Regents Review Packet Page 1 Regents Review Packet

Regents Review Packet Page 1

Regents Review Packet Page 1 Day: Friday Date: June 19 th Time: 8 AM-11 AM Where: OLD GYM …and so is the REGENTS Exam, so please study …address conflicts- show schedule

TOPIC 1 -INTRO TO ES Page 1 KNOW THE DEFINITIONS OF OBSERVATION, INFERENCE, & CLASSIFICATION 1. Mass is the amount of matter in an object, weight is the measure of how much gravity pulls on an object 2. SEE DIAGRAM 3. 2 g/cm 3 4. 20 cm 3 OR ml or cc

TOPIC 1 -INTRO TO ES Decreases 6. Increases 7. Remains the same 5. Page 1

ES Regents Review Packet If density of an object is < 1. 0 g/cm 3 Page 1 9. Solid, water, liquid, 4°C 8. 10. 11.

ES Regents Review Packet 12. 13. Δ field value TIME 15. 2. 5 km/yr. 16. A changing balance, the balancing of opposing forces (i. e. erosion & deposition) 14. Page 1

ES Regents Review Packet 1. 2. 3. 4. 5. 6. 7. 4 1 2 3 3 1 4 8. 9. 10. 11. 12. 13. 14. 2 3 4 1 3 3 3 Page 2

Topic 2 Measuring Earth Page 3

Topic 3 Measuring Earth Page 3 Oblate Spheroid 2. Equator, b/c further from center of Earth 3. PHOTOS FROM SPACE, Lunar eclipses, sailing ships, varying angles of the sun’s rays 1. 4. 5. 25° N

Topic 3 Measuring Earth 6. Cannot see Polaris Page 3 7. City Elmira Plattsburgh 42°N, 76° 45’W 44° 40’N, 73° 28’W

Fractions of a Degree Ø 1 degree = 60 minutes or… Ø 1 minute is 1/60 th of a degree 30’ minutes is halfway between degrees

Fractions of a Degree Ø Use minutes if a location is not directly on a latitude /longitude line Ø Written ----- Degree/minute = XX° xx’ compass direction Ø For example, point A 5° 45’N, 71° 50’W 30’ minutes is half -way between degrees

Topic 3 Measuring Earth Page 3 15°/hr 9. ADD time 10. 11 AM 11. Isobars, Isotherms 12. Lines that connect points of equal elevation on a topographic map 13. Opposite the Vs, flows from high elevation to low, bends in the contours point upstream 8.

Topic 3 Measuring Earth Contours are close together Page 3 15. A depression or a drop in elevation 16. First set of hachured lines is equal in value as the adjacent contour line 17. Δ field value ÷ distance 18. Next Tile 19. . 5°C/m 14.

18. The elevation of Albany is 282 feet. The elevation at Binghamton is 1634 feet. What is the gradient in feet/mile? Show all work. gradient = change in elevation distance = 1634 -282 115 miles Page 3 = 1352 ft 115 miles = 11. 8 ft/mile JVolpe 10/19/10 16

ES Regents Review Packet 1. 2. 3. 4. 5. 6. 7. 4 4 3 1 2 4 1 1 9. 3 No #. 3 10. 3 11. 2 8. Page 4

Page 5 20 feet 2. South East, the Creek flows opposite the Vs 1.

Page 5 699 feet 4. South, Contour lines are closest togethere 3.

Page 5 720 feet 6. 9 miles 5.

Page 5 . . . Profile- Youtube video

Page 6 Draw 250 contour 9. Draw X at 55 feet elevation 8. X X X

Page 6 SE 11. 28. 6 m/km 10. X X X

Page 6 12. X X X Construct a profile

Page 7 13. 14. 15. 16. 17. Elmira Alleghany Plateau Southeast 1, 700 feet 833. 3 ft/mi

Page 7 10 feet 19. 40 feet 20. 31 feet 18.

