The post-Columbian panmictic “natural experiment” | Gene Expression

Economists in the last few years have been shifting toward testing their theoretical models, whether through the experiments of behavioral economics, or, “natural experiments.” The reason economists have had issues with testing their models is that experimentation on humans has some natural constraints. Macroeconomists have an even greater problem, as experimentation on whole societies not only presents ethical conundrums, but there’s no way to fund or implement experiments on this scale. Macroeconomists turn out to be the paleontologists of economics.

Of course economists aren’t the only ones who’ve had this sort of problem with humans. The reason that geneticists focused on organisms such as flies, mice and fish is partly that these taxa breed fast and are easy to maintain in laboratories. But obviously there are things you can do, such as mutagenesis, with model organisms which you can not do with humans. Human genetics has traditionally relied on “natural experiments” of a sort, inbred lineages, recurrent recessive diseases, etc. Genetics has been a supplementary handmaid to medicine by and large. But sometimes history can load the die in genetics’ favor as well.

624px-Zoe_Saldana_at_2010_ODuring the “Columbian Exchange” the New and Old World engaged in a massive transfer of ideas and individuals. The Old World received potatoes, maize, and tomatoes (to name a few). The New World…well, the New World received black people and white people. As documented in works such as 1491 the indigenous populations of the New World collapsed with the introduction of Old World diseases. Native peoples disappeared from the Caribbean, and were marginalized on the mainland excepting ecologically remote (e.g., the Guatemalan highlands) or forbidding (e.g., the Peruvian highlands) regions. But of course despite the obliteration of indigenous cultural self-consciousness and identity, the native populations did not totally disappear, they persisted genetically in the numerically dominant mestizo populations of much of Latin America. You don’t need genetics to understand what happened, books like Mestizaje in Ibero-America outline in detail using conventional historical archives how Spanish men arrived in New World and entered into relationships with indigenous women. Often several at a time, in contravention of the Catholic Church’s requirement of monogamy.

But in the post-genomic era we have more to go on than impressions, we can quantitize the extent and nature of the admixture, something of importance when considering medical research. A new paper in PNAS adds some more to the growing body of results on Latin American genomics by including populations which have traditionally been overlooked, and also putting a spotlight on the long term impact of sex-biased admixture. Genome-wide patterns of population structure and admixture among Hispanic/Latino populations:

Hispanic/Latino populations possess a complex genetic structure that reflects recent admixture among and potentially ancient substructure within Native American, European, and West African source populations. Here, we quantify genome-wide patterns of SNP and haplotype variation among 100 individuals with ancestry from Ecuador, Colombia, Puerto Rico, and the Dominican Republic genotyped on the Illumina 610-Quad arrays and 112 Mexicans genotyped on Affymetrix 500K platform. Intersecting these data with previously collected high-density SNP data from 4,305 individuals, we use principal component analysis and clustering methods FRAPPE and STRUCTURE to investigate genome-wide patterns of African, European, and Native American population structure within and among Hispanic/Latino populations. Comparing autosomal, X and Y chromosome, and mtDNA variation, we find evidence of a significant sex bias in admixture proportions consistent with disproportionate contribution of European male and Native American female ancestry to present-day populations. We also find that patterns of linkage-disequilibria in admixed Hispanic/Latino populations are largely affected by the admixture dynamics of the populations, with faster decay of LD in populations of higher African ancestry. Finally, using the locus-specific ancestry inference method LAMP, we reconstruct fine-scale chromosomal patterns of admixture. We document moderate power to differentiate among potential subcontinental source populations within the Native American, European, and African segments of the admixed Hispanic/Latino genomes. Our results suggest future genome-wide association scans in Hispanic/Latino populations may require correction for local genomic ancestry at a subcontinental scale when associating differences in the genome with disease risk, progression, and drug efficacy, as well as for admixture mapping.

The issue here is that “Hispanic” and/or “Latino” is not a race. In fact, as American readers may be aware the category emerged in 1970 as a way of organizing ethnic and racial identity for the Census. Despite a real pan-American consciousness there is obviously a great deal of cultural and genetic variation in Latin America. Caribbean nations which a large African component have a different identity from Mexico, where the non-Spanish segment is indigenous. Conversely, Argentina has a self conception as a white nation, despite some ambiguity in genetics.

