Environment-Clean-Generations

Environment-Clean-Generations
THE DEFINITIVE BLOG FOR EVERYTHING YOU NEED TO KNOW ABOUT THE ENVIRONMENT YOU LIVE IN, WITH REFERENCE TO LIFE, EARTH AND COSMIC SPACE SCIENCES, PRESENTED BY ENVIRONMENTAL ENGINEER DORU INDREI, ENVIRONMENTAL QUALITY AND ENERGY SPACIALIST
"Life is not about what we know, but what we don't know, craving the unthinkable makes it so amazing, that is worth dying for." Doru Indrei
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Clouds Closer to Earth


Chicken Licken was right, the sky really is falling. Nasa satellite data has shown that the Earth's cloud tops have been lowering over the last decade.


 Cloud-top height fell one percent on average between March 2000 and February 2010, according to measurements from the multi-angle imaging spectroradiometer mounted on Nasa's Terra satellite. That one percent means a reduction of 30 to 40 metres in the average maximum height of clouds, during the 00s.

While the short record means it's difficult to draw any strong conclusions from the data, it does hint towards a longer-term trend. Roger Davies, the lead researcher on the project, warns that it's something that should be monitored in the coming decades to determine how significant it is for global temperatures.




If there is indeed a consistent reduction in cloud height, and this isn't just natural variability, then Earth would begin cooling to space more efficiently, reducing the surface temperatures and slowing the effects of climate change. 

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"We don't know exactly what causes the cloud heights to lower," says Davies. "But it must be due to a change in the circulation patterns that give rise to cloud formation at high altitude." The Terra spacecraft, which launched in 1999 and records three-dimensional images of clouds around the globe, will continue gathering data in the coming years.

Hubble Telescope Spots Exoplanet Made of Water


GJ 1214b, a planet some 40 light-years from Earth, is a water world. It's almost entirely made of liquid, has an estimated temperature of 230C and is enshrouded by a steamy atmosphere.

"The high temperatures and high pressures would form exotic materials like hot ice or superfluid water: substances that are completely alien to our everyday experience," explains Zachory Berta of the Harvard-Smithsonian Center for Astrophysics.




It's classified as a super-Earth, as the planet is about 2.7 times Earth's diameter and weighs almost seven times as much. It orbits its star every 38 hours at a distance of just two million kilometres, resulting in those super-hot temperatures.



The planet was first discovered in 2009, by the ground-based MEarth Project. The next year, astronomers from the Harvard-Smithsonian Center for Astrophysics (CfA) measured the exoplanet's atmosphere, and found that it could be composed mainly of water.

But those observations could also be explained if the planet just had a thick, hazy atmosphere. So, the team waited for GJ 1214b to cross in front of its host star (a red dwarf). When that happens, the star's light is filtered through the planet's atmosphere, giving hints to the mix of gases it contains.

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"We're using Hubble to measure the infrared colour of sunset on this world," explained the CfA team leader.
The team used Hubble's Wide Field Camera 3 (WFC3) to watch the planet's transit, and found the spectrum of GJ 1214b to be featureless over a wide range of wavelengths. That's consistent with a dense atmosphere of water vapour, suggesting the planet is covered by steam -- not haze.

Because the team knows the planet's mass and size, they can calculate the density. It comes out at about about two grams per cubic centimetre -- seeing as water has a density of one gram per cubic centimetre, and the Earth's average density is 5.5 grams per cubic centimetre, GJ 1214b has much more water and much less rock than our so-called "Blue Marble".

The liquid planet has been flagged as a "prime candidate" for study by Hubble's successor: the James Webb Space Telescope, when it launches around 2018.

Solid Buckyballs in Space Found by Spitzer Telescope


After finding gaseous clouds of buckyballs in space last year, astronomers have now discovered the carbon balls in a solid form, around a pair of stars some 6,500 light-years from Earth.

Buckyballs are microscopic spheres, where 60 carbon atoms are arranged -- with alternating patterns of hexagons and pentagons -- into a football-like pattern. The unusual structure makes them incredibly strong, and ideal candidates for things like superconducting materials, medicines, water purification and armour.




They got their name because of their resemblance to the geodesic domes of the architect Buckminster Fuller.


