In situ occurrence of Muong Nong-type Australasian tektite fragments from the Quaternary deposits near Huai Om, northeastern Thailand

There are several reports of Australasian tektites found within a stratum called “laterite” layer widely distributed in Indochina. However, it has been debated whether these tektites are in situ or reworked. This uncertainty is because a detailed description of their field occurrence is lacking. Here, we describe the detailed occurrence of a cluster of tektite fragments recovered from the “laterite” layer near Huai Om, northeastern Thailand, and demonstrate the evidence of in situ occurrence of the tektites. At least 331 tektite fragments with a total weight of 713 g were found from a 40 × 30 cm area with 10 cm thickness in the uppermost part of the “laterite” layer. The very angular shapes and very poorly sorted nature of the fragments, restoration of larger tektite fragments into one ellipsoidal Muong Nong-type (MN) tektite mass, and the similar chemical composition of the fragments suggest that these MN tektite fragments represent a tektite mass that fragmented in situ. The fact that the fragments were found within the “laterite” layer is inconsistent with a previous interpretation that the upper surface of the “laterite” layer is a paleo-erosional surface, on which the tektites are reworked. The size distribution of the fragments is bi-fractal following two power laws in the range from 10 to 26 mm and from 26 to 37 mm, respectively, with fractal dimensions (Ds) of 2.2 and 7.5. The Ds for the coarse fraction of the tektite fragments is larger than the Ds for rock fragments generated by rockfalls and rock avalanches and similar to the Ds for the coarser fraction fragments generated by high-speed impact experiments, suggesting that the tektite fragments were formed through intense fragmentation by a relatively high energetic process. The occurrence of the fragments forming a cluster indicates that the fragments were not moved apart significantly after fragmentation and burial. Based on these results, we concluded that the mass of a tektite was fragmented at the time of the landing on the ground after traveling a ballistic trajectory and has not been disturbed further.


Introduction
Tektites are objects composed entirely of glass formed by meteorite impacts (Koeberl 1994). Tektites are found from at least four broad areas of the Earth's surface, called strewn fields (e.g., Koeberl 1994;Glass and Simonson 2012). The Australasian tektites were formed ca. 0.8 Ma and occur as the largest and youngest strewn field extending from southwestern China, through Indochina, Australia to Antarctica (Folco et al. 2016). Despite the largest size and youngest age of the strewn field, the source crater has never been identified. Nevertheless, it is expected that the record of the impact and consequent environmental perturbations are well preserved because the impact event which made Australasian tektites (here we term the Australasian Tektite Event; AATE) is the youngest among the large impact events on the Earth. Thus, the AATE has broader significance to the study of the meteorite impact phenomena on Earth.
Although there are a large number of studies on the geochemistry and microstructure of Australasian tektites, many of them were conducted on samples of unknown or uncertain provenance (e.g., Fudali et al. 1987;  Table 1). The names of locations mentioned in the text are also shown Tada et al. Progress in Earth and Planetary Science (2020)  Wasson 1991; Schnetzler and McHone 1996;Herzog et al. 2008). There are several reports of tektites found in the Quaternary deposits of Indochina ( Fig. 1), of which some occurrences are listed in Table 1 ( Barnes and Pitakpaivan 1962;Tamura 1992;Wasson et al. 1995;Fiske et al. 1996Fiske et al. , 1999Schnetzler and McHone 1996;Songtham et al. 2011Songtham et al. , 2012. In these studies, tektites were found in a loose gravel (granule to pebble-bearing sand) layer with abundant reddish-black spherical-to irregular-shaped ferruginous nodules, called a "laterite" layer, but the details of the occurrence of the tektites were not described. Several authors have considered that the tektites recovered from the "laterite" layer were directly deposited in the strata from which they were recovered and hence were found in situ (Wongsomsak 1986;Tamura 1992;Songtham et al. 2011Songtham et al. , 2012Nuchanong et al. 2014). However, the possibility that