15+ Breathtaking Pics Of Volcano Eruption In Chile That Forced 4,000 To Evacuate


Calbuco, a 2,000m (6,572ft) volcano in Chile, has erupted twice in the past day, sending emergency services (and photographers) into overdrive. The eruption has prompted the evacuation of roughly 4,000 citizens from nearby cities and villages, and the Argentinian authorities have warned their citizens about volcanic ash as well.
The volcano overlooks the cities of Puerto Montt and Puerto Varas, which have a combined population of roughly 250,000 people. It last erupted in 1972, so authorities were somewhat surprised by the outburst. Calbuco is a stratovolcano (also known as a composite volcano), and these are best known for having explosive eruptions – the infamous Krakatoa, Vesuvius and Mt. St. Helens volcanoes are all stratovolcanoes. We can only hope that Calbuco does not decide to blow its top as well.
With the authorities on the ground doing their jobs to keep people safe, we can turn our attention to the photographers that have been having a field day with the eruption. Stunning photos of smoke columns painted red by lava and enormous ash plumes laced with lightning have been pouring out of the area. Check out some of the photos and footage below!

Volcano Eruption In Calbuco, Chile
Volcano Eruption In Calbuco, Chile
Volcano Eruption In Calbuco, ChileVolcano Eruption In Calbuco, Chile

Cold cosmic mystery solved: Largest known structure in the universe leaves its imprint on CMB radiation

A cold cosmic mystery solved
The Cold Spot area resides in the constellation Eridanus in the southern galactic hemisphere. The insets show the environment of this anomalous patch of the sky as mapped by Szapudi's team using PS1 and WISE data and as observed in the cosmic 
In 2004, astronomers examining a map of the radiation leftover from the Big Bang (the cosmic microwave background, or CMB) discovered the Cold Spot, a larger-than-expected unusually cold area of the sky. The physics surrounding the Big Bang theory predicts warmer and cooler spots of various sizes in the infant universe, but a spot this large and this cold was unexpected.
Now, a team of astronomers led by Dr. Istvan Szapudi of the Institute for Astronomy at the University of Hawaii at Manoa may have found an explanation for the existence of the Cold Spot, which Szapudi says may be "the largest individual structure ever identified by humanity."
If the Cold Spot originated from the Big Bang itself, it could be a rare sign of exotic physics that the standard cosmology (basically, the Big Bang theory and related physics) does not explain. If, however, it is caused by a foreground structure between us and the CMB, it would be a sign that there is an extremely rare large-scale structure in the mass distribution of the universe.
Using data from Hawaii's Pan-STARRS1 (PS1) telescope located on Haleakala, Maui, and NASA's Wide Field Survey Explorer (WISE) satellite, Szapudi's team discovered a large supervoid, a vast region 1.8 billion light-years across, in which the density of galaxies is much lower than usual in the known universe. This void was found by combining observations taken by PS1 at optical wavelengths with observations taken by WISE at infrared wavelengths to estimate the distance to and position of each galaxy in that part of the sky.
Earlier studies, also done in Hawaii, observed a much smaller area in the direction of the Cold Spot, but they could establish only that no very distant structure is in that part of the sky. Paradoxically, identifying nearby large structures is harder than finding distant ones, since we must map larger portions of the sky to see the closer structures. The large three-dimensional sky maps created from PS1 and WISE by Dr. András Kovács (Eötvös Loránd University, Budapest, Hungary) were thus essential for this study. The supervoid is only about 3 billion light-years away from us, a relatively short distance in the cosmic scheme of things.
Imagine there is a huge void with very little matter between you (the observer) and the CMB. Now think of the void as a hill. As the light enters the void, it must climb this hill. If the universe were not undergoing accelerating expansion, then the void would not evolve significantly, and light would descend the hill and regain the energy it lost as it exits the void. But with the accelerating expansion, the hill is measurably stretched as the light is traveling over it. By the time the light descends the hill, the hill has gotten flatter than when the light entered, so the light cannot pick up all the energy it lost upon entering the void. The light exits the void with less energy, and therefore at a longer wavelength, which corresponds to a colder temperature.
Getting through a supervoid can take millions of years, even at the speed of light, so this measurable effect, known as the Integrated Sachs-Wolfe (ISW) effect, might provide the first explanation one of the most significant anomalies found to date in the CMB, first by a NASA satellite called the Wilkinson Microwave Anisotropy Probe (WMAP), and more recently, by Planck, a satellite launched by the European Space Agency.
While the existence of the supervoid and its expected effect on the CMB do not fully explain the Cold Spot, it is very unlikely that the supervoid and the Cold Spot at the same location are a coincidence. The team will continue its work using improved data from PS1 and from the Dark Energy Survey being conducted with a telescope in Chile to study the Cold Spot and supervoid, as well as another large void located near the constellation Draco.
The study is being published online on April 20 in Monthly Notices of the Royal Astronomical Society by the Oxford University Press. In addition to Szapudi and Kovács, researchers who contributed to this study include UH Manoa alumnus Benjamin Granett (now at the National Institute for Astrophysics, Italy), Zsolt Frei (Eötvös Loránd), and Joseph Silk (Johns Hopkins).
from :-
phys.org

