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inhandnetworks-blog · 5 years
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Curiosity Team Selects Second Drilling att certified   Location on Mars
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This map shows the location of “Cumberland,” the second rock-drilling target for NASA’s Mars rover Curiosity, in relation to the rover’s first drilling target, “John Klein,” within the southwestern lobe of a shallow depression called “Yellowknife Bay.” Cumberland, like John Klein, is a patch of flat-lying bedrock with pale veins and bumpy surface texture. The bumpiness is due to erosion-resistant nodules within the rock, which have been identified as concretions resulting from the action of mineral-laden water. North is to the top of the map. The scale bar is 50 meters (164 feet). Cumberland lies about nine feet (2.75 meters) west of John Klein. The base map is part of an image from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA’s Mars Reconnaissance Orbiter. The mapped area is within Gale Crater and north of the mountain called Mount Sharp in the middle of the crater. Credit: NASA/JPL-Caltech/Univ. of Arizona
Scientists have chosen the second drilling site for the Curiosity rover on Mars.
Pasadena, California — The team operating NASA’s Curiosity Mars rover has selected a second target rock for drilling and sampling. The rover will set course to the drilling location in coming days.
This second drilling target, called “Cumberland,” lies about nine feet (2.75 meters) west of the rock where Curiosity’s drill first touched Martian stone in February. Curiosity took the first rock sample ever collected on Mars from that rock, called “John Klein.” The rover found evidence of an ancient environment favorable for microbial life. Both rocks are flat, with pale veins and a bumpy surface. They are embedded in a layer of rock on the floor of a shallow depression called “Yellowknife Bay.”
This second drilling is intended to confirm results from the first drilling, which indicated the chemistry of the first powdered sample from John Klein was much less oxidizing than that of a soil sample the rover scooped up before it began drilling.
“We know there is some cross-contamination from the previous sample each time,” said Dawn Sumner, a long-term planner for Curiosity’s science team at the University of California at Davis. “For the Cumberland sample, we expect to have most of that cross-contamination come from a similar rock, ra Vending Telemetry  ther than from very different soil.”
Although Cumberland and John Klein are very similar, Cumberland appears to have more of the erosion-resistant granules that cause the surface bumps. The bumps are concretions, or clumps of minerals, which formed when water soaked the rock long ago. Analysis of a sample containing m DIN-Rail router  ore material from these concretions could provide information about the variability within the rock layer that includes both John Klein and Cumberland.
Mission engineers at NASA’s Jet Propulsion Laboratory in Pasadena, California, recently finished upgrading Curiosity’s operating software following a four-week break. The rover continued monitoring the Martian atmosphere during the break, but the team did not send any new commands because Mars and the sun were positioned in such a way the sun could have blocked or corrupted commands sent from Earth.
Curiosity is about nine months into a two-year prime mission since landing inside Gale Crater on Mars in August 2012. After the second rock drilling in Yellowknife Bay and a few ot ethernet switch  her investigations nearby, the rover will drive toward the base of Mount Sharp, a 3-mile-tall (5-kilometers) layered mountain inside the crater.
JPL, a division of the California Institute of Technology, Pasadena, manages the Mars Science Laboratory Project, of which Curiosity is the centerpiece, for NASA’s Science Mission Directorate in Washington.
For more information about the mission, visit: msl , msl and msl . To follow the mission on Facebook and Twitter visit: marscuriosity and marscuriosity.
Image: NASA/JPL-Caltech/Univ. of Arizona
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inhandnetworks-blog · 5 years
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Curiosity Rover Provides First Confirmation of a Mineral Mapp industrial cellular modem3g modem  ed from Orbit
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This image shows the first holes drilled by NASA’s Mars rover Curiosity at Mount Sharp. The loose material near the drill holes is drill tailings and an accumulation of dust that slid down the rock during drilling. Image Credit: NASA/JPL-Caltech/MSSS
A sample of powdered rock extracted by the Curiosity rover’s drill from the “Confidence Hills” target has provided NASA scientists with the first confirmation of a mineral mapped from orbit.
“This connects us with the mineral identifications from orbit, which can now help guide our investigations as we climb the slope and test hypotheses derived from the orbital mapping,” said Curiosity Project Scientist John Grotzinger, of the California Institute of Technology in Pasadena.
Curiosity collected the powder by drilling into a rock out iiot  crop at the base of Mount Sharp in late September. The robotic arm delivered a pinch of the sample to the Chemistry and Mineralogy (CheMin) instrument inside the rover. This sample, from a target called “Confidence Hills” within the “Pahrump Hills” outcrop, contained much more hematite than any rock or soil sample previously analyzed by CheMin during the two-year-old mission. Hematite is an iron-oxide mineral that gives clues about ancient environmental conditions from when it formed.
In observations reported in 2010, before selection of Curiosity’s landing site, a mineral-mapping instrument on NASA’s Mars Reconnaissance Orbiter provided evidence of hematite in the geological unit that includes the Pahrump Hills outcrop. The landing site is inside Gale Crater, an impact basin about 96 miles (154 kilometers) in diameter with the layered Mount Sharp rising about three miles (five kilometers) high in the center.
“We’ve reached the part of the crater where we have the mineralogical information that was important in selection of Gale Crater as the landing site,” said Ralph Milliken of Brown University, Providence, Rhode Island. He is a member of Curiosity’s science team and was lead author of that 2010 report in Geophysical Research Letters identifying minerals based on observations of lower Mount Sharp by the orbiter’s Compact Reconnaissance Imaging Spectrometer for Mars (CRISM). “We’re Industrial IoT Router/Gateway   now on a path where the orbital data can help us predict what minerals we’ll find and make good choices about where to drill. Analyses like these will help us place rover-scale observations into the broader geologic history of Gale that we see from orbital data.”
Much of Curiosity’s first year on Mars was spent investigating outcrops in a low area of Gale Crater called “Yellowknife Bay,” near the spot where the rover landed. The rover found an ancient lakebed. Rocks there held evidence of wet environmental conditions billions of years ago that offered ingredients and an energy source favorable for microbial life, if Mars ever had microbes. Clay minerals of interest in those rocks at Yellowknife Bay had not been detected from orbit, possibly due to dust coatings that interfere with CRISM’s view of them.
The rover spent much of the mission’s second year driving from Yellowknife Bay to the base of Mount Sharp. The hematite found in the first sample from the mountain tells about environmental conditions different from the conditions recorded in the rocks of Yellowknife Bay. The rock material interacted with water and atmosphere to become more oxidized.
The rocks analyzed earlier also contain iron-oxide minerals, mostly magnetite. One way to form hematite is to put magnetite in oxidizing conditions. The latest sample has about eight percent hematite and four percent magnetite. The drilled rocks at Yellowknife Bay and on the way to Mount Sharp contain at most about one percent hematite and much higher amounts of magnetite.
“There’s more oxidation involved in the new sample,” said CheMin Deputy Principal Investigator David Vaniman of the Planetary Science Institute in Tucson, Arizona.
The sample is only partially oxidized, and preservation of magnetite and olivine indicates a gradient of oxidation levels. That gradient could have provided a chemical energy source for microbes.
The Pahrump HIlls outcrop includes multiple layers uphill from its lowest layer, where the Confidence Hills sample was drilled. The layers vary in texture and may also vary in concentrations of hematite and other minerals. The rover team is now using Curiosity to survey the outcrop and assess possible targets for close inspection and drilling.
The mission may spend weeks to months at Pahrump Hills before proceeding farther up the st applications  ack of geological layers forming Mount Sharp. Those higher layers include an erosion-resistant band of rock higher on Mount Sharp with such a strong orbital signature of hematite, it is called “Hematite Ridge.” The target drilled at Pahrump Hills is much softer and more deeply eroded than Hematite Ridge.
Another NASA Mars rover, Opportunity, made a key discovery of hematite-rich spherules on a different part of Mars in 2004. That finding was important as evidence of a water-soaked history that produced those mineral concretions. The form of hematite at Pahrump Hills is different and is most important as a clue about oxidation conditions. Plenty of other evidence in Gale Crater has testified to the ancient presence of water.