the tektites have been reworked has been claimed based on reasoning advanced below (Fiske et al. 1996;Koeberl and Glass 2000;Keates 2000;Langbroek 2015). Fiske et al. (1996) conducted field surveys at two sites: Huai Sai and Huai Om in northeastern Thailand. At Huai Om, they found two MN tektite fragments from the top of the "laterite" layer exposed along a dam spillway. At Huai Sai, they excavated a 2 × 3 m area and found 1139 fragments of a MN tektite forming a cluster at the top boundary of the "laterite" layer. Based on the size distribution of the tektite fragments that follows a power law, similar chemical composition of each fragment, and the fact that many fragments form a cluster, Fiske et al. (1996) concluded that the tektite fragments originated from one large tektite mass that underwent fragmentation. Fiske et al. (1996) interpreted the top of the "laterite" layer as a paleo-erosional surface based on the hardcemented appearance (of the upper surface of the "laterite" layer) that looks like an erosional pavement and interpreted the MN tektite fragments found at the upper boundary of the "laterite" layer to have been reworked on the paleo-erosional surface. However, the interpretation that the upper boundary of the "laterite" layer represents a paleo-erosional surface is based only on their visual observation of the upper surface of the "laterite" layer in the field. Despite concluding that the tektites are reworked, Fiske et al. (1996) noted that there was little evidence that the tektite fragments have undergone significant lateral transport and remained clustered. Thus, the interpretation of Fiske et al. (1996) that tektites found at the top of the "laterite" layer are of reworked origin does not seem to be well supported by their own observations. Nonetheless, this point has long been overlooked and their conclusion that most tektites have been reworked has been widely accepted. Australasian tektites in Australia generally are found in deposits that have been dated as younger in age than the impact event, and thus, these tektites are considered to be reworked (e.g., Fudali 1993). By analogy with the observation in Australia, Koeberl and Glass (2000) and Keates (2000) argued that tektites found in Indochina might also have been reworked, although no field evidence from SE Asia was advanced.
In this study, we report a detailed occurrence of tektite fragments found within the "laterite" layer at a section designated HO06 located about 15 km southwest of Huai Om in northeastern Thailand in order to test whether the MN tektite fragments of similar occurrence are of primary depositional origin or reworked. We conducted a field survey at the HO06 section and made a detailed description of the field occurrence of the MN tektite fragments. We also measured the major element compositions of nine MN tektite fragments by electron probe microanalysis (EPMA) to confirm that these glass fragments are Australasian MN tektites and to demonstrate that these fragments have chemical composition similar to each other. We restored a part of an original tektite mass using large tektite fragments recovered from a block sample to demonstrate that tektite fragments forming a cluster originally formed a large MN tektite mass.

Study site and lithostratigraphy
The HO06 section (14°34′ 45.2″ N 105°16′ 30.0″ E) is located about 15 km southwest of Huai Om, Ubon Ratchatani Province, northeastern Thailand (Fig. 1). As noted above, Fiske et al. (1996) reported MN tektites from the top of the "laterite" layer at Huai Om. The HO06 section is exposed along the spillway of reservoirs named Huai Phueng and Phlan Suea Ton Lang (Fig. 2). The weathered Cretaceous sedimentary basement and overlying Quaternary deposits are exposed continuously laterally for at least 200 m along both sides of the spillway. A cluster of Australasian MN tektite fragments was found in the section at the north bank. We did not find any evidence of tectonic disturbance of the basement and the overlying Quaternary deposits.
The basement rock at the HO06 section is whitish gray (weathered) to purplish-gray (less weathered) very fine quartzo-feldspathic sandstone of the Cretaceous Khok Kruat Formation, the uppermost part of the Khorat Group (Nuchanong et al. 2014). The exposed thickness of the basement sandstone is approximately 2 m. The basement sandstone dips approximately 10°to the west and is exposed continuously along the spillway (Fig. 3a, b).
