A | B |
Electromagnetic Spectrum | a way of organizing all types of light waves according to frequency |
Galaxy Cluster | a system of galaxies containing from several to thousands of member galaxies |
Doppler Effect | describes how wavelength changes as the source moves toward or away from the observer |
Sun | an average sized star that is the source of all energy on our planet |
Apparent Magnitude | the brightness of a star as viewed from Earth |
Galaxy | a collection of stars, dust, and gasses held together by gravity |
Milky Way | our galaxy |
Nebula | a cloud of dust and gases in which stars form |
Protostar | a developing star not yet hot enough to perform nuclear fusion |
Main Sequence | where stars spend 90% of their lives |
Red Giant | a large, cool, bright star that is found in the upper right corner of the HR diagram |
Super Giant | what very large stars become after they run out of hydrogen fuel |
Supernova | an exploding star that increases in brightness several times |
Black Hole | a massive star that has collapsed to such a small volume that its gravity prevents the escape of everything, including light |
Neutron Star | a star of extremely high density composed entirely of neutrons |
Pulsar | a spinning neutron star |
Big Bang | theory that explains the origin of the universe |
Cosmic Background Radiation | low frequency EM radiation that is thought to be leftover from the Big Bang |
Reflecting | a telescopes that uses large mirrors to focus visible light into an image |
Gamma Ray | highest frequency EM radiation; used in chemotherapy |
X Ray | invisible EM radiation that is used in medical imaging |
Visible Light | all the color of the rainbow - ROY G BIV! |
Wavelength | distance between two adjacent wave crests |
Frequency | the number of wave crests that pass a certain point in a certain time |
Period | the time it takes for a wave to complete one wave cycle; the inverse of the frequency |
Amplitude | how "big" a wave is; distance from midpoint to a wave crest or trough |
Binary Star | one of two stars revolving around a common center of mass because of their mutual gravitational attraction |
Solar Flare | a sudden and tremendous explosion in the solar atmosphere |
Absorption Spectrum | also known as a dark-line spectrum; created when white light is passed through a cool gas |
Emission Spectrum | also known as a bright-line spectrum; created by a hot glowing gas |
Continuous Spectrum | spectrum that shows all the colors of the rainbow; created when white light is passed through a prism |
Hertzsprung-Russell Diagram | diagram that shows the relationship between stars' temperature and brightness |
Microwave | low frequency, invisible EM radiation; used for communications and cooking |
Infrared Radiation | EM radiation just outside the visible range; heat energy |
Core | layer of the sun in which nuclear fusion occurs |
Radiation Zone | layer of the sun in which energy moves out from the core |
Convection Zone | layer of the sun in which matter moves in density cycles |
Photosphere | layer of the sun that we can see; brightest layer |
Chromosphere | layer of the sun only visible during a solar eclipse; named for the red color that helium produces |
Solar Prominence | a concentration of gases above the solar surface that appears as a bright archlike structure |
Corona | the weak outer layer of the solar atmosphere; only visible during a solar eclipse |
Sunspot | a large dark spot on the sun; cool relative to the surrounding bright areas; caused by interference of convection cycles by sun's magnetic field |
Granulation | speckled appearance of the sun's photosphere; caused by convection currents |
Aurora Borealis | colored light show caused by charged particles in the solar wind interacting with atoms in the Earth's atmosphere |
Solar Wind | streams of charged particles ejected at high speeds from the solar corona |
Solar Eclipse | occurs when the moon moves in a line directly between Earth and the sun, casting a shadow on the Earth |