Sunday, July 19, 2009

Dryden Flight Research Center's Contributions to Apollo's Moon Landing Success

The late Joseph Algranti maneuvers the first Lunar Landing Research Vehicle, or LLRV, over Edwards Air Force Base' South Base ramp area on Aug. 19, 1966.NASA's Flight Research Center at Edwards Air Force Base (renamed the Dryden Flight Research Center), generally thought of as an aeronautical flight-test facility in the 1960s, made a number of contributions to the NASA space program during that era as well.

For example, researchers explored the concept of paraglider landings for a space vehicle and the use of wingless spacecraft that could glide to precise landings, but it was the X-15 hypersonic research program and the Lunar Landing Research Vehicle that had the most direct impact on the Apollo missions to the Moon.

The North American Aviation X-15 rocket planes--designed to explore the problems of atmospheric and space flight at supersonic and hypersonic speeds--served as flying laboratories, carrying scientific experiments above the reaches of the atmosphere. Many research results from the X-15 program at Dryden Flight Research Center contributed directly to the success of the Apollo lunar missions, now being celebrated on the 40th anniversary of the first moon landing on July 20, 1969. North American – later North American Rockwell, then Rockwell International – served as prime contractor for both the X-15 and Apollo Command/Service Module spacecraft.

Designers of the Apollo CSM drew upon experience from the X-15 program, and even used the X-15 as a test bed for new materials. Advanced titanium and nickel-steel alloys developed for the X-15 were used in the Apollo and later spacecraft designs. The discovery of localized hot spots on the X-15, for example, led to development of a bi-metallic 'floating retainer' concept to dissipate stresses in the X-15's windshield. This technology was subsequently applied to the Apollo and space shuttle orbiter windshields.

The X-15's performance allowed researchers to accurately simulate the aerodynamic heating conditions that the Apollo Saturn rocket would face, and allowed full recovery of test equipment, calibration of results, and repeated testing where necessary. In 1967, technicians applied samples of cryogenic insulation--designed for use on the Apollo Saturn V second stage--to the X-15's speed brakes to test the material's adhesive characteristics and response to high temperatures.

X-15 re-entry experience and heat-transfer data were also valuable, and led to design of a computerized mathematical model for aerodynamic heating that was used in the initial Apollo design study. Lessons learned from X-15 turbulent heat-transfer studies contributed to the design of the Apollo CSM because designers found that they could build lighter-weight vehicles using less thermal protection than was previously thought possible.

Following the challenge by president John F. Kennedy in 1962 to land on the moon, two groups began working on a way to prepare astronauts for the critical descent and landing on the moon. The problems facing them were considerable: how to build a free-flying simulator that could negate 5/6ths of the Earth's gravity while entirely eliminating the effects of the atmosphere, since the moon had no atmosphere and only 1/6th of Earth's gravity.

Ideas for this unique type of flying machine had begun circulating at Dryden Flight Research Center, a year earlier. Center engineers initially didn't know that Bell Aircraft Company, later Bell Aerosystems, was also working on the task, but by the end of the year, the center had awarded a study contract to Bell. Bell was the only firm in the United States that had significant experience developing vertical takeoff aircraft using jet lift for takeoff and landing. After winning a contract from the center to design and build the machines in 1963, Bell delivered two Lunar Landing Research Vehicles or LLRVs--often called 'flying bedsteads' due to their ungainly appearance--to the Flight Research Center in 1964 for flight testing and development.

The LLRV had a jet engine hung vertically in the middle of the frame, fixed inside two gimbals, allowing the vehicle itself to rotate as much as 40 degrees in any direction while the jet remained vertically aligned. A series of hydrogen peroxide thrusters, eight around the frame's center and four at each corner, provided lunar simulation thrust that the pilot controlled.

