Thursday, March 4, 2010

JRF New Delhi March 10 deadline

Hello,

Department of Geology, Centre of Advanced Studies
Delhi University, Delhi 110 007

Applications are invited for two JRF positions with monthly emoluments
@ Rs 12,000 + HRA (30%) for
one year (may be extendable for 3 years) to work on two different
research projects.

JRF 1: First JRF position is in the sponsored research project
entitled ‘River Dynamics and Flood
Risk Evaluation of the Kosi River, North Bihar Plains: An Integrated
Approach’ supported by
Ministry of Earth Sciences, Government of India.

JRF 2: Second JRF position is in the sponsored research project
entitled ‘Morphotectonic
Variability Along the NW Himalayan Front: Tectonics-Climate Coupling’
supported by Department
of Science and Technology (DST), Government of India.

The candidates should have M.Sc./M.Tech. degree in Geology/Applied
Geology/Earth Sciences/
Geography or related subjects. Applicant with some experience in
Remote sensing/GIS analysis
and/or fluvial geomorphology will be preferred. The application
(mentioning the research project and
properly signed by the applicant) on a plain paper may be submitted to
Dr Vikrant Jain
Department of Geology, Centre of Advanced
Studies, Delhi University, Delhi 110 007 within March 15, 2010
Applications can also be submitted through e-mail to Dr Vikrant Jain
(vjain@geology.du.ac.in; vikrantgeo@gmail.com).

best wishes
Dr.R.V.Rajan

Two posts of geologist in Hutti Gold Mines

Hello,

Two posts of geologist in Hutti Gold Mines

Geologists
2 Posts
First Class PG Degree in Geology/Applied Geology. 1-2 years experience
in exploration and mining for gold preferred. Computer Knowledge of
GIS & GPS software as well as Geological & Mining software essential.

30 years.

Rs.12800-425-14050-475-16400-525-18500-575-20800-625-23300-675-26000.

Apply as early as possible.

Age will be relaxed in case of exceptionally suitable candidates.
Knowledge of Kannada is essential.
Preference will be given to candidates having Industrial experience in
the respective discipline, relaxation in experience will be given in
exceptional cases.
Candidates applying for the posts are eligible for the following
Besides pay Dearness Allowance as admissible as per the rules of the
Company, contribution to Provident Fund, Semi-furnished accommodation
and Medical facilities for self and family plus other perquisites as
admissible to the Officers as per the Rules of the Company. Interested
candidates may apply within 15 days from the date of publication of
this advertisement giving full bio-data along with copies of academic
qualifications and caste certificate to the Executive Director, Hutti
Gold Mines Co. Ltd., PO HUTTI – 584 115, Raichur District, Karnataka
State.
www.huttigold.org

Cheers

Dr.R.V.Rajan

NASA Radar Finds Ice Deposits at Moon's North Pole; Additional Evidence of Water Activity on Moon

------------------------------------------------------------------------------------------------------

 Mini-SAR map of the Circular Polarization Ratio (CPR) of the north pole of the Moon. Fresh, "normal" craters (red circles) show high values of CPR inside and outside their rims. This is consistent with the distribution of rocks and ejected blocks around fresh impact features, indicating that the high CPR here is surface scattering. The "anomalous" craters (green circles) have high CPR within, but not outside their rims. Their interiors are also in permanent sun shadow. These relations are consistent with the high CPR in this case being caused by water ice, which is only stable in the polar dark cold traps. We estimate over 600 million cubic meters (1 cubic meter = 1 metric ton) of water in these features. (Credit: NASA)

---------------------------------------------------------------------------------------------------

Using data from a NASA radar that flew aboard India's Chandrayaan-1 spacecraft, scientists have detected ice deposits near the moon's north pole. NASA's Mini-SAR instrument, a lightweight, synthetic aperture radar, found more than 40 small craters with water ice. The craters range in size from 1 to 9 miles (2 to15 km) in diameter. Although the total amount of ice depends on its thickness in each crater, it's estimated there could be at least 600 million metric tons of water ice.

"The emerging picture from the multiple measurements and resulting data of the instruments on lunar missions indicates that water creation, migration, deposition and retention are occurring on the moon," said Paul Spudis, principal investigator of the Mini-SAR experiment at the Lunar and Planetary Institute in Houston. "The new discoveries show the moon is an even more interesting and attractive scientific, exploration and operational destination than people had previously thought."

