{"id":141600,"date":"2024-05-24T11:11:24","date_gmt":"2024-05-24T15:11:24","guid":{"rendered":"https:/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600//www.ucf.edu/news/wp-json/wp/v2/posts/141600//news/news/wp-json/wp/v2/posts/141600//?p=141600"},"modified":"2025-04-14T12:55:50","modified_gmt":"2025-04-14T16:55:50","slug":"scientists-discover-co2-and-co-ices-in-outskirts-of-solar-system-for-the-first-time","status":"publish","type":"post","link":"https:/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600//www.ucf.edu/news/wp-json/wp/v2/posts/141600//news/news/wp-json/wp/v2/posts/141600//scientists-discover-co2-and-co-ices-in-outskirts-of-solar-system-for-the-first-time/news/wp-json/wp/v2/posts/141600//","title":{"rendered":"Scientists Discover CO2 and CO Ices in Outskirts of Solar System"},"content":{"rendered":"<p>For the first time, carbon dioxide and carbon monoxide ices have been observed in the far reaches of our solar system on trans-Neptunian objects (TNOs).</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>A research team, led by planetary scientists M/news/wp-json/wp/v2/posts/141600/u00e1rio Nascimento De Pr/news/wp-json/wp/v2/posts/141600/u00e1 and Noem/news/wp-json/wp/v2/posts/141600/u00ed Pinilla-Alonso from the 麻豆原创&#8217;s Florida Space Institute (FSI), made the findings by using the infrared spectral capabilities of the James Webb Space Telescope (JWST) to analyze the chemical composition of 59 trans-Neptunian objects and Centaurs.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>The pioneering study, published this week in <em>Nature Astronomy</news/wp-json/wp/v2/posts/141600//em><em>,</news/wp-json/wp/v2/posts/141600//em>&nbsp;suggests that carbon dioxide ice was abundant in the cold outer regions of the protoplanetary disk, the vast rotating disk of gas and dust from which the solar system formed. Further investigation is needed to understand the carbon monoxide ice/news/wp-json/wp/v2/posts/141600/u2019s origins, as it also prevalent on the TNOs in the study.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>The researchers reported the detection of carbon dioxide in 56 TNOs and carbon monoxide in 28 (plus six with dubious or marginal detections), out of a sample of 59 objects observed with the JWST. Carbon dioxide was widespread on the surfaces of the trans-Neptunian population, independent of the dynamical class and body size while carbon monoxide was detected only in objects with a high carbon dioxide abundance, according to the study.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>The work is part of the 麻豆原创-led Discovering the Surface Compositions of Trans-Neptunian Objects program (DiSCo-TNOs), one of the JWST programs focused on analyzing our solar system.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<figure id=/news/wp-json/wp/v2/posts/141600/"attachment_141607/news/wp-json/wp/v2/posts/141600/" style=/news/wp-json/wp/v2/posts/141600/"max-width: 1200px;/news/wp-json/wp/v2/posts/141600/" class=/news/wp-json/wp/v2/posts/141600/"figure mx-auto d-block/news/wp-json/wp/v2/posts/141600/"><noscript><img decoding=/news/wp-json/wp/v2/posts/141600/"async/news/wp-json/wp/v2/posts/141600/" width=/news/wp-json/wp/v2/posts/141600/"1200/news/wp-json/wp/v2/posts/141600/" height=/news/wp-json/wp/v2/posts/141600/"800/news/wp-json/wp/v2/posts/141600/" class=/news/wp-json/wp/v2/posts/141600/"figure-img img-fluid w-100 wp-image-141607 size-full/news/wp-json/wp/v2/posts/141600/" src=/news/wp-json/wp/v2/posts/141600/"https:/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600//www.ucf.edu/news/wp-json/wp/v2/posts/141600//wp-content/news/wp-json/wp/v2/posts/141600//blogs.dir/news/wp-json/wp/v2/posts/141600//20/news/wp-json/wp/v2/posts/141600//files/news/wp-json/wp/v2/posts/141600//2024/news/wp-json/wp/v2/posts/141600//05/news/wp-json/wp/v2/posts/141600//nep.jpg/news/wp-json/wp/v2/posts/141600/" alt=/news/wp-json/wp/v2/posts/141600/"Spectrum of the surface of a trans-Neptunian object rich in carbon volatile ices obtained with JWST as part of the DiSCo Large Program. Absorptions of carbon dioxide (CO2), its isotopologue (13CO2), and carbon monoxide are highlighted in yellow. The light of the Sun (close to the center of the