High Energy Astrophysicsfor Everybody
Sounds like another dry scientific meeting, right?
"We selected the attendees in part by asking how they would share their knowledge with others," says Janet Mattei, director of the American Association of Variable Star Observers (AAVSO), which is co-sponsoring the meeting along with the Marshall Space Flight Center. "We got some fantastic responses from astronomy club presidents, planetarium workers, and teachers ... just wonderful responses. There's a real need to bring high-energy astronomy to the attention of the public, and we think these are the right people to do it."
"The usual connotation of 'amateur' really doesn't apply here," says NASA/Marshall's Dr. Jerry Fishman, one of the workshop's organizers. "These are dedicated, well-prepared and knowledgeable astronomers who use very sophisticated equipment -- often comparable to professional observatories. Many of them are able to contribute astronomical data used in forefront astronomical research."
Monitoring fireballs from gamma-ray bursts and tracking the light curves of variable stars are two areas where amateur data can make an impact, says Fishman. The workshop will touch on those topics and more, ranging from gamma-ray explosions at the edge of the universe to cosmic rays here in the solar system. There will be a special session entitled "Rapid Observations of GRBs by Amateurs" prompted in part by the recent detections of gamma-ray burst afterglows by amateurs. The three-day meeting will conclude on Saturday, April 15 with a lecture by Astronaut Dr. John Grunsfield entitled "The 1999 HST Servicing Mission and Remarks on High Energy Astrophysics."
The Invisible, Violent Heavens
High energy astrophysics is the study of the most violent events in the universe. Colliding neutron stars, gamma-ray bursts (GRBs), swirling accretion disks around black holes -- these are just a few of the cosmic wonders visible in the x-ray and gamma-ray regions of the electromagnetic spectrum. Unfortunately, the short wavelengths where these events shine brightest are inaccessible from Earth because our atmosphere filters out most forms of high-energy radiation. (This is a real nuisance for gamma-ray astronomers, but a good thing for life on our planet!) To study these objects, astronomers use ultraviolet, x-ray, and gamma-ray detectors on Earth-orbiting satellites.
"Amateurs have been helping scientists with satellite-based research in variable stars since 1975," says Mattei. "For example, when the Rossi X-ray Timing Explorer and the Extreme Ultraviolet Explorer (both are orbiting observatories) were scheduled to observe the cataclysmic variable star, SS Cygni, the AAVSO was asked to help. Our members around the world kept a vigil and when the star flared at optical wavelengths we immediately called our professional colleagues." Thanks to the rapid alert, professional astronomers were able to point their satellites at SS Cygni while it was flaring and monitor the enigmatic star at many wavelengths for the first time.
"In this particular case everything worked! Optical,
x-ray, extreme ultraviolet-- we got it all."
This summer scientists will try to observe another outburst from SS Cygni using NASA's newest Great Observatory, the Chandra x-ray telescope. Once again the AAVSO will be called upon to alert professionals that SS Cygni is erupting, says Mattei.
Another Glowing Accomplishment....
Right: Nestled 7 arc seconds from a 17th magnitude foreground
star, the 20th magnitude afterglow of GRB 000301C is circled
in this CCD image from the US Naval Observatory 1m telescope
in Flagstaff, AZ. Credit: Arne Henden.The optical afterglow
was first detected by the Nordic Optical Telescope in La Palma,
Spain and later recorded by amateur astronomers in Buffalo, NY.
Theorists believe that studying gamma-ray bursts at optical wavelengths might help unravel one of the biggest mysteries in modern astronomy: what causes these powerful gamma-ray explosions? Since astronomers detected the first optical counterpart of a gamma-ray burst in 1997, they have vigorously pursued the afterglows using some of the most powerful telescopes including Hubble, Keck, and Palomar.
Powerful telescopes are important for monitoring afterglows because they fade quickly, usually dimming to 19th magnitude or fainter just a few hours after the onset of the explosion. Advances in CCD technology are now bringing these faint fireballs within reach of dedicated amateur observatories. The afterglow recorded by amateurs in March, for instance, was 20th magnitude. Astronomy club observatories still can't record the spectra required to measure redshift-based distances to afterglows and they probably never will. The objects are simply too faint for spectroscopy. Redshifts will remain the province of Hubble and Keck for the foreseeable future.
Nevertheless, amateurs maintain one important advantage over
their professional counterparts -- telescope time. Telescopes
like Hubble and Keck are heavily oversubscribed. These behemoths
simply can't turn to look at every single gamma-ray burst that
comes along (GRBs are detected once or twice a day by Earth-orbiting
satellites). With little competition for telescope time, amateur
observatories are much more flexible. Eventually a global network
of amateurs might monitor GRB afterglows nearly around the clock,
a feat no single professional observatory can match.
"Measuring the optical light curves of gamma-ray bursts would be a very important contribution to astrophysics and there seems to be no question -- they [the amateurs] can do it." says Dr. Marshall Joy, an x-ray astronomer at the NASA/Marshall Space Flight Center who will deliver a lecture on Future Observations in X-ray Astronomy.
Left: Using graphics and data from NASA's Compton Gamma Ray Observatory, this animation illustrates one of the most exciting mysteries of modern astrophysics, gamma-ray bursts. [more information from the NASA/Goddard Astronomy Picture of the Day]
In fact, amateur observations of gamma-ray bursts seem so
promising that the organizers have scheduled a special session
of the workshop on Rapid Observations of GRBs by Amateurs.
"The most important thing we're doing in this workshop is bringing interested members of the public into the scientific enterprise and making them a valuable part of it," concluded Joy. "These people are going to be the true ambassadors of high-energy astrophysics."
Stay tuned to Science@NASA for more news from the High Energy
Workshop for Amateur Astronomers, held April 12 - 14 near the
NASA/Marshall Space Flight Center in Huntsville, AL.
The MSFC-AAVSO High Energy Astronomy Workshop will be held in conjunction with the 89th Meeting of the American Association of Variable Star Observers (AAVSO). This meeting will be held the day after the Workshop, at the same venue (The Huntsville Marriott).
Schedule of Speakers
Wednesday, April 12
Thursday, April 13
Friday, April 14
Sign-up for the AAVSO Gamma-ray Burst Network -- although this page says there is a Dec. 1, 1999 deadline, you can still register!
American Association of Variable Star Observers -- home page, from the Marshall home page