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When the sun’s ultraviolet light hits Venus’ atmosphere, it breaks up large molecules1 into fragments. As those atoms recombine later, some of their energy is released as light. If they recombine on Venus’ night side in large enough amounts, the glow can be detected. So far, scientists have found nitric oxide2, oxygen, and hydroxyl radicals3 glowing at altitudes between 55 and 75 miles. So, if I had a big telescope and looked at Venus’ dark side, I’d be able to see it glowing? Well, no. The glow is in the infrared4, a part of the light spectrum5 human eyes can’t see. But we’re lucky that we have Venus Express, a European spacecraft with VIRTIS, out there watching. VIRTIS? That's a Visible and Infrared Thermal6 Imaging Spectrophotometer. It can see infrared. If we can't see it, what's the point? Scientists are using the data to learn about the temperature, the wind direction, and the composition of Venus’ atmosphere. But they don’t understand everything. Sometimes different molecules glow simultaneously7, other times separately. They haven’t figured out why the glows happen when they do.
1 molecules | |
分子( molecule的名词复数 ) | |
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2 oxide | |
n.氧化物 | |
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3 radicals | |
n.激进分子( radical的名词复数 );根基;基本原理;[数学]根数 | |
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4 infrared | |
adj./n.红外线(的) | |
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5 spectrum | |
n.谱,光谱,频谱;范围,幅度,系列 | |
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6 thermal | |
adj.热的,由热造成的;保暖的 | |
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7 simultaneously | |
adv.同时发生地,同时进行地 | |
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