Tanis (fossil site)

Last updated

Tanis is a paleontological site in southwestern North Dakota, United States. It is part of the heavily studied Hell Creek Formation, a geological region renowned for many significant fossil discoveries from the Upper Cretaceous and lower Paleocene. Uniquely, Tanis appears to record in detail, extensive evidence of the direct effects of the giant Chicxulub asteroid impact which struck the Gulf of Mexico 66.043 million years ago, and wiped out all non-avian dinosaurs and many other species (the so-called "K-Pg" or "K-T" extinction). The extinction event caused by this impact began the Cenozoic, in which mammals—including humans—eventually came to dominate life on Earth.

Contents

Discoveries

Various fossils from the Tanis site Goddard Scientific Colloquium, Tanis fossils.jpg
Various fossils from the Tanis site

The site was originally discovered in 2008 by University of North Georgia Professor Steve Nicklas and field paleontologist Rob Sula. Their team successfully removed fossil field jackets that contained articulated sturgeons, paddlefish, and bowfins. These fossils were delivered for research to the Field Museum of Natural History in Chicago. Recognizing the unique nature of the site, Nicklas and Sula brought in Robert DePalma, a University of Kansas graduate student, to perform additional excavations. The site was systematically excavated by Robert DePalma over several years beginning in 2012, working in near-total secrecy. [1] :pg.11 Key findings were presented in two conference papers in October 2017. [2] [3] The full paper introducing Tanis was widely covered in worldwide media on 29 March 2019, in advance of its official publication three days later. The co-authors included Walter Alvarez and Jan Smit, both renowned experts on the K-Pg impact and extinction.

At Tanis, unlike any other known Lagerstätte site, it appears specific circumstances allowed for the preservation of exquisite, moment-by-moment details caused by the impact event. These include finds which allow examination of the direct effects of the impact on plants and animals alive at the time of the large impact some 3,000 km (1,900 mi) distant. The events at Tanis occurred too soon after impact to be caused by the megatsunamis expected from any large impact near large bodies of water. Instead, much faster seismic waves from the magnitude 10 – 11.5 earthquakes [1] :p.8 probably reached the Hell Creek area as soon as ten minutes after the impact, creating seiche waves between 10–100 m (33–328 ft) high in the Western Interior Seaway. [1] :p.8 The site formed part of a bend in an ancient river on the westward shore of the seaway, [1] :p.8192 [4] :pp.5,6,23 and was flooded with great force by these waves, which carried sea, land, freshwater animals and plants, and other debris several miles inland. The seiche waves exposed and covered the site twice, as millions of tiny microtektite droplets and debris from the impact were arriving on ballistic trajectories from their source in what is now the Yucatán Peninsula.

Reported findings include:

Analysis of the fish skeletons found them to be in the spring phase of their annual cyclical changes, implying that the impact had occurred in spring. [9] [10]

The hundreds of fish remains are distributed by size, and generally show evidence of tetany (a body posture related to suffocation in fish), suggesting the suffocation of an entire population. Fragile remains spanning the layers of debris show the site was laid down in a single brief event.

The exceptional nature of the findings and conclusions led some scientists to await further scrutiny before agreeing that the discoveries at Tanis had been correctly understood. [11] The site continues to be explored.

Background

The K-Pg extinction event

North America laea relief location map with borders.jpg
Red pog.svg
Chicxulub crater
Red pog.svg
Tanis (approx.)
North america 65mya.png
Red pog.svg
Chicxulub crater
Red pog.svg
Tanis (approx.)
Location of Tanis and of the Chicxulub crater
Left: present day, Right: at impact 66 million years ago
K-Pg boundary sample from Wyoming. The intermediate claystone layer contains 1000 times more iridium than the upper and lower layers (San Diego Natural History Museum). K-T-boundary.JPG
K-Pg boundary sample from Wyoming. The intermediate claystone layer contains 1000 times more iridium than the upper and lower layers (San Diego Natural History Museum).

