29 Oct 2014

NASA’s Wallops Flight Facility Completes Initial Assessment after Orbital Launch Mishap

Wallops launch pad looking south after launch failure
An aerial view of the Wallops Island launch facilities taken by the Wallops Incident Response Team Oct. 29 following the failed launch attempt of Orbital Science Corp.'s Antares rocket Oct. 28.
Image Credit: 
NASA/Terry Zaperach
The Wallops Incident Response Team completed today an initial assessment of Wallops Island, Virginia, following the catastrophic failure of Orbital Science Corp.’s Antares rocket shortly after liftoff at 6:22 p.m. EDT Tuesday, Oct. 28, from Pad 0A of the Mid-Atlantic Regional Spaceport at NASA’s Wallops Flight Facility in Virginia.
“I want to praise the launch team, range safety, all of our emergency responders and those who provided mutual aid and support on a highly-professional response that ensured the safety of our most important resource -- our people,” said Bill Wrobel, Wallops director. “In the coming days and weeks ahead, we'll continue to assess the damage on the island and begin the process of moving forward to restore our space launch capabilities. There's no doubt in my mind that we will rebound stronger than ever.”
The initial assessment is a cursory look; it will take many more weeks to further understand and analyze the full extent of the effects of the event. A number of support buildings in the immediate area have broken windows and imploded doors. A sounding rocket launcher adjacent to the pad, and buildings nearest the pad, suffered the most severe damage.
At Pad 0A the initial assessment showed damage to the transporter erector launcher and lightning suppression rods, as well as debris around the pad.
The Wallops team also met with a group of state and local officials, including the Virginia Department of Environmental Quality, the Virginia Department of Emergency Management, the Virginia Marine Police, and the U.S. Coast Guard.
The Wallops environmental team also is conducting assessments at the site. Preliminary observations are that the environmental effects of the launch failure were largely contained within the southern third of Wallops Island, in the area immediately adjacent to the pad. Immediately after the incident, the Wallops’ industrial hygienist collected air samples at the Wallops mainland area, the Highway 175 causeway, and on Chincoteague Island. No hazardous substances were detected at the sampled locations.
Additional air, soil and water samples will be collected from the incident area as well as at control sites for comparative analysis.
The Coast Guard and Virginia Marine Resources Commission reported today they have not observed any obvious signs of water pollution, such as oil sheens. Furthermore, initial assessments have not revealed any obvious impacts to fish or wildlife resources. The Incident Response Team continues to monitor and assess.
Following the initial assessment, the response team will open the area of Wallops Island, north of the island flagpole opposite of the launch pad location, to allow the U.S. Navy to return back to work.
Anyone who finds debris or damage to their property in the vicinity of the launch mishap is cautioned to stay away from it and call the Incident Response Team at 757-824-1295.
Further updates on the situation and the progress of the ongoing investigation will be available at:
and
-end-

NASA’s LRO Spacecraft Captures Images of LADEE’s Impact Crater

NASA’s LRO Spacecraft Captures Images of LADEE’s Impact Crater
October 28, 2014
Before and After Images: 
handle
Caption: 
These images show the area of the LADEE impact before and after spacecraft's planned impact into the eastern rim of Sundman V crater. Use the slider to switch between images.
Image Credit: 
NASA/Goddard/Arizona State University
NASA’S Lunar Reconnaissance Orbiter (LRO) spacecraft has spied a new crater on the lunar surface; one made from the impact of NASA’s Lunar Atmosphere and Dust Environment Explorer (LADEE) mission.
“The Lunar Reconnaissance Orbiter Camera (LROC) team recently developed a new computer tool to search Narrow Angle Camera (NAC) before and after image pairs for new craters, the LADEE impact event provided a fun test, said Mark Robinson, LROC principal investigator from Arizona State University in Tempe. “As it turns there were several small surface changes found in the predicted area of the impact, the biggest and most distinctive was within 968 feet (295 meters) of the spot estimated by the LADEE operations team. What fun!”
