Universe Today

April 9, 2011April 13, 2022 by Ken Kremer

Countdown to Yuri’s Night and the 50th Anniversary of Human Spaceflight !

Celebrate Yuri’s Night on April 12, 2011 -- 50th Anniversary of Human Spaceflight
On April 12, 1961, Russian cosmonaut Yuri Gagarin (left, on the way to the launch pad) became the first human in space, making a 108-minute orbital flight in his Vostok 1 spacecraft.
Newspapers like The Huntsville Times (right) trumpeted Gagarin's accomplishment.
Credit: NASA
Send Ken your Yuri’s Night event reports and photos

Mark your calendars. April 12, 2011 marks the 50th Anniversary of Human Spaceflight and Cosmonaut Yuri Gagarin’s astonishing First Orbit of our precious planet Earth on April 12, 1961. Gagarin was the first human to enter outer space and see what no one else had ever witnessed – our commonly shared Earth as a planet and beautiful blue globe with no borders.

Space enthusiasts worldwide are celebrating this watershed moment in Human history at a network of over 400 “Yuri’s Night” parties taking place in more than 70 countries on 6 continents and 2 worlds, according to the official “Yuri’s Night” website.

Gagarin’s flight took place in the midst of the inflammatory Cold War rivalry between the Soviet Union and the United States and shocked the world into new realities. The Space Race led to the first lunar landing by the United States and Neil Armstrong’s first steps on the moons surface in 1969. Eventually, the world’s superpowers beat swords into plowshares and united their efforts to build the International Space Station.

Yuri Gagarin - first human in space. Credit: Russian Archives

Yuri Gagarin was the first person to boldly leave the bonds of Earth’s gravity and thus became the first “Spaceman”. Gagarin blasted off inside the bell-shaped Vostok 1 spaceship from the launch pad at Baikonur at 9:07 a.m, Moscow time (607 UTC) to begin the era of human spaceflight.

Gagarin flew around the Earth in a single orbit at an altitude of 302 kilometers (187 miles). The flight lasted 108 minutes and safely ended when he descended back and parachuted to the ground, just north of the Caspian Sea. At the age of 27, Gagarin was instantly transformed into a worldwide hero. After the momentous flight he soon embarked on an international tour.

20 years later on April 12, 1981, NASA’s first space shuttle blasted off on the STS-1 mission on a daring test flight with astronauts John Young and Bob Crippen strapped inside Space Shuttle Columbia.

The first “Yuri’s Night – World Space Party” was held on April 12, 2001 to commemorate the 40th anniversary of Gagarin’s spaceflight. Over 10,000 people attended 64 events located worldwide. The goal was to inspire people, increase awareness and support for space exploration across the globe and foster the spread of new ideas to broaden our access to space.

“Yuri’s Night” has been growing in popularity every year. Events range in size from a few folks to numbers in the thousands. Attendees range from astronauts and cosmonauts, NASA and global space agency officials and reps, scientists and engineers, famous actors, playwrights, writers, artists, athletes and musicians to just everyday folks and kids of all ages and backgrounds. Everyone can get involved.

In honor of the 50th anniversary of Gagarin’s flight, documentary film maker Christopher Riley conceived and created a film titled “First Orbit” to try and show the approximate view of Earth that Gagarin actually saw. There is only scant footage of Gagarin’s actual flight and he himself took no pictures of the Earth from orbit.

“First Orbit” recreates much of the view of the Earth’s surface that Gagarin would have seen fifty years ago. Mostly he flew over the world oceans as well as the Soviet Union and Africa.

Riley collaborated with the astronauts aboard the International Space Station, chiefly Paolo Nespoli of ESA, who took film footage from the new 7 windowed Cupola as the station matched the actual flight path of Gagarin and Vostok 1 as closely as possible. The free film celebrates 50 years of human spaceflight.

“First Orbit” premiers worldwide on YouTube in a special global streaming event for Yuri’s Night on April 12 . Watch the short trailer below, with original and stirring music by Philip Sheppard.