So far, they've only been found in gas form in space. In 2010, astronomers using the Spitzer space telescope found the balls in a planetary nebula called Tc 1.
But with this latest discovery, again using data from Nasa's Spitzer space telescope, astronomers found particles consisting of stacked buckyballs. They had stacked together like oranges in a crate to form a solid shape.

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"The particles we detected are minuscule, far smaller than the width of a hair, but each one would contain stacks of millions of buckyballs," said the paper's lead author Nye Evans of Keele University in England.
The research team was able to identify the solid form of buckyballs in the Spitzer data because they emit light in a unique way that differs from the gaseous form. In all, the team detected enough solid buckyballs to fill the equivalent in volume to 10,000 Mount Everests.

"This exciting result suggests that buckyballs are even more widespread in space than the earlier Spitzer results showed," said Mike Werner, project scientist for Spitzer at Nasa's Jet Propulsion Laboratory. "They may be an important form of carbon, an essential building block for life, throughout the cosmos."

New Blood Types Discovered



You probably know your blood type: A, B, AB or O. You may even know if you're Rhesus positive or negative. But how about the Langereis blood type? Or the Junior blood type? Positive or negative? Most people have never even heard of these.
Yet this knowledge could be "a matter of life and death," says University of Vermont biologist Bryan Ballif.
While blood transfusion problems due to Langereis and Junior blood types are rare worldwide, several ethnic populations are at risk, Ballif notes. "More than 50,000 Japanese are thought to be Junior negative and may encounter blood transfusion problems or mother-fetus incompatibility," he writes.


 But the molecular basis of these two blood types has remained a mystery — until now.
In the February issue of Nature Genetics, Ballif and his colleagues report on their discovery of two proteins on red blood cells responsible for these lesser-known blood types.
Ballif identified the two molecules as specialized transport proteins named ABCB6 and ABCG2.
"Only 30 proteins have previously been identified as responsible for a basic blood type," Ballif notes, "but the count now reaches 32."

The last new blood group proteins to be discovered were nearly a decade ago, Ballif says, "so it's pretty remarkable to have two identified this year."

Both of the newly identified proteins are also associated with anticancer drug resistance, so the findings may also have implications for improved treatment of breast and other cancers.
As part of the international effort, Ballif, assistant professor in UVM's biology department, used a mass spectrometer funded by the Vermont Genetics Network. With this machine, he analyzed proteins purified by his longtime collaborator, Lionel Arnaud at the French National Institute for Blood Transfusion in Paris, France.

Ballif and Arnaud, in turn, relied on antibodies to Langereis and Junior blood antigens developed by Yoshihiko Tani at the Japanese Red Cross Osaka Blood Center and Toru Miyasaki at the Japanese Red Cross Hokkaido Blood Center.

After the protein identification in Vermont, the work returned to France. There Arnaud and his team conducted cellular and genetic tests confirming that these proteins were responsible for the Langereis and Junior blood types. "He was able to test the gene sequence," Ballif says, "and, sure enough, we found mutations in this particular gene for all the people in our sample who have these problems."

Beyond the ABO blood type and the Rhesus (Rh) blood type, the International Blood Transfusion Society recognizes twenty-eight additional blood types with names like Duffy, Kidd, Diego and Lutheran. But Langereis and Junior have not been on this list. Although the antigens for the Junior and Langereis (or Lan) blood types were identified decades ago in pregnant women having difficulties carrying babies with incompatible blood types, the genetic basis of these antigens has been unknown until now.

Therefore, "very few people learn if they are Langereis or Junior positive or negative," Ballif says.
"Transfusion support of individuals with an anti-Lan antibody is highly challenging," the research team wrote in Nature Genetics, "partly because of the scarcity of compatible blood donors but mainly because of the lack of reliable reagents for blood screening." And Junior-negative blood donors are extremely rare too. That may soon change.

With the findings from this new research, health care professionals will now be able to more rapidly and confidently screen for these novel blood group proteins, Ballif wrote in a recent news article. "This will leave them better prepared to have blood ready when blood transfusions or other tissue donations are required," he notes.




"Now that we know these proteins, it will become a routine test," he says.

