log in


Website URL:

Cern OPERA experiment reports anomaly


OPERA experiment reports anomaly in flight duration of neutrinos from CERN to Gran Sasso

Geneva, 23 September 2011. The OPERA1 experiment, which observes a neutrino beam from CERN2 730 km away at Italy’s INFN Gran Sasso Research laboratory,have presented brand-new results in a seminar located at CERN.

The OPERA result are based on the observation of over 15000 neutrino events measured at Gran Sasso, and appears to indicate that the neutrinos travel at a velocity 20 parts per million above the speed of light, nature’s cosmic speed limit. Given the potential far-reaching consequences of such a result, independent measurements are needed before the effect can either be refuted or firmly established. This is why the OPERA collaboration has decided to open the result to broader scrutiny. The collaboration’s result is available on the preprint server arxiv.org: http://arxiv.org/abs/1109.4897.

The OPERA measurement is at odds with well-established laws of nature, though science frequently progresses by overthrowing the established paradigms. For this reason, many searches have been made for deviations from Einstein’s theory of relativity, so far not finding any such evidence. The strong constraints arising from these observations makes an interpretation of the OPERA measurement in terms of modification of Einstein’s theory unlikely, and give further strong reason to seek new independent measurements.

“This result comes as a complete surprise,” said OPERA spokesperson, Antonio Ereditato of the University of Bern. “After many months of studies and cross checks we have not found any instrumental effect that could explain the result of the measurement. While OPERA researchers will continue their studies, we are also looking forward to independent measurements to fully assess the nature of this observation.”

 “When an experiment finds an apparently unbelievable result and can find no artefact of the measurement to account for it, it’s normal procedure to invite broader scrutiny, and this is exactly what the OPERA collaboration is doing, it’s good scientific practice,” said CERN Research Director Sergio Bertolucci. “If this measurement is confirmed, it might change our view of physics, but we need to be sure that there are no other, more mundane, explanations. That will require independent measurements.”

In order to perform this study, the OPERA Collaboration teamed up with experts in metrology from CERN and other institutions to perform a series of high precision measurements of the distance between the source and the detector, and of the neutrinos’ time of flight. The distance between the origin of the neutrino beam and OPERA was measured with an uncertainty of 20 cm over the 730 km travel path. The neutrinos’ time of flight was determined with an accuracy of less than 10 nanoseconds by using sophisticated instruments including advanced GPS systems and atomic clocks. The time response of all elements of the CNGS beam line and of the OPERA detector has also been measured with great precision.

"We have established synchronization between CERN and Gran Sasso that gives us nanosecond accuracy, and we’ve measured the distance between the two sites to 20 centimetres,” said Dario Autiero, the CNRS researcher who will give this afternoon’s seminar. “Although our measurements have low systematic uncertainty and high statistical accuracy, and we place great confidence in our results, we’re looking forward to comparing them with those from other experiments."

“The potential impact on science is too large to draw immediate conclusions or attempt physics interpretations. My first reaction is that the neutrino is still surprising us with its mysteries.” said Ereditato. “Today’s seminar is intended to invite scrutiny from the broader particle physics community.”

The OPERA experiment was inaugurated in 2006, with the main goal of studying the rare transformation (oscillation) of muon neutrinos into tau neutrinos. One first such event was observed in 2010, proving the unique ability of the experiment in the detection of the elusive signal of tau neutrinos.


The Disclosure Petition


log paradigm research group
The Disclosure Petition



The Disclosure Petition is now active on the White House website at the above link. The wording of the petition is as follows:

"We, the undersigned, strongly urge the President of the United States to formally acknowledge an extraterrestrial presence engaging the human race and immediately release into the public domain all files from all agencies and military services relevant to this phenomenon."

[Note to all those outside the US: a US Zip Code is required for registering.]

Should this petition receive a significant number of signatures it will draw media attention which will generate more signatures. It can become a direct referendum on the matter of Disclosure if the link to the petition can be taken viral on the Internet.

If you wish to support this petition, use Facebook, MySpace, Twitter, YouTube, blogs, bulletin boards, email lists, websites and all other social media to take the link viral. YouTubers can create Disclosure Petition videos and include the petition link. Webmasters can go to www.disclosurepetition.info and find graphic banners for attaching the petition link.

The link to the petition on the White House website is: http://wh.gov/gKC

Paradigm Research Group 4938 Hampden Lane, #161, Bethesda, MD 20814 This email address is being protected from spambots. You need JavaScript enabled to view it. 202-215-8344 www.paradigmresearchgroup.org

"Tatooine-like" planet found in our galaxy

The actual existence of a world with a double setting sun, as pictured in the film Star Wars more than thirty years ago, is now scientific fact. NASA's Kepler mission has made the first unambiguous discovery of a circumbinary planet -- a planet revolving around two stars -- 200 light-years from Earth.

As opposed to Star Wars’ Tatooine, the planet is very cold, gaseous and not believed to harbor life, however its discovery shows the diversity of planets in our universe. Previous studies have hinted at the existence of circumbinary planets, but clear evidence proved elusive. Kepler detected such a planet, known as Kepler-16b, by observing transits, when the brightness of a parent star dims from the planet crossing in front of it.

