Add to ORKGOne long-standing problem in the application of Al-Mg isotopic systematics to the chronology of CAI is the enigmatic Mg isotopic record of hibonite. Hibonite (ideally, CaAI_(12)O_(19)) is one of the first major element bearing phases to appear in the condensation sequence [1] and occurs as a major constituent only in CAI whose bulk composition is considerably more refractory than Allende Type Bl CAI
The timescale for injection of fresh nucleosynthetic material and for the formation of the first sol...
Of the possible processes involved in Type B CAI history, igneous processes are the most tractable f...
Hibonite is a comparatively rare, primary phase found in some CAIs from different chondrite groups a...
Abstract- Hibonite-bearing Ca,AI-rich inclusions (CA ls) usually occur in e M and CH chondrites and ...
Hibonite-bearing Ca,Al-rich inclusions (CAIs) usually occur in CM and CH chondrites and possess petr...
We have studied the Mg and Ca isotopic compositions of an unusual Allende inclusion dominated by hib...
We have made aluminum-magnesium isotopic measurements on 4 melilite-bearing calcium-aluminum-rich in...
The defining characteristic of type B1 CAIs is a large (.5- 3mm) concentric melilite mantle [1]. In ...
One of the least well understood and most controversial aspects of CAI is the degree to which their...
Ca-Al-rich inclusions (CAIs) are the earliest formed crystalline material in our solar system and th...
A study of the Mg isotopic composition and mineralogy of fine-grained, Ca-Al-rich inclusions has bee...
We have made aluminum-magnesium isotopic measurements on 4 melilite-bearing calcium-aluminum-rich in...
The measurements of magnesium and potassium isotopic compositions of refractory minerals in Allende ...
The chemical and isotopic compositions of calcium-aluminum-rich inclusions (CAIs) can be used to und...
The precise knowledge of the initial 26Al/27Al ratio [(26Al/27Al)0] is crucial if we are to use the ...
The timescale for injection of fresh nucleosynthetic material and for the formation of the first sol...
Of the possible processes involved in Type B CAI history, igneous processes are the most tractable f...
Hibonite is a comparatively rare, primary phase found in some CAIs from different chondrite groups a...
Abstract- Hibonite-bearing Ca,AI-rich inclusions (CA ls) usually occur in e M and CH chondrites and ...
Hibonite-bearing Ca,Al-rich inclusions (CAIs) usually occur in CM and CH chondrites and possess petr...
We have studied the Mg and Ca isotopic compositions of an unusual Allende inclusion dominated by hib...
We have made aluminum-magnesium isotopic measurements on 4 melilite-bearing calcium-aluminum-rich in...
The defining characteristic of type B1 CAIs is a large (.5- 3mm) concentric melilite mantle [1]. In ...
One of the least well understood and most controversial aspects of CAI is the degree to which their...
Ca-Al-rich inclusions (CAIs) are the earliest formed crystalline material in our solar system and th...
A study of the Mg isotopic composition and mineralogy of fine-grained, Ca-Al-rich inclusions has bee...
We have made aluminum-magnesium isotopic measurements on 4 melilite-bearing calcium-aluminum-rich in...
The measurements of magnesium and potassium isotopic compositions of refractory minerals in Allende ...
The chemical and isotopic compositions of calcium-aluminum-rich inclusions (CAIs) can be used to und...
The precise knowledge of the initial 26Al/27Al ratio [(26Al/27Al)0] is crucial if we are to use the ...
The timescale for injection of fresh nucleosynthetic material and for the formation of the first sol...
Of the possible processes involved in Type B CAI history, igneous processes are the most tractable f...
Hibonite is a comparatively rare, primary phase found in some CAIs from different chondrite groups a...