- Aether
Also referred to as ether.
A hypothetical medium to allow transmission of light, similar to the way the air acts as a medium to allow transmission of sound.
Following the Michelson-Morley Experiment it is generally accepted that this aether does not exist.
- Aphelion
The point when a planet, following its orbital path, is
farthest from the Sun.
- Apollo Program
The space program that took man to the moon in 1969, more information can be found in Space-Uplink's Space Race section.
- Astronomical Unit (A.U.)
-
An Astronomical Unit is the mean distance between the Earth and the Sun, i.e. the
Earth orbits at a distance of 1 AU from the Sun. It is equal to 149,597,870.691 kilometers.
- Chromatic
Aberration
Chromatic aberrations are caused by the lens in a refracting
telescope failing to focus different wavelengths of light (i.e. the
different colours of the spectrum that make up white light) onto
the exact same focal plane (i.e. it focuses them at slightly different distances).
It's effect is to create a purple blurring on the images.
Today this is overcome by either using a double lens or, in large
telescopes, by using process of reflection (mirrors) rather than
refraction (lenses)
.
- Doppler shift (also known as
Doppler Effect)
This effects both light and sound. It is caused by a change
in wavelength of the sound or light as a object moves relative to
the observer.
If the object is moving towards the observer the wavelength is
compressed, if it moving away the wavelength is stretched.
The apparent effect for light is the objects visible light is
altered, the spectrum is shifted towards blue if an object
approaches (blueshift) and towards red if the object recedes
(redshift). The effect for sound is a change in the pitch.
The amount of change is determined by the relative velocity of the
object.
- Dynamics
The study of the behaviour of motion on the Earth's
surface.
- E=mc^2
Einstein's famous equation known as the energy-mass relation. This basically states that mass and energy are interchangeable,
with the amount of energy released in conversion been equal to the mass converted multiplied by the speed of light squared. In other
words a small amount of mass converted releases a tremendous amount of energy. Nuclear fission, nuclear fusion and the antimatter annihilation all
produce energy in this method, in increasing orders of amount of mass converted.
- Energy Density
Simply the amount of energy available in a specific quantity of propellant.
- Galilean Moons (or Galilean
Satellites)
This refers to the 4 largest moons around Jupiter. Galileo
was the first to discover them in 1640 and are thus credited to
him in name.
The four satellites are known as Io, Europa, Ganymede and
Callisto.
Interestingly these same satellites were discovered independently
by Marius, and it is he who is responsible for their individual
names.
- Geocentric
Theory
Vision of the universe that places the Earth at it's centre
and proposes that the whole universe revolves around it.
- GIRD
Gruppa Isutcheniya Reakivnovo Dvisheniya, or Group for
Investigation of Reactive Motion. This was the USSR rocket
organisation.
- Heliocentric
Theory
This theory places the Sun at the centre of our solar
system, with the Earth, along with the rest of the planets,
revolving around it.
This theory is, of course, long proved correct.
- Hypersonic
High velocity flight, once passing around Mach 5, i.e. around 5500 km/h, the vehicle is termed hypersonic.
- Ionised
The state in which an atom is missing one or more of its electrons, and is therefore
positively charged. In an ionised gas some or all of the atoms are ionised, as opposed
to being electrically neutral as is the norm.
- Law of the Conservation of
Momentum
A fundamental law of motion, which states the momentum of a
system or an object is constant and cannot change due to any
internal interactions. Or in other words the momentum will remain
unchanged unless acted upon by an external force.
- Mass and
Weight
A body's mass would be constant on both the Earth and the
Moon (and anywhere else for that matter), however a body's weight
on the Moon would only be 1/6 of its weight on the Earth.
Why? Weight is simply the gravitational force exerted on a body
and therefore it is determined by the strength of the
gravitational field at your location. So the reason for the
body's weight being 6 times greater on the Earth than the Moon is
that gravity is 6 times stronger on the Earth's surface.
- Multi-Stage Rocket
This is a rocket with two or more engines lined along its
length. When the first engine burns out it ignites the next
engine, then releases itself from the rocket and falls
away.
You cannot use too many stages due to the excess weight the first
engine would have to carry.
- Nebulae (plural of
nebula)
The term used to refer to anything that astronomers could not
classify, for example when distant galaxies were first observed
as 'fuzzy patches of light' and it was not known as
to what they were they were simply labelled nebulae.
In modern times the word has been used to describe large clouds
of gas in space (they can be huge - 10's of light years
across!).