The Cretaceous–Paleogene ("K-Pg" or "K-T") extinction event around 66 million years ago wiped out all non-avian dinosaurs and many other species. Proposed by Luis and Walter Alvarez, it is now widely accepted that the extinction was caused by a huge asteroid or bolide that impacted Earth in the shallow seas of the Gulf of Mexico, leaving behind the Chicxulub crater. [12] [13] The impactor tore through the Earth's crust, creating huge earthquakes, giant waves, and a crater 180 kilometers (112 mi) wide, and blasted aloft trillions of tons of dust, debris, and climate-changing sulfates from the gypsum seabed, and it may have created firestorms worldwide. With the exception of some ectothermic species such as the ancestors of the modern leatherback sea turtle and crocodiles, no tetrapods weighing more than 25 kg (55 lb) survived. [14] It marked the end of the Cretaceous period and the Mesozoic Era, opening the Cenozoic Era that continues today.

However, because it is rare in any case for animals and plants to be fossilized, the fossil record leaves some major questions unanswered. One of these is whether dinosaurs were already declining at the time of the event due to ongoing volcanic climate change. Also, there is little evidence on the detailed effects of the event on Earth and its biosphere. No fossil beds were yet known that could clearly show the details that might resolve these questions. There is considerable detail for times greater than hundreds of thousands of years either side of the event, and for certain kinds of change on either side of the K-Pg boundary layer. But relatively little fossil evidence is available from times nearer the crucial event, a difficulty known as the "Three metre problem".

Hell Creek Formation

The Hell Creek Formation is a well-known and much-studied fossil-bearing formation (geological region) of mostly Upper Cretaceous and some lower Paleocene rock, that stretches across portions of Montana, North Dakota, South Dakota, and Wyoming in North America. The formation is named for early studies at Hell Creek, located near Jordan, Montana, and it was designated as a National Natural Landmark in 1966. [15]

The formation contains a series of fresh and brackish-water clays, mudstones, and sandstones deposited during the Maastrichtian and Danian (respectively, the end of the Cretaceous and the beginning of the Paleogene periods) by fluvial activity in fluctuating river channels and deltas and very occasional peaty swamp deposits along the low-lying eastern continental margin fronting the late Cretaceous Western Interior Seaway. The iridium-enriched Cretaceous–Paleogene boundary, which separates the Cretaceous from the Cenozoic, is distinctly visible as a discontinuous thin marker above and occasionally within the formation. Numerous famous fossils of plants and animals, including many types of dinosaur fossils, have been discovered there.[ citation needed ]

At the time of the Chicxulub impact, the present-day North American continent was still forming. Most of central North America had recently been a large shallow seaway, called the Western Interior Seaway (also known as the North American Sea or the Western Interior Sea), and parts were still submerged. This had initially been a seaway between separate continents, but it had narrowed in the late Cretaceous to become, in effect, a large inland extension to the Gulf of Mexico. The Hell Creek Formation was at this time very low-lying or partly submerged land at the northern end of the seaway, and the Chicxulub impact occurred in the shallow seas at the southern end, approximately 3,050 km (1,900 mi) from the site. [1] :p.8

Although Tanis and Chicxulub were connected by the remaining Interior Seaway, the massive water waves from the impact area were probably not responsible for the deposits at Tanis. Any water-borne waves would have arrived between 18 and 26 hours later, [1] :p.24 long after the microtektites had already fallen back to earth, and far too late to leave the geological record found at the site. It is not even clear whether the massive waves were able to traverse the entire Interior Seaway. [1] :p.8 Instead, the initial papers on Tanis conclude that much faster earthquake waves, the primary waves travelling through rock at about 5 km/s (11,000 mph), [1] :p.8 probably reached Hell Creek within six minutes, and quickly caused massive water surges known as seiches in the shallow waters close to Tanis. [1] :p.8 Seiche waves often occur shortly after significant earthquakes, even thousands of miles away, and can be sudden and violent. Some recent examples include the 1964 Alaskan earthquake (seiches in Puerto Rico), [16] the 1950 Assam-Tibet earthquake (India/China) (seiches in England and Norway), the 2010 Chile earthquake (seiches in Louisiana). Notably, the powerful magnitude 9.0 – 9.1 Tōhoku earthquake in 2011, slower secondary waves traveled over 8,000 km (5,000 mi) in less than 30 minutes to cause seiches around 1.5–1.8 m (4.9–5.9 ft) high in Norway. [17] [1] :p.8

