The document provides information about the Earth and its position in the solar system. It discusses the Earth's rotation and revolution, and how this affects seasons. It also describes the globe and important lines of latitude and longitude that are used to locate places. Key features of the Earth such as its shape, layers, continents and oceans are summarized. Different types of maps and their uses are also outlined.
The document discusses the motions of the Earth, including its rotation on its axis and revolution around the Sun. It explains that rotation causes day and night and leads to the possibility of life, while revolution causes the changing of seasons. The Earth revolves around the Sun in an elliptical orbit over the course of 365.25 days to complete one year. The tilt of the Earth's axis relative to its orbital plane also helps determine the seasons.
The document summarizes key concepts about the Earth, moon, sun, and universe. It describes how the Earth rotates daily and revolves yearly around the sun, causing day/night and seasons. It also discusses the moon's phases, tides, and eclipses due to the positions of the Earth, moon and sun. Finally, it briefly outlines historic models of our solar system and discoveries about gravity and our sun.
1) The Earth revolves around the sun in an elliptical orbit over the course of 1 year, and its axial tilt of 23.5 degrees relative to the orbital plane causes the seasons.
2) As the Earth revolves, its hemispheres alternate between tilting towards and away from the sun, resulting in the summer and winter seasons in each hemisphere.
3) An analemma diagram can be used to determine the position of the subsolar point, solar noon time, and solar altitude for any location on Earth on any given date throughout the year.
The document describes the relative sizes and motions of the Earth, Moon, and Sun as seen from Mars. The Earth and Moon are spherical, and the Moon is about 1/4 the size of Earth. The Moon orbits Earth every 28 days and Earth orbits the Sun every 365 days. The Sun is about 110 times bigger than Earth and appears to move across the sky and rise in the east and set in the west, causing the cycle of night and day.
The document discusses the Sun, Earth, and Moon. The Sun is a big ball of gases that is the source of all energy. It takes 8.4 minutes for light from the Sun to reach Earth. The Earth orbits the Sun and is the only planet that supports life. The Moon orbits the Earth and reflects light from the Sun, taking 28 days to revolve around the Earth. Day and night on Earth occur due to its rotation, while the year occurs due to its revolution around the Sun.
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
-Windspeed and Direction
The document provides information about the Earth and its position in the solar system. It discusses the Earth's rotation and revolution, and how this affects seasons. It also describes the globe and important lines of latitude and longitude that are used to locate places. Key features of the Earth such as its shape, layers, continents and oceans are summarized. Different types of maps and their uses are also outlined.
The document discusses the motions of the Earth, including its rotation on its axis and revolution around the Sun. It explains that rotation causes day and night and leads to the possibility of life, while revolution causes the changing of seasons. The Earth revolves around the Sun in an elliptical orbit over the course of 365.25 days to complete one year. The tilt of the Earth's axis relative to its orbital plane also helps determine the seasons.
The document summarizes key concepts about the Earth, moon, sun, and universe. It describes how the Earth rotates daily and revolves yearly around the sun, causing day/night and seasons. It also discusses the moon's phases, tides, and eclipses due to the positions of the Earth, moon and sun. Finally, it briefly outlines historic models of our solar system and discoveries about gravity and our sun.
1) The Earth revolves around the sun in an elliptical orbit over the course of 1 year, and its axial tilt of 23.5 degrees relative to the orbital plane causes the seasons.
2) As the Earth revolves, its hemispheres alternate between tilting towards and away from the sun, resulting in the summer and winter seasons in each hemisphere.
3) An analemma diagram can be used to determine the position of the subsolar point, solar noon time, and solar altitude for any location on Earth on any given date throughout the year.
The document describes the relative sizes and motions of the Earth, Moon, and Sun as seen from Mars. The Earth and Moon are spherical, and the Moon is about 1/4 the size of Earth. The Moon orbits Earth every 28 days and Earth orbits the Sun every 365 days. The Sun is about 110 times bigger than Earth and appears to move across the sky and rise in the east and set in the west, causing the cycle of night and day.
The document discusses the Sun, Earth, and Moon. The Sun is a big ball of gases that is the source of all energy. It takes 8.4 minutes for light from the Sun to reach Earth. The Earth orbits the Sun and is the only planet that supports life. The Moon orbits the Earth and reflects light from the Sun, taking 28 days to revolve around the Earth. Day and night on Earth occur due to its rotation, while the year occurs due to its revolution around the Sun.
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
-Windspeed and Direction
The document provides information about the Earth-Moon system including:
1) The Earth rotates daily and revolves yearly around the Sun, causing seasons to change. It is tilted on its axis.
2) The Moon rotates and revolves around the Earth, always showing the same face. It reflects sunlight and has phases as its illuminated portion changes daily.
3) Humans have explored the Moon through missions like Apollo and Clementine, landing astronauts on the Moon from 1969-1972.
The moon orbits the Earth in a nearly perfect circle over the course of approximately 27 days, with the same side always facing the Earth. The Earth rotates on its axis over the course of 24 hours, causing the cycle of day and night, and revolves around the sun over the course of 365 days, causing the seasons. Additionally, the sun rotates on its axis once every 27 days.
