Atomic Concepts and Bright-Line Spectrum in Astronomy
Delve into the atomic concepts and the application of bright-line spectrum in identifying elements in stars. Explore the relationship between electrons, energy, and spectrum production. Discover the significance of spectrum types like continuous, emission, and absorption in scientific analysis. Engage with interactive demos and questions to deepen your understanding of atomic structures and spectral analysis.
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Presentation Transcript
ATOMIC CONCEPT OCTOBER 2, 2015
QUIZ 4 10/02/2015 Clear your desk PENCIL only 10 minutes Individual work and you are silent If you finish early, silently review your work NOTE: make sure to complete the header
NOTEBOOK CHECK NOTEBOOK CHECK 2 TODAY PUT IN GREEN BIN AT END OF CLASS REGENT PERIODIC TABLE ATOMIC TIMELINE DO NOW FOR 9/28 DO NOW FOR 9/30 DO NOW 10/1 COMPLETED QUESTIONS TO CONSIDER QUIZ 4
AIM How can bright-line spectrum be utilized to identify elements in a star?
Three Views Spectrum Demonstrator http://astro.unl.edu/classaction/animations /light/threeviewsspectra.html Point the flashlight directly at light bulb Point the flashlight at the gas cloud Point the flashlight at the gas cloud away from the light bulb
SPECTRUM CONTINUOUS SPECTRUM EMISSION SPECTRUM ABSORPTION SPECTRUM
BRIGHT-LINE SPECTRUM EMISSION SPECTRUM
HW-01-02 Q1: State the total number of valence electrons in a cadmium atom in the ground state.
Q2 Identify all the elements in the mixture
Q3 Explain, in terms of both electrons and energy, how the bright-line spectrum of an element is produced.
Q4 List all elements present in unknown sample W.
Q5 List all elements present in unknown sample X.
Q6 List all elements present in unknown sample Y.
Q7 List all elements present in unknown sample Z.
Q8 REAL LIFE APPLICATION How can bright-line spectrum be utilized to identify elements in a star?
HOMEWORK REMINDER Study for Quiz 3