Geography Notes
Form 1 Geography Notes
Form 2 Geography Notes
Form 3 Geography Notes
Form 4 Geography Notes
FORM I GEOGRAPHY
INTRODUCTION TO GEOGRAPHY
The meaning of Geography
- Scientific study of the earth as a home of man.
- Study of interrelationship on natural and human phenomena on the earth’s surface.
Environment
- The surroundings
- All external conditions surrounding an organism which has influence over its behaviour.
Environment can be divided into two:
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- The Physical Environment
- Natural physical conditions of weather, climate, vegetation, animals, soil, landforms and drainage.
- The Human Environment
- Human activities such as farming, forestry, mining, tourism, settlement, transportation, trade and industry.
Branches of Geography
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- Physical Geography
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- Deals with the study of natural physical environment of human kind.
The areas covered include:
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- Geology-study of the origin, structure and composition of the earth. It includes study of rocks.
- Geomorphology- the study of internal and external land forming processes and landforms.
- Climatology- the study of climate and weather
- Pedology- the study of soils
- Biogeography – the study of soils, vegetation and animals.
- Hydrology- the study of water bodies
- Spatial geography-study of space
2. Human and Economic Geography
-Study of people and their activities on the earth’s surface.
The areas covered include:
- Mining
- Forestry
- Agriculture
- Fishing
- Wildlife and tourism
- Industry
- Energy etc.
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- Practical Geography
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-A smaller branch which equips the learner with practical skills that enhance their understanding and interpretation of human and physical geographical information.
The areas are:
- Statistical methods
- Map work
- Field work
- Photograph work
Importance of Studying Geography
- Facilitates good relationship among nations by studying geography of other regions of the world.
- It’s a career subject in that it enables one to go for advanced studies in specialised fields e.g. geography teachers, meteorology, surveying etc.
- Enables us to appreciate other people’s way of life by learning economic activities of different communities within our country and other parts of the world.
- Enables us to conserve our environment when we learn negative and positive effects of human activities on the environment.
- Enables us to conserve our resources when we learn wise use of resources in conservation and management of resources e.g. wildlife, forests, energy, etc.
- Inculcates in us virtues of cooperation and patience as we work in groups.
- Makes us to appreciate manual work as we are involved in practical geography which may lead to self employment.
- Promotion of industry such as tourism by guiding tourists to places of interest by using maps, calculations of distances etc.
Relationship between Geography and Other Subjects
- Mathematics-mathematical techniques are used in drawing graphs and pie charts and mathematical formulae are used in geography to calculate distances, areas, population density, population densities, etc.
- History-history uses geographical tools like maps, charts and graphs to show where past events took place e.g. the movement of people in the past.
- Biology-Geography explains the distribution of organisms and factors influencing their distribution on the earth’s surface.
- Physics-geography uses physics principles and formulae to calculate and describe aspects such as magnetic field, gravity, vibrations of the earth etc.
- Chemistry-geography applies chemistry in studying chemical composition and chemical changes which take place in soils and rocks.
- Agriculture-geography studies farming systems, their distribution and factors affecting farming activities.
- Meteorology-geography uses meteorological information in the study of weather and in classifying climatic regions and mapping them.
- Geology-geography studies rocks.
The Earth and the Solar System
Solar system is the group of heavenly bodies comprising the sun and the nine planets.
The origin of the Solar System
Theories
A theory is a set of reasoned ideas intended to explain facts or events
- Passing Star Theory
- A star with a greater gravitational pull passed near the sun
- It attracted large quantities of gaseous materials from the sun
- The materials split, cooled and condensed to form planets
- The planets were set in orbit by the passing star
Weaknesses
- Doesn’t explain the origin of the sun and star.
- Minimal chance of a star approaching another
- Materials would disperse than condense
- Collision Theory
- Star with greater gravitational pull passed near the sun
- It attracted large quantities of gaseous materials
- The materials split into portions
- Large portions collided with smaller ones and swept them to form planets.
The weaknesses are the same as the passing star’s Theory.
- Nebula Clod Theory
- There was a slowly rotating cloud of dust and gas called Nebula
- It cooled and began to contact
- Rotation speed increased and successive rings of gaseous materials were formed.
- The rings condensed to form planets
- The central gaseous material remained as the sun
Evidence
- Rotation and revolution of planets in anticlockwise direction
Weakness
The origin of nebular is not explained.
- Supernova/explosion Theory
- There was a violent explosion of a star.
- A cloud of dust (nebular) remained from the star.
- There was fast movement of the cloud due to the force of explosion.
- Rotation speed increased due to gravitational attraction
- The cloud flattened into a disc.
