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Mesoarchean Era

The Mesoarchean  is a geologic era within the Archean, spanning 3,200 to 2,800 million years ago. The period is defined chronometrically and is not referenced to a specific level in a rock section on Earth. Fossils from Australia show that stromatolites have lived on Earth since the Mesoarchean. The Pongola glaciation occurred at 2,900 million years ago. The first supercontinent Vaalbara broke up during this time around 2,800 million years ago.

Note : The above story is based on materials provided by Wikipedia

Paleoarchean Era

The Paleoarchean (/ˌpeɪlɪ.oʊ.ɑrˈkiːən/; also spelled Palaeoarchaean (Formerly known as early Archean)) is a geologic era within the Archaean. It spans the period of time 3,600 to 3,200 million years ago—the period being defined chronometrically and not referenced to a specific level in a rock section on Earth. The name derives from Greek “Palaios” ancient.
The oldest ascertained life form (well-preserved bacteria older than 3,460 million years found in Western Australia) is from this period. The 1st supercontinent Vaalbara formed during this period.

Stromatolites – Pilbara craton Western Australia

Note : The above story is based on materials provided by Wikipedia

Jefferson River

Confluence of Beaverhead and Big Hole Rivers forming the Jefferson near Twin Bridges, Montana

The Jefferson River is a tributary of the Missouri River, approximately 83 miles (134 km) long, in the U.S. state of Montana. The Jefferson River and the Madison River form the official beginning of the Missouri at Missouri Headwaters State Park near Three Forks. It is joined 0.6 miles (1.0 km) downstream (northeast) by the Gallatin.

From broad valleys to a narrow canyon, the Jefferson River passes through a region of significant geological diversity, with some of the oldest and youngest rocks of North America and a diversity of igneous, metamorphic, and sedimentary formations.

The region was only intermittently inhabited by Native Americans until relatively recent times, and no single tribe had exclusive use of the Jefferson River when the Lewis and Clark Expedition first ascended the river in 1805. Today, the Jefferson River retains much of its scenic beauty and wildlife diversity from the days of Lewis and Clark, yet is threatened by water use issues and encroaching development. The Jefferson is a segment of the Lewis and Clark National Historic Trail, administered by the National Park Service.

Table of Contents

Course

Jefferson River near Parrot Castle, October 2007

From the Rocky Mountains of southwestern Montana, three small rivers converge to form the headwaters of the Jefferson River. The longest begins at Brower’s Spring, 9,030 feet (2,750 m) above sea level, on the northern flank of the Centennial Mountains. The site is marked by pile of rocks. The water flows west then north as Hell Roaring Creek before merging with Rock Creek and flowing west through Upper and Lower Red Rock Lakes. Here it becomes the Red Rock River, flowing west through Lima Reservoir and then northwest into Clark Canyon Reservoir near Dillon. Below the dam, the river is known as the Beaverhead River. It is joined by the Ruby River above the town of Twin Bridges and converges with the Big Hole River to form the Jefferson about two miles downstream from town.

The Jefferson River flows north through the Jefferson Valley towards Whitehall and then east, where it is joined by the Boulder River before passing through the narrow Jefferson River canyon near Lewis and Clark Caverns State Park. After the canyon, the river passes into a broad valley again near Willow Creek. The Jefferson converges with the Madison River at Missouri Headwaters State Park near Three Forks to form the Missouri River, joined a short distance downstream by the Gallatin River.

Geology

The geology of the Jefferson River and the surrounding mountain ranges includes some of the oldest rocks found in North America, dating back to the Archean Eon, 2.7 billion years ago. Found primarily in the Tobacco Root and Ruby ranges, these ancient rocks are metamorphic, having been highly compressed and nearly re-melted by geologic forces over eons of time. Frequently found along the Jefferson River, these rocks include layered feldspars, gneiss, glassy quartz, heavy dark amphibolite, and sometimes marble.
Small marine fossils can be found in the Madison Group limestone that makes up the steep, narrow section of the Jefferson River canyon.
About a billion years ago, the Willow Creek Fault, north of the Jefferson River canyon, dropped down deeply and filled with seawater, stretching north to Alberta and British Columbia. Eventually, the sea receded and erosion wore away intervening geologic history until about 530 million years ago, during the Cambrian Period of the Paleozoic Era.

A new sea encroached on the land, depositing sedimentary layers of limestone, dolomite, shale, and sandstone over several hundred million years. Limestone is generally made of calcium from marine animals that have been compacted and cemented together. Dolomite is similar but has more magnesium. Shale is formed from fine-grained mud, silts, and clays that have been compacted and cemented together. The sandstone is made up of quartz and feldspar.By the Mississippian Period, 340 million years ago, much of western North America was covered with a warm, shallow sea, much like the Gulf Coast of Florida today. Small marine fossils can be found in the Madison Group limestone that makes up the steep, narrow section of the Jefferson River canyon today.

Gentle uplift eventually raised the region above sea level again. Rainwater percolated down through cracks in the limestone, dissolving rock and creating caves such as those found at Lewis and Clark Caverns State Park.

Local mountains, such as the Tobacco Roots were formed from the Boulder Batholith. The batholith is composed of at least seven, and possibly as many as fourteen, discrete igneous rock masses called plutons, which formed beneath the Earth’s surface during a period of magma intrusion about 73 to 78 million years ago during the Late Cretaceous. The rising buoyant plutons resulted from subduction along what was then the west coast of North America. Regional uplift brought the deep-seated granite to the surface, where erosion exposed the rocks and the mineral veins they contained. The granite generally consists of quartz, hornblende, and feldspars. Gold, silver, and other semi precious minerals are also associated with batholiths.

The ancient metamorphic and more recent sedimentary layers above the batholiths eroded away as the magma pushed up through the crust. Thus, the granite batholiths are typically found at the center of local mountain ranges, while the much older metamorphic gneiss is usually found lower in the mountains, and limestone layers are mostly found in the foothills nearest the Jefferson River.

The Rocky Mountains began a new and continuing phase of crustal stress 5 to 10 million years ago as tectonic forces began to pull the region apart. Blocks of earth dropped down to form valleys, and the Jefferson River eroded a channel through rock to form the Jefferson River canyon.

Note : The above story is reprinted from materials provided by Wikipedia

Delafossite

Locality: Clara Mine, Rankach valley, Oberwolfach, Wolfach, Black Forest, Baden-Württemberg, Germany Field of view: 2.12 mm Copyright © Gerhard Niceus

Chemical Formula: CuFeO2
Locality: Calumet and Arizona mine, Bisbee, Cochise Co., Arizona, USA.
Name Origin: Named for Gabrial Delafosse (1796-1878), French mineralogist and crystallographer.

Delafossite is a copper iron oxide mineral with formula CuFeO2 or Cu1+Fe3+O2. It is member of the delafossite mineral group with a general formula ABO2, a group characterized by a sheet of linearly coordinated A cations stacked between edge-shared octahedral layers (BO6).

Delafossite along with other minerals of the ABO2 group has been recognized for its electrical properties from insulation to metallic conduction. Delafossite is usually a secondary mineral that crystallizes near oxidized copper and is rarely a primary mineral.

