Search Results - "CIESLA, Fred J."

Transport of CO in Protoplanetary Disks: Consequences of Pebble Formation, Settling, and Radial Drift by Krijt, Sebastiaan, Schwarz, Kamber R., Bergin, Edwin A., Ciesla, Fred J.

“…Current models of (exo)planet formation often rely on a large influx of so-called "pebbles" from the outer disk into the planet formation region. In this…”
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Outward Transport of High-Temperature Materials Around the Midplane of the Solar Nebula by Ciesla, Fred J

“…The Stardust samples collected from Comet 81P/Wild 2 indicate that large-scale mixing occurred in the solar nebula, carrying materials from the hot inner…”
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CO Depletion in Protoplanetary Disks: A Unified Picture Combining Physical Sequestration and Chemical Processing by Krijt, Sebastiaan, Bosman, Arthur D., Zhang, Ke, Schwarz, Kamber R., Ciesla, Fred J., Bergin, Edwin A.

“…The gas-phase CO abundance (relative to hydrogen) in protoplanetary disks decreases by up to two orders of magnitude from its interstellar medium value of…”
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TRACING WATER VAPOR AND ICE DURING DUST GROWTH by Krijt, Sebastiaan, Ciesla, Fred J., Bergin, Edwin A.

“…ABSTRACT The processes that govern the evolution of dust and water (in the form of vapor or ice) in protoplanetary disks are intimately connected. We have…”
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Organic Synthesis via Irradiation and Warming of Ice Grains in the Solar Nebula by Ciesla, Fred J., Sandford, Scott A.

“…Complex organic compounds, including many important to life on Earth, are commonly found in meteoritic and cometary samples, though their origins remain a…”
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DUST DIFFUSION AND SETTLING IN THE PRESENCE OF COLLISIONS: TRAPPING (SUB)MICRON GRAINS IN THE MIDPLANE by Krijt, Sebastiaan, Ciesla, Fred J.

“…ABSTRACT In protoplanetary disks, the distribution and abundance of small (sub)micron grains are important for a range of physical and chemical processes. For…”
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Dust Transport and Processing in Centrifugally Driven Protoplanetary Disk Winds by Giacalone, Steven, Teitler, Seth, Königl, Arieh, Krijt, Sebastiaan, Ciesla, Fred J.

“…There is evidence that protoplanetary disks-including the protosolar one-contain crystalline dust grains on spatial scales where the dust temperature is lower…”
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The Exoplanet Population Observation Simulator. II. Population Synthesis in the Era of Kepler by Mulders, Gijs D., Mordasini, Christoph, Pascucci, Ilaria, Ciesla, Fred J., Emsenhuber, Alexandre, Apai, Dániel

“…The collection of planetary system properties derived from large surveys such as Kepler provides critical constraints on planet formation and evolution. These…”
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Quantifying the High Early Solar Cosmic-Ray Flux with Cosmogenic Neon Isotopes in Refractory Minerals by Yang, Xin, Ciesla, Fred J., Heck, Philipp R.

“…An enhancement in the activity of the early young Sun resulting in a high charged particle flux has been invoked to explain excesses in spallation-induced…”
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Sensitivities of Earth's core and mantle compositions to accretion and differentiation processes by Fischer, Rebecca A., Campbell, Andrew J., Ciesla, Fred J.

“…The Earth and other terrestrial planets formed through the accretion of smaller bodies, with their core and mantle compositions primarily set by metal–silicate…”
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Chemical Feedback of Pebble Growth: Impacts on CO depletion and C/O ratios by Van Clepper, Eric, Bergner, Jennifer B., Bosman, Arthur D., Bergin, Edwin, Ciesla, Fred J.

“…Observations of protoplanetary disks have revealed them to be complex and dynamic, with vertical and radial transport of gas and dust occurring simultaneously…”
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Dynamics of the terrestrial planets from a large number of N-body simulations by Fischer, Rebecca A., Ciesla, Fred J.

“…The agglomeration of planetary embryos and planetesimals was the final stage of terrestrial planet formation. This process is modeled using N-body accretion…”
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Early aqueous activity on the ordinary and carbonaceous chondrite parent bodies recorded by fayalite by Doyle, Patricia M., Jogo, Kaori, Nagashima, Kazuhide, Krot, Alexander N., Wakita, Shigeru, Ciesla, Fred J., Hutcheon, Ian D.

“…Chronology of aqueous activity on chondrite parent bodies constrains their accretion times and thermal histories. Radiometric 53 Mn– 53 Cr dating has been…”
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The effects of disk building on the distributions of refractory materials in the solar nebula by YANG, Le, CIESLA, Fred J.

“…– Refractory materials, such as calcium‐aluminum‐rich inclusions (CAIs) and crystalline silicates, are widely found in chondritic meteorites as well as comets,…”
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Destruction of Refractory Carbon in Protoplanetary Disks by Anderson, Dana E., Bergin, Edwin A., Blake, Geoffrey A., Ciesla, Fred J., Visser, Ruud, Lee, Jeong-Eun

“…The Earth and other rocky bodies in the inner solar system contain significantly less carbon than the primordial materials that seeded their formation. These…”
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Post-impact thermal evolution of porous planetesimals by Davison, Thomas M., Ciesla, Fred J., Collins, Gareth S.

“…Impacts between planetesimals have largely been ruled out as a heat source in the early Solar System, by calculations that show them to be an inefficient heat…”
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The D/H ratio of water in the solar nebula during its formation and evolution by Yang, Le, Ciesla, Fred J., Alexander, Conel M.O’D.

“…•We explore D–H exchange among major gas species in an evolving protoplanetary disk.•The evolving disk accounts for disk formation and angular momentum…”
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Measuring the level of interstellar inheritance in the solar protoplanetary disk by Alexander, Conel M. O'D., Nittler, Larry R., Davidson, Jemma, Ciesla, Fred J.

“…The timing and extent to which the initial interstellar material was thermally processed provide fundamental constraints for models of the formation and early…”
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Exoplanet Volatile Carbon Content as a Natural Pathway for Haze Formation by Bergin, Edwin A., Kempton, Eliza M.-R., Hirschmann, Marc, Bastelberger, Sandra T., Teal, D. J., Blake, Geoffrey A., Ciesla, Fred J., Li, Jie

“…We explore terrestrial planet formation with a focus on the supply of solid-state organics as the main source of volatile carbon. For the water-poor Earth, the…”
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The early impact histories of meteorite parent bodies by Davison, Thomas M., O'Brien, David P., Ciesla, Fred J., Collins, Gareth S.

“…We have developed a statistical framework that uses collisional evolution models, shock physics modeling, and scaling laws to determine the range of plausible…”
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