the actual (true) brightness of a star
the brightness of a star as seen from Earth
barred spiral galaxy
a galaxy that is similar to a spiral galaxy, except that the spiral arm pattern originates from a bar of material that passes through the nucleus of the galaxy.
a system of two stars that revolve around each other under their mutual gravitation
final stage in the evolution of a very massive star, where the core's mass collapses to a point that its gravity is so strong that not even light can escape
stars that appear to travel in a circle around the celestial poles
A group of stars that form a pattern in the sky
a galaxy shaped like a round or flattened ball, generally containing only old stars
a collection of stars, dust, and gas bound together by gravity
a very large, cool, bright star; much larger than the sun
spherically shaped group of hundreds of stars located around the core of the Milky Way Galaxy
Hertzsprung-Russell diagram, a graph that shows the relationship between a star's surface temperature and absolute magnitude
a galaxy that does not fit into any other category; one with an irregular shape
the distance light travels in one year (9.5 trillion kilometers)
a normal star that is undergoing nuclear fusion of hydrogen into helium. Our sun is a typical main sequence star.
a large cloud of dust and gas that can break apart into smaller pieces and form stars, large cloud of gas and dust that contracts under gravitational force and breaks apart into smaller pieces, each of which might collapse to form a star
collapsed core of a supernova consisting of a small, extremely dense ball of neutrons
white dwarf star that explodes as it cools, temporarily becoming thousands of times brighter
a star cluster that has a loose, disorganized appearance and contains no more than a few thousand stars
method of determining the distance from the earth to a star based on the shift in the apparent position of the star when viewed from different angles
expanding shell of gases shed by a dying star
Early form of a star; This stage lies between the collapsing of dust and gas and the beginning of nuclear fusion
neutron star that emits two beams of radiation that sweep across space
a starlike object that may send out radio waves and other forms of energy
the change in the wavelength of light due to an object moving away from the observer.
a galaxy with a bulge in the middle and arms that spiral outward in a pinwheel pattern
a body of gases that gives off a tremendous amount of radiant energy in the form of light and heat
an extremely large, giant star
the brilliant explosion of a dying supergiant star
a small, hot, dim star that is the leftover center of an old star
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