Geologic occurrence

In 1873, delafossite was discovered by Charles Friedel in a region of Ekaterinbug, Siberia. Since its discovery it has been identified as a fairly common mineral found in such places as the copper mines of in Bisbee, Arizona. Delafossite is usually a secondary mineral often found in oxidized areas of copper deposits although it can be a primary mineral as well. Delafossite can be found as massive, relatively distinct crystals on hematite. Delafossite has since been found in mines around the world from Germany to Chile.

Physical Properties of Delafossite

Cleavage: {1010} Indistinct
Color: Black.
Density: 5.41
Diaphaneity: Opaque
Fracture: Brittle – Generally displayed by glasses and most non-metallic minerals.
Hardness: 5.5 – Knife Blade
Luminescence: Non-fluorescent.
Luster: Metallic
Magnetism: Magnetic after heating
Streak: black

Photo :

This sample of delafossite is displayed in the Smithsonian Museum of Natural History. This sample is about 10×10 cm overall. It is from Calumet and Arizona Mine, Cochise County, Arizona.
Delafossite, Cuprite Locality: Le Moulinal Mine, Saint-Jean-de-Jeannes, Paulinet, Alban, Tarn, Midi-Pyrénées, France Dimensions: 41 mm x 35 mm x 31 mm Field of View: 9 mm Copyright © Pascale & Daniel Journet
Delafossite, Copper Locality: Clara Mine, Rankach valley, Oberwolfach, Wolfach, Black Forest, Baden-Württemberg, Germany FOV: 3 mm. Copyright © Stephan Wolfsried

Megafloods: What They Leave Behind

Stubby Canyon, Malad Gorge State Park, Idaho. (Credit: Michael Lamb)

South-central Idaho and the surface of Mars have an interesting geological feature in common: amphitheater-headed canyons. These U-shaped canyons with tall vertical headwalls are found near the Snake River in Idaho as well as on the surface of Mars, according to photographs taken by satellites. Various explanations for how these canyons formed have been offered — some for Mars, some for Idaho, some for both — but in a paper published the week of December 16 in the online issue of Proceedings of the National Academy of Sciences, Caltech professor of geology Michael P. Lamb, Benjamin Mackey, formerly a postdoctoral fellow at Caltech, and W. M. Keck Foundation Professor of Geochemistry Kenneth A. Farley offer a plausible account that all these canyons were created by enormous floods.

Canyons in Malad Gorge State Park, Idaho, are carved into a relatively flat plain composed of a type of volcanic rock known as basalt. The basalt originated from a hotspot, located in what is now Yellowstone Park, which has been active for the last few million years. Two canyons in Malad Gorge, Woody’s Cove and Stubby Canyon, are characterized by tall vertical headwalls, roughly 150 feet high, that curve around to form an amphitheater. Other amphitheater-headed canyons can be found nearby, outside the Gorge — Box Canyon, Blue Lakes Canyon, and Devil’s Corral — and also elsewhere on Earth, such as in Iceland.

To figure out how they formed, Lamb and Mackey conducted field surveys and collected rock samples from Woody’s Cove, Stubby Canyon, and a third canyon in Malad Gorge, known as Pointed Canyon. As its name indicates, Pointed Canyon ends not in an amphitheater but in a point, as it progressively narrows in the upstream direction toward the plateau at an average 7 percent grade. Through Pointed Canyon flows the Wood River, a tributary of the larger Snake River, which in turn empties into the Columbia River on its way to the Pacific Ocean.

Geologists have a good understanding of how the rocks in Woody’s Cove and Stubby Canyon achieved their characteristic appearance. The lava flows that hardened into basalt were initially laid down in layers, some more than six feet thick. As the lava cooled, it contracted and cracked, just as mud does when it dries. This produced vertical cracks across the entire layer of lava-turned-basalt. As each additional sheet of lava covered the same land, it too cooled and cracked vertically, leaving a wall that, when exposed, looks like stacks of tall blocks, slightly offset from one another with each additional layer. This type of structure is called columnar basalt.

While the formation of columnar basalt is well understood, it is not clear how, at Woody’s Cove and Stubby Canyon, the vertical walls became exposed or how they took on their curved shapes. The conventional explanation is that the canyons were formed via a process called “groundwater sapping,” in which springs at the bottom of the canyon gradually carve tunnels at the base of the rock wall until this undercutting destabilizes the structure so much that blocks or columns of basalt fall off from above, creating the amphitheater below.

This explanation has not been corroborated by the Caltech team’s observations, for two reasons. First, there is no evidence of undercutting, even though there are existing springs at the base of Woody’s Cove and Stubby Canyon. Second, undercutting should leave large boulders in place at the foot of the canyon, at least until they are dissolved or carried away by groundwater. “These blocks are too big to move by spring flow, and there’s not enough time for the groundwater to have dissolved them away,” Lamb explains, “which means that large floods are needed to move them out. To make a canyon, you have to erode the canyon headwall, and you also have to evacuate the material that collapses in.”

That leaves waterfall erosion during a large flood event as the only remaining candidate for the canyon formation that occurred in Malad Gorge, the Caltech team concludes.

No water flows over the top of Woody’s Cove and Stubby Canyon today. But even a single incident of overland water flow occurring during an unusually large flood event could pluck away and topple boulders from the columnar basalt, taking advantage of the vertical fracturing already present in the volcanic rock. A flood of this magnitude could also carry boulders downstream, leaving behind the amphitheater canyons we see today without massive boulder piles at their bottoms and with no existing watercourses.

Additional evidence that at some point in the past water flowed over the plateaus near Woody’s Cove and Stubby Canyon are the presence of scour marks on surface rocks on the plateau above the canyons. These scour marks are evidence of the type of abrasion that occurs when a water discharge containing sediment moves overland.

Taken together, the evidence from Malad Gorge, Lamb says, suggests that “amphitheater shapes might be diagnostic of very large-scale floods, which would imply much larger water discharges and much shorter flow durations than predicted by the previous groundwater theory.” Lamb points out that although groundwater sapping “is often assumed to explain the origin of amphitheater-headed canyons, there is no place on Earth where it has been demonstrated to work in columnar basalt.”

Closing the case on the canyons at Malad Gorge required one further bit of information: the ages of the rock samples. This was accomplished at Caltech’s Noble Gas Lab, run by Kenneth A. Farley, W. M. Keck Foundation Professor of Geochemistry and chair of the Division of Geological and Planetary Sciences.

The key to dating surface rocks on Earth is cosmic rays — very high-energy particles from space that regularly strike Earth. “Cosmic rays interact with the atmosphere and eventually with rocks at the surface, producing alternate versions of noble gas elements, or isotopes, called cosmogenic nuclides,” Lamb explains. “If we know the cosmic-ray flux, and we measure the accumulation of nuclides in a certain mineral, then we can calculate the time that rock has been sitting at Earth’s surface.”

At the Noble Gas Lab, Farley and Mackey determined that rock samples from the heads of Woody’s Cove and Stubby Canyon had been exposed for the same length of time, approximately 46,000 years. If Lamb and his colleagues are correct, this is when the flood event occurred that plucked the boulders off the canyon walls, leaving the amphitheaters behind.