The LADEE mission ended on April 18, 2014, with the spacecraft’s planned impact into the eastern rim of Sundman V crater on the far side of the moon.
LRO has imaged the LADEE impact site on the eastern rim of Sundman V crater.
LRO has imaged the LADEE impact site on the eastern rim of Sundman V crater. The image was created by ratioing two images, one taken before the impact and another afterwards. The bright area highlights what has changed between the time of the two images, specifically the impact point and the ejecta.
Image Credit: 
NASA/Goddard/Arizona State University
Artist concept of the Lunar Reconnaissance Orbiter with Apollo mission imagery of the moon in the background.
Artist concept of the Lunar Reconnaissance Orbiter with Apollo mission imagery of the moon in the background.
Image Credit: 
NASA's Goddard Space Flight Center
An artist's concept of NASA's Lunar Atmosphere and Dust Environment Explorer (LADEE) spacecraft seen orbiting near the surface of the moon.
An artist's concept of NASA's Lunar Atmosphere and Dust Environment Explorer (LADEE) spacecraft seen orbiting near the surface of the moon.
Image Credit: 
NASA Ames/Dana Berry
LADEE's engines fired April 11, 2014, to perform a final orbital maintenance maneuver and adjust to guarantee it would impact on the farside of the moon and away from the Apollo landing sites. Over a seven-day period, LADEE's orbit decreased and the spacecraft orbited very low to the surface and close to the walls of lunar craters and mountain ridges to give the team a chance to collect valuable science data. Finally, LADEE impacted the eastern rim of Sundman V crater on April 18. The impact site is about half a mile (780 meters) from the crater rim with an altitude of about 8,497 feet (2,590 meters) and was only about two tenths of a mile (300 meters) north of the location mission controllers predicted based on tracking data.
The impact crater is small, less than ten feet (three meters) in diameter, barely resolvable by the LROC NAC. The crater is small because the spacecraft -- compared to most celestial impacts -- was not traveling very fast, approximately 3,800 miles per hour (1,699 meters per second) and had a low mass and a low density. The size of the impact crater made it hard to identify among the myriad of small fresh craters on the lunar surface. Images acquired of the impact region before the impact, were compared with images obtained after the impact to identify the crater.
Since the NAC images are so large (250 mega-pixels) and the new crater is so small, the LROC team co-registered the before and after images (called a temporal pair) and then divided the before image by the after image. By doing this, changes to the surface become evident.
The ejecta from the impact forms a triangular pattern primarily downrange to the west, extending about 656-984 feet (200-300 meters) from the impact site. There is also a small triangular area of ejecta up range but it extends only about 66-98 feet (20-30 meters). The ejecta pattern is oriented northwest, consistent with the direction the spacecraft was traveling when it impacted the surface.
"I'm happy that the LROC team was able to confirm the LADEE impact point," said Butler Hine, LADEE project manager at Ames Research Center in Moffett Field, California. "It really helps the LADEE team to get closure and know exactly where the product of their hard work wound up."
LADEE launched Sept. 6, 2013 from Pad 0B at the Mid-Atlantic Regional Spaceport, at NASA's Wallops Flight Facility, Wallops Island, Virginia. LADEE gathered detailed information about the structure and composition of the thin lunar atmosphere and determining whether dust is being lofted into the lunar sky.
LRO launched September 18, 2009. LRO continues to bring the world astounding views of the lunar surface and a sizable collection of lunar data for research.
LRO recently received a second two-year extended mission. Under the extended mission, LRO will study the seasonal volatile cycle; determine how many small meteorites are currently hitting the moon and their effects; characterize the structure of the lunar regolith; investigate the moon’s interaction with the space environment; and reveal more about the lunar interior using observations of the moon’s surface.
“With LRO, NASA will study our nearest celestial neighbor for at least two more years,” said John Keller, LRO project scientist from NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “LRO continues to increase our understanding of the moon and its environment.”
NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the LRO mission. NASA's Ames Research Center in Moffett Field, California, designed, built, tested and managed operations for the LADEE mission.
For information on LRO, visit: http://www.nasa.gov/lro
For more information on LROC, visit: http://lroc.sese.asu.edu

It’s Anchors Aweigh on Modifications to NASA’s Pegasus Barge

It’s Anchors Aweigh on Modifications to NASA’s Pegasus Barge
October 28, 2014
NASA’s Pegasus barge, shown transporting the external tank during the space shuttle era, is now undergoing major modifications required to carry the core stage of the Space Launch System for testing and launch.
NASA’s Pegasus barge, shown transporting the external tank during the space shuttle era, is now undergoing major modifications required to carry the core stage of the Space Launch System for testing and launch.
Image Credit: 
NASA
Crews at Conrad Shipyard LLC in Morgan City, Louisiana, are building a new, 165-foot section for the Pegasus barge, which will lengthen the vessel from 260 feet to 310 feet.
Crews at Conrad Shipyard LLC in Morgan City, Louisiana, are building a new, 165-foot section for the Pegasus barge, which will lengthen the vessel from 260 feet to 310 feet.
Image Credit: 
NASA/Steven Seipel
It’s anchors aweigh on refurbishments to NASA’s Pegasus barge, which will be used to ferry the massive core stage of America’s next great ship -- the Space Launch System.
SLS will be the most powerful rocket ever built for deep space missions, including to an asteroid and ultimately to Mars. The core stage, towering more than 200 feet tall with a diameter of 27.6 feet, will store cryogenic liquid hydrogen and liquid oxygen that will feed the vehicle’s RS-25 engines.
The core stage is made up of five parts: the engine section, liquid hydrogen tank, intertank, liquid oxygen tank and forward skirt. Work is currently underway at NASA's Michoud Assembly Facility in New Orleans to build the core stage using state-of-the-art welding techniques and machinery.
During the space shuttle era, Pegasus was used to carry shuttle external tanks and other hardware from Michoud to NASA’s Kennedy Space Center in Florida.
"Modifications were needed to the barge due to the sheer size of the SLS -- which is more than 50 feet taller than the shuttle, and will launch more than three times as much weight into space," said Alan Murphy, team lead for the Pegasus project at NASA’s Marshall Space Flight Center in Huntsville, Alabama. "The core stage is 59 feet longer and more than 500,000 pounds heavier, including the ground support equipment, than the space shuttle external tank. The modification work is on schedule, and we look forward to seeing the barge back in the water for a new era of exploration."
Pegasus -- housed since 2011 at NASA’s Stennis Space Center near Bay St. Louis, Mississippi -- is now docked at Conrad Shipyard LLC in Morgan City, Louisiana. Conrad will perform all necessary modifications and refurbishments to ensure the restored vessel meets American Bureau of Shipping standards, including load line certification, or verification of the barge's legal loading limit to safely maintain buoyancy during water travel.
The Corps of Engineers’ Marine Design Center in Philadelphia, Pennsylvania -- utilizing the engineering expertise of Bristol Harbor Group of Bristol, Rhode Island -- is performing the architecture and engineering work for the barge modification, as well as managing the Conrad contract.
Conrad crews are currently building a new, 165-foot center section for the barge. The modifications will bring the total length of the barge from 260 feet to 310 feet -- a little more than the length of a football field. A 115-foot center section of the existing barge will be removed and the new piece installed later this fall. Work is expected to be completed in early 2015.
Once the modifications are complete, the Pegasus will be stationed at Michoud for operational readiness and maintenance. The first planned set of voyages for the Pegasus will be from Michoud to the Marshall Center to deliver the core stage structural test articles for testing to ensure that these huge structures can withstand the incredible stresses of launch.
The barge also will deliver the flight core stage from Michoud to Stennis, where it will be tested in late 2016 and early 2017 on the B-2 test stand. The core stage will be installed on the stand -- currently undergoing its own modifications -- for propellant fill and drain testing and a hot fire test.
