History of the Earth

Giovanni ArduinoThe most recent 66 million years of earth history is the Cenozoic Era. Cenozoic comes from “cene” for “new” or “recent” plus “zoic” for “life,” in comparison to the Paleozoic, ancient life, and Mesozoic, middle life. The big subdivisions of earth history, the eras, came into common use about the start of the 19th Century. The first scheme, devised by Italian scientist Giovanni Arduino in the 1750s, subdivided the rocks into Primary, Secondary, and Tertiary, coinciding more or less with the Precambrian, Paleozoic, and Mesozoic and later rocks. The fourth grand division following the numerical scheme, Quaternary, was added in 1830 to account for the very recent glacial deposits found in Europe. As the terms Precambrian, Paleozoic, and Mesozoic came into use in the early 1800s, the Primary and Secondary names were abandoned, but Tertiary and Quaternary were retained as periods of the Cenozoic Era. It took a long time for geology to outgrow the early terminology – it wasn’t until 2004 that the Tertiary was officially abandoned by international agreement. And now, the Cenozoic is divided into three periods – the older Paleogene and the more recent Neogene, whose names mean “ancient things” and “new things,” respectively, plus the Quaternary, an anachronistic name still retained. The Quaternary includes the present day. Because the changes in nomenclature are so recent, I can guarantee that you’ll still find lots of references to the Tertiary, and I’ll probably use it too. I’ll talk a bit more about additional subdivisions of Cenozoic time tomorrow. Because the Cenozoic is so recent, the past 66 million years, we have a relatively good handle on it in terms of events, life, evolution, and timing, so it makes sense to have closely defined subdivisions. And because we do know so much about it, it also makes it a little harder for me to decide on which 31 topics to cover this month. But we’ll manage. I want to remind you again of the scale of our journey, and the fact that it’s not a proper scale. The entire Cenozoic, 66 million years, which we’ll cover this month, is less than 1.5% of all earth history. To do this at the correct scale, the entire Cenozoic would have to be squeezed into the last five days of December. —Richard I. Gibson Image of Arduino in public domain

The end of the Cretaceous – and the end of the Mesozoic Era – were marked by a mass extinction, one of the largest in earth history. Unlike some of the earlier extinctions, we pretty much have a smoking gun for this one: the impact of an asteroid in what is now northwestern Yucatan, Mexico.  Not that it was an easy sell. Since I was a grown-up geologist in the early 1980s when the team led by Luis Alvarez and his son Walter began to suggest the impact as the cause of the extinction, I remember some of the controversy. It was a radical idea; any kind of catastrophe flew in the face of the long-accepted idea of uniformitarianism, that changes on earth resulted from the application of slow, steady changes over long, long times. I’m really not sure why the idea that catastrophes DID happen was so hard to accept, but it was. The Alvarezes were ridiculed in some professional circles. But accumulating evidence really pretty rapidly, in just a few years, convinced I would say all but a few geoscientists of the validity of the impact as at least a major factor in the extinction.  Gravity map of Chixulub crater (source: NASA)The evidence includes a layer around the world right at the top of the Cretaceous, coinciding with the extinction, of iridium, an element that’s abundant in asteroids. Shocked quartz grains are present as well, and result from impacts. Rocks of the right age in Texas and elsewhere in the Gulf of Mexico and Caribbean region look like gigantic tsunami deposits. And finally, magnetic data being analyzed by geophysicist Glen Penfield for oil exploration in Yucatan defined a likely crater on the northwestern coast of the peninsula. It took a while for the age of the Chicxulub impact crater to be determined accurately, but now it is considered to have happened at 66.04 million years ago. It is within 33,000 years of the best estimate for the extinction event, so practically, the two are simultaneous. The Chixulub crater shows up nicely in gravity data too, and even today the cenotes, natural sinkholes scattered across Yucatan, follow the crater margin even though it is deep in the subsurface. The potential effects of such an impact can be estimated from the size of the crater and the impact angle. Vast quantities of dust, ash, and aerosols likely went into the atmosphere, creating toxicity as well as probably a nuclear winter; it’s been speculated that most of North America burned in an incendiary forest fire across the continent. The effects resulted in the destruction of about 75% of all species on earth. The most famous victims are the non-avian dinosaurs, all of which perished. All the ammonites died. The giant marine reptiles and the pterosaurs were gone. Pretty much every group, including things like mammals and birds that survived as a class, lost many members. Everything from plankton to plants to snakes and turtles suffered. Surviving birds and mammals did undergo a dramatic diversification and radiation soon after the extinction – a typical reaction, as the survivors adapt and expand into niches vacated by other animals. While it’s pretty much agreed that the impact was a major factor in the extinction that ended the Mesozoic, there’s still debate about whether it was the only factor. Other things were going on that might have had roles. We’ve talked several times in this series about massive volcanism as a possible factor in extinctions, especially the Siberian flood basalts at the end of the Permian. From about 68 to 66 million years ago in India, similar flood basalts erupted to create the Deccan Traps. Before the asteroid impact was known, the Deccan was usually seen as the gradual, 2-million-year cause of the extinction. There are some declines in diversity among several groups, including some dinosaurs, that may be related to an ongoing effect of the Deccan. The asteroid might have simply been an exclamation point on an already-in-progress extinction. Besides the Deccan volcanics, there were oth