Further evidence supporting the team’s theory can be found in Pointed Canyon. Rock samples collected along the walls of the first kilometer of the canyon show progressively more exposure in the downstream direction, suggesting that the canyon is still being carved by Wood River. Using the dates of exposure revealed in the rock samples, Lamb reconstructed the probable location of Pointed Canyon at the time of the formation of Woody’s Cove and Stubby Canyon. At that location, where the rock has been exposed approximately 46,000 years, the surrounding canyon walls form the characteristic U-shape of an amphitheater-headed canyon and then abruptly narrow into the point that forms the remainder of Pointed Canyon. “The same megaflood event that created Woody’s Cove and Stubby Canyon seems to have created Pointed Canyon,” Lamb concludes. “The only difference is that the other canyons had no continuing river action, while Pointed Canyon was cut relatively slowly over the last 46,000 years by the Wood River, which is not powerful enough to topple and pluck basalt blocks from the surrounding plateau, resulting in a narrow channel rather than tall vertical headwalls.”

Solving the puzzle of how amphitheater-headed canyons are created has implications reaching far beyond south-central Idaho because similar features — though some much larger — are also present on the surface of Mars. “A very popular interpretation for the amphitheater-headed canyons on Mars is that groundwater seeps out of cracks at the base of the canyon headwalls and that no water ever went over the top,” Lamb says. Judging from the evidence in Idaho, however, it seems more likely that on Mars, as on Earth, amphitheater-headed canyons were created by enormous flood events, suggesting that Mars was once a very watery planet.

Note : The above story is based on materials provided by California Institute of Technology. The original article was written by Cynthia Eller. 

Soil production breaks geologic speed record

Isaac Larsen collects a sand sample at the Rapid Creek test site. Credit: Krista Larsen

Geologic time is shorthand for slow-paced. But new measurements from steep mountaintops in New Zealand show that rock can transform into soil more than twice as fast as previously believed possible.The findings were published Jan. 16 in the early online edition of Science.

“Some previous work had argued that there were limits to soil production,” said first author Isaac Larsen, who did the work as part of his doctoral research in Earth sciences at the University of Washington. “But no one had made the measurements.”

The finding is more than just a new speed record. Rapidly eroding mountain ranges account for at least half of the total amount of the planet’s weathering and sediment production, although they occupy just a few percent of the Earth’s surface, researchers said.

So the record-breaking production at the mountaintops has implications for the entire carbon cycle by which the Earth’s crust pushes up to form mountains, crumbles, washes with rivers and rainwater to the sea, and eventually settles to the bottom to form new rock.

“This work takes the trend between soil production rates and chemical weathering rates and extends it to much higher values than had ever been previously observed,” said Larsen, now a postdoctoral researcher at the California Institute of Technology in Pasadena.

The study site in New Zealand’s Southern Alps is “an extremely rugged mountain range,” Larsen said, with rainfall of 10 meters (33 feet) per year and slopes of about 35 degrees.

To collect samples Larsen and co-author André Eger, then a graduate student at Lincoln University in New Zealand, were dropped from a helicopter onto remote mountaintops above the tree line. They would hike down to an appropriate test site and collect 20 pounds of dirt apiece, and then trek the samples back up to their base camp. The pair stayed at each of the mountaintop sites for about three days.

“I’ve worked in a lot of places,” Larsen said. “This was the most challenging fieldwork I’ve done.”

Researchers then brought soil samples back to the UW and measured the amount of Beryllium-10, an isotope that forms only at the Earth’s surface by exposure to cosmic rays. Those measurements showed soil production rates on the ridge tops ranging from 0.1 to 2.5 millimeters (1/10 of an inch) per year, and decrease exponentially with increasing soil thickness.

The peak rate is more than twice the proposed speed limit for soil production, in which geologists wondered if in places where soil is lost very quickly, the soil production just can’t keep up. In earlier work Larsen had noticed vegetation on very steep slopes and so he proposed this project to measure soil production rates at some of the steepest, wettest locations on the planet.

The new results show that soil production and weathering rates continue to increase as the landscape gets steeper and erodes faster, and suggest that other very steep locations such as the Himalayas and the mountains in Taiwan may also have very fast soil formation.

“A couple millimeters a year sounds pretty slow to anybody but a geologist,” said co-author David Montgomery, a UW professor of Earth and space sciences. “Isaac measured two millimeters of soil production a year, so it would take just a dozen years to make an inch of soil. That’s shockingly fast for a geologist, because the conventional wisdom is it takes centuries.”

The researchers believe plant roots may be responsible here. The mountain landscape was covered with low, dense vegetation. The roots of those plants reach into cracks in the rocks, helping break them apart and expose them to rainwater and chemical weathering.

“This opens up new questions about how soil production might happen in other locations, climates and environments,” Larsen said.

Note : The above story is based on materials provided by University of Washington

Datolite

Dal’negorsk (Dalnegorsk; Tetyukhe; Tjetjuche; Tetjuche), Kavalerovo Mining District, Primorskiy Kray, Far-Eastern Region, Russia © 2001 John H. Betts

Chemical Formula: Ca(HBSiO5)
Locality: Diabases of the Connecticut River valley, USA.
Name Origin: From the Greek, dateisthai, meaning “to divide,” because granular aggregates crumble readily.

Datolite is a calcium boron hydroxide nesosilicate, Ca(HBSiO5). It was first observed by Jens Esmark in 1806, and named by him from δατεῖσθαι, “to divide,” and λίθος, “stone,” in allusion to the granular structure of the massive mineral.

Datolite crystallizes in the monoclinic system forming prismatic crystals and nodular masses. The luster is vitreous and may be brown, yellow, light green or colorless. The Mohs hardness is 5.5 and the specific gravity is 2.8 – 3.0.

The type localities are in the diabases of the Connecticut River valley and Arendal, Aust-Agder, Norway. Associated minerals include prehnite, danburite, babingtonite, epidote, native copper, calcite, quartz and zeolites. It is common in the copper deposits of the Lake Superior region of Michigan. It occurs as a secondary mineral in mafic igneous rocks often filling vesicles along with zeolites in basalt. Unlike most localities throughout the world, the occurrence of datolite in the Lake Superior region is usually fine grained in texture and possesses colored banding. Much of the coloration is due to the inclusion of copper or associated minerals in progressive stages of hydrothermal precipitation.

Botryolite is a botryoidal form of datolite.

Physical Properties of Datolite

Cleavage: None
Color: Brown, Colorless, Yellow, White, Light green.
Density: 2.8 – 3, Average = 2.9
Diaphaneity: Transparent to translucent
Fracture: Brittle – Generally displayed by glasses and most non-metallic minerals.
Hardness: 5.5 – Knife Blade
Luminescence: Non-fluorescent.
Luster: Vitreous (Glassy)
Streak: white

Photos:

This sample is described as datolite with quartz. It is about 12 cm across and is from Paterson, New Jersey. This sample of datolite displayed in the Smithsonian Museum of Natural History.
Datolite 4.1×4.0x2.3 cm La Baja Mine Charcas, San Louis de Potosi Mexico Copyright © 2011 David K. Joyce Minerals
This sample is described as datolite with copper. It is about 7cm across and is from Lake Superior District, Michigan. This sample of datolite displayed in the Smithsonian Museum of Natural History.
Datolite – Bor Pit, Dal’negorsk B deposit, Dal’negorsk, Primorskiy Kray, Russia Size: 12.2 x 4.6 x 2.3 cm Copyright © danweinrich

Eoarchean Era

In the geologic record the Eoarchean (/ˌiːoʊ.ɑrˈkiːən/; also spelled Eoarchaean) Era or erathem is the earliest time following the solidification of Earth’s crust. It follows the Hadean and precedes the Paleoarchean Era of the geologic timescale. The approximate abiotic origins of life (abiogenesis) have been dated to a time window from 4,000 to 3,600 million years ago when atmospheric pressure values ranged from ca. 100 to 10 bar.