The Chicxulub impact is believed to have triggered earthquakes estimated at magnitude 10 – 11.5, [1] :p.8 releasing up to 4000 times the energy of the Tohoku quake. Note 1 Co-author Mark Richards, a professor of earth sciences focusing on dynamic earth crust processes, [18] suggests that the resulting seiche waves would have been approximately 10–100 m (33–328 ft) high in the Western Interior Seaway near Tanis [1] :p.8 and credibly, could have created the 10 – 11 m (33 – 36 feet) high water movements evidenced inland at the site; the time taken by the seismic waves to reach the region and cause earthquakes almost exactly matched the flight time of the microtektites found at the site. [19] This would resolve conflicting evidence that huge water movements had occurred in the Hell Creek region near Tanis much less than an hour after impact, although the first megatsunamis from the impact zone could not have arrived at the site for almost a full day.

Site description

Site details are as follows: Note1

The Tanis river

The site was originally a point bar—a gently sloped crescent-shaped area of deposit that accumulates on the inside bend of streams and rivers below the slip-off slope. Point bars are common in mature or meandering streams. Both the site and the river are called Tanis.

From the size of the deposits beneath the flood debris, the Tanis River was a "deep and large" river with a point bar that was towards the larger size found in Hell's Creek, suggesting a river tens or hundreds of meters wide. [1] :p.8192 The river flowed eastward [1] :p.8192 from an inland area to the west, and the site itself was in an ancient river valley close to the western shore of the Interior Seaway. [1] :Fig.1 and p.9181-8192 Although other flooding is evidenced in Hells Creek, the Tanis deposit does not appear to relate to any other known marine transgression (inland shoreline movement). [1] :p.8193

Characteristics of the site include: [1] :Fig.1 and p.9181-8193

  • "the fluctuating, reticulated terminal-Cretaceous shoreline was not far away from the Tanis region"
  • "The Event Deposit is a 1.3-m-thick bed that shows an overall grading upward from coarse sand to fine silt/clay and is associated with a deeply incised, large meandering river ... [and] sharply overlies the aggrading surface of a point bar..."
  • "the point bar exhibits ~10.5 m of isochronous elevation change along its inclined surface and its width extends <50 m perpendicular to (ancient) flow direction. These dimensions are in the upper size range for point bars in the Hell Creek Formation and compare favorably with ... modern rivers with large channels that are tens to hundreds of meters wide"
  • "[The Event flood deposits are] indicative of a westward or inland flow direction that is opposite of the natural (ancient) current of the ... Tanis River"
  • "[The] Event Deposit is restricted to (an ancient) river valley and is conspicuously absent from the adjacent floodplains."
  • "Tanis exhibits a depositional scenario that was unusual in being highly conducive to exceptional (largely three dimensional) preservation of many articulated carcasses (Konservat-Lagerstätte). Such Konservat-Lagerstätten are rare ... because they require special depositional circumstances. Tanis is the only known site in the Hell Creek Formation where such conditions were met, [so] the deposit attests to the exceptional nature of the [Event]. The findings each preclude correlation with either the Cantapeta or Breien marine incursions (inland-directed floodings) ... the Tanis Event Deposit cannot be correlated with the known Hell Creek marine transgressions."
The event deposit

The deposit itself is about 1.3m thick, sharply overlaying the point bar, in a drape-like manner. It comprises two layers with sand and silt grading (coarse sands at the bottom, finer silt/clay particles at the top). It can be divided into two layers, a bottom layer about 0.5m thick ("unit 1"), and a top layer about 0.8m thick (unit 2), capped by a 1 – 2 cm layer of impactite tonstein that is indistinguishable from other dual layered KPg impact ejection materials found in Hells Creek, and finally a layer around 6 cm thick of plant remains. The excavated pointbar and event deposits show that the point bar had been exposed to the air for a considerable time, with evidence of habitation and filled burrows, before an abrupt, turbulent, high energy event filled these burrows and laid down the deposits. The event included waves with at least 10 meters run-up height (the vertical distance a wave travels after it reaches land).

