Exposure history of the Torino meteorite
dc.contributor.author | Wieler, R | en_AU |
dc.contributor.author | Graf, T | en_AU |
dc.contributor.author | Signer, P | en_AU |
dc.contributor.author | Vogt, S | en_AU |
dc.contributor.author | Herzog, GF | en_AU |
dc.contributor.author | Tuniz, C | en_AU |
dc.contributor.author | Fink, D | en_AU |
dc.contributor.author | Fifield, LK | en_AU |
dc.contributor.author | Klein, J | en_AU |
dc.contributor.author | Middleton, R | en_AU |
dc.contributor.author | Jull, AJT | en_AU |
dc.contributor.author | Pellas, P | en_AU |
dc.contributor.author | Masarik, J | en_AU |
dc.contributor.author | Dreibus, G | en_AU |
dc.date.accessioned | 2021-12-21T01:19:42Z | en_AU |
dc.date.available | 2021-12-21T01:19:42Z | en_AU |
dc.date.issued | 1996-03 | en_AU |
dc.date.statistics | 2021-10-21 | en_AU |
dc.description.abstract | We determined He, Ne, Ar, 10Be, 26Al, 36Cl, and 14C concentrations, as well as cosmic-ray track densities and halogen concentrations in different specimens of the H6 chondrite Torino, in order to constrain its exposure history to cosmic radiation. The Torino meteoroid had a radius of ∼20 cm and travelled in interplanetary space for 2.5–10 Ma. Earlier, Torino was part of a larger body. The smallest possible precursor had a radius of 55 cm and a journey through space longer than ∼65 Ma. If the first-stage exposure took place in a body with a radius of >3 m or in the parent asteroid, then it lasted nearly 300 Ma. The example of Torino shows that it is easy to underestimate first-stage exposure ages when constructing two-stage histories. © 1999-2021 John Wiley & Sons, Inc. | en_AU |
dc.identifier.citation | Wieler, R., Graf, T., Signer, P., Vogt, S., Herzog, G. F., Tuniz, C., Fink, D., Fifield, L. K., Klein, J., Middleton, R., Jull, A. J. T., Pellas, P., Masarik, J., & Dreibus, G. (1996). Exposure history of the Torino meteorite. Meteoritics & Planetary Science, 31(2), 265-272. doi:10.1111/j.1945-5100.1996.tb02022.x | en_AU |
dc.identifier.issn | 1945-5100 | en_AU |
dc.identifier.issue | 2 | en_AU |
dc.identifier.journaltitle | Meteoritics & Planetary Science | en_AU |
dc.identifier.pagination | 265-272 | en_AU |
dc.identifier.uri | https://doi.org/10.1111/j.1945-5100.1996.tb02022.x | en_AU |
dc.identifier.uri | https://apo.ansto.gov.au/dspace/handle/10238/12610 | en_AU |
dc.identifier.volume | 31 | en_AU |
dc.language.iso | en | en_AU |
dc.publisher | Wiley | en_AU |
dc.subject | Meteorites | en_AU |
dc.subject | Radiation doses | en_AU |
dc.subject | Halogens | en_AU |
dc.subject | Interplanetary space | en_AU |
dc.subject | Asteroids | en_AU |
dc.subject | Density | en_AU |
dc.title | Exposure history of the Torino meteorite | en_AU |
dc.type | Journal Article | en_AU |
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