Want To Do A Little Astrophysics? This App Detects Cosmic Rays

App turns a smartphone into a pocket-sized cosmic ray detector

Smart phones contain a silicon chip inside the camera that might be used to detect rare, high energy particles from outer space.
Smart phones contain a silicon chip inside the camera that might be used to detect rare, high energy particles from outer space.
J. Yang/Courtesy of WIPAC
Scientists in California are hoping to use your smart phone to solve a cosmic mystery. They're developing an app to turn your phone into a cosmic ray detector. If enough people install the app, the scientists think they'll be able to figure out once and for all what's producing the very energetic cosmic rays that occasionally hit the Earth.
The project is the brainchild of physicists Daniel Whiteson at the University of California, Irvine, and his buddy Michael Mulhearn at the University of California, Davis. Both spend time in Switzerland, working on the giant particle accelerator known as the Large Hadron Collider. Whiteson says the Large Hadron Collider, located in a tunnel beneath the Swiss-French border near Geneva, is so huge and so complicated that scientists must share their time on the collider.
"The two of us each work on these enormous collaborations of about 3,000 scientists," he says. "And while that's very interesting, and you a meet lot of sharp people, it's also nice sometimes to do a smaller project where you can be in control of what's happening."

That's where the smart phone comes in. Whiteson and his California pals, as well as new collaborator, Kyle Cranmer at New York University, are building an app that turns the CMOS chip in the phones camera into a particle detector. They're hoping millions of people all over the globe will download the app.
When a high energy cosmic ray hits the top of Earth's atmosphere, it creates a shower of new energetic particles.
"So if we have a bunch of users nearby each other, all running the app, they will all see hits in their phone, they'll see particles being detected by our app in their phone in the same moment," says Whiteson.
And by analyzing the distribution of the particle shower detected by the phones, Whiteson says, the astrophysicists will learn more about the high energy cosmic ray that produced the shower.
That's the idea, anyway.
Whiteson says the reaction from other astrophysicists to his scheme ranges from bemused to skeptical. But he thinks that's reasonable.
"We don't yet know if it's the best idea we ever had, or the silliest idea that we ever had," he says. "But one thing we do know is, it's one of the funnest to work on."