In this paper they focused on 100 individuals from Mexico, Columbia, Ecuador, Dominican Republic and Puerto Rico. This gives them a good coverage of different regions of Latin America, and also looks into populations which are not often included in these studies, such as Dominicans. A series of figures highlights the primary results.

I’ve rotated this figure to maintain its resolution. It’s a Frappe analysis of the ancestry of individuals within various populations assuming K ancestral populations. With Latin Americans the idea of ancestral populations makes a bit more sense, since we know what the ancestral populations are! They use the HGDP populations as a reference for points of comparison.

F1.large

Since we’re focused on native, Africa and white ancestry, K = 3 is probably more important. No surprise that the Latin America populations exhibit variation in ancestral quanta within them. Some Mexicans look like Europeans. Some Mexicans look like Native Americans. And some Mexicans look mixed. I assume that most readers are aware of this, assuming that they encounter Mexicans at all in their daily life.

Of course the ancestry came in through different avenues. The sexual exploitation of black females by white males in the United States is well known, but it does seem that the same dynamic, at least in terms of the genetic combination, existed in Latin America for much of its history, with black females being complemented by indigenous females. Figure 5 illustrates this well. You see the various Latin American populations (the abbreviations should be obvious). The boxes span the 1st to 3rd quartile in ancestry within each subpopulation from each respective ancestral group (the whiskers represent the ranges). Note the differences between the X chromosome, which spends 2/3 of its time in females, and the autosome, which is not sex biased.

F5.large

Ah, but we can get more precise than that. They typed these individuals on their mtDNA, which is passed purely through women, and their Y chromosomes, which is passed purely through men. These loci do not recombine, and so are transmitted in such a manner that it is relatively easy to reconstruct their phylogenies. There has been a great deal of phylogeographic exploration of these two loci. In the next figure what you see are the position of the individuals in this study in terms of total genome content distance from the three ancestral populations, but, the color of their positions is dictated by the origin of their mtDNA and Y lineages.

F6.largeThe top panel are male lineages, and the bottom panel are female lineages. The preponderance of European ancestry, in relation to native and African ancestry, seems rather clear on the autosomal genome. There is admixture, but you have more people concentrating at the European vertex than at the other two. Most of the Y lineages, presumably men, are European. Some are African, and a few are native. Interestingly they note in the text that several lineages associated with North Africa and the Middle East are found in these populations. Why? The answer seems relatively simple: they were brought by the Muslim invaders, or were Jews, who later became Christian. There have been many phylogeographic analyses of Y lineage distributions, and believe it or not Iberia and North Africa are actually strongly differentiated. The Middle Eastern lineages I’m betting are from Sephardic Jews; most of the “Moors” who settled in Spain are likely to have had more Berber than Arab ancestry.

The maternal lineages show a really interesting pattern. There are a preponderance of native mtDNA lineages, and a significant number of African ones. But notice that most people of overwhelming European ancestry nevertheless retain a native maternal lineage! We saw this in Argentina, a population which identifies as white, seems to be highly admixed on the mtDNA. I suspect that what you’re seeing is the long reach of the first mothers, whose descendants intermarried with Spanish men who relocated to the New World. The Aztec and Inca nobility gave their daughters to the Spaniards who arrived, and I suspect that the predominantly European elites of Latin America still carry those lineages with them, despite their overwhelming limpieza de sangre. Another important point is that both Dominicans, and especially Puerto Ricans, carry signatures of these first mothers (as well as total genome content). 20 of 27 Puerto Ricans carry native mtDNA. This is somewhat shocking, as these Caribbean islands were reputed to have been nearly devoid of indigenous populations only a generation after First Contact, in large part due to disease.