Orbital flight path of Yuri Gagarin and Vostok 1 on April 12, 1961
Gagarin’s call sign was Cedar or Kder - which means Siberian Pine in Russian. Map courtesy of Sven Grahn

It’s easy and free to register your local party at the Yuri’s Night event website. There is still time to register your Yuri’s Night party – Indeed the list has grown as I typed out this story !

Some events are already set to kick off this weekend. I’ll be presenting at an interactive and free Yuri’s Night evening event in Princeton Junction, New Jersey, about Gagarin’s flight and my experiences with the space shuttle and what‘s beyond.

Send Ken your “Yuri’s Night” event photos/short report to post in a round up story at Universe Today about the global festivities celebrating the historic achievement of Yuri Gagarin. Email kremerken at yahoo dot com

First Orbit Trailer II

Russian built Mini Research Module MRM-1 launched aboard US Space Shuttle Atlantis in May 2010.
Shuttle Atlantis delivered MRM-1 (known as Rassvet) to the International Space Station.
MRM-1 undergoes final prelaunch processing inside clean room at Astrotech Space Operations Facility in Florida. Docking port to ISS is protected by red colored covering. Equipment airlock for experiments at top. Russian Flag mounted at left.
Rassvet underscores the cooperation that exists today, in stark contrast to their rivalry during the Cold War. Russia, the United States, Europe, Japan and Canada have now united their space exploration efforts to build the International Space Station. The worlds space powers cooperate in other space exploration projects today as well that venture to the Moon, Mars and beyond to Deep Space. Credit: Ken Kremer

Read Ken’s other stories about Yuri Gagarin and Yuri’s Night:
Yuri Gagarin and Vostok 1 Photo Album – 50th Anniversary of Human Spaceflight
Stirring Video Tributes to Yuri Gagarin

Yuri’s Night Website
Yuri’s Night Party list
Yuri’s Night Party with Ken in Princeton Junction, NJ, USA
First Orbit Website
STS-1 NASA Mission Website
Ken Kremer

April 8, 2011December 24, 2015 by Nancy Atkinson

How Would a Government Shutdown Affect NASA?

NASA faces the curtaillment of many jobs and services during a government shutdown including website updates. Image credit: (and with thanks) Heather Archuletta.

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The big question weighing on the minds of anyone involved or interested in US space exploration is how a US government shutdown would affect the space agency. In short, if a NASA job or service is curtailed or a department or building is closed and it doesn’t threaten a life, a spacecraft, data, or a mission, it won’t be continued during a government shutdown. That means thousands of NASA employees would be furloughed, scientists for robotic missions won’t be able to work on gathering new data, and the STS-134 launch could be delayed indefinitely until Congress passes a budget.

While the shuttle mission wouldn’t launch as scheduled on April 29 to the International Space Station because of a shutdown, all NASA workers essential to the ISS and its operations would continue to work, as well as those who keep the space shuttle Endeavour – out on the launchpad – safe and stable. Additionally, engineers involved with NASA’s many space probes and Earth orbiting satellites who monitor spacecraft health and keep them functioning – those “necessary to prevent harm to life or property” as NASA put it, would keep working. But scientists and researchers involved with those missions will likely be sent home.

In a letter to the Office of Management and Budget, NASA Chief Financial Officer Elizabeth Robinson provided an update on how NASA will function in the event of a government funding hiatus. “The decision on what personnel should be excepted from furlough is very fact specific, and Directors in charge of NASA Centers are in the best position to make detailed decisions regarding the suspension of ongoing, regular functions which could imminently threaten the safety of human life or the protection of property,” Robinson wrote.

For example, at NASA Headquarters, there are 1,611 total employees, and only 22 are considered “essential” and would not be furloughed. At NASA’s Ames Research Center, only 25 out of 1250 full time employees would not be furloughed if and when shutdown happens.