LINK_----------> DOWNLOAD - THE -APP

CLOUD


Could there be a link between galactic cosmic rays and cloud formation? An experiment at CERN is using the cleanest box in the world to find out
The Cosmics Leaving Outdoor Droplets (CLOUD) experiment uses a special cloud chamber to study the possible link between galactic cosmic rays and cloud formation. Based at the Proton Synchrotron (PS) at CERN, this is the first time a high-energy physics accelerator has been used to study atmospheric and climate science. The results should contribute much to our fundamental understanding of aerosols and clouds, and their affect on climate.
Cosmic rays are charged particles that bombard the Earth's atmosphere from outer space. Studies suggest they may influence cloud cover either through the formation of new aerosols (tiny particles suspended in the air that can grow to form seeds for cloud droplets) or by directly affecting clouds themselves. Clouds exert a strong influence on the Earth’s energy balance; changes of only a few per cent have an important effect on the climate. However, despite its importance for climate, aerosol formation is poorly understood. Measuring the underlying microphysics in controlled laboratory conditions is important for a better understanding of atmospheric aerosol and is the key to unravelling the possible connection between cosmic rays and clouds.
The CLOUD experiment involves an interdisciplinary team of scientists from 17 institutes in nine countries, comprising atmospheric physicists and chemists, and cosmic-ray and particle physicists. The Proton Synchrotron provides an artificial source of “cosmic rays” that simulates natural conditions between ground level and the stratosphere. A beam of particles is passed through the cloud chamber and its effects on aerosol production or on liquid or ice clouds inside the chamber are recorded and analysed.
The experiment includes an advanced cloud chamber equipped with a wide range of external instrumentation to monitor and analyse its contents. The temperature conditions anywhere in the atmosphere can be recreated within the chamber. All experimental conditions can be controlled and measured, including the “cosmic ray” intensity and the trace atmospheric vapours in the chamber, which are set to levels of only a few molecules per trillion.

from http://home.web.cern.ch/about/experiments/cloud

Antarctica Recorded Its Hottest Temperature On Record This Week


 
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"Antarctica Recorded Its Hottest Temperature On Record This Week"
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CREDIT: shutterstock
The coldest place on Earth just got warmer than has ever been recorded.
According to the weather blog Weather Underground, on Tuesday, March 24, the temperature in Antarctica rose to 63.5°F (17.5C) — a record for the polar continent. Part of a longer heat wave, the record high came just a day after the previous record was set at 63.3°F.
Tuesday’s temperature was taken at the Argentina’s Esperanza Base, located near the northern tip of the Antarctic Peninsula. The Monday record was from Marambio Base, about 60 miles southeast of Esperanza. Both are records for the locations, however the World Meteorological Organization is yet to certify that the temperatures are all-time weather records for Antarctica. Before these two chart-toppers, the highest recorded temperature from these outposts was 62.8°F in 1961.
Setting a new all-time temperature record for an entire continent is rare and requires the synthesizing of a lot of data. As Weather Underground’s weather historian, Christopher C. Burt, explains, there is debate over what exactly is included in the continent Antarctica, and by the narrowest interpretation, which would include only sites south of the Antarctic Circle, Esperanza would not be part of the continent.
According to the WMO, the official keeper of global temperature records, the all-time high temperature for Antarctica was 59°F in 1974. As Mashable reports, the verification process for these new records could take months as the readings must be checked for accuracy.
 
Departure of temperature from average for Tuesday, March, 24, 2015, over Antarctica.
Departure of temperature from average for Tuesday, March, 24, 2015, over Antarctica.
CREDIT: University of Main Climate Reanalyzer.

Even in their unofficial capacity, the readings are stunning.
As Burt reports, these temperature records occurred nearly three months past the warmest time of year in the Antarctic Peninsula, December, when the average high is 37.8°F. The average high for March is 31.3°F, making this week’s records more than 30°F above average. Burt also points out that temperature records for Esperanza have previously occurred in October and April, so these spikes are not unheard of.
They should also not be unexpected: the poles are warming faster than any part of the planet and rapid ice melt is being observed at increased rates in Antarctica. According to a new study, ice shelves in West Antarctica have lost as much as 18 percent of their volume over the last two decades, with rapid acceleration occurring over the last decade. The study found that from 1994 to 2003, the overall loss of ice shelf volume across the continent was negligible, but over the last decade West Antarctic losses increased by 70 percent.
According to the British Antarctic Survey, since records for the Antarctic Peninsula began half a century ago, the average temperature has risen about 5°F, making it “the most rapidly warming region in the Southern Hemisphere – comparable to rapidly warming regions of the Arctic.”
While the polar regions are feeling the most severe temperature changes brought on by the rise in greenhouse gas concentrations in the atmosphere, areas across the globe are setting record highs at a much faster rate than record lows. Since 2010, 46 nations or territories out of 235 have set or tied record highs. Only four have set record lows. According to the Weather Underground, so far this year, five nations or territories have tied or set all-time records for their highest temperature: Antarctica, Equatorial Guinea, Ghana, Wallis and Futuna Territory, and Samoa.

