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Astronomy The Stars Star cluster NGC 457, the Owl Cluster, in the constellation of Cassiopeia http://www.buytelescopes.com/gallery/view_photo.asp?pid=10298&sg=9&page=3
Distances to the Stars ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Stellar Parallax ,[object Object],[object Object],Earth in summer Earth in winter Star close to our sun
Parallax Animation http://www.astro.washington.edu/labs/parallax/solar.html Cool parallax demo:
Arc Seconds ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Parsec ,[object Object],[object Object],[object Object],[object Object],[object Object]
Newton’s Prism Experiment (1665) ,[object Object],[object Object],[object Object]
Visual Spectrum
Overhead Spectra Demo ,[object Object]
Spectrum of Light ,[object Object],[object Object],[object Object]
Spectra of Stars ,[object Object],[object Object],[object Object],[object Object]
Three Types of Spectra Solid array of rainbow colors Mostly dark with a few brightly colored lines Mostly continuous but with a few missing dark lines
Spectral Tube Demo ,[object Object]
Animation ,[object Object]
Spectroscope
Elements ,[object Object],[object Object],[object Object],[object Object]
Bohr Model ,[object Object],[object Object]
Bohr Model of Nitrogen ,[object Object],[object Object],Nucleus Energy levels http://education.jlab.org/qa/atom_model.html
Binding Energy ,[object Object],[object Object]
Jumping Electrons ,[object Object],[object Object],[object Object],[object Object]
Excite Me ,[object Object],[object Object]
Animation ,[object Object]
Emission Lines ,[object Object],[object Object],Emission spectra of various elements
Emission Spectrum of an Element By analyzing the light of a burning element in the laboratory, its unique bright spectral lines can be observed and recorded
Absorption Lines ,[object Object],[object Object],[object Object],[object Object]
Spectra of Hydrogen ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Stellar Spectra ,[object Object],[object Object],[object Object],[object Object]
Absorption Spectra O B A F G K M Coolest stars Hottest stars ,[object Object],[object Object],[object Object]
Stellar Spectra Spectral Classes Cooler stars display more absorption lines
Chemical Composition of Stars ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Fraunhofer Lines Some of Fraunhofer’s original drawings of the sun’s spectrum
Stellar Elements Comparison of the sun’s absorption spectrum with the emission spectrum of iron allows the identification of iron in the sun’s outer atmosphere
Betelgeuse Spectra ,[object Object]
Spectral Classes ,[object Object],[object Object]
Politically Incorrect
Temperature of Stars ,[object Object],[object Object],[object Object],[object Object],[object Object]
Spectral Class and Star Color ,[object Object],[object Object],Click:  Stellar Spectra Mini Exercise
Star Colors: Big & Little Dippers Where is Polaris?
Orion Betelgeuse Rigel ,[object Object],[object Object],Belt Sword Orion Nebula in Sword of Orion
Andromeda www.scienceandart.com Galaxy (M31) The Andromeda Galaxy is visible to the naked eye—at 2.3 million light years it is the most distant object visible to the naked eye
Planck Curves and Blackbodies ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
3 Planck Curves ,[object Object]
[object Object],[object Object],[object Object],[object Object],[object Object],Wien’s Law governs the peak wavelength, Stephan-Boltzmann governs the intensity
Stars and Blackbodies (Planck Curves) ,[object Object],[object Object],[object Object],[object Object]
Blackbody Radiation Example ,[object Object],[object Object],WHEN FIRST HEATED THE POKER GLOWS DIMMLY AND IS RED AS THE TEMPERATURE RISES, THE POKER BECOMES BRIGHTER AND GLOWS ORANGE AT HIGHER TEMPERATURES THE POKER BECOMES EVEN BRIGHTER AND GLOWS YELLOW
Stars emit light that is close to an ideal blackbody.  We can estimate the surface temperature of a star by examining the intensity of emitted light across a wide range of wavelengths.
