- All News
- Search News
- Archived News
- Physicist Steven Cundiff Elected as Fellow of AAAS
- Observing the Dance of Ten Million Quantum Dots
- Physics Professor Tim McKay Explains ECoach Tool Now Used for All First-Year U-M Students
- Physicist Mark Newman's Scientific Cartogram Maps Featured in Washington Post
- U-M Physics Professor Tim McKay Developed Coaching Software to Help Students
- 11 Surprising Predictions for 2017 From Some of The Biggest Names In Science
- New Metamaterial Can Switch from Hard to Soft—And Back Again
- Physicist Lu Li and Team First to Uncover Rotational Symmetry Breaking in Magnetic Property of Unconventional Superconductor
- Physicist Michal Zochowski Collaborates with LSA Professor Sara Aton for ‘The Science of Sleep’
- Next-Gen Dark Matter Detector in a Race to Finish Line
- Physicist Roberto Merlin Selected as 2017 OSA Lippincott Award Recipient
- Michigan at the March for Science
- All Events
- Special Lectures
- K-12 Programs
- Saturday Morning Physics
- Seminars & Colloquia
ANN ARBOR, Mich.— University of Michigan astrophysicists have recently discovered two of the brightest optical flashes from Gamma-Ray Bursts (GRBs).
GRBs are the brightest explosions in the universe, releasing as much energy in tens of seconds as the Sun will release in its entire lifetime. They are luminous enough to be visible from over 10 billion light-years away with modestly sized telescopes. GRBs are believed to be formed when a massive rotating star collapses in a "hypernova" explosion, releasing energy in gamma-rays as well as a short, bright optical flash. On average, two GRBs per day are visible at the earth; they are detected in the gamma-rays with orbiting space telescopes such as NASA's Swift Satellite.
The Robotic Optical Transient Search Experiment (ROTSE) telescopes comprise a global array of small automated telescopes designed for rapid (5 second) responses to GRB triggers from satellites such as Swift. The two bright record-breaking flashes detected recently, GRB060927 and GRB061007, were both observed by the ROTSE-IIIa instrument at Siding Spring Observatory, Australia. GRB060927 (see picture) was bright enough to be visible at the Earth, although it occurred 12 billion light-years away, when the Universe was just 8% of its present age. The fact that time is stretched out at such a large distance means that we can probe the very beginning of the optical event, less than 3 seconds after the start of gamma-ray emission. At that time, the optical counterpart was the brightest object in the Universe, although it faded very rapidly.
GRB061007 was much nearer to the Earth—only 5 billion light-years away—but was bright enough to be seen with high powered binoculars. This was a dramatic event that increased in brightness by a factor of 15 in just 6 seconds. The automated analysis software run by the ROTSE team was able to rapidly identify this new transient, and an alert to the community was released in just 4 minutes from the start of the event, allowing other observers to plan their follow-up observations when the object was brightest and easiest to detect.
“Each of these bursts was bright enough that if they had occurred in the neighboring Andromeda galaxy, they would have been visible to observers on the Earth as brighter than the full moon, said U-M Physics Department Visiting Scholar Eli Rykoff. He further explains that fortunately for people on the Earth; GRBs are extremely infrequent events, particularly in the neighborhood of our local galaxies.
“These two events demonstrate the power of fast robotic systems such as ROTSE to explore even very distant reaches of the Universe,” commented U-M Physics Professor and leader of the ROTSE collaboration, Carl Akerlof.