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43 Cards in this Set
- Front
- Back
dark energy
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mysterious energy that seems to cause the acceleration of expansion of the universe
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cosmic microwave background
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radiation coming from all the directions in space as a consequence of the big bang
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dark matter
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mysterious unseen matter that accounts for about 23% of the mass of the universe
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cosmology
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the branch of astronomy that studies the structure and evolution of the universe
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Hubble's Law
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the greater the recessional velocity of a galaxy, the farther away it is
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big bang
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astronomer's theory to origin of universe, the model says the universe was condense and hot billions of years ago, and has been expanding and cooling ever since
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3 sources of evidence for big bang theory
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cosmological redshift, cosmic microwave background radiation, 3:1 ratio of hydrogen to helium in universe
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age of universe
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13.7 billion years
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Quasars
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short for "quasi-stellar radio sources, believed to be cores of galaxies that were formed when universe was young, extreme source of radio waves, the most distant object in universe
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barred spiral galaxy
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spiral galaxy with two broad bars extending from opposite sides of central bulge, the spirals arms extend from ends to bars
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normal sprial galaxy
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galaxy with a disk shape, central bulge and curved spiral arms
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irregular galaxy
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galaxy with no regular shape
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elliptical galaxy
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galaxy with an elliptical shape
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local group
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the 40 or so galaxies which the milky way is a member
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Universe
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the totality of all matter, energy, and space
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Galaxy
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an extremely large collection of stars
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Globular clusters
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a halo of about 200 of these surround the milky way, each consist of 10,000 stars
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Milky way galaxy
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galaxy which contains our solar system, a spiral galaxy with massive black hole at its center
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proton-proton chain
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the series of three reactions by which hydrogen is fused into helium in the sun
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age of our sun
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5 billion yrs
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photosphere
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the bright, visible surface of the sun, temp is 6,000 K
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Core of Sun
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interior of sun were nuclear reactions convert hydrogen to helium and energy core temp. is 15 mil. degrees K
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Solar wind
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charged particles that stream out into space from the sun, the solar wind fills a vol. of space outwards to a distance of 50 AU and is called the heliosphere
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corona
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Sun's most outer layer, the origin of the solar wind
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Chromosphere
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layer of sun above the photosphere, temp 50,000 k
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prominences
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enormous filaments of excited gas that arch over and return to the Sun's surface
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flares
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material explosively ejected in space from sun's surface
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sunspots
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dark patches of cooler material on the surface of the sun, the number of sunspots varies over an 11 year cycle, in 1600s the # of sunspots was fewer and the experience a mini ice age
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nucleosynthesis
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The creation of nuclei of elements inside stars
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event horizon
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boundary around a black hole from which no matter or radiation can escape from
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Schwarzschild radius
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distance from black hole's singularity to its event horizon
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event horizon
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boundary around a black hole from which no matter or radiation can escape from
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singularity
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extremely dense point at center of a black hole
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black hole
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an object so dense that not even light can escape its gravity
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pulsar
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fast rotating neutron star that radiates radio waves in a rotating pattern
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neutron star
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a super dense star of which pulsars are one type
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supernova
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the most catastrophic explosion of a high-mass star, the end results are either a neutron star or a black hole
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nova
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relative small nuclear explosion on the surface of a white dwarf
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white dwarfs
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hot, small, very dim stars formed at the end of low-mas star's lives
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planetary nebulae
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a shell of material ejected from a variable star late in its life
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protostar
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name given to condensed nebula before it becomes a star
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brown dwarfs
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failed stars
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nebulae
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cool, dense clouds of gas and dust in space.
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