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Ch 11 '14
Galaxies are cool in life
Term | Definition |
---|---|
asteroid | Small rocky bodies in our solar systems, most of which orbit the Sun Mars and Jupiter. |
axis | An imaginary line through Earth, extending from the North pole to the South Pole. |
black hole | A large sphere of incredibly tightly packed material with an extraordinary amount of gravitational pull created when a star collapses into itself. Not even light can escape it. |
comet | A small body made up of rocky material and ice that occurs in the Kuiper Belt and the Oort Cloud; when a comet is bumped into the inner solar system, the Sun's light may make the comet's tail visible from earth. |
Doppler effect | The change in wavelengths of electromagnetic radiation or sound that occurs because of the movement of the source relative to the observer. |
fusion | The process in which the nuclei of atoms fuse together to form larger single atoms, creating an enormous amount of energy. |
interstellar matter | The material that fills space, made up of gas( mostly hydrogen)and dust. |
light-year | The distance that light which moves at 300000km/sec, travels in a year; equals about 9.5 trillion km. |
moon | Celestial bodies that orbit a planet. |
parallax | the apparent shift of an object against a stationary background caused by a change in the position of the observer. |
planet | A celestial planet that orbits one or more stars, is large enough that its own gravity holds its spherical shape and is the only body occupying the orbital path. |
revolution | The motion of earth as it orbits the Sun. |
rotation | The motion of Earth as it spins on its axis from west to east. |
solar system | A group of planets circling one or more stars. |
star | A celestial body of hot gases with a core like a furnace that makes its own thermal energy. |
supernova | A dramatic, massive explosion that occurs when a large, high mass star collapses in on itself. |
triangulation | A technique for determining the distance to a visible object by creating an imaginary triangle between the observer and the object and then calculating the distance. |