打開一顆星看看

人類平均80年的生命裡，<br>或許沒機會親眼看見一顆恆星的殞落──超新星爆炸；<br>目前也尚未有技術探索恆星生命不同階段其內部的變化。<br>但藉由電腦運算模擬、調控不同的物理參數，<br>模擬天文學家們試著重現一顆顆恆星的爆炸過程。

展覽頁面呈現形式

橫式

策展者

陳科榮 [ASIAA 助研究員]

凡木文化（編輯）

陳文翊、歐柏昇（協力）

中研院數位文化中心（協辦）

展覽封面

f6e34495d4daa3683e20e815661df7bf

展覽資料

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"musicText": "", "musicURL": "" }, "basic-zazrn3ltmw": { "id": "basic-zazrn3ltmw", "type": "basic", "sortable": true, "primaryObj": { "oid": "8f9fe33df4f3ea189be05777b8f06266", "fileType": "video", "fileURI": "https://openmuseum.tw/muse_download/24a5f7ceceb8f256f1aecfa5f1ff4f0f", "level": "primary", "title": "磁星驅動超亮超新星動態影像", "desc": "超新星由於中子星（磁星）的能量產生第二次爆炸，這種超新星會形成很亮的光，此二維模擬的結構與蟹狀星雲相似。", "thumbURI": "https://openmuseum.tw/files/muse_portal/styles/square_thumbnail_100/public/externals/18f58d4a7b7988401e1d47069b9a61ae.jpg?itok=LhLf7axD", "thumbMediumURI": "https://openmuseum.tw/files/muse_portal/styles/thumbnail_medium/public/externals/18f58d4a7b7988401e1d47069b9a61ae.jpg?itok=6mxjvLxl", "thumbBigURI": "https://openmuseum.tw/files/muse_portal/styles/thumbnail_big/public/externals/18f58d4a7b7988401e1d47069b9a61ae.jpg?itok=zsm3yqMT", "background": "https://openmuseum.tw/files/muse_portal/styles/w1920/public/externals/18f58d4a7b7988401e1d47069b9a61ae.jpg?itok=d5rM5Wd5", "mfid": "24a5f7ceceb8f256f1aecfa5f1ff4f0f", "musicURL": "", "musicName": "", "fileCreator": "Ken Chen", "rights": "Ken Chen", "rightsLogo": "https://openmuseum.tw/files/muse_portal/styles/square_thumbnail_100/public/default_rights/memder_non-03.png?itok=h0rkcAOw", "fileLicence": "著作權利所有-可用於本站提供的服務", "fileDisableLink": 0, "sourceID": "", "creator": "", "fileOversize": false }, "title": "謎樣的超亮｜模擬磁星驅動超亮超新星爆炸", "desc": "運用二維（2D）模擬第一次超新星爆炸後形成於恆星中心的磁星，透過扭曲磁場產生強力的輻射，促成超新星的第二次爆炸。震波由左下的爆炸點向外傳遞的能量與密度的累積，造成恆星物質的流體不穩定性（瑞利-泰勒不穩定性 Rayleigh-Taylor Instability），解開其超亮的原因。<br>", "musicName": "無", "musicTip": "聽導覽", "weight": 16, "musicText": "", "musicURL": "" }, "highlight_basic-jkxmf1446m": { "id": "highlight_basic-jkxmf1446m", "type": "highlight_basic", "sortable": true, "primaryObj": { "oid": "ea4f66f3e583d71aaf5e138f44bf9954", "fileType": "image", "fileURI": "https://openmuseum.tw/files/muse_portal/muse_styles/w1024/mcode/5e7b588026f098f9fd76eef46d7a96a7.jpg?itok=UTtFvIQg", "level": "primary", "title": "蟹狀星雲與模擬超新星結構比較圖", "desc": "", "thumbURI": "https://openmuseum.tw/files/muse_portal/muse_styles/square_thumbnail_100/mcode/5e7b588026f098f9fd76eef46d7a96a7.jpg?itok=IufdzAEC", "thumbMediumURI": "https://openmuseum.tw/files/muse_portal/muse_styles/thumbnail_medium/mcode/5e7b588026f098f9fd76eef46d7a96a7.jpg?itok=BoxOZQiY", "thumbBigURI": "https://openmuseum.tw/files/muse_portal/muse_styles/thumbnail_big/mcode/5e7b588026f098f9fd76eef46d7a96a7.jpg?itok=VFvH3SMc", "background": "https://openmuseum.tw/files/muse_portal/muse_styles/w1920/mcode/5e7b588026f098f9fd76eef46d7a96a7.jpg?itok=Yj6A6GQ_", "mfid": "5e7b588026f098f9fd76eef46d7a96a7", "musicURL": "", "musicName": "", "fileCreator": "Ken