August
2009

 

Our Vision
The world’s finest educators supporting science, technology, engineering, and math learning for pre-kindergarten to post-graduate students using real-world applications from satellites and satellite data.

Our Mission
To enhance the education environment to excite students about science, technology, engineering, and math through space-based technology – satellites and satellite data.

TABLE OF CONTENTS CLICK ON THE RED LINKS BELOW TO VIEW ARTICLES

Air Force Report

Space makes case in youth education

Fall Project

Celebrate the 10th Anniversary of World Space Week, October 4-10, 2009

From Scientific Computing

Computing Climate Change: Just the Tip of the Iceberg

A Look Back

Science remains driving force of space exploration

News From NOAA

Help Wanted: Be a NOAA National Weather Service Storm Spotter
And
NOAA Scientists Look Beyond Earth to Understand Auroras

News From NASA

Bolden takes control of NASA
And
GOES-14 Shows First Image

Education Tools

An out-of-the-box web resource for faculty and students of science

Go to SEA's Home Page

Visit the Satellite Educators Association home page


Space makes case in youth education
By: Thea Skinner, 21st Space Wing Public Affairs staff writer
U.S. Air Force


As the new school year approaches, new educational opportunities are becoming available to area students. 

Education is a crucial element of the 21st Space Wing's installation support mission, and one of the Peterson initiatives is the addition of a full-time school liaison education specialist. 

"Leadership recognizes the importance of a quality and positive educational experience for our children, and we believe that it is our duty to partner with parents and advocate for our children's needs," said Col. Emily Buckman, 21st Mission Support Group commander. 

Peterson Air Force Base leadership has developed a close working relationship with Colorado Springs School District 11, said Colonel Buckman, who is also the Peterson school liaison officer. "We have encouraged the district in its efforts to improve many of its processes - to include care for special needs children, raising CSAP scores, and developing advanced and alternative learning opportunities." 

Some of the fruit from the D-11 and Peterson relationship is bearing includes a new space academy. 

Held through a network of community educational leaders throughout the Pikes Peak region, local youth now have access to space and engineering educational career paths. From the new Colorado Springs School District 11 Jack Swigert Aerospace Academy to a possible aerospace-themed curriculum at the base museum, the options provide choice for students and parents alike. 

The JSA Academy is a middle school, located in the former Emerson Middle School at 4220 E. Pikes Peak Ave. This academy is one of several educational paths available to fifth through eighth grade students that will incorporate a space-related curriculum designed to drive proficiency in science, technology, engineering and mathematics. The Space Foundation, an international nonprofit organization and space industry advocate, will provide an on-site curriculum focused on rocketry principles, astronomy, earth systems science, and principles of flight. 

Many opportunities abound and the district is seeking about 500 students to attend the academy, said Tom Strand, the district's school board vice president. 

According to the U.S. Department of Education Impact Aid program, out of 29,842 enrolled students in the district, 2,351 students were military dependants in the 2007-2008 school year. 

"We have had great relationships and ongoing conversations with leadership at Peterson for about eight years," said Elaine Naleski, the district's communications director. "We offer a district-wide program as a response to intervention - a customized individual learning plan for each student." 

The learning plans are offered at all the district's schools. For instance, when a child struggles with math a mentor is embedded into the classroom with the child as a form of intervention. The intervention allows the child to continue on a path of increased student learning. 

"A team will diagnose and prescribe a learning need - it is occurring all throughout the school day," she said. "Let's say your child is gifted, same thing - what can we do to keep him challenged and not get bored." 

Youth who attend the Swigert academy and Christa McAuliffe Elementary generally continue their educational career path at Mitchell High School, which plans to add an additional aerospace curriculum. The high school is already home to a JROTC program.
Classes such as geometry and construction at Mitchell provide students with a skill set, in which students learn to build and sell a house. 

"We are trying to get them (youth) to explore their passion," said Mike Poore, district deputy superintendent, Educational Support Services. "They design skateboard parks - there are all these things you can engage them in by using their skill sets."

Lisa Ballard is the Airman and Family Readiness Center Military Child Education coordinator at Peterson. Ballard interfaces with the Peterson community and all regional school districts. 

In keeping with the 21st Space Wing priority to develop and care for Airmen and their families, Peterson educational leaders are considering developing a similar aerospace educational class on base. 