Other media

A BBC documentary on Tanis, titled Dinosaurs: The Final Day , with Sir David Attenborough, was broadcast on 15 April 2022. This program was also aired as "Dinosaur Apocalypse: The Last Day" on PBS Nova starting 11 May 2022. [20] [21]

Notes

^Note 1 This section is drawn from the original 2019 paper [1] and its supplementary materials, [4] which describe the site in detail. Page numbers in this section refer to those papers.

Related Research Articles

<span class="mw-page-title-main">Deccan Traps</span> Large igneous province in India

The Deccan Traps is a large igneous province of west-central India. It is one of the largest volcanic features on Earth, taking the form of a large shield volcano. It consists of numerous layers of solidified flood basalt that together are more than about 2,000 metres (6,600 ft) thick, cover an area of about 500,000 square kilometres (200,000 sq mi), and have a volume of about 1,000,000 cubic kilometres (200,000 cu mi). Originally, the Deccan Traps may have covered about 1,500,000 square kilometres (600,000 sq mi), with a correspondingly larger original volume. This volume overlies the Archean age Indian Shield, which is likely the lithology the province passed through during eruption. The province is commonly divided into four subprovinces: the main Deccan, the Malwa Plateau, the Mandla Lobe, and the Saurashtran Plateau.

<span class="mw-page-title-main">Chicxulub crater</span> Prehistoric impact crater in Mexico

The Chicxulub crater is an impact crater buried underneath the Yucatán Peninsula in Mexico. Its center is offshore, but the crater is named after the onshore community of Chicxulub Pueblo. It was formed slightly over 66 million years ago when a large asteroid, about ten kilometers in diameter, struck Earth. The crater is estimated to be 200 kilometers in diameter and 20 kilometers in depth. It is the second largest confirmed impact structure on Earth, and the only one whose peak ring is intact and directly accessible for scientific research.

<span class="mw-page-title-main">Impact winter</span> Hypothesized climate effects due to an asteroid or comet impact on Earth

An impact winter is a hypothesized period of prolonged cold weather due to the impact of a large asteroid or comet on the Earth's surface. If an asteroid were to strike land or a shallow body of water, it would eject an enormous amount of dust, ash, and other material into the atmosphere, blocking the radiation from the Sun. This would cause the global temperature to decrease drastically. If an asteroid or comet with the diameter of about 5 km (3.1 mi) or more were to hit in a large deep body of water or explode before hitting the surface, there would still be an enormous amount of debris ejected into the atmosphere. It has been proposed that an impact winter could lead to mass extinction, wiping out many of the world's existing species. The Cretaceous–Paleogene extinction event probably involved an impact winter, and led to mass extinction of most tetrapods weighing more than 25 kilograms.

In science, an experimentum crucis is an experiment capable of decisively determining whether or not a particular hypothesis or theory is superior to all other hypotheses or theories whose acceptance is currently widespread in the scientific community. In particular, such an experiment must typically be able to produce a result that rules out all other hypotheses or theories if true, thereby demonstrating that under the conditions of the experiment, those hypotheses and theories are proven false but the experimenter's hypothesis is not ruled out.

The Late Cretaceous is the younger of two epochs into which the Cretaceous Period is divided in the geologic time scale. Rock strata from this epoch form the Upper Cretaceous Series. The Cretaceous is named after creta, the Latin word for the white limestone known as chalk. The chalk of northern France and the white cliffs of south-eastern England date from the Cretaceous Period.