NASA’s Jet Propulsion Laboratory, a division of Caltech in Pasadena, manages the Mars Reconnaissance Orbiter and Mars Science Laboratory projects for NASA’s Science Mission Directorate in Washington, and built the Curiosity rover. NASA’s Ames Research Center, Moffett Field, California, developed CheMin and manages instrument operations. The Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland, developed and operates CRISM.
Image: NASA/JPL-Caltech/MSSS
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inhandnetworks-blog · 5 years
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Curiosity Sends Back Radioed Words and New Telephoto industrial wireless router   View of Mars
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A chapter of the layered geological history of Mars is laid bare in this postcard from NASA’s Curiosity rover. The image shows the base of Mount Sharp, the rover’s eventual science destination. Image credit: NASA/JPL-Caltech/MSSS
Using the 100-millimeter telephoto lens and the 34-millimeter wide angle lens of the Mast Camera instrument, Curiosity beamed back a new image of the base of Mount Sharp and also sent back the first planet to planet radioed words.
Pasadena, California — NASA’s Mars Curiosity has debuted the first recorded human voice that traveled from Earth to another planet and back.
In spoken words radioed to the rover on Mars and back to NASA’s Deep Space Network (DSN) on Earth, NASA Administrator Charles Bolden noted the difficulty of landing a rover on Mars, congratulated NASA employees and the agency’s commercial and government partners on the successful landing of Curiosity earlier this month, and said curiosity is what drives humans to explore.
“The knowledge we hope to gain from our observation and analysis of Gale Crater will tell us much about the possibility of life on Mars as well as the past and future possibilities for our own planet. Curiosity will bring benefits to Earth and inspire a new generation of scientists and explorers, as it prepares the way for a human mission in the not too distant future,” Bolden said in the recorded message.
The voice playback was released along with new telephoto camera views of the varied Martian landscape during a news conference today at NASA’s Jet Propulsion Laboratory, Pasadena, California.
“With this voice, another small step is taken in extending human presence beyond Earth, and the experience of exploring remote worlds is brought a little closer to us all,” said Dave Lavery, NASA Curiosity program executive. “As Curiosity continues its mission, we hope these words will be an inspiration to someone alive today who will become the first to stand upon the surface of Mars. And like the great Neil Armstrong, they will speak aloud of that next giant leap in human exploration.”
The telephoto images beamed back to Earth show a scene of eroded knobs and gulches on a mountainside, with geological layering clearly exposed. The new views were taken by the 100-millimeter telephoto lens and the 34-milllimeter wide angle lens of the Mast Camera (Mastcam) instrument. Mastcam has photographed the lower slope of the nearby mountain called Mount Sharp.
“This is an area on Mount Sharp where Curiosity will go,” said Mastcam principal investigator Michael Malin, of Malin Space Science Systems in San Diego. “Those layers are our ultimate objective. The dark dune field is between us and those layers. In front of the dark sand you see redder sand, with a different composition suggested by its different color. The rocks in the foreground show diversity — some rounded, some angular, with different histories. This is a very rich geological site to look at and eventually to drive through.”
A drive early Monday placed Curiosity directly over a patch where one of the spacecraft’s landing engines scoured away a few inches of gravelly soil and exposed underlying rock. Researchers plan to use a neutron-shooting instrument on the rover to check for water molecules bound into minerals at this partially excavated target.
During the news conference, the rover team reported the results of a Prognostics and Health Management   test on Curio vending vms sity’s Sample Analysis at Mars (SAM) instrument, which can measure the composition of samples of atmosphere, powdered rock or soil. The amount of air from Earth’s atmosphere remaining in the instrument after Curiosity’s launch was more than expected, so a difference in pressure on either side of tiny pumps led SAM operators to stop pumping out the remaining Earth air as a precaution. The pumps subsequently worked, and a chemical analysis was completed on a sample of  Vending Telemetry  Earth air.
“As a test of the instrument, the results are beautiful confirmation of the sensitivities for identifying the gases present,” said SAM principal investigator Paul Mahaffy of NASA’s Goddard Space Flight Center in Greenbelt, Md. “We’re happy with this test and we’re looking forward to the next run in a few days when we can get Mars data.”
Curiosity already is returning more data from the Martian surface than have all of NASA’s earlier rovers combined.
“We have an international network of telecommunications relay orbiters bringing data back from Curiosity,” said JPL’s Chad Edwards, chief telecommunications engineer for NASA’s Mars Exploration Program. “Curiosity is boosting its data return by using a new capability for adjusting its transmission rate.”
Curiosity is 3 weeks into a two-year prime mission on Mars. It will use 10 science instruments to assess whether the selected study area ever has offered environmental conditions favorable for microbial life.
JPL manages the mission for NASA’s Science Mission Directorate in Washington. The rover was designed, developed and assembled at JPL. NASA’s DSN is an international network of antennas that supports interplanetary spacecraft missions and radio and radar astronomy observations for the exploration of the solar system and the universe. The network also supports selected Earth-orbiting missions.
Image: NASA/JPL-Caltech/MSSS
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inhandnetworks-blog · 5 years
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Curiosity Rover Samples Active Linear Dune on t industrial 4G/3G router  he Surface of Mars
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This view from the Mast Camera (Mastcam) on NASA’s Curiosity Mars rover shows two scales of ripples, plus other textures, in an area where the mission examined a linear-shaped dune in the Bagnold dune field on lower Mount Sharp in March and April 2017.
From February to April 2017, NASA’s Curiosity Mars Rover examined linear sand dunes to compare with what it found in 2015 and 2016 during an investigation of crescent-shaped dunes. This two-phase campaign is the first close-up study of active dunes anywhere other than Earth.
As it drives uphill from a band of rippled sand dunes, Curiosity is toting a fistful of dark sand for onboard analysis that will complete the rover’s investigation of those dunes.
Among the questions this Martian dune campaign is addressing is how winds shape dunes that are relatively close together, on the same side of the same mountain, into different patterns. Others include whether Martian winds sort grains of sand in ways that affect the distribution of mineral compositions, which would have implications for studies of Martian sandstones.
“At these linear dunes, the wind regime is more complicated than at the crescent dunes we studied earlier,” said Mathieu Lapotre of Caltech, in Pasadena, California, who helped lead the Curiosity science team’s planning for the duneGrid Analytics campaign. “There seems to be more contribution from the wind coming down the slope of the mountain here compared with the crescent dunes farther north.”
This 360-degree panorama was acquired by the Mast Camera (Mastcam) on NASA’s Curiosity rover looking out over part of an area called Bagnold Dunes, which stretch for miles on Mars. This location, called “Ogunquit Beach,” is on the northwestern flank of lower Mount Sharp. Points of interest include the dune’s ripples, and bedrock made from sediments deposited in lakes billions of years ago.
The linear dunes lie uphill and about a mile (about 1.6 kilometers) south from the crescent dunes. Both study locations are part of a dark-sand swath called the Bagnold Dunes, which stretches several miles in length. This dune field lines the northwestern flank of  Grid Analytics System  Mount Sharp, the layered mountain that Curiosity is climbing.
“There was another key difference between the first and second phases of our dune campaign, besides the shape of the dunes,” Lapotre said. “We were at the crescent dunes during the low-wind season of the Martian year and at the linear dunes during the high-wind season. We got to see a lot more movement of grains and ripples at the linear dunes.”
To assess wind strength and direction, the rover team now uses change-detection pairs of images taken at different times to check for movement of sand grains. The wind-sensing capability of the Curiosity’s Rover Environmental Monitoring Station (REMS) is no longer available, though that instrument still returns other Mars-weather data daily, such as temperatures, humidity and pressure. Two of the six wind sensors on the rover’s mast were found to be inoperable upon landing on Mars in 2012. The remainder provided wind information throughout the rover’s prime mission and first two-year extended mission.
A sample of sand that Curiosity scooped up from a linear dune is in the sample-handling device at the end of the rover’s arm. One portion has been analyzed in the Sample Analysis at Mars (SAM) instrument inside the rover. The science team plans to deliver additional sample portions to SAM and to the rover’s Chemistry and Mineralogy (CheMin) instrument.
