Concept 3: Longitude and earth’s rotation I. Rotation is the spinning of an object on its axis (imaginary.

Slides:



Advertisements
Similar presentations
Insolation Insolation = Incoming Solar Radiation Energy in = Energy out or, Insolation In = Heat Out (Earth only emits heat)
Advertisements

Topic IV: Motions of the Earth, Moon and Sun
Section 2: Movements of the Earth
Section 2: Movements of the Earth
Unit III: The Earth in Space
Motions of the Earth, Moon and Sun
Insolation Insolation = Incoming Solar Radiation Insolation In = Heat Out.
Earth’s Rotation and Revolution
Earth’s Rotation and Revolution
Earth’s Revolution Earth revolves around the sun in a slightly eccentric elliptical path once a year  Ellipse ~ Oval  It takes Earth days to.
The Reason for the Seasons
Topic 4 Motions of the Earth, Moon, and Sun
The Reasons for the Seasons. Rotation Earth spins on axis (imaginary line through center of Earth from North to South Pole) Earth spins on axis (imaginary.
The Reasons for the Seasons
MOTIONS OF EARTH, MOON AND SUN
Earth Science Topic #4 Review Game
Earth Motions and the Heavens
Chapter 26 Studying Space 26.2 Movements of Earth
26.2 Movements of Earth.
Celestial Observations
Motions in the Sky (Part I)
Astronomy.
Aim: What are the apparent motions of the stars and planets?
Motions of Earth, Moon, and Sun. Apparent Motions of Celestial Objects An apparent motion is a motion that an object appears to make. Apparent motions.
Constellations A constellation is a region of the sky.
Trivia Question of the Day. Astronomy Picture of the Day Astronomy Picture of the Day.
Solar Motion. Label front flap MOTIONS OF THE EARTH -DAY & NIGHT.
Earth’s Rotation and Revolution
Space, Earth and Celestial Objects © Lisa Michalek.
Rotation and Revolution What causes night and day? What causes the seasons to change?
Astronomy The study of the moon, stars, and other objects in space Study the movements of the sun, and moon as they appear to travel across the sky Will.
SOLAR SYSTEM MODELS  EARTH CENTERED SYSTEM DEVELOPED BY PTOLEMY  WAS ACCEPTED UNTIL THE 1960’S  SUN CENTERED SYSTEM DEVELOPED BY COPERNICUS  MODERN.
Movements of the Earth The Earth’s Motion in Space.
Aim: What are some celestial and terrestrial observations? A. Celestial Object Object – any object observed in the sky during the day or night (ex: stars,
Earth in Space Chapter 19 Section 1 Pages Chapter 19 Section 1 Pages
Celestial Objects and Motions
The Reason for the Seasons. ___________ Earth _______ on ________ (imaginary line through center of Earth from North to South Pole) Earth _______ on ________.
Earth, Sun, Moon and the Seasons Topic 4 and 6 Discussion Question Review Question.
How do they work together to help life survive? Seasons
Earth-Sun Relationships The Reasons for the Seasons.
EARTH IN SPACE. A reminder about earth  The earth is almost a sphere  We locate points on the sphere with 3 coordinates – Longitude (180º W º.
Earth in Space.
Climates, Seasons, & Days
Chapter 23 Sun, Earth, Moon System. Position? Center of the universe? No, the Sun is the center of our solar system; Earth travels around the Sun. Shape?
Astronomy: Apparent Motions Making sense of celestial observations.
TOPIC 4 REVIEW. This topic is about what we can see occurring in our sky when we stand on Earth – Or rather, our CELESTIAL SPHERE.
Reason for Seasons Aim: How does the tilt of Earth’s axis and Earth’s movement cause seasons?
Unit III: The Earth in Space. Celestial Objects Celestial Sphere.
What are the motions of the Earth?. Earth and the Moon in Space The Earth and the moon are part of the sun’s planetary system. Pulled by the sun’s gravity,
Earth Motions 1)Rotation – the spinning of an object on its axis. (Like a figure skater or a CD) 2)Direction of Rotation – Earth turns west to east or.
New observations lead to changes in scientific theory What’s wrong with the image on the right, which shows Ptolemy’s popular scientific theory 2000 years.
Earth Science Topic #4 Review Game
 .
Reason for Seasons Aim: How does the tilt of Earth’s axis and Earth’s movement cause seasons?
Question of the Day What is the Shape of Earth’s Orbit?
Planetary winds in the Northern Hemisphere
Sun, Moon, & Earth’s Motions
Rotation and Revolution
Inertia Gravity 1. a tendency 1. a force 2. Newton’s 1st law Both
Astronomy Motions of the Earth and Sun
TOPIC 3 EARTH MOTIONS.
Insolation Insolation = Incoming Solar Radiation Energy in = Energy out or, Insolation In = Heat Out (Earth only emits heat)
November 8,2010 Celestial Motions.
Reason for Seasons.
The Earth’s Rotation, Revolution Around the Sun, and the Seasons
Earth’s Movement and Seasons
Mr. Ahearn Earth Science 2010
What are the motions of the Earth?
Aim: The Sun’s path each Season
Space motion.
Presentation transcript:

Concept 3: Longitude and earth’s rotation I. Rotation is the spinning of an object on its axis (imaginary line through the poles and center). Our axis is from the north pole through the south pole. 1. Earth rotates at a rate of 360o in 24 hours, or 15o/hr. 2. Rotation gives us our daily clock time and day and night.

