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RAS PN 08/47: “Naked eye” gamma ray burst was aimed squarely at Earth

Last Updated on Tuesday, 06 April 2010 15:21
Published on Wednesday, 10 September 2008 17:00
An international team of scientists have deduced that the beam from a 'gamma ray burst' seen in March this year pointed directly at the Earth.

ROYAL ASTRONOMICAL SOCIETY PRESS INFORMATION NOTE

EMBARGOED UNTIL 1800 BST (LONDON TIME), 1300 US EASTERN DAYLIGHT TIME, 10TH SEPTEMBER 2008

Date: 9th September 2008
Ref.: PN 08/47

Issued by:
Dr Robert Massey
Press and Policy Officer
Royal Astronomical Society
Burlington House
Piccadilly
London W1J 0BQ
Tel: +44 (0)794 124 8035, +44 (0)20 7734 4582
E-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.

RAS website: www.ras.org.uk

RAS PN 08/47 (EMBARGOED): “NAKED EYE” GAMMA RAY BURST WAS AIMED SQUARELY AT EARTH

The brightest explosion ever seen was observed in March this year. Now a team of astronomers from around the world, including the University of Leicester, the Mullard Space Science Laboratory of University College London and Liverpool John Moores University, have combined their data from satellites and observatories to explain what happened. They show that the jet from a powerful stellar explosion in a galaxy halfway across the Universe was aimed almost directly at Earth. The event, called a Gamma-Ray Burst (GRB), was bright enough for human eyes to see.

GRBs are the Universe's most luminous explosions. Early in the morning of March 19, the Swift satellite, a joint NASA/UK/Italian mission, pinpointed an extremely bright GRB and immediately sent out an alert to observatories around the world. Two robotic wide-field optical cameras in Chile also observed the brief flash: "Pi of the Sky," which is operated by the Centre for Theoretical Physics in Warsaw, Poland, and TORTORA, based at ESO’s La Silla Observatory. TORTORA is operated by a Russian-Italian collaboration. Within minutes many more telescopes were observing, allowing for the most detailed study of a bright GRB ever undertaken using data from gamma-ray to radio wavelengths.

A team of astronomers led by Judith Racusin of Penn State University, present their findings in a paper to appear in the September 10 issue of the journal Nature, following work first presented at the May meeting of the Royal Astronomical Society. The team conclude that the extraordinary brightness of the March 19 burst arose from a narrow jet that shot material directly toward Earth at 99.99995 percent of the speed of light. The data clearly reveal the complexity of a GRB in which a narrow, ultra-fast jet is present within a wider, slightly slower jet.

Dr. Paul O’Brien of the University of Leicester, part of the Swift team, said “We normally detect only the wide jet of a GRB as the inner jet is very narrow, equivalent to not much more than 1/100th the angular size of the full Moon. It seems that to see a very bright GRB the narrow jet has to be pointing precisely at the Earth. We would expect that to happen only about once per decade. On March 19th, we got lucky.”

Dr. Patricia Schady of the Mullard Space Science Laboratory, also part of the Swift team, commented “The GRB was created when a massive star ran out of nuclear fuel. The star's core collapsed to form a black hole, driving powerful jets outward. These jets are amongst the fastest bulk flow of matter in the cosmos, moving close to the speed of light.”

By rapidly coordinating their efforts using data sent over the Internet, astronomers were able to ensure they made the best possible use of all available British and international telescopes to observe this extraordinarily bright event. Among the telescopes which responded to the alert from Swift was the UK’s largest robotic telescope, the Liverpool Telescope, located on the island of La Palma. Dr Robert Smith from the Liverpool John Moores University, which operates the telescope, said “As the GRB jets move outwards they strike gas previously shed by the star and heat it. This generates emission called the ‘afterglow’. The Liverpool Telescope and other telescopes detected this emission which confirmed the width of the jets.”

Dr. Jonathan Granot from the University of Hertfordshire, lead theorist on the paper, explained “What really makes this GRB unique is its extremely bright prompt optical emission (visible with the naked-eye), which coincides in time with the gamma-rays, and was recorded with amazing time resolution. The optical and gamma-rays are in distinct spectral components, produced by a different emission mechanisms, but most likely came from the same physical region, far from the progenitor star.”

For related images (these will be live 30 minutes before the embargo expires and will be presented at a teleconference)
http://www.nasa.gov/mission_pages/swift/bursts/naked_eye_telecon.html

RAS website
http://www.ras.org.uk

Video of the first presentation of the work at the Royal Astronomical Society by Leicester University Research Associate Dr. Rhaana Starling
http://clients.mediaondemand.net/ras/09052008/player.aspx?externalRAS=externalRas123&id=3

CAPTIONS AND CREDITS

Images
Swift imaged GRB 080319B with its Ultraviolet and Optical Telescope (UVOT, left) and X-ray Telescope (XRT). The event set a record for the brightest-ever gamma-ray burst. NASA/Swift/Stefan Immler

Image movie
This sequence dissolves from Swift’s UVOT image to its XRT view of the "naked-eye" GRB. The burst was so intense it initially saturated both instruments. NASA/Swift/Stefan Immler

Illustration
This artist's concept shows the "naked-eye" GRB close up. Observations indicate material shot outward in a two-component jet (white and green beams). NASA/Swift/Mary Pat Hrybyk-Keith and John Jones

Animation
This animation shows how astronomers think GRB 080319B erupted. A narrow, ultrafast jet punches through the star at nearly the speed of light, followed by a wider, less energetic jet. NASA/Swift/Cruz deWilde

NOTES FOR EDITORS

CONTACTS

Dr. Paul O’Brien
Department of Physics & Astronomy
University of Leicester
Phone: 0116 252 5203
Mobile:  07891 894 071
E-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.

Dr. Patricia Schady
Mullard Space Science Laboratory
University College London
Phone: 01483 204 261
Mobile: 07815 977 736
E-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.

Dr. Robert Smith
Astrophysics Research Institute
Liverpool John Moores University
Mobile: +1 650 625 1265
E-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.

Dr Jonathan Granot
School of Physics, Astronomy & Mathematics
University of Hertfordshire
Phone:  01707 284569
Mobile: 07972 164 442
E-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.

Swift, launched in November 2004, is a NASA mission in partnership with the Italian Space Agency and the Science and Technology Facilities Council, United Kingdom. Swift is managed by NASA Goddard. Penn State University controls science and flight operations from the Mission Operations Centre in University Park, Pennsylvania.  Los Alamos National Laboratory provides gamma-ray imaging analysis.
http://www.swift.ac.uk/

The Liverpool Telescope is funded by Liverpool John Moores University and the Science and Technology Facilities Council, United Kingdom.
http://telescope.livjm.ac.uk/

The TORTORA camera is mounted on the Italian REM telescope at the European Southern Observatory in Chile. It was built and is being operated by collaboration between Italy's Bologna State University and Brera Observatory and Russia's Special Astrophysical Observatory and Institute of Precise Instrumentation.

The Royal Astronomical Society (RAS), founded in 1820, encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science. The RAS organizes scientific meetings, publishes international research and review journals, recognizes outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 3000 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others.