Extraterrestrial construction materials

MZ Naser - Progress in materials science, 2019 - Elsevier
In recognition of the 50th anniversary of the first manned lunar landing, the National
Aeronautics and Space Administration (NASA), together with the European Space Agency …

[HTML][HTML] Physical properties of the stone meteorites: Implications for the properties of their parent bodies

GJ Flynn, GJ Consolmagno, P Brown, RJ Macke - Geochemistry, 2018 - Elsevier
The physical properties of the stone meteorites provide important clues to understanding the
formation and physical evolution of material in the Solar protoplanetary disk as well …

Chelyabinsk airburst, damage assessment, meteorite recovery, and characterization

OP Popova, P Jenniskens, V Emel'yanenko… - Science, 2013 - science.org
The asteroid impact near the Russian city of Chelyabinsk on 15 February 2013 was the
largest airburst on Earth since the 1908 Tunguska event, causing a natural disaster in an …

The trajectory, structure and origin of the Chelyabinsk asteroidal impactor

J Borovička, P Spurný, P Brown, P Wiegert, P Kalenda… - Nature, 2013 - nature.com
Earth is continuously colliding with fragments of asteroids and comets of various sizes. The
largest encounter in historical times occurred over the Tunguska river in Siberia in 1908 …

Low thermal conductivity boulder with high porosity identified on C-type asteroid (162173) Ryugu

M Grott, J Knollenberg, M Hamm, K Ogawa… - Nature …, 2019 - nature.com
C-type asteroids are among the most pristine objects in the Solar System, but little is known
about their interior structure and surface properties. Telescopic thermal infrared …

[HTML][HTML] Boulder size and shape distributions on asteroid Ryugu

T Michikami, C Honda, H Miyamoto, M Hirabayashi… - Icarus, 2019 - Elsevier
Abstract In 2018, the Japanese spacecraft Hayabusa2, arrived at the small asteroid Ryugu.
The surface of this C-type asteroid is covered with numerous boulders whose size and …

The strength of regolith and rubble pile asteroids

P Sánchez, DJ Scheeres - Meteoritics & Planetary Science, 2014 - Wiley Online Library
We explore the hypothesis that, due to small van der Waals forces between constituent
grains, small rubble pile asteroids have a small but nonzero cohesive strength. The nature of …

Radar-enabled recovery of the Sutter's Mill meteorite, a carbonaceous chondrite regolith breccia

P Jenniskens, MD Fries, QZ Yin, M Zolensky, AN Krot… - Science, 2012 - science.org
Doppler weather radar imaging enabled the rapid recovery of the Sutter's Mill meteorite after
a rare 4-kiloton of TNT–equivalent asteroid impact over the foothills of the Sierra Nevada in …

The current martian cratering rate

IJ Daubar, AS McEwen, S Byrne, MR Kennedy… - Icarus, 2013 - Elsevier
The discovery of 248 dated impact sites known to have formed within the last few decades
allows us to refine the current cratering rate and slope of the production function at Mars. We …

A history of mild shocks experienced by the regolith particles on hydrated asteroid Ryugu

N Tomioka, A Yamaguchi, M Ito, M Uesugi, N Imae… - Nature …, 2023 - nature.com
Micrometeorites, a possible major source of Earth's water, are thought to form from explosive
dispersal of hydrated chondritic materials during impact events on their parental asteroids …