Thursday, 8 October 2015

Ebola hits Nigeria again, 10 quarantined in Calabar

University of Calabar Teaching Hospital, UCTH, has quarantined ten persons following the death of a patient in the hospital on Wednesday with symptoms suspected to be Ebola virus.
ebolaaDr. Queeneth Kalu, Chairman of  Medical Advisory Committee of the hospital who made the revelation on Thursday in Calabar while addressing pressmen  said blood samples have been sent to the Ebola Diagnosing Centre in Benin Edo State.
“On Wednesday, 7th October, 2015, we managed a patient who presented with symptoms mimicking viral hemorrhage (Ebola Virus) and have decided to take the necessary measures”.
Dr. Kalu stated that those quarantined are principally nurses who attended to the patient and those who  came in contact with him before his death.
‘”The following have been informed: National Centre for Disease Control, Federal Ministry of Health,  The Cross River State Government, Calabar Municipality, and the Department of State Security Services, DSS”
She said further information will be provided to the public as soon as the test results of blood samples sent for analysis in received by the hospital.

Friday, 18 September 2015

11 Facts About the September 27/ 28, 2015 Blood Moon (Lunar Eclipse)


On September 28, 2015, a rare Total Lunar Eclipse of a Super Full Moon will be visible from most of North America, South America, Europe, West Asia and parts of Africa. Here are 11 facts you should know about this eclipse.
Different stages of Total Lunar Eclipse over Indianapolis, United States in February 2008.
Different stages of a Total Lunar Eclipse.
©bigstockphoto.com/alexeys

1. A Rare Eclipse of a Supermoon

The full Moon of September 27/28 is aSupermoon – the Moon will be closest to the Earth. or at its perigee, as it turns into a full Moon. A rising Super Full Moon can look larger and brighter to spectators on Earth.
Total eclipses of Super Full Moons are rare. According to NASA, they have only occurred 5 times in the 1900s – in 1910,192819461964 and 1982. After the September 27/ 28, 2015 Total Lunar Eclipse, a Supermoon eclipse will not happen again for another 18 years, untilOctober 8, 2033.

2. People in the US Will Get Front Row Seats

People in eastern and central areas of the United States and Canada will have some of the best views of the Total Lunar Eclipse on the night of September 27, 2015, weather permitting. Here, the eclipse will begin after moonrise and finish around midnight (00:00 on September 28).
Those on the West Coast will miss the beginning stages of the eclipse because they will happen before moonrise.
It will be the last Total Lunar Eclipse visible from mainland USA until January 31, 2018.

3. Late Night & Early Morning Eclipse

While North and South Americans will be able to see the eclipse after sunset on September 27, 2015, people in Africa, Europe and Middle East can view it during the early hours of September 28, before the Sun rises.

4. No Need for Eye Protection

Lunar eclipses can be spectacular and they are easy to see with the naked eye. Unlike solar eclipses, which require protective eye wear, a lunar eclipse can be viewed without specialized eye wear.
Illustration image
A partial solar eclipse looks like the Moon has taken a bite of the Sun.
©bigstockphoto.com/underworld1

5. A Solar Eclipse Takes Place Two Weeks Before

Solar and lunar eclipses come in pairs – a lunar eclipse always takes place two weeks before or after a solar eclipse. The September 27/ 28, 2015 Total Lunar Eclipse will be preceded by a Partial Solar Eclipse onSeptember 13, 2015.

6. It's Part of a Lunar Tetrad

The September 28, 2015 Total Lunar Eclipse is the fourth and final eclipse in a series of four total lunar eclipses called the lunar tetrad. The first three eclipses of the tetrad took place on April 15, 2014October 8, 2014 and onApril 4, 2015.
Notice something interesting about the dates? Each of the eclipses in the tetrad occurs about 6 months apart and have 5 full Moons between them!
Lunar tetrads can be rare in some centuries and can occur frequently in others. The 21st century will have 8 lunar tetrads, the maximum number of lunar tetrads that can occur in a century. The last time this happened was in the 9th century!
The next lunar tetrad of the 21st century will start with the April 25, 2032 Total Lunar Eclipse.

