Publications by authors named "Fulvio D"

Article Synopsis
  • Ceres has notable amounts of aliphatic organics, with concentrations ranging from 5 to over 30 weight % in certain areas of its surface.
  • The origins and longevity of these organics are questioned, especially since radiation levels in Ceres' orbit should typically break them down, complicating their detection.
  • Laboratory experiments suggest that organic materials degrade quickly under radiation, indicating that buried organics may have been exposed in the recent past, and estimates show the initial abundance of aliphatics could be 2 to 30 times higher than what is currently observed.
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Article Synopsis
  • Researchers investigated how heat and UV light interact to produce complex organic molecules in cosmic ice analogues at different temperatures (75, 120, and 150 K), relevant to the environments where stars and planets form.
  • The combination of heat and UV irradiation led to the detection of multiple complex molecules, including acetaldehyde, urea, and tentatively glycine, indicating their potential as prebiotic building blocks.
  • Experiments showed that reactions were more effective on flat KBr substrates than on amorphous silicate grains, suggesting that the unique properties of cosmic dust affect surface chemistry significantly.
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Article Synopsis
  • Understanding life’s origins involves studying prebiotic systems through physical, chemical, and biological lenses, focusing on Complex Organic Molecules (COMs) as potential prebiotic precursors.
  • COMs have been identified in various astrophysical settings, including interstellar clouds and comets, but the exact processes behind their formation remain unclear.
  • Laboratory experiments simulating space conditions provide insights into COMs' formation and evolution, and the review discusses prevalent detection techniques, their pros and cons, and offers perspectives on emerging methods to address existing experimental hurdles.
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Water ice exists on many objects in space. The most abundant icy species, among them water, are present in the icy satellites of the outer Solar System giant planets. The nuclei of comets, which are mainly composed of water ice, give another example of its abundance.

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We present a novel experimental study on solid CHDOH pure and in astrophysical relevant mixtures. Solid samples were accreted under ultra high vacuum conditions at 17 K and were analyzed by mid-infrared transmission spectroscopy. Refractive index, density, and mid-IR band strength values were measured for pure solid CHDOH.

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We study the potentialities of a two-color Surface Plasmon Resonance (SPR) spectroscopy nanosizer by monitoring the assembling of a colloidal dispersion of citrate stabilized gold nanoparticles (AuNPs) on SiO surface. When the AuNPs/water composite's optical density layer is negligible and the electron mean-free path limitation is taken into account in the AuNPs' dielectric constant;s formulation, the surface density σ of the nanoparticle array and the statistical mean size of the nanoparticles can be straightly determined by using two-color SPR spectroscopy in the context of Maxwell's Garnett theory. The optical method, demonstrated experimentally for AuNPs with a nominal mean diameter of 15 nm, can, theoretically, be extended to bigger nanoparticles, based on a simple scaling relation between the extinction cross section of the single nanoparticle σ and the surface density σ.

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Ion implantation experiments were carried out on amorphous (30 K) and crystalline (80 K) solid CO2 using both reactive (D(+), H(+)) and non-reactive (He(+)) ions, simulating different irradiation environments on satellite and dust grain surfaces. Such ion irradiation synthesized several new species in the ice including ozone (O3), carbon trioxide (CO3), and carbon monoxide (CO) the main dissociation product of carbon dioxide. The yield of these products was found to be strongly dependent upon the ion used for irradiation and the sample temperature.

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We present novel measurements of the refractive index, density and integrated band strengths of mid-infrared features of solid N(2)O at 16K and of NO(2) and N(2)O(4) in two frozen NO(2):N(2)O(4) mixtures deposited at 16 and 60K. The refractive index and density measurements were performed also for frozen O(2) deposited at 16K. In this case, the integrated band strength values could not be determined since O(2) is a homonuclear molecule and therefore its fundamental mode is not infrared active.

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