<span class="mw-page-title-main">Alvarez hypothesis</span> Asteroid impact hypothesis as cause of the Cretaceous–Paleogene extinction

The Alvarez hypothesis posits that the mass extinction of the non-avian dinosaurs and many other living things during the Cretaceous–Paleogene extinction event was caused by the impact of a large asteroid on the Earth. Prior to 2013, it was commonly cited as having happened about 65 million years ago, but Renne and colleagues (2013) gave an updated value of 66 million years. Evidence indicates that the asteroid fell in the Yucatán Peninsula, at Chicxulub, Mexico. The hypothesis is named after the father-and-son team of scientists Luis and Walter Alvarez, who first suggested it in 1980. Shortly afterwards, and independently, the same was suggested by Dutch paleontologist Jan Smit.

<span class="mw-page-title-main">Hell Creek Formation</span> Geological formation in the United States

The Hell Creek Formation is an intensively studied division of mostly Upper Cretaceous and some lower Paleocene rocks in North America, named for exposures studied along Hell Creek, near Jordan, Montana. The formation stretches over portions of Montana, North Dakota, South Dakota, and Wyoming. In Montana, the Hell Creek Formation overlies the Fox Hills Formation. The site of Pompeys Pillar National Monument is a small isolated section of the Hell Creek Formation. In 1966, the Hell Creek Fossil Area was designated as a National Natural Landmark by the National Park Service.

<span class="mw-page-title-main">Lance Formation</span> Geological formation in the United States

The Lance (Creek) Formation is a division of Late Cretaceous rocks in the western United States. Named after Lance Creek, Wyoming, the microvertebrate fossils and dinosaurs represent important components of the latest Mesozoic vertebrate faunas. The Lance Formation is Late Maastrichtian in age, and shares much fauna with the Hell Creek Formation of Montana and North Dakota, the Frenchman Formation of southwest Saskatchewan, and the lower part of the Scollard Formation of Alberta.

<span class="mw-page-title-main">Dakota Formation</span> Rock units in midwestern North America

The Dakota is a sedimentary geologic unit name of formation and group rank in Midwestern North America. The Dakota units are generally composed of sandstones, mudstones, clays, and shales deposited in the Mid-Cretaceous opening of the Western Interior Seaway. The usage of the name Dakota for this particular Albian-Cenomanian strata is exceptionally widespread; from British Columbia and Alberta to Montana and Wisconsin to Colorado and Kansas to Utah and Arizona. It is famous for producing massive colorful rock formations in the Rocky Mountains and the Great Plains of the United States, and for preserving both dinosaur footprints and early deciduous tree leaves.

<span class="mw-page-title-main">Cretaceous–Paleogene boundary</span> Geological formation between time periods

The Cretaceous–Paleogene (K–Pg) boundary, formerly known as the Cretaceous–Tertiary (K–T) boundary, is a geological signature, usually a thin band of rock containing much more iridium than other bands. The K–Pg boundary marks the end of the Cretaceous Period, the last period of the Mesozoic Era, and marks the beginning of the Paleogene Period, the first period of the Cenozoic Era. Its age is usually estimated at 66 million years, with radiometric dating yielding a more precise age of 66.043 ± 0.011 Ma.

<span class="mw-page-title-main">Dinosaur Ridge</span> Natural heritage site in Colorado, United States

Dinosaur Ridge is a segment of the Dakota Hogback in the Morrison Fossil Area National Natural Landmark located in Jefferson County, Colorado, near the town of Morrison and just west of Denver.

This is an overview of the fossil flora and fauna of the Maastrichtian-Danian Hell Creek Formation.

<span class="mw-page-title-main">Tropic Shale</span>

The Tropic Shale is a Mesozoic geologic formation. Dinosaur remains are among the fossils that have been recovered from the formation, including Nothronychus graffami. The Tropic Shale is a stratigraphic unit of the Kaiparowits Plateau of south central Utah. The Tropic Shale was first named in 1931 after the town of Tropic where the Type section is located. The Tropic Shale outcrops in Kane and Garfield counties, with large sections of exposure found in the Grand Staircase–Escalante National Monument.