"One direction we are hoping to go in, is developing an aerospace-themed curriculum at our base museum to expose children to the science and technology fields," Ms. Ballard said "We've also had a successful tutoring program for K-12 children of deployed members and will continue this during the next school year."

The curriculum is designed to provide more options to parents.

"Whether classes are held at the base museum, or eventually are part of the curriculum of an on-base school, parents and students will have more options available to them," she said. "A more integrated community feeling will be established. Of course, D-11 students who are not affiliated with the U.S. Air Force will gain more exposure and insight to life on an Air Force installation - great for recruiting future leaders in the aerospace industry.

"We are certainly in the information-gathering stage and will be working closely with parents and hosting forums to determine exactly what issues our families face. We strongly encourage parents to voice their concerns," Ms. Ballard said.

In 2010 the district will offer an online curriculum with virtual classrooms for kindergarteners through eighth graders. The district also offers a charter school called Life Skills Center of Colorado Springs, and two alternative high schools for youth with jobs, behavioral issues, or in need of child care services.

To address concerns or issues with any schools contact Ms. Ballard at 556-6141 or lisa.ballard@peterson.af.mil. The district's school registration deadline is July 31 and the District 11 school year begins Aug. 18.

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Celebrate the 10th Anniversary of World Space Week, October 4-10, 2009

This October 4-10, the world will have a very special celebration of the contributions of space to humankind. It will be the 10th celebration of UN-declared World Space Week.

(Media-Newswire.com) - This October 4-10, the world will have a very special celebration of the contributions of space to humankind. It will be the 10th celebration of UN-declared World Space Week.

You are invited to amplify your outreach by participating in the largest public space event on Earth. World Space Week is the best time every year to get your space-related messages to the public, students, teachers, employees, government, the media, and other audiences.

To participate, simply schedule space-related programs during October 4-10, promote them as part of World Space Week, and enter them in the global calendar. In doing so, you would join organizations in over 60 nations. With each new event, all participants benefit from the increased global attention to space that week.

In 2009, World Space Week has a special focus on youth. With the theme "Space for Education," participants are encouraged to inspire the next generation using the excitement of space, and educate the educators about the value of space in the classroom.

Designed by noted space artist Pat Rawlings of SAIC, the World Space Week 2009 poster captures the powerful inspiration of space on children.

You can help deliver this important message by putting this year's poster in classrooms by October 4. Teachers, parents, and community-minded organizations can order the poster and can also download free World Space Week teacher guides.

World Space Week National Coordinators can receive free copies of the poster thanks to a grant from the United Nations Office of Outer Space Affairs.

The poster is imprinted in the 6 official UN languages. The artwork without text is also available for use where other languages are spoken.

Click here to learn more.

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Computing Climate Change: Just the Tip of the Iceberg
By: Phillip M. Dickens, Ph.D

Calculating the impact of environmental changes on the world is a complex assignment that must consider myriad variables spanning ocean, air and earth, and nearly everything that comes into contact with them. My team at the University of Maine’s Computer Science Department is focusing on one small piece of the puzzle — climate change. While most scientists conceal research findings until their work is published, we see enormous potential in sharing findings, especially when it comes to climate change. Our team is developing Maine’s first scientific grid portal that will execute climate-change models and provide high-resolution visualizations of output data in real time for use by researchers as well as students and educators in the state’s public school system.

Research in a small power envelope  

Distilling complex global warming research down for students’ desktop computers requires a large, high-productivity computing (HPC) system that is powerful enough to create simulations of ice sheets, animations and other visual information in real time — all while making the research results easy to interpret, whether the ‘student’ is a Ph.D. or a fifth grader. More importantly, the scientific knowledge gleaned from large-scale climate models is directly related to the resolution of the models, and higher resolution models require more computing power. Thus, in designing the portal, we required an HPC system that could deliver enough compute power to satisfy complex problems, but that also would require little space and electricity from the university’s limited resources.

Often, high-powered HPC systems require special housing equipped with advanced cooling systems because they tend to run hot. Unfortunately, even small computing clusters require more power than was available within the department’s power envelope. In fact, installing additional air conditioners in the laboratory was banned due to the strain they would put on the existing electrical system. Moreover, constructing a separate data center to house the HPC system would have proven too costly.