"This breakthrough discovery confirms a new class of planetary systems which could harbor life," Kepler principal researcher William Borucki said. "Given that many stars in our galaxy are part of a binary system, this means the possibilities for life are much greater than if planets form only around single stars. This  breakthrough discovery confirms a theory that scientists have had for many years but could not prove until now."

A research team led by Laurance Doyle of the SETI Institute in Mountain View, Calif., utilized data from the Kepler space telescope, which measures dips in the brightness of more than 150,000 stars, to find transiting planets. Kepler is the first NASA mission able to find Earth-size planets in or near to the "habitable zone," the region in a planetary system where liquid h2o (water) can can be found on the surface of the orbiting planet.

Scientists discovered the new planet in the Kepler-16 system, a pair of orbiting stars that eclipse each other from our vantage point on Earth. Whenever the smaller star partially obstructs the larger star, a primary eclipse takes place, and a secondary eclipse occurs when the smaller sized star is occulted, or totally blocked, by the larger star.

Astronomers further more noticed that the brightness of the system dropped even when the stars were not eclipsing each other, hinting at a 3rd body. The additional dimming in brightness events, called the tertiary and quaternary eclipses, reappeared at unpredictable intervals of time, indicating the stars were in different positions in their orbit each time the third body passed. This confirmed the third body was circling, not merely one, but both stars, in a wide circumbinary orbit.

The gravitational pull on the stars, measured by alterations in their eclipse times, was a good indicator of the mass of the 3rd body. Only a very minor gravitational pull was detected, one that only could be caused by a small mass. The actual findings are described in a new study released Friday, Sept. 16, in the journal Science.

"Most of what we know about the sizes of stars comes from such eclipsing binary systems, and most of what we know about the size of planets comes from transits," said Doyle, who also is the lead author and a Kepler participating scientist. "Kepler-16 brings together the very best of both worlds, with stellar eclipses and planetary transits in a single system."

This discovery shows that Kepler-16b is an unfriendly, cold world about the size of Saturn and believed to be made up of about 50 % rock and 50 % gas. The parent stars are smaller than our sun. One is 69 % the mass of the sun and the other only 20 %. Kepler-16b orbits around the two stars every 229 days, comparable to Venus’ 225-day orbit, but lies outside the system’s habitable region, where liquid water could exist on the surface, because the stars are cooler than our sun.

"Working in motion picture, we regularly are tasked with producing something never before seen," said visual effects manager John Knoll of Industrial Light & Magic, a division of Lucasfilm Ltd., in San Francisco. "However, in many cases, scientific discoveries prove to be a lot more spectacular than anything we dare imagine. There's no question these discoveries influence and inspire storytellers. Their very existence serves as cause to dream even bigger and open our imagination to new possibilities beyond what we think we 'know.'

Viewing Vesta upclose

Four years after launch out of Cape Canaveral, NASA's ion-drive Dawn spacecraft is finally in orbit around the asteroid Vesta, checking out the second largest body within the rubble-strewn belt in between Mars and Jupiter in unmatched detail. Photos unveiled today show a unusually tortured world along with enormous parallel lines separating the intensely cratered northern hemisphere from clearer terrain in the south covered with the chaotic remains of a devastating impact.

"All these photographs have been already a fantastic revelation to the team about what the surface is like," Christopher Russell, the mission's primary investigator, told journalists today. "We did not imagine the detail we're seeing and the various processes that we're seeing evidence of now. These are really insightful into this kind of building block of the premature solar system...It's actually a stunning and exciting little world sitting there in the center of the asteroid belt that we're going to learn a great deal about."

NASA's Dawn spacecraft, right now in orbit around the asteroid Vesta, is beaming back exciting photos displaying huge equatorial grooves, upper left, separating the heavily-cratered northern hemisphere through smoother terrain in the south, where a catastrophic impact took place the distant past.

Discovered in 1807, Vesta is just about spherical, measuring about 359 miles by 284 miles. It's the biggest member of the asteroid belt yet visited by a robotic spacecraft, 2nd in size only to Ceres, Dawn's following target and, together with Pluto, one of just five known dwarf planets. NASA is actually spending $466 million to understand more about Vesta and Ceres throughout the course of a 10-year mission.

Vesta's surface area is believed to be composed of basaltic rock that ran out of a presumably scorching interior when the asteroid formed some 4.5 billion years in the past. Because of its small size, the asteroid probably cooled rapidly and did not undergo subsequent resurfacing just like larger worlds.

As such, Vesta might have one of the oldest, most captivating surfaces in the solar system, a icy snapshot of the components and conditions that was around at the dawn of the solar system.

"We believe that this goes back to the initial 5 million years of the solar system," Russell suggested. "What occurred back then was that the material that was orbiting that was going to end up being the sun began to condense. We have evidence of what was taking place through very primitive meteorites which have fallen to the Earth.

"Right when Vesta began to come together, we believe there seemed to be a supernova that irradiated the material and added radioactive material to it that when the materials joined together, it had an additional heat source and several of these bodies which were formed melted and then differentiated, they provided a crust of lava and an iron core. Those are examples of the oldest bodies out there."