This 360-degree scene from the Mastcam on NASA’s Curiosity Mars rover includes part of a linear-shaped dune the rover examined in early 2017 for comparison with what it found previously at crescent-shaped dunes. The view shows the dark, rippled surface of the active dune, near sedimentary bedrock.
One factor in choosing to drive farther uphill before finishing analysis of the scooped sand is the sta industrial router  tus of Curiosity’s rock-sampling drill, which has not been used on a rock since a problem with the drill feed mechanism appeared five months ago. Engineers are assessing how the use of vibration to deliver samples may affect the drill feed mechanism, which is used to move the drill bit forward and backwards. In addition, high winds at the linear-dunes location were complicating the process of pouring sample material into the entry ports for the laboratory instruments.
“A balky brake appears to be affecting drill feed mechanism performance,” said Curiosity Deputy Project Manager Steven Lee, of NASA’s Jet Propulsion Laboratory, Pasadena, California. “In some cases, vibration has been observed to change feed effectiveness, so we’re proceeding cautiously until we better understand the behavior. In the meantime, the engineering team is developing several methods to improve feed reliability.”
Curiosity landed near Mount Sharp in August 2012. It reached the base of the mountain in 2014 after successfully finding evidence on the surrounding plains that ancient Martian lakes offered conditions that would have been favorable for microbes if Mars has ever hosted life. Rock layers forming the base of Mount Sharp accumulated as sediment within ancient lakes billions of years ago.
On Mount Sharp, Curiosity is investigating how and when the ancient habitable conditions known from the mission’s earlier findings evolved into drier conditions that were less favorable for life.
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inhandnetworks-blog · 5 years
Text
Curiosity Technology Adapted to Detect Gas Leaks from  wordpress plugins  Pipelines
www.inhandnetworks.com
This artist’s concept features NASA’s Mars Science Laboratory Curtouch screen for vending machineiosity rover, a mobile robot for investigating Mars’ past or present ability to sustain microbial life. Image Credit: NASA/JPL-Caltech
Technology adapted from NASA’s Mars rover program is being used to develop a hand-held device that will help find and fix natural gas leaks from gas pipelines, with the goal of reducing emissions of greenhouse gases.
In collaboration with NASA’s Jet Propulsion Laboratory in Pasadena, California, Pacific Gas and Electric Company (PG&E) announced that it is testing state-of-the-art technology adapted from NASA’s Mars rover program. Originally designed to find methane on the Red Planet, this laser-based technology is lightweight and has superior sensitivity to methane, a major component of natural gas. The technology applied back on Earth helps guide PG&E crews using a tablet interface to identify possible leak locations, fast-tracking their ability to repair gas leaks.
“Our pursuit of this technology is evidence of our commitment to our mission of becoming the safest, most reliable utility in the country. We are using out-of-this-woindustrial l2tp cellular routerrld technology to find and fix even the smallest leaks in our system. By investing in innovation today, we are helping build a positive energy future,” said Nick Stavropoulos, PG&E’s executive vice president of gas operations.
On September 29, a new law, SB 1371, required the California Public Utilities Commission (CPUC) to open a proceeding to adopt rules and procedures that minimize natural gas leaks from gas pipelines, with the goal of reducing emissions of greenhouse gases, such as methane.
The hand-held device is the latest piece of advanced leak detection technology being embraced by the utility and is expected to be available for use in 2015. The development of this to IoT Remote Monitoring  ol is part of a collaborative research effort at Pipeline Research Council International (PRCI).
“It’s rewarding to be involved in projects that translate JPL technological capabilities to meet industry needs, technologies which ultimately should help enhance safety and reliability. PG&E’s role as a collaborator with JPL on our PRCI-funded effort is essential to efficiently adapt the JPL methane sensor into a field-ready hand-held leak detection system,” said Andrew Aubrey, JPL technologist.
Pacific Gas and Electric Company, a subsidiary of PG&E Corporation (NYSE:PCG), is one of the largest combined natural gas and electric utilities in the United States. Based in San Francisco, with more than 20,000 employees, the company delivers some of the nation’s cleanest energy to nearly 16 million people in Northern and Central California.
Image: NASA/JPL-Caltech
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inhandnetworks-blog · 5 years
Text
Controlled Trial Sh Remote Automation  ows Cannabis Reduces Some Symptoms of MS
www.inhandnetworks.com
A newly published research study shows the benefits of smoking cannabis for spasticity in multiple sclerosis. Using 30 adult patients with multiple sclerosis, the researchers found that smoked cannabis was superior to a placebo in reducing symptoms and pain in patients with treatment-resistant spasticity, or excessive muscle contractions.
A clinical study of 30 adult patients with multiple sclerosis (MS) at the University of California, San Diego School of Medicine has shown that smoked cannabis may be an effective treatment for spasticity – a common and disabling symptom of this neurological disease.
The placebo-controlled trial al wireless m2m  so resulted in reduced perception of pain, although participants also reported short-term, adverse cognitive effects and increased fatigue. The study will be published in the Canadian Medical Association Journal on May 14.
Principal investigator Jody Corey-Bloom, MD, PhD, professor of neurosciences and director of the Multiple Sclerosis Center at UC San Diego, and colleagues randomly assigned participants to either the intervention group (which smoked cannabis once daily for three days) or the control group (which smoked identical placebo cigarettes, also once a day for three days). After an 11-day interval, the participants crossed over to the other group.
“We found that smoked cannabis was superior to placebo in reducing symptoms and pain in patients with treatment-resistant spasticity, or excessive muscle contractions,” said Corey-Bloom.
Earlier reports suggested that the active compounds of medical marijuana were potentially effective in treating neurologic conditions, but most studies focused on orally administered cannabinoids. There were also anecdotal reports of MS patients that endorsed smoking marijuana to relieve symptoms of spasticity.
However, this trial used a more objective measurement, a modified Ashworth scale which graded the intensity of muscle tone by measuring such things as resistance in range of motion and rigidity. The secondary outcome, pain, was measured using a visual analogue scale. The researchers also looked at physical performance (using a timed walk) and cognitive function and – at the end of each visit – asked patients to assess their feeling of “highness.”
Although generally well tolerated, smoking cannabis did have mild effects on attention and concentration. The researchers noted that larger, long-terms studies are needed to confirm their findings and determine whether lower doses can result in beneficial effects with less cognitive impact.
The current study is the fifth clinical test of the possible efficacy of cannabis for clinical use reported by the University of California Center for Medicinal Cannabis Research (CMCR). Four other human studies on control of cellular router  neuropathic pain also reported positive results.
“T vending PC he study by Corey Bloom and her colleagues adds to a growing body of evidence that cannabis has therapeutic value for selected indications, and may be an adjunct or alternative for patients whose spasticity or pain is not optimally managed,” said Igor Grant, MD, director of the CMCR, which provided funding for the study.
Additional contributors include Tanya Wolfson, Anthony Gamst, PhD, Shelia Jin, MD, MPH, Thomas D. Marcotte, PhD, Heather Bentley and Ben Gouaux, all from UC San Diego School of Medicine.
Image: Cannabis from Shutterstock
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inhandnetworks-blog · 5 years
Text
Conformational Changes of EF-G on the Ribosome During tRNA  magento themes  Translocation
www.inhandnetworks.com
New research from Yale University provides insights into the conformational space that EF-G samples on the ribosome and reveals that tRNA translocation on the ribosome is facilitated by a structural transition of EF-G from a compact to an elongated conformation, which can be prevented by the antibiotic dityromycin.
The ribosome is the protein-making “factory” within cells responsible for knitting together amino acids into polypeptide chains that form proteins.
This process requires numerous factors. One of the most crucial is elongation factor G (EF-G), shown in color in the accompanying illustration of the ribosome. EF-G is responsible for movement within the ribosome of messenger RNA (mRNA) and transfer RNA (tRNA), the molecules that carry out instructions contained in DNA. But ho vending retrofit w does this happen?
