Stable isotopic measurements of the low-temperature nitrogen components in ALH 84001

Geochemistry of the Martian meteorite ALH 84001, revisited

Major and trace element abundances were determined on powders prepared from four distinct chips from Allan Hills (ALH) 84001 to constrain the bulk rock composition, and to assess the trace element abundances of orthopyroxenes and phosphates. Our new determinations were used to evaluate the composition of the parental melt of this stone. An unrealistic light rare earth element (REE)-enriched par...

Geochemistry of the martian meteorite ALH 84001 , revisited by

Major and trace element abundances were determined on powders prepared from four distinct chips from ALH84001 in order to constrain the bulk rock composition, and to assess the trace element abundances of orthopyroxenes and phosphates. Our new determinations were used to evaluate the composition of the parental melt of this stone. An unrealistic light-REE enriched parental melt is calculated fr...

Martian Aqueous Alterations in Alh 84001 and the Nakhlite Meteorites

Carbonates. The dominant aqueous deposits in ALH 84001 are carbonate minerals, which form ellipsoids, discs, and other space-filling shapes, Figure 1 [1,4,5,6 etc]. These deposits are chemically zoned, nearly continuously from calcitic and ankeritic cores to magnesite-siderite compositions ranging from nearly pure magnesite to ~Mg45Fe45Ca10 (Fig. 2); hydromagnesite is not reported. The carbonat...

Carbonate formation events in ALH 84001 trace the evolution of the Martian atmosphere.

Carbonate minerals provide critical information for defining atmosphere-hydrosphere interactions. Carbonate minerals in the Martian meteorite ALH 84001 have been dated to ∼ 3.9 Ga, and both C and O-triple isotopes can be used to decipher the planet's climate history. Here we report Δ(17)O, δ(18)O, and δ(13)C data of ALH 84001 of at least two varieties of carbonates, using a stepped acid dissolu...

Stable nitrogen isotopic composition of amino acids reveals