TY  - JOUR
AU  - Nagy, Balázs
AU  - Kovács, József
AU  - Ignéczi, Ádám
AU  - Beleznai, Szabolcs
AU  - Mari, László
AU  - Kereszturi, Ákos
AU  - Szalai, Zoltán
TI  - The thermal behavior of ice-bearing ground : the highest cold, dry desert on Earth as an analog for conditions on Mars, at Ojos del Salado, Puna de Atacama-Altiplano Region
JF  - ASTROBIOLOGY
J2  - ASTROBIOLOGY
VL  - 20
PY  - 2020
IS  - 6
SP  - 701
EP  - 722
PG  - 22
SN  - 1531-1074
DO  - 10.1089/ast.2018.2021
UR  - https://m2.mtmt.hu/api/publication/31344017
ID  - 31344017
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Pál, Bernadett
AU  - Kereszturi, Ákos
TI  - Annual and daily ideal periods for deliquescence at the landing site of InSight based on GCM model calculations
JF  - ICARUS
J2  - ICARUS
VL  - 340
PY  - 2020
SN  - 0019-1035
DO  - 10.1016/j.icarus.2020.113639
UR  - https://m2.mtmt.hu/api/publication/31159376
ID  - 31159376
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Skultéti, Ágnes
AU  - Kereszturi, Ákos
AU  - Szabó, Máté Zoltán
AU  - Kereszty, Zs
AU  - Cipriani, F.
TI  - Mid-infrared spectroscopic investigation of meteorites and perspectives for thermal infrared observations at the binary asteroid Didymos
JF  - PLANETARY AND SPACE SCIENCE
J2  - PLANET SPACE SCI
VL  - 184
PY  - 2020
SN  - 0032-0633
DO  - 10.1016/j.pss.2020.104855
UR  - https://m2.mtmt.hu/api/publication/31345290
ID  - 31345290
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Skultéti, Ágnes
AU  - Kereszturi, Ákos
AU  - Kereszty, Zs
AU  - Pál, Bernadett
AU  - Szabó, Máté Zoltán
AU  - Cipriani, F
TI  - Role of spectral resolution for infrared asteroid compositional analysis using meteorite spectra
JF  - MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
J2  - MON NOT R ASTRON SOC
VL  - 496
PY  - 2020
IS  - 1
SP  - 689
EP  - 694
PG  - 6
SN  - 0035-8711
DO  - 10.1093/mnras/staa1475
UR  - https://m2.mtmt.hu/api/publication/31403943
ID  - 31403943
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Gyollai, Ildikó
AU  - Kereszturi, Ákos
AU  - Chatzitheodoridis, E
TI  - Analysis of shock metamorphic processes in the Zagami meteorite
JF  - CENTRAL EUROPEAN GEOLOGY
J2  - CENT EUR GEOL
VL  - 62
PY  - 2019
IS  - 1
SP  - 56
EP  - 82
PG  - 27
SN  - 1788-2281
DO  - 10.1556/24.61.2018.12
UR  - https://m2.mtmt.hu/api/publication/30803007
ID  - 30803007
LA  - English
DB  - MTMT
ER  - 

TY  - CONF
AU  - Gyollai, Ildikó
AU  - Kereszturi, Ákos
AU  - Szabó, Máté Zoltán
AU  - Kereszty, Zs.
ED  - Louise, Prockter
TI  - New inputs on CAI formation based on a new CV3 meteorite Northwest Africa 10261.
T2  - 50th Lunar and Planetary Science Conference - LPSC
PB  - Lunar and Planetary Institute
C1  - The Woodlands (TX)
PY  - 2019
PG  - 2
UR  - https://m2.mtmt.hu/api/publication/30421140
ID  - 30421140
LA  - English
DB  - MTMT
ER  - 

TY  - CONF
AU  - Kapui, Zsuzsanna
AU  - Kereszturi, Ákos
AU  - Józsa, Sándor
AU  - Király, Csilla
AU  - Szalai, Zoltán
AU  - Újvári, Gábor
ED  - Louise, Prockter
TI  - Surface textural analysis of Mars relevant fluvial and aeolian basaltic grains by scanning electron microscopy
T2  - 50th Lunar and Planetary Science Conference - LPSC
PB  - Lunar and Planetary Institute
C1  - The Woodlands (TX)
PY  - 2019
PG  - 2
UR  - https://m2.mtmt.hu/api/publication/30421154
ID  - 30421154
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Orgel, Csilla
AU  - Hauber, Ernst
AU  - Gasselt, Stephan
AU  - Reiss, Dennis
AU  - Johnsson, Andreas
AU  - Ramsdale, Jason D.
AU  - Smith, Isaac
AU  - Swirad, Zuzanna M.
AU  - Séjourné, Antoine
AU  - Wilson, Jack T.
AU  - Balme, Matthew R.
AU  - Conway, Susan J.
AU  - Costard, Francois
AU  - Eke, Vince R.
AU  - Gallagher, Colman
AU  - Kereszturi, Ákos
AU  - Łosiak, Anna
AU  - Massey, Richard J.
AU  - Platz, Thomas
AU  - Skinner, James A.
AU  - Teodoro, Luis F. A.
TI  - Grid Mapping the Northern Plains of Mars: A New Overview of Recent Water‐ and Ice‐Related Landforms in Acidalia Planitia
JF  - JOURNAL OF GEOPHYSICAL RESEARCH: PLANETS
J2  - J GEOPHYS RES PLANET
VL  - 124
PY  - 2019
IS  - 2
SP  - 454
EP  - 482
PG  - 29
SN  - 2169-9097
DO  - 10.1029/2018JE005664
UR  - https://m2.mtmt.hu/api/publication/30618316
ID  - 30618316
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Pál, Bernadett
AU  - Kereszturi, Ákos
AU  - Forget, Francois
AU  - Smith, Michael D.