A government employee told us that during a furlough, even if someone is classified as “essential” or “exempted” and has to come in and work, they won’t get paid until later. For “non-essential” employees, there is no guarantee the government will provide any compensation for the time the government offices are is closed. “For the shutdown in 1995, they DID give everyone back pay,” said the employee, who wished to remain anonymous. “But this time? Who knows?”

For anyone who lives and breathes NASA on the internet, you will find your lifeblood cut. NASA TV will not broadcast. NASA websites will not be updated including the main nasa.gov site; the NASA Earth Observatory website sent out an email to notify subscribers that they will not be able to update starting April 9 if the shutdown occurs. This is for security reasons, since IT people won’t be there to maintain and secure the websites.

NASA employees, including astronauts who have “official” Twitter accounts have been ordered not to Tweet under a government shutdown and the same goes for Facebook updates for any official NASA account or mission. One exception is that ESA astronaut Paolo Nespoli on board the ISS can still use Twitter.

Any tours and public access to NASA Centers and facilities will be canceled, and any NASA instructors at schools or universities will be ordered not to report. A news conference scheduled for April 12 at the Kennedy Space Center to announce which museums will have won the rights to display NASA’s three space shuttles would has been put on hold pending the government shutdown.

These and other things will occur if no agreement is reached on a fiscal year 2011 budget by midnight tonight, (Friday, April 8, 2011). For more details, see this NASA page which includes three pdf documents which outline what happens for the space agency during a government shutdown. Without getting into the politics, the entire situation is very sad and disheartening.

Thanks to Heather Archuletta (Pillownaut) for the lead image.

April 8, 2011December 24, 2015 by VirtualAstro

How to find Saturn in the Sky this Weekend

If you want to find the planet Saturn in the sky this weekend, but aren’t sure where to look, this guide should help you.

Saturn is visible all night long at the moment and is quite easy to find, as it is just past opposition which makes it quite bright.

Find the constellation of Leo the Lion (high in the Southern sky at around 10pm) by looking for the backwards question mark asterism (red in the diagram), which is the head of Leo. Find the last 2 stars in Leo’s body and draw an imaginary line through these 2 stars, and arc to the left and down until you reach a bright yellowish star. This is Saturn.

If you continue drawing this imaginary line a little further you will find the bright bluish white star Spica, in the constellation of Virgo.

Right now, Saturn should be an easy target to spot with the naked eye, but looks great through binoculars and is truly amazing through any telescope.

April 8, 2011January 18, 2016 by Nancy Atkinson

Spring Fireballs

For reasons yet unknown, the rate of midnight fireballs increases during the weeks around the vernal equinox. It’s a beautiful display, but where do they come from? Last month, we reported on a network of fireball cameras that NASA is building, which is now tracking incoming fireballs — and just in time, too, for the fireball season. This video is part of a new series by NASA called ScienceCast, which will be a weekly feature highlighting a topic in NASA science news.

April 8, 2011December 24, 2015 by Jon Voisey

Halos Gone MAD

Distribution of dark matter when the Universe was about 3 billion years old, obtained from a numerical simulation of galaxy formation. The left panel displays the continuous distribution of dark matter particles, showing the typical wispy structure of the cosmic web, with a network of sheets and filaments, while the right panel highlights the dark matter halos representing the most efficient cosmic sites for the formation of star-bursting galaxies with a minimum dark matter halo mass of 300 billion times that of the Sun. Credit: VIRGO Consortium/Alexandre Amblard/ESA

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One of the successes of the ΛCDM model of the universe is the ability for models to create structures of with scales and distributions similar to those we view in the universe today. Or, at least that’s what astronomers tell us. While computer simulations can recreate numerical universes in a box, interpreting these mathematical approximations is a challenge in and of itself. To identify the components of the simulated space, astronomers have had to develop tools to search for structure. The results has been nearly 30 independent computer programs since 1974. Each promises to reveal the forming structure in the universe by finding regions in which dark matter halos form. To test these algorithms out, a conference was arranged in Madrid, Spain during the May of 2010 entitled “Haloes going MAD” in which 18 of these codes were put to the test to see how well they stacked up.

