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AS101 Final
key words to know
| Question | Answer |
|---|---|
| absolute luminosity | the total amount of light that an object puts out per second. |
| amplitude | the height of a wave above its undisturbed state. |
| apparent luminosity | the amount of light that an observer sees at their distance from an object. |
| astronomical unit (AU) | the average distance of the Earth from the Sun. |
| cepheid variable | a variable star that cycles from brighter to dimmer and back again with a regular pattern that is related to the stars absolute luminosity. |
| dark matter | material that is difficult to see outside the universe but whose gravitational effects are obvious. EX: black wholes,dust, red dwarfs. |
| doppler effect | observed wavelengths seen by an observer change as the observer moves toward or away from a source of light. toward=shorter away=longer |
| electromagnetism | 1 out of 4 forces in the universe. holds atoms together. produces light in the form of photons |
| electron | a negatively charged particle that orbits the nucleus of an atom. |
| falsified | when the prediction of a hypotheses does NOT match the experimental results |
| flux | the amount of light crossing an observer per second per unit area from some light source |
| frequency | the number of cycles a wave completes per second. |
| Galileo | Italian math professor who used the telescope to show that the heliocentric model was indeed true |
| geocentrism | idea that the earth is the center of the universe and that the sun and the planets orbit the earth. |
| gravity | 1 out of 4 forces. objects with mass attract one another with a force that depends on the inverse of the square of the distance between the two objects |
| heliocentrism | presented by copernicus, that the earth was like the rest of the planets and orbited the sun |
| edwin hubble | american astronomer discovered universe was bigger than the milky way. showed the universe was expanding |
| hubbles law | galaxies that are farther away appear to be moving away from earth faster than galaxies that are closer. |
| hypothesis | an idea of some feature of nature works that also makes a prediction of some testable measurement related to the explanation. |
| johann kepler | german minister who was a mathematician. worked out proof the planets orbit the sun in elliptical orbits. |
| light year | distance light travels in one year |
| isaac newton | english math professor who invented calculus. |
| neutron | neutral particle in the center of an atom. |
| nucleus | center of an atom that contains protons, neutrons. |
| parallax | observation that the apparent position of a distant object changes depending upon where the observer is. |
| parsec | distance required for a star to produce a parallax angle of 1 arc second with the earth have a baseline of 1 AU |
| period | length of time to complete one cycle of a wave |
| photon | a particle of light. all of them have the same speed, but can have different energy, frequency,or wavelength. NO MASS |
| proton | positively charged particle at the center of an atom |
| speed of light | instantaneous speed of light is 3 x 10^8 m/s |
| standard candle | object out in space with a known absolute luminosity. |
| strong force | 1 out of 4 forces. this one holds nuclei of atoms together |
| theory | a well verified hypothesis |
| type 1A supernova | a pair of stars that go through a sequence of dying. first star becomes a white dwarf then draws matter off of the second star. white dwarf explodes |
| type 2 supervova | enormous star that explodes with bright explostion when it dies. mot a standard candle. after the explosion it becomes a neutron star or a stellar sized black hole |
| verified | when a prediction of a hypothesis matches the results |
| wavelength | the physical length of one complete cycle of a wave |
| weak force | 1 out of the 4 forces. responsible for allowing particles to change identity from one type to another. |