The Quaternary deposits overlie the Cretaceous basement unconformably and can be divided into three lithostratigraphic units (Units 1 to 3 in ascending order; Fig. 3) that are similar to those reported at Huai Om Tada et al. Progress in Earth and Planetary Science (2020) Barnes and Pitakpaivan 1962 Huai Sai Thailand N 14°53′ E 105°25′ MN A cluster of 1139 MN tektite fragments with a total mass of 6 kg was partly exposed at the surface. The largest piece weighed 701.7 g. The fragments were concentrated in 2 × 3 m area and 30 cm in depth. These fragments were in the uppermost light gray sandy soil layer and in the upper 10 cm of the quartz pebble-bearing "laterite" layer. Most of the fragments were found at the boundary of these two layers Fiske et al. 1996 Huai Om Thailand N 14°35′ E 105°17′ MN Two MN tektite fragments with a total weight of 2 g were found from the top of the "laterite" layer. 14 MN tektite fragments with a total weight of 43.5 g were in float but clearly derived from the immediate strata above Ban Non Chai Thailand N 16°22.83′ E 102°51.45′ Not described One tektite is from the "laterite" layer, partly exposed in the ground surface Tamura 1992 Ban Samran Thailand N 16°32.73′ E 102°49.85′ Not described One tektite is from the "laterite" layer, partly exposed in the ground surface Tamura 1992 Ban Khan Kaem Khun Thailand N 16°40.50′ E 102°48.33′ Not described One tektite is from the "laterite" layer, partly exposed in the ground surface Tamura 1992 Noen Sa-nga Thailand N 15°36.50′ E 101°58.00′ Irregular shape A small piece of an irregular-shaped tektite with a weight of 8.75 g is found at the top of the "laterite" layer section where lithological description was reported (Tada et al. 2019). Unit 1 is a whitish-gray silty very fine sand layer. The thickness of this unit is 70 cm. The basal contact is sharp, largely horizontal, slightly undulating, and forms an angular unconformity (Fig. 3). Unit 2 is a reddish-brown, poorly sorted, granule-to pebble-bearing medium to coarse sand layer. The thickness of this unit is 55 cm. The basal contact is sharp and generally planar. The gravel clasts are 0.2-3 cm in diameter and are composed mainly of white quartzite pebbles and their fragments ( Fig. 3e). This unit is partly cemented by reddishbrown iron oxides to form reddish black pebble size spherical-to irregular-shaped nodules, which are coalescent to each other in some cases (Fig. S1). This observation is consistent with the descriptions of the "laterite" layer (e.g., Songtham et al. 2011Songtham et al. , 2012. Unit 3 is composed of whitish-to brownish-gray massive fine sand of 2 m thickness (Fig. 3d). It overlies Unit 2 with a sharp, planar conformable contact with no evidence of erosion. This unit is capped by ca. 20 cm thick modern soil with a gradational contact. The MN tektite fragment cluster was found in the upper part of Unit 2 (ca. 10 cm below the upper unit boundary) (Fig. 2, 4). The detailed occurrence of the MN tektite fragments is described in the "Results and discussion" section.

Methods
A block sample of 25 × 15 cm area with 10 cm thickness was taken for three-dimensional (3D) computed tomography (CT) scanning from the area where the MN tektite fragment cluster was found, using a handheld electric cutter. The block sample was dismantled in the laboratory after the CT scanning, and MN tektite fragments larger than 5 mm diameter were recovered. After taking the block sample, we further recovered MN tektite fragments by gradually expanding the excavated area until no large (> 1 cm diameter) tektite fragments were found. In total, a ca. 40 × 30 cm area was excavated. There is a possibility that we overlooked small (< 1 cm diameter) tektite fragments spread further away.
The major element compositions of nine selected tektite fragments were determined by EPMA on thin sections. EPMA was conducted using a JEOL JXA-8900 L electron probe microanalyzer at the Department of Earth and Planetary Science, the University of Tokyo. The analysis was performed using 15-kV accelerating voltage and 7.5-nA beam current, with a defocused electron beam of 5 μm. Counting times were 10 s on peak and 5 s on the background. Analyzed elements were Si, Al, Fe, K, Mg, Ca, Na, Ti, and Mn. Sodium and potassium were analyzed before other elements to reduce possible volatilization effects followed by the method of Glass et al. (2020). The precision of the EPMA was evaluated by the analysis of the composition-known magnetite. Based on the analysis of the magnetite that was repeated ten times, the analytical precision was better than 0.5% in concentration for all the elements.