Three analog computers took data on side forces and vehicle weight and produced just enough jet thrust so that, in lunar simulation, the LLRV descended as though in lunar gravity. Any gusts of wind were cancelled when the computers sensed them and fired thrusters to automatically cancel the wind. There were no mechanical links between the pilot and the engine or thrusters: everything was sent to the computers that, in turn, commanded the thrust desired.

During flight tests, a pilot directed the LLRV to climb about 300 feet, initiated lunar simulation mode, and then had less than eight minutes to complete a safe descent. Research flying over the next two-and-half years yielded a configuration suitable for astronaut training, and Bell subsequently built three similar craft--Lunar Landing Training Vehicles--that were sent to the Manned Spaceflight Center in Houston, now the Johnson Space Center. One of the LLRVs at the Flight Research Center was also sent to Houston for the training.

Apollo 11 commander Neil Armstrong recalled later that his landing on the moon on July 20, 1969 was a familiar job because of the LLTV’s authenticity.

As a side note, today's aircraft with fly-by-wire digital electronic control systems trace their lineage to the LLRV and its analog computers, and to the engineers who worked on that project. They cut their teeth on computer-controlled flight systems with the LLRV, allowing them the confidence to modify an F-8 jet fighter into the first aircraft with pure digital fly-by-wire electronic controls.

Partially restored by a movie company in the late 1990s, one of the two original Lunar Landing Research Vehicles remains on sheltered display today at NASA Dryden.

Mystery Source of Solar Wind Heating Identified

The solar wind, shown here in a plot of data from the Ulysses spacecraft, flows away from the sun at a million miles per hour and is heated by a turbulent cascade.The solar wind is hotter than it should be, and for decades researchers have puzzled over the unknown source of energy that heats it. In a paper published in the June 12 issue of Physical Review Letters, NASA scientists say they may have found the answer.

"The energy source is turbulence," says co-author Melvyn Goldstein, chief of the Geospace Physics Laboratory at NASA's Goddard Space Flight Center, Greenbelt, Md. "The sun heats the solar wind by stirring it up."

It's a bit like stirring your coffee--in reverse. When you stir your morning cup of Joe, the coffee cools off. But when the sun stirs the solar wind, the solar wind heats up.

The basic concept introduced by physicist Lewis Richardson in 1920.A true cascade of water and turbulence at the Iguazu Falls in Argentina.Jupiter's swirling Great Red Spot surrounded by turbulent swirls and eddies.Consider the coffee. When you stir it with a spoon, the stirring produces swirls and vortices in the liquid. The vortices fragment into smaller and smaller eddies until, at the smallest scales, the motions dissipate and the energy turns into heat. Because energy cascades down from the large swirls to the smaller ones, the process is called a turbulent cascade.

Theoretically, the turbulent cascade should heat the coffee. Real coffee cools off, however, because the act of stirring brings warm coffee from the depths of the cup into contact with cooler air above. Cool air absorbs the heat—the heat the coffee had to begin with plus the heat you added by stirring—and you can take a sip without scalding yourself.

But there is no cool air in space, and therein lies the difference between coffee and solar wind.

The sun stirs the solar wind with fast streams of gas that pour out of holes in the sun's atmosphere. Essentially, the solar wind stirs itself. The stirring produces swirls and eddies; larger eddies break into smaller ones, producing a cascade of energy that eventually dissipates as heat. The temperature shoots up and there is no cool air to stop it.

"We've suspected for years that turbulence heats the solar wind," says Fouad Sahraoui, lead author of the paper and a visiting NASA Fellow from the Centre National de la Recherche Scientifique (CNRS) in France. "Now we're getting detailed measurements of the process in action."

The key data came from a quartet of European spacecraft collectively known as Cluster, launched in 2000 to study the giant bubble of magnetism that surrounds Earth. The magnetosphere protects our planet from solar wind and cosmic rays. It contains the Van Allen radiation belts, auroras, and giant electrical "ring currents" of staggering power. Cluster spends much of its time inside the magnetosphere, where the spacecraft can study the wide variety of phenomena at work there.