A handful of people have asked about donations to be sponsors for the podcast. That’s really not on the list; the budget for the whole production is about $39- $35 for the digital voice recorder, plus $4 for replacement AAA batteries. I was trying to make it through the whole year on the first set of batteries, but the originals died the other day. Otherwise, there’s no cost other than my time. I hate commercial announcements enough, even on public broadcasting, that I’m not interested in accepting sponsors for this podcast. I’m not rich, but I can afford to do this, and it’s really a labor of love. Thanks for your support. Likewise, I’m not in it for the clicks. I’m glad to see my statistics showing 4,000 pageviews per month on the blog, and as near as I can tell, about 1,000 downloads a day of the podcast, but I’d keep doing it if those numbers were 100 people I don’t know. I don’t do much to promote the podcast other than getting it listed on iTunes and other providers, so it is what it is. Clearly a lot of people find it through search engines. Again, thanks for your support and interest. To repeat my disclaimer, I’m not an expert in everything – I like to think of myself as a geological generalist, although of course I do have specialties, strengths, ranging from kidney stone mineralogy to gravity and magnetics in oil exploration. Please take these podcasts or the blog as summaries of the topics. I try to be even handed and unbiased, but I don’t guarantee that. If something I talk about strikes your fancy, by all means, investigate more! There’s a vast amount of information out there on everything I talk about. Or feel free to ask me questions. I’m happy to say “I don’t know,” but like most geologists, that won’t stop me from expounding on something – but I’ll try to make it clear that I may be approaching the topic from a point of general knowledge but specific ignorance.  * * * So on to today’s Cretaceous topic – the Verkhoyansk Fold-Thrust Belt. We talked a lot about the collision on the west coast of North America that formed much of the basis for the modern geography of the Rocky Mountains, including such details as oil fields. Similar things were happening in other parts of the world during the Cretaceous too. The tectonic framework of far eastern Asia is really a mess. There were microcontinents, island arcs, entrapped oceanic crust, and more, all becoming amalgamated to what we think of today as the far eastern part of Eurasia. One aspect of it that is moderately well documented is the collision between a small, almost circular microcontinent called the Kolyma Block and the eastern side of the Siberian Craton. Tectonic Map of far eastern Siberia (Khain, 1973) The Siberian Craton is one of the really old, fundamental continental blocks, like the Superior Craton in North America or the Baltica Craton in Europe. By the Cretaceous, it was firmly attached to Europe and the Kazakhstan Craton, so the concept of Eurasia was a reasonable one at that time. The details were still in progress, especially on the eastern and southern margins of the young Eurasia. What I’m saying about this collision and fold belt is based in part on my own work on the magnetic map of the former Soviet Union. The Kolyma Block, that I’m calling a microcontinent, has a magnetic character that’s a lot like Kansas or Texas – magnetic character that says it’s probably Precambrian crust, but the Kolyma Block was a relatively small, independent block, not part of a major continental terrane until the Cretaceous. This eastern margin of Siberia was for millions of years a passive margin – like the Atlantic coast of North America today, with lots of various sedimentary units accumulating. The rocks are as old as Cambrian, but most of the sedimentary pile is Carboniferous to Jurassic in age. Beginning in late Jurassic time and continuing into the Cretaceous, the Kolyma block began to collide with Siberia, pushing the older passive-margin rocks agains

Besides Tyrannosaurus rex, the iconic dinosaur of the Cretaceous is probably Triceratops – or to be specific, Triceratops horridus to give the best known species its full name. Triceratops was a contemporary in time, the very late Cretaceous, 68 to 66 million years ago, and space, the margins of the Interior Seaway in western North America, with Tyrannosaurus. Tyrannosaurs were the principal predators threatening the herbivorous Triceratops. Triceratops, whose name means ‘three-horn-face,’ was a ceratopsian, a group that includes dozens of families. What they had in common was complex ornamentation on their skulls, ranging from ornate frills to horns to fancy spines. They also typically had beak-like mouths. Triceratops fossils were discovered near Denver, Colorado, in 1887. Paleontologist O.C. Marsh initially misidentified the age of the rocks it was from, and thought it was a Cenozoic mammal, but within a year additional specimens and more information led him to recognize its Cretaceous age and dinosaurian nature, and he named it Triceratops. The role of the frills and other complex ornamentation has been debated over time. Some researchers considered them to be aspects of temperature regulation, like the sail on the back of the Permian Dimetrodon, but this idea is not the favored one. Display – for defense, or for sexual competition or courtship, or all three – is I think the consensus explanation for the wide variety of distinctive appearances among ceratopsians. Support for the idea that the frills might be used in combat, either against predators like Tyrannosaurs, which are known to have fed on Triceratops, or in sexual combat, comes from the nature of the bony tissue in the frills. It’s a type that heals rapidly, helping seal wounds. Triceratops grew to 8 or 9 meters in length, 26 to 30 feet. Its skull was among the largest of any dinosaur, or any land animal, presumably big to support the complex bony ornamentation and horns. The earliest ceratopsians appeared in the Jurassic. They had pretty minimal skull decorations, and it was not until the early part of the Late Cretaceous that the first horned, frilled ceratopsians developed. Enough specimens have been found that we now see the evolutionary process that led to Triceratops as one that took at least a couple million years, as reported by researchers at Montana State University in June 2014. Ceratopsians comprise one of the major lineages of the dinosaurs. They’re not especially close to the Sauropods, but I’ll end this episode with a note about the Sauropods. Just recently, in 2011, the first discovery was announced of sauropod fossils from Antarctica, reported by a team of Argentinean scientists. This confirms the global distribution of the gigantic herbivorous Sauropods by Late Cretaceous time, at least. During the late Cretaceous, Antarctica was near the south pole, and except for an increasingly tenuous connection to Australia, it was isolated from the other continents. Dinosaurs truly were worldwide in their range. —Richard I. Gibson Links: Sauropod in Antarctica  Triceratops' horns developed over millions of years

