Australasian strewnfield
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The Australasian strewnfield, covering at least one-tenth of the Earth's surface, is the largest and the youngest of the tektite strewnfields. The 800,000 year-old strewnfield includes most of Southeast Asia (Vietnam, Thailand, Southern China, Laos and Cambodia). The material from the impact stretches across the ocean to include the islands of the Philippines, Indonesia, Malaysia and Java and reaches far out into the Indian Ocean and south to the western side of Australia.
The impact crater may have been between 32 and 114 kilometres in diameter. Also, some recent estimates suggest that the strewn field may cover 30% of the earths surface (Povenmire et.al).
[edit] References and further reading
- Paine M. (2001) "Source of the Australasian Tektites?" Meteorite, Feb 2001.
- Schmidt G. and Wasson J. (1993) "Iridium in sediments containing large abundances of Australasian microtektites from DSDP hole 758B in the Eastern Indian ocean and from DSDP hole 769A in the Sulu Sea," Proceedings of 24th Lunar and Planetary Science conference
- Hartung J. and Koberl C. (1994) "In search of the Australasian tektite source crater: the Tonle sap hypothesis", Meteoritics.
- Schnetzler C. C. and Mchone J.F. (1996) "Masses of the impactor, the Australasian tektites, and size estimates of the main source crater," Meteoritics, vol 28 no .3 , 430, July 1993.
- Glass B.P. (1999) "Muong Nong-type Australasian tektites: implications regarding the parent material and source area," Ninth Annual V.B.m Goldschmidt Conference, Massachusetts, August 1999.
- Glass B.P. and Pizzuto J.E. (1994) "Geographic variation in Australasian microtektite concentrations: Implications concerning the location and size of the source crater," J of Geophysical Research, vol 99, no E9, 19075-19081, Sept 1994 (abstract only).
- Povenmire H., Liu W. and Xianlin I. (1999) "Australasian tektites found in Guangxi Province, China," 30th Annual Lunar and Planetary Scinece Conference, Houston, March 1999.
