The team measured the cold cosmic dust in 'Cassiopeia A', the remnant of a supernova explosion in our own Galaxy, about 11,000 light years from Earth. The amount of dust was a thousand times what had been previously detected, suggesting that these powerful explosions are one of the most efficient ways to create cosmic dust. This also answers the riddle of how large quantities of dust recently discovered in the early universe were formed.
Unlike household dust, cosmic 'dust' actually consists of tiny solid grains (mostly carbon and silicates) floating around in interstellar space, with similar sizes to the particles in cigarette smoke. The presence of dust grains around young stars helps them to form and they are also the building blocks of planets.
Dr. Loretta Dunne from Cardiff University, who led the research, says "Effectively, we live on a very large collection of cosmic dust grains! The question of the origin of cosmic dust is in fact that of the origin of our planet and others."
The Smoking Gun
Supernovae are the violent explosions of stars at the ends of their lives. In a single instant, a supernova can release more energy than our Sun will produce in its entire nine billion year lifetime. They also make large amounts of heavy elements like carbon and oxygen and throw them out into interstellar space. Since these are the ingredients of cosmic dust grains, it was suspected that supernovae might be important in explaining the origin of dust. However, until now, only tiny amounts of dust had ever been found in supernovae - leaving astronomers with a smoking gun, but not enough smoke.
Haley Morgan, a Ph.D. student at Cardiff University, explains "Some supernovae are the violent ends of stars that live fast and die young. These stars are many times the mass of our own Sun, and they burn their fuel thousands of times faster, in only a few million years. If supernovae were efficient dust 'factories' they would each be producing more than the mass of the Sun in dust."
The team looked at 'Cassiopeia A', the 300 year-old supernova remnant created when a star about 30 times more massive than the Sun exploded. The material from the explosion is still travelling outwards at speeds of 10,000 km per second, sweeping up the surrounding gas and dust into a blast wave shell.
Dust grains block half of all the visible light from stars and galaxies, but this dusty cloud has a silver lining as they also shine this stolen starlight back out as far-infrared and submillimetre waves (at wavelengths between 0.1 and 1 millimetre). To detect these wavelengths, the team used 'SCUBA', the world's most powerful submillimetre-wave camera, attached to the James Clerk Maxwell Telescope in Hawaii.
Cold Hard Evidence
SCUBA detected a dust shell in Cassiopeia A with a total mass around 1-4 times that of the Sun. Dr. Steve Eales, also of Cardiff University, says "This is over a thousand times what's been seen before! Cassiopeia A must have been extremely efficient at creating dust from the elements available."
Prof. Mike Edmunds, head of the School of Astronomy at Cardiff, adds "Astronomers have been searching for dust in supernova remnants for decades, but they could only detect the tiny fraction of dust which was relatively warm. With SCUBA we can at last see the dust which is very cold, at a temperature of -257 degrees Celsius."
In recent years, SCUBA has also found distant galaxies full of dust, more than ten billion light years from Earth. The light from them has taken so long to reach us that we are seeing them as they were when the universe was only about one billion years old - less than one tenth of its current age.
Supernova Sleuths
The origin of this ancient dust was a mystery. Astronomers had thought that dust was mostly made in the winds from cool, giant stars in the late stages of their lives. But stars such as our Sun take about nine billion years to reach this stage, so it was impossible for the dust to be created by stellar winds within the first billion years of the universe. With dust created quickly in supernovae, the mystery has been solved.
Dunne says "Dust has been swept under the cosmic carpet - for years astronomers have treated it as a nuisance because of the way it hides the light from the stars. But then we found that there is dust right at the edge of the Universe in the earliest stars and galaxies, and we realised that we were ignorant of even its basic origin. Now, with these supernova dust factories, we can explain how that dust was made."
Dr. Rob Ivison of the UK Astronomy Technology Centre in Edinburgh says, "Massive stars become supernovae in the blink of an eye by astronomical standards, so we can now explain why the early universe is so dusty."
"These observations give us a tantalising glimpse of how the first solid particles in the universe were created," adds Haley Morgan.
This work will be published in Nature, 17th July 2003, Vol. 474, p.285.
NOTES FOR EDITORS
SCUBA
SCUBA (the Submillimetre Common-User Bolometer Array) is the world's most powerful submillimetre-wave camera. It is attached to the James Clerk Maxwell Telescope, and contains sensitive detectors called bolometers, which are cooled to 60 milliKelvin, 0.06 degrees above absolute zero (60 milliKelvin is about -273.1 Celsius, -459.6 Fahrenheit).