Ten to twenty points were measured on each thin section. Because the total percentage of measured elements varies between 96 and 100 wt. %, we used data, the total percentage of which is larger than 98%, for calculating an average and standard deviation of major oxide composition for each thin section. After the data screening, each thin section still has ten to fifteen measured points. The standard deviation of major oxide compositions, which is 1.3% as a maximum (Table 2), includes variation due to heterogeneity of sample and uncertainty of measurement.
Consideration of the distribution of fragments sizes is often used to infer fragmentation processes (e.g., Farris and Paterson 2007;Bjørk et al. 2009;Roy et al. 2012). Fragmentation due to crushing or fracturing rock or glass leads to mass distributions that can be described by power law functions in which fragment frequency increases with a decrease in fragment size, due to scale invariance of the fragmentation process (e.g., Turcotte 1986). The relationship between fragment size and cumulative frequency can be represented by the power law equation where r is a radius of a fragment, N (≥ r) is the number of fragments with a radius greater than r, and k is a fitting parameter. Ds is the fractal dimension for fragment size distribution.
The size and weight of each fragment was recorded in the laboratory. We measured the long, intermediate, and short axes (a, b, and c axes) defined as the dimensions of a fragment in three mutually orthogonal planes (a > b > c). The dimensions were measured using a caliper with an accuracy of 0.05 mm.
The block sample was subjected to X-ray CT imaging using micro-CT scanner TESCO TXS320-ACTIS at the National Museum of Nature and Science, Tokyo. Each MN tektite fragment was separated using the segmentation editor in Amira 5.4.3 software based on the contrast of X-ray transmittance between tektite fragments and surrounding matrix. Because smaller tektite fragments are more difficult to recognize on CT images, we identified tektite fragments larger than 1 cm. The identification of the tektite fragments in the CT images was confirmed by comparing each fragment to the tektite fragments collected from the dismantled block sample. In this study, only the preliminary result of observation of CT images is presented.

Description of the MN tektite fragments
The MN tektite fragments found at the HO06 section are black in color, vesicular, and show submillimeterscale layering (Fig. 5). Under an optical microscope, thin sections of the fragments show layering composed of the dark-brownish-colored and light greenish-colored glass stripes, which are parallel to each other. Each stripe has 10-μm scale subparallel lamination characterized by alternation of dark-brownish and pale greenish lenses. Elongated vesicles of submillimeter size, the long axes of which are roughly parallel to the layering, are occasionally observed (Fig. 6). Mineral inclusions which are several micrometers in diameter are sparsely contained, but they are too small to identify mineral species under an optical microscope. These characteristics are typical for MN Australasian tektites found in Indochina (e.g., Wasson 1991; Glass et al. 2020). Three-hundred and thirty-one MN tektite fragments were found in the small (~40 cm × 30 cm) area with 10 cm in thickness in the upper part of Unit 2 ( Fig. 4) (One-hundred and seventy-seven fragments were recovered in the field after taking the block sample, and 154 fragments were recovered in the laboratory from the dismantled block sample.) The total weight of the 331 fragments is 713 g.
