|
patterns of stars in the sky
|
Constellation
|
|
|
the light you see with your eyes
|
visible light
|
|
|
energy that can travel through space in the form of waves
|
electromagnetic radiation
|
|
|
the distance between the crest of one wave and the crest of the next wave
|
wavelength
|
|
|
a range of different colors with different wavelengths
|
spectrum
|
|
|
uses convex lenses to gather a large amount of light and focus it on a small area
|
refracting telescope
|
|
|
a piece of transparent glass curved so that the middle is thicker than the edges
|
convex lens
|
|
|
uses a mirror to gather a large amount of light and focus it on a small area
|
reflecting telescope
|
|
|
detects radio waves from objects in space
|
radio telescope
|
|
|
a building that contains one or more telescopes; usually built on mountaintops
|
observatory
|
|
|
breaks light from an object into colors and photographs the resulting spectrum; provides astronomers information about stars chemical composition and temperature
|
spectrograph
|
|
|
a structure that contains billions of stars
|
galaxy
|
|
|
all of space and everything in it
|
universe
|
|
|
the distance light travels in one year; about 9.5 million, million kilometers; a unit of distance not time
|
light-year
|
|
|
the apparent change in position of an object when you look at it from different places
|
parallax
|
|
|
very large stars
|
giant star
|
|
|
a star’s brightness as seen from Earth
|
apparent magnitude
|
|
|
the brightness a star would have if it were a standard distance from Earth
|
absolute magnitude
|
|
|
a graph that shows the relationship between a star’s brightness and temperature
|
Hertzsprung-Russell diagram
|
|
|
90% of all stars; a diagonal line of stars on the H-R diagram; surface temperature increases as brightness increases
|
main sequence
|
|
|
a tiny star left over when a giant star explodes; a neutron star that gives off radio waves
|
pulsar
|
|
|
where stars begin their lives; a large amount of gas and dust spread out in an immense volume
|
nebula
|
|
|
the earliest stage of a star’s life
|
protostar
|
|
|
formed when red giants grow bigger and the outer parts drift out into space leaving the blue-white core of the star
|
white dwarf
|
|
|
when a giant or supergiant star suddenly explodes and becomes very bright
|
supernova
|
|
|
the material left after a supernova, smaller and denser than white dwarfs
|
neutron star
|
|
|
remains of a massive star that has died; due to extreme mass, gravity is strong
|
black hole
|
|
|
bright objects that are very far away; the most distant objects in the universe
|
quasar
|
|
|
star systems with two stars
|
binary star
|
|
|
a star system in which one star blocks the light from another star
|
eclipsing binary
|
|
|
a large group of stars that have arms that spiral outward, like a pinwheel; the Milky Way is this type of galaxy
|
spiral galaxy
|
|
|
a large group of stars that look like flattened disks; have very little gas and dust between the stars
|
elliptical galaxy
|
|
|
large groups of stars without a definite shape
|
irregular galaxy
|
|
|
the theory that states the universe formed in an enormous explosion 10 to 15 billion years ago
|
big bang
|
|