The NASA “Worm” Logo

http://www.dailymail.co.uk/news/article-2973592/Tearful-William-Shatner-pictured-hours-death-brother-Leonard-Nimoy-echoes-Spock-actor-s-final-tweet-telling-fans-Live-Long-Prosper.html

William Shatner pictured hours after the death of Leonard Nimoy @MailOnline

Eta Carinae and Keyhole Nebula (NGC 3324), inside the Carina Nebula (NGC 3372)

ABRACADABRA (A Broadband/Resonant Approach to Cosmic Axion Detection with an Amplifying B-field Ring Apparatus), consists of a series of magnetic coils, wound in the shape of a toroid, or donut, which is then encased in a layer of superconducting metal and kept at temperatures just above absolute zero. The scientists plan to use a highly sensitive magnetometer, placed inside the donut hole, to detect any signs of axions’ influence. MIT physicists are proposing a new experiment to detect a dark matter particle called the axion. If successful, the effort could crack one of the most perplexing unsolved mysteries in particle physics, as well as finally yield a glimpse of dark matter. Axions are hypothetical elementary particles that are thought to be among the lightest particles in the universe — about one-quintillionth the size of a proton. These ultralight particles are virtually invisible, yet if they exist, axions and other yet-unobserved particles may make up 80 percent of the material in the universe, in the form of dark matter. In a paper published online in Physical Review Letters, the MIT team proposes an experiment to detect axions by simulating an extreme astrophysical phenomenon known as a magnetar — a type of neutron star that generates an immensely powerful magnetic field. The physicists reasoned that in the presence of an axion such a huge magnetic field should waver ever so slightly, producing a second, vastly smaller magnetic field as a signature of the axion itself. The team consists of MIT associate professor of physics Jesse Thaler, MIT Pappalardo Fellow Benjamin Safdi, and Yonatan Kahn PhD ’15, now a postdoc at Princeton University. Together, they designed an experiment to recreate the physics of a magnetar in a controlled laboratory environment, using technology borrowed from magnetic resonance imaging (MRI). The core of the experiment, which they’ve named ABRACADABRA (A Broadband/Resonant Approach to Cosmic Axion Detection with an Amplifying B-field Ring Apparatus), consists of a series of magnetic coils, wound in the shape of a toroid, or donut, which is then encased in a layer of superconducting metal and kept in a refrigerator at temperatures just above absolute zero, to minimize external noise. The scientists plan to use a highly sensitive magnetometer, placed inside the donut hole, to detect any signs of axions’ influence. “Axions are very strange, counterintuitive particles,” Thaler says. “They’re extremely light, with feeble interactions, and yet this particle may dominate the matter budget of the universe and be five times more abundant by mass than ordinary matter. So we really had to think hard on whether these particles are in principle detectable using current technology. It’s extremely daunting.” A “tantalizing” particle If they are detected, axions may also explain an outstanding dilemma in particle physics, known as the Strong CP (charge parity) problem: Since the 1970s, scientists have grown increasingly puzzled over what Safdi describes as “the indifference of neutrons to electric fields.” Neutrons are elementary particles that are found in the nucleus of almost every atom in matter, and they do not carry a net charge. “We don’t expect neutrons to accelerate in the presence of an electric field because they don’t carry electric charge, but you might expect them to rotate,” Safdi says. “That’s because we expect them to have an electric dipole moment, where you can think of a neutron having a plus charge on one side and a minus charge on the other. But from our current understanding, this rotation effect does not exist, whereas theory says it should.” Scientists have hypothesized that this bizarre effect may be explained by the axion, which would somehow remove a neutron’s electric dipole moment. If so, the axion would modify electric and magnetic phenomena in a way that could be detectable experimentally. “It’s very tantalizing to say there might be a particle that serves this deep purpose, and even more so if we were to detect the presence of these particles in the form of dark matter,” Thaler says. The hunt is on Currently, Thaler says most axion hunting has been carried out by researchers at the University of Washington who are running the Axion Dark Matter Experiment, or ADMX. The experiment uses a resonant microwave cavity, set within a large superconducting magnet, to detect very weak conversions of axions to microwave photons. The experiment is tuned to look for axions within a specific range of around one quadrillionth the mass of a proton. Thaler and his team realized that they could extend this range, and look for much smaller, lighter particles, on the order of one quintillionth the mass of a proton, by recreating the physics of magnetars, in the lab. “The Strong CP problem is associated with whether a neutron’s spin responds to electric effects, and you can kind of think of a magnetar as one gigantic spin with big magnetic fields,” Thaler explains. “If axions are coming in and changing the properties of nuclear matter to resolve the Strong CP problem, maybe axions can interact with this magnetar and allow you to see it in a new way. So the subtle effects of axions should be amplified.” The team’s prototype design is surprisingly small — “about the palm of your hand,” Safdi says. The researchers, who are theoretical physicists by training, are now working with experimentalists at MIT to build the prototype, which is designed to generate a baseline magnetic field of about 1 tesla, comparable to current MRI machines. If axions are present, that field should waver slightly, producing a very tiny oscillation at a frequency that is directly related to the axion’s mass. Using a high-precision magnetometer, Thaler hopes to pick up that frequency and ultimately use it to identify the axion’s size. “Only recently have there been many good ideas to search for [low-frequency axions],” says Gray Rybka, an assistant professor of physics at the University of Washington and an ADMX researcher, who was not involved in the research. “The experiment proposed here builds on previous ideas and, if the authors are correct, may be the most practical experimental configuration that can explore some of the plausible lower-frequency axion regimes.” “We have an instrument that’s sensitive to many wavelengths, and we can tickle it with an axion of one particular wavelength, and ABRACADABRA will resonate,” Thaler says. “And we will be going into uncharted territory, where we could possibly see dark matter from this prototype. That would be amazing.” This research was supported, in part, by the U.S. Department of Energy and the Alfred P. Sloan Foundation. 

