{"id":319343,"date":"2025-11-20T02:29:19","date_gmt":"2025-11-19T16:29:19","guid":{"rendered":"https:\/\/www.nasa.gov\/?p=921355"},"modified":"2025-11-20T02:29:19","modified_gmt":"2025-11-19T16:29:19","slug":"nasa-cassini-study-finds-organics-fresh-from-ocean-of-enceladus-2","status":"publish","type":"post","link":"https:\/\/www.vibewire.com.au\/?p=319343","title":{"rendered":"NASA Cassini Study Finds Organics \u2018Fresh\u2019 From Ocean of Enceladus"},"content":{"rendered":"
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\"NASA<\/a><\/figure>
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In this image captured by NASA\u2019s Cassini spacecraft in 2009, dramatic plumes of water ice and vapor are seen erupting from the south pole of Saturn\u2019s moon Enceladus.<\/div>\n
NASA\/JPL\/Space Science Institute<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n

Researchers dove deep into information gathered from the ice grains that were collected during a close and super-fast flyby through a plume of Saturn\u2019s icy moon.<\/em><\/p>\n

A new analysis of data from NASA\u2019s Cassini mission found evidence of previously undetected organic compounds in a plume of ice particles ejected from the ocean that lies under the frozen shell of Saturn\u2019s moon Enceladus. Researchers spotted not only molecules they\u2019ve found before but also new ones that lay a potential path to chemical or biochemical activity.<\/p>\n

The ice grains studied were collected just 13 miles (21 kilometers) from the moon\u2019s surface and mark the first time scientists have observed this diversity of organics in fresh particles ejected from the subsurface water of Enceladus. Published<\/a> Wednesday in Nature Astronomy, the findings signal an important step toward confirming active organic chemistry below the moon\u2019s surface. This is the kind of chemical activity that could support compounds that are important to biological processes and are an essential component of life on Earth.<\/p>\n

Besides increasing the diversity of detected organics, the recent work added a new layer to earlier findings by analyzing particles that the Cassini<\/a> spacecraft collected when it flew directly through a plume \u2014 the next-best thing to diving directly into the moon\u2019s ocean.<\/p>\n

\u201cPreviously, we detected organics in ice grains<\/a> that were years old and potentially altered by the intense radiation environment surrounding them,\u201d said Nozair Khawaja of the Freie Universit\u00e4t Berlin, lead author of the study. \u201cThese new organic compounds were just minutes old, found in ice that was fresh from the ocean below Enceladus\u2019 surface.\u201d <\/p>\n

Scientists knew from previous Cassini data-mining that nitrogen- and oxygen-bearing organic compounds were present in particles from Saturn\u2019s E ring, a faint, wide outer band around the planet fed by the icy material that fans out from Enceladus\u2019 plumes. But the new research analyzed ice grains from a moon plume itself \u2014 in other words, grains found closest to their subsurface origin.<\/p>\n

\u201cThese molecules we found in the freshly ejected material prove that the complex organic molecules Cassini detected in Saturn\u2019s E ring<\/a> are not just a product of long exposure to space, but are readily available in Enceladus\u2019 ocean,\u201d said coauthor Frank Postberg, also of Freie Universit\u00e4t Berlin.<\/p>\n

Fast and fruitful<\/strong><\/h3>\n

The data was collected and sent to Earth in 2008, when ice particles impacted Cassini\u2019s Cosmic Dust Analyzer instrument. Besides being directly sourced from a plume, the ice grains had another thing going for them: They\u2019d been smashed to smithereens as they struck the instrument during the spacecraft\u2019s fast fly-through at 11 miles per second (about 18 kilometers per second relative to the moon).<\/p>\n

The energy of the impact vaporized the ice grains and ionized a substantial fraction of them. Those ions were then analyzed by the instrument\u2019s mass spectrometer, which examined their chemical makeup.<\/p>\n

The study\u2019s authors were able to analyze the tiniest of fragments \u2014 smaller than a thousandth of a millimeter, smaller even than a flu virus \u2014 and identify organic compounds they hadn\u2019t seen before in plume particles.<\/p>\n

The newly detected compounds included those from the aliphatic and cyclic ester and ether families, some with double bonds in their molecular structures. Together with the confirmed aromatic, nitrogen- and oxygen-bearing compounds, these compounds can form the building blocks to support chemical reactions and processes that could have led to more complex organic chemistry \u2014 the kind that is of interest to astrobiology and narrows the focus of where we search for life in the solar system.<\/p>\n

After flying through the plume, the spacecraft, managed by NASA\u2019s Jet Propulsion Laboratory in Southern California, explored the complex Saturn system for nearly another decade.<\/p>\n

More about Cassini<\/strong><\/h3>\n

The Cassini-Huygens mission was a cooperative project of NASA, ESA (European Space Agency), and the Italian Space Agency. A division of Caltech in Pasadena, JPL managed the mission for NASA\u2019s Space Mission Directorate in Washington and designed, developed, and assembled the Cassini orbiter.<\/p>\n

To learn more about Cassini, visit:<\/p>\n

https:\/\/science.nasa.gov\/mission\/cassini\/<\/strong><\/a><\/p>\n

News Media Contacts<\/strong><\/h3>\n

Scott Hulme
Jet Propulsion Laboratory, Pasadena, Calif.
818-653-9131
scott.d.hulme@jpl.nasa.gov<\/a><\/p>\n

Alise Fisher \/ Molly Wasser
NASA Headquarters, Washington
202-617-4977 \/ 240-419-1732
alise.m.fisher@nasa.gov<\/a> \/ molly.l.wasser@nasa.gov<\/a><\/p>\n

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Researchers dove deep into information gathered from the ice grains that were collected during a close and super-fast flyby through a plume of Saturn\u2019s icy moon. A new analysis of data from NASA\u2019s Cassini mission found evidence of previously undetected organic compounds in a plume of ice particles ejected from the ocean that lies under [\u2026]<\/p>\n","protected":false},"author":13,"featured_media":0,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"om_disable_all_campaigns":false,"_monsterinsights_skip_tracking":false,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0,"_uf_show_specific_survey":0,"_uf_disable_surveys":false,"footnotes":""},"categories":[16009,17501,18818,16726,16727],"tags":[],"class_list":["post-319343","post","type-post","status-publish","format-standard","hentry","category-astrobiology","category-cassini","category-enceladus","category-saturn","category-saturn-moons"],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/319343","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/users\/13"}],"replies":[{"embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=319343"}],"version-history":[{"count":2,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/319343\/revisions"}],"predecessor-version":[{"id":319439,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/319343\/revisions\/319439"}],"wp:attachment":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=319343"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=319343"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=319343"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}