Which brings me back to Neandertals. Non-African humans may carry somewhat less than 5% of their ancestry from this population. But to my knowledge there is no cultural continuity, and we do conceive of ourselves as fundamentally different from the Neander-kind. And yet genetically the Neandertals are highly successful through us The chaos, havoc, and population collapse wrecked by the Europeans when they encountered native New World populations may be somewhat analogous to what happened to archaic groups who had to face the oncoming demographic blast of African humans. And yet some of the genetic material of the locals was absorbed just before their extinction. The half-Taino children whose fathers were Spanish may have had the genetic defenses of European diseases which allowed them to survive the hardships of their lives. Granted, these children lost a genuine connection with their Taino ancestors, but the descent of those native peoples still persists onward. Interestingly, some readers of this weblog have had the same reaction to the idea that Neandertals persist in our own genome. Ultimately the reaction and response to this is not a scientific issue, but a normative one. Dare I even say, a spiritual one?

Citation: Bryc K, Velez C, Karafet T, Moreno-Estrada A, Reynolds A, Auton A, Hammer M, Bustamante CD, & Ostrer H (2010). In the Light of Evolution IV: The Human Condition Sackler Colloquium: Genome-wide patterns of population structure and admixture among Hispanic/Latino populations. Proceedings of the National Academy of Sciences of the United States of America PMID: 20445096

Image Credit: Cristiano Del Riccio

Testimony Highlights 3 Major Failures That Caused Gulf Spill | 80beats

gulfspill511Like the CEOs of failing car companies and steroid-suspected baseball players before them, the leaders of BP, Transocean, and Halliburton had to trek up to Capitol Hill today to stand before Congress. The three company executives played circle-of-blame in front of the Senate Energy and Natural Resources Committee. To sum up their statements:

BP: It was Transocean’s fault.

Transocean: It was Halliburton’s fault.

Halliburton: It was BP’s fault.

Since we may not know the whole story about the Deepwater Horizon’s explosion and sinking that resulted in the current environmental disaster in the Gulf, let’s recap the technical failures.

1. Blowout preventer

This piece of equipment, previously anonymous to most of the public, is now notorious for its failure to do its job—closing off the well automatically in response to a sudden emergency. Lamar McKay, president and chairman of BP America, used that fact to deflect blame:

Since Transocean owned the rig’s safety equipment, Mr. McKay said that Transocean was responsible; he added that there were “anomalous pressure test readings” before the explosion that “could have raised concerns” [The New York Times].

However, just after the accident, BP’s CEO Tony Heyward said that a blowout preventer’s failure was “unprecedented.” Not exactly, according to the AP’s investigation, which found many examples of accidents this decade in which failed blowout preventers played a role. Transocean knew about the issues, the AP says, but so did the federal government.

In the late 1990s, the industry appealed for fewer required pressure tests on these valves. The federal [Minerals Management Service] did two studies, each finding that failures were more common than the industry said. But the agency, known as MMS, then did its turnaround and required tests half as often. It estimated that the rule would yield an annual savings of up to $340,000 per rig. An industry executive praised the “flexibility” of regulators, long plagued with accusations that it has been too cozy with the industry it supervises [AP].

2. Cementing

OK, Transocean chief executive Steve Newman said, there was a blowout preventer failure, but that was not the root cause of the explosion or the leak.

“The one thing we know with certainty is that on the evening of April 20 there was a sudden, catastrophic failure of the cement, the casing, or both,” Newman said. The cementing job was done by Halliburton [The Washington Post].

In fact, Halliburton was still working on its cementing job 20 hours before the explosion.

There was already a pipe in the well for the oil to flow through, but no oil was supposed to flow yet. Cementing, one of the last steps in well construction, seals the crack between the pipe and the wall of rock. Crews pump the cement through the pipe, but it ends up on the outside of the pipe, in the space between the pipe and the rock wall. The cement also caps the bottom of the pipe [NPR].

Cementing could go bad if the material isn’t mixed to the correct consistency. If any oil and gas leaks out early, NPR reports, it can cause a pocket in the cement that doesn’t seal up. And if cement doesn’t set properly, oil and gas could escape the well and even explode.

3. Oversight, and response failures

While Transocean owned the rig and Halliburton poured the concrete, this was BP’s show. And, so, the other two companies also employed the “just following orders” defense.

Halliburton was “contractually bound,” to follow BP’s instructions, Tim Probert, president of global business lines for the Houston-based energy services company, will tell the panel.