The McMurray Formation is a package of Cretaceous rocks in northern Alberta and adjacent areas of Canada that was laid down in early Cretaceous time, so I should have talked about it earlier this month, but I didn’t.  The basin that the McMurray sediments accumulated in was an early aspect of the Cretaceous Interior Seaway that reached its height in Late Cretaceous time. The sea invaded from the north, the Arctic, so the transgression of the sea affected Canada earlier than it did the western United States. The McMurray environment was similar to that of the shores of the later Cretaceous Interior Seaway – rivers, deltas, estuaries, and coastal plains. Settings like that typically give rise to interbedded and alternating sands in river channels and beaches, silts in the more distant parts of deltas and estuaries, and muds in overbank deposits, flood plains, and in the parts of the coastal sea even more distant from shore.  What makes the McMurray special is that it holds one of the largest accumulations of hydrocarbons in the world – the Athabasca Tar Sands. You sometimes hear this called oil sands, but it really isn’t oil in the sense of liquid oil. It’s solid bitumen, tar, oil that has lost the volatile components that help make oil liquid. It’s called the Athabasca Tar Sands because the McMurray formation crops out in the drainage basin of the Athabasca River. Map by Norman Einstein, released to public domain. There’s an estimated 1.7 trillion barrels of hydrocarbon in place in these deposits, similar to or more than all the rest of the known conventional oil in the world. Only about 179 billion barrels is listed as economically producible – but that’s “only” about the same as all the oil in Saudi Arabia. This stuff, because it is solid, is a lot harder to produce. About half of production is mined, dug out of the outcrop, and the rest is produced using steam injection and other methods to essentially melt the material in the subsurface to liquefy it. All methods combined yield about 2.3 million barrels of oil per day – more than half of Canada’s total oil output. Canada is the #5 oil producer in the world, after the U.S., Russia, Saudi Arabia, and China, and Canada is the leading source of U.S. imports, at more than 3.5 million barrels per day – more than all OPEC nations combined. Canadian imports amount to more than one-third of all US imports, which totaled about 9.2 million barrels a day in September 2014, and Canadian imports made for about 19% of total US consumption, which is just over 19 million barrels a day. Canada projects that it may be able to double its production of oil from tar sands by 2020. Leaving apart the controversies over this production, I’m going to focus on the origin of the deposit. I used to think it was more or less just an oil reservoir at the surface with the volatiles gone, but it’s more complicated than that. First, there’s the question of the source rocks for the bitumen. The most common speculations for source rocks include marine Devonian carbonates or Triassic-Jurassic shales, or both. Those rocks are known to be the sources of conventional oil in the Western Canada Sedimentary Basin, but they may be inadequate to generate the volumes we see in the tar sands. It’s been suggested that they formed in place, from organic matter washed into the McMurray formation along with the sands and shales, or that it was derived from non-marine Jurassic and Lower Cretaceous coals. There’s also argument about the migration history – how the bitumen got there – ranging from in-place formation to migration from deep sources. The process was complicated by dissolution and collapse of salt-bearing horizons in the Devonian. Their collapse changed the topography of the surface the McMurray sands were deposited upon, so that some places had thicker sands than others, and were more favorable for the oil and bitumen to accumulate. Agreement is not unanimous, but I think there’s at least a slight pref

The Cretaceous Interior Seaway of western North America was a great abode for life, both in the waters and on the adjacent tropical or subtropical lands. You remember the chalk cliffs of Dover, England – the chalk that gave the name to the Cretaceous, which means “chalk-bearing”? The North American interior seaway also contained a lot of those microscopic coccolithophores whose shells accumulated to make chalk.  Probably the most famous example is the Niobrara Chalk, a prominent part of the Cretaceous stratigraphic section especially in Nebraska and Kansas which were under the waters of the seaway. Most of the fossils from the Niobrara are, as you’d expect, marine fossils – fish, turtles, plesiosaurs. But it also contains occasional land-dwelling dinosaurs, whose bodies must have been washed offshore, and there are winged vertebrates as well. Pteranodons, winged reptiles that are not dinosaurs, flew in the late Cretaceous skies above and near the western interior seaway and what is now the Gulf Coastal Plain around 85 million years ago. Despite their relatively short existence, probably not much more than two or three million years, they are well known because more than 1,200 specimens have been found, the most of any pterosaur. “Pteranodon” means “winged, toothless,” and they had typical wingspans of 6 meters, about 20 feet. Pteranodons shared the skies with birds, which were becoming much more diverse during the Cretaceous. Ichthyornis was a small toothed bird that probably occupied ecological niches similar to gulls. Many specimens of Ichthyornis have been found in the Niobrara Chalk. Its time range is about 95 to 85 million years ago, and it is interpreted to be of a bird lineage that was near that of modern birds, but it was probably not a direct ancestor to them. Its name means “fish-bird,” and it’s among the best-represented birds in the fossil record – but “well represented” probably means a few hundred specimens, not thousands.  Hesperornis fossil (Smithsonian) photo by Quadell, used under Creative Commons license.  Hesperornis, whose name means “western bird,” was a flightless bird – based on its size, its wings were useless for flight. It was most likely a penguin-like, or more accurately loon-like, fully aquatic bird, demonstrating that birds had evolved and adapted to the marine realm as early as 84 million years ago. Hesperornis was pretty big, about 6 feet or almost 2 meters long. Its fossils have been found in Russia and Europe as well as many places in the western North American Interior Seaway, so as a group it clearly had a wide range. Both Ichthyornis and Hesperornis were extinct well before the end of the Cretaceous, at about 85 and 78 million years ago, respectively. —Richard I. Gibson Ichthyornis Hesperornis Hesperornis fossil (Smithsonian) photo by Quadell, used under Creative Commons license. 