Chen,陳文翊", "rights": "Ken Chen", "rightsLogo": "https://openmuseum.tw/files/muse_portal/styles/square_thumbnail_100/public/default_rights/memder_non-05.png?itok=0rVBS4da", "fileLicence": "著作權利所有-可用於本站提供的服務", "fileDisableLink": 0, "sourceID": "", "creator": "", "fileOversize": false }, "title": "交互印證｜觀測與模擬的爆炸結構", "desc": "模擬結果與觀測到的超新星殘骸蟹狀星雲比較，竟有著意外相似的手指狀結構。推測蟹狀星雲的複雜結構由此類爆炸機制而來，1054年的超新星爆炸很可能是核心塌縮型超新星爆炸。我們竟然能透過短短幾十秒的模擬，看見歷經數百年變化的結構。", "musicName": "無", "musicTip": "聽導覽", "weight": 17, "musicText": "", "musicURL": "" }, "basic-omn5bfbt3p": { "id": "basic-omn5bfbt3p", "type": "basic", "sortable": true, "primaryObj": { "oid": "3fcac7fad1802dd7b20bb5643cb87ab7", "fileType": "image", "fileURI": "https://openmuseum.tw/files/muse_portal/muse_styles/w1024/mcode/da62302464331c2dcf7deb66ed9a60ce.jpg?itok=RoHb2l2B", "level": "primary", "title": "中子星噴流", "desc": "中子星Swift J0243.6+6124發出輻射噴流的的想像圖。", "thumbURI": "https://openmuseum.tw/files/muse_portal/muse_styles/square_thumbnail_100/mcode/da62302464331c2dcf7deb66ed9a60ce.jpg?itok=Jfc2ikJo", "thumbMediumURI": "https://openmuseum.tw/files/muse_portal/muse_styles/thumbnail_medium/mcode/da62302464331c2dcf7deb66ed9a60ce.jpg?itok=yPilGTOC", "thumbBigURI": "https://openmuseum.tw/files/muse_portal/muse_styles/thumbnail_big/mcode/da62302464331c2dcf7deb66ed9a60ce.jpg?itok=PIwZHdEu", "background": "https://openmuseum.tw/files/muse_portal/muse_styles/w1920/mcode/da62302464331c2dcf7deb66ed9a60ce.jpg?itok=I2RAl998", "mfid": "da62302464331c2dcf7deb66ed9a60ce", "musicURL": "", "musicName": "", "fileCreator": "ICRAR/University of Amsterdam.", "rights": "ICRAR", "rightsLogo": "https://openmuseum.tw/files/muse_portal/styles/square_thumbnail_100/public/default_rights/memder_non-04.png?itok=gq-PTcKL", "fileLicence": "創用CC 姓名標示-非商業性", "fileDisableLink": 0, "sourceID": "", "creator": "", "fileOversize": false }, "title": "請輸入頁面標題", "desc": "藉由科學藝術繪圖，呈現出中子星周圍的磁力線，磁場影響形成兩極噴流。模擬圖則能觀察到因磁力與紊流造成之雙極噴流的現象與脈動。<br>", "musicName": "無", "musicTip": "聽導覽", "weight": 18, "secondaryObj": { "level": "secondary", "oid": "3f25e1857064fb62f680b58c3ebe6a80", "title": "超級電腦模擬「磁星」驅動超新星爆炸", "desc": "", "thumbURI": 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"著作權利所有-姓名標示-非商業性的教育與研究使用", "fileDisableLink": 0, "sourceID": "", "creator": "", "fileOversize": false }, "musicText": "", "musicURL": "" }, "basic-z7w9a2uygb": { "id": "basic-z7w9a2uygb", "type": "basic", "sortable": true, "primaryObj": { "oid": "6c8c7ef3e17d806958513e2dfc761610", "fileType": "image", "fileURI": "https://openmuseum.tw/files/muse_portal/muse_styles/w1024/mcode/7cb8ac5d5824a86ec37f33373d63c864.jpg?itok=BaoOaFjV", "level": "primary", "title": "以超級電腦模擬「磁星」驅動超新星爆炸的景象/磁星驅動熱氣泡三維模擬圖像", "desc": "超新星爆炸是宇宙中最壯麗的恆星爆炸，是現代天文物理熱門主題之一。