For more on the Fermi Paradox and why alien life hasn’t found us yet. (Infographic via futurism)

Is Proxima b another Earth? It’s difficult to answer because no one has actually “seen” this distant planet which orbits the red dwarf star Proxima Centauri right in theGoldilocks Zone. Scientists have merely concluded that Proxima b (which is about 4.2 light years away from Earth) is right where it should be, by observing the regular, subtle changes in Proxima Centauri’s color. Proxima b is tidally locked to its star — which means one side of it is always facing Proxima Centauri, and the other side is perpetually dark. With just an 11.2-year revolution, it lies very close to its star, although red-dwarf stars are not as hot as yellow-dwarves (like our Sun).  There is a possibility that water exists on Proxima b, and that it has an atmosphere protecting it from extreme heat, and scattering heat even to its dark side.  How can we be sure? Harvard’s Avi Loeb and astronomer Laura Kreidberg propose that we use NASA’s James Webb Space Telescope (JWST). UNCERTAINTIES The long-delayed JWST is set to launch by 2018 (originally 2011). Loeb explains that if a rocky planet, like Proxima b, has an atmosphere, it would absorb light from its star and re-emit it as infrared light. Incidentally, the JWST is specifically designed to observe infrared light. The JWST can take photos of infrared light on the surface Proxima b, looking for patterns that would confirm whether or not this exoplanet has water or is covered by an atmosphere. Things aren’t so simple, however. The proposed method may be doable. But there are other factors that have to be considered. For instance, the existence of an atmosphere may not guarantee life, says astrophysicist Ed Turner of Princeton University. Proxima b may be like Venus, with an atmosphere 90 times thicker than ours, and extreme heat. Still, Loeb’s and Kriedberg’s plan is the only option we have for a glimmer of an answer about this “Earth next-door”. References: Business Insider, Scientific American

There are some that fly an airplane, and there are those who become one with the air and machine.  Sad news today.  Bob Hoover passed away at the age of 94.  A stick and rudder pilot for the ages.  I met and got an autograph back in the late 1990s.  A class act all the way.  Mr. Hoover brought flying to an artistic level.  RIP Mr. Hoover, you took to the skies, dazzling and inspiring so many.  We mourn his loss, and celebrate a life. 

Robert A. “Bob” Hoover (January 24, 1922 - October 25, 2016)

http://www.flyingmag.com/aviation-legend-bob-hoover-dies-at-94

RIP

While flying over Boston, Leonard Nimoy’s birthplace, NASA Astronaut Terry Virts pays tribute to the Star Trek star http://nbcnews.to/1AUElvf

NASA tested new “eyes” for its next Mars rover mission on a rocket built by Masten Space Systems in Mojave, California, thanks in part to NASA’s Flight Opportunities Program, or FOP.

