Andrew Yee
March 17th 06, 07:39 PM
Office of News and Information
Johns Hopkins University
901 South Bond Street, Suite 540
Baltimore, Maryland 21231
Phone: 443-287-9960
Fax: 443-287-9920
CONTACT:
Lisa De Nike, (443) 287-9960
PRINCETON CONTACT:
Eric Quinones, (609) 258-5748
FOR IMMEDIATE RELEASE: March 16, 2006
New Satellite Data on Universe's First Trillionth Second
Scientists peering back to the oldest light in the universe have new
evidence for what happened within its first trillionth of a second, when
the universe suddenly grew from submicroscopic to astronomical size in far
less than a wink of the eye.
Using new data from a NASA satellite, scientists have the best evidence
yet to support this scenario, known as "inflation." The evidence, from the
Wilkinson Microwave Anisotropy Probe (WMAP) satellite, was gathered during
three years of continuous observations of remnant afterglow light --
cosmic background radiation that lingers, much cooled, from the universe's
energetic beginnings 13.7 billion years ago.
In 2003, NASA announced that the WMAP satellite had produced a detailed
picture of the infant universe by measuring fluctuations in temperature of
the afterglow -- answering many longstanding questions about the
universe's age, composition and development. The WMAP team has built upon
those results with a new measurement of the faint glare from the afterglow
to obtain clues about the universe's first moments, when the seeds were
sown for the formation of the first stars 400 million years later.
"It amazes me that we can say anything about what transpired within the
first trillionth of a second of the universe, but we can," said Charles
L. Bennett (pictured at right), WMAP principal investigator and a
professor in the Henry A. Rowland Department of Physics and Astronomy at
The Johns Hopkins University. "We have never before been able to
understand the infant universe with such precision. It appears that the
infant universe had the kind of growth spurt that would alarm any mom or
dad."
WMAP results have been submitted to the Astrophysical Journal and are
posted online at
http://wmap.gsfc.nasa.gov/results
The newly detected pattern, or polarization signal, in the glare of the
afterglow is the weakest cosmological signal ever detected -- less than a
hundredth of the strength of the temperature signal reported three years
ago. "This is brand new territory," said Princeton University physicist
Lyman Page, a WMAP team member. "We are quantifying the cosmos in a
different way to open up a new window for understanding the universe in
its earliest times."
Comparing the brightness of broad features to compact features in the
afterglow light (like comparing the heights of short-distance ripples
versus long-distance waves on a lake) helps tell the story of the infant
universe. One long-held prediction was that the brightness would be the
same for features of all sizes. In contrast, the simplest versions of
inflation predict that the relative brightness decreases as the features
get smaller. WMAP data are new evidence for the inflation prediction.
The new WMAP data, combined with other cosmology data, also support
established theories on what has happened to matter and energy over the
past 13.7 billion years since its inflation, according to the WMAP
researchers. The result is a tightly constrained and consistent picture of
how our universe grew from microscopic quantum fluctuations to enable the
formation of stars, planets and life.
According to this picture, researchers say that only 4 percent of the
universe is ordinary familiar atoms; another 22 percent is an as-yet
unidentified dark matter, and 74 percent is a mysterious dark energy. That
dark energy is now causing another growth spurt for the universe,
fortunately, they say, more gentle than the one 13.7 billion years ago.
WMAP was launched on June 30, 2001, and is now a million miles from Earth
in the direction opposite the sun. It is able to track temperature
fluctuations at levels finer than a millionth of a degree.
The WMAP team includes researchers at the Goddard Space Flight Center in
Greenbelt, Md.; The Johns Hopkins University; Princeton University; the
Canadian Institute of Theoretical Astrophysics in Toronto; the University
of Texas at Austin; Cornell University; the University of Chicago; Brown
University in Providence, R.I.; the University of British Columbia; the
University of Pennsylvania; and the University of California, Los Angeles.
