Authors (*Denotes Presenter)
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Abstract Title and Summary
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Ipatov S. I.
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Delivery of Bodies to the Earth and the Moon from the Zone of the Outer Asteroid Belt [#6040]
The probability of a collision with the Earth of a body with semi-major axis between 3 and 4 AU could be greater than that for greater semi-major axes. The zone of the outer asteroid belt could be one of the sources of the late heavy bombardment.
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Ipatov S. I.
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Delivery of Icy Planetesimals to Inner Planets in the Proxima Centauri System [#6042]
A lot of icy material (more than to the Earth) could be delivered to the inner exoplanets b and in the Proxima Centauri planetary system. A cometary cloud similar to the Oort cloud can exist in this system.
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Johnson P. A. Johnson J. C. Mardon A.
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Near-Earth Objects Impact Hazard Assessment Scales [#6001]
We describe the strengths and limitations of the Torino Scale and Palermo Technical Impact Hazard Scale for impact hazard assessment and future avenues for impact hazard modelling.
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Kuznetsov E. D.
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Orbital Evolution of Phaethon Cluster [#6100]
The age of the pair (3200) Phaethon – (155140) 2005 UD is more than 1 Myr. The age of the pair (3200) Phaethon – (225416) 1999 YC exceeds 100 kyr. The age of the pair (155140) 2005 UD – (225416) 1999 YC may be 50 kyr or more.
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Kuznetsov E. D. Vasileva M. A. Rosaev A. E. Plavalova E.
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Some Examples of Close Asteroid pairs Interactions with Resonances [#6170]
Encounters with Mars have the strongest effect on the orbital evolution of pairs (9068) 1993 OD – (455327) 2002 OP28 and (88666) 2001 RP79 – (501710) 2014 UY23, moving in the vicinity of the 10–7S–3J three-body resonance with Saturn and Jupiter.
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Ohnishi I. Kadoi M. Shibata M.
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Preparation of TEM Specimens for Olivine with Specific Crystal Orientations from the Matrix in Allende CV3 Chondrite Using FIB-SEM and EBSD [#6053]
We prepared the TEM specimens from the randomly oriented olivine grains in the Allende matrix by a method combined with FIB (Focused Ion Beam) and EBSD (Electron Back Scattered Diffraction). Here, we report de-tails of the procedure and its results.
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Bruno A.
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An Archival and Oral History of the Tunguska Explosion [#6178]
This poster presentation will describe the research and results of a book project by a professional historian on the history of investigations into the Tunguska explosion of 1908 in Siberia.
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Kling A. M. Benner M. C. Thompson M. S. Greer J. Diaz R. E. Heck P. R.
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The Search for Water in Lunar Soils Through Coordinated Analysis of Space Weathering Characteristics in an Apollo 17 Sample [#6241]
Hollow nanophase iron particles were identified in a vesicle-rich region of the space weathered rim in a mature lunar mare grain. Coordinated analyses may shed light on the relationship between vesicles, water, and the hollow nanoparticles.
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Krämer Ruggiu L. Beck P. Gattacceca J. Eschrig J.
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Visible-Infrared Spectroscopy of Ungrouped and Rare Meteorites Brings Further Constraints on Meteorite-Asteroid Connections [#6160]
We studied 25 ungrouped chondrites and rare meteorite groups using VIS-NIR reflectance spectroscopy and compared their spectra to end-members spectra of asteroids taxonomy to find potential link of ungrouped meteorites to their parent bodies.
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Kampf C. E. Hamann C. Schäffer S. Heunoske D. Hasse T. Hecht L. Greshake A. Osterholz J.
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Laser-Irradiation of an Ordinary Chondrite: Simulation of Atmospheric Entry of Chondritic Materials and Links to the Formation of Micrometeorites [#6256]
Here we compare petrography and microchemistry of quenched melts produced from an ordinary chondrite in a 1-bar laser-irradiation experiment to recently described urban micrometeorites and fusion crusts developed around ordinary chondrites.
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Hill P. J. A. Chevalier M. Herd C. D. K. Hilts R. W.
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Advancing the Curation of Aldehydes and Ketones for Applications to Carbonaceous Chondrite Curation and Cometary Nucleus Sample Return [#6119]
The aim of this study is to examine the reactivity of carbonyl compounds under a variety of conditions to provide insight into the curation and handling requirements of organic-rich astromaterials.
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Nissinen M. Gritsevich M. Oksanen A. Suomela J.
