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Neptunite

Neptunite, Joaquinite 4.6×3.1×3.2 cm Gem Mine, San Benito Co., California, USA Copyright © David K. Joyce Minerals

Chemical Formula: Na2KLi(Fe2+,Mn2+)2Ti2(Si8O24)
Locality: Benitoite mine, San Benito, Co., California, USA.
Name Origin: Named for Neptune, the Roman god of the sea, because it was found with aegirine, named for the Scandinavian god of the sea.

Neptunite is a silicate mineral with the formula Na2KLi(Fe2+,Mn2+)2Ti2(Si8O24). With increasing manganese it forms a series with mangan-neptunite. Watatsumiite is the variety with vanadium replacing the titanium in the formula.

It was first described in 1893 for an occurrence in the Narssârssuk pegmatite of West Greenland. It is also found within natrolite veins in glaucophane schist within serpentinite in San Benito County, California, USA. It also occurs in Mont Saint-Hilaire, Quebec and in the Kola Peninsula of Russia.

The mineral is named for Neptune, Roman god of the sea because of its association with aegirine from Àgir, the Scandinavian sea-god.

The Gemological Institute of America (GIA) identified an 11.78-carat faceted specimen as neptunite based on Raman spectroscopy.

History

Discovery date : 1893
Town of Origin : NARNARSUK
Country of Origin: GROENLAND

Optical properties

Optical and misc. Properties: Translucide – Opaque
Refractive Index: from 1,69 to 1,73
Axial angle 2V : ~40°

Physical Properties

Cleavage: {110} Good
Color: Black, Red.
Density: 3.23
Diaphaneity: Translucent
Fracture: Conchoidal – Fractures developed in brittle materials characterized by smoothly curving surfaces, (e.g. quartz).
Hardness: 5-6 – Between Apatite and Orthoclase
Luminescence: Non-fluorescent.
Luster: Vitreous (Glassy)
Streak: brown

Photos :

Neptunite Dallas Mine, San Benito County, California, USA Miniature, 3.4 x 2.4 x 1.8 cm “Courtesy of Rob Lavinsky, The Arkenstone, www.iRocks.com”
Neptunite Dallas/Benitoite Gem Mine San Benito County California USA Size: 4.3 x 3.5 x 1.7 cm Weight: 16.2 g © SpiriferMinerals

Forging new ground in oil forensics

Researchers used comprehensive two-dimensional gas chromatography (GCxGC) in their oil spill forensics to measure levels of degradation in biomarkers. THe biomarkers here are shown inside the dotted line. Credit: Christoph Aeppli, Bigelow Laboratory for Ocean Sciences

Years after the 2010 Deepwater Horizon Oil spill, oil continues to wash ashore as oil-soaked “sand patties,” persists in salt marshes abutting the Gulf of Mexico, and questions remain about how much oil has been deposited on the seafloor. Scientists from Woods Hole Oceanographic Institution and Bigelow Laboratory for Ocean Sciences have developed a unique way to fingerprint oil, even after most of it has degraded, and to assess how it changes over time. Researchers refined methods typically used to identify the source of oil spills and adapted them for application on a longer time frame to successfully identify Macondo Well oil, years after the spill.

“We were looking at two questions: how could we identify the oil on shore, now four years after the spill, and how the oil from the spill was weathering over time,” explained Christoph Aeppli, Senior Research Scientist at Bigelow Laboratory for Ocean Sciences in East Boothbay, Maine, and lead author of the study reported in Environmental Science & Technology. Aeppli worked with his then-colleagues at Woods Hole Oceanographic Institution, and University of California, Santa Barbara on the investigation and report.

Researchers used comprehensive two-dimensional gas chromatography (GCxGC) in their oil spill forensics to measure levels of degradation in biomarkers. Biomarkers are molecular fossils. Each reservoir has specific amounts of different biomarkers, so oil biomarkers serve as identifiers much like human fingerprints. Biomarkers are usually recalcitrant in reservoirs, but when exposed for a long time to the environment, some are altered due to natural processes. Oil consists of tens of thousands of compounds, and many of them can be degraded by bacteria or broken down by sunlight. This research was designed to determine the resiliency of specific biomarkers and to see how they held up when exposed to environmental conditions on shore.

“We found that some biomarkers — homohopanes and triaromoatic steroids (TAS), specifically — degraded within a few years following the Deepwater Horizon spill,” said Chris Reddy, a scientist at Woods Hole Oceanographic Institution and co-author of the paper. “These biomarkers are not as resilient as once thought and they may provide a future window into determining how much, and how quickly, these oil components may linger in the environment when exposed to air, sunlight, and the elements.”

Researchers sought to determine the specific source of the biomarkers degradation. Through analysis of oil-soaked “sand patties” collected along the Gulf shore over a 28-month period, they found that most biomarker compounds were recalcitrant and could be used to identify DWH oil. Some biomarkers, however, degraded. “This knowledge is helping us improve our oil spill forensics. It is providing a foundation for better, longer-term identification techniques that account for exposure of oil to wind, waves, sunlight, and microbial degradation over long times,” added Aeppli.

Aeppli, Reddy and colleague Dave Valentine from UC Santa Barbara will apply this new oil fingerprinting technique to process tens of thousands of samples collected shortly after the DWH spill.

Note : The above story is based on materials provided by Bigelow Laboratory for Ocean Sciences.

Plate tectonics: Studies show movements of continents speeding up after slow ‘middle age’

The tectonic plates of the world were mapped in the second half of the 20th century. usgs

Two studies show that the movement rate of plates carrying Earth’s crust may not be constant over time. This could provide a new explanation for the patterns observed in the speed of evolution and has implications for the interpretation of climate models. The work is presented today at Goldschmidt 2014, the premier geochemistry conference taking place in Sacramento, California, USA.

Earth’s continental crust can be thought of as an archive of Earth’s history, containing information on rock formation, the atmosphere and the fossil record. However, it is not clear when and how regularly crust formed since the beginning of Earth history, 4.5 billion years ago.

Researchers led by Professor Peter Cawood, from the University of St. Andrews, UK, examined several measures of continental movement and geologic processes from a number of previous studies. They found that, from 1.7 to 0.75 billion years ago (termed Earth’s middle age), Earth appears to have been very stable in terms of its environment, with little in the way of crust building activity, no major fluctuations in atmospheric composition and few major developments seen in the fossil record. This contrasts markedly with the time periods either side of this, which contained major ice ages and changes in oxygen levels. Earth’s middle age also coincides with the formation of a supercontinent called Rodinia, which appears to have been stable throughout this time.

Professor Cawood suggests this stability may have been due to the gradual cooling of Earth’s crust over time. “Before 1.7 billion years ago, the Earth’s crust would have been substantially hotter, meaning that continental plate movement may have been governed by different rules to those that operate today,” said Professor Cawood. “0.75 billion years ago, the crust reached a point where it had cooled sufficiently to allow modern day plate tectonics to start working, in particular allowing subduction zones to form (where one plate of the crust moves under another). This increase in activity could have kick-started a myriad of changes including the break-up of Rodinia and changes to levels of key elements in the atmosphere and seas, which in turn may have induced evolutionary changes in the life forms present.”