The length of a, b, and c axes of the fragments ranges from 2.00 to 52.80 mm, 1.95 to 40.00 mm, and 0.70 to 30.80 mm, respectively. The average length and standard deviation (in parenthesis) are 16.3 (8.7), 11.3 (7.1), and 7.2 (5.5) mm, respectively. These large standard deviations of the size of the tektite fragments correspond to "very poor sorting" in the scale of sorting for sediments (Folk and Ward 1957). The fragments are very angular, and fragile edges are well preserved, as shown in Fig. 5. Forty-six large fragments recovered from inside the block sample and seven large fragments recovered in the field after taking the block sample (53 tektite fragments in total) are fitted together to form a large MN tektite mass of~370 g that shows an ellipsoidal shape (Fig. 7a). The rest of the fragments are too small and so many that it is difficult to find their positions to conduct restoration of the original tektite mass. However, the preliminary restoration result strongly suggests that tektite fragments forming the cluster composed one large tektite mass of > 713 g weight before the landing. The majority of the outermost part of the restored tektite mass was peeled off showing the section of the internal layered structure (Fig. 7b), while a typical pitted and grooved surface similar to that in splash-form tektites was preserved in some part (Fig. 7c) suggesting the original surface of the tektite mass was preserved. The fracture surfaces of the MN tektite fragments from HO06 are matt compared to a fresh fracture surface due to the presence of small pits, as shown in Fig. 7d. These matt surfaces of the tektites were formed by soil etching after their burial (Rost 1969;La Marche et al. 1984), suggesting that fracturing occurred in the geological past. Nearly all fragments have iron-oxide cement and calcite cement in some cases adhering to some of the fragment surfaces, and some vesicles open to the surface are filled with the iron-oxide and calcite cement materials indicating that the laterization of Unit 2 occurred after their fragmentation.  The fact that most of large tektite fragments recovered from the block sample fitted together to form a large ellipsoidal tektite mass with the original surface partly preserved indicates the tektite fragments were formed as a result of the fragmentation of one large tektite mass. The very poorly sorted nature of the MN tektite fragments, the very angular shapes with well-preserved fragile edges, and the occurrence of tektite fragments forming a cluster suggest that these MN tektite fragments were not transported a long distance but rather fragmented in situ.

Major element composition
The major element compositions of all nine MN tektite fragments from the HO06 section, together with their average compositions and standard deviations, are given in Table 2. The major element compositions of these samples fall within the range of compositions of previous analyses of MN tektites from Ubon Ratchathani province within 1σ, for most elements (Glass and Koeberl 1989;Koeberl 1992;Fiske et al. 1996;Herzog et al. 2008) (Fig. 8a), indicating that they are not distinguishable chemically from previously reported Australasian MN tektites from Ubon Ratchathani province. Figure 8b shows SiO 2 vs Al 2 O 3 , FeO, K 2 O, and MgO values for the nine MN tektite fragments from the HO06 section plotted with values reported for other Australasian MN tektites from Ubon Ratchatani province ( Glass and Koeberl 1989;Koeberl 1992;Fiske et al. 1996;Herzog et al. 2008). The major element composition of the nine fragments is closely plotted in a narrow area and indistinguishable from each other within 1σ. This narrow range of the major element composition of the nine fragments is consistent with the idea that the MN tektite fragments collected at HO06 section originally formed one large MN tektite mass.

Size distribution of the MN tektite fragments
Ds for the fragments generated by fragmentation of rocks or glass is proportional to the intensity of fracturing in which fragments generated by higher magnitude and rate of stress loading tend to have higher value of Ds, although Ds is affected also by the inherent strength properties of the rock or glass (e.g., Takagi et al. 1984;Jébrak 1997;Roy et al. 2012;Xu 2018). For instance, Ds for rock fragments generated by weathering of andesite in the field and hammering of a limestone cube by hand is 2.5-2.7 (calculated from the data of Domokos et al. 2015), and that for rock fragments generated by rockfalls and rock avalanches with various lithology ranges from 1.6 to 4.7 (Crosta et al. 2007;Ruiz-Carulla and Corominas, 2020). Rock fragments generated by complete fragmentation of target rocks in hypervelocity impact experiments show bi-or tri-fractal distributions in which Ds for the finer fraction is 1.7 to 4.3 and Ds for the coarser fraction is 4.8 to 11.9 (calculated from the data of Takagi et al. 1984;Michikami et al. 2016). The Ds for fragments of a block on the Moon fragmented by a small meteorite impact is around or higher than 4 (Ruesch et al. 2020). Figure 9 shows the cumulative size distribution of the MN tektite fragments at HO06 section. The size of the fragment is represented by the length of its equivalent spherical diameter (r = ffiffiffiffiffiffiffi abc 3 p ). The cumulative size dis-tribution increases rapidly from 37 to 26 mm and then increases slowly in a range smaller than 26 mm. It shows a bi-fractal distribution described by two power laws in the range from 10 to 26 mm and from 26 to 