7. ...And is Being Called a Blood Moon

An eclipsed Moon can take on a reddish glow during totality
Rayleigh scattering can cause the Moon to look red during a lunar eclipse.
©bigstockphoto.com/Medardus
In recent years, the term Blood Moon has been frequently used to refer to total lunar eclipses. Some sources suggest that the term stems from the Bible. Christian pastors Mark Blitz and John Hagee claim that the eclipses of the 2014-2015 lunar tetrad fulfill a Biblical prophecy of forthcoming difficult and trying times.
Astronomers do not use Blood Moon as a scientific term. However, it is possible that the term came to describe total lunar eclipses because of the reddish color the eclipsed Moon takes on during totality. This happens because of Rayleigh scattering, the same mechanism that causes colorful sunrises and sunsets.

8. Despite Rumors, the World Will Not End

Illustration image
Relax! The World will not end.
©iStockphoto.com/DNY59
The views of pastors Blitz and Hagee gathered attention in early 2014, because the eclipses in the tetrad coincide with important Jewish festivals. The eclipses in April 2014and April 2015 occured at the same time asPassover, while the October 2014 andSeptember 2015 eclipses occur during theFeast of Tabernacles. Some people took this coincidence as a sign of the end of times.
Others have dismissed any apocalyptic significance of the tetrad. Data of past eclipses show that at least eight lunar tetrads have coincided with Jewish holidays since the First Century.
The Jewish Calendar is a lunar calendar and Passover always occurs around a full Moon. Since a total lunar eclipse can only occur on a full Moon night, it is very likely that an eclipse will take place on or near Passover.
In conclusion, scientists and astronomers have found no reason to believe that the current lunar tetrad is a sign of the world to end. Even mainstream religious organizations have debunked this claim, so don't start hoarding end-of-the-world supplies just yet!

9. It will Happen on Harvest Moon

Harvest Moon is the Northern Hemisphere's first fall (autumn) full Moon.
The Harvest Moon is the first full Moon of the Northern Hemisphere fall (autumn).
©iStockphoto.com/klagyivik
The Lunar Eclipse on September 27/ 28, 2015 will occur during the Northern Hemisphere's first fall (autumn) full Moon. Called the Harvest Moon in many northern cultures, it is the full Moon closest to theSeptember Equinox, and is astronomically significant.
On average the Moon rises about 50 minutes later every successive day in a lunar month – the time period between two full Moons or two new Moons. In New York, for example, a new Moon will rise at 6:50 am on September 13. On September 14, the Moon will rise almost 60 minutes later at 7:46 am.
Around the Northern Hemisphere's Harvest Moon, this time difference between two successive moonrises decreases to about 30-40 minutes for a few days. In New York, a full Moon will rise at 6:36 pm (18:36) on September 27 and on September 28, the Moon will rise 40 minutes later at 7:16 pm (19:16).
This curious phenomenon, which is also sometimes called the Harvest Moon Effect occurs because of the low angle that the Moon's path around the Earth makes with the horizon during the northern fall (autumn) months. This effect reverses during the Northern Hemisphere spring. The large angle that the lunar orbit makes with the horizon ensures that the moon rises more than 50 minutes later every day around the northern Spring Equinox.
Because seasons in the Southern Hemisphere are opposite to the seasons in the North, the Harvest Moon Effect occurs around the southern Fall (Autumn) Equinox in March.
Wat arun in night with super full moon
A Super Full Moon is also known as a Perigee Moon.
©bigstockphoto.com/Prasit Rodphan

10. It is Part of Lunar Saros Series 137

Like solar eclipses, lunar eclipses tend to occur in 18 year long cycles called Saros cycles. Lunar eclipses separated by a Saros cycle share similar features, including time of the year and the distance of the Moon from the Earth. Eclipses that are separated by a Saros cycle are included in a Saros series.
The September 27/ 28, 2015 Lunar Eclipse belongs to Saros Series 137. It is the 28th eclipse and the last total lunar eclipse in a series of 81 lunar eclipses. The series began with a penumbral eclipse on December 17, 1564 and will end with another penumbral eclipse on April 20, 2953.

