Asteroid (4) Vesta: I. The howardite-eucrite-diogenite (HED) clan of meteorites
DW Mittlefehldt - Geochemistry, 2015 - Elsevier
The howardite, eucrite and diogenite (HED) clan of meteorites are ultramafic and mafic
igneous rocks and impact-engendered fragmental debris derived from a thoroughly …
igneous rocks and impact-engendered fragmental debris derived from a thoroughly …
[HTML][HTML] Melting and differentiation of early-formed asteroids: The perspective from high precision oxygen isotope studies
RC Greenwood, TH Burbine, MF Miller, IA Franchi - Geochemistry, 2017 - Elsevier
A number of distinct methodologies are available for determining the oxygen isotope
composition of minerals and rocks, these include laser-assisted fluorination, secondary ion …
composition of minerals and rocks, these include laser-assisted fluorination, secondary ion …
Radar-enabled recovery of the Sutter's Mill meteorite, a carbonaceous chondrite regolith breccia
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 …
a rare 4-kiloton of TNT–equivalent asteroid impact over the foothills of the Sierra Nevada in …
Very low strengths of interplanetary meteoroids and small asteroids
O Popova, J Borovička, WK Hartmann… - … & Planetary Science, 2011 - Wiley Online Library
We have assembled data on 13 cases of meteorite falls with accurate tracking data on
atmospheric passage. In all cases, we estimate the bulk strength of the object corresponding …
atmospheric passage. In all cases, we estimate the bulk strength of the object corresponding …
Mineralogy of asteroids
MJ Gaffey - AIP Conference Proceedings, 2011 - pubs.aip.org
Reflectance spectroscopy is a powerful tool for the investigation of the nature, history,
evolution, and relationships between asteroids and meteorites. This information provides a …
evolution, and relationships between asteroids and meteorites. This information provides a …
Dynamical evolution of basaltic asteroids outside the Vesta family in the inner main belt
V Troianskyi, P Kankiewicz, D Oszkiewicz - Astronomy & Astrophysics, 2023 - aanda.org
Context. Basaltic V-type asteroids are leftovers from the formation and evolution of
differentiated planetesimals. They are thought to originate from mantles and crusts of …
differentiated planetesimals. They are thought to originate from mantles and crusts of …
Spins and shapes of basaltic asteroids and the missing mantle problem
Basaltic V-type asteroids are common in the inner part of the Main Asteroid Belt and much
less abundant in the mid and outer parts. They are of scientific interest because they sample …
less abundant in the mid and outer parts. They are of scientific interest because they sample …
[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 …
Mineralogy and surface composition of asteroids
Methods to constrain the surface mineralogy of asteroids have seen considerable
development during the last decade, with advancement in laboratory spectral calibrations …
development during the last decade, with advancement in laboratory spectral calibrations …
The impact and recovery of asteroid 2018 LA
P Jenniskens, M Gabadirwe, QZ Yin… - … & planetary science, 2021 - Wiley Online Library
The June 2, 2018 impact of asteroid 2018 LA over Botswana is only the second asteroid
detected in space prior to impacting over land. Here, we report on the successful recovery of …
detected in space prior to impacting over land. Here, we report on the successful recovery of …