Wednesday, September 10, 2008

GRB 080319B - March 19, 2008 at 02:13 EDT

RELEASE: 08-223

"NAKED-EYE" GAMMA-RAY BURST WAS AIMED SQUARELY AT EARTH

WASHINGTON -- Data from satellites and observatories around the globe show a jet from a powerful stellar explosion witnessed March 19 was aimed almost directly at Earth.

NASA's Swift satellite detected the explosion - formally named GRB 080319B - at 2:13 a.m. EDT that morning and pinpointed its position in the constellation Bootes. The event, called a gamma-ray burst, became bright enough for human eyes to see. Observations of the event
are giving astronomers the most detailed portrait of a burst ever recorded. "Swift was designed to find unusual bursts," said Swift principal investigator Neil Gehrels at NASA's Goddard Space Flight Center in Greenbelt, Md. "We really hit the jackpot with this one."

In a paper to appear in Thursday's issue of Nature, Judith Racusin of Penn State University and a team of 92 coauthors report on observations across the spectrum that began 30 minutes before the explosion and followed its afterglow for months. The team concludes the burst's extraordinary brightness arose from a jet that shot material directly toward Earth at 99.99995 percent the speed of light.

At the same moment Swift saw the burst, the Russian KONUS instrument on NASA's Wind satellite also sensed the gamma rays and provided a wide view of their spectral structure. A robotic wide-field optical camera called "Pi of the Sky" in Chile simultaneously captured the
burst's first visible light. The system is operated by institutions from Poland.

Within the next 15 seconds, the burst brightened enough to be visible in a dark sky to human eyes. It briefly crested at a magnitude of 5.3 on the astronomical brightness scale. Incredibly, the dying star was 7.5 billion light-years away.

Telescopes around the world already were studying the afterglow of another burst when GRB 080319B exploded just 10 degrees away. TORTORA, a robotic wide-field optical camera operated in Chile with Russian-Italian collaboration, also caught the early light. TORTORA's
rapid imaging provided the most detailed look yet at visible light associated with a burst's initial gamma-ray blast.

Immediately after the blast, Swift's UltraViolet and Optical Telescope and X-Ray Telescope indicated they were effectively blinded. Racusin initially thought something was wrong. Within minutes, however, as reports from other observers arrived, it was clear this was a special
event.

Gamma-ray bursts are the universe's most luminous explosions. Most occur when massive stars run out of nuclear fuel. As a star's core collapses, it creates a black hole or neutron star that, through processes not fully understood, drive powerful gas jets outward. These jets punch through the collapsing star. As the jets shoot into space, they strike gas previously shed by the star and heat it. That generates bright afterglows.

The team believes the jet directed toward Earth contained an ultra-fast component just 0.4 of a degree across. This core resided within a slightly less energetic jet about 20 times wider. "It's this wide jet that Swift usually sees from other bursts," Racusin explained. "Maybe every gamma-ray burst contains a narrow jet, too, but astronomers miss them because we don't see them head-on." Such an alignment occurs by chance only about once a decade, so a GRB 080319B is a rare catch.

Swift is managed by Goddard. It was built and is being operated in collaboration with Penn State, the Los Alamos National Laboratory, and General Dynamics in the U.S.; the University of Leicester and Mullard Space Sciences Laboratory in the United Kingdom; Brera Observatory and the Italian Space Agency in Italy; plus additional partners in Germany and Japan.

Thursday, January 31, 2008

Mercury fly-by benefits

MESSENGER flew past the planet Mercury a few weeks ago with all its instruments gathering a wealth of data.

The preliminary science results were presented at a press conference on Jan 30, and those results are summarized well in the Planetary Society's blog.

As the author of that blog noted, however, there was another outcome in the press conference.

One of the press questions at the end was from a tiny local radio station who said that he knew he was being listened to by an audience of schoolkids; what would the science panel say to those kids? One panelist, Bob Strom, talked briefly about how much of a "turn-on" science was, which was a bit awkward; but, with a couple more minutes to think, Sean Solomon [the MESSENGER PI] really stepped up. Here's what he said:

Space exploration is a lot more than space science. We're flying a spacecraft that owes its origin and livelihood to hundreds of engineers and technicians who designed it, who worried about how it would survive so close to the Sun, how it would survive radiation, how it would live for nearly 8 years, how it would communicate its scientific findings back to the Earth, how it would get launched, how it would find its way billions of miles, 15 times around the Sun, to get into Mercury orbit 6 and a half years following its launch. There are a lot of ways to contribute to space exploration. Science is one of them. The engineering of building, operating, and maintaining spacecraft is a terrific field, and we [gesturing to the panel] would not be up here if we did not have an outstanding team of engineers who put this spacecraft together and keep it going.


I couldn't say it better myself!