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Study shows men won't be losing their Y chromosome anytime soon

Y Chromosome
© Knorre/Shutterstock
Finally, some good news for men, as a new study in PLOS Genetics has found that the human race may not be losing the Y chromosome after all. Some popular theories have posited that the male sex chromosome is destined to diminish and disappear.

"The Y chromosome has lost 90 percent of the genes it once shared with the X chromosome, and some scientists have speculated that the Y chromosome will disappear in less than 5 million years," said study author Melissa A. Wilson Sayres, a post-doctoral evolutionary biologist at the University of California, Berkeley.

Some mammal species have lost their Y chromosome, yet still have the ability to sexually reproduce viable offspring - fueling suspicions that the chromosome may not be essential in humans.

"Our study demonstrates that the genes that have been maintained, and those that migrated from the X to the Y, are important, and the human Y is going to stick around for a long while," Wilson Sayres said.

Based the Y chromosome analysis of 16 men, researchers found genetic evidence of natural selection maintaining the chromosome's content, which has been shown to mostly play a role in male fertility. The researchers said the Y chromosome's diminutive size is a sign that it is stripped down to its 27 essential genes.

Chalkboard

Does a woolly mammoth need a lawyer?

Image
© Flying Puffin on FlickrWoolly mammoth at Royal BC Museum in Victoria.
In 2009, a biologist named Daniel Gluesenkamp was driving through San Francisco when he saw a ghost. Draped over a bluff by the side of the road was a twenty-foot wide shrub festooned with cream-colored flowers. Gluesenkamp immediately recognized the plant as Franciscan manzanita, or Arctostaphylos hookeri franciscana. He was astonished, because it had been considered extinct in the wild for decades. The last known wild Franciscan manzanita had been bulldozed in a graveyard in 1947.

Before 1947, a few clippings of Franciscan manzanita had ended up in nurseries. Today you can buy the plant online. But the nursery form is the result of hybridization and extreme breeding; it's now about as much like wild Franciscan manzanita as a German shepherd is like a wolf. It's unlikely it could survive in the wild anymore. For thousands of years, wild Franciscan manzanita had grown luxuriantly in the prairies that carpeted much of the California coast. Now the wild plants were all gone - or almost, it turned out.

Before Gluesenkamp's discovery, the U.S. government officially listed Franciscan manzanita as extinct in the wild. But then three organizations - the Wild Equity Institute, Center for Biological Diversity, and California Native Plant Society - petitioned the U.S. government to change its status. In 2012, the Fish and Wildlife Service agreed to the request and reclassified Franciscan manzanita from extinct to endangered. Its known wild population was precisely one.

This wasn't exactly the original plan for the Endangered Species Act when it was enacted in 1973. It was intended to protect species that were moving in the other direction, from healthy populations towards extinction. But once the single wild Franciscan manzanita plant came to light, the government decided that it deserved protection, too.

Question

Is it a planet or a star? Or is all our theories all wrong? Backwards astronomers don't understand why a newly discovered 'brown dwarf' can't be a brown dwarf!

Mystery Object
© Courtesy of Thayne CurrieThis is an image of the ROXs 42B system obtained with the Keck telescope. The star is located in the center of the masked region. ROXs 42Bb orbits at about 150 astronomical units (AU). (1 AU=the distance from Earth to the Sun.) The other object ("c") is a likely unrelated background star.
One of the more interesting questions in astronomy surrounds how solar system objects actually form. Astronomers are particularly concerned about the boundary between a planet and a star. When examining the objects in our own solar neighborhood, the question seems trivial - the Sun dominates the mass of our system, while even the largest planet, Jupiter, is dwarfed by comparison.

In other parts of the galaxy, stars exist that are only a tiny fraction of the size of our Sun, yet scientists have discovered planets that are many times larger than Jupiter. At around a dozen Jupiter-masses, the line between star and planet begins to blur, and astronomers refer to these objects as brown dwarfs.

They are massive enough that simple proton-proton fusion exists in their cores, yet the energy produced by this mechanism is not sufficient enough to sustain it as a star. For this reason brown dwarfs are sometimes also known as failed stars. However, new data is complicating their classification even further.

Located about 440 light-years from Earth is a strange object that has the properties of a brown dwarf. However, a careful study of its mass indicates that it is not massive enough to be categorized as such.

Comment: The 'new research' they need is already available in the Thunderbolts Project's Electric Sky and Electric Universe.