The document discusses the motions and major divisions of the Earth. It describes how the Earth rotates on its axis once every 24 hours, causing the cycle of day and night. It also revolves around the sun once every 365 days. The document outlines the Equator and important latitudes and longitude lines that divide the Earth, such as the Tropic of Cancer and Prime Meridian. It explains phenomena related to day and night, such as varying day length depending on location and season, as well as different timekeeping systems used worldwide.
The document summarizes key concepts about the Earth's motion, including its rotation on its axis daily and revolution around the sun yearly. It describes how rotation causes day and night and affects the Earth's speed at different latitudes. Revolution is defined as the Earth's elliptical orbit around the sun, taking 365 days to complete. Seasons and solstices/equinoxes are explained in relation to the tilt of the Earth's axis. Other geographic concepts like latitude, longitude, the International Date Line and Prime Meridian are also briefly outlined.
The document describes Earth's rotation and revolution around the sun and how it causes the seasons. It states that Earth rotates on its axis over 24 hours, creating day and night, and revolves around the sun over 365 days, creating years. It also explains that Earth is tilted on its axis by 23.5 degrees and that the seasons occur due to whether the northern or southern hemispheres receive more direct sunlight from the sun throughout the year as Earth revolves.
The document discusses how Earth's interactions with the sun and moon cause night and day, seasons, and climate patterns. It explains that Earth's rotation on its axis causes day and night, while its revolution around the sun over the course of a year determines the seasons. The tilt of Earth's axis and latitude affect how direct sunlight hits different areas of the planet, making the equator warmer and poles colder. Seasons occur because the amount of direct sunlight varies throughout the year in different hemispheres.
The document provides information about the Solar System and celestial bodies. It discusses that the Solar System consists of the Sun and eight planets that orbit it, as well as asteroids, comets, and moons. It describes the Sun as the largest object and center of the Solar System. It also summarizes the basic characteristics and classifications of planets, asteroids, comets, and natural satellites or moons.
The document discusses different ways of representing the Earth, including globes, maps, and coordinate systems. It explains that globes accurately portray the spherical shape of the Earth, while maps are flat representations that provide more detailed information. It also describes how latitude and longitude are used to precisely locate places on maps using lines of meridians and parallels that divide the Earth into hemispheres and time zones.
The document discusses the motions of the Earth - rotation and revolution. It provides the following key details:
1. The Earth rotates on its axis, completing one rotation in 24 hours, which causes day and night. It revolves around the Sun, taking 365.25 days to complete one revolution.
2. The Earth's axis is inclined at an angle of approximately 23.5 degrees relative to the orbital plane. This inclination causes the seasons.
3. A leap year has 366 days to account for the extra time in the Earth's revolution around the Sun.
The Moon is Earth's only natural satellite and orbits our planet at a distance of about 384,000 kilometers. Though smaller than Earth, the Moon has a diameter of approximately 3,476 kilometers. The Moon revolves around Earth in a westward direction and appears differently throughout its monthly phases as the relative positions of the Moon, Earth, and Sun change. During a new moon, the side of the Moon facing Earth is not illuminated by the Sun.
Rotation and Revolution of the Earth
Aphelion and Perihelion
Four Seasons
Seasonal Changes
Solstice and Equinoxes
Standard Time Zones
Land of the Midnight Sun
This presentation discusses the effects of rotation and revolution on Earth. Rotation is the movement of Earth on its axis, causing day and night as well as high and low tides. Revolution is Earth's orbit around the sun, which causes the four seasons due to the tilt of Earth's axis. Revolution also results in varying lengths of days and nights throughout the year and changes in the altitude of the midday sun.
This document contains questions and answers about the rotation and revolution of the Earth and the causes of seasons. It explains that Christmas is celebrated in summer in Australia due to the Southern Hemisphere's opposite seasons. It also describes that the Earth's daily rotation causes day and night while its yearly revolution around the sun causes seasons. Additionally, it discusses how the tilt of the Earth's axis results in varying day lengths and 6 months of continuous daylight or darkness at the poles.
The document describes the rotation and revolution of the Earth. Rotation is the movement of the Earth on its axis, taking about 24 hours to complete one rotation. Revolution is the movement of the Earth around the Sun in a fixed orbit, taking 3651⁄4 days (one year) to revolve. Due to the tilt of the Earth's axis and its elliptical orbit, the Earth experiences seasons as different parts of the globe are exposed to more or less direct sunlight throughout the year.
The Giant Impact Theory proposes that the Moon was formed about 4.5 billion years ago from the debris of a collision between the early Earth and a Mars-sized protoplanet. This collision created a disk of molten rock and debris that eventually consolidated to form the Moon. Some earlier ideas on the Moon's formation included it forming alongside Earth or being captured after forming elsewhere in the solar system.
The Earth rotates on its axis, causing day and night. It takes 24 hours to complete one rotation. The Earth also revolves around the sun, which takes 365 days to complete one revolution. Due to the Earth's tilted axis and elliptical orbit, different parts of the Earth receive different intensities of sunlight over the course of a year, causing the seasons to change.
1. Earth rotates on its axis once every 24 hours, causing day and night. It also revolves around the sun once every 365.25 days in an elliptical orbit.
2. Earth's axis is tilted at an angle of 23.5 degrees, which causes seasons. It is closest to the sun in January and farthest in July.
3. In addition to rotating and revolving, Earth's axis undergoes a very slow wobble over 26,000 years called precession.
1) The seasons are caused by the tilt of the Earth's axis of rotation as it revolves around the sun, not by variations in distance from the sun.