Numerical simulations for universes, like the famous Millennium Simulation begin with nothing more than “particles”. While these were undoubtedly small on a cosmological scale, such particles represent blobs of dark matter with millions or billions solar masses. As time is run forwards, they are allowed to interact with one another following rules that coincident with our best understanding of physics and the nature of such matter. This leads to an evolving universe from which astronomers must use the complicated codes to locate the conglomerations of dark matter inside which galaxies would form.

One of the main methods such programs use is to search for small overdensities and then grow a spherical shell around it until the density falls off to a negligible factor. Most will then prune the particles within the volume that are not gravitationally bound to make sure that the detection mechanism didn’t just seize on a brief, transient clustering that will fall apart in time. Other techniques involve searching other phase spaces for particles with similar velocities all nearby (a sign that they have become bound).

To compare how each of the algorithms fared, they were put through two tests. The first, involved a series of intentionally created dark matter halos with embedded sub-halos. Since the particle distribution was intentionally placed, the output from the programs should correctly find the center and size of the halos. The second test was a full fledged universe simulation. In this, the actual distribution wouldn’t be known, but the sheer size would allow different programs to be compared on the same data set to see how similarly they interpreted a common source.

In both tests, all the finders generally performed well. In the first test, there were some discrepancies based on how different programs defined the location of the halos. Some defined it as the peak in density, while others defined it as a center of mass. When searching for sub-halos, ones that used the phase space approach seemed to be able to more reliably detect smaller formations, yet did not always detect which particles in the clump were actually bound. For the full simulation, all algorithms agreed exceptionally well. Due to the nature of the simulation, small scales weren’t well represented so the understanding of how each detect these structures was limited.

The combination of these tests did not favor one particular algorithm or method over any other. It revealed that each generally functions well with regard to one another. The ability for so many independent codes, with independent methods means that the findings are extremely robust. The knowledge they pass on about how our understanding of the universe evolves allows astronomers to make fundamental comparisons to the observable universe in order to test the such models and theories.

The results of this test have been compiled into a paper that is slated for publication in an upcoming issue of the Monthly Notices of the Royal Astronomical Society.

April 8, 2011December 24, 2015 by Ken Kremer

Curiosity Mars Rover Almost Complete

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NASA’s massive ‘Curiosity’ rover is almost ready to begin the first leg of its long trek to the surface of the Red Planet. Engineers at NASA’s Jet Propulsion Laboratory in California are nearly finished with assembling and testing all the components of the Mars Science Laboratory (MSL) mission (see photos above and below).

The MSL team plans to ship Curiosity as well as the cruise stage, descent stage and back shell to the Kennedy Space Center (KSC) in May and June. After arriving at KSC, all the pieces will be integrated together and tested during final assembly in a clean room. The rover will then be installed inside a 5 meter diameter nose cone, shipped the short distance to Cape Canaveral and then bolted atop an Atlas V rocket (photo below).

Top of Mars Rover Curiosity's Remote Sensing Mast.
The remote sensing mast on NASA Mars rover Curiosity holds two science instruments for studying the rover's surroundings and two stereo navigation cameras for use in driving the rover and planning rover activities. Credit: NASA/JPL-Caltech

The launch window for Curiosity extends from Nov. 25 to Dec. 18, 2011. The first stage of the powerful Atlas V rocket will be augmented with four solid rocket boosters. The Atlas V has previously launched two planetary missions; the Mars Reconnaissance Orbiter (MRO) and the New Horizons mission to Pluto.

Take a long gander at the 3 meter long rover because its appearance is now very much how it will look while it’s roving along intriguing martian landscapes for at least two earth years after landing in August 2012.

NASA Mars Rover Curiosity at JPL, View from Front Left Corner.
Support equipment is holding the Mars rover Curiosity slightly off the floor. When the wheels are on the ground, the top of the rover's mast is about 2.2 meters (7 feet) above ground level. Credit: NASA/JPL-Caltech

The mini-Cooper sized Curiosity rover is equipped with 10 science instruments to investigate Martian soil and rock samples in far greater detail than ever before. Curiosity’s science payload weighs ten times more than any prior Mars rover mission.