image) is dimmed billions of miles away, where the trans-Neptunian objects reside. Graphic rendering credit: William Gonzalez Sierra, Florida Space Institute /news/wp-json/wp/v2/posts/141600/" srcset=/news/wp-json/wp/v2/posts/141600/"https:/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600//www.ucf.edu/news/wp-json/wp/v2/posts/141600//wp-content/news/wp-json/wp/v2/posts/141600//blogs.dir/news/wp-json/wp/v2/posts/141600//20/news/wp-json/wp/v2/posts/141600//files/news/wp-json/wp/v2/posts/141600//2024/news/wp-json/wp/v2/posts/141600//05/news/wp-json/wp/v2/posts/141600//nep.jpg 1200w, https:/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600//www.ucf.edu/news/wp-json/wp/v2/posts/141600//wp-content/news/wp-json/wp/v2/posts/141600//blogs.dir/news/wp-json/wp/v2/posts/141600//20/news/wp-json/wp/v2/posts/141600//files/news/wp-json/wp/v2/posts/141600//2024/news/wp-json/wp/v2/posts/141600//05/news/wp-json/wp/v2/posts/141600//nep-300x200.jpg 300w, https:/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600//www.ucf.edu/news/wp-json/wp/v2/posts/141600//wp-content/news/wp-json/wp/v2/posts/141600//blogs.dir/news/wp-json/wp/v2/posts/141600//20/news/wp-json/wp/v2/posts/141600//files/news/wp-json/wp/v2/posts/141600//2024/news/wp-json/wp/v2/posts/141600//05/news/wp-json/wp/v2/posts/141600//nep-768x512.jpg 768w, https:/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600//www.ucf.edu/news/wp-json/wp/v2/posts/141600//wp-content/news/wp-json/wp/v2/posts/141600//blogs.dir/news/wp-json/wp/v2/posts/141600//20/news/wp-json/wp/v2/posts/141600//files/news/wp-json/wp/v2/posts/141600//2024/news/wp-json/wp/v2/posts/141600//05/news/wp-json/wp/v2/posts/141600//nep-600x400.jpg 600w, https:/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600//www.ucf.edu/news/wp-json/wp/v2/posts/141600//wp-content/news/wp-json/wp/v2/posts/141600//blogs.dir/news/wp-json/wp/v2/posts/141600//20/news/wp-json/wp/v2/posts/141600//files/news/wp-json/wp/v2/posts/141600//2024/news/wp-json/wp/v2/posts/141600//05/news/wp-json/wp/v2/posts/141600//nep-360x240.jpg 360w/news/wp-json/wp/v2/posts/141600/" sizes=/news/wp-json/wp/v2/posts/141600/"(max-width: 1200px) 100vw, 1200px/news/wp-json/wp/v2/posts/141600/"></news/wp-json/wp/v2/posts/141600//noscript><img decoding=/news/wp-json/wp/v2/posts/141600/"async/news/wp-json/wp/v2/posts/141600/" width=/news/wp-json/wp/v2/posts/141600/"1200/news/wp-json/wp/v2/posts/141600/" height=/news/wp-json/wp/v2/posts/141600/"800/news/wp-json/wp/v2/posts/141600/" class=/news/wp-json/wp/v2/posts/141600/"figure-img img-fluid w-100 wp-image-141607 size-full lazyload/news/wp-json/wp/v2/posts/141600/" src=/news/wp-json/wp/v2/posts/141600/"data:image/news/wp-json/wp/v2/posts/141600//svg+xml,%3Csvg%20xmlns%3D%22http%3A%2F%2Fwww.w3.org%2F2000%2Fsvg%22%20viewBox%3D%220%200%201200%20800%22%3E%3C%2Fsvg%3E/news/wp-json/wp/v2/posts/141600/" alt=/news/wp-json/wp/v2/posts/141600/"Spectrum of the surface of a trans-Neptunian object rich in carbon volatile ices obtained with JWST as part of the DiSCo Large Program. Absorptions of carbon dioxide (CO2), its isotopologue (13CO2), and carbon monoxide are highlighted in yellow. The light of the Sun (close to the center of the image) is dimmed billions of miles away, where the trans-Neptunian objects reside. Graphic rendering credit: William Gonzalez Sierra, Florida Space Institute /news/wp-json/wp/v2/posts/141600/" srcset=/news/wp-json/wp/v2/posts/141600/"data:image/news/wp-json/wp/v2/posts/141600//svg+xml,%3Csvg%20xmlns%3D%22http%3A%2F%2Fwww.w3.org%2F2000%2Fsvg%22%20viewBox%3D%220%200%201200%20800%22%3E%3C%2Fsvg%3E 1200w/news/wp-json/wp/v2/posts/141600/" sizes=/news/wp-json/wp/v2/posts/141600/"(max-width: 1200px) 100vw, 1200px/news/wp-json/wp/v2/posts/141600/" data-srcset=/news/wp-json/wp/v2/posts/141600/"https:/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600//www.ucf.edu/news/wp-json/wp/v2/posts/141600//wp-content/news/wp-json/wp/v2/posts/141600//blogs.dir/news/wp-json/wp/v2/posts/141600//20/news/wp-json/wp/v2/posts/141600//files/news/wp-json/wp/v2/posts/141600//2024/news/wp-json/wp/v2/posts/141600//05/news/wp-json/wp/v2/posts/141600//nep.jpg 