TI  - Global seasonal variations of the near-surface relative humidity levels on present-day Mars
JF  - ICARUS
J2  - ICARUS
VL  - 333
PY  - 2019
SP  - 481
EP  - 495
PG  - 15
SN  - 0019-1035
DO  - 10.1016/j.icarus.2019.07.007
UR  - https://m2.mtmt.hu/api/publication/30810334
ID  - 30810334
N1  - Funding Agency and Grant Number: NKFIH [COOP - NN - 116927]; EXODRILTECH project [4000119270]; National Research, Development and Innovation Office (NKFIH, Hungary) [GINOP-2.3.2-15-2016-00003]; Origins and evolution of life on Earth and in the Universe COST actions [TD1308, 39045, 39078]
            Funding text: This work was funded by the COOP - NN - 116927 project of NKFIH, EXODRILTECH (4000119270) project, the GINOP-2.3.2-15-2016-00003 grant of the National Research, Development and Innovation Office (NKFIH, Hungary) and the TD1308 Origins and evolution of life on Earth and in the Universe COST actions numbers 39045 and 39078. Special thanks to Vladimir V. Zakharov for his invaluable help with the NetCDF file handling. The NetCDF files were visualized with the NASA GISS Panoply viewer developed by Dr. Robert B. Schmunk. The thermal inertia map (Fig. 6.) was created by Vilmos Steinmann. Special thank you for Gerard Willinger and Laszlo Szabados for the improvement of the language of the manuscript. We also thank the referees for their valuable input which have greatly improved this manuscript.
AB  - We investigate the global seasonal variations of near-surface relative humidity and relevant attributes, like temperature and water vapor volume mixing ratio on Mars using calculations from modelled and measurement data. We focus on 2 AM local time snapshots to eliminate daily effects related to differences in insolation, and to be able to compare calculations based on modelling data from the Laboratoire de Meteorologie Dynamique Mars General Circulation Model with the observations of Mars Global Surveyor Thermal Emission Spectrometer. We study the seasonal effects by examining four specific dates in the Martian year, the northern spring equinox, summer solstice, autumn equinox, and winter solstice. We identify three specific zones, where the near-surface relative humidity levels are systematically higher than in their vicinity regardless of season. We find that these areas coincide with low thermal inertia features, which control surface temperatures on the planet, and are most likely covered with unconsolidated fine dust with grain sizes smaller than similar to 40 mu m. By comparing the data of relative humidity, temperature and water vapor volume mixing ratio at three different heights (near-surface, similar to 4 m and similar to 23 m above the surface), we demonstrate that the thermal inertia could play an important role in determining near-surface humidity levels. We also notice that during the night the water vapor levels drop at similar to 4 m above the surface. This, together with the temperature and thermal inertia values, shows that water vapor likely condenses in the near-surface atmosphere and on the ground during the night at the three aforementioned regions. This condensation may be in the form of brines, wettening of the fine grains by adsorption or deliquescence. This study specifies areas of interest on the surface of present day Mars for the proposed condensation, which may be examined by in-situ measurements in the future.
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Séjourné, Antoine
AU  - Costard, Francois
AU  - Swirad, Zuzanna M.
AU  - Łosiak, Anna
AU  - Bouley, Sylvain
AU  - Smith, Isaac
AU  - Balme, Matthew R.
AU  - Orgel, Csilla
AU  - Ramsdale, Jason D.
AU  - Hauber, Ernst
AU  - Conway, Susan J.
AU  - Gasselt, Stephan
AU  - Reiss, Dennis
AU  - Johnsson, Andreas
AU  - Gallagher, Colman
AU  - Skinner, James A.
AU  - Kereszturi, Ákos
AU  - Platz, Thomas
TI  - Grid Mapping the Northern Plains of Mars: Using Morphotype and Distribution of Ice‐Related Landforms to Understand Multiple Ice‐Rich Deposits in Utopia Planitia
JF  - JOURNAL OF GEOPHYSICAL RESEARCH: PLANETS
J2  - J GEOPHYS RES PLANET
VL  - 124
PY  - 2019
IS  - 2
SP  - 483
EP  - 503
PG  - 21
SN  - 2169-9097
DO  - 10.1029/2018JE005665
UR  - https://m2.mtmt.hu/api/publication/30618309
ID  - 30618309
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Bowles, N.E.
AU  - Snodgrass, C.
AU  - Gibbings, A.
AU  - Sanchez, J.P.
AU  - Arnold, J.A.
AU  - Eccleston, P.
AU  - Andert, T.
AU  - Probst, A.
AU  - Naletto, G.
AU  - Vandaele, A.C.
AU  - de Leon, J.
AU  - Nathues, A.
AU  - Thomas, I.R.
AU  - Thomas, N.
AU  - Jorda, L.
AU  - Da Deppo, V.
AU  - Haack, H.
AU  - Green, S.F.
AU  - Carry, B.
AU  - Donaldson Hanna, K.L.
AU  - Leif Jorgensen, J.
AU  - Kereszturi, Ákos
AU  - DeMeo, F.E.
AU  - Patel, M.R.
AU  - Davies, J.K.
AU  - Clarke, F.
AU  - Kinch, K.
AU  - Guilbert-Lepoutre, A.
AU  - Agarwal, J.
AU  - Rivkin, A.S.
AU  - Pravec, P.
AU  - Fornasier, S.
AU  - Granvik, M.
AU  - Jones, R.H.
AU  - Murdoch, N.
AU  - Joy, K.H.
AU  - Pascale, E.
AU  - Tecza, M.
AU  - Barnes, J.M.
AU  - Licandro, J.
AU  - Greenhagen, B.T.
AU  - Calcutt, S.B.
AU  - Marriner, C.M.
AU  - Warren, T.
AU  - Tosh, I.
AU  - Bowles, N. E.
AU  - Snodgrass, C.
AU  - Gibbings, A.
AU  - Sanchez, J.P.
AU  - Arnold, null
AU  - J.A., null
AU  - Eccleston, P.
AU  - Andert, T.
AU  - Probst, A.
AU  - Naletto, G.
AU  - Vandaele, A.C.
AU  - de Leon, J.
AU  - Nathues, A.
AU  - Thomas, I.R.
AU  - Thomas, N.