Table of Contents

Chronology

It was formerly officially unnamed and usually referred to as the first part of the Early Archean (now an obsolete name) together with the later Paleoarchean Era.

The International Commission on Stratigraphy now officially recognizes the Eoarchean Era as the first part of the Archaean Eon, preceded by the Hadean Eon, during which the Earth is believed to be essentially molten.

The International Commission on Stratigraphy currently does not recognize the lower boundary of the era which has been provisionally placed at 4,000 million years ago nor that of the preceding Hadean Eon.

The Eoarchean was followed by the Paleoarchean Era.

The name comes from two Greek words: eos (dawn) and archaios (ancient). The first supercontinent Vaalbara appeared around the end of this period around 3,600 million years ago.

Geology

A characteristic of the Eoarchean is that Earth possessed a firm crust for the first time. However, this crust may have been incomplete at many sites and areas of lava may have existed at the surface. The beginning of the Eoarchean is characterized by heavy asteroid bombardment within the inner solar system: the Late Heavy Bombardment. The Eoarchean is the first phase of our planet from which solid rock formations survived. The largest is the Isua Greenstone Belt at the south-west coast of Greenland. It appeared during the Eoarchean around 3.8 billion years ago. The Acasta Gneiss within the Canadian Shield have been dated to be 4,030 Ma and are therefore the oldest preserved rock formations. In 2008 another rock formation was discovered in the Nuvvuagittuq greenstone belt in northern Québec in Canada which has been dated to be 4,280 million years ago. These formations are presently under intense investigation.
Note : The above story is based on materials provided by Wikipedia

How Earth’s devastating super-volcanoes might erupt

Thank goodness Mount Sinabung isn’t a supervolcano. Credit: Binsar Bakkara/AP

Devastating supervolcanoes can erupt simply due to changes that happen in their giant magma chambers as they slowly cool, according to a new study. This finding marks the first time researchers have been able to explain the mechanism behind the eruptions of the largest volcanoes on Earth.

Geologists have identified the roots of a number of ancient and possible future supervolcanoes across the globe. No supervolcano has yet exploded in human history, but the rock record demonstrates how devastating any eruption would be to today’s civilisation. Perhaps most famous is the Yellowstone supervolcano in Wyoming, which has erupted three times in the past two million years (the last eruption occurred 600,000 years ago).

These giant volcanic time bombs seem to explode once every few hundred thousand years, and when they do, they throw huge volumes of ash into the sky. At Yellowstone, the eruption that happened two million years ago ejected more than 2,000km3 of material – enough to cover Greater London in a mile-thick layer of ash.

It is estimated that a super-eruption like that would drive a global temperature drop of 10˚C for more than a decade. Such a dramatic change in global climate is difficult to comprehend. Aside from the instant local devastation, there would be global impacts such as crop failures, followed by large famines.

Despite their potential threat, comparable to a large asteroid impact, the mechanisms and origins of super-eruptions have remained obscure. Modestly sized volcanoes operate on different time-scales and magnitudes, and their eruptions appear to be triggered by pulses of molten rock (magma), which increase the pressure in the underground magma chambers that feed their vents.

Two papers recently published in the journal Nature Geoscience try to solve the mystery of how super volcanoes are formed and how they erupt.
Using experiments and computer modelling, scientists have discovered what drives a super-eruption. They find that, over time, the underground magma becomes increasingly more buoyant. Eventually, it becomes a bit like a beach ball held down beneath the waves—when it is released, it shoots into the air, forced up by the dense water around it.

In the first paper, a team led by Wim Malfait and Carmen Sanchez-Valle of ETH Zurich used a synchrotron (an accelerator that can generate intense X-rays) to measure the density, temperature, and pressure of molten rock held in conditions resembling those of a magma chamber several kilometres below the surface. This required them to mimic deep Earth conditions in the lab at the European Synchrotron Radiation Facility, holding samples at temperatures up to 1,700˚C and the pressure of 36,000 atmospheres.

To feed a supervolcano you need a huge magma chamber. The Zurich team’s results show that, as the magma chamber cools, it begins to solidify and crystals grow in it that are denser than the magma. As these fall to the base of the chamber, the remaining molten rock gets progressively less dense. If there is enough of it, their measurements indicate that the magma eventually becomes light enough that it can force its way through more than 10km of Earth’s overlying crust.

Co-author Carmen Sanchez-Valle, also at ETH Zurich, said: “Our research has shown that the pressure is actually large enough for the Earth’s crust to break. As it rises to the surface, the magma will expand violently, which is a well known origin of a volcanic explosion”.

The second paper by Luca Caricchi and colleagues at the University of Bristol, describes computer simulations of the same processes, finding that the buoyancy of melt in maturing magma chambers is also key to these huge events.

This contrasts with the way that more familiar smaller volcanoes erupt. There, blasts follow directly from rapid injections of magma, or from external events that release the pressure on it, such as earthquakes or even the melting of overlying glaciers, as seen in Iceland recently.

The results indicate that supervolcanoes just require a steady accumulation of molten rock that remains hot enough that it does not completely solidify—a massive eruption is then simply a matter of time. Thus, the eruption of massive supervolcanoes seems to be an inevitable part of their “life cycle”. Just as a sufficiently large star will necessarily generate a supernova, so a huge magma chamber should eventually become a massive eruption.

Note : This story is published courtesy of The Conversation (under Creative Commons-Attribution/No derivatives).

Danburite

Locality: Tre Croci, Vetralla, Vico Lake, Viterbo Province, Latium, Italy FOV: 07 mm Copyright © Di Domenico Dario

Chemical Formula: CaB2Si2O8
Locality: Danbury, Connecticut.
Name Origin: Named after its location.

Danburite is a calcium boron silicate mineral with a chemical formula of CaB2Si2O8.

It has a Mohs hardness of 7 to 7.5 and a specific gravity of 3.0. The mineral has an orthorhombic crystal form. It is usually colourless, like quartz, but can also be either pale yellow or yellowish-brown. It typically occurs in contact metamorphic rocks.

The Dana classification of minerals categorizes danburite as a sorosilicate, while the Strunz classification scheme lists it as a tectosilicate; its structure can be interpreted as either.

Its crystal symmetry and form are similar to topaz; however, topaz is a calcium fluorine bearing nesosilicate. The clarity, resilience, and strong dispersion of danburite make it valuable as cut stones for jewelry.

It is named for Danbury, Connecticut, United States, where it was first discovered in 1839 by Charles Upham Shephard.

