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25 Cards in this Set

  • Front
  • Back

Spectrum

A range of colors

Apparent magnitude

How bright a light looks

Absolute magnitude

The actual brightness of a star

Light year

The distance that light travels In one year.



Parallax

The apparent shift in a stars location

H-R diagram

A graph showing the relationship between a stars temp. and it's absolute magnitude

Main sequence

The diagonal patten of stars on a H-R diagram

White dwarf

Small hot stars that are the leftover centers from larger old stars

Red giant

A star that has grown very large

Supernova

The death of a large star by an explosion

Neutron star

Forms when the particles inside a star turn to neutrons

Pulsar

A spinning neutron star

Black hole

When a supernova collapses

Galaxies

Large round groups of stars

Spiral galaxies

galaxies in the shape of a spiral

Elliptical galaxies

have very bright centers and very little dust and gas

Irregular galaxies

galaxies that don't fit into any other class

nebulas

giant clouds of gas and dust

Globular clusters

groups of older stars

Open clusters

groups of stars that are located along a spiral disc of a galaxy

quasars

galaxies in the process of forming

cosmology

study of the origin and the future of the universe

big bang theory

states that the universe began with a big explosion

cosmic background radiation

radiation left over in space

The

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