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ASTRONOMY ,[object Object]
I. Earth’s Place in the Universe ,[object Object]
2. Our Solar System ,[object Object],3:47
The Planets ,[object Object],3:41
3.  Milky Way Galaxy ,[object Object]
4.  Universe ,[object Object]
II.  Models of the Universe ,[object Object],[object Object]
E.  Models of the Universe ,[object Object]
3.  Ptolemy’s Geocentric model, as illustrated on the next page, can be summarized as follows: ,[object Object],[object Object]
[object Object],[object Object]
Retrograde Motion
d.  This model was accepted for almost 1400 years because it explained celestial observations made from Earth and………  it seemed obvious. ,[object Object],[object Object],[object Object],[object Object]
B.  Heliocentric Model ,[object Object],[object Object],2:08
B.  Heliocentric Model ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
However….. ,[object Object]
Brainstorming Rules ,[object Object],[object Object],[object Object],[object Object],[object Object]
STEPS ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
This animation shows twelve images of the sun, each taken through a telescope on Earth, one month apart. The dates range from August 2000 to July 2001. The dark markings on the sun are sunspots—regions where the surface is slightly cooler than the surrounding area. Notice how the size of the sun appears to change in a regular pattern.
SO..The question is: ,[object Object],[object Object]
C.  Kepler’s Heliocentric Model ,[object Object]
This is because….. ,[object Object]
a.  Kepler’s First Law ,[object Object]
An Ellipse –  draw the parts in your notes ,[object Object],[object Object],[object Object]
√  Eccentricity ,[object Object],[object Object],[object Object],[object Object],Reference Table page  1
2. Eccentricity ,[object Object]
 