HPC for climate change simulations 

Complex climate change modeling requires an HPC system with many nodes, but with minimal switches to interconnect each node to minimize message-passing costs. This means that, if our team opted for a conventional HPC system, we faced a potential trade-off between computing power and a fast interconnection network due to capital and energy constraints.

UMISM calculated velocities for ice streams on the Pine Island and Twaites GlaciersBased on research during the acquisition process, as well as evaluation of the success of machines installed at Argonne National Laboratory, our team ultimately selected two HPC systems. The first is a 72-core desktop system that is used for code development. The other is equipped with four boards and features 27 nodes per board. Each node shares four gigabytes of memory between six cores, each of which operates at a speed of 733 MHz. The interconnection fabric is extremely fast with an approximate two microsecond message-passing delay between nodes. These systems were selected based on their performance in:

• HPC power and productivity: The two machines deliver ample HPC power and productivity using minimal space and electricity to run the complex simulations within the existing space of the lab. Between the two systems, we are able to achieve 720 core processors running at 733 MHz for a theoretical maximum of 979 gigaflops per second. Moreover, housing the computers in close proximity within the Computer Science Laboratory — as opposed to being located in a separate data center — helps to boost productivity, while delivering the needed computing power at the lowest purchase and operating costs.

• Ease of installation: The machines’ compact design — with a self-contained, single cabinet and single plug system — was an important factor in fitting the high-productivity system within our existing, small physical footprint. In fact, recently, when I was asked how much preparation was required before installing the systems directly into the lab, my response was “I think we had to sweep the floor first.” Energy efficiency: Energy consumption also was considered. Like many computer scientists, we are continually searching for new ways to reduce the amount of energy it takes to operate the systems. Traditional HPC systems require vast amounts of electricity to run, and often require an equal amount to keep cool, resulting in electricity bills that quickly outpace the initial cost of the computer itself. The selected machines achieve the highest level of energy efficiency available in an HPC system, and their power requirements are low enough that no updates were needed to the existing electrical system in our department’s antiquated lab space.

Accessing the grid  

Climate change research requires a multidisciplinary approach, including physicists, computer scientists, network specialists and computational scientists. In using the new system, our computer science researchers are embracing the general trend of a grid model in HPC, where virtual organizations can cooperate even when they are geographically distributed. Research initiatives, such as this University of Maine project, enable collaboration throughout disciplines and locations. The grid portal will give users the opportunity to experiment with environmental parameters and to receive immediate feedback through real-time animations on the impact of these changes.

Our team’s vision is that students and powerful research groups alike will ultimately use the research and tools available through the grid portal, which can be accessed over the state’s high performance optical network. We are trying to make some of our research available to the public, and are designing a special interface so it can be accessed by the public and students in K-12. Of course, the project not only addresses the needs of researchers and grade school students; it also presents enormous learning opportunities for the department’s undergraduate students. Funded through a research grant provided by the National Science Foundation (NSF), the grid will give University of Maine students dual learning experience in research and supercomputing, as well as experience with team collaboration — classroom and real-world experiences that will prepare them for a wide spectrum of future careers.

Research collaboration 

When it launches this fall, the grid will enable collaborating scientists to both use and access data, as evidenced by a planned partnership between our University of Maine research team and the Jackson Laboratory, a leading genetics research center that is immersed in highly intensive applications. Researchers at Jackson Laboratory will be able to upload data to University of Maine systems for processing, and the supercomputers will then compute the models and send back the visual renderings of the lab’s data — a true collaboration in solving large problems and a first for the state of Maine. This technology makes it possible to solve problems that are too large to execute at either facility alone by distributing the task across both the University of Maine system and the Jackson Lab cluster so that they can execute the task concurrently.

Similarly, a future interface will enable climate change researchers to remotely input their own data in existing climate change models, such as the University of Maine Ice Sheet Model (UMISM), which was developed by physicist James Fastook to very quickly execute high-resolution models of a piece of the Antarctic ice sheet. The original version of the model, which looks at all variables that affect behavior and cause change in the ice sheet, was running on a Mac Pro. In order to obtain higher resolution, the model will be spread out over many processors on the new system. This parallelization will produce much finer resolution and allow real-time animation of the output of the model. With these interactive simulation capabilities, researchers will be able to create and make adjustments to steer the simulation as the model is running, providing immediate feedback on the effect of the changes.

