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Leucite

Leucite Location: Roccamonfina, Caserta Province, Campania, Italy. Scale: 20x20x20 mm. Copyright: © John Betts – Fine Minerals

Chemical Formula: K(AlSi2O6)
Locality: Bearpaw Mountains., Montana, USA.
Name Origin: From the Greek leukos – “white.”

Leucite is a rock-forming mineral composed of potassium and aluminium tectosilicate K(AlSi2O6). Crystals have the form of cubic icositetrahedra but, as first observed by Sir David Brewster in 1821, they are not optically isotropic, and are therefore pseudo-cubic.

Goniometric measurements made by Gerhard vom Rath in 1873 led him to refer the crystals to the tetragonal system. Optical investigations have since proved the crystals to be still more complex in character, and to consist of several orthorhombic or monoclinic individuals, which are optically biaxial and repeatedly twinned, giving rise to twin-lamellae and to striations on the faces. When the crystals are raised to a temperature of about 500 °C they become optically isotropic and the twin-lamellae and striations disappear, although they reappear when the crystals are cooled again. This pseudo-cubic character of leucite is very similar to that of the mineral boracite.

The crystals are white or ash-grey in colour, hence the name suggested by A. G. Werner in 1701, from ‘λευκος’, ‘(matt) white’. They are transparent and glassy when fresh, albeit with a noticeably subdued ‘subvitreous’ lustre due to the low refractive index, but readily alter to become waxy/greasy and then dull and opaque; they are brittle and break with a conchoidal fracture. The Mohs hardness is 5.5, and the specific gravity 2.47. Inclusions of other minerals, arranged in concentric zones, are frequently present in the crystals. On account of the color and form of the crystals the mineral was early known as white garnet. French authors in older literature may employ René Just Haüy’s name amphigène, but ‘leucite’ is the only name for this mineral species that is recognised as official by the International Mineralogical Association.

History

Discovery date : 1791
Town of Origin : MT. VESUVE (VOLCAN), NAPLES, CAMPANIE
Country of Origin : ITALIE

Optical properties

Optical and misc. Properties: Translucent to transparent
Refractive Index : 1,50
Axial angle 2V : TRES PETIT

Physical Properties

Cleavage: {110} Indistinct
Color:     Colorless, Gray, Yellow gray, White.
Density: 2.47
Diaphaneity: Translucent to transparent
Fracture: Brittle – Conchoidal – Very brittle fracture producing small, conchoidal fragments.
Hardness: 6 – Orthoclase
Luminescence: Non-fluorescent.
Luster: Vitreous (Glassy)
Magnetism: Nonmagnetic
Streak: white

Photos :

Leucite Roccamonfina Volcanic Complex, Caserta Province, Campania, Italy Size: 2.7 x 2.0 x 1.6 cm (thumbnail) © danweinrich
Leucite Magnet Cove, Hot Spring County, Arkansas Miniature, 5 x 4.4 x 4.3 cm © irocks
Leucite Corcolle, Tivoli, Latium, Italy Specimen weight:116 gr. Crystal size:13 mm Overall size: 55mm x 50 mm x 38 mm © minservice
Leucite Loučná, Ostrov, Karlovy Vary Region, Bohemia, Czech Republic Specimen weight:130 gr. Crystal size:3,2 cm Overall size:8 x 5,5 x 4 cm © minservice
Emmelberg, Üdersdorf, Daun, Eifel, Rhineland-Palatinate, Germany © JDehove

Mekong River

This is a map of the Mekong River watershed. I, Pfly, made it, based on USGS data.

The Mekong is a trans-boundary river in Southeast Asia. It is the world’s 12th-longest river and the 7th-longest in Asia. Its estimated length is 4,350 km (2,703 mi), and it drains an area of 795,000 km2 (307,000 sq mi), discharging 457 km3 (110 cu mi) of water annually.

From the Tibetan Plateau this river runs through China’s Yunnan province, Burma (Myanmar), Laos, Thailand, Cambodia and Vietnam. In 1995, Laos, Thailand, Cambodia and Vietnam established the Mekong River Commission to assist in the management and coordinated use of the Mekong’s resources. In 1996 China and Burma (Myanmar) became “dialogue partners” of the MRC and the six countries now work together within a cooperative framework.

The extreme seasonal variations in flow and the presence of rapids and waterfalls in this river have made navigation difficult. The river is a major trading route linking China’s southwestern province of Yunnan to Laos, Burma (Myanmar) and Thailand to the south, an important trade route between western China and Southeast Asia.

Course

The Mekong rises as the Lancang (Lantsang) in the “Three Rivers Area” on the Tibetan Plateau in the Sanjiangyuan National Nature Reserve; the reserve protects the headwaters of, from north to south, the Yellow (Huang He), the Yangtze and the Mekong Rivers. It flows southeast through Yunnan Province, and then through the Three Parallel Rivers Area in the Hengduan Mountains, along with the Yangtze to its north and the Salween River (Nujiang in Chinese) to its south.

The Mekong then meets the tripoint of China, Burma (Myanmar) and Laos. From there it flows southwest and forms the border of Burma and Laos for about 100 kilometres (62 mi) until it arrives at the tripoint of Burma, Laos, and Thailand. This is also the point of confluence between the Ruak River (which follows the Thai-Burma border) and the Mekong. The area of this tripoint is sometimes termed the Golden Triangle, although the term also refers to the much larger area of those three countries that is notorious as a drug producing region.

From the Golden Triangle tripoint, the Mekong turns southeast to briefly form the border of Laos with Thailand. It then turns east into the interior of Laos, flowing first east and then south for some 400 kilometres (250 mi) before meeting the border with Thailand again. Once more, it defines the Laos-Thailand border for some 850 kilometres (530 mi) as it flows first east, passing in front of the capital of Laos, Vientiane, then turns south. A second time, the river leaves the border and flows east into Laos soon passing the city of Pakse. Thereafter, it turns and runs more or less directly south, crossing into Cambodia.

At Phnom Penh the river is joined on the right bank by the river and lake system the Tonlé Sap. When the Mekong is low, the Tonle Sap is a tributary; water flows from the lake and river into the Mekong. When the Mekong floods, the flow reverses; the floodwaters of the Mekong flow up the Tonle Sap.

Immediately after the Sap River joins the Mekong by Phnom Penh, the Bassac River branches off the right (west) bank. The Bassac River is the first and main distributary of the Mekong; thus, this is the beginning of the Mekong Delta. The two rivers, the Bassac to the west and the Mekong to the east, enter Vietnam very soon after this. In Vietnam, the Bassac is called the Hậu River (Sông Hậu or Hậu Giang); the main, eastern, branch of the Mekong is called the Tiền River or Tiền Giang. In Vietnam, distributaries of the eastern (main, Mekong) branch include the Mỹ Tho River, the Ba Lai River, the Hàm Luông River, and the Cổ Chiên River.

Drainage basin

The Mekong Basin can be divided into two parts: the ‘Upper Mekong Basin’ in Tibet and China, and the ‘Lower Mekong Basin’ from Yunnan downstream from China to the South China Sea. From the point where it rises to its mouth, the most precipitous drop in the Mekong occurs in Upper Mekong Basin, a stretch of some 2,200 km (1,400 mi). Here, it drops 4,500 metres (14,800 ft) before it enters the Lower Basin where the borders of Thailand, Laos, China and Burma (Myanmar) come together in the Golden Triangle. Downstream from the Golden Triangle, the river flows for a further 2,600 km (1,600 mi) through Laos, Thailand and Cambodia before entering the South China Sea via a complex delta system in Vietnam.

Upper Mekong Basin

The Upper Basin makes up 24% of the total area and contributes 15 to 20% of the water that flows into the Mekong River. The catchment here is steep and narrow. Soil erosion has been a major problem and approximately 50% of the sediment in the river comes from the Upper Basin.

In Yunnan province in China, the river and its tributaries are confined by narrow, deep gorges. The tributary river systems in this part of the basin are small. Only 14 have catchment areas that exceed 1,000 km2 (390 sq mi), yet the greatest amount of loss of forest cover in the entire river system per square kilometer has occurred in this region due to heavy unchecked demand for natural resources. In the south of Yunnan, in Simao and Xishuangbanna Prefectures, the river changes as the valley opens out, the floodplain becomes wider, and the river becomes wider and slower.