The James Clerk Maxwell Telescope (JCMT)
The JCMT is the world's largest single-dish submillimetre-wave telescope. It collects faint submillimetre-wavelength signals with its 15 metre diameter dish. It is situated near the summit of Mauna Kea on the Big Island of Hawaii, at an altitude of approximately 4000 metres (14000 feet) above sea level. It is operated by the Joint Astronomy Centre, on behalf of the UK Particle Physics and Astronomy Research Council, the Canadian National Research Council, and the Netherlands Organisation for Scientific Research.
Supernovae
Supernovae happen about once every 50 years in our Galaxy, and there are two main types - 1a and II. Cassiopeia A is an example of a type II. Type II supernovae are the explosions of very massive stars, more than 8 times larger than the Sun. These stars are 'live fast-die young' using up their hydrogen and helium fuel in only a few million years (thousands of times faster than the Sun burns it's fuel).
When the fuel supply is exhausted the star must make heavier and heavier elements until, finally, when it can do no more to keep itself alive the central part of the star collapses to become a neutron star or Black Hole, and the outer parts are flung off in the cataclysm we call a supernova.
The explosion of a supernova acts like the explosion of a nuclear bomb, driving a blast-wave into the surrounding material. The gas is heated to very high temperatures (over a million degrees) so that it produces X-rays, and it also generates powerful radio emission as electron spiral in strong magnetic fields. If the nearest massive star, Betelgeuse, were to go supernova it would (for a short time) be brighter than the full moon.
Formation of dust in the atmospheres of stars
Elements such as silicate and carbon are formed in stars and can condense out of the gas to make solid dust grains. This happens when certain conditions of temperature and pressure are met, the process is similar to how snowflakes form but happens at much higher temperatures.
IMAGES
TO ACCESS THESE IMAGES DURING THE EMBARGO YOU WILL NEED TO SUPPLY THE USERNAME 'press' AND THE PASSWORD 'casanature'. In case of problems, please contact Douglas Pierce-Price (contact details in main text).
The "Cassiopeia A" supernova remnant as seen by SCUBA, revealing a shell of cosmic dust about 12 light years across. This is an image taken with submillimetre wavelengths of light. The black and dark blue colours represent fainter emission, whilst the light blue and white areas shine the brightest. CREDIT: Loretta Dunne (Cardiff University) et al.
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Photograph of the James Clerk Maxwell Telescope, atop Mauna Kea on the Big Island of Hawaii. CREDIT: Nik Szymanek.
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CONTACTS
Cardiff University
Dr. Loretta Dunne
Between 18th July and 28th July, contact by email or via Dr. Douglas Pierce-Price (details below).
Dept. of Physics and Astronomy, Cardiff University
Email: loretta.dunne@astro.cf.ac.uk
Tel: 44-292-087-6782
Fax: 44-292-087-4056
Dr. Steve Eales
Dept. Physics and Astronomy, Cardiff University
Email: steve.eales@astro.cf.ac.uk
Tel 44-292-087-6168
Fax: 44-292-087-4056
Miss Haley Morgan
Dept. Physics and Astronomy, Cardiff University
Email: haley.morgan@astro.cf.ac.uk
Tel: 44-292-087-6782
Fax: 44-292-087-4056
For expert comment in Welsh contact:
Dr. Rhodri Evans
Dept. Physics and Astronomy, Cardiff University
Email: rhodri.evans@astro.cf.ac.uk
Tel 44-292-087-6274 / 876992
Astronomy Technology Centre
Dr. Rob Ivison
UK Astronomy Technology Centre, Royal Observatory Edinburgh
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Fax: 44-131-668-8407
Eleanor Gilchrist
Press Office
Email efg@roe.ac.uk
Tel: 44-131-668-8397
Joint Astronomy Centre, Hawaii
For information about SCUBA and the James Clerk Maxwell Telescope:
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Joint Astronomy Centre, Hawaii
Email: outreach@jach.hawaii.edu
Tel: 808-969-6524
Fax: 808-961-6516
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The Particle Physics and Astronomy Research Council (PPARC) is the UK's strategic science investment agency. It funds research, education and public understanding in four broad areas of science - particle physics, astronomy, cosmology and space science.
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Journal
Nature