Earth_Rotation_and_Revolution presentation.ppt
- 1. Earth’s Rotation and Revolution
- 2. Earth’s Rotation – Causes daily changes (like day and night) • The spinning of earth on its AXIS – the imaginary line through the planet from the North Pole to the South Pole – is its rotation • The axis of the earth is tilted 23.5° from a line perpendicular to the plane of its orbit of the sun.
- 3. Earth’s Rotation • As the earth revolves around the sun, Earth’s axis remains tilted at 23.5° • The north end of the axis points toward the north star (Polaris) • Earth rotates 360° from west to east (counter clockwise looking down from the north pole) in 24 hours, at an angular rate of l5° per hour (360°/24 hours = 15°/hour)
- 4. Tilt of the axis always stays the same
- 5. 1. Evidence of Earth’s Rotation • 1851, Foucault’s pendulum will appear to change in a predictable way. • Why is this evidence? There is no force acting on the pendulum to make its plane of oscillation rotate or go around its own axis • It would continue to swing in the original path if Earth did not rotate.
- 6. No force that makes pendulum rotate – must be earth that is rotating!!!
- 8. 2. Evidence for Rotation • Coriolis Effect – the tendency of objects moving over the earth (air, water, planes, projectiles) to be deflected (curve away) from a straight line path. The French scientist, Gaspard Coriolis, first explained the deflection of objects moving over the surface due to Earth’s rotation • The deflection is to the right in the Northern Hemisphere and to the left in the Southern Hemisphere. • This deflection occurs because Earth’s surface is rotating with respect to the objects.
- 13. What are the APPARENT MOTIONS of Celestial Objects • An apparent motion is a motion an object appears to make • An apparent motion can be real or an illusion • For example, the stars appear to move across the sky from east to west • However, the apparent motion is caused by Earth’s rotation
- 14. Stars in constellations are often very far from one another but we see them in the same direction in the sky. Big Dipper
- 15. Pointer Stars point to Polaris
- 16. Some Definitions • Celestial Sphere: A huge imaginary sphere around the Earth to which the stars appear to be attached. • Constellation: An arbitrary grouping of stars in the Sky that are in the same general direction. The modern ones are fixed by international agreement to map the entire Sky. • Celestial Equator: Projection of the Earth’s Equator onto the Celestial Sphere.
- 17. Imagine all the stars moved down onto a big glass sphere around the Earth. Stars Celestial equator Stars
- 19. •Looking upward we see the stars fixed on the celestial sphere •Earth’s eastward rotation makes the stars between the equator and north celestial pole appear to move westward •Rise in the east and set in the west. • Timed photography showing stars rising in the east
- 20. Stars appear to be moving from east to west. Stars rising in the east.
- 21. Stars appear to be moving from east to west. Rise in the east and set in the west.
- 22. Northern part of the sky around Polaris CCW Moving west to east
- 23. Earth’s counter clockwise rotation makes the stars appear to rotate counter clockwise around the north celestial pole (Polaris).
- 25. The complete circular path can be seen for stars in the northern part of the sky around Polaris Circumpolar constellations never set. Circumpolar constellations change with latitude… sky changes with latitude
- 26. Daily Motions • Some of the stars near Polaris appear to move in a complete circle in 24 hours. • The paths of all celestial objects moving in the sky are circular or parts of a circle called an arc. • All motion occurs at a constant rate of approximately l5° per hour or 360° in 24 hours.
- 27. Earth’s Revolution • Earth revolves around the sun in a slightly eccentric elliptical orbit or path once a year • It takes Earth 365.25 days to revolve 360° in its orbit around the sun. It moves approximately 1° per day. (360°/365.26 days = 1° per day)
- 28. Evidence of Earth’s Revolution around the Sun • Seasonal Constellations: Because of the Sun’s annual motion, some constellations are visible at night only during certain seasons. • Constellations are visible when the dark side of Earth (away from sun) faces toward the constellation.
- 29. The 13 constellations the sun appears to travel through during the year
- 30. Different constellations at different times of the year
- 31. Evidence of Revolution Parallax Shift • Because of Earth’s revolution about the sun, near stars seem to shift their position against the farther stars (closer star – greater the shift) • If you observe the same star while earth is at 2 different points during its orbit around the sun, the star’s position relative to the more distant background stars will appear to change.
- 34. Parallax Shift
- 35. Apparent Motion of Sun due to Rotation and Revolution • Rotation: Sun – apparent daily path from sunrise to sunset has the shape of an arc moving l5° per hour. • Revolution: However, the sun’s arc changes both its position and its length with the seasons
- 37. Earth’s Revolution around the Sun – the tilt of Earth’s axis does not change producing a cyclical change of seasons
- 38. Because of the tilt of the Earth’s axis, the sun’s rays are only perpendicular (directly overhead) at noon, between 23.5° N and 23.5° S during the year June 21 23.5° N Dec. 21 23.5° S March/Sept. 21
- 40. Zenith Position of the Sun • Because of the earth’s spherical shape, on any particular date, there is just 1 place where insolation (incoming solar radiation) is at an angle of 90°. All other places are less than 90°. • Does the 90° ever reach the United States? • An observer in New York State will never see the Sun directly overhead.
- 42. Summer maximum altitude of noon sun is 73°, Winter is 26° Spring/Autumn?
- 48. Summary • Rotation: Earth rotates l5° per hour in 24 hours. • Revolution: Earth takes 365.25 days to revolve around the sun moving approximately 1° per day.