Lower Mekong Basin

Major tributary systems develop in the Lower Basin. These systems can be separated into two groups: tributaries that contribute to the major wet season flows, and tributaries that drain low relief regions of lower rainfall. The first group are left bank tributaries that drain the high-rainfall areas of Lao PDR. The second group are those on the right bank, mainly the Mun and Chi rivers, that drain a large part of Northeast Thailand.

Laos lies almost entirely within the Lower Mekong Basin. Its climate, landscape and land use are the major factors shaping the hydrology of the river. The mountainous landscape means that only 16% of the country is farmed under lowland terrace or upland shifting cultivation. With upland shifting agriculture (slash and burn), soils recover within 10 to 20 years but the vegetation does not. Shifting cultivation is common in the uplands of Northern Laos and is reported to account for as much as 27% of the total land under rice cultivation. As elsewhere in the basin, forest cover has been steadily reduced during the last three decades by shifting agriculture and permanent agriculture. The cumulative impacts of these activities on the river regime have not been measured. However, the hydrological impacts of land-cover changes induced by the Vietnam War were quantified in two sub-catchments of the Lower Mekong River Basin.

Loss of forest cover in the Thai areas of the Lower Basin has been the highest in all the Lower Mekong countries over the past 60 years. On the Korat Plateau, which includes the Mun and Chi tributary systems, forest cover was reduced from 42% in 1961 to 13% in 1993. Although this part of Northeast Thailand has an annual rainfall of more than 1,000 mm, a high evaporation rate means it is classified as a semi arid region. Consequently, although the Mun and Chi Basins drain 15% of the entire Mekong Basin, they only contribute 6% of the average annual flow. Sandy and saline soils are the most common soil types, which makes much of the land unsuitable for wet rice cultivation. In spite of poor fertility, however, agriculture is intensive. Glutinous rice, maize and cassava are the principal crops. Drought is by far the major hydrological hazard in this region.

As the Mekong enters Cambodia, over 95% of the flows have already joined the river. From here on downstream the terrain is flat and water levels rather than flow volumes determine the movement of water across the landscape. The seasonal cycle of changing water levels at Phnom Penh results in the unique “flow reversal” of water into and out of the Great Lake via the Tonle Sap River. Phnom Penh also marks the beginning of the delta system of the Mekong River. Here the mainstream begins to break up into an increasing number of branches.

In Cambodia, the wet rice is the main crop and is grown on the flood plains of the Tonle Sap, Mekong and Bassac (the Mekong delta distributary known as the Hậu in Vietnam) rivers. More than half of Cambodia remains covered with mixed evergreen and deciduous broadleaf forest, but forest cover has decreased from 73% in 1973 to 63% in 1993. Here, the river landscape is flat. Small changes in water level determine the direction of water movement, including the large-scale reversal of flow into and out of the Tonle Sap basin from the Mekong River.

The Mekong Delta in Viet Nam is farmed intensively and has little natural vegetation left. Forest cover is less than 10%. In the Central Highlands of Vietnam, forest cover was reduced from over 95% in the 1950s to around 50% in the mid 1990s. Agricultural expansion and population pressure are the major reasons for land use and landscape change. Both drought and flood are common hazards in the Delta, which many people believe is the most sensitive to upstream hydrological change.

Geology

The internal drainage patterns of the Mekong are unusual when compared to those of other large rivers. Most large river systems that drain the interiors of continents, such as the Amazon, Congo, and Mississippi, have relatively simple dendritic tributary networks that resemble a branching tree.

Typically, such patterns develop in basins with gentle slopes where the underlying geological structure is fairly homogenous and stable, exerting little or no control on river morphology. In marked contrast, the tributary networks of the Salween, Yangtze, and particularly the Mekong, are complex with different sub-basins often exhibiting different, and distinct, drainage patterns. These complex drainage systems have developed in a setting where the underlying geological structure is heterogeneous and active, and is the major factor controlling the course of rivers and the landscapes they carve out.

The elevation of the Tibetan Plateau during the Tertiary period was an important factor in the genesis of the south-west monsoon, which is the dominant climatic control influencing the hydrology of the Mekong Basin. Understanding the nature and timing of the elevation of Tibet (and the Central Highlands of Viet Nam) therefore helps explain the provenance of sediment reaching the delta and the Tonle Sap Great Lake today. Studies of the provenance of sediments in the Mekong Delta reveal a major switch in the source of sediments about eight million years ago (Ma). From 36 to 8 Ma the bulk (76%) of the sediments deposited in the delta came from erosion of the bedrock in the Three Rivers Area. From 8 Ma to the present, however, the contribution from the Three Rivers Area fell to 40%, while that from the Central Highlands rose from 11 to 51%. One of the most striking conclusions of provenance studies is the small contribution of sediment from the other parts of the Mekong Basin, notably the Khorat Plateau, the uplands of northern Lao PDR and northern Thailand, and the mountain ranges south of the Three Rivers Area.

The last glacial period came to an abrupt end about 19,000 years ago (ka) when sea levels rose rapidly, reaching a maximum of about 4.5 m above present levels in the early Holocene at about 8 ka. At this time the shoreline of the South China Sea almost reached Phnom Penh and cores recovered from near Angkor Borei contained sediments deposited under the influence of tides, and salt marsh and mangrove swamp deposits. Sediments deposited in the Tonle Sap Great Lake about this time (7.9–7.3 ka) also show indications of marine influence, suggesting a connection to the South China Sea. Although the hydraulic relationships between the Mekong and the Tonle Sap Great Lake systems during the Holocene are not well understood, it is clear that between 9,000 and 7,500 years ago the confluence of the Tonle Sap and the Mekong was in close proximity to the South China Sea.

The present river morphology of the Mekong Delta developed over the last 6,000 years. During this period, the delta advanced 200 km over the continental shelf of the South China Sea, covering an area of more than 62,500 km2. From 5.3 to 3.5 ka the delta advanced across a broad embayment formed between higher ground near the Cambodian border and uplands north of Ho Chi Minh City. During this phase of its development the delta was sheltered from the wave action of long-shore currents and was constructed largely through fluvial and tidal processes. At this time the delta was advancing at a rate of 17–18 m per year. After 3.5 ka, however, the delta had built out beyond the embayment and became subject to wave action and marine currents. These deflected deposition south-eastwards in the direction of the Cà Mau Peninsula, which is one of the most recent features of the delta.

For much of its length the Mekong flows through bedrock channels, i.e. channels that are confined or constrained by bedrock or old alluvium in the bed and riverbanks. Geomorphologic features normally associated with the alluvial stretches of mature rivers, such as meanders, oxbow lakes, cut-offs, and extensive floodplains are restricted to a short stretch of the mainstream around Vientiane and downstream of Kratie where the river develops alluvial channels that are free of control exerted by the underlying bedrock.

The Mekong Basin is not normally considered a seismically active area as much of the basin is underlain by the relatively stable continental block. Nonetheless, the parts of the basin in northern Laos, northern Thailand, Burma (Myanmar) and China do experience frequent earthquakes and tremors. The magnitude of these earthquakes rarely exceeds 6.5 on the Richter scale and is unlikely to cause material damage.

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

Crater discovery’s impact echoes still today

PhD student Lisa Cupelli sits atop rocks in the heart of South Africa’s Vredefort impact crater, where she and Western Earth Sciences professor Desmond Moser, below, confirmed the rocks are some of the only remains of a magma sea created more than 2 billion years ago. Credit: Desmond Moser

Desmond Moser never gives up. Twenty years ago, the now Western Earth Sciences professor first visited the heart of South Africa’s Vredefort impact crater, locating what he believed to be some of the only remains of a magma sea created more than 2 billion years ago in a 300-kilometre-wide crater.

He published his finding in 1997 in the journal Geology and awaited praise from peers.

But it never came.

“It was the first paper I ever published and people keep following it up by publishing stuff knocking it. I said it looked like impact rock, while everyone else said it wasn’t. But I was still convinced I was right,” said Moser, of what he refers to as the Vredefort Gabbronorite.

In 2009, Moser, along with PhD student Lisa Cupelli, returned to the South African site to see if they could once and for all confirm his original findings.

Scientists place the asteroid that struck Vredefort among the latest ever to hit the Earth, estimating its size at 5-10-km in diameter.

Given the original location was staked out in pre-GPS 1994, the pair had only an old map and a 35mm slide to guide them.

