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Flying Formation - Around the Moon at 3,600 MPH

noreply@blogger.com (Unknown) — Wed, 04 Apr 2012 12:02:00 +0000

The act of two or more aircraft flying together in a disciplined, synchronized manner is one of the cornerstones of military aviation, as well as just about any organized air show. But as amazing as the U.S. Navy's elite Blue Angels or the U.S. Air Force's Thunderbirds are to behold, they remain essentially landlocked, anchored if you will, to our planet and its tenuous atmosphere. What if you could take the level of precision of these great aviators to, say, the moon?

"Our job is to ensure our two GRAIL spacecraft are flying a very, very accurate trail formation in lunar orbit," said David Lehman, GRAIL project manager at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "We need to do this so our scientists can get the data they need."

Essentially, trail formation means one aircraft (or spacecraft in this case), follows directly behind the other. Ebb and Flow, the twins of NASA's GRAIL (Gravity Recovery And Interior Laboratory) mission, are by no means the first to synch up altitude and "air" speed while zipping over the craters, mountains, hills and rills of Earth's natural satellite. That honor goes to the crew of Apollo 10, who in May 1969 performed a dress rehearsal for the first lunar landing. But as accurate as the astronauts aboard lunar module "Snoopy" and command module "Charlie Brown" were in their piloting, it is hard to imagine they could keep as exacting a position as Ebb and Flow. "It is an apples and oranges comparison," said Lehman. "Lunar formation in Apollo was about getting a crew to the lunar surface, returning to lunar orbit and docking, so they could get back safely to Earth. For GRAIL, the formation flying is about the science, and that is why we have to make our measurements so precisely."

As the GRAIL twins fly over areas of greater and lesser gravity at 3,600 mph (5,800 kilometers per hour), surface features such as mountains and craters, and masses hidden beneath the lunar surface, can influence the distance between the two spacecraft ever so slightly.

How slight a distance change can be measured by the science instrument beaming invisible microwaves back and forth between Ebb and Flow?

How about one-tenth of one micron? Another way to put it is that the GRAIL twins can detect a change in their position down to one half of a human hair (0.000004 inches, or 0.00001 centimeters). For those of you who are hematologists or vampires (we are not judging here), any change in separation between the two twins greater than one half of a red corpuscle will be duly noted aboard the spacecraft's memory chips for later downlinking to Earth. Working together, Ebb and Flow will make these measurements while flying over the entirety of the lunar surface.

This begs the question, why would scientists care about a change of distance between two spacecraft as infinitesimal as half a red corpuscle a quarter million miles from Earth?

"Mighty oaks from little acorns grow – even in lunar orbit," said Maria Zuber, principal investigator of the GRAIL mission from the Massachusetts Institute of Technology, Cambridge. "From the data collected during these minute distance changes between spacecraft, we will be able to generate an incredibly high-resolution map of the moon's gravitational field. From that, we will be able to understand what goes on below the lunar surface in unprecedented detail, which will in turn increase our knowledge of how Earth and its rocky neighbors in the inner solar system developed into the diverse worlds we see today."

Getting the GRAIL twins into a hyper-accurate formation from a quarter million miles away gave the team quite a challenge. Launched together on Sept. 10, 2011, Ebb and Flow went their separate ways soon after entering space. Three-and-a-half months and 2.5 million miles (4 million kilometers) later, Ebb entered lunar orbit. Flow followed the next day (New Year's Day 2012).

"Being in lunar orbit is one thing, being in the right lunar orbit for science can be something else entirely," said Joe Beerer, GRAIL's mission manager from JPL. "The twins initial orbit carried them as close to the lunar surface as 56 miles (90 kilometers) and as far out as 5,197 miles (8,363 kilometers), and each revolution took approximately 11.5 hours to complete. They had to go from that to a science orbit of 15 by 53 miles (24.5 by 86 kilometers) and took all of 114 minutes to complete."

To reduce and refine Ebb and Flow's orbits efficiently and precisely required the GRAIL team to plan and execute a series of trajectory modification burns for each spacecraft. And each maneuver had to be just right.

"Because each one of these maneuvers was so important, we did a lot of planning and testing for each," said Beerer. "Over eight weeks, we did nine maneuvers with Ebb and 10 with Flow to establish the science formation. We would literally be watching our screens for a signal telling us about an Ebb rocket burn, then go into a meeting about the next burn for Flow. Our schedule was very full."

Today, the calendar for GRAIL's flight team remains a busy one with the day-to-day operations of keeping NASA's lunar twins in synch. But as busy as the team gets, they still have time to peer skyward.

"Next time you look up and see the moon, you might want to take a second and think about our two little spacecraft flying formation, zooming from pole to pole at 3,600 mph," said Lehman. "They're up there, working together, flying together, getting the data our scientists need. As far as I'm concerned, they're putting on quite a show."

NASA's Jet Propulsion Laboratory in Pasadena, Calif., manages the GRAIL mission for NASA's Science Mission Directorate, Washington. The Massachusetts Institute of Technology, Cambridge, is home to the mission's principal investigator, Maria Zuber. The GRAIL mission is part of the Discovery Program managed at NASA's Marshall Space Flight Center in Huntsville, Ala. Lockheed Martin Space Systems in Denver built the spacecraft. JPL is a division of the California Institute of Technology in Pasadena.

Synchronized NASA and ESA flights across Arctic Ocean - a success!

noreply@blogger.com (Unknown) — Wed, 04 Apr 2012 11:47:00 +0000

By Malcolm Davidson/ESA and Michael Studinger/NASA

Arctic sea-ice from the NASA P-3 (NASA/M. Studinger)

Monday April 2 has been much anticipated by the teams in Thule, Greenland (NASA) and Alert, Canada (ESA). While the objectives for the day were clear – jointly fly with all available planes beneath CryoSat’s early morning pass over the Arctic Ocean – the execution of such flights is and always will be a challenge.

Flying joint multi-plane missions is a rather daunting task. Departure and rendezvous times and locations need to be calculated and maintained to ensure that the instruments on the different planes will see the same sea-ice floes below (these move after all), flight altitudes need to be established and maintained for safety reasons, instruments need to be warmed up and ready ‘in-time’, somewhat grumpy firefighters need to be coaxed out to the airstrip ahead of working hours to support an early departure and the list goes on.

With both teams committed to the flights, the first task early this morning was to check the weather forecast for the day. These proved to be good with temperatures of –29°C (–20°F) and generally clear skies; but not ideal! Some rather worrying cloud formations featured near the coast in satellite images.

NASA P-3 cockpit (NASA/M. Studinger)

Nevertheless, after a quick phone call between the NASA and ESA coordinators (at a time before most people have yet to reach for their mug of morning coffee) the decision was made: it's a go.

From then on it there was a flurry of activity on both sides, pilots warmed up their planes, instrument teams checked out their instruments, flight plans were programmed into the onboard computers and so on.

Twin Otter takes off

The NASA P-3 plane was the first to go out, leaving Thule a full hour before the two ESA planes located closer to the track. On the tarmac in Alert there was the first casualty of the day – despite heroic efforts the EM-bird ice-thickness instrument could not be coaxed into life. The die was cast – the second Twin-Otter plane would have to go it alone and meet up with the NASA P-3.

NASA’s sea-ice mission plan for April 2 (yellow). We teamed up with ESA at 10520 north of Alert. (NASA/M. Studinger)

Around 07:30 (local time) the CryoSat satellite – always on schedule – ripped above the Arctic Ocean taking about one minute to race along the 500-km (310 mile) transect that would later take several hours of plane time to cover.

At 08:00 both the ESA and NASA planes reached the edge of the Arctic Ocean almost simultaneously and headed across the sea ice flying exactly along the same line that CryoSat had just covered. The timing was so good that, for the first time, there was visual contact between the planes, a remarkable achievement!

The image below, which is a DMS mosaic from Eric Fraim shows one of the many leads we saw from the NASA P-3 today with a variety of different types of sea ice.

