Miguel Covarrubias - My Blog

Fifteen-hundred hours, 62 days, nine weeks, or two months -- any way you look at it, a group of Wisconsin middle school students spent a lot of time working on a winning project for NASA's 2011 Waste Limitation, Management and Recycling (WLMR) Design Challenge.

From October 2010 to May 2011, Katelyn, Brianna, Amy, Julia and Maeve, along with their mentor, Christopher Deleon, worked through lunch and after school to develop a highly advanced water recycling system.

They were all good students, but I think they went to a whole other level with this project," Deleon said of the five girls.

WLMR challenged fifth- through eighth-grade students nationwide to design and test a water recycling system that could be used in space. The reason: It's really expensive to transport critical supplies to destinations beyond Earth's atmosphere, so sustainability is the key to affordability for NASA's future expeditions.

Twenty-five teams submitted a final design, tested their systems on a simulated wastewater stream and reported results to a NASA panel comprised of three subject matter experts and three professional educators. Team QNA's Michael Roberts, a lead for Sustainable Systems Research at Kennedy, said the panel was looking for an innovative design that could function in space for long periods of time without the need for a lot of energy or re-supply.

Called "Aqua De Vida," which means "water of life" or "the fountain of youth," the winning team concocted a closed-loop water recycling system design that uses multi-stage filtration, biological treatment and distillation to mimic water recovery on Earth. Their design uses gravity to sieve wastewater through a sand and gravel filter, then through an activated charcoal filter. Filtered water then flows into a biofiltration pond containing bacteria to break down ammonia and Spirulina, a carbon-absorbing and protein-rich, edible cyanobacteria, formerly called blue-green algae. From there, the water trickles into a distillation chamber, where it vaporizes and condenses into drinkable water.

"We all had our own ideas and bringing those together was a challenge," Brianna said. "We really learned to work as a team."

Julia said this solution-seeking project has helped her realize that she would like to be a doctor someday. This solution involved more than just quantity, though; the teammates also had to test the quality of their finished product. To do so, they used a pH test kit, ammonia tester and conductivity meter to determine the number of impurities and nutrients in their filtered water.

"They spent a lot of time researching, building and testing,"Deleon said. "I think this was a great learning experience for them to acknowledge that if they put their minds to something, anything is possible."

Part of their kudos for a job well-done included a trip to Kennedy Space Center, where they toured the Space Station Processing Facility, the Vehicle Assembly Building, Orbiter Processing Facility-2, Launch Pad 39A, where space shuttle Atlantis awaits its STS-135 launch, and the Space Life Sciences Lab. They also toured the Indian River Lagoon on a boat and met with NASA scientists and engineers to discuss their design and learn about other sustainability challenges the agency is working to conquer.

"I think our design can help outside of the space industry, too," said Amy after meeting with Kennedy employees, "Maybe in disaster-stricken areas, like Japan where a tsunami just hit."

Even though Aqua De Vida's system seems complex and is quite bulky, taking up about 8 feet of real estate on the ground, the team says its design can be scaled down for easier transport.

The possibilities don't end there. The system eventually could help boost the immune systems of astronauts on long-duration missions. That's something that could benefit Maeve years from now if she decides to transition from her chosen career path of a member of the Marine Corps to the Astronaut Corps.

"Some of the algae that we used really helps with preventing radiation sickness, or treating it," said Katelyn, who now is considering a career in engineering.

"This NASA middle school opportunity meets science, technology, engineering and mathematics content standards while challenging students to participate in the real-world integrated, multidisciplinary environment critical to the next generation of scientists and engineers," said Cheryl Johnson Thornton, lead of Kennedy's Informal Education.

Other upcoming educational challenges, initiatives and opportunities include an art contest, Student Launch Initiative, One Stop Shopping Initiative, DIME Microgravity Challenge, HAM Radio for International Space Station and a MooonBuggy race.

For more information visit http://www.nasa.gov/offices/education/centers/kennedy/home/WLMR.html

Chefs across the globe may not know it yet, but their baker's yeast just left the kitchen and blasted off into low Earth orbit. Hitching a ride on the space shuttle Atlantis on July 8, 2011, the samples will be grown on the International Space Station as part of the Genotypic and Phenotypic Changes in Yeast Related to Selective Growth Pressures Unique to Microgravity or Micro-4 investigation. Capable of raising more than just breads, this useful organism will help researchers better understand the impact of the space environment on live cells in humans.

This yeast -- S. cerevisiae -- has been of use since the ancient Egyptians first figured out how to harness it for wine and bread making. In modern times it is still used for baking and was the first organism to have its genome fully sequenced. Scientists hope that by studying the changes of yeast in microgravity, they will better understand the changes human cells may experience during long-duration spaceflight. Gaining better knowledge of genetic alterations by studying yeast growth during this microgravity research may also help in understanding how these changes could manifest in human disease here on Earth.