“I told her this is the situation: If we can find more of the stuff, and we can prove it, it’s going to be good news. Or, it could be a total bust,” he said. “There are hundreds, if not thousands, of geologists going to the area all the time, but they are just walking over the stuff.”

After and hour-and-a-half, Moser and Cupelli found the site where he collected his first sample, thanks to the marking of an windmill that still stood nearby in what was now a farmer’s field.

They spent the next two-and-a-half weeks mapping and collecting samples. And the result was just what he expected.

A sample of the Vredefort Gabbronorite rock Western Earth Sciences professor Desmond Moser confirmed was impact rock created more than 2 billion years ago in South Africa. Credit: Paul Mayne / Western News

“It is definitely a rock that crystalized from the mini-sea of magma, which was created by the impact crater,” he said.

To this day, detractors still think Moser is mistaken.

“Everyone assumed over the years it (the rock) had simply been worn away. It’s not target impact that I found, but rock that is produced from the heat of the magma ocean and, once crystalized, turns into rock – new impact-created rock.”

One of the reasons Moser said other geologists kept missing the point was it didn’t look like what you expect it to look like, even to Moser.

“I did say no at first. But what people usually don’t look at is the micro-minerals,” he said. “When I brought it back to the lab, most of the rocks I got from there had all these smashed and corrupted crystals. But with this particular one they were gem-quality, beautiful little prisms, crystal clean. And then I dated them and they came out to be the age of the impact.

“Then, I knew I had something.”

Moser’s re-confirmation of his earlier work, published in this month’s Geology, will keep geologists on both sides of the fence or, in this case, both sides of the crater, debating whether or not Moser’s discovery is what he says it is.

“I think there is more to be found. We may be walking over more impact rock, but just not assuming what it is,” he said.

One thing for sure, Moser still has the scientific evidence to prove his 20-year-old point.

“I’m a big believer in the truth, and sometimes it takes that long,” he said. “But science works.”

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

Lepidolite

Lepidolite (floater crystal) Virgem de Lapa, Minas Gerais, Brazil Thumbnail, 2.4 x 2.1 x 0.7 cm © irocks
Chemical Formula: K(Li,Al,Rb)3(Al,Si)4O10(F,OH)2
Locality: Pala, San Diego Co., California, USA.
Name Origin: From the Greek lepidion – “scale” and lithos – “stone.”Lepidolite is a lilac-gray or rose-colored member of the mica group with formula  K(Li,Al,Rb)3(Al,Si)4O10(F,OH)2. It is a secondary source of lithium. It is a phyllosilicate mineral and a member of the polylithionite-trilithionite series.It is associated with other lithium-bearing minerals like spodumene in pegmatite bodies. It is one of the major sources of the rare alkali metals rubidium and caesium. In 1861 Robert Bunsen and Gustav Kirchhoff extracted 150 kg of lepidolite and yielded a few grams of rubidium salts for analysis, and therefore discovered the new element rubidium.

It occurs in granite pegmatites, in some high-temperature quartz veins, greisens and granites. Associated minerals include quartz, feldspar, spodumene, amblygonite, tourmaline, columbite, cassiterite, topaz and beryl.

Notable occurrences include Brazil; Ural Mountains, Russia; California, United States; Tanco Mine, Bernic Lake, Manitoba, Canada; and Madagascar.

History

Discovery date : 1792
Town of Origin : ROZNA, BYSTRICE, MORAVIE
Country of Origin : TCHEQUIE

Optical properties

Optical and misc. Properties : Translucent
Refractive Index : from 1,52 to 1,58
Axial angle 2V : 0-58°

Physical Properties

Cleavage: {001} Perfect
Color: Colorless, Gray white, Lilac, Yellowish, White.
Density: 2.8 – 2.9, Average = 2.84
Diaphaneity: Translucent
Fracture: Uneven – Flat surfaces (not cleavage) fractured in an uneven pattern.
Hardness: 2.5-3 – Finger Nail-Calcite
Luminescence: Non-fluorescent.
Luster: Vitreous – Pearly
Streak: white

 Photos:

Lepidolite Itinga, Minas Gerais, Brazil Cabinet, 18.5 x 15.1 x 12.5 cm © irocks
Lepidolite Little Three Mine, Ramona, San Diego Co., California, USA Miniature, 5 x 4 x 3.5 cm © irocks
Himalaya Mine (Himalaya dikes; Himalaya pegmatite), Gem Hill, Mesa Grande District, San Diego Co., California, USA © Eric Graff

Understanding the planets through volcanoes

Data from the Moon Mineralogy Mapper show the presence of cryptomaria (“hidden seas,” outlined in yellow). Primary material of the lunar crust is shown as blue. Areas show as yellow indicate basalt that originated below the surface.

Billions of years ago, volcanoes sent material from inside planetary bodies to the surface. Subsequent impacts have covered those original deposits. Jennifer Whitten, who receives her Ph.D. in geological sciences this year, has figured out a way to study those “hidden seas” and learn more about the early volcanic history the Moon and Mercury.
Volcanism is a planet’s way of turning itself inside out. For scientists, material blasted to the surface from volcanoes is a goldmine of information about a planet’s past.

“Volcanic deposits are important because you get a picture of how the surface has been modified, but you can also learn so much about the interior of a planet,” said Jennifer Whitten, who will receive her Ph.D. this week from the Department of Geological Sciences. “So you get a picture of the inside and the outside.”

For her dissertation, Whitten studied volcanic deposits on the Moon and Mercury that date back billions of years. She hopes that a better understanding of these ancient deposits will shed light on the formation and early evolution of those two planetary bodies.
It might also deepen our understanding of Earth in its infancy. On our home planet, ancient volcanic deposits are often ground away by the constant churning of tectonic plates. So to truly understand how volcanism shapes a young planet, Whitten says, it’s essential to look beyond the Earth.
“One of the most perplexing questions about the earliest history of the planets, including Earth, is the amount of volcanic activity that occurs then,” said Jim Head, professor of geological sciences and Whitten’s adviser. “The observational techniques Jennifer Whitten has developed have contributed greatly to our understanding of these early volcanic processes.”

Hidden volcanoes on the Moon and Mercury

On the Moon, some volcanic deposits are easy to spot. The lunar maria—the dark splotches that form the iconic “man in the Moon”—are composed largely of volcanic basalts. Termed “mare,” the Greek word for sea, because early astronomers mistook them for bodies of water, they were formed billions of years ago when molten lava flowed up from the depths and filled in deep basins formed by asteroids and other impactors.
But there are other volcanic deposits on the Moon—many of them older than the visible maria—that are hidden from view. As impacts pounded the Moon’s surface, some ancient volcanic deposits were covered with debris blasted out of impact craters. The debris, which is generally a bright whitish color, hides the dark-colored basalt from view. Those hidden maria—called “cryptomaria” after the Greek for hidden or secret seas—are what Whitten wanted to explore. Understanding where these deposits are located and what they’re made of helps to fill in missing pieces of the Moon’s volcanic history.
Whitten used a variety of techniques to look through the veneer of impact debris and definitively identify cryptomaria deposits on the Moon. One of those techniques involved looking for a very specific type of crater. When a small impactor strikes a cryptomare deposit, it digs up some of the volcanic material beneath the impact debris. The result is a crater surrounded by a dark halo of mare material.
Using these dark-halo craters as a guide, Whitten was able to identify 18 deposits of cryptomaria on the Moon. Having mapped the deposits, she was able to answer some critical questions about them.
First, she was able to use data from the Moon Mineralogy Mapper, which flew aboard India’s Chandrayaan-1 spacecraft, to identify the composition of the deposits. She found that cryptomaria had a composition similar to the visible maria—something that had been the subject of speculation before now.
“I’ve been able to show that it is actually mare basalt,” she said. “We can use the term cryptomaria and know that it means what we think it means.”
Second, Whitten was able to show that cryptomaria are concentrated on the Moon’s near side—the side facing Earth. It’s long been known that the lunar far side lacks the visible mare deposits that dominate the near side. But it wasn’t clear whether or not there may have been some cryptomaria hiding on the far side.
“Secretly I really wanted to find some major deposit on the far side so I could say, ‘Look everyone; it’s not all on the near side,'” Whitten said. “But that didn’t happen.”
The finding suggests that volcanism throughout the Moon’s history was concentrated on the near side. That appears to be in part because the crust is thinner on the nearside, allowing volcanic material to flow through more easily.
Whitten used similar techniques to look for signs of ancient volcanism on Mercury. There, she was able to show vast areas of the planet’s northern hemisphere, known as the intercrater plains, have a volcanic origin. The work added substantially to the inventory of volcanic material on the surface of Mercury.

