A satellite is any object
that orbits a planet. The Moon is the Earth's only natural
satellite. There are at least 60 natural satellites in the
solar system. Some of these, such as Ganymede, the largest
satellite of Jupiter, are larger than the smallest planets,
Pluto and Mercury. The planet with the
greatest number of natural satellites is Saturn with
18. A man-made satellite is
known as an artificial satellite. Orbits can be
equatorial,
polar
or geostationary. A quantity that has
magnitude (or size) but not direction; e.g. . The following
quantities are scalar: average speed, energy,
power, time,
temperature,
potential
difference.
See
also vector The name given to the
deflection of particles of matter or electromagnetic
radiation by the
particles that make up the material through which they
pass. Scattering of
alpha
particles by the
nuclei of gold atoms enabled Ernest Rutherford (1871-1937),
the New Zeland physicist to discover the structure
of the atom. The
experiment, performed in Manchester University in 1911 by
Hans Geiger (1882-1945), a German physicist, working for
Rutherford, is known as alpha-particle
scattering. Scattering of visible
light by molecules of gas that make up our atmosphere is the
reason why a clear daytime sky is blue. The second is the unit of
time. There are 60 x 60 (or 3,600) seconds in one
hour. WWW:
SECOND Newton's second law of
motion states that the rate of change of momentum
of a body is proportional to the unbalanced
force action on
it. In other words, an
unbalanced force is needed to change the velocity of an
object. This definition leads to
the formula: Secondary waves (also
known as S-waves) are transverse
seismic
waves that are
caused by earthquakes.
S-waves can't travel through liquid, which is why they can't
be detected over a wide region of the Earth's surface
directly opposite their source. This fact was used by
geologists to show that the Earth must have a liquid
core. Seismic waves are powerful
vibrations due to earthquakes. There are two types of
seismic wave: P-waves
and S-waves.
These vibrations travel
through the Earth until they reach the surface. They are the
most useful information that scientists have with which to
study the Earth's inner structure. WWW:
SEISMIC
WAVES A substance that has
electrical properties that lie between a conductor
and an insulator.
Silicon and germanium are natural semiconductors.
If a small amount of a
foreign substance added to a semiconductor (a process known
as doping), the original material can become a normal
conductor. An electrical
circuit in which
components are connected one after the other. The current
through each component is the same as its
neighbours. When a short circuit
occurs in an electrical
circuit the
current does not flow around the whole circuit. Instead it
bypasses some or all the components and returns to the
supply by a path of low resistance either because the
uninsulated leads from the supply have made contact or
because a wire is used to bridge the components. A short circuit often
results in a large current being drawn from the supply,
which can damage either the supply or the leads through
which the current flows, or both. The leads may heat up
enough to cause a fire. The solar constant is the
amount of energy that reaches each square metre of the
Earth's surface from the Sun per second. The average value
of the solar constant at the top of the atmosphere is 1400
W/m2 . Solar power is the general
name given to the Sun's radiant
energy. This can
be a source of thermal
energy, when it is
used to heat water in passive solar panels, or of
electrical
energy in
photovoltatic
cells. The system of
planets,
moons,
asteroids,
comets
& dust centred on the Sun. WWW:
ABOUT
PLANETS A state of matter in which
atoms are in close contact and exert forces on one another
when they move from their equilibrium position. Atoms in the
solid state therefore vibrate
about a mean position. The amplitude
of vibration depends on temperature:
the hotter the solid, the larger the amplitude of vibration.
This is why solids expand when heated. Sound is the
vibration
of a medium that is audible to the human ear. The perfect
human ear is sensitive to frequencies
between 20 hz and 20,000 hz. In practice, few people are
sensitive to the highest frequencies. Furthermore, one loses
sensitivity to high frequency as one gets older. Vibrations with
frequencies less than 20 hz are called infrasound,
and those with frequencies above 20,000 hz are called
ultrasound.