AU  - Jorda, J.
AU  - Da, Deppo V.
AU  - Haack, H.
AU  - Green, J.F.
AU  - Carry, B.
AU  - Donaldson, Hanna K.L.
AU  - Leif, Jorgensen J. Kereszturi A.
AU  - DeMeo, E.F.
AU  - Patel, M.R.
AU  - Davies, J.K.
AU  - Clarke, F. Kinch K.
AU  - Guilbert-Lepoutre, A.
AU  - Agarwal, J.
AU  - Rivkin, A.S.
AU  - Pravec, P.
AU  - Fornasier, S.
AU  - Granvik, M.
AU  - Jones, R.H.
AU  - Murdoch, N.
AU  - Joy, K.H.
AU  - Pascale, E.
AU  - Tecza, M.
AU  - Barnes, J.M.
AU  - Licandro, J.
AU  - Greenhagen, B:T.
AU  - Calcutt, S.B.
AU  - Marriner, C.M.
AU  - Warren, T.
AU  - Tosh, I.
TI  - CASTAway: An asteroid main belt tour and survey
JF  - ADVANCES IN SPACE RESEARCH
J2  - ADV SPACE RES
VL  - 62
PY  - 2018
IS  - 8
SP  - 1998
EP  - 2025
PG  - 28
SN  - 0273-1177
DO  - 10.1016/j.asr.2017.10.021
UR  - https://m2.mtmt.hu/api/publication/30359085
ID  - 30359085
LA  - English
DB  - MTMT
ER  - 

TY  - CHAP
AU  - Dunér, D
AU  - Capova, K A
AU  - Gargaud, M
AU  - Geppert, W
AU  - Kereszturi, Ákos
AU  - Persson, E
ED  - Capova, Klara Anna
ED  - Persson, Erik
ED  - Milligan, Tony
ED  - Dunér, David
TI  - Astrobiology and Society in Europe
T2  - Astrobiology and Society in Europe Today
PB  - Springer Netherlands
CY  - Cham (Németország)
SN  - 9783319962658
T3  - SpringerBriefs in Astronomy
PY  - 2018
SP  - 7
EP  - 10
PG  - 4
DO  - 10.1007/978-3-319-96265-8_2
UR  - https://m2.mtmt.hu/api/publication/3428657
ID  - 3428657
AB  - There is only, as we know it, one planet with life—our own Earth. However, current research in astrobiology searches for a second sample of a living world. Astrobiology, which concerns the origin, evolution, and future of life here on Earth and beyond, has become a rapidly expanding research field during the last two decades. European researchers are playing a leading role. Thousands of planets in other solar systems have been discovered. Knowledge about life’s evolutionary origin, and its requirements and environmental conditions have expanded considerably. It is not unlikely that one day—some say that this could happen within the next few decades—we will discover evidence of the existence of another living planet. Living or fossilized microbes could be found within our Solar System, or we could find signs of biological processes on planets in other solar systems. But even if this never happens, astrobiological research will still give us a new understanding of how life emerged on our planet, how it evolved, and what environmental conditions it needs in order to survive. In all, current and future research in astrobiology will change the view of how humans look at themselves, what it means to be a human, to be alive, to survive, where we come from, and where we are heading (Fig. 2.1). Astrobiology has clear existential implications, but beyond these, it also has concrete cultural, ethical, societal, educational, political, economic, and legal consequences. How will the general public react if we discover life on another planet? What pedagogic role can astrobiology play in elementary and higher education? To what extent should we utilise space for commercial and industrial purposes? How should this be politically managed and how should it be legally regulated? This White Paper on the societal implications of astrobiology research in Europe, which is a joint interdisciplinary effort of Working Group 5 within the COST Action TD1308 “Origins and Evolution of Life on Earth and in the Universe”, aims to gather together these challenges and implications, and in so doing lay the ground for a European Astrobiology Institute.
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kapui, Zsuzsanna
AU  - Kereszturi, Ákos
AU  - Kiss, Klaudia
AU  - Szalai, Zoltán
AU  - Újvári, Gábor
AU  - Hickman-Lewis, K
AU  - Foucher, F
AU  - Westall, F
TI  - Fluvial or aeolian grains? Separation of transport agents on Mars using Earth analogue observations
JF  - PLANETARY AND SPACE SCIENCE
J2  - PLANET SPACE SCI
VL  - 163
PY  - 2018
SP  - 56
EP  - 76
PG  - 21
SN  - 0032-0633
DO  - 10.1016/j.pss.2018.06.007
UR  - https://m2.mtmt.hu/api/publication/3391390
ID  - 3391390
N1  - Institute for Geological and Geochemical Research, MTA Research Center for Astronomy and Earth Sciences, Budaörsi str. 45, Budapest, 1112, Hungary            
            Konkoly Observatory, MTA Research Center for Astronomy and Earth Sciences, 15-17, Road Konkoly Thege Miklós, Budapest, 1121, Hungary            
            Geographical Institute, MTA Research Center for Astronomy and Earth Sciences, 45., Road Budaörsi, Budapest, 1112, Hungary            
            CNRS Centre de Biophysique Moléculaire, Rue Charles Sadron, Cedex 2, Orléans, 45071, France            
            Dipartmento di Scienze biologiche, geologiche e ambientale, Università di Bologna, Italy            
            Cited By :3            
            Export Date: 25 November 2019            
            CODEN: PLSSA            
            Correspondence Address: Kapui, Z.; Institute for Geological and Geochemical Research, MTA Research Center for Astronomy and Earth Sciences, Budaörsi str. 45, Hungary; email: kapui.zsuzsanna@csfk.mta.hu
AB  - The particle size, shape, surface texture and composition of aeolian and fluvial sedimentary samples were analyzed and compared using optical microscope-based automatized image analysis, in order to suggest indicators that could discriminate these two modes of transport on Mars. The principal goal is to assess if such indicators - established on Earth - could be used on Mars thereby aiding interpretations on the origin of sediments analysed by the ExoMars 2020 rover during its mission. Wind and water transported sand from, respectively, the Sahara Desert and the Maros river bar in Hungary were investigated and treated as mainly aeolian and fluvial end-members. In addition, two Mars-analogue aeolian and fluvial basaltic sediments from Iceland were analysed similarly.