In this simplified illustration, Yale research scientist Jcredit card vending machineinzhong Lin and colleagues in the lab of Nobe Remote PLC programming  l laureate Thomas Steitz in the Department of Molecular Biophysics and Biochemistry show that portions of EF-G (in green, yellow and red) function something like a motor and force tRNA to move forward after the addition of each amino acid, a necessary step to add to the developing polypeptide chain.
Publication: Jinzhong Lin, et al., “Conformational Changes of Elongation Factor G on the Ribosome during tRNA Translocation,” Cell, Volume 160, Issues 1–2, 15 January 2015, Pages 219–227; doi:10.1016/j.cell.2014.11.049
Image: Yale University
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inhandnetworks-blog · 5 years
Text
Consortium to Focus on Developin fcc certified  g a New Architecture for the Internet
www.inhandnetworks.com
NDN leverages evidence about what has worked on the Internet over the past 30-plus years.
UCLA will host a consortium of universities and leading technology companies on September 4 and 5 to promote the development and adoption of Named Data Networking (NDN) – an emerging Internet architecture that promises to increase network security, accommodate growing bandwidth requirements and simplify the creation of increasingly sophisticated applications.
The consortium is being organized by a team of NDN researchers at the UCLA Henry Samueli School of Engineering and Applied Science. Other founding academic members of the NDN project are UC San Diego, Colorado State University, the University of Arizona, the University of Illinois Urbana–Ch Dual SIM M2M router ampaign, the University of Memphis, the University of Michigan and Washington University in St. Louis.
The first NDN community meeting will be held September 4 and 5 at UCLA’s School of Theater, Film and Television, which has played a key role in envisioning the future of human communication over NDN since the project’s origins in 2010.
Among the industry partners planning to participate are Verisign, Cisco Systems and Panasonic. They will be joined by representatives from Anyang University (Korea), Tongji University and Tsinghua University (China), the University of Basel (Switzerland) and Waseda University (Japan).
“Collaboration with industry is an important step toward bringing Future Internet Architectures out of the laboratory and into the real world,” said Darleen Fisher, the NSF program officer who oversees the Future Internet Architectures program supporting NDN.
The NDN team’s goal is to build a replacement for Transmission Control Protocol/Internet Protocol, or TCP/IP, the current underlying approach to all communication over the Internet. The consortium aims to generate a vibrant ecosystem of research and experimentation around NDN; preserve and promote the Industrial 3G Router   openness of the core NDN architecture; and organize community meetings, workshops and other activities.
“NDN has built significant momentum through a commitment to an open approach that aims to limit proprietary intellectual property claims on core elements of the architecture,” said Lixia Zhang, UCLA’s Jonathan B. Postel Chair in Computer Science and a co-leader of the project.
“This has spurred substantial interest from both academia and industry. Our goal with the consortium is to accelerate the development of architecture that will lift the Internet from its origins as a messaging and information tool and better prepare it for the wide-ranging uses it has today and will have tomorrow,” Zhang said.
NDN leverages empirical evidence about what has worked on the Internet and what hasn’t, adapting to changes in usage over the past 30-plus years and  da monitoring  simplifying the foundation for development of mobile platforms, smart cars and the Internet of Things — in which objects and devices are equipped with embedded software and are able to communicate with wireless digital networks.
Since 2010, the National Science Foundation’s Future Internet Architectures program has provided more than $13.5 million to the NDN project led by UCLA, including a grant of $5 million that was announced in May.
“Cisco Systems is enthusiastic about the formation of the NDN community,” said David Oran, a Cisco Fellow and a pioneer in Internet Protocol technologies. “It will help evolve NDN by establishing a multifaceted community of academics, industry and users. We expect this consortium to be a major help in advancing the design, producing open-source software, and fostering standardization and adoption of the technology.”
The NDN project is co-led by Zhang and Van Jacobson, a UCLA adjunct professor and member of the Internet Hall of Fame. UCLA became the birthplace of the Internet in 1969, when a message from the lab of UCLA computer science professor Leonard Kleinrock was sent to the Stanford Research Institute — the first-ever message transmitted over the network that later became known as the Internet.
Image: UCLA newsroom
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inhandnetworks-blog · 5 years
Text
Cont remote access IoTrolled Synthesis of Single-Walled Carbon Nanotubes
www.inhandnetworks.com
On a Platinum surface, the planar hydrocarbon precursor folds into an end cap, that in turn acts as seed for the growth of a well-defined (6,6) carbon nanotube. Credit: Empa / Juan Ramon Sanchez Valencia
A new study details how researchers from the Max Planck Institute and EMPA succeeded in “growing” single-wall carbon nanotubes with a single predefined structure for the first time.
For the first time, researchers at EMPA and the Max Planck Institute for Solid State Research have succeeded in “growing” single-wall carbon nanotubes (CNT) with a single predefined structure – and hence with identical electronic properties. And here is how they pulled it off: the CNTs “a remote maintenance  ssembled themselves”, as it were, out of tailor-made organic precursor molecules on a platinum surface, as reported by the researchers in the latest issue of the journal “Nature”. In future, CNTs of this kind may be used in ultra-sensitive light detectors and ultra-small transistors.
For 20 years, carbon nanotubes (CNTs) have been the subject of intensive fundamental as well as applied research. With their extraordinary mechanical, thermal and el Remote Machine Monitoring & Maintenance System  ectronic properties, these tiny tubes with their graphitic honeycomb lattice have become the paragon of nanomaterials. They could help to create next-generation electronic and electro-optical components that are smaller than ever before, and thus to achieve even faster switching times.
As uniform as possible With a diameter of roughly one nanometer, single-wall CNTs (or SWCNTs) need to be considered as quantum structures; the slightest structural changes, such as differences in diameter or in the alignment of the atomic lattice, may result in dramatic changes to the electronic properties: one SWCNT may be metallic, whilst another one with a slightly different structure is a semiconductor. Hence, there is a great deal of interest in reliable methods of making SWCNTs as structurally uniform as possible. In fact, corresponding synthesis concepts were formulated about 15 years ago. However, it is only now that surface physicists at Empa and chemists at the Max Planck Institute have successfully implemented one of these ideas in the laboratory. In the latest issue of “Nature”, they describe how, for the first time, it has been possible to “grow” structurally homogenous SWCNTs and, hence, managed to clearly define their electronic properties.
For some time, the Empa team working under the direction of Roman Fasel, Head of the “[email protected]” Laboratory at Empa and Professor of Chemistry and Biochemistry at the University of Berne, has been investigating the subject of “how molecules can be transformed or joined together to form complex nanostructures on a surface”. For instance, by means of “bottom-up” synthesis, the Empa researchers managed to produce specific nanostructures such as defined chains of “buckyballs” (essentially, CNTs shrunk into ball form) or flat nanoribbons on gold substrates. “The great challenge was to find the suitable starting molecule that would also actually ‘germinate’ on a flat surface to form the correct seed,” says Fasel, whose team has gained broad expertise in the field of molecular self-organization over the years. Finally, their colleagues at the Max Planck Institute in Stuttgart successfully synthesized the suitabmedium voltage smart grid sensorle starting molecule, a hydrocarbon with no fewer than 150 atoms.
On a Platinum surface, the planar hydrocarbon precursor folds into an end cap, that in turn acts as seed for the growth of a well-defined (6,6) carbon nanotube. Source: Empa / Juan Ramon Sanchez Valencia
Molecular origami Now how does the process actually work? In the first step, in a manner reminiscent of origami, the flat starting molecule must be transformed into a three-dimensional object, the germling. This takes place on a hot platinum surface (Pt(111)) by means of a catalytic reaction in which hydrogen atoms are split off and new carbon-carbon bonds are formed at very specific locations. The “germ” – a small, dome-like entity with an open edge that sits on the platinum surface – is “folded” out of the flat molecule. This “end cap” forms the “lid” of the growing SWCNT. In a second chemical process, further carbon atoms are attached, which originate from the catalytic decomposition of ethylene (C2H4) on the platinum surface. They position themselves on the open edge between the platinum surface and the end cap and raise the cap higher and higher; the nanotube grows slowly upwards. Only the germ defines the latter’s atomic structure, as the researchers were able to demonstrate through the analysis of the vibration modes of the SWCNTs and scanning tunnel microscope (STM) measurements. Further investigations using the new scanning helium ion microscope (SHIM) at Empa show that the resulting SWCNTs reach lengths in excess of 300 nanometers.
