Chapter 4 Astronomy

telescope

A device built to observe distant objects by making them appear closer

electromagnetic radiation

a form of energy that exhibits wavelike behavior as it travels through space

visible light

Electromagnetic radiation that can be seen with the unaided eye

wavelength

Horizontal distance between the crests or between the troughs of two adjacent waves

spectrum

BAND OF COLORS PRODUCED WHEN SUNLIGHT PASSES THROUGH A PRISM

optical telescope

a telescope that uses lenses or mirrors to collect and focus visible light

refracting telescope

A telescope that uses convex lenses to gather and focus light

convex lens

A lens that is thicker in the middle than at the edges.

reflecting telescope

A telescope that uses a curved mirror to collect and focus light

radio telescopes

Devices used to detect radio waves from objects in space

observatory

a building that contains one or more telescopes

constellations

A group of stars that forms a shape or pattern.

spectrograph

An instrument that separates light into colors and makes an image of the resulting spectrum.

apparent brightness

the brightness of a star as seen from Earth

absolute brightness

the brightness a star would have if it were at a standard distance from earth

light year

Distance light travels in one year.

parallax

An apparent shift in the position of an object when viewed from different locations

Hertzsprung-Russell diagram

a graph relating the surface temperatures and absolute brightness of stars

main sequence

a diagonal area on an H-R diagram that includes more than 90 percent of all stars

nebula

A large cloud of dust and gas in space

protostar

A contracting cloud of gas and dust; the earliest stage of a star's life

white dwarf

A small, hot, dim star that is the leftover center of an old star

supernova

A gigantic explosion in which a massive star collapses and throws its outer layers into space

neutron star

the small, dense remains of a high-mass star after a supernova

black hole

An object in space whose gravity is so strong not even light can escape.

binary stars

when only two stars are gravitationally bound together and orbit a common center of mass

eclipsing binary

A binary star system in which one star periodically blocks the light from the other.

open cluster

a star cluster that has a loose, disorganized appearance and contains no more than a few thousand stars

globular cluster

a large, round, densely-packed grouping of older stars

spiral galaxy

a galaxy with a bulge in the middle and arms that spiral outward in a pinwheel pattern

elliptical galaxy

A galaxy shaped like a round or flattened ball, generally containing only old stars

irregular galaxy

A galaxy that does not have a regular shape

quasar

An enormously bright, distant galaxy with a giant black hole at its center

universe

All of space and everything in it

scientific notation

A method of writing or displaying numbers in terms of a decimal number between 1 and 10 multiplied by a power of 10.

big bang

(cosmology) the theory that the universe originated 20 billion years ago from the cataclysmic explosion of a small mass of matter at extremely high density and temperature

Hubble's Law

proves that the universe is expanding. The farther a galaxy is, the faster it moves away from us. V = H x d

cosmic background radiation

The electromagnetic radiation left over from the big bang

solar nebula

the cloud of gas and dust that formed our solar system

planetesimals

Small planetary objects that form through the action of gravity during the birth of a solar system

dark matter

Matter that does not give off electromagnetic radiation

dark energy

A mysterious force that appears to be causing the expansion of the universe to accelerate