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ANNOUNCER:
EXPLORATIONS -- a program in Special English by the Voice of America.
(MUSIC)
Today, Richard Rael and Tony Riggs tell the story of American astronomer1 Edwin Hubble. He changed our ideas about the universe and how it developed.
Edwin Hubble made his most important discoveries in the nineteen twenties. Today, other astronomers2 continue the work he began. Many of them are using the Hubble space telescope that is named after him.
(MUSIC)
VOICE TWO:
Edwin Hubble
Edwin Powell Hubble was born in eighteen eighty-nine in Marshfield, Missouri. He spent his early years in the state of Kentucky. Then he moved with his family to Chicago, Illinois. He attended the University of Chicago. He studied mathematics and astronomy3.
Hubble was a good student. He was a good athlete, too. He was a member of the University of Chicago championship basketball team in nineteen-oh-nine. He also was an excellent boxer4. Several people urged him to train for the world heavyweight boxing championship after college. Instead, he decided5 to continue his studies. He went to Queen's College at Oxford6, England.
At Oxford, Hubble studied law. He was interested in British Common Law, because his family had come to America from England many years before. He spent three years at Oxford.
In nineteen thirteen, Hubble returned to the United States. He opened a law office in Louisville, Kentucky. After a short time, however, he decided he did not want to be a lawyer. He returned to the University of Chicago. There, once again, he studied astronomy.
VOICE ONE:
Hubble watched the night sky with instruments at the university's Yerkes Observatory7. His research involved a major question astronomers could not answer: What are nebulae?
The astronomical9 term "nebulae", Hubble explained, had come down through the centuries. It was the name given to permanent, cloudy areas in the sky outside our solar system. Some astronomers thought nebulae were part of our Milky10 Way Galaxy11. Others thought they were island universes farther away in space.
In his research paper, Hubble said the issue could be decided only by more powerful instruments. And those instruments had not yet been developed.
VOICE TWO:
In nineteen seventeen, the United States was fighting in World War One in Europe. Edwin Hubble joined the American army and served in France.
Earlier, astronomer George Ellery Hale had offered Hubble a position at the Mount12 Wilson Observatory in southern California. When Hubble returned to the United States after World War One, he accepted Hale's offer. Hubble was thirty years old. He was just beginning the work that would make him famous.
VOICE ONE:
Edwin Hubble
In his first observations from Mount Wilson, Hubble used a telescope with a mirror one hundred fifty-two centimeters across. He studied objects within our own galaxy. And he made an important discovery about nebulae.
Hubble said the light that appeared to come from nebulae really came from stars near the nebulae. The nebulae, he said, were clouds of atoms and dust. They were not hot enough -- like stars-- to give off light.
Soon after, Hubble began working with a larger and more powerful telescope at Mount Wilson. Its mirror was two hundred fifty centimeters across. It was the most powerful telescope in the world for twenty-five years. It had the power Hubble needed to make his major discoveries.
VOICE TWO:
From nineteen twenty-two on, Edwin Hubble began examining more and more distant objects. His first great discovery was made when he recognized a Cepheid variable star. It was in the outer area of the great nebula8 called Andromeda. Cepheid variable stars are stars whose brightness13 changes at regular periods.
An astronomer at Harvard College, Henrietta Leavitt, had discovered that these periods of brightness could be used to measure the star's distance from Earth. Hubble made the measurements. They showed that the Andromeda nebula lay far outside our Milky Way Galaxy.
Hubble's discovery ended a long dispute. He proved wrong those who believed nebulae lay inside the Milky Way. And he proved that nebulae were galaxies14 themselves. Astronomers now agree that far distant galaxies do exist.
VOICE ONE:
A NASA image of the Andromeda Galaxy
Hubble then began to observe more details about galaxies. He studied their shape and brightness. By nineteen twenty-five, he had made enough observations to say that the universe is organized into galaxies of many shapes and sizes.
As stars differ from one another, he said, so do galaxies. Some are spiral15 galaxies like the Milky Way and Andromeda. They have a center, and arms of matter that seem to circle the center like a pinwheel. Others are shaped like baseballs or eggs. A few have no special shape.
