  {"id":80834,"date":"2018-06-12T11:23:16","date_gmt":"2018-06-12T21:23:16","guid":{"rendered":"https:\/\/www.hawaii.edu\/news\/?p=80834"},"modified":"2020-05-08T11:44:21","modified_gmt":"2020-05-08T21:44:21","slug":"experiments-trace-interstellar-dust-back-to-solar-systems-formation","status":"publish","type":"post","link":"https:\/\/www.hawaii.edu\/news\/2018\/06\/12\/experiments-trace-interstellar-dust-back-to-solar-systems-formation\/","title":{"rendered":"Experiments trace interstellar dust back to solar system&#8217;s formation"},"content":{"rendered":"<span class=\"span-reading-time rt-reading-time\" style=\"display: block;\"><span class=\"rt-label rt-prefix\">Reading time: <\/span> <span class=\"rt-time\"> 2<\/span> <span class=\"rt-label rt-postfix\">minutes<\/span><\/span><figure id=\"attachment_80854\" aria-describedby=\"caption-attachment-80854\" style=\"width: 676px\" class=\"wp-caption alignleft\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.hawaii.edu\/news\/wp-content\/uploads\/2018\/06\/soest-interplanetary-dust-particles.jpg\" alt=\"\" width=\"676\" height=\"381\" class=\"size-full wp-image-80854\" srcset=\"https:\/\/www.hawaii.edu\/news\/wp-content\/uploads\/2018\/06\/soest-interplanetary-dust-particles.jpg 676w, https:\/\/www.hawaii.edu\/news\/wp-content\/uploads\/2018\/06\/soest-interplanetary-dust-particles-300x169.jpg 300w\" sizes=\"auto, (max-width: 676px) 100vw, 676px\" \/><figcaption id=\"caption-attachment-80854\" class=\"wp-caption-text\">Cometary-type interplanetary dust particle collected by <abbr title=\"National Aeronautics and Space Administration\">NASA<\/abbr> aircraft. (Credit: Hope Ishii, <abbr title=\"University of Hawaii\">糖心Vlog官方<\/abbr> M\u0101noa)<\/figcaption><\/figure>\n<figure id=\"attachment_80852\" aria-describedby=\"caption-attachment-80852\" style=\"width: 300px\" class=\"wp-caption alignright\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.hawaii.edu\/news\/wp-content\/uploads\/2018\/06\/soest-interplanetary-dust-particles-comet.jpg\" alt=\"comet flying over trees\" width=\"300\" height=\"334\" class=\"size-full wp-image-80852\" srcset=\"https:\/\/www.hawaii.edu\/news\/wp-content\/uploads\/2018\/06\/soest-interplanetary-dust-particles-comet.jpg 300w, https:\/\/www.hawaii.edu\/news\/wp-content\/uploads\/2018\/06\/soest-interplanetary-dust-particles-comet-269x300.jpg 269w\" sizes=\"auto, (max-width: 300px) 100vw, 300px\" \/><figcaption id=\"caption-attachment-80852\" class=\"wp-caption-text\">Comets can release dust that can be collected on Earth. (Credit: Philipp Salzgeber, <abbr>CC<\/abbr> <abbr>BY<\/abbr>&#8211;<abbr>SA<\/abbr> 2.0)<\/figcaption><\/figure>\n<p>A team of scientists led by <a href=\"https:\/\/manoa.hawaii.edu\/\">University of <span aria-label=\"Hawaii\">Hawai&#699;i<\/span> at M\u0101noa<\/a> <a href=\"https:\/\/www.soest.hawaii.edu\/soestwp\/\">School of Ocean and Earth Science and Technology<\/a> (<abbr>SOEST<\/abbr>) researcher <a href=\"https:\/\/www.higp.hawaii.edu\/cgi-directory\/directory.cgi?func=disp&#038;searchname=HopeA.Ishii\"><strong>Hope Ishii<\/strong><\/a> has discovered that certain interplanetary dust particles (<abbr>IDPs<\/abbr>) contain dust leftover from the initial formation of the solar system.<\/p>\n<p>The initial solids from which the solar system formed consisted almost entirely of amorphous silicate, carbon and ices. This dust was mostly destroyed and reworked by processes that led to the formation of planets. Surviving samples of pre-solar dust are most likely to be preserved in comets&#8212;small, cold bodies that formed in the outer solar nebula.<\/p>\n<p>In a relatively obscure class of <abbr>IDPs<\/abbr> believed to originate from comets, there are tiny glassy grains called <abbr title=\"glass embedded with metal and sulfides\">GEMS<\/abbr>, or glass embedded with metal and sulfides&#8212;typically only tens to hundreds of nanometers in diameter, less than 1\/100th the thickness of human hair.<\/p>\n<h2>Building blocks of planets and stars<\/h2>\n<figure id=\"attachment_80853\" aria-describedby=\"caption-attachment-80853\" style=\"width: 300px\" class=\"wp-caption alignright\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.hawaii.edu\/news\/wp-content\/uploads\/2018\/06\/soest-interplanetary-dust-particles-gems-300x214.jpg\" alt=\"\" width=\"300\" height=\"214\" class=\"size-medium wp-image-80853\" srcset=\"https:\/\/www.hawaii.edu\/news\/wp-content\/uploads\/2018\/06\/soest-interplanetary-dust-particles-gems-300x214.jpg 300w, https:\/\/www.hawaii.edu\/news\/wp-content\/uploads\/2018\/06\/soest-interplanetary-dust-particles-gems.jpg 676w\" sizes=\"auto, (max-width: 300px) 100vw, 300px\" \/><figcaption id=\"caption-attachment-80853\" class=\"wp-caption-text\">Elemental map of <abbr>GEMS<\/abbr> by microscopy. (Credit: Hope Ishii, <abbr title=\"University of Hawaii\">糖心Vlog官方<\/abbr> M\u0101noa. Reproduced with permission from <abbr>PNAS<\/abbr>).