The Dergaon (H5) chondrite: Fall, classification, petrological and chemical characteristics, cosmogenic effects, and noble gas records
| dc.contributor.author | Shukla, P. N. | |
| dc.contributor.author | Shukla, A. D. | |
| dc.contributor.author | Rai, V. K. | |
| dc.contributor.author | Murty, S. V. S. | |
| dc.contributor.author | Bhandari, N. | |
| dc.contributor.author | Goswami, J. N. | |
| dc.contributor.author | Mazumdar, A. C. | |
| dc.contributor.author | Phukon, P. | |
| dc.contributor.author | Duorah, K. | |
| dc.contributor.author | Greenwood, R. E. | |
| dc.contributor.author | Franchi, I. A. | |
| dc.date.accessioned | 2021-02-12T21:17:22Z | |
| dc.date.available | 2021-02-12T21:17:22Z | |
| dc.date.issued | 2005-01-01 | |
| dc.identifier.citation | Shukla, P. N., Shukla, A. D., Rai, V. K., Murty, S. V. S., Bhandari, N., Goswami, J. N., ... & Franchi, I. A. (2005). The Dergaon (H5) chondrite: Fall, classification, petrological and chemical characteristics, cosmogenic effects, and noble gas records. Meteoritics & Planetary Science, 40(4), 627-637. | |
| dc.identifier.issn | 1945-5100 | |
| dc.identifier.doi | 10.1111/j.1945-5100.2005.tb00967.x | |
| dc.identifier.uri | http://hdl.handle.net/10150/655991 | |
| dc.description.abstract | A multiple fall of a stony meteorite occurred near the town of Dergaon in Assam, India, on March 2, 2001. Several fragments weighing <2 kg and a single large fragment weighing ~10 kg were recovered from the strewn field, which extended over several tens of square kilometers. Chemical, petrographic, and oxygen isotopic studies indicate it to be, in most aspects, a typical H5 chondrite, except the unusually low K content of ~340 ppm. A cosmic ray exposure of 9.7 Ma is inferred from the cosmogenic noble gas records. Activities of eleven cosmogenic radionuclides were measured. 26Al and 22Na activities as well as the 22Na/26Al activity ratio are close to the values expected on the basis of solar modulation of galactic cosmic rays. The low 60Co activity (<1 dpm/kg) is indicative of a small preatmospheric size of the meteorite. Cosmic ray heavy nuclei track densities in olivine grains range from ~10^6 cm^(-2) in samples from the largest fragment to approximately (4-9) x 105 cm^(-2) in one of the smaller fragments. The combined track, radionuclide, and noble gas data suggest a preatmospheric radius of ~20 cm for the Dergaon meteorite. | |
| dc.language.iso | en | |
| dc.publisher | The Meteoritical Society | |
| dc.relation.url | https://meteoritical.org/ | |
| dc.rights | Copyright © The Meteoritical Society | |
| dc.rights.uri | http://rightsstatements.org/vocab/InC/1.0/ | |
| dc.subject | Dergaon (H5) chondrite | |
| dc.subject | strewn field | |
| dc.subject | oxygen isotope studies | |
| dc.title | The Dergaon (H5) chondrite: Fall, classification, petrological and chemical characteristics, cosmogenic effects, and noble gas records | |
| dc.type | Article | |
| dc.type | text | |
| dc.identifier.journal | Meteoritics & Planetary Science | |
| dc.description.collectioninformation | The Meteoritics & Planetary Science archives are made available by the Meteoritical Society and the University of Arizona Libraries. Contact lbry-journals@email.arizona.edu for further information. | |
| dc.eprint.version | Final published version | |
| dc.description.admin-note | Migrated from OJS platform February 2021 | |
| dc.source.volume | 40 | |
| dc.source.issue | 4 | |
| dc.source.beginpage | 627 | |
| dc.source.endpage | 637 | |
| refterms.dateFOA | 2021-02-12T21:17:22Z |
