Showing posts with label NASA news. Show all posts
Showing posts with label NASA news. Show all posts

Thursday, October 22, 2020

NASA COVID-19 Testing Request for Information / Sources Sought Notice

NASA is looking at strategies for testing employees in the course of executing essential and / or mission critical agency activities, to include:

Travel Related Testing- Many countries, and even some states and private companies, are requiring a test 72 hours prior to travel. Several countries are requiring this test to be a polymerase chain reaction (PCR) test, due to the higher sensitivity.

Mission Related Testing- In the course of keeping critical personnel safe and preventing a mission impact, it is becoming increasingly necessary to test personnel who have access to the astronauts (trainers, rescue personnel, etc). It is also becoming necessary to maintain the vigilance and safety of NASA critical operations.

Employees Identified in a Case Tracing at Work- If the employee was exposed in the course of doing work, they may require testing both to ensure the safety of their family, in accordance with public health strategies for quarantine, and to identify those critical workers that may need to return to work if un-infected.

Employees Returning from Foreign Travel- Prolonged exposures in a commercial aircraft, multiple social contacts in the course of doing business abroad, reliance of outside vendors for food and transport, all may put employees at increased risk for infection especially if they were in areas where the viral cases are endemic or increasing.

The Agency Office of the Chief Medical Officer has determined that the polymerase chain reaction (PCR) test has the broadest application for those undertaking travel, those working critical operations, those identified in a workplace case tracing, and those returning from overseas travel. NASA is seeking a provider that is able to provide nationwide service in which PCR is the method of testing.

Tuesday, May 26, 2020

FAA post flight restrictions around Cape Canaveral for historic manned space launch

The Federal Aviation Administration (FAA) has issued multiple Notice to Airmen (NOTAMS) Temporary Flight Restrictions around Cape Canaveral, Fla., through Wednesday.

The NOTAMS are in preparation for NASA’s historic manned space flight to the International Space Station aboard the SpaceX Crew Dragon capsule. This is the first launch of astronauts to Earth orbit on an American-built spacecraft from American soil since 2011.

“The FAA’s role is to ensure the safety of the airspace by prohibiting all aircraft operations within 30 nautical miles of NASA’s Kennedy Space Center during the reported timeframe unless the operation is exempted,” the agency said on Tuesday. “There are three types of NOTAMs: airspace, to close the airspace near the launch; flow, to provide route guidance to aviation operators; and security, to implement security measures for aircraft and Unmanned Aircraft Systems (UAS) in the area."

Aircraft operations involving UAS, flight training, aerobatic, glider, seaplane, parachute, ultralight, hang gliding, balloon, agriculture/crop dusting and more are prohibited. 

Pilots who do not comply with the requirements, special instructions or procedures in the NOTAM may be intercepted, detained by law enforcement, and subjected to any of the following additional actions: 
  • Civil penalties and the suspension or revocation of airmen certificates; or  
  • Criminal charges, including charges under Title 49 of the United States Code, Section 46307; or  
  • The U.S. Government may use deadly force against the airborne aircraft, if it is determined that the aircraft poses an imminent security threat.

Sunday, May 17, 2020

Super-secret military spaceplane in Earth orbit once again

A United Launch Alliance (ULA) Atlas V 501 rocket carrying the Air Force's X-37B Orbital Test Vehicle (OTV-6) lifted off on Sunday at 9:14 a.m. EDT, from Space Launch Complex-41. This marks the 84th successful launch of an Atlas V rocket. This is the sixth flight of the X-37B. Details of the mission are classified.

Along with OTV-6, this mission deployed FalconSat-8, a small satellite developed by the U.S. Air Force Academy and sponsored by the Air Force Research Laboratory to conduct experiments on orbit. The mission also carried two NASA experiments, including a material sample plate to determine the results of radiation and other space effects on various materials, and an experiment which will assess space effects on seeds used to grow food. Another experiment sponsored by the Naval Research Laboratory will examine the ability to transform solar power into radio frequency microwave energy which could be transmitted to the ground.

ULA's next launch is NASA's Mars 2020 mission carrying the Perseverance rover on an Atlas V rocket. The launch is scheduled for July 17 from Space Launch Complex-41 at Cape Canaveral Air Force Station, Fla.