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SCIENTIFIC TERMS


Absolute Zero
Acceleration
Accretion Disk
Andromeda Galaxy
Anthropic Principle
Antimatter
Apogee
Astronomical Unit
Atom
Big Bang
Binary Star
Black Holes
Cepheid Variable
Chandracekhar Mass
Corona
Cosmic Microwave Background
Coordinates
Cosmic Ray
Electron
Event Horizon
Fusion
Gamma Ray
Globular Cluster
Gravity
Gravitational Redshift
Heliosphere
Hertz
Hubble Constant
Inclination
Inverse-Square Law
Lagrangian Points
Law of Conservation of Energy
Mesons
Microwaves
Neutrinos
Parsec
Photon
Plasma
Quark
Singularity
Spectrum
Strong Force
Ultraviolet
Weak Force
X-Rays





Accretion Disk



Material gravitationally captured from a normal companion star, gas, nebula, or anything that strays near a massive object that causes a gravitational well (such as a black hole, neutron star, etc.) will spiral down into or onto the object. As it does, the material is heated by compression (the internal friction) to temperatures of up to 106K° centigrade, or possibly more. Matter at such a temperature will radiate strongly at the x-ray wavelength.


Andromeda Galaxy



The nearest spiral type galaxy similar to our own Milky Way. The Andromeda Galaxy is 2 million light years away (1.1749×1019 miles away. That is 11,749,000,000,000,000,000 miles) so we see it as it was 2 million years ago. Slightly bigger than our own galaxy, Andromeda has about 300 billion stars, compared to our 100 billion.


Antimatter



The opposite of the basic unit of matter. Consists of a nucleus (negatrons and neutrons) orbited by positrons. The development of a theroy combining the Special Theroy of relativity with Quantam Mechanics led to the prediction of the existance of antimatter, which has been proven since. Antimatter behaves in almost all respects like ordinary matter. In a striking demonstration of the equivalence of restmass and energy, a particle of matter and its antiparticle counterpart can be simultaneously created from the pure energy of a photon.


Black Holes



Any star over a value of 2-3 solar masses will cause its remnant core to collapse indefinately, becoming a black hole. The implosion takes perhaps one ten-thousandth of a second (1/0.0001 of a second). Perhaps the oddest thing about black holes is what we call Time Dialation, where time actually slows to a stop at the event horizon(depending upon point of view).


Globular Clusters



A dense symmetrical cluster of 105 to 106 stars. Generally found in the halo of the galaxy. Globular clusters are generally thought to represent remenants of the formation of galaxies.


Parsec



1 parsec is the distance at which one Astronomical Unit (the Earth orbit radius) subtends one arcsecond. 1 pc = 3.086×1018cm = 3.26 light years.


Lagrangian Points



Stable points in the orbit of a third body in a binary system. (ex. A planet in a binary star system. ex2. The third star ina trinary system.)


Red Giant Star



A star in which the helium core is fusing. Subsequent to the Red Subgiant stage.


Chandracekhar Mass



Maximum mass of a cold star that can support itself by internal pressure against gravitational collapse. Approx. 1.4 solar masses.


Event Horizon



Surface of a black hole: the boundry enclosing the region of spacetime that cannot communicate with the external universe. A one-way membrane accross which falling matteror light is captured and can never on its own escape.


Singularity



Region of infinate gravity, spacetime distortion, and mass at the center of a black hole.


Inclination



Angle of tilt of the orbital plane with respect to the fundamental plane.


Mesons



Elementary particles that decay within a short lifetime.


Heliospere



The area of space around a star that is dominated by the solar winds.


Absolute Zero



Tempurature at which a gas has no thermal energy. This is at 0ºK or at -459.69ºF.


Apogee



For an object in an elliptical orbit around another object. The point in its orbit of greatest enlongation.


Astronomical Unit



The average distance between the sun and the Earth; equal to 147,597,900 km.


Big Bang



The primordal explosion about 15 billion years ago that launched the expansion of the Universe to its present size.


Binary Star



Two stars in orbit around their common center of mass.


Cepheid Variable



A giant pulsating star whos period of variation is related to its absolute luminosity.


Corona



A mexican beer. Also the outermost portions of the solar atmosphere reaching millions of kilometers into space in the range of millions of degrees.


Cosmic Microwave Background



A relic radiation of the big bang. It now pervades the entire Universe with a charactoristic temp of 2.7ºK.


Cosmic Ray



Mostly electrons, protons, and helium nuclei moving through the galaxy at nearly the speed of light.


Electron



An elementary particle with one unit of negatice charge, and a mass of 9.1×10-20grams.


Fusion



Nuclear process that builds up heavier nuclei by joining protons and neutrons with the release of enormous amounts of energy.


Gamma Ray



Photons with the highest energies (in excess of 1 million electron volts) and highest frequencies (above 1020Hz).


Gravity



Force of attraction that matter exerts on other matter proportional to the product of the masses of two objects and inversely proportional to the square of their distance of seperation.


Gravitational Redshift



A decrease in the energy of a photon as it leaves the surface of a massive object. The shift of the wavelength to the red is proportional to the mass of the object divided by the radius of its surface.


Hertz



A unit of frequency equal to one cycle per second.


Hubble's Constant



The constant of proportionality that relates to the velocities of recession of galaxies to their distance.


Inverse-Square Law



The apparent brightness of a source decreases in proportion to the square of its distance. A star 100 light years away looks 1/4 as bright as the same star at a distance of 50 light years.


X-Rays



Photons of energies greater than that of gamma rays with frquencies from 1017 to 1020 hertz.


Weak Force



A washed up Jedi Knight or one of the four fundamental forces that acts only between certain elementary particles in a nucleus.


Ultraviolet



Photons of higher frequencies than visible light in the range of 1015 to 1016 hertz.


Strong Force



One of the four fundamental forces that is always active and operates only at distances less than 10-13 centimeters to hold together the nucleons inside an atomic nucleus.


Spectrum



The distribution of wavelength or frequency of the number of photons emitted or absorbed by a source.


Quark



Bar owner of DS9. Also an elementary particle that comes in several forms. Three quarks make up a proton or a neutron.


Plasma



An ionized gas in which the electrons that have been removed are free to move about.


Photon



A quantam packet of electromagnetic raditation with no mass and no electric charge, traveling at the speed of light.


Neutrino



An elementary particle with zero or very small rest mass and no electric charge that travels close to the speed of light.


Microwaves



Radio photons with wavelengths between 1 millimeter and a few centimeters.


Acceleration



The rate at which the speed of an object is changing.


Anthropic Principle



We see the Universe as it is because if it were different, we would not be here to observe it.


Atom



The basic unit of matter. Consisting of a nucleus (protons and neutrons) orbited by electrons.


The Law of Conservation of Energy



The law of science that states that energy (or its equivilent in mass) can neither be created or destroyed.


Coordinates



Numbers that specify the position of an object in space and time.