 3. The earth's true rotation makes the sun appear to move. This is called the sun's apparent motion. (How fast does the sun appear to move each day? The stars? The moon?)  4. The sun appears to make an arc through the sky at 15o/hr.

 5. Because the earth really rotates from west to east, or counterclockwise, an observer (person standing in one spot on earth) anywhere on earth will see sunrise (sun appears over horizon in morning) towards the east and the sunset (disappear below the horizon in evening) towards the west.

 6. Where the sun is during the rest of the day depends on the observer's latitude  7. For New York State, the sun is always in our southern sky during the day.

 8. At solar noon we say the sun has reached its highest point of the day. In New York State, the sun is never ever ever directly over our heads. (In other words, the sun is never at zenith in New York State).

 9. Evidence of rotation:  a. Coriolis Effect is the deflection of wind and water from straight line motion. If the earth did not rotate, winds and water would not curve, they’d go in a straight line.  4/es1904page01.cfm?chapter_no=visualization 4/es1904page01.cfm?chapter_no=visualization 4/es1904page01.cfm?chapter_no=visualization

 b. Foucault Pendulum appears to change direction in a circle during 24 hours. However, the pendulum is actually going in a straight line, it is the room that is rotating around it!!! 

 c. Circumpolar constellations (always above the horizon) move around Polaris during the night, giving the suggestion that we rotate.  vieid=dipperclock&width=850&height=340&version= vieid=dipperclock&width=850&height=340&version= vieid=dipperclock&width=850&height=340&version=6.0.0

Concept 3: Latitude, seasons and revolution  1. Revolution is an object moving continuously around another object due to gravity.  Earth is a satellite (object revolving around another object) of the sun.  ator.swf&movieid=configurationssimulator&width=850&height=680&version=6.0.0 from classaction, planetary motion ator.swf&movieid=configurationssimulator&width=850&height=680&version= ator.swf&movieid=configurationssimulator&width=850&height=680&version=6.0.0

 Our orbit (path around the sun) takes us one year or days (creating leap year) at a rate of earth’s orbit is 3600/365 days, or 1 0 /day. Think: if our orbital radius is 92 million miles, how fast, in miles/day, is our orbit? C=2  r.) Slide 24 Slide 24Slide 24

3. Ancient proofs of earth's revolution:  a. Seasons (change in weather in a cyclic fashion).  The size of the sun changes during the year. We are CLOSER to the sun in WINTER.

Parallax of stars:  closer stars seem to shift position relative to farther stars during the year.

 Seasonal constellations: the constellations we see in fall are different than those we see in winter, spring, etc. The change is cyclic  earth orbit and seasonal stars

Models of the Solar System (and universe)  Geocentric Model: earth-centered. Geocentric Model: earth-centered. Heliocentric Model: sun- centered.(Copernican model)  retrograde motion and the ptolemic and Copernican explanations  ptolemic retrograde  copernican retrograde

4. Causes of Seasons; a. Tilt of axis: our axis is tilted, with reference to the sun's rays, at an angle of 23.5o (look at any globe)  movieid=obliquity&width=600&height=400&version= movieid=obliquity&width=600&height=400&version= movieid=obliquity&width=600&height=400&version=6.0.0  b. Parallelism of the axis: our North Pole always points toward Polaris. (see wall chart)

c. Revolution: We orbit the sun on a tilted planet, causing different parts of the earth to have more light seasonally. mulator&width=970&height=710&version= mulator&width=970&height=710&version= mulator&width=970&height=710&version=6.0.0

5. Important dates:  Equinoxes: “equal night”. Sun is overhead at equator. September 22 and March 21  Solstice: ‘sun stop’. Sun is either at Tropic of Capricorn (winter begins December 21) or Tropic of Cancer (summer begins June 21).  Each day, the sun seems to move a little bit between 23.5 North and 23.5 South

 Actual position of sunrise changes with seasons, but is always east  Position of sunset changes with seasons, but is always west.

 retrograde motion and the ptolemic and Copernican explanations  ptolemic retrograde  copernican retrograde  rationssimulator.swf&movieid=configurationssimulator&width=850&height=680&versi on=6.0.0 from classaction, planetary motion rationssimulator.swf&movieid=configurationssimulator&width=850&height=680&versi on= rationssimulator.swf&movieid=configurationssimulator&width=850&height=680&versi on=6.0.0  aic.swf&movieid=ptolemaic&width=900&height=660&version=6.0.0 ptolemic phases of venus aic.swf&movieid=ptolemaic&width=900&height=660&version= aic.swf&movieid=ptolemaic&width=900&height=660&version=6.0.0  ade.swf&movieid=retrograde&width=700&height=600&version=6.0.0 retrograde animation ade.swf&movieid=retrograde&width=700&height=600&version= ade.swf&movieid=retrograde&width=700&height=600&version=6.0.0  physics animations   earth orbit and seasonal stars

 C= 2 x 92 million x 3.14 = 580 million miles orbit  Speed of orbit = 580 million miles / 365 days = 1.6 million miles / day  Hours in a day = 24  Speed per hour = 1.6 million miles/ day x 1day/ 24 hours = 67, 000 mph