Is this ET? Mystery of strange radio bursts from space

  • 31 March 2015 by Sarah Scoles
Mysterious radio wave flashes from far outside the galaxy are proving tough for astronomers to explain. Is it pulsars? A spy satellite? Or an alien message?
BURSTS of radio waves flashing across the sky seem to follow a mathematical pattern. If the pattern is real, either some strange celestial physics is going on, or the bursts are artificial, produced by human – or alien – technology.
Telescopes have been picking up so-called fast radio bursts (FRBs) since 2001. They last just a few milliseconds and erupt with about as much energy as the sun releases in a month. Ten have been detected so far, most recently in 2014, when the Parkes Telescope in New South Wales, Australia, caught a burst in action for the first time. The others were found by sifting through data after the bursts had arrived at Earth. No one knows what causes them, but the brevity of the bursts means their source has to be small – hundreds of kilometres across at most – so they can't be from ordinary stars. And they seem to come from far outside the galaxy.
The weird part is that they all fit a pattern that doesn't match what we know about cosmic physics.

To calculate how far the bursts have come, astronomers use a concept called the dispersion measure. Each burst covers a range of radio frequencies, as if the whole FM band were playing the same song. But electrons in space scatter and delay the radiation, so that higher frequency waves make it across space faster than lower frequency waves. The more space the signal crosses, the bigger the difference, or dispersion measure, between the arrival time of high and low frequencies – and the further the signal has travelled.
Michael Hippke of the Institute for Data Analysis in Neukirchen-Vluyn, Germany, and John Learned at the University of Hawaii in Manoa found that all 10 bursts' dispersion measures are multiples of a single number: 187.5 . This neat line-up, if taken at face value, would imply five sources for the bursts all at regularly spaced distances from Earth, billions of light-years away. A more likely explanation, Hippke and Lerned say, is that the FRBs all come from somewhere much closer to home, from a group of objects within the Milky Way that naturally emit shorter-frequency radio waves after higher-frequency ones, with a delay that is a multiple of 187.5 (arxiv.org/abs/1503.05245).
They claim there is a 5 in 10,000 probability that the line-up is coincidence. "If the pattern is real," says Learned, "it is very, very hard to explain."
Cosmic objects might, by some natural but unknown process, produce dispersions in regular steps. Small, dense remnant stars called pulsars are known to emit bursts of radio waves, though not in regular arrangements or with as much power as FRBs. But maybe superdense stars are mathematical oddities because of underlying physics we don't understand.
It's also possible that the telescopes are picking up evidence of human technology, like an unmapped spy satellite, masquerading as signals from deep space.
The most tantalising possibility is that the source of the bursts might be a who, not a what. If none of the natural explanations pan out, their paper concludes, "An artificial source (human or non-human) must be considered."
"Beacon from extraterrestrials" has always been on the list of weird possible origins for these bursts. "These have been intriguing as an engineered signal, or evidence of extraterrestrial technology, since the first was discovered," says Jill Tarter, former director of the SETI Institute in California. "I'm intrigued. Stay tuned."
Astronomers have long speculated that a mathematically clever message – broadcasts encoded with pi, or flashes that count out prime numbers, as sent by aliens in the film Contact – could give away aliens' existence. Perhaps extraterrestrial civilisations are flagging us down with basic multiplication.