For images and more information:
http://wmap.gsfc.nasa.gov/results
Johns Hopkins University
901 South Bond Street, Suite 540
Baltimore, Maryland 21231
Phone: 443-287-9960
Fax: 443-287-9920
CONTACT:
Lisa De Nike, (443) 287-9960
PRINCETON CONTACT:
Eric Quinones, (609) 258-5748
FOR IMMEDIATE RELEASE: March 16, 2006
New Satellite Data on Universe's First Trillionth Second
Scientists peering back to the oldest light in the universe have new
evidence for what happened within its first trillionth of a second, when
the universe suddenly grew from submicroscopic to astronomical size in far
less than a wink of the eye.
Using new data from a NASA satellite, scientists have the best evidence
yet to support this scenario, known as "inflation." The evidence, from the
Wilkinson Microwave Anisotropy Probe (WMAP) satellite, was gathered during
three years of continuous observations of remnant afterglow light --
cosmic background radiation that lingers, much cooled, from the universe's
energetic beginnings 13.7 billion years ago.
In 2003, NASA announced that the WMAP satellite had produced a detailed
picture of the infant universe by measuring fluctuations in temperature of
the afterglow -- answering many longstanding questions about the
universe's age, composition and development. The WMAP team has built upon
those results with a new measurement of the faint glare from the afterglow
to obtain clues about the universe's first moments, when the seeds were
sown for the formation of the first stars 400 million years later.
"It amazes me that we can say anything about what transpired within the
first trillionth of a second of the universe, but we can," said Charles
L. Bennett (pictured at right), WMAP principal investigator and a
professor in the Henry A. Rowland Department of Physics and Astronomy at
The Johns Hopkins University. "We have never before been able to
understand the infant universe with such precision. It appears that the
infant universe had the kind of growth spurt that would alarm any mom or
dad."
WMAP results have been submitted to the Astrophysical Journal and are
posted online at
http://wmap.gsfc.nasa.gov/results
The newly detected pattern, or polarization signal, in the glare of the
afterglow is the weakest cosmological signal ever detected -- less than a
hundredth of the strength of the temperature signal reported three years
ago. "This is brand new territory," said Princeton University physicist
Lyman Page, a WMAP team member. "We are quantifying the cosmos in a
different way to open up a new window for understanding the universe in
its earliest times."
Comparing the brightness of broad features to compact features in the
afterglow light (like comparing the heights of short-distance ripples
versus long-distance waves on a lake) helps tell the story of the infant
universe. One long-held prediction was that the brightness would be the
same for features of all sizes. In contrast, the simplest versions of
inflation predict that the relative brightness decreases as the features
get smaller. WMAP data are new evidence for the inflation prediction.
The new WMAP data, combined with other cosmology data, also support
established theories on what has happened to matter and energy over the
past 13.7 billion years since its inflation, according to the WMAP
researchers. The result is a tightly constrained and consistent picture of
how our universe grew from microscopic quantum fluctuations to enable the
formation of stars, planets and life.
According to this picture, researchers say that only 4 percent of the
universe is ordinary familiar atoms; another 22 percent is an as-yet
unidentified dark matter, and 74 percent is a mysterious dark energy. That
dark energy is now causing another growth spurt for the universe,
fortunately, they say, more gentle than the one 13.7 billion years ago.
WMAP was launched on June 30, 2001, and is now a million miles from Earth
in the direction opposite the sun. It is able to track temperature
fluctuations at levels finer than a millionth of a degree.
The WMAP team includes researchers at the Goddard Space Flight Center in
Greenbelt, Md.; The Johns Hopkins University; Princeton University; the
Canadian Institute of Theoretical Astrophysics in Toronto; the University
of Texas at Austin; Cornell University; the University of Chicago; Brown
University in Providence, R.I.; the University of British Columbia; the
University of Pennsylvania; and the University of California, Los Angeles.
For images and more information:
http://wmap.gsfc.nasa.gov/results