More research ahead

Recently, Whitten accepted a position as a postdoctoral researcher at the Smithsonian Air and Space Museum in Washington, D.C. There, she’ll be involved a project that uses radar to look for more buried volcanic deposits on the Moon.
“I’m excited about learning a new technique that provides access to the few upper meters of the lunar surface, especially since my dissertation was focused on finding buried volcanic deposits,” she said. “I am optimistic about finding interesting volcanic features.”
Those features could help deepen our understanding of the solar system.
“In the big picture, understanding volcanic deposits can give a sense of the initial composition of these planets,” Whitten said. “That tells you about the materials in the cloud that formed the solar system.”
It also helps us learn about our own planet. The types of deposits Whitten looked at on the Moon and Mercury are called large igneous provinces or LIPs. LIPs have been fairly common throughout Earth’s history and have been linked to several major extinction events. So understanding how they work could be of critical importance.
“The LIPs on Earth have been eroded or are under the ocean, so it’s hard to study them,” Whitten said. “But you can get an idea of the size of these things and what affects their size because we can study them on Moon or Mercury. I think it’s really exciting that by understanding what’s happening on the Moon and Mercury, you can better understand the early history of the Earth.”
Note : The above story is based on materials provided by  Brown University

International Chronostratigraphic Chart 2014

Click here (PDF or JPG) to download the latest version (v 2014/02) of the International Chronostratigraphic Chart.

Translations of the chart: Chinese  (v2013-01: PDF or JPG), Spanish (v2013-01), Portuguese (v2013-01: PDF or JPG), Norwegian (v2013-01: PDF or JPG), Basque (v2013-01: PDF or JPG), Catalan (v2013-01: PDF or JPG), French (v2012) and Japanese (v2012).

The old versions can be download at the following links: 2008 (PDF or JPG), 2009 (PDF or JPG), 2010 (PDF or JPG), 2012 (PDF or JPG), 2013/01 (PDF or JPG).
© 2013-2014 International Commission on Stratigraphy – ALL RIGHTS RESERVED

Lepidocrocite

Quartz with Lepidocrocite Goboboseb Mountains, Brandberg District, Namibia miniature – 4 x 3 x 2.5 cm © marinmineral.

Chemical Formula: γ-FeO(OH)
Locality: Common world wide.
Name Origin: From the Greek lipis – “scale” and krokis – “fibre.”
Lepidocrocite (γ-FeO(OH)), also called esmeraldite or hydrohematite, is an iron oxide-hydroxide mineral. Lepidocrocite has an orthorhombic crystal structure, a hardness of 5, specific gravity of 4, a submetallic luster and a yellow-brown streak. It is red to reddish brown and forms when iron-containing substances rust underwater. Lepidocrocite is commonly found in the weathering of primary iron minerals and in iron ore deposits. It can be seen as rust scale inside old steel water pipes and water tanks.

The structure of lepidocrocite is similar to the boehmite structure found in bauxite and consists of layered iron(III) oxide octahedra bonded by hydrogen bonding via hydroxide layers. This relatively weakly bonded layering accounts for the scaley habit of the mineral.

It was first described in 1813 from the Zlaté Hory polymetallic ore deposit in Moravia, Czech Republic. The name is from the Greek lipis for scale and krokis for fibre.

History

Discovery date : 1813
Town of Origin : EISENZECHE, EISERFELD, SIEGEN
Country of Origin : ALLEMAGNE

Optical properties

Optical and misc. Properties : Opaque
Refractive Index : from 1,94 to 2,51
Axial angle 2V: 83°

Physical Properties

Cleavage: {010} Perfect
Color:     Red, Yellowish brown, Blackish brown.
Density: 4
Diaphaneity: Opaque
Fracture: Uneven – Flat surfaces (not cleavage) fractured in an uneven pattern.
Hardness: 5 – Apatite
Luminescence: Non-fluorescent.
Luster: Sub Metallic
Streak: dark yellow brown

Photos:

Quartz (Var.: Amethyst), Lepidocrocite Locality: Huaron Mining District, San Jose de Huayllay District, Cerro de Pasco, Daniel Alcides Carrión Province, Pasco Department, Peru Dimensions: 11.5 cm x 9.5 cm x 4.7 cm Photo Copyright © Rob Lavinsky & irocks
Lepidocrocite in Quartz
Clara Mine, Rankach valley, Oberwolfach, Wolfach, Black Forest, Baden-Württemberg, Germany © Stephan Wolfsried

Fossil avatars are transforming palaeontology

Digital reconstructions of the skull of the dinosaur Erlikosaurus made from a CT scan Credit: Dr Stephan Lautenschlager

New techniques for visualizing fossils are transforming our understanding of evolutionary history according to a paper published by leading palaeontologists at the University of Bristol.

Palaeontology has traditionally proceeded slowly, with individual scientists labouring for years or even decades over the interpretation of single fossils which they have gradually recovered from entombing rock, sand grain by sand grain, using all manner of dental drills and needles.

The introduction of X-ray tomography has revolutionized the way that fossils are studied, allowing them to be virtually extracted from the rock in a fraction of the time necessary to prepare specimens by hand and without the risk of damaging the fossil.

The resulting fossil avatars not only reveal internal and external anatomical features in unprecedented and previously unrealized detail, but can also be studied in parallel by collaborating or competing teams of scientists, speeding up the pace at which evolutionary history is revealed.

These techniques have enabled palaeontologists to move beyond ‘just so stories’, explanations for why sauropod dinosaurs had such long necks, for example, by subjecting digital models of the fossils to biomechanical analysis, including using the same computer techniques that engineers use to design test bridges and aircraft.

However, the scientists from Bristol’s School of Earth Sciences highlight that the potential benefits of fossil avatars are not being realized.

Lead author Dr John Cunningham said: “At a practical level, we simply don’t have the infrastructure for storing and sharing the vast datasets that describe fossils, and the policies of world-leading museums which protect the copyright of fossils are preventing data sharing at a legal level.”

Co-author Dr Stephan Lautenschlager added: “The increasing availability of fossil avatars will allow us to bring long-extinct animals back to life, virtually, by using computer models to work out how they moved and fed. However, in many cases we are hampered by our limited understanding of the biology of the modern species to which we would ideally like to compare the fossils.”

Dr Imran Rahman, also an author of the agenda-setting study, said: “Palaeontologists are making their fossil avatars freely available as files for 3-D printing and so, soon, anyone who wants one, can have a scientifically accurate model of their favourite fossil, for research, teaching, or just for fun!”

Journal Reference:
John A. Cunningham, Imran A. Rahman, Stephan Lautenschlager, Emily J. Rayfield, Philip C.J. Donoghue. A virtual world of paleontology. Trends in Ecology & Evolution, 2014; 29 (6): 347 DOI: 10.1016/j.tree.2014.04.004

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

Groundwater could fuel life under glaciers

Subglacial lakes in Antarctica might have nutrient-rich groundwater flowing into them, say scientists investigating the origin of the water in ice streams.

Ice streams are huge, fast-flowing glaciers that meander across Antarctica. They are responsible for nearly all of the Antarctic’s contribution to sea-level rise, yet scientists have little understanding of where the water flowing through them comes from. This means that the contents of the subglacial lakes which lie underneath these streams is also a mystery.

The new research, published in Geophysical Research Letters shows for the first time where the water going in and out of these ice streams – their hydrologic budget – comes from.

‘It’s important to understand and quantify the hydrologic budget of these ice streams, as this can control the lubrication and ultimately how fast these ice streams move,’ explains Dr Poul Christoffersen of the Scott Polar Research Institute, lead researcher on the study.

‘Some of these glaciers are slowing, some are speeding up and that’s all in response to changes in the configuration of sources and sinks of water. If we’re trying to understand what they’ll be doing in future we need to understand how they have behaved in the past.’

The team studied five ice streams. They found that the water flowing into them comes mostly from the ice sheet’s deep interior. They also identified a large groundwater reservoir beneath these glacier, which the ice streams draw on to compensate when there is not enough water from the ice sheet to maintain the ice streams fast flow.

The team found that two of the streams moved much faster than three located further south.