2) As the Earth revolves around the sun, different parts of the planet are tilted either toward or away from the sun, receiving different amounts of sunlight and experiencing different seasons.
3) The tilt of the Earth's axis remains fixed at 23.5 degrees, causing the northern hemisphere to be tilted toward the sun during northern hemisphere summer and away from the sun during winter.
Grade 6 Ncert chapter 3 Motions of the EarthSreeDarshann
The document discusses the motions of the Earth - its rotation on its axis and revolution around the Sun. The Earth's rotation causes day and night and takes 24 hours. Without rotation, one side would always experience day and the other night. The Earth revolves around the Sun in an elliptical orbit, completing one revolution, or year, in 365.25 days. Its tilted axis and orbital position cause the seasons to change.
Rita and Gita are surprised to receive a letter from their friend Rahul in Singapore saying that Singapore is two hours ahead of India. They look at a globe to see the exact location of Singapore and see lines running across countries. The document goes on to explain that these lines are latitudes and longitudes, which help calculate the positions of countries and have been useful for explorers, the military, and pilots. It provides details on what a globe is, the axis and equator, hemispheres, parallels of latitude that run parallel to the equator, important parallels like the Tropics of Cancer and Capricorn, how latitude is measured, and heat zones on Earth based on latitude.
The document discusses latitudes and longitudes on a globe. It describes how the globe is tilted on its axis with the North and South poles. It discusses the equator line and parallels of latitude that run parallel to it. Important parallels mentioned include the Tropic of Cancer, Tropic of Capricorn, Arctic Circle, and Antarctic Circle. It also discusses longitude lines and the Prime Meridian that passes through Greenwich, England. Time zones are based on longitude, with places east of the Prime Meridian being ahead in time and places west being behind.
The document provides information about the Earth-Moon system including:
1) The Earth rotates daily and revolves yearly around the Sun, causing seasons to change. It is tilted on its axis.
2) The Moon rotates and revolves around the Earth, always showing the same face. It reflects sunlight and has phases as its illuminated portion changes daily.
3) Humans have explored the Moon through missions like Apollo and Clementine, landing astronauts on the Moon from 1969-1972.
The moon orbits the Earth in a nearly perfect circle over the course of approximately 27 days, with the same side always facing the Earth. The Earth rotates on its axis over the course of 24 hours, causing the cycle of day and night, and revolves around the sun over the course of 365 days, causing the seasons. Additionally, the sun rotates on its axis once every 27 days.
The document discusses the motions and major divisions of the Earth. It describes how the Earth rotates on its axis once every 24 hours, causing the cycle of day and night. It also revolves around the sun once every 365 days. The document outlines the Equator and important latitudes and longitude lines that divide the Earth, such as the Tropic of Cancer and Prime Meridian. It explains phenomena related to day and night, such as varying day length depending on location and season, as well as different timekeeping systems used worldwide.
The document summarizes key concepts about the Earth's motion, including its rotation on its axis daily and revolution around the sun yearly. It describes how rotation causes day and night and affects the Earth's speed at different latitudes. Revolution is defined as the Earth's elliptical orbit around the sun, taking 365 days to complete. Seasons and solstices/equinoxes are explained in relation to the tilt of the Earth's axis. Other geographic concepts like latitude, longitude, the International Date Line and Prime Meridian are also briefly outlined.
The document describes Earth's rotation and revolution around the sun and how it causes the seasons. It states that Earth rotates on its axis over 24 hours, creating day and night, and revolves around the sun over 365 days, creating years. It also explains that Earth is tilted on its axis by 23.5 degrees and that the seasons occur due to whether the northern or southern hemispheres receive more direct sunlight from the sun throughout the year as Earth revolves.
The document discusses how Earth's interactions with the sun and moon cause night and day, seasons, and climate patterns. It explains that Earth's rotation on its axis causes day and night, while its revolution around the sun over the course of a year determines the seasons. The tilt of Earth's axis and latitude affect how direct sunlight hits different areas of the planet, making the equator warmer and poles colder. Seasons occur because the amount of direct sunlight varies throughout the year in different hemispheres.
The document provides information about the Solar System and celestial bodies. It discusses that the Solar System consists of the Sun and eight planets that orbit it, as well as asteroids, comets, and moons. It describes the Sun as the largest object and center of the Solar System. It also summarizes the basic characteristics and classifications of planets, asteroids, comets, and natural satellites or moons.
The document discusses different ways of representing the Earth, including globes, maps, and coordinate systems. It explains that globes accurately portray the spherical shape of the Earth, while maps are flat representations that provide more detailed information. It also describes how latitude and longitude are used to precisely locate places on maps using lines of meridians and parallels that divide the Earth into hemispheres and time zones.
The document discusses the motions of the Earth - rotation and revolution. It provides the following key details:
1. The Earth rotates on its axis, completing one rotation in 24 hours, which causes day and night. It revolves around the Sun, taking 365.25 days to complete one revolution.
2. The Earth's axis is inclined at an angle of approximately 23.5 degrees relative to the orbital plane. This inclination causes the seasons.