DMS mosaic of lead in the sea ice (NASA/DMS/E. Fraim)

The rest of the day turned out very well indeed. The clouds that had worried the teams in the morning only formed only a thin band near the coast. The rest of the line out on the ocean was clear and beautifully lit by the oblique Arctic Sun. All the onboard scientific instruments on both planes worked well so that by the end of the day it was clear that the day had been a success.

By joining forces both the ESA and NASA teams collected a highly valuable dataset that will benefit the scientific achievements of ESA’s CryoSat and NASA’s future ICESat-2 mission to better monitor sea ice from space.

Space Is My Mistress

noreply@blogger.com (Unknown) — Wed, 04 Apr 2012 11:34:00 +0000

Seeing as how April is National Poetry Month….

Space is My Mistress

Space is my Mistress,
and she beckons my return.
Since our departure I think of you
and yearn to fly across the heavens arm in arm.
I marvel at your figure,
defined by the edges of continents.
You gaze at me with turquoise eyes,
perhaps mistaken for ocean atolls.
You tease me to fall into your bosom,
sculptured by tectonic rifts,
only to move away as if playing some tantalizing game.
Time and time we turn together,
through day, and night, and day,
repeating encounters every 90 minutes with a freshness,
as if we have never seen our faces before.
We stroll outside together,
enveloped by naked cosmos,
filled with desire to be one.
So close,
you sense my every breath,
which masks your stare through visor haze.
We dance on the swirls of cloud tops,
while skirting the islands of blue.
You know my heart beats fast for you.
Oh, Space is my mistress,
and when our orbits coincide,
we will once again make streaks of aurora across the sky.

NASA GRAIL Returns First Student-Selected Moon Images

noreply@blogger.com (Unknown) — Tue, 27 Mar 2012 12:48:00 +0000

PASADENA, Calif. -- One of two NASA spacecraft orbiting the moon has beamed back the first student-requested pictures of the lunar surface from its onboard camera. Fourth grade students from the Emily Dickinson Elementary School in Bozeman, Mont., received the honor of making the first image selections by winning a nationwide competition to rename the two spacecraft.

The image was taken by the MoonKam, or Moon Knowledge Acquired by Middle school students. Previously named Gravity Recovery And Interior Laboratory (GRAIL) A and B, the twin spacecraft are now called Ebb and Flow. Both washing-machine-sized orbiters carry a small MoonKAM camera. Over 60 student–requested images were taken by the Ebb spacecraft from March 15-17 and downlinked to Earth March 20.

"MoonKAM is based on the premise that if your average picture is worth a thousand words, then a picture from lunar orbit may be worth a classroom full of engineering and science degrees," said Maria Zuber, GRAIL mission principal investigator from the Massachusetts Institute of Technology in Cambridge, Mass. "Through MoonKAM, we have an opportunity to reach out to the next generation of scientists and engineers. It is great to see things off to such a positive start."

GRAIL is NASA's first planetary mission to carry instruments fully dedicated to education and public outreach. Students will select target areas on the lunar surface and request images to study from the GRAIL MoonKAM Mission Operations Center in San Diego.

The MoonKAM program is led by Sally Ride, America's first woman in space, and her team at Sally Ride Science in collaboration with undergraduate students at the University of California in San Diego. More than 2,700 schools spanning 52 countries are using the MoonKAM cameras.

"What might seem like just a cool activity for these kids may very well have a profound impact on their futures," Ride said. "The students really are excited about MoonKAM, and that translates into an excitement about science and engineering."

Launched in September 2011, Ebb and Flow will answer longstanding questions about the moon and give scientists a better understanding of how Earth and other rocky planets in the solar system formed.

NASA's Jet Propulsion Laboratory in Pasadena, Calif., manages the GRAIL mission for NASA's Science Mission Directorate in Washington. The Massachusetts Institute of Technology, Cambridge, is home to the mission's principal investigator, Maria Zuber. GRAIL is part of the Discovery Program managed at NASA's Marshall Space Flight Center in Huntsville, Ala. Lockheed Martin Space Systems in Denver built the spacecraft. The California Institute of Technology in Pasadena manages JPL for NASA.

NASA GRACE Data Hit Big Apple on World Water Day

noreply@blogger.com (Unknown) — Sat, 24 Mar 2012 09:16:00 +0000

To highlight declines in the world's groundwater supplies, a new visualization of Earth's groundwater reserves, created in part with space data from the joint NASA/German Aerospace Center (DLR) Gravity Recovery and Climate Experiment (GRACE) mission, debuted on New York's Times Square on March 22, International World Water Day.

The 30-second animation, titled "Visualizing Seasonal and Long-term Changes in Groundwater Levels," will be on display several times each hour through April 22 on Times Square's massive Thomson Reuters and NASDAQ digital signboards. Viewers of the interactive animation are invited to use their mobile devices to submit their city and add a graph to the sign.

Netherlands designer Richard Vijgen developed the animation using GRACE data analyzed by professor Jay Famiglietti, director of the UC Center for Hydrologic Modeling at the University of California, Irvine; and from United States Geological Survey data supplied by Leonard Konikow. Vijgen was the winning entry in an international design visualization competition sponsored by the organization HeadsUP!, in collaboration with Visualizing.org. Founded by digital media artist Peggy Weil, HeadsUp! challenges designers to visualize critical global issues and create a shared sign for the public square.

Groundwater is a critical, but often overlooked, natural resource. According to a U.N. report, more than 1.5 billion people around the world depend on groundwater for their drinking water. It comes from the natural percolation of precipitation and other surface waters down through Earth's soil and rock, accumulating in cavities and layers of porous rock, gravel, sand or clay. Groundwater levels respond slowly to changes in weather and can take months or years to replenish once pumped for irrigation or other uses.

Famiglietti's analyses show that groundwater is being depleted at alarming rates in many of the world's major aquifers. "The GRACE data set is exciting, because it gives us the first global pictures of Earth's changing freshwater," he said.

The twin GRACE satellites, which celebrated their 10th year in orbit this week, measure minute changes in Earth's gravity field by measuring micron-scale variations in the separation between the two spacecraft, flying in formation 137 miles (220 kilometers) apart in low Earth orbit. These variations in gravitational pull are caused by local changes in Earth's mass. Masses of water, ice, air and solid Earth can be moved by weather patterns, seasonal change, climate change and even tectonic events such as large earthquakes. GRACE was developed by NASA's Jet Propulsion Laboratory, Pasadena, Calif.

The depletion of groundwater from large aquifers due to drought and human activities affects gravity enough to provide a signal that GRACE can measure, in concert with other remote sensing data. After accounting for other mass variations, such changes in gravity can be translated into an equivalent change in water. GRACE has been used to detect major depletion of groundwater in northern India, California's Central Valley and elsewhere around the globe.

Groundwater levels are monitored by local sensors as well as from space with GRACE, but the data are formatted for expert hydrologists, rather than concerned citizens. Underground and out of sight, the public lacks a clear indicator of changing groundwater levels. By using the GRACE satellite data, HeadsUP! offered designers the chance to visualize the water under the surface of Earth, as "seen" from space.

What's Next For NASA?

noreply@blogger.com (Unknown) — Mon, 19 Mar 2012 09:15:00 +0000

The end of the space shuttle program does not mean the end of NASA, or even of NASA sending humans into space. NASA has a robust program of exploration, technology development and scientific research that will last for years to come. Here is what's next for NASA:

Exploration
NASA is designing and building the capabilities to send humans to explore the solar system, working toward a goal of landing humans on Mars. We will build the Multi-Purpose Crew Vehicle, based on the design for the Orion capsule, with a capacity to take four astronauts on 21-day missions.

NASA is also moving forward with the development of the Space Launch System -- an advanced heavy-lift launch vehicle that will provide an entirely new national capability for human exploration beyond Earth's orbit. The SLS rocket will use a liquid hydrogen and liquid oxygen propulsion system, which will include shuttle engines for the core stage and the J-2X engine for the upper stage.

We are developing the technologies we will need for human exploration of the solar system, including solar electric propulsion, refueling depots in orbit, radiation protection and high-reliability life support systems.