透過超級電腦進行超大尺度、精密的模擬計算，等於相當於拿起一把手術刀，開始解剖一個超新星，或許對所知仍有限的超新星爆炸現象，提出有力洞見。", "thumbURI": "https://openmuseum.tw/files/muse_portal/muse_styles/square_thumbnail_100/mcode/7cb8ac5d5824a86ec37f33373d63c864.jpg?itok=ZrH84kN4", "thumbMediumURI": "https://openmuseum.tw/files/muse_portal/muse_styles/thumbnail_medium/mcode/7cb8ac5d5824a86ec37f33373d63c864.jpg?itok=9R7Iw4sh", "thumbBigURI": "https://openmuseum.tw/files/muse_portal/muse_styles/thumbnail_big/mcode/7cb8ac5d5824a86ec37f33373d63c864.jpg?itok=9a9IsONw", "background": "https://openmuseum.tw/files/muse_portal/muse_styles/w1920/mcode/7cb8ac5d5824a86ec37f33373d63c864.jpg?itok=7ggi4hyc", "mfid": "7cb8ac5d5824a86ec37f33373d63c864", "musicURL": "", "musicName": "", "fileCreator": "陳科榮", "rights": "中央研究院天文及天文物理研究所", "rightsLogo": "https://openmuseum.tw/files/muse_portal/styles/square_thumbnail_100/public/default_rights/memder_non-03.png?itok=h0rkcAOw", "fileLicence": "創用CC 姓名標示-非商業性-禁止改作", "fileDisableLink": 0, "sourceID": "", "creator": "", "fileOversize": false }, "title": "解析核心｜驅動爆炸的中心磁星", "desc": "透過三維（3D）模擬超亮超新星的中心磁星，中子星的快速旋轉牽動電磁場變化，造成輻射能量傳遞導致爆炸。色彩代表密度，視覺化地呈現中心產生的輻射與高速旋轉的磁星形成強烈紊流。我們彷彿置身紊流中隨之旋轉。<br><br>下一頁探索 SN 1987A 的三維超新星爆炸模型，顏色代表不同的元素在非對稱爆炸後預測的分佈情形。（CC BY 4.0 Deed | 姓名標示4.0 國際）<div><br><br><br></div>", "musicName": "無", "musicTip": "聽導覽", "weight": 19, "musicText": "", "musicURL": "" }, "embed_html-vij100s2vn": 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target=\"_blank\" rel=\"nofollow\" href=\"https://sketchfab.com/3d-models/elements-in-a-ccsn-s198-fid-clipped-54345fdaf60b4f849a98873ac48fc420\">超新星爆炸3D模型</a>／小野勝臣<br>⊕<a target=\"_blank\" rel=\"nofollow\" href=\"https://www.asiaa.sinica.edu.tw/news/shownews.php?i=85125cc067712b4f5a1a7d5070787e54\">發現大質量恆星的瘦身秘密</a>／歐柏昇<br>⊕<a target=\"_blank\" rel=\"nofollow\" href=\"https://www.asiaa.sinica.edu.tw/news/shownews.php?i=dab114e1871b1b33dfcc818e71635556\">不甘寂寞的大質量恆星</a>／蔡松翰<br>⊕<a target=\"_blank\" rel=\"nofollow\" href=\"https://www.asiaa.sinica.edu.tw/news/shownews.php?i=95ee99c1e61dfd42f93ba7f5816ce86a\">破解星系中心大黑洞的成長之謎</a>／林祺紘<br><br>主題I <a target=\"_blank\" rel=\"nofollow\" href=\"https://openmuseum.tw/muse/exhibition/8dbd58ea32ac7abeb4c0cf3e758422b2\">恆星的華麗謝幕</a><br>主展頁｜<a target=\"_blank\" rel=\"nofollow\" href=\"https://openmuseum.tw/muse/curation/6acf805d345a4ca50fb7450883133e8b\">解析恆星的衰亡與重生</a><br>", "musicName": "無", "musicTip": "聽導覽", "weight": 23, "musicText": "", "musicURL": 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rel=\"nofollow\" href=\"https://openmuseum.tw/muse/curation/6acf805d345a4ca50fb7450883133e8b\">主展頁｜解析恆星的衰亡與重生</a><br><a target=\"_blank\" rel=\"nofollow\" href=\"https://openmuseum.tw/muse/exhibition/8dbd58ea32ac7abeb4c0cf3e758422b2\">主題I｜恆星的華麗謝幕</a><br><br>策展團隊｜<br>中研院天文所陳科榮助研究員<br>臺大物理系博士班/中研院天文所博士生陳文翊、歐柏昇<br>凡木文化有限公司<br>藝術示意繪圖｜胡文鋒<br>策展行政協力｜<br>中研院天文所黃珞文<br>中研院數位文化中心藍萱<br><br><br><br>", "weight": 24 } }

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