37 mm, with Ds of 2.2 and 7.5, respectively. The position of the point dividing the two power laws is calculated by adjusting the dividing point every 0.5 cm to maximize the average of the R 2 values. The bi-fractal distribution of fragment size implies that the size distribution of the fragments was affected by two different fragmentation mechanisms (e.g., Schultz and Gault 1990). Although the effect of the difference of physical properties between the tektite glass and rocks need to be considered, the high Ds value (7.5) for the coarse fraction of the tektite fragments is larger than the range of Ds previously reported for rock fragments generated by rockfalls and rock avalanches (1.6-4.7; Crosta et al. 2007;Ruiz-Carulla and Corominas 2020) and similar to the Ds for the coarser fraction fragments generated by hyperspeed impact experiments (4.8-11.9; calculated from the data of Takagi et al. 1984;Michikami et al. 2016) and impact fragmentation on the Moon (3.3-6; Ruesch et al. 2020), suggesting that the tektite fragments were formed through intense fragmentation by a relatively high energetic process. Based on the close spatial association of the MN tektite fragments at Huai Sai, Fiske et al. (1996) proposed that the fragmentation of an original MN tektite mass was a low-energy process such as weather or climaterelated temperature-induced fracturing after the deposition of the MN tektite mass. However, as is mentioned (See figure on previous page.) Fig. 8 Major element compositions of the MN tektite fragments from the HO06 section. a Comparison of the major element compositions of the MN tektite fragments from the HO06 section and the average of other MN tektites from the same region, Ubon Ratchathani province, previously reported. b X-Y plots of the concentrations of SiO 2 versus Al 2 O 3 , FeO, K 2 O, and MgO of the MN tektite fragments from the HO06 section compared with other MN tektites from the same region, Ubon Ratchathani province, previously reported by Koeberl (1992), Fiske et al. (1996), Herzog et al. (2008), and Glass and Koeberl (1989). The error bars represent 1σ of ten to fifteen measurements of each section Fig. 9 Cumulative size distribution of the MN tektite fragments from the HO06 section for size range of r > 10 mm Tada et al. Progress in Earth and Planetary Science (2020)  above, the size distribution of the coarse fraction of the MN tektite fragments from HO06 section measured in this study suggests a relatively high-energy process rather than a low-energy process such as weather or climate-related temperature-induced fracturing. The possibility that the MN tektite mass was broken by tectonic movement after deposition is also unlikely because we did not see any evidence of tectonic deformation at the outcrop. The other possibility is that the fragmentation occurred during the flight by high-speed collision of ejecta materials before the deposition. However, this possibility is also unlikely because if the fragmentation occurred during the flight, the fragments would have separated before they landed on the ground and would not have formed a cluster. Consequently, the timing of the fragmentation of the MN tektite mass is constrained to the time of the landing on the ground. We propose that an original tektite mass was fragmented by collision of the MN tektite mass with the ground. Either the MN tektite fragments were considered to have been codeposited with other ejecta materials immediately after (or almost the same time) the fragmentation or the MN tektite mass was fragmented during penetration into the unconsolidated ejecta of Unit 2 so that the fragments remained as a cluster. As for the fragmentation mechanism for the finer fraction of the MN tektite fragments, one possibility is that some of the tektite fragments were further fractured by weather or climate-related thermal fracturing after the deposition. Another possibility is that some of the tektite fragments generated by the collision of the original tektite mass with the ground surface were secondarily fractured by collision with the surrounding other ejecta materials immediately after the first fragmentation, resulting in the bi-fractal size distribution of the tektite fragments. In any case, the whole size distribution of the tektite fragments, especially the high Ds value for the coarse fraction, is different from the size distributions of rock fragments generated by low-energy processes.

Preliminary observation of CT scan 3D image of the block sample
In CT cross-section images, tektite fragments appear as angular-shaped areas with moderate X-ray transmittance, exhibiting elongated vesicles. The preliminary CT scan 3D image observation of the block sample revealed that the MN tektite fragments are distributed in 20 × 10 × 10 cm space as if they were expanded from the original tektite mass by fragmentation. This distribution of the tektite fragments suggests either that the tektite fragments were buried immediately after fragmentation on landing by co-deposited other ejecta materials of Unit 2 or that fragmentation occurred during the tektite mass penetrated into the ground cover of unconsolidated ejecta (granule to pebble-bearing sand) of Unit 2 so that tektite fragments have not been spread significantly. This distribution of the tektite fragments is inconsistent with the previous interpretation in which these tektites were considered to have been reworked on the paleo surface because if reworked on the paleo surface, the fragments would be distributed on a plane.