11. It's the Last Eclipse of 2015

2015 has 4 eclipses, the minimum number of eclipses that can happen in a calendar year. The September 28 Total Lunar Eclipse marks the last eclipse of the year. It will be preceded by a partial solar eclipse on September 13, 2015.
The first eclipse of the year, a total solar eclipse took place on March 20. Two weeks later, on April 4, 2015 the first lunar eclipse of 2015 took place.

Monday, 7 September 2015

Deformed craton under North America

In the course of billions of years continents break up, drift apart, and are pushed back together again. The cores of continents are, however, geologically extremely stable and have survived up to 3.8 billions of years. These cores that are called cratons are the oldest known geological features of our planet. It was assumed that the cratons are stable because of their especially solid structure due to relatively low temperatures compared to the surrounding mantle. A team of German-American scientists now discovered that these cratons that were assumed to be "as solid as a rock" are not that solid after all. The team leading by Dr. Mikhail Kaban from the GFZ German Research Centre for Geosciences now discovered that the craton below the North American continent is extremely deformed: its root is shifted relative to the center of the craton by 850 kilometers towards the west-southwest.
This fact is in contrast to the prevailing assumptions that these continental roots did not undergo substantial changes after their formation 2.5 to 3.8 billion years ago. The study that appears in the latest online publication of "Nature Geoscience" contradicts this traditional view. "We combined and analyzed several data sets from Earth's gravity field, topography, seismology, and crustal structure and constructed a three dimensional density model of the composition of the lithosphere below North America," explains GFZ scientist Mikhail Kaban. "It became apparent that the lower part of the cratonic root was shifted by about 850 kilometers."
What caused the deformation of the stable and solid craton? A model of the flows in Earth's mantle below North America, developed by the scientists, reveals that the mantle material below 200 kilometers flows westward at a velocity of about 4 millimeters per year. This is in concordance with the movement of the tectonic plate. Due to the basal drag of this flow the lower part of the cratonic lithosphere is shifted. "This indicates that the craton is not as solid and as insensitive to the mantle flow as was previously assumed," Kaban completes. There is far more mechanical, chemical, and thermal interaction between the craton of billions of years in age and its surrounding in the upper mantle of Earth than previously thought.

Oldest Fossil Sea Turtle Discovered

Scientists at the Senckenberg Research Institute in Frankfurt have described the world’s oldest fossil sea turtle known to date. The fossilized reptile is at least 120 million years old – which makes it about 25 million years older than the previously known oldest specimen. The almost completely preserved skeleton from the Cretaceous, with a length of nearly 2 meters, shows all of the characteristic traits of modern marine turtles. The study was published today in the scientific journal “PaleoBios.”
Santanachelys gaffneyi is the oldest known sea turtle” – this sentence from the online encyclopedia Wikipedia is no longer up to date.  “We described a fossil sea turtle from Colombia that is about 25 million years older,” rejoices Dr. Edwin Cadena, a scholar of the Alexander von Humboldt foundation at the Senckenberg Research Institute. Cadena made the unusual discovery together with his colleague from the US, J. Parham of California State University, Fullerton.
“The turtle described by us as Desmatochelys padillai sp. originates from Cretaceous sediments and is at least 120 million years old,” says Cadena. Sea turtles descended from terrestrial and freshwater turtles that arose approximately 230 million years ago. During the Cretaceous period, they split into land and sea dwellers. Fossil evidence from this time period is very sparse, however, and the exact time of the split is difficult to verify. “This lends a special importance to every fossil discovery that can contribute to clarifying the phylogeny of the sea turtles,” explains the turtle expert from Columbia.
The fossilized turtle shells and bones come from two sites near the community of Villa de Leyva in Colombia. The fossilized remains of the ancient reptiles were discovered and collected by hobby paleontologist Mary Luz Parra and her brothers Juan and Freddy Parra in the year 2007. Since then, they have been stored in the collections of the “Centro de Investigaciones Paleontológicas” in Villa Leyva and the “University of California Museum of Paleontology.”
Cadena and his colleague examined the almost complete skeleton, four additional skulls and two partially preserved shells, and they placed the fossils in the turtle group Chelonioidea, based on various morphological characteristics. Turtles in this group dwell in tropical and subtropical oceans; among their representatives are the modern Hawksbill Turtle and the Green Sea Turtle of turtle soup fame.
“Based on the animals‘ morphology and the sediments they were found in, we are certain that we are indeed dealing with the oldest known fossil sea turtle,” adds Cadena in summary.