International Space Station
The International Space Station is the centerpiece of our human spaceflight activities in low Earth orbit. The ISS is fully staffed with a crew of six, and American astronauts will continue to live and work there in space 24 hours a day, 365 days a year. Part of the U.S. portion of the station has been designated as a national laboratory, and NASA is committed to using this unique resource for scientific research.

The ISS is a test bed for exploration technologies such as autonomous refueling of spacecraft, advanced life support systems and human/robotic interfaces. Commercial companies are well on their way to providing cargo and crew flights to the ISS, allowing NASA to focus its attention on the next steps into our solar system.

Aeronautics
NASA is researching ways to design and build aircraft that are safer, more fuel-efficient, quieter, and environmentally responsible. We are also working to create traffic management systems that are safer, more efficient and more flexible. We are developing technologies that improve routing during flights and enable aircraft to climb to and descend from their cruising altitude without interruption.

We believe it is possible to build an aircraft that uses less fuel, gives off fewer emissions, and is quieter, and we are working on the technologies to create that aircraft. NASA is also part of the government team that is working to develop the Next Generation Air Transportation System, or NextGen, to be in place by the year 2025. We will continue to validate new, complex aircraft and air traffic control systems to ensure that they meet extremely high safety levels.

Science
NASA is conducting an unprecedented array of missions that will seek new knowledge and understanding of Earth, the solar system and the universe. NASA has observatories in Earth orbit and deep space, spacecraft visiting the moon and other planetary bodies, and robotic landers, rovers, and sample return missions. NASA's science vision encompasses questions as practical as hurricane formation, as enticing as the prospect of lunar resources, and as profound as the origin of the Universe.

5 NASA rockets to light up stretch of East Coast skies

noreply@blogger.com (Unknown) — Thu, 15 Mar 2012 10:21:00 +0000

A quintuple rocket launch promises to put on a spectacular, but brief, overnight light show of luminescent vapor trails in the skies above the U.S. East Coast tonight, weather permitting. The sky display may puzzle and amaze some unsuspecting observers, so before you make that phone call to your local news or police, here is why this is happening and when you may see it.

The bright phenomenon will be caused by NASA's Anomalous Transport Rocket Experiment (ATREX), which will launch five chemical-bearing suborbital rockets in about five minutes to test the flow of winds and electrical currents at high altitudes. The rockets will blast off from NASA's Wallops Flight Facility on Wallops Island, Va., on the Atlantic coast during a window that opens tonight at midnight EDT and closes at 1:30 a.m. EDT Thursday.

As part of the mission, the five rockets will each release a chemical tracer that should inscribe brilliant milky white trails in the nighttime sky and allow scientists and the general public to actually "see" high-altitude winds at the edge of space, according to a NASA description.

Midnight launch lights
If all goes well, NASA intends to photograph the trails from three different sites: Wallops Island, southern New Jersey and the outer banks of North Carolina. Should weather conditions be unfavorable, the firings will be delayed to another night, with alternate launch dates available between March 16 and April 3.

Three different types of sounding rockets will be used to create the five cloud trails: two Terrier Improved Malemutes, two Terrier Improved Orions and one Terrier Oriole. These small rockets are powerful enough to launch instruments off the planet on short flights, but not strong enough to reach orbit and circle the Earth.

Each rocket will eject a stream of the chemical trimethyl aluminum (TMA), which will be illuminated at high altitudes by the sun (which will be below the local horizon at ground level). Initially, the clouds are expected to glow in reddish hues, then quickly turn to white, They could persist in the sky for as long as 20 minutes before fading completely away.

The ATREX project is aimed at gathering information to better understand the processes responsible for the high-altitude jet stream winds located 60 to 65 miles (97 to 105 kilometers) above the surface of the Earth.

That works out to a potential viewing radius of up to 450 miles (725 km), suggesting that the resultant cloud trails might be glimpsed from perhaps as far north as southern Vermont and New Hampshire, as far south as the border of coastal North and South Carolina and as far west as central West Virginia.

NASA's Goddard, Glenn Centers Look to Lift Space Astronomy out of the Fog

noreply@blogger.com (Unknown) — Tue, 13 Mar 2012 06:44:00 +0000

A fogbank is the least useful location for a telescope, yet today's space observatories effectively operate inside one. That's because Venus, Earth and Mars orbit within a vast dust cloud produced by comets and occasional collisions among asteroids. After the sun, this so-called zodiacal cloud is the solar system's most luminous feature, and its light has interfered with infrared, optical and ultraviolet observations made by every astronomical space mission to date.

"To put it simply, it has never been night for space astronomers," said Matthew Greenhouse, an astrophysicist at NASA's Goddard Space Flight Center in Greenbelt, Md. Light from zodiacal dust can be a thousand times brighter than the sources astronomers actually target, limiting sensitivity in much the same way that bright moonlight hampers ground-based observatories. The dust and its unwanted illumination are greatest in the plane of Earth's orbit, the same plane in which every space telescope operates.

Placing future astronomy missions on more tilted orbits would let spacecraft spend significant amounts of time above and below the thickest dust and thereby reduce its impact on observations. So Greenhouse teamed with Scott Benson at NASA's Glenn Research Center in Cleveland, Ohio, to investigate how these "dark sky" or extra-zodiacal orbits might improve mission science and to develop a means of cost-effectively reaching them.

"Just by placing a space telescope on these inclined orbits, we can improve its sensitivity by a factor of two in the near-ultraviolet and by 13 times in the infrared," Greenhouse explained. "That's a breakthrough in science capability with absolutely no increase in the size of the telescope's mirror."

Greenhouse, Benson and the COllaborative Modeling and Parametric Assessment of Space Systems (COMPASS) study team at NASA Glenn designed a mission that utilizes new developments in solar arrays, electric propulsion and lower-cost expendable launch vehicles. Their proof-of-concept mission is the Extra-Zodiacal Explorer (EZE), a 1,500-pound EX-class observatory that could accommodate a telescope in the size range of the recently completed WISE mission — all within the cost and schedule constraints of NASA’s Explorer Program.

Launched on a SpaceX Falcon 9 rocket, EZE would use a powerful new solar-electric drive as an upper stage to direct the spacecraft on a gravity-assist maneuver past Earth or Mars. This flyby would redirect the mission into an orbit inclined by as much as 30 degrees to Earth's.

The result, the scientists say, will be the highest-performance observatory ever achieved in the decades-long history of NASA's Explorer program.

"We see EZE as a game-changer, the first step on a new path for NASA Explorers that will yield major science goals despite limited resources," said Benson, who previously managed the new electric propulsion technology project.

Solar storm shakes Earth magnetic field

noreply@blogger.com (Unknown) — Fri, 09 Mar 2012 12:21:00 +0000

WASHINGTON (AP) — A solar storm shook the Earth's magnetic field early Friday, but scientists said they had no reports of any problems with electrical systems.

After reports Thursday of the storm fizzling out, a surge of activity prompted space weather forecasters to issue alerts about changes in the magnetic field.

"We really haven't had any reports from power system operators yet," Rob Steenburgh, a space weather forecaster at the National Oceanic and Atmospheric Administration's Space Weather Prediction Center in Boulder, Colo., said early Friday. "But sometimes they don't come in until after the storm."

He said the storm reached a moderate level late Thursday, before going to a strong level early Friday. For most of Thursday, it was rated as minor.

Scientists say such storms don't pose a threat to people, just technology.

The space weather center's website says a storm rated as strong could force corrections to voltage systems and trigger false alarms on some protection devices, as well as increase drag on satellites and affect their orientation.

The forecasters weren't aware of any significant impact to electrical or technological systems, but said there was a two-hour blackout of high frequency radio communications — affecting mainly ham radio operations — stretching from eastern Africa to eastern Australia.

Steenburgh also said that there was another solar flare late Thursday, similar to the one a few days ago that set off the current storm.

"Right now we're still analyzing when it will arrive" and how strong it could be, he said.

The space weather center had reports of Northern Lights across Canada and dipping into the northern tier of U.S. states, Steenburgh said.