Previous observations by the Hubble Space Telescope demonstrated what appeared to be a huge impact crater near Vesta's south pole that expands some 285 miles across and measures some 8 miles deep. In excess of 200,000 cubic miles of debris were blasted into space, according to on the Dawn press package, a few of which ultimately made its way to Earth as meteorites.

To put the impact into perspective, a proportionately sized crater on Earth might possibly be around the size of the Pacific Ocean.

Images from Dawn show chaotic landscapes near the south pole covered with a magnificent central peak and huge ripple-like lines extending around the asteroid's equator. Terrain north of the lines is much more heavily cratered.

"Those lines are pretty much in the equatorial area and they're very much perpendicular to the direction we assume the impact was going when it struck Vesta," Russell said. "So one thing it could be is that when the compression of that amazing impact came, Vesta got smaller in that direction for a while and after that expanded which caused tectonic features around the equatorial region."

Launched on top of a United Launch Alliance Delta 2 rocket on September 27, 2007, Dawn is the first operational deep space mission to be designed with an ion propulsion system. Instead of burning up liquid propellants in short, high-power bursts, Dawn's propulsion system works by utilizing electrical power to ionize and accelerate electrically charged xenon to velocities ten times more than the exhaust from chemical type rockets.

Dawn's ion propulsion system "only pushes on the spacecraft as hard as this individual sheet of paper pushes on my hand," said Marc Rayman, mission supervisor and chief engineer, holding up a single piece of paper. "And yet little by little, over time, the result of this whisper-like thrust can develop and produce exceptionally high velocity. So this is what I like to call acceleration with patience. And now, our patience is paying off very handsomely indeed."

During final approach to Vesta, Dawn's final velocity was just 60 miles per hour relative to the asteroid. Finally, on July 15, the spacecraft was taken by Vesta's weak gravity, placing it in orbit.

"Thanks to all the thrusting we've been doing all along the way, Dawn was able to gradually creep up on Vesta and slip ever so gently into orbit with similar grace and elegance it's displayed in nearly 1000 days of inner planetary ion thrusting," Rayman explained.

Dawn's preliminary orbit around Vesta carries it over the asteroid's poles at an height of roughly 1,700 miles. The actual orbit's orientation keeps the spacecraft and its massive solar panels in direct sunlight to supply power for its instruments and its propulsion system.

Traveling from north to south, Dawn will accomplish one orbit every three Earth days. Simply because Vesta completes one rotation or "day," every five hours and twenty minutes, Dawn should be able to observe the asteroid's complete illuminated surface every orbit. During south-to-north passes above Vesta's night side, Dawn will transmit saved images and other data back to Earth.

Operating in the initially high survey orbit, Dawn's instruments can provide a global view of Vesta in ultraviolet, visible and infra-red wavelengths. A mapping spectrometer will observe the surface area with a image resolution of 2,300 feet per pixel while the spacecraft's visible-light cameras will resolve features as small as 820 feet across, around 150 times better than photographs taken by the Hubble Space Telescope.

Dawn's gamma ray and neutron detector will assist researchers characterize the surface composition of Vesta while evaluation of subtle changes in the spacecraft's radio signal, triggered by slight changes in Dawn's orbital velocity, will help scientists map out the actual asteroids gravity field and internal structure.

After seven orbits, or around three weeks in the survey orbit, Dawn's ion propulsion system will spend 30 days or so slowly decreasing the orbit to an altitude of about 420 miles, permitting the spacecraft to circle the asteroid twice each Earth day.

Dawn will complete around 60 trips around Vesta in this so-called high-altitude mapping orbit, or HAMO, surveying the asteroid in outstanding detail, permitting scientists to build topographic maps showing the elevation of hills and mountains and the absolute depths of the craters covering its surface.

After HAMO operations are complete, Dawn will spend about 6 weeks lowering down to a low-altitude mapping orbit, or LAMO, at less than one hundred and ten miles, circling Vesta every 4 hours.

While the lower orbit provides Dawn's cameras sharp views of Vesta's surface, the main goal of this 10-week stage of the mission is to permit the gamma ray and neutron detector to monitor cosmic ray impacts on the surface. High-energy cosmic radiation hitting atoms in the upper three feet of the surface area will generate gamma rays and neutrons that can be used to discover the identities of the original atoms.

The impact of Vesta's gravity on Dawn's orbit will be more noticeable in the low-altitude orbit, allowing scientists to map out its inner mass distribution.

When the low-altitude stage of the mission is complete, Dawn will spend an additional six weeks spiraling out for a 2nd set of observations at an altitude of 420 miles, comparable to the earlier high-altitude mapping orbit. Because approximately eight months will have passed between the 2 sets of observations, a greater portion of Vesta's northern hemisphere will be illuminated as the asteroid's seasons progress and areas not observed earlier will be mapped at the identical level of detail.

If all goes well, Dawn will commence its departure from Vesta in Summer of 2012, setting off on a two-and-a-half-year journey to Ceres. The mission is funded through July 2015.

Subscribe to this RSS feed