final Flashcards
which scientist discovered that the equations he had derived predicted an expanding universe, then modified his equations to eliminate this expansion?
Albert Einstein
what do cosmologists study
origin, structure and evolution of the universe
why is the universe expanding
spacetime itself is expanding, carrying the galaxies (superclusters of galaxies) with it.
which on of the following statements is a correct description of the expansion of the universe
spacetime is something real, with galaxies inside it; as spacetime expands, the galaxies( or superclusters of galaxies) are carried along by the expansion
what is the cosmological redshift
stretching of the wavelengths of photons as they travel through expanding space
the cosmological redshift of the light from very distant galaxies is caused by the
expansion of space, stretching the photon’s wavelength while the photon is traveling toward earth
what is it that keeps localized regions of space, such as things on earth, planetary systems, star clusters, and whole galaxies, from participating in the general expansion of the universe?
mutual gravitational attraction between objects in these systems
what is the cosmic microwave background radiation?
radiation left over from the Big Bang after the universe expanded and cooled
the cosmic background radiation is
low intensity radio noise, with a 3K blackbody temperature, almost uniform in intensity in all directions.
the cosmic background radiation is the
electromagnetic remnants of the explosion in which the universe was born.
good evidence for an original Big Bang that “created” our universe comes from
a background “glow” of microwaves, with blackbody temperature of about 3k
in relation to the universe, what does isotropy mean
the universe looks the same in all directions
what do we mean when we say that the universe is homogeneous
at any given time, the universe looks the same at all locations
how many fundamental forces are there in nature at the present time under normal conditons
four: strong, weak, electromagnetic and gravitational
what is the range of the electromagnetic force (the maximum distance over which it acts?
infinity
which is the four fundamental forces holds the electrons in the atom/
electromagnetic force
what is the gravitational force ( the maximum distance over which it acts)
infinity
what makes gravity the main force determining the large scale structure of the universe
while the electromagnetic force of a charged particle has an infinite range, it is usually screened and limited by the existence of charges of the opposite sign. Ordinary matter has only one sign and therefore does not screen other gravitational forces.
what are quarks
component particles making up protons and neutrons
what are the particles that make up protons and neutrons
quarks
most quasar produce their strongest emissions in which region of the electromagnetic spectrum
infrared
what is the most outstanding feature of a quasar compared with other objects in deep space
prodigious output of energy
quasars in our universe are
relatively common. Over 10000 have been identified so far
quasars all appear to be
moving away from us at very high speeds, up to about 90 of the speed of light
the specific characteristics that identify most quasars are
bright, starlike appearance with very high redshifts and hence very large distances indicating very energetic sources.
an intense radio source is found to coincide with a starlike object whose spectrum contains a pattern of intense emission lines in in the visible range that matches that of the Lyman uv hydrogen spectral lines but is very redshifted. what is this object
quasars
the extreme redshifts of quasar spectra are caused by
very high recession speeds of the sources away from the Milky Way galaxy
compared with the total output of energy from the Milky Way galaxy, what is the equivalent output of a typical quasar?
100 times brighter
seyfert galaxies are
active galaxies with bright starlike nuclei
seyfert galaxies are a distinct class of galaxies because they
have very bright, very hot starlike central cores with variable energy output