During the past year, the Mini-SAR mapped the moon's permanently-shadowed polar craters that aren't visible from Earth. The radar uses the polarization properties of reflected radio waves to characterize surface properties. Results from the mapping showed deposits having radar characteristics similar to ice.

"After analyzing the data, our science team determined a strong indication of water ice, a finding which will give future missions a new target to further explore and exploit," said Jason Crusan, program executive for the Mini-RF Program for NASA's Space Operations Mission Directorate in Washington.

The Mini-SAR's findings are being published in the journal Geophysical Research Letters. The results are consistent with recent findings of other NASA instruments and add to the growing scientific understanding of the multiple forms of water found on the moon. The agency's Moon Mineralogy Mapper discovered water molecules in the moon's polar regions, while water vapor was detected by NASA's Lunar Crater Observation and Sensing Satellite, or LCROSS.

Mini-SAR and Moon Mineralogy Mapper are two of 11 instruments on the Indian Space Research Organization's Chandrayaan-1. The Applied Physics Laboratory in Laurel, Md., performed the final integration and testing on Mini-SAR. It was developed and built by the Naval Air Warfare Center in China Lake, Calif., and several other commercial and government contributors.

For more information about NASA's Mini-SAR, also known as Mini-RF, visit: http://www.nasa.gov/mini-rf

For more information about the Moon Mineralogy Mapper, visit: http://m3.jpl.nasa.gov

For more information about LCROSS, visit: http://www.nasa.gov/lcross

For more information about Chandrayaan-1, visit: http://www.isro.org/Chandrayaan
Adapted from materials provided by NASA.

Mass Loss from Alaskan Glaciers Overestimated?


Mass Loss from Alaskan Glaciers Overestimated? Previous Melt Contributed a Third Less to Sea-Level Rise Than Estimated

-----------------------------------------------------------------------------------------------------

 NAU geographer Erik Schiefer surveys a debris-covered glacier margin.
(Credit: Photo by Amanda Stan)
----------------------------------------------------------------------------------------------------
The melting of glaciers is well documented, but when looking at the rate at which they have been retreating, a team of international researchers steps back and says not so fast.

Previous studies have largely overestimated mass loss from Alaskan glaciers over the past 40-plus years, according to Erik Schiefer, a Northern Arizona University geographer who coauthored a paper in the February issue of Nature Geoscience that recalculates glacier melt in Alaska.

The research team, led by Étienne Berthier of the Laboratory for Space Studies in Geophysics and Oceanography at the Université de Toulouse in France, says that glacier melt in Alaska between 1962 and 2006 contributed about one-third less to sea-level rise than previously estimated.

Schiefer said melting glaciers in Alaska originally were thought to contribute about .0067 inches to sea-level rise per year. The team's new calculations put that number closer to .0047 inches per year. The numbers sound small, but as Schiefer said, "It adds up over the decades."

While the team looked at three-fourths of all the ice in Alaska, Schiefer noted, "We're also talking about a small proportion of ice on the planet. When massive ice sheets (such as in the Antarctic and Greenland) are added in, you're looking at significantly greater rates of sea-level rise."

Schiefer said the team plans to use the same methodologies from the Alaskan study in other glacial regions to determine if further recalibrations of ice melt are in order. These techniques use satellite imagery that spans vast areas of ice cover.

Previous methods estimated melt for a smaller subset of individual glaciers. The most comprehensive technique previously available used planes that flew along the centerlines of selected glaciers to measure ice surface elevations. These elevations were then compared to those mapped in the 1950s and 1960s. From this, researchers inferred elevation changes and then extrapolated this to other glaciers.

Two factors led to the original overestimation of ice loss with this method, Schiefer said. One is the impact of thick deposits of rock debris that offer protection from solar radiation and, thus, melting. The other was not accounting for the thinner ice along the edges of glaciers that also resulted in less ice melt.

Schiefer and his colleagues used data from the SPOT 5 French satellite and the NASA/Japanese ASTER satellite and converted the optical imagery to elevation information. They then compared this information to the topographical series maps of glacial elevations dating back to the 1950s.