One day in March 2006, the four spacecraft took a brief excursion outside the bubble into the solar wind. For three hours, their sensors made rapid-fire measurements of electromagnetic waves and turbulent eddies in the million-kilometer-per-hour gas flowing past them.

"That was when we made the discovery," says Goldstein. "Turbulent energy was cascading from large scale structures around 1,000,000 kilometers (621,400 miles) in size all the way down to structures as small as 3 kilometers (1.8 miles). At the small end of the cascade, energy was absorbed by electrons in the solar wind."

Sahraoui and Goldstein would like to confirm their findings and flesh out the details by sending Cluster back into the solar wind for more than "three lucky hours." But the basic result seems solid enough: Turbulent heating boosts the temperature of the solar wind near Earth from tens of thousands of degrees (the value theoreticians expect) to hundreds of thousands or more.

Goldstein says such turbulent heating probably happens in many other astrophysical situations, from stellar winds to planetary magnetospheres to black holes. There's even a down-to-Earth application: nuclear fusion reactors. Turbulence inside experimental fusion chambers can produce instabilities that destroy the confinement of the fusion plasma.

"The solar wind is a natural laboratory for understanding this physics," says Sahraoui, "and we are planning more observations to see how common the phenomenon might be."

Related Links:

Cluster – home page
http://sci.esa.int/science-e/www/area/index.cfm?fareaid=8

Cluster's insight into space turbulence – press release
http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=44480

The Solar Wind – a tutorial
http://solarscience.msfc.nasa.gov/SolarWind.shtml

Evidence of a Cascade and Dissipation of Solar-Wind Turbulence at the Electron Gyroscale, F. Sahraoui et al, Phys. Rev. Lett. 102, 231102 (2009)
http://scitation.aip.org/getabs/servlet/GetabsServlet?prog=normal&id=PRLTAO000102000023231102000001&idtype=cvips&gifs=yes

Apollo 11 40th Anniversary: Celebrating the 'Giant Leap'

Waste and Hygiene Compartment Status

Aboard the International Space Station, astronauts Mike Barratt and Frank De Winne will be replacing parts of the U.S. Destiny laboratory’s Waste and Hygiene Compartment, or WHC. The parts likely were contaminated earlier today when the system’s dose pump failed after running for about 15 minutes. The pump introduces the correct amount of chemicals into the system to help separate liquids from solid waste. About six liters of pre-treated water may have flowed into the pump separator and other areas it does not belong, flooding the separator.

Space Shuttle Mission: STS-127


Integrated Cargo Carrier
Crews Tackle Robotics, Prepare for Monday Spacewalk

The Space Shuttle Endeavour and International Space Station crews were successful in their robotic arm tasks today, but encountered a problem with one of the bathrooms on the station.

Robotic arm operators aboard Endeavour and the station installed the Integrated Cargo Carrier – Vertical Light Deployable, or ICC-VLD --- a cargo pallet--- on the port side of the space station’s mobile base system. Station arm operators Julie Payette and Tim Kopra finished the move at 12:55 p.m. EDT.

The pallet contains three hardware spares that spacewalkers Dave Wolf and Tom Marshburn will move to a stowage platform on the outside of the Port 3 truss during Monday’s spacewalk.

The Kibo robotic arm was commanded through a series of calibrations in preparation for later use in the mission, when Japan Aerospace Exploration Agency payloads will be transferred from the Exposed Section, another platform where the experiments are temporarily mounted, to the newly installed Exposed Facility for operation. The Exposed Facility was installed on the aft end of Kibo Saturday.

Wolf and Marshburn spent the remainder of their day preparing special tools, reviewing procedures and beginning their campout for the second spacewalk, which is set to start Monday at 11:28 a.m.

