True ZITs: can such things be?True ZITs: Can such things be? When observers discovered the cosmicbackground of microwave radio radiation 20 years ago, they were happy with its apparent smooth isotropy isotropy the quality or condition of being isotropic. . In any direction they looked, they saw radiation of the same temperature, and that was good because they believed that the universe was homogenous homogenous - homogeneous and isotropic Refers to properties that do not differ no matter which direction is measured. For example, an isotropic antenna radiates almost the same power in all directions. In practice, antennas cannot be 100% isotropic. , and so the microwave background, which comes down to undisturbed from early times, should have been smooth. Now, observers would like to find minutefluctuations in the temperature of the background radiation. If they don't eventually find them, a good deal of present cosmological theory will go overboard. The good news is that scientists havereported three measurements that could be one sort of the desired anisotropies. More work is necessary to find out if they are the real things, but one of the experts in the field, David Wilkinson of Princeton (N.J.) University, comments: "It smells as though we're getting close to anisotropy anisotropy /an·isot·ro·py/ (an?i-sot´rah-pe) the quality of being anisotropic. anisotropy (an´āsôt´r , close to a real detection." In general, observers distinguish threesize scales of temperature fluctuation in the background radiation. One refers to the present time, and two refer to distant epochs in the past. The large scale covers an area in the sky 90[deg.] across of greater, with the background slightly warmer over the area of that size and slightly cooler over another. This scale refers to the present time, and an anisotropy on this scale, the "dipole anisotropy," has been known for several years. Astronomers take it as the result of a motion of our galaxy toward the galaxies in the Virgo cluster. The smallest scale, fluctuationsaround a minute of arc in extent, would result from fluctuations in the density of matter in the universe that occured at the very beginning and might have been the seed around which galaxies and clusters of galaxies formed. No hint of these has been seen. The present tentative results concernthe middle range, areas a few degrees across. At the recent 13th Texas Symposium on Relativistic rel·a·tiv·is·tic adj. 1. Of or relating to relativism. 2. Physics a. Of, relating to, or resulting from speeds approaching the speed of light: relativistic increase in mass. Astrophysics held in Chicago, three groups reported apparent fluctuations of temperature in areas 5[deg.] or 8[deg.] across. They are Edward Fomalont and Kenneth I. Kellermann of the National Radio Astronomy Observatory National Radio Astronomy Observatory (NRAO), federal observatory for radio astronomy, founded in 1956 and operated under contract with the National Science Foundation by Associated Universities, Inc., a group of major universities. in Charlottesville, Va., who worked with the Very Large Array (VLA VLA abbr. Very Large Array ) of radiotelescopes near Socorro, N.M.; Bruce Partridge of Haverford (Pa.) College, who also worked with the VLA; and Rod Davies of the Nuffield Radio Astronomy Laboratories Nuffield Radio Astronomy Laboratories: see Jodrell Bank Observatory. in Jodrell Bank, England, and Anthony Lasonby of Cambridge University, both working with an antenna in the Canary Islands. Typical of what these groups find is atemperature variation of 5 parts in 100,000 over an area of 8[deg.] in the sky. Mapped with false colors to indicate temperature differences, such a pattern looks like acne, and so some of the scientists involved call this the ZIT model. The ZITs refer to an interesting time, ascosmologists describe it, back at a red-shift of 1,000. (For comparison, the most distant and oldest quasars we can see have redshifts around 4.) Wilkinson translates a redshift redshift Displacement of the spectrum of an astronomical object toward longer wavelengths (visible light shifts toward the red end of the spectrum). In 1929 Edwin Hubble reported that distant galaxies had redshifts proportionate to their distances (see of 1,000 as when the universe was 100,000 years old (compared with a present age between 10 billion and 20 billion years). The ZITs thus refer to fluctuations in the famous cold, dark matter that seems to pervade per·vade tr.v. per·vad·ed, per·vad·ing, per·vades To be present throughout; permeate. See Synonyms at charge. [Latin perv the universe and may be enough to close it. They also refer to regions that in earlier times had developed out of contact with each other and were then beginning to overlap each other. In the earliest days of the universe, twodifferent expansions were concurrently going on. These were the expansion of space -- that is, of the universe itself -- and the expansion of our (or any observer's) horizon. Astrophysicist David Schramm of the University of Chicago says that people may deceive themselves if they imagine the Big Bang as a kind of explosion. He prefers to use the analogy of raisin-bread dough. As the dough rises, it expands everywhere fairly evenly. As a result, the raisins are carried farther and farther from each other, even though they do not move with respect to the dough right around them. Galaxies, like the raisins, are carried farther and farther from each other as the space between them (like the dough) expands, but they do not necessarily move with respect to the space right around them. Meanwhile our horizon is expanding,too. At any time we can see only the objects from which light has had time to get to us since the beginning of the universe. If we could have been around when the cosmos was 1 second old, we would have seen only objects less than 1 light-second away, not as far as the moon now is. As time goes on, each observer sees objects farther and farther away. Horizons expand at the speed of light; space expands presumably pre·sum·a·ble adj. That can be presumed or taken for granted; reasonable as a supposition: presumable causes of the disaster. at a different speed. Expanding horizons may gradually gain on the expansion of space, or they may not. It is not clear how big the universe wasat time zero, though it seems to have been extremely smaller than it is now. However, in the earliest moments, a number of regions could have developed independently of one another, because their horizons did not overlap and they could not communicate and so could not affect events in each other. Eventually horizons began to overlap. Each observer began to see regions that had developed independently of his or her own immediate surroundings. The differences between them should show up as minute variations in the equilibrium temperature of the cosmic microwave background Noun 1. cosmic microwave background - (cosmology) the cooled remnant of the hot big bang that fills the entire universe and can be observed today with an average temperature of about 2. , on the order of 1 part in 1,000 or less. Such phenomena should produce the ZITs. Are the reported observations reallyZITs? Wilkinson cautions that they could be galactic bremsstrahlung bremsstrahlung (brĕm`shträ'ləng): see X ray. bremsstrahlung (German; “braking radiation”) , radiation produced by galaxies moving through the intergalactic in·ter·ga·lac·tic adj. Being or occurring between galaxies: intergalactic space. in gas. Spectra will tell the difference: True ZITs will have the blackbody blackbody Theoretical surface that absorbs all radiant energy that falls on it, and radiates electromagnetic energy at all frequencies, from radio waves to gamma rays, with an intensity distribution dependent on its temperature. spectrum characteristic of the cosmic microwave background. The present observations are all at single frequencies, because radiotelescopes observe one frequency at a time. Astronomers are now planning to look at other frequencies to see whether they can fill in the proper spectra. |
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