<span class="mw-page-title-main">Paleontology in Iowa</span>

Paleontology in Iowa refers to paleontological research occurring within or conducted by people from the U.S. state of Iowa. The paleozoic fossil record of Iowa spans from the Cambrian to Mississippian. During the early Paleozoic Iowa was covered by a shallow sea that would later be home to creatures like brachiopods, bryozoans, cephalopods, corals, fishes, and trilobites. Later in the Paleozoic, this sea left the state, but a new one covered Iowa during the early Mesozoic. As this sea began to withdraw a new subtropical coastal plain environment which was home to duck-billed dinosaurs spread across the state. Later this plain was submerged by the rise of the Western Interior Seaway, where plesiosaurs lived. The early Cenozoic is missing from the local rock record, but during the Ice Age evidence indicates that glaciers entered the state, which was home to mammoths and mastodons.

The climate across the Cretaceous–Paleogene boundary is very important to geologic time as it marks a catastrophic global extinction event. Numerous theories have been proposed as to why this extinction event happened including an asteroid known as the Chicxulub asteroid, volcanism, or sea level changes. While the mass extinction is well documented, there is much debate about the immediate and long-term climatic and environmental changes caused by the event. The terrestrial climates at this time are poorly known, which limits the understanding of environmentally driven changes in biodiversity that occurred before the Chicxulub crater impact. Oxygen isotopes across the K–T boundary suggest that oceanic temperatures fluctuated in the Late Cretaceous and through the boundary itself. Carbon isotope measurements of benthic foraminifera at the K–T boundary suggest rapid, repeated fluctuations in oceanic productivity in the 3 million years before the final extinction, and that productivity and ocean circulation ended abruptly for at least tens of thousands of years just after the boundary, indicating devastation of terrestrial and marine ecosystems. Some researchers suggest that climate change is the main connection between the impact and the extinction. The impact perturbed the climate system with long-term effects that were much worse than the immediate, direct consequences of the impact.

<span class="mw-page-title-main">Cretaceous–Paleogene extinction event</span> Mass extinction event about 66 million years ago

The Cretaceous–Paleogene (K–Pg) extinction event, also known as the Cretaceous–Tertiary(K–T)extinction, was a sudden mass extinction of three-quarters of the plant and animal species on Earth, approximately 66 million years ago. The event caused the extinction of all non-avian dinosaurs. Most other tetrapods weighing more than 25 kilograms also became extinct, with the exception of some ectothermic species such as sea turtles and crocodilians. It marked the end of the Cretaceous period, and with it the Mesozoic era, while heralding the beginning of the Cenozoic era, which continues to this day.

<span class="mw-page-title-main">Timeline of Cretaceous–Paleogene extinction event research</span> Research timeline

Since the 19th century, a significant amount of research has been conducted on the Cretaceous–Paleogene extinction event, the mass extinction that ended the dinosaur-dominated Mesozoic Era and set the stage for the Age of Mammals, or Cenozoic Era. A chronology of this research is presented here.

<span class="mw-page-title-main">Geology of South Dakota</span>

The geology of South Dakota began to form more than 2.5 billion years ago in the Archean eon of the Precambrian. Igneous crystalline basement rock continued to emplace through the Proterozoic, interspersed with sediments and volcanic materials. Large limestone and shale deposits formed during the Paleozoic, during prevalent shallow marine conditions, followed by red beds during terrestrial conditions in the Triassic. The Western Interior Seaway flooded the region, creating vast shale, chalk and coal beds in the Cretaceous as the Laramide orogeny began to form the Rocky Mountains. The Black Hills were uplifted in the early Cenozoic, followed by long-running periods of erosion, sediment deposition and volcanic ash fall, forming the Badlands and storing marine and mammal fossils. Much of the state's landscape was reworked during several phases of glaciation in the Pleistocene. South Dakota has extensive mineral resources in the Black Hills and some oil and gas extraction in the Williston Basin. The Homestake Mine, active until 2002, was a major gold mine that reached up to 8000 feet underground and is now used for dark matter and neutrino research.

