HIGH RES IMAGES OF GALACTIC CENTER

HIGH RES IMAGES OF GALACTIC CENTER

Credit: W. M. Keck Observatory/ UCLA Galactic Center Group

The center of our Milky Way galaxy, as seen in the infrared using the Keck Laser Guide Star. The white cross marks the location of the supermassive black hole.

UCLA PRESS RELEASE (December 12th, 2005) UCLA astronomers and colleagues published the first high-resolution images of the center of our Milky Way galaxy, including the area surrounding the supermassive black hole, using a new technology at the W.M. Keck Observatory in Hawaii.

“Everything is much clearer now,” said Andrea Ghez, UCLA professor of physics and astronomy, who headed the research team. “We used a laser to improve the telescope’s vision – a spectacular breakthrough that will help us understand the black hole’s environment and physics. It’s like putting on glasses, and will revolutionize what we can do in astronomy.”

The new technology, called Laser Guide Star Adaptive Optics, will lead to important advances for the study of planets in our solar system and outside of our solar system, as well as galaxies, black holes, and how the universe formed and evolved, Ghez said.

“We have worked for years on techniques for ‘beating the distortions in the atmosphere’ and producing high-resolution images,” she said. “We are pleased to report the first Laser Guide Star Adaptive Optics observations of the center of our galaxy.”

Ghez and her colleagues took “snapshots” of the center of the galaxy, targeting the supermassive black hole 26,000 light years away, at different wavelengths. This approach allowed them to study substantial emission emanating from an enormous hot plasma just outside the black hole’s “event horizon,” about to be pulled through. Plasma is a hot, ionized, gas-like matter – the fourth state of matter, distinct from solids, liquids and gases – believed to make up more than 99 percent of the visible universe, including the stars, galaxies and the vast majority of the solar system.

“We are learning the conditions of the plasma and whether this plays a role in the growth of the supermassive black hole,” Ghez said. “The plasma varies dramatically in intensity from week-to-week, day-to-day, and even within a single hour.”

The research, federally funded by the National Science Foundation, will be published Dec. 20 in the Astrophysical Journal Letters.

The research was conducted using the 10-meter Keck II Telescope, which is the world’s first 10-meter telescope with a laser. Laser Guide Star Adaptive Optics allows astronomers to generate an artificial guide star exactly where they want it, helping to reveal the atmosphere’s distortions.

Since 1995, Ghez has been using the W.M. Keck Observatory to study the galactic center and the movement of 200 nearby stars.

Black holes are collapsed stars so dense that nothing can escape their gravitational pull, not even light. Black holes cannot be seen directly, but their influence on nearby stars is visible, and provides a signature, Ghez said. The supermassive black hole, with a mass more than three million times that of our sun, is in the constellation of Sagittarius. The galactic center is located due south in the summer sky.

The black hole came into existence billions of years ago, perhaps as very massive stars collapsed at the end of their life cycles and coalesced into a single, supermassive object, Ghez said.

Co-authors on the research include UCLA graduate students Seth Hornstein and Jessica Lu; the adaptive optics team at W. M. Keck Observatory: David Le Mignant, Marcos Van Dam and Peter Wizinowich; Antonin Bouchez (formerly with the W. M. Keck Observatory) and Keith Matthews at Caltech; Mark Morris, a UCLA professor of physics and astronomy; and Eric Becklin, a UCLA professor of physics and astronomy.

RELATED LINKS

Ghez provides more information, and images of the galactic center, at:

Galactic Center (html)

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The sky is ready for MOSFIRE and DEIMOS. Our observers from CIT and UCI are also ready. Sun set 05:52:00pm rise 06:27:00am
Keck 1 MOSFIRE is scheduled with Subaru observers. Keck 2 DEIMOS is scheduled for UCI observers. Sun set 05:52:00pm rise 06:26:00am
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Observers from CIT will use MOSFIRE on Keck 1, while on Keck 2, CIT observers will use DEIMOS. Sun set 05:52:00pm rise 06:24:00am