The goal is to search for clues to environmental conditions favorable for microbial life and for preserving evidence about whether Martian life ever existed in the past or today. NASA is scrutinizing a list of four potential landing sites for the best chance of finding a habitable zone.

Arm and Mast of Curiosity Mars Rover.
Curiosity's arm and remote sensing mast carry science instruments and other tools for the mission. This image, taken April 4, 2011, inside the Spacecraft Assembly Facility at JPL shows the arm on the left and the mast just right of center. Credit: NASA/JPL-Caltech

Atlas V rocket at pad 41 at Cape Canaveral Air Force Station.
An Atlas V rocket similar to this one with a 5 meter diameter nose cone – but with 4 solid rocket boosters added - will launch Curiosity to Mars in late 2011. Credit: Ken Kremer

Atlas V launch vehicle will blast Curiosity to Mars

April 7, 2011December 24, 2015 by Nancy Atkinson

10 Years of the Mars Odyssey

This view across western Candor Chasma on Mars was created with data from the 2001 Mars Odyssey. Credit: NASA/JPL/Arizona State University, R. Luk

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A 2001 space odyssey indeed! On this day in 2001, the Mars Odyssey spacecraft launched, and now, 3,333 days later, the robotic spacecraft is still going strong. In orbit around the Red Planet, Mars Odyssey has collected more than 130,000 images and continues to send information to Earth about Martian geology, climate, and mineralogy. Last December, Mars Odyssey broke the record for the longest-serving spacecraft at Mars, besting the Mars Global Surveyor, which operated in orbit of Mars from 1997 to 2006.

An artist's impression of the Odyssey orbiter around Mars. . Image Credit: NASA

Measurements by Odyssey have enabled scientists to create maps of minerals and chemical elements and identify regions with buried water ice. Images that measure the surface temperature have provided spectacular views of Martian topography.

Early in the mission, Odyssey determined that radiation in low-Mars orbit is twice that in low-Earth orbit. This is an essential piece of information for eventual human exploration because of its potential health effects — Odyssey has provided vital support to ongoing exploration of Mars by relaying data from the Mars rovers to Earth via the spacecraft’s UHF antenna.

Odyssey will support the 2012 landing of the Mars Science Laboratory and surface operations of that mission. Mars Science Laboratory, a.k.a Curiosity, will assess whether its landing area has had environmental conditions favorable for microbial life and preserving evidence about whether life has existed there. The rover will carry the largest, most advanced set of instruments for scientific studies ever sent to the Martian surface.

Mars Odyssey carries three main science instruments: The Gamma Ray Spectrometer (GRS), the Thermal Emission Imaging System (THEMIS), and the Mars Radiation Environment Experiment (MARIE).

More info: Mars Odyssey website, THEMIS website (tons of great images)

April 7, 2011December 24, 2015 by Tammy Plotner

Global Lunar Week – April 10 to 16, 2011

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In 2009, hundreds of thousands of people participated in one way or another with the International Year of Astronomy, and there’s no reason to let the excitement die! Astronomers Without Borders are celebrating the entire month of April as Global Astronomy Month and one of the focus points is just three days from arrival… Global Lunar Week!

” A week-long series of programs, from April 10 through 16, will be dedicated to the Moon during Global Astronomy Month to help people rediscover our closest companion in space.” says AWB. “Lunar Week takes place while the Moon is well-placed for observation in the evening sky. As the Moon’s phases and positions change during its orbit around the Earth, there will be Moon-themed star parties to observe the Moon by telescope and naked eye, educational programs, online observing events, competitions and a celebration of the Moon in different cultures.”

Astronomers Without Borders has a theme – One People * One Sky. For all of those who read Universe Today, we realize quickly how astonomy can bring together friends from different countries, different cultures and different time zones. Wouldn’t it be wonderful if we could all observe together?