VOICE TWO:
Hubble proposed a system to describe galaxies by their shape. His system still is used today. He also showed that galaxies are similar in the kinds of bright objects they contain. All galaxies, he said, are related to each other, much as members of a family are related to each other.
In the late nineteen twenties, Hubble studied the movement of galaxies through space. His investigation16 led to the most important astronomical discovery of the Twentieth century -- the expanding universe.
VOICE ONE:
Earlier observations about the movement of galaxies had been done by V. M. Silpher. He discovered that galaxies are moving away from Earth at speeds between three hundred kilometers a second and one thousand eight hundred kilometers a second.
Hubble understood the importance of Silpher's findings. He developed a plan for measuring both the distance and speed of as many galaxies as possible. With his assistant at Mount Wilson, Milton Humason, Hubble measured the movement of galaxies. The two men did this by studying what Hubble called the "red shift." It also is known as the "Doppler effect."
The Doppler effect explains changes in the length of light waves or sound waves as they move toward you or away from you. Light waves from an object speeding away from you will stretch into longer wavelengths17. They appear red. Light waves from an object speeding toward you will have shorter wavelengths. They appear blue.
VOICE TWO:
Observations of forty-six galaxies showed Hubble that the galaxies were traveling away from Earth. The observations also showed that the speed was linked directly to the galaxies' distance from Earth. Hubble discovered that the farther away a galaxy is, the greater its speed. This scientific rule is called "Hubble's Law."
Hubble's discovery meant a major change in our idea of the universe. The universe had not been quiet and unchanging since the beginning of time, as many people had thought. It was expanding. And that, Hubble said, meant it probably began with an explosion of unimaginable force. The explosion often is called "the big bang."
VOICE ONE:
Hubble's work did not end with this discovery. He continued to examine galaxies. He continued to gain new knowledge about them. Astronomers from all over the world went to study with him.
Hubble left the Mount Wilson Observatory during World War Two. He did research for the United States War Department. He returned after the war. Then, he spent much of his time planning a new, much larger telescope in southern California. The telescope was completed in nineteen forty-nine. It had a mirror five hundred centimeters across. It was named after astronomer George Ellery Hale.
VOICE TWO:
Edwin Hubble was the first person to use the Hale Telescope. He died in nineteen fifty-three while preparing to spend four nights looking through the telescope at the sky.
Hubble's work led to new research on the birth of the universe. One astronomer said scientists have been filling in the details ever since. And, he said, there is a long way to go.
(MUSIC)
ANNOUNCER:
This Special English program was written by Marilyn Rice Christiano. Your narrators were Richard Rael and Tony Riggs. Listen again next week for another EXPLORATIONS program on the Voice of America.
1 astronomer | |
n.天文学家 | |
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2 astronomers | |
n.天文学者,天文学家( astronomer的名词复数 ) | |
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3 astronomy | |
n.天文学 | |
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4 boxer | |
n.制箱者,拳击手 | |
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5 decided | |
adj.决定了的,坚决的;明显的,明确的 | |
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6 Oxford | |
n.牛津(英国城市) | |
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7 observatory | |
n.天文台,气象台,瞭望台,观测台 | |
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8 nebula | |
n.星云,喷雾剂 | |
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9 astronomical | |
adj.天文学的,(数字)极大的 | |
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10 milky | |
adj.牛奶的,多奶的;乳白色的 | |
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11 galaxy | |
n.星系;银河系;一群(杰出或著名的人物) | |
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12 mount | |
n.山峰,乘用马,框,衬纸;vi.增长,骑上(马);vt.提升,爬上,装备 | |
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13 brightness | |
n.明亮,亮度,聪颖,光泽度,灯火通明 | |
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14 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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15 spiral | |
adj.螺旋的;n.螺旋(线);vi.盘旋上升(或下降) | |
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16 investigation | |
n.调查,调查研究 | |
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17 wavelengths | |
n.波长( wavelength的名词复数 );具有相同的/不同的思路;合拍;不合拍 | |
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