1200w, https:/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600//www.ucf.edu/news/wp-json/wp/v2/posts/141600//wp-content/news/wp-json/wp/v2/posts/141600//blogs.dir/news/wp-json/wp/v2/posts/141600//20/news/wp-json/wp/v2/posts/141600//files/news/wp-json/wp/v2/posts/141600//2024/news/wp-json/wp/v2/posts/141600//05/news/wp-json/wp/v2/posts/141600//nep-300x200.jpg 300w, https:/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600//www.ucf.edu/news/wp-json/wp/v2/posts/141600//wp-content/news/wp-json/wp/v2/posts/141600//blogs.dir/news/wp-json/wp/v2/posts/141600//20/news/wp-json/wp/v2/posts/141600//files/news/wp-json/wp/v2/posts/141600//2024/news/wp-json/wp/v2/posts/141600//05/news/wp-json/wp/v2/posts/141600//nep-768x512.jpg 768w, https:/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600//www.ucf.edu/news/wp-json/wp/v2/posts/141600//wp-content/news/wp-json/wp/v2/posts/141600//blogs.dir/news/wp-json/wp/v2/posts/141600//20/news/wp-json/wp/v2/posts/141600//files/news/wp-json/wp/v2/posts/141600//2024/news/wp-json/wp/v2/posts/141600//05/news/wp-json/wp/v2/posts/141600//nep-600x400.jpg 600w, https:/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600//www.ucf.edu/news/wp-json/wp/v2/posts/141600//wp-content/news/wp-json/wp/v2/posts/141600//blogs.dir/news/wp-json/wp/v2/posts/141600//20/news/wp-json/wp/v2/posts/141600//files/news/wp-json/wp/v2/posts/141600//2024/news/wp-json/wp/v2/posts/141600//05/news/wp-json/wp/v2/posts/141600//nep-360x240.jpg 360w/news/wp-json/wp/v2/posts/141600/" data-src=/news/wp-json/wp/v2/posts/141600/"https:/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600//www.ucf.edu/news/wp-json/wp/v2/posts/141600//wp-content/news/wp-json/wp/v2/posts/141600//blogs.dir/news/wp-json/wp/v2/posts/141600//20/news/wp-json/wp/v2/posts/141600//files/news/wp-json/wp/v2/posts/141600//2024/news/wp-json/wp/v2/posts/141600//05/news/wp-json/wp/v2/posts/141600//nep.jpg/news/wp-json/wp/v2/posts/141600/"><figcaption class=/news/wp-json/wp/v2/posts/141600/"figure-caption/news/wp-json/wp/v2/posts/141600/">Spectrum of the surface of a trans-Neptunian object rich in carbon volatile ices obtained with JWST as part of the DiSCo Large Program. Absorptions of carbon dioxide (CO2), its isotopologue (13CO2), and carbon monoxide are highlighted in yellow. The light of the Sun (close to the center of the image) is dimmed billions of miles away, where the trans-Neptunian objects reside. Graphic rendering credit: William Gonzalez Sierra, Florida Space Institute</news/wp-json/wp/v2/posts/141600//figcaption></news/wp-json/wp/v2/posts/141600//figure>/news/wp-json/wp/v2/posts/141600/n<p>/news/wp-json/wp/v2/posts/141600/u201cIt is the first time we observed this region of the spectrum for a large collection of TNOs, so in a sense, everything we saw was exciting and unique,/news/wp-json/wp/v2/posts/141600/u201d says de Pr/news/wp-json/wp/v2/posts/141600/u00e1, who co-authored the study. /news/wp-json/wp/v2/posts/141600/u201cWe did not expect to find that carbon dioxide was so ubiquitous in the TNO region, and even less that carbon monoxide was present in so many TNOs./news/wp-json/wp/v2/posts/141600/u201d</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>The discovery of the ices can further help us understand the formation of our solar system and how celestial objects may have migrated, he says.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>/news/wp-json/wp/v2/posts/141600/u201cTrans-Neptunian Objects are relics from the process of planetary formation,/news/wp-json/wp/v2/posts/141600/u201d de Pr/news/wp-json/wp/v2/posts/141600/u00e1 says. /news/wp-json/wp/v2/posts/141600/u201cThese findings can impose important constraints about where these objects were formed, how they reached the region they inhabit nowadays, and how their surfaces evolved since their formation.&nbsp;Because they formed at greater distances to the Sun and are smaller than the planets, they contain the pristine information about the original composition of the protoplanetary disk./news/wp-json/wp/v2/posts/141600/u201d</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<h2>Chronicling Ancient Ice</news/wp-json/wp/v2/posts/141600//h2>/news/wp-json/wp/v2/posts/141600/n<p>Carbon monoxide ice was observed on Pluto by the New Horizons probe, but not until JWST was there an observatory powerful enough to pinpoint and detect traces of carbon monoxide ice or carbon dioxide ice on the largest population of TNOs.