Inspiring The Engineers & Scientists of Tomorrow, Today! |
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| WELCOME TO THE REACH FOR THE STARS MATRIX! | ||||||
| SCIENCE APPLICATION AND TECHNOLOGY | ||||||
| Definitions | ||||||
| Other
Dictionaries: Imagine the Universe Additional Definitions Link Definitions -1 Definitions -2 Definitions -3
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| Absolute Magnitude: is a measure of the inherent brightness of a celestial object. This scale is defined as the apparent magnitude a star would have if it were seen from a standard distance of 32.6 light-years (10 parsecs). The lower the number, the brighter the object. Negative numbers indicate extreme brightness. | ||||||
| Apparent Magnitude: is a measure of the brightness of a celestial object as seen from Earth. The lower the number, the brighter the object. Negative numbers indicate extreme brightness. The full moon has an apparent magnitude of -12.6; the sun's is -26.8. We can see objects up to 6th magnitude without a telescope. Apparent magnitude is abbreviated m. This system of rating the brightness of celestial objects was developed by the Greek astronomer Hipparchus in 120 B.C. | ||||||
| Atmospheres: 1.013 bars = 1.03 kg/cm2 = 14.7 pounds per square inch, standard atmospheric pressure at sea level on Earth. | ||||||
| Aurora's:
A phenomena created by
an interaction between highly charged particles from solar
flares, the
earths magnetic field and the earth's atmosphere.
Charged
particles from a solar flare are channeled over the earths magnetic field
much like a rock in a stream. The particles force the first magnetic field
lines it encounters to break and then reconnect on the night side of the
Earth. When this magnetic reconnection (animation)
occurs out in space the particles flow back towards Earth along the
magnetic field lines and enter the atmosphere at the poles.
The charged ions impact with gases in the atmosphere and give
off different colors of light. Periodically the poles shift
polarity meaning some day the north pole will shift to the current
south pole position. This process is thought to take about 2000 to
3000 years during which time Aurora's will occur all around the Earth
rather than at the poles.
HEAVEN'S
FIRE : (The Aurora's) Images Courtesy of
Current
Aurora Activity (Site I) Current
Aurora Activity (Site II)
Sounds
of the Magnetosphere (An Auroral Presentation)
Want to see Images of the Aurora around the world as they occurred on March 31, 2001? They saw it as far south as Houston Texas and there is a picture from Payson, Arizona. Keep looking up and you just might see it tonight. Follow this link
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| Celestial Sphere, Equator & Poles : The equatorial coordinate system is based on the celestial sphere. The celestial sphere is a giant imaginary globe surrounding Earth. This sphere has north and south celestial poles directly above Earth's North and South poles. It has a celestial equator, directly above Earth's equator. | ||||||
| Corona : | ||||||
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Density
:
Amount
of a substance contained within a specific area. In physics, density is
the ratio of the mass
of a substance to its volume,
and it can be calculated by dividing the mass by the volume. Density is
often expressed in units such as grams per cubic centimeter (g/cm3) or
pounds per cubic foot (lb/ft3). The density of a substance can vary under different conditions. Substances expand and contract as their temperature changes, and as a result their density also changes. Precise measurements of density therefore include the temperature at which they were taken. "Density," Microsoft® Encarta® Online
Encyclopedia 2001 ©
1997-2001 Microsoft Corporation. All rights reserved. |
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| Ecliptic Plane : The ecliptic plane is the imaginary plane (like a disc) containing the Earth's orbit around the Sun. As seen in the sky the sun follows this path during the day and the planets all tend to lie near this path as well. This plane was created during the formation of our Sun as it was spinning, creating the flattened, proto-planetary disk. | ||||||
| Heliosphere
: The
heliosphere is a bubble in space produced by the solar wind. Although
electrically neutral, atoms from interstellar space can penetrate this
bubble, virtually all of the material in the heliosphere emanates from the
Sun itself. This
sphere is comprised of the heliopause and helio-sheath. Source : http://science.msfc.nasa.gov/ssl/pad/solar/heliosph.htm |
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Heliopause
& Helio-sheath :
(Info-link)
- The solar wind streams off of the Sun in all directions at speeds of
several hundred km/s (about 1,000,000 mph in the Earth's vicinity). At
some distance from the Sun, well beyond the orbit of Pluto, this
supersonic wind must slow down to meet the gases in the interstellar
medium. It must first pass through a shock, the termination
shock, to become subsonic. It then slows down and gets turned in
the direction of the ambient flow of the interstellar medium to form a
comet-like tail behind the Sun.