This science may be especially important to organ transplant patients. "As we get better and better at transplants, we do everything we can to make a good match," Ballif says. But sometimes a tissue or organ transplant, that looked like a good match, doesn't work — and the donated tissue is rejected, which can lead to many problems or death.

"We don't always know why there is rejection," Ballif says, "but it may have to do with these proteins."

The rejection of donated tissue or blood is caused by the way the immune system distinguishes self from not-self. "If our own blood cells don't have these proteins, they're not familiar to our immune system," Ballif says, so the new blood doesn't "look like self" to the complex cellular defenses of the immune system. "They'll develop antibodies against it," Ballif says, and try to kill off the perceived invaders. In short, the body starts to attack itself.

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"Then you may be out of luck," says Ballif, who notes that in addition to certain Japanese populations, European Gypsies are also at higher risk for not carrying the Langereis and Junior blood type proteins.
"There are people in the United States who have these challenges too," he says, "but it's more rare."
Ballif and his international colleagues are not done with their search. "We're following up on more unknown blood types," he says. "There are probably on the order of 10 to 15 more of these unknown blood type systems — where we know there is a problem but we don't know what the protein is that is causing the problem."
Although these other blood systems are very rare, "if you're that one individual, and you need a transfusion," Ballif says, "there's nothing more important for you to know."

No Men Extinction, We Will Always Be Here!



Over the last few decades, scientists and journalists have speculated that the end of man—men, that is—was nigh. The biological reason for this possibility is the ever-shrinking Y chromosome: 300-200 million years ago, the Y, like females’ X chromosome, had hundreds of genes, but it now contains less than 80, 19 of which code for specifically male traits such as sperm production. 


 This remarkable contraction set people’s imaginations spinning, especially after an opinion piece said in Nature 10 years ago that the Y chromosome might disappear, as it already has in voles, in 10 million years.




A Nature paper published this week, however, may indicate that the Y is sticking around. Biologists at the Whitehead Institute have compared the Y chromosome of rhesus monkeys with the human Y chromosome, and they’ve found that the two have the same number but one of key male-specific genes. This implies that the human Y chromosome’s shrinkage, at least when it comes to key genes, stopped at least around 25 million years ago, when the common ancestor of humans and rhesus monkeys was alive. 

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The team says that this 25 million years of stasis indicates that the Y’s days of sloughing genes are over, that the genes it carries now are the essential ones and cannot be removed without seriously impacting reproductive function, while the genes lost in the past were expendable.

It’s hard to say that evolution of the Y chromosome has categorically ceased, though—evolution doesn’t necessarily follow a straight line. And it’s worth remembering that we had males before we had the Y chromosome: the male genes, at that time, were just spread across the genome. Even if more shrinking events eventually do send the Y the way of the leisure suit, it doesn’t mean that males will follow suit.

Huge Avalanche near Mars's North Pole



A Nasa spacecraft has captured an avalanche of fine ice and dust thundering over a cliff near Mars's north pole. 

It's not the first avalanche captured by the HiRISE camera aboard the Mars Reconnaissance Orbiter - Nasa first detected the phenomenon in 2008, believed to be caused by a thin 'crust' of frozen carbon dioxide (dry ice) which forms during the Martian winter. 

 Ice and dust cascade over a Martian cliff: The camera on the Mars Reconnaissance Orbiter captured the avalanche near Mars's north pole

The HiRISE high resolution camera took the amazing photograph at 85 degrees north on the planet.
The HiRISE camera is one of several hi-tech instruments on board Mars Reconnaissance Orbiter. It's the largest camera ever carried into deep space.
Nasa's ground team says that the events are detectable by a cloud of fine material that erupts when avalanches collapse down slopes on the planet.




Some avalanches on Mars are caused by meteorite impacts, but others are thought to be the result of 'seasons' on the planet, which has winters, just like Earth.
Planetary scientist Ingrid Daubar Spitale of the University of Arizona, who first noticed the avalanches in photos taken by the Mars Reconnaissance Orbiter said, 'It's great to see something so dynamic on Mars. A lot of what we see there hasn't changed for millions of years.'


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Fine ice and dust cascades over a martian polar cliff in March 2010 in another picture captured by the Mars Reconnaissance Orbiter's HiRISE camera.

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