Results 131 to 140 of about 45,209 (160)
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Solar Wind Sputtering of Secondary Ions from Water-ice-covered Regolith Analogs
The Planetary Science JournalThe surfaces of airless bodies in space are constantly bombarded by solar wind and magnetospheric ions that sputter regolith grains and eject secondary particles into the exosphere.
Micah J. Schaible +4 more
semanticscholar +1 more source
Meteoritics & Planetary Science
Sierra Gorda 013 (SG 013) is an unusual CBa‐like chondrite containing two texturally different, isotopically identical lithologies—chondritic (L1) and achondritic (L2), which should have a common origin.
Marina A. Ivanova +4 more
semanticscholar +1 more source
Sierra Gorda 013 (SG 013) is an unusual CBa‐like chondrite containing two texturally different, isotopically identical lithologies—chondritic (L1) and achondritic (L2), which should have a common origin.
Marina A. Ivanova +4 more
semanticscholar +1 more source
Noble gases and nitrogen in material from asteroid Bennu
Meteoritics & Planetary ScienceWe report the elemental and isotopic abundances of all stable noble gases (helium, neon, argon, krypton, and xenon) in eight particles from asteroid Bennu returned by NASA's OSIRIS‐REx mission.
B. Marty +7 more
semanticscholar +1 more source
The Planetary Science Journal
We performed experiments of implantation of energetic sulfur ions (105 keV) into 2:1 water:propane ices at 80 K and analyzed the resulting refractory organic matter with ultrahigh-resolution mass spectrometry.
A. Bouquet +18 more
semanticscholar +1 more source
We performed experiments of implantation of energetic sulfur ions (105 keV) into 2:1 water:propane ices at 80 K and analyzed the resulting refractory organic matter with ultrahigh-resolution mass spectrometry.
A. Bouquet +18 more
semanticscholar +1 more source
Meteoritics & Planetary Science
CM chondrites are samples from primitive water‐rich asteroids that formed early in the solar system; many record evidence for silicate rock–liquid water interaction.
I. Kouvatsis +2 more
semanticscholar +1 more source
CM chondrites are samples from primitive water‐rich asteroids that formed early in the solar system; many record evidence for silicate rock–liquid water interaction.
I. Kouvatsis +2 more
semanticscholar +1 more source
Meteoritics & Planetary Science
The temperature and pressure conditions experienced by rocks during an impact event can be constrained using petrologic and microstructural analysis and is crucial to providing ground truth to the impact cratering process.
A. Stadermann +7 more
semanticscholar +1 more source
The temperature and pressure conditions experienced by rocks during an impact event can be constrained using petrologic and microstructural analysis and is crucial to providing ground truth to the impact cratering process.
A. Stadermann +7 more
semanticscholar +1 more source
Earth-Moon refractory element similarity constrains a thoroughly-mixed Moon-forming disk
Earth and Planetary Science LettersH. Fu, Stein B. Jacobsen
semanticscholar +1 more source
Ti isotopic evidence for a non-CAI refractory component in the inner Solar System
Earth and Planetary Science Letters, 2018S. Ebert +6 more
semanticscholar +1 more source
The “lost” aqueous supercritical fluids recorded in highly refractory mantle peridotites
Earth and Planetary Science LettersHaochen Duan +4 more
semanticscholar +1 more source