‘For two of the ice streams there was a balance between recharge and depletion so they continually flow fast, but for the other three the system doesn’t have enough to provide replenishment, and so they end up losing water. Some are slowing down now, and one stopped altogether about 170 years ago,’ Christoffersen says.

It’s like when water from groundwater reservoirs flow into rivers in England. When an ice stream has little water flowing in from melting ice, the groundwater begins to flow into the stream instead. but unlike England it all happens beneath the ice. If this happens, and there’s lots of groundwater in the network, then the connected subglacial lakes beneath the ice streams are likely to have a a much higher nutrient content, meaning researchers are more likely to find life in them than in the subglacial lakes fed by pure glacial water.

‘Water that’s been stored for thousands of years in the pore spaces of sediments beneath the ice streams are mixing with the water in the subglacial hydrological network. These ancient waters are full of nutrients from the sediment, enough that they could provide life to a thriving microbial habitat,’ explains Christoffersen.

‘A hydrologic system that receives groundwater contributions is much more likely to have high nutrient levels compared to the fast flowing systems which are fed by pure glacial meltwater. That water is pure with very little biochemical material to provide life,’ he says.

More information: Christoffersen, P., M. Bougamont, S. P. Carter, H. A. Fricker, and S. Tulaczyk (2014), “Significant groundwater contribution to Antarctic ice streams hydrologic budget,” Geophys. Res. Lett., 41, 2003-2010, DOI: 10.1002/2014GL059250.

Note : The above story is based on materials provided by PlanetEarth Online

Legrandite

Legrandite Ojuela Mine, Mapimi, Durango, Mexico Miniature, 3.2 x 2.6 x 1.2 cm “Courtesy of Rob Lavinsky, The Arkenstone, www.iRocks.com”

Chemical Formula: Zn2(AsO4)(OH)·H2O
Locality: Ojuela mine near Mapimi, Durango.
Name Origin: Named after the Belgian mining engineer, Legrande.

Legrandite is a rare zinc arsenate mineral, Zn2(AsO4)(OH)·H2O.
It is an uncommon secondary mineral in the oxidized zone of arsenic bearing zinc deposits and occurs rarely in granite pegmatite. Associated minerals include: adamite, paradamite, kottigite, scorodite, smithsonite, leiteite, renierite, pharmacosiderite, aurichalcite, siderite, goethite and pyrite. It has been reported from Tsumeb, Namibia; the Ojuela mine in Durango, Mexico and at Sterling Hill, New Jersey, USA.

It was first described in 1934 for an occurrence in the Flor de Peña Mine, Nuevo Leon, Mexico and named after M. Legrand, a Belgian mining engineer .

History

Discovery date : 1932
Town of Origin : MINE FLOR DE PENA, LAMPAZOS, NUOVA LEON
Country of Origin : MEXIQUE

Optical properties

Optical and misc. Properties : Translucent
Refractive Index: from 1,67 to 1,74
Axial angle 2V: 50°

Physical Properties

Cleavage: {100} Imperfect
Color: Yellow, Yellowish orange.
Density: 4
Diaphaneity: Translucent
Fracture: Brittle – Conchoidal – Very brittle fracture producing small, conchoidal fragments.
Hardness: 4-5 – Fluorite-Apatite
Luster: Vitreous (Glassy)
Streak: white

Photos :

Legrandite Ojuela Mine, Mapimí, Mun. de Mapimí, Durango, Mexico Thumbnail, 2.8 x 0.6 x 0.3 cm “Courtesy of Rob Lavinsky, The Arkenstone, www.iRocks.com”
Legrandite Ojuela Mine, Mapimi, Mun. de Mapimi, Durango, Mexico Size: 2.0 x 1.3 x 1.3 cm (thumbnail) © danweinrich
Ojuela Mine, Mapimí, Mun. de Mapimí, Durango, Mexico © 2004 JBS

Earth’s lower mantle chemistry breakthrough

Diagram of the Earth. Credit: Kelvinsong/Wikipeida

Breaking research news from a team of scientists led by Carnegie’s Ho-kwang “Dave” Mao reveals that the composition of the Earth’s lower mantle may be significantly different than previously thought. These results are to be published by Science.

The lower mantle comprises 55 percent of the planet by volume and extends from 670 and 2900 kilometers in depth, as defined by the so-called transition zone (top) and the core-mantle boundary (below). Pressures in the lower mantle start at 237,000 times atmospheric pressure (24 gigapascals) and reach 1.3 million times atmospheric pressure (136 gigapascals) at the core-mantle boundary.

The prevailing theory has been that the majority of the lower mantle is made up of a single ferromagnesian silicate mineral, commonly called perovskite (Mg,Fe)SiO3) defined through its chemistry and structure. It was thought that perovskite didn’t change structure over the enormous range of pressures and temperatures spanning the lower mantle.

Recent experiments that simulate the conditions of the lower mantle using laser-heated diamond anvil cells, at pressures between 938,000 and 997,000 times atmospheric pressure (95 and 101 gigapascals) and temperatures between 3,500 and 3,860 degrees Fahrenheit (2,200 and 2,400 Kelvin), now reveal that iron bearing perovskite is, in fact, unstable in the lower mantle.

The team finds that the mineral disassociates into two phases one a magnesium silicate perovskite missing iron, which is represented by the Fe portion of the chemical formula, and a new mineral, that is iron-rich and hexagonal in structure, called the H-phase. Experiments confirm that this iron-rich H-phase is more stable than iron bearing perovskite, much to everyone’s surprise. This means it is likely a prevalent and previously unknown species in the lower mantle. This may change our understanding of the deep Earth.

“We still don’t fully understand the chemistry of the H-phase,” said lead author Li Zhang, also of Carnegie. “But this finding indicates that all geodynamic models need to be reconsidered to take the H-phase into account. And there could be even more unidentified phases down there in the lower mantle as well, waiting to be identified.”

More information: “Disproportionation of (Mg,Fe)SiO3 perovskite in Earth’s deep lower mantle,” by L. Zhang et al . Science, 2014. www.sciencemag.org/lookup/doi/10.1126/science.1250274

Note : The above story is based on materials provided by Carnegie Institution for Science

New insight into the temperature of deep Earth

Clouds over Australia are shown. Credit: NASA

Scientists from the Magma and Volcanoes Laboratory (CNRS) and the European Synchrotron, the ESRF, have recreated the extreme conditions 600 to 2900 km below the Earth’s surface to investigate the melting of basalt in the oceanic tectonic plates. They exposed microscopic pieces of rock to these extreme pressures and temperatures while simultaneously studying their structure with the ESRF’s extremely powerful X-ray beam.
The results show that basalt produced on the ocean floor has a melting temperature lower than the peridotite which forms the Earth’s mantle. Near the core-mantle boundary, where the temperature rises rapidly, the melting basalt produces liquids rich in silica (SiO2), which react rapidly with the mantle and indicate a speedy dissolution of the basalt back into the depths of the Earth. These experiments provide a new explanation for seismic anomalies at the base of the mantle while fixing its temperature in the region of 4000 K.

The results are published in Science on the 23 May 2014.

The Earth is an active planet. The heat it contains is capable of inducing the mantle convection responsible for plate tectonics. This energy comes from the heat accumulated during the formation of our planet, the latent heat of crystallization of the inner core, and radioactive decay. The temperatures inside the Earth, however, are not well known.

Convection causes hot material to rise to the surface of the Earth and cold material to sink towards the core. Thus, when the ascending mantle begins to melt at the base of the oceanic ridges, the basalt flows along the surface to form what we call the oceanic crust. “Over the course of millennia the crust will then undergo subduction, its greater density causing it to sink into the mantle. This is why the Earth’s continents are known to be several billion years old, while the oldest oceanic crust only dates back 165 million years” said Mohamed Mezouar, scientist at the ESRF.

The temperature at the core-mantle boundary (also known as the D” region) is thought to increase by more than 1000 degrees over a few hundred kilometers, which is significant compared to the temperature gradient across the rest of the mantle. Previous authors have suggested that this temperature rise could cause the partial melting of the mantle, but this hypothesis leaves a number of geophysical observations unexplained. Firstly, the anomalies in the propagation speed of seismic waves do not match those expected for a partial melting of the mantle, and secondly, the melting mantle should lead to the production of liquid pockets in the lowermost mantle, a phenomenon which has never been observed.