This investigation is a collaboration with BioServe Space Technologies, Durham Veterans Affairs Medical Center, and the University of Toronto. According to Michael Costanzo, Ph.D. and one of the co-investigators for Micro-4 at the University of Toronto, the similarities between human cells and the yeast's genetic makeup makes it ideal for study in space. "We are examining which genes are important for cell growth and survival in a zero gravity environment. The results of our 'yeastnaut' experiments may provide insight into which set of human genes are important and how these genes work together to help organisms/humans deal with extreme environments associated with space travel -- such as zero-gravity and elevated radiation."

Two different sets of experiments will take place as part this study. The first will grow yeast cells in petri dishes using temperature-controlled chambers. On July 12, scientists on the ground remotely changed the temperature from 4° C to 30° C -- the optimal temperature for yeast cell growth -- to activate the on-orbit samples. The cells continue to grow for 48 hours before the temperature is cooled again and the samples are stowed for return to Earth for analysis. The second experiment includes the use of a liquid media to grow the yeast. During the mission, astronauts will transfer the samples to fresh liquid media twice before stowing them, as well.

Both studies will look at how cells adapt to the space environment using the yeast deletion series -- a collection of ≈ 5000 yeast strains, each of which has been deleted for a different gene. In other words, a collection of yeast cells that have been genetically engineered to help scientists to figure out what genes are important for specific responses to microgravity. The goal is to see which strain is best suited to spaceflight, showing researchers which genetic traits are capable of survival in microgravity.

The convenience of yeast as a test subject also provides an important avenue to understanding how living things adapt to space. Due to the small number of humans who have traveled in space, as well as the short duration of their exposure, little is known about the effects of long-term zero gravity on biological systems. "In contrast," said Corey Nislow, Ph.D. and co-investigator from the University of Toronto, "in both our experiments, we have huge sample sizes -- millions of cells -- and they will be monitored for 20 generations, the equivalent of 400 human years."

Control studies will take place on the ground at Kennedy Space Center, Fla. The space shuttle will also carry an identical set of samples to those that will transfer to the space station. These duplicate samples, however, will remain on the shuttle to be "flown, not grown," explained Nislow. Returning to Earth with Atlantis, these duplicate samples will be activated on the ground to investigate growth in tandem timing to those aboard the station.

While the STS-135 mission is the final shuttle flight for NASA, scientists for this study will not have to wait for the certification of new flight vehicles to continue their research. The hardware designed and used for Micro-4 is not limited to the harsh environment of space, but may also find use in Earth-based extremes for future yeast experiments. "It is important to remember that it's fun to fantasize about life in other parts of the solar system, yet we sometimes overlook the fact that life thrives at incredible extremes here on Earth," commented Nislow. "Such as in boiling water around ocean vents, in the polar ice caps, and even in environments so acidic that they would melt metal!"

For more information visit http://www.nasa.gov/mission_pages/station/research/news/Micro_4.html

New findings from NEOWISE, the asteroid- and comet-hunting portion of NASA's Wide-field Infrared Survey Explorer mission, show that comet Hartley 2 leaves a pebbly trail as it laps the sun, dotted with grains as big as golf balls.

Previously, NASA's EPOXI mission, which flew by the comet on Nov. 4, 2010, found golf ball- to basketball-sized fluffy ice particles streaming off comet Hartley 2. NEOWISE data show that the golf ball-sized chunks survive farther away from the comet than previously known, winding up in Hartley 2's trail of debris. The NEOWISE team determined the size of these particles by looking at how far they deviated from the trail. Larger particles are less likely to be pushed away from the trail by radiation pressure from the sun.

The observations also show that the comet is still actively ejecting carbon dioxide gas at a distance of 2.3 astronomical units from the sun, which is farther away from the sun than where EPOXI detected carbon dioxide jets streaming from the comet. An astronomical unit is the average distance between Earth and the sun.

"We were surprised that carbon dioxide plays a significant role in comet Hartley 2's activity when it's farther away from the sun," said James Bauer, the lead author of a new paper on the result in the Astrophysical Journal. An abstract of the scientific paper is online at http://arxiv.org/abs/1107.2637, with the option of downloading a full PDF.

JPL manages and operates the Wide-field Infrared Survey Explorer for NASA's Science Mission Directorate, Washington. The principal investigator, Edward Wright, is at UCLA. The mission was competitively selected under NASA's Explorers Program managed by the Goddard Space Flight Center, Greenbelt, Md. The science instrument was built by the Space Dynamics Laboratory, Logan, Utah, and the spacecraft was built by Ball Aerospace & Technologies Corp., Boulder, Colo. 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.

For more information visit http://www.nasa.gov/mission_pages/WISE/news/wise20110714.html

It's what Bill Patzert, a climatologist and oceanographer at NASA's Jet Propulsion Laboratory in Pasadena, Calif., likes to call a "La Nada" – that puzzling period between cycles of the El Niño-Southern Oscillation climate pattern in the Pacific Ocean when sea surface heights in the equatorial Pacific are near average.

