Dissemin is shutting down on January 1st, 2025

Published in

Wiley, Meteoritics & Planetary Science, 2(36), p. 231-237, 2001

DOI: 10.1111/j.1945-5100.2001.tb01867.x

Links

Tools

Export citation

Search in Google Scholar

Thermal history of the Ibitira noncumulate eucrite as inferred from pyroxene exsolution lamella: Evidence for reheating and rapid cooling

Journal article published in 2001 by M. Miyamoto, T. Mikouchi ORCID, K. Kaneda
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

Green circle
Preprint: archiving allowed
Orange circle
Postprint: archiving restricted
Red circle
Published version: archiving forbidden
Data provided by SHERPA/RoMEO

Abstract

Abstract— Ibitira is a strongly recrystallized and unbrecciated noncumulate eucrite. We measured Ca compositional profiles of Ibitira pyroxene by electron microprobe and computed the cooling rate and burial depth from pyroxene exsolution profiles to gain information on early thermal history of Ibitira. Pyroxene begins to exsolve at 1082 °C and cools down to 550 °C at a rate of 0.02 °C/year, forming an augite lamella about 7.0 μm in width. A notable characteristic of the Ca profile of augite lamellae in Ibitira pyroxene is a gradient near the interface between augite and low-Ca pyroxene (pigeonite). This profile suggests that after thermal metamorphism Ibitira pyroxene experienced a sudden temperature rise to above solidus temperature of pyroxene (∼1082 °C), and subsequent rapid cooling. The 39Ar-40Ar age of 4.485 Ga for Ibitira, which is the oldest 39Ar-40Ar age for noncumulate eucrites, may date this reheating event.