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Kepler's Laws
Three laws that describe the motion of planets around the sun: 1) planets move in elliptical orbits, 2) a line segment joining a planet and the sun sweeps out equal areas during equal intervals of time, 3) the square of the period of a planet is proportional to the cube of the semi-major axis of its orbit.
Luminosity
The total amount of energy emitted by a star or other celestial body per unit time.
Redshift
The phenomenon where the wavelength of light from an object is increased (shifted to the red end of the spectrum) as the object moves away from an observer, indicating the universe is expanding.
Black Hole
A region in space where the gravitational pull is so strong that nothing, not even light, can escape from it.
Event Horizon
The boundary around a black hole beyond which no light or other radiation can escape.
Gravity
The force that attracts two bodies towards each other, proportional to their masses and inversely proportional to the square of the distance between them.
Supernova
A powerful and luminous explosion of a star that occurs at the end of its life cycle.
Neutron Star
A compact celestial object composed almost entirely of neutrons, formed by the gravitational collapse of a massive star after a supernova.
Planetary Nebula
A ring-shaped nebula formed by the expansion of gas from a red giant star at the end of its life.
Red Giant
A late phase in the life cycle of a star, characterized by a large size and a reddish color due to cooler surface temperatures