Massive-star supernovae found to be major space dust factories

They report in Science Express that Type II supernovae - where a massive star comes to the end of its life and releases its cataclysmic energy - are the culprits.
Space dust is composed of small particles, made of elements such as carbon, silicon, magnesium, iron and oxygen, which are the building blocks from which the earth was made. Until recently, it was thought that this dust was mainly formed by old sun-like stars known as red giants. But the amount of dust found in young galaxies in the early universe seems unlikely to be due to old stars.

Supernovae produced by short-lived massive stars have long been suspected as the dust factories but they are fairly rare events that only happen approximately once every hundred years in a galaxy, making it harder for researchers to find and analyse whether dust is formed in their aftermath.

NASA's Spitzer Space Telescope allowed the researchers to peer further into the universe, allowing them to observe a supernova whose explosion was discovered in 2003 in the spiral galaxy Messier 74, which is approximately 30 million light-years away. Their results suggest for the first time that dust can form efficiently in supernovae, using up about five per cent of the heavy elements available.

Professor Mike Barlow, of the UCL Department of Physics & Astronomy and one of the authors of the study, says: "Dust particles in space are the building blocks of comets, planets and life, yet our knowledge of where this dust was made is still incomplete. These new observations show that supernovae can make a major contribution to enriching the dust content of the universe."

The researchers used the space-based Spitzer and Hubble telescopes and the ground-based Gemini North Telescope atop Mauna Kea in Hawaii. The study was led by Dr Ben Sugerman of the Space Telescope Science Institute in Baltimore, and members of the Survey for the Evolution of Emission from Dust in Supernovae (SEEDS) collaboration, which is led by Professor Barlow.

Although researchers have detected many supernovae in the past at visible wavelengths, supernova 2003gd is only one of three in the universe that have been seen at infrared wavelengths producing dust. Supernovae dim and expand into space fairly quickly, so scientists require extremely sensitive telescopes to study them even a few months after the initial explosion. While astronomers have suspected that most supernovae do produce dust, their ability to study this dust production in the past has been limited by technology.

Image Credit: NASA/JPL-Caltech/STScI

This image is the galaxy M74, as seen by Spitzer's infrared array camera. The white box to the left of the galaxy's center identifies the location of the supernova remnant. In all the images, the blue dots represent hot gas and stars. The galaxy's cool dust is shown in red. The dust factory, also known as supernova SN 2003gd, is shown at the center of the two small insets from Spitzer's infrared array camera. A white arrow points to its exact location.

The images are false-color, infrared composites, in which 3.6-micron light is blue, 4.5-micron light is green, and 8-micron light is red.




Image Credit: NASA/JPL-Caltech/STScI

The yellow-green dot shown in the July 2004 inset (see figure 2) shows that the source's temperature is warmer than the surrounding material. This is because newly formed dust within the supernova is just starting to cool.




Image Credit: NASA/JPL-Caltech/STScI

By January 2005, the dust had cooled and completely faded from the camera's view. However, it was still detected in January 2005 by another instrument aboard Spitzer called the multiband imaging photometer. The image from that instrument is not shown here.

As dust condenses in supernova ejections it produces three observable phenomena: (1) emission at infrared wavelengths; (2) an increase in obscuration of the supernova's light at visible wavelengths; (3) greater obscuration by the newly formed dust of emission from gas that is expanding away from us, on the far side of the supernova, than from gas expanding towards us, at the front of the supernova.

"One of the difficulties in trying to detect infrared emissions from distant galaxies is the extreme sensitivity of the detectors to heat from other sources," explains Professor Barlow.

"Infrared is primarily heat radiation, so the Spitzer Space Telescope must be cooled to near absolute zero (-273 degrees Celsius) so that it can observe infrared signals from space without interference from the telescope's own heat."

Infrared measurements of supernova 2003gd made 500-700 days after the outburst revealed emission consistent with newly formed cooling dust. Sophisticated modelling of the observed infrared emission and of the measured obscuration at visible wavelengths implied that solid dust particles equivalent to up to seven thousand earth masses had formed.

Dr Ben Sugerman, of the Space Telescope Science Institute in Baltimore who led the study, says: "People have suspected for 40 years that supernovae could be producers of dust, but the technology to confirm this has only recently become available. The advantage of using Spitzer is that we can actually see the warm dust as it forms."

Professor Robert Kennicutt, of the University of Cambridge's Institute of Astronomy and a co-author of the study, added: "These results provide an impressive demonstration of how Spitzer observations of supernovae can provide unique new insights into the processes that produce dust in the universe."

University College London News Release