“All offshore oil and gas production projects begin and end with the operator,” Stephen Newman, chief executive officer of Swiss drilling company Transocean said in his prepared remarks. BP, the London-based oil company, decided “where and how” its well was to be drilled, Newman said [BusinessWeek].

Whatever BP’s failures were in administering the the drilling operation and preventing an accident (and those will most likely continue to leak out, like oil into the Gulf), the company’s attempts to mitigate the spill have met with limited success. BP’s initial attempt to shut of the flow, using robot submersibles to close of the valves, has failed. After the company built its 100-ton containment dome to try to capture the flow and pump it to a tanker on the surface, icy buildup of methane and water at the depth of 5,000 feet prevented the dome from getting a seal.

The methane that caused the original explosion remains gaseous down to -161°C. The “ice” that’s forming is actually a solidified mixture of methane and water called a clathrate [Ars Technica].

Faced with dwindling options and still two months before a relief well could be completed, BP is even considering throwing garbage at the leak in the form of a “junk shot” in a last-ditch effort to stem the flow.

“They have horribly underestimated the likelihood of a spill and therefore horribly underestimated the consequences of something going wrong,” said Robert Bea, a professor at the University of California, Berkeley, who studies offshore drilling. “So what we have now is some equivalent of a fire drill with paper towels and buckets for cleanup” [Dallas Morning News].

Previous posts on the BP oil spill:
80beats: 5 Offshore Oil Hotspots Beyond the Gulf That Could Boom—Or Go Boom
80beats: Gulf Oil Spill: Do Chemical Dispersants Pose Their Own Environmental Risk?
80beats: Gulf Oil Spill: Fisheries Closed; Louisiana Wetlands Now in Jeopardy
80beats: Gulf Oil Spill Reaches U.S. Coast; New Orleans Reeks of “Pungent Fuel Smell”
80beats: Uh-Oh: Gulf Oil Spill May Be 5 Times Worse Than Previously Thought

Image: U.S. Coast Guard


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U.S. Government Granted Exemptions after Oil Leak

*Video: best and worst case scenarios from homeland security secretary janet napolitano in biloxi, miss., last week.

In this video, Homeland Security Secretary Janet Napolitano discusses worst and best case scenarios while in Biloxi, Miss., last week. McClatchy media has uncovered an astounding bit of information, given the devastation that is happening in the Gulf of Mexico.   There should, right now, be a moratorium on new drilling permits in the Gulf of Mexico, or at least that is what we have been led to believe.   It’s not the truth, though. Exemptions for new drilling are being granted dirty oil production in the Gulf of Mexico, even while the current disaster is still unfolding.*

WASHINGTON — Since the Deepwater Horizon oil drilling rig exploded on April 20, the Obama administration has granted oil and gas companies at least 27 exemptions from doing in-depth environmental studies of oil exploration and production in the Gulf of Mexico.

The waivers were granted despite President Barack Obama’s vow that his administration would launch a “relentless response effort” to stop the leak and prevent more damage to the gulf. One of them was dated Friday — the day after Interior Secretary Ken Salazar said he was temporarily halting offshore drilling

The exemptions, known as “categorical exclusions,” were granted by the Interior Department’s Minerals Management Service (MMS) and included waiving detailed environmental studies for a BP exploration plan to be conducted at a depth of more than 4,000 feet and an Anadarko Petroleum Corp. exploration plan at more 9,000 feet.

“Is there a moratorium on off shore drilling or not?” asked Peter Galvin, conservation director with the Center for Biological Diversity, the environmental group that discovered the administration’s continued approval of the exemptions. “Possibly the worst environmental disaster in U.S. history has occurred and nothing appears to have changed.”

MMS officials said the exemptions are continuing to be issued because they do not represent final drilling approval.”

Or, we are not being told the truth about what the U.S. government is really doing or intending to do about offshore drilling.  Now that we know President Obama doesn’t appear to be serious about fighting climate change, he was probably never serious about a “clean green economy” either.  Oil and gas and coal run the U.S. economy, they control our Congress, and it appears that they also control all facets of our government. We are a corporation controlled economy, and this is led by big fossil fuel companies and giant banks. It’s time for some real reform in the U.S.