B.  Kepler’s Second Law ,[object Object],[object Object],Maximum speed Minimum speed Decreasing speed
B.  Kepler’s Second Law ,[object Object],[object Object]
C.  Kepler’s Third Law ,[object Object],[object Object],[object Object]
Table on Page 15 247  years 3 3675 Pluto * 164  years 3.4 2795 Neptune 84.01  years 4 1784 Uranus 29.46  years 6 887 Saturn 11.6  years 8 484 Jupiter 687  days 15 142 Mars 365.25  days 19 93 Earth 224  days 22 67 Venus 88  days 30 36 Mercury Period of Revolution Speed  mile/sec. Distance  (millions of miles) Planet
D.  Sir Isaac Newton ,[object Object],[object Object],[object Object]
Newton’s Laws of Gravity ,[object Object],[object Object]
Newton’s Laws of Gravity ,[object Object],[object Object]
2.  Gravity and Inertia
a.  Newton’s Law of Inertia  ,[object Object],Inertia Gravity Stable Orbit
B.  Gravity and Inertia ,[object Object],[object Object]
History Summary  (16 m)
Rotation ,[object Object]
III. Rotation ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
B.  Effects of Earth’s Rotation ,[object Object]
B.  Effects of Earth’s Rotation ,[object Object],[object Object],[object Object]
B.  Effects of Earth’s Rotation ,[object Object],[object Object]
Looking East Looking West Looking North Looking South
B.  Effects of Earth’s Rotation ,[object Object]
B.  Effects of Earth’s Rotation ,[object Object]
4 3:00 pm 3 9:00 am 2 3:00 am 1 9:00 pm Position of the big dipper Mid October Date New York State Location of Observer
B.  Effects of Earth’s Rotation ,[object Object]
Star trail photographs looking north, south, east and west A.  North D.  East C.  West B.  South
Celestial Poles – video clip
IV. Revolution ,[object Object],[object Object],[object Object],[object Object],[object Object]
B.  Effects of Earth’s Revolution ,[object Object],[object Object]
3.  Zodiac  – a band of 12 constellations that forms a background for the Sun as seen from  the revolving Earth.
Continued:  Effects of Earth’s Revolution ,[object Object],1 2 3 4
4 Summer 3 Spring 2 Winter 1 Fall Position of the Big Dipper 12:00 Midnight Time of Day NYS Location of Observer
3.  Seasons  – a yearly cycle
5.  Seasons of the Year ,[object Object],[object Object],[object Object],[object Object]
B.  Earth’s axis is tilted  23.5 0   relative to the plane of it’s orbit. ,[object Object],NYS 43  o Tropic of Cancer Equator Tropic of Capricorn
C.  Earth revolves around the Sun in a yearly cycle of 365 ¼ days. D.  As Earth revolves,  its axis always points in the same direction   (parallelism of axis) December 21 March 21 June 21 Sept. 20
E.  The apparent path of the sun changes with the  seasons  and with  latitude . ,[object Object],24 o 47 o 71 o
2. Equator 0 o  Latitude 67 o 67 o
F.  Length of Daylight (duration of daylight) – changes with  seasons  and with  latitude .
G.  Angle of Insolation (Sunlight) and Heating of Earth’s Surface High Angle High Intensity Low Angle Low Intensity 1.
G.  Angle of Insolation (Sunlight) and Heating of Earth’s Surface ,[object Object],[object Object]
H.  Factors affecting Insolation ,[object Object]
2. As latitude increases, the angle of insolation  decreases , and the intensity of insolation  decreases . ,[object Object],[object Object],Angle of insolation 0 o   Latitude  90 o Intensity of insolation 0 o   Latitude  90 o
3.  Season of the Year ,[object Object]
b.  Key:   Direct Ray of Sunlight (Perpendicular to Earth’s Surface; 90 o )   Ray of Sunlight (striking NYS at an angle less than 90 o )
C.  Maximum angle of insolation at 12 noon for mid N.Y.S. (Lat. 43 o  N) 1. Dec. 21 2. Mar/Sep. 21 3. June 21 24.5 48 71.5 Low angle Low intensity Medium angle Medium intensity High angle High intensity
4.  Time of Day ,[object Object]
b.  Angle of Insolation vs. Time
d.  Looking South ,[object Object]
V.  Celestial Observations ,[object Object],[object Object]
V.  Celestial Observations ,[object Object]
Celestial Sphere ,[object Object],[object Object]
E.  Location on the Celestial Sphere – THE HORIZON SYSTEM ,[object Object]
Location on the Celestial Sphere – THE HORIZON SYSTEM ,[object Object],[object Object]
3.  Model problems ,[object Object],[object Object],[object Object],[object Object],[object Object]
Our Sun – Future
VI The Moon ,[object Object],[object Object],[object Object]
B.  Physical Properties of the Moon ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
2.  Atmosphere ,[object Object],[object Object],[object Object],[object Object]
3.  Temperatures ,[object Object],[object Object],[object Object]
4.  Lunar Topography – surface features of the moon
“ The Dark Side of The Moon”
a.  Craters  – bowl-shaped depressions formed primarily as a result of impact of meteors. ,[object Object],[object Object],[object Object],[object Object]
b.  Maria ,[object Object],[object Object],[object Object]
MOON FUN FACTS ,[object Object],[object Object],[object Object],[object Object]
5.  The Moon’s Revolution ,[object Object],[object Object],[object Object],[object Object],[object Object]
6.  Phases of the Moon ,[object Object],[object Object]
7.  Moon Rotation ,[object Object]
Eclipses  ,[object Object],[object Object],[object Object]
 
10.  Tides ,[object Object],[object Object],[object Object]
[object Object],[object Object]
Surf’s Up!
VII.  Earth’s Place in the Universe ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Scale Model Distance
B.  Galaxies ,[object Object],[object Object],[object Object]
Side View of Spiral Galaxy
b.  Elliptical
c.  Irregular Galaxy
D.  The Milky Way Galaxy ,[object Object],[object Object]
a. Top View
b.  Side View
Life Cycle of Stars – H.R.Diagram
VIII.  Evolution of the Universe ,[object Object],[object Object],[object Object]
Electromagnetic Spectrum  (4.5 min)
[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
 
Dark line Spectrum
B. Doppler Effect –  apparent change in the wavelength of light (or sound) that occurs when an object is moving toward or away from the observer .
2.  Red Shift – Blue Shift
[object Object],[object Object]
C.  The Big Bang Theory ,[object Object]
Big Bang Video Clip
D.  Evolution of the Universe Cosmic Evolution Big Bang Origin of Matter Formation of Milky Way Formation of Earth Present

