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Scientists Discover a New Kind of Star Explosion
Scientists who study stars have detected a previously1 unknown kind of event called a micronova.
The event involves thermonuclear explosions that take place on a star called a white dwarf2. The explosions happen because the white dwarf's gravity has pulled material from a companion star.
Astronomers4 said recently that a micronova is by far the least powerful kind of star explosion now known.
Micronovae are observed from Earth as bursts of light lasting5 about 10 hours. They have been documented on three white dwarf stars: one 1,680 light years away from Earth, one 3,720 light years away, and one 4,900 light years away. A light year is the distance light travels in one year.
Simone Scaringi of Durham University in England was the lead writer of the study that appeared in the publication Nature.
"The discovery was an unexpected surprise," Scaringi said. He added that finding these events "requires looking at the right place at the right time."
White dwarf stars are among the densest6 objects in the universe. They result from the collapse7 of a dying star's core. They have the mass of our sun but are about the size of Earth. Most stars, including the sun, will end their existence in this way.
Some white dwarfs8 are part of what is called a binary9 system, meaning that they are in an orbit with another star.
Micronovae happen in special binary systems with a white dwarf star possessing a strong magnetic field and a low-mass normal star. The white dwarf's gravity can pull hydrogen gas from the companion star's surface. The hydrogen then flows toward the white dwarf's magnetic poles.
At the white dwarf's poles, the pressure and temperature rise. This causes thermonuclear fusion10 that converts hydrogen into helium and releases energy.
"...This fusion is explosive, and the micronova occurs: a thermonuclear 'bomb' goes off," said astronomer3 Paul Groot who helped write the study.
The explosion is not widespread and does not destroy the white dwarf. In fact, micronova events can repeat many times.
"Only a very small percentage of the white dwarf participates in this explosion, roughly about one millionth of the surface area...this would be an area of about, say, the city of London," Groot added.
Each micronova event burns through material equal to one large asteroid11, or just over one millionth of Earth's mass, Scaringi said.
A micronova is similar to a nova, a thermonuclear explosion involving a whole star. With novae, the white dwarf does not have a strong magnetic field, meaning that hydrogen stolen from the companion star is spread rather than staying at the poles. Novae can last for weeks or months, burning through about a million times more mass than micronovae, Scaringi said.
The researchers discovered the micronovae when examining data from NASA's TESS space telescope. They used the European Southern Observatory's Very Large Telescope in Chile to confirm the explosions involving white dwarfs.
There are other kinds of star explosions as well. A kilonova takes place when two neutron12 stars or a neutron star and a black hole merge13. A hypernova is a kind of supernova involving a large star exploding at the end of its life and collapsing14 to form a black hole. And a luminous15 red nova involves two stars merging16.
Words in This Story
thermonuclear – adj. Of or relating to transformations17 in the nuclei18 of atoms of low atomic weight (such as hydrogen)
companion – n. a celestial19 body that appears close to another but that may or may not be associated with it in space
astronomer –n. a scientist who studies stars, planets and objects in outer space
burst –n. a short period of producing something suddenly
merge – v. to become combined into one
1 previously | |
adv.以前,先前(地) | |
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2 dwarf | |
n.矮子,侏儒,矮小的动植物;vt.使…矮小 | |
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3 astronomer | |
n.天文学家 | |
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4 astronomers | |
n.天文学者,天文学家( astronomer的名词复数 ) | |
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5 lasting | |
adj.永久的,永恒的;vbl.持续,维持 | |
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6 densest | |
密集的( dense的最高级 ); 密度大的; 愚笨的; (信息量大得)难理解的 | |
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7 collapse | |
vi.累倒;昏倒;倒塌;塌陷 | |
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8 dwarfs | |
n.侏儒,矮子(dwarf的复数形式)vt.(使)显得矮小(dwarf的第三人称单数形式) | |
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9 binary | |
adj.二,双;二进制的;n.双(体);联星 | |
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10 fusion | |
n.溶化;熔解;熔化状态,熔和;熔接 | |
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11 asteroid | |
n.小行星;海盘车(动物) | |
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12 neutron | |
n.中子 | |
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13 merge | |
v.(使)结合,(使)合并,(使)合为一体 | |
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14 collapsing | |
压扁[平],毁坏,断裂 | |
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15 luminous | |
adj.发光的,发亮的;光明的;明白易懂的;有启发的 | |
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16 merging | |
合并(分类) | |
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17 transformations | |
n.变化( transformation的名词复数 );转换;转换;变换 | |
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18 nuclei | |
n.核 | |
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19 celestial | |
adj.天体的;天上的 | |
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