Add to ORKGEucrites, a member of the howardite-eucritediogenite (HED) group, are basaltic meteorites that are believed to come from the asteroid Vesta [e.g., 1]. A recent study of water concentration and hydrogen isotope of eucrite apatite [2] suggested an early accretion of water from a carbonaceous chondrite– like source on Earth, Vesta and other planetary bodies in the inner solar system. In this study, we present results of OH and D/H analyses of apatites from more eucrite samples
Cumulate eucrites and noncumulate (ordinary) eucrites are considered to have come from one (or simil...
Howardite, eucrite and diogenite meteorites likely come from asteroid 4 Vesta [1]. Howardites - phys...
The Howardite, Eucrite, Diogenite (HED) meteorites are a group of achondrite meteorites that likely ...
Eucrites, a member of the howardite-eucritediogenite (HED) group, are basaltic meteorites that are ...
Volatile elements play a key role in the dynamics of planetary evolution. Extensive work has been ca...
Recent in situ measurements of volatiles (H2O, Cl and F), particularly in lunar and martian samples,...
Recent advancements in analytical instrumentation and techniques have enabled high-precision volatil...
International audienceGenerally, terrestrial rocks, martian and chondritic meteorites exhibit a rela...
Meteorites provide the only direct record of the chronology and nature of the processes that occurre...
We conducted a petrologic study of apatite within eight unbrecciated, non-cumulate eucrites and two ...
Eucrites are a class of basaltic meteorites that, along with the howardites and diogenites, likely d...
The Howardite-Eucrite-Diogenite (HED) meteorites are a suite of basalts, cumulates and breccias whi...
Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the ...
The achondritic howardites, eucrites, and diogenites (HED), along with the stony-iron mesosiderites,...
The abundance and isotopic composition of volatile elements in meteorites are critical for understan...
Cumulate eucrites and noncumulate (ordinary) eucrites are considered to have come from one (or simil...
Howardite, eucrite and diogenite meteorites likely come from asteroid 4 Vesta [1]. Howardites - phys...
The Howardite, Eucrite, Diogenite (HED) meteorites are a group of achondrite meteorites that likely ...
Eucrites, a member of the howardite-eucritediogenite (HED) group, are basaltic meteorites that are ...
Volatile elements play a key role in the dynamics of planetary evolution. Extensive work has been ca...
Recent in situ measurements of volatiles (H2O, Cl and F), particularly in lunar and martian samples,...
Recent advancements in analytical instrumentation and techniques have enabled high-precision volatil...
International audienceGenerally, terrestrial rocks, martian and chondritic meteorites exhibit a rela...
Meteorites provide the only direct record of the chronology and nature of the processes that occurre...
We conducted a petrologic study of apatite within eight unbrecciated, non-cumulate eucrites and two ...
Eucrites are a class of basaltic meteorites that, along with the howardites and diogenites, likely d...
The Howardite-Eucrite-Diogenite (HED) meteorites are a suite of basalts, cumulates and breccias whi...
Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the ...
The achondritic howardites, eucrites, and diogenites (HED), along with the stony-iron mesosiderites,...
The abundance and isotopic composition of volatile elements in meteorites are critical for understan...
Cumulate eucrites and noncumulate (ordinary) eucrites are considered to have come from one (or simil...
Howardite, eucrite and diogenite meteorites likely come from asteroid 4 Vesta [1]. Howardites - phys...
The Howardite, Eucrite, Diogenite (HED) meteorites are a group of achondrite meteorites that likely ...