A 42. LPSC, 2011, márc. 7-11. Houston, NASA konferenciára elfogadva:
42nd Lunar and Planetary Science Conference (2011) Teljes lista
1039: Gyollai Ildikó et al.: Vizes átalakulások: Kaba és Yamato (dec. 15)
1157: Gucsik A. et al.: Kaba forszterit (dec. 29.)
1227: Futó P., Gucsik A.: Carbon Planet Model with SiC Mantle Compound.
1229: Futó P., Gucsik A.: Coreless Earth-Mass Exomoon of an EGP.
1285: Nagy Sz. et al.: NWA 5011 (jan. 2. délben)
1296: Lang Ágota et al.: Husar-5. Red Planet? Red River! (jan. 2. fél 5-kor)
1305: Orgel Csilla: Cryokarstic surface patterns on Debris Aprons …of Mars.
1348: Bérczi Zsófi et al.: Színházi planetomorfológia (jan. 3. 11-kor)
1351: Kereszturi Á.: Mars.
1354: Illes-Almar E.: Comet Hartley and the two kinds of cometary sub-nuclei.
1366: Horváth A., Illés-Almar E.: A Lutetia felszíni rovátkarendszere.
1410: Deák M.: Puli leszállási helyek a Holdon.
1688: Horváth et ESA MAG: DDS, Inca City (jan. 4. fél 12)
1931: Bérczi et Planeto-Kör.: Atlasz-13 (jan. 4. fél 5)
1990: Hegyi S et al.: PTE eLearning kurzus (jan. 4. fél 7)
2014: Vizi P.: Magyarok a Marson robotvetélkedő.
2150: Varga T. N. et al. (VTP, Meteorit-Kör).: Ries-suevit impact…
2345: Kabai et al.: Reconfig. Robots (Wolfram Math.) (jan. 410 óra)
2777: Vizi P.: Nem állami űrtevékenység – mikro- és nano-űrszondák - Puli.
Tuesday, March 8, 2011
POSTER SESSION I: ASTEROID PHOTOGEOLOGY sess311.pdf
6:00 p.m. Town Center Exhibit Area
Horváth A. Illés-Almár E.
Grooves on 21 Lutetia Indicate a Layered Structure [#1366]
On the image of asteroid 21 Lutetia craters as well as grooves can be identified. On the basis of the existence of parallel grooves we suggest that Lutetia might be a near-surface block of an ancient, larger differentiated body.
Tuesday, March 8, 2011
POSTER SESSION I: IMPACTS II: TERRESTRIAL CRATERS sess321.pdf
6:00 p.m. Town Center Exhibit Area
Varga T. N. Gucsik A. Bérczi Sz. Nagy Sz. Veres M. Varga T. P.
Micro-Raman Properties of Quartz in Suevite Breccia from Ries Impact Crater, Germany [#2150]
The purpose of this study is to determine the possible shock pressures observable in the suevite found in the Ries Crater by micro-Raman spectroscopy, and by comparison with previous studies, thus utilizing the method of shock barometry.
Tuesday, March 8, 2011
POSTER SESSION I: CRYOSPHERE: ICY INSIGHTS INTO MARS PALEOCLIMATE sess327.pdf
6:00 p.m. Town Center Exhibit Area
Orgel Cs.
Analysis of Cryokarstic Surface Patterns on Debris Aprons at the Mid-Latitudes of Mars [#1305]
This work focuses on the morphological analysis of the surface patterns (mounds, furrows, craters) and surface types (smooth surface, corn-like surface, polygonal mantling material, brain-like texture) on debris apron surfaces using HiRISE’s images.
Tuesday, March 8, 2011
POSTER SESSION I: SEASONAL ICE PROCESSES sess329.pdf
6:00 p.m. Town Center Exhibit Area
Horvath A. Bérczi Sz. Kereszturi A. Sik A. Szathmáry E.