Read more here: http://www.mcclatchydc.com/2010/05/07/93761/despite-spill-feds-still-giving.html#none#ixzz0nhnSvVUY

Could our government’s plan be to completely trash the Atlantic Ocean? That’s what it looks like. We now know without a doubt that big corporations like Transocean, Halliburton, and BP don’t care anything about our environment. Their product is dirty and polluting, from the moment it’s pumped out [...]

NASA Deploys Planes, Targets Satellites to Aid in Oil Spill Response

NASA sent its ER-2 research aircraft from California to Texas on May 6 for a series of flights to map the oil spill and coastal areas with an advanced instrument onboardNASA has mobilized its remote-sensing assets to help assess the spread and impact of the Deepwater Horizon BP oil spill in the Gulf of Mexico at the request of U.S. disaster response agencies.

As part of the national response to the spill, NASA deployed its instrumented research aircraft the Earth Resources-2 (ER-2) to the Gulf on May 6. The agency is also making extra satellite observations and conducting additional data processing to assist the National Oceanic and Atmospheric Administration (NOAA), the U.S. Geological Survey (USGS), and the Department of Homeland Security in monitoring the spill.

"NASA has been asked to help with the first response to the spill, providing imagery and data that can detect the presence, extent, and concentration of oil," said Michael Goodman, program manager for natural disasters in the Earth Science Division of NASA's Science Mission Directorate in Washington. "We also have longer-term work we have started in the basic research of oil in the ocean and its impacts on sensitive coastal ecosystems."

At NOAA's request, NASA sent the ER-2 outfitted with the Airborne Visible/Infrared Imaging Spectrometer (AVIRIS) and the Cirrus Digital Camera System to collect detailed images of the Gulf of Mexico and its threatened coastal wetlands. The camera system is supplied by NASA’s Ames Research Center, Moffett Field, Calif.

NASA pilots flew the ER-2 from NASA's Dryden Flight Research Center in California to a temporary base of operations at Johnson Space Center's Ellington Field in Houston. Along the way, the plane collected data over the Gulf coast and the oil slick to support spill mapping and document the condition of coastal wetlands before oil landfall. The ER-2 made a second flight on May 10 and more flights are planned.

The AVIRIS team led by Robert Green of NASA's Jet Propulsion Laboratory is measuring how the water absorbs and reflects light in order to map the location and concentration of oil, which separates into a widespread, thin sheen and smaller thick patches. Satellites can document the overall extent of the oil but cannot distinguish between the sheen and thick patches. While the sheen represents most of the area of the slick, the majority of the oil is concentrated in the thicker part. AVIRIS should be able to identify the thicker parts, helping oil spill responders know where to deploy oil-skimming boats and absorbent booms.

Researchers also plan to measure changes in vegetation along the coastline and assess where and how oil may be affecting marshes, swamps, bayous, and beaches that are difficult to survey on the ground. The combination of satellite and airborne imagery will assist NOAA in forecasting the trajectory of the oil and in documenting changes in the ecosystem.

From the outset of the spill on April 20, NASA has provided satellite images to federal agencies from the Moderate Resolution Imaging Spectroradiometer (MODIS) instruments on NASA's Terra and Aqua satellites; the Japanese Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) on Terra; and the Advanced Land Imager (ALI) and Hyperion instruments on NASA's Earth Observing-1 (EO-1) satellite. All of these observations have been funneled to the Hazards Data Distribution System operated by the USGS.

With its very wide field of view, MODIS provides a big-picture of the oil spill and its evolution roughly twice per day. The Hyperion, ALI, and ASTER instruments observe over much smaller areas in finer detail but less often (every 2-5 days).

Other NASA satellite and airborne instruments are collecting observations of the spill to advance basic research and to explore future remote-sensing capabilities. From space, the Multi-angle Imaging Spectroradiometer (MISR) on Terra and the Atmospheric Infrared Sounder (AIRS) on Aqua as well as the Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) on the joint NASA-France CALIPSO satellite are collecting data.

