Mashable 01月15日
Webb sees shockwave continuing hundreds of years after supernova blast
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科学家利用詹姆斯·韦伯太空望远镜探测到一颗超新星爆炸后遗留的冲击波,该冲击波在数百年后仍然在星际空间中回荡。这个冲击波如同宇宙中的手电筒,照亮了原本神秘的星际物质,揭示了其从未被观测到的细节。研究人员发现星际物质呈现出类似洋葱的层状结构,并包含密度较高的尘埃区域。这种现象被称为光回波,当冲击波穿过星际云时,会使尘埃发出红外光,从而被韦伯望远镜捕捉到。这一发现有助于我们理解星系的结构和恒星的生命周期。

🔭 詹姆斯·韦伯太空望远镜捕捉到超新星冲击波在星际空间中回荡的现象,如同宇宙中的手电筒,揭示了星际物质的细节。

🧅 研究发现星际物质呈现出类似洋葱的层状结构,其中包含密度较高的尘埃区域,这为研究星际物质的内部结构提供了新的视角。

✨ 超新星冲击波穿过星际云时,会使尘埃发出红外光,这种现象被称为光回波,韦伯望远镜能够捕捉到这些红外光,从而揭示了星际尘埃的分布和性质。

🧲 研究人员还发现星际介质中存在令人惊讶的微小、片状结构和致密结,这些结构被认为与磁场有关,这为研究星际磁场提供了新的线索。

Scientists have probed the remains of a star that died in a violent supernova and discovered that its shockwave continued reverberating through space, hundreds of years later.

That shockwave eventually reached interstellar space, the medium that fills regions between stars. Researchers used the James Webb Space Telescope, a collaboration of NASA and its European and Canadian counterparts, to find that the ancient pulse, like a cosmic flashlight, had lit up never-before-seen details in the otherwise mysterious material.

"We see layers like an onion," said Josh Peek of the Space Telescope Science Institute in Baltimore, a member of the research team, in a statement. "We think every dense, dusty region that we see, and most of the ones we don’t see, look like this on the inside. We just have never been able to look inside them before."

The James Webb Space Telescope's ability to detect light at infrared wavelengths allowed scientists to see the effects of a supernova shockwave on interstellar space. Credit: NASA GSFC / CIL / Adriana Manrique Gutierrez illustration

Interstellar space is full of gas and dust clouds, but they're often invisible unless something illuminates them. This interstellar material is thought to consist of several elements: leftover ingredients from galaxy formation, star debris, and the building blocks for future stars and planets. Scientists want to study this stuff to understand the structure of galaxies and the life cycles of stars.

The shockwave Webb studied emerged from Cassiopeia A, now a neutron star, about 11,000 light-years from Earth. After the massive star collapsed, the pulse surged from its core outward, shooting X-rays and ultraviolet light through space. 

Some 350 years later, it traveled through interstellar clouds, causing them to glow in infrared light. The phenomenon is what's known as a light echo. Light echoes at visible wavelengths are due to light reflecting off interstellar material. Light echoes at infrared wavelengths are caused when energetic radiation warms dust that then glows. The latter are rare because they require a special kind of supernova to occur, astronomers say.

Webb was built to detect invisible light at infrared wavelengths. Dust and gas in space obscure the view to extremely distant and inherently dim light sources, but infrared waves can pierce through the clouds. One Webb scientist likened the strength of the telescope to being able to sense the heat of a single bumblebee on the moon.

The new images have allowed astronomers to map the 3D structure of interstellar gas and dust for the first time. In particular, the researchers learned that the interstellar medium had surprisingly small, sheet-like features and dense knots. Both are thought to be related to magnetic fields. 

The findings were presented at the 245th meeting of the American Astronomical Society in Maryland.

"Even as a star dies," said outgoing NASA administrator Bill Nelson, "its light endures — echoing across the cosmos."

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超新星 冲击波 星际空间 詹姆斯·韦伯太空望远镜 光回波
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