Future expansion will allow more scientists to run their work on the portal, including the University of Maine’s Climate Change Institute, an interdisciplinary research unit organized to conduct world-class research, graduate education and environmental outreach focused on the variability of Earth’s climate system, as well as on the interaction between humans and the natural world. Ultimately, as more of the state’s research facilities join the grid portal, it will have the computing power and expertise to solve problems of national and global significance.

Conclusion

Going forward, the team plans to work closely with other scientists to parallelize their code so they can take advantage of the opportunities the grid provides, as well as significantly increase the models made available through the portal. The project also will provide functions to other scientific modelers so they can utilize University of Maine code to work on the system through remote visualization and still interact and receive images as their model is executing. Other challenges, such as those presented by multiple simultaneous users running independent versions of the model at the same time, will be tackled as well.

Acknowledgements

Dr. Dickens’ research is funded by Grants 0702748, 0723093, and 0737870 from the National Science Foundation.

References

1. Lang, O., Rabus, B., and Dech, S. (2004). Velocity map of the Thwaites Glacier catchment, West Antarctica. Journal of Glaciology, 50(168).
2. Rignot, E., R.H. Thomas, P. Kanagaratnam, G. Casassa, E. Frederick, P. Gogineni, W. Krabill, A. Rivera, R. Russell, J. Sonntag, R. Swift, and J. Yungel, Improved estimate of the mass balance of glaciers draining into the Amundsen Sea of West Antarctica from CECS/NASA 2002 campaign, Annals of Glaciology, 39, 231-237, 2004.


Phillip Dickens is an assistant professor of computer science at the University of Maine. He may be reached at editor@ScientificComputing.com.

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Science remains driving force of space exploration
by Ken Newton
StJoeNews.net

No man ever looked so heroic stepping off a ladder.

Neil Armstrong remains a fixture of collective memory and imagination, an American in bulky gear frozen forever in murky black and white.

His words, with electronic crackle from roughly 238,000 miles overhead, have the staying power of that visual. Few denied, among the half-billion people watching on television worldwide, it was “a giant leap for mankind.”

The first moon landing, with Mr. Armstrong’s historic descent onto a surface not Earth, happened 40 years ago on Monday. Just 66 years after man achieved powered flight, astronauts rode a rocket to another world and radioed back to tell about it.

Citizens of the world leaned their heads back and let their jaws drop.

“It gave me sort of a sense of pride that human beings could accomplish something so seemingly impossible,” said Dr. Christopher Godfrey, who teaches physics at Missouri Western State University. “It gave you confidence in the future of what could be done.”

For Americans, the achievement proved a particular triumph. The nation remained mired in Vietnam. The 1960s had long before spun out of control, with civil unrest, Cold War tensions and political assassinations.

Yet here arrived a challenge fulfilled, a goal met to reach the moon before decade’s end. Americans accomplished this through a union of sciences and engineering and gumption. Our side crossed the finish line first, a chest-beating win in the race started by the ideologically wayward Soviets.

“Can-do” became the operative description of a nation. And there was some sci-fi adventure thrown in for good measure.

Then, the adventure subsided. The space agency NASA wanted to make its flights routine, and it did so. American attention strayed. Twelve men would walk on the moon, the last in 1972. In the years since, no manned vehicle has strayed beyond Earth’s orbit.

A space program mishap refocuses people occasionally. But a shuttle full of U.S. astronauts circles the planet this weekend after a launch on Wednesday, and a small percentage of Americans know or care.

“We’ve become numb to some of that,” conceded Jay Meyers, the St. Joseph School District’s secondary science coordinator.

Focus on science

Science in the post-Sputnik days focused on a mission, that of discovery but also succeeding ahead of an adversary. Today, Mr. Meyers said, science education includes a technical application.

The monumental achievement of the moon landing, he said, was the bringing together of so many disciplines ... physics and astronomy, chemistry and biology, engineering and mathematics. An academic upsurge in those areas followed.

“We do science for a wide number of reasons,” Mr. Meyers said, “but one of them is to make our lives better.”

Dr. John Shaw, who teaches physics at Northwest Missouri State University, grew as a space-race kid, smuggling a transistor radio into his grade school classroom to listen to Alan Shepard’s flight in a Mercury capsule.

While space flight impacted his life and others of his generation, the broader influence was short-lived. He noted that American doctoral degrees awarded in physics peaked in 1973, and engineering bachelor’s degrees amount to 5 percent or less of the nation’s undergraduate total. In some nations, 30 percent of graduates get engineering degrees.

