click below
click below
Normal Size Small Size show me how
Astronomy part 2
| Term | Definition |
|---|---|
| photosphere | luminous visble surface of sun, shallow layer of strong ionized gases |
| chromosphere | gaseous envelope surrounding a star (on the sun: outside of photosphere) |
| corona | faintly luminous envelope outside of sun's chromosphere, inner part made of highly ionized elements |
| solar wind | emanation from sun's corona, flow of charged particles, interacts with magnetic field of earth and other planetry bodies |
| sunspot | dark patch appears periodically on the surface of the sun, affects terrestrial magnetism and other phenomena |
| prominence | flamelike eruption of relatively cool, high-density gas from sun's chromosphere into corona |
| solar flare | sudden burst or flame |
| aurora | radiant emission from upper atmosphere happens sporadically over middle and high of both hemispheres looks like limunous bands |
| nuclear fusion | reaction in the nucleaus of light atoms formed to make a heavier atom |
| constellation | any group of stars to which a name has been given |
| binary star | two stars that revolve about their common center of mass |
| light year | unit of astronomical distance equivalent to distance that light travels in 1 year |
| apparent magnitude | how an observor on earth sees the magnitude of a star |
| absolute magnitude | how a hypothetical observer would view the magnitude of a star (viewer is light years away) |
| main sequence star | stary laying on a diagonal band that extends from hot stars to cool stars |
| red giant | star in intermediate stage of evolution, large volume, low surface temperature, reddish hue |
| supergiant | star whose diameter is more than 100 times the size of the sun's, extremely bright |
| cepheid variable | variable star, changes in brightness are due to alternate contractions and volume changes |
| nova | a star that suddenly becomes 100 times brighter and then fades back to its original intensity |
| nebulae | a cloud on intersellar gas and dust |
| hertzsprung russell diagram | graph showing absolute magnitude plotted against surface temperature for stars |
| protostar | early stage in evolution of star |
| supernova | explosion of star |
| white dwarf | star about the size of earth, has underagone gravitational collapse and is in final stage of evolution for low mass stars |
| neutron star | extremely dense compact star, primarly made of neutrons |
| pulsar | one of several hundred celestial bodies, rapidly rotating neutron stars, emit pulses of radiation, |
| black hole | theoretical massive object at beginning of universe |
| galaxy | system of stars held together by mutual gravitation, isolated from similar systems |
| hubble's law | velocity of recession of distant galaxies from our own is proportional to their distance from us |
| big bang theory | a theory that deduces a cataclysmic birth of the universe |