Mashable 02月19日
Scientists just looked inside a truly sci-fi planet
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天文学家利用四架望远镜观测遥远行星WASP-121b,发现其大气层深处存在前所未有的活动。这颗行星形状像橄榄球,还会下宝石雨。研究揭示了WASP-121b大气层中独特的风层结构,包括底层的铁风、中层的快速钠射流和顶层的氢风。钠射流在行星的向阳面加速,引发强烈的风暴,远超太阳系中最强烈的飓风。这项研究挑战了我们对行星天气运作方式的理解,为未来的系外行星研究开辟了新的方向,未来将借助更大的望远镜探索更小的岩石行星。

🪐WASP-121b是一颗“热木星”系外行星,它被潮汐锁定,一面总是炙热,另一面则黑暗寒冷。天文学家通过观测其大气层,发现了前所未有的活动。

💨WASP-121b的大气层具有独特的层状结构,包括:底层是铁风,从行星面向恒星的一侧吹离;中层是快速移动的钠射流,速度超过行星自转速度;顶层是氢风。这种分层风结构在其他行星上从未见过。

🌪️钠射流在流入行星炎热的白昼一侧时会加速,扰乱大气层,并产生强烈的风暴。与太阳系中最强烈的飓风相比,这些风暴显得更为剧烈。

The distant world WASP-121b is already bizarre. It's football-shaped and rains gems.

Now, astronomers leveraged the power of four telescopes to observe what's transpiring deep inside this giant exoplanet's swirling atmosphere. They found never-before-seen activity.

"This planet’s atmosphere behaves in ways that challenge our understanding of how weather works — not just on Earth, but on all planets. It feels like something out of science fiction," Julia Victoria Seidel, a researcher at the European Southern Observatory who led the new research, said in a statement.

The research has been published in the peer-reviewed journal Nature.

WASP-121b is an exoplanet (meaning a world beyond our solar system) called a "hot Jupiter" because it's a gaseous giant that orbits close to its searing star. Crucially, the planet is tidally locked to its star — like the moon is locked to Earth — meaning that one side of WASP-121b is incessantly seared by its star, while the other is dark and cooler.

The combined light from four of the telescopes comprising the European Southern Observatory’s Very Large Telescope — located at 8,648 feet of elevation in the Chilean desert — observed WASP-121b, located some 900 light-years away in deep space (a single light-year is nearly 6 trillion miles). As the planet passed in front of its nearby star, the telescopes detected the starlight passing through WASP-121b's atmosphere, enabling the astronomers (with the help of an instrument called a spectrograph that can detect materials in far-off objects) to see different chemical elements moving through different atmospheric layers.

Because each layer in the planet's atmosphere hosts unique winds carrying different elements, the researchers could map an unprecedented 3D structure of an exoplanet's atmosphere.

As the graphic below shows, WASP-121b contains iron winds at its lowest known layer, which blow away from the point on the exoplanet where its extremely close star is located overhead. In the middle is a quickly moving jet stream of sodium, which moves faster than the planet rotates. Finally, the planet is topped with an upper layer of hydrogen winds.

"This kind of climate has never been seen before on any planet," Seidel explained.

"This kind of climate has never been seen before on any planet."

"It’s truly mind-blowing that we’re able to study details like the chemical makeup and weather patterns of a planet at such a vast distance," added Bibiana Prinoth, an astrophysicist at Lund Observatory who coauthored the research.

Planets like Earth and Jupiter have jet streams, too, but they don't contain this onion-like layer of rapidly moving winds.

A graphic showing the different layers of winds on WASP-121b. Credit: ESO / M. Kornmesser

That sodium jet stream is particularly potent. It accelerates as it flows into the planet's hot dayside, roiling the atmosphere and spawning potent storms.

"Even the strongest hurricanes in the Solar System seem calm in comparison," Seidel said.

With the bigger, looming telescopes of the future, exoplanet researchers plan to peer into much smaller, rocky worlds — perhaps somewhat like Earth. The Extremely Large Telescope (ELT) — packing a 128-foot-wide mirror that will make it the world's largest visible and infrared light telescope — is under construction and slated to start operating in 2028 atop Chile's Atacama Desert.

What will we find in the clouds of more alien worlds?

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WASP-121b 系外行星 大气层 天文学
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