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0E-Gravity-SolarSys
Gravity & the Solar System
Question | Answer |
---|---|
acceleration due to gravity | 9.8 m/s/s - every second, a falling object will travel faster than it was a second ago. On Earth objects fall 9.5 meters per second faster every second |
accretion | growing in size due to the gradual accumulation of layers |
Astronomical Unit (AU) | the mean (average) distance from the center of the Earth to the center of the Sun. |
Big Bang Theory | a theory that says the universe began as a small point that expanded rapidly about 13.7 billion years ago |
escape velocity | the lowest velocity a body must have in order to escape the gravitational attraction of a particular planet |
force | a push or pull that can change the motion of an object |
gravity | a distortion of space (spacetime) caused by the presence of matter or energy (Einstein’s theory) |
inertia | the tendency of an object to resist a change in motion |
light year | the distance that light travels in one year |
mass | a measure of how much matter is in a substance |
model | a three-dimensional representation of something, typically on a smaller scale than the original |
Newton | SI unit of measurement for weight |
orbit | a curved path followed by an object as it revolves around another object |
bound orbit | Orbit in which an makes multiple (or continuous) loops around another object |
unbound orbit | Smaller object is attracted to bigger object, but not enough to begin to orbit |
minimal orbital speed | The slowest orbital speed an object can have and still stay in orbit – orbit is circular |
preferred orbital direction | The direction that the majority (often all) of the orbiting objects are traveling (clockwise or counter-clockwise) |
scale | an accurate representation of something which has been either reduced or enlarged from its original size keeping the proportions accurate |
terminal velocity | the constant speed a falling object reaches when it cannot accelerate any further due to resistance |
velocity | speed with direction |
weight | the heaviness of an object – how much gravity is pulling on an object’s mass |
asteroid | large and small rocks or metallic masses orbiting the sun |
asteroid belt | the space between the orbits of Mars and Jupiter in which most asteroids are found |
comet | a celestial object consisting of a nucleus of ice and dust and, when near the sun, a “tail” of gas and dust particles pointing away from the sun |
dust | tiny particles of matter floating in space, condenses under gravity to form stars and planets |
galaxy | a large grouping of stars in a space |
gas | a form of matter with indefinite shape and volume |
Kuiper Belt | a region beyond the orbit of Neptune believed to contain many comets, asteroids, and other small bodies made largely of ice |
Kuiper Belt object | ice-rock bodies that inhabit the outer Solar System |
Milky Way | a spiral galaxy that contains our Solar System along with several hundred billion stars |
moon | a celestial body that revolves around a planet |
Oort Cloud | a theoretical concept of a cloud of predominantly icy planetesimals proposed to surround the Sun at distances ranging from 2,000 to 200,000 AU |
planet | any of the large celestial bodies that revolve around the Sun in the solar system |
satellite | a natural or artificial body in orbit around Earth or another planet |
solar system | the Sun and the planets and other celestial bodies that are held by their gravitational attraction and revolve around the Sun |
star | a large, spherical celestial body consisting of a mass of gas that is hot enough to sustain nuclear fusion and thus produce radiant energy |
stellar system | a star with one or more objects in orbit around it – (the second object could be another star, multiple stars, planets, etc.) |
sun | the luminous star around which Earth and other planets revolve; composed mainly of hydrogen and helium |