According to conventional astronomical theory, brown dwarfs are small stars nearing the end of their life because their 'internal Fermi reactions' are decreasing due to lack of fuel (hydrogen), making them progressively dimmer and dimmer. However, there are several problems with this model. For starters, brown dwarfs emit X-rays:
The orbiting x-ray telescope Chandra recently discovered a brown dwarf (spectral class M9) emitting an x-ray flare. This poses an additional problem for the advocates of the stellar fusion model. A star this cool should not be capable of x-ray flare production. How 'gravitational collapse' can produce x-rays remains unexplained. "We were shocked," said Dr. Robert Rutledge of the California Institute of Technology in Pasadena, the lead author on the discovery paper to appear in the July 20 issue of Astrophysical Journal Letters. "We didn't expect to see flaring from such a lightweight object. This is really the 'mouse that roared.'" [Scott D., The Electric Sky, p. 127]
So, in standard astronomical models, brown dwarfs are 'supposed to be' too cool and too small to maintain fusion reactions in their cores. The minimum temperature 'should be' three million degrees kelvin and the mass should be at least seven percent of the Sun's mass, but some previously classified 'brown dwarfs' have actually not met those requirements, and, as a result, are too small to generate a gravitational collapse to trigger nuclear fusion and subsequent X-ray radiation.

But a brown dwarf presents no such anomaly in electric models. It's simply a star that is not glowing because the local electric field is too weak. From this perspective it's not the size (and therefore the limited gravitational field) that makes a star dark, but the electric stress. If the electric stress is too low, the star (whatever its size) doesn't glow. Thus the maximum size determined by mainstream science to define brown dwarfs is irrelevant.


Cassiopaea

'Hand of God' spotted by NASA space telescope

Hand of God
© NASA/JPL-Caltech/McGill The hand might look like an X-ray from the doctor's office, but it is actually a cloud of material ejected from a star that exploded. NASA's NuSTAR spacecraft has imaged the structure in high-energy X-rays for the first time, shown in blue. Lower-energy X-ray light previously detected by NASA's Chandra X-ray Observatory is shown in green and red.
Religion and astronomy may not overlap often, but a new NASA X-ray image captures a celestial object that resembles the "Hand of God."

The cosmic "hand of God" photo was produced when a star exploded and ejected an enormous cloud of material, which NASA's Nuclear Spectroscopic Telescope Array, or NuSTAR, glimpsed in high-energy X-rays, shown in blue in the photo. NASA's Chandra X-ray Observatory had imaged the green and red parts previously, using lower-energy X-rays.

"NuSTAR's unique viewpoint, in seeing the highest-energy X-rays, is showing us well-studied objects and regions in a whole new light," NuSTAR telescope principal investigator Fiona Harrison, of the California Institute of Technology in Pasadena, said in a statement.

The new image depicts a pulsar wind nebula, produced by the dense remnant of a star that exploded in a supernova. What's left behind is a pulsar, called PSR B1509-58 (B1509 for short), which spins around 7 times per second blowing a wind of particles into material ejected during the star's death throes.

Nuke

Radioactive particles from nuclear tests still prevalent in atmosphere

Nuclear Explosion
© AmazingFacts
A new study has found that radioactive particles from nuclear tests that took place decades ago persist in the upper atmosphere.

Previously, scientists believed that nuclear debris found high above the Earth would now be negligible.

However, this research shows that plutonium and caesium isotopes are still present at surprisingly high concentrations, the BBC reported.

Lead author Dr Jose Corcho Alvarado, from the Institute of Radiation Physics at Lausanne University Hospital in Switzerland, said that most of the radioactive particles are removed in the first few years after the explosion, but a fraction remains in the stratosphere for a few decades or even hundreds or thousands of years.

However, he said that the levels were not high enough to pose a risk to human health.

At the height of the Cold War, when the nuclear arms race was in full swing, weapons were being developed and tested around the world.

But more than 50 years on, their radioactive legacy remains.

Cassiopaea

A rare crash at the Milky Way's core

Astronomers have a front-row seat to observe a mysterious gas cloud spiraling toward our galaxy's supermassive black hole.

Milky Way
© Nathalie DegenaarThe galactic center as imaged by the Swift X-ray Telescope. This image is a montage of all data obtained in the monitoring program from 2006-2013.
University of Michigan astronomers could be the first to witness a rare collision expected to happen at the center of our galaxy by spring.

With NASA's orbiting Swift telescope, the University of Michigan team is taking daily images of a mysterious gas cloud about three times the mass of Earth that's spiraling toward the supermassive black hole at the Milky Way's core. From our vantage point, the core lies more than 25,000 light-years away in the southern summer sky near the constellations Sagittarius and Scorpius.

In 2011, German astronomers discovered a gas cloud called G2. They expected it to hit the black hole called Sagittarius A* (pronounced "Sagittarius A-star") late last year. That didn't happen, but the cloud continues to drift closer. Astronomers now predict that the impact will occur in the next few months.