<\/figcaption><\/figure>\n<p>Using transmission electron microscopy, Ishii and colleagues made maps of the element distributions and discovered that these glassy grains are made up of subgrains that aggregated together in a different environment and prior to the formation of the comet parent body. This aggregate is encapsulated by carbon of a different type than the carbon that forms a matrix gluing together <abbr>GEMS<\/abbr> and other components of cometary dust.<\/p>\n<p>The types of carbon that rims the subgrains and that forms the matrix in these particles decomposes with even weak heating, suggesting that the <abbr>GEMS<\/abbr> could not have formed in the hot inner solar nebula, and instead formed in a cold, radiation-rich environment, such as the outer solar nebula or pre-solar molecular cloud.<\/p>\n<p>&ldquo;Our observations suggest that these exotic grains represent surviving pre-solar interstellar dust that formed the very building blocks of planets and stars,&rdquo; said Ishii, who is based at the <abbr>糖心Vlog官方<\/abbr> M\u0101noa <a href=\"https:\/\/www.higp.hawaii.edu\/\"><span aria-label=\"Hawaii\">Hawai&#699;i<\/span> Institute of Geophysics and Planetology<\/a>. &ldquo;If we have at our fingertips the starting materials of planet formation from 4.6 billion years ago, that is thrilling and makes possible a deeper understanding of the processes that formed and have since altered them.&rdquo;<\/p>\n<h2>Excellence in space science at <abbr>糖心Vlog官方<\/abbr><\/h2>\n<p><abbr>糖心Vlog官方<\/abbr> has a strong footprint in space science and state-of-the-art instrumentation and is recognized as world-class in this field.<\/p>\n<p>&ldquo;This is an example of research that seeks to satisfy the human urge to understand our world&#8217;s origins and serves the people of <span aria-label=\"Hawaii\">Hawai&#699;i<\/span> by boosting our reputation for excellence in space science and as a training ground for our students to be engaged in exciting science,&rdquo; said Ishii.<\/p>\n<p>The team plans to search the interiors of additional comet dust particles, especially those that were well-protected during their passage through the Earth&#8217;s atmosphere, to increase understanding of the distribution of carbon within <abbr>GEMS<\/abbr> and the size distributions of <abbr>GEMS<\/abbr> subgrains.<\/p>\n<h2>Funding and collaboration<\/h2>\n<p>This work was funded by <abbr title=\"National Aeronautics and Space Administration's\">NASA&#8217;s<\/abbr> Cosmochemistry, Emerging Worlds and Laboratory Analysis of Returned Samples Programs and was enabled, in part, by the <a href=\"http:\/\/www.soest.hawaii.edu\/AEMC\/\">Advanced Electron Microscopy Center<\/a> at <abbr>糖心Vlog官方<\/abbr>. Portions of the work were also performed at national user facilities at the Molecular Foundry and the Advanced Light Sourceat Lawrence Berkeley National Laboratory, which are supported by the Office of Science, Basic Energy Sciences, U.S. Department of Energy.<\/p>\n<p><em>&#8212;By Marcie Grabowski<\/em><\/p>\n","protected":false},"excerpt":{"rendered":"<p>A team of scientists led by School of Ocean and Earth Science and Technology researcher Hope Ishii has discovered that certain interplanetary dust particles contain dust leftover from the initial formation of the solar system.<\/p>\n","protected":false},"author":16,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[30],"tags":[34,170,92,9],"class_list":["post-80834","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-research","tag-astronomy","tag-hawaii-institute-of-geophysics-and-planetology","tag-school-of-ocean-and-earth-science-and-technology","tag-uh-manoa","entry","has-media"],"aioseo_notices":[],"jetpack_featured_media_url":"","_links":{"self":[{"href":"https:\/\/www.hawaii.edu\/news\/wp-json\/wp\/v2\/posts\/80834","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.hawaii.edu\/news\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.hawaii.edu\/news\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.hawaii.edu\/news\/wp-json\/wp\/v2\/users\/16"}],"replies":[{"embeddable":true,"href":"https:\/\/www.hawaii.edu\/news\/wp-json\/wp\/v2\/comments?post=80834"}],"version-history":[{"count":11,"href":"https:\/\/www.hawaii.edu\/news\/wp-json\/wp\/v2\/posts\/80834\/revisions"}],"predecessor-version":[{"id":117846,"href":"https:\/\/www.hawaii.edu\/news\/wp-json\/wp\/v2\/posts\/80834\/revisions\/117846"}],"wp:attachment":[{"href":"https:\/\/www.hawaii.edu\/news\/wp-json\/wp\/v2\/media?parent=80834"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.hawaii.edu\/news\/wp-json\/wp\/v2\/categories?post=80834"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.hawaii.edu\/news\/wp-json\/wp\/v2\/tags?post=80834"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}