SlideShare a Scribd company logo
1 of 27
EIGHT MOTIONS OF EARTH
MEMB ER S:
MARY JOY BERNABE
NELMARIE RIVERA
NICOLE ANDRIEL PRAGOSO
NOVA UGBINADA
PAMELA RICO
RHODARINE BANTAD
ROSALIEALITAO
OBJECTIVE:
• Differentiating the types of
varations and emotions of the
effects.
• Explaining different land forms area
of the Earth
1. The Earth Rotates About Its Axis
 Earth moves through space in several important ways. One type of
motion is called rotation. A rotation is a spin around a center.
 Earth also spins around a central line called an axis. Earth’s axis is an
imaginary vertical line that runs through the planet from the North Pole
to the South Pole.
• The Earth has a circumference (measured around at the Equator) of
approximately 40,075 km (24,901 mi). And 40,007.863 km
(24,859.734 mi) when measured around the poles.
• The Earth rotates on its axis relative to the Sun in one “Mean Solar Day"
• It rotates exactly 360° in one "Mean Sidereal Day" which is 86,164.0909
seconds, or 23 hrs 56 min 4.0909 seconds.
Solar day (24 hours)
The Earth makes one rotation compared with the Sun.
3 minutes 56 seconds longer than a sidereal day.
Sidereal day (23 hours 56 minutes 4.0909 seconds)
The Earth makes one rotation compared with the distant
stars.
3 minutes 56 seconds shorter than a solar day
2. Earth-Moon System Orbits a "Gravitational Centre"
● Both the Moon and the Earth orbit
a common centre of gravity
● The mass of the Earth (ME) is
5.9742 * 1024 kg, and the mass of
the Moon is 7.349 * 1022 kg - the
Ratio of the masses is 81.3
● So the centre of gravity is
therefore located 1 unit from the
Earth's centre and 81.3 units from
the Moon's centre
● Earth pivots around this point
once every Lunar Month
● The Earth's orbit around the Sun is an
ellipse and travels at different speeds
during the year - slowest at Aphelion
(furthest point from the Sun) and fastest
at Perihelion (closest point to the Sun)
● Earth's orbit (the path) is approximately
940,000,000 km (580,000,000 mi) in
365.2421896698 days
● So the "year" is not exactly 365¼ days
(sometimes called the Julian Year).
● Earth's speed around the sun Speed =
distance/time = circumference/time =
939,951,145 km / (365.2421896698 days
* 24 hr/day) = 107,229 km/hr (66,629
mi/hr)
3. The Earth Revolves Around the Sun Once a Year
● The Sun's mass is 1.9891 * 1030 kg it is 332,950 times
heavier than the Earth. The Earth does cause the Sun to
wobble but it is a very tiny motion.
● On the other hand, Jupiter (the heaviest planet in the
solar system) causes a much more appreciable wobble in
the Sun.
● Sun wobbles around a point just outside its surface every
11.859 years (the length of Jupiter's orbit).
● Although slow, this wobble is detectable - and it also
means the Earth is orbiting a slowly wobbling Sun
4. The Sun and Earth Revolve Around the Solar
System "Gravitational Centre"
● The Earth's North-South rotation
axis "wobbles" like the slow
rotational tilting of a spinning top
over a period of 25,770 years. This
is known as Precession and affects
the direction in the sky to which
the North Pole points and, in fact,
the orientation of the entire orbital
path of the Earth.
5. The Earth's Orbit Precesses every 25,770 years
● Precession is caused by
the gravitational
attraction of the Sun
(and the Moon) tugging
on the Earth's equatorial
bulge.
● The Sun is located near the Orion
arm, between two major arms
(Perseus and Sagittarius). The
diameter of the Milky Way is about
100,000 light-years and the Sun
is located about 28,000 light-
years from the Galactic Center.
● It takes the sun approximately
255-250 years to complete one
journey.
6. The Sun Revolves Around the Galaxy Once Every
250 Million Years
● The Milky Way Galaxy and the Andromeda
Galaxy are approaching each other at
about 400 km/s