- The matter began to accumulate towards the centre to form a proto-sun which later began to shine.
- The rest of the cloud collapsed to form planets.
Weaknesses
- Doesn’t explain the origin of the star
- Doesn’t explain the cause of explosion
Composition of the Solar System
1. The Sun
It’s the centre of the universe.
Characteristics
- It’s a star.
A star is a heavenly possessing its own light which it transmits.
Nebula/galaxy is a cluster of stars.
The earth is in a galaxy called The Milky Way.
- It’s made of very hot gases mainly hydrogen (70%) and helium (30%).
- Has a diameter of 1392000km.
- Surrounded by a layer of gas which has boiled from its surface which is called corona.
- Rotates on its own axis in anticlockwise direction.
- Has gravitational pull which holds all the planets in orbit around it.
An orbit is a path which a planet or a satellite follows around a star or a planet.
- Temperature at its centre is 15m◦c and at the surface is 5500◦c.
- Radiates solar energy which is very important for all forms of life on the earth.
2. The Planets
Planets are large spherical celestial/heavenly bodies in space.
There are 9 planets in our solar system.
Characteristics
- Spherical in shape
- Don’t have their own light but reflect it from the sun.
- Revolve around the sun in anticlockwise direction.
- Have their own force of gravity
- Only one is known to support life.
The following are the planets arranged in order from the one nearest to the sun.
Mercury
- Nearest from the sun
- Its 58m km from the sun
- Has no satellites
- Takes approximately 88 earth days to revolve around the sun
Venus
- 2nd planet from the sun
- It’s 108m km from the sun
- One of the brightest planets
- Can be seen clearly with naked eyes
- Takes approximately 225 earth days to revolve around the sun
- Slightly smaller than the earth
- Has no satellites
- Together with the earth they are called twin planets due to having many similarities
Earth
- The 3rd planet from the sun
- The earth and the heavenly bodies make the universe
- The only planet that supports life
- The home of man
- Approximately 149m km from the sun
- Takes 365 ¼ days to revolve around the sun
- Has one satellite, the moon
Mars
- Also called The Red Planet because when it’s observed through a telescope it appears reddish.
- The 4th from the sun
- Slightly smaller than the earth
- Approximately 228m km from the sun
- Takes 687 earth days to revolve around the sun
- Between Mass and Jupiter there are small celestial bodies called planetoids.
- Has no satellite.
Jupiter
- 5th planet from the sun
- Approximately 778m km from the sun
- Largest in the universe
- Rotates on its own axis at very fast speed
- Has flattened poles due to its fast speed of rotation
- Has very thick layers of ice on its surface
- takes 12 earth years to revolve around the sun
- Has 16 satellites
Saturn
- 6th planet from the sun
- Second largest planet
- Approximately 1427m km from the sun
- Takes 29 ½ earth years to revolve around the sun
- Has a ring around it
- Has 18 satellites
Uranus
- 7th planet from the sun
- About 4 times bigger than the earth
- Approximately 2870m km from the sun
- Also rotates very fast
- Also has flattened poles due to fast speed of rotation
- It appears greenish foe being surrounded by methane gas
- Has 8 satellites
- Takes 84 earth years to revolve around the sun
Neptune
- One of the farthest from the sun
- 8th planet from the sun
- Approximately 4497m km from the sun
- Has 8 satellites
- Takes 165 earth years to revolve around the sun
- Very similar in size, colour and character with Uranus
Pluto
- 9th planet from the earth
- Farthest from the sun
- The smallest
- 1/6 the size of the earth
- Approximately 5900m km from the sun
- Takes 248 earth years to revolve around the sun
- Has one satellite
- Very little is known about it
Other Celestial Bodies
Natural Satellites
- Any natural heavenly body that orbits around a planet e.g. moon for earth, tritan for Saturn and Triton for Neptune.
Asteroids/Planetoids
- Also called minor planets.
- Are small fragments of rocks left going around the sun when the solar system was formed
- Found between Mass and Jupiter
- Are 1500 in number
- They sometimes collide with each other and planets due to Jupiter’s gravitational pull causing them to move in erratic orbits.
Comets
- Heavenly bodies which appear to have a head and a long tail
- Made of ice, dust and frozen gas
- The head is made of many particles of dust, rock and frozen gases.
- Their tail is made of gases and points away from the sun.
- Move around the sun in extremely long and oval orbits
- Their orbits cross the earth’s orbits e.g. Halley’s Comet which appears after every 76 years.
Meteoroid
- Small heavenly body which strays from its orbit in the solar system and enters the earth’s atmosphere at very high speed.
