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E.S. Chapter 30
Question | Answer |
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chromosphere | layer of the Sun's atmosphere above the photosphere. Usually only visible during a solar eclipse. |
corona | top layer of the Sun's atmosphere. Extends several million km from the chronosphere . Has temperatures ranging from 1 -2 million K. |
fission | splitting of heavy atomic nuclei into smaller, lighter atomic nuclei. Occurs on Earth |
fusion | combining of lightweight atomic nuclei into heavier nuclei. Occurs on the sun, not on earth. |
photosphere | lowest layer of the Sun's atmosphere. The visible surface of the sun. Most of the light from the sun comes from here. |
prominence | Arc of gas ejected from the chromosphere. Associated with sunspots. |
solar flare | violent eruptions from the Sun's surface. Associated with sunspots. Often leave the surface of the sun and are part of the solar winds that can affect Earth. |
solar wind | Charged particles (ions) that leave the sun's corona at great speeds to travel through the solar system. |
sunspot | Dark spots found on the surface of the photosphere associated with cooler regions on the Sun's surface. Located in spots where the sun's magnetic field pokes through the photosphere. |
absolute magnitude | Brightness an object appears at 10 parsecs from Earth. Lower the number the brighter the star |
apparent magnitude | How bright a star appears to be. From the early Greeks. Lower the number the brighter the star. |
binary star | Two stars gravitationally bound and orbit a common center of mass. |
constellation | Grouping of stars, Could be animals, common objects, mythological characters. |
H-R diagram | Hertzsprung-Russell Diagram. Demonstrates mass, luminosity, temperature and diameter of stars as they relate to each other. |
luminosity | energy out put of a star per second. |
main sequence | About 90% of all stars. Run from the upper left corner to the lower right corner of an H-R diagram. |
parallax | An apparent shift in position of a star due to the shift in position of the observer. |
black hole | Small, extremely dense object that is left after a large star collapses. Because of its gravity, not even light can escape. Perhaps found in the center of galaxies. |
nebula | cloud of dust and gas between the stars (interstellar) |
neutron star | Occurs after the collapse of a star. Neutron's resistance to being squeezed halts the collapse of the core. Incredible density. 1 t = a ton. |
protostar | Disk shape that forms in the center of a nebula that will become a new star. |
supernova | Huge explosion created as a star is falling inward. Creates elements heavier than iron and enriches the universe. |