While some experts thought the threat from the solar storm passed by earlier Thursday, the space weather center maintained the storm's effects could continue through Friday morning.

The current storm, which started with a solar flare Tuesday evening, caused a stir Wednesday because forecasts were for a strong storm with the potential to knock electrical grids offline, mess with GPS and harm satellites. It even forced airlines to reroute a few flights on Thursday.

It was never seen as a threat to people, just technology, and teased skywatchers with the prospect of colorful Northern Lights dipping further south.

But when the storm finally arrived around 6 a.m. EST Thursday, after traveling at 2.7 million mph, it was more a magnetic breeze than a gale. The power stayed on. So did GPS and satellites. And the promise of auroras seemed to be more of a mirage.

Scientists initially figured the storm would be the worst since 2006, but now seems only as bad as ones a few months ago, said Joe Kunches, a scientist at the NOAA center. The strongest storm in recorded history was probably in 1859, he said.

"It's not a terribly strong event. It's a very interesting event," Kunches said.

Forecasters can predict the speed a solar storm travels and its strength, but the north-south orientation is the wild card. This time it was a northern orientation, which is "pretty benign," Kunches said. Southern would have caused the most damaging technological disruption and biggest auroras.

On Thursday, North American utilities didn't report any problems, said Kimberly Mielcarek, spokeswoman for the North American Electric Reliability Corporation, a consortium of electricity grid operators. Her office didn't respond to a phone call early Friday.

NASA Mars Orbiter Catches Twister in Action

noreply@blogger.com (Unknown) — Thu, 08 Mar 2012 05:44:00 +0000

An afternoon whirlwind on Mars lofts a twisting column of dust more than half a mile (800 meters) high in an image from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter.

HiRISE captured the image on Feb. 16, 2012, while the orbiter passed over the Amazonis Planitia region of northern Mars. In the area observed, paths of many previous whirlwinds, or dust devils, are visible as streaks on the dusty surface.

The active dust devil displays a delicate arc produced by a westerly breeze partway up its height. The dust plume is about 30 yards or meters in diameter.

The image was taken during the time of Martian year when that planet is farthest from the sun. Just as on Earth, winds on Mars are powered by solar heating. Exposure to the sun's rays declines during this season, yet even now, dust devils act relentlessly to clean the surface of freshly deposited dust, a little at a time.

Dust devils occur on Earth as well as on Mars. They are spinning columns of air, made visible by the dust they pull off the ground. Unlike a tornado, a dust devil typically forms on a clear day when the ground is heated by the sun, warming the air just above the ground. As heated air near the surface rises quickly through a small pocket of cooler air above it, the air may begin to rotate, if conditions are just right.

The Mars Reconnaissance Orbiter has been examining Mars with six science instruments since 2006. Now in an extended mission, the orbiter continues to provide insights into the planet's ancient environments and how processes such as wind, meteorite impacts and seasonal frosts continue to affect the Martian surface today. This mission has returned more data about Mars than all other orbital and surface missions combined.

More than 21,700 images taken by HiRISE are available for viewing on the instrument team's website: http://hirise.lpl.arizona.edu . Each observation by this telescopic camera covers several square miles, or square kilometers, and can reveal features as small as a desk.

NASA finds thickest parts of Arctic ice cap melting faster

noreply@blogger.com (Unknown) — Thu, 01 Mar 2012 09:00:00 +0000

A new NASA study revealed that the oldest and thickest Arctic sea ice is disappearing at a faster rate than the younger and thinner ice at the edges of the Arctic Ocean's floating ice cap. The thicker ice, known as multi-year ice, survives through the cyclical summer melt season, when young ice that has formed over winter just as quickly melts again. The rapid disappearance of older ice makes Arctic sea ice even more vulnerable to further decline in the summer, said Joey Comiso, senior scientist at NASA Goddard Space Flight Center, Greenbelt, Md., and author of the study, which was recently published in Journal of Climate.

The new research takes a closer look at how multi-year ice, ice that has made it through at least two summers, has diminished with each passing winter over the last three decades. Multi-year ice "extent" -- which includes all areas of the Arctic Ocean where multi-year ice covers at least 15 percent of the ocean surface -- is diminishing at a rate of -15.1 percent per decade, the study found.

There's another measurement that allows researchers to analyze how the ice cap evolves: multi-year ice "area," which discards areas of open water among ice floes and focuses exclusively on the regions of the Arctic Ocean that are completely covered by multi-year ice. Sea ice area is always smaller than sea ice extent, and it gives scientists the information needed to estimate the total volume of ice in the Arctic Ocean. Comiso found that multi-year ice area is shrinking even faster than multi-year ice extent, by -17.2 percent per decade.

"The average thickness of the Arctic sea ice cover is declining because it is rapidly losing its thick component, the multi-year ice. At the same time, the surface temperature in the Arctic is going up, which results in a shorter ice-forming season," Comiso said. "It would take a persistent cold spell for most multi-year sea ice and other ice types to grow thick enough in the winter to survive the summer melt season and reverse the trend."

Scientists differentiate multi-year ice from both seasonal ice, which comes and goes each year, and "perennial" ice, defined as all ice that has survived at least one summer. In other words: all multi-year ice is perennial ice, but not all perennial ice is multi-year ice (it can also be second-year ice).

Comiso found that perennial ice extent is shrinking at a rate of -12.2 percent per decade, while its area is declining at a rate of -13.5 percent per decade. These numbers indicate that the thickest ice, multiyear-ice, is declining faster than the other perennial ice that surrounds it.

As perennial ice retreated in the last three decades, it opened up new areas of the Arctic Ocean that could then be covered by seasonal ice in the winter. A larger volume of younger ice meant that a larger portion of it made it through the summer and was available to form second-year ice. This is likely the reason why the perennial ice cover, which includes second year ice, is not declining as rapidly as the multiyear ice cover, Comiso said.

Multi-year sea ice hit its record minimum extent in the winter of 2008. That is when it was reduced to about 55 percent of its average extent since the late 1970s, when satellite measurements of the ice cap began. Multi-year sea ice then recovered slightly in the three following years, ultimately reaching an extent 34 percent larger than in 2008, but it dipped again in winter of 2012, to its second lowest extent ever.

Alien Genetic Material

noreply@blogger.com (Unknown) — Wed, 29 Feb 2012 06:03:00 +0000

Astrobiologists are not certain whether alien would be a carbon-based like or not. Experiments are currently focusing on building alternative kinds of genetic codes and how these codes could evolve.

One of the interesting topics discussed during a public event featuring biologist Richard Dawkins and physicist Lawrence Krauss was the thought that life could be built with an alien biochemistry. The event was attended by more than 3,000 people and was held at Arizona State University in Tempe.

Dawkins said that 99 percent of living things that used to exist are no longer in existence.

Krauss said that laws of physics and chemistry might favor carbon-based life resembling human.

Dawkins said that it is possible that life could exist in more diverse forms, provided that it has a code-carrying system just like DNA, copying itself with high fidelity.

In the same university, biochemist John Chaput was creating what he called TNA, an alternative version of DNA. He published the first evidence that TNA can undergo Darwinian evolution in January. Chaput agrees to Dawkins the need for genetic material for life to exist in more diverse forms just like DNA and RNA.

Alternative code-carriers were also experimented by NASA. The space agency claimed that scientists tried to substitute arsenic phosphorus of bacteria in their DNA. However, they never presented enough evidence that alternative life really existed, according to chemist Steve Benner.

Biochemist Rosemary Redfield duplicated the same process but the bacteria failed to grow when fed arsenic and no phosphorus.

Alien Ship Allegedly Found by Apollo 16 Astronauts

noreply@blogger.com (Unknown) — Wed, 29 Feb 2012 06:00:00 +0000

Moon explorations have been carried out not only by the U.S. and Russia but also countries from Asia including Japan, China and India. Even the European Space Agency has also sent robotic spacecraft to the moon.