Obviously we can’t leave the Cretaceous without at least a mention of Tyrannosaurus rex. The tyrant lizard king – that’s what the name means – only lived during a relatively brief span of geologic time, a million years from 67 to 66 million years ago, just before the end of the Cretaceous. It was one of the largest land predators of all time, at 12 meters or 40 feet in length. Henry Fairfield Osborn described the species from specimens collected at Hell Creek, Montana, in 1902 and 1908. Since then fossils from more than 50 individuals have been found. There’s enough individual variation that there are also specimens originally assigned to other species that were reassigned to Tyrannosaurus rex after further study, but there are also other species within the overall group of tyrannosaurids. Photo of Sue, the most complete T. rex specimen known, in the Chicago Field Museum, by Connie Ma, used under Creative Commons license.   They were bipedal carnivores, and the debate continues over whether they were active predators, scavengers, or both. Most researchers today seem to agree that Tyrannosaurus rex was an opportunist that both scavenged and caught live prey. It had a really strong bite that would force its teeth – up to 12 inches long – into pretty much whatever it wanted to bite. Another current debate is whether T. rex was warm-blooded or cold-blooded. As near as I can tell, the jury is still out on that question. The Hell Creek Formation, the rocks in which many T. rex fossils have been found, was laid down on the margin of the Cretaceous Interior Seaway that we talked about a few days ago. The setting was one of coastal flood plains and deltas, with rivers and some swampy areas. The climate must have been subtropical or tropical and clearly supported a wide range of life. There were lush forests of angiosperms, conifers, gingkoes, and cycads. Besides the famous T. rex, the Hell Creek Formation contains mammals, birds, pterosaurs, lizards, snakes, turtles, crocodilians, and a wide range of dinosaurs large and small. The more marine sediments contain fish, plesiosaurs, ammonites, sharks and rays, and there were snails, oysters, and clams in the marine and fresh waters. Lots of life, a long, tall food chain with carnivores like Tyrannosaurus rex at or near the top. Tyrannosaurs only represent about 4% of the dinosaur fossils in the Hell Creek. The most numerous group were the Ceratopsians, horned dinosaurs, of which the most famous member is probably Triceratops, which we’ll talk about a little more in a few days. There is of course a vast amount of information readily available about Tyrannosaurus rex. I have links below to a video and a podcast, both with Tyrannosaur expert Dr. Thomas Holtz who is at the University of Maryland, for more information. —Richard I. Gibson Video: The Life and times of Tyrannosaurus rex with Thomas Holtz  Podcast link: New understanding  Photo of Sue, the most complete T. rex specimen known, in the Chicago Field Museum, by Connie Ma, used under Creative Commons license.    