Meanwhile, station flight controllers and crew members spent part of the day troubleshooting a problem with the Waste and Hygiene Compartment, or WHC, the toilet in the U.S. Destiny module. The system’s dose pump failed after running for about 15 minutes Sunday. The pump introduces the correct amount of chemicals into the system to help separate liquids from solid waste. Expedition 20 flight engineers Mike Barratt and Frank De Winne began work on the toilet to replace parts that likely were contaminated.

The WHC is one of two toilet systems aboard the space station. Temporarily, the six station crew members will use the facilities in the Russian Zvezda module while the seven Endeavour astronauts will use the shuttle Waste Compartment System, or WCS, that is located in Endeavour’s middeck.

The temporary shutdown of the U.S. toilet on the station will not impact joint docked operations.

› Read more

STS-127 Additional Resources
› Mission Press Kit (6.9 Mb PDF)
› Mission Summary (429 Kb PDF)
› Meet the STS-127 Crew

Saturday, July 18, 2009

Apollo 11 Overview


NASA’s Unmanned Aircraft 'Fired Up' For Arctic Sea Ice Expedition

The Science Instrumentation Environmental Remote Research Aircraft (SIERRA), an unmanned aircraft system used in the CASIE mission.Scientists using 2009 NASA satellite data have reported a rapid and extreme loss of the oldest and thickest types of ice from within the Arctic Ocean. Since 1988, the oldest ice types have declined 74 percent and today cover only two percent of the Arctic Ocean, compared to 20 percent coverage in the 1980s.

A team of experts from NASA, the University of Colorado, Boulder, Brigham Young University, Provo, Utah, Fort Hays State University, Kansas and the National Center for Atmospheric Research, Boulder, Colorado are conducting an unmanned aircraft expedition to study the receding Arctic sea ice to better understand its life cycle and the long-term stability of the Arctic ice cover.

"We’re attempting to answer some of the most basic questions regarding the future of the Arctic’s sea ice cover," said James Maslanik, a research professor at the University of Colorado at Boulder, Colo., and principal investigator for the NASA mission. "Not only does this change affect the total amount of ice in the Arctic, but it also affects the ability of the ice cover to resist increased warming."

Today, NASA's Characterization of Arctic Sea Ice Experiment (CASIE) successfully flew the first of a series of unmanned aircraft system (UAS) flights in coordination with satellites. The UAS is used like a miniature spyplane targeting thick, old slabs of ice as they drift from the Arctic Ocean south through Fram Strait -- which lies between Greenland and Svalbard, Norway -- into the North Atlantic Ocean. This unmanned aircraft maps and measures ice conditions below cloud cover to as low as 300 feet, weaving a pattern over open ocean and sea ice.

NASA’s CASIE, which runs through July 24, is the aircraft campaign portion of the larger, NASA-funded project titled “Sea Ice Roughness as an Indicator of Fundamental Changes in the Arctic Ice Cover: Observations, Monitoring, and Relationships to Environmental Factors. This three -year research effort combines satellite data analysis, modeling, and aircraft observations. The project also supports the goals of the International Polar Year, a major international scientific research effort involving many NASA research efforts to study large-scale environmental change in Earth's polar regions.

The mission is being conducted from the Ny-Alesund research base on the island of Svalbard, located near the northeastern tip of Greenland. Mission planners are using satellite data to direct weekly flights of a NASA flight-certified UAS laden with scientific instruments.

Aircraft provide a necessary perspective on Earth system processes and serve to complement NASA satellite missions. UAS are of particular value where long duration or long range measurement requirements preclude a human pilot, or where the remoteness and harshness of the environment put pilots and aircraft at risk.

NASA Ames Research Center’s Science Instrumentation Evaluation Remote Research Aircraft, or SIERRA, is a medium class, medium duration UAS originally designed by the Naval Research Laboratory (NRL). Researchers at NASA Ames Research Center, Moffett Field, Calif. developed a partnership with NRL to evaluate the utility of this class of aircraft to the NASA Earth science community. The relatively large payload (appproximately 100 lbs.) coupled with a significant range (500 miles) and small size (20-ft. wingspan) makes it an attractive observational platform that complements NASA’s current suite of modified science aircraft. This UAS conducts very low altitude missions for tropospheric chemistry sampling and remote area surveys, such as arctic ice reconnaissance.

