{"id":470,"date":"2025-12-03T03:00:33","date_gmt":"2025-12-03T02:00:33","guid":{"rendered":"https:\/\/100blogs.ovh\/36\/index.php\/2025\/12\/03\/sugars-gum-stardust-found-in-nasas-asteroid-bennu-samples\/"},"modified":"2026-01-12T11:33:14","modified_gmt":"2026-01-12T10:33:14","slug":"sugars-gum-stardust-found-in-nasas-asteroid-bennu-samples","status":"publish","type":"post","link":"https:\/\/100blogs.ovh\/36\/index.php\/2025\/12\/03\/sugars-gum-stardust-found-in-nasas-asteroid-bennu-samples\/","title":{"rendered":"Sugars, \u2018Gum,\u2019 Stardust Found in NASA\u2019s Asteroid Bennu Samples"},"content":{"rendered":"
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The asteroid Bennu continues to provide new clues to scientists\u2019 biggest questions about the formation of the early solar system and the origins of life. As part of the ongoing study of pristine samples delivered to Earth by NASA\u2019s OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer) spacecraft, three new papers published Tuesday by the journals Nature Geosciences and Nature Astronomy present remarkable discoveries: sugars essential for biology, a gum-like substance not seen before in astromaterials, and an unexpectedly high abundance of dust produced by supernova explosions.<\/p>\n<\/p>\n

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Sugars essential to life<\/strong><\/p>\n

Scientists led by Yoshihiro Furukawa of Tohoku University in Japan found sugars essential for biology on Earth in the Bennu samples, detailing their findings in the journal Nature Geoscience<\/a>. The five-carbon sugar ribose and, for the first time in an extraterrestrial sample, six-carbon glucose were found. Although these sugars are not evidence of life, their detection, along with previous detections<\/a> of amino acids, nucleobases, and carboxylic acids in Bennu samples, show building blocks of biological molecules were widespread throughout the solar system.<\/p>\n

For life on Earth, the sugars deoxyribose and ribose are key building blocks of DNA and RNA, respectively. DNA is the primary carrier of genetic information in cells. RNA performs numerous functions, and life as we know it could not exist without it. Ribose in RNA is used in the molecule\u2019s sugar-phosphate \u201cbackbone\u201d that connects a string of information-carrying nucleobases.<\/p>\n

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\u201cAll five nucleobases used to construct both DNA and RNA, along with phosphates, have already been found in the Bennu samples brought to Earth by OSIRIS-REx,\u201d said Furukawa. \u201cThe new discovery of ribose means that all of the components to form the molecule RNA are present in Bennu.\u201d<\/p>\n

The discovery of ribose in asteroid samples is not a complete surprise. Ribose has previously been found in two meteorites<\/a> recovered on Earth. What is important about the Bennu samples is that researchers did not find deoxyribose. If Bennu is any indication, this means ribose may have been more common than deoxyribose in environments of the early solar system.\u00a0<\/p>\n

Researchers think the presence of ribose and lack of deoxyribose supports the \u201cRNA world\u201d hypothesis, where the first forms of life relied on RNA as the primary molecule to store information and to drive chemical reactions necessary for survival.\u00a0<\/p>\n

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A team of Japanese and US scientists have discovered the bio-essential sugars ribose and glucose in samples of asteroid Bennu that were collected by NASA\u2019s OSIRIS-REx mission. This finding builds on the earlier discovery of nucleobases (the genetic components of DNA and RNA), phosphate, and amino acids (the building blocks of proteins) in the Bennu samples, showing that the molecular ingredients of life could have been delivered to early Earth by meteorites. Download this graphic from NASA\u2019s Scientific Visualization Studio website: https:\/\/svs.gsfc.nasa.gov\/14932<\/div>\n
NASA\/Goddard\/University of Arizona\/Dan Gallagher\u00a0<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n

\u201cPresent day life is based on a complex system organized primarily by three types of functional biopolymers: DNA, RNA, and proteins,\u201d explains Furukawa. \u201cHowever, early life may have been simpler. RNA is the leading candidate for the first functional biopolymer because it can store genetic information and catalyze many biological reactions.\u201d<\/p>\n

The Bennu samples also contained one of the most common forms of \u201cfood\u201d (or energy) used by life on Earth, the sugar glucose, which is the first evidence that an important energy source for life as we know it was also present in the early solar system.<\/p>\n

Mysterious, ancient \u2018gum\u2019<\/strong><\/p>\n

A second paper, in the journal Nature Astronomy<\/a> led by Scott Sandford at NASA\u2019s Ames Research Center in California\u2019s Silicon Valley and Zack Gainsforth of the University of California, Berkeley, reveals a gum-like material in the Bennu samples never seen before in space rocks \u2013 something that could have helped set the stage on Earth for the ingredients of life to emerge. The surprising substance was likely formed in the early days of the solar system, as Bennu\u2019s young parent asteroid warmed.<\/p>\n