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>Carbon dioxide is commonly found in many objects in our solar system. So, the DiSCo team was curious to see if it existed in greater quantities beyond the reaches of Neptune.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>Possible reasons for the lack of previous detections of carbon dioxide ice on TNOs include a lower abundance, non-volatile carbon dioxide becoming buried under layers of other less volatile ices and refractory material over time, conversion into other molecules through irradiation, and simple observational limitations, according to the study.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>The discovery of carbon dioxide and carbon monoxide on the TNOs provides some context while also raising many questions, de Pr/news/wp-json/wp/v2/posts/141600/u00e1 says.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>/news/wp-json/wp/v2/posts/141600/u201cWhile the carbon dioxide was probably accreted from the protoplanetary disk, the origin of the carbon monoxide is more uncertain,/news/wp-json/wp/v2/posts/141600/u201d he says. /news/wp-json/wp/v2/posts/141600/u201cThe latter is a volatile ice even in the cold surfaces of the TNOs. We can/news/wp-json/wp/v2/posts/141600/u2019t rule out the carbon monoxide was primordially accreted and somehow was retained until present date.&nbsp;However, the data suggests that it could be produced by the irradiation from carbon-bearing ices./news/wp-json/wp/v2/posts/141600/u201d</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<h2>An Avalanche of Answers</news/wp-json/wp/v2/posts/141600//h2>/news/wp-json/wp/v2/posts/141600/n<p>Confirming the presence of carbon dioxide and carbon monoxide on TNOs opens many opportunities to further study and quantify how or why it is present, says Pinilla-Alonso, who also co-authored the study and leads the DiSCo-TNOs program.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>/news/wp-json/wp/v2/posts/141600/u201cThe discovery of carbon dioxide on trans-Neptunian objects was thrilling, but even more fascinating were its characteristics,/news/wp-json/wp/v2/posts/141600/u201d she says. /news/wp-json/wp/v2/posts/141600/u201cThe spectral imprint of carbon dioxide revealed two distinct surface compositions within our sample. In some TNOs, carbon dioxide is mixed with other materials like methanol, water ice, and silicates. However, in another group /news/wp-json/wp/v2/posts/141600/u2014 where carbon dioxide and carbon monoxide are major surface components /news/wp-json/wp/v2/posts/141600/u2014 the spectral signature was strikingly unique. This stark carbon dioxide imprint is unlike anything observed on other solar system bodies or even replicated in laboratory settings./news/wp-json/wp/v2/posts/141600/u201d</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>It now seems clear that when carbon dioxide is abundant, it appears isolated from other materials, but this alone doesn&#8217;t explain the band shape, Pinilla-Alonso says. Understanding these carbon dioxide bands is another mystery, likely tied to their unique optical properties and how they reflect or absorb specific colors of light, she says.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>It was commonly theorized that perhaps carbon dioxide may be present in TNOs as carbon dioxide exists in a gaseous state in comets, which are comparable in composition, Pinilla-Alonso says.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>/news/wp-json/wp/v2/posts/141600/u201cIn comets, we observe carbon dioxide as a gas, released from the sublimation of ices on or just below the surface,/news/wp-json/wp/v2/posts/141600/u201d she says. /news/wp-json/wp/v2/posts/141600/u201cHowever, since carbon dioxide had never been observed on the surface of TNOs, the common belief was that it was trapped beneath the surface. Our latest findings upend this notion. We now know that carbon dioxide is not only present on the surface of TNOs but is also more common than water ice, which we previously thought was the most abundant surface material. This revelation