Lunar Reconnaissance Orbiter (LRO) of NASA is most likely the most productive among all moon explorations as it already gathered almost a million pictures on the surface of the moon that are so vivid, even a coffee table can be seen in the midst of boulders.

Citizen science program has been encouraged by physicist and astrobiologist Paul Davies to examine closely these public-accessible photos of LRO to locate any artifacts that are extraterrestrial in origin.

However, parapsychology followers believe that NASA has been hiding evidence of aliens discovered on the surface of the moon. They say mind-travelers, who use a psychic technique known as remote viewing to travel other planets, have seen alien-looking things on the lunar surface.

The popularity of remote viewing started when U.S. government supported different parapsychology studies in 1970s and lasted until 1990s. After the funding was ended, an executive summary concluded that the psychic technique test results were “vague and ambiguous.”

More..

NASA’s Hubble Space Telescope discovers Black Hole surrounded by Star Cluster

noreply@blogger.com (Unknown) — Mon, 20 Feb 2012 13:01:00 +0000

Astronomers know how massive stars collapse to form black holes but it is not clear how supermassive black holes, which can weigh billions of times the mass of our sun, form in the cores of galaxies. One idea is that supermassive black holes may build up through the merger of smaller black holes.

Sean Farrell of the Sydney Institute for Astronomy in Australia discovered a middleweight black hole in 2009 using the European Space Agency’s XMM-Newton X-ray space telescope. Known as HLX-1 (Hyper-Luminous X-ray source 1), the black hole has an estimated weight of about 20,000 solar masses. It lies towards the edge of the galaxy ESO 243-49, 290 million light-years from Earth.

Farrell then observed HLX-1 simultaneously with NASA’s Swift observatory in X-ray and Hubble in near infrared, optical and ultraviolet wavelengths. The intensity and the color of the light may indicate the presence of a young, massive cluster of blue stars, perhaps 250-light-years across, encircling the black hole. Hubble can’t resolve the stars individually because the suspected cluster is too far away. The brightness and color is consistent with other clusters of stars seen in other galaxies, but some of the light may be coming from the gaseous disk around the black hole.

“Before this latest discovery, we suspected that intermediate-mass black holes could exist, but now we understand where they may have come from,” Farrell said. “The fact that there seems to be a very young cluster of stars indicates that the intermediate-mass black hole may have originated as the central black hole in a very-low-mass dwarf galaxy. The dwarf galaxy might then have been swallowed by the more massive galaxy, just as happens in our Milky Way.”

From the signature of the X-rays, Farrell’s team knew there would be some blue light emitted from the high temperature of the hot gas in the disk swirling around the black hole. They couldn’t account for the red light coming from the disk. It would have to be produced by a much cooler gas, and they concluded this would most likely come from stars.

Infrared Sounder on NASA's Suomi NPP Starts its Mission

noreply@blogger.com (Unknown) — Thu, 09 Feb 2012 13:47:00 +0000

A powerful new infrared instrument, flying on NASA's newest polar-orbiting satellite, designed to give scientists more refined information about Earth's atmosphere and improve weather forecasts and our understanding of climate, has started sending its data back to Earth.

The Cross-track Infrared Sounder (CrIS) joins four other new instruments aboard the Suomi National Polar-orbiting Partnership (NPP) satellite, which NASA launched on Oct. 28, 2011 from Vandenberg Air Force Base in California. The Suomi NPP mission is the bridge between NOAA's Polar Operational Environmental Satellite (POES) and NASA's Earth Observing System satellites and the next-generation Joint Polar Satellite System (JPSS).

Since it reached orbit, Suomi NPP and its suite of five instruments are undergoing extensive checkouts before starting regular science observations. Suomi NPP is the result of a partnership between NASA, NOAA and the Department of Defense.

CrIS, an advanced spectrometer with 1,305 infrared spectral channels, is designed to provide high vertical resolution information on the atmosphere's three-dimensional structure of temperature and water vapor. The Atmospheric Infrared Sounder (AIRS) on the EOS Aqua mission, launched in 2002, demonstrated how useful this type of data could be for understanding the atmosphere. CrIS will continue this data record and provide data for use in NOAA's numerical weather prediction models to forecast severe weather days in advance.

"Significant overlap between AIRS and CrIS will provide the Earth science research community the ability to maintain the unprecedented accuracy and stability of the temperature and moisture data record initiated by AIRS," said Diane Wickland, Suomi NPP program scientist at NASA Headquarters.

"Having data from CrIS will only improve the quality, timeliness and accuracy of NOAA's weather and climate predictions, which directly affect everyone in America," said Mary Kicza, assistant administrator for NOAA's Satellite and Information Service (NESDIS).

"Over longer periods, data from CrIS will help NOAA to better understand climate phenomena such as El Niño and La Niña that impact global weather patterns," said Mitch Goldberg, NOAA's JPSS program scientist.

The Advanced Technology Microwave Sounder (ATMS), which measures temperature and humidity in both clear and cloudy conditions, was the first Suomi NPP instrument activated. ATMS and CrIS data together will be used operationally in weather forecasts beginning in the Spring of 2012.

NASA Enhances Solar squall Forecasting

noreply@blogger.com (Unknown) — Wed, 01 Feb 2012 11:28:00 +0000

Space agency uses technology to generate up to 100 computerized forecasts to enhanced predict the path and effect of solar storms.

NASA is applying existing technology called "ensemble forecasting" that's been used to predict hurricanes in its observations of solar weather to better predict the trail and effect of solar storms.

The use of the computational predictive technique couldn't come as a better time, as the sun is entering its solar maximum, or period of maximum activity, which will spur an increase in space weather, according to the agency.

Researchers at the Space Weather Laboratory of Goddard Space Flight Research Center have begun to implement ensemble forecasting--which allows them to produce as many as 100 computerized forecasts at once--with full accomplishment in three years' time, according to NASA.

Support from NASA's Space Technology Program Game Changing Program is allowing for the use of the technology, which meteorologists already use to track the potential trail or impact of hurricanes and other forms of severe weather.

Indeed, solar flare and storm activity has increased in latest months as the sun begins to wake up from years of relative inactivity, according to NASA. To organize for it, the agency has been working for some time to improve its forecasting of solar weather.

The sun emitted two considerable corona mass ejections (CMEs)--or billion-ton clouds of solar plasma launched by sun explosions--in the last six months, one on Aug 4 and one in mid January, the latter of which caused some airlines to divert flights. And earlier this week, the most powerful solar flare so far this year erupted from the similar region that caused last week's CME.

As the sun enters its peak of activity, CMEs become more frequent and can affect planets or spacecrafts in their path, as well as disrupt satellite-based communications or power grids on earth.

3 smallest planets outside solar system found

noreply@blogger.com (Unknown) — Sat, 21 Jan 2012 09:15:00 +0000

Washington: A team of astronomers has discovered the three smallest confirmed planets ever detected outside our solar system.

The three planets, discovered by scientists led by Philip Muirhead from the University of California, all orbit a single star, are smaller than Earth and appear to be rocky with a solid surface.

Until now, astronomers have found at most only four other rocky planets, also called terrestrial planets, around other stars.

The trio of new planets is too close to the central star to be in its habitable zone, the ring-shaped region around a star where the temperature is mild enough for liquid water, and possibly life, to exist.

However, the planets are the first rocky ones to be found orbiting a type of dim, small star called a red dwarf, the most common kind in the Milky Way. Their existence suggests that the galaxy could be teeming with similarly rocky planets and that there’s a good chance that many are in the habitable zone.

The red dwarf, called KOI-961, was first flagged as a potential planetary system by the Kepler mission, a space telescope that looks for planets around sunlike stars by scanning the sky for stars that periodically dip in brightness—the result of one or more planets passing in front of them.

Although Kepler reported 900 potential planetary systems in February, only about 85 of those were red-dwarf systems. The fact that a relatively small sample of red dwarfs produced three terrestrial planets means that either the Caltech-led team was really lucky or, more likely, that these planets are commonly found around red dwarfs.