This view is backed up by work from Professor Kent Condie from New Mexico Tech, USA, which suggests the movement rate of Earth’s crust is not constant but may be speeding up over time. Professor Condie examined how supercontinents assemble and break up. “Our results challenge the view that the rate of plate movement is stable over time,” said Professor Condie. “The interpretation of data from many other disciplines such as stable isotope geochemistry, palaeontology and paleoclimatology in part rely on the assumption that the movement rate of the Earth’s crust is constant.”

Results from these fields may now need to be re-examined in light of Condie’s findings. “We now urgently need to collect further data on critical time periods to understand more about the constraints on plate speeds and the frequency of collision between continental blocks,” concluded Professor Condie.

Note : The above story is based on materials provided by European Association of Geochemistry.

Nepheline

Nepheline with Schorlomite garnet Bou-Agrao Mt., Tamazeght complex, High Atlas Mts, Khenifra Province, Morocco Small Cabinet, 8.8 x 6.0 x 4.2 cm © irocks

Chemical Formula: (Na,K)AlSiO4
Locality: Magnet Cove, Magnet Cove, Ouachita Mountains, Hot Spring County, Arkansas, USA.
Name Origin: From the Greek nephele, “cloud,” because it becomes clouded when put in strong acid.

Nepheline, is a feldspathoid: a silica-undersaturated aluminosilicate, Na3KAl4Si4O16, that occurs in intrusive and volcanic rocks with low silica, and in their associated pegmatites.

Nepheline crystals are rare and belong to the hexagonal system, usually having the form of a short, six-sided prism terminated by the basal plane. The unsymmetrical etched figures produced artificially on the prism faces indicate, however, that the crystals are hemimorphic and tetartohedral, the only element of symmetry being a polar hexad axis. It is found in compact, granular aggregates, and can be white, yellow, gray, green, or even reddish (in the eleolite variety). The hardness is 5.5 – 6, and the specific gravity 2.56 – 2.66. It is often translucent with a greasy luster.

History

Discovery date : 1801
Town of Origin : MONTE SOMMA, MT. VESUVE (VOLCAN), NAPLES, CAMPANIE
Country of Origin : ITALIE

Optical properties

Optical and misc. Properties: Transparent –  Opaque –  Translucide
Refractive Index: from 1,52 to 1,54

Physical Properties

Cleavage: {1010} Poor
Color: White, Gray, Brown, Brownish gray, Reddish white.
Density: 2.55 – 2.65, Average = 2.59
Diaphaneity: Transparent to translucent to opaque
Fracture: Sub Conchoidal – Fractures developed in brittle materials characterized by semi-curving surfaces.
Hardness: 6 – Orthoclase
Luminescence:     Non-fluorescent.
Luster: Vitreous – Greasy
Streak: white

Photos :

Nepheline syenite of Tanguá, Rio de Janeiro, Brazil. ©  Motoki et al., 2011a
Nepheline, Schorlomite Locality: Jebel Bou-Agrao, Tamazeght Mountain Range, Khénifra Province, Meknès-Tafilalet Region, Morocco Dimensions: 6 cm x 4.4 cm x 3.8 cm Photo Copyright © Rob Lavinsky & irocks
Nosean, Sodalite, Nepheline, Phlogopite, Calcite, Pyrite Locality: Nepheline occurrence, Ladjuar Medam (Lajur Madan; Lapis-lazuli Mine; Lapis-lazuli deposit), Sar-e Sang (Sar Sang; Sary Sang), Koksha Valley (Kokscha Valley; Kokcha Valley), Khash & Kuran Wa Munjan Districts, Badakhshan Province (Badakshan Province; Badahsan Province), Afghanistan Photo Copyright © Gary Ansell

Finlay River

Map of the Finlay River

The Finlay River is a 402 km long river in north-central British Columbia flowing north and thence south from Thutade Lake in the Omineca Mountains to Williston Lake, the impounded waters of the Peace River formed by the completion of the W.A.C. Bennett Dam in 1968. Prior to this, the Finlay joined with the Parsnip River to form the Peace. The headwaters of the Finlay at Thutade Lake are considered the ultimate source of the Mackenzie River. Deserters Canyon is located just north of Williston Lake.

The Finlay drains an area of 43,000 square kilometres and discharges at a mean rate of 600 cubic metres per second. Major tributaries of the Finlay include the Ospika, Ingenika, Warneford, Fox, Toodoggone, and Firesteel Rivers (the Ospika now enters Lake Williston directly, however). Located in a remote part of the province, there are no population centres along the river, however, there is a small First Nations community, Fort Ware, located at the junction of the Finlay and Warneford. Tatlatui Provincial Park protects the area of the Tatlatui Range, where Thutade Lake is located.
Map of the Stikine Territory. The line of the Finlay River is the southeast boundary of the territory, which was absorbed into the Colony of British Columbia in 1863.

The Finlay River is named for the explorer John Finlay, who travelled a short way up the river in 1797. The first European to journey its length to its source was the fur trader and explorer Samuel Black in 1824. The river was the eastern half of the northern boundary of the Colony of British Columbia at the time of its creation in 1858, north of which was the North-Western Territory; the western half of the boundary was the Nass River and from 1862 to 1863 it was briefly the southern boundary of the Stickeen Territories (Stikine Territory) which had been formed from the North-Western Territory in response to the Peace and Stikine Gold Rushes and which was amalgamated with the Colony of British Columbia in the following year.

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

Subseafloor bacteria survive by over-activating DNA-repair and antibiotic target genes

Photomicrographs of a subseafloor thermophile isolated from deep-sea hydrothermal vent fluids. This organism eats sulfur and hydrogen and fixes its own carbon from carbon dioxide. (A, B) Scanning electron micrographs, and (C, D) transmission electron micrographs thin sections. Image courtesy of Julie Huber.

The subseafloor is home to over 1/3 of the bacteria on the planet, but up until recently it was unclear if this huge microbial biosphere was alive and dividing. Now the same group that demonstrated this activity has shown that bacteria from the hostile sea-floor environment have adapted by over-activating stress response and DNA-repair mechanisms, to cope with the harsh conditions.

 

Subseafloor sediment contains Earth’s largest habitat for microbial life — over 1/3 of all the planets microbial biomass. By drilling deep into the sea floor and taking samples, it can be proven that the subseafloor contains a variety of microbial lifeforms, but it’s only in the last year that researchers have proven that sea floor microbes are actually active in in their natural sea-bed situation — it is difficult to analyse lifeforms which live hundreds of metres below the sea surface because of their low activity levels. A group of researchers at Woods Hole Oceanographic Institute and University of Delaware developed techniques to analyse the messenger

RNA (mRNA) molecules produced by subseafloor microbes. Unlike DNA, which is a fairly robust molecule that can survive intact for thousands of years under certain conditions, mRNA (messenger RNA) has a short half-life. It is produced by cells, which are “turning on” genes, so it is an indication that genes are active. This means that mRNA can be used as evidence (a proxy) for present biological activity.