Our analyses demonstrated that useful parameters for the distinction of aeolian and fluvial transport included the degree of sorting, the grain diameter/perimeter ratio, the circularity (reflecting the sphericity of the grains) and convexity (showing roughness of the grains) of particles. Mature aeolian sands are always well-sorted with high diameter/perimeter ratios since they are dominated by rounded grains. Differences were observed in both surface textures and the range of mineral compositions, wherein the aeolian samples reflect a more mature state. Separation of the two Icelandic samples with different origins was less straightforward due to both shorter transport distances and the fact that the fluvial sample was made of scoria, although the intermixing of grains with a probable aeolian origin could be also determined. The characteristics of grain size and shape parameters are potential indicators allowing the separation of the two transport modes, and their determination is shown to be feasible based on high resolution Close-UP Imager (CLUPI) observations. Nonetheless, knowledge of the geological context - for instance sedimentary facies, layering, sorting of the sediments and grain shape - is a requirement for proper interpretations. These sedimentary features could be party determined by MaMISS, CLUPI and PanCam observations. Differences between aeolian and fluvial grains are expected to be more pronounced on Mars than on Earth due to the episodic and likely short-term subaqueous transport, as opposed to the long-term activity of wind. However, future interpretations of the ExoMars 2020 rover images of martian sedimentary grains will be hampered by the limited knowledge of fluvial/aeolian transport on Mars. Based on our results, future research should focus on determining the dominant transport mode of any sediment and the degree of grain mixing, which strongly based on the transport mode.
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
AU  - Kapui, Zsuzsanna
AU  - Ori, G.G.
AU  - Taj-Eddine, K.
AU  - Újvári, Gábor
TI  - Mars-Relevant Field Experiences in Morocco: The Importance of Spatial Scales and Subsurface Exploration
JF  - ASTROBIOLOGY
J2  - ASTROBIOLOGY
VL  - 18
PY  - 2018
IS  - 10
SP  - 1329
EP  - 1350
PG  - 22
SN  - 1531-1074
DO  - 10.1089/ast.2017.1676
UR  - https://m2.mtmt.hu/api/publication/30309717
ID  - 30309717
N1  - \n Konkoly Thege Miklos Astronomical Institute, Research Centre for Astronomy and Earth Sciences, Konkoly Thege Miklos 15-17, Budapest, H-1121, Hungary \n Institute for Geological and Geochemical Research, Research Centre for Astronomy and Earth Sciences, Budapest, Hungary \n Ibn Battuta Centre, Cadi Ayyad University Marrakech, Morocco \n International Research School on Planetary Sciences, Pescara, Italy \n Export Date: 6 November 2018 \n Correspondence Address: Kereszturi, A.; Konkoly Thege Miklos Astronomical Institute, Research Centre for Astronomy and Earth Sciences, Konkoly Thege Miklos 15-17, Hungary; email: kereszturi.akos@csfk.mta.hu
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Fulvio, Daniele
AU  - Góbi, Sándor
AU  - Jäger, Cornelia
AU  - Kereszturi, Ákos
AU  - Henning, Thomas
TI  - Laboratory Experiments on the Low-temperature Formation of Carbonaceous Grains in the ISM
JF  - ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
J2  - ASTROPHYS J SUPPL S
VL  - 233
PY  - 2017
IS  - 1
PG  - 11
SN  - 0067-0049
DO  - 10.3847/1538-4365/aa9224
UR  - https://m2.mtmt.hu/api/publication/3303390
ID  - 3303390
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Góbi, Sándor
AU  - Kereszturi, Ákos
TI  - Role of serpentinisation in the thermal and connected mineral evolution of planetesimals – evaluating possible consequences for exoplanetary systems
JF  - MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
J2  - MON NOT R ASTRON SOC
VL  - 466
PY  - 2017
IS  - 2
SP  - 2099
EP  - 2110
PG  - 12
SN  - 0035-8711
DO  - 10.1093/mnras/stw3223
UR  - https://m2.mtmt.hu/api/publication/3156478
ID  - 3156478
N1  - WoS:hiba:000398284600057 2020-08-30 23:37 év nem egyezik
AB  - This work gives an overview on the general consequences of serpentinization occurring in the planetesimals of any planetary system. These processes were studied by numerical simulations and the model used - based on earlier works - was developed by implementing the effect of interfacial water. As liquid water is fundamentally required for serpentinization, previous simulations considered only such cases when the initial temperature inside the planetesimal was above the melting point of ice thus neglecting the effect of microscopic water layer completely. However, our results show that it must be taken into account and since it facilitates the reaction to occur at temperatures even as low as 200 K - at which bulk liquid water is completely absent - it substantially broadens the initiation of this alteration regarding the range of possible objects. Investigating the effect of changing the initial parameters helps examine the serpentinization in more general terms. Consequently, the findings described here are ubiquitous and can be applied to any exoplanetary system, even if the initial conditions differ considerably from those that were characteristic to our early Solar system. As a first step towards the generalization of such heating processes, we evaluate the role of composition, starting temperature, porosity and planetesimal size on this heating effect. Besides heat generated by decay of radioactive nuclei, serpentinization should be considered as a 'universal process' in the thermal evolution of planetesimals, and variations of parameters considered in this model might provide an insight into differences between objects in various protoplanetary discs.
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Gucsik, Arnold
AU  - Nakamura, T.
AU  - Jäger, C.
AU  - Ninagawa, K.
AU  - Nishido, H.
AU  - Kayama, M.
AU  - Tsuchiyama, A.
AU  - Ott, U.