This report comes just a few weeks after the Kepler team announced it had detected two rocky planets around a sunlike star—Kepler-20e and Kepler-20f—the first Earth-sized planets ever found and the smallest known at the time.

In January 2011, the Kepler team reported the discovery of the first unequivocally rocky planet around another star, Kepler-10b. Another planet—Corot-7b, which was found in 2009—could also be a rocky planet.

With the exception of Kepler-20e, which is about the size of Venus, the other previously discovered planets are all bigger than Earth. All three of the ones found by the Caltech-led team are smaller—the outermost one is about half the size of Earth and the other two are three-fourths the size of Earth.

In fact, the entire KOI-961 planetary system is remarkably tiny. KOI-961 has a diameter one-sixth that of the sun’s, making it just 70 percent bigger than Jupiter.

Each of the three planets needs less than two days to zip around their star, and all three are about one hundred times closer to that star than Earth is to the sun.

Since they’re so close to their star, they’re hot—the outermost planet is estimated to be about 200 degrees Celsius while the innermost planet is a scorching 500 degrees Celsius.

“The really amazing thing about this system is that the closest size comparison is to Jupiter and its moons,” John Johnson, one of the paper’s co-authors, said.

“This is causing me to have to fully recalibrate my notion of planetary and stellar systems,” he said.

Kepler’s initial measurements, which are automated to help it sift through roughly 150,000 stars, underestimated the size of KOI-961 and any planets it might have had.

No one realized this until amateur astronomer and paper coauthor Kevin Apps alerted Muirhead and his team to the idea that KOI-961 bore a remarkable resemblance to another red dwarf called Barnard''s Star, a nearby star that’s one of the most well-studied.

When the astronomers used telescopes at the Palomar and Keck Observatories to take a closer look at both stars, they found that the two are practically twins.

The characteristics of Barnard’s Star allowed the team to infer the properties of KOI-961, which is needed to deduce the nature of the planetary system from the star’s light curve, a plot of how the star dims over time due to transiting planets. In particular, the depth of the light curve, that is, how much the curve dips reveals the planets’ sizes.

Because the planets are so small, the only way they could have enough gravity to hold themselves together is if they are balls of rock, like Mercury, Venus, Earth, and Mars.

“Just three years ago, just talking about a rocky planet would have been pure speculation,” Johnson said.

“But these are unambiguously rocky,” he said.

Still, before they could make any conclusions, the researchers had to confirm that the dips in light detected by Kepler really were due to planets—and not something else, such as a pair of background stars in orbit around each other.

Cassini Testing Part of Its Radio System

noreply@blogger.com (Unknown) — Tue, 17 Jan 2012 14:02:00 +0000

PASADENA, Calif. -- Engineers with NASA's Cassini mission are conducting diagnostic testing on a part of the spacecraft's radio system after its signal was not detected on Earth during a tracking pass in late December. The spacecraft has been communicating with Earth using a backup part.

The issue occurred with the ultra-stable oscillator, which is used for one type of radio science experiment and also as a means of sending data back to Earth. The spacecraft is currently using an auxiliary oscillator, whose frequency stability is adequate for transmitting data from the spacecraft to Earth. Tests later this month will help mission managers decide whether it will be possible to bring the ultra-stable oscillator back into service.

Some of the data collected for the radio science experiment using the auxiliary oscillator will be of lesser quality than that from the ultra-stable oscillator. Signals used for occultation experiments – where scientists analyze how radio signals are affected as they travel through Saturn's rings or the atmospheres of Saturn and its moons back to Earth – will be of lesser quality. A second kind of radio science investigation using gravity measurements to probe the internal structure of Saturn or its moons will not be affected. Cassini carries 12 science experiments.

The cause is still under investigation, but age may be a factor. The spacecraft launched in 1997 and has orbited Saturn since 2004. Cassini completed its prime mission in 2008 and has had two additional mission extensions. This is the first time its ultra-stable oscillator has had an issue.

Will NASA’s Kepler find another Earth? Possibly in 2012 say scientists

noreply@blogger.com (Unknown) — Sat, 31 Dec 2011 06:40:00 +0000

It’s the question the entire scientific community is asking: Will NASA’s Kepler find another Earth, and how soon?

2011 was full of reports that astronomers are one step closer to discovering another habitable Earth-like planet outside of our own solar system. NASA earlier this year confirmed the discovery of the first-ever planet in a habitable zone outside our solar system. That planet is roughly twice the size of Earth. French astronomers earlier this year confirmed the first exoplanet to meet key requirements for sustaining life, and just last week NASA announced the discovery of the first two Earth-sized planets orbiting a sun-like star.

In September, Kepler scientists turned science fiction into reality when they announced the first observation of a planet with two suns — such as Luke Skywalker’s home planet Tatooine in the “Star Wars” film series. Such planets are called “circumbinary” planets because they orbit a “binary pair” of stars. Until a few months ago, people only suspected two-star planets might exist.

The latest batch of discovery has left NASA clamoring for more. Speaking earlier this year, Geoffrey Marcy of the University of California, Berkeley, said he expects NASA’s Kepler Telescope to discover a habitable planet within the coming year.

“Sooner or later, Kepler will find a lukewarm planet with a size making it probably Earthlike,” said Geoffrey Marcy of the University of California, Berkeley. “We’re no more than a year away” from such a discovery, he said.

“We are finally there,” said David Charbonneau, an astronomer at the Harvard-Smithsonian Center for Astrophysics, who is part of the team leading the Kepler mission, led by colleague Francois Fressin. “This demonstrates for the first time that Earth-size planets exist around other stars and that we can detect them,” Fressin said.

NASA officials announced earlier this year that the Kepler telescope, which has reportedly already discovered more than 2,000 new planet candidates, is nearly doubling its previously known count. Still, scientists said the space agency should focus on identifying which planets are most likely to maintain the environment necessary for water to exist, and, possibly, life.

Meanwhile, a number of scientists said the latest news is exciting in that Kepler’s batch of discoveries show a number of Earth-like planets exist outside of the Solar System. Astronomers says the number of discoveries in 2011 prove that Kepler can indeed find planets as small as our own, an encouraging sign that planet hunters would someday succeed in the goal of finding Earth-like abodes in the heavens. Since the first Jupiter-size exoplanets, as they are known, were discovered nearly 15 years ago, astronomers have been chipping away at the sky, finding smaller and smaller planets.

“The primary goal of the Kepler mission is to find Earth-sized planets in the habitable zone,” said Francois Fressin of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts, lead author of a new study published in the journal Nature. “This discovery demonstrates for the first time that Earth-size planets exist around other stars, and that we are able to detect them.”

The Kepler science team uses ground-based telescopes and the Spitzer Space Telescope to review observations on planet candidates the spacecraft finds. The star field that Kepler observes in the constellations Cygnus and Lyra can only be seen from ground-based observatories in spring through early fall. The data from these other observations help determine which candidates can be validated as planets.

noreply@blogger.com (Unknown) — Wed, 28 Dec 2011 07:11:00 +0000

Astronomers using NASA’s Spitzer and Hubble space telescopes have discovered that one of the most distant galaxies known is churning out stars at a shockingly high rate. The blob-shaped galaxy, called GN-108036, is the brightest galaxy found to date at such great distances.

The galaxy, which was discovered and confirmed using ground-based telescopes, is 12.9 billion light-years away. Data from Spitzer and Hubble were used to measure the galaxy’s high star production rate, equivalent to about 100 Suns per year. For reference, our Milky Way Galaxy is about five times larger and 100 times more massive than GN-108036, but makes roughly 30 times fewer stars per year.

“The discovery is surprising because previous surveys had not found galaxies this bright so early in the history of the universe,” said Mark Dickinson from the National Optical Astronomy Observatory in Tucson, Arizona. “Perhaps those surveys were just too small to find galaxies like GN-108036. It may be a special, rare object that we just happened to catch during an extreme burst of star formation.”

The international team of astronomers, led by Masami Ouchi from the University of Tokyo, Japan, first identified the remote galaxy after scanning a large patch of sky with the Subaru Telescope atop Mauna Kea in Hawaii. Its great distance was then carefully confirmed with the W.M. Keck Observatory, also on Mauna Kea.