7. The Galaxy is moving through the Universe
● The Earth wobbles causing the location of the
North and South Poles to vary by 3 to 15 m.
● This Chandler Wobble causes the latitude of any
position on the Earth to move a few metres in this
14 month cycle and affects GPS readings
8.Polar Variation - small but needs to be mentioned
DIFFERENT FORMS LAND AREA OF
THE EATH
● Mountains are landforms
higher than the surrounding
areas. They are formed due
to the tectonic movements,
earthquakes, volcanic
eruptions and erosion of the
surrounding areas caused
due to wind, water and ice.
Mountains are found in the
oceans and on land.
Mountains
● Plateaus are flat highlands
that are separated from the
surroundings due to steep
slopes. They are formed by
collisions of tectonic
plates, magma action that
causes the elevation in
earth’s crust.
Plateaus
● Valleys are low-lying areas of land
between hills and mountains that
are formed due to the actions of
glaciers and rivers over millions of
years. Depending on the shape
they are classified as V shaped
valleys and U shaped valleys. V-
shaped valleys are formed by the
flowing rivers and U-shaped valleys
are formed due to glaciers.
Valleys
● Due to lack of adequate rainfall,
desert is a dry piece of land with
little or no vegetation. They are
mostly found mainly in rain
shadow areas which are leeward of
a mountain range with respect to
the wind direction. In deserts, the
atmospheric air is very dry, and
daytime temperature is high.
Deserts
● Dunes are mounds or small hills
made up of sand that are created
due to the action of and water flow
(under water dunes). It may be
dome-shaped, crescent-shaped,
star-shaped, linear-shaped, and
many more. The height of a dune
hill can be as low as 1 meter, or as
high as 10 meter and more.
Dunes
● An island is a piece of
land which is
surrounded by water
from all sides and
formed either due to
volcanic eruptions or
due to hot spots in the
lithosphere.
Islands
● Plains are flat or the low relief
areas on the surface of the
earth. It might be formed as a
result of the sedimentation of
eroded soil from the top of the
hills and mountains or might be
due to flowing lava deposited by
the agents of wind, water, and
ice.
Plains
● Rivers are natural
flowing streams of fresh
water descending from
mountains. They
mostly flow toward a
lake, sea, ocean or
another river.
Rivers
● Oceans are the biggest water
bodies found on earth and are
saline in nature. Oceans cover
over 71% of the earth’s surface
and are responsible in
controlling the weather and
climate of the earth. Oceans
originated due to continental
drifts i.e. the movement of the
earth’s tectonic plates.
Oceans
● Loess are deposition of
silt, with a little amount
of sand and clay. They
appear yellowish or
brownish in color. Wind
action or glacial
activities are responsible
for formation of loess.
Loess
● Glaciers are slow moving huge
bodies of ice formed due to
the compression of the snow
layers. They move depending
on the pressure and gravity.
There are two types of
glaciers, the alpine glaciers
which can be located in high
mountains and the
continental glaciers which can
be located in cold Polar
regions.
Glaciers
● Peninsulas are large land
areas that extend into
water bodies. They remain
surrounded by water on
three sides. Peninsulas are
formed by lithospheric
movements and action of
water currents.
Peninsulas
● Deltas are low-lying,
triangle-shaped areas,
located at the mouth of
rivers. In the course of
creating a delta, the sand,
silt, and rock particles are
accumulated in a nearly
triangular shape.
Deltas
‘Mississippi river delta’
THE MODERN ATOMIC THEORY
R EF ER ENC Es:
 http: / / earthsci.org/ space/ space/ earth8/ earth8
.html
 https: / / schooltutoring.com/ help/ earth
sciences types of landforms/
F
O

