Motion of earth
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The document discusses the two types of motions of the Earth: rotation and revolution. Rotation is the movement of the Earth on its axis, which takes 24 hours to complete one rotation. Revolution is the movement of the Earth around the sun, which takes 365.25 days to complete one revolution. Due to these motions, different parts of the Earth experience day and night, and the seasons change throughout the year.
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rotation and revolution
The document discusses different types of rotational and orbital motions of objects in space, including the Earth. It explains that the Earth's rotation on its axis causes day and night, while its revolution around the sun over the course of a year leads to seasonal variations due to changes in the sun's angle and day length. Examples of rotation are a top spinning on its axis or the Earth each day, while examples of revolution are the Earth orbiting the sun each year or the moon revolving around the Earth.
Motion of the earth
The document discusses the two types of motion of the Earth: rotation and revolution. It explains that the Earth rotates on its axis once every 24 hours, causing day and night. It also revolves around the Sun, completing one revolution every 365.25 days, and this revolution causes the changing of seasons as the Earth's distance from the Sun and the angle of sunlight hitting the Earth vary throughout the year.
Motion of the earth
A power point that is designed to explain the effects of the Rotation and Revolution on the Earth.
-Day and Night
-The four seasons
-Solstice and Equinox
-High tide and low tide
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Class6 Earth Rotation And Revolution
The document discusses the two motions of the Earth: rotation and revolution. It notes that rotation is the Earth spinning on its axis once every 24 hours, which causes day and night. Revolution is the Earth orbiting the Sun in an elliptical orbit, taking 365 days to complete one revolution and causing the seasons due to changes in distance from the Sun throughout the year. The rotation of the Earth occurs at approximately 15 degrees per hour and spins at over 1600 km/hr at the equator.
Earths movement-rotation-vs-revolution-powerpoint-english
The document discusses the Earth's rotation and revolution in space. It explains that the Earth rotates on its axis once every 24 hours, causing day and night, and revolves around the Sun once every 365.25 days, creating the seasons. The tilt of the Earth's axis combined with its revolution is what causes the seasons in both the northern and southern hemispheres.
The Earth, Rotation and Revolution
The Earth has two movements: rotation and revolution. Rotation is the Earth spinning on its axis every 24 hours, causing day and night. Revolution is the Earth orbiting the Sun every 365 days, causing seasons and years. Due to these movements, different parts of the Earth receive varying amounts of sunlight, influencing climate zones and seasons. The tilt of the Earth's axis and its position in orbit also affect the length of daylight and temperature changes throughout the year.
Motions of earth school level
The document discusses the rotation and revolution of Earth and their effects. It notes that Earth rotates on its axis in a counter-clockwise direction over 24 hours, causing day and night. Earth also revolves around the sun in an elliptical orbit over approximately 1 year, resulting in varying lengths of day and causing the changing of seasons. Specifically, it explains that summer solstice occurs when the North Pole is tilted toward the sun, winter solstice when it is tilted away, and equinoxes when sunlight is equal between hemispheres.
The movements of the Earth
The Earth moves in two ways: by rotating on its axis daily, and by revolving around the Sun yearly. The Earth's tilted axis and oval-shaped orbit cause the seasons by changing the angle and duration of sunlight received in different parts of the world throughout the year. The rotation of the Earth causes day and night, and the revolution around the Sun in 365 days causes the four seasons as the Earth's positioning shifts solstices and equinoxes.
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rotation and revolution
The document discusses different types of rotational and orbital motions of objects in space, including the Earth. It explains that the Earth's rotation on its axis causes day and night, while its revolution around the sun over the course of a year leads to seasonal variations due to changes in the sun's angle and day length. Examples of rotation are a top spinning on its axis or the Earth each day, while examples of revolution are the Earth orbiting the sun each year or the moon revolving around the Earth.
Motion of the earth
The document discusses the two types of motion of the Earth: rotation and revolution. It explains that the Earth rotates on its axis once every 24 hours, causing day and night. It also revolves around the Sun, completing one revolution every 365.25 days, and this revolution causes the changing of seasons as the Earth's distance from the Sun and the angle of sunlight hitting the Earth vary throughout the year.
Motion of the earth
A power point that is designed to explain the effects of the Rotation and Revolution on the Earth.
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-The four seasons
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-High tide and low tide
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The document discusses the two motions of the Earth: rotation and revolution. It notes that rotation is the Earth spinning on its axis once every 24 hours, which causes day and night. Revolution is the Earth orbiting the Sun in an elliptical orbit, taking 365 days to complete one revolution and causing the seasons due to changes in distance from the Sun throughout the year. The rotation of the Earth occurs at approximately 15 degrees per hour and spins at over 1600 km/hr at the equator.
Earths movement-rotation-vs-revolution-powerpoint-english
The document discusses the Earth's rotation and revolution in space. It explains that the Earth rotates on its axis once every 24 hours, causing day and night, and revolves around the Sun once every 365.25 days, creating the seasons. The tilt of the Earth's axis combined with its revolution is what causes the seasons in both the northern and southern hemispheres.
The Earth, Rotation and Revolution
The Earth has two movements: rotation and revolution. Rotation is the Earth spinning on its axis every 24 hours, causing day and night. Revolution is the Earth orbiting the Sun every 365 days, causing seasons and years. Due to these movements, different parts of the Earth receive varying amounts of sunlight, influencing climate zones and seasons. The tilt of the Earth's axis and its position in orbit also affect the length of daylight and temperature changes throughout the year.