Lead researcher William Orsi said: “This is the largest microbial biosphere on Earth, composed of cells living deep beneath the surface. We have recently shown for the first time that these cells, the “deep biosphere,” are actually dividing and not in a dormant state. This means that the deep biosphere is active and due to its sheer size likely plays an important role in global elemental cycles over geological timescales.” Now in a presentation to the Goldschmidt conference in Sacramento, California, Dr Orsi will detail just how these seabed bacteria had managed to survive in such an inhospitable environment.

“It’s a really difficult environment to study, so understanding how microbes survive there has been a puzzle” he said, “but we have discovered that they ramp-up some coping mechanisms which have helped them adapt to this stressful environment, where they exist under high pressure and are starved of nutrients.”

The group sampled drill cores from the continental shelf off the coast of Peru. They compared gene expression at several depths spanning 5-159 meters below the seafloor. They found that the expression of DNA repair genes, such as recA, increases with the amount of time the microbes have been buried in the seafloor.

Dr Orsi continued: “Subseafloor microbes have adapted to live in especially harsh conditions. We found that they significantly overexpress genes involved in cellular stress responses like recA. This gene is a central to the bacterial “SOS response,” which is a way bacteria cope with many different environmental stressors including antibiotics. We have found that subseafloor microbes increasingly express this gene with time after they become “buried alive” in the subseafloor.”

“High-throughput omics techniques are proving to have a range of applications in sedimentary systems. For example, marine sedimentary paleogenomics is a new field, which is opening windows into the past effects of climate on marine life. Dr Marco Coolen is the leader of this new field, and we worked together to analyse ancient plankton DNA from the Black Sea. We showed that it opened to the oceans around 9,600 years ago and that historical large-scale climate changes had a significant effect on marine plankton. These techniques are difficult, but they can tell us how biology responds to climate changes over geological timescales. Looking into the past can help us predict the future effects of climate change on marine life.”

Note : The above story is based on materials provided by European Association of Geochemistry.

Nagyagite

Nagyágite Locality: Nagyag, Sacarimb, Romania Size: small cabinet, 7.5 x 4.6 x 3.7 cm © irocks

Chemical Formula: Pb5Au(Te,Sb)4S5-8
Locality: Nagyag mine (now Sacaramb), Romania.
Name Origin: Named after the locality.

Nagyágite (Pb5Au(Te,Sb)4S5-8) is a rare sulfide mineral with known occurrence associated with gold ores. Nagyágite crystals are opaque, monoclinic and dark grey to black coloured.

It was first described in 1845 for an occurrence at the type locality of the Nagyág mine, Săcărâmb, Hunedoara County, Romania.

It occurs in gold–tellurium epithermal hydrothermal veins. Minerals associated with nagyágite include: altaite, petzite, stutzite, sylvanite, tellurantimony, coloradoite, krennerite, native arsenic, native gold, proustite, rhodochrosite, arsenopyrite, sphalerite, tetrahedrite, calaverite, tellurobismuthite, galena and pyrite.

History

Discovery date : 1845
Town of Origin: SACARAMB (NAGYAG), COMTE DE HUNEDOARA, TRANSYLVANIE
Country of Origin: ROUMANIE

Optical properties

Optical and misc. Properties : Opaque
Reflective Power: 37,5-41,5% (580)

Physical Properties

Cleavage: {010} Perfect
Color: Lead gray, Black.
Density: 7.5
Diaphaneity: Opaque
Fracture: Hackly – Jagged, torn surfaces, (e.g. fractured metals).
Hardness: 1.5-2 – Talc-Gypsum
Luminescence: Non-fluorescent.
Luster: Metallic
Magnetism: Nonmagnetic
Streak: gray black

Photos :

Nagyagite Location: Sacaramb (Nagyag), Romania. Scale: Crystal size 1 cm. Copyright: © John Veevaert
Nagyágite and Rhodochrosite Locality: Sacarîmb (Nagyág), Thunedoara, Transylvania, Romania (Type Locality for Nagyágite) Overall Size: 4x3x3 cm Crystals: 5-15 mm © JohnBetts-FineMinerals

New fossil find pinpoints the origin of jaws in vertebrates

Left: This is an illustration of Metaspriggina swimming. Drawing by: Marianne Collins. © Conway Morris and Caron. Right: This is a fossil of Metaspriggina from Marble Canyon — head to the left with two eyes, and branchial arches at the top. Photo by: Jean-Bernard Caron © ROM. Credit: Left: Drawing by Marianne Collins / Copyright Conway Morris and Caron. Right: Photo by Jean-Bernard Caron / Copyright ROM.

A major fossil discovery in Canada sheds new light on the development of the earliest vertebrates, including the origin of jaws, the first time this feature has been seen so early in the fossil record.
A key piece in the puzzle of the evolution of vertebrates has been identified, after the discovery of fossilised fish specimens, dating from the Cambrian period (around 505 million years old), in the Canadian Rockies. The fish, known as Metaspriggina, shows pairs of exceptionally well-preserved arches near the front of its body. The first of these pairs, closest to the head, eventually led to the evolution of jaws in vertebrates, the first time this feature has been seen so early in the fossil record.

Fish fossils from the Cambrian period are very rare and usually poorly preserved. This new discovery shows in unprecedented detail how some of the earliest vertebrates developed — the starting point of a story which led to animals such as later fish species, but also dinosaurs and mammals such as horses and even ourselves. The findings are published in the 11 June edition of the journal Nature.

Fossils of Metaspriggina were recovered from several locations including the Burgess Shale site in Canada’s Rocky Mountains, one of the richest Cambrian fossil deposits in the world. These fossils shed new light on the Cambrian ‘explosion’, a period of rapid evolution starting around 540 million years ago, when most major animal phyla originated.

Previously, only two incomplete specimens of Metaspriggina had been identified. During expeditions conducted by the Royal Ontario Museum in 2012, 44 new Burgess Shale fossils were collected near Marble Canyon in Kootenay National Park in British Columbia, which provide the basis for this study. Researchers from the University of Cambridge and the Royal Ontario Museum/University of Toronto used these fossils, along with several more specimens from the eastern United States, to reclassify Metaspriggina as one of the first vertebrates.

The fossils, which date from 505 million years ago, also show clearly for the first time how a series of rod-like structures, known as the gill or branchial arches, were arranged in the earliest vertebrates. These arches have long been known to have played a key role in the evolution of vertebrates, including the origin of jaws, and some of the tiny bones in the ear which transmit sound in mammals. Until now, however, a lack of quality fossils has meant that the arrangement of these arches in the first vertebrates had been hypothetical.

Vertebrates first appear in the fossil record slightly earlier than these finds, but pinpointing exactly how they developed is difficult. This is because fossils of such animals are rare, incomplete and open to varying interpretations, as they show soft tissues which are difficult to identify with complete certainty.

The new fossils of Metaspriggina are remarkably well-preserved. The arrangement of the muscles shows these fish were active swimmers, not unlike a trout, and the animals saw the world through a pair of large eyes and sensed their surrounding environment with nasal structures.

“The detail in this Metaspriggina fossil is stunning,” said lead author Professor Simon Conway Morris of Cambridge’s Department of Earth Sciences. “Even the eyes are beautifully preserved and clearly evident.”