“We checked our results on three different occasions over two years, and each time confirmed the previous measurement,” said Yoshiaki Ono from the University of Tokyo.

GN-108036 lies near the beginning of time itself, a mere 750 million years after our universe was created 13.7 billion years ago in the “Big Bang.” Its light has taken 12.9 billion years to reach us, so we are seeing it as it existed in the distant past.

Astronomers refer to the object’s distance by a number called its “redshift,” which relates to how much of its light has stretched to longer, redder wavelengths due to the expansion of the universe.

NASA shuts doors, pulls plug on shuttle Discovery

noreply@blogger.com (Unknown) — Mon, 19 Dec 2011 12:54:00 +0000

NASA powered down the space shuttle Discovery for a final time Friday , more than 28 years after the agency's retired fleet leader first came alive. The vehicle was "unplugged" inside Orbiter Processing Facility-1 (OPF-1) at the Kennedy Space Center in Florida.

The electrical shutdown, which came soon after technicians closed the shuttle's twin 60-foot long payload bay doors, was a milestone in Discovery's transition from a space-worthy orbiter to a museum exhibit. The shuttle, the oldest of NASA's remaining orbiters, is destined for display next spring at the Smithsonian National Air and Space Museum's Steven F. Udvar-Hazy Center in Virginia.

Discovery's cargo hold — which carried to orbit the Hubble Space Telescope and Ulysses solar probe along with modules for the International Space Station and more than a dozen satellites — was closed for what may be its last time. The Smithsonian plans to display the shuttle with its bay doors shut, at least initially.

The power down was much more permanent. Though Discovery's three electricity-generating fuel cells were reinstalled last week, they were first drained of all their reactants, and their feed lines were purged. Other than serving as an engineering example for researchers, they will never work again.

Since landing back on Earth after its 39th and final mission in March, Discovery has been carefully taken apart to preserve some of its components for future use while making the vehicle safe for public display. Its engines have been removed and replaced with replicas and its thrusters cleaned of their hazardous materials.

Inside its crew cabin, Discovery's waste collection system — otherwise known as its toilet — was removed, cleaned, and replaced, and its flight deck configured to appear ready for another mission, one that will never come. As with the fuel cells, the Smithsonian requested NASA keep Discovery as complete as possible so as to serve as a resource for future study.

Discovery is targeted to make one last flight in April 2012, though not under its own power and well within the atmosphere.

NASA ISS On-Orbit Status

noreply@blogger.com (Unknown) — Mon, 05 Dec 2011 10:09:00 +0000

All ISS systems continue to function nominally, except those noted previously or below. Sunday - Crew off day. Ahead: Week 3 of Increment 30 (three-person crew).

* Today 13 years ago (1998), the US-built Node-1 "Unity", 2nd component of ISS, was launched on STS-88/Endeavour, crewed by CDR Bob Cabana (today Director of NASA/KSC), PLT Fred Sturckow, and Mission Specialists Jerry Ross, Nancy Currie, Jim Newman & Sergey Krikalev (today Director of GCTC/Gagarin Cosmonaut Training Center, Star City, Russia). "Unity" was mated to the Russian-built FGB "Zarya" by Currie on 12/6, and Bob & Sergey entered the rudimentary space station jointly.

After wakeup, FE-1 Shkaplerov performed the routine inspection of the SM (Service Module) PSS Caution & Warning panel as part of regular Daily Morning Inspection.

Anton also conducted the routine daily servicing of the SOZh system (Environment Control & Life Support System, ECLSS) in the SM. This included the weekly collection of the toilet flush (SP) counter and water supply (SVO) readings for calldown to TsUP-Moscow, as well as the weekly checkup on the Russian POTOK-150MK (150 micron) air filter unit of the SM's & FGB's SOGS air revitalization subsystem, gathering weekly data on total operating time & "On" durations for calldown. [SOZh servicing includes checking the ASU toilet facilities, replacement of the KTO & KBO solid waste containers and replacement of EDV-SV waste water and EDV-U urine containers].

CDR Burbank took the (approx.) monthly O-OHA (On-Orbit Hearing Assessment) test, his first, a 30-min NASA environmental health systems examination to assess the efficacy of acoustic countermeasures, using a special software application on the MEC (Medical Equipment Computer) laptop. [The O-OHA audiography test involves minimum audibility measurements for each ear over a wide range of frequencies (0.25-10 kHz) and sound pressure levels, with the crewmembers using individual-specific Prophonics earphones, new Bose ANC headsets (delivered on 30P) and the SLM (sound level meter). To conduct the testing, the experimenter is supported by special EarQ software on the MEC, featuring an up/down-arrow-operated slider for each test frequency that the crewmember moves to the lowest sound pressure level at which the tone can still be heard. The baseline test is required not later than about Flight Day 14 for each new Expedition and is then generally performed once per month. Note: There has been temporary hearing deficits documented on some U.S. and Russian crewmembers, all of which recovered to pre-mission levels.]

Later, Dan performed the VolSci (Voluntary Weekend Science) activity selected for today, an EPO (Educational Payload Operations) demo of 3 student-designed games,- Save the World, Alligator Clip Capture, and Independence Day. The demos were filmed with the G1 camcorder for subsequent downlink via HD MPC (Multi-Protocol Converter) on Ku-band. [EPO Demos are educational videos conducted by crewmembers on-board the ISS. Today's video is intended to be edited on the ground and will be seen by grade 5-8 students and educators. Demo 1: Using a dartboard, Dan demonstrated "sports in space", showing how Newton's Laws of Motion are applied to games in microgravity space. This video will be used on the Space Out Sports Website at http://education.ssc.nasa.gov/spacedoutsports.asp . Demo 2: Crewmember was to release 5 alligator clips in the cabin, allowing them to float, then floated up to capture each alligator clip, from underneath and above the clip (created by students at Kinser Elementary {Department of Defense} School in Okinawa, Japan. Demo 3: Earning points by successfully tossing a baton-like object through a floating ring, cut from a sheet of paper and pasted appropriately. Crewmember then was to repeatedly toss unsharpened pencil (or like object) through the floating paper rings (created by students at Manhattan Beach Middle, Manhattan Beach, CA.]

Anton & Anatoly finished up their lengthy IFM (Inflight Maintenance) on the TVIS treadmill, performing the long-term periodic chassis Inspection which they had been unable to finish on 12/2. Afterwards, Anatoly was to perform the speed characterization test while recording acoustic survey data, which of course was also not done on 12/2. [The inspection included the belt slats, weld nuts, treadbelt, drum set screws, 50 truss blue roller assemblies, side black rollers, and bottom black rollers. The crew also replaced 3 misaligned belt slat screws.]

At ~4:45am EST, Anton Shkaplerov & Anatoly Ivanishin participated in an event set up for them in Moscow to cast their ballot in the Elections to the 6th State Duma of the Russian Federation Federal Assembly and Moscow Regional Duma Elections, formally authorizing their proxy agent Dmitry Alexandrovich Zhukov to fill out the ballot for them, with the required confidentiality being observed. [Alexander Ivanovich Popkov, chairman of the local election committee of Korolev City, Moscow Region, explained the ballot procedure and read out the ballot bulletin, then asked "Dear Anton Nikolayevich and Anatoly Alexeyevich, do you authorize Dmitry Alexandrovich Zhukov to fill out ballot bulletins thus giving effect to your will?" After filling out the forms in secrecy, D. A. Zhukov invited the participants to the voting room and dropped the ballots in a portable box while providing voice commentary of his actions to Anton & Anatoly, who thanked them thusly: "Participation in Russia's political life is a crucial right of every citizen of the country! By casting our vote we shape the direction our nation will take in the future. Our future depends on our vote!" Besides a group of political and communal VIPs, assembled media included "Novosti Cosmonavtiki" magazine; "Russia Today" TV company; ZVEZDA TV Channel; ITAR-TASS news agency; Branch of "Podmoskovye" TV Channel (City of Losino-Petrovsky); NTV TV company; Channel 1 TV company; and RIA Novosti.]