Meteor
- A meteoroid which is burning out due to friction after entering the earth’s atmosphere.
Meteorite
- Remains of a meteoroid which have reached the earth’s surface or incompletely burnt up meteoroid.
- When they fall they sink into the ground forming craters
- They are rich in iron
The Moon
- A natural satellite
- Receives its light from the sun and reflects it onto the earth.
- It revolves around the earth
- Takes 29.5 days to complete one revolution around the earth
- Its orbit is almost circular
- As it revolves around the sun it appears in various shapes ranging from crescent/new moon, half moon, gibbons moon and full moon.
- Has gravitational pull which causes the rising and falling of the ocean level
- As the moon orbits around the earth it creates an event called eclipse.
Eclipse
-Phenomenon occurring when the rays of the sun are blocked from reaching the earth or the moon.
Solar/Sun Eclipse
- The moon comes between the earth and the sun
- The moon’s shadow is cast on the earth
- The sun appears to be covered by darkness
Lunar/moon Eclipse
- The earth comes between the moon and the sun
- The earth’s shadow is cast on the moon
- The moon appears to be covered by darkness
The Origin of the earth
- A star with a greater gravitational pull passed near the sun
- It attracted large quantities of gaseous materials from the sun
- The materials split, cooled and condensed
- Heavier materials collected at the centre to form the core
- Less dense materials collected around the core to form the mantle
- The lightest materials formed the crust
The shape of the earth
The shape of the earth is called geoid/ovoid/oblate spheroid due to being an imperfect sphere by being wide at the equator and flat at the poles.
Proofs/Evidence That the Earth Is Spherical
- If one moves towards the east in a straight line he will end up where he started.
- Satellite photographs taken from space show that the earth is like a sphere.
- Places in the east see the sun earlier than those in the west.
- When a ship is approaching the smoke is seen first, then the mast and finally the whole ship.
- All the planets are spherical so the earth being one of them is also spherical.
- During the moon eclipse the earth casts a spherical shadow on the moon.
- The earth’s horizon appears curved when observed from a very high point like a tower.
The size of the earth
- Equatorial diameter-12756km
- Equatorial circumference-40085km
- Polar diameter-39995km
- Surface area of the earth-510×106 km2
- Water surface-73%.
The Movement of the Earth
There are 2 movements of the earth namely:
- Rotation of the earth on its axis
- Revolution of the earth around the sun
Rotation of the Earth
-Movement of the earth on its own axis (imaginary line through the centre from N pole to S pole.
- Rotates through 360◦.
- Takes 24 hours (day) to complete 1 rotation.
- Rotates in an anticlockwise direction (west to east).
Effects of Rotation of the Earth
- Creates day and night because at any one time one side of the earth faces the sun (day) and the other remains in darkness (night).
- Causes deflection of winds and ocean currents in the N hemisphere to the left and in the S hemisphere to the right.
- It causes rising and falling of ocean tides.
- Causes time difference between longitudes.
- Takes one hour to go through 15◦.
- 4 min to go through 1◦.
Calculation of Local Time
-The time recorded in places within the same longitude.
A longitude is an imaginary line running from N to S which shows how far E or W a place is from the prime meridian.
Greenwich Meridian (0◦) longitude is the point of reference when calculating time.
Time is gained towards the E and lost towards the W.
Examples
- Suppose the time at GWM is 12 noon what is the local time at Watamu 40◦E?
Time gained=40×4=160min=2 hours 40min
Local time at Watamu is 12.00+2.40=14.40-1200=2.40pm.
- At Dar-es-Salaam 40◦E time is 12pm what is the time at Ecuador 40◦E?
40◦+20◦=60◦
60×4=240min=4hours
Ecuador is behind in time =12.00-4=8 am.
If the places are on the same side subtract the degrees to get the difference and add or subtract from the reference time depending on which side the place is.
Calculation of Longitude
What is the longitude of place x whose local time is 8 am when local time at GWM is noon?
Time difference =12.00-8=4 hours
Degrees=4×15=60◦
Since x is behind in time its then 60◦W.
Standard Time and Zones
- Standard time is time recorded by countries within the same time zone.
- Standard time was come up with due to confusion resulting from time changing at every longitude.
- The world has 24 time zones.
The International Date Line
It’s the 180◦ longitude.
Effects of Crossing It
- One gains time when he crosses it from W to E and has to adjust the clock ahead by 24 hours.
- One loses time when he crosses it from E to W and has to adjust the clock backwards by 24 hours.
Revolution of the Earth
- Movement of the earth in its orbit around the sun.
- It’s in anticlockwise direction.
