Mashable 09月05日
新生恒星的巨大影响
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詹姆斯·韦伯太空望远镜揭示了一个名为Pismis 24的年轻星团,该星团位于距离地球约5500光年的天蝎座。令人意外的是,这些年轻、质量巨大的恒星并非温顺的存在,而是通过其超热辐射和恒星风,强力地塑造着周围的环境,甚至阻碍了新恒星的形成。它们如同宇宙中的“推土机”,摧毁了可能用于孕育下一代恒星的气体和尘埃墙。这一发现挑战了人们对恒星诞生过程的传统认知,展示了年轻大质量恒星对宇宙演化的强大影响力。

💥 宇宙中的“破坏者”:与人们的普遍认知不同,新生恒星并非脆弱的存在,而是具有强大的影响力。位于天蝎座的Pismis 24星团中的年轻大质量恒星,通过其强烈的辐射和恒星风,正在积极地重塑周围的空间环境,甚至决定了新恒星的诞生地点。

💨 恒星风的“推土机”效应:这些年轻恒星释放出的超热辐射和恒星风具有惊人的强度,它们如同“推土机”一般,夷平了巨大的气体和尘埃墙。这些被摧毁的物质原本可能用于形成新的恒星,但现在却被新生恒星的力量所阻挡。

🌌 塔状尘埃结构揭示恒星影响:望远镜的图像清晰地展示了由热、年轻恒星塑造出的高耸的、手指状的尘埃和气体结构。这些结构指向恒星的源头,显示了恒星对周围物质的定向影响。其中最长的“手指”尖端,其宽度是太阳系的200多倍,这凸显了新生恒星力量的巨大。

🌟 Pismis 24-1的揭秘:星团中心曾被认为是已知最巨大的恒星Pismis 24-1,后被证实是由至少两颗恒星组成。这两颗恒星的质量分别是太阳的74倍和66倍,是迄今为止发现的最巨大、最明亮的恒星之一,它们的存在进一步印证了年轻大质量恒星的强大能量。

Despite what you might assume, newborn stars aren't dainty, fragile creatures of the cosmos. They terrorize the neighborhood, reshaping space around them and deciding where the next stars can — or can't — be born. 

Using the James Webb Space Telescope, scientists took an infrared image of a young star cluster called Pismis 24, a spot within the Lobster Nebula about 5,500 light-years away in the constellation Scorpius. NASA has described the dazzling scene of gas and dust as resembling glowing mountains, "kissed by wispy clouds." 

But this stellar nursery, according to recent observations, is anything but cute. Astronomers were surprised by how much influence these young, massive stars had on their surroundings. Webb revealed that their super-hot radiation and stellar winds are so intense, they're bulldozing enormous walls of gas and dust that could have otherwise been used to form other stars. 

"This dramatic scene captured by NASA’s James Webb Space Telescope looks like a fantastical tableau from J. R. R. Tolkien’s The Lord of the Rings," said the Space Telescope Science Institute in Baltimore, which runs the observatory on behalf of NASA. "But truth is even stranger than fiction." 

Webb, a joint partnership of NASA and its European and Canadian counterparts, blasted off on Christmas in 2021 and now circles the sun about 1 million miles from Earth. From the start, NASA said Webb would revolutionize our understanding of the universe. And it delivered: when scientists saw the very first images, one even admitted to having an "ugly cry" because they were so sharp and detailed.

In just a short time, Webb has kicked off what astronomers are calling a golden age of discovery. It’s looking back to less than 300 million years after the Big Bang, when the first stars and galaxies lit up, and it’s also peering into the atmospheres of far-flung planets. Pam Melroy, a former astronaut who served as deputy administrator for NASA during the Biden administration, said the telescope's reign will continue for a long time, carrying enough fuel to run for at least 20 years. 

The James Webb Space Telescope explores star cluster Pismis 24 and finds massive young stars have outsize influence on new star births. Credit: NASA GSFC / CIL / Adriana Manrique Gutierrez illustration

Astronomers didn't fully appreciate how much influence young stars have on their surroundings until Webb peered into this cluster, one of the closest regions to Earth of new massive stars. 

The image shows it clearly: Rather than star birth being a gentle process hidden in a nest of clouds, the massive babies act like tropical storms, violently disrupting their environments by igniting or shutting down star formation. Some of these newborns are nearly eight times hotter than the sun. 

The towering, fingerlike structures of dust and gas extend from the glowing wall of gas, pointing toward the hot, young stars that shaped them. New stars are emerging within. The tallest finger is enormous, with a tip more than 200 times as wide as our solar system, according to NASA. And this image is only a small section of the nebula, which extends far beyond this frame.

The image also reveals thousands of stars ranging in color and size. The ones showcasing six-point spikes — diffraction caused by how light bends around Webb's mirrors — are the most massive stars in the cluster. Perhaps thousands of smaller stars appear as white, yellow, or red, depending on their type and the amount of dust obscuring them. 

At the center of the cluster is Pismis 24-1. Scientists once thought this object was the most massive star they had ever observed. They later realized what appeared to be one mega star was at least two. Still, at 74 and 66 times heavier than the sun each, the two known stars that compose Pismis 24-1 are among the most massive and luminous ever discovered.

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詹姆斯·韦伯太空望远镜 恒星形成 Pismis 24 宇宙学 天文学 James Webb Space Telescope Star Formation Pismis 24 Cosmology Astronomy
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