90° Page 8 21. 12 hours 22. on diagram 24. 10 AM st rd 25. March 21 or Sept 23 26. B has a lower latitude 27. 15°/hr 20.

Page 8 28. B 29.

Page 8 30. ISOTHERMS 31. 1. 1°C/m

Page 8 32. 60°N, 90°E 33. X 34. 2 PM 35. A, X, C

Topics 3 & 4 ASTRONOMY Page 9

ES Regents Review Packet 1. Heliocentric, Geocentric 2. Ellipses 3. Spin on one’s axis 4. 24 hrs 5. 15°/hr, 45° Page 9

ES Regents Review Packet 6. 7. 8. 9. CCW or west to east Day & night, Foucault pendulum, Coriolis effect, star trails Right, Earth’s rotation, Left orbit OR revolve aroud a star Page 9

ES Regents Review Packet 10. 365. 25 days (in ESRT) 11. 12. 13. 14. Page 9 Changing seasons & Constellations Revolution, Tilt, parallelism Duh? Next tile Doppler Red Shift & cosmic background radiation(ECHO)

The Big Bang Theory States: Ø All the matter in the universe, is thought to be contained in an area no larger than a grain of sand Ø This area was under extreme pressure and measured an infinite density Ø The matter exploded and traveled outward at an extreme rate Ø This matter is still expanding and moving outward after billions of years Ø This theory explains the origin of the universe Ø It is known as the BIG BANG THEORY Page 9

ES Regents Review Packet 15. 16. 17. 18. Distortion of waves caused by movement of the object emitting the energy waves towards or away from the observer Yes, b/c we observe a Doppler Red shift of distant galaxies 13. 7 b. y. o. Page 9 4. 6 b. y. o.

ES Regents Review Packet 19. How the SS formed- video 4: 2 20. Page 9

ES Regents Review Packet Terrestrials are: Rocky, dense, small, & close to the sun… 22. Mercury, Venus, Earth, & Mars 23. Jupiter, Saturn, Uranus, Page 9 Neptune 21.

ES Regents Review Packet 24. 25. 26. 27. 28. Between Mars & Jupiter Page 9 Jupiter, Mercury Venus Mercury Velocity , gravity between earth & sun

ES Regents Review Packet 29. 30. 31. 32. 33. 34. Nuclear fusion Classifies stars 1 Red, blue Initial mass Main sequence, mature Page 9

HR Diagram Page 9

ES Regents Review Packet Red giant, white dwarf Page 9 36. White dwarfs 37. Rigel 35.

ES Regents Review Packet Red supergiants 39. Milky Way 40. 2/3 the way out on a spiral arm 38. Page 11

Milky Way Galaxy Page 11 You are here A spiral shaped galaxy

Page 11 Kepler’s 1 st Law The Ellipse Law: Ø Each planet moves around the Sun in an ellipse with the Sun at one focus Planet Major Axis: Orbit: The path of an object revolving around another object; such as the Earth around the sun. Minor Axis Focus Sun The longest diameter (axis) of an ellipse, running through the center and foci. Focus Sun D= Origin Half the major axis is semi major axis

Page 11 Kepler’s 1 st Law: Definitions Ø Eccentricity: Ø The degree of flatness or “ovalness” of an ellipse l l How out of round the shape is *Eccentricity of a circle= 0 Straight line= 1 Circle= 0 Comet

Page 11 Calculating eccentricity of an ellipse: When the distance between foci get larger what happens to the ellipse? Formula: length of major axis (e) eccentricity = (d) distance between foci (L) length of major axis

Kepler’s nd 2 Page 11 Law- Equal Time, Equal Area Ø What does Kepler's second law indicate about the orbital speed of a planet? Ø A planet moves at its fastest when it is closest to the Sun

Increasing speed Page 11 Perihelion Jan. 4 th Aphelion Decreasing speed Max. speed July 4 th Max. Gravitational Attraction Min speed Greatest Apparent Diameter Min Gravity Smallest diameter Page 17