The team led by Professor Denis Andrault from the Université Blaise Pascal decided instead to study the melting point of basalt at high depths, and found that it was significantly lower than that of the mantle. The melting of sub-oceanic basalt piles could therefore be responsible for the previously unexplained seismic anomalies. The researchers also showed that the melting basalt generates a liquid rich in SiO2. As the mantle itself contains large quantities of MgO, the interaction of these liquids with the mantle is expected to produce a rapid reaction leading to the formation of the solid MgSiO3 perovskite. This would explain why no liquid pockets have been detected by seismologists in the deep mantle: any streams of liquid should rapidly re-solidify.

If it is indeed the basalt and not the mantle whose melting in the D”-region is responsible for the observed seismic anomalies, then the temperature at the core-mantle boundary must be between 3800 and 4150 Kelvin, between the melting points of basalt and the Earth’s mantle. If this hypothesis is correct, this would be the most accurate determination of the temperature at the core-mantle boundary available today.

“It could solve a long time controversy about the peculiar role of the core-mantle boundary in the dynamical properties of the Earth mantle, said Professor Denis Andrault. ”We know now that the cycle of crust formation at the mid-ocean ridges and crust dissolution in the lowermost mantle may have occured since plate tectonics were active on our planet”, he added.

More information: “Melting of subducted basalt at the core-mantle boundary,” by D. Andrault et al. Science: www.sciencemag.org/lookup/doi/10.1126/science.1250466

Note : The above story is based on materials provided byEuropean Synchrotron Radiation Facility

Leadhillite

Leadhillite Locality: Thorikos Bay slag locality, Thorikos area, Lavrion District slag localities, Lavrion District (Laurion; Laurium), Attikí Prefecture (Attica; Attika), Greece Field of view 6 mm Photo Copyright © M. Kampf

Chemical Formula: Pb4SO4(CO3)2(OH)2
Locality: Leadhills, Lanarkshire, Scotland.
Name Origin: Named for the localiy.

Leadhillite is a lead sulfate carbonate hydroxide mineral, often associated with anglesite. It has the formula Pb4SO4(CO3)2(OH)2. Leadhillite crystallises in the monoclinic system, but develops pseudo-hexagonal forms due to crystal twinning. It forms transparent to translucent variably coloured crystals with an adamantine lustre. It is quite soft with a Mohs hardness of 2.5 and a relatively high specific gravity of 6.26 to 6.55.

It was discovered in 1832 in the Susannah Mine, Leadhills in the county of Lanarkshire, Scotland. It is trimorphous with susannite and macphersonite (these three minerals have the same formula, but different structures). Leadhillite is monoclinic, susannite is trigonal and macphersonite is orthorhombic. Leadhillite was named in 1832 after the locality.

Physical Properties

Cleavage: {001} Perfect, {100} Indistinct
Color: Colorless, Gray, Yellowish, White, Light blue.
Density: 6.26 – 6.55, Average = 6.4
Diaphaneity: Transparent to translucent
Fracture: Sectile – Curved shavings or scrapings produced by a knife blade, (e.g. graphite).
Hardness: 2.5 – Finger Nail
Luminescence: Fluorescent, Short UV=weak gray yellow, Long UV=weak grey yellow.
Luster: Adamantine
Streak: white

Photos :

Leadhillite San Benedetto Mine, Iglesias, Province of Carbonia-Iglesias, Sardinia, Italy Specimen weight:73 gr. Crystal size:. Overall size:4,5 x 4 x 4 cm © minservice
Leadhillite with Cerussite Tsumeb Mine, Tsumeb, Otjikoto Region, Namibia Size: 7.0 x 5.0 x 4.0 cm (small cabinet) © danweinrich
Leadhills, South Lanarkshire, Strathclyde (Lanarkshire), Scotland, UK © Brent Thorne

Study shows iron from melting ice sheets may help buffer global warming

The Antarctic ice sheet. Credit: Stephen Hudson / Wikipedia

A newly-discovered source of oceanic bioavailable iron could have a major impact our understanding of marine food chains and global warming. A UK team has discovered that summer meltwaters from ice sheets are rich in iron, which will have important implications on phytoplankton growth. The findings are reported in the journal Nature Communications on 21st May, 2014.

It is well known that bioavailable iron boosts phytoplankton growth in many of the Earth’s oceans. In turn phytoplankton capture carbon – thus buffering the effects of global warming. The plankton also feed into the bottom of the oceanic food chain, thus providing a food source for marine animals.

The team, comprising researchers from the Universities of Bristol, Leeds, Edinburgh and the National Oceanography Centre, collected meltwater discharged from the 600 km2 Leverett Glacier in Greenland over the summer of 2012, which was subsequently tested for bioavailable iron content. The researchers found that the water exiting from beneath the melting ice sheet contained significant quantities of previously-unconsidered bioavailable iron. This means that the polar oceans receive a seasonal iron boost as the glaciers melt.

Jon Hawkings (Bristol), the lead author, said: “The Greenland and Antarctic Ice Sheets cover around 10% of global land surface. Iron exported in icebergs from these ice sheets have been recognised as a source of iron to the oceans for some time. Our finding that there is also significant iron discharged in runoff from large ice sheet catchments is new. ”

“This means that relatively high iron concentrations are released from the ice sheet all summer, providing a continuous source of iron to the coastal ocean”

Iron is one of the most important biochemical elements, due to its impact on ocean productivity. Despite being the fourth most abundant element in the Earth’s crust, it is mostly not biologically available because it is largely present as unreactive minerals in natural waters. Over the last 20 years there has been controversy over the role of iron in marine food chains and the global carbon cycle, with some groups experimenting with dumping iron into the sea in order to accelerate plankton growth – with the idea that increased plankton growth would capture man made CO2. This work indicates that ice sheets may already be carrying out this process every summer.

Based on their results the team estimates that the flux of bioavailable iron associated with glacial runoff is between 400,000 and 2,500,000 tonnes per year in Greenland and between 60,000 and 100,000 tonnes per year in Antarctica. Taking the combined average figures, this would equal the weight of around 125 Eiffel Towers, or around 3000 fully-laden Boeing 747s being added to the ocean each year.

Jon Hawkings added: “This is a substantial release of iron from the ice sheet, similar in size to that supplied to the oceans by atmospheric dust, another major iron source to the world’s oceans.

At the moment it is just too early to estimate how much additional iron will be carried down from ice sheets into the sea. Of course, the iron release from ice sheet will be localised to the Polar Regions around the ice sheets, so the importance of glacial iron there will be significantly higher. Researchers have already noted that glacial meltwater run-off is associated with large phytoplankton blooms – this may help to explain why”.

Commenting on the relevance of this study, Professor Andreas Kappler (geomicrobiologist at the University of Tübingen, Germany, who is also secretary of the European Association of Geiochemistry) said:

“This study shows that glacier meltwater can contain iron concentrations that are high enough to significantly stimulate biological productivity in oceans that otherwise are oftentimes limited in the element iron that is essential to most living organisms. Although the global importance of this flux of iron into oceans needs to be quantified and the bioavailability of the iron species found should be demonstrated experimentally in future studies, the present study provides a plausible path for nutrient supply to oceanic life.”

More information: Ice sheets as a significant source of highly reactive nanoparticulate iron to the oceans. Authors Jon R. Hawkings, Jemma L. Wadham, Martyn Tranter, Rob Raiswell, Liane G. Benning, Peter J. Statham, Andrew Tedstone, Peter Nienow, Katherine Lee & Jon Telling Nature Communications , 5:3929 , DOI: 10.1038/ncomms4929, published 21 May 2014

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

Ape ancestors’ teeth provide glimpse into their diets and environments

Great ape dietary specialization allowed spread in Eurasia, and also lead to extinction

Newly analyzed tooth samples from the great apes of the Miocene indicate that the same dietary specialization that allowed the apes to move from Africa to Eurasia may have led to their extinction, according to results published May 21, 2014, in the open access journal PLOS ONE by Daniel DeMiguel from the Institut Catalá de Palontologia Miquel Crusafont (Spain) and colleagues.

Apes expanded into Eurasia from Africa during the Miocene (14 to 7 million years ago) and evolved to survive in new habitat. Their diet closely relates to the environment in which they live and each type of diet wears the teeth differently. To better understand the apes’ diet during their evolution and expansion into new habitat, scientists analyzed newly-discovered wearing in the teeth of 15 upper and lower molars belonging to apes from five extinct taxa found in Spain from the mid- to late-Miocene (which overall comprise a time span between 12.3?.2 and 9.7 Ma). They combined these analyses with previously collected data for other Western Eurasian apes, categorizing the wear on the teeth into one of three ape diets: hard-object feeders (e.g., hard fruits, seeds), mixed food feeders (e.g. fruit), and leaf feeders.

