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Scientists have released new information about an area around a bright star called Fomalhaut in the Milky1 Way galaxy2. The observations, made by the James Webb Space Telescope, provide details about three rings, or belts, of debris3 orbiting Fomalhaut.
Fomalhaut, one of the brightest stars in our night sky, is about 25 light years from Earth. A light year is the distance light travels in a year, about 9.5 trillion kilometers.
Researchers first discovered a belt of debris around Fomalhaut in 1983. The Webb found two other rings nearer to the star - a bright inner one and a narrow middle one.
These three belts appear to be populated by solid objects called planetesimals. Some planetesimals are thought to join together early in a star system's history to form planets, while others remain as debris like asteroids5 and comets.
Andras Gaspar of the University of Arizona was the lead author of the study published in Nature Astronomy.
"Much like our solar system, other planetary systems harbor disks of asteroids and comets - leftover6 planetesimals from the epoch7 of planet formation - that continuously grind themselves down" during collisions, he said.
Fomalhaut is 16 times brighter than the sun and almost twice as massive. It is about 440 million years old - less than a tenth the age of the sun - but is probably almost halfway8 through its life.
The three belts surround Fomalhaut from as far as 23 billion kilometers away. That is about 150 times the distance of Earth to the sun.
While no planets have been discovered yet around Fomalhaut, the researchers suspect the belts were created by gravitational forces of planets. Our solar system has two such belts - the main asteroid4 belt between Mars and Jupiter, and the Kuiper belt beyond Neptune9.
The gravitational influence of Jupiter, our solar system's largest planet, affects the main asteroid belt. Neptune's gravitational influence shapes the inner edge of the Kuiper belt.
Gaspar said that observations of Fomalhaut suggest the presence of a huge icy planet in the system.
Debris belts could offer information about planetary beginnings.
"Understanding this formation process requires a complete understanding of how these disks form and evolve," said study co-author Schuyler Wolff.
There are many open questions about the dust in the disks, the scientist added. Debris disks are the remains10 of a planet formation process, Wolff said, so their structure can provide valuable information about the underlying11 planet population and history.
Words in This Story
debris – n. : the pieces that are left after something has been destroyed
harbor – v. to hold or contain (something)
epoch – n. an event or a time marked by an event that begins a new period or development
disk – n. a shape that is flat and round in appearance
grind – v. to crush or break (something) into very small pieces
1 milky | |
adj.牛奶的,多奶的;乳白色的 | |
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2 galaxy | |
n.星系;银河系;一群(杰出或著名的人物) | |
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3 debris | |
n.瓦砾堆,废墟,碎片 | |
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4 asteroid | |
n.小行星;海盘车(动物) | |
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5 asteroids | |
n.小行星( asteroid的名词复数 );海盘车,海星 | |
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6 leftover | |
n.剩货,残留物,剩饭;adj.残余的 | |
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7 epoch | |
n.(新)时代;历元 | |
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8 halfway | |
adj.中途的,不彻底的,部分的;adv.半路地,在中途,在半途 | |
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9 Neptune | |
n.海王星 | |
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10 remains | |
n.剩余物,残留物;遗体,遗迹 | |
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11 underlying | |
adj.在下面的,含蓄的,潜在的 | |
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