It works! Thus the researchers have proved that, by using made-to-measure molecular “germs”, it is possible to clearly predefine the growth (and thus the structure) of long SWCNTs. The SWCNTs synthesized in this study are mirror-image symmetrical entities. However, depending on the manner in which the honeycombed atomic lattice is derived from the starting molecule (“straight” or “oblique” in relation to the CNT axis), it would also possible be possible to produce helically-wound nanotubes, i.e. nanotubes twisting to the right or left, which are not mirror-image symmetrical. And this very structure also determines the electronic, thermoelectric and optical properties of the material. Therefore, in principle, the researchers can produce materials with different properties in a targeted manner, by selecting the starting molecule. As their next step, Fasel and his colleagues intend to gain an even better understanding of the way in which SWCNTs populate a surface. Although well over 100 million nanotubes per square centimeter are already grown on the platinum surface, actual “fully-grown” nanotubes only grow from a comparatively small proportion of the germs. This raises the questions: which processes are responsible for this, and how can the yield be increased?
The project was supported by the Swiss National Science Foundation (FNSNF).
Publication: Juan Ramon Sanchez-Valencia, et al., “Controlled synthesis of single-chirality carbon nanotubes,” Nature 512, 61–64 (07 August 2014); doi:10.1038/nature13607
Images: Empa / Juan Ramon Sanchez Valencia
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inhandnetworks-blog · 5 years
Text
Contrary to Previous The openvpn  ories, Massive Galaxies Slow Their Growth Over Time
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This image shows two of the galaxy clusters observed by NASA’s Wide-field Infrared Survey Explorer (WISE) and Spitzer Space Telescope missions. Galaxy clusters are among the most massive structures in the universe. The central and largest galaxy in each grouping, called the brightest cluster galaxy or BCG, is seen at the center of each image. The left image shows the cluster known as Abell 2199, which is relatively nearby at a distance of 400 million light-years from Earth (redshift of 0.0302). This image combines infrared data from WISE (in red) with shorter wavelengths of light extending into the visible spectrum from the Sloan Digital Sky Survey (in blue and green). The image on the right is the cluster ISCS 1433.9+3330, which is significantly farther away at a distance of 4.4 billion light-years (redshift of 0.42). Infrared data from Spitzer (red) is combined with similar shorter wavelength data taken by the Mayall Telescope on Kitt Peak, Arizona.
Using data from Spitzer and WISE, scientists reveal in a new study that massive galaxies appear to slow their growth over time, feeding less and less off neighboring galaxies.
Our universe is filled with gobs of galaxies, bound together by gravity into larger families called clusters. Lying at the heart of most clusters is a monster galaxy thought to grow in size by merging with neighboring galaxies, a process astronomers call galactic cannibalism.
New research from NASA’s Spitzer Space Telescope and Wide-field Infrared Survey Explorer (WISE) is showing that, contrary to previous theories, these gargantuan galaxies appear to slow their growth over time, feeding less and less off neighboring galaxies.
“We’ve found that these massive galaxies may have started a diet in the last 5 billion years, and therefore have not gained much weight lately,” said Yen-Ting Lin of the Academia Sinica in Taipei, Taiwan, lead author of a study published in the Astrophysical Journal.
Peter Eisenhardt, a co-author from NASA’s Jet Propulsion Laboratory in Pasadena, Calif., said, “WISE and Spitzer are letting us see that there is a lot we do understand — but also a lot we don’t understand — about the mass of the most massive galaxies.” Eisenhardt identified the sample of galaxy clusters studied by Spitzer, and is the project scientist for WISE.
The new findings will help researchers understand how galaxy clusters — among the most massive structures in our universe — form and evolve.
Galaxy clusters are made up of thousands of galaxies, gathered around their biggest member, what astronomers call the brightest cluster galaxy, or BCG. BCGs can be up to dozens of times the mass of galaxies like our own Milky Way. They plump up in size by cannibalizing other galaxies, as well as assimilating stars that are funneled into the middle of a growing cluster.
To monitor how this process works, the astronome distribution automation  rs surveyed nearly 300 galaxy clusters spanning 9 billion years of cosmic time. The farthest cluster dates back to a time when the universe was 4.3 billion years old, and the closest, when the universe was much older, 13 billion years old (our universe is presently 13.8 billion years old).
“You can’t watch a galaxy grow, so we took a population census,” said Lin. “Our new approach allows us to connect the average properties of clusters we observe in the relatively recent past with ones we observe further back in the history of the universe.”
Spitzer and WISE are both infrared telescopes, but they have unique characteristics that complement each other in studies like these. For instance, Spitzer can see more detail than WISE, which enables it to capture the farthest clusters best. On the other hand, WISE, an infrared all-sky survey, is better at capturing images of nearby clusters, thanks to its larger field of view. Spitzer is still up and observing; WISE went into hibernation in 2011 after successfully scanning the sky twice.
The findings showed that BCG growth proceeded along rates predicted by theories until 5 billion years ago, or a time when the universe was about 8 billion years old. After that time, it appears the galaxies, for the most part, stopped munching on other galaxies around them.
The scientists are uncertain about the cause of BCGs’ diminished appetites, but the results suggest current models need tinkering.
“BCGs are a bit like blue whales — both are gigantic and very rare in number. Our census of the population of BCGs is in a way similar to measuring how the whales gain their weight as they age. In our case, the whales aren’t gaining as much weight as we thought. Our theories aren’t matching what we observed, leading us to new questions,” said Lin.
Another possible explanation is that the surveys are missing large numbers of stars in the more mature clusters. Clusters can be violent environments, where stars are stripped from colliding galaxies and flung into space. If the recent observations are not detecting those stars, it’s possible that the enormous galaxies are, in fact, cont inhand networks inuing to bulk up.
Future studies from Lin and others should reveal more about the feeding habits of one of nature’s largest galactic species.
JPL manages the Spitzer Space Telescope mission for NASA’s Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology in Pasadena. Data are archived at the Infrared Science Archive housed at the Infrared Processing and Analysis Center at Caltech. Caltech manages JPL for NASA. For more information about Spitzer, visit /www.nasa.gov/spitzer.
JPL managed and operated WISE for NASA’s Science Mission Directorate. Edward Wright is the principal investigator and is at UCLA. The mission was selected competitively under NASA’s Explorers Program managed by the agency’s Goddard Space Flight Center in Greenbelt, Maryland. The science instrument was built by the Space Dynamics Laboratory in Logan, Utah. The spacecraft was built by Ball Aerospace & Technologies Corp. in Boulder, Colorado. Science operations and data processing take place at the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena. Caltech manages JPL for NASA. More information is online at wise and /jpl.nasa.gov/wise.
Publication: Yen-Ting Lin, et al., “The Stellar Mass Growth of Brightest Cluster Galaxies in the IRAC Shallow Cluster Survey,” 2013, ApJ, 771, 61; doi:10.1088/0004-637X/771/ Distribution Power Line Monitoring System  1/61
PDF Copy of the Study: The Stellar Mass Growth of Brightest Cluster Galaxies in the IRAC Shallow Cluster Survey
Image: NASA/JPL-Caltech/SDSS/NOAO
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Chemists Develop Simple, Cost-Effective Method to Break Down Water Pol hardware  lutants
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Chemists from Martin Luther University Halle-Wittenberg (MLU) have found out how stubborn pollutants in water can be disintegrated easily and cost-effectively. To do so researchers only need a green LED light, a catalyst and vitamin C. In this way, they can produce special types of electrons that reliably destroy the pollutants in  remote communication  the water. Until now, complex laser systems were required for this. The study was recently published in the international journal Angewandte Chemie.
Researchers in photochemistry are working on the question of how light can be used to initiate chemical reactions. “The idea is that light penetrates a molecule and triggers a reaction there,” says chemist Professor Martin Goez from MLU, whose research group developed the new process. Of particular interest are electrons, which are released by the light energy from their molecular compound in vitamin C and then exist freely in the water. “These so-called ‘hydrated electrons’ are extremely reactive and can, for example, help break down pollutants. The advantage over other substances is that the electrons have completely disappeared after the reaction, meaning they do not leave any harmful residues,” Goez continues. These special electrons can even react with very stable substances and break them down into their individual components.