Previous data collected elsewhere in Europe and Turkey suggested that the great ape’s diet evolved from hard-shelled fruits and seeds to leaves, but these findings only contained samples from the early-Middle and Late Miocene, while lack data from the epoch of highest diversity of hominoids in Western Europe.

In their research, the scientists found that in contrast with the diet of hard-shelled fruits and seeds at the beginning of the movement of great apes to Eurasia, soft and mixed fruit-eating coexisted with hard-object feeding in the Late Miocene, and a diet specializing in leaves did not evolve. The authors suggest that a progressive dietary diversification may have occurred due to competition and changes in the environment, but that this specialization may have ultimately lead to their extinction when more drastic environmental changes took place.

Citation: DeMiguel D, Alba DM, Moya-Sola S (2014) Dietary Specialization during the Evolution of Western Eurasian Hominoids and the Extinction of European Great Apes. PLoS ONE 9(5): e97442. doi:10.1371/journal.pone.0097442

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

Lead

Calcite, Galena Locality: Elmwood mine, Smith County, Tennessee, USA Size: small cabinet, 6.9 x 6.0 x 4.4 cm © Rob Lavinsky / iRocks

Chemical Formula: Pb
Locality: Langban, Sweden.
Name Origin: Anglo-Saxon, lead; Latin plumbum.

Lead is a chemical element in the carbon group with symbol Pb and atomic number 82. Lead is a soft and malleable heavy and post-transition metal. Metallic lead has a bluish-white color after being freshly cut, but it soon tarnishes to a dull grayish color when exposed to air. Lead has a shiny chrome-silver luster when it is melted into a liquid. It is also the heaviest non-radioactive element.

Lead is used in building construction, lead-acid batteries, bullets and shot, weights, as part of solders, pewters, fusible alloys, and as a radiation shield. Lead has the highest atomic number of all of the stable elements, although the next higher element, bismuth, has one isotope with a half-life that is so long (over one billion times the estimated age of the universe) that it can be considered stable. Lead’s four stable isotopes have 82 protons, a magic number in the nuclear shell model of atomic nuclei. The isotope lead-208 also has 126 neutrons, another magic number, and is hence double magic, a property that grants it enhanced stability: lead-208 is the heaviest known stable isotope.

If ingested, lead is poisonous to animals and humans, damaging the nervous system and causing brain disorders. Excessive lead also causes blood disorders in mammals. Like the element mercury, another heavy metal, lead is a neurotoxin that accumulates both in soft tissues and the bones. Lead poisoning has been documented from ancient Rome, ancient Greece, and ancient China.

Physical Properties

Cleavage: None
Color: Lead gray, Gray white.
Density: 11.37
Diaphaneity: Opaque
Fracture: Malleable – Deforms rather than breaking apart with a hammer.
Hardness: 2-2.5 – Gypsum-Finger Nail
Luminescence: Non-fluorescent.
Luster: Metallic
Magnetism: Nonmagnetic
Streak: lead gray

Photos:

Lead with Garnet Garpenberg Norra Mine, Garpenberg, Hedemora, Dalarna  Sweden (2011) Specimen size: 4.7 × 2.9 × 2.3 cm = 1.9” × 1.1” × 0.9” © Fabre Minerals
Lead on Hausmannite Langban, Vermland, Sweden Miniature, 4 x 3.7 x 2.2 cm © irocks
Lead and minium (Piombo e minio) Långban – Filipstad- Warmland – Sweden Specimen weight:30 gr. Overall size: 12mm x 8 mm x 22 mm © minservice
Långban, Filipstad, Värmland, Sweden © RWMW

Shattering past of the ‘island of glass’

Dr. Rebecca Williams and the remarkable volcanic deposit on Pantelleria island are shown. Credit: Credit: Mike Branney/ University of Leicester

University of Leicester team uncover explosive history of a ‘celebrity hotspot’

A tiny Mediterranean island visited by the likes of Madonna, Sting, Julia Roberts and Sharon Stone is now the focus of a ground-breaking study by University of Leicester geologists.

Pantelleria, a little-known island between Sicily and Tunisia, is a volcano with a remarkable past: 45 thousand years ago, the entire island was covered in a searing-hot layer of green glass.

Volcanologists Drs Mike Branney, Rebecca Williams and colleagues at the University of Leicester Department of Geology have been uncovering previously unknown facts about the island’s physical history.

And their study, published in “Geology” earlier this year, also provides insights into the nature of hazardous volcanic activity in other parts of the world.

Describing the volcanic activity on the island, Dr Branney said: “A ground-hugging cloud of intensely hot gases and volcanic dust spread radially out from the erupting volcano in all directions.

“Incandescent rock fragments suspended in the all-enveloping volcanic cloud were so hot, molten and sticky that they simply fused to the landscape forming a layer of glass, over hills and valleys alike. The hot glass then actually started flowing down all the slopes rather like sticky lava. ‘Ground zero’ in this case was the entire island – nothing would have survived – nature had sterilized and completely enamelled the island.

“Today Pantelleria is verdant and has been re-colonised, but even as you approach it by ferry you can see the green layer of glass covering everything – even sea cliffs look like they’ve been draped in candle wax. Exactly how this happened has only recently come to light.”

The Leicester team have reconstructed how the incandescent density current gradually inundated the entire island. They carefully mapped-out how the chemistry of the glass varies from place to place, and use this to show in unparalleled detail how the ground-hugging current at first was restricted to low, central areas, but then gradually advanced radially towards hills, eventually overtopping them all. Even more remarkably, the devastating current then gradually retreated from hill-tops, and the area covered by it gradually decreased so that, by the end of the eruption, only lower ground, close to the volcano continued to be immersed by it. Such advance-retreat behaviour may be typical of catastrophic currents in nature, such as at other volcanoes, and it may help us better understand undersea currents that are triggered by earthquakes.

“We are trying to ascertain whether this volcanic eruption was just a freak, oddball event. Well, it turns out that the delightful island, now used as a quiet getaway by celebrities, has been the site of at least five catastrophic eruptions of similar type.

“The remarkable volcanic activity on the island was not just a one-off. And as the volcano continues to steam away quite safely, it seems reasonable that in thousands of years time, it may once again erupt with devastating effect.

“Our investigations should help us understand what happens during similar and much larger explosive eruptions elsewhere around the world, such as the Yellowstone–Snake River region of USA”.

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

New, fossil-fuel-free process makes biodiesel sustainable

Allison Speers, MSU graduate student, works on a fuel cell that can eliminate biodiesel producers’ hazardous wastes and dependence on fossil fuels. Photo by Kurt Stepnitz

A new fuel-cell concept, developed by an Michigan State University researcher, will allow biodiesel plants to eliminate the creation of hazardous wastes while removing their dependence on fossil fuel from their production process.

The platform, which uses microbes to glean ethanol from glycerol and has the added benefit of cleaning up the wastewater, will allow producers to reincorporate the ethanol and the water into the fuel-making process, said Gemma Reguera, MSU microbiologist and one of the co-authors.

“With a saturated glycerol market, traditional approaches see producers pay hefty fees to have toxic wastewater hauled off to treatment plants,” she said. “By cleaning the water with microbes on-site, we’ve come up with a way to allow producers to generate bioethanol, which replaces petrochemical methanol. At the same time, they are taking care of their hazardous waste problem.”

The results, which appear in the journal Environmental Science and Technology, show that the key to Reguera’s platform is her patented adaptive-engineered bacteria – Geobacter sulfurreducens.

Geobacter are naturally occurring microbes that have proved promising in cleaning up nuclear waste as well in improving other biofuel processes. Much of Reguera’s research with these bacteria focuses on engineering their conductive pili or nanowires. These hair-like appendages are the managers of electrical activity during a cleanup and biofuel production.

MSU is working to eliminate biodiesel producers’ hazardous wastes and dependence on fossil fuels. Courtesy of Gemma Reguera

First, Reguera, along with lead authors and MSU graduate students Allison Speers and Jenna Young, evolved Geobacter to withstand increasing amounts of toxic glycerol. The next step, the team searched for partner bacteria that could ferment it into ethanol while generating byproducts that ‘fed’ the Geobacter.