dramatically changes our understanding of the composition of TNOs and suggests that the processes affecting their surfaces are more complex than we realized./news/wp-json/wp/v2/posts/141600/u201d</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<h2>Thawing the Data</news/wp-json/wp/v2/posts/141600//h2>/news/wp-json/wp/v2/posts/141600/n<p>Study co-authors Elsa H/news/wp-json/wp/v2/posts/141600/u00e9nault, a doctoral student at the Universit/news/wp-json/wp/v2/posts/141600/u00e9 Paris-Saclay/news/wp-json/wp/v2/posts/141600/u2019s Institut d&#8217;Astrophysique Spatiale, and French National Center of Scientific Research, and Rosario Brunetto, H/news/wp-json/wp/v2/posts/141600/u00e9nault/news/wp-json/wp/v2/posts/141600/u2019s supervisor, brought a laboratory and chemical perspective into the interpretation of JWST observations.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>H/news/wp-json/wp/v2/posts/141600/u00e9nault analyzed and compared the absorption bands of carbon dioxide and carbon monoxide across all objects. While there was ample evidence of the ice, there was a great diversity in abundance and distribution, H/news/wp-json/wp/v2/posts/141600/u00e9nault says.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>/news/wp-json/wp/v2/posts/141600/u201cWhile we found CO2 to be ubiquitous across TNOs, it is definitely not uniformly distributed,/news/wp-json/wp/v2/posts/141600/u201d she says. /news/wp-json/wp/v2/posts/141600/u201cSome objects are poor in carbon dioxide while others are very rich in carbon dioxide and show carbon monoxide. Some objects display pure carbon dioxide while others have it mixed with other compounds. Linking the characteristics of carbon dioxide to orbital and physical parameters allowed us to conclude that carbon dioxide variations are likely representative of the objects/news/wp-json/wp/v2/posts/141600/u2019 different formation regions and early evolution./news/wp-json/wp/v2/posts/141600/u201d</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>Through analysis, it is very likely that carbon dioxide was present in the protoplanetary disk, however, carbon monoxide is unlikely to be primordial, H/news/wp-json/wp/v2/posts/141600/u00e9nault says.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>/news/wp-json/wp/v2/posts/141600/u201cCarbon monoxide could be efficiently formed by the constant ion bombardment coming from our sun or other sources,/news/wp-json/wp/v2/posts/141600/u201d she says. /news/wp-json/wp/v2/posts/141600/u201cWe are currently exploring this hypothesis by comparing the observations with ion irradiation experiments that can reproduce the freezing and ionizing conditions of TNO surfaces./news/wp-json/wp/v2/posts/141600/u201d</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>The research brought some definite answers to longstanding questions dating back to the discovery of TNOs nearly 30 years ago, but researchers still have a long way to go, H/news/wp-json/wp/v2/posts/141600/u00e9nault says.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>/news/wp-json/wp/v2/posts/141600/u201cOther questions are now raised,/news/wp-json/wp/v2/posts/141600/u201d she says. /news/wp-json/wp/v2/posts/141600/u201cNotably, considering the origin and evolution of the carbon monoxide. The observations across the complete spectral range are so rich that they will definitely keep scientists busy for years to come./news/wp-json/wp/v2/posts/141600/u201d</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>Although the DiSCo program observations are nearing a conclusion, the analysis and discussion of the results still have a long way to go. The foundational knowledge gained from the study will prove to be an important supplement for future planetary science and astronomy research, de Pr/news/wp-json/wp/v2/posts/141600/u00e1 says.