An International team of
astronomers (including the U.K.) has produced the first ever image
of an astronomical object using high energy gamma rays, helping to
solve a 100 year old mystery - an origin of cosmic rays.
Their research, published
in Nature, was carried out using the High Energy Stereoscopic
System (HESS), an array of four telescopes, in Namibia, SouthWest
Africa.
The astronomers studied the
remnant of a supernova that exploded some 1,000 years ago, leaving
behind an expanding shell of debris which, seen from the Earth, is
twice the diameter of the Moon.
The resulting image helps
to solve a mystery that has been puzzling scientists for almost one
hundred years - the origin of cosmic rays.
Giant particle accelerator
Cosmic rays are extremely
energetic particles that continually bombard the Earth, thousands
of them passing through our bodies every day.
The production of gamma
rays in this supernova shock wave tells us that it is acting like a
giant particle accelerator in space, and thus a likely source of the
cosmic rays in our galaxy, Dr Paula Chadwick of the University of
Durham said
"This picture really is a
big step forward for gamma-ray astronomy and the supernova remnant
is a fascinating object. If you had gamma-ray eyes and were in the
Southern Hemisphere, you could see a large, brightly glowing ring in
the sky every night." Professor Ian Halliday, CEO of PPARC which
funds U.K. participation in HESS said.
"These results provide the
first unequivocal proof that supernovae are capable of producing
large quantities of galactic cosmic rays - something we have long
suspected, but never been able to confirm.’"
Gamma rays are the most
penetrating form of radiation we know, around a billion times more
energetic than the X-rays produced by a hospital X-ray machine.
Atmosphere shields
This makes it very
difficult to use them to create an image they just pass straight
through any surface, which we might use to reflect them, for
instance.
However, luckily for life
on Earth, gamma rays from objects in outer space are stopped by the
atmosphere; when this happens, a faint flash of blue light is
produced, lasting for a few billionths of a second.
The astronomers used images
of these flashes of light, called Cherenkov radiation, to make a
gamma ray ‘image’ for the first time.