Physical Properties of Danburite

Cleavage: {001} Poor
Color: Colorless, White, Gray, Brownish white, Straw yellow.
Density: 2.97 – 3.02, Average = 2.99
Diaphaneity: Transparent to translucent
Fracture: Sub Conchoidal – Fractures developed in brittle materials characterized by semi-curving surfaces.
Hardness: 7 – Quartz
Luminescence: Fluorescent and thermoluminescent (red), Short UV=violet blue, Long UV=blue to blue-green.
Luster: Vitreous – Greasy
Streak: white

 Photos :

These samples are on display in the Smithsonian Museum of Natural History. The danburite crystal shown is on the order of 4 cm diameter. The gem is 18.5 carats. The origin of this sample is Burma.
These samples are on display in the Smithsonian Museum of Natural History. This danburite sample is about 25×25 cm and is from Charcas, San Louis Potosi, Mexico.
Danburite Locality: Alto Chapare District, Chapare Province, Cochabamba Department, Bolivia Specimen Size: 3.3 x 2.4 x 1.7 cm (thumbnail) Largest Crystal: 8 mm Copyright © Brian Kosnar and Mineral Classics
Toroku mine, Takachiho, Miyazaki Prefecture, Kyushu Region, Japan © 2003 John H. Betts

Land bulge clue to aviation threat from volcanoes

The eruption plume from Grímsvön a few hours after the start of the eruption. Credit: Bergrún Arna Óladóttir

Bulging in land that occurs before a volcano erupts points to how much ash will be spewed into the sky, providing a useful early warning for aviation, geologists in Iceland said on Sunday.

The telltale came from data from Global Positioning System (GPS) sensors placed around the notorious Icelandic volcano Grimsvoetn, they said.

Just before Grimsvoetn blew its stack in May 2011, the ground around the volcano started to bulge.

In a brief but violent eruption, it disgorged a 20-kilometre-high (12-mile) plume of ash, equivalent to 0.27 square kilometres (0.06 cubic miles) of material.

By matching the ground deformation with the volume of the ash, the scientists got a snapshot of conditions that prevailed in the magma chamber below the volcano before the eruption.

The magma chamber is a vessel that progressively fills with injections of molten rock.

When the pressure becomes too great, the magma is expelled through cracks, forming ash as it cools in its passage through the air.

The timing of the eruption and the size of the ash plume depend on several factors within this chamber.

They include the volume of magma, the force at which it is expelled and the resilience of the rock walls of the chamber itself to the mounting pressure.

In the study published in Nature Geoscience, the team, led by Sigrun Hreinsdottir of the Nordic Volcanological Centre in Reykjavik said the magma chamber was about three kilometres (1.9 miles) beneath Grimsvoetn.

The signature from the groundswell points to a drop in pressure about 1.7 kms (1.06 miles) beneath the surface, about an hour before the eruption, as the magma headed upwards.

In volcanoes that are under close surveillance, the method could help warn of imminent eruptions and forecast the possible altitude of ash clouds, the authors said.

“If interpreted in near-real time, these observations could greatly improve forecasting of the onset and evolution of explosive eruptions and volcanic plume height,” they said.

Located at the heart of Iceland’s biggest glacier, Vatnajoekull, Grimsvoetn is Iceland’s most active volcano. Prior to 2011, it had erupted nine times between 1922 and 2004.

The 2011 eruption raised fears of a repeat of the air travel chaos caused by a blast the previous year at the nearby Eyjafjoell volcano, which led to the world’s biggest airspace shutdown since World War II, affecting more than 100,000 flights and eight million passengers.

Despite spewing out more ash in 24 hours than Eyjafjoell did in three weeks, Grimsvoetn caused far fewer disruptions.

The eruption swiftly ended, and the number of flights grounded counted in the hundreds.

The study appears in the journal Nature Geoscience.

Note : The above story is based on materials provided by © 2014 AFP

Volcanic lightning recreated in the lab

Credit: B. Scheu

An LMU team has, for the first time, created volcanic lightning in the lab and captured it on film. The new findings may permit rapid characterization of ash clouds released by volcanic eruptions and improve forecasting of their behavior.
When the Icelandic volcano Eyjafjallajökull erupted in April 2010, launching a towering column of ash into the skies, the cloud was observed to be laced with lightning flashes. LMU volcanologists led by Professor Donald Dingwell, Director of the Department of Earth and Environmental Sciences at LMU, have now generated such volcanic lightning in the laboratory, as they report in a recent issue of the journal Geology. “Our experiments demonstrate that there is a relationship between the concentration of fine particles in the ash plume and the number of flashes produced,” says departmental researcher Dr. Corrado Cimarelli.

Turbulence and particle charging

The volcanologists performed their experiments with natural ash obtained from several volcanoes, including Eyjafjallajökull. The ash was loaded into a shock tube and subjected to the kinds of pressures found in the magma chambers of active volcanos just prior to an eruption. Upon sudden decompression, the ash is expelled vertically in a turbulent plume made up of a mixture of gas and solid particles of ash. And indeed, the researchers observe lightning flashes, on the order of tens of centimeters in length, within the column, where collision and fragmentation of ash particles leads to the creation of charged surfaces. When oppositely charged surfaces interact, the electrical energy is dissipated as lightning.

The team recorded the dynamics of the process with the help of high-speed cameras which can capture motions that are imperceptible to the naked eye. In addition, they measured the distribution of electrically charge using two antennas. Videos of the experiments are available on the website maintained by the Department of Earth and Environmental Sciences.

The new study confirms that the incidence of lightning is related to the relative amount of very fine particles in the plume. The smaller the particles, the larger the number of flashes observed. “That in turn implies that observations of volcanic lightning could allow one to deduce the concentration and size distribution of the ash particles released during an eruption. And that information is crucial for efforts to predict how the particles will behave in the atmosphere, and how they might affect air traffic,” says Corrado Cimarelli. – Everyone remembers the disruption caused to transatlantic and European flight schedules by the clouds of ash released during the eruption of Eyjafjallajökull in April 2010.

The new findings also contribute to a better understanding of the mechanisms that underlie the self-charging of dust particles that are subjected to turbulence. They are thus relevant not only to other atmospheric phenomena, such as sandstorms, but also to industrial processes that involve interactions between mobile streams of particulate matter.

Note : The above story is based on materials provided by Ludwig Maximilian University of Munich

Cylindrite

Locality: Trinacria Mine, Callipampa, Poopó Province, Oruro Department, Bolivia Dimensions: 2.9 cm x 2 cm x 1.2 cm “Courtesy of Rob Lavinsky, The Arkenstone, www.iRocks.com”

Chemical Formula: Pb3Sn4FeSb2S14
Locality: Poopo, in Oruro, Boliva.
Name Origin: From the Greek, kylindros, “cylinder.”

Cylindrite is a sulfosalt mineral containing tin, lead, antimony and iron with formula: Pb3Sn4FeSb2S14. It forms triclinic pinacoidal crystals which often occur as tubes or cylinders which are in fact rolled sheets. It has a black to lead grey metallic colour with a Mohs hardness of 2 to 3 and a specific gravity of 5.4.

It was first discovered in the Santa Cruz mine, Oruro Department, Bolivia in 1893. The name arises from its curious cylindrical crystal which it forms almost uniquely among minerals.