Power source

But a fast radio burst is definitely not the easiest message aliens could send. As Maura McLaughlin of West Virginia University, who was part of the first FRB discovery points out, it takes a lot of energy to make a signal that spreads across lots of frequencies, instead of just a narrow one like a radio station. And if the bursts come from outside the galaxy, they would have to be incredibly energetic to get this far.
If the bursts actually come from inside the Milky Way, they need not be so energetic (just like a nearby flashlight can light up the ground but a distant light does not). Either way, though, it would require a lot of power. In fact, the aliens would have to be from what SETI scientists call a Kardashev Type II civilisation .
But maybe there's no pattern at all, let alone one that aliens embedded. There are only 10 bursts, and they fit into just five groups. "It's very easy to find patterns when you have small-number statistics," says McLaughlin. "On the other hand, I don't think you can argue with the statistics, so it is odd."
The pattern might disappear as more FRBs are detected. Hippke and Learned plan to check their finding against new discoveries, and perhaps learn something about the universe. "Science is the best game around," says Learned. "You don't know what the rules are, or if you can win. This is science in action."
If the result holds up, says Hippke, "there is something really interesting we need to understand. This will either be new physics, like a new kind of pulsar, or, in the end, if we can exclude everything else, an ET."
Hippke is cautious, but notes that remote possibilities are still possibilities. "When you set out to search for something new," he says, "you might find something unexpected."
This article appeared in print under the headline "Cosmic radio plays an alien tune"

Giant Radio Telescope Peels Away Magnetic Field Shrouding Black Hole




A Black Hole's Surroundings
An artist's impression shows a black hole's surroundings, including its accretion disk, jet and magnetic field.
Credit: ESO/L. Calçada
Astronomers have peeled away most of the gas and dust enshrouding a monster black hole, taking a close look at the giant that lies some 68 thousand light-years away.
A Swedish team of scientists has used the Atacama Large Millimeter/submillimeter Array (ALMA) — a huge radio telescope in Chile — to unmask a supermassive black hole's extremely powerful magnetic field. The team, led by Ivan Marti-Vidal from the Onsala Space Observatory and Chalmers University of Technology, was therefore able to peer deep into the heart of the distant galaxy where the black hole lies, and see the region just light-days away from the behemoth.
"Our discovery is a giant leap in terms of observing frequency, thanks to the use of ALMA, and in terms of distance to the black hole where the magnetic field has been probed," said co-author Sebastien Muller, also from Onsala Space Observatory and Chalmers University of Technology, in a statement.

Supermassive black holes loom in the centers of the majority of massive galaxies. Some of these black holes, like the one in the Milky Way's center, lie dormant. Others (so-called quasars) actively chow down on gas, causing them to radiate like brilliant beacons of light. They can therefore be seen from across the universe.
Although these monsters clearly accrete huge amounts of matter, some material escapes. It's flung out into space at close to the speed of light in a jet of plasma. Astronomers don't understand the physical mechanism at play here, but think it has to do with a strong magnetic field close to the black hole itself.
Luckily, magnetic field lines leave an imprint on any light that passes through them. The magnetic field will twist light so that it is circularly polarized, meaning the electric and magnetic fields rotate continuously as the wave moves, in a corkscrew motion. The stronger the magnetic field, the stronger this imprint.
Until now, only weak magnetic fields located several light-years from the black hole have been caught on camera via this twisting of light. But by looking at higher energies, like the ones visible with ALMA, astronomers can probe more powerful magnetic fields, which lie closer to their black hole counterparts.