Alan Russell Hildebrand is a planetary scientist and Associate Professor in the Department of Geoscience at the University of Calgary. He has specialized in the study of asteroid impact cratering, fireballs and meteorite recovery. His work has shed light on the extinction event caused by the Chicxulub asteroid at the end of the Cretaceous period. Hildebrand is one of the leaders of the Prairie Meteorite Network search project.

Dinosaurs: The Final Day with David Attenborough is a British documentary programme that aired on BBC One on 15 April 2022. Presented by David Attenborough, the documentary follows the final days of non-avian dinosaurs through the Cretaceous–Paleogene extinction event, similar to Apple TV+’s Prehistoric Planet. Like that series, the programme's creatures were also made with computer-generated imagery.

References

  1. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 DePalma, Robert A.; Smit, Jan; Burnham, David A.; Kuiper, Klaudia; Manning, Phillip L.; Oleinik, Anton; Larson, Peter; Maurrasse, Florentin J.; Vellekoop, Johan; Richards, Mark A.; Gurche, Loren; Alvarez, Walter (23 April 2019). "A seismically induced onshore surge deposit at the KPg boundary, North Dakota". Proceedings of the National Academy of Sciences. 116 (17): 8190–8199. Bibcode:2019PNAS..116.8190D. doi: 10.1073/pnas.1817407116 . PMC   6486721 . PMID   30936306.
  2. DePalma, R. et al. (2017) Life after impact: A remarkable mammal burrow from the Chicxulub aftermath in the Hell Creek Formation, North Dakota Archived 3 June 2018 at the Wayback Machine Paper No. 113-16, presented 23 October 2017 at the GSA Annual Meeting, Seattle, Washington, USA.
  3. Smit, J., et al. (2017) Tanis, a mixed marine-continental event deposit at the KPG Boundary in North Dakota caused by a seiche triggered by seismic waves of the Chicxulub Impact Archived 2 June 2018 at the Wayback Machine Paper No. 113-15, presented 23 October 2017 at the GSA Annual Meeting, Seattle, Washington, USA.
  4. 1 2 Supplementary Information for A seismically induced onshore surge deposit at the KPg boundary, North Dakota (2019) Archived 8 April 2022 at the Wayback Machine - supporting and supplementary material, and further analysis for the main 2019 paper]
  5. Hilton, Eric J.; During, Melanie A.D.; Grande, Lance; Ahlberg, Per E. (11 April 2023). "New paddlefishes (Acipenseriformes, Polyodontidae) from the Late Cretaceous Tanis Site of the Hell Creek Formation in North Dakota, USA". Journal of Paleontology . 97 (3): 675–692. doi: 10.1017/jpa.2023.19 .
  6. Hond, Bas den (23 October 2021). "Asteroid impact in vivid detail". New Scientist. 252 (3357): 13. Bibcode:2021NewSc.252...13H. doi:10.1016/S0262-4079(21)01869-8. S2CID   239954523.
  7. "A Turtle from the Tanis KPG Mass-Death Assemblage: Further Evidence for Circum-Riparian Disruption by a Massive Chicxulub Impact-Triggered Surge". Geological Society of America Abstracts with Programs. 53 (6). 10 October 2021. Archived from the original on 29 December 2021. Retrieved 29 December 2021.
  8. DePalma, Robert (6 April 2022). "A Blast from the Past: Geochemical Identity of the Chicxulub Bolide and Immediate Effects of the Impact, recorded at Tanis, North Dakota". NASA's Goddard Scientific Colloquium. Retrieved 10 April 2022.