While the team determined a lower rate of glacial melt during a greater than 40-year span, Schiefer said other studies have demonstrated the rate of ice loss has more than doubled in just the last two decades.

"With current projections of climate change, we expect that acceleration to continue," Schiefer said. This substantial increase in ice loss since the 1990s is now pushing up the rise in sea level to between .0098 inches and .0118 inches per year -- more than double the average rate for the last 40 years.

Working on the Alaskan glacial melt revision with Schiefer and Berthier were Garry Clarke of the University of British Columbia, Brian Menounos of the University of Northern British Columbia and Frédérique Rémy of the Université de Toulouse.
Adapted from materials provided by Northern Arizona University.

Journal Reference:
E. Berthier, E. Schiefer, G. K. C. Clarke, B. Menounos & F. Rémy. Contribution of Alaskan glaciers to sea-level rise derived from satellite imagery. Nature Geoscience, 2010; 3 (2): 92 DOI: 10.1038/ngeo737

'Missing Link' Fossil, Not Human Ancestor?


'Missing Link' Fossil Was Not Human Ancestor as Claimed, Anthropologists Say
---------------------------------------------------------------------------------------------------
Radiographs of the type specimen of Darwinius masillae, new genus and species, from Messel in Germany. (Credit: Franzen JL, Gingerich PD, Habersetzer J, Hurum JH, von Koenigswald W, et al. Complete Primate Skeleton from the Middle Eocene of Messel in Germany: Morphology and Paleobiology. PLoS ONE, 2009; 4(5): e5723 DOI: 10.1371/journal.pone.0005723)
---------------------------------------------------------------------------------------------------

A fossil that was celebrated last year as a possible "missing link" between humans and early primates is actually a forebearer of modern-day lemurs and lorises, according to two papers by scientists at The University of Texas at Austin, Duke University and the University of Chicago.

In an article now available online in the Journal of Human Evolution, four scientists present evidence that the 47-million-year-old Darwinius masillae is not a haplorhine primate like humans, apes and monkeys, as the 2009 research claimed.

They also note that the article on Darwinius published last year in the journal PLoS ONE ignores two decades of published research showing that similar fossils are actually strepsirrhines, the primate group that includes lemurs and lorises.

"Many lines of evidence indicate that Darwinius has nothing at all to do with human evolution," says Chris Kirk, associate professor of anthropology at The University of Texas at Austin. "Every year, scientists describe new fossils that contribute to our understanding of primate evolution. What's amazing about Darwinius is, despite the fact that it's nearly complete, it tells us very little that we didn't already know from fossils of closely related species."

His co-authors are anthropologists Blythe Williams and Richard Kay of Duke and evolutionary biologist Callum Ross of the University of Chicago. Williams, Kay and Kirk also collaborated on a related article about to be published in the Proceedings of the National Academy of Sciences that reviews the early fossil record and anatomical features of anthropoids -- the primate group that includes monkeys, apes, and humans.

Last spring's much-publicized article on Darwinius was released in conjunction with a book, a History Channel documentary, and an exhibit in the American Museum of Natural History. At a news conference attended by New York Mayor Michael Bloomberg, the authors unveiled the nearly complete fossil of a nine-month-old female primate that had been found at the site of Messel in Germany.

But other anthropologists were immediately skeptical of the conclusions and began writing the responses that are being published this month.

"Just because it's a complete and well-preserved fossil doesn't mean it's going to overthrow all our ideas," says Williams, the lead author. "There's this enormous body of literature that has built up over the years. The Darwinius research completely ignored that body of literature."

That literature centers on the evolution of primates, which include haplorhines (apes, monkeys, humans, tarsiers) and strepsirrhines (lemurs, lorises). The two groups split from each other nearly 70 million years ago.

The fossil group to which Darwinius belongs -- the adapiforms -- have been known since the early 1800s and includes dozens of primate species represented by thousands of fossils recovered in North America, Europe, Asia and Africa. Some adapiforms, like North American Notharctus, are known from nearly complete skeletons like that of Darwinius. Most analyses of primate evolution over the past two decades have concluded that adapiforms are strepsirrhines, and not direct ancestors of modern humans.