AU  - Kereszturi, Ákos
TI  - Luminescence spectroscopical properties of plagioclase particles from the Hayabusa Sample Return Mission: An implication for study of space weathering processes in the asteroid Itokawa
JF  - MICROSCOPY AND MICROANALYSIS
J2  - MICROSC MICROANAL
VL  - 23
PY  - 2017
IS  - 1
SP  - 179
EP  - 186
PG  - 8
SN  - 1431-9276
DO  - 10.1017/S1431927617000046
UR  - https://m2.mtmt.hu/api/publication/32033582
ID  - 32033582
LA  - English
DB  - MTMT
ER  - 

TY  - CHAP
AU  - Gyollai, Ildikó
AU  - Józsa, Sándor
AU  - Kereszturi, Ákos
AU  - Kereszty, Zs
AU  - Kiss, Klaudia
AU  - Ringer, Marianna
AU  - Szabó, Máté Zoltán
AU  - Szalai, Zoltán
AU  - Veres, Miklós
ED  - Griffith, R
ED  - Hansen, S.
TI  - Shock alterations in meteorites
T2  - Meteorites:Classification, chemical composition, and impacts
PB  - Nova Science Publishers
CY  - New York, New York
SN  - 9781536123456
PY  - 2017
SP  - 17
EP  - 28
PG  - 17
UR  - https://m2.mtmt.hu/api/publication/3266361
ID  - 3266361
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Gyollai, Ildikó
AU  - Kereszturi, Ákos
AU  - Kereszty, Zs.
AU  - Szabó, Máté Zoltán
AU  - Chatzitheodoridis, E.
TI  - Shock-induced alterations in the recently found H chondrite Csátalja meteorite and its implications
JF  - CENTRAL EUROPEAN GEOLOGY
J2  - CENT EUR GEOL
VL  - 60
PY  - 2017
IS  - 2
SP  - 173
EP  - 200
PG  - 28
SN  - 1788-2281
DO  - 10.1556/24.60.2017.007
UR  - https://m2.mtmt.hu/api/publication/3266347
ID  - 3266347
AB  - Shock-driven annealing of pyroxene and shock deformation of 
olivine were analyzed in a recently found H chondrite called 
Csátalja. The most characteristic infrared (IR) spectral 
shape of shock-annealed sub-grained pyroxene was identified: 
the strongest peak occurs at 860 cm−1 with a smaller shoulder 
at 837−840 cm−1, and small bands are at 686, 635−638, and 
1,044−1,050 cm−1. The appearance of forbidden bands in 
pyroxene and shift of band positions to a lower wave number 
in olivines clearly demonstrate the crystal lattice 
disordering due to shock metamorphism. The shock annealing 
produced mixed dark melt along fractures, which consists of 
feldspar−pyroxene and olivine−pyroxene melt. The dark shock 
melt at sub-grain boundaries of shocked pyroxenes and along 
fracture of pyroxenes is characterized by elevated Ca, Na, 
and Al content relative to its environment, detected by 
element mapping. So far, shock deformation of pyroxene and 
olivine was not studied by IR spectroscopy; this method has 
turned out to be a powerful tool in identifying the mixed 
composition of shock melt minerals. Further study of shock 
annealing of minerals, together with the context of shock 
melting at sub-grain boundaries, will provide a better 
understanding of the formation of high P–T minerals.

http://akademiai.com/doi/pdf/10.1556/24.60.2017.007
LA  - English
DB  - MTMT
ER  - 

TY  - CHAP
AU  - Hargitai, Henrik
AU  - Wang, J.
AU  - Stooke, P.J.
AU  - Karachevtseva, I.
AU  - Kereszturi, Ákos
AU  - Gede, Mátyás
ED  - Miljenko, Lapaine
ED  - E., Lynn Usery
TI  - Map Projections in Planetary Cartography
T2  - Choosing a Map Projection
PB  - Springer Netherlands
CY  - Cham (Németország)
SN  - 9783319518343
T3  - Lecture Notes in Geoinformation and Cartography, ISSN 2195-1705
PY  - 2017
SP  - 177
EP  - 202
PG  - 20
DO  - 10.1007/978-3-319-51835-0_7
UR  - https://m2.mtmt.hu/api/publication/3146247
ID  - 3146247
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
AU  - Gyollai, Ildikó
AU  - Kereszty, Zs
AU  - Kiss, Klaudia
AU  - Szabó, Máté Zoltán
AU  - Szalai, Zoltán
AU  - Ringer, Marianna
AU  - Veres, Miklós
TI  - Analyzing Raman – Infrared spectral correlation in the recently found meteorite Csátalja
JF  - SPECTROCHIMICA ACTA PART A-MOLECULAR AND BIOMOLECULAR SPECTROSCOPY
J2  - SPECTROCHIM ACTA A
VL  - 173
PY  - 2017
SP  - 637
EP  - 646
PG  - 10
SN  - 1386-1425
DO  - 10.1016/j.saa.2016.10.012
UR  - https://m2.mtmt.hu/api/publication/3130280
ID  - 3130280
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
AU  - Steinmann, Vilmos
TI  - Characteristics of small young lunar impact craters focusing on current production and degradation on the Moon
JF  - PLANETARY AND SPACE SCIENCE
J2  - PLANET SPACE SCI
VL  - 148
PY  - 2017
SP  - 12
EP  - 27
PG  - 16
SN  - 0032-0633
DO  - 10.1016/j.pss.2017.09.010
UR  - https://m2.mtmt.hu/api/publication/3302518
ID  - 3302518
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Pál, Bernadett
AU  - Kereszturi, Ákos
TI  - Possibility of microscopic liquid water formation at landing sites on Mars and their observational potential
JF  - ICARUS
J2  - ICARUS
VL  - 282
PY  - 2017
SP  - 84
EP  - 92
PG  - 9
SN  - 0019-1035
DO  - 10.1016/j.icarus.2016.09.006
UR  - https://m2.mtmt.hu/api/publication/3117302
ID  - 3117302
AB  - Abstract Microscopic liquid brines, especially calcium-perchlorate could emerge by deliquescence on Mars during night time hours. Using climate model computations and orbital humidity observations, the ideal periods and their annual plus daily characteristics at various past, current and future landing sites were compared. Such results provide context for future analysis and targeting the related observations by the next missions for Mars. Based on the analysis, at most (but not all) past missions’ landing sites, microscopic brine could emerge during night time for different durations. Analysing the conditions at ExoMars rover’s primary landing site at Oxia Planum, the best annual period was found to be between Ls 115 - 225, and in L o c a l T i m e 2 - 5, after midnight. In an ideal case, 4 hours of continuous liquid phase can emerge there. Local conditions might cause values to differ from those estimated by the model. Thermal inertia could especially make such differences (low TI values favour fast cooling and H2O cold trapping at loose surfaces) and the concentration of calcium-perchlorate salt in the regolith also influences the process (it might occur preferentially at long-term exposed surfaces without recent loose dust coverage). These factors should be taken into account while targeting future liquid water observations on Mars.