But it is the branchial arches which makes this discovery so important. Previously, they were thought to exist as a series of single arches, but Metaspriggina now shows that they in fact existed in pairs. The anteriormost pair of arches is also slightly thicker than the remainder, and this subtle distinction may be the very first step in an evolutionary transformation that in due course led to the appearance of the jaw. “Once the jaws have developed, the whole world opens,” said Professor Conway Morris. “Having a hypothetical model swim into the fossil record like this is incredibly gratifying.”

Reference:
Simon Conway Morris, Jean-Bernard Caron. A primitive fish from the Cambrian of North America. Nature, 2014; DOI: 10.1038/nature13414

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

Cracks in Pluto’s moon could indicate it once had an underground ocean

This artist concept shows Pluto and some of its moons, as viewed from the surface of one of the moons. Pluto is the large disk at center. Charon is the smaller disk to the right. Credit: NASA, ESA and G. Bacon (STScI)

If the icy surface of Pluto’s giant moon Charon is cracked, analysis of the fractures could reveal if its interior was warm, perhaps warm enough to have maintained a subterranean ocean of liquid water, according to a new NASA-funded study.
Pluto is an extremely distant world, orbiting the sun more than 29 times farther than Earth. With a surface temperature estimated to be about 380 degrees below zero Fahrenheit (around minus 229 degrees Celsius), the environment at Pluto is far too cold to allow liquid water on its surface. Pluto’s moons are in the same frigid environment.

Pluto’s remoteness and small size make it difficult to observe, but in July of 2015, NASA’s New Horizons spacecraft will be the first to visit Pluto and Charon, and will provide the most detailed observations to date.

“Our model predicts different fracture patterns on the surface of Charon depending on the thickness of its surface ice, the structure of the moon’s interior and how easily it deforms, and how its orbit evolved,” said Alyssa Rhoden of NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “By comparing the actual New Horizons observations of Charon to the various predictions, we can see what fits best and discover if Charon could have had a subsurface ocean in its past, driven by high eccentricity.” Rhoden is lead author of a paper on this research now available online in the journal Icarus.

Some moons around the gas giant planets in the outer solar system have cracked surfaces with evidence for ocean interiors — Jupiter’s moon Europa and Saturn’s moon Enceladus are two examples.

As Europa and Enceladus move in their orbits, a gravitational tug-of-war between their respective parent planets and neighboring moons keeps their orbits from becoming circular. Instead, these moons have eccentric (slightly oval-shaped) orbits, which raise daily tides that flex the interior and stress the surface. It is thought that tidal heating has extended the lifetimes of subsurface oceans on Europa and Enceladus by keeping their interiors warm.

In Charon’s case, this study finds that a past high eccentricity could have generated large tides, causing friction and surface fractures. The moon is unusually massive compared to its planet, about one-eighth of Pluto’s mass, a solar system record. It is thought to have formed much closer to Pluto, after a giant impact ejected material off the planet’s surface. The material went into orbit around Pluto and coalesced under its own gravity to form Charon and several smaller moons.

Initially, there would have been strong tides on both worlds as gravity between Pluto and Charon caused their surfaces to bulge toward each other, generating friction in their interiors. This friction would have also caused the tides to slightly lag behind their orbital positions. The lag would act like a brake on Pluto, causing its rotation to slow while transferring that rotational energy to Charon, making it speed up and move farther away from Pluto.

“Depending on exactly how Charon’s orbit evolved, particularly if it went through a high-eccentricity phase, there may have been enough heat from tidal deformation to maintain liquid water beneath the surface of Charon for some time,” said Rhoden. “Using plausible interior structure models that include an ocean, we found it wouldn’t have taken much eccentricity (less than 0.01) to generate surface fractures like we are seeing on Europa.”

“Since it’s so easy to get fractures, if we get to Charon and there are none, it puts a very strong constraint on how high the eccentricity could have been and how warm the interior ever could have been,” adds Rhoden. “This research gives us a head start on the New Horizons arrival — what should we look for and what can we learn from it. We’re going to Pluto and Pluto is fascinating, but Charon is also going to be fascinating.”

Based on observations from telescopes, Charon’s orbit is now in a stable end state: a circular orbit with the rotation of both Pluto and Charon slowed to the point where they always show the same side to each other. Its current orbit is not expected to generate significant tides, so any ancient underground ocean may be frozen by now, according to Rhoden.

Since liquid water is a necessary ingredient for known forms of life, the oceans of Europa and Enceladus are considered to be places where extraterrestrial life might be found. However, life also requires a useable energy source and an ample supply of many key elements, such as carbon, nitrogen, and phosphorus. It is unknown if those oceans harbor these additional ingredients, or if they have existed long enough for life to form. The same questions would apply to any ancient ocean that may have existed beneath the icy crust of Charon.

This research was funded by the NASA Postdoctoral Program at the NASA Goddard Space Flight Center, administered by Oak Ridge Associated Universities, and NASA Headquarters through the Science Innovation Fund.

Journal Reference:

Alyssa Rose Rhoden, Wade Henning, Terry A. Hurford, Douglas P. Hamilton. The interior and orbital evolution of Charon as preserved in its geologic record. Icarus, 2014; DOI: 10.1016/j.icarus.2014.04.030

Note : The above story is based on materials provided by NASA/Goddard Space Flight Center.

Nadorite

Nadorite Djebel Debar, Hamman, Meskhootine, Constantine Province, Algeria (TYPE LOCALITY) Miniature, 4.7 x 2.9 x 2.7 cm “Courtesy of Rob Lavinsky, The Arkenstone, www.iRocks.com”

Chemical Formula: PbSbClO2
Locality: Djebel Nador, Constantine, Algeria.
Name Origin: Named for the locality

Nadorite is a mineral with the chemical formula PbSbClO2. It crystallizes in the orthorhombic crystal system and is brown, brownish-yellow or yellow in colour, with a white or yellowish-white streak.

Nadorite is named after Djebel Nador in Algeria, where it was first identified in 1870. Djebel Nador and Djebel Debbar (both in the Constantine Province of Algeria) are its co-type localities.

History

Discovery date : 1870
Town of Origin: DJEBEL NADOR ET DJEBEL DEBAR, QACENTINA (CONSTANTINE)
Country of Origin: ALGERIE

Optical properties

Optical and misc. Properties: Translucide
Refractive Index: from 2,30 to 2,40
Axial angle 2V : LARGE

Physical Properties

Cleavage: {010} Perfect
Color:     Brown, Brownish yellow, Grayish brown, Yellow.
Density: 7.02
Diaphaneity: Translucent
Fracture: Brittle – Generally displayed by glasses and most non-metallic minerals.
Hardness: 3.5-4 – Copper Penny-Fluorite
Luster: Adamantine – Resinous
Streak: yellow white

Photos:

Nadorite Locality: Djebel Nador, Constantine Province, Algeria (Locality at mindat.org) Size: miniature, 4.1 x 3.8 x 3.2 cm “Courtesy of Rob Lavinsky, The Arkenstone, www.iRocks.com”
Bindheimite replacing Nadorite Djebel Nador, Constantine Province, Algeria 60mm x 35mm x 20mm © Weinrich Minerals

New hi-tech approach to studying sedimentary basins

A radical new approach to analysing sedimentary basins also harnesses technology in a completely novel way. An international research group, led by the University of Sydney, will use big data sets and exponentially increased computing power to model the interaction between processes on the earth’s surface and deep below it in ‘five dimensions’.