Violent Methane Storms on Titan May Explain Strange Dunes



Titan Methane Ice Cloud
A methane ice cloud is seen over the north pole of Saturn's moon Titan in this view captured by NASA's Cassini spacecraft in December 2006. Scientists suspect that intense methane storms on Titan may also sculpt towering dunes at the moon's equator.
Credit: NASA/JPL/University of Arizona/LPGNantes
Rare tropical methane storms could help solve the mystery of how strange, giant dunes form on Titan, Saturn's largest moon, researchers say.
When NASA's Cassini spacecraft began exploring Titan in2004, its most dramatic discovery was the field of dunes that covers nearly 15 percent of Titan's surface along its equator. These dark, massive dunes — the largest of their kind in the solar system — are made of exotic sand composed of hydrogen and carbon. They can be more than 330 feet (100 meters) high and are typically 18 to 31 miles (30 to 50 kilometers) long.
These long, colossal dunes pose one of Titan's greatest mysteries, as they seem to grow eastward, whereas models of Titan's atmosphere predict that surface winds at its equatorial latitudes would blow westward. However, prior research found that Titan's winds do blow eastward at altitudes above about 3 miles (5 km). This finding has led scientists to wonder if these high winds might somehow help solve this puzzle, even though they blow far above these dunes.

Now, researchers have found that rare methane storms could help sculpt the moon's surface.
"Clouds and storms are rare on Titan," said Benjamin Charnay, a planetary scientist at the Dynamic Meteorology Laboratory in Paris and lead author of the study detailing the new findings. "They were not expected to have an impact on dunes."
Sand Dunes on Titan
Sand dunes on Saturn's largest moon Titan dominate this image captured by NASA's Cassini spacecraft in 2009. This image is centered on a region just north of Titan's equator. Scientists suspect Titan's giant dunes at the equator may be sculpted by intense methane storms.
Credit: NASA/JPL-Caltech/ASI
Titan is the only moon in the solar system with a thick atmosphere. Its atmosphere is composed mostly of nitrogen, with a trace of methane that can form into clouds. During the equinox, when days and nights are about the same length, Titan experiences huge, violent methane storms in the tropical regions around its equator.
Computer models of weather on Titan revealed that methane clouds can reach altitudes of 15.5 miles (25 kilometers), where the high, fast eastward winds blow. The researchers found that, as a result, methane storms can produce downdrafts that flow eastward on strong gusts after they reach Titan's surface.
The researchers estimated that these eastward gusts can reach up to 22 mph (36 km/h) — 10 times faster than the usual winds close to Titan's surface.
"We were very surprised by the intensity of the storm gusts," Charnay said. "For Titan, it is like a hurricane."
The researchers suggested that these storm gusts may explain the shape, size, spacing and eastward growth of Titan's dunes. If scientists can get a better understanding of how these dunes form on Titan, it could reveal more insight into the moon's present and past atmosphere.
"There are long dunes on Titan which formed over a very long period of time, likely more than 1 million years," Charnay said. "Others are shorter and formed during the last 100,000 years."
By studying Titan's dunes, scientists can also learn more about dune formation on Earth. For example, in this new study, the researchers developed a new growth mechanism for dunes that may answer questions about how dunes form on Earth, Charnay said.
The scientists detailed their findings online April 13 in the journal Nature Geoscience

News

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SpaceX Dragon cargo ship reaches space station