Attached files

  • Dr. Edwin Cadena holds the skull of the ancient sea turtle © Edwin Cadena

  • The skeleton of the fossilized sea turtle measures almost 2 meters. © PaleoBios/Cadena

  • The skeleton of Desmatochelys padillai sp. is almost completely preserved. © PaleoBios/Cadena

  • This is what the habitat of the sea turtle might have looked like 120 million years ago. © Jorge Blanco

Sunday, 12 April 2015

New evidence for combat and cannibalism in tyrannosaurs

A new study documents injuries inflicted in life and death to a large tyrannosaurine dinosaur. The paper shows that the skull of a genus of tyrannosaur called Daspletosaurus suffered numerous injuries during life, at least some of which were likely inflicted by another Daspletosaurus. It was also bitten after death in an apparent event of scavenging by another tyrannosaur. Thus there's evidence of combat between two large carnivores as well as one feeding on another after death.
Daspletosaurus was a large carnivore that lived in Canada and was only a little smaller than its more famous cousin Tyrannosaurus. Like other tyrannosaurs it was most likely both an active predator and scavenger. The individual in question, from Alberta Canada, was not fully grown and would be considered a 'sub-adult' in dinosaur terms (approximately equivalent to an older teenager in human terms). It would have been just under 6 m long and around 500 kg when it died.
Researchers found numerous injuries on the skull that occurred during life. Although not all of them can be attributed to bites, several are close in shape to the teeth of tyrannosaurs. In particular one bite to the back of the head had broken off part of the skull and left a circular tooth-shaped puncture though the bone. The fact that alterations to the bone's surface indicate healing means that these injuries were not fatal and the animal lived for some time after they were inflicted.
Lead author Dr David Hone from Queen Mary, University of London said "This animal clearly had a tough life suffering numerous injuries across the head including some that must have been quite nasty. The most likely candidate to have done this is another member of the same species, suggesting some serious fights between these animals during their lives."
There is no evidence that the animal died at the hands (or mouth) of another tyrannosaur. However, the preservation of the skull and other bones, and damage to the jaw bones show that after the specimen began to decay, a large tyrannosaur (possibly of the same species) bit into the animal and presumably ate at least part of it.
Combat between large carnivorous dinosaurs is already known and there is already evidence for cannibalism in various groups, including tyrannosaurs. This is however an apparently unique record with evidence of both pre- and post-mortem injuries to a single individual.

