Search Results - "Durda, Daniel D."
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New Horizons Observations of the Cosmic Optical Background
Published in The Astrophysical journal (01-01-2021)“…Abstract We used existing data from the New Horizons Long-range Reconnaissance Imager (LORRI) to measure the optical-band (0.4 ≲ λ ≲ 0.9 μ m) sky brightness…”
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Delivery of dark material to Vesta via carbonaceous chondritic impacts
Published in Icarus (New York, N.Y. 1962) (01-11-2012)“…► Dark material on Vesta observed by Dawn is remnant carbonaceous chondrite impactor. ► Global abundance of carbonaceous chondrite material <6vol.% similar to…”
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Momentum transfer in hypervelocity cratering of meteorites and meteorite analogs: Implications for orbital evolution and kinetic impact deflection of asteroids
Published in International journal of impact engineering (01-02-2020)“…•Ejecta from hypervelocity impact cratering results in significant momentum transfer, equaling or exceeding the direct momentum transfer from the…”
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A comparison between rubble-pile and monolithic targets in impact simulations: Application to asteroid satellites and family size distributions
Published in Icarus (New York, N.Y. 1962) (01-05-2012)“…► We compare impact simulations of rubble-pile and monolithic targets. ► Size–frequency distributions (SFDs) for each type display different features. ► The…”
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Hypervelocity cratering and disruption of porous pumice targets: Implications for crater production, catastrophic disruption, and momentum transfer on porous asteroids
Published in Planetary and space science (01-03-2015)“…Most asteroids for which porosities have been inferred have porosities from 20% to>50%. To investigate the effects of target porosity on cratering, impact…”
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The shapes of fragments from catastrophic disruption events: Effects of target shape and impact speed
Published in Planetary and space science (01-03-2015)“…We conducted impact experiments at the NASA Ames Vertical Gun Range in the context of an ongoing set of experiments to investigate both target shape and impact…”
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Experimental determination of the coefficient of restitution for meter-scale granite spheres
Published in Icarus (New York, N.Y. 1962) (2011)“…We present results of a series of large-scale experiments to measure the coefficient of restitution for 1-m-diameter rocky bodies in impacts with collision…”
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Trajectories and distribution of material ejected from the Chicxulub impact crater: Implications for postimpact wildfires
Published in Journal of Geophysical Research - Planets (01-08-2002)“…The trajectories of low‐ and high‐energy ejecta from the Chicxulub impact crater have been computed using a numerical code and compared with analyses of debris…”
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Experimental investigation of the impact fragmentation of blocks embedded in regolith
Published in Meteoritics & planetary science (01-01-2011)“…– We present results of a set of impact experiments designed to examine the effects of impacts onto rocky blocks resting on and embedded within regoliths. The…”
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Ignition threshold for impact-generated fires
Published in Journal of Geophysical Research - Planets (01-08-2004)“…Widespread fires can be generated after large impact events by atmospheric heating caused by the reaccretion of high‐energy, vapor‐rich plume material. We…”
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Momentum enhancement simulations for hypervelocity impacts on sandstone
Published in International journal of impact engineering (01-05-2021)“…•Generated material constants from test and literature data that capture the proper physics (pressure dependence, strain rate, strength of failed material,…”
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The fossilized size distribution of the main asteroid belt
Published in Icarus (New York, N.Y. 1962) (01-05-2005)“…Planet formation models suggest the primordial main belt experienced a short but intense period of collisional evolution shortly after the formation of…”
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Linking the collisional history of the main asteroid belt to its dynamical excitation and depletion
Published in Icarus (New York, N.Y. 1962) (01-12-2005)“…The main belt is believed to have originally contained an Earth mass or more of material, enough to allow the asteroids to accrete on relatively short…”
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Size–frequency distributions of fragments from SPH/N-body simulations of asteroid impacts: Comparison with observed asteroid families
Published in Icarus (New York, N.Y. 1962) (01-02-2007)“…We investigate the morphology of size–frequency distributions (SFDs) resulting from impacts into 100-km-diameter parent asteroids, represented by a suite of…”
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Hypervelocity cratering and disruption of the Northwest Africa 869 ordinary chondrite meteorite: Implications for crater production, catastrophic disruption, momentum transfer and dust production on asteroids
Published in Planetary and space science (01-12-2018)“…Most asteroids for which porosities have been inferred have porosities from 20% to more than 50%, comparable to the range measured on chondritic meteorites. To…”
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A New Facility for Airborne Solar Astronomy: NASA's WB-57 at the 2017 Total Solar Eclipse
Published in The Astrophysical journal (01-06-2020)“…NASA's WB-57 High Altitude Research Program provides a deployable, mobile, and stratospheric platform for scientific research. Airborne platforms are of…”
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Detecting crater ejecta-blanket boundaries and constraining source crater regions for boulder tracks and elongated secondary craters on Eros
Published in Meteoritics & planetary science (01-06-2012)“…– We present results of a numerical model of the dynamics of ejecta emplacement on asteroid 433 Eros. Ejecta blocks represent the coarsest fraction of Eros’…”
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Karin cluster formation by asteroid impact
Published in Icarus (New York, N.Y. 1962) (01-08-2006)“…Insights into collisional physics may be obtained by studying the asteroid belt, where large-scale collisions produced groups of asteroid fragments with…”
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The formation of asteroid satellites in large impacts: results from numerical simulations
Published in Icarus (New York, N.Y. 1962) (01-07-2004)“…We present results of 161 numerical simulations of impacts into 100-km diameter asteroids, examining debris trajectories to search for the formation of bound…”
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Collisional Models and Scaling Laws: A New Interpretation of the Shape of the Main-Belt Asteroid Size Distribution
Published in Icarus (New York, N.Y. 1962) (01-10-1998)“…Numerical models of the collisional evolution of the main-belt asteroids lead to a new interpretation of the shape of the observed size distribution. Using…”
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