Quasars: the brightest and the farthest.Astronomers have discovered the most brilliant known object in the universe. The luminosity luminosity, in astronomy, the rate at which energy of all types is radiated by an object in all directions. A star's luminosity depends on its size and its temperature, varying as the square of the radius and the fourth power of the absolute surface temperature. of this celestial power-house--a quasar quasar (kwā`sär), one of a class of blue celestial objects having the appearance of stars when viewed through a telescope and currently believed to be the most distant and most luminous objects in the universe; the name is shortened from glowing with the brightness of more than [10.sup.15] suns--exceeds by 25 percent that of the two previous record-holding quasars Proper naming of quasars are by Catalogue Entry, Qxxxx±yy using B1950 coordinates, or QSO Jxxxx±yyyy using J2000 coordinates. This page lists quasars.
The quasar's light, which takes 12 billion years to reach Earth, enables researchers to peer back in time to shortly after the Big Bang big bang Model of the origin of the universe, which holds that it emerged from a state of extremely high temperature and density in an explosive expansion 10 billion–15 billion years ago. . The brilliance of this light also makes it easier to examine the galaxies and hydrogen gas clouds lying between the quasar and Earth, says Richard McMahon of the University of Cambridge in England. In fact, he notes, a telltale absorption of blue light by hydrogen helped him and his colleagues to identify the ultrabright quasar. McMahon, working with Michael Irwin Michael Henry Knox Irwin (5 June 1931 - ) is a retired GP and former medical director of the United Nations. He is a humanist and secularist activist and a campaigner for voluntary euthanasia. of the Royal Greenwich Observatory Royal Greenwich Observatory, astronomical observatory established in 1675 by Charles II of England; formerly known as the Royal Observatory and located at Greenwich, it moved to Herstmonceux Castle, Sussex, in 1946. In the 1990 new headquarters at Cambridge Univ. in Cambridge and Cyril Hazard of the University of Pittsburgh, computer-scanned some 25 million celestial objects depicted on photographic plates from the U.K. Schmidt Telescope Schmidt telescope: see telescope. in Epping, Australia Epping, Australia may refer to one of these suburbs:
The quasar's luminosity and distance may pose new problems for the "cold-dark-matter" theory of galaxy formation (SN: 1/26/91, p.52), McMahon says. The simplest version of this popular theory suggests that fluctuations in the density of primordial matter could not have grown fast enough to form most galaxies soon after the Big Bang. But most cosmologists contend that quasars, thought to lie at the center of some galaxies, form only after galaxies emerge. In addition, black holes or other quasar-fueling objects inside galactic cores would need time to evolve--particularly the more massive power sources required by the brightest quasars. Thus, the extreme features of BR 1202-07 indicate that some galaxies must have existed when the universe was only 7 percent of its current age--during the first billion or so years of its existence, according to some estimates. The cold-dark-matter theory cannot easily explain such an early origin, McMahon says. Another recent quasar discovery, widely discussed among astronomers but not yet publicly announced, may also strain the theory of cold dark matter, several scientists say. Using the 5-meter telescope at Palomar Observatory near Escondido, Calif., James E. Gunn
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 about 4.9 indicates the object dates to a time when the universe was about 6.7 percent of its current age. "It's a consensus finding," says McMahon, noting that the two discoveries may pose similar challenges to the cold-dark-matter theory. Gunn told SCIENCE NEWS he would not disclose details of the work until his team announces the results. He cautions that the handful of distant quasars so far observed cannot overturn -- or even force major alterations in -- accepted cosmological theories, which rely largely on statistical arguments. "As long as one has just one or two other [very distant] objects, as we do at the moment, it is very hard to make quantitative statements that will get theories in trouble," says Gunn. He notes, however, that several proposed scenarios for the evolution of the universe would have difficulty accounting for the presence of many distant quasars. McMahon adds that if the search for faraway quasars ever reveals a distance limit, it may indicate when galaxies first turned on and quasars first shined. |
|
||||||||||||||||||

Printer friendly
Cite/link
Email
Feedback
Reader Opinion