More Related Content

Similar to Group-3-Science-Motions-of-Earth-SUPER-FINAL.pptx

Similar to Group-3-Science-Motions-of-Earth-SUPER-FINAL.pptx (20)

Geogpraphy capsule
Geogpraphy capsuleGeogpraphy capsule
Geogpraphy capsule
 
Geogpraphy capsule
Geogpraphy capsuleGeogpraphy capsule
Geogpraphy capsule
 
Climatology - Introduction.pptx
Climatology - Introduction.pptxClimatology - Introduction.pptx
Climatology - Introduction.pptx
 
22 earth in space
22 earth in space22 earth in space
22 earth in space
 
1 hrly gs ch 02 earth movement
1 hrly gs ch 02 earth movement1 hrly gs ch 02 earth movement
1 hrly gs ch 02 earth movement
 
Seasons of the phils
Seasons of the philsSeasons of the phils
Seasons of the phils
 
Sun, Moon, and Earth system
Sun, Moon, and Earth systemSun, Moon, and Earth system
Sun, Moon, and Earth system
 
Revolution and rotation
Revolution and rotationRevolution and rotation
Revolution and rotation
 
Satuito. Earth's Motion2
Satuito. Earth's Motion2Satuito. Earth's Motion2
Satuito. Earth's Motion2
 
THE EARTH-SOL_EQUINOX.pdf
THE EARTH-SOL_EQUINOX.pdfTHE EARTH-SOL_EQUINOX.pdf
THE EARTH-SOL_EQUINOX.pdf
 
6 -earth_s_motions
6  -earth_s_motions6  -earth_s_motions
6 -earth_s_motions
 
218087672 mokgopa.sun&earth presentation
218087672 mokgopa.sun&earth presentation218087672 mokgopa.sun&earth presentation
218087672 mokgopa.sun&earth presentation
 
1st term answer key
1st term answer key1st term answer key
1st term answer key
 
Earth movements.pdf
Earth movements.pdfEarth movements.pdf
Earth movements.pdf
 
World Geography.pdf
World Geography.pdfWorld Geography.pdf
World Geography.pdf
 
The Earth, Rotation and Revolution
The Earth, Rotation and RevolutionThe Earth, Rotation and Revolution
The Earth, Rotation and Revolution
 
sunearthmoonsystem PPT notes.ppt
sunearthmoonsystem PPT notes.pptsunearthmoonsystem PPT notes.ppt
sunearthmoonsystem PPT notes.ppt
 
QUICK GEOGRAPHY (1).pdf
QUICK GEOGRAPHY (1).pdfQUICK GEOGRAPHY (1).pdf
QUICK GEOGRAPHY (1).pdf
 
Jupiter
JupiterJupiter
Jupiter
 
Generalknowledge
GeneralknowledgeGeneralknowledge
Generalknowledge
 

Recently uploaded

BASLIQ CURRENT LOOKBOOK LOOKBOOK(1) (1).pdf
BASLIQ CURRENT LOOKBOOK  LOOKBOOK(1) (1).pdfBASLIQ CURRENT LOOKBOOK  LOOKBOOK(1) (1).pdf
BASLIQ CURRENT LOOKBOOK LOOKBOOK(1) (1).pdfSoniaTolstoy
 
Grant Readiness 101 TechSoup and Remy Consulting
Grant Readiness 101 TechSoup and Remy ConsultingGrant Readiness 101 TechSoup and Remy Consulting
Grant Readiness 101 TechSoup and Remy ConsultingTechSoup
 
Organic Name Reactions for the students and aspirants of Chemistry12th.pptx
Organic Name Reactions  for the students and aspirants of Chemistry12th.pptxOrganic Name Reactions  for the students and aspirants of Chemistry12th.pptx
Organic Name Reactions for the students and aspirants of Chemistry12th.pptxVS Mahajan Coaching Centre
 
Alper Gobel In Media Res Media Component
Alper Gobel In Media Res Media ComponentAlper Gobel In Media Res Media Component
Alper Gobel In Media Res Media ComponentInMediaRes1
 