As announced by the Federal Minister for Education today, the University’s School of Geosciences will lead the Basin GENESIS Hub that has received $5.4 million over five years from the Australian Research Council (ARC) and industry partners.

The multitude of resources found in sedimentary basins includes groundwater and energy resources. The space between grains of sand in these basins can also be used to store carbon dioxide.

“This research will be of fundamental importance to both the geo-software industry, used by exploration and mining companies, and to other areas of the energy industry,” said Professor Dietmar Müller, Director of the Hub, from the School of Geosciences.

“The outcomes will be especially important for identifying exploration targets in deep basins in remote regions of Australia. It will create a new ‘exploration geodynamics’ toolbox for industry to improve estimates of what resources might be found in individual basins.”

Sedimentary basins form when sediments eroded from highly elevated regions are transported through river systems and deposited into lowland regions and continental margins. The Sydney Basin is a massive basin filled mostly with river sediments that form Hawkesbury sandstone. It is invisible to the Sydney population living above it but has provided building material for many decades.

“Previously the approach to analysing these basins has been based on interpreting geological data and two-dimensional models. We apply infinitely more computing power to enhance our understanding of sedimentary basins as the product of the complex interplay between surface and deep Earth processes,” said Professor Müller.

Associate Professor Rey, a researcher at the School of Geosciences and member of the Hub said, “Our new approach is to understand the formation of sedimentary basins and the changes they undergo, both recently and over millions to hundreds of millions of years, using computer simulations to incorporate information such as the evolution of erosion, sedimentary processes and the deformation of the earth’s crust.”

The researchers will incorporate data from multiple sources to create ‘five-dimensional’ models, combining three-dimensional space with the extra dimensions of time and estimates of uncertainty.

The modelling will span scales from entire basins hundreds of kilometres wide to individual sediment grains.

Key geographical areas the research will focus on are the North-West shelf of Australia, Papua New Guinea and the Atlantic Ocean continental margins.

The Hub’s technology builds upon the exponential increase in computational power and the increasing amount of available big data (massive data sets of information). The Hub will harness the capacity of Australia’s most powerful computer, launched in 2013.

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

Directionality of crystal elasticity offers explanation for variable seismic character of the inner Earth

Figure 1: The Earth consists of a surficial crust, a hot, viscous mantle of silicate minerals, a liquid outer core of iron and nickel, and a solid inner core. The D” layer occurs just above the core–mantle boundary. Credit: Alfred Baron, RIKEN SPring-8 Center

Seismic studies enable geoscientists to map the Earth’s internal structure. Certain seismic observations, however, remain puzzling, such as the unexpected spatial variability in the speed of seismic waves in a thin zone called the D′′ layer at the boundary between the core and mantle (Fig. 1).
Alfred Baron who leads the Materials Dynamics Laboratory at the RIKEN SPring-8 Center, along with Akira Yoneda of Okayama University and colleagues, have now found that these observations can be explained by the structure and orientation of microcrystals that comprise the D′′ layer.

The D′′ layer is composed mainly of magnesium silicate (MgSiO3) microcrystals with a post-perovskite (pPv) structure. Seismological studies have shown that in the D′′ layer beneath the rim of the Pacific Ocean, horizontal shear waves travel faster than vertical shear waves. Beneath the central Pacific Ocean, however, the relative speeds differ, and underneath the Atlantic Ocean they become equal.

The speed of shear waves through a crystal is related to the crystal’s elasticity. The researchers therefore measured the elasticity of microcrystals with the pPv structure. As pPv-MgSiO3 is unstable at ambient pressure, a more stable mineral with the same crystal structure, pPv-calcium iridate (CaIrO3), was studied. “Even that easier experiment is challenging,” says Baron, “as the very small crystals of CaIrO3 are not amenable to most methods of sound velocity measurement.” Fortunately, such measurements are possible using the inelastic x-ray scattering (IXS) spectrometer built by Baron and his colleagues at the SPring-8 synchrotron radiation facility.

Applying an analysis technique developed by co-author Hiroshi Fukui, the researchers were able to measure the different speeds that shear waves travel through pPv-CaIrO3. The results indicate that the elasticity of the pPv structure is strongly directional, suggesting that the different shear wave velocities observed for the D′′ layer are due to regional differences in the predominant orientation of the microcrystals in the layer.

To explain the observed variation, the researchers suggest that when a slab of material moves downward beneath the Pacific rim, it transforms into pPv-MgSiO3 with a crystallographic orientation that allows horizontal shear waves to travel faster than vertical shear waves. As the slab moves under the central Pacific Ocean, it deforms, leading to a change in crystal orientation and a change in the relative seismic velocities.

Baron’s laboratory is now using the IXS technique to determine the speed of sound waves in polycrystalline materials and liquid iron alloys under extreme conditions similar to those of the Earth’s core.

More information:
Yoneda, A., Fukui, H., Xu, F., Nakatsuka, A., Yoshiasa, A., Seto, Y., Ono, K., Tsutsui, S., Uchiyama, H. & Baron, A. Q. R. “Elastic anisotropy of experimental analogues of perovskite and post-perovskite help to interpret D” diversity.” Nature Communications 5, 3453 (2014). DOI: 10.1038/ncomms4453

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

Muscovite

Fluorapatite with Muscovite Chumar Bakhoor, Hunza Valley, Gilgit District, Gilgit-Baltistan, Pakistan Size: 8.5 x 5.0 x 5.0 cm © Dan Weinrich

Chemical Formula: KAl2(AlSi3O10)(OH)2
Locality: Common world wide.
Name Origin: From Muscovy glass, alluding to the Russian province of Muscovy.

Muscovite  is a phyllosilicate mineral of aluminium and potassium . It has a highly-perfect basal cleavage yielding remarkably-thin laminæ (sheets) which are often highly elastic. Sheets of muscovite 5×3 m have been found in Nellore, India.

Muscovite has a Mohs hardness of 2–2.25 parallel to the [001] face, 4 perpendicular to the [001] and a specific gravity of 2.76–3. It can be colorless or tinted through grays, browns, greens, yellows, or (rarely) violet or red, and can be transparent or translucent. It is anisotropic and has high birefringence. Its crystal system is monoclinic. The green, chromium-rich variety is called fuchsite; mariposite is also a chromium-rich type of muscovite.

Muscovite is the most common mica, found in granites, pegmatites, gneisses, and schists, and as a contact metamorphic rock or as a secondary mineral resulting from the alteration of topaz, feldspar, kyanite, etc. In pegmatites, it is often found in immense sheets that are commercially valuable. Muscovite is in demand for the manufacture of fireproofing and insulating materials and to some extent as a lubricant.

The name muscovite comes from Muscovy-glass, a name given to the mineral in Elizabethan England due to its use in medieval Russia as a cheaper alternative to glass in windows. This usage became widely known in England during the sixteenth century with its first mention appearing in letters by George Turberville, the secretary of England’s ambassador to the Russian tzar Ivan the Terrible, in 1568.