“It took some tweaking, but we eventually developed a robust bacterium to pair with Geobacter,” Reguera said. “We matched them up like dance partners, modifying each of them to work seamlessly together and eliminate all of the waste.”

Together, the bacteria’s appetite for the toxic byproducts is inexhaustible.

“They feast like they’re at a Las Vegas buffet,” she added. “One bacterium ferments the glycerol waste to produce bioethanol, which can be reused to make biodiesel from oil feedstocks. Geobacter removes any waste produced during glycerol fermentation to generate electricity. It is a win-win situation.”

The hungry microbes are the featured component of Reguera’s microbial electrolysis cells, or MECs. These fuel cells do not harvest electricity as an output. Rather, they use a small electrical input platform to generate hydrogen and increase the MEC’s efficiency even more.

The promising process already has caught the eye of economic developers, who are helping scale up the effort. Through a Michigan Translational Research and Commercialization grant, Reguera and her team are developing prototypes that can handle larger volumes of waste.

Reguera also is in talks with MBI, the bio-based technology “de-risking” enterprise operated by the MSU Foundation, to develop industrial-sized units that could handle the capacities of a full-scale biodiesel plant. The next step will be field tests with a Michigan-based biodiesel manufacturer.

Note : The above story is based on materials provided by Michigan State University

Lazurite

Lazurite (Lapis Lazuli) Koksha Valley, Badakhshan Province, Afghanistan Small Cabinet, 6.1 x 4.7 x 4.5 cm © irocks

Chemical Formula: (Na,Ca)8[(S,Cl,SO4,OH)2|(Al6Si6O24)]
Locality: District of Badakhshan, Afghanistan.
Name Origin: From the Persian lazward – “blue.”

Lazurite is a tectosilicate mineral with sulfate, sulfur and chloride with formula: (Na,Ca)8[(S,Cl,SO4,OH)2|(Al6Si6O24)]. It is a feldspathoid and a member of the sodalite group. Lazurite crystallizes in the isometric system although well formed crystals are rare. It is usually massive and forms the bulk of the gemstone lapis lazuli.

Lazurite is a deep blue to greenish blue. The colour is due to the presence of S−3 anions. It has a Mohs hardness of 5.0 to 5.5 and a specific gravity of 2.4. It is translucent with a refractive index of 1.50. It is fusible at 3.5 and soluble in HCl. It commonly contains or is associated with grains of pyrite.

Lazurite is a product of contact metamorphism of limestone and typically is associated with calcite, pyrite, diopside, humite, forsterite, hauyne and muscovite.

History

Discovery date : 1890
Town of Origin : BADAKHSTAN PROV.
Country of Origin: AFGHANISTAN

Optical properties

Optical and misc. Properties : Translucent
Refractive Index: from 1,50 to 1,52

Physical Properties

Cleavage: {110} Imperfect
Color:  Blue, Azure blue, Violet blue, Greenish blue.
Density:  2.38 – 2.42, Average = 2.4
Diaphaneity:  Translucent
Fracture: Conchoidal – Fractures developed in brittle materials characterized by smoothly curving surfaces, (e.g. quartz).
Hardness:  5.5 – Knife Blade
Luminescence:  Non-Fluorescent.
Luster:   Vitreous – Dull
Streak:   light blue

Photos:

Lazurite on Marble Sar-E-Sang, Badakhshan, Afghanistan Miniature, 3.1 x 2.7 x 2.2 cm © irocks
Lazurite – Sar-e-Sang distr. Koksha valley – Badakhshan prov. – Afghanistan Specimen weight:224 gr. Crystal size:mm. 20 Overall size: 57mm x 60 mm x 62 mm © minservice
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 © H. Obodda

Lena River

River Lena and its watershed

The Lena is the easternmost of the three great Siberian rivers that flow into the Arctic Ocean (the other two being the Ob River and the Yenisei River). It is the 11th longest river in the world and has the 9th largest watershed. It is the largest among the rivers whose watershed is entirely within the Russian territorial boundaries.

Course

Rising at a height of 1,640 metres (5,381 ft) at its source in the Baikal Mountains south of the Central Siberian Plateau, 7 kilometres (4 mi) west of Lake Baikal, the Lena flows northeast, being joined by the Kirenga River, Vitim River and Olyokma River. From Yakutsk it enters the lowlands and flows north until joined by its right-hand tributary the Aldan River. The Verkhoyansk Range deflects it to the north-west; then after receiving its most important left-hand tributary, the Vilyuy River, it makes its way nearly due north to the Laptev Sea, a division of the Arctic Ocean, emptying south-west of the New Siberian Islands by the Lena Delta – 30,000 square kilometres (11,583 sq mi) in area, and traversed by seven principal branches, the most important being the Bykov, farthest east.

Basin

Neighbourhood of the sources of Lena River to Lake Baikal

The total length of the river is estimated at 4,400 km (2,700 mi). The area of the Lena river basin is calculated at 2,490,000 square kilometres (961,394 sq mi). Gold is washed out of the sands of the Vitim and the Olyokma, and mammoth tusks have been dug out of the delta.

Tributaries

The Kirenga River flows north between the upper Lena and Lake Baikal. The Vitim River drains the area northeast of Lake Baikal. The Olyokma River flows north. The Amga River makes a long curve southeast and parallel to the Lena and flows into the Aldan. The Aldan River makes similar curve southeast of the Aldan and flows into the Lena north of Yakutsk. The Maya River, a tributary of the Aldan, drains an area almost to the Sea of Okhotsk. The T-shaped Chona-Vilyuy River system drains most of the area to the west.

History

It is commonly believed that the river Lena derives its name from the original Even-Evenk name Elyu-Ene, which means “the Large River”.

According to folktales related a century after the fact, in the years 1620–23 a party of Russian fur hunters under the leadership of Demid Pyanda sailed up Lower Tunguska, and discovered the proximity of Lena and either carried their boats there or built new ones. In 1623 Pyanda explored some 2,400 kilometers of the river from its upper rocky part to its wide flow in the central Yakutia. In 1628 Vasily Bugor and ten men reached the Lena, collected yasak from the natives and founded Kirinsk in 1632. In 1631 the voyevoda of Yeniseisk sent Pyotr Beketov and twenty men to found an ostrog at Yakutsk (founded in 1632). From Yakutsk other expeditions spread out to the south and east. The Lena delta was reached in 1633.

Baron Eduard Von Toll, accompanied by Alexander von Bunge, carried out an expedition to the Lena delta area and the islands of New Siberia on behalf of the Russian Imperial Academy of Sciences in 1885. They explored the Lena delta with its multitude of arms that flow towards the Arctic Ocean. Then in spring 1886 they investigated the New Siberian Islands and the Yana River and its tributaries. During one year and two days the expedition covered 25,000 km, of which 4,200 km were up rivers, carrying out geodesic surveys en route.

Vladimir Ilyich Ulyanov may have taken his alias, Lenin, from the river Lena, when he was exiled to the Central Siberian Plateau, but the origin of his pen name is uncertain.

Lena delta

Lena river Delta by Landsat 2000

At the end of the Lena River there is a large delta that extends 100 kilometres (62 mi) into the Laptev Sea and is about 400 km (250 mi) wide. The delta is frozen tundra for about 7 months of the year, but in May transforms the region into a lush wetland for the next few months. Part of the area is protected as the Lena Delta Wildlife Reserve.

The Lena delta divides into a multitude of flat islands. The most important are (from west to east): Chychas Aryta, Petrushka, Sagastyr, Samakh Ary Diyete, Turkan Bel’keydere, Sasyllakh Ary, Kolkhoztakh Bel’keydere, Grigoriy Diyelyakh Bel’kee (Grigoriy Islands), Nerpa Uolun Aryta, Misha Bel’keydere, Atakhtay Bel’kedere, Arangastakh, Urdiuk Pastakh Bel’key, Agys Past’ Aryta, Dallalakh Island, Otto Ary, Ullakhan Ary and Orto Ues Aryta.

Turukannakh-Kumaga is a long and narrow island off the Lena delta’s western shore.

One of the Lena delta islands, Ostrov Amerika-Kuba-Aryta or Ostrov Kuba-Aryta, was named after the island of Cuba during Soviet times. It is on the northern edge of the delta.

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

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