Physical Properties of Cylindrite

Cleavage: None
Color: Lead gray, Grayish black.
Density: 5.4 – 5.42, Average = 5.41
Diaphaneity: Opaque
Fracture: Malleable – Deforms rather than breaking apart with a hammer.
Hardness: 2.5 – Finger Nail
Luster: Metallic
Streak: black

Photos :

Cylindrite Santa Cruz mine, Poopó, Bolivia Specimen weight:93 gr. Crystal size:18 mm Overall size: 48mm x 35 mm x 35 mm Copyright © minservice
Cylindrite 2.4×2.0x1.4 cm Santa Cruz Mine, Poopo, Oruro, Bolivia Copyright © 2011 David K. Joyce Minerals
Cylindrite 7.0×5.7×5.4 cm Santa Cruz Mine, Poopo, Oruro, Bolivia Copyright © 2011 David K. Joyce Minerals
Santa Cruz Mine, Poopó town, Poopó Province, Oruro Department, Bolivia

Iconic Australasian Trees Found as Fossils in South America

Fossil of leafy Agathis tree branch. (Credit: Peter Wilf/Penn State)

Today in Australia they call it Kauri, in Asia they call it Dammar, and in South America it does not exist at all unless planted there. But 52 million years ago the giant coniferous evergreen tree known to botanists as Agathis thrived in the Patagonian region of Argentina, according to an international team of paleobotanists, who have found numerous fossilized remains there.

 

“These spectacular fossils reveal that Agathis is old and had a huge range that no one knew about — from Australia to South America across Antarctica,” said Peter Wilf, professor of geoscience, Penn State.

Agathis trees currently grow thousands of miles from Argentina, ranging from Sumatra to New Zealand. They often prefer mountain rainforests, where it is wet and warm all year round. They can grow as tall as 200 feet, but are usually between 130 and 150 feet at maturity. Economically, they are prized and heavily cut for their soft, workable wood. In the past, the Agathis resin, known as manila copal, was exploited for linoleum and varnishes, but synthetics replaced most of that use.

The researchers report in the current issue of American Journal of Botany that “Agathis was a dominant, keystone element of the Patagonian Eocene floras, alongside numerous other plant taxa that still associate with it in Australasia and Southeast Asia.”

“There is a fossil record of Agathis in Australia and New Zealand, where it still lives,” said Wilf. “However, Agathis fossils have never been found anywhere else until now, and they have never been as complete as these.”

Wilf and his colleagues work at two sites in Patagonia, Argentina: Laguna del Hunco that dates to the early Eocene at about 52.2 million years ago, and Río Pichileufú dating to about 47.7 million years ago.

“These sites were discovered in the 1920s and 1930s, but the remoteness of the locations and the hardness of the rock are why they hadn’t been investigated in detail before we started in 1999,” said Wilf. “Now, with modern amenities — satellite phones for example — and especially the presence of our partner institution, the Egidio Feruglio Museum, in the same region as the dig sites, recovering these fossils becomes much easier.”

Agathis grew in Patagonia when South America was part of the remainder of the southern supercontinent of Gondwana, composed of South America, Antarctica and Australia. Much earlier, India, Madagascar, New Zealand and Africa separated and moved north, but around the time of these fossils, South America was just beginning to part from Antarctica, which was not ice covered at the time.

“Agathis probably existed in all three areas, Australia, Antarctica and South America, at that time,” said Wilf. “Climate change in Antarctica — the cold and ice — killed them there, and a change to seasonal dryness in southern South America put an end to them in Patagonia.”

Subsequently, the trees, which are wind dispersed, moved away from the cooling south, and some left northward-moving Australia for southeast Asia, where they thrive except for human interference, but they no longer grow in cold, often dry, Patagonia.

Wilf ‘s team recovered not only leaves, but also numerous branches, pollen cones, seed cones and even a winged seed still attached to the cone. The various species of Agathis are usually identified by their pollen cones, so this is the first time that a fossil Agathis could be directly compared to trees growing today.

“We also went to Borneo and studied the most similar living relative of the fossil Agathis, a threatened species there,” said Wilf. “We collected DNA samples to better understand the fossil-modern relationship.”

According to the researchers, the Argentinian fossil Agathis clearly belongs to the same natural group as those living today up to almost 10,000 miles away in the tropical West Pacific.

“Agathis is a very dramatic example of survival via huge range shifts, from the far south to the tropics, in response to climate change and land movement over millions of years,” said Wilf. “It is not clear that Agathis can adapt to the severely more rapid human-induced pressures it is experiencing now from deforestation, selective logging and climate change.”

Also working on this research are Ignacio H. Escapa and Rubén Cúneo, Consejo Nacional de Investigaciones Científicas y Técnicas and Museo Paleontológico Egidio Feruglio, Chubut, Argentina; Robert M. Kooyman, National Herbarium of New South Wales, Sydney; Kirk R. Johnson, Smithsonian Institution; and Ari Iglesias, Consejo Nacional de Investigaciones Científicas y Técnicas and División Palontología, Universidad Nacional del Comahue, Río Negro, Argentina.

The National Science Foundation, the David and Lucile Packard Foundation, National Geographic Society,University of Pennsylvania Research Foundation and the Andrew W. Mellon Foundation supported this work.

Note : The above story is based on materials provided by Penn State. 

Massive Exoplanets May Be More Earth-Like Than Thought

This artist’s concept depicts Kepler-69c, a super-Earth-size planet in the habitable zone of a star like our sun, located about 2,700 light-years from Earth in the constellation Cygnus. (Credit: NASA Ames/JPL-Caltech)

Massive terrestrial planets, called “super-Earths,” are known to be common in our galaxy, the Milky Way. Now a Northwestern University astrophysicist and a University of Chicago geophysicist report the odds of these planets having an Earth-like climate are much greater than previously thought.

 

Nicolas B. Cowan and Dorian Abbot’s new model challenges the conventional wisdom which says super-Earths actually would be very unlike Earth — each would be a waterworld, with its surface completely covered in water. They conclude that most tectonically active super-Earths — regardless of mass — store most of their water in the mantle and will have both oceans and exposed continents, enabling a stable climate such as Earth’s.

Cowan is a postdoctoral fellow at Northwestern’s Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), and Abbot is an assistant professor in geophysical sciences at UChicago.

“Are the surfaces of super-Earths totally dry or covered in water?” Cowan said. “We tackled this question by applying known geophysics to astronomy.

“Super-Earths are expected to have deep oceans that will overflow their basins and inundate the entire surface, but we show this logic to be flawed,” he said. “Terrestrial planets have significant amounts of water in their interior. Super-Earths are likely to have shallow oceans to go along with their shallow ocean basins.”

In their model, Cowan and Abbot treated the intriguing exoplanets like Earth, which has quite a bit of water in its mantle, the rocky part that makes up most of the volume and mass of the planet. The rock of the mantle contains tiny amounts of water, which quickly adds up because the mantle is so large. And a deep water cycle moves water between oceans and the mantle. (An exoplanet, or extrasolar planet, is a planet outside our solar system.)

Cowan presented the findings at a press conference, “Windows on Other Worlds,” held Jan. 7 at the 223rd meeting of the American Astronomical Society (AAS) annual meeting in Washington, D.C.