“As someone with an intense interest in science, I’m not sure why it has become so unfashionable,” Dr. Shaw said.

Science remains the driving force of the space program, according to James Bangerter, who followed a path from St. Joseph to NASA.

A manager in communications network integration at the Goddard Space Flight Center in Maryland, Mr. Bangerter says the motivation of space exploration is as old as ancient man’s desire to see over the top of the next hill. It remains essential to human nature.

“We explore, we experiment, we discover, in ways no one else can,” the Central High School graduate said. “Science and discovery is what NASA does best.”

Mr. Bangerter said all NASA employees involved in human space flight missions understand the history of manned programs. He said the lessons of Mercury and Apollo carry forward to all agency endeavors, including the Constellation program that will follow the space shuttle accomplishments.

“(Constellation) borrows a great deal of its mission concepts from the Apollo program, integrating the best of the past with the best of the present,” he said.

Cooper Snapp, a Benton High School graduate who has settled into a NASA career, regards the agency’s science as a good investment of taxpayer dollars.

“It is very hard to pick up an issue of Popular Science and not see how a NASA spinoff is helping society,” he said.

An engineer and a manager in NASA’s development of spacecraft thermal protection, Mr. Snapp said the agency’s goals to return to the moon and explore other planets should capture the imagination of young people and advance the nation’s understanding of energy sources such as nuclear and solar.

He admits, though, that not everyone has a sense of NASA’s history. When Mr. Snapp moved from Florida to Houston, he encountered Apollo 13 commander Jim Lovell in the NASA badging office. The young woman making the badges failed to recognize the former astronaut.

“He commented, ‘Come on, I was the guy that Tom Hanks played in the movie,’” Mr. Snapp recalled.

Still an interest

While young people may not hold the fascination with space travel like they did at the time of the moon landing, they remain interested in the stars. Jerry Wilkerson directs shows at Missouri Western’s Bushman Planetarium, about 35 a year for elementary students.

The kids always stay afterward and ask questions about the solar system.

“It’s kind of human nature to be interested in what’s up there,” he said.

Janet Fite, a St. Joseph teacher for more than 30 years, watched the moon landing from her Savannah home with a father entranced by rocketry. They were always launching something.

With a laugh, she recalls one occasion of having to stay with her grandparents when a rocket fuel incident smelled up their house.

“If you’ve ever seen the movie ‘October Sky,’ that was my life,” she said.

A recipient of fellowships to study at NASA facilities, Ms. Fite works to pass along her knowledge of space to young people. This extends to evenings outdoors with her grandchildren, eyes upward to study the heavens.

She remains heartened by their interest.

“I guess the whole idea is that there is so much out there we don’t know,” the educator said. “If we don’t explore, then we’ve lost that opportunity.”
 

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Help Wanted: Be a NOAA National Weather Service Storm Spotter

NOAA's National Weather Service meteorologists across the country could use a hand — or more precisely extra eyes — to help them produce the most accurate weather information possible. If you are fascinated by weather, you have the opportunity to become a trained volunteer SKYWARN® storm spotter for your local weather forecast office. 

Your Eyes on the Skies

Storm spotters provide valuable information on all types of weather hazards to meteorologists in their local National Weather Service forecast offices. Meteorologists use this information, especially when it comes to severe storms, to create a more complete picture of area weather conditions.

The SKYWARN program helps improve the timeliness and accuracy of weather warnings. When coupled with Doppler radar imagery, satellite and other data, reports from storm spotters help forecasters know exactly what is happening on the ground with rapidly developing storms.

“The more lead time we can provide with our warnings, the more time people have to take cover from life-threatening storms,” says Christopher Maier, who oversees the national SKYWARN program.

Training in Your Area

You can take storm spotter training through your local weather forecast office. Classes are free and each last about two hours. Covered topics include thunderstorm development, storm structure, severe weather features, weather reporting, and weather safety.

To find out when classes are offered in your area, contact your local weather forecast office. NOAA logo.

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GOES-14 Shows First Image

From 22,336 miles in space, NOAA’s newest Geostationary Operational Environmental Satellite – GOES-14 – took its first full-disc visible image on July 27 at 2 p.m. EDT. GOES-14 joins three other operational NOAA GOES spacecraft that help the agency’s forecasters track life-threatening weather and solar activity that can impact the satellite-based electronics and communications industry.