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Ramsdale, Jason D
AU  - Balme, Matthew R
AU  - Conway, Susan J
AU  - Gallagher, Colman
AU  - van Gasselt, Stephan A
AU  - Hauber, Ernst
AU  - Orgel, Csilla
AU  - Séjourné, Antoine
AU  - Skinner, James A
AU  - Costard, Francois
AU  - Johnsson, Andreas
AU  - Losiak, Anna
AU  - Reiss, Dennis
AU  - Swirad, Zuzanna M
AU  - Kereszturi, Ákos
AU  - Smith, Isaac B
AU  - Platz, Thomas
TI  - Grid-based mapping: A method for rapidly determining the spatial distributions of small features over very large areas
JF  - PLANETARY AND SPACE SCIENCE
J2  - PLANET SPACE SCI
VL  - 140
PY  - 2017
SP  - 49
EP  - 61
PG  - 13
SN  - 0032-0633
DO  - 10.1016/j.pss.2017.04.002
UR  - https://m2.mtmt.hu/api/publication/3249078
ID  - 3249078
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Dobos, Vera Zsuzsa
AU  - Kereszturi, Ákos
AU  - Pál, András
AU  - Kiss, L. László
TI  - Possibility for albedo estimation of exomoons: Why should we care about M dwarfs?
JF  - ASTRONOMY & ASTROPHYSICS
J2  - ASTRON ASTROPHYS
VL  - 592
PY  - 2016
PG  - 13
SN  - 0004-6361
DO  - 10.1051/0004-6361/201526672
UR  - https://m2.mtmt.hu/api/publication/3096097
ID  - 3096097
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Domagal-Goldman, S D
AU  - Wright, K E
AU  - Adamala, K
AU  - de la, Rubia R A
AU  - Bond, J
AU  - Dartnell, L R
AU  - Goldman, A D
AU  - Lynch, K
AU  - Naud, M -E
AU  - Paulino-Lima, I G
AU  - Singer, K
AU  - Walter-Antonio, M
AU  - Abrevaya, X C
AU  - Anderson, R
AU  - Arney, G
AU  - Atri, D
AU  - Azúa-Bustos, A
AU  - Bowman, J S
AU  - Brazelton, W J
AU  - Brennecka, G A
AU  - Carns, R
AU  - Chopra, A
AU  - Colangelo-Lillis, J
AU  - Crockett, C J
AU  - DeMarines, J
AU  - Frank, E A
AU  - Frantz, C
AU  - de la, Fuente E
AU  - Galante, D
AU  - Glass, J
AU  - Gleeson, D
AU  - Glein, C R
AU  - Goldblatt, C
AU  - Horak, R
AU  - Horodyskyj, L
AU  - Kaçar, B
AU  - Knowles, E
AU  - Kereszturi, Ákos
AU  - Mayeur, P
AU  - McGlynn, S
AU  - Miguel, Y
AU  - Montgomery, M
AU  - Neish, C
AU  - Noack, L
AU  - Rugheimer, S
AU  - Stüeken, E E
AU  - Tamez-Hidalgo, P
AU  - Walker, S I
AU  - Wong, T
TI  - The Astrobiology Primer v2.0
JF  - ASTROBIOLOGY
J2  - ASTROBIOLOGY
VL  - 16
PY  - 2016
IS  - 8
SP  - 561
EP  - 653
PG  - 93
SN  - 1531-1074
DO  - 10.1089/ast.2015.1460
UR  - https://m2.mtmt.hu/api/publication/3122816
ID  - 3122816
N1  - Megjegyzés-26088218
N1 Funding Details: ANU, Australian National University
N1 Funding Details: FAPESP, São Paulo Research Foundation
N1 Funding Details: NASA, National Aeronautics and Space Administration
N1 Funding Details: NPP/ORAU, ORAU, Oak Ridge Associated Universities
AB  - Not Available
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
AU  - Rivera-Valentin, E
TI  - Possible water lubricated grain movement in the circumpolar region of Mars
JF  - PLANETARY AND SPACE SCIENCE
J2  - PLANET SPACE SCI
VL  - 125
PY  - 2016
SP  - 130
EP  - 145
PG  - 16
SN  - 0032-0633
DO  - 10.1016/j.pss.2016.03.015
UR  - https://m2.mtmt.hu/api/publication/3075385
ID  - 3075385
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
AU  - Noack, L
TI  - Review on the role of planetary factors on habitability
JF  - ORIGINS OF LIFE AND EVOLUTION OF BIOSPHERES
J2  - ORIGINS LIFE EVOL B
VL  - 46
PY  - 2016
SP  - 473
EP  - 486
PG  - 14
SN  - 0169-6149
DO  - 10.1007/s11084-016-9514-1
UR  - https://m2.mtmt.hu/api/publication/3088922
ID  - 3088922
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
AU  - Chathiteodoridis, E
TI  - Searching for the source crater of nakhlite meteorites
JF  - ORIGINS OF LIFE AND EVOLUTION OF BIOSPHERES
J2  - ORIGINS LIFE EVOL B
VL  - 46
PY  - 2016
SP  - 455
EP  - 471
PG  - 17
SN  - 0169-6149
DO  - 10.1007/s11084-016-9498-x
UR  - https://m2.mtmt.hu/api/publication/3088941
ID  - 3088941
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
AU  - Ormándi, Szilvia
AU  - Józsa, Sándor
TI  - Possible melting produced chondrule destruction in NWA 6604 CK4 chondrite
JF  - METEORITICS & PLANETARY SCIENCE
J2  - METEORIT PLANET SCI
VL  - 50
PY  - 2015
IS  - 7
SP  - 1295
EP  - 1309
PG  - 15
SN  - 1086-9379
DO  - 10.1111/maps.12458
UR  - https://m2.mtmt.hu/api/publication/2922726
ID  - 2922726
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
AU  - Ormándi, Szilvia
AU  - Józsa, Sándor
TI  - Processing in a transitional environment of CV and CK chondrites' parent bodies in the light of mineralogical and petrological analysis of NWA 1465 CV3 meteorite
JF  - PLANETARY AND SPACE SCIENCE
J2  - PLANET SPACE SCI
VL  - 109
PY  - 2015
SP  - 175
EP  - 186
PG  - 12
SN  - 0032-0633
DO  - 10.1016/j.pss.2015.02.016
UR  - https://m2.mtmt.hu/api/publication/2879279
ID  - 2879279
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
AU  - Gyollai, Ildikó
AU  - Szabó, Máté Zoltán
TI  - Case study of chondrule alteration with IR spectroscopy in NWA 2086 CV3 meteorite
JF  - PLANETARY AND SPACE SCIENCE
J2  - PLANET SPACE SCI
VL  - 106
PY  - 2015