Accelerating Universe? Not So Fast

Certain types of supernovae, or exploding stars, are more diverse than previously thought, a University of Arizona-led team of astronomers has discovered. The results, reported in two papers published in the Astrophysical Journal, have implications for big cosmological questions, such as how fast the universe has been expanding since the Big Bang.
Most importantly, the findings hint at the possibility that the acceleration of the expansion of the universe might not be quite as fast as textbooks say.
The team, led by UA astronomer Peter A. Milne, discovered that type Ia supernovae, which have been considered so uniform that cosmologists have used them as cosmic "beacons" to plumb the depths of the universe, actually fall into different populations. The findings are analogous to sampling a selection of 100-watt light bulbs at the hardware store and discovering that they vary in brightness.
"We found that the differences are not random, but lead to separating Ia supernovae into two groups, where the group that is in the minority near us are in the majority at large distances -- and thus when the universe was younger," said Milne, an associate astronomer with the UA's Department of Astronomy and Steward Observatory. "There are different populations out there, and they have not been recognized. The big assumption has been that as you go from near to far, type Ia supernovae are the same. That doesn't appear to be the case."
The discovery casts new light on the currently accepted view of the universe expanding at a faster and faster rate, pulled apart by a poorly understood force called dark energy. This view is based on observations that resulted in the 2011 Nobel Prize for Physics awarded to three scientists, including UA alumnus Brian P. Schmidt.
The Nobel laureates discovered independently that many supernovae appeared fainter than predicted because they had moved farther away from Earth than they should have done if the universe expanded at the same rate. This indicated that the rate at which stars and galaxies move away from each other is increasing; in other words, something has been pushing the universe apart faster and faster.
"The idea behind this reasoning," Milne explained, "is that type Ia supernovae happen to be the same brightness -- they all end up pretty similar when they explode. Once people knew why, they started using them as mileposts for the far side of the universe.
"The faraway supernovae should be like the ones nearby because they look like them, but because they're fainter than expected, it led people to conclude they're farther away than expected, and this in turn has led to the conclusion that the universe is expanding faster than it did in the past."
Milne and his co-authors -- Ryan J. Foley of the University of Illinois at Urbana-Champaign, Peter J. Brown at Texas A&M University and Gautham Narayan of the National Optical Astronomy Observatory, or NOAO, in Tucson -- observed a large sample of type Ia supernovae in ultraviolet and visible light. For their study, they combined observations made by the Hubble Space Telescope with those made by NASA's Swift satellite.
The data collected with Swift were crucial because the differences between the populations -- slight shifts toward the red or the blue spectrum -- are subtle in visible light, which had been used to detect type Ia supernovae previously, but became obvious only through Swift's dedicated follow-up observations in the ultraviolet.
"These are great results," said Neil Gehrels, principal investigator of the Swift satellite, who co-authored the first paper. "I am delighted that Swift has provided such important observations, which have been made toward a science goal that is completely independent of the primary mission. It demonstrates the flexibility of our satellite to respond to new phenomena swiftly."
"The realization that there were two groups of type Ia supernovae started with Swift data," Milne said. "Then we went through other datasets to see if we see the same. And we found the trend to be present in all the other datasets.
"As you're going back in time, we see a change in the supernovae population," he added. "The explosion has something different about it, something that doesn't jump out at you when you look at it in optical light, but we see it in the ultraviolet.
"Since nobody realized that before, all these supernovae were thrown in the same barrel. But if you were to look at 10 of them nearby, those 10 are going to be redder on average than a sample of 10 faraway supernovae."
The authors conclude that some of the reported acceleration of the universe can be explained by color differences between the two groups of supernovae, leaving less acceleration than initially reported. This would, in turn, require less dark energy than currently assumed.
"We're proposing that our data suggest there might be less dark energy than textbook knowledge, but we can't put a number on it," Milne said. "Until our paper, the two populations of supernovae were treated as the same population. To get that final answer, you need to do all that work again, separately for the red and for the blue population."
The authors pointed out that more data have to be collected before scientists can understand the impact on current measures of dark energy. Scientists and instruments in Arizona will play important roles in these studies, according to Milne. These include projects led by NOAO; the Large Synoptic Survey Telescope, or LSST, whose primary mirror was produced at the UA; and a camera built by the UA's Imaging Technology Lab for the Super-LOTIS telescope on Kitt Peak southwest of Tucson. Super-LOTIS is a robotic telescope that will use the new camera to follow up on gamma-ray bursts -- the "muzzle flash" of a supernova -- detected by Swift.

Thursday, 26 February 2015

A possible answer to the origin of matter

Most of the laws of nature treat particles and antiparticles equally, but stars and planets are made of particles, or matter, and not antiparticles, or antimatter. That asymmetry, which favors matter to a very small degree, has puzzled scientists for many years.