Mammals diversified during the Cretaceous, so that by the end of the period, the two major modern groups, the placentals and the marsupials, were well established. Placental mammals include most modern types including rodents, primates – most every kind of mammal other than marsupials and the egg-laying monotremes, which are platypuses and spiny anteaters. The mutituberculates were rodent-like mammals that got started during the Jurassic, thrived in the Cretaceous and survived the end-Cretaceous extinction, only to disappear in the Oligocene about 30 million years ago. Their 120-million-year run is the longest of any mammal lineage, and their diversity is reflected in at least 200 different species. Their name comes from their teeth, which have rows of little points, or tubercules. Although they occupied rodent-like niches, including burrows and trees, and were superficially much like squirrels and rats and other rodents, they are classed taxonomically in their own order, and they have no modern descendents. It looks like the true rodents displaced them in the early part of the Cenozoic Era, which we’ll talk about next month.    Brian Switek has a post this week on a new Cretaceous mammal discovery, Vintana, a muskrat-like critter that lived in Madagascar a few million years after that island finally became separated from larger land masses. Madagascar had pulled away from Africa while it was still attached to India during the latter part of the Early Cretaceous epoch. India and Madagascar separated around 90 million years ago, and Vintana dates to about 70 million years ago, so it might be a reflection of evolution in the relative isolation of a small island continent. Check the Laelaps blog at phenomena.nationalgeogeographic.com for more information on this and many other fossil topics.  Repenomamus with dinosaur bones in stomach – photo by David Wong, used under Creative Commons license.   The common view of Cretaceous mammals living in fear of dinosaur predators, creeping through the underbrush at night, was turned topsy-turvy by the discovery of a meter-long mammal in China, called Repenomamus. One specimen was found with fragments of a juvenile herbivorous dinosaur in its stomach. We don’t know if it scavenged, or chased small dinosaurs down, or maybe it preyed on the young. But it did eat dinosaurs. At a meter long, three feet or so, Repenomamus is the largest known Mesozoic mammal. Most Cretaceous mammals were around 3 to 10 inches long. Many are known only from a single tooth or a few bones, so they are not really very well known. Some spectacular exceptions exist, including an early Cretaceous mammal fossil from China in which the 4-inch-long animal’s fur can be clearly seen. We’re coming up on the end of the Cretaceous in a week, and the last day of November will be devoted to the extinction event at the end of the period. I wanted to mention today some ideas that addresses the question of how mammals and birds survived the extinction event when, so far as we know, no dinosaurs did. One popular idea has been that birds and mammals in general were smaller in size than most dinosaurs, although there were a few exceptions at times. Smaller size would have allowed animals to maintain and regulate body temperature more easily, in the event of climatic extremes such as those that might have accompanied the end-Cretaceous extinction. And many mammals were burrowers, which would also afford protections from cold or other climate changes. Mammal and bird brains might have become complex enough by the end of the Cretaceous, and more complex than the non-avian dinosaurs, so that as individuals and as groups they were simply more adaptable to the challenging conditions during the extinction event. Some mammals and birds did die off at the end of the Cretaceous, so it was most definitely not a case of all mammals and birds good, all dinosaurs bad. The idea of long-term hibernation, say something li

The subduction that became quite active in the Jurassic and continued into the Cretaceous and eventually created the Sierra Nevada Batholith was probably related to the two styles of mountain building we have talked about recently, the Laramide and Sevier Orogenies. The subduction itself was also complicated. By Cretaceous time, some subduction was taking place much further east than the magmatic arc where the Sierra Nevada Mountains are today. It’s 750 kilometers, 450 miles, from Sacramento, California, to Boise, Idaho, but that’s about how far you have to go to find the continuation of the batholiths that resulted from Cretaceous subduction. In central Idaho, the granitic igneous rock is called the Idaho Batholith. It’s only about half as long as the Sierra Nevada Batholith – still huge, about 200 miles long, and generally it’s younger – formed about 100 to 54 million years ago, mostly Late Cretaceous, but some of it dates to the time a few million years after the Cretaceous ended. Geologic map (from USGS, National Atlas) with batholiths emphasized. Sierra Nevada is mostly Jurassic; Idaho and Boulder Batholiths are mostly late Cretaceous in age. Why is the Idaho Batholith so far east? There must have been a sharp break in the shape of western North America, or the stuff colliding, or both, to account for this. Because the Sierra Nevada and Idaho Batholiths are separated in time as well as space, there’s plenty of opportunity for things to change. Bottom line, subduction was taking place further east during Late Cretaceous time than it was during the Jurassic. Even further east there’s an even smaller batholith in southwestern Montana, the Boulder Batholith. It’s only about 75 miles by 25 miles in size, extending from Helena, Montana to the Highland Mountains south of Butte. Butte, where I live, here in the Boulder Batholith, is today’s topic, because it holds “The Richest Hill On Earth.” That’s a nickname applied to the mineral district at Butte, and it might even be true. In the United States, there is no question – the US Geological Survey has calculated the value of the big mineral districts, and Butte is definitely the most valuable. It’s a little harder to say for sure in the entire world, because we don’t really know the value of mineral production from the Roman Empire, Incas, or whatever. But for one little mineral district, only about 6 square miles in area, it probably is the most valuable on the planet. I admit that I’m a little prejudiced about it, but still, it’s pretty likely. There are rich metalliferous deposits scattered through the Rockies, the mountains of Mexico, and the Andes, all related to subduction of various oceanic plates beneath the North and South American continents. In terms of US production, Butte ranks #2 in copper, but #1 in produced copper plus reserves, #2 in silver, but #1 in terms of produced silver plus reserves, #6 in Zinc, and among the leading producers of manganese, lead, and molybdenum. It’s also produced large amounts of gold, cadmium, bismuth, and other metals. In terms of weight, Butte has produced about 24 billion pounds of copper, 5 billion pounds of zinc, almost 4 billion pounds of manganese, and almost three-quarters of a billion ounces of silver. That silver production probably places Butte third in the world, after Potosi, Bolivia, and Coeur d’Alene-Kellogg, Idaho. Why? Why, within the 75 by 25 mile Boulder Batholith, is so much mineral wealth concentrated in a 6-square-mile area? The bottom line is, we don’t know. We know all sorts of things about how the veins formed, the way the mineral deposit is zoned, with more copper toward the center and more silver and zinc around the margin. We can talk about intersecting fractures that helped channel the hot waters carrying the minerals, concentrating them into this one area. But the ultimate question of why is unanswered. One idea suggests that in the subducting oceanic crust, there was a zone that was very rich in copper and

