NASA Hosts Conference on Advances in Aeronautics & Access to Space
 The Turning Goals into Reality Conference, May 18-19 at NASA's Marshall Space Flight Center in Huntsville, AL, is an opportunity for NASA and its industry partners to acknowledge major technological advances in the aeronautics and space access. NASA managers and other government leaders will participate in discussions about the impact of technology in such areas as global civil aviation, advanced space launch, and revolutionary aviation mobility. Awards for technology development leaders and technology status briefings, demonstrations, and tours of the Marshall Center are included. For information or to register follow the link.
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At first appearance, quasars appear to be stars. On closer inspection, it is found that their redshift of their emitted light is great enough to place them as the most distant objects in the universe. For them to be visible at such distances, they have to be very bright and highly energetic, far more so than any star known, so they have been dubbed quasi-stellar objects.
The spectrum emitted by quasars shows that they are travelling incredibly fast away from us. On standard assumptions, then, they are some of the oldest objects that we can see.
Today the nature of quasars is not yet understood, and they are a dynamic area of research.
For more information on quasars, see
Bill Keel's WWW Gallery - Active Galaxies and Quasars
Quasars from Lake Afton Public Observatory
Quasars: "The Light Fantastic"
QUASARS: "THE LIGHT FANTASTIC"
Quasars have been so elusive and mysterious that the hunt to define them would have taxed even the superior analytical skills of detective Sherlock Holmes.
Since their discovery in 1963, astronomers have been trying to crack the mystery of how these compact dynamos of light, which lie at the outer reaches of the universe, produce so much energy. Quasars are no larger than our solar system but outshine galaxies of hundreds of billions of stars. These light beacons have left trails of evidence and plenty of clues, but scientists have only just begun to understand their behavior.
For centuries, quasars went undetected, appearing in the sky as faint stars. No one suspected anything more. In the 1940s, however, radio scientists discovered that celestial objects emitted radio waves, giving birth to radio astronomy.
Soon astronomers began examining the sky to find as many objects as possible that radiated radio waves and tried to link them to optical objects. Their search led to several radio sources whose positions coincided with blue starlike objects.
Astronomers Allan Sandage and Thomas Matthews attempted to uncloak these mysterious objects in 1960. They were puzzled to find a strange source of radio emission that, in visible light, looked like a faint star. But this object was emitting more intense radio waves and ultraviolet radiation than a typical star.
In 1962 British radio astronomer Cyril Hazard took a crack at solving the mystery. He had an ingenious method of using the moon as a marker to pinpoint a radio source. When the moonwould pass in front of a particular radio source (called an occultation), he noted the precise instant the radio signal stopped and then reemerged.
But he almost didn't get the opportunity to record the information. Hazard was at the University of Sydney and had arranged to make the observation at Parkes Radio Telescope, located several hundred miles away in the Australian outback. The night the occultation occurred, Hazard took the wrong train and missed the observation. Luckily, observatory director John Bolton and other astronomers made the observation. But Bolton also had his own problems. He couldn't tip the telescope over far enough to record the observation. So, he cut down a bunch of trees. Then he removed the telescope's safety bolts and tilted the several thousand ton telescope over enough to catch the occultation.
The astronomers observed a radio source that could be traced to a single starlike object, then known as 3C 273, in the constellation Virgo. Although this object looked like an ordinary star, it exhibited peculiar behavior. The object was emitting a tremendous quantity of radio signals. An optical analysis of the object's spectrum was unlike anything previously encountered.
What was it? In 1963 Maarten Schmidt at Mount Palomar observatory deciphered the code. The spectrum contained a few strange wide emission lines, which at first seemed pretty confusing. Schmidt soon realized he was looking at normal spectral lines for hydrogen. The lines, however, were shifted toward the red end of the visible spectrum, making them almost unrecognizable. There was only one explanation: This object was receding away from Earth at almost 30,000 miles per second, which meant that it was 3 billion light-years away. Astronomers quickly dubbed the objects quasi-stellar radio sources.
"Once Maarten Schmidt cracked the safe, all of a sudden things began to fall into place," says John Bahcall, who was a young physics professor at Caltech when Schmidt made his discovery.
Now the hunt was on to define these objects. How were they formed? What fueled them? Do they reside in galaxies? How can such tiny objects only a few light-months across emit so much radiation?
"Hunting for quasars became a major sport," says astronomer Mike Disney, who decided to become an astronomer after reading a story about the discovery of quasars. "It was an exciting thing. Clearly, it was a new physical phenomenon."
Astronomers rushed to discover more of these objects. Since then, thousands of them have been identified. Sandage found quasars that don't emit any radio waves. These "radio quiet" quasars now comprise about 99 percent of the population.
Theories also abounded about the nature of these objects. One theory questioned the definition of red shift, the measure of an object's recession velocity. The farther away an object is, the longer and hence redder the wavelength. Maybe quasars - which had high red shifts because they were far away - weren't so far away. Perhaps red shift is a measure of something else. But most astronomers quickly rejected this theory.
Russian scientist Yakov Zeldovich proposed yet another theory, which astronomers still believe today: Black holes provide the power that turns on quasars. A black hole is created when a giant star collapses to a tiny point of infinite density. Astronomers believe that a quasar turns on when a black hole at a galaxy's core feeds on gas and stars. As matter falls into the black hole, intense radiation is emitted.
Astronomers were making considerable progress towards explaining quasars, but there still were many questions they couldn't answer. Quasars were so bright that they drowned out everything around them. What objects were near quasars?
Did quasars reside in galaxies? Ground-based telescopes didn't give astronomers many clues. Some ground-based images hinted that quasars reside in galaxies, but astronomers couldn't see the surroundings clearly.
Finding the answers to many pressing quasar questions was a major reason for the push for a space telescope. Bahcall was a principal advocate for the telescope, telling Congress in 1978 that "one needs to observe quasars with the space telescope to find out whether or not these bright point-objects, quasars, are surrounded by fainter, more diffuse light of galaxies."
Bahcall was right. Spectacular images from the Hubble Space Telescope have shown that quasars indeed reside in galaxies. But the images have revealed other surprising information: Quasars live in a variety of galaxies. Some galaxies are quite normal, others are colliding with their neighbors.
Although Hubble has yielded more clues, many questions still remain unanswered about these enigmatic objects.
"I'd like to know what turns on a quasar," Bahcall says. "We've got some clues, but not definitive answers."
Disney wants to figure out whether quasars are "light bulbs or lighthouses. We don't know if they are pointing their energy at us or pointing it in all directions. And how long are they turned on? Are they short-lived or long-lived? We're only just getting some ideas to these questions."
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