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>/news/wp-json/wp/v2/posts/141600/u201cWe have only scratched the surface of what these objects are made of and how they came to be,/news/wp-json/wp/v2/posts/141600/u201d he says. /news/wp-json/wp/v2/posts/141600/u201cWe now need to understand the relationship between these ices with the other compounds present in their surfaces and understand the interplay between their formation scenario, dynamical evolution, volatile retention and irradiation mechanisms throughout the history of the solar system./news/wp-json/wp/v2/posts/141600/u201d</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<h2>Team Effort</news/wp-json/wp/v2/posts/141600//h2>/news/wp-json/wp/v2/posts/141600/n<p>Study co-authors also included Ana Carolina de Souza Feliciano, Charles Schambeau, Yvonne Pendelton, Dale Cruikshank and Brittany Harvison with 麻豆原创; Bryan Holler and John Stansberry with the Space Telescope Science Institute; Jorge Carvano with the Observatorio Nacional do Rio de Janeiro in Brazil; &nbsp;Javier Licandro and Vania Lorenzi with the Instituto de Astrof/news/wp-json/wp/v2/posts/141600/u00edsica de Canarias in Spain; Thomas M/news/wp-json/wp/v2/posts/141600/u00fcller with the Max-Planck-Institut f/news/wp-json/wp/v2/posts/141600/u00fcr extraterrestrische Physik in Germany; Nuno Peixinho with the Instituto de Astrof/news/wp-json/wp/v2/posts/141600/u00edsica e Ciencias do Espa/news/wp-json/wp/v2/posts/141600/u00e7o in Portugal; Aur/news/wp-json/wp/v2/posts/141600/u00e9lie Guilbert-Lepoutre with the Laboratoire de G/news/wp-json/wp/v2/posts/141600/u00e9ologie de Lyon in France; Michele Bannister with the University of Canterbury in New Zealand; and Joshua Emery and Lucas McClure with Northern Arizona University.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p><strong>Researchers&#8217; Credentials:</news/wp-json/wp/v2/posts/141600//strong></news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>De Pr/news/wp-json/wp/v2/posts/141600/u00e1 joined 麻豆原创 FSI in 2022 as an assistant scientist. He previously spent nearly four years as a <a href=/news/wp-json/wp/v2/posts/141600/"https:/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600//graduate.ucf.edu/news/wp-json/wp/v2/posts/141600//postdoc-funding-resources/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600/">preeminent postdoctoral</news/wp-json/wp/v2/posts/141600//a> associate at FSI. De Pr/news/wp-json/wp/v2/posts/141600/u00e1 received his doctorate in astronomy in 2017 at the Observat/news/wp-json/wp/v2/posts/141600/u00f3rio Nacional do Rio de Janeiro, Brazil. He works with observational planetary sciences using several ground and space-based telescopes to study the connection between different small body populations.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n<p>Pinilla-Alonso is a professor at FSI and joined in 2015. She received her doctorate in astrophysics and planetary sciences from the Universidad de La Laguna in Spain. Pinilla-Alonso also holds a joint appointment as a professor in 麻豆原创/news/wp-json/wp/v2/posts/141600/u2019s&nbsp;<a href=/news/wp-json/wp/v2/posts/141600/"https:/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600//sciences.ucf.edu/news/wp-json/wp/v2/posts/141600//physics/news/wp-json/wp/v2/posts/141600///news/wp-json/wp/v2/posts/141600/">Department of Physics</news/wp-json/wp/v2/posts/141600//a>&nbsp;and has led numerous international observational campaigns in support of NASA missions such as New Horizons, OSIRIS-REx and Lucy.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n","protected":false},"excerpt":{"rendered":"<p>A 麻豆原创-led research team/news/wp-json/wp/v2/posts/141600/u2019s findings revealed a vast presence of ancient carbon dioxide and carbon monoxide ices on trans-Neptunian objects, suggesting carbon dioxide may have existed at the formation of our solar system.</news/wp-json/wp/v2/posts/141600//p>/news/wp-json/wp/v2/posts/141600/n","protected":false},"author":199,"featured_media":141604,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"lazy_load_responsive_images_disabled":false,"footnotes":"","_links_to":"","_links_to_target":"","_wp_rev_ctl_limit":""},"categories":[5,23,24],"tags":[1775,54386,14916,4361],"tu_author":[],"class_list":["post-141600","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-colleges","category-research","category-science-technology","tag-florida-space-instit","tag-noemi-pinilla-alonso","tag-research","tag-space"],"yoast_head":"<!-- This site is optimized with the Yoast SEO Premium plugin v22.3 (Yoast SEO v27.3) - 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