A few days ago we talked about the Laramide Orogeny, the brittle breaking of the continental crust into huge uplifts along relatively high-angle faults with miles and miles of throw. And I mentioned a different style of mountain building that took place partially at the same time and in some areas, in the same places. That aspect of the deformation is called the Sevier Orogeny – and again that’s not “severe” but “Sevier,” from a place in Utah. Just to keep things confusing. Sevier vs Laramide (source) The basic difference between the Sevier part of the activity and the Laramide part is that instead of those big brittle breaks in the crust, in the Sevier we had much thinner slices of rock – mostly the bedded sedimentary rock – being pushed over each other in generally low-angle thrust faults with often only a few thousand feet of displacement, but sometimes more. This is the fairly typical result of collisions. Think of a short pile of carpets and sheets and bedspreads all nicely on top of each other in horizontal layers. That’s the sedimentary package of rocks in western North America, ranging in age from Precambrian to the early Cretaceous. There’s been some bumping and breaking and so on, but on the whole, those carpets and sheets are still more or less intact and relatively horizontal. Now set a file cabinet on one side of the pile, and start pushing. The fabrics will fold and push up and over each other. In the real world of rocks, they are brittle enough to eventually break and slide over each other, and those breaks are called thrust faults. But the floor, the crystalline granitic rocks underneath the sediments, does not break. Well, it did in the Laramide Orogeny that we talked about the other day. But not in this more straightforward pushing we had during the Sevier Orogeny. In the real world, as the rocks that are the equivalent of our carpets and sheets piled up on top of each other, two things happened. First, the tops start eroding, with the eroded sediments shedding off to the east of the uplifted, thrusted mountains. And second, the weight of the thrust sheets, plus the sediment, was enough to bow down the crystalline granitic floor. Not really enough to break it, but to make it sag. We’ve just created a classic foreland basin. The foreland is the territory toward the craton, in this case the North American continent, inboard from the mountains created by the collision off to the west. The deepest part was in the west closest to the collision zone, where the thrust sheets and sediment piles were thickest, then it gets shallower and shallower, really pretty quickly, as you head east onto the strong craton. We can see the evidence for this in changes in sedimentation from west to east. Here in Montana, where I live, along the Big Hole River, the Kootenai Formation of early Cretaceous age is something like 3,000 feet thick. Just 50 miles to the east, the Kootenai is about 400 feet thick. That change in thickness reflects the bottom falling out – the crust subsiding – in the western part of the foreland basin. To an extent it’s a self-perpetuating event: as more and more sediment and thrust sheets come in, the crust bows down more and more, allowing for more and more sediment to pile into the basin. Eventually, of course, it slows down or stops, once the collision has stopped and the mountains have been eroded to a level where they don’t contribute sediments in huge volume any more. One important difference between the Laramide style and the Sevier style of mountain building is that the Laramide was pretty much a case of brittle breaking. The crust is thick, relatively uniform, and brittle, so it tends to break rather than bend. The sedimentary pile, on the other hand, was a package of diverse rocks that overall was a bit more plastic, and could fold before it broke. In detail, of course, there are brittle units and more plastic units – sandstones and limestones tend to be stronger and more brittle, and shales tend

One of the findings that helped convince geologists on the American side of the Atlantic  that continental drift was a reality was the discovery of sea-floor spreading – the idea that new oceanic crust is generated at the mid-ocean ridges, and that new crust pushes older crust out of the way, away from the mid-ocean ridge, thereby making the ocean basins wider and wider at about the rate your fingernails grow. The discovery of sea-floor spreading came through geophysics – specifically, measurements of the earth’s magnetic field as it is preserved in formerly molten rock. When molten rock, magma, solidifies, tiny particles of magnetic minerals, mostly the mineral magnetite, an iron oxide, become frozen in place with the orientation of the magnetic field that’s present at the time the rock solidified. That’s all well and good, but so what? It’s useful because the earth’s magnetic field has changed over time, and is changing right now. The positions of the north and south magnetic poles change, the strength of the magnetic field changes, and the whole system even reverses its polarity, so that the north magnetic pole becomes the south magnetic pole and vice versa. There’s a lot of research and a lot of debate about how a magnetic field reversal happens. Increasing evidence shows that it may take place over a period of a few thousand or even a few hundred years – instantaneous, geologically. It must have something to do with flow in the molten outer core of the earth, where the magnetic field is generated by electrical currents in the liquid rock there. For now, let’s just recognize that these reversals have indeed happened in the geologic past. We can use measurements of the rocks with opposite polarity to figure out a lot of geological things. Reversal pattern at mid-ocean ridgeAs new oceanic crust is generated at a mid-ocean ridge by upwelling magma, each new intrusion splits the previous rock into two, one slice on each side of the rift. The two slices are pushed aside by the new intrusion. Do this hundreds of times, and on both sides of a mid-ocean ridge you have pairs of almost identical stripes of rock representing the continual intrusion of new rock at the ridge axis. As the different intrusive magmas solidify, they record the magnetic field in place at that time. Because the field reverses, we end up with alternating high and low magnetic values, reflecting the alternating polarity of the field resulting from reversals. In practice, this gives a uniform striping to the map of the magnetic field along mid-ocean ridges – symmetrical, alternating, long linear magnetic highs and lows. We can figure out things like the direction of spreading, its speed, and more. An incredibly useful tool for understanding plate tectonics. Reversal chartThere have been at least 180 magnetic field reversals in the past 80 or so million years, with a seemingly random periodicity. The length of time that the magnetic field remains stable in either north or south polarity is also pretty variable, ranging from a million years or more to a few hundred years. The last major magnetic field reversal happened about 780,000 years ago, although there was a short-lived event about 41,000 years ago as well. I mentioned back in the Jurassic that almost all the present-day oceanic crust is of Jurassic age or younger, because most of the older oceanic crust has been subducted, recycled and melted down inside the earth. So we can’t use this tool for times before the Jurassic, at least not using oceanic crust, but we can look at the magnetic field frozen into other magnetite-bearing igneous rocks that are of all ages. I’ve brought this topic up now, during the Cretaceous, because the Cretaceous was a time when the earth’s magnetic field did not reverse as it has so often at other times. For 38 million years, 121 to 83 million years ago, the earth’s magnetic field didn’t flip, a time called the Cretaceous Normal Superchron, normal because it was the same as