New research by UCLA physicists, published in the journal Physical Review Letters, offers a possible solution to the mystery of the origin of matter in the universe.
Alexander Kusenko, a professor of physics and astronomy in the UCLA College, and colleagues propose that the matter-antimatter asymmetry could be related to the Higgs boson particle, which was the subject of prominent news coverage when it was discovered at Switzerland's Large Hadron Collider in 2012.
Specifically, the UCLA researchers write, the asymmetry may have been produced as a result of the motion of the Higgs field, which is associated with the Higgs boson, and which could have made the masses of particles and antiparticles in the universe temporarily unequal, allowing for a small excess of matter particles over antiparticles.
If a particle and an antiparticle meet, they disappear by emitting two photons or a pair of some other particles. In the "primordial soup" that existed after the Big Bang, there were almost equal amounts of particles of antiparticles, except for a tiny asymmetry: one particle per 10 billion. As the universe cooled, the particles and antiparticles annihilated each other in equal numbers, and only a tiny number of particles remained; this tiny amount is all the stars and planets, and gas in today's universe, said Kusenko, who is also a senior scientist with the Kavli Institute for the Physics and Mathematics of the Universe.
The research also is highlighted by Physical Review Letters in a commentary in the current issue.
The 2012 discovery of the Higgs boson particle was hailed as one of the great scientific accomplishments of recent decades. The Higgs boson was first postulated some 50 years ago as a crucial element of the modern theory of the forces of nature, and is, physicists say, what gives everything in the universe mass. Physicists at the LHC measured the particle's mass and found its value to be peculiar; it is consistent with the possibility that the Higgs field in the first moments of the Big Bang was much larger than its "equilibrium value" observed today.
The Higgs field "had to descend to the equilibrium, in a process of 'Higgs relaxation,'" said Kusenko, the lead author of the UCLA research.
Two of Kusenko's graduate students, Louis Yang of UCLA and Lauren Pearce of the University of Minnesota, Minneapolis, were co-authors of the study. The research was supported by the U.S. Department of Energy (DE-SC0009937), the World Premier International Research Center Initiative in Japan and the National Science Foundation (PHYS-1066293).
Story Source:
The above story is based on materials provided by University of California - Los Angeles

Sunday, 8 February 2015

Another reason to drink wine: it could help you burn fat

The findings suggest that consuming dark-colored grapes, whether eating them or drinking juice or wine, might help people better manage obesity and related metabolic disorders such as fatty liver.
Neil Shay, a biochemist and molecular biologist in OSU's College of Agricultural Sciences, was part of a study team that exposed human liver and fat cells grown in the lab to extracts of four natural chemicals found in Muscadine grapes, a dark-red variety native to the southeastern United States.
One of the chemicals, ellagic acid, proved particularly potent: It dramatically slowed the growth of existing fat cells and formation of new ones, and it boosted metabolism of fatty acids in liver cells.
These plant chemicals are not a weight-loss miracle, cautions Shay. "We didn't find, and we didn't expect to, that these compounds would improve body weight," he said. But by boosting the burning of fat, especially in the liver, they may improve liver function in overweight people.
"If we could develop a dietary strategy for reducing the harmful accumulation of fat in the liver, using common foods like grapes," Shay said, "that would be good news."
The study, which Shay conducted with colleagues at the University of Florida and University of Nebraska, complements work with mice he leads at his OSU laboratory. In one 2013 trial, he and his graduate students supplemented the diets of overweight mice with extracts from Pinot noir grapes harvested from Corvallis-area vineyards.
Some of the mice were fed a normal diet of "mouse chow," as Shay calls it, containing 10 percent fat. The rest were fed a diet of 60 percent fat -- the sort of unhealthy diet that would pile excess pounds on a human frame.
"Our mice like that high-fat diet," said Shay, "and they overconsume it. So they're a good model for the sedentary person who eats too much snack food and doesn't get enough exercise."
The grape extracts, scaled down to a mouse's nutritional needs, were about the equivalent of one and a half cups of grapes a day for a person. "The portions are reasonable," said Shay, "which makes our results more applicable to the human diet."
Over a 10-week trial, the high-fat-fed mice developed fatty liver and diab
etic symptoms -- "the same metabolic consequences we see in many overweight, sedentary people," Shay said.
But the chubby mice that got the extracts accumulated less fat in their livers, and they had lower blood sugar, than those that consumed the high-fat diet alone. Ellagic acid proved to be a powerhouse in this experiment, too, lowering the high-fat-fed mice's blood sugar to nearly the levels of the lean, normally fed mice.
When Shay and his colleagues analyzed the tissues of the fat mice that ate the supplements, they noted higher activity levels of PPAR-alpha and PPAR-gamma, two proteins that work within cells to metabolize fat and sugar.
Shay hypothesizes that the ellagic acid and other chemicals bind to these PPAR-alpha and PPAR-gamma nuclear hormone receptors, causing them to switch on the genes that trigger the metabolism of dietary fat and glucose. Commonly prescribed drugs for lowering blood sugar and triglycerides act in this way, Shay said.
The goal of his work, he added, is not to replace needed medications but to guide people in choosing common, widely available foods that have particular health benefits, including boosting metabolic function.
"We are trying to validate the specific contributions of certain foods for health benefits," he said. "If you're out food shopping, and if you know a certain kind of fruit is good for a health condition you have, wouldn't you want to buy that fruit?"
The research was supported by the Institute of Food and Agricultural Science at the University of Florida and Florida Department of Agriculture and Consumer Services. The study appears in the January issue of the Journal of Nutritional Biochemistry.
Shay's research with mice was supported by the Blue Mountain Horticultural Society, the Erath Family Foundation, and the OSU College of Agricultural Sciences.