"Today, we demonstrated the utility of small to medium class UAS for gathering science data in remote harsh environments during the CASIE mission," said Matt Fladeland, CASIE project and SIERRA manager.

UAS observations are complemented by NASA satellite large-scale views of many different features of the Arctic ice. The Moderate Resolution Imaging Spectroradiometer (MODIS), aboard NASA's Aqua satellite, will be used to identify the ice edge location, ice features of interest, and cloud cover. Other sensors, such as the Advanced Microwave Scanning Radiometer - Earth Observing System (AMSR-E) on NASA’s Aqua satellite and the Quick Scatterometer (QuikSCAT) can penetrate cloud cover and analyze the physical properties of ice. By using multiple types of satellite products, more can be learned about ice conditions than is possible by using one or two data analysis methods.

"Ny-Alesund is really a cool research station with more than 100 researchers present from many nations during the summer,” said S. Pete Worden, director of NASA Ames Research Center. “It was a great day for flying here in Ny-Alesund. We got SIERRA out on the runway and fired up and ready for our first flight. We are really excited about the research we can do on polar ice characteristics."

The CASIE expedition is providing mission updates on Twitter and Blogs at:

http://blogs.nasa.gov/cm/blog/CASIE

http://twitter.com/NASA_CASIE

For more information about NASA's Characterization of Arctic Sea Ice Experiment, visit:

http://www.espo.nasa.gov/casie/

Some Shovels of Dirt Ring in NASA Langley's Future

With a push of her right foot on a shovel Friday morning, Lesa Roe celebrated the 92nd birthday of NASA's Langley Research Center by ushering in its future.

Helping Roe, Langley's center director, in breaking ground for New Town Building 1 were Hampton Mayor Molly Ward; Rob Hewell, from the General Services Administration, and Charles Scales, NASA associate deputy administrator.

New Town groundbreaking.
"We've waited and budgeted and planned for this day with a great deal of anticipation," Roe said. "New Town focuses on the future requirements of the center while maintaining our tradition of technical excellence."

The building will be the first of six in the project, which is expected to be constructed over 15 years. The six will include three laboratories, a second office building and a joint-use facility.

Groundbreaking for Building 2 is expected in 2011.

Building 1 will house administrative offices in a three-story, $23 million, 72,000-square-foot structure built with an accent on environmental soundness. Construction will be aimed at the U.S. Green Building Council's Leadership in Energy and Environmental Design (LEED) standards.

NASA construction requires "silver" status on a LEED certified, silver, gold, platinum scale. Building 1 is expected to attain "gold" in a review that will follow its completion.

Much of that rating will be generated by a building that will save approximately 85 percent of energy costs associated with a similar structure not built with conservation and cost consciousness in mind.

"The geothermal system is the big one," said Tom Quenville, who has nursed the New Town project along since 2004. "It has an underground heating and cooling system. … You're basically using the energy in the ground to heat and cool the building.

"And the 'green' roof is also new for us. We have all of these firsts for Langley: the first green roof, the first geothermal system."

The "green" roof will involve plants that will be grown on the top of the building to insulate it from the sun and hold in water.

The building also will have photo-voltaics on its roof to provide power. Better insulation and energy-efficient windows add to that environmental friendliness.

The 85 percent savings are based on a building model. An average building is said to use about 200,000 BTUs of energy per square foot per year. "Our building will be 29,000 BTUs per square foot," Quenville said.

Guests were effusive in their praise of the New Town concept.

"Welcome to the beginning of Langley's future," Scales told the assembly of about 200 under a tent on the building site along Langley Boulevard.