SP  - 122
EP  - 131
PG  - 10
SN  - 0032-0633
DO  - 10.1016/j.pss.2014.12.015
UR  - https://m2.mtmt.hu/api/publication/2815474
ID  - 2815474
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
TI  - Case study of climatic changes in Martian fluvial systems at Xanthe Terra
JF  - PLANETARY AND SPACE SCIENCE
J2  - PLANET SPACE SCI
VL  - 96
PY  - 2014
SP  - 35
EP  - 50
PG  - 16
SN  - 0032-0633
DO  - 10.1016/j.pss.2014.03.014
UR  - https://m2.mtmt.hu/api/publication/2598176
ID  - 2598176
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
AU  - Góbi, Sándor
TI  - Possibility of Hˇ2Oˇ2 decomposition in thin liquid films on Mars
JF  - PLANETARY AND SPACE SCIENCE
J2  - PLANET SPACE SCI
VL  - 103
PY  - 2014
SP  - 153
EP  - 166
PG  - 14
SN  - 0032-0633
DO  - 10.1016/j.pss.2014.07.017
UR  - https://m2.mtmt.hu/api/publication/2744772
ID  - 2744772
AB  - Abstract In this work the pathways and possibilities of H2O2 decomposition on Mars in microscopic liquid interfacial water were analyzed by kinetic calculations. Thermal and photochemical driven decomposition, just like processes catalyzed by various metal oxides, is too slow compared to the annual duration while such microscopic liquid layers exist on Mars today, to produce substantial decomposition. The most effective analyzed process is catalyzed by Fe ions, which could decompose H2O2 under pH<4.5 with a half life of 1–2 days. This process might be important during volcanically influenced periods when sulfur release produces acidic pH, and rotational axis tilt change driven climatic changes also influence the volatile circulation and spatial occurrence just like the duration of thin liquid layer. Under current conditions, using the value of 200 K as the temperature in interfacial water (at the southern hemisphere), and applying Phoenix lander׳s wet chemistry laboratory results, the pH is not favorable for Fe mobility and this kind of decomposition. Despite current conditions (especially pH) being unfavorable for H2O2 decomposition, microscopic scale interfacial liquid water still might support the process. By the reaction called heterogeneous catalysis, without acidic pH and mobile Fe, but with minerals surfaces containing Fe decomposition of H2O2 with half life of 20 days can happen. This duration is still longer but not several orders than the existence of springtime interfacial liquid water on Mars today. This estimation is relevant for activation energy controlled reaction rates. The other main parameter that may influence the reaction rate is the diffusion speed. Although the available tests and theoretical calculations do not provide firm values for the diffusion speed in such a “2-dimensional” environment, using relevant estimations this parameter in the interfacial liquid layer is smaller than in bulk water. But the 20 days׳ duration mentioned above is still relevant, as the activation energy driven reaction rate is the main limiting factor in the decomposition and not the diffusion speed. The duration of dozen(s) days is still longer but not with orders of magnitude than the expected duration for the existence of springtime interfacial liquid water on Mars today. The results suggest such decomposition may happen today, however, because of our limited knowledge on chemical processes in thin interfacial liquid layers, this possibility waits for confirmation – and also points to the importance of conducting laboratory tests to validate the possible process. Although some tests were already realized for diffusion in an almost 2-dimensional liquid, the same is not true for activation energy, where only the value from the “normal” measurements was applied. Even if H2O2 decomposition is too slow today, the analysis of such a process is important, as under volcanic influence more effective decomposition might take place in thin interfacial liquids close to the climate of today if released sulfur produces pH<4.5. Large quantity and widespread occurrence of bulk liquid phase are not expected in the Amazonian period, but interfacial liquid water probably appeared regularly, and its locations, especially during volcanically active periods, might make certain sites than others more interesting for astrobiology with the lower concentration of oxidizing H2O2.
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
TI  - Surface processes in microgravity for landing and sampling site selection of asteroid missions – suggestions for MarcoPolo-R
JF  - PLANETARY AND SPACE SCIENCE
J2  - PLANET SPACE SCI
VL  - 101
PY  - 2014
SP  - 65
EP  - 76
PG  - 12
SN  - 0032-0633
DO  - 10.1016/j.pss.2014.06.005
UR  - https://m2.mtmt.hu/api/publication/2727406
ID  - 2727406
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Orgel, Csilla
AU  - Kereszturi, Ákos
AU  - Váczi, Tamás
AU  - Groemer, G.
AU  - Sattler, B.
TI  - Scientific Results and Lessons Learned from an Integrated Crewed Mars Exploration Simulation at the Rio Tinto Mars Analogue Site.