Friday, 6 February 2015

What does measles actually do?

The United States is now experiencing what promises to be one of the worst outbreaks of measles since the virus was declared eliminated from the country in 2000.  Itbegan in early January at Disneyland Resort in Anaheim,paramyxovirus from the genus Morbillivirus, is one of the most contagious diseases in the world, infecting more than 90% of susceptible hosts that come in contact with an afflicted individual. In the absence of widespread vaccination, the average person with measles will infect an average of 12 to 18 other people; in contrast, Ebola is typically transmitted to 1.5 to 2.5 people. Children, in particular, are more likely to experience complications as a result of a measles infection. Although the overall mortality rate for children who get measles is only between 0.1% and 0.2%, as many as one out of every 20 children will also develop pneumonia. The disease symptoms can be managed with common anti-inflammatory drugs, hydration, and rest, but like many other viral illnesses, there is no cure and antibiotics will have no effect. Death rates are much higher in developing countries.
California, and has since spread to 14 states and infected 84 people, according to the U.S. Centers for Disease Control and Prevention (CDC). Measles, caused by a
What does measles do to the immune system?
Measles virus is spread from person to person through the air in coughed-out aerosolized droplets that are inhaled. The virus typically first comes in contact with host lung tissue, where it infects immune cells called macrophages and dendritic cells, which serve as an early defense and warning system. From there, the infected cells migrate to the lymph nodes where they transfer the virus to B and T cells. A surface protein on these white blood cells, known as CD150, serves as the virus’s point of entry during this critical step. The infected B and T cells then migrate throughout the body releasing virus particles into the blood. The spleen, lymph nodes, liver, thymus, skin, and lungs are eventual destinations for the virus. In rare instances (about one in 1000 cases), the virus can cross the blood-brain barrier and cause dangerous swelling of the brain; infection of lung cells causes a hacking cough that keeps the virus circulating in the population.
Why does measles cause a rash?
One of the classic presentations of a measles infection is a rash characterized by flat red blotches that starts on the face and moves down the body all the way to the feet over a few days. The rash is a symptom of inflammation occurring in the skin. As the virus travels in the blood, it infects capillaries in the skin. Immune cells detect the infection and respond by releasing chemicals such as nitric oxide and histamines, which destroy the viral invaders and call other immune cells into action. These same chemicals, however, cause swelling and damage to host cells, resulting in the often itchy skin rash, which usually occurs concurrently with a fever that can reach as high as 40°C. 
Why is measles back?
Measles has actually been back. Last year was one of the worst years in recent history for the United States: CDC reported 644 cases from 23 separate outbreaks during 2014; between 2001 and 2013, no single year saw more than 250 cases. (Because measles was declared “eliminated” in the United States in 2000, outbreaks have been triggered by virus “imported” from other countries, which then finds an unvaccinated person.) With 84 people infected already in 2015, things are not off to the best start.
CDC
Number of measles infections each year from 2001 through 2014.
Part of the reason for the resurgence is a rise in the number of parents who refuse to vaccinate their children against the virus.Despite an overwhelming amount of scientific and medical evidence demonstrating both the safety and efficacy of the measles vaccine, some parents refuse to vaccinate their children for reasons of personal belief. The problem is compounded because many like-minded parents are geographically clustered. For the entire state of California, the vaccine refusal rate is only 2.6%, indicating that most citizens are cognizant of the benefits of immunization. However, a recent study of pediatric health records revealed that in some areas the vaccine refusal rate is as high as 13.5%. Other factors such as a lack of time, education, or money can cause parents to inadvertently fall behind on their children’s immunizations.
Disneyland provided an ideal starting point for an epidemic. In such a crowded atmosphere, a single infected individual might come in contact with hundreds or thousands of people in a day. Even if 90% of people are immunized, the virus’s high infectivity will allow it to spread through the population by jumping between susceptible individuals.
How can I protect my children from getting measles?
Get them vaccinated.