 

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NOAA Scientists Look Beyond Earth to Understand Auroras

The eerie beauty of the northern and southern lights has evoked visions of the supernatural for centuries: foxes of fire whisking their tales, the fighting souls of dead warriors or ancestors dancing around a ceremonial fire.

The English poet Sir Walter Scott in 1805 conjured up otherworldly beings when he wrote, "He knew, by the streamers that shot so bright, That spirits were riding the northern light."

But it was a French scientist, not a poet, who named the sight after Roman gods. In 1621, Pierre Cassendi paired Aurora, goddess of dawn, with Boreas, god of the north wind, to christen the northern lights “aurora borealis.” Those centered above the South Pole are called aurora australis for “southern dawn.”

Even today, scientists and forecasters at NOAA’s Space Weather Prediction Center in Boulder, Colo., look beyond the Earth itself for the first step in a chain of events that ultimately paints brilliant hues across the night sky at opposite ends of the planet

The Anatomy of an Aurora

Deep within the Sun, 93 million miles away, roiling plasma rises and bursts through the solar atmosphere, sometimes thrusting highly charged protons and electrons our way. When this so-called solar wind arrives near Earth, it energizes protons and electrons trapped in the planet’s magnetic field.

These charged particles then travel down magnetic field lines, like beads slipping along a string, into Earth’s upper atmosphere near the poles. There the particles in turn excite atoms and molecules of oxygen, nitrogen, and other atmospheric gases. As these atoms relax back down into their normal state, they release the excess energy as visible light, forming an aurora oval loosely centered on the magnetic pole.

During an aurora, vivid arcs, curls, waves and bands of green, red, and sometimes blue dance across the sky for minutes or hours, peaking near midnight — all between 60 and 600 miles above the ground.

Many people think auroras are rare events, but there’s almost always an aurora of some size in the sky near the poles. Seeing one is another matter.

Auroras are most often visible in regions bordering the Arctic Circle: Canada, Alaska, northern Greenland, the Scandinavian coast, and Siberia. In the south, you need to be visiting Antarctica to see an aurora frequently. But the larger the solar storm reaching Earth’s upper atmosphere, the farther the aurora extends from the poles. Residents of New England or southern Chile might see an aurora every few years. If you live in Florida or Italy, you’d be lucky to see an aurora once in your lifetime.

How Space Weather Affects Us

One of the nation’s critical operations centers, NOAA’s Space Weather Prediction Center keeps a close eye on solar activity that precedes an aurora. When a major storm explodes on the sun, followed by a suddenly intensified solar wind heading toward Earth, the center alerts airlines, the military, the communications industry, power companies and the media that a storm is on its way.

Why do NOAA scientists care about this odd “weather” on the sun and in space? NOAA monitors solar storms because they can disrupt satellite functions, power grid operations, GPS signals, high-frequency communications used by airlines and the military, and other space-based technologies that we depend on. Solar radiation could also threaten astronauts’ safety if they happen to be outside the space shuttle as it zooms past.

Visit the Space Weather Prediction Center’s aurora Web site to view the current shape and size of the auroras around the two poles. If the auroras shown there are exceptionally large and you’re in a far northern or far southern latitude, look for those spirits hurtling across the midnight sky!

Tips on Seeing an Aurora

Best time of night: 10:00 p.m. to 2:00 a.m.
Best conditions: clear night with no moon and far from light pollution
Best season: mid-winter
Best phase of the solar cycle: maximum
Best years in the sun’s current cycle: 2012 to 2013
Best position on Earth: far northern or southern latitudes NOAA logo.

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Bolden takes control of NASA

The US Senate has easily confirmed former astronaut Charles Frank Bolden as the new NASA administrator, along with Lori Beth Garver as his deputy.

F8FF6B45-156E-4843-9ED4-E84DFA64F746.jpgBolden, a former Marine Corp pilot, flew in the space shuttle four times between 1986 and 1994 (STS-61C, STS-31, STS-45, and STS-60), which included the 1990 deployment of the Hubble Space Telescope.

Bolden said in a press release, "It is an honor to have been nominated by President Obama and confirmed by the Senate to lead this great NASA team. Today, we have to choose. Either we can invest in building on our hard-earned world technological leadership or we can abandon this commitment, ceding it to other nations who are working diligently to push the frontiers of space."

