Hibonite is a comparatively rare, primary phase found in some CAIs from different chondrite groups and is also common in Wark-Lovering rims [1]. Hibonite is predicted to be one of the earliest refractory phases to form by equilibrium condensation from a cooling gas of solar composition [2] and, therefore, can be a potential recorder of very early solar system processes. In this study, we describe the microstructures of hibonite from one CAI in ALH A77307 (CO3.0) using FIB/TEM techniques in order to reconstruct its formational history
Calcium, Aluminum-rich Inclusions (CAIs) were the first formed solids in our Solar System, with mine...
One long-standing problem in the application of Al-Mg isotopic systematics to the chronology of CAI ...
Abstract- Hibonite-bearing Ca,AI-rich inclusions (CA ls) usually occur in e M and CH chondrites and ...
Hibonite (CaAl12O19) is a primary, highly refractory phase occurring in many Ca-Al-rich inclusions (...
Hibonite (CaAl12O19) is a primary, highly refractory phase occurring in many Ca-Al-rich inclusions (...
Hibonite is a primary ultra-refractory mineral occurring in many Ca-Al-rich inclusions (CAIs) and is...
The demonstration of the presence of ^(41)Ca in the early solar system, based on the observation of ...
Calcium-aluminum-rich refractory inclusions (CAIs) are thought to be the first-formed solids in the ...
Introduction: Hibonite is a primary refractory phase occurring in many CAIs, typically with spinel a...
We have studied the mineralogy and petrology of 229 calcium-aluminum-rich inclusions (CAIs) from ten...
Northwest Africa (NWA) 10758 is a newly identified carbonaceous chondrite that is a Bali-like oxidiz...
Hibonite-bearing Ca,Al-rich inclusions (CAIs) usually occur in CM and CH chondrites and possess petr...
We report the discovery of a circumstellar hibonite (CaAI_(12)O_(19)) showing clear evidence of ^(41...
Wark-Lovering (WL) rims are thin multilayered mineral sequences that surround most Ca, Al-rich inclu...
Fine-grained, spinel-rich Ca-Al-rich inclusions (FGIs) in carbonaceous chondrites consist of numerou...
Calcium, Aluminum-rich Inclusions (CAIs) were the first formed solids in our Solar System, with mine...
One long-standing problem in the application of Al-Mg isotopic systematics to the chronology of CAI ...
Abstract- Hibonite-bearing Ca,AI-rich inclusions (CA ls) usually occur in e M and CH chondrites and ...
Hibonite (CaAl12O19) is a primary, highly refractory phase occurring in many Ca-Al-rich inclusions (...
Hibonite (CaAl12O19) is a primary, highly refractory phase occurring in many Ca-Al-rich inclusions (...
Hibonite is a primary ultra-refractory mineral occurring in many Ca-Al-rich inclusions (CAIs) and is...
The demonstration of the presence of ^(41)Ca in the early solar system, based on the observation of ...
Calcium-aluminum-rich refractory inclusions (CAIs) are thought to be the first-formed solids in the ...
Introduction: Hibonite is a primary refractory phase occurring in many CAIs, typically with spinel a...
We have studied the mineralogy and petrology of 229 calcium-aluminum-rich inclusions (CAIs) from ten...
Northwest Africa (NWA) 10758 is a newly identified carbonaceous chondrite that is a Bali-like oxidiz...
Hibonite-bearing Ca,Al-rich inclusions (CAIs) usually occur in CM and CH chondrites and possess petr...
We report the discovery of a circumstellar hibonite (CaAI_(12)O_(19)) showing clear evidence of ^(41...
Wark-Lovering (WL) rims are thin multilayered mineral sequences that surround most Ca, Al-rich inclu...
Fine-grained, spinel-rich Ca-Al-rich inclusions (FGIs) in carbonaceous chondrites consist of numerou...
Calcium, Aluminum-rich Inclusions (CAIs) were the first formed solids in our Solar System, with mine...
One long-standing problem in the application of Al-Mg isotopic systematics to the chronology of CAI ...
Abstract- Hibonite-bearing Ca,AI-rich inclusions (CA ls) usually occur in e M and CH chondrites and ...