"One of the legacies of space exploration has been the focus that has been put back on Earth. We have learned just how fragile Earth is, so we need to do everything that we can to make sure that we take care of it. This new facility will help toward that."

Hewell lauded the companies involved, including Whiting-Turner, which is the prime contractor for Building 1.

Ward cited Langley's contribution to her city and the region, then later pointed to the national and local economies.

"It's exciting in these economic times to see something coming out of the ground," she said. "We're excited about the 'green' building technology.

"And we're excited about what it means for the future of Langley Research Center and for the investment the government is making here that shows a commitment to the center and to Hampton."

For Roe, New Town is the culmination of an effort that has been ongoing since she became center director five years ago. At that time, jobs were being lost and rumors ran rampant that the center's future was in jeopardy.

"This is a far cry from that," Roe said of New Town's benchmark status for a bright future for the center. "It means a lot. It's great for morale. It just brings excitement! And it's the first of these and the second one is on the way."

Cronkite Remembered for Coverage of Apollo Launches

Walter Cronkite. Credit: CBS/NASANASA fondly remembers veteran broadcast journalist Walter Cronkite who died July 17 at his home. › Read More › Neil Armstrong's Statement | › Administrator Bolden's Statement | › Video: Cronkite on Apollo 11 | › Photo Gallery

Spacewalkers Camping Out in Airlock; Station Steering Clear of Debris

A minor reboost of the International Space Station will be performed at NASA Space Station 8:27 p.m. EDT to ensure plenty of clearance in relation to an unknown piece of space station debris. That maneuver using Endeavour’s small vernier thrusters will last about 15 minutes and change the overall velocity of the shuttle/station complex by about 0.8 meter per second.

Spacewalkers of NASA Space station Dave Wolf and Tim Kopra will begin their “campout” at 9:28 p.m., spending the night in the Quest airlock to reduce the preparation time needed for the mission’s first spacewalk on Saturday. The International space station crew is scheduled to go to bed at about 10:30 p.m. and the space shuttle mission crew 30 minutes later at 11. Wake up for both crews Saturday is scheduled for 7:03 a.m.

International Space Shuttle Mission: STS-127


S127-E-006351 -- Space Shuttle Endeavour
International Space, Shuttle, Station Crews Begin 11 Days of Joint Operations

The International space shuttle and space station mission Endeavour docked with the International Space Station at 1:47 p.m. EDT, delivering the final pieces of the Japanese Kibo complex and a new flight engineer to join the Expedition 20 crew.

Nasa space station Endeavour Commander Mark Polansky guided the space shuttle to a docking as the two aircraft flew 220 miles about the northern coast of Australia. Before closing the final 600 feet to the international space station, Polansky commanded Endeavour through a “backflip” allowing the space station’s Expedition 20 Commander Gennady Padalka and Flight Engineer Michael Barratt to take photos that imagery experts will review to assess the health of Endeavour’s heat shield.

The space shuttle and space station crews opened hatches and greeted one another at 3:48 p.m., beginning more than a week of joint operations between the two crews. One of the first major tasks of the space station crews was to swap station crew member Koichi Wakata for NASA space station astronaut Tim Kopra.

The official swap occurred when a specially fitted seat liner was installed in the Soyuz crew vehicle. That swap at 5:22 p.m. signified the official designation change making Kopra an Expedition 20 flight engineer and Wakata a space station as well as shuttle mission specialist.

STS-127 Additional Resources

› Mission PressKit (6.9 Mb PDF)
›Mission Summary (429 Kb PDF)
›Meet the STS-127 Crew

Bolden Takes the Helm at NASA

Charles F. Bolden, Jr. enters the Administrator's office at NASA Headquarters on Friday, July 17. Lori B. Garver will serve as Deputy Administrator.

Bolden enters the NASA Administrator's office to start his first day. Credit: NASA, Bill Ingalls