航空宇宙局 明らかにする／漏らすs how the sun will look when it DIES

By SAM TONKIN

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This image, captured by NASA's James Webb Space Telescope (JWST), reveals the final stages of a distant star's life, offering a glimpse into our own sun's future in about 5 billion years. The picture showcases the Ring Nebula (Messier 57), a captivating doughnut-like structure of glowing gas, located around 2,600 light-years from Earth. Formed from a dying star's ejected layers, the cosmic masterpiece's unique structure and vibrant colors are on display, with new details in its outer regions revealed by JWST's different camera.

This image, 逮捕（する）d by 航空宇宙局's James Webb Space Telescope (JWST), 明らかにする／漏らすs the final 行う／開催する／段階s of a distant 星／主役にする's life, 申し込む／申し出ing a glimpse into our own sun's 未来 in about 5 billion years. The picture showcases the （犯罪の）一味 星雲 (Messier 57), a captivating doughnut-like structure of glowing gas, 位置を示すd around 2,600 light-years from Earth. Formed from a dying 星／主役にする's 排除する／（飛行機などから）緊急脱出するd 層s, the cosmic masterpiece's unique structure and vibrant colors are on 陳列する，発揮する, with new 詳細（に述べる）s in its outer 地域s 明らかにする／漏らすd by JWST's different camera.?

"This image from James Webb's MIRI reveals new details beyond what NIRCam could capture," said Prof. Mike Barlow from University College London, the JWST Ring Nebula Project lead. The arcs in the image formed during the star's red giant phase, caused by a low-mass companion star with an eccentric orbit passing by every 280 years. Webb's images showcase the Ring Nebula's intricate structures, offering unprecedented detail of its rings, bubbles, and wispy clouds.

"This image from James Webb's MIRI 明らかにする／漏らすs new 詳細（に述べる）s beyond what NIRCam could 逮捕（する）," said Prof. マイク Barlow from University College London, the JWST （犯罪の）一味 星雲 事業／計画（する） lead. The arcs in the image formed during the 星／主役にする's red 巨大（な） 段階, 原因（となる）d by a low-集まり companion 星／主役にする with an eccentric 軌道 passing by every 280 years. Webb's images showcase the （犯罪の）一味 星雲's intricate structures, 申し込む／申し出ing 前例のない 詳細（に述べる） of its （犯罪の）一味s, 泡s, and wispy clouds.?

The main nebula ring comprises 20,000 dense molecular hydrogen clumps, Earth-sized each. Webb's MIRI image showed 10 concentric arcs beyond it, forming every 280 years. These likely emerged from the red giant's interaction with a distant companion star, akin to Pluto's distance from our sun. Dr. Roger Wesson of Cardiff University noted, 'Our MIRI images unveiled the faint halo with unprecedented clarity, revealing regularly spaced concentric features previously unseen due to telescope limitations.'

The main 星雲 （犯罪の）一味 構成するs 20,000 dense molecular hydrogen clumps, Earth-sized each. Webb's MIRI image showed 10 concentric arcs beyond it, forming every 280 years. These likely 現れるd from the red 巨大（な）'s interaction with a distant companion 星／主役にする, akin to Pluto's distance from our sun. Dr. Roger Wesson of Cardiff University 公式文書，認めるd, 'Our MIRI images 明かすd the faint halo with 前例のない clarity, 明らかにする／漏らすing 定期的に spaced concentric features 以前 unseen 予定 to telescope 制限s.'?

By studying the Ring Nebula's images, researchers aim to comprehend its formation and evolution processes. Messier 57 in the Lyra constellation captivates stargazers with its doughnut-like glowing gas structure. Planetary nebulae like this are alluring due to their varied shapes, including radiant rings, expanding bubbles, and intricate clouds. These objects emit specific colored light due to diverse chemical elements, enabling detailed studies of their chemical evolution. In about five billion years, our sun is expected to become a red giant star, vastly larger than its current size.

By 熟考する／考慮するing the （犯罪の）一味 星雲's images, 研究員s 目的（とする） to comprehend its 形式 and 進化 過程s. Messier 57 in the Lyra 星座 captivates stargazers with its doughnut-like glowing gas structure. Planetary 星雲 like this are alluring 予定 to their 変化させるd 形態／調整s, 含むing radiant （犯罪の）一味s, 拡大するing 泡s, and intricate clouds. These 反対するs 放出する 明確な／細部 colored light 予定 to diverse 化学製品 elements, enabling 詳細（に述べる）d 熟考する／考慮するs of their 化学製品 進化. In about five billion years, our sun is 推定する／予想するd to become a red 巨大（な） 星／主役にする, vastly larger than its 現在の size.?

In the future, our sun will expel gas and dust, forming an 'envelope' that might account for half its mass. The core will become a white dwarf star, illuminating the envelope to create a ring-shaped planetary nebula like the Ring Nebula. This transformation could potentially affect life on Earth, and the survival of the rocky core remains uncertain. Launched on Christmas Day 2021, Webb aims to explore the universe's early history from the sun-Earth balance point called L2, using the infrared spectrum to peer through gas and dust clouds where stars form, providing insights into events shortly after the Big Bang. Read the full story:?https://www.dailymail.co.uk/sciencetech/article-12429133/How-sun-look-DIES-NASA-image-gives-glimpse-whats-store-home-star-dont-worry-weve-got-5-billion-years-left.html?ito=msngallery

In the 未来, our sun will 追放する gas and dust, forming an 'envelope' that might account for half its 集まり. The 核心 will become a white dwarf 星／主役にする, illuminating the envelope to create a （犯罪の）一味-形態／調整d planetary 星雲 like the （犯罪の）一味 星雲. This 変形 could 潜在的に 影響する／感情 life on Earth, and the 生き残り of the rocky 核心 remains uncertain. 開始する，打ち上げるd on Christmas Day 2021, Webb 目的（とする）s to 調査する the universe's 早期に history from the sun-Earth balance point called L2, using the infrared spectrum to peer through gas and dust clouds where 星／主役にするs form, 供給するing insights into events すぐに after the Big Bang. Read the 十分な story:?https://www.dailymail.co.uk/sciencetech/article-12429133/How-sun-look-DIES-航空宇宙局-image-gives-glimpse-whats-蓄える／店-home-星／主役にする-dont-worry-weve-got-5-billion-years-left.html?ito=msngallery?

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