Sarah Keegan Headquarters, Washington, D.C. September 21, 1994 (Phone: 202/358-1547) Jim Elliott Goddard Space Flight Center, Greenbelt, Md. (Phone: 301/286-6256) Ray Villard Space Telescope Science Institute, Baltimore, Md. (Phone: 410/338-4514) RELEASE: 94-160 HUBBLE UNCOVERS A HIDDEN QUASAR IN A NEARBY GALAXY Astronomers using NASA's Hubble Space Telescope have found a new quasar -- not billions of light years away like its known cousins, but a mere 600 million light years, the equivalent of Earth's cosmic backyard. "I was stunned when we realized we had a quasar; it was a total surprise," said Dr. Anne Kinney of the Space Telescope Science Institute, Baltimore, Md. Until this discovery all known quasars existed in the early universe. "So it is unusual to find one in our own epoch," Dr. Kinney said. The discovery in galaxy Cygnus A will give astronomers their first opportunity for detailed study of a quasar, an object which looks like a pinpoint of light (as does a star) to a ground-based telescope. A quasar, though, emits hundreds of times more energy than an entire galaxy with more than 100 billion stars. There is evidence that the quasars -- short for "quasi-stellar radio sources" -- found in the remote galaxies are powered by supermassive black holes that devour dust, gas and stars from the host galaxies, producing enormous amounts of energy in the process. Beyond that, little is known about them, which makes this discovery so important. Dr. Kinney emphasized that this unexpected result implies that all radio galaxies might harbor quasars that are hidden from view. The observations were made by Robert Antonucci and Todd Hurt of the University of California at Santa Barbara, and Kinney. Their results appear in the September 22 issue of Nature. Though Cygnus A is categorized as an elliptical galaxy, it has an unusual peanut shape due to a dark band of dust encircling the enigmatic nucleus. The Hubble astronomers could only peek into the core by taking advantage of a natural "periscope effect." Dust outside of the nucleus acts like a mirror to reflect the shorter wavelengths, or blue component, of the light toward Earth. The astronomers used the ultraviolet sensitivity of the Faint Object Spectrograph to look for the spectral signature of extremely hot, supermassive stars hidden in the nucleus. Such stars are theorized as one possible explanation for Cygnus A's powerful optical emissions. Instead, the resulting ultraviolet spectrum was so unusual that astronomers puzzled over the data for three months before reaching their startling conclusion. After much analysis, they realized it was in part composed of the typical spectrum of a quasar. Such a spectrum possesses broad emission lines that indicate that gas in the nucleus is swirling at high speeds. "One caveat is that the broad emission line could possibly be many narrow emission lines blended together," Kinney said. "We will double check that possibility with more observations." HST's ultraviolet sensitivity allowed this spectrum to be distinguished more easily from the galaxy's starlight. Kinney emphasized that it is probably more than coincidence to find a quasar embedded in the nearest extremely powerful radio galaxy to Earth. These results suggest that quasars might be common to radio galaxies and might explain their powerful radio emissions, she added. Though this provides an unexpected opportunity for close-up study of the mysterious "engine" behind a quasar, these results add further mystery as to the true nature of the powerhouse. Previous ground-based radio observations show that there is an elongated object in Cygnus A's core. This is inconsistent with black hole models that predict a compact point source of radiation. Supermassive black holes are a leading candidate for explaining a quasar's prodigious outpouring of energy. The astronomers plan to use the Hubble Space Telescope to study the spectrum of other radio galaxies and look for fingerprints of other quasars. The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency (ESA). - end - NASA press releases and other information are available automatically by sending an Internet electronic mail message to domo@hq.nasa.gov. In the body of the message (not the subject line) users should type the words "subscribe press-release" (no quotes). The system will reply with a confirmation via E-mail of each subscription. A second automatic message will include additional information on the service. Questions should be directed to (202) 358-4043.