Abstract:Abstract. Organic compounds are ubiquitous in space: they are found in diffuse clouds, in the envelopes of evolved stars, in dense star-forming regions, in protoplanetary disks, in comets, on the surfaces of minor planets, and in meteorites and interplanetary dust particles. This brief overview summarizes the observational evidence for the types of organics found in these regions, with emphasis on recent developments. The Stardust sample-return mission provides the first opportunity to study primitive cometary… Show more
“…These ices are exposed to the stellar UV flux and may ultimately produce tholin-like organic residues. 7 A porosity in the range of is expected for dust aggregates 0.80 Շ P Շ 0.97 formed through coagulation as shown both theoretically (Cameron & Schneck 1965;Wada et al 2008) and experimentally (Blum et al 2006). tron microscope imaging.…”
The red spectral shape of the visible to near infrared reflectance spectrum
of the sharply-edged ring-like disk around the young main sequence star HR
4796A was recently interpreted as the presence of tholin-like complex organic
materials which are seen in the atmosphere and surface of Titan and the
surfaces of icy bodies in the solar system. However, we show in this Letter
that porous grains comprised of common cosmic dust species (amorphous silicate,
amorphous carbon, and water ice) also closely reproduce the observed
reflectance spectrum, suggesting that the presence of complex organic materials
in the HR 4796 disk is still not definitive.Comment: 6 pages, 3 figures; To be published in The Astrophysical Journal
Letter
“…These ices are exposed to the stellar UV flux and may ultimately produce tholin-like organic residues. 7 A porosity in the range of is expected for dust aggregates 0.80 Շ P Շ 0.97 formed through coagulation as shown both theoretically (Cameron & Schneck 1965;Wada et al 2008) and experimentally (Blum et al 2006). tron microscope imaging.…”
The red spectral shape of the visible to near infrared reflectance spectrum
of the sharply-edged ring-like disk around the young main sequence star HR
4796A was recently interpreted as the presence of tholin-like complex organic
materials which are seen in the atmosphere and surface of Titan and the
surfaces of icy bodies in the solar system. However, we show in this Letter
that porous grains comprised of common cosmic dust species (amorphous silicate,
amorphous carbon, and water ice) also closely reproduce the observed
reflectance spectrum, suggesting that the presence of complex organic materials
in the HR 4796 disk is still not definitive.Comment: 6 pages, 3 figures; To be published in The Astrophysical Journal
Letter
“…On Earth, organic materials are carbon-based compounds that have come from the remains of organisms and their waste products. In space, organic compounds are ubiquitous, as they are found in diffuse clouds, in the envelopes of evolved stars, in dense starforming regions, in protoplanetary discs, in comets, on the surfaces of minor planets, in meteorites and in interplanetary dust particles (van Dishoeck 2008). Stars at different evolutionary phases are able to produce complex organic compounds and eject them into space, filling the regions between the stars.…”
Section: Introductionmentioning
confidence: 99%
“…Studying carbonaceous chondrites, the most primitive and least processed meteorites, may provide the closest picture of the chemical composition of non-volatile, organic cometary matter. Most of the organics found in carbonaceous chondrites are in an insoluble macro-molecular form, often described as kerogen-like (van Dishoeck 2008). The remaining part consists of soluble organics, such as corboxylic acids, PAHs, fullerenes, purines, amides and other prebiotic molecules (Botta & Bada 2002).…”
Knowledge of the mechanical properties of protoplanetary and cometary matter is of key importance to better understand the activity of comets and the early stages of planet formation. The tensile strength determines the required pressure to lift off grains, pebbles and agglomerates from the cometary surface and also describes how much strain a macroscopic body can withstand before material failure occurs. As organic materials are ubiquitous in space, they could have played an important role during the planet formation process. This work provides new data on the tensile strength of five different micro-granular organic materials, namely, humic acid, paraffin, brown coal, charcoal and graphite. These materials are investigated by the so-called Brazilian Disc Test and the resulting tensile strength values are normalised to a standard grain size and volume filling factor. We find that the tensile strength of these materials ranges over four orders of magnitude. Graphite and paraffin possess tensile strengths much higher than silica, whereas coals have very low tensile strength values. This work demonstrates that organic materials are not generally stickier than silicates, or water ice, as often believed.
scite is a Brooklyn-based organization that helps researchers better discover and understand research articles through Smart Citations–citations that display the context of the citation and describe whether the article provides supporting or contrasting evidence. scite is used by students and researchers from around the world and is funded in part by the National Science Foundation and the National Institute on Drug Abuse of the National Institutes of Health.