History

Discovery date : 1850

Optical properties

Optical and misc. Properties: Transparent – Translucent
Refractive Index : from 1,55 to 1,61
Axial angle 2V : 30-47°

Physical Properties

Cleavage: {001} Perfect
Color:     White, Gray, Silver white, Brownish white, Greenish white.
Density: 2.77 – 2.88, Average = 2.82
Diaphaneity: Transparent to translucent
Fracture: Brittle – Sectile – Brittle fracture with slightly sectile shavings possible.
Hardness: 2-2.5 – Gypsum-Finger Nail
Luminescence: Non-fluorescent.
Luster: Vitreous (Glassy)
Streak: white

Photos :

Muscovite, Albite (Var: Cleavelandite) Locality: Divino das Laranjeiras, Doce valley, Minas Gerais, Brazil Dimensions: 6 cm x 5.3 cm x 3.9 cm Photo Copyright © Rob Lavinsky & irocks
Brazilianite on Muscovite Corrego Frio, Minas Gerais, Brazil Miniature, 4.9 x 4.3 x 2 cm © irocks
Cassiterite on Muscovite Aracuai, Minas Gerais, Brazil Small Cabinet, 6.9 x 5.1 x 3.5 cm © irocks
Apatite-CaF and muscovite Zé Pinto prospect, Minas Gerais, Brazil Specimen weight:358 gr. Crystal size:32 mm Overall size: 130mm x 130 mm x 85 mm © minservice
Cassiterite with Muscovite Huya deposit, Mt Xuebaoding, Pingwu Co., Mianyang Prefecture, Sichuan Province, China Size: 11.5 x 9.5 x 8.5 cm (cabinet) © danweinrich
Arsenopyrite-Marcasite with Muscovite Minas da Panasqueira, Aldeia de São Francisco de Assis, Covilhã, Castelo Branco, Centro  Portugal (1987-2013) Specimen size: 5.5 × 5.4 × 3.7 cm = 2.2” × 2.1” × 1.5” Main crystal size: 1.5 × 1 cm = 0.6” × 0.4” © Fabre Minerals

Why Diplodocus did not put all her eggs in one basket

Model diplodocus. Credit: © Katja Xenikis / Fotolia

If you thought the largest dinosaurs to have walked the Earth produced the biggest eggs, you’d be mistaken. Scientists have discovered that both individual egg size and clutch size for the sauropods — which includes Diplodocus — were a lot smaller than might be expected for such enormous creatures.

A team of scientists have suggested reasons why the largest dinosaurs ever to have walked the Earth produced smaller eggs than might be expected.

One of the defining characteristics of the dinosaurs was their vast size, and the sauropods — a suborder of dinosaurs which includes the famous Diplodocus — were the largest of all.

Yet scientists have been puzzled at the relatively small size of sauropod eggs. Both individual egg size and clutch size are smaller than might be expected for such enormous creatures, relative to modern egg-laying animals.

Researchers have now concluded that the substantial incubation time required for sauropod embryos to develop and hatch may have been an important constraint and that this could explain the small individual size of sauropod eggs.

The findings are published in the summer 2014 issue of the Paleontological Society’s journal, Paleobiology. The team, which included biologists from the University of Lincoln, UK, and George Mason University, Virginia, US, with lead researcher Professor Graeme Ruxton from the University of St Andrews, used data from modern birds and reptiles to investigate factors affecting clutch size in this group of dinosaurs.They estimated that the time from laying to hatching of eggs, which were incubated in underground nests, was between 65 and 82 days.

This long incubation time increases the risk of predation, which coupled with the relatively low temperatures expected in the nest, may have been a significant factor in limiting the egg and clutch size.

Having larger eggs than are in the fossil record may have been advantageous because of larger hatchling size but this may have been outweighed by the increased risk of predation during the egg stage.

Dr Charles Deeming, from the School of Life Sciences, University of Lincoln, UK, said: “We think that a long incubation period of sauropods is likely to have led to very high mortality through predation. We suggest that the females laid their eggs in small clutches, possibly in different nesting sites, as an adaptive strategy to mitigate the high predation risk associated with long time of exposure in the egg stage.”

Professor Ruxton, from the School of Biology at the University of St Andrews, added: “The living bird with the largest eggs, the ostrich, has to incubate its eggs for 42 days; during which time many eggs are lost to predators. An ostrich weighs about 100kg and lays a 1.5kg egg; a sauropod dinosaur might be 50 times heavier than an adult ostrich but its eggs were only a little heavier than an ostrich egg. Some people might find it a bit disappointing that giant dinosaurs didn’t lay equally giant eggs — but it’s very satisfying to think that we might finally understand why.”

There may also have been a finite limit to the period over which environmental temperatures are high enough for egg development.

The team believe their conclusions could be extended to other groups of dinosaurs.

Journal Reference:

Graeme D. Ruxton, Geoffrey F. Birchard, D. Charles Deeming. Incubation time as an important influence on egg production and distribution into clutches for sauropod dinosaurs. Paleobiology, 2014; 40 (3): 323 DOI: 10.1666/13028

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

Scientists discover link between climate change and ocean currents over 6 million years

The research vessel JOIDES Resolution arriving Lisbon after the IODP Expedition 339. Credit: Prof. F. Barriga

Scientists have discovered a relationship between climate change and ocean currents over the past six million years after analysing an area of the Atlantic near the Strait of Gibraltar, according to research published today (Friday, 13 June) in the journal Science.
An expedition of scientists, jointly led by Dr Javier Hernandez-Molina, from the Department of Earth Sciences at Royal Holloway, University of London, examined core samples from the seabed off the coast of Spain and Portugal which provided proof of shifts of climate change over millions of years.

The team also discovered new evidence of a deep-earth tectonic pulse in the region, as well as thick layers of sand within mountains of mud in a vast sheet, spreading out nearly 100km into the Atlantic from the Gibraltar gateway. The quantity of sand is far more than was expected and has been caused by the strength, speed and long duration of bottom currents flowing through the Strait of Gibraltar from the Mediterranean.

“The sediments we examined show various shifts of climate change over millions of years,” Dr Hernandez-Molina said. “In addition, our findings could herald a significant shift in future targets for oil and gas exploration in deep-water settings. The thickness, extent and properties of these sands make them an ideal target in places where they are buried deep enough to allow for the trapping of hydrocarbons. The sand is especially clean and well sorted and therefore very porous and permeable.”

The expedition, carrying an international team of 35 scientists from 14 countries, recovered 5km of core samples from an area along the Gulf of Cadiz and west of Portugal.

The research found that a powerful cascade of Mediterranean water spilling into the Atlantic was scouring the rocky seafloor, carving deep-sea channels and building up mountains of mud. This is due to Mediterranean water being saltier than the Atlantic and therefore denser, causing it to plunge downwards.

Dr Hernandez-Molina added: “We set out to understand how the Strait of Gibraltar acted first as a barrier and then a gateway over the past six million years. The fascinating results we came back with have hugely increased our understanding of the Mediterranean Outflow Water (MOW) that flows through the Gibraltar gateway and have led to some key discoveries about the relationship between climatic shifts, deep-water circulation and plate tectonic events over a huge timescale.”