There are many different forms of nebula and their formation is
often based on some stage of a star's life - anywhere from the
formation of the star (such as the great Orion Nebula which is a
region of star formation in the Orion system) until the death of
the star (Planetary nebulae are clouds of gas blown free from a
dying star and the Crab Nebula is a remnant of a star gone
supernova in the Taurus system).
- Nuclear Fusion Break-even Point
The break-even point for nuclear fusion occurs when you harness as much energy from the reaction as you put in to achieve the reaction in the first place. Currently we are well below the break-even point, i.e. it takes much more energy to create the reaction than can be obtained from the reaction.
- Oort Cloud
The Oort Cloud is a massive spherical cloud of rocks and dust that may surround our solar
system. It is thought to exist between 50,000 to 100,000 A.U. from the Sun and may contain
anywhere from billions to trillions of comets.
It has not been directly observed, its existance is inferred from the orbits of
the long period comets.
- Perihelion
The point when a planet, following its orbital path, is
nearest to the Sun.
- Ramjet
A jet (air-breathing) engine that has no moving parts. Instead the air is compressed in the engine by the current speed of the aircraft.
This means that the engine has a relatively narrow operating range, the craft must be supersonic to gain a high enough compression, with the upper limit being between Mach 4 and 5
- Retrograde
Motion
The normal direction of a planets motion as we see it from
Earth is West to East against the background of the stars.
Occasionally, however, the planets outside the Earth's orbit can
be seen, over a number of nights, to slow, eventually to stop and
then to reverse direction (i.e. East to West against the
background) for a time! They will then appear to slow again, stop
and resume their original direction.
This caused real problems for the geocentric theory, and
Plotemy's attempts to explain the observed motion led to the
theory becoming very complex.
The correct reason for this motion was first realised by Copernicus in his
heliocentric theory, but it was not until Kepler produced his
work that it was conclusively understood.
The correct theory is that as Earth's orbital velocity is greater
than the planets outside it, so it will slowly catch up and
overtake these planets. The effect of this as viewed from Earth
is that their velocity across the sky will slow down as Earth
closes in to 'overtake' it, as Earth is passing their
path will seem to reverse for a short time and once passed the
path will revert to its original course.
- Scramjet
This is a Supersonic-combustion ramjet. Similar to the ramjet but provides correct compression at sustained hyersomic flight. Aircraft must be travelling over about Mach 4 for the scramjet to work. This engine should continue to accelerate all the way up to Mach 12-15.
The scramjet is not fully developed yet.
- Semimajor Axis
The semimajor axis is the distance from the centre of an ellipse
to the most distant point on its perimeter.
Due to the Sun not being at the centre of a planet's elliptical
orbit, but being offset, the semimajor axis defines a planet's
average distance from the Sun.
- Specific Impulse
A measurement for determining the relative performances of a rocket propellant that demonstrates how efficient the rocket is.
Specific impulse is basically equivalent to exhaust velocity, it is actually exhaust velocity divided by the constant g. As a result, specific impulse has units of seconds.
Physically, it is the number of seconds a rocket engine can produce one pound of thrust from one pound of fuel, so a specific impulse of 1,000,000 means that the engine gives 1,000,000 pounds of thrust, for one second, for every pound of fuel consumed.
The higher the specific impulse a rocket has, the less fuel it requires to produce a given amount of thrust.
- STM/AFM
Scanning Tunneling Microscopy (STM)
A type of scanning probe microscopy in which a very sharp tip is moved to within 1
nanometer of the sample. This starts a tiny tunneling current to flow between the
sample and the tip, which is accurately measured to produce 3 dimensional topographs
of the sample.
Atomic Force Microscopy (AFM)
This is very similar to the STM but here the tip actually physically rides over the sample
and its tiny movements are recorded, again allowing a 3 dimensional topograph to be created.
Both of these techniques of microscopy are able to anaylse down to individual atoms and
even move them with atomic precision, the limitation here is they may only move 1 atom at
a time.
- Sunspots
These are temporary areas of magnetic field concentration on
the Sun's photosphere (the visible surface of the Sun). In these
areas the magnetic concentration prevents the heat from the core
of the Sun escaping to the surface, which results in the area
being cooler. This is why these areas appear darker in the
images.
- Thrust
Thrust is a measure of how much force an engine can push with, it is equal to the exhaust velocity x the propellant mass (mass exhausted by the rocket) every second.
More properly, we speak of a propulsion system's thrust-to-weight ratio (T/W). This gives the acceleration that the engine can produce in units of Earth gravities. E.g. 2g means an acceleration of 2 x 9.8 or 19.6m/s2.
- Verein Fur
Raumschiffahrt
The German 'Society for Space Travel' that was to
investigate rockets for use in space.