Humans are unable to hear either infrasound or
ultrasound. A spark is a brief
electrical current that flows between charged bodies or a
charged body and the earth when the electrical insulation of
the air gap between them breaks down due to ionisation
of the air. Dry air is ionised when an electrical
field reaches
about 30kV/cm, i.e. 3,000,000 Volts per metre. Since water
vapour is always present in the atmosphere to some degree,
sparks usually occur at much lower electric field
strengths. Specific heat
capacity (or s.h.c.) is the quantity of internal energy
required to change the temperature of one kilogram of a
substance by one degree Celsius or Kelvin. The unit of
s.h.c. is 'Joules per kilogram per degree Kelvin'. Each
substance has its own unique specific heat capacity. Water
has the largest s.h.c. (4200 J/kgK). Metals have low s.h.c.
compared to liquids. This means that it takes less heat to
warm up an object made of metal than one which is a liquid
(given that they have the same mass).. Specific latent heat (or
s.l.h.) is the quantity of energy required to
change
the state of 1 kg
of a substance. The science of producing
and analysing spectra
using spectroscope, which is an instrument that forms a
spectrum of a source of light or other electromagnetic
radiation. A spectrum is a range of
properties arranged in order of size. A spectrum of white light
is created when a narrow beam of white light passes through
a prism or a diffraction grating. The resulting spectrum
consists of the following colours in order: red, orange,
yellow, gree, blue and violet. The inclusion of the
'seventh' colour, indigo, is an artifice introduced to
satisfy Isaac Newton's numerological fancy. Indigo is
not visible in the spectrum of white
light. The average
velocity
at which an object moves between two points. Speed is total
distance covered / total time taken. Speed is a
scalar
quantity. All electromagnetic
waves travel
through a vacuum
at the same speed, 300,000,000 metres per second. This is
known as the speed of light, and it is the greatest speed at
which electromagnetic waves can travel. Electromagnetic
waves travel more slowly through transparent materials such
as glass and water. The speed of light in a medium other
than a vacuum can be calculated from the refractive
index of the
medium. 300,000,000 m/s is
approximately the same as 1,000,000,000 km/hr (one billion
kilometres per hour), which in some ways is a more useful
way to think about the speed of light. For example, Saturn
is about 1.5 billion kilometres from the Sun so light takes
about 1.5 hours to reach Saturn from the Sun. WWW:
SPEED
OF LIGHT A star is a large body
composed mainly of hydrogen and helium that emits visible
light and other forms of electromagnetic energy due to a
thermonuclear
reaction at its
core. Stars differ from one
another in mass and brightness: the more massive a star the
brighter it is. The Sun is a star. Most stars are smaller
and less hot then the Sun. WWW:
STAR The apparent shift in the
position of a nearby star relative to more distant stars due
to changes in the Earth's position as it orbits the Sun.
Stellar parallax is greatest when a star is observed 6
months apart. Stellar parallax is imperceptible to the naked
eye. See also
parsec The shortest distance in
which a moving vehicle (motorcycle, car, bus, truck etc.)
can be brought to rest by its brakes. On the
web: When an object is
stretched or squeezed elastically,
the work done in deforming it is stored as energy. This
energy is known as strain energy. A catapult is an example
in which strain energy is stored by stretching rubber. When
the elastic cord is released, the strain energy is
transferred into kinetic
energy in the
projectile being launched. The stratosphere is the
second major layer of air in the atmosphere.
It lies above the troposphere
and stretches from 10 to 50 km above the Earth's surface.
The air temperature in the stratosphere remains relatively
constant up to an altitude of 25 km. Then it increases
gradually to 200-220 degrees Kelvin (K). Because the air
temperature in the stratosphere increases with altitude, it
does not cause convection and has a stabilizing effect on
atmospheric conditions in the region. The Sun is a
star.
It has a diameter of 1,394,000
km (about 110 times the diameter of Earth) and a mass of
1.99 x
1030 kg (
about 99.9% of the total mass of the Solar System.)
The source of the Sun's
energy is nuclear
fusion that takes
place within its core (which makes up the innermost 10% of
the Sun.) The core temperature is about 15 million
Kelvin
, and it's surface temperature is 6000 K. The total lifetime
of the Sun is estimated as 10 billion years. It is about
half way through its life now. The Sun emits
radiant
energy from its
surface mainly as infrared, visible light and ultraviolet.
The Sun will become a
white
dwarf after it has
exhausted its nuclear fuel. The final stage in the
life of a massive star. This happens when it has exhausted
its nuclear fuel and so fusion
reactions are no longer possible. The star then first
collapses and this is followed by an explosion in which so
much energy is released that the supernova can outshine an
entire galaxy
of several billion stars, if only for a few minutes. The
remains of the exploded star becomes a neutron
star or, in the
case of the most massive stars, it becomes a
black
hole. The Systeme International
(or SI) has been adopted for most scientific work. It is
based on the metric system. There are seven base units for
seven base quantities Length Mass Time Current Temperature Luminous
intensity amount of
substance metre kilogram second Ampere Kelvin candela mole

WWW:
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back
to GCSE syllabus
Date Last
Modified: April
2003
Emanuel School, London SW11 1HS
All text and diagrams copyright of J.C.Naylor