He also will discuss the research at a scientific session to be held from 2 to 3:30 p.m. EST Wednesday, Jan. 8, at the AAS meeting (Potomac Ballroom D, Gaylord National Resort and Convention Center). The study will be published Jan. 20 in the Astrophysical Journal.

Water is constantly traded back and forth between the ocean and the rocky mantle because of plate tectonics, Cowan and Abbot said. The division of water between ocean and mantle is controlled by seafloor pressure, which is proportional to gravity.

Accounting for the effects of seafloor pressure and high gravity are two novel factors in their model. As the size of the super-Earths increase, gravity and seafloor pressure also go up.

“We can put 80 times more water on a super-Earth and still have its surface look like Earth,” Cowan said. “These massive planets have enormous seafloor pressure, and this force pushes water into the mantle.”

It doesn’t take that much water to tip a planet into being a waterworld. “If Earth was 1 percent water by mass, we’d all drown, regardless of the deep water cycle,” Cowan said. “The surface would be covered in water. Whether or not you have a deep water cycle really matters for planets that are one one-thousandth or one ten-thousandth water.”

The ability of super-Earths to maintain exposed continents is important for planetary climate. On planets with exposed continents, like Earth, the deep carbon cycle is mediated by surface temperatures, which produces a stabilizing feedback (a thermostat on geological timescales).

“Such a feedback probably can’t exist in a waterworld, which means they should have a much smaller habitable zone,” Abbot said. “By making super-Earths 80 times more likely to have exposed continents, we’ve dramatically improved their odds of having an Earth-like climate.”

Cowan and Abbot accede that there are two major uncertainties in their model: that super-Earths have plate tectonics and the amount of water Earth stores in its mantle.

“These are the two things we would like to know better to improve our model,” Cowan said. “Our model is a shot from the hip, but it’s an important step in advancing how we think about super-Earths.”

Note : The above story is based on materials provided by Northwestern University. The original article was written by Megan Fellman. 

Cyanotrichite

Locality: Hilarion area, Kamariza Mines (Kamareza Mines), Agios Konstantinos [St Constantine] (Kamariza), Lavrion District Mines, Lavrion District (Laurion; Laurium), Attikí Prefecture (Attica; Attika), Greece Field of View: 6 mm Copyright © Fritz Schreiber
Chemical Formula: Cu4Al2(SO4)(OH)12 · 2H2O
Locality: Moldava Noua (Moldawa, Új Moldova), Banat, Romania.
Name Origin: From the Greek, kyaneos, “blue” and triches, “hair,” hence, blue hair.

Cyanotrichite is a hydrous copper aluminium sulfate mineral with formula Cu4Al2(SO4)(OH)12 · 2H2O, also known as lettsomite. Cyanotrichite forms velvety radial acicular crystal aggregates of extremely fine fibers. It crystallizes in the orthorhombic system and forms translucent bright blue acicular crystal clusters or drusey coatings. The Mohs hardness is 2 and the specific gravity ranges from 2.74 to 2.95. Refractive indices are nα=1.588 nβ=1.617 nγ=1.655.

Occurrence and discovery

It is an oxidation product of primary copper mineralization in a weathering environment with abundant aluminium and sulfate. Associated minerals include brochantite, spangolite, chalcophyllite, olivenite, tyrolite, parnauite, azurite and malachite.

The main deposits are Cap la Garrone in the Var (France), Romania and Arizona (USA).

It was first described in 1839 from Moldova Nouă, Banat, Romania. The name is from Greek kyaneos for “blue” and triches for “hair” referring to the typical color and habit. Its earlier name, Lettsomite, is taken from the name of William Garrow Lettsom (1804–1887), co-author of the 1858 Manual of the Mineralogy of Great Britain and Ireland.

Physical Properties of Cyanotrichite

Cleavage: {???} Good
Color: Sky blue, Light blue, Dark blue.
Density: 2.74 – 2.95, Average = 2.84
Fracture: Uneven – Flat surfaces (not cleavage) fractured in an uneven pattern.
Hardness: 2 – Gypsum
Luminescence: Non-fluorescent.
Luster: Silky
Streak: pale blue

Photo

Locality: Grand View Mine (Last Chance Mine; No. 1 Pat claim 3591; No. 5 Pat claim 3592a; No. 4 Pat claim 3592a; Canyon Copper Mine; Grand Canyon Mine), Horseshoe Mesa, Grandview District, Coconino Co., Arizona, USA Dimensions: 3.8 cm x 3.7 cm x 1.2 cm “Courtesy of Rob Lavinsky, The Arkenstone, www.iRocks.com”
Locality: Grand View Mine (Last Chance Mine; No. 1 Pat claim 3591; No. 5 Pat claim 3592a; No. 4 Pat claim 3592a; Canyon Copper Mine; Grand Canyon Mine), Horseshoe Mesa, Grandview District, Coconino Co., Arizona, USA FOV: 20 x 17 mm Copyright © Michael C. Roarke
Locality: Hilarion area, Kamariza Mines (Kamareza Mines), Agios Konstantinos [St Constantine] (Kamariza), Lavrion District Mines, Lavrion District (Laurion; Laurium), Attikí Prefecture (Attica; Attika), Greece Field of View: 5 mm Copyright © Fritz Schreiber
Locality: Grand View Mine (Last Chance Mine; No. 1 Pat claim 3591; No. 5 Pat claim 3592a; No. 4 Pat claim 3592a; Canyon Copper Mine; Grand Canyon Mine), Horseshoe Mesa, Grandview District, Coconino Co., Arizona, USA FOV: 5mm. Copyright © Michael Clin

Neolithic mural may depict ancient eruption

This is the Hasan Dagi volcano. Credit: Janet C. Harvey

Volcanic rock dating suggests the painting of a Çatalhöyük mural may have overlapped with an eruption in Turkey according to results published January 8, 2014, in the open access journal PLOS ONE by Axel Schmitt from the University of California Los Angeles and colleagues from other institutions.

Scientists analyzed rocks from the nearby Hasan Dagi volcano in order to determine whether it was the volcano depicted in the mural from ~6600 BC in the Catalhöyük Neolithic site in central Turkey. To determine if Hasan Dagi was active during that time, scientists collected and analyzed volcanic rock samples from the summit and flanks of the Hasan Dagi volcano using (U-Th)/He zircon geochronology. These ages were then compared to the archeological date of the mural.

Volcanic rock textures and ages support the interpretation that residents of Çatalhöyük may have recorded an explosive eruption of Hasan Dagi volcano. The dating of the volcanic rock indicated an eruption around 6900 BC, which closely overlaps with the time the mural was estimated to have been painted in Çatalhöyük. The overlapping timeframes indicate humans in the region may have witnessed this eruption.

Alternative interpretations of the mural include the depiction of a leopard skin, consistent with other art at the Çatalhöyük site.

Schmitt adds, “We tested the hypothesis that the Çatalhöyük mural depicts a volcanic eruption and discovered a geological record consistent with this hypothesis. Our work also demonstrates that Hasan Dagi volcano has potential for future eruptions.”