Source : http://science.msfc.nasa.gov/ssl/pad/solar/heliosph.htm |
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| Helium (He): A colorless, odorless gas which is the second lightest known element in the universe containing two protons, two neutrons and two electrons. Helium is the second element created in the process of nucleosynthesis. Second element in the periodic table. 4.002602 atomic mass. Atomic number 2. One of the three basic elements created in the big bang. Hydrogen and Lithium are the other two. (periodic table) | ||||||
| Hydrogen (H): A colorless, odorless gas which is the lightest known element in the universe containing one proton, one neutron and one electron. Hydrogen is the base element upon which all other elements are built. (see nucleosynthesis) First element in the periodic table. 1.00794 atomic mass. Atomic number 1 Most abundant element in the universe was one of the three basic elements created in the big bang. Helium and Lithium are the other two. (periodic table) | ||||||
| Kelvin (K): 0 Kelvin is absolute zero; H2O (water-ice) melts at 273 K (= 0° C = 32° F); H2O boils at 373 K (= 100° C = 212° F). (developed by William Thomson). | ||||||
| Mass:
In
physics, the amount of matter that a body contains, and a measure of the
inertial property of that body, that is, of its resistance to change of
motion (see Inertia).
Mass is different from weight, which is a measure of the attraction of the
earth for a given mass (see Gravitation).
Inertial mass and gravitational mass are identical. Weight, although
proportional to mass, varies with the position of a given mass relative to
the earth; thus, equal masses at the same location in a gravitational
field will have equal weights. A mass in interstellar space may have zero
weight. A fundamental principle of classical physics is the law of
conservation of mass, which states that matter cannot be created or
destroyed. This law holds true in chemical reactions but is modified in
cases where atoms disintegrate and matter is converted to energy
or energy is converted to matter (see Nuclear
Energy; X
Ray: Pair Production). The theory of relativity, initially formulated in 1905 by the German-born American physicist Albert Einstein, did much to change traditional concepts of mass. In modern physics, the mass of an object is regarded as changing as its velocity approaches that of light, that is, when it approaches 300,000 km/sec (about 186,000 mi/sec); an object moving at a speed of approximately 260,000 km/sec (about 160,000 mi/sec), for example, has a mass about double its so-called rest mass. Where such velocities are involved, as in nuclear reactions, mass can be converted into energy and vice versa, as suggested by Einstein in his famous equation E = mc2 (energy equals mass multiplied by the velocity of light squared). "Mass
(physics)," Microsoft® Encarta® Online Encyclopedia 2001 © 1997-2001 Microsoft Corporation. All rights reserved. |
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| Magnetosphere
: (Info-Link)
A
region above the planetary surface in which charged particles (from a solar
wind) are affected by the planet's magnetic field. The solar wind in turn
shapes and deforms the magnetic field creating a fluctuating
equilibrium. The magnetosphere fluctuates constantly even flipping
it's magnetic north / south poles periodically. Mercury and Earth are
the only inner planets known to have magnetic fields which are thought to
be a result of liquid cores and the planets rotation. Components: Bowshock, Magnetosheath, Magnetopause, Plasma Sphere Trapping Region (Plasma Sheet), Lobes, Radiation Belts, Currents, Magnetic Flux
Earth's Bow Shock &
Magnetopause (realtime anim)
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| Nuclear fusion : | ||||||
| Nucleosynthesis : (Info-link) The process that occurs in stars that converts hydrogen to helium and so on into successively heavier elements up to and including iron. (see periodic table) The creation of elements heavier than iron was, until recently, thought to occur only when a supernova event happened. A discovery in Aug. 2001 pointed to stars which can produce elements up to lead without the supernova event occurring. | ||||||
| Radiation : | ||||||
| Solar
wind : (Info-Link)-
The solar wind streams off of the Sun in all directions at speeds of about
400 km/s (about 1 million miles per hour). The source of the solar wind is
the Sun's hot corona.
The temperature of the corona is so high that the Sun's gravity cannot
hold on to it. Although we understand why this happens we do not
understand the details about how and where the coronal gases are
accelerated to these high velocities. The solar wind is made of Hydrogen
(95%) and Helium (4%) and Carbon, Nitrogen, Oxygen, Neon, Magnesium,
Silicon and Iron (~1%). These atoms are all in the form of a plasma
of positive ions
which means they have lost electrons because the temperature is so hot.
This question is related to the
question of coronal
heating. Source : http://science.msfc.nasa.gov/ssl/pad/solar/sun_wind.htm |
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| Speed of Light : 300,000 km/sec (about 186,000 mi/sec) | ||||||
| Superposition: A term synonymous with geology The law states "that strata that are younger will be deposited on top of strata that are older, given normal conditions of deposition." Relative to identifying the order of occurrence of geological activity and impact craters on planetary bodies. This term relates to the ordering of events based on the interruption of boundaries in a geological or impact event. Essentially if a crater boundary disrupts the line of a fault then the crater is more recent. | ||||||
| Volume
: In
mathematics,
the amount of space occupied by a solid figure. Volume is measured in
terms of cubic units, such as cubic inches or cubic feet in the English
system of weights and measures, and in cubic centimeters or cubic meters
in the metric
system. Volume may also be expressed in such liquid or dry measures as
liters and bushels. See Weights
and Measures. "Volume,"
Microsoft® Encarta® Online Encyclopedia 2001
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