The most recent such analysis, published last year in the journal Nature, concluded that Darwinius is an early strepsirrhine and a close relative of the 39-million-year- old primate Mahgarita stevensi from West Texas.

Nevertheless, the scientists who last year formally described Darwinius concluded that it was an early haplorhine, and even suggested that Darwinius and other adapiform fossils "could represent a stem group from which later anthropoid primates evolved."

For example, they note that Darwinius has a short snout and a deep jaw -- two features that are found in monkeys, apes, and humans.

However, Kirk, Williams and their colleagues point out that short snouts and deep jaws are known to have evolved multiple times among primates, including several times within the lemur/loris lineage. They further argue that Darwinius lacks most of the key anatomical features that could demonstrate a close evolutionary relationship with living haplorhines (apes, monkeys, humans, and tarsiers).

For instance, haplorhines have a middle ear with two chambers and a plate of bone that shields the eyes from the chewing muscles.

"There is no evidence that Darwinius shared these features with living haplorhines," says Kirk. "And if you can't even make that case, you can forget about Darwinius being a close relative of humans or other anthropoids."
Adapted from materials provided by University of Texas at Austin, via EurekAlert!, a service of AAAS.

Journal Reference:
Blythe A. Williams, Richard F. Kay, E. Christopher Kirk, Callum F. Ross. Darwinius masillae is a strepsirrhine -- a reply to Franzen et al. (2009). Journal of Human Evolution, 2010; DOI: 10.1016/j.jhevol.2010.01.003

Stars in the Making on Outskirts of Orion


'Cosmic Bat': Island of Stars in the Making on Outskirts of Orion

----------------------------------------------------------------------------------------------------

The Cosmic Bat -- NGC 1788. (Credit: ESO)

---------------------------------------------------------------------------------------------------
The delicate nebula NGC 1788, located in a dark and often neglected corner of the Orion constellation, is revealed in a new and finely nuanced image that the European Southern Observatory is releasing. Although this ghostly cloud is rather isolated from Orion's bright stars, the latter's powerful winds and light have had a strong impact on the nebula, forging its shape and making it home to a multitude of infant suns.

Stargazers all over the world are familiar with the distinctive profile of the constellation of Orion (the Hunter). Fewer know about the nebula NGC 1788, a subtle, hidden treasure just a few degrees away from the bright stars in Orion's belt.

NGC 1788 is a reflection nebula, whose gas and dust scatter the light coming from a small cluster of young stars in such a way that the tenuous glow forms a shape reminiscent of a gigantic bat spreading its wings. Very few of the stars belonging to the nebula are visible in this image, as most of them are obscured by the dusty cocoons surrounding them. The most prominent, named HD 293815, can be distinguished as the bright star in the upper part of the cloud, just above the centre of the image and the pronounced dark lane of dust extending through the nebula.

Although NGC 1788 appears at first glance to be an isolated cloud, observations covering a field beyond the one presented in this image have revealed that bright, massive stars, belonging to the vast stellar groupings in Orion, have played a decisive role in shaping NGC 1788 and stimulating the formation of its stars. They are also responsible for setting the hydrogen gas ablaze in the parts of the nebula facing Orion, leading to the red, almost vertical rim visible in the left half of the image.

All the stars in this region are extremely young, with an average age of only a million years, a blink of an eye compared to the Sun's age of 4.5 billion years. Analysing them in detail, astronomers have discovered that these "preschool" stars fall naturally into three well separated classes: the slightly older ones, located on the left side of the red rim, the fairly young ones, to its right, making up the small cluster enclosed in the nebula and illuminating it, and eventually the very youngest stars, still deeply embedded in their nascent dusty cocoons, further to the right. Although none of the latter are visible in this image because of the obscuring dust, dozens of them have been revealed through observations in the infrared and millimetre wavelengths of light.

This fine distribution of stars, with the older ones closer to Orion and the younger ones concentrated on the opposite side, suggests that a wave of star formation, generated around the hot and massive stars in Orion, propagated throughout NGC 1788 and beyond.

This image has been obtained using the Wide Field Imager on the MPG/ESO 2.2-metre telescope at ESO's La Silla Observatory in Chile.
Adapted from materials provided by European Southern Observatory - ESO.