- The orbit of the earth’s revolution is elliptical.
- Takes 365 ¼ days in a year or 366 days in a leap year (every 4 years).
- The sun moves from the tropic of cancer to the equator and then towards tropic of Capricorn and back to the tropic of cancer.
- 21st march and 23rd September are called equinoxes because the length of day and night is equal. The sun is vertically overhead at noon at the equator.
- 21st June is called summer solstice because its summer in the N hemisphere. The sun is vertically overhead at noon at the tropic of cancer.
- 22nd December is called winter solstice because its winter in the S. hemisphere. The sun is vertically overhead at noon at noon at the tropic of Capricorn.
- Solstice is the period of maximum tilting of the earth towards the sun.
Effects of the Revolution of the earth
- Causes the four seasons summer, autumn, winter and spring due to the movement of overhead sun causing changes in the heat belt.
- Causes variation of day and night’s lengths due to the earth’s axis being inclined to the path of revolution at an angle of 60◦.
- Equinoxes have equal lengths of day and night.
- Summers have longer days and shorter nights.
- Winters have longer nights and shorter days.
- Causes changes in the altitude of the midday sun due to the earth’s orbit being elliptical.
- Highest altitude during equinox
- Lowest altitude during solstices
- Causes lunar eclipse due to revolution bringing the earth in line with the sun and the moon.
The Structure of the Earth
Internal Structure of the Earth
The evidence used to study the earth’s interior are
- mining
- drilling
- quarrying/excavation
A. Crust/Lithosphere
- Outermost layer of the earth
- Made of soils and other loose deposits of sand
- The dominant rocks are granites.
- Extends 0-50km
- Has 2 layers
1. Sial
- Also called continental crust
- Made of light coloured rocks
- Called sial because it’s made up of silica and aluminium.
2. Sima
- Also called oceanic crust
- Mainly made of basaltic rocks which are brittle.
- Called sima because it is made of silica magnesium and iron.
Mohorovicic Discontinuity (Moho)
- A definite zone of discontinuity between the crust and the mantle.
- Was discovered by Dr. Andrija Mohorovicic in 1909.
B. The Mantle/Asthenosphere
- Layer lying between the crust and the core
- Made of iron and magnesium
- Has two layers
- Upper mantle
- Rocks are more elastic than those of sima.
- Temperature is about 1000◦c.
- lower mantle
- Rocks are like very viscous liquid.
- Temperature ranges between 1000◦c to 3000◦c.
Why the Interior of Earth Is Very Hot
- Due radio-active decay causing most of the heating.
- Due to great pressure as a result of overlying crustal materials.
- The original heat resulting from slow cooling of the materials which were pulled off the sun
Gutenberg Discontinuity
- A definite zone of discontinuity between mantle and core.
C. Core/barysphere/Centrosphere
- The innermost/central layer of the earth.
- Has 2 layers
Outer Core
- Composed of very dense rocks
- Made up of nickel and iron
- Temperatures are up to 3700◦c.
Inner Core
- A solid mass of mainly iron
- Temperatures are estimated to be 4500◦c to 5000◦c.
External Structure of the Earth
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- The Atmosphere
- Layer of gases surrounding the earth.
- The earth revolves with it because its held onto it by gravity
- It’s about 330km thick.
Composition of the Atmosphere
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- Gases-exist as a mixture
- Smoke particles
- Dust particles
- Water vapour
The structure of the Atmosphere
It’s divided into 4 layers/zones namely:
- Troposphere
-Lowest layer of the atmosphere
-Contains 90% of water vapour
-Rainfall is got from it
-Temperature decreases with increase in altitude (lapse rate)
-Air is turbulent due to mixing of air
-Contains dust particles
-There is a zone of transition between troposphere and stratosphere called tropopause.
- Stratosphere/ozonosphere
-Layer lying next to troposphere
-Has layers
-Lower isothermal layer in which temperature is constant
-Upper layer of temperature inversion in which temperature increases with increasing altitude
-Has ozone layer which absorbs harmful ultraviolet radiation.
-Air is calm so it’s used by passenger jets
-Limited amounts of water vapour
-There is a zone of transition between stratosphere and mesosphere called stratopause.
- Mesosphere
-Middle layer of the atmosphere.
-Temperature decreases with increasing altitude.
-There is a zone of transition between mesosphere and thermosphere called mesopause which is an inversion layer.
- Thermosphere/ionosphere
- High radiation is present.
- The pressure is very low.
- Gases and molecules in this layer exist as ions due to high radiation.
- Has no definite top but merges gradually into the outermost part of the atmosphere called exosphere.