Once testing is complete at Stennis, the Pegasus will transport the core stage to Kennedy Space Center for preparation and integration into the SLS flight vehicle in the Vehicle Assembly Building.
The first flight test of the SLS will be configured for a 70-metric-ton (77-ton) lift capacity and carry an uncrewed Orion spacecraft beyond low-Earth orbit to test the performance of the integrated system. As the SLS evolves, it will be the most powerful rocket ever built and provide an unprecedented lift capability of 130 metric tons (143 tons) to enable missions even farther into our solar system.
For more information on SLS, visit:
Shannon Ridinger
Marshall Space Flight Center, Huntsville, Ala.

It's Alive! Ames Engineers Harvest and Print Parts for New Breed of Aircraft

It's Alive! Ames Engineers Harvest and Print Parts for New Breed of Aircraft
October 27, 2014
3-D printed wing part
3-D printed wing part for the FrankenEye aircraft.
Image Credit: 
NASA/Ames/Dominic Hart
It's more an engineer's dream than nightmare - to rapidly prototype and redesign aircraft using 3-D printed parts. That's just what a team of student interns and engineers at NASA's Ames Research Center in Moffett Field, California, got to do: custom-build aircraft by repurposing surplus Unmanned Aerial Vehicles (UAVs). Grafting fuselages side-by-side adds more motors, propellers and batteries to improve power and performance capacity. By lengthening the wings, the team was able to improve aerodynamic efficiency and help extend the flight time of small, lightweight electric aircraft. 
The prototype aircraft are constructed using components from Aerovironment RQ-14 Dragon Eye UAVs that NASA acquired from the United States Marine Corps via the General Services Administration's San Francisco office. Unmodified, these small electric aircraft weigh 5.9 pounds, have a 3.75-foot wingspan and twin electric motors, and can carry a one-pound instrument payload for up to an hour. NASA can use these Dragon Eyes to penetrate the dangerous airspace within the plume of the volcanoes because their electric motors do not ingest and are not affected by the contaminated air. The Dragon Eyes are proving to be an effective way to gather crucial data about volcanic ash and gas emissions. 
The team – comprised of full-time students and summer interns from Stanford University, University of California (UC) Los Angeles, UC Santa Cruz, UC Davis, Virginia Polytechnic Institute and Northeastern University, as well as Ames engineers – modified Dragon Eyes by harvesting spare parts from other Dragon Eyes and reassembling them along with specially designed 3-D manufactured parts to create new aircraft the team dubbed “FrankenEye.” 
The NASA team created the name FrankenEye to reference "Frankenstein." The student teams participating in summer activities harvested parts from surplus aircraft and reanimated them using new 3-D printed parts with the goal of increasing payload capacity and endurance for use in Earth Science missions.
Ames engineers work on the FrankenEye aircraft
Engineers at NASA's Ames Research Center in Moffett Field, California, build the FrankenEye aircraft.
Image Credit: 
NASA/Ames/Dominic Hart
"We essentially created two entirely new machines," said Kevin Reynolds, principal investigator of the FrankenEye project at Ames. "We worked alongside a group of students to rapidly prototype, manufacture, test and demonstrate key capabilities in preparation for next year's volcano plume-sampling field work." 
The FrankenEye project team used 3-D printers at Ames and Stanford to create prototypes and make conceptual models. The donated stock UAVs did not come with any blueprints so 3-D scanning technology was essential to design the interface to existing hardware, and create mechanical drawings. After finalizing designs that featured longer and more slender wings and dual fuselages, the teams printed new parts including wing sections, nose cones, winglets, control surfaces, wing ribs and even propellers using the NASA Ames SpaceShop. The 3-D printed wing sections were reinforced using carbon fiber tubing or aluminum rods to give them extra strength without adding significant weight.