Kisan Call Centre - To harness potential of ICT in Agriculture by answer farm...
Kisan Call Centre - To harness potential of ICT in Agriculture by answer farm...Kisan Call Centre - To harness potential of ICT in Agriculture by answer farm...
Kisan Call Centre - To harness potential of ICT in Agriculture by answer farm...Krashi Coaching
 
The basics of sentences session 2pptx copy.pptx
The basics of sentences session 2pptx copy.pptxThe basics of sentences session 2pptx copy.pptx
The basics of sentences session 2pptx copy.pptxheathfieldcps1
 
mini mental status format.docx
mini    mental       status     format.docxmini    mental       status     format.docx
mini mental status format.docxPoojaSen20
 
Science 7 - LAND and SEA BREEZE and its Characteristics
Science 7 - LAND and SEA BREEZE and its CharacteristicsScience 7 - LAND and SEA BREEZE and its Characteristics
Science 7 - LAND and SEA BREEZE and its CharacteristicsKarinaGenton
 
CARE OF CHILD IN INCUBATOR..........pptx
CARE OF CHILD IN INCUBATOR..........pptxCARE OF CHILD IN INCUBATOR..........pptx
CARE OF CHILD IN INCUBATOR..........pptxGaneshChakor2
 
Industrial Policy - 1948, 1956, 1973, 1977, 1980, 1991
Industrial Policy - 1948, 1956, 1973, 1977, 1980, 1991Industrial Policy - 1948, 1956, 1973, 1977, 1980, 1991
Industrial Policy - 1948, 1956, 1973, 1977, 1980, 1991RKavithamani
 
“Oh GOSH! Reflecting on Hackteria's Collaborative Practices in a Global Do-It...
“Oh GOSH! Reflecting on Hackteria's Collaborative Practices in a Global Do-It...“Oh GOSH! Reflecting on Hackteria's Collaborative Practices in a Global Do-It...
“Oh GOSH! Reflecting on Hackteria's Collaborative Practices in a Global Do-It...Marc Dusseiller Dusjagr
 
Sanyam Choudhary Chemistry practical.pdf
Sanyam Choudhary Chemistry practical.pdfSanyam Choudhary Chemistry practical.pdf
Sanyam Choudhary Chemistry practical.pdfsanyamsingh5019
 
_Math 4-Q4 Week 5.pptx Steps in Collecting Data
_Math 4-Q4 Week 5.pptx Steps in Collecting Data_Math 4-Q4 Week 5.pptx Steps in Collecting Data
_Math 4-Q4 Week 5.pptx Steps in Collecting DataJhengPantaleon
 
Presiding Officer Training module 2024 lok sabha elections
Presiding Officer Training module 2024 lok sabha electionsPresiding Officer Training module 2024 lok sabha elections
Presiding Officer Training module 2024 lok sabha electionsanshu789521
 
Software Engineering Methodologies (overview)
Software Engineering Methodologies (overview)Software Engineering Methodologies (overview)
Software Engineering Methodologies (overview)eniolaolutunde
 
Q4-W6-Restating Informational Text Grade 3
Q4-W6-Restating Informational Text Grade 3Q4-W6-Restating Informational Text Grade 3
Q4-W6-Restating Informational Text Grade 3JemimahLaneBuaron
 
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...EduSkills OECD
 
How to Make a Pirate ship Primary Education.pptx
How to Make a Pirate ship Primary Education.pptxHow to Make a Pirate ship Primary Education.pptx
How to Make a Pirate ship Primary Education.pptxmanuelaromero2013
 

Recently uploaded (20)

BASLIQ CURRENT LOOKBOOK LOOKBOOK(1) (1).pdf
BASLIQ CURRENT LOOKBOOK  LOOKBOOK(1) (1).pdfBASLIQ CURRENT LOOKBOOK  LOOKBOOK(1) (1).pdf
BASLIQ CURRENT LOOKBOOK LOOKBOOK(1) (1).pdf
 
TataKelola dan KamSiber Kecerdasan Buatan v022.pdf
TataKelola dan KamSiber Kecerdasan Buatan v022.pdfTataKelola dan KamSiber Kecerdasan Buatan v022.pdf
TataKelola dan KamSiber Kecerdasan Buatan v022.pdf
 