  9. During, Melanie A. D.; Smit, Jan; Voeten, Dennis F. A. E.; Berruyer, Camille; Tafforeau, Paul; Sanchez, Sophie; Stein, Koen H. W.; Verdegaal-Warmerdam, Suzan J. A.; van der Lubbe, Jeroen H. J. L. (23 February 2022). "The Mesozoic terminated in boreal spring". Nature. 603 (7899): 91–94. Bibcode:2022Natur.603...91D. doi:10.1038/s41586-022-04446-1. PMC   8891016 . PMID   35197634.
  10. Price, Michael (6 December 2022). "Paleontologist accused of faking data in dino-killing asteroid paper". www.science.org. Retrieved 7 December 2022.
  11. Barras, Colin (1 April 2019). "Astonishment, skepticism greet fossils claimed to record dinosaur-killing asteroid impact". Science. doi:10.1126/science.aax5400. S2CID   193142856.
  12. "International Consensus — Link Between Asteroid Impact and Mass Extinction Is Rock Solid". www.lpi.usra.edu. Archived from the original on 16 March 2018. Retrieved 28 October 2015.
  13. Schulte, Peter; Alegret, Laia; Arenillas, Ignacio; Arz, José A.; Barton, Penny J.; Bown, Paul R.; Bralower, Timothy J.; Christeson, Gail L.; Claeys, Philippe; Cockell, Charles S.; Collins, Gareth S.; Deutsch, Alexander; Goldin, Tamara J.; Goto, Kazuhisa; Grajales-Nishimura, José M.; Grieve, Richard A. F.; Gulick, Sean P. S.; Johnson, Kirk R.; Kiessling, Wolfgang; Koeberl, Christian; Kring, David A.; MacLeod, Kenneth G.; Matsui, Takafumi; Melosh, Jay; Montanari, Alessandro; Morgan, Joanna V.; Neal, Clive R.; Nichols, Douglas J.; Norris, Richard D.; Pierazzo, Elisabetta; Ravizza, Greg; Rebolledo-Vieyra, Mario; Reimold, Wolf Uwe; Robin, Eric; Salge, Tobias; Speijer, Robert P.; Sweet, Arthur R.; Urrutia-Fucugauchi, Jaime; Vajda, Vivi; Whalen, Michael T.; Willumsen, Pi S. (5 March 2010). "The Chicxulub Asteroid Impact and Mass Extinction at the Cretaceous-Paleogene Boundary". Science. 327 (5970): 1214–1218. Bibcode:2010Sci...327.1214S. doi:10.1126/science.1177265. PMID   20203042. S2CID   2659741.
  14. Muench, David; Muench, Marc; Gilders, Michelle A. (2000). Primal Forces. Portland: Graphic Arts Center Publishing. p. 20. ISBN   978-1-55868-522-2.
  15. "National Natural Landmarks – National Natural Landmarks (U.S. National Park Service)". www.nps.gov. Archived from the original on 9 May 2021. Retrieved 22 March 2019. Year designated: 1966
  16. "Seiche". School of Ocean and Earth Science and Technology, University of Hawaii at Manoa. 19 May 1996. Archived from the original on 26 January 2019. Retrieved 10 April 2019.
  17. Fjorden svinga av skjelvet Archived 18 March 2011 at the Wayback Machine Retrieved on 17 March 2011.
  18. "Mark Richards academic profile". Earth and Planetary Science, University of California, Berkeley. 3 April 2019. Archived from the original on 3 April 2019. Retrieved 9 April 2019.
  19. "Fossil site is first ever to show deaths from mass extinction asteroid impact". Newatlas.com. 29 November 2017. Archived from the original on 5 April 2019. Retrieved 10 April 2019.
  20. "Tanis: Fossil of dinosaur killed in asteroid strike found, scientists claim". BBC News. 6 April 2022. Archived from the original on 7 April 2022. Retrieved 7 April 2022.
  21. Amos, Jonathan (24 February 2022). "'Dinosaur asteroid' wrought springtime devastation". BBC News Online . Archived from the original on 4 April 2022. Retrieved 6 April 2022.
Supporting material and analysis for above paper (2019) - Public readable version, containing supplementary text, analysis, and data referred to in the main paper

46°01′18″N103°47′28″W / 46.0218°N 103.7910°W / 46.0218; -103.7910