Until now, expensive and complex high-power lasers were required to generate these types of electrons. Using this kind of equipment is also linked to strict safety precautions. In contrast, the development made by Goez’ team at MLU is significantly easier and more cost-effective. “Our system consists of a standard green light-emitting diode, traces of a metal complex that act as a catalyst and vitamin C. This method can be taught to undergrad students at a very early stage,” says the chemist Goez. The research group tested the new method on chloroacetic acid, an extremely toxic and very stable substance. With their system, the researchers were able to destroy the compound into its harmless components. They were also able to demonstrate that their cost-effective alternative could generate just as many electrons as a high-power la wastewater treatment  ser.
The development by the MLU’s research group is not only suitable for decomposing harmful chlorides or fluorides; the approach can be applied to many other photochemical reactions that are difficult to initiate by other means.
Publication: Robert Naumannbest industrial wifi router, et al., “Generating Hydrated Electrons for Chemical Syntheses by Using a Green Light-Emitting Diode (LED),” Angewandte Chemie, 2018; DOI: 10.1002/anie.201711692
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Chemical Models Help Astronomers Study the Atmospheres of  cellular router manufacturer  Hot Exoplanets
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This is an artist’s impression showing a Jupiter-like transiting planet around a solar-like host star. Credit: ESO/L. Calçada
Chemical models developed to help limit the emission of pollutants by car engines are being used to study the atmospheres of hot exoplanets orbiting close to their stars. The results of a collaboration between French astronomers and applied combustion experts will be presented by Dr Oliva Venot and Dr Eri M2M gateway c Hébrard at the European Week of Astronomy and Space Science (EWASS) 2018 in Liverpool.
Large planets similar to Neptune or Jupiter, orbiting 50 times closer to their star than the Earth does from the Sun, are thought to be composed of hydrogen-rich gas at temperatures between one and three thousand degrees Celsius, circulating at enormous speeds of nearly 10,000 kilometres per hour. With these extreme conditions, the interplay of various physical processes, such as vertical transp Global Leader in Industrial IoTort, circulation or irradiation, can drive the atmospheres of these hot exoplanets out of chemical equilibrium, resulting in deviations that are difficult to explain through standard astrophysical models and observations.
Venot, of the Laboratoire Interuniversitaire des Systèmes Atmosphériques, explains: “The philosophy of our team in solving problems is to search for and import well-tried methods from any other field whenever they exist. Back in 2012, we first noticed the overlap of temperature and pressure conditions between the atmospheres of hot Jupiters and car engines. Chemical networks developed for car engines are very robust as a result of years of intense R&D, laboratory studies and validation through comparison with numerous measurements performed under various conditions. The car models are valid for temperatures up to over 2,000 degrees Celsius and a wide range of pressures, so are relevant to the study of a large diversity of warm and hot exoplanet atmospheres.”
The project grew out of an initial collaboration between the Laboratoire d’Astrophysique de Bordeaux and the Laboratoire Réactions et Génie des Procédés in Nancy. Over the past six years, the team has developed models of the chemical composition of hot Jupiter and warm Neptune atmospheres based on one or several networks of chemical reactions. These chemical networks have been made available through an open access database and are now widely used and recognised in the international astrophysics community.
“It is an important part of our team’s philosophy to make input data and tools available to the community,” says Hébrard, of the University of Exeter.
In addition t m2m connectivity  o car testing, the team has also drawn on the expertise of researchers working on particle accelerators. Data on the ability of molecules to absorb ultraviolet light have, to date, been available mainly at room temperature. Experiments at synchrotron facilities at the Laboratoire Interuniversitaire des Systèmes Atmosphériques will enable measurements to be made at temperatures relevant for exoplanet atmospheres.
“Other fields of research have an important role to play in the characterisation of the fantastic diversity of worlds in the Universe and in our understanding of their physical and chemical nature,” says Venot.
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inhandnetworks-blog · 5 years
Text
Chemical Makeup Impa low-cost cellular router   cts Evolution of the Host Star and Habitability of Planets that Orbit It
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Astrobiologists and planetary scientists agree that a planet’s distance from its parent star is of paramount importance for creating those optimum conditions. A new study by Arizona State University researchers suggests that the host star’s chemical makeup can also impact conditions of habitability of planets that orbit them. Photo by: NASA
Newly published research from scientists at ASU suggests that the host star’s chemical makeup has a substantial impact on the evolution of the host star and the extent of its habitable zone.
The search for potentially habitable planets involves discussion of what is sometimes referred to as the Goldilocks Zone – the relatively thin band in a solar system in which conditions on a planet can support life.
Astrobiologists and planetary scientists agree that a planet’s distance from its parent star is of paramount importance for creating those optimum conditions – like Goldilocks’ porridge, it has to be just right.
A new study by Arizona State University researchers suggests that the host star’s chemical makeup also can impact conditions of habitability of planets that orbit them. The team’s paper, published in the August issue of The Astrophysical Journal Letters, demonstrates that subtle differences in a star’s internal chemistry can have huge effects on a planet’s chances of long-term habitability.
“We have identified changes in the ratios of different elements as particularly important for a given solar system’s habitability,” says Patrick Young, an assistant professor in ASU’s School of Earth and Space Exploration and lead author on the paper. “The more abundant elements carbon, oxygen, silicon, magnesium and sodium are particularly important. The greater the abundances of these four elements in a star, the slower it, and the location of its Goldilocks Zone, will evolve.”
As a star evolves, it becomes brighter, causing the habitable zone to move outwards through its solar system. The team’s study indicates that a greater abundance of oxygen, carbon, sodium, magnesium and silicon should be a plus for an inner solar system’s long-term habitability because the abundance of these elements make the star cooler and cause it to evolve more slowly, thereby giving planets in its habitable zone more time to develop life as we know it.
To explore whether stellar internal chemistr industrial cellular vpn routerIndustrial 3g router  y causes significant changes in the evolution of stars and therefore their habitable zones, Young and his colleagues, graduate students Mike Pagano and Kelley Liebst, did simulations of stars that are like our sun.
“We used spectra from 145 broadly sun-like stars targeted by planet to estimate the amount of variation in the abundance ratios of elements,” explains Pagano, who is a graduate student in the School of Earth and Space Exploration astrophysics program. “For each model, we varied the amount of one element to the extremes of variation we estimated from our analysis of the observations.”
The largest changes, unsurprisingly, arise from variation in oxygen.
“Oxygen is the most abundant element in the universe besides hydrogen and helium, so a change in the oxygen abundance results in a significant change in the total amount of heavy elements in the star,” Pagano said. “Oxygen turns out to be highly  industrial IoT gateway variable in abundance. The effect of increased heavy element abundance on a star is to make it harder for the energy produced by nuclear fusion to escape the star. This means less energy needs to be produced to support the star, and it can live longer.”
The stellar abundance of oxygen seems crucial in determining how long planets stay in the habitable zone around their host star. If there had been less oxygen in the Sun’s chemical makeup, for example, Earth likely would have been pushed out of the Sun’s habitable zone about a billion years ago, well before complex organisms evolved. Considering the first complex multicellular organisms only arose about 650 million years ago, such a move would have likely destroyed any chance of complex life taking hold on Earth.
Planets being searched for signs of life may be about to leave their habitable zones or only have just entered them.
“Habitability is very difficult to quantify because it depends on a huge number of variables, some of which we have yet to identify,” says Young. “It also depends on the definition of habitable that we choose to use. We chose to use a relatively simple model that predicts whether a planet can sustain liquid water on its surface with reasonable assumptions about planetary atmospheres.”
