Astronomers Discover Universe's 'Smoking Gun'


An image from the Spitzer Space Telescope covering the entire galaxy NGC 628 (taken July 28, 2004). Normal stars appear blue, hot dust (about 200 deg Celsius) appears green, and cooler dust appears red. NGC 628 is 30 million light years away from Earth. The green object at the centre of the white box is the supernova 2003gd. (Image courtesy of McMaster University)

Massive star supernovae have been major "dust factories" ever since the first generations of stars formed several hundred million years after the Big Bang, according to an international study published in Science Express.

The scientific team trained their telescopes on Supernova 2003gd, which exploded in the NGC 628 spiral galaxy 30 million light-years from Earth. The light from the 2003gd first reached Earth on March 17, 2003. At its brightest, it could be seen in an amateur astronomer's telescope. While many supernovae are discovered each year, this particular one stood out because it was relatively nearby and could be followed for a longer-than-usual time by the specialized infrared detectors of the Spitzer Space Telescope, and by a spectrograph on the Gemini North telescope.

"2003gd is, quite literally, the smoking gun," says Doug Welch, professor, physics & astronomy at McMaster University, and one of 17 astronomers involved in the study. "These carbon and silicon dust particles which form from the supernovae blast make possible the many generations of high-mass stars and all the heavy elements they produce. These are elements which make up the bulk of everything around us on Earth, including you and me."

Welch and co-author Geoff Clayton of Louisiana State University, visited the Gemini North telescope in Hawaii to take spectra of ancient massive star supernovae in their hunt for the formation of dust.

Making space dust requires elements heavier than hydrogen and helium - the only elements in existence after the Big Bang. Once dust is available, stars form much more quickly and efficiently. Up until now, the efficiency and rapidity of the creation of dust by massive star supernovae has been unknown.

Related articles
A White Dwarf Explodes Inside a Dense
Big stars born near black hole
Circumstellar Disk
'Compact Jets' From Neutron Star
Cool brown dwarf may give birth to planets
Cosmic catastrophe may have struck star
First starlight
First Supernova Companion Star Found
Giant star's corona brightens with age, Chandra shows
Hubble Captures A 'Five-star' Rated Gravitational Lens
... Origin Of Elements In Galaxy Clusters
Reborn Star Surprises Astronomers
Red giants discovered in Milky Way
Smallest star found, say astronomers
...Sun May Have a Companion
Supernova Storm Wiped Out Mammoths?
...Titan has dunes
Unraveling Brown Dwarf Origins

"We have finally shown that supernovae could have been major contributors to the dust present in the early Universe," said Ben Sugerman, of the Space Telescope Science Institute in Baltimore, MD. "Until now, the available evidence has pointed to the contrary."

Supernovae expand and dissipate into space quickly, so scientists require extremely sensitive telescopes to study them even a few months after the initial explosion. Dust does not begin to form until two years after an explosion, so while astronomers have suspected that most supernovae do produce dust, their ability to confirm this stellar dust production in the past was limited by the available technology.

The study utilized Hubble Space Telescope data as well as new observations from the Spitzer Space Telescope (currently trailing the Earth along its orbit) and the Gemini North telescope of the Gemini Observatory on Mauna Kea, Hawaii.

"This work demonstrates the enormous value of working in different parts of the spectrum and the critical need for both ground-based and space-based facilities," says Welch.

Funding for the research was provided in part by the Natural Sciences and Engineering Research Council. Canada's participation in the Gemini Observatory is funded by the National Research Council of Canada's Herzberg Institute for Astrophysics.