1. Vesta, the second largest object in the asteroid belt, was recently imaged for the first time by the robotic Dawn satellite that arrived last month.

2. Homework #3 Will be posted soon The first exam has been shifted to Monday, October 3.

3. Don’t confuse mass and weight Weight is the force due to gravity that acts on a given mass

4. Same mass different weight

5. ConceptTest The gravitational potential energy of an interstellar cloud of gas that is slowly shrinking in size … (yellow) stays the same (red) slowing changes into other forms of energy (green) slowly increases (blue) interstellar clouds do not have gravitational potential energy

6. ConceptTest The gravitational potential energy of an interstellar cloud of gas that is slowly shrinking in size … (yellow) stays the same (red) slowing changes into other forms of energy (green) slowly increases (blue) interstellar clouds do not have gravitational potential energy

7. ConceptTest In the not too distant future scientists will develop an engine that produces more energy than it uses. This statement is … (yellow) likely to be true (red) false (green) difficult to determine if this will happen or not. (blue) this has already happened, but the government is suppressing this discovery.

8. ConceptTest In the not too distant future scientists will develop an engine that produces more energy than it uses. This statement is … (yellow) likely to be true (red) false (green) difficult to determine if this will happen or not. (blue) this has already happened, but the government is suppressing this discovery.

9. Radiative energy: energy carried by electromagnetic waves (light).

10. Properties of Waves WAVELENGTH (  : Distance between adjacent crests FREQUENCY (f) : number of crests that pass through a point each second. It is measured in units of hertz (Hz), which are the number of cycles per second. AMPLITUDE: A measure of the strength of the wave. SPEED ( s) : how fast the wave pattern moves. For any wave: s = f

11. Light as a Wave The speed of light is a constant: s = c !!! Therefore, for light: f = c The higher f is, the smaller is, and vice versa. In the visible part of the spectrum, our eyes recognize f (or ) as color!

12. Light as a Particle  Light can also be treated as photons – packets of energy.  The energy carried by each photon depends on its frequency (color)  Energy: E = hf = hc / [“h” is called Planck’s Constant] Shorter wavelengths: more energy per photon.

13. higher energy lower energy The Electromagnetic Spectrum Spectroscopy: The quantitative analysis of spectra

14. The spectroscopic analysis of an object’s spectrum can reveal the object’s: Composition Temperature Velocity Spectroscopy: The quantitative analysis of spectra

15. Four Ways in Which Light can Interact with Matter 1. emission – matter releases energy as light 2. absorption – matter takes energy from light 3. transmission – matter allows light to pass through it 4. reflection – matter reflects light The type of interaction is determined by characteristics of the “matter” and the wavelength of light.

16. Different wavelengths of light interact differently with the atmosphere

17. Three types of spectra  Continuous spectra  Absorption spectra  Emission line spectra

18. An example: stars have many colors

19.  Continuous spectra are usually related to the temperature of an object that is emitting radiation.  Absorption & emission line spectra are related to the composition of the material absorbing or emitting radiation.

20. Thermal Emission A hot, dense glowing object (solid or gas) emits a continuous spectrum.

21. 1.Hotter objects emit more total radiation per unit surface area. 2.Hotter objects have peak emissions at shorter wavelengths (they will appear “bluer”) Rules for Thermal Emission by Opaque Objects 5000 K 3000 K 4000 K Wavelength Energy emitted per square meter

22. The sun emits its peak radiation in the yellow portion of the visible spectrum. The human eye has its peak sensitivity at the same wavelength. Coincidence?

23. At “room temperature”, or “body-temperature”, objects emit their peak radiation in the infrared. The surface of the Earth emits radiation in the infrared. infrared visible Extremely hot objects will emit most of their radiation in the ultraviolet, x-ray or even the gamma ray portion of the spectrum

24. Intermission time

26. A B Total Energy output per second Wavelength Which of the two stars (A or B) emits light that has a peak emission with the longer wavelength? (red) Star A (blue) Star B (green) The stars’ peak emissions are at the same wavelength (yellow) None of the above VIBGYOR visible range

27. A B Wavelength Which of the two stars (A or B) emits light that has a peak emission with the longer wavelength? (red) Star A (blue) Star B (green) The stars’ peak emissions are at the same wavelength (yellow) None of the above VIBGYOR visible range Total Energy output per second

28. A B Wavelength Which of the two stars (A or B) would appear red? (red) Star A (blue) Star B (green) Neither would appear red (yellow) There is insufficient information to determine the star’s color VIBGYOR visible range Total Energy output per second

29. A B Wavelength Which of the two stars (A or B) would appear red? (red) Star A (blue) Star B (green) Neither would appear red (yellow) There is insufficient information to determine the star’s color VIBGYOR visible range Total Energy output per second

30. The figure shows the spectra of two stars. Which star is hotter? (red) A (blue) C (yellow) neither A C WavelengthVIBGYOR visible range Total Energy output per second

31. The figure shows the spectra of two stars. Which star is hotter? (red) A (blue) C (yellow) neither A C Energy output per second WavelengthVIBGYOR visible range Total Energy output per second

32. A C Energy output per second Wavelength Which of the following is possible to infer about stars A and C based upon the information provided in the graph? (red) Star A is smaller than star C (blue) Star A is larger than star C (green) The stars are the same size (yellow) It is not possible to infer any of these relationships VIBGYOR visible range Total Energy output per second

33. A C Energy output per second Wavelength Which of the following is possible to infer about stars A and C based upon the information provided in the graph? (red) Star A is smaller than star C (blue) Star A is larger than star C (green) The stars are the same size (yellow) It is not possible to infer any of these relationships VIBGYOR visible range Total Energy output per second

34. “Matter” and Light

35. Atom nucleus electron e-e- (proton,neutrons) p+p+ n ● 10,000,000 atoms can fit across a period in your textbook. ● The nucleus is nearly 100,000 times smaller than the entire atom (if atom filled the classroom auditorium, the nucleus would be barely visible at its center). ● Although it is the smallest part of the atom, most of the atom’s mass is contained in the nucleus.

36. Incorrect view better view Electrons do not “orbit” the nucleus; they are “smeared out” in a cloud which give the atom its size.

37. Atomic NumberElement 1Hydrogen (H) 2Helium (He) 3Lithium (Li) 4Beryllium (Be) 5Boron (B) 6Carbon (C) 7Nitrogen (N) 8Oxygen (O) The number of protons in the nucleus, i.e., the “atomic number”, determines the element

38. Relative abundances of elements in the universe

39. Every element has multiple isotopes  same number of protons (same element)  different numbers of neutrons