Image: NASA
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Chemical Engineers Develop a  Remote access IoTNew Conductive Coating for Flexible Electronics
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Fig. 1Structural and morphological characterizations of MXene multilayers.(A) Schematic of the PDAC/MXene LbL assembly process. Images of (B) immersion and (C) spray assembly of multilayer coatings of varying number of layer pai substation monitoring  rs on glass. (D) A cross-sectional SEM image of the multilayer coating. (E) Ultraviolet–visible (UV-vis) spectra of MXene multilayers on glass. (F) Absorbance values at 770 nm versus number of layer pairs. a.u., arbitrary units. (G) Growth profile of the multilayers on glass. (H) Root-mean-square (RMS) roughness versus number of layer pairs.Hyosung An, et al., Science Advances 09 Mar 2018: Vol. 4, no. 3, eaaq0118; DOI: 10.1126/sciadv.aaq0118
A team of researchers from the College of Engineering at Texas A&M University have developed a mechanically robust conductive coating that can maintain performance under heavy stretching and bending.
Stretchable, bendable and foldable electronics are crucial for the development of emerging technologies like adaptive displays, artificial skin, and biometric and wearable devices. This presents a unique challenge of balancing electronic performance and mechanical flexibility. The difficulty lies in finding a material that can withstand a wide array of deformations, like stretching, bending  Fault detection & location  and twisting, all while maintaining electrical conductivity. Adding to the challenge is the need for this conductivity to be engineered into a variety of different surfaces, such as cloth, fiber, glass or plastic.
A collaborative team from the Artie McFerrin Department of Chemical Engineering and the Department of Materials Science and Engineering led by Dr. Jodie Lutkenhaus , associate professor and holder of the William and Ruth Neely Faculty Fellowship, has solved this problem through the development of a new surface-agnostic stretchable, bendable and foldable conductive coating, opening the door for a wide variety of flexible electronics.
Two-dimensional metal carbides (MXenes) were chosen as the main focus of the research as previous research has shown them to have a metallic-like conductivity. The previous research on MXenes has focused primarily on the materials in the form of sheets. Although these sheets have the desired c VPN gateway  onductivity, they are not stretchable and their integration into different surfaces has not been shown.
Fig. 2Surface-agnostic conductive coatings.(A) Digital images of 40-layer-pair coatings on various substrates (sheet resistance of coatings on slide glass, PDMS, PET, and kirigami PET: 7, 7, 4, and 4 kilohm per square, respectively). (B) A digital image and SEM images of bare nylon fiber and 20-layer-pair–coated nylon fiber. (C) Images to demonstrate conductive coating on nylon fiber (R= 26.5 megohm). (D) Sheet resistance of the MXene multilayers on glass. (E) Schematic illustration of an electric circuit with a battery, a light-emitting diode (LED), and the MXene multilayer (LbL film). Digital images to demonstrate the conductive coating on PET under bending and folding.Hyosung An, et al., Science Advances 09 Mar 2018: Vol. 4, no. 3, eaaq0118; DOI: 10.1126/sciadv.aaq0118
Rather than using MXene sheets, the Texas A&M research team created MXene coatings through the sequential adsorption of negatively charged MXene sheets and positively charged polyelectrolytes using an aqueous assembly process known as layer-by-layer (LbL) assembly (See image 1-A). The results of this process, described in depth in the latest issue of Science Advances, demonstrate that MXene multilayer coatings that can undergo large-scale mechanical deformation while maintaining a high level of conductivity (see video). The team has also successfully deposited the MXene multilayer coatings onto flexible polymer sheet, stretchable silicones, nylon fiber, glass and silicon.
Publication: Hyosung An, et al., “Surface-agnostic highly stretchable and bendable conductive MXene multilayers,” Science Advances 09 Mar 2018: Vol. 4, no. 3, eaaq0118; DOI: 10.1126/sciadv.aaq0118
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Chemical Engineers Design New Self-He industrial networking  aling Hydrogel for Drug Delivery
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These scanning electron microscopy images, taken at different magnific wastewater treatment  ations, show the structure of new hydrogels made of nanoparticles interacting with long polymer ch industrial IoT Gateway  ains.
Chemical engineers from MIT have designed a new type of self-healing hydrogel that consists of a mesh network made of two components: nanoparticles made of polymers entwined within strands of another polymer, such as cellulose.
Scientists are interested in using gels to deliver drugs because they can be molded into specific shapes and designed to release their payload over a specified time period. However, current versions aren’t always practical because must be implanted surgically.
To help overcome that obstacle, MIT chemical engineers have designed a new type of self-healing hydrogel that could be injected through a syringe. Such gels, which can carry one or two drugs at a time, could be useful for treating cancer, macular degeneration, or heart disease, among other diseases, the researchers say.
The new gel consists of a mesh network made of two components: nanoparticles made of polymers entwined within strands of another polymer, such as cellulose.
“Now you have a gel that can change shape when you apply stress to it, and then, importantly, it can re-heal when you relax those forces. That allows you to squeeze it through a syringe or a needle and get it into the body without surgery,” says Mark Tibbitt, a postdoc at MIT’s Koch Institute for Integrative Cancer Research and one of the lead authors of a paper describing the gel in Nature Communications on February 19.
Koch Institute postdoc Eric Appel is also a lead author of the paper, and the paper’s senior author is Robert Langer, the David H. Koch Institute Professor at MIT. Other authors are postdoc Matthew Webber, undergraduate Bradley Mattix, and postdoc Omid Veiseh.
Heal thyself
Scientists have previously constructed hydrogels for biomedical uses by forming irreversible chemical linkages between polymers. These gels, used to make soft contact lenses, among other applications, are tough and sturdy, but once they are formed their shape cannot easily be altered.
The MIT team set out to create a gel that could survive strong mechanical forces, known as shear forces, and then reform itself. Other researchers have created such gels by engineering proteins that self-assemble into hydrogels, but this approach requires complex biochemical processes. The MIT team wanted to design something simpler.
“We’re working with really simple materials,” Tibbitt says. “They don’t require any advanced chemical functionalization.”
The MIT approach relies on a combination of two readily available components. One is a type of nanoparticle formed of PEG-PLA copolymers, first developed in Langer’s lab decades ago and now commonly used to package and deliver drugs. To form a hydrogel, the researchers mixed these particles with a polymer — in this case, cellulose.
Each polymer chain forms weak bonds with many nanoparticles, producing a loosely woven lattice of polymers and nanoparticles. Because each attachment point is fairly weak, the bonds break apart under mechanical stress, such as when injected through a syringe. When the shear forces are over, the polymers and nanoparticles form new attachments with different partners, healing the gel.
Using two components to form the gel also gives the researchers the opportunity to deliver two different drugs at the same time. PEG-PLA nanoparticles have an inner core that is ideally suited to carry hydrophobic small-molecule drugs, which include many chemotherapy drugs. Meanwhile, the polymers, which exist in a watery solution, can carry hydrophilic molecules such as proteins, including antibodies and growth factors.
Long-term drug delivery
In this study, the researchers showed that the gels survived injection under the skin of mice and successfully released two drugs, one hydrophobic and one hydrophilic, over several days.
This type of gel offers an important advantage over injecting a liquid solution of drug-delivery nanoparticles: While a solution will immediately disperse throughout the body, the gel stays in place after injection, allowing the drug to be targeted to a specific tissue. Furthermore, the properties of e M2M router ach gel component can be tuned so the drugs they carry are released at different rates, allowing them to be tailored for different uses.
The researchers are now looking into using the gel to deliver anti-angiogenesis drugs to treat macular degeneration. Currently, patients receive these drugs, which cut off the growth of blood vessels that interfere with sight, as an injection into the eye once a month. The MIT team envisions that the new gel could be programmed to deliver these drugs over several months, reducing the frequency of injections.
Another potential application for the gels is delivering drugs, such as growth factors, that could help repair damaged heart tissue after a heart attack. The researchers are also pursuing the possibility of using this gel to deliver cancer drugs to kill tumor cells that get left behind after surgery. In that case, the gel would be loaded with a chemical that lures cancer cells toward the gel, as well as a chemotherapy drug that would kill them. This could help eliminate the residual cancer cells that often form new tumors following surgery.
“Removing the tumor leaves behind a cavity that you could fill with our material, which would provide some therapeutic benefit over the long term in recruiting and killing those cells,” Appel says. “We can tailor the materials to provide us with the drug-release profile that makes it the most effective at actually recruiting the cells.”