3. A leap year has 366 days to account for the extra time in the Earth's revolution around the Sun.
The Moon is Earth's only natural satellite and orbits our planet at a distance of about 384,000 kilometers. Though smaller than Earth, the Moon has a diameter of approximately 3,476 kilometers. The Moon revolves around Earth in a westward direction and appears differently throughout its monthly phases as the relative positions of the Moon, Earth, and Sun change. During a new moon, the side of the Moon facing Earth is not illuminated by the Sun.
Rotation and Revolution of the Earth
Aphelion and Perihelion
Four Seasons
Seasonal Changes
Solstice and Equinoxes
Standard Time Zones
Land of the Midnight Sun
This presentation discusses the effects of rotation and revolution on Earth. Rotation is the movement of Earth on its axis, causing day and night as well as high and low tides. Revolution is Earth's orbit around the sun, which causes the four seasons due to the tilt of Earth's axis. Revolution also results in varying lengths of days and nights throughout the year and changes in the altitude of the midday sun.
This document contains questions and answers about the rotation and revolution of the Earth and the causes of seasons. It explains that Christmas is celebrated in summer in Australia due to the Southern Hemisphere's opposite seasons. It also describes that the Earth's daily rotation causes day and night while its yearly revolution around the sun causes seasons. Additionally, it discusses how the tilt of the Earth's axis results in varying day lengths and 6 months of continuous daylight or darkness at the poles.
The document describes the rotation and revolution of the Earth. Rotation is the movement of the Earth on its axis, taking about 24 hours to complete one rotation. Revolution is the movement of the Earth around the Sun in a fixed orbit, taking 3651⁄4 days (one year) to revolve. Due to the tilt of the Earth's axis and its elliptical orbit, the Earth experiences seasons as different parts of the globe are exposed to more or less direct sunlight throughout the year.
The Giant Impact Theory proposes that the Moon was formed about 4.5 billion years ago from the debris of a collision between the early Earth and a Mars-sized protoplanet. This collision created a disk of molten rock and debris that eventually consolidated to form the Moon. Some earlier ideas on the Moon's formation included it forming alongside Earth or being captured after forming elsewhere in the solar system.
The Earth rotates on its axis, causing day and night. It takes 24 hours to complete one rotation. The Earth also revolves around the sun, which takes 365 days to complete one revolution. Due to the Earth's tilted axis and elliptical orbit, different parts of the Earth receive different intensities of sunlight over the course of a year, causing the seasons to change.
1. Earth rotates on its axis once every 24 hours, causing day and night. It also revolves around the sun once every 365.25 days in an elliptical orbit.
2. Earth's axis is tilted at an angle of 23.5 degrees, which causes seasons. It is closest to the sun in January and farthest in July.
3. In addition to rotating and revolving, Earth's axis undergoes a very slow wobble over 26,000 years called precession.
1) The seasons are caused by the tilt of the Earth's axis of rotation as it revolves around the sun, not by variations in distance from the sun.
2) As the Earth revolves around the sun, different parts of the planet are tilted either toward or away from the sun, receiving different amounts of sunlight and experiencing different seasons.
3) The tilt of the Earth's axis remains fixed at 23.5 degrees, causing the northern hemisphere to be tilted toward the sun during northern hemisphere summer and away from the sun during winter.
Grade 6 Ncert chapter 3 Motions of the EarthSreeDarshann
The document discusses the motions of the Earth - its rotation on its axis and revolution around the Sun. The Earth's rotation causes day and night and takes 24 hours. Without rotation, one side would always experience day and the other night. The Earth revolves around the Sun in an elliptical orbit, completing one revolution, or year, in 365.25 days. Its tilted axis and orbital position cause the seasons to change.
Rita and Gita are surprised to receive a letter from their friend Rahul in Singapore saying that Singapore is two hours ahead of India. They look at a globe to see the exact location of Singapore and see lines running across countries. The document goes on to explain that these lines are latitudes and longitudes, which help calculate the positions of countries and have been useful for explorers, the military, and pilots. It provides details on what a globe is, the axis and equator, hemispheres, parallels of latitude that run parallel to the equator, important parallels like the Tropics of Cancer and Capricorn, how latitude is measured, and heat zones on Earth based on latitude.
The document discusses latitudes and longitudes on a globe. It describes how the globe is tilted on its axis with the North and South poles. It discusses the equator line and parallels of latitude that run parallel to it. Important parallels mentioned include the Tropic of Cancer, Tropic of Capricorn, Arctic Circle, and Antarctic Circle. It also discusses longitude lines and the Prime Meridian that passes through Greenwich, England. Time zones are based on longitude, with places east of the Prime Meridian being ahead in time and places west being behind.
This document discusses how coordinate systems using longitude and latitude can be used to locate places on Earth. Longitude lines run north-south and are used to locate west-east positions. Latitude lines run east-west and locate north-south positions. Key points include the Prime Meridian at 0 degrees longitude, the Equator at 0 degrees latitude, and the poles at 90 degrees latitude. Several activities are provided to practice identifying locations based on their longitude and latitude coordinates.
1. A globe is a miniature model of the Earth that shows its true spherical shape and allows locations to be precisely pinpointed using lines of latitude and longitude.
2. The globe can be rotated on its axis and is marked with the Equator, Tropic of Cancer at 23.5° N, Tropic of Capricorn at 23.5° S, and other important parallels of latitude. Meridians of longitude divide the globe into Eastern and Western hemispheres.