Motions of earth school level
The document discusses the rotation and revolution of Earth and their effects. It notes that Earth rotates on its axis in a counter-clockwise direction over 24 hours, causing day and night. Earth also revolves around the sun in an elliptical orbit over approximately 1 year, resulting in varying lengths of day and causing the changing of seasons. Specifically, it explains that summer solstice occurs when the North Pole is tilted toward the sun, winter solstice when it is tilted away, and equinoxes when sunlight is equal between hemispheres.
The movements of the Earth
The Earth moves in two ways: by rotating on its axis daily, and by revolving around the Sun yearly. The Earth's tilted axis and oval-shaped orbit cause the seasons by changing the angle and duration of sunlight received in different parts of the world throughout the year. The rotation of the Earth causes day and night, and the revolution around the Sun in 365 days causes the four seasons as the Earth's positioning shifts solstices and equinoxes.
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The document summarizes the rotation and revolution of the Earth. It explains that the Earth rotates on its axis from west to east over 24 hours, causing day and night. It also revolves around the sun, completing one revolution every 365.25 days. The tilt of the Earth's axis at 23.4 degrees, combined with its revolution, causes the seasons by influencing the distribution of sunlight through the year. Leap years add an additional day every four years to synchronize the calendar year with the astronomical year.
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This lesson plan is for a 6th grade class on the rotation and revolution of the Earth. It includes objectives for students to understand key terms like rotation, revolution, axis, and seasons. Activities include using a globe to demonstrate rotation, a poster on revolution, and a worksheet. A video and diagrams are provided. Formative assessments include labeling diagrams, questions, and crosswords. The lesson aims to help students understand why the sun's position changes and what causes seasons.
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Understanding the concept of continuous and comprehensive evauation.
Understanding the concept of continuous and comprehensive evauation.
Educational technology presenting the art of teaching in
Educational technology presenting the art of teaching in
Motion of earth
- 1. Pooja Singhal, Ph.D Research Scholar, JMI. OF EARTH MOTION
- 2. Pooja Singhal, Ph.D Research Scholar, JMI. OF MOTIONS TWO TYPES EARTH HAS
- 3. Pooja Singhal, Ph.D Research Scholar, JMI. EARTH REVOLUTION ROTATION
- 4. Pooja Singhal, Ph.D Research Scholar, EARTH ON ITS AXIS JMI. MOVEMENT OF THE ROTATION
- 5. REVOLUTION JMI. Pooja Singhal, Ph.D Research Scholar, MOVEMENT OF THE EARTH AROUND THE SUN
- 6. Pooja Singhal, Ph.D Research Scholar, JMI. AXIS
- 7. CIRCLE OF ILLUMINATION DUE TO SPERICAL SHAPE, HALF OF THE JMI. Pooja Singhal, Ph.D Research Scholar, EARTH FACE SUN
- 8. JMI. Pooja Singhal, Ph.D Research Scholar, SIDE FACING THE SUN HAVE DAY AND THE OTHER SIDE EXPERIENCE NIGHT
- 9. THE CIRCLE THAT DIVIDES THE DAY FROM NIGHT ON THE GLOBE IS CALLED CIRCLE OF JMI. Pooja Singhal, Ph.D Research Scholar, ILLUMINATION
- 10. EARTH TAKES 24 HOURS TO COMPLEATE ONE JMI. Pooja Singhal, Ph.D Research Scholar, ROTATION THISPERIOD IS CALLED EARTH DAY
- 11. Pooja Singhal, Ph.D Research Scholar, JMI. DO YOU THINK IMPORTANT? ROTATION IS
- 12. Pooja Singhal, Ph.D Research Scholar, JMI. NOT ROTATE? EARTH DID HAPPEN IF WHAT WILL
- 13. Pooja Singhal, Ph.D Research Scholar, JMI. AROUND THE SUN TAKES PLACE REVOLUTION
- 14. IT TAKES 365.25 DAYS TO REVOVE AROUND THE JMI. Pooja Singhal, Ph.D Research Scholar, SUN
- 15. JMI. Pooja Singhal, Ph.D Research Scholar, WE TAKE 365 DAYS IN A YEAR AND IGNORE 6 HOURS
- 16. KEEP ON ADDING THESE SIX HOURS FOR JMI. Pooja Singhal, Ph.D Research Scholar, FOUR YEARS
- 17. 6+6+6+6= 24 HOURS= 1 DAY JMI. Pooja Singhal, Ph.D Research Scholar, THE FORTH YEAR WILL BE OF 366 YRS = LEAP YEAR
- 18. IN LEAP YEAR 1 DAY IS ADDED TO THE MONTH OF FEBRUARY JMI. Pooja Singhal, Ph.D Research Scholar, FEBURARY= 28 DAYS FEBURARY= 29 DAYS (LEAP YEAR)
- 19. Pooja Singhal, Ph.D Research Scholar, JMI. SEASONS DO WE HOW MANY HAVE ON EARTH?
- 20. 1 YEAR IS DIVIDED INTO FOUR YEARS SUMMER WINTER JMI. Pooja Singhal, Ph.D Research Scholar, SEASONS SPRING AUTUMN
- 21. Pooja Singhal, Ph.D Research Scholar, JMI. CHANGES TAKES HOW DOES SEASONS? PLACE IN
- 22. Pooja Singhal, Ph.D Research Scholar, JMI. THINK? THINK? THINK?