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Astronomy - Notes

  • 1.
  • 2.
  • 3.
  • 4.
  • 5.
  • 6.
  • 7.
  • 8.
  • 9.
  • 10.
  • 12.
  • 13.
  • 14.
  • 15.
  • 16.
  • 17.
  • 18. This animation shows twelve images of the sun, each taken through a telescope on Earth, one month apart. The dates range from August 2000 to July 2001. The dark markings on the sun are sunspots—regions where the surface is slightly cooler than the surrounding area. Notice how the size of the sun appears to change in a regular pattern.
  • 19.
  • 20.
  • 21.
  • 22.
  • 23.
  • 24.
  • 25.
  • 26.  
  • 27.
  • 28.
  • 29.
  • 30. Table on Page 15 247 years 3 3675 Pluto * 164 years 3.4 2795 Neptune 84.01 years 4 1784 Uranus 29.46 years 6 887 Saturn 11.6 years 8 484 Jupiter 687 days 15 142 Mars 365.25 days 19 93 Earth 224 days 22 67 Venus 88 days 30 36 Mercury Period of Revolution Speed mile/sec. Distance (millions of miles) Planet
  • 31.
  • 32.
  • 33.
  • 34. 2. Gravity and Inertia
  • 35.
  • 36.
  • 37. History Summary (16 m)
  • 38.
  • 39.
  • 40.
  • 41.
  • 42.
  • 43. Looking East Looking West Looking North Looking South
  • 44.
  • 45.
  • 46. 4 3:00 pm 3 9:00 am 2 3:00 am 1 9:00 pm Position of the big dipper Mid October Date New York State Location of Observer
  • 47.
  • 48. Star trail photographs looking north, south, east and west A. North D. East C. West B. South
  • 49. Celestial Poles – video clip
  • 50.
  • 51.
  • 52. 3. Zodiac – a band of 12 constellations that forms a background for the Sun as seen from the revolving Earth.
  • 53.
  • 54. 4 Summer 3 Spring 2 Winter 1 Fall Position of the Big Dipper 12:00 Midnight Time of Day NYS Location of Observer
  • 55. 3. Seasons – a yearly cycle
  • 56.
  • 57.
  • 58. C. Earth revolves around the Sun in a yearly cycle of 365 ¼ days. D. As Earth revolves, its axis always points in the same direction (parallelism of axis) December 21 March 21 June 21 Sept. 20
  • 59.
  • 60. 2. Equator 0 o Latitude 67 o 67 o
  • 61. F. Length of Daylight (duration of daylight) – changes with seasons and with latitude .
  • 62. G. Angle of Insolation (Sunlight) and Heating of Earth’s Surface High Angle High Intensity Low Angle Low Intensity 1.
  • 63.
  • 64.
  • 65.
  • 66.
  • 67. b. Key: Direct Ray of Sunlight (Perpendicular to Earth’s Surface; 90 o ) Ray of Sunlight (striking NYS at an angle less than 90 o )
  • 68. C. Maximum angle of insolation at 12 noon for mid N.Y.S. (Lat. 43 o N) 1. Dec. 21 2. Mar/Sep. 21 3. June 21 24.5 48 71.5 Low angle Low intensity Medium angle Medium intensity High angle High intensity
  • 69.
  • 70. b. Angle of Insolation vs. Time
  • 71.
  • 72.
  • 73.
  • 74.
  • 75.
  • 76.
  • 77.
  • 78. Our Sun – Future
  • 79.
  • 80.
  • 81.
  • 82.
  • 83. 4. Lunar Topography – surface features of the moon
  • 84. “ The Dark Side of The Moon”
  • 85.
  • 86.
  • 87.
  • 88.
  • 89.
  • 90.
  • 91.
  • 92.  
  • 93.
  • 94.
  • 96.
  • 98.
  • 99. Side View of Spiral Galaxy
  • 101. c. Irregular Galaxy
  • 102.
  • 104. b. Side View
  • 105. Life Cycle of Stars – H.R.Diagram
  • 106.
  • 108.
  • 109.  
  • 111. B. Doppler Effect – apparent change in the wavelength of light (or sound) that occurs when an object is moving toward or away from the observer .
  • 112. 2. Red Shift – Blue Shift
  • 113.
  • 114.
  • 115. Big Bang Video Clip
  • 116. D. Evolution of the Universe Cosmic Evolution Big Bang Origin of Matter Formation of Milky Way Formation of Earth Present