Once soft and flexible, but since hardened, this ancient \u201cspace gum\u201d consists of polymer-like materials extremely rich in nitrogen and oxygen. Such complex molecules could have provided some of the chemical precursors that helped trigger life on Earth, and finding them in the pristine samples from Bennu is important for scientists studying how life began and whether it exists beyond our planet.<\/p>\n

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On this primitive asteroid that formed in the early days of the solar system, we\u2019re looking at events near the beginning of the beginning.<\/span><\/h2>\n<\/p><\/div>\n
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\"Scott<\/figure>\n<\/div>\n
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Scott SandFord<\/p>\n

Astrophysicist, NASA’s Ames Research Center<\/p>\n<\/p><\/div>\n<\/p><\/div>\n<\/p><\/div>\n<\/p><\/div>\n<\/p><\/div>\n<\/div>\n

Bennu\u2019s ancestral asteroid formed from materials in the solar nebula \u2013 the rotating cloud of gas and dust that gave rise to the solar system \u2013 and contained a variety of minerals and ices. As the asteroid began to warm, due to natural radiation, a compound called carbamate formed through a process involving ammonia and carbon dioxide. Carbamate is water soluble, but it survived long enough to polymerize, reacting with itself and other molecules to form larger and more complex chains impervious to water. This suggests that it formed before the parent body warmed enough to become a watery environment.<\/p>\n

\u201cWith this strange substance, we\u2019re looking at, quite possibly, one of the earliest alterations of materials that occurred in this rock,\u201d said Sandford. \u201cOn this primitive asteroid that formed in the early days of the solar system, we\u2019re looking at events near the beginning of the beginning.\u201d<\/p>\n

Using an infrared microscope, Sandford\u2019s team selected unusual, carbon-rich grains containing abundant nitrogen and oxygen. They then began what Sandford calls \u201cblacksmithing at the molecular level,\u201d using the Molecular Foundry at Lawrence Berkeley National Laboratory (Berkeley Lab) in Berkeley, California. Applying ultra-thin layers of platinum, they reinforced a particle, welded on a tungsten needle to lift the tiny grain, and shaved the fragment down using a focused beam of charged particles.<\/p>\n

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A microscopic particle of asteroid Bennu, brought to Earth by NASA\u2019s OSIRIS-REx mission, is manipulated under a transmission electron microscope. In order to move the fragment for further analysis, researchers first reinforced it with thin strips of platinum (the \u201cL\u201d shape on the particle\u2019s surface) then welded a tungsten microneedle to it. The asteroid fragment measures 30 micrometers (about one-one thousandth of an inch) across.<\/div>\n
NASA\/University of California, Berkeley<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n

When the particle was a thousand times thinner than a human hair, they analyzed its composition via electron microscopy at the Molecular Foundry and X-ray spectroscopy at Berkeley Lab\u2019s Advanced Light Source. The ALS\u2019s high spatial resolution and sensitive X-ray beams enabled unprecedented chemical analysis.<\/p>\n

\u201cWe knew we had something remarkable the instant the images started to appear on the monitor,\u201d said Gainsforth. \u201cIt was like nothing we had ever seen, and for months we were consumed by data and theories as we attempted to understand just what it was and how it could have come into existence.\u201d\u00a0<\/p>\n

The team conducted a slew of experiments to examine the material\u2019s characteristics. As the details emerged, the evidence suggested the strange substance had been deposited in layers on grains of ice and minerals present in the asteroid.<\/p>\n

It was also flexible \u2013 a pliable material, similar to used gum or even a soft plastic. Indeed, during their work with the samples, researchers noticed the strange material was bendy and dimpled when pressure was applied. The stuff was translucent, and exposure to radiation made it brittle, like a lawn chair left too many seasons in the sun.<\/p>\n

\u201cLooking at its chemical makeup, we see the same kinds of chemical groups that occur in polyurethane on Earth,\u201d said Sandford, \u201cmaking this material from Bennu something akin to a \u2018space plastic.\u2019\u201d\u00a0<\/p>\n

The ancient asteroid stuff isn\u2019t simply polyurethane, though, which is an orderly polymer. This one has more \u201crandom, hodgepodge connections and a composition of elements that differs from particle to particle,\u201d said Sandford. But the comparison underscores the surprising nature of the organic material discovered in NASA\u2019s asteroid samples, and the research team aims to study more of it.<\/p>\n