The crew worked out with their regular 2-hr physical exercise protocol on the CEVIS cycle ergometer with vibration isolation (CDR), ARED advanced resistive exercise device (CDR, FE-1, FE-2) and T2/COLBERT advanced treadmill (FE-1, FE-2).

Lightning-made Waves in Earth's Atmosphere Leak Into Space

noreply@blogger.com (Unknown) — Fri, 02 Dec 2011 11:36:00 +0000

At any given moment about 2,000 thunderstorms roll over Earth, producing some 50 flashes of lightning every second. Each lightning burst creates electromagnetic waves that begin to circle around Earth captured between Earth's surface and a boundary about 60 miles up. Some of the waves – if they have just the right wavelength – combine, increasing in strength, to create a repeating atmospheric heartbeat known as Schumann resonance. This resonance provides a useful tool to analyze Earth's weather, its electric environment, and to even help determine what types of atoms and molecules exist in Earth's atmosphere, but until now they have only ever been observed from below.

Now, NASA's Vector Electric Field Instrument (VEFI) aboard the U.S. Air Force's Communications/Navigation Outage Forecast System (C/NOFS) satellite has detected Schumann resonance from space. This comes as a surprise, since current models of Schumann resonance predict these waves should be caged at lower altitude, between the ground and a layer of Earth's atmosphere called the ionosphere.

"Researchers didn't expect to observe these resonances in space," says Fernando Simoes, a scientist at NASA's Goddard Space Flight Center in Greenbelt, Md. "But it turns out that energy is leaking out and this opens up many other possibilities to study our planet from above."

Simoes is the first author on a paper about these observations that appeared online in the journal Geophysical Research Letters on November 16 and will appear in the print publication in December. He explains that the concept of resonance in general is fairly simple: adding energy at the right time will help any given phenomenon grow. Think of a swing – if you push it back just as it hits the top of its arc, you add speed. Push it backwards in the middle of its swing, and you will slow it down. When it comes to waves, resonance doesn't occur because of a swing-like push, but because a series of overlapping waves are synchronized such that the crests line up with the other crests and the troughs line up with the other troughs. This naturally leads to a much larger wave than one where the crests and troughs cancel each other out.

The waves created by lightning do not look like the up and down waves of the ocean, but they still oscillate with regions of greater energy and lesser energy. These waves remain trapped inside an atmospheric ceiling created by the lower edge of the "ionosphere" – a part of the atmosphere filled with charged particles, which begins about 60 miles up into the sky. In this case, the sweet spot for resonance requires the wave to be as long (or twice, three times as long, etc) as the circumference of Earth. This is an extremely low frequency wave that can be as low as 8 Hertz (Hz) – some one hundred thousand times lower than the lowest frequency radio waves used to send signals to your AM/FM radio. As this wave flows around Earth, it hits itself again at the perfect spot such that the crests and troughs are aligned. Voila, waves acting in resonance with each other to pump up the original signal.

UK space radar project initiated

noreply@blogger.com (Unknown) — Wed, 30 Nov 2011 09:53:00 +0000

The UK government is to kick-start an innovative project to fly radar satellites around the Earth, with an initial investment of £21m.

Radar spacecraft can see the planet's surface in all weathers, day and night.It is hoped that a series of satellites could eventually be launched, enabling any place on Earth to be imaged inside 24 hours - a powerful capability.

The radar money is part of a £200m boost for science announced by the Chancellor in his Autumn Statement.George Osborne's investment will be matched by industry.

Radar is one of the most useful tools in Earth observation because of its ability to track objects and events on the ground even when there is thick cloud.

The project being backed by government has been developed by Surrey Satellite Technology Limited (SSTL), which specialises in building small, low-cost spacecraft, and its parent company, Astrium, which makes some of the biggest satellites in orbit today.

Engineers at the two firms have produced a compact radar platform they believe could win many overseas orders, and are keen to demonstrate its capabilities in space.

The new S-band radar satellite is called NovaSar-S ("Sar" stands for synthetic aperture radar). It is a 3m-by-1m spacecraft with a plank-like appearance, weighing just shy of 400kg.

Engineers have found a way to make it considerably smaller than most radar platforms in operation today, and with a price tag that would also be a fraction of that charged for bigger radar satellites.

SSTL says it can build, launch and insure a NovaSar-S for a customer for about £45m.

Mr Osborne's investment, together with SSTL's and Astrium's own money, will enable the first NovaSar-S to be put in orbit. It will be ready for launch in two to three years' time.

Assuming this pathfinder meets its design performance and begins to earn money from the sale of its imagery, SSTL plans to launch further spacecraft, to create a constellation in the sky.

Prof Sir Martin Sweeting is the executive chairman of SSTL. He told BBC News: "We're hoping we can use this commitment from the UK government to go out to our international customers, who we know have had an interest in radar for a long time, and get them to participate in the first mission, to start with, but then to take up one or two of the other satellites so that we can build a constellation in orbit."

A NovaSar-S will produce what are termed medium-resolution images, meaning details on the ground larger than 6m across would be discernable.

NASA Launches Super-Size Mars Rover to Red Planet

noreply@blogger.com (Unknown) — Mon, 28 Nov 2011 12:53:00 +0000

CAPE CANAVERAL, Fla. – The world's biggest extraterrestrial explorer, NASA's Curiosity rover, rocketed toward Mars on Saturday on a search for evidence that the red planet might once have been home to itsy-bitsy life.

It will take 8 1/2 months for Curiosity to reach Mars following a journey of 354 million miles.

An unmanned Atlas V rocket hoisted the rover, officially known as Mars Science Laboratory, into a cloudy late morning sky. A Mars frenzy gripped the launch site, with more than 13,000 guests jamming the space center for NASA's first launch to Earth's next-door neighbor in four years, and the first send-off of a Martian rover in eight years.

NASA astrobiologist Pan Conrad, whose carbon compound-seeking instrument is on the rover, had a shirt custom made for the occasion. Her bright blue, short-sleeve blouse was emblazoned with rockets, planets and the words, "Next stop Mars!"

The 1-ton Curiosity -- as large as a car -- is a mobile, nuclear-powered laboratory holding 10 science instruments that will sample Martian soil and rocks, and analyze them right on the spot.

There's a drill as well as a stone-zapping laser machine.

It's "really a rover on steroids," said NASA's Colleen Hartman, assistant associate administrator for science. "It's an order of magnitude more capable than anything we have ever launched to any planet in the solar system."

The primary goal of the $2.5 billion mission is to see whether cold, dry, barren Mars might have been hospitable for microbial life once upon a time -- or might even still be conducive to life now.

No actual life detectors are on board; rather, the instruments will hunt for organic compounds.

Curiosity's 7-foot arm has a jackhammer on the end to drill into the Martian red rock, and the 7-foot mast on the rover is topped with high-definition and laser cameras. No previous Martian rover has been so sophisticated or capable.

With Mars the ultimate goal for astronauts, NASA also will use Curiosity to measure radiation at the red planet. The rover also has a weather station on board that will provide temperature, wind and humidity readings; a computer software app with daily weather updates is planned.

The world has launched more than three dozen missions to the ever-alluring Mars, most like Earth than the other solar-system planets. Yet fewer than half of those quests have succeeded.

Just two weeks ago, a Russian spacecraft ended up stuck in orbit around Earth, rather than en route to the Martian moon Phobos.

"Mars really is the Bermuda Triangle of the solar system," Hartman said. "It's the death planet, and the United States of America is the only nation in the world that has ever landed and driven robotic explorers on the surface of Mars, and now we're set to do it again."

Curiosity's arrival next August will be particularly hair-raising.

In a spacecraft first, the rover will be lowered onto the Martian surface via a jet pack and tether system similar to the sky cranes used to lower heavy equipment into remote areas on Earth.

Curiosity is too heavy to use air bags like its much smaller predecessors, Spirit and Opportunity, did in 2004. Besides, this new way should provide for a more accurate landing.