Kepler’s 3 rd Law- the Harmonic Law Page 11 Ø The Harmonic Law-A planet’s orbital period (P) squared is proportional to its average distance from the sun (a) cubed: Period= The orbit of a planet; 1 revolution Py 2 = a. AU 3 What does it mean? (Py = period in years; a. AU = distance in AU) The time it takes a planet to orbit around the sun is a function of how far away it is Try Kepler’s Third Law Calculator

ES Regents Review Packet 42. 43. 44. 45. 46. Increases Decreases Furthest, July 4 th Closest, Jan 4 th Celestial sphere Page 11

How to draw celestial sphere Page 11

Page 17

ES Regents Review Packet 47. 48. 49. 50. 51. 52. 25°, 50°, 75° No Two 23. 5°N, 23. 5°S E to W Noon Page 11

ES Regents Review Packet 25°, 50°, 75° 48. No 47. Page 11

ES Regents Review Packet 49. 50. 51. 52. 53. 54. Twice Page 12 23°N to 23°S 3 to 5 PM June 21 st Late July/ Early August st st June 21 & Dec 21

ES Regents Review Packet Late July, August Page 12 st st 56. June 21 , December 21 57. Decreases 58. December 21 st 59. b/c the moon revolves around the earth 55.

ES Regents Review Packet 60. 61. 62. 63. 27. 3 days Page 12 29. 5 days Synchronous motion cyclic

68. S M E New SEM Full Spring 64. Full & New, S E M 64. 65. 66. 67. Page 12

ES Regents Review Packet & quarter, Sun Page 12 Moon and Earth @ right angles 71. Label phases Next tile 70. st 1 rd 3

71. Label phases Page 17

ES Regents Review Packet 1. 2. 3. 4. 5. 6. 2 1 3 4 3 3 7. 8. 9. 10. 11. 12. 3 3 1 1 1 4 13. 14. 15. 16. 17. 18. 1 4 3 2 2 4 Pages 14 & 15 4 20. 4 21. 1 19.

ES Regents Review Packet 22. 23. 24. 25. 26. 27. 2 4 2 2 4 1 28. 29. 30. 31. 32. 33. 3 34. 2 2 35. 4 1 1 3 2 Page 16

Page 17 1. 2. 3. 4. b/c the Sun gets higher in the sky Draw 11 am Draw 2 pm Increases decreases increases

5. 6. 7. 8. June 21 st 2 4 Draw polaris on C. S. Page 17

9. 10. 11. 12. 13. 14. Location B Location D, b/c Sun is in the North Location C Location A, b/c Sun is at the zenith on the Equinox 24 hours On location B draw 12/21 path Page 17

Page 18 9. 10. 11. 12. 13. B Shade night on B & D on diagram , 23. 5° South 23. 5° North

Page 18 14. 15. 16. 17. 18. 0°, Equator B 12/21 Ellipses Not a perfect circle, eccentricity greater that 0

Page 18 12/21 21. C 20. A 23. 24 hrs 24. decreases 22.

Page 19 25. Label New Moon (N) 26. Label Full Moon (F) 27. Label third Quarter Moon (3) 28. Square solar 29. Triangle lunar

Page 19 b/c E M S aren’t always in perfect alignment 26. Waxes or 27. Moon’s revolution 28. 27. 3 days (ESRT) 29. 5 days 30. Synchronous motion, period of rotation & revolution are the same 25.

Page 19 36. 37. Jupiter, Saturn, Uranus, Neptune As distance period of revolution

Page 20 Saturn or Neptune or Uranus 39. Earth has a smaller diameter & a greater density 40. Yellow & 1 38.

Page 20 Acceptable answers are: Kingston, Binghamton, Elmira, Jamestown 42. March 21 st Or Sept 23 rd 41.

Page 20 Draw 6/21 path altitude of 73° 44. Draw 12/21 path altitude of 24° 45. Label the zenith 43.

Page 20 Increases 47. Label sunrise on Sun’s Path 46.

End of PPT