Tektites: The Natural Glass an Ancient Impact Scattered Across Asia

Tektites are not meteorites. They are Earth rock, melted by the violence of an extraterrestrial impact, thrown so high and fast that they cooled in near-vacuum before falling back as glass. The result is chemically unlike any volcanic glass: almost no water content, no crystals, and a composition that matches the target geology of wherever the impactor struck, not the impactor itself.

The Australasian strewn field is the largest and youngest of the four known tektite fields on Earth. It covers roughly 50 million square kilometres, about a tenth of the planet's surface, spreading from southern China and Indochina through the Philippines, across Australia, and into the Southern Ocean. Specimens from this field turn up in layers of sediment dated to approximately 790,000 years ago. That date is not contested. The crater is.


Australasian tektites come in several forms depending on how far they travelled and how they moved through the atmosphere on the way down. Splash-form tektites, spheres, dumbbells, teardrops, discs, cooled while spinning in free flight and carry that rotation in their shape. Muong Nong-type tektites, found mainly in Laos and Thailand, are layered slabs that barely left the ground; they landed close to the source and kept their bulk. Microtektites, recovered from deep-sea sediment cores across the Indian Ocean and beyond, are the finest spray from the same event, invisible to the naked eye and identified only under a microscope.


The glass itself is typically dark olive to black, translucent when sliced thin, and reads under analysis as a mix of silica, aluminium oxide, and iron that matches upper-crustal rock rather than mantle material. Some Australasian tektites contain lechatelierite, pure silica glass that forms only above 1700 degrees Celsius, which places the temperature of the impact melt beyond anything a volcano produces.


For every other major tektite field, a source crater exists. The North American field traces to the Chesapeake Bay impact structure. The Central European field links to the Nördlingen Ries crater in Bavaria. The Ivory Coast field matches the Bosumtwi crater in Ghana. The Australasian field has no confirmed match.

The leading candidate since the 2000s is a buried structure in the Bolaven Plateau region of southern Laos, identified partly through gravity anomaly surveys and partly through the concentration of Muong Nong-type tektites nearby. A 2019 study in PNAS by Kerry Sieh and colleagues at the Earth Observatory of Singapore made a detailed case for a crater 13 kilometres wide hidden beneath a volcanic plateau that erupted after the impact and buried the evidence. The geology is consistent. The crater has not been drilled to confirmation.

Other researchers have proposed locations in the South China Sea or under the Mekong Delta, where sediment accumulation since the Pleistocene could conceal a structure of the right age and size. Until a drill core pulls up shocked quartz and impact melt from a single buried feature, the Australasian strewn field remains the only young, large tektite field without a verified source.

The Australasian strewn field reaches into the Indian subcontinent. Tektites recovered from sites in peninsular India, sometimes called indochinites in older literature, fall within the chemical and age range of the broader Australasian population. They arrived here the same way they arrived in Thailand and the Philippines: as molten glass raining from the upper atmosphere after an impact that happened somewhere to the east.

India also has its own separate tektite locality with no connection to the Australasian event. The Lonar crater in Maharashtra, formed roughly 570,000 years ago by a meteorite impact into the Deccan Traps basalt, produced impact glass and shocked minerals that are studied in their own right. Lonar is one of only four known impact craters in basaltic rock on Earth, and the Geological Survey of India has documented its structure extensively. It is not a tektite source in the classical sense, the ejecta did not travel far, but it is the clearest impact scar on Indian soil and gives geologists a local reference point for what a confirmed crater looks like from the inside.

Finding the Australasian source crater matters beyond completing a catalogue. The 790,000-year-old impact happened during the Pleistocene, when early humans were present in Southeast Asia. An impactor large enough to melt and scatter glass across 50 million square kilometres would have released energy far beyond any historical volcanic eruption. Whether it left a detectable signature in the fossil or archaeological record of the region is an open question, one that requires knowing where, exactly, the energy was released.

The tektites themselves are the only physical record of the event that is both abundant and precisely dated. They sit in museum drawers, in farmers' fields in Laos, in deep-sea cores pulled from the floor of the Indian Ocean. Each one is a piece of Earth that briefly left the planet and came back as glass. The crater that made them is somewhere under a few hundred metres of basalt or sediment, waiting for a drill to find it.