Computer Science
Scientific paper
Sep 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995metic..30r.575s&link_type=abstract
Meteoritics, vol. 30, no. 5, page 575
Computer Science
1
Impact Craters, Australasian, Indochinites, Laos, Tektites
Scientific paper
Approximately 770,000 years ago an asteroid or comet crashed with the Earth somewhere in southeast Asia, in what was arguably the largest terrestrial impact in the past several 10's of millions of years. Evidence for this impact is not a crater but ejecta from a crater - tektites, microtektites and impact debris - which are found over more than one-tenth of the Earth's surface. Despite its relative youth and the large size of the ejecta field, the structure produced by this impact has not yet been discovered. In the past few years searches have focused on eastern Indochina, specifically in northeast Thailand [1], Cambodia [2] and Laos [3]. In February, 1995 we spent ten days in southern Laos looking for the source crater. The trip was an outgrowth of an investigation using satellite imagery and a digital topographic database, which suggested the impact site might be one of several structures in southern Laos. The primary purpose of the trip was to investigate these structures; a secondary objective was to document tektite localities and to collect samples of known provenance. One crater-like structure identified from digital topographic and multispectral images seemed to be especially interesting due to its quasi-circular shape and relatively youthful appearance. Three additional suspicious structures were identified near this primary target, but these appeared much more subdued and highly eroded. All of these features lie in southern Laos within the broad region of Mesozoic marine sedimentary rocks, primarily sandstones interbedded with shales and limestones, which covers much of central Indochina. The top-priority structure, centered at 16.35 degrees N/106.15 degrees E, is a ring of steep-sided hills 35 to 40 km in diameter, rising 70 to several hundred meters above the surrounding flat plain. It also has a central elevated area rising about 100 meters above the floor, suggesting an eroded central uplift. Despite difficult field conditions we successfully reconnoitered all four potential impact structures. None showed obvious evidence of formation by extraterrestrial impact. A small domal feature near the city of Savannakhet is probably a salt diapir, and a nearby larger eviscerated domal form to the southeast is similarly related to broadscale evaporite tectonics. The 90 km diameter Savannakhet Basin shows no evidence of impact damage and has been a stable sedimentary trap since Mesozoic times. Our prime target, the 35 to 40 km diameter craterlike depression south of Muong Phin, is an erosional feature etched into upper layers of a sedimentary section. Its "central peak" is a fortuitous resistant erosional remnant. Not a great deal of time was available for the secondary objective, i.e., to look for tektites which occur in Indochina in two forms: layered form (Muong Nong-type) which appear to have flowed over the ground and splash form which solidified during atmospheric flight. We identified ten new sites and collected samples from some of these sites. Nine sites were in southern Laos, and all contained only layered tektites. Three of these sites were found by us in road-material quarries south of the village of Xeno. Here the yellow loessial soil overburden had been scraped off to expose a laterite layer rich in quartz pebbles, where small tektites were found after only a short search. This same technique, looking for road-material quarries beside the highway, was used to find layered tektites by Wasson's 1994 field expedition in Thailand [1] about 200 km to the southwest of our areas in Laos. Our new sites support a working theory [3, 4] that this area is rich in layered tektites but there are no splash-form tektites over a broad area of southern NE Thailand and neighboring Laos. The approximate dimensions of this area appears to be at least 200 by 350 km. Acknowledgments: Work was supported in part by NASA and the Barringer Crater Company. References: [1] Wasson J. T. et al. (1995) JGR, in press. [2] Hartung J. and Koeberl C. (1994) Meteoritics, 29, 411-416. [3] Schnetzler C. C. (1992) Meteoritics, 27, 154-165. [4] Wasson J. T. (1993) Eos Trans. AGU, 74, 390.
McHone John F. Jr.
Schnetzler Charles C.
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