Grant Readiness 101 TechSoup and Remy Consulting
Grant Readiness 101 TechSoup and Remy ConsultingGrant Readiness 101 TechSoup and Remy Consulting
Grant Readiness 101 TechSoup and Remy Consulting
 
Organic Name Reactions for the students and aspirants of Chemistry12th.pptx
Organic Name Reactions  for the students and aspirants of Chemistry12th.pptxOrganic Name Reactions  for the students and aspirants of Chemistry12th.pptx
Organic Name Reactions for the students and aspirants of Chemistry12th.pptx
 
Alper Gobel In Media Res Media Component
Alper Gobel In Media Res Media ComponentAlper Gobel In Media Res Media Component
Alper Gobel In Media Res Media Component
 
Kisan Call Centre - To harness potential of ICT in Agriculture by answer farm...
Kisan Call Centre - To harness potential of ICT in Agriculture by answer farm...Kisan Call Centre - To harness potential of ICT in Agriculture by answer farm...
Kisan Call Centre - To harness potential of ICT in Agriculture by answer farm...
 
The basics of sentences session 2pptx copy.pptx
The basics of sentences session 2pptx copy.pptxThe basics of sentences session 2pptx copy.pptx
The basics of sentences session 2pptx copy.pptx
 
mini mental status format.docx
mini    mental       status     format.docxmini    mental       status     format.docx
mini mental status format.docx
 
Science 7 - LAND and SEA BREEZE and its Characteristics
Science 7 - LAND and SEA BREEZE and its CharacteristicsScience 7 - LAND and SEA BREEZE and its Characteristics
Science 7 - LAND and SEA BREEZE and its Characteristics
 
CARE OF CHILD IN INCUBATOR..........pptx
CARE OF CHILD IN INCUBATOR..........pptxCARE OF CHILD IN INCUBATOR..........pptx
CARE OF CHILD IN INCUBATOR..........pptx
 
Código Creativo y Arte de Software | Unidad 1
Código Creativo y Arte de Software | Unidad 1Código Creativo y Arte de Software | Unidad 1
Código Creativo y Arte de Software | Unidad 1
 
Industrial Policy - 1948, 1956, 1973, 1977, 1980, 1991
Industrial Policy - 1948, 1956, 1973, 1977, 1980, 1991Industrial Policy - 1948, 1956, 1973, 1977, 1980, 1991
Industrial Policy - 1948, 1956, 1973, 1977, 1980, 1991
 
“Oh GOSH! Reflecting on Hackteria's Collaborative Practices in a Global Do-It...
“Oh GOSH! Reflecting on Hackteria's Collaborative Practices in a Global Do-It...“Oh GOSH! Reflecting on Hackteria's Collaborative Practices in a Global Do-It...
“Oh GOSH! Reflecting on Hackteria's Collaborative Practices in a Global Do-It...
 
Sanyam Choudhary Chemistry practical.pdf
Sanyam Choudhary Chemistry practical.pdfSanyam Choudhary Chemistry practical.pdf
Sanyam Choudhary Chemistry practical.pdf
 
_Math 4-Q4 Week 5.pptx Steps in Collecting Data
_Math 4-Q4 Week 5.pptx Steps in Collecting Data_Math 4-Q4 Week 5.pptx Steps in Collecting Data
_Math 4-Q4 Week 5.pptx Steps in Collecting Data
 
Presiding Officer Training module 2024 lok sabha elections
Presiding Officer Training module 2024 lok sabha electionsPresiding Officer Training module 2024 lok sabha elections
Presiding Officer Training module 2024 lok sabha elections
 
Software Engineering Methodologies (overview)
Software Engineering Methodologies (overview)Software Engineering Methodologies (overview)
Software Engineering Methodologies (overview)
 
Q4-W6-Restating Informational Text Grade 3
Q4-W6-Restating Informational Text Grade 3Q4-W6-Restating Informational Text Grade 3
Q4-W6-Restating Informational Text Grade 3
 
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...
 