Photo of Xiphactinus from Kansas by Spacini, used under Creative Commons license. Teleost fish are known as far back as the Triassic, but they diversified mightily in the Cretaceous. This is the group that includes about 96% of all modern fishes, many of which began in the Cretaceous. More than 26,000 living species of fish are teleosts.   Teleosts have some skeletal differences that distinguish them from earlier fish, including a movable jaw and a spine that ends before the tail fin.  While the Cretaceous saw the expansion of many groups of fish alive today, including salmon, bass, and cod, on an individual species level there were plenty of comings and goings – new species appearing, while others went extinct, which is always happening. On the whole you’d probably be hard pressed to see any big differences between many Cretaceous teleosts and modern varieties. Xiphactinus, whose name means sword-fin, was one huge teleost that reached 20 feet in length. They were fanged predators who lived in the late Cretaceous seas of Kansas, where they were first discovered in the 1850s, and at other locations in North America as well as Europe, Australia, and South America. Many fossil specimens include the skeletons of large prey in the stomachs of Xiphactinus. The name teleost is from the Greek meaning “complete” and “bone” – a nicely, completely, boned fish. —Richard I. Gibson Photo of Xiphactinus by Spacini, used under Creative Commons license.

Eighty million years ago, while the Laramide Orogeny was getting underway in western North America, central and south Texas were parts of the shallow carbonate bank that developed on the North American side of the Gulf of Mexico. The Gulf had begun to form during the Jurassic as Yucatan pulled away from what is now Texas and Louisiana. These Cretaceous rocks are part of the Gulf Coastal Plain that we talked about a few days ago.  Remember the rudists? The tubular clams a meter high that trapped sediment to help form reefs? They grew in this area too. It was overall a quiet, shallow sea, perhaps something like today’s Florida Shelf. The setting was not one where you’d expect volcanoes, but that’s what we got.  In a long, linear zone east of a line from Waco to Austin and on south to San Antonio and Uvalde, Texas, there’s a string of more than 200 little volcanoes that erupted into the carbonate sediments. They’re basically piles of volcanic ash together with some basaltic flows, and some of them today are resistant enough to form mounds on the land surface. One well-known example is at Pilot Knob, not too far from Austin. Pilot Knob is about two miles across.  Most of these volcanic bodies are buried in the subsurface and have no expression that we can see on the land, but most of them are basaltic and contain a lot of magnetite. This gives them a distinct expression in a magnetic map. That characteristic was useful in oil exploration, because the volcanics and the surrounding carbonate rocks contain oil in 35 or 40 of the known volcanoes. Something like 50 million barrels of oil have been produced from several accumulations since the first field was discovered in the 1910s. Magnetic map of Uvalde and Medina Counties, Texas (from USGS). Most of the little pimple-like bumps represent igneous plugs of Cretaceous age. The margin of the old Texas Craton, the Precambrian core of this region, is called the Balcones Escarpment, a topographic feature that follows a fault zone separating the older rocks of central Texas from the Cretaceous and younger rocks of the Gulf Coastal Plain. The Balcones Escarpment is followed by Interstate 35 from Waco to Austin to San Antonio, just about the same zone where the volcanic centers are found. It’s not completely clear why these volcanoes erupted into this tectonically quiet region. Probably the best explanation is that there was a pulse of extension, pulling apart, that opened deep-seated faults and fractures through which the magma rose. The weakest zone was along the old break between the strong craton and the stretched crust to the south and east that was pulled and stretched by Yucatan’s departure in the Jurassic. The magmas are not all basaltic, which makes it difficult to say, for example, that they simply came from the mantle – there must have been some melting of other rocks and mixing of magmas to get the kinds of igneous rocks we see. —Richard I. Gibson Cretaceous volcanism in South Texas and oil  Pilot Knob Magnetic modeling   Magnetic map (USGS OFR-02-0049)   and this one  