The comings and goings of El Niño and La Niña are part of a long-term, evolving state of global climate, for which measurements of sea surface height are a key indicator. For the past three months, since last year's strong La Niña event dissipated, data collected by the U.S.-French Ocean Surface Topography Mission (OSTM)/Jason-2 oceanography satellite have shown that the equatorial Pacific sea surface heights have been stable and near average. Elsewhere, however, the northeastern Pacific Ocean remains quite cool, with sea levels much lower than normal. The presence of cool ocean waters off the U.S. West Coast has also been a factor in this year's cool and foggy spring there.

The current state of the Pacific is shown in this OSTM/Jason-2 image, based on the average of 10 days of data centered on June 18, 2011. The image depicts places where Pacific sea surface height is higher (warmer) than normal as yellow and red, while places where the sea surface is lower (cooler) than normal are shown in blue and purple. Green indicates near-normal conditions. Sea surface height is an indicator of how much of the sun's heat is stored in the upper ocean.

For oceanographers and climate scientists like Patzert, "La Nada" conditions can bring with them a high degree of uncertainty. While some forecasters (targeting the next couple of seasons) have suggested La Nada will bring about "normal" weather conditions, Patzert cautions previous protracted La Nadas have often delivered unruly jet stream patterns and wild weather swings.

In addition, some climatologists are pondering whether a warm El Niño pattern (which often follows La Niña) may be lurking over the horizon. Patzert says that would be perfectly fine for the United States.

"For the United States, there would be some positives to the appearance of El Niño this summer," Patzert said. "The parched and fire-ravaged southern tier of the country would certainly benefit from a good El Niño soaking. Looking ahead to late August and September, El Niño would also tend to dampen the 2011 hurricane season in the United States. We've had enough wild and punishing weather this year. Relief from the drought across the southern United States and a mild hurricane season would be very welcome."

Jason-2 scientists will continue to monitor Pacific Ocean sea surface heights for signs of El Niño, La Niña or prolonged neutral conditions.

For more information visit http://www.nasa.gov/topics/earth/features/lanada20110629.html

On June 7, 2011, Earth-orbiting satellites detected a flash of X-rays coming from the western edge of the solar disk. Registering only "M" (for medium) on the Richter scale of solar flares, the blast at first appeared to be a run-of-the-mill eruption--that is, until researchers looked at the movies.

"We'd never seen anything like it," says Alex Young, a solar physicist at the Goddard Space Flight Center. "Half of the sun appeared to be blowing itself to bits."

"In terms of raw power, this really was just a medium-sized eruption," says Young, "but it had a uniquely dramatic appearance caused by all the inky-dark material. We don't usually see that."

Solar physicist Angelos Vourlidas of the Naval Research Lab in Washington DC calls it a case of "dark fireworks."

"The blast was triggered by an unstable magnetic filament near the sun's surface," he explains. "That filament was loaded down with cool plasma, which exploded in a spray of dark blobs and streamers. "Cool" has a special meaning on the sun: The plasma blobs registered a temperature of 20,000 Kelvin or less. That is relatively cool. Most of the surrounding gas had temperatures between 40,000 K and 1,000,000 K.

The plasma blobs were as big as planets, many larger than Earth. They rose and fell ballistically, moving under the influence of the sun's gravity like balls tossed in the air, exploding "like bombs" when they hit the stellar surface.

Some blobs, however, were more like guided missiles. "In the movies we can see material 'grabbed' by magnetic fields and funneled toward sunspot groups hundreds of thousands of kilometers away," notes Young.

SDO also detected a shadowy shock wave issuing from the blast site. The 'solar tsunami' propagated more than halfway across the sun, visibly shaking filaments and loops of magnetism en route. [91 MB Quicktime] Long-range action has become a key theme of solar physics since SDO was launched in 2010. The observatory frequently sees explosions in one part of the sun affecting other parts. Sometimes one explosion will trigger another ... and another ... with a domino sequence of flares going off all around the star.

"The June 7th blast didn't seem to trigger any big secondary explosions, but it was certainly felt far and wide," says Young.

It's tempting to look at the movies and conclude that most of the exploded material fell back--but that wouldn't be true, according to Vourlidas. "The blast also propelled a significant coronal mass ejection (CME) out of the sun's atmosphere."

He estimates that the cloud massed about 4.5 x1015 grams, placing it in the top 5% of all CMEs recorded in the Space Age. For comparison, the most massive CME ever recorded was 1016 grams, only a factor of ~2 greater than the June 7th cloud. The amount of material that fell back to the sun on June 7 was approximately equal to the amount that flew away, Vourlidas says.

As remarkable as the June 7th eruption seems to be, Young says it might not be so rare. "In fact," he says, "it might be downright common."

Before SDO, space-based observatories observed the sun with relatively slow cadences and/or limited fields of view. They could have easily missed the majesty of such an explosion, catching only a single off-center snapshot at the beginning or end of the blast to hint at what actually happened.

If Young is right, more dark fireworks could be in the offing. Stay tuned.

For more information visit http://www.nasa.gov/mission_pages/sunearth/news/dark-fireworks.html