Tonight's Sky
Sun
Sun
Moon
Moon
Mercury
Mercury
Venus
Venus
Mars
Mars
Jupiter
Jupiter
Saturn
Saturn

Tonight's Sky — Change location

OR

Searching...

Tonight's Sky — Select location

Tonight's Sky — Enter coordinates

° '
° '

Distant supernovae trace early universe's deceleration

The most distant supernovae ever seen confirm that the universe's expansion first slowed down before it started speeding up.
Amanda Gefter
Hubble Space Telescope
Sunrise illuminates Hubble's golden solar arrays from behind, providing a stark contrast to the blackness of space. Arching between the body of the telescope and the array on the right is the thin line of Earth's atmosphere.
NASA
October 26, 2003
Cosmologists are a rare breed of detectives, trying to piece together the shadowy tale of the universe's evolution. Their clues lurk in the farthest reaches of outer space and in the remotest times of the distant past. Now Adam Riess of the Space Telescope Science Institute in Baltimore has detected crucial new evidence, bringing us one step closer to understanding the history and fate of the universe.

Using the Hubble Space Telescope, Riess and his team measured light bursting from a handful of type Ia supernovae whose distances correspond to nearly three-quarters back toward the beginning of time. There they found clear evidence of the deceleration that occurred before dark energy took the reigns roughly five billion years ago and began accelerating the universe's expansion.

The scientific community has eagerly awaited these results since 1998, when news that the universe is expanding faster and faster had come as an astonishing twist in the cosmological plot. Two teams of observers — the Supernova Cosmology Project and the High-Z Supernovae Search Team — had been studying type Ia supernovae to determine the expansion rate of the universe. By comparing these supernovae's intrinsic brightness to their apparent brightness, astronomers can determine their distance; their redshift then reveals how greatly space has expanded in the time it took for their light to reach us.

The teams found their supernovae to be dimmer than expected, which meant that the universe's expansion is currently accelerating. Their results, combined with evidence from the cosmic microwave background radiation, forced scientists to conclude that some repulsive form of energy makes up over 70% of the contents of the universe.
Supernovae in Distant Universe
Studies of distant supernovae suggest the expansion of the universe was slowing down after the Big Bang, but today, the universe's expansion rate is accelerating. The Hubble Space Telescope's Advanced Camera for Surveys (ACS) recently discovered two type Ia supernovae that may have existed during the transition phase when the universe's expansion began to accelerate.
NASA / A. Feild (STScI)
But cosmologists quickly realized that the universe could not have been accelerating all along. It must have first slowed down after the extraordinarily fast expansion of inflation in order for gravity to sculpt stars and galaxies. To see the initial deceleration, though, would require astronomers to look even farther back in space and time than they already had.

Riess, who was a member of the High-Z Supernovae Search Team, has done just that with the Hubble Higher-z Supernova Search Team. Using the Hubble Space Telescope, the team found six of the seven most distant supernovae found to date. "We got the first really significant sample of supernovae that were at such high redshift you could see the slowing down of the expansion of the universe preceding the speeding up," Riess says.

Knowing when the universe switched from deceleration to acceleration will help narrow down the now-exorbitant number of theoretical models hoping to explain the existence of dark energy.

The finding also assures astronomers that the observed acceleration is real and not due to something prosaic like cosmic dust. If dust was the culprit, the dimming of supernovae would increase the farther back you look. But the distant supernovae Riess and his team observed are brighter than expected, confirming that gravity applied the brakes on cosmic expansion before dark energy let a heavy foot down on the gas. "This is one way we can be sure that we're not being fooled," says Dartmouth College physicist Robert Caldwell.

The detective work is far from over, but at least cosmologists know they're hot on the trail of the elusive dark energy. "We still have a long way to go in understanding the onset and evolution of acceleration," says University of Chicago physicist Sean Carroll. "A lot of effort will be going into this problem — it's by far the biggest puzzle in cosmology today."
0

JOIN THE DISCUSSION

Read and share your comments on this article
Comment on this article
Want to leave a comment?
Only registered members of Astronomy.com are allowed to comment on this article. Registration is FREE and only takes a couple minutes.

Login or Register now.
0 comments
ADVERTISEMENT

FREE EMAIL NEWSLETTER

Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter.

ADVERTISEMENT
ADVERTISEMENT
BoxProductcovernov

Click here to receive a FREE e-Guide exclusively from Astronomy magazine.

Find us on Facebook

Loading...