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Modeling of Cometary Dust Trails [#6010]
We present the ‘Dust Trail kit’ model describing the evolution of cometary dust trails. As a case study, we demonstrate our analysis of the physical and spatial characteristics of the dust trail produced by the 2007 explosion of comet 17P/Holmes.
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MSPG2 Team Beaty D. W. Carrier B. L. Kminek G. Meyer M. A. Haltigin T. Hays L. E. Agee C. B. Busemann H. Cavalazzi B. Cockell C. S. Debaille V. Glavin D. P. Grady M. M. Hauber E. Hutzler A. Marty B. McCubbin F. M. Pratt L. M. Regberg A. B. Smith A. L. Smith C. L. Summons R. E. Swindle T. D. Tait K. T. Tosca N. J. Udry A. Usui T. Velbel M. A. Wadhwa M. Westall F. Zorzano M.-P.
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Summary of Mars Sample Return (MSR) Science Planning Group 2: Planning for the Arrival and Analysis of MSR Samples at Earth [#6242]
MSPG2’s overarching aims were to build upon previous efforts in defining an end-to-end MSR Science Program, and addressing important issues that will influence the design and implementation of the Sample Receiving Facility.
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Safronova V. S. Kuznetsov E. D.
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Estimation of the Age of Two Young Pairs of Asteroids [#6144]
The age of the pair (87887) 2000 SS286 – (415992) 2002 AT49 ranges from 7.58 ± 0.035 to 8.8 ± 0.043 kyr; for the pair (320025) 2007 DT76 – (489464) 2007 DP16 one ranges from 15.4 ± 0.96 to 29.5 ± 0.04 kyr depends on the semimajor axis Yarkovsky drift.
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Ovcharenko A. V. Schapov V. A. Muravyev L. A.
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Geophysical Search of the Sterlitamak Meteorite [#6046]
We describe the results of our geophysical studies (magnetic survey) on the territory of the crater formed after the fall of the sterlitamak meteorite. On our opinion, a significant mass of the meteorite may still be in the crater.
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Christ O. Barbaro A. Brenker F. E. Domeneghetti M. C. Nestola F.
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Shock Temperature Records in Graphite from the Northwest Africa 6871 Ureilite [#6052]
Northwest Africa 6871 was studied by XRD and µ-Raman. It contains aggregates of nanographite and micro/nanodiamond. A graphite-geothermometer revealed a temperature of 1412 °C, which we ascribed to the shock event which destroyed the parent body.
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Andreev A. O. Nefedyev Y. A.
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Analysis of Broadband Color Characteristics and Spectral Distribution of Asteroids with Small Perihelion Distances [#6057]
The purpose of this study is to analyze the genetic relationships of asteroids with small perihelion distances with meteor showers by broadband color characteristics based on modern optical observations with various color filters.
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Andreev A. O. Nefedyev Y. A.
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Creation of an Imitation Model of Near-Sun Asteroids with Small Perihelion Distances [#6058]
The work is focused on creating a simulation model of near-Sun asteroids (NSAs) with small perihelion distances. The model includes astrophysical parameters of these objects, size distribution and their dynamic behavior in space.
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Churkin K. O. Nefedyev Y. A. De La Morena C. Andreev A. O. Ahmedshina E. N.
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Analysis of Digital Model of Titan Using Fractal Geometry and Automated Complex for Studies [#6113]
This work aims at considering the issues of regression modeling of the surface of Saturn’s moon, Titan and at studying the produced model by means of fractal geometry. Based on data collected by NASA Cassini the Titan surface model was created.
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Churkin K. O. Andreev A. O. Nefedyev Y. A.
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Creation of a Unified Selenocentric System Using Quantum Optical Systems [#6114]
The work is devoted to the development of a method for creating a unified selenocentric system for a space satellite in a circumlunar orbit (SSCLO) and reference objects on the lunar surface using quantum optical devices.
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Nefedyev Y. A. Sergienko M. V. Andreev A. O.
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Analysis of Orbital Elements of Near Earth Objects over a Long-Term Period [#6087]
The aim of this work is to analyze the changes in orbital elements of near earth objects (NEO) and to identify them with the meteor shower Delta Cancrids (MSDC). For MSDC connections with asteroids were investigated.
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Nefedyev Y. A. Sergienko M. V. Andreev A. O.
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The Coordinate Ranging of the Delta Cancrids Meteor Shower [#6088]
The aim of this work is to refine the radiants distribution of the meteor shower Delta Cancrids (MSDC) branches and their drift motion and to study features of radiants distribution and orbit elements for MSDC using television observations.
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