Another NASA research aircraft, the King Air B-200 from Langley Research Center in Hampton, Va., was previously scheduled to fly to California this week but changed its flight plan to collect data over the area of the oil spill. It completed its first flight over the spill on May 10.

The High Spectral Resolution Lidar (HSRL) onboard the plane uses pulses of laser light to locate and identify particles in the environment. Led by Chris Hostetler of Langley, HSRL provides measurements similar to those from the CALIOP instrument on CALIPSO. Data from these space-based and airborne lidars will be used to investigate the thickness of the oil spill below the surface of the water and evaluate the impacts of dispersants used to break up the oil.

"Although NASA's primary expertise is in using remote-sensing instruments to conduct basic research on the entire Earth system, our observations can be used for societal benefit in response to natural and technological disasters like this oil spill," said Goodman.

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NASA Joins in National Lab Day Events to Promote ‘Educate to Innovate’ Campaign

Rockets Aloft

Fifth grade students hold their model rockets aloft as they pose for a photo with Aerospace Education Specialist Elicia Fullwood, left, at the Langdon Education Campus, Tuesday, May 11, 2010 in Washington. NASA staff, including Administrator Bolden, visited Langdon in support of National Lab Day to bring hands-on learning to students across the country.

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X-ray Discovery Points to Location of Missing Matter

Artist concept of the so-called Sculptor WallUsing observations with NASA's Chandra X-ray Observatory and ESA's XMM-Newton, astronomers have announced a robust detection of a vast reservoir of intergalactic gas about 400 million light years from Earth. This discovery is the strongest evidence yet that the "missing matter" in the nearby Universe is located in an enormous web of hot, diffuse gas.

This missing matter -- which is different from dark matter -- is composed of baryons, the particles, such as protons and electrons, that are found on the Earth, in stars, gas, galaxies, and so on. A variety of measurements of distant gas clouds and galaxies have provided a good estimate of the amount of this "normal matter" present when the universe was only a few billion years old. However, an inventory of the much older, nearby universe has turned up only about half as much normal matter, an embarrassingly large shortfall.

The mystery then is where does this missing matter reside in the nearby universe? This latest work supports predictions that it is mostly found in a web of hot, diffuse gas known as the Warm-Hot Intergalactic Medium (WHIM). Scientists think the WHIM is material left over after the formation of galaxies, which was later enriched by elements blown out of galaxies.

"Evidence for the WHIM is really difficult to find because this stuff is so diffuse and easy to see right through," said Taotao Fang of the University of California at Irvine and lead author of the latest study. "This differs from many areas of astronomy where we struggle to see through obscuring material."

To look for the WHIM, the researchers examined X-ray observations of a rapidly growing supermassive black hole known as an active galactic nucleus, or AGN. This AGN, which is about two billion light years away, generates immense amounts of X-ray light as it pulls matter inwards.

Lying along the line of sight to this AGN, at a distance of about 400 million light years, is the so-called Sculptor Wall. This "wall", which is a large diffuse structure stretching across tens of millions of light years, contains thousands of galaxies and potentially a significant reservoir of the WHIM if the theoretical simulations are correct. The WHIM in the wall should absorb some of the X-rays from the AGN as they make their journey across intergalactic space to Earth.

Using new data from Chandra and previous observations with both Chandra and XMM-Newton, absorption of X-rays by oxygen atoms in the WHIM has clearly been detected by Fang and his colleagues. The characteristics of the absorption are consistent with the distance of the Sculptor Wall as well as the predicted temperature and density of the WHIM.

This result gives scientists confidence that the WHIM will also be found in other large-scale structures.

Several previous claimed detections of the hot component of the WHIM have been controversial because the detections had been made with only one X-ray telescope and the statistical significance of many of the results had been questioned.

"Having good detections of the WHIM with two different telescopes is really a big deal," said co-author David Buote, also from the University of California at Irvine. "This gives us a lot of confidence that we have truly found this missing matter."

In addition to having corroborating data from both Chandra and XMM- Newton, the new study also removes another uncertainty from previous claims. Because the distance of the Sculptor Wall is already known, the statistical significance of the absorption detection is greatly enhanced over previous "blind" searches. These earlier searches attempted to find the WHIM by observing bright AGN at random directions on the sky, in the hope that their line of sight intersects a previously undiscovered large-scale structure.