He continued: "If we choose to lead, we must build on our investment in the International Space Station, accelerate development of our next generation launch systems to enable expansion of human exploration, enhance NASA's capability to study Earth's environment, lead space science to new achievements, continue cutting-edge aeronautics research, support the innovation of American entrepreneurs, and inspire a rising generation of boys and girls to seek careers in science, technology, engineering and math."

The theme was highlighted in his confirmation hearings when Bolden emphasized that NASA needed to re-ignite public interest in the space program, particularly among children. "If I go to a classroom today, it's different from when I went as an astronaut in 1980," he told members of the US Senate Committee on Commerce, Science and Transportation.

"I could ask, 'How many of you want to be an astronaut?' Every hand went up in the class. When I go to a school today and ask that question, I may see three hands. All of them want to go into business."
Bolden will have a number of critical issues to manage at NASA. The space shuttle is scheduled to be retired next year and the White House is reviewing plans for its replacement.

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M.Y. S.P.A.C.E. Photos from the conference posted.
Click Here

Artist concept of the albedo effect

Be a M.Y. S.P.A.C.E. Teacher
Click here
to find out how

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An out-of-the-box web resource for faculty and students of science

Screen shot of the websiteVisionlearning is a very useful out-of-the-box educational resource for faculty and students.  It is an online endeavour of years of individual and collaborative effort towards improving teaching and learning Science subjects.

Visionlearning hosts at http://www.visionlearning.com, high-quality science learning modules that can be quite effective than traditional textbooks in teaching science. The Visionlearning’s Library comprises an award-winning collection of peer-reviewed learning modules written by professional educators and scientists.

These modules provide text, interactive animations, glossary definitions, current news and research, scientist biographies and practice exercises to provide a comprehensive learning environment. These modules can be sorted by subject or science standard and can also be customised in the ‘MyClassroom’ space. The subjects covered include Biology, Chemistry, Earth Science, General Science, Physics, Process of Science, Toxicology and Pharmacology, and Trigonometry.

Under Biology the chapters included are Adaptation: The Case of Penguins; Cells: Discovery and Basic Structure; Charles Darwin I, II and III; Genetics; Taxonomy; and Nomenclature.

The section related to Chemistry includes these chapters: Acids and Bases: An Introduction; Atomic Theory I: The Early Days; Atomic Theory II: Ions, Isotopes and Electron Shells; Carbohydrates; Chemical Bonding; Chemical Equations; Chemical Reactions; Fats and Proteins; Matter: Atoms from Democritus to Dalton; Matter: States of Matter; Nuclear Chemistry:  An Introduction; Organic Chemistry: An Introduction; The Mole: Its History and Use; The Periodic Table of Elements; and Water: Properties and Behaviour;
The Earth Science section includes: Earth Structure: A Virtual Journey to the Centre of the Earth; Earth's Atmosphere: Composition and Structure; Minerals I: Definitions; Minerals II: Properties; Minerals III: The Silicates; Plate Tectonics I: The Evidence for a Geologic Revolution; Plate Tectonics II: Plates, Plate Boundaries, and Driving Forces; The Carbon Cycle: What Goes Around Comes Around; The Hydrologic Cycle: Water's Journey through Time; The Nitrogen Cycle: Of Microbes and Men; and The Rock Cycle: Uniformitarianism and Recycling.

The section on General Science includes: Density; Energy: An Introduction; Temperature; The Metric System: Metric and Scientific Notation; The Scientific Method; and Unit Conversion: Dimensional Analysis. The Physics section has chapters on Gravity: Newtonian Relationships; Light I: Particle or Wave?; Light II: Electromagnetism; and Waves & Wave Motion: Describing Waves. The Process of Science contains chapters on Data: Analysis and Interpretation; Statistics; Uncertainty; Error and Confidence; and Using Graphs and Visual Data.

The work-in-progress
Visionlearning website continues to grow with new modules being added each month. Its salient features include: Special Events in Science feature which highlights a key date in scientific discovery every month, News & Events section of the modules provides links to current science news stories, and its USP is of course the MyClassroom feature. This lets users to download a pdf file of an entire classroom with a single click, lets instructors create custom quizzes associated with modules in their MyClassrooms. The soon-to-be-added features include a system that will allow instructors to create custom modules, and a series of teaching tips associated with the modules that are publicly available on the site.

 

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