3. Locations are specified using their latitude and longitude coordinates - degrees north or south of the Equator, and degrees east or west of the Prime Meridian passing through Greenwich, England. This grid system allows any place
_L-14 The Globe- Latitudes and Longitudes new.pptxpadminijyothi
Here are the answers:
1. The local time of a place situated 60° W of London will be 6 pm if it is noon in London. Since each 15° of longitude represents a 1 hour time difference, and the place is 60° west of London, the time difference will be 60/15 = 4 hours. So if it is noon in London, the local time at the place 60° W will be noon + 4 hours = 6 pm.
2. The local time of a place situated 90° E of London will be 3 pm if it is 9 am in London. Since each 15° of longitude represents a 1 hour time difference, and the place is 90° east of London, the time difference will be
1. The document discusses the structure and content of a unit on planet Earth and its representation. It will cover topics like the shape and movements of the Earth, coordinates, maps, and time zones.
2. Key concepts that will be explained include the rotation and revolution of the Earth, latitude and longitude, map projections that represent the spherical Earth on a flat surface, and different types of maps and scales.
3. Questions to be answered relate to the position of Earth in the solar system, its movements and seasons, geographic coordinates, representations of Earth, and defining features of maps like scale and time zones. Useful vocabulary is also provided.
The seasons are caused by two factors: 1) the tilt of the Earth's axis of rotation relative to its orbit around the Sun, and 2) the Earth's revolution around the Sun. The tilt causes different amounts of sunlight to reach different parts of the Earth throughout the year, with more direct sunlight during the summer and less direct sunlight during the winter. Additionally, the Earth's revolution means different hemispheres receive more or less direct sunlight over the course of a year, contributing to the seasons.
The Earth is not a perfect sphere, but is slightly flattened at the poles. The Earth rotates daily on its tilted axis, causing seasons and influencing climate. Parallels of latitude and meridians of longitude form a grid system to locate positions on the Earth's surface. The Earth revolves around the Sun annually in an elliptical orbit, with the seasons resulting from the tilt of its axis of rotation. Precise geodetic coordinates define locations on the reference ellipsoid used to model the oblate spheroid shape of the Earth.
This document provides an introduction to Antarctica and the Antarctic region. It explains that Antarctica refers to the continent, while Antarctic refers to the entire southern polar region including surrounding oceans. Most of Antarctica is covered by over 2 km of snow and ice, and large glaciers flow toward the coast, forming ice shelves over the ocean. The polar regions are colder than other areas due to the low angle of incoming sunlight, which provides less energy. Additionally, the polar night during winters leads to long periods without any sunlight. Compared to the Arctic, Antarctica experiences colder average temperatures because it is surrounded by cold ocean currents that do not mix with warmer waters, its higher average elevation, and its position as a continental landmass surrounded by ocean
This document provides an introduction to Antarctica and the Antarctic region. It explains that Antarctica refers to the continent, while Antarctic refers to the entire southern polar region surrounding the continent. Most of Antarctica is covered by over 2 km of snow and ice. The Antarctic region is defined either by ocean boundaries or as anywhere south of the Antarctic Circle, which experiences at least one day and one night of sunlight/darkness per year. The polar regions are colder due to the low angle of incoming sunlight, which provides less energy, as well as periods of extended darkness. Antarctica is even colder than the Arctic because it is surrounded by cold ocean waters that do not mix with warmer currents, it is higher in altitude, and its sea ice reflects
The document summarizes key information about planet Earth and its place in the solar system. It describes Earth's structure, including the atmosphere, hydrosphere, and lithosphere. It also discusses Earth's rotation and revolution around the sun, which causes seasons. The document explains how to locate places using latitude and longitude coordinates on maps and read different types of maps. It provides details on time zones and how the Earth is divided for time.
The seasons are caused by two factors: 1) the tilt of the Earth's axis and 2) the Earth's revolution around the sun. The tilt of the Earth's axis causes different locations to receive different amounts of solar radiation throughout the year, similar to how the intensity of light from a flashlight changes depending on its angle. Additionally, the Earth's revolution means the most direct sunlight shifts between the Northern and Southern hemispheres over the course of a year, bringing warmer weather to each hemisphere in turn.
The seasons are caused by two factors: 1) the tilt of the Earth's axis and 2) the Earth's revolution around the Sun. The tilt of the Earth's axis causes different intensities of sunlight throughout the year depending on the angle of sunlight. The Earth's revolution means that different parts of the Earth receive more direct sunlight during different parts of the year, causing the seasons to shift. Specifically, summer occurs in the Northern Hemisphere when it is tilted toward the Sun, winter when it is tilted away, and spring and fall during the equinoxes when the sunlight is most indirect.
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.
This document provides information about the Earth's geography. It begins by describing the Earth's shape as a sphere and its rotation on an axis. It then defines key geographic terms like poles, hemispheres, and latitude and longitude. Subsequent sections explain concepts such as time zones, ocean currents, climate zones, and the composition of the Earth. Activities are included throughout to reinforce the material. The document serves as a comprehensive overview of basic Earth science concepts.
The document discusses key concepts related to globes and maps. It explains that a globe is a miniature model of the Earth that can be rotated to accurately show the sizes and positions of continents, oceans, and other geographic features. Parallels of latitude and meridians of longitude form a grid system on a globe, with the equator dividing it into northern and southern hemispheres. The Prime Meridian passes through Greenwich, England and longitude is measured in degrees east and west from there. The document also discusses time zones and how local times differ depending on a place's longitude.
