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By David McAlary
Washington
17 March 2006
Scientists report evidence that the universe was born in less than the blink of an eye, expanding instantly from sub-microscopic1 size to astronomical2 proportions. The conclusion comes from data gathered by a U.S. satellite that has been peering for clues to the origin of the cosmos3 in a faint glow of background radiation that is almost as old as the universe.
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Inflation means one thing to economists4 and another to cosmologists. When applied5 to the universe, it means the expansion from its tiny origins nearly 14 billion years ago.
Time line of the Universe
Now, scientists have a better idea of how fast this happened, thanks to a U.S. satellite orbiting four times farther than the moon. It is called the Wilkinson Microwave Anisotropy Probe, or WMAP for short, launched in 2001.
The probe's chief investigator6, astrophysicist Charles Bennett of The Johns Hopkins University in Baltimore, says the data reveal that the infant universe just popped out suddenly from almost nothing. It inflated7 from the size of a pea to a volume larger than all current observable space in less than one-trillionth of a second.
"It amazes me that we can say anything at all about what transpired8 in the first trillionth of a second, but we can," he said. "It appears that the universe had a growth spurt9 that would alarm any mom or dad."
This conclusion comes after three years of continuous observations of the oldest light in the universe. Bennett says it is the remnant afterglow of light that first appeared when the universe was just 300,000-years-old, a faint microscopic radiation that lingers at temperatures close to absolute zero, the temperature at which all atomic motion stops.
"WMAP measures the patterns of the light as a geologist10 might examine a fossil for clues of the past," he explained.
WMAP has produced a new, more detailed11 picture of the infant universe. Colors indicate "warmer" (red) and "cooler" (blue) spots
The WMAP results give the most detailed picture yet of the minute brightness and temperature variations in this light, heat differences of less than one-millionth of a degree. Those variations, first measured in the 1990s by a previous U.S. satellite, are microwave fossils revealing the emerging structure of the infant universe.
The slightly warmer, brighter regions represent areas where matter began clumping12 together, eventually growing into galaxies13, stars and planets. The cooler, darker areas were less dense14, becoming the space between these structures.
It is in these patterns that the researchers discerned the details of the universe's beginning, aided by a new map of the polarization, or direction, of the faint microwave radiation.
The WMAP researchers say their findings, combined with other cosmology information, support established theories on the universe's expansion. These theories hold that at the outset, short-lived bursts of energy at the atomic level were converted during the rapid inflation into the fluctuations15 of matter WMAP has measured more precisely16 than ever.
"WMAP has subjected our basic cosmological model to its most rigorous test and passed with flying colors," said Princeton University team member David Spergel.
Content of the Universe
The new data also inform scientists that only four-percent of the universe is ordinary matter that we can see. Twenty-two percent is unidentified dark matter, and 74 percent is a mysterious dark energy. This is a force scientists believe counters the gravitational pull of matter and is causing another rapid expansion of the universe, although not nearly as forceful as the first one.
"The observations are spectacular and the conclusions are stunning," he said.
This is Columbia University cosmology theorist Peter Greene, who was not part of the WMAP research team.
"Our species is one that seeks its origin, and the deepest of all questions of origin is, how did the universe begin? WMAP has certainly not answered this question, but WMAP's data is taking us one giant step closer to the answer by giving us a precise quantitative17 look at what happened literally18 at time zero itself," he said.
The WMAP data are to be published in the Astrophysical Journal. The WMAP satellite will continue to refine its data on a mission expected to last until 2009.
1 microscopic | |
adj.微小的,细微的,极小的,显微的 | |
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2 astronomical | |
adj.天文学的,(数字)极大的 | |
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3 cosmos | |
n.宇宙;秩序,和谐 | |
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4 economists | |
n.经济学家,经济专家( economist的名词复数 ) | |
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5 applied | |
adj.应用的;v.应用,适用 | |
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6 investigator | |
n.研究者,调查者,审查者 | |
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7 inflated | |
adj.(价格)飞涨的;(通货)膨胀的;言过其实的;充了气的v.使充气(于轮胎、气球等)( inflate的过去式和过去分词 );(使)膨胀;(使)通货膨胀;物价上涨 | |
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8 transpired | |
(事实,秘密等)被人知道( transpire的过去式和过去分词 ); 泄露; 显露; 发生 | |
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9 spurt | |
v.喷出;突然进发;突然兴隆 | |
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10 geologist | |
n.地质学家 | |
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11 detailed | |
adj.详细的,详尽的,极注意细节的,完全的 | |
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12 clumping | |
v.(树、灌木、植物等的)丛、簇( clump的现在分词 );(土、泥等)团;块;笨重的脚步声 | |
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13 galaxies | |
星系( galaxy的名词复数 ); 银河系; 一群(杰出或著名的人物) | |
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14 dense | |
a.密集的,稠密的,浓密的;密度大的 | |
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15 fluctuations | |
波动,涨落,起伏( fluctuation的名词复数 ) | |
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16 precisely | |
adv.恰好,正好,精确地,细致地 | |
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17 quantitative | |
adj.数量的,定量的 | |
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18 literally | |
adv.照字面意义,逐字地;确实 | |
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