Summary : Properties of Stars ,[object Object],[object Object],[object Object]
Apparent Motion of Stars ,[object Object],[object Object],[object Object]
Stars Move Through Space ,[object Object],[object Object],[object Object],[object Object],[object Object]
Sun’s Revolution in Milky Way http://www.envirotruth.org/images/graphics/suns_path.jpg ,[object Object],[object Object],[object Object]
Space Motions of Stars ,[object Object],[object Object],[object Object],[object Object]
Star Motions ,[object Object],[object Object],[object Object],[object Object],[object Object],star  The star moved along the blue arrow in the observation period
Doppler Shift ,[object Object],[object Object],[object Object],[object Object]
Doppler Shift of Sound S = A moving source of sound such as a train whistle Observer 2 hears a higher pitch whistle, and the pitch drops suddenly when the source passes Observer 1 hears a lower pitch whistle than observe 2 For observer 2, the waves are pushed together
Doppler Shift cont. ,[object Object],[object Object]
Blueshift and Redshift ,[object Object],[object Object]
Redshift ,[object Object],[object Object],Reference Twin spectral lines
Proper Motion ,[object Object],[object Object],[object Object]
Slow Motion ,[object Object],[object Object],[object Object]
Big Dipper Proper Motion
Barnard’s Star ,[object Object],[object Object]
61 Cygni Proper Motion http://www.almanak.hi.is/61cygni.html
Hipparcos Web Site ,[object Object],[object Object]
Luminosity ,[object Object],[object Object],[object Object],[object Object],[object Object]
Propagation of Light ,[object Object],[object Object],[object Object]
Propagation ,[object Object],[object Object],[object Object],[object Object],[object Object],Each sphere represents the same amount of light from the star Star
Apparent Magnitude ,[object Object],[object Object],[object Object],[object Object]
Modern Magnitude Scale ,[object Object],[object Object],[object Object],Magnitude scale from a star map
Magnitude Scale ,[object Object],[object Object],[object Object],> Mag = < Bright The magnitude scale can be considered a type of number line 8-in BN
Little Dipper Magnitudes ,[object Object],[object Object],Polaris is a 2 nd  magnitude star
Absolute Magnitude ,[object Object],[object Object],Sirius is the brightest star in our sky, which star, Sirius or Polaris, is truly the brightest? Star Polaris Sirius Apparent  Magnitude +2.3 -1.5 Absolute  Magnitude -4.6 +1.4 Distance 240 Parsecs 2.7 Parsecs
Apparent & Absolute Magnitudes http://media.skytonight.com/images/Sirius_Mags_m.gif ,[object Object],[object Object]
Comparisons Star App Mag Abs Mag Spectral Class Parallax Alpha Centauri -0.3 4.1 G 0.750” Thuban 4.7 5.9 K 0.176” Barnard’s Star 9.5 13.2 M 0.545” Altair 0.8 2.3 A 0.202”
Comparisons Cont. ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Comparisons Cont. ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
H-R Diagram ,[object Object],[object Object],[object Object],[object Object]
[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],H-R Diagram cont.
H-R Diagram Sun
H-R Diagram again Click http://en.wikipedia.org/wiki/Hertzsprung-Russell_diagram
HR Diagram Regions http://zebu.uoregon.edu/~soper/Stars/hrdiagram.html
Main Sequence ,[object Object],[object Object],[object Object],[object Object]
Mass-Luminosity Relationship ,[object Object],[object Object],http://zebu.uoregon.edu/~soper/Stars/hrdiagram.html
Sizes of Stars ,[object Object],[object Object],[object Object],[object Object],[object Object]
Main Sequence Star Sizes
Giant Star Example The star V838 Monocerotis would extend beyond the orbit of Mars in our solar system
Double Stars ,[object Object],[object Object],[object Object],[object Object],[object Object]
Albireo ,[object Object],[object Object],[object Object]
Northern Cross ,[object Object],[object Object],[object Object]
Dog Star and Pup ,[object Object],[object Object],Orbital diagram of the Sirius system. Closest separation occurred in 1997 Sirius Sirius B (“Pup”)
Canis Major http://www.winshop.com.au/annew/CanisMajor.html Sirius
150 Binary Stars ,[object Object]

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Notes de l'éditeur

  1. pp. 504-506
  2. pp. 159-163
  3. pp. 507-510
  4. pp. 163-165
  5. From space, (as this diagram shows) the Sun’s spectrum peaks in the blue-green wavelengths. The Sun appears yellow to us because our atmosphere scatters the shorter wavelength blue light.
  6. pp. 166-167
  7. pp. 595 (Special Topic)
  8. pp. 502-507
  9. pp. 513-517
  10. pp. 510-512