The document discusses globes and maps. It explains that a globe is a small model of the Earth that shows its round shape and can be used to study concepts like day and night and seasons. A globe also shows the Earth's axis that it rotates around and identifies the North and South Poles. The document further explains other important lines and features on globes like the Equator, Prime Meridian, hemispheres, latitudes and longitudes. It describes how these are used to locate different places on Earth.
The document discusses how the Earth moves in space and why seasons change. It explains that the Earth rotates on its axis over 24 hours, causing day and night, and revolves around the Sun over the course of a year. The Earth's tilted axis and elliptical orbit cause the seasons, with regions facing the Sun more directly experiencing longer days and warmer temperatures. The document also describes the latitudinal zones of the tropics, temperate, and polar regions and how temperatures vary across these zones.
Aerial NAVIGATION and FLIGHT PLANNING.pptxEhtasham Amir
Air navigation for BS aviation
undergraduate programme . This ppt explains basic concepts of air navigation. this is used to teach BS aviation, undergrad
The document discusses political parties in India. It begins by defining what a political party is and their key functions, which include contesting elections, putting forward policies, making laws, forming governments, and acting as opposition. It then discusses the types of political parties in India, distinguishing between national parties and state or regional parties. The national parties that are recognized by the Election Commission are discussed. Finally, it outlines some challenges faced by political parties such as lack of internal democracy, dynastic succession, money and muscle power influence, and lack of meaningful choice for voters.
What does democracy do?
What outcomes can we reasonably expect of democracy?
Does democracy fulfil these expectations in real life?
How to assess the outcomes of democracy?
Democracy is better because
Accountable, responsive and legitimate government
ELECTION,DEBATE AND INFORMATION
PEOPLE’S NEED AND CORRUPTION
Economic growth and development
Reduction of inequality and poverty
Accommodation of social diversity
Dignity and freedom of the citizens
Means of Transportations
Roadways
Golden Quadrilateral Super Highways
• National Highways
State Highways:
District Roads
Other Roads
Border Road
Railways
Pipelines
Waterways
Major Sea Ports
Airways
Communication
International Trade
Tourism as a Trade
GLOBALISATION AND INDIAN ECONOMY CLASS 10 X NCERT CBSEMahendra SST
How do we understand these rapid transformations?
PRODUCTION ACROSS COUNTRY
SPREADING Of PRODUCTION By MNC –
INTERLINKING PRODUCTION ACROSS COUNTRY-
MNCs set up production jointly with some of the local companies.
FOREIGN TRADE AND INTEGRATION OF MARKET –
WHAT IS GLOBALISATION-
FACTORS THAT ENABLED GLOBALISATION-
LIBERLISATION –
Removing barriers or restrictions set by the government is what is known as liberalisation.
WORLD TRADE ORGANISATION-
DEVELOPMENT
What is Development –
What Development Promises – Different People Different Goal
Income And Other Goal
National Development
How To Compare Different Countries Or States
Income And Other Criteria
Public Facilities
Sustainability of Development
ncert cbse class 10ecinomics
2 role of the government in health class vii 7Mahendra SST
NCERT CBSE SOCIAL SCIENCE CLASS 6,7,8,9,10 HISTORY POLITICAL SCIENCE GEOGRAPHY ECONOMICS
IN THIS CHAPTER YOU WILL GET ACCESS ABOUT CLASS SUBJECT SPL CHAPTER ROLE OF GOVT IN HEALTH What is health?
THE COST OF A CURE
Division Of Health Services
(a) Public health services and
(b) Private health facilities
Is adequate healthcare available to all?
What can be done?
The Kerala experience
The Costa Rican approach
1 tracing changes through a thousand yearsMahendra SST
This document provides an overview of changes in India from approximately 700 CE to 1750 CE. It discusses how maps of India changed significantly over this thousand-year period as information improved. New social and political groups emerged during this time taking advantage of economic opportunities. Religions like Hinduism and Islam saw major developments as beliefs evolved with changes in social organization. Historians study this period using sources like manuscripts, coins, inscriptions and architecture, though manuscripts pose challenges due to copying errors over time.
NCERT CBSE SOCIAL SCIENCE CLASS 6,7,8,9,10 HISTORY POLITICAL SCIENCE GEOGRAPHY ECONOMICS
IN THIS CHAPTER YOU WILL GET ACCESS ABOUT CLASS 6 HISORY CHAPTER WHAT WHERE HOW AND WHEN
NCERT CBSE SOCIAL SCIENCE CLASS 6,7,8,9,10 HISTORY POLITICAL SCIENCE GEOGRAPHY ECONOMICS
IN THIS CHAPTER YOU WILL GET ACCESS ABOUT CLASS 6 HISORY CHAPTER WHAT WHERE HOW AND WHEN
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CBSE NCERT SOCIAL SCIENCE HISTORY GEOGRAPHY ECONOMICS POLITICAL SCIENCE CLASS 9 CHAPTER the story of village palampur factors of production farming in palampur non farming activities land labour physical capital fixed capital working capital human capital
CBSE NCERT SOCIAL AND POLITICAL LIFE CLASS 6 CHAPTER GOVERNMENT ITS FUNCTIONS DIFFERENCE BETWEEN MONARCHY AND DEMOCRACY DEMOCRATIC REPRESENTATIVE GOVT RIGHT TO VOTE
The document summarizes information about the ancient Indus Valley Civilization city of Harappa. It describes how Harappa was discovered in modern-day Pakistan when engineers building railway lines removed bricks from old buildings. Archaeologists later realized it was an ancient city dating back 4,700 years. These cities had fortified walls, elaborate baths and storehouses, and houses built around courtyards connected to drainage systems. Residents practiced crafts like weaving and metalworking. The cities organized trade networks to obtain raw materials from distant lands. By around 3,900 years ago, many cities were abandoned as the rulers lost control and residents moved to smaller settlements, though the exact reasons for the civilization's decline are unknown.