The dream can come true…

Sander Klieverik from AstronomyLive is working with telescopes around the world to celebrate Global Lunar Week and bring the view right to you.

“The week will start with an amazing broadcast from the historic Chamberlin observatory of the Denver university (with the help of Prof. R. Stencel). It will start april 9th between 7-10pm local time (Denver), which is 01-04 GMT April 10th.” says Sander. “Our goal is to get as many telescopes pointed towards the Moon as possible. I hope that there will be a continuous view of the Moon somewhere from the globe the whole week.”

How can you participate? It’s easy! Just tune into the AstronomyLive Website and follow the instructions. “During the Lunar Week, AstronomyLive will host at least two broadcasts, currently scheduled 15th and 16th of April.” instructs Klieverik. “The first broadcast will take you on a journey across the 85% illuminated lunar surface, on the hunt for the most beautiful craters during this phase, the ´Crater hunt´. The craters at the terminator will receive special attention, the dark side of the moon that changes during the Moon phase. Please know that you will see a LIVE view of the Moon and not some Moon photo. The same accounts for the “Apollo Hop”.

Come one, come all… Lunatics are welcome!

April 7, 2011December 24, 2015 by Nancy Atkinson

Space Telescopes Observe Unprecedented Explosion

mages from Swift's Ultraviolet/Optical (white, purple) and X-ray telescopes (yellow and red) were combined in this view of GRB 110328A. The blast was detected only in X-rays, which were collected over a 3.4-hour period on March 28. Credit: NASA/Swift/Stefan Immler

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From a NASA press release:

NASA’s Swift, Hubble Space Telescope and Chandra X-ray Observatory have teamed up to study one of the most puzzling cosmic blasts yet observed. More than a week later, high-energy radiation continues to brighten and fade from its location.

Astronomers say they have never seen anything this bright, long-lasting and variable before. Usually, gamma-ray bursts mark the destruction of a massive star, but flaring emission from these events never lasts more than a few hours.

Although research is ongoing, astronomers say that the unusual blast likely arose when a star wandered too close to its galaxy’s central black hole. Intense tidal forces tore the star apart, and the infalling gas continues to stream toward the hole. According to this model, the spinning black hole formed an outflowing jet along its rotational axis. A powerful blast of X- and gamma rays is seen if this jet is pointed in our direction.

On March 28, Swift’s Burst Alert Telescope discovered the source in the constellation Draco when it erupted with the first in a series of powerful X-ray blasts. The satellite determined a position for the explosion, now cataloged as gamma-ray burst (GRB) 110328A, and informed astronomers worldwide.

This is a visible-light image of GRB 110328A's host galaxy (arrow) taken on April 4 by the Hubble Space Telescope's Wide Field Camera 3. The galaxy is 3.8 billion light-years away. Credit: NASA/ESA/A. Fruchter (STScI)

As dozens of telescopes turned to study the spot, astronomers quickly noticed that a small, distant galaxy appeared very near the Swift position. A deep image taken by Hubble on April 4 pinpoints the source of the explosion at the center of this galaxy, which lies 3.8 billion light-years away.

That same day, astronomers used NASA’s Chandra X-ray Observatory to make a four-hour-long exposure of the puzzling source. The image, which locates the object 10 times more precisely than Swift can, shows that it lies at the center of the galaxy Hubble imaged.

“We know of objects in our own galaxy that can produce repeated bursts, but they are thousands to millions of times less powerful than the bursts we are seeing now. This is truly extraordinary,” said Andrew Fruchter at the Space Telescope Science Institute in Baltimore.

NASA's Chandra X-ray Observatory completed this four-hour exposure of GRB 110328A on April 4. The center of the X-ray source corresponds to the very center of the host galaxy imaged by Hubble (red cross). Credit: NASA/CXC/ Warwick/A. Levan

“We have been eagerly awaiting the Hubble observation,” said Neil Gehrels, the lead scientist for Swift at NASA’s Goddard Space Flight Center in Greenbelt, Md. “The fact that the explosion occurred in the center of a galaxy tells us it is most likely associated with a massive black hole. This solves a key question about the mysterious event.”