How to Make a Pirate ship Primary Education.pptx
How to Make a Pirate ship Primary Education.pptxHow to Make a Pirate ship Primary Education.pptx
How to Make a Pirate ship Primary Education.pptx
 

Group-3-Science-Motions-of-Earth-SUPER-FINAL.pptx

  • 1. EIGHT MOTIONS OF EARTH MEMB ER S: MARY JOY BERNABE NELMARIE RIVERA NICOLE ANDRIEL PRAGOSO NOVA UGBINADA PAMELA RICO RHODARINE BANTAD ROSALIEALITAO
  • 2. OBJECTIVE: • Differentiating the types of varations and emotions of the effects. • Explaining different land forms area of the Earth
  • 3. 1. The Earth Rotates About Its Axis  Earth moves through space in several important ways. One type of motion is called rotation. A rotation is a spin around a center.  Earth also spins around a central line called an axis. Earth’s axis is an imaginary vertical line that runs through the planet from the North Pole to the South Pole. • The Earth has a circumference (measured around at the Equator) of approximately 40,075 km (24,901 mi). And 40,007.863 km (24,859.734 mi) when measured around the poles. • The Earth rotates on its axis relative to the Sun in one “Mean Solar Day" • It rotates exactly 360° in one "Mean Sidereal Day" which is 86,164.0909 seconds, or 23 hrs 56 min 4.0909 seconds.
  • 4. Solar day (24 hours) The Earth makes one rotation compared with the Sun. 3 minutes 56 seconds longer than a sidereal day. Sidereal day (23 hours 56 minutes 4.0909 seconds) The Earth makes one rotation compared with the distant stars. 3 minutes 56 seconds shorter than a solar day
  • 5. 2. Earth-Moon System Orbits a "Gravitational Centre" ● Both the Moon and the Earth orbit a common centre of gravity ● The mass of the Earth (ME) is 5.9742 * 1024 kg, and the mass of the Moon is 7.349 * 1022 kg - the Ratio of the masses is 81.3 ● So the centre of gravity is therefore located 1 unit from the Earth's centre and 81.3 units from the Moon's centre ● Earth pivots around this point once every Lunar Month
  • 6. ● The Earth's orbit around the Sun is an ellipse and travels at different speeds during the year - slowest at Aphelion (furthest point from the Sun) and fastest at Perihelion (closest point to the Sun) ● Earth's orbit (the path) is approximately 940,000,000 km (580,000,000 mi) in 365.2421896698 days ● So the "year" is not exactly 365¼ days (sometimes called the Julian Year). ● Earth's speed around the sun Speed = distance/time = circumference/time = 939,951,145 km / (365.2421896698 days * 24 hr/day) = 107,229 km/hr (66,629 mi/hr) 3. The Earth Revolves Around the Sun Once a Year
  • 7. ● The Sun's mass is 1.9891 * 1030 kg it is 332,950 times heavier than the Earth. The Earth does cause the Sun to wobble but it is a very tiny motion. ● On the other hand, Jupiter (the heaviest planet in the solar system) causes a much more appreciable wobble in the Sun. ● Sun wobbles around a point just outside its surface every 11.859 years (the length of Jupiter's orbit). ● Although slow, this wobble is detectable - and it also means the Earth is orbiting a slowly wobbling Sun 4. The Sun and Earth Revolve Around the Solar System "Gravitational Centre"
  • 8. ● The Earth's North-South rotation axis "wobbles" like the slow rotational tilting of a spinning top over a period of 25,770 years. This is known as Precession and affects the direction in the sky to which the North Pole points and, in fact, the orientation of the entire orbital path of the Earth. 5. The Earth's Orbit Precesses every 25,770 years
  • 9. ● Precession is caused by the gravitational attraction of the Sun (and the Moon) tugging on the Earth's equatorial bulge.
  • 10. ● The Sun is located near the Orion arm, between two major arms (Perseus and Sagittarius). The diameter of the Milky Way is about 100,000 light-years and the Sun is located about 28,000 light- years from the Galactic Center. ● It takes the sun approximately 255-250 years to complete one journey. 6. The Sun Revolves Around the Galaxy Once Every 250 Million Years