CBSE NCERT SOCIAL SCIENCE HISTORY GEOGRAPHY ECONOMICS POLITICAL SCIENCE CLASS 10 CHAPTER money and credit barter system modern form of noney formal and informal sectors of credit collateral terms of credit
CBSE NCERT SOCIAL SCIENCE HISTORY GEOGRAPHY ECONOMICS POLITICAL SCIENCE CLASS 10 CHAPTER political parties components of political parties national and state parties how can political parties are reformed
CBSE NCERT SOCIAL SCIENCE HISTORY GEOGRAPHY ECONOMICS POLITICAL SCIENCE CLASS 9 CHAPTER our detailed election process constituencies candidate nomination challenges to election process
This document provides information about minerals and energy resources in India. It discusses the different types of minerals found in India such as iron ore, manganese, copper, bauxite, mica and limestone. It describes where these minerals are located and how they are used. It also covers the major forms in which minerals occur, including in igneous and sedimentary rocks, as residual deposits, and in ocean waters. In addition, the document discusses India's energy resources such as coal, petroleum, natural gas, hydroelectricity, and non-conventional sources like solar and wind energy. It provides details on production of coal, petroleum and natural gas in key regions of India.
Main Java[All of the Base Concepts}.docxadhitya5119
This is part 1 of my Java Learning Journey. This Contains Custom methods, classes, constructors, packages, multithreading , try- catch block, finally block and more.
This slide is special for master students (MIBS & MIFB) in UUM. Also useful for readers who are interested in the topic of contemporary Islamic banking.
How to Make a Field Mandatory in Odoo 17Celine George
In Odoo, making a field required can be done through both Python code and XML views. When you set the required attribute to True in Python code, it makes the field required across all views where it's used. Conversely, when you set the required attribute in XML views, it makes the field required only in the context of that particular view.
This document provides an overview of wound healing, its functions, stages, mechanisms, factors affecting it, and complications.
A wound is a break in the integrity of the skin or tissues, which may be associated with disruption of the structure and function.
Healing is the body’s response to injury in an attempt to restore normal structure and functions.
Healing can occur in two ways: Regeneration and Repair
There are 4 phases of wound healing: hemostasis, inflammation, proliferation, and remodeling. This document also describes the mechanism of wound healing. Factors that affect healing include infection, uncontrolled diabetes, poor nutrition, age, anemia, the presence of foreign bodies, etc.
Complications of wound healing like infection, hyperpigmentation of scar, contractures, and keloid formation.
This presentation includes basic of PCOS their pathology and treatment and also Ayurveda correlation of PCOS and Ayurvedic line of treatment mentioned in classics.
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A review of the growth of the Israel Genealogy Research Association Database Collection for the last 12 months. Our collection is now passed the 3 million mark and still growing. See which archives have contributed the most. See the different types of records we have, and which years have had records added. You can also see what we have for the future.
LAND USE LAND COVER AND NDVI OF MIRZAPUR DISTRICT, UPRAHUL
This Dissertation explores the particular circumstances of Mirzapur, a region located in the
core of India. Mirzapur, with its varied terrains and abundant biodiversity, offers an optimal
environment for investigating the changes in vegetation cover dynamics. Our study utilizes
advanced technologies such as GIS (Geographic Information Systems) and Remote sensing to
analyze the transformations that have taken place over the course of a decade.
The complex relationship between human activities and the environment has been the focus
of extensive research and worry. As the global community grapples with swift urbanization,
population expansion, and economic progress, the effects on natural ecosystems are becoming
more evident. A crucial element of this impact is the alteration of vegetation cover, which plays a
significant role in maintaining the ecological equilibrium of our planet.Land serves as the foundation for all human activities and provides the necessary materials for
these activities. As the most crucial natural resource, its utilization by humans results in different
'Land uses,' which are determined by both human activities and the physical characteristics of the
land.
The utilization of land is impacted by human needs and environmental factors. In countries
like India, rapid population growth and the emphasis on extensive resource exploitation can lead
to significant land degradation, adversely affecting the region's land cover.
Therefore, human intervention has significantly influenced land use patterns over many
centuries, evolving its structure over time and space. In the present era, these changes have
accelerated due to factors such as agriculture and urbanization. Information regarding land use and
cover is essential for various planning and management tasks related to the Earth's surface,
providing crucial environmental data for scientific, resource management, policy purposes, and
diverse human activities.