"The more weight we carry in material is less weight we can carry in sensors or batteries," said Reynolds. "Dragon Eyes can fly approximately one hour using the existing lithium-ion battery. But with two fuselages – meaning two batteries – and a more efficient wing design that allows it to fly slower and conserve energy, our variants can fly up to three times as long using electric power."
Within two months, the student interns also customized open source flight and navigation software to conduct nine test flights of two variants of modified aircraft named "Chimera" and "Alicanto" at Stanislaus County's Crows Landing Facility in California. The teams demonstrated the ability of their aircraft to take off autonomously, navigate through a series of waypoints, enter into a glide and land at a predetermined location without pilot intervention. 
"This project is very exciting for us because it has demonstrated a new capability for quickly and inexpensively modifying existing aircraft to tailor them to specific mission goals," said Matt Fladeland, Ames co-investigator on the FrankenEye and Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) validation projects. “In this case the modified aircraft will be able to stay up longer while carrying more science payload over the volcano." 
The Costa Rican Airborne Research and Technology Application 2015 mission will be the latest in a series of deployments of small unmanned aircraft (UAVs), led by David Pieri, volcanologist at NASA’s Jet Propulsion Laboratory in Pasadena, California, and is supported by the NASA Earth Surface and Interior Focus Area, the ASTER Mission and a consortium of NASA centers, including Ames, NASA's Goddard Space Flight Center in Greenbelt, Maryland and NASA's Wallops Flight Facility in Wallops Island, Virginia and the agency's Glenn Research Center in Cleveland, as well as the University of Costa Rica (CICANUM) GasLab.
Flying as high as 12,500 feet above sea level, multiple small converted Dragon Eye UAVs, including the specialized and highly modified “FrankenEye” platform, will study the chemistry of the eruption plume emissions from Turrialba volcano, near San Jose, Costa Rica. 
The goal of the activity is to improve satellite data research products, such as computer models of the concentration and distribution of volcanic gases, and transport-pathway models of volcanic plumes. Some volcanic plumes can reach miles above a summit vent, and drift hundreds to thousands of miles from an eruption site and can pose a severe public heath risk, as well as a potent threat to aircraft.
"The use of UAVs to carry out potentially hazardous sampling of volcanic gas emissions sharply reduces risk to volcano researchers," said Pieri. "Such data also will be used to help mitigate risk for people living on or near active volcanoes and for passengers and crews flying over them."
Three Dragon Eye aircraft on a hillside waiting for deployment
During the 2013 research flights, scientists from NASA Ames prepare Dragon Eye UAVs to study the plume above the Turrialba Volcano in Costa Rica.
Image Credit: 
NASA/Randy Berthold
The project directly supports the current Terra and ASTER missions and NASA's planned Hyperspectral Infrared Imager (HyspIRI) mission by improving satellite data-based observations of gases and aerosols associated with volcanic activity as well as volcanic emission transport models.
Turrialba was chosen because the continuously-erupting volcano has a relatively minimal updraft and wind shear with minimal ash content. In addition, commercial and private air traffic is very infrequent in the airspace around and over Turrialba volcano.
During the research flights in 2013, the team coordinated its data gathering with the ASTER instrument on NASA's Terra spacecraft, allowing scientists to compare sulfur dioxide concentration measurements from the satellite with measurements taken from within the plume. 
Through the fall, the FrankenEye project will continue to develop the aircrafts' capabilities by focusing on sensor integration and a larger triple-fuselage design. This research effort seeks to show that FrankenEye is more than the sum of its parts and can be optimized to be more capable than its individual units.
Next spring, members of the FrankenEye team will witness their creations take flight over Turrialba volcano. Working alongside NASA Earth science researchers, they will fly the aircraft over and into the volcano's sulfur dioxide plume. Scientists believe computer models derived from this study will help safeguard the National and International Airspace System, improve global climate predictions, and mitigate environmental hazards (e.g., sulfur dioxide containing volcanic smog or "vog") for people who live around volcanoes.