Irene Klotz, Spaceflight Correspondent
17 April 2015, 12:37 UTC
Sen—A SpaceX Dragon cargo ship wrapped up a 2.5-day journey to the International Space Station Friday, positioning itself within reach of the outpost’s 57ft-long robotic arm for capture and berthing.
Italian astronaut Samantha Cristoforetti, working inside the windowed cupola module, nosed the outstretched crane to Dragon’s grapple fixture and snared the capsule at 6:55 a.m. EDT/1055 UTC as the station sailed about 260 miles over the Pacific Ocean just east of Japan.
Dragon, loaded with more than 4,300 pounds of food, clothing, equipment and science experiments, blasted off aboard a SpaceX Falcon 9 rocket on Tuesday, the sixth of a recently extended 15-flight contract with NASA to run cargo to the station.
This time, Dragon’s unpressurized trunk, which typically holds experiments and instruments installed outside the station, is empty so that the pressurized section could be stuffed full. The cargo includes:
*A replacement nanosatellite for Planetary Resources, an aspiring asteroid mining outfit that lost its Arkyd 3 technology demonstrator during Orbital ATK’s botched Antares launch in October. Comprised of three CubeSats, Arkyd 3 will be deployed from the station’s Kibo module by NanoRack’s satellite launcher.
*14 Earth-observation CubeSats, called Doves and owned by San Francisco-based Planet Labs.
*20 mice that will serve as subjects for an experiment investigating how microgravity impacts bones. The rodents will be euthanized and dissected in orbit, and the samples sent back to Earth when Dragon returns in May. The Rodent Research Facility made its debut flight to the station last year. The bone loss study is sponsored by Novartis under a commercial agreement with the Center for the Advancement of Science in Space, which manages station research under a U.S. National Laboratory program.
*A synthetic muscle material developed by Ras Labs, a Massachusetts Institute of Technology spinoff company that wants to test how radiation impacts the electroactive polymer. The material contracts with an electric current and expands back to its original state when the charge is reversed.
Initial ground-based experiments show the materials are resistant to radiation, said lead researcher Lenore Rasmussen. For their debut space run, the materials, which have different additives and coatings, will be attached inside the station and photographed over the next three months. They will be returned to Earth for analysis.
*An Italian-made espresso machine called “ISSPresso” specially modified to work—or hopefully work—in the challenging conditions of zero gravity. A joint project of Argotec, Lavazza and the Italian Space Agency, the machine, which will be attached to a wall with bungee cords, was modified to fit the station’s standard-size water pouches.
“We have been thinking about taking the espresso into space for some time,” Lavazza vice president Giuseppe Lavazza said in a statement. “We hope (it) will improve the living and nutrition quality of astronauts engaged on long missions.”
Dragon also is carrying food, clothing and care packages for the astronauts; dozens of experiments, including studies devoted for the station’s first year-long crew; environmental control and life support equipment; computers and other electronics; photo and TV gear; and components for the U.S. spacesuits.
The capsule is expected to remain in orbit until May 21.
- See more at: http://sen.com/news/supply-chain-from-enceladus-to-saturn-s-e-ring-observed#sthash.xdG7MKve.dpuf

Gravitational Wave Detection Update: Prospects for Impacts on Fundamental Physics










Author(s) Schutz, Bernard (speaker)
Corporate author(s) CERN. Geneva
Imprint 2015-04-15. - Streaming video.
Series (TH Theoretical Seminar)
Lecture note on 2015-04-15T14:00:00
Subject category TH Theoretical Seminar
Copyright/License © 2015 CERN
Submitted by gavin.salam@cern.ch



click here to get the link




CERN webcast: "The Odyssey of Voyager" by Prof. Edward C. Stone, as part of the AMS days at CERN



webcast link click here

Launched in 1977 to explore Jupiter, Saturn, Uranus, and Neptune, the two Voyager spacecraft continued their journeys beyond the planets as they searched for the edge of heliosphere, the giant bubble of wind surrounding the sun. Beyond the bubble lies interstellar space, the space between the stars filled with matter from the explosions of other stars and by the magnetic field of the Milky Way. After a thirty-five year journey taking it eighteen billion kilometers from the Earth, Voyager 1 became the first human-made object to enter interstellar space. Voyager’s odyssey continues as it explores the space between the stars.

Edward C. Stone is the David Morrisroe Professor of Physics and Vice Provost for Special Projects at the California Institute of Technology (Caltech). He is also the Executive Director of the TMT International Observatory LLC and a former Director of NASA’s Jet Propulsion Laboratory. Read more about his role and background via https://indico.cern.ch/event/387001/

This public talk is part of a 3-day colloquium "AMS days at CERN". The Alpha Magnetic Spectrometer (AMS) Experiment on the International Space Station has to date recorded over 60 billion cosmic ray events (e-, e+, p, antiproton, He, Li, B/C ...) up to TeV energies. AMS is a precision particle physics detector, assembled and extensively calibrated at CERN before its launch in 2011.

For more about the colloquium, see: http://indico.cern.ch/event/381134/ or watch the webcast via https://webcast.web.cern.ch/webcast/play.php?event=381134