Accurate understanding of land use and cover is imperative for the development planning
of any area. Consequently, a wide range of professionals, including earth system scientists, land
and water managers, and urban planners, are interested in obtaining data on land use and cover
changes, conversion trends, and other related patterns. The spatial dimensions of land use and
cover support policymakers and scientists in making well-informed decisions, as alterations in
these patterns indicate shifts in economic and social conditions. Monitoring such changes with the
help of Advanced technologies like Remote Sensing and Geographic Information Systems is
crucial for coordinated efforts across different administrative levels. Advanced technologies like
Remote Sensing and Geographic Information Systems
9
Changes in vegetation cover refer to variations in the distribution, composition, and overall
structure of plant communities across different temporal and spatial scales. These changes can
occur natural.
Chapter wise All Notes of First year Basic Civil Engineering.pptxDenish Jangid
Chapter wise All Notes of First year Basic Civil Engineering
Syllabus
Chapter-1
Introduction to objective, scope and outcome the subject
Chapter 2
Introduction: Scope and Specialization of Civil Engineering, Role of civil Engineer in Society, Impact of infrastructural development on economy of country.
Chapter 3
Surveying: Object Principles & Types of Surveying; Site Plans, Plans & Maps; Scales & Unit of different Measurements.
Linear Measurements: Instruments used. Linear Measurement by Tape, Ranging out Survey Lines and overcoming Obstructions; Measurements on sloping ground; Tape corrections, conventional symbols. Angular Measurements: Instruments used; Introduction to Compass Surveying, Bearings and Longitude & Latitude of a Line, Introduction to total station.
Levelling: Instrument used Object of levelling, Methods of levelling in brief, and Contour maps.
Chapter 4
Buildings: Selection of site for Buildings, Layout of Building Plan, Types of buildings, Plinth area, carpet area, floor space index, Introduction to building byelaws, concept of sun light & ventilation. Components of Buildings & their functions, Basic concept of R.C.C., Introduction to types of foundation
Chapter 5
Transportation: Introduction to Transportation Engineering; Traffic and Road Safety: Types and Characteristics of Various Modes of Transportation; Various Road Traffic Signs, Causes of Accidents and Road Safety Measures.
Chapter 6
Environmental Engineering: Environmental Pollution, Environmental Acts and Regulations, Functional Concepts of Ecology, Basics of Species, Biodiversity, Ecosystem, Hydrological Cycle; Chemical Cycles: Carbon, Nitrogen & Phosphorus; Energy Flow in Ecosystems.
Water Pollution: Water Quality standards, Introduction to Treatment & Disposal of Waste Water. Reuse and Saving of Water, Rain Water Harvesting. Solid Waste Management: Classification of Solid Waste, Collection, Transportation and Disposal of Solid. Recycling of Solid Waste: Energy Recovery, Sanitary Landfill, On-Site Sanitation. Air & Noise Pollution: Primary and Secondary air pollutants, Harmful effects of Air Pollution, Control of Air Pollution. . Noise Pollution Harmful Effects of noise pollution, control of noise pollution, Global warming & Climate Change, Ozone depletion, Greenhouse effect
Text Books:
1. Palancharmy, Basic Civil Engineering, McGraw Hill publishers.
2. Satheesh Gopi, Basic Civil Engineering, Pearson Publishers.
3. Ketki Rangwala Dalal, Essentials of Civil Engineering, Charotar Publishing House.
4. BCP, Surveying volume 1
A workshop hosted by the South African Journal of Science aimed at postgraduate students and early career researchers with little or no experience in writing and publishing journal articles.
5. AXIS
A needle is fixed through the globe in a tilted
manner, which is called its axis.
Two points on the globe through which the needle
passes are two poles – North Pole and South Pole.
The real earth has no such needle. It moves
around its axis, which is an imaginary line
8. LATITUDE
An imaginary line running on the globe divides it into two equal parts. This
line is known as the equator
the equator is an imaginary circular line
All parallel circles from the equator up to the poles are called parallels of
latitudes. Latitudes are measured in degrees.
The equator represents the zero degree latitude.
The northern half of the earth is known as the Northern Hemisphere and
the southern half is known as the Southern Hemisphere
12. HEAT ZONES OF THE EARTH
Torrid Zone - The mid-day sun is exactly overhead at least once a year on
all latitudes in between the Tropic of Cancer and the Tropic of Capricorn.
This area, therefore, receives the maximum heat and is called the Torrid
Zone
13. HEAT ZONES OF THE EARTH
Temperate Zones -The mid-day sun never shines overhead on any latitude
beyond the Tropic of Cancer and the Tropic of Capricorn. The angle of the
sun’s rays goes on decreasing towards the poles. As such, the areas
bounded by the Tropic of Cancer and the Arctic Circle in the Northern
Hemisphere, and the Tropic of Capricorn and the Antarctic Circle in the
Southern Hemisphere, have moderate temperatures. These are,
therefore, called Temperate Zones
14. HEAT ZONES OF THE EARTH
Frigid Zones - Areas lying between the Arctic Circle and the North Pole in
the Northern Hemisphere and the Antarctic Circle and the South Pole in
the Southern Hemisphere, are very cold. It is because here the sun does
not rise much above the horizon. Therefore, its rays are always slanting
and provide less heat. These are, therefore, called Frigid Zones (very
cold).
15. VOTE OF THANKS
1 NCERT BOOKS
2 INTERNERT AND GOOGLE
3 ENCYCLOPEDIA BRITANNICA
4 MY VIEWERS