Astronomers have never seen anything like this, much less with a front-row seat.

"Everyone wants to see the event happening because it's so rare," said Nathalie Degenaar from the Department of Astronomy at the College of Literature, Science and the Arts.

Galaxy

Rare eclipsing binary asteroid discovered by astronomy students

doppler asteroid
© Loretta KuoStudents in a University of Maryland undergraduate astronomy class have made a startling discovery. A previously unstudied asteroid isn't just one object, but is instead made up of a pair of asteroids that orbit and regularly eclipse each other. In this artist's rendering, the newly-identified binary asteroid 3905 Doppler approaches an eclipse as the larger asteroid begins to pass in front of the smaller one, as seen from a vantage point on Earth
Students in a University of Maryland undergraduate astronomy class have made a startling discovery. A previously unstudied asteroid isn't just one object, but is instead made up of a pair of asteroids that orbit and regularly eclipse each other. The rare discovery may help researchers investigate these sorts of asteroids in the future.

So far, fewer than 100 eclipsing binary asteroids have been identified in the main asteroid belt between Mars and Jupiter. This latest discovery, known as 3905 Doppler, is therefore unusual. It was first detected in 1984, but over the next few decades, it attracted scant attention. Then in September 2013, the students chose to study it due to its position in the autumn sky.

Blue Planet

Plateau du Vercors: Mountain formation ain't what it used to be

Mont Aiguille
© Philippe StoopMont Aiguille and the Grand Veymont region
Aciculate peaks and curvilinear ridges outline giant circular depressions in the French Alps.

As previously written, stone monoliths can be found all over the world. There are colossal formations that make up the French Alps, for instance. In particular, Mont Aiguille (Needle Mountain) is similar to the structures from the Amazonian region of South America that were discussed in another Picture of the Day.

Flat-topped mesas are common throughout Europe, the southwestern United States, the Amazon, and elsewhere. Arizona's Monument Valley includes elevations that almost exactly mirror those found in the Alps, although they are composed of different rock matrices. Those in Arizona are sandstone tors with sharply delineated sidewalls and those in the French Alps, such as Mont Aiguille, are composed of limestone.

Mail

Think metadata isn't intrusive? Read this

Metadata
© EWSolutions
You've probably heard politicians or pundits say that "metadata doesn't matter." They argue that police and intelligence agencies shouldn't need probable cause warrants to collect information about our communications. Metadata isn't all that revealing, they say, it's just numbers.

But the digital metadata trails you leave behind every day say more about you than you can imagine. Now, thanks to two MIT students, you don't have to imagine - at least with respect to your email.

Deepak Jagdish and Daniel Smilkov's Immersion program maps your life, using your email account. After you give the researchers access to your email metadata - not the content, just the time and date stamps, and "To" and "Cc" fields - they'll return to you a series of maps and graphs that will blow your mind. The program will remind you of former loves, illustrate the changing dynamics of your professional and personal networks over time, mark deaths and transitions in your life, and more. You'll probably learn something new about yourself, if you study it closely enough. (The students say they delete your data on your command.)

Whether or not you grant the program access to your data, watch the video embedded below to see Jagdish and Smilkov show illustrations from Immersion and talk about what they discerned about themselves from looking at their own metadata maps. While you're watching, remember that while the NSA and FBI are collecting our phone records in bulk, and using advanced computer algorithms to make meaning from them, state and local government officials can often also get this information without a warrant.

Info

Invisible light patterns help bees find food even on cloudy days

Bee
© Thinkstock
Bees are excellent navigators. Once they stumble upon a food source, they keep coming back to the same spot without faltering. They also have a great sense of smell and can recognize color patterns and symmetry in flowers - admirable feats for an insect whose brain is the size of a sesame seed.

Scientists have long known that bees use the sunlight like a compass to map their route to the flowers full of succulent dew. They also know that bees use a seemingly complex and deceptively random waggle dance to let their mates know where to find the food source. Scientists are now able to "understand" most of the dance movements, and have striven to figure out how bees translate the map in their tiny heads into these movements.

For some time now, scientists have also believed that bees use a pattern of light in the sky called polarized light in their navigation system. Polarized light is created from sunlight scattered in the sky by particles in the air, and is invisible to the human eye.

New research shows that bees use this polarized light to guide their movements, even when there's no sunlight.

The study was published in the journal Philosophical Transactions of the Royal Society B.

In the study, the researchers directed bees down a tunnel towards a sugar source. The tunnel blocked out sunlight and only polarized light was made to shine down on the bees from above. At times, the light was shining along the direction of the tunnel, at times at right angles to it. The researchers then watched to see how the bees waggled about the location of the food source to their mates.