per milligram.
Fusion reaction • Much more complicated than 4 protons → helium-4 + 2 neutrinos + energy
Deuteron – Deuterium (hydrogen with a neutron) nucelus
Proton-Proton Chain Reaction • This reaction occurs ~1038 times each second • It if occurred faster, Sun would run out of fuel
Neutrinos • Neutrinos – almost massless particles • No charge • It takes a neutrino about 2 seconds to exit the Sun
Fusion • The rate of nuclear fusion is a function of temperature • Hotter temperature – higher fusion rate • Lower temperature – lower fusion rate • If the Sun gets hotter or colder, it may not be good for life on Earth
What is happening to the amount of Helium in the Sun? • A) Its increasing • B) its decreasing • C) Its staying the same
What is happening to the amount of Helium in the Sun? • A) Its increasing • B) its decreasing • C) Its staying the same
Valence Electrons • Electrons in the outermost occupied shell of an atom • Forms chemical bonds
Ion • Ion – an electrically charged particle created when an atom either loses or gains one or more electrons
Ionic Bond • Ionic bond – chemical bond in which an attractive electric force holds an opposite charge together
Covalent Bond • Covalent bond – a chemical bond in which atoms are held by their mutual attraction for two or more electrons share • Covalent bonds form molecules
Metallic Bonds • A chemical bond in which positively charged metal ions are held together within a “fluid” • Electromagnetic interaction between conduction electrons and gathered in an "electron sea“ • Atoms "share" electrons that float about in a general electron cloud
Charges need to balance • Na ions carry a +1 charge • Cl ions carry a -1 charge • Na+ + Cl- → Na. Cl (Sodium chloride)
• HCl – Hydrogen Chloride • Li 2 O – Lithium Oxide • CO – Carbon Monoxide • CO 2 – Carbon Dioxide
Any Questions?
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