Confirmed detections of the WHIM have been made difficult because of its extremely low density. Using observations and simulations, scientists calculate the WHIM has a density equivalent to only 6 protons per cubic meter. For comparison, the interstellar medium -- the very diffuse gas in between stars in our galaxy -- typically has about a million hydrogen atoms per cubic meter.

"Evidence for the WHIM has even been much harder to find than evidence for dark matter, which is invisible and can only be detected indirectly," said Fang.

There have been important detections of possible WHIM in the nearby Universe with relatively low temperatures of about 100,000 degrees using ultraviolet observations and relatively high temperature WHIM of about 10 million degrees using observations of X-ray emission in galaxy clusters. However, these are expected to account for only a relatively small fraction of the WHIM. The X-ray absorption studies reported here probe temperatures of about a million degrees where most of the WHIM is predicted to be found.

These results appear in the May 10th issue of The Astrophysical Journal. NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory controls Chandra's science and flight operations from Cambridge, Mass.

More information, including images and other multimedia, can be found at:

http://chandra.harvard.edu

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Rock and Roll: Titan’s Gem Tumbler

The left-hand image, obtained by the European Space Agency's  Huygens probe, shows rounded rocks from the surface of Saturn's moon  Titan.
The left-hand image, obtained by the European Space Agency's Huygens probe, shows rounded rocks from the surface of Saturn's moon Titan. Huygens rode with NASA's Cassini spacecraft to the Saturn system. The right-hand image, taken by amateur photographer Sandra M. Matheson, shows river rocks on Earth. › Larger image

It appears flash flooding has paved streambeds in the Xanadu region of Saturn's moon Titan with thousands of sparkling crystal balls of ice, according to scientists with NASA's Cassini spacecraft. By analyzing the way the terrain has scattered radar beams, scientists deduce the spheres measure at least a few centimeters (inches) and maybe up to a couple of meters (yards) in diameter. The spheres likely originated as part of water-ice bedrock in higher terrain in Xanadu.

"What we believe happened in this area is a lot like what creates polished river rocks on Earth," said Alice Le Gall, a postdoctoral fellow at NASA's Jet Propulsion Laboratory, Pasadena, Calif., and the lead author of the study, which used the Cassini radar instrument. "Bouncing downstream smoothes out the edges of rocks."

As foothill residents know in southern California and other areas, sudden rains can trigger mudslides and flooding at the mountainous fringes of desert areas. Those flows can pick up boulders and debris and tumble them downstream. On Titan, the flows appear to have occurred periodically for eons, on a catastrophic scale. The process on Titan, however, involves rain made of liquid methane and ethane, rather than Earth's water rain. Titan's rocks are believed to be made primarily of water ice frozen into a hard mass about minus 180 degrees Celsius (minus 290 degrees Fahrenheit), rather than Earth's mineral rocks.

Earth-like river rocks have already been observed on Titan at the landing site of the European Space Agency's Huygens probe, near the equator in the borderland between the Adiri and Shangri-la regions. The landing site also showed signs of flash flooding that deposited cobblestones about 2 to 20 centimeters (1 to 8 inches) in diameter.

But the spidery channels in this southern lowland part of Xanadu looked brighter to Cassini's radar instrument than the Huygens landing area. In fact, the channels, which were scanned by Cassini in May 2008, are among the brightest features ever seen on Titan by the radar instrument.

In a paper now available online in the journal Icarus, Le Gall and colleagues concluded that the most plausible explanation for the extreme brightness of the Xanadu channels was a collection of transparent spherical sediments, packed more tightly together than the cobblestones at the Huygens landing site. The effect would be similar to bejeweling an area with light-catching rhinestones.

The spheres appear to be made of water ice – possibly doped with ammonia – that would look bright to the microwaves used by Cassini's radar. Spheres are good at sending light back in the direction it came from. This property has actually led manufacturers to use plastic spheres in reflective paints and tape, Le Gall said.

