103 citations
- Hungarian Academy of SciencesHU16 papers
- HUN-REN Research Centre for Astronomy and Earth SciencesHU15 papers
- University of Colorado BoulderUS13 papers
- Tokyo Institute of TechnologyJP11 papers
- Life Science InstituteJP6 papers
- Earth-Life Science InstituteJP5 papers
- Eötvös Loránd UniversityHU5 papers
- Konkoly ObservatoryHU5 papers
- University of DundeeGB4 papers
- University of OsloNO4 papers
- Geographical InstituteHU3 papers
- John Templeton FoundationUS3 papers
21 papers
Irradiation induced mineral changes of NWA10580 meteorite determined by infrared analysis
I. Gyollai, S. Biri, Z. Juhász +10
Context. Identifying minerals on asteroid surfaces is difficult as space weathering modifies the minerals infrared spectra. This shouldbe better understood for proper interpretatio…
Review of synergic meteor observations: linking the results from cameras, ionosondes, infrasound and seismic detectors
Á. Kereszturi, V. Barta, I. Bondár +6
Joint evaluation of different meteor observation types support the better understanding of both the meteor phenomenon and the terrestrial atmosphere. Two types of examples are pres…
Europium as a lodestar: diagnosis of radiogenic heat production in terrestrial exoplanets
Haiyang S. Wang, Thierry Morel, Sascha P. Quanz +1
Long-lived radioactive nuclides, such as K, Th, U and U, contribute to persistent heat production in the mantle of terrestrial-type planets. As refra…
Cold, dry, windy, and UV irradiated -- surveying Mars relevant conditions in Ojos del Salado Volcano (Andes Mountains, Chile)
Á. Kereszturi, J. Aszalós, Zs. Heiling +8
The Special Collection of papers in this issue of Astrobiology provide an overview of the characteristics and potential for future exploration of the Ojos del Salado volcano, locat…
Role of spectral resolution for infrared asteroid compositional analysis using meteorite spectra
A. Skulteti, A. Kereszturi, Zs. Kereszty +3
In this work the potential mineral identification of meteorites is analysed for the mid-infrared range, to evaluate observational possibilities for future missions targeting small…
Impact bombardment chronology of the terrestrial planets from 4.5 Ga to 3.5 Ga
R. Brasser, S. C. Werner, S. J. Mojzsis
Subsequent to the Moon's formation, late accretion to the terrestrial planets modified their silicate crusts and mantles. We combine dynamical N-body and Monte Carlo simulations to…