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103 Exam 2 Review. 12 November 2007. General Comments. 35 Multiple Choice Questions Concepts and Ideas Lecture Focused Review Slides Answer Practice Questions and understand them Review HW and Book Objects -- emphasis on the Sun. Topics to Review. Nature of Light Blackbodies
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103 Exam 2 Review 12 November 2007
General Comments • 35 Multiple Choice Questions • Concepts and Ideas • Lecture Focused • Review Slides • Answer Practice Questions and understand them • Review HW and Book • Objects -- emphasis on the Sun
Topics to Review • Nature of Light • Blackbodies • Kirchoff’s Laws • Doppler Shift • Telescopes • Parallax • Sun • Parts of the sun • Hydrostatic equilibrium (“sun’s thermostat”) • Sun’s source of energy (fusion)
Light • What are the relationships between wavelength, frequency, the speed of light, energy, etc? • How do a star’s brightness and luminosity change with distance? • What is the difference between blackbody emission and emission lines? What types of objects give this emission?
This is an inverse-square law – the brightness decreases as the square of the distance (d) from the source Light
Wien’s Law Stefan-Boltzman Law Light Gentle collisions Hard collisions
Telescopes • What is the difference between resolution and sensitivity? What do those terms mean? • What determines a telescope’s resolution? • What role to Earth’s atmosphere play in telescope design and placement? What telescopes go into space?
Telescopes • Sensitivity: Amount of light ResolutionRefraction, Dispersion, Diffraction
Sun • What keeps the sun balanced? • Where does the sun get its energy? • What defines the various parts of the sun? What makes them all interesting? • What is the “neutrino problem?” • What effects does the magnetic field in the sun lead to? (there are many)
Sun “Thermostat”
Sun FUSION! Requires high density, temp
Sun FUSION! Proton-Proton Chain Gives off a “neutrino”
Sun Other Things: Sun Spots Solar Wind Solar Flares
Sun Role of Magnetic Field: Heats corona Causes sun spots Leads to solar cycle