- Exosphere consists of rare gases like hydrogen and helium.
- Beyond the atmosphere there is the outer space.
- Outer space is the universe beyond the atmosphere in which other planets and stars exist.
Significance of Atmosphere
- Animals and plants breathe in from it oxygen for respiration.
- Plants use carbon dioxide from it for photosynthesis.
- Water vapour in the atmosphere condenses to form clouds which give us rain.
- Ozone layer in the stratosphere shields us from ultraviolet radiation which may cause cancers.
- Carbon dioxide and methane in the atmosphere cause global warming through the green house effect.
b) The Hydrosphere
- Part of the earth’s surface covered by water masses e.g. oceans, seas, lakes, rivers and even underground water.
- It comprises 73% of the earth’s surface area.
- The atmosphere and hydrosphere are related in that atmospheric gases penetrate to the ocean depth in solution form.
- The lower atmosphere, hydrosphere and the upper part of the earth’s crust are called biosphere meaning the sphere of the earth in which organic life exists.
WEATHER
–Daily atmospheric conditions of a place at a particular time.
Elements of Weather
- Temperature
- Humidity precipitation
- Precipitation
- Atmospheric pressure
- Wind
- Sunshine
- Cloud cover
A Weather Station
–A place where observation, measuring and recording of weather elements is done
Factors to Be Taken Into Account When Sitting a Weather Station
- An open place where there is little obstruction of weather elements.
- Accessible place so that recording can be done easily.
- A fairly level or gently sloping ground (5◦) so that it’s easy to position weather instruments.
- The place should provide a wide view of the surrounding landscape and the sky.
- The site should be free from flooding.
- The place should have security.
Instruments for Measuring Elements of Weather
- Thermometer-temperature
- Hygrometer-humidity
- Rain gauge-rainfall
- Barometer-air pressure
- Sunshine recorder-sunshine duration and intensity
- Wind vane –wind direction
- Anemometer-wind speed
- Evaporimeter-rate and amount of evaporation.
The Stevenson Screen
A white wooden box mounted on 4 legs used to house thermometers and hygrometers.
The instruments which are found in it are:
- Maximum thermometer
- minimum thermometer
- Six’s thermometer
- hygrometer-wet bulb and dry bulb thermometer
Importance
- Provide shade conditions for accurate temperature recording.
- Ensure safety of thermometers because they are delicate.
Qualifications Which Make Stevenson Screen Suitable For Its Work
- Painted white for little absorption of solar heat energy.
- Made of wood which is a bad conductor of heat.
- Well ventilated to allow easier flow of air inside it.
- Raised to prevent contact with terrestrial radiation.
- Has double roof which acts as an insulator to prevent direct heating from the sun.
Recording and Calculating Weather Conditions
Temperature
-Degree of hotness of an object or a place.
It’s measured using 3 types of thermometers namely:
- Maximum thermometer
- Minimum thermometer
- Six’s thermometer
Maximum Thermometer
It’s used to measure the highest temperature reached in a day.
It uses mercury.
How It’s Used/Works
- Temperature rises causing mercury to expand.
- Mercury pushes the index up.
- When temperature falls mercury contracts.
- The maximum temperature is read from the scale at the lower end of the index.
- Thermometer is reset by shaking it to force mercury back into the bulb.
Minimum Thermometer
It’s used to record the lowest temperature reached in a day.
It uses alcohol.
How it’s Used/Works
- Temperature falls causing alcohol to contract.
- Alcohol pulls the index down.
- When temperature rises alcohol expands and rises in the tube.
- The index remains where it was pulled.
- Minimum temperature reading is obtained from the scale at the lower end of the index.
Calculating Temperature
- Diurnal/daily Temperature range
–Difference between the maximum and minimum temperature for any one day.
- Mean Daily Temperature
–Average of the maximum and the minimum daily temperatures.
- Mean Monthly temperature
-Sum of mean daily temperatures in a month divided by the number of days in that month.
- Mean Monthly minimum Temperature
–Sum of daily minimum temperatures divided by the number of days in that month.
- Mean Monthly Maximum Temperature
-Sum of daily maximum temperatures divided by the number of days in that month.
- Mean Annual Temperature
-Sum of mean monthly temperatures divided by 12.
- Mean Annual Temperature Range
–Difference between the highest and the lowest mean monthly temperatures in a year.
- ◦k=◦c+273
- ◦F=(◦c×1.8)+32 derive the rest from the formulas.
Rainfall
HOW TO MAINTAIN A POSITIVE ATTITUDE IN THE FACE OF ADVERSITY
HOW TO WORK SMARTER NOT HARDER.
well written notes