JF  - ACTA ASTRONAUTICA
J2  - ACTA ASTRONAUT
VL  - 94
PY  - 2014
IS  - 2
SP  - 736
EP  - 748
PG  - 13
SN  - 0094-5765
DO  - 10.1016/j.actaastro.2013.09.014
UR  - https://m2.mtmt.hu/api/publication/2471183
ID  - 2471183
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
AU  - Rivera-Valentin, EG
TI  - Locations of thin liquid water layers on present-day Mars
JF  - ICARUS
J2  - ICARUS
VL  - 221
PY  - 2012
IS  - 1
SP  - 289
EP  - 295
PG  - 7
SN  - 0019-1035
DO  - 10.1016/j.icarus.2012.08.004
UR  - https://m2.mtmt.hu/api/publication/2198257
ID  - 2198257
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
TI  - Crater wall outcrop analysis for targeting subsurface sampling on Mars
JF  - PLANETARY AND SPACE SCIENCE
J2  - PLANET SPACE SCI
VL  - 67
PY  - 2012
IS  - 1
SP  - 14
EP  - 27
PG  - 14
SN  - 0032-0633
DO  - 10.1016/j.pss.2012.02.011
UR  - https://m2.mtmt.hu/api/publication/2198278
ID  - 2198278
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
TI  - Landing site rationality scaling for subsurface sampling on Mars—Case study for ExoMars Rover-like missions
JF  - PLANETARY AND SPACE SCIENCE
J2  - PLANET SPACE SCI
VL  - 72
PY  - 2012
IS  - 1
SP  - 78
EP  - 90
PG  - 13
SN  - 0032-0633
DO  - 10.1016/j.pss.2012.07.007
UR  - https://m2.mtmt.hu/api/publication/2198261
ID  - 2198261
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
TI  - Review of wet environment types on Mars with focus on duration and volumetric issues.
JF  - ASTROBIOLOGY
J2  - ASTROBIOLOGY
VL  - 12
PY  - 2012
IS  - 6
SP  - 586
EP  - 600
PG  - 15
SN  - 1531-1074
DO  - 10.1089/ast.2011.0686
UR  - https://m2.mtmt.hu/api/publication/2198272
ID  - 2198272
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Marschall, Marianna
AU  - Dulai, Sándor András
AU  - Kereszturi, Ákos
TI  - Migrating and UVscreening subsurface zone on Mars as target for the analysis of photosynthetic life and astrobiology
JF  - PLANETARY AND SPACE SCIENCE
J2  - PLANET SPACE SCI
VL  - 72
PY  - 2012
IS  - 1
SP  - 146
EP  - 153
PG  - 8
SN  - 0032-0633
DO  - 10.1016/j.pss.2012.05.019
UR  - https://m2.mtmt.hu/api/publication/2016957
ID  - 2016957
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Nagy, S
AU  - Józsa, Sándor
AU  - Gucsik, Arnold
AU  - Bérczi, Szaniszló
AU  - Ninagawa, K
AU  - Nishido, H
AU  - Veres, Miklós
AU  - Kereszturi, Ákos
AU  - Hargitai, Henrik
TI  - Shock and thermal annealing history of the ALH 77005 Martian meteorite: A micro-Raman spectroscopical investigation
JF  - CENTRAL EUROPEAN GEOLOGY
J2  - CENT EUR GEOL
VL  - 55
PY  - 2012
IS  - 1
SP  - 33
EP  - 48
PG  - 16
SN  - 1788-2281
DO  - 10.1556/CEuGeol.55.2012.1.3
UR  - https://m2.mtmt.hu/api/publication/2149903
ID  - 2149903
AB  - We studied optical microscopic and micro-Raman spectroscopic signatures of shocked olivine from the ALH 77005 Martian meteorite sample. The purpose of this study is to document pressure and temperature-related effects in olivine over the entire sample, which can aid in understanding structural changes due to shock metamorphism and the post-shock thermal annealing processes of lherzolitic Martian meteorites. According to the optical microscope observations, three areas may be discernible in olivine of the ALH 77005 in the vicinity of the melt pocket. The first area is the thermally undisturbed part of a grain, which contains a high density of shock-induced planar microdeformations such as Planar Deformation Features (PDFs) and Planar Fractures (PFs). Compared to the first area, the second area shows less shock-induced microstructures, while the third area is a strongly recrystallized region, but not formed from a melt.A common Raman spectral feature of these olivines is a regular doublet peak centered at 823 and 852 cm-1; additionally, two new peaks at 535 and 755 cm -1 appear in the weakly annealed transition zones.
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
TI  - Geologic field work on Mars: distance and time issues during surface exploration
JF  - ACTA ASTRONAUTICA
J2  - ACTA ASTRONAUT
VL  - 68
PY  - 2011
IS  - 11-12
SP  - 1686
EP  - 1701
PG  - 16
SN  - 0094-5765
DO  - 10.1016/j.actaastro.2010.11.008
UR  - https://m2.mtmt.hu/api/publication/2199436
ID  - 2199436
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Kereszturi, Ákos
TI  - Analysis of two sections of Shalbatana Vallis' tributary channels
JF  - PLANETARY AND SPACE SCIENCE
J2  - PLANET SPACE SCI
VL  - 58
PY  - 2010
IS  - 14-15
SP  - 2008
EP  - 2021
PG  - 14
SN  - 0032-0633
DO  - 10.1016/j.pss.2010.10.001
UR  - https://m2.mtmt.hu/api/publication/2810238
ID  - 2810238
LA  - English
DB  - MTMT
ER  - 

TY  - CONF
AU  - Horvai, F
AU  - Kereszturi, Ákos
TI  - Geology of Mars: New University Course in Hungary
T2  - 40th Lunar and Planetary Science Conference
PB  - Lunar and Planetary Institute
C1  - Houston (TX)
T3  - LPI Contribution Series ; 1468.
PY  - 2009
UR  - https://m2.mtmt.hu/api/publication/2812765
ID  - 2812765
LA  - English
DB  - MTMT
ER  -