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 earths 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
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 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◦.
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.
2. 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
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
Causes lunar eclipse due to
revolution bringing the earth in line with the sun and the moon.