4 Light travels through empty space at a speed of 300,000 km/s In 1676, Danish astronomer Olaus Rømer discovered that the exact time of eclipses of Jupiter’s moons depended on the distance of Jupiter to Earth
5 Light travels at 300,000 km/sec About how fast does your car travel in km/hour when you are on the freeway?About how fast does your car travel in km/sec when you are on the freeway?If it takes light 8 minutes to travel from the sun to Earth, how long would it take you to drive?
6 Approximately what was the difference in time of the eclipses that Olaus Rømer observed?
7 Determining the Speed of Light Galileo tried unsuccessfully to determine the speed of light using an assistant with a lantern on a distant hilltop
8 In 1850 Fizeau and Foucalt also experimented with light by bouncing it off a rotating mirror and measuring timeThe light returned to its source at a slightly different position because the mirror has moved during the time light was travelingd=rt again gave c
9 Light is electromagnetic radiation and is characterized by its wavelength ()
24 Because of its electric and magnetic properties, light is also called electromagnetic radiation Visible light falls in the 400 to 700 nm rangeStars, galaxies and other objects emit light in all wavelengths
25 Which of the following has the highest frequency? Visible lightRadio wavesMicrowavesX-RaysInfrared lightUltraviolet lightGamma rays
26 Which of the following has the highest wavelength? Visible lightRadio wavesMicrowavesX-RaysInfrared lightUltraviolet lightGamma rays
27 Which of the following has the highest speed? Visible lightRadio wavesMicrowavesX-RaysInfrared lightUltraviolet lightGamma rays
28 Which of the following has the highest energy E (h is a constant)? Visible lightRadio wavesMicrowavesX-RaysInfrared lightUltraviolet lightGamma rays
36 Spectral lines are produced when an electron jumps from one energy level to another within an atom The nucleus of an atom is surrounded by electrons that occupy only certain orbits or energy levelsWhen an electron jumps from one energy level to another, it emits or absorbs a photon of appropriate energy (and hence of a specific wavelength).The spectral lines of a particular element correspond to the various electron transitions between energy levels in atoms of that element.Bohr’s model of the atom correctly predicts the wavelengths of hydrogen’s spectral lines.
37 Measurements in Astronomy In astronomy, we need to make remote and indirect measurementsThink of an example of a remote and indirect measurement from everyday lifeThis may be a good time to have them work in groups to come up with answers. You may also want to try to get them to think and debate the distinction between what defines a direct versus an indirect measurement.
38 Using LightLight has many properties that we can use to learn about what happens far awayLight interacts with matter in a special way
39 X Only photons with special wavelengths will interact with atom How will this affect what a person will see at point X?When is the atom “hotter”?From Universe Section 5.2X
40 Why is UV light usually blamed for skin cancer Why is UV light usually blamed for skin cancer? What is special about it compared to other light sources?
43 Continuous SpectrumAt this point I go back to the dryer lint question and ask what it has to do with light. If they do not get it, I ask if their dryer lint ever came out red and why. When they get the answer, ask why it is gray instead of white (among other reasons, because you usually wash whites separate).A blackbody emits photons with many energies (wavelengths) – a continuous spectrumA prism bends photons more or less depending on their wavelength
44 What will the spectrum look like here? Note that the original image said “Cloud of cool gas”. I covered up the “cool” because some people thought it would mean that the gas was so cold that we would not see anything on the spectrum (they were actually thinking about the radiated power amplitude according to the blackbody curve being very low in the visible range for a cold gas).What will the spectrum look like here?
47 What type of spectrum is produced when the light emitted from a hot, dense object passes through a prism?What type of spectrum is produced when the light emitted directly from a cloud of gas passes through a prism?Describe the source of light and the path the light must take to produce an absorption spectrumThere are dark lines in the absorption spectrum that represent missing light. What happened to this light that is missing in the absorption line spectrum?From Lecture Tutorials for Introductory Astronomy, page 61.
48 Each chemical element produces its own unique set of spectral lines
49 Stars like our Sun have low-density, gaseous atmospheres surrounding their hot, dense cores. If you were looking at the spectra of light coming from the Sun (or any star), which of the three types of spectra would be observed?If a star existed that was only a hot dense core and did not have a low-density atmosphere surrounding it, what type of spectrum would you expect this particular star to give off?Two students are looking at a brightly lit full Moon, illuminated by reflected light from the Sun. Consider the following discussion between two students about what the spectrum of moonlight would look like:I think moonlight is just reflected sunlight, so we will see the Sun’s absorption line spectrum.I disagree, an absorption spectrum has to come from a hot, dense object. Since thie Moon is not a hot, dense object, it can’t give off an absorption line spectrum.Do you agree or disagree with either or both of these students? Explain your reasoning.
50 Imagine that your are looking at two different spectra of the Sun Imagine that your are looking at two different spectra of the Sun. Spectrum #1 is obtained using a telescope that is in a high orbit far above Earth’s atmosphere. Spectrum #2 is obtained using a telescope located on the surface of Earth. Label each spectrum below as either Spectrum #1 or Spectrum #2.
51 Would this make sense?This dark line was removed
52 Energy and electromagnetic radiation Planck’s law relates the energy of a photon to its frequency or wavelengthE = energy of a photonh = Planck’s constantc = speed of lightl = wavelength of lightThe value of the constant h in this equation, called Planck’s constant, has been shown in laboratory experiments to beh = x 10–34 J s