Today I’m tacking the Laramide Orogeny of western United States. It’ll be a long one, in part because I’ve done work on it myself, both for general academic understanding and for oil exploration, and because it's a complex system of mountain building. You recall that ‘orogeny’ is just Greek for mountain building, and over the course of these podcasts I’ve talked about enough complications that you know such an ‘event’ is anything but instantaneous, nor is it always the same in all places. This one is even more complicated, perhaps in part because it is young enough that we see a lot of its effects and therefore understand it a little better. First let’s try to deal with some nomenclature issues. What do I mean when I say “Laramide Orogeny”? The question has to be asked because sometimes geologists use the phrase to refer to a particular time interval – in this case, mostly late Cretaceous into the early Cenozoic, around 75 to 40 million years ago – but some use the name Laramide to refer to a general geographic location, from Canada to Mexico, but generally in the eastern section of what we call the Rocky Mountains today, and extending as far east as the Black Hills of South Dakota. The expression is probably best in Wyoming, and the orogeny is named for the Laramie Mountains of southeastern Wyoming. Double Lake, in the Precambrian of the Wind River Mountains, a Laramide uplift. Photo by Richard Gibson (1982)Yet another meaning for “Laramide Orogeny,” and the one that I’ll try to use, is the structural style, the nature of the folding and faulting, because it is distinctly different from typical collisions that produce mountain ranges. What happened that’s unusual is that the continental crust, the strong, granitic craton well inboard from the point of collision and action to the west, that crust broke in gargantuan brittle faults. This kind of faulting is also called “thick-skinned” because it affected the thick continental crust, in contrast to the thin sheets of sedimentary and other rocks that are typically pushed over each other in thrust faults as a result of many types of collisions. In fact, to some extent overlapping in both time and space, that kind of action – “thin-skinned” – was happening at the same time as the Laramide Orogeny. To make things more confusing, that aspect of the event is called the Sevier Orogeny – and it isn’t spelled ‘severe’, but “Sevier”, named for a location in Utah where it’s expressed pretty well. I’m going to talk a bit more specifically about the Sevier Orogeny in a few days, but it really isn’t separate from the Laramide in many ways, and the two are both the rather different results of the same tectonic action. Map of Laramide structures by Hamilton (1981), USGS. Contributions to Geology - University of Wyoming, V. 19, no. 2. So let’s focus on Wyoming, where the Laramide Orogeny is probably best expressed. Most of the big mountain ranges in and near Wyoming are the result of this unusual intense breaking of the continental crust. The Uinta in Utah, the Wind River, the small Owl Creek Range, the Beartooth in Wyoming and Montana, the Bighorn, the Sierra Madre, the Laramie Range, and the Black Hills of South Dakota, all are the result of huge reverse faults that bring the deep Precambrian rocks not just up to the surface, but high above the present surface. In the Wind Rivers at Gannett Peak, the Precambrian is at the surface almost 14,000 feet above sea level, and equivalent rocks in the Green River Basin west of the Wind Rivers are about 32,000 feet below sea level. That’s a difference of more than 45,000 feet – almost nine miles. The break that separates them is one relatively narrow fault zone, the Wind River Fault, along the west side of the mountains. That’s really a huge amount of offset along a fault. The Wind River Fault slopes off to the east, under the Wind River Mountains, so the Precambrian rocks have been brought not just up, but up and over much younger rocks, including roc

Hypsilophodon drawing by ArthurWesaley, used under Creative Commons license.  The ornithopods were some of the most successful and diverse dinosaurs of the Cretaceous. They typically had three toes, but some had four, and despite the name, which means “bird foot,” ornithopods were not in the dinosaur lineage that led to birds. Like many types of dinosaur, they began during the Jurassic, but in Cretaceous time herbivorous ornithopods dominated many landscapes. They were typically smaller than the huge Sauropods, on the order of three to ten feet long, though a few species grew to perhaps 50 feet in length.  Hypsilophodon, discovered on the Isle of Wight in England in 1849, was about 2 meters or 6 feet long and ran on two legs as most ornithopods did, although they probably functioned as quadrupeds at times. Its skeletal anatomy indicates that it was a ground-living animal that could probably run pretty fast – presumably for defensive escape, like a deer or gazelle, since it was a plant-eater. Because of their herbivorous natures, many Cretaceous ornithopods had lost most of their front teeth, which were replaced by a hard, beak-like mouth structure.    Hadrosaur photo by Lisa Andres from Riverside, USA, used under Creative Commons license.The culmination of evolution among the ornithopods and their kin was probably the hadrosaurs – the duck-billed dinosaurs that were abundant in late Cretaceous time. Some hadrosaurs really did have a face that was elongated into a bill-like structure presumably used for snagging leaves and twigs, but they did have grinding teeth in the back of the mouth. Duck-billed dinosaurs also had complex crests on the tops of their heads – at least some species did, but some had no ornamentation at all. The role in life of the hollow crests has been discussed for years, and I think today the consensus is that they may have been used for both audible hooting and as a visual display. Hadrosaurs probably descended from Iguanodons or their relatives, which we discussed earlier this month. They lived in what are now Asia, Europe, and North America and are dated mostly to the last 10 or 15 million years of the Cretaceous period. All went extinct at the end of the Cretaceous. —Richard I. Gibson Reference: Holtz, Thomas R. Jr. (2012) Dinosaurs: The Most Complete, Up-to-Date Encyclopedia for Dinosaur Lovers of All Ages Hypsilophodon drawing by ArthurWesaley, used under Creative Commons license.  Hadrosaur photo by Lisa Andres from Riverside, USA, used under Creative Commons license.