  • 11. ● The Milky Way Galaxy and the Andromeda Galaxy are approaching each other at about 400 km/s 7. The Galaxy is moving through the Universe
  • 12. ● The Earth wobbles causing the location of the North and South Poles to vary by 3 to 15 m. ● This Chandler Wobble causes the latitude of any position on the Earth to move a few metres in this 14 month cycle and affects GPS readings 8.Polar Variation - small but needs to be mentioned
  • 13. DIFFERENT FORMS LAND AREA OF THE EATH
  • 14. ● Mountains are landforms higher than the surrounding areas. They are formed due to the tectonic movements, earthquakes, volcanic eruptions and erosion of the surrounding areas caused due to wind, water and ice. Mountains are found in the oceans and on land. Mountains
  • 15. ● Plateaus are flat highlands that are separated from the surroundings due to steep slopes. They are formed by collisions of tectonic plates, magma action that causes the elevation in earth’s crust. Plateaus
  • 16. ● Valleys are low-lying areas of land between hills and mountains that are formed due to the actions of glaciers and rivers over millions of years. Depending on the shape they are classified as V shaped valleys and U shaped valleys. V- shaped valleys are formed by the flowing rivers and U-shaped valleys are formed due to glaciers. Valleys
  • 17. ● Due to lack of adequate rainfall, desert is a dry piece of land with little or no vegetation. They are mostly found mainly in rain shadow areas which are leeward of a mountain range with respect to the wind direction. In deserts, the atmospheric air is very dry, and daytime temperature is high. Deserts
  • 18. ● Dunes are mounds or small hills made up of sand that are created due to the action of and water flow (under water dunes). It may be dome-shaped, crescent-shaped, star-shaped, linear-shaped, and many more. The height of a dune hill can be as low as 1 meter, or as high as 10 meter and more. Dunes
  • 19. ● An island is a piece of land which is surrounded by water from all sides and formed either due to volcanic eruptions or due to hot spots in the lithosphere. Islands
  • 20. ● Plains are flat or the low relief areas on the surface of the earth. It might be formed as a result of the sedimentation of eroded soil from the top of the hills and mountains or might be due to flowing lava deposited by the agents of wind, water, and ice. Plains
  • 21. ● Rivers are natural flowing streams of fresh water descending from mountains. They mostly flow toward a lake, sea, ocean or another river. Rivers
  • 22. ● Oceans are the biggest water bodies found on earth and are saline in nature. Oceans cover over 71% of the earth’s surface and are responsible in controlling the weather and climate of the earth. Oceans originated due to continental drifts i.e. the movement of the earth’s tectonic plates. Oceans
  • 23. ● Loess are deposition of silt, with a little amount of sand and clay. They appear yellowish or brownish in color. Wind action or glacial activities are responsible for formation of loess. Loess
  • 24. ● Glaciers are slow moving huge bodies of ice formed due to the compression of the snow layers. They move depending on the pressure and gravity. There are two types of glaciers, the alpine glaciers which can be located in high mountains and the continental glaciers which can be located in cold Polar regions. Glaciers
  • 25. ● Peninsulas are large land areas that extend into water bodies. They remain surrounded by water on three sides. Peninsulas are formed by lithospheric movements and action of water currents. Peninsulas
  • 26. ● Deltas are low-lying, triangle-shaped areas, located at the mouth of rivers. In the course of creating a delta, the sand, silt, and rock particles are accumulated in a nearly triangular shape. Deltas ‘Mississippi river delta’
  • 27. THE MODERN ATOMIC THEORY R EF ER ENC Es:  http: / / earthsci.org/ space/ space/ earth8/ earth8 .html  https: / / schooltutoring.com/ help/ earth sciences types of landforms/ F O