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THE EARTH AND THE SOLAR SYSTEM

THE EARTH AND THE SOLAR SYSTEM

The Earth and the Solar System

Solar system is the group of heavenly bodies comprising the sun and the nine planets.

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The origin of the Solar System

Theories

A theory is a set of reasoned ideas intended to explain facts or events

  1. 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
  1. 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.

  1. Nebula Clod Theory

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  • 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.

THE EARTH AND THE SOLAR SYSTEM

  1. 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.
  1. The Planets

Planets are large spherical celestial/heavenly bodies in space.

There are 9 planets in our solar system.

Characteristics

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  • 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

THE EARTH AND THE SOLAR SYSTEM

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

              Solar/Sun Eclipse

-Phenomenon occurring when the rays of the sun are blocked from reaching the earth or the moon.

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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 earths shadow is cast on the moon
  • The moon appears to be covered by darkness

THE EARTH AND THE SOLAR SYSTEM

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

  1. If one moves towards the east in a straight line he will end up where he started.
  2. Satellite photographs taken from space show that the earth is like a sphere.
  3. Places in the east see the sun earlier than those in the west.
  4. When a ship is approaching the smoke is seen first, then the mast and finally the whole ship.
  5. All the planets are spherical so the earth being one of them is also spherical.
  6. During the moon eclipse the earth casts a spherical shadow on the moon.
  7. 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 EARTH AND THE SOLAR SYSTEM

The Movement of the Earth

There are 2 movements of the earth namely:

  1. Rotation of the earth on its axis
  2. 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

  1. 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).
  2. Causes deflection of winds and ocean currents in the N hemisphere to the left and in the S hemisphere to the right.
  3. It causes rising and falling of ocean tides.
  4. Causes time difference between longitudes.
  • Takes one hour to go through 15◦.
  • 4 min to go through 1◦.

THE EARTH AND THE SOLAR SYSTEM

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

  1. 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.

  1. 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

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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.

THE EARTH AND THE SOLAR SYSTEM

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

  1. Causes the four seasons summer, autumn, winter and spring due to the movement of overhead sun causing changes in the heat belt.
  2. 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.
  3. 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
  1. Causes lunar eclipse due to revolution bringing the earth in line with the sun and the moon.

THE EARTH AND THE SOLAR SYSTEM

The Structure of the Earth

Internal Structure of the Earth

The evidence used to study the earth’s interior are

  1. mining
  2. drilling
  3. quarrying/excavation
  4. 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 al
  1. 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.
  1. The Mantle/Asthenosphere
  • Layer lying between the crust and the core
  • Made of iron and magnesium
  • Has two layers
  1. Upper mantle
  • Rocks are more elastic than those of sima.
  • Temperature is about 1000◦c.
  1. lower mantle
  • Rocks are like very viscous liquid.
  • Temperature ranges between 1000◦c to 3000◦c.

Why the Interior of Earth Is Very Hot

  1. Due radio-active decay causing most of the heating.
  2. Due to great pressure as a result of overlying crustal materials.
  3. The original heat resulting from slow cooling of the materials which were pulled off the sun

THE EARTH AND THE SOLAR SYSTEM

Gutenberg Discontinuity

  • A definite zone of discontinuity between mantle and core.
  1. 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

  1. 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.

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Composition of the Atmosphere

  1. Gases-exist as a mixture
  2. Smoke particles
  3. Dust particles
  4. Water vapour

THE EARTH AND THE SOLAR SYSTEM

The structure of the Atmosphere

It’s divided into 4 layers/zones namely:

  1. 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.

  1. 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 its used by passenger jets

Limited amounts of water vapour

There is a zone of transition between stratosphere and mesosphere called stratopause.

  1. 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.

  1. 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

  1. Animals and plants breathe in from it oxygen for respiration.
  2. Plants use carbon dioxide from it for photosynthesis.
  3. Water vapour in the atmosphere condenses to form clouds which give us rain.
  4. Ozone layer in the stratosphere shields us from ultraviolet radiation which may cause cancers.
  5. Carbon dioxide and methane in the atmosphere cause global warming through the green house effect.
  6. 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 earths crust are called biosphere meaning the sphere of the earth in which organic life exists.

THE EARTH AND THE SOLAR SYSTEM

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