YOU ARE HERE: Home

I want information on:

Information for:

Articles

‘Cosmic GDP’ crashes 97% as star formation slumps

While parts of the world experience economic hardship, a team of Portuguese, UK, Japanese, Italian and Dutch astronomers has found an even bigger slump happening on a cosmic scale. In the largest ever study of its kind, the international team of astronomers has established that the rate of formation of new stars in the Universe is now only 1/30th of its peak and that this decline is only set to continue. The team, led by David Sobral of the University of Leiden in the Netherlands, publish their results in the journal Monthly Notices of the Royal Astronomical Society.

GDP crash smallThis diagram indicates the changing ‘GDP’ of the Universe over time. The new results indicate that, measured by mass, the production rate of stars has dropped by 97% since its peak 11 billion years ago. Credit: D. Sobral. Click for a high-resolution version.The accepted model for the evolution of the Universe suggests that stars began to form about 13.4 billion years ago, or around three hundred million years after the Big Bang. Many of these first stars are thought to have been monsters by today's standards, and were probably hundreds of times more massive than our Sun. Such beasts aged very quickly, exhausted their fuel, and exploded as supernovae within a million years or so. Lower mass stars in contrast have much longer lives and last for billions of years.

Much of the dust and gas from stellar explosions was (and is still) recycled to form newer and newer generations of stars. Our Sun, for example, is thought to be a third generation star, and has a very typical mass by today's standards. But regardless of their mass and properties, stars are key ingredients of galaxies like our own Milky Way. Unveiling the history of star formation across cosmic time is fundamental to understanding how galaxies form and evolve.

In the new study, scientists used the UK Infrared Telescope (UKIRT), the Very Large Telescope (VLT) and the Subaru telescope to carry out the most complete survey ever made of star-forming galaxies at different distances, with around ten times the data of any previous effort. With the range of distances, the time taken for the light to reach us means that we see identically selected galaxies at different periods in the history of the universe, so we can really understand how conditions change over time.

By looking at the light from clouds of gas and dust in these galaxies where stars are forming, the team are able to assess the rate at which stars are being born. They find that the production of stars in the universe as a whole has been continuously declining over the last 11 billion years, being 30 times lower today than at its likely peak, 11 billion years ago.

Dr Sobral comments: "You might say that the universe has been suffering from a long, serious "crisis": cosmic GDP output is now only 3% of what it used to be at the peak in star production!"

'If the measured decline continues, then no more than 5% more stars will form over the remaining history of the cosmos, even if we wait forever. The research suggests that we live in a universe dominated by old stars. Half of these were born in the 'boom' that took place between 11 and 9 billion years ago and it took more than five times as long to produce the rest. "The future may seem rather dark, but we're actually quite lucky to be living in a healthy, star-forming galaxy which is going to be a strong contributor to the new stars that will form.

'Moreover, while these measurements provide a sharp picture of the decline of star-formation in the Universe, they also provide ideal samples to unveil an even more fundamental mystery which is yet to be solved: why?"

 

 


Science contact

 

David Sobral

Tel: +31715278421

Mob: +351916700769 / +31652492051

This email address is being protected from spambots. You need JavaScript enabled to view it.

 

 


Media contact

 

Robert Massey

Royal Astronomical Society

Burlington House

Piccadilly

London W1J 0BQ

Tel: + 44 (0)20 7734 3307 x214

Mob: +44 (0)794 124 8035

This email address is being protected from spambots. You need JavaScript enabled to view it.

 

 


Images and captions (downloadable at high resolution)

 

1. This schematic diagram shows how the Universe is thought to have evolved from the Big Bang to the present day. Data from the UKIRT, VLT and Subaru observatories allowed the astronomers to take four precise and comparable snapshots of the Universe when it was, 2, 4, 6 and 9 billion years old, each containing hundreds of star-forming galaxies. By comparing the different snapshots, astronomers were able to accurately track what has changed over the last 11 billion years. Credit: Chandra / NASA / NOAO / KIPAC

http://home.strw.leidenuniv.nl/~sobral/FIG1.jpg

 

2. This diagram indicates the changing 'GDP' of the Universe over time. The new results indicate that, measured by mass, the production rate of stars has dropped by 97% since its peak 11 billion years ago. Credit: D. Sobral

http://home.strw.leidenuniv.nl/~sobral/FIG2_G.jpg

 

3. This diagram shows how the total mass of stars in the Universe should have changed over the last 11 billion years based on the new observations (lines) and how it actually did (symbols; different measurements by other teams). This provides an excellent agreement between both and strengthens the prediction of the new results that no more than a further 5% of stars will come into existence, even if we wait forever. Credit: D. Sobral

http://home.strw.leidenuniv.nl/~sobral/FIG3_G.jpg

 

 


Further information

 

The work, led by David Sobral (started while he was based at the University of Edinburgh and completed at Leiden University), was also done by Ian Smail (Durham University), Philip Best (University of Edinburgh), James Geach (McGill University, Canada), Yuichi Matchuda (Caltech, USA), John Stott (Durham University), Michele Cirasuolo (ATC and University of Edinburgh) and Jaron Kurk (MPA, Germany).

The research appears in "A large Hα survey at z=2.23, 1.47, 0.84 & 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS", D. Sobral, I. Smail, P. N. Best, J. E. Geach, Y. Matsuda, J. P. Stott, M. Cirasuolo, J. Kurk, Monthly Notices of the Royal Astronomical Society.

A preprint of the paper is available from http://arxiv.org/abs/1202.3436

 

 


Notes for editors

 

The Royal Astronomical Society (RAS, www.ras.org.uk), 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 3500 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others.

Follow the RAS on Twitter via @royalastrosoc