Journal Reference:

F. J. Hernandez-Molina, D. A. V. Stow, C. A. Alvarez-Zarikian, G. Acton, A. Bahr, B. Balestra, E. Ducassou, R. Flood, J.-A. Flores, S. Furota, P. Grunert, D. Hodell, F. Jimenez-Espejo, J. K. Kim, L. Krissek, J. Kuroda, B. Li, E. Llave, J. Lofi, L. Lourens, M. Miller, F. Nanayama, N. Nishida, C. Richter, C. Roque, H. Pereira, M. F. Sanchez Goni, F. J. Sierro, A. D. Singh, C. Sloss, Y. Takashimizu, A. Tzanova, A. Voelker, T. Williams, C. Xuan. Onset of Mediterranean outflow into the North Atlantic. Science, 2014; 344 (6189): 1244 DOI: 10.1126/science.1251306

Note : The above story is based on materials provided by Royal Holloway, University of London.

Mottramite

Mottramite Ojuela Mine, Mapimi, Mun. de Mapimi, Durango, Mexico Size: 13.0 x 11.0 x 8.0 cm (cabinet) © danweinrich

Chemical Formula: PbCu(VO4)(OH)
Locality: Mottram, St. Andrews, Cheshire, England.
Name Origin: Named for the locality.

Mottramite is an orthorhombic mineral, PbCu(VO4)(OH), at the copper end of the descloizite group. It was formerly called cuprodescloizite or psittacinite (this mineral characterized in 1868 by Frederick Augustus Genth).

History

Discovery date : 1876
Town of Origin: MOTTRAM, ST. ANDREW’S, CHESHIRE
Country of Origin : ANGLETERRE

Optical properties

Optical and misc. Properties: Transparent to Opaque
Refractive Index: from 2,17 to 2,32
Axial angle 2V : ~73°

Physical Properties

Cleavage: None
Color:     Brown, Brown red, Brownish black, Green, Dark green.
Density: 5.9 – 6, Average = 5.95
Diaphaneity: Transparent to Opaque
Fracture: Brittle – Generally displayed by glasses and most non-metallic minerals.
Hardness: 3.5 – Copper Penny
Luster: Greasy (Oily)
Streak: light brownish green

Photos:

Mottramite 5.2×3.6×2.3 cm Tsumeb Corp. Mine Tsumeb Namibia Copyright © David K. Joyce Minerals
Mottramite Ojuela Mine, Mapimi, Mun. de Mapimi, Durango, Mexico Size: 2.9 x 2.0 x 0.8 cm (thumbnail) © danweinrich
Cerussite on Mottramite Tsumeb Mine, Tsumeb, Otjikoto Region, Namibia Cabinet, 9.4 x 6.3 x 5.3 cm © irocks

New evidence for oceans of water deep in the Earth

Researchers from Northwestern University and the University of New Mexico report evidence for potentially oceans worth of water deep beneath the United States. Though not in the familiar liquid form — the ingredients for water are bound up in rock deep in the Earth’s mantle — the discovery may represent the planet’s largest water reservoir.

The presence of liquid water on the surface is what makes our “blue planet” habitable, and scientists have long been trying to figure out just how much water may be cycling between Earth’s surface and interior reservoirs through plate tectonics.

Northwestern geophysicist Steve Jacobsen and University of New Mexico seismologist Brandon Schmandt have found deep pockets of magma located about 400 miles beneath North America, a likely signature of the presence of water at these depths. The discovery suggests water from the Earth’s surface can be driven to such great depths by plate tectonics, eventually causing partial melting of the rocks found deep in the mantle.

The findings, to be published June 13 in the journal Science, will aid scientists in understanding how the Earth formed, what its current composition and inner workings are and how much water is trapped in mantle rock.

“Geological processes on the Earth’s surface, such as earthquakes or erupting volcanoes, are an expression of what is going on inside the Earth, out of our sight,” said Jacobsen, a co-author of the paper. “I think we are finally seeing evidence for a whole-Earth water cycle, which may help explain the vast amount of liquid water on the surface of our habitable planet. Scientists have been looking for this missing deep water for decades.”

Scientists have long speculated that water is trapped in a rocky layer of the Earth’s mantle located between the lower mantle and upper mantle, at depths between 250 miles and 410 miles. Jacobsen and Schmandt are the first to provide direct evidence that there may be water in this area of the mantle, known as the “transition zone,” on a regional scale. The region extends across most of the interior of the United States.

Schmandt, an assistant professor of geophysics at the University of New Mexico, uses seismic waves from earthquakes to investigate the structure of the deep crust and mantle. Jacobsen, an associate professor of Earth and planetary sciences at Northwestern’s Weinberg College of Arts and Sciences, uses observations in the laboratory to make predictions about geophysical processes occurring far beyond our direct observation.

The study combined Jacobsen’s lab experiments in which he studies mantle rock under the simulated high pressures of 400 miles below the Earth’s surface with Schmandt’s observations using vast amounts of seismic data from the USArray, a dense network of more than 2,000 seismometers across the United States.

Jacobsen’s and Schmandt’s findings converged to produce evidence that melting may occur about 400 miles deep in the Earth. H2O stored in mantle rocks, such as those containing the mineral ringwoodite, likely is the key to the process, the researchers said.

“Melting of rock at this depth is remarkable because most melting in the mantle occurs much shallower, in the upper 50 miles,” said Schmandt, a co-author of the paper. “If there is a substantial amount of H2O in the transition zone, then some melting should take place in areas where there is flow into the lower mantle, and that is consistent with what we found.”

If just one percent of the weight of mantle rock located in the transition zone is H2O, that would be equivalent to nearly three times the amount of water in our oceans, the researchers said.

This water is not in a form familiar to us — it is not liquid, ice or vapor. This fourth form is water trapped inside the molecular structure of the minerals in the mantle rock. The weight of 250 miles of solid rock creates such high pressure, along with temperatures above 2,000 degrees Fahrenheit, that a water molecule splits to form a hydroxyl radical (OH), which can be bound into a mineral’s crystal structure.

Schmandt and Jacobsen’s findings build on a discovery reported in March in the journal Nature in which scientists discovered a piece of the mineral ringwoodite inside a diamond brought up from a depth of 400 miles by a volcano in Brazil. That tiny piece of ringwoodite — the only sample in existence from within the Earth — contained a surprising amount of water bound in solid form in the mineral.

“Whether or not this unique sample is representative of the Earth’s interior composition is not known, however,” Jacobsen said. “Now we have found evidence for extensive melting beneath North America at the same depths corresponding to the dehydration of ringwoodite, which is exactly what has been happening in my experiments.”

For years, Jacobsen has been synthesizing ringwoodite, colored sapphire-like blue, in his Northwestern lab by reacting the green mineral olivine with water at high-pressure conditions. (The Earth’s upper mantle is rich in olivine.) He found that more than one percent of the weight of the ringwoodite’s crystal structure can consist of water — roughly the same amount of water as was found in the sample reported in the Nature paper.

“The ringwoodite is like a sponge, soaking up water,” Jacobsen said. “There is something very special about the crystal structure of ringwoodite that allows it to attract hydrogen and trap water. This mineral can contain a lot of water under conditions of the deep mantle.”

