Lunar impact glasses: Probing the Moon's surface and constraining its impact history
NEB Zellner - Journal of Geophysical Research: Planets, 2019 - Wiley Online Library
Lunar impact glasses, formed during impact events when the regolith is quenched during
the ejecta's ballistic flight, are small samples whose information can lead to important …
the ejecta's ballistic flight, are small samples whose information can lead to important …
The origin and evolution of organic matter in carbonaceous chondrites and links to their parent bodies
The nature of organic matter in meteorites reveals information about early solar system
chemistry and the histories of parent bodies as recorded in the effects of physical and …
chemistry and the histories of parent bodies as recorded in the effects of physical and …
[HTML][HTML] Identification of meteorite source regions in the Solar System
M Granvik, P Brown - Icarus, 2018 - Elsevier
Over the past decade there has been a large increase in the number of automated camera
networks that monitor the sky for fireballs. One of the goals of these networks is to provide …
networks that monitor the sky for fireballs. One of the goals of these networks is to provide …
[HTML][HTML] In-situ phosphate U-Pb ages of the L chondrites
The thermal history of asteroids is recorded by the radioisotopic ages of meteorites that
derive from them. Radioisotopic ages may date a number of events, such as the cooling of a …
derive from them. Radioisotopic ages may date a number of events, such as the cooling of a …
Mechanical properties of particles from the surface of asteroid 25143 Itokawa
Aims. Asteroids have been exposed to impacts since their formation, and as a consequence
their surfaces are covered by small particles, pebbles, and boulders. The Japanese …
their surfaces are covered by small particles, pebbles, and boulders. The Japanese …
Chelyabinsk–a rock with many different (stony) faces: An infrared study
In order to provide spectral ground truth data for remote sensing applications, we have
measured mid-infrared spectra (2–18 µm) of three typical, well-defined lithologies from the …
measured mid-infrared spectra (2–18 µm) of three typical, well-defined lithologies from the …
Shock stage distribution of 2280 ordinary chondrites—Can bulk chondrites with a shock stage of S6 exist as individual rocks?
A Bischoff, M Schleiting… - Meteoritics & Planetary …, 2019 - Wiley Online Library
The brecciation and shock classification of 2280 ordinary chondrites of the meteorite thin
section collection at the Institut für Planetologie (Münster) has been determined. The shock …
section collection at the Institut für Planetologie (Münster) has been determined. The shock …
A 187Re-187Os, 87Rb-87Sr, highly siderophile and incompatible trace element study of some carbonaceous, ordinary and enstatite chondrite meteorites
Abstract New 187 Re-187 Os, 87 Rb-87 Sr, triple O-isotope isotope, bulk rock highly
siderophile-(HSE: Os, Ir, Ru, Pt, Pd, Re), major-and trace-element abundance data are …
siderophile-(HSE: Os, Ir, Ru, Pt, Pd, Re), major-and trace-element abundance data are …
Variability of Chelyabinsk meteoroid stones studied by Mössbauer spectroscopy and X-ray diffraction
MI Oshtrakh, AA Maksimova, AV Chukin… - … Acta Part A: Molecular …, 2019 - Elsevier
The meter-scale variations of material properties of the 20-m sized Chelyabinsk meteoroid
are critical for understanding why the meteoroid fragmented the way it did and caused the …
are critical for understanding why the meteoroid fragmented the way it did and caused the …
[HTML][HTML] The Renchen L5-6 chondrite breccia–The first confirmed meteorite fall from Baden-Württemberg (Germany)
Abstract On July 10, 2018 at 21: 29 UT extended areas of South-Western Germany were
illuminated by a very bright bolide. This fireball was recorded by instruments of the …
illuminated by a very bright bolide. This fireball was recorded by instruments of the …