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This is Scientific American's 60-Second Science. I'm Steve Mirsky. Got a minute?
You could think of it as the real dancing with the stars. Two white dwarf1 stars have been found twirling around each other to make a complete orbit in less than every 13 minutes. And they provide a chance to test ideas about general relativity and gravitational waves. The system is described in a paper accepted by the Astrophysical Journal Letters.
One of the stars is about the size of Earth, but has more than half the mass of the Sun. A penny as dense2 as the star would weigh half a ton here. The other star is about 60 times our size and has about half the mass of its companion.
Astronomers3 estimate that the partners will collide in about 900,000 years. At that time, they could form a stable binary4 star, or merge5 into a single, rapidly spinning white dwarf, or go supernova. In the meantime, they provide a place to look for gravitational waves. Because they're not exchanging mass now, gravitational waves should account for the loss of energy that brings them closer every year. Which for each of them around the other is just a few podcasts long.
Thanks for the minute. For Scientific American's 60-Second Science, I'm Steve Mirsky.
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1 dwarf | |
n.矮子,侏儒,矮小的动植物;vt.使…矮小 | |
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2 dense | |
a.密集的,稠密的,浓密的;密度大的 | |
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3 astronomers | |
n.天文学者,天文学家( astronomer的名词复数 ) | |
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4 binary | |
adj.二,双;二进制的;n.双(体);联星 | |
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5 merge | |
v.(使)结合,(使)合并,(使)合为一体 | |
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