By pursuing clues about what went on long ago, deep inside an asteroid, scientists can better understand the young solar system \u2013 revealing the precursors to and ingredients of life it already contained, and how far those raw materials may have been scattered, thanks to asteroids much like Bennu.<\/p>\n

Abundant supernova dust<\/strong><\/p>\n

Another paper in the journal Nature Astronomy<\/a>, led by Ann Nguyen of NASA\u2019s Johnson Space Center in Houston, analyzed presolar grains \u2013\u00a0dust from stars predating our solar system \u2013 found in two different rock types in the Bennu samples to learn more about where its parent body formed and how it was altered by geologic processes. It is believed that presolar dust was generally well-mixed as our solar system formed. The samples had six-times the amount of supernova dust than any other studied astromaterial, suggesting the asteroid\u2019s parent body formed in a region of the protoplanetary disk<\/a> enriched in the dust of dying stars.\u00a0\u00a0<\/p>\n

The study also reveals that, while Bennu\u2019s parent asteroid experienced extensive alteration by fluids, there are still pockets of less-altered materials within the samples that offer insights into its origin.<\/p>\n

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An artistic visualization of the OSIRIS-REx spacecraft descending towards asteroid Bennu to collect a sample.<\/div>\n
NASA\/Goddard\/University of Arizona<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n

\u201cThese fragments retain a higher abundance of organic matter and presolar silicate grains, which are known to be easily destroyed by aqueous alteration in asteroids,\u201d said Nguyen. \u201cTheir preservation in the Bennu samples was a surprise and illustrates that some material escaped alteration in the parent body. Our study reveals the diversity of presolar materials that the parent accreted as it was forming.\u201d<\/p>\n<\/p>\n

NASA\u2019s Goddard Space Flight Center provided overall mission management, systems engineering, and the safety and mission assurance for OSIRIS-REx. Dante Lauretta of the University of Arizona, Tucson, is the principal investigator. The university leads the science team and the mission\u2019s science observation planning and data processing. Lockheed Martin Space in Littleton, Colorado, built the spacecraft and provided flight operations. Goddard and KinetX Aerospace were responsible for navigating the OSIRIS-REx spacecraft. Curation for OSIRIS-REx takes place at NASA\u2019s Johnson Space Center in Houston. International partnerships on this mission include the OSIRIS-REx Laser Altimeter instrument from CSA (Canadian Space Agency) and asteroid sample science collaboration with JAXA\u2019s (Japan Aerospace Exploration Agency\u2019s) Hayabusa2 mission. OSIRIS-REx is the third mission in NASA\u2019s New Frontiers Program, managed by NASA\u2019s Marshall Space Flight Center in Huntsville, Alabama, for the agency\u2019s Science Mission Directorate in Washington.<\/p>\n

For more information on the OSIRIS-REx mission, visit:<\/p>\n

https:\/\/www.nasa.gov\/osiris-rex<\/strong><\/a><\/p>\n

Karen Fox \/ Molly Wasser
Headquarters, Washington
202-285-5155 \/ 240-419-1732
<\/a>karen.c.fox@nasa.gov<\/a> \u00a0\u00a0\/ molly.l.wasser@nasa.gov<\/a><\/p>\n<\/div>\n","protected":false},"excerpt":{"rendered":"

The asteroid Bennu continues to provide new clues to scientists\u2019 biggest questions about the formation of the early solar system and the origins of life. As part of the ongoing study of pristine samples delivered to Earth by NASA\u2019s OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer) spacecraft, three new papers published Tuesday by […]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[4],"tags":[],"class_list":["post-470","post","type-post","status-publish","format-standard","hentry","category-ciencia"],"_links":{"self":[{"href":"https:\/\/100blogs.ovh\/36\/index.php\/wp-json\/wp\/v2\/posts\/470","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/100blogs.ovh\/36\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/100blogs.ovh\/36\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/100blogs.ovh\/36\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/100blogs.ovh\/36\/index.php\/wp-json\/wp\/v2\/comments?post=470"}],"version-history":[{"count":1,"href":"https:\/\/100blogs.ovh\/36\/index.php\/wp-json\/wp\/v2\/posts\/470\/revisions"}],"predecessor-version":[{"id":1032,"href":"https:\/\/100blogs.ovh\/36\/index.php\/wp-json\/wp\/v2\/posts\/470\/revisions\/1032"}],"wp:attachment":[{"href":"https:\/\/100blogs.ovh\/36\/index.php\/wp-json\/wp\/v2\/media?parent=470"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/100blogs.ovh\/36\/index.php\/wp-json\/wp\/v2\/categories?post=470"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/100blogs.ovh\/36\/index.php\/wp-json\/wp\/v2\/tags?post=470"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}