Friday, 9 January 2015

Eight New Planets Found in "Goldilocks" Zone

Astronomers announced today that they have found eight new planets in the "Goldilocks" zone of their stars, orbiting at a distance where liquid water can exist on the planet's surface. This doubles the number of small planets (less than twice the diameter of Earth) believed to be in the habitable zone of their parent stars. Among these eight, the team identified two that are the most similar to Earth of any known exoplanets to date.
"Most of these planets have a good chance of being rocky, like Earth," says lead author Guillermo Torres of the Harvard-Smithsonian Center for Astrophysics (CfA).
These findings were announced today in a press conference at a meeting of the American Astronomical Society.
The two most Earth-like planets of the group are Kepler-438b and Kepler-442b. Both orbit red dwarf stars that are smaller and cooler than our Sun. Kepler-438b circles its star every 35 days, while Kepler-442b completes one orbit every 112 days.
With a diameter just 12 percent bigger than Earth, Kepler-438b has a 70-percent chance of being rocky, according to the team's calculations. Kepler-442b is about one-third larger than Earth, but still has a 60-percent chance of being rocky.
To be in the habitable zone, an exoplanet must receive about as much sunlight as Earth. Too much, and any water would boil away as steam. Too little, and water will freeze solid.
"For our calculations we chose to adopt the broadest possible limits that can plausibly lead to suitable conditions for life," says Torres.
Kepler-438b receives about 40 percent more light than Earth. (In comparison, Venus gets twice as much solar radiation as Earth.) As a result, the team calculates it has a 70 percent likelihood of being in the habitable zone of its star.
Kepler-442b get about two-thirds as much light as Earth. The scientists give it a 97 percent chance of being in the habitable zone.
"We don't know for sure whether any of the planets in our sample are truly habitable," explains second author David Kipping of the CfA. "All we can say is that they're promising candidates."
Prior to this, the two most Earth-like planets known were Kepler-186f, which is 1.1 times the size of Earth and receives 32 percent as much light, and Kepler-62f, which is 1.4 times the size of Earth and gets 41 percent as much light.
The team studied planetary candidates first identified by NASA's Kepler mission. All of the planets were too small to confirm by measuring their masses. Instead, the team validated them by using a computer program called BLENDER to determine that they are statistically likely to be planets. BLENDER was developed by Torres and colleague Francois Fressin, and runs on the Pleaides supercomputer at NASA Ames. This is the same method that has been used previously to validate some of Kepler's most iconic finds, including the first two Earth-size planets around a Sun-like star and the first exoplanet smaller than Mercury.
After the BLENDER analysis, the team spent another year gathering follow-up observations in the form of high-resolution spectroscopy, adaptive optics imaging, and speckle interferometry to thoroughly characterize the systems.
Those follow-up observations also revealed that four of the newly validated planets are in multiple-star systems. However, the companion stars are distant and don't significantly influence the planets.
As with many Kepler discoveries, the newly found planets are distant enough to make additional observations challenging. Kepler-438b is located 470 light-years from Earth while the more distant Kepler-442b is 1,100 light-years away.
The paper reporting these results has been accepted for publication in The Astrophysical Journal and is available online.
Headquartered in Cambridge, Mass., the Harvard-Smithsonian Center for Astrophysics (CfA) is a joint collaboration between the Smithsonian Astrophysical Observatory and the Harvard College Observatory. CfA scientists, organized into six research divisions, study the origin, evolution and ultimate fate of the universe.