Most galaxies, including our own, contain central black holes with millions of times the sun’s mass; those in the largest galaxies can be a thousand times larger. The disrupted star probably succumbed to a black hole less massive than the Milky Way’s, which has a mass four million times that of our sun

Astronomers previously have detected stars disrupted by supermassive black holes, but none have shown the X-ray brightness and variability seen in GRB 110328A. The source has repeatedly flared. Since April 3, for example, it has brightened by more than five times.

Scientists think that the X-rays may be coming from matter moving near the speed of light in a particle jet that forms as the star’s gas falls toward the black hole.

“The best explanation at the moment is that we happen to be looking down the barrel of this jet,” said Andrew Levan at the University of Warwick in the United Kingdom, who led the Chandra observations. “When we look straight down these jets, a brightness boost lets us view details we might otherwise miss.”

This brightness increase, which is called relativistic beaming, occurs when matter moving close to the speed of light is viewed nearly head on.

Astronomers plan additional Hubble observations to see if the galaxy’s core changes brightness.

For more information see this NASA press release.

April 7, 2011December 24, 2015 by Nancy Atkinson

Particle Physicists See Something Little That Could be Really Big

The dijet invariant mass distribution seen by Fermilab. The blue histogram represents something that is not predicted by the Standard Model. Credit: Fermilab

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Physicists from Fermilab have seen a “bump” in their data that could indicate a brand new particle unlike any ever seen before. If verified, this could re-write particle physics as we know it. “Essentially, the Tevatron has seen evidence for a new particle, 150 times mass of proton, that doesn’t behave like a standard Higgs particle,” said physicist Brian Cox on Twitter. “If this stands up to scrutiny and more data (there is not yet enough data for a “discovery”), then it is RIP Standard Model.”

“It was hard for us to not go crazy when we saw the results,” said Viviana Cavaliere from the University of Illinois (UIUC), one of the 500-member team working with the CDF particle detector at Fermi National Accelerator Laboratory in Batavia, Illinois, speaking on a webcast on April 6. “But for now, we need to stay focused on what we do know.”

The result comes from CDF’s (the Collider Detector at Fermilab) analysis of billions of collisions of protons and antiprotons produced by Fermilab’s Tevatron collider. In high energy collisions, subatomic particles can be detected that otherwise can’t be seen. Physicists try to identify the particles they see by studying the combinations of more-familiar particles into which they decay, while trying to find new particles, such as the theoretical Higgs Boson which is predicted by the Standard Model of particle physics.

The Standard Model contains a description of the elementary particles and forces inside atoms which make up everything around us. The model has been successful at making predictions that have been subsequently verified. There are sixteen named particles in the Standard Model, and the last particles discovered were the W and Z bosons in 1983, the top quark in 1995, and the tauon neutrino in 2000. But most physicists agree the Standard Model is probably not the final word in particle physics.

The researchers at Fermilab were searching for collisions that produced a W boson, which weighs about 87 times as much as a proton, as well as some other particles that disintegrate into two sprays of particles called “jets,” which are produced when a collision scatters out a particle called a quark.

Instead, they saw about 250 events which indicate a new particle weighing about 150 times as much as a proton, the team said at the webcast from Fermilab and in their paper on arXiv.

The researchers estimate the statistical chances of random jets or jet pairs from other sources producing a fake signal that strong at 1 in 1300.

The Standard Model does not predict anything like what was seen in the CDF experiment, and since this particle has not been seen before and appears to have some strange properties, the physicists want to verify and retest before claiming a discovery.

“If it is not a fluctuation, it is a new particle,” Cox said.

The Tevatron accelerator at Fermilab is scheduled to be shut down later this year, due to lack of funding and because of sentiments that it would be redundant to the Large Hadron Collider.

You can see more complete discussions and interpretations of the results at:

Cosmic Variance

Science News

MSNBC