Xanadu may be an especially good gem grinder because of its broad expanse and gentle southward slope. Flows could have traveled long distances there and tumbled the chunks for hundreds of kilometers (miles). The subtle work to shape them into spheres could have come from fine grit rubbing against the rocks in the flowing methane. Or, ice may be malleable in Titan's cold temperatures, deforming plastically during the collisions rather than fracturing. The flows that transported these icy spheres probably traveled around 1 meter per second (2 mph).

"It's been really hard for a long time for people to understand why Xanadu is so bright," said Steve Wall, a radar team member at JPL. "You might not expect these kinds of geometries in a natural setting, but we believe this can explain the enigma."

The radar team plans to continue looking for other instances of small, smooth spheres in nature to increase their confidence about the explanation. They also said more study is needed on the mechanical properties of water ice at such cold temperatures.

"Here is yet another example of Titan as a world with Earth-like processes," said Linda Spilker, Cassini project scientist at JPL. "As the seasons change on Titan, maybe we'll get a chance to see methane flow through some of the river channels."

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL. The radar instrument was built by JPL and the Italian Space Agency, working with team members from the United States and several European countries.

For more information about the Cassini-Huygens mission visit

http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov.

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Herschel Finds a Hole in Space

The dark hole seen in the green cloud at the top of this image was likely carved out by multiple jets and blasts of radiation. Image credit: ESA/NASA/JPL-Caltech/Univ. of Toledo

The Herschel Space Observatory has made an unexpected discovery: a gaping hole in the clouds surrounding a batch of young stars. The hole has provided astronomers with a surprising glimpse into the end of the star-forming process.

Stars are born hidden in dense clouds of dust and gas, which can now be studied in remarkable detail with Herschel, a European Space Agency mission with important NASA participation. Although jets and winds of gas have been seen streaming from young stars in the past, it has always been a mystery exactly how a star uses the jets to blow away its surroundings and emerge from its birth cloud. For the first time, Herschel may be seeing an unexpected step in this process.

A cloud of bright reflective gas known to astronomers as NGC 1999 sits next to a black patch of sky. For most of the 20th century, such black patches were known to be dense clouds of dust and gas that block light from passing through.

When Herschel looked in its direction to study nearby young stars, astronomers were surprised to see the cloud continued to look black, which shouldn't have been the case. Herschel's infrared eyes are designed to see into such clouds. Either the cloud was immensely dense or something was wrong.

Investigating further using ground-based telescopes, astronomers found the same story no matter how they looked: this patch looks black not because it is a dense pocket of gas but because it is truly empty. Something has blown a hole right through the cloud.

"No one has ever seen a hole like this," says Tom Megeath of the University of Toledo, Ohio, the principal investigator of the research. "It's as surprising as knowing you have worms tunneling under your lawn, but finding one morning that they have created a huge, yawning pit."

The astronomers think that the hole must have been opened when the narrow jets of gas from some of the young stars in the region punctured the sheet of dust and gas that forms NGC 1999. The powerful radiation from a nearby adolescent star may also have helped to clear the hole. Whatever the precise chain of events, it could be an important glimpse into the way newborn stars rip apart their birth clouds.

Other members of the research team include Thomas Stanke of the European Southern Observatory, Germany; Amy Stutz of the Max-Planck Institute for Astronomy, Germany, and the Steward Observatory, Tucson; John Tobin of the University of Michigan, Ann Arbor; Lori Allen of the National Optical Astronomy Observatory, Tucson; Ali Babar of the NASA Herschel Science Center at the California Institute of Technology, Pasadena; and Will Fischer and Erin Kryukova, University of Toledo, Ohio.

Herschel is a European Space Agency cornerstone mission, with science instruments provided by consortia of European institutes and with important participation by NASA. NASA's Herschel Project Office is based at NASA's Jet Propulsion Laboratory, Pasadena, Calif. JPL contributed mission-enabling technology for two of Herschel's three science instruments. The NASA Herschel Science Center, part of the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena, supports the United States astronomical community. Caltech manages JPL for NASA.

More information is online at http://www.herschel.caltech.edu , http://www.nasa.gov/herschelhttp://www.esa.int/SPECIALS/Herschel/index.html.

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