Observation of a Transitional Reversal During the Seasonal Defrosting of DDS at the Southern Polar Region of Mars [#1688]
We observed a transitional reversal in the advancing dark dune spot (DDS) defrosting process in spring. After this interruption the defrosting process continued till the summer total defrosting of the surface in the Inca City Region of Mars.
Tuesday, March 8, 2011
POSTER SESSION I: PLANETARY MISSION CONCEPTS sess334.pdf
6:00 p.m. Town Center Exhibit Area
Vizi P. G.
Possibilities After Governmental Space Research like Micro and Nano Space Probes — The Hungarian Puli Space [#2777]
Governmental operation is decreasing and private inventions are increasing. Is this a reachable goal to make a new generation of devices like cube sats and micro probes to use for lunar and planetary research?.
Deák M.
Landing Site Analysis for Low-Budget Lunar Missions — Landing Site Candidates of Team Puli Space, Participant of the Google Lunar X Prize [#1410]
The landing site analysis of privately funded low-budget lunar missions, for example, the mission of the Google Lunar X Prize participant Team Puli Space, is more influenced by technological possibilities than the government-funded missions.
Tuesday, March 8, 2011
POSTER SESSION I: EDUCATION AND PUBLIC OUTREACH: UNDERGRADUATE EDUCATION sess339.pdf
6:00 p.m. Town Center Exhibit Area
Hegyi S. Bérczi Sz. Kereszturi A. Hargitai H.
E-Learning — Innovative Pedagogical Project in the Higher Education to Promote and Support Space Sciences and Technology [#1990]
The Pécs University’s e-Learning method of presentations represents a new online up-to-date system for the new web oriented student generation in sciences and mathematics, focusing on space sciences and technology, in accord with NASA STEM project.
Tuesday, March 8, 2011
POSTER SESSION I: EDUCATION AND PUBLIC OUTREACH: HIGH SCHOOL RESEARCH/COMPETITION sess341.pdf
6:00 p.m. Town Center Exhibit Area
Sipos A. Vizi P. G.
Simulated Mars Rover Model Competition 2010–2011 [#2014]
This is a report about the organization and management of the Simulated Mars Rover Competition events of 2010 and 2011.
Lang Á. Erdélyi S. Nickl I. Cserich D. Kiss D. Bérczi Sz.
Red Planet? Red River! Field Works on the Red-Mud Flood Polluted Marcal Riverside: pH Measurements by the Husar-5 NXT-Based Rover Model of the Széchenyi István High School, Sopron, Hungary [#1296]
We took planetary analog field measurements of pH by the HUSAR-5 rover along the red-mud polluted riverside of the Marcal river after the sludge catastrophe in Ajka Alumina Plant, Hungary, and observed the gradually decreasing pH values.
Csütörtök
Thursday, March 10, 2011
POSTER SESSION II: PRIMITIVE METEORITES I: DIVERSITY sess608.pdf
6:00 p.m. Town Center Exhibit Area
Nagy Sz. Gyollai I. Józsa S. Bérczi Sz.
Observation of Colouration of Ringwoodite in the NWA 5011 L5-6 Chondrite [#1285]
In this abstract we are doing a proof to summarize our observation about the colours of the ringwoodite aggregates, and we propose a possible new idea for the origin of the colorless parts in blue aggregates.
Swindle et al. Three heavily shocked L6 chondrites clearly record resetting of their K-Ar systems in the last ~1000 Ma. However, their Ar systematics are complicated enough that it is not obvious whether they were involved in the 475 Ma L-chondrite event.
Thursday, March 10, 2011
POSTER SESSION II: PRIMITIVE METEORITES II: CARBONACEOUS CHONDRITES AND NEW MINERALS sess609.pdf
6:00 p.m. Town Center Exhibit Area
Gyollai I. Nagy Sz. Bérczi Sz. Gucsik A.
Comparison of Aqueous Alteration of Two CV3 (Kaba and Yamato-86751) Chondrites [#1039]
The Kaba meteorite has more pervasive aqueous alteration inside their chondrules; the Y-86751 CV3 chondrite has more altered matrix with flow structure, but much better preserved chondrules.
