New Satellite Data On Universe's First Trillionth Second

In summary, the WMAP team has found evidence that the universe underwent a rapid growth spurt in its first trillionth of a second, which is consistent with the theory of inflation.
  • #1
Silverbackman
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http://map.gsfc.nasa.gov/m_or/PressRelease_03_06.html

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, 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

Perhaps expansion has been going on forever and size isn't really an entity in terms of infinite mass.

Thoughts?
 
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  • #2
hey silverbackman

this article refers to the third year data release by the WMAP team. There have been a couple threads debating what, if any, new statements about the universe can be made from the refined data.

cheers
gabe
 
  • #3
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1. What is the significance of the universe's first trillionth second?

The first trillionth second of the universe refers to the earliest moments after the Big Bang, when the universe was only one trillionth of a second old. This is a crucial time period for understanding the formation and evolution of the universe.

2. How did scientists gather satellite data from this time period?

Scientists gathered satellite data from the first trillionth second of the universe using the European Space Agency's Planck satellite. This satellite was specifically designed to study the cosmic microwave background radiation, which is the leftover radiation from the Big Bang.

3. What can the new satellite data tell us about the early universe?

The new satellite data can tell us about the temperature, density, and composition of the early universe. It can also provide insights into the structure and evolution of the universe, including the formation of galaxies and the distribution of dark matter.

4. How does this new data impact our understanding of the Big Bang theory?

This new data significantly strengthens the evidence for the Big Bang theory, which is the prevailing scientific explanation for the origins of the universe. It provides more precise measurements and further supports the idea that the universe began as a hot, dense, and expanding singularity.

5. What future research can be done using this satellite data?

Future research using this satellite data can focus on refining our understanding of the early universe and addressing remaining questions about the origins and evolution of the universe. This could include studying the polarization of the cosmic microwave background radiation and searching for evidence of cosmic inflation, which is the rapid expansion of the universe in its earliest moments.

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