For the study reported in Science, Jacobsen subjected his synthesized ringwoodite to conditions around 400 miles below the Earth’s surface and found it forms small amounts of partial melt when pushed to these conditions. He detected the melt in experiments conducted at the Advanced Photon Source of Argonne National Laboratory and at the National Synchrotron Light Source of Brookhaven National Laboratory.

Jacobsen uses small gem diamonds as hard anvils to compress minerals to deep-Earth conditions. “Because the diamond windows are transparent, we can look into the high-pressure device and watch reactions occurring at conditions of the deep mantle,” he said. “We used intense beams of X-rays, electrons and infrared light to study the chemical reactions taking place in the diamond cell.”

Jacobsen’s findings produced the same evidence of partial melt, or magma, that Schmandt detected beneath North America using seismic waves. Because the deep mantle is beyond the direct observation of scientists, they use seismic waves — sound waves at different speeds — to image the interior of the Earth.

“Seismic data from the USArray are giving us a clearer picture than ever before of the Earth’s internal structure beneath North America,” Schmandt said. “The melting we see appears to be driven by subduction — the downwelling of mantle material from the surface.”

The melting the researchers have detected is called dehydration melting. Rocks in the transition zone can hold a lot of H2O, but rocks in the top of the lower mantle can hold almost none. The water contained within ringwoodite in the transition zone is forced out when it goes deeper (into the lower mantle) and forms a higher-pressure mineral called silicate perovskite, which cannot absorb the water. This causes the rock at the boundary between the transition zone and lower mantle to partially melt.

“When a rock with a lot of H2O moves from the transition zone to the lower mantle it needs to get rid of the H2O somehow, so it melts a little bit,” Schmandt said. “This is called dehydration melting.”

“Once the water is released, much of it may become trapped there in the transition zone,” Jacobsen added.

Just a little bit of melt, about one percent, is detectible with the new array of seismometers aimed at this region of the mantle because the melt slows the speed of seismic waves, Schmandt said.

Journal Reference:

B. Schmandt, S. D. Jacobsen, T. W. Becker, Z. Liu, K. G. Dueker. Dehydration melting at the top of the lower mantle. Science, 2014; 344 (6189): 1265 DOI: 10.1126/science.1253358

Note : The above story is based on materials provided by Northwestern University.

‘Pocket sauropod’ sheds light on giant’s evolution

Europasaurus holgeri skull reconstruction in A, left lateral; B, occipital; and C, dorsal views. Credit: Image courtesy of Taylor & Francis

In a new study published in Journal of Systematic Palaeontology presents a detailed description of the skull bones of a dwarf sauropod, together with an updated reconstruction of an adult Europasaurus skull.
At 40 metres long and 100 tonnes in weight, and with an exceptionally long neck and small head, the herbivorous sauropod dinosaurs were the largest animals ever to have walked the Earth. In 2006, fossil remains of a diminutive form of sauropod – Europasaurus, measuring only 6 metres long and weighing just 0.8 tonnes – were discovered at a quarry in northern Germany. The fossils from the quarry are the best sauropod remains ever discovered, since they include most bones of the skull, as well as different growth stages.

In a new study published in Journal of Systematic Palaeontology, Martin Sander, Professor of Vertebrate Paleontology at the Steinmann-Institute of Geology, Mineralogy and Paleontology of the University of Bonn, and colleagues present a detailed description of the skull bones of this dwarf sauropod, together with an updated reconstruction of an adult Europasaurus skull.

In the Late Jurassic, 150 million years ago, Europe was an archipelago, and most reptile fossils from the continent are those of marine species. The few dinosaur remains that have been found would have been washed into the sea from the islands of the archipelago. Europasaurus would have lived on one of these islands, evolving as a dwarf island species.

Earlier analysis of backbone remains had suggested the existence of two different types (sizes) of Europasaurus. The current study, in its extensive analysis of the skull remains, confirms this dimorphism.

There are several hypotheses for the dimophism observed in the Europasaurus remains. The two types could be examples of male and female sauropods. Another possibility is that populations from two different islands have been preserved in the quarry. A third theory is that the quarry has preserved two populations that were separated in time by several thousand years.

The study contributes to an understanding of the evolutionary dwarfing of Europasaurus, which in turn sheds light on the unique gigantism of sauropod dinosaurs. The fossils will continue to yield important insights into sauropod dinosaur evolution and biology for years to come, and researchers hope that new fossils will continue to be found at the quarry for many years to come.

Journal Reference:

Jean Sebastian Marpmann, José Luis Carballido, P. Martin Sander, Nils Knötschke. Cranial anatomy of the Late Jurassic dwarf sauropodEuropasaurus holgeri(Dinosauria, Camarasauromorpha): ontogenetic changes and size dimorphism. Journal of Systematic Palaeontology, 2014; 1 DOI: 10.1080/14772019.2013.875074

Note : The above story is based on materials provided by Taylor & Francis.

Montroydite

Montroydite Locality: Terlingua District, Brewster Co., Texas, USA Photo Copyright © 2003 Robert O. Meyer

Chemical Formula: HgO
Locality: Terlingua, Texas, USA.
Name Origin: Named for Montroyd Sharp, an owner of the mercury deposit at Terlingua, Texas, USA.

History

Discovery date : 1903
Town of Origin : TERLINGUA, BREWSTER CO., TEXAS
Country of Origin : USA

Optical properties

Optical and misc. Properties:     Transparent to Translucent
Refractive Index : from 2,37 to 2,65
Axial angle 2V: LARGE

Physical Properties

Cleavage: {010} Perfect
Color:     Red, Brownish red, Brown.
Density: 11.2
Diaphaneity: Transparent to Translucent
Fracture: Sectile – Curved shavings or scrapings produced by a knife blade, (e.g. graphite).
Hardness: 1.5-2 – Talc-Gypsum
Luminescence: Non-fluorescent.
Luster: Adamantine
Magnetism: Nonmagnetic
Streak: reddish orange

Photos :

Montroydite Locality: Socrates Mine, Castle Rock Springs area, West Mayacmas District, Mayacmas Mts (Mayacamas Mts), Sonoma Co., California, USA Field of view: 5.6mm Photo Copyright © Marko Burkhardt
Montroydite Location: Terlingua, Brewster County, Texas, USA. Copyright: © Jeff Weissman

Chilean scientists make huge fossil find

Remains of ichthyosaur, which lived between the Triassic and Cretaceous periods, unearthed in Torres del Paine national park

Paleontologists have discovered nearly 50 entire ichthyosaur fossils in southern Chile, one of the best finds of its kind to date, they said.
The fossils of the dolphin-like creature were unearthed in the Torres del Paine national park, whose spiky peaks and brilliant turquoise lakes make it a magnet for trekkers and nature lovers.

Researchers said the marine reptiles, buried by rocks from the Tyndall glacier, lived between the Triassic and Cretaceous periods, which extended from 250m to 66m years ago.

“This great ichthyosaur cemetery, the way the remains are deposited, is unique,” Christian Salazar, paleontologist researcher and natural history museum curator, said.

“It’s the most recent great find in their history. That’s going to answer a lot of questions about how they became extinct, where they migrated to, how they lived,” he said.

The 46 fossils were found in about three months of excavating, Salazar added, and more were likely to be found.

Video :

The above story is based on materials provided by theguardian.com

 

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