Stratigraphic position of MN Australasian tektite in Indochina
As is proposed in the previous sections, the fragmentation of the MN tektite mass occurred at the time of the landing on the ground, and either the fragments were buried immediately with other ejecta materials or the tektite mass penetrated into the ground covered by unconsolidated ejecta deposit and fragmented within the ejecta. In either case, the fragments were preserved as a cluster. Thus, the MN tektite fragments in the upper part of Unit 2 ("laterite" layer) at the HO06 section are considered as in primary position. Fiske et al. (1996) considered that layered tektites found at the top of Unit 2 at the Huai Om and Huai Sai sections to be reworked because, in their opinion, the top of Unit 2 represents a paleo-erosional surface. However, the fact that MN tektite fragments are found not at the top of the "laterite" layer but within the "laterite" layer at the HO06 section does not support this interpretation. Also, there was no evidence of erosion at the top of Unit 2 at the nearby Huai Om section (Tada et al. 2019) as well as several other sections in the region. Furthermore, our field observation of the "laterite" layer in other localities (for example, an active sand pit at Noen Sa-nga in Chaiyaphum province) suggests that laterization (precipitation of iron hydroxides) of this layer can occur within a few years after road cuts and pit walls were formed, indicating that the hard-cemented appearance of the "laterite" layer was not formed as an erosional pavement before the impact, but formed on the outcrop surface by recent ferricretization (Fig. S2). Koeberl and Glass (2000) and Keates (2000) pointed out that the Australasian tektites in Australia generally are found in deposits younger than the age of the impact, and interpreted by analogy that the tektites in Indochina may be of similar reworked origin. However, this analogy is not based on observational evidence. It should also be considered that dating of Quaternary sediments in Indochina is replete with methodological difficulties that may result in young ages being reported for strata that are considerably older (Carling et al. 2020).
The in situ occurrence of the MN tektite fragments in Unit 2 at the HO06 section supports the idea that the Quaternary depositional sequence of Units 1-3 in this region is an ejecta deposit of the Australasian tektite event based on the finding of shocked quartz from Units 1-3 at Huai Om section (Tada et al. 2019). The fact that Tada et al. Progress in Earth and Planetary Science (2020)  both the MN and splash-form tektites generally were found in the upper part of or at the top of the "laterite" layer at sites in the wide area of eastern Indochina (Table 1, Fig. 1) further supports the idea that the Australasian tektites found from the "laterite" layer were deposited in situ as an ejecta.

Conclusions
We described in detail the occurrence of a cluster of MN tektite fragments found at the HO06 section, Ubon Ratchathani province, northeastern Thailand. At least 331 fragments of MN tektite with a total weight of 713 g were concentrated in a small (40 × 30 cm) area within the upper part of a sandy gravel layer corresponding to the "laterite" layer. The occurrence as a cluster, the very angular shapes and the very poorly sorted nature of the fragments, the restoration of larger tektite fragments into one ellipsoidal MN tektite mass, and the similar chemical composition of the fragments suggest that these MN tektite fragments were not transported in long distances but rather fragmented in situ at the landing from a ballistic trajectory. This conclusion is contrary to the previous interpretation that similar tektite fragments were reworked on the upper surface of the "laterite" layer which was interpreted as the paleoerosional surface (Fiske et al. 1996). The size distribution of the MN tektite fragments is bifractal following two power laws in the range from 10 to 26 mm and from 26 to 37 mm in r, respectively, with Ds of 2.2 and 7.5. The high Ds value for the coarse fraction of the tektite fragments is larger than the range of Ds previously reported for rock fragments generated by rockfalls and rock avalanches and similar to Ds for the coarser fraction fragments generated by hyperspeed impact experiments, suggesting that the tektite fragments were formed through intense fragmentation by a relatively high energetic process at the landing on the ground.