Galactic Baby Boomers
Two of NASA’s Great Observatories , bolstered by the largest ground-based telescopes around the world, are beginning to harvest new clues to the origin and evolution of the universe’s largest building block, the galaxies. It’s a bit like finding a family scrapbook containing snapshots that capture the lives of family members from infancy through adolescence to adulthood.
|Seeing backwards to the beginning. Credit: NASA/STScI|
"This is the first time that the cosmic tale of how galaxies build themselves has been traced reliably to such early times in the universe’s life," says Mauro Giavalisco, head of the Hubble Space Telescope portion of the survey, and research astronomer at the Space Telescope Science Institute (STScI) in Baltimore, Md.
So far, the Hubble Space Telescope has joined forces with the Chandra X-ray Observatory to survey a relatively broad swath of sky encompassing tens of thousands of galaxies stretching far back into time. This unprecedented survey will soon be joined by the Space Infrared Telescope Facility (SIRTF), which is to be launched in August 2003.
Called the Great Observatories Origins Deep Survey (GOODS), astronomers are studying galaxy formation and evolution over a wide range of distances and ages. The project is tracing the assembly history of galaxies, the evolution of their stellar populations, and the gusher of energy from star formation and active nuclei powered by immense black holes.
Deepest Field Gets Deeper
In preliminary results soon to be published in the Astrophysical Journal, Hubble astronomers report that the sizes of galaxies clearly increase continuously from the time the universe was about 1 billion years old to an age of 6 billion years. (This is approximately at half the current age of the universe, 13.7 billion years.) GOODS astronomers also find that the star birth rate rose mildly (by about a factor 3) between the time the universe was about one billion years old and 1.5 billion years old, and remained high until about 7 billion years ago, when it quickly dropped to one-tenth the earlier "baby boomer" rate. This is further evidence that major galaxy building trailed off when the universe was about half its current age.
This increase in galaxy size is consistent with "bottom-up" models, where galaxies grow hierarchically, through mergers and accretion of smaller satellite galaxies. This is also consistent with the idea that the sizes of galaxies match hand-in-glove to a certain fraction of the sizes of their dark-matter halos. Dark matter is an invisible form of mass that comprises most of the matter in the universe. The theory is that dark matter essentially pooled into gravitational "puddles" in the early universe that then collected normal gas that quickly contracted to build star clusters and small galaxies. These dwarf galaxies merged piece-by-piece over billions of years to build the immense spiral and elliptical galaxies we see today.
|The Universe is much more than what meets the eye. Credit: NASA/WMAP|
The Chandra observations amounted to a " high-energy core sample " of the early universe, allowing us to "study the history of black holes over almost the entire age of the universe," said Niel Brandt of Penn State University, a co-investigator on the Chandra GOODS team, who studied the X-ray results. One of the fascinating findings in this deepest X-ray image ever taken is the discovery of mysterious black holes, which have no optical counterparts.
"We found seven mysterious sources that are completely invisible in the optical with Hubble," said Anton Koekemoer of the STScI, a co-investigator on both the Hubble and Chandra GOODS teams, who compared the X-ray and optical reslts. "Either they are the most distant black holes ever detected, or they are less distant black holes that are the most dust enshrouded known, a surprising result as well."
When comparing the Hubble and Chandra fields, astronomers also found that active black holes in distant, relatively small galaxies were rarer than expected. This may be due to the effects of early generations of massive stars that exploded as supernovae, evacuating galactic gas and thus reducing the supply of gas needed to feed a supermassive black hole.
In mid-August, NASA will launch the Space Infrared Telescope Facility (SIRTF) the fourth and final element in the family of Great Observatories. Each observatory examines the heavens in a different electromagnetic spectrum . Because they are space borne telescopes, orbiting above the distorting atmosphere of the Earth, they are able to gain unprecedented views of the universe. The most famous is the Hubble Space Telescope, the visible light telescope, and it is expected to operate until 2010. The Compton Observatory , launched in 1991, examined gamma rays until its mission ended in 1999. The Chandra Observatory , launched in 1999, examines X-rays and is scheduled to operate through 2004.
Like the Hubble Space Telescope , SIRTF has large mirrors that will provide unprecedented views of the universe . But while Hubble is mainly a visible-light telescope, SIRTF will detect infrared light. In other words, SIRTF will be hunting for heat.
That’s why SIRTF’s position in space will be very different from Hubble’s orbit around the Earth. SIRTF won’t circle the Earth at all – instead it will circle the sun . The observatory will tailgate the Earth, following a few million miles behind our planet in the same solar orbit. Infrared light can also be used to study cooler objects in space, such as brown dwarfs , asteroids , and comets .
These and other results from the GOODS project will be published in a special issue of the Astrophysical Journal Letters, entirely devoted to the team’s results. The Chandra results are found in papers led by Koekemoer and Stefano Cristiani of the Trieste Astronomical Observatory. Hubble’s findings came from papers led by Giavalisco, Mark Dickinson, and Harry Ferguson of the STScI.