1. Astronomy 101 The Solar System Tuesday, Thursday 2:30-3:45 pm Hasbrouck 20 Tom Burbine tomburbine@astro.umass.edu

2. Course Course Website: –http://blogs.umass.edu/astron101-tburbine/http://blogs.umass.edu/astron101-tburbine/ Textbook: –Pathways to Astronomy (2nd Edition) by Stephen Schneider and Thomas Arny. You also will need a calculator.

3. Office Hours Mine Tuesday, Thursday - 1:15-2:15pm Lederle Graduate Research Tower C 632 Neil Tuesday, Thursday - 11 am-noon Lederle Graduate Research Tower B 619-O

4. Homework We will use Spark https://spark.oit.umass.edu/webct/logonDisplay.d owebcthttps://spark.oit.umass.edu/webct/logonDisplay.d owebct Homework will be due approximately twice a week

5. HW #5 Due today

6. HW #6 Due Tuesday

7. http://www.post-gazette.com/pg/09271/1000779-369.stm

8. Messenger just flew by Mercury http://www.msnbc.msn.com/id/33092470/ns/technology_and_science-space/

9. Energy Energy is the ability to generate motion

10. Conservation of Energy Energy is neither created or destroyed – it just changes forms Conservation of Energy –The energy in a closed system may change form, but the total amount of energy does not change as a result of any process.

11. Energy units In English Units, we use calories to measure energy In science (and in this class), we will use joules to measure energy 1 Joule = 1 kg * m 2 /s 2

13. 3 basic categories of energy Kinetic energy – energy of motion Potential energy – energy being stored for possible conversion into kinetic energy Radiative energy – energy carried by light

14. Kinetic energy Kinetic energy = ½ mv 2 m is mass in kg v is velocity in meters/s Remember: a joule has units of kg * m 2 /s 2

15. How much kinetic energy does a 2 kg rock have if it is thrown at 20 m/s? Kinetic energy = ½ mv 2 A) 200 J B) 400 J C) 40 J D) 800 J

16. Answer KE = ½ * 2 * (20) *(20) = 400 joules

17. Thermal energy (kind of kinetic energy) Temperature is a measure of the average kinetic energy of the particles Higher temperature – more kinetic energy, particles moving faster For examples, air molecules around you are moving at ~600 m/s http://eo.ucar.edu/webweather/molecules.html

18. Temperature scales In America, we use Fahrenheit Water freezes at 32 degrees F Water boils at 212 degrees F Everywhere else, they use Celsius Water freezes at 0 degrees C Water boils at 100 degrees C

19. In Science Temperature is measured in Kelvin Zero Kelvin is absolute zero – nothing moves Add 273.15 to the Celsius temperature to get the Kelvin temperature 273.15 Kelvin = 0 degrees Celsius

22. Gravitational Potential Energy Gravitational Potential Energy released as an object falls depends on its mass, the strength of gravity, and the distance it falls For example, your gravitational potential energy increases as you go farther up in the air This is because you hit the ground at a faster speed if you jump from a higher distance

23. Gravitational Potential Energy PE = -G m*M/r G is the Gravitational constant m is mass of one body M is mass of second body r is distance (people also use variable d)

24. KE + PE = 0 As kinetic energy increases, potential energy decreases

25. Converting Mass to Energy What is the most famous formula in the world?

26. E = mc 2 m is mass in kilograms c is speed of light in meters/s (3 x 10 8 m/s) So E is in joules very small amounts of mass may be converted into a very large amount of energy and

27. Who came up with it?

29. How much energy can be produced if you can convert 10 kg of material totally into energy? E = mc 2 A) 3.0 x 10 8 J B) 3.0 x 10 16 J C) 9.0 x 10 17 J D) 9.0 x 10 10 J

30. Answer E = 10 kg * (3 x 10 8 m/s) * (3 x 10 8 m/s) E = 10* (9 x 10 16 ) J E = 90 x 10 16 J E = 9.0 x 10 17 J

31. Mass-Energy E=mc 2 So Mass is a form of potential energy Where is one place where you see mass converted into energy?

33. Light Light is a form of energy

34. Light These are all forms of light –Gamma rays –X-rays –Ultraviolet light –Visible light –Infrared light –Radio waves

35. Light Can act as a particle Can also act as a wave

36. Particle aspect Particles called photons stream from the Sun and can be blocked by your body

37. Photons Light is quantized Comes in discrete packets called photons

38. Wave aspect

39. Thomas Young Experiment http://micro.magnet.fsu.edu/primer/java/interference/dou bleslit/http://micro.magnet.fsu.edu/primer/java/interference/dou bleslit/

40. Characteristics of waves velocity = wavelength x frequency Wavelength = distance Frequency = cycles per second = hertz

41. For light c = wavelength x frequency In vacuum, speed of light stays the same So if wavelength goes up Frequency does down f = frequency λ = wavelength c = λ x f

42. Calculations c = λ x f So if the wavelength is 1 x 10 -12 m 3 x 10 8 m/s = 1 x 10 -12 m * f f = 3 x 10 8 m/s/1 x 10 -12 m f = 3 x 10 20 s -1 = 3 x 10 20 Hz

43. Calculations c = λ x f So if the frequency is 1 x 10 15 Hz 3 x 10 8 m/s = λ * 1 x 10 15 Hz λ = 3 x 10 8 m/s/1 x 10 15 Hz λ = 3 x 10 -7 m

44. Energy of light Energy is directly proportional to the frequency E = h * f h = Planck’s constant = 6.626 x 10 -34 J*s since f = c/λ Energy is inversely proportional to the wavelength E = hc/λ

45. Higher the frequency, Higher the energy of the photon Higher the wavelength, Lower the energy of the photon redviolet VIBGYOR

46. ROYGBIV Red – long wavelength Violet – short wavelength

47. http://www.arpansa.gov.au/images/basics/emr.jpg

48. Calculations What is the energy of a radio wave with a frequency of 1 x 10 7 Hz? E = h * f h = Planck’s constant = 6.626 x 10 -34 J/s E = 6.626 x 10 -34 J/s * 1 x 10 7 E = 6.626 x 10 -27 J

49. Calculations What is the energy of a gamma ray photon with wavelength of 1 x 10 -15 m E = hc/λ h = Planck’s constant = 6.626 x 10 -34 J/s E = 6.626 x 10 -34 J/s * 3 x 10 8 m/s / 1 x 10 -15 m E = 1.99 x 10 -10 J

50. So why are some types of radiation dangerous? Higher the energy, the farther the photons can penetrate So gamma and X-rays can pass much more easily into your the body These high-energy photons can ionize atoms in cells Ionization means removes electrons from an atom

51. More dangerous

52. When you measure an astronomical body You measure intensity Intensity – amount of radiation

53. Matter Matter is material

54. Atoms Atoms are made up of 3 types of particles Protons – positive charge (+1) Electrons – negative charge (-1) Neutrons – neutral charge (no charge) Protons and Neutrons are found in the nucleus

57. Elements Different elements have different numbers of protons The properties of an atom are a function of the electrical charge of its nucleus

58. Charge If an atom has the same number of electrons and protons, it has a neutral charge More electrons than protons, negatively charged More protons than electrons, positive charged Neutrons have neutral charge so don’t affect the charge of an atom

60. Definitions Atomic Number – Number of protons Atomic Mass – Number of protons and neutrons U 235 – atomic mass 92- atomic number Isotopes – Same number of protons but different numbers of neutrons

61. Any Questions?