The agency’s Jet Propulsion Laboratory in Pasadena, California, is leading development of the Mars 2020 rover and its Lander Vision System, or LVS. In 2014, the prototype vision system launched 1,066 feet (325 meters) into the air aboard Masten’s rocket-powered “Xombie” test platform and helped guide the rocket to a precise landing at a predesignated target. LVS flew as part of a larger system of experimental landing technologies called the Autonomous Descent and Ascent Powered-flight Testbed, or ADAPT.

LVS, a camera-based navigation system, photographs the terrain beneath a descending spacecraft and matches it with onboard maps allowing the craft to detect its location relative to landing hazards, such as boulders and outcroppings.

The system can then direct the craft toward a safe landing at its primary target site or divert touchdown toward better terrain if there are hazards in the approaching target area. Image matching is aided by an inertial measurement unit that monitors orientation.

The Flight Opportunities Program funded the Masten flight tests under the Space Technology Mission Directorate. The program obtains commercial suborbital space launch services to pursue science, technology and engineering to mature technology relevant to NASA’s pursuit of space exploration. The program nurtures the emerging suborbital space industry and allows NASA to focus on deep space.

Andrew Johnson, principal investigator in development of the Lander Vision System development, said the tests built confidence that the vision system will enable Mars 2020 to land safely.

“By providing funding for flight tests, FOP motivated us to build guidance, navigation and control payloads for testing on Xombie,” Johnson said. “In the end we showed a closed loop pinpoint landing demo that eliminated any technical concerns with flying the Lander Vision System on Mars 2020.”

According to “Lander Vision System for Safe and Precise Entry Descent and Landing,” a 2012 abstract co-authored by Johnson for a Mars exploration workshop, LVS enables a broad range of potential landing sites for Mars missions.

Typically, Mars landers have lacked the ability to analyze and react to hazards, the abstract says. To avoid hazards, mission planners selected wide-open landing sites with mostly flat terrain. As a result, landers and rovers were limited to areas with relatively limited geological features, and were unable to access many sites of high scientific interest with more complex and hazardous surface morphology. LVS will enable safe landing at these scientifically compelling Mars landing sites.

An LVS-equipped mission allows for opportunities to land within more challenging environments and pursue new discoveries about Mars. With LVS baselined for inclusion on Mars 2020, the researchers are now focused on building the flight system ahead of its eventual role on the Red Planet.

To learn more about NASA’s flight opportunities program, visit:

https://flightopportunities.nasa.gov/

To read more about NASA’s Mars 2020 rover, visit:

http://mars.nasa.gov/mars2020/

The arrangement of the spiral arms in the galaxy Messier 63, seen here in an image from the NASA/ESA Hubble Space Telescope, recall the pattern at the center of a sunflower. So the nickname for this cosmic object -- the Sunflower Galaxy -- is no coincidence. Discovered by Pierre Mechain in 1779, the galaxy later made it as the 63rd entry into fellow French astronomer Charles Messier's famous catalogue, published in 1781. The two astronomers spotted the Sunflower Galaxy's glow in the small, northern constellation Canes Venatici (the Hunting Dogs). We now know this galaxy is about 27 million light-years away and belongs to the M51 Group -- a group of galaxies, named after its brightest member, Messier 51, another spiral-shaped galaxy dubbed the Whirlpool Galaxy. Galactic arms, sunflowers and whirlpools are only a few examples of nature's apparent preference for spirals. For galaxies like Messier 63 the winding arms shine bright because of the presence of recently formed, blue-white giant stars and clusters, readily seen in this Hubble image.  Image credit: ESA/Hubble & NASA Text credit: European Space Agency Hubble Space Telescope

InSight Mission to Mars

Our InSight mission will place a fixed science outpost on Mars to study its deep interior. Findings and research from this project will address one of the most fundamental questions we have about planetary and solar system science – How in the world did these rocky planets form?

By investigating the interior structure and processes of Mars, the InSight mission will gain a better understanding of the evolutionary formation of planets, including Earth.

InSight will record Mars’ vital signs to learn more about the planet, including:

Seismic Activity:

A seismometer will be used to record the seismic activity on Mars. This will give us information on the crust, mantel and core; and the relationship between them.

Temperature:

A heat flow probe will be used to take Mars’ temperature and determine the change over the course of a full Martian year.

Reflexes:

By looking at how the rotation of Mars wobbles, we will better understand what the core size may be and its composition.

Launch for the InSight mission is scheduled for March 2016, and even though you can’t physically travel with the lander, you can send your name to the Red Planet onboard. Make sure to submit your name before Sept. 8!

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