The research was funded by the Wellcome Trust, the Misrock Foundation, the Department of Defense, and the National Institutes of Health.
Publication: Eric A. Appel, et al., “Self-assembled hydrogels utilizing polymer–nanoparticle interactions,” Nature Communications 6, Article number: 6295; doi:10.1038/ncomms7295
Image: Courtesy of the researchers
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Chandra Discovers a Ring of Black Holes in Galaxy AM 06 dual sim  44-741
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Astronomers have used NASA’s Chandra X-ray Observatory to discover a ring of black holes or neutron stars in a galaxy 300 million light years from Earth.
This ring, while not wielding power over Middle Earth, may help scientists better understand what happens when galaxies smash into one another in catastrophic impacts.
In this new composite image of the galaxy AM 0644-741 (AM 0644 for short), X-rays from Chandra (purple) have been combined with optical data from NASA’s Hubble Space Telescope (red, green, and blue). The Chandra data reveal the presence of very bright X-ray sources, most likely binary systems powered by either a stellar-mass black hole or neutron star, in a remarkable ring. The results are reported in a new paper led by Anna Wolter from INAF-Osservatorio Astronomico di Brera in Milano, Italy.
Where did the ring of black holes or neutron stars in AM 0644 come from? Astronomers think that it was created when one galaxy was pulled into another galaxy by the force of gravity. The first galaxy generated ripples in the gas of the second galaxy, AM 0644, located in the lower right. These ripples then produced an expanding ring of gas in AM 0644 that triggered the birth of new stars. The first galaxy is possibly the one located in the lower left of the image.
The most massive of these fledgling stars will lead short lives — in cosmic terms — of millions of years. After that, their nuclear fuel is spent and the stars explode as supernovas leaving behind either black holes with masses typically between about five to twenty times that of the Sun, or neutron stars with a mass approximately equal to that of the Sun.
Some of these black holes or neutron stars have close companion stars, and siphon gas from their stellar partner. This gas falls towards the black hole or neutron star, forming a spinning disk like water circling a drain, a Vending Telemetry  nd becomes heated by friction. This superheated gas produces large amounts of X-rays that Chandra can detect.
While a ring of black holes or neutron stars is intriguing in itself, there is more to the story of AM 0644. All of the X-ray sources detected in the ring of AM 0644 are bright enough to be classified as ultraluminous X-ray sources (ULXs). This is a class of objects that produce hundreds to thousands of times more X-rays than most “normal” binary systems in which a companion star is in orbit around a neutron star or black hole. Until recently most astronomers thought that ULXs generally contained stellar-mass black holes, with the possible presence in some cases of intermediate-mass black holes (IMBHs) that contain over a hundred times the mass of the Sun. However, this thinking was overturned when a few ULXs in other galaxies, including M82 and M51, were found to contain neutron stars.
Several other explanations besides IMBHs have been suggested for the intense X-ray emission of ULXs. They include unusually rapid growth of the black hole or neutron star, or geometrical effects arising from the funneling of infalling material along magnetic field lines.
The identity of the individual ULXs in AM 0644 is currently unknown. They m data terminal unit  ay be a mixture of black holes and neutron stars, and it is also possible that they are all black holes or all neutron stars.
Not all of the X-ray sources in the image are located in the ring of AM 0644. One of the sources is a rapidly growing black hole that’s located well behind the galaxy at a distance of 9.1 billion light years from Earth. Another intriguing source detected by Chandra is a growing supermassive black hole located at the center of the Grid Analytics System   galaxy. In the new study, the researchers also used Chandra observations to study six other ring galaxies in addition to AM 0644. A total of 63 sources were detected in the seven galaxies, and 50 of them are ULXs. The authors see a larger average number of ULXs per galaxy in these ring galaxies than in other types of galaxies. Ring galaxies have stimulated the interest of astronomers because they are ideal testbeds for examining models of how double stars form, and understanding the origin of ULXs.
The paper describing the study of AM 0644 and its sister ring galaxies appeared in the August 10, 2018 issue of the Astrophysical Journal and is available online. The co-authors of the paper are Antonella Fruscione from the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass., and Michela Mapelli from INAF-Osservatorio Astronomico di Padova in Padova, Italy.
NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA’s Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra’s science and flight operations.
Paper: The X-Ray Luminosity Function of Ultra Luminous X-Ray Sources in Collisional Ring Galaxies
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inhandnetworks-blog · 5 years
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Chandra Releases Five New Images to Celebrate wireless communication   the International Year of Light
www.inhandnetworks.com
To celebrate the International Year of Light, five Chandra images (M51, SNR E0519-69.0, MSH 11-62, Cygnus A, and RCW 86) have been released.
To celebrate the International Year of Light (2015) new images are being released from NASA’s Chandra X-ray Observatory, along with data in other types of light from various telescopes.
The year of 2015 has been declared the International Year of Light (IYL) by the United Nations. Organizations, institutions, and individuals involved in the science and applications of light will be joining together for this yearlong celebration to help spread the word about the wonders of light.
In many ways, astronomy uses the science of light. By building telescopes that can detect light in its many forms, from radio waves on one end of the “electromagnetic spectrum” to gamma rays on the other, scientists can get a better understanding of the processes at work in the Universe.
NASA’s Chandra X-ray Observatory explores the Universe in X-rays, a high-energy form of light. By studying X-ray data and comparing them with observations in other types of light, scientists can develop a better understanding of objects likes stars and galaxies that generate temperatures of millions  industrial transport  of degrees and produce X-rays.
To recognize the start of IYL, the Chandra X-ray Center is releasing a set of images that combine data from telescopes tuned to different wavelengths of light. From a distant galaxy to the relatively nearby debris field of an exploded star, these images demonstrate the myriad ways that information about the Universe is communicated to us through light.
The images, beginning at the upper left and moving clockwise, are:
Messier 51 (M51): This galaxy, nicknamed the “Whirlpool,” is a spiral galaxy, like our Milky Way, located about 30 million light years from Earth. This composite image combines data colle Transformer Monitoring  cted at X-ray wavelengths by Chandra (purple), ultraviolet by the Galaxy Evolution Explorer (GALEX, blue); visible light by Hubble (green), and infrared by Spitzer (red).
SNR 0519-69.0: When a massive star exploded in the Large Magellanic Cloud, a satellite galaxy to the Milky Way, it left behind an expanding shell of debris called SNR 0519-69.0. Here, multimillion degree gas is seen in X-rays from Chandra (blue). The outer edge of the explosion (red) and stars in the field of view are seen in visible light from Hubble.
MSH 11-62: When X-rays, shown in blue, from Chandra and XMM-Newton are joined in this image with radio data from the Australia Telescope Compact Array (pink) and visible light data from the Digitized Sky Survey (DSS, yellow), a new view of the region emerges. This object, known as MSH 11-62, contains an inner nebula of charged particles that could be an outflow from the dense spinning core left behind when a massive star exploded.
RCW 86: This supernova remnant is the remains of an exploded star that may have been witnessed by Chinese astronomers almost 2,000 years ago. Modern telescopes have the advantage of observing this object in light that is completely invisible to the unaided human eye. This image combines X-rays from Chandra (pink and blue) along with visible emission from hydrogen atoms in the rim of the remnant, observed with the 0.9-m Curtis Schmidt telescope at the Cerro Tololo Inter-American Observatory (yellow).
Cygnus A: This galaxy, at a distance of some 700 million light years, contains a giant bubble filled with hot, X-ray emitting gas detected by Chandra (blue). Radio data from the NSF’s Very Large Array (red) reveal “hot spots” about 300,000 light years out from the center of the galaxy where powerful jets emanating from the galaxy’s supermassive black hole end. Visible light data (yellow) from both Hubble and the DSS complete this view.
In addition to these newly released images, the Chandra X-ray Center has created a new online repository of images called “Light: Beyond the Bulb” for IYL. This project places astronomical objects in context with light in other fields of science and research.
NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA’s Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra’s science and flight operations.
Image: NASA/CXC/SAOplc router
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