Gucsik A. Endo T. Nakazato E. Nishido H. Ninagawa K. Kayama M. Bérczi Sz. Nagy Sz. Ábrahám P. Kimura Y. Gyollai I. Simonia I. Rózsa P. Posta J. Nagy M. Mihályi K. Apai D. Futó P.
Cathodoluminescence Characterization of the Forsterite in Kaba Meteorite: An Astromineralogical Application [#1157]
A combined CL and SEM study implies that the aqueous alteration on the Kaba forsterite might eliminate intrinsic structural defects progressively from the rim of the grain to the core, accompanied by the migration of diffusible ions of Mn, Cr, and Fe to the rim.
Thursday, March 10, 2011
POSTER SESSION II: PLANETARY DIFFERENTIATION sess627.pdf
6:00 p.m. Town Center Exhibit Area
Futó P. Gucsik A.
Carbon Planet Model with SiC Mantle Compound [#1227]
The existence of a carbon planet is highly probable by reason of astrophysical consideration. For the case of the same mass and core mass fraction (CMF) ratios their diameters are slightly larger than that of a terrestrial planet.
Thursday, March 10, 2011
POSTER SESSION II: INSTRUMENT AND PAYLOAD CONCEPTS sess636.pdf
6:00 p.m. Town Center Exhibit Area
Kabai S. Bérczi Sz.
A Study of Possible Geometries of Modules for Shape Changing and Self Reconfigurable Robots with the Use of Interactive Wolfram Mathematica Demonstrations [#2345]
The self-reconfiguration of modules in robots could be used to change the overall functionality of the robots serving specific purposes. This abstract shows a few examples from the many different solutions we studied.
PRINT ONLY: SMALL BODIES sess. 804.
Illés-Almár E.
Comet Hartley 2 and the Two Kinds of Cometary Sub-Nuclei [#1354]
The images of the nucleus of Comet Hartley 2 strengthen our earlier hypothesis that the subnuclei, building up the nucleus of a comet, can be of different hardness.
PRINT ONLY: PLANETARY DYNAMICS AND TECTONICS sess. 806
Futó P. Gucsik A.
Coreless Earth-Mass Exomoon of an EGP [#1229]
Physical properties for a modeled moon: radius is about 7008 km (1.1 REarth with roughly 2% uncertainty) and continental lithospheric thickness is 114 km; surface gravity is 8.1 m/s2, which is 82.5% of the Earth average value.
PRINT ONLY: MISSION, INSTRUMENTS, AND PAYLOAD CONCEPTS sess. 815
Kereszturi A.
Extrapolation of Shallow Subsurface Structures from Orbital Data — Case Study for ExoMars Rover Mission [#1351]
This paper presents the basis of the methods for how the location and parameters of subsurface features accessible by the drill sampling equipment of ExoMars Rover could be estimated from remote sensing data.
PRINT ONLY: EDUCATION AND PUBLIC OUTREACH sess. 817.
Bérczi Sz. Hargitai H. Homolya E. Illés E. Kereszturi A. Mörtl M. Sik A. Tasnádi P. Weidinger T.
Liquids in the Solar System: New Concise Atlas in the Solar System Series of Textbooks at Eötvös University, Hungary [#1931]
The new Solar System Liquids atlas deals with (1) cloud droplets and cloud formation processes in planetary atmospheres; (2) liquids on planetary surfaces and below surfaces; (3) liquids deep inside planetary bodies and eruptions to surfaces.
Bérczi Zs. Bérczi Sz. Terebessy T.
Planetary Geology Education on the Stage: Dynamics of Planetary Morphology in Theatre Performance [#1348]
The Living Picture Company planned and produced a performance, where planetary surface dynamics were realized and planetary morphology processes were animated, both of which are useful in planetary morphology education.
http://www.lpi.usra.edu/meetings/lpsc2011/pdf/program.pdf