1. Introduction to Physical Science Monday, Wednesday, Thursday Tom Burbine tomburbine@astro.umass.edu

2. Schedule December 6 - December 7 (1:30 pm) (optional) – Field Trip to look at rocks –Will replace your lowest Lab score December 8 - December 9 – Presentations –5-10 minutes –On how you would teach something you learned in class to your students December 13 – Final –Covers everything from midterm –Can bring in one sheet of paper with anything you wanted written on it –Also, your mineral identification sheets

3. Final Coulomb’s Law Electric Potential Electric current Electrical resistance Ohm’s Law Voltage = current x resistance Power = current x voltage Series Circuit Parallel Circuit

4. Final Magnetism Waves Light c = λ*f E = h*f Electromagnetic spectrum Doppler shift

5. Final Atoms Radioactive dating Chemistry –I will give you a periodic table on the test Minerals –You can bring in the mineral sheets that you filled out Rocks

6. Final Geologic Time Earth’s Interior Plate tectonics Moon Mars Stars Life elsewhere in the Universe Galaxies Fate of the Universe

7. Mars http://www.daviddarling.info/images/Mars_large.jpg

8. Mars Names after Mars, Roman God of War Mars has two tiny natural moons, Phobos and Deimos, which orbit very close to the planet and are thought to be captured asteroids. Both satellites were discovered in 1877 by Asaph Hall, and are named after the characters Phobos (panic/fear) and Deimos (terror/dread) who, in Greek mythology, accompanied their father Ares, God of War

9. Percival Lowell (1855-1916) Lowell produced intricate drawings of the Red Planet Finding hundreds of straight lines (termed "canals")

11. He thought Lowell concluded that the bright areas were deserts and the dark were patches of vegetation Lowell thought the canals were constructed by intelligent beings who once flourished on Mars.

12. For years People thought life could exist on Mars and Venus, the closest planets to Earth

13. However, Venus is extremely hot (~700-800 K) Atmospheric pressure is 90 times that of Earth

14. What happened on October 30, 1938?

15. http://sounds.mercurytheatre.info/mercury/381030.mp3http://sounds.mercurytheatre.info/mercury/381030.mp3

16. Mars The average recorded temperature on Mars is -63 °C with a maximum temperature of 20 °C and a minimum of -140 °C Atmospheric pressure is 1/100 of Earth’s Mars is often enveloped by planet-wide dust storms

17. Dust Devils http://en.wikipedia.org/wiki/Image:Marsdustdevil2.gif

18. Dust Devils Dust devils are smaller and weaker than tornadoes They are caused by convection on hot, calm summer days. Air near the surface becomes much warmer than the air above, creating an updraft.

20. Key to Life All life on Earth depends on water So if you find water, you may find life

21. Habitable Zone The region around a star in which planets could potentially have surface temperatures which liquid water could exist

23. In the past Mars appeared to be warmer and wetter

24. Atmospheres Layer of gases that surround a body with sufficient mass Gravity keeps the gases around the body

25. Phase Diagram http://img.search.com/thumb/d/dc/Phase-diag.png/300px-Phase-diag.png

26. http://science.nasa.gov/headlines/y2000/ast29jun_1m.htm Mars

29. The Valles Marineris is a system of canyons located just south of the Martian equator. The system is about 4000 km long,

30. Valles Marineris

31. How did Mars lose its water?

32. One possibility: On Earth, we're protected from the solar wind by a global magnetic field Mars appears to have had a global magnetic field, which turned off When it turned off, Mars’ atmosphere may have been eroded by the solar wind

33. http://upload.wikimedia.org/wikipedia/commons/d/dd/Karte_Mars_Schiaparelli_MKL1888.png In September 1877, Italian astronomer Giovanni Schiaparelli used a 22 cm telescope to help produce the first detailed map of Mars. These maps notably contained features he called canali, which were later shown to be an optical illusion.

34. Percival Lowell map of Mars from ~1914 http://en.wikipedia.org/wiki/Image:Lowell_Mars_channels.jpg

35. MOLA MOLA is the Mars Orbiter Laser Altimeter on Mars Global Surveyor (MGS) spacecraft This altitude determination process works by measuring the time that a pulse of light takes to leave the spacecraft, reflect off of the ground, and return to MOLA's collecting mirror. By multiplying the reflection time by the speed of light, scientists are able to calculate Surveyor's altitude above the local terrain to within 30 meters (98 feet) or better.

36. Two Hemispheres Northern Plains Southern Highlands

38. blue is low red/white are high These two hemispheres are centered on the Tharsis plateau (including the Valles Marineris and the large volcanos) and on the Isidis impact basin (with the Hellas basin to the south)

39. Topography Northern plains flattened by lava flows contrast with the southern highlands, pitted and cratered by ancient impacts.

40. The northern hemisphere is much flatter The northern hemisphere was formed from lava flows The northern hemisphere is also lower than the southern hemisphere, with an elevation difference between the two of about 5 km (3 mi)

41. What caused this difference? http://www.world-science.net/othernews/080625_mars.htm http://www.astrobio.net/news/article58.html Glancing impact –“The impact would have to be big enough to blast the crust off half of the planet, but not so big that it melts everything” Huge ocean covered Northern Hemisphere?

42. Olympus Mons The shield volcano, Olympus Mons (Mount Olympus), is at 26 km the highest known mountain in the solar system.

43. Hellas Basin 2,300 km in diameter 9 km depth http://upload.wikimedia.org/wikipedia/commons/f/fc/Hellas_basin_topo.jpg

44. Northern Polar Cap Permanent ice cap comprised mainly of water and carbon dioxide ice http://en.wikipedia.org/wiki/Planum_Boreum Crater is 80 m in diameter

46. Evidence organic molecules Magnetite (Fe 3 O 4 ) that looks like it formed from biologic activity nanofossil-like structures

53. http://www.guidescope.net/solarsys/mars_map2.jpg

54. Viking Missions Missions to Mars that landed in 1976 to look for Life Viking 1 - July 20, 1976 Viking 2 - September 3, 1976

57. Red Color The red color of the planet comes from the oxidation of iron minerals in the soil. Fe 2+ is becoming Fe 3+ Rusting

60. Experiments Three of the four experiments to look for life produced positive results But results could all be explained through non- biologic chemistry

62. The Labeled Release Experiment (LR) Was set up to detect the uptake of a radioactively- tagged liquid nutrient by microbes. The idea was that gases emitted by these microbes would show the tagging. Initial results were in line with this prediction but in the end, the overall results were inconsistent.

63. The Labeled Release (LR) experiment When we consume food, some is processed and combined with oxygen to produce energy. Carbon dioxide is produced. Carbon atoms in the food were radioactive and therefore could be detected in the air if a creature in the Martian soil processed the food and generated carbon dioxide (or some other gas containing carbon). A radioactive broth was added to a sample of Martian soil in a closed chamber. A detector in a side chamber measured the amount of radioactivity in the air.

66. Spirit and Opportunity I used to live in an Orphanage. It was dark and cold and lonely. At night, I looked up at the sparkly sky and felt better. I dreamed I could fly there. In America, I can make all my dreams come true..... Thank-you for the "Spirit" and the "Opportunity" — Sofi Collis, age 9

68. Spirit

70. Husband Hill

71. Opportunity

72. Opportunity Ledge Rocks seem layered. Either due to sediments or volcanic ash

73. Hematite (Fe 2 O 3 ) formed as deposits in water?

74. http://video.pbs.org/video/1114436021/

75. Any Questions?