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Light Year
The distance light travels in one year
Speed of Light
~300,000,000m/s
Age of the Universe
13.77 Billion years old
Diameter of the Observable Universe
93 Billion light years
Space flight is mostly Powered, or Free flight
Free Flight
Rocket
A gas chamber filled with gas under pressure
First artificial Satellite sent into space
Sputnik 1, USSR 1957
Atoms
The smallest division of a chemical element
Isotope
Atom with a different number of protons in the nucleus
Molecule
Molecule
Most abundant element in the universe
Hydrogen (75%)
Geospace
Near Earth, goes to the edge of the Magnetosphere
Cislunar Space
The space between the Earth and the Moon
Heliosphere
Spherearound the planets in the solar system
Interplanetary Space
The space between the planets in the solar system
Interstellar Space
The space between the stars
Intergalactic Space
The space between galaxies
Terrestrial Planets
Inner planets with rocky surfaces
Jovian Planets
Outer planets that are gaseous
Remote Sensing
Observation of objects in space from a distance
Passive Remote Sensing
Receiving and recording radiation using a telescope
Active Remote Sensing
Using a Laser beam to detect distances
Order of radiation waves (Low to High)
Radio, Microwave, Infrared, Visible, UV, X-Ray, Gamma
Seeing Effect
Pockets of turbulent air in the atmosphere cause stars to twinkle
Direct Sensing
Physically landing on an object for study
Need Reference Point
To determine location at different points
Day
One rotation of Earth about its axis
Month
One revolution of the moon about the Earth
Synodic Month
The completion of the entire cycle of a moons phases
Synchronized Orbits
The Earth and the Moon have the same rate of spinning about their axes
Year
One revolution of the Earth around the sun
Gregorian Calendar
365.25 days in a year, leap year every 4 years
Conjuction
When the moon is in between the Earth and the Sun
Opposition
When the Earth is in between the moon and the Sun
Space Flight Coordinates
Time, Down Range, Ground Track
Zenith
The point directly over head of an observer
Azimuth
The angle measured from N to E to determine horizontal location
Altitude
Angle from equator to N or S to determine location
Ecliptic
The path of the sun on the celestial sphere
Eudoxus
First to sytematically plot the constellations in the sky
Heliocentric
The sun is at the center of the Solar System
Johannes Kepler
German scientist who came up with 3 planetary laws
Minor Axis
The smallest axis of an ellipse
Major Axis
The largest axis of an ellipse
Ellipse
A geometric shape in which every point is the same distance from the two foci
Kepler's First Law
The orbits of the planets are ellipses around the sun
Aphelion
The point of Earth farthest from the Sun
Perihelion
The point of Earth closest to the sun
Kepler's Second Law
Aplanet moves along its elliptical path with a speed that changes in such a waythat a line from the planet to the Sun, the radius vector, sweeps out equalareas in equal intervals of time
Kepler's Third Law
P2=a3, using the semi-major axis
Solar Nebula Hypothesis
The solar system came about from rotating gas forming the planets and the center Sun

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