Mashable 03月27日
Webb telescope captures weird auroras on Neptune for the first time
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詹姆斯·韦伯空间望远镜(JWST)首次清晰捕捉到海王星的极光景象,揭示了其独特的发光特征。不同于其他行星的极光,海王星的极光出现在其中纬度,而非两极。通过JWST的观测,科学家们不仅发现了海王星极光中存在的三氢阳离子,还观察到海王星大气层在过去三十多年中急剧降温,这与极光的微弱有关。这些发现为研究海王星的磁场和大气层变化提供了新的线索。

🌌 海王星极光新发现:JWST首次清晰捕捉到海王星极光,显示其位于行星的中纬度区域,而非两极,这与地球等行星的极光现象大相径庭。

✨ 关键分子确认:JWST探测到海王星极光中存在三氢阳离子,这与在其他气态巨行星极光中发现的分子相同,证实了相同的物理过程正在海王星上发生。

🌡️ 大气层温度变化:JWST观测到海王星大气层在过去34年里急剧降温,温度下降数百摄氏度,这可能是导致海王星极光难以被探测到的原因之一。

🔄 磁场倾斜与偏移:海王星的磁场相对于其自转轴倾斜47度,并偏离行星中心,这可能是导致极光位置异常的原因。

🔭 未来研究方向:科学家计划利用JWST继续研究海王星,探索其磁场倾斜的原因,以及大气层温度变化的背后机制,以更好地理解这颗遥远行星的奥秘。

Even at Neptune's incredible distance from the sun, astronomers have long suspected it has auroras, though they had never seen them until now. 

The James Webb Space Telescope, a collaboration of NASA and its Canadian and European space agency counterparts, has finally captured clear images of these magnificent Neptunian light shows. 

"As a long-time Neptunophile, anticipation of these images was one of the key reasons I became a JWST Interdisciplinary Scientist," said Heidi Hammel, a Neptune expert, in a post on X. "Kudos to the team for realizing my dream!"

But Webb's observations didn't just provide new pretty pictures of the ice giant planet's greenish-blue splotches. It revealed how odd Neptune's auroras are compared to other planets', glowing over its midriff rather than its poles. The new research was published in Nature Astronomy.

With Hubble and the James Webb space telescopes' data combined, right, Neptune's auroras are revealed in greenish-blue splotches. Credit: NASA / ESA / CSA / STScI / Heidi Hammel / Henrik Melin / Leigh Fletcher / Stefanie Milam

Neptune, at some 3 billion miles from the sun, is a dark, blustery world, whipped by winds faster than the speed of sound. As the most distant planet in the solar system, it only receives a dim twilight's worth of sunshine at its high noon. It takes about 165 years for the ice giant to make one loop around our star, and it's not visible to the naked eye from Earth. 

For three decades, scientists have studied how Jupiter, Saturn, and Uranus interact with space by looking at light emitted from charged molecules in their upper atmospheres. When the sun blasts out radiation, charged particles travel along a planet's invisible magnetic field lines. When these particles strike gases, they heat up and glow. The results are colorful light displays. 

On Earth, the colors differ depending on the type of atmospheric gas and its altitude. Oxygen glows red or blue, while nitrogen can create green, blue, or pink. The recent strong solar storm conditions — a byproduct of the sun being at solar maximum — are causing auroras around the North Pole to sprawl, allowing people who live farther south to see them. 

Similar to storm seasons on Earth, the sun experiences a weather pattern that repeats every 11 years. At the beginning and end of this cycle, the activity is at its calmest. But solar activity increases, climaxing in the middle of the cycle and causing the sun to roil with giant eruptions.

NASA's Voyager 2 mission, the only spacecraft to visit Neptune, was unable to get a clear picture of the planet's auroras in 1989. Credit: NASA illustration

NASA’s Voyager 2 spacecraft found hints of auroras on Neptune in 1989, but scientists couldn’t get a clear picture then. Using Webb’s near-infrared instrument in June 2023, they not only got the shots but also discovered the key molecule found in auroras of the other gas giants, called trihydrogen cation. That detection confirms the same processes are occurring on Neptune. 

Webb has filled in many gaps left by Voyager 2, the only spacecraft to visit the planet. In 2022, the telescope captured Neptune's ghostly rings and revealed a band of clouds around a known vortex at the planet's south pole for the first time.

But the Voyager 2 mission did discover the strange nature of Neptune's magnetic field, tilted at a steep angle. Unlike Earth’s steady magnetic field, Neptune’s shifts and twists. Because auroras occur where magnetic fields converge with a planet's atmosphere, Neptune's are far from its poles. 

"Neptune's aurora shines over latitudes comparable to South America on Earth," Hammel said. "This is because Neptune's magnetic field is seriously tilted from the planet's rotation axis (by 47 degrees!) and offset from the center of the planet (by half a planetary radius!)."

The James Webb Space Telescope is advancing astronomers' knowledge of Neptune, such as revealing the planet's ghostly rings in 2022. Credit: NASA / ESA / CSA / STScI

Voyager 2 also took Neptune's upper atmosphere temperature. Webb scientists were surprised to learn that the planet has cooled over the past 34 years by hundreds of degrees. It's now about half as warm as it was in 1989. 

This extreme plunge may have something to do with why Neptune’s auroras have been so hard to detect. Scientists had assumed they would be as bright as those on some other planets, but the colder atmosphere likely made them fainter. The finding also suggests that Neptune's atmosphere changes more frequently than its seasons, which last about 40 years, and perhaps even the solar cycle. This means some other mysterious forces are at play that they'd like to get to the bottom of. 

Astronomers plan to use Webb to continue studying Neptune over a full solar cycle. They hope to figure out why Neptune's magnetic field is so tilted and what caused it.

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海王星 极光 詹姆斯·韦伯空间望远镜 天文学
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