Note : The above story is based on materials provided by Public Library of Science

Curite

Shinkolobwe Mine (Kasolo Mine), Shinkolobwe, Katanga Copper Crescent, Katanga (Shaba), Democratic Republic of Congo (Zaïre) © Stephan Wolfsried

Chemical Formula: Pb3(UO2)8O8(OH)6 · 3H2O
Locality: Shinkolobwe Mine (Kasolo Mine), Shinkolobwe, Katanga Copper Crescent, Katanga (Shaba), Democratic Republic of Congo (Zaïre)
Name Origin: Named for Pierre Curie (1859-1906) and Marie Curie-Sklodowska (1867 – 1934), French research team of radioactive minerals. Discoverd the element radium.

Curite is a lead uranium oxide mineral with formula: Pb3(UO2)8O8(OH)6 · 3H2O. It is named after the physicists Marie and Pierre Curie, who are both known for their work on radioactivity. The type locality is the Shinkolobwe Mine.

Physical Properties of Curite

Cleavage: {100} Good, {110} Good
Color: Yellow, Reddish orange, Brownish yellow.
Density: 7.19
Diaphaneity: Transparent to Translucent
Fracture: Brittle – Generally displayed by glasses and most non-metallic minerals.
Hardness: 4-5 – Fluorite-Apatite
Luster: Adamantine
Streak: orange

Photo

Locality: South Alligator River, West Arnhem Region, Northern Territory, Australia FOV: 2.16 mm Copyright © Matteo Chinellato
Locality: Shinkolobwe Mine (Kasolo Mine), Shinkolobwe, Katanga Copper Crescent, Katanga (Shaba), Democratic Republic of Congo (Zaïre) Picture width 3 mm. Copyright © Stephan Wolfsried
Curite, Metatorbernite Locality: Shinkolobwe Mine (Kasolo Mine), Shinkolobwe, Katanga Copper Crescent, Katanga (Shaba), Democratic Republic of Congo (Zaïre) Copyright © Collection and photo, Paul De Bond
Curite, Soddyite, Torbernite, Heterogenite Locality: Shinkolobwe Mine (Kasolo Mine), Shinkolobwe, Katanga Copper Crescent, Katanga (Shaba), Democratic Republic of Congo (Zaïre) Specimen size, 55 mm. Copyright © Collection and photo, Paul De Bondt

Mega-landslide in giant Utah copper mine may have triggered earthquakes

This is Figure 1 from K.L. Pankow et al. of megalandslide at the Bingham Canyon Mine, Utah. Landslide image copyright Kennecott Utah Copper. Credit: Seismic/Infrasound image by K.L. Pankow et al. Landslide image copyright Kennecott Utah Copper.

Landslides are one of the most hazardous aspects of our planet, causing billions of dollars in damage and thousands of deaths each year. Most large landslides strike with little warning—and thus geologists do not often have the ability to collect important data that can be used to better understand the behavior of these dangerous events. The 10 April 2013 collapse at Kennecott’s Bingham Canyon open-pit copper mine in Utah is an important exception.

Careful and constant monitoring of the conditions of the Bingham Canyon mine identified slow ground displacement prior to the landslide. This allowed the successful evacuation of the mine area prior to the landslide and also alerted geologists at the University of Utah to enable them to successfully monitor and study this unique event.

The landslide—the largest non-volcanic landslide in the recorded history of North America—took place during two episodes of collapse, each lasting less than two minutes. During these events about 65 million cubic meters of rock—with a total mass of 165 million tons—collapsed and slid nearly 3 km (1.8 miles) into the open pit floor.

In the January 2014 issue of GSA Today, University of Utah geologists, led by Dr. Kristine Pankow, report the initial findings of their study of the seismic and sound-waves generated by this massive mega-landslide. Pankow and her colleagues found that the landslide generated seismic waves that were recorded by both nearby seismic instruments, but also instruments located over 400 km from the mine. Examining the details of these seismic signals, they found that each of the two landslide events produced seismic waves equivalent to a magnitude 2 to 3 earthquake.

Interestingly, while there were no measurable seismic events prior to the start of the landslide, the team did measure up to 16 different seismic events with characteristics very much like normal “tectonic” earthquakes beneath the mine. These small (magnitude less than 2) earthquakes happened over a span of 10 days following the massive landslide and appear to be a rare case of seismic activity triggered by a landslide, rather than the more common case where an earthquake serves as the trigger to the landslide.

Later studies of both the seismic and sound waves produced by this landslide will allow Pankow and her team to characterize the failure and displacement of the landslide material in much more detail.

Note : The above story is based on materials provided by Geological Society of America

First Dinosaurs Identified from Saudi Arabia

Adaffa Theropod Tooth: This isolated tooth evidences the first identifiable carnivorous theropod dinosaur from the Arabian Peninsula. Abelisaurids like this specimen have been found in the ancient Gondwanan landmasses of North Africa, Madagascar and South America. (Credit: Photo by Maxim Leonov (Palaeontological Institute, Moscow) / Creative Commons Attribution, No Derivatives)

Dinosaur fossils are exceptionally rare in the Arabian Peninsula. An international team of scientists from Uppsala University, Museum Victoria, Monash University, and the Saudi Geological Survey have now uncovered the first record of dinosaurs from Saudi Arabia.What is now dry desert was once a beach littered with the bones and teeth of ancient marine reptiles and dinosaurs.

A string of vertebrae from the tail of a huge “Brontosaurus-like” sauropod, together with some shed teeth from a carnivorous theropod represent the first formally identified dinosaur fossils from Saudi Arabia, and were found in the north-western part of the Kingdom along the coast of the Red Sea.

The remains were discovered during excavations conducted by a team of scientists working under the auspices of the Saudi Geological Survey, Jeddah.

The dinosaur finds were recently published in the scientific journal PLOS ONE and jointly authored by participating researchers from Sweden, Australia and Saudi Arabia.

“Dinosaur fossils are exceptionally rare in the Arabian Peninsula, with only a handful of highly fragmented bones documented this far” says Dr Benjamin Kear, based at Uppsala University in Sweden and lead author of the study.

“This discovery is important not only because of where the remains were found, but also because of the fact that we can actually identify them. Indeed, these are the first taxonomically recognizable dinosaurs reported from the Arabian Peninsula” Dr Kear continues.

“Dinosaur remains from the Arabian Peninsula and the area east of the Mediterranean Sea are exceedingly rare because sedimentary rocks deposited in streams and rivers during the Age of Dinosaurs are rare, particularly in Saudi Arabia itself” says Dr Tom Rich from Museum Victoria in Australia.

When these dinosaurs were alive, the Arabian landmass was largely underwater and formed the north-western coastal margin of the African continent.

“The hardest fossil to find is the first one. Knowing that they occur in a particular area and the circumstances under which they do, makes finding more fossils significantly less difficult” says Dr Rich.

The teeth and bones are approximately 72 million years old.

Two types of dinosaur were described from the assemblage, a bipedal meat-eating abelisaurid distantly related to Tyrannosaurus but only about six metres long, and a plant-eating titanosaur perhaps up to 20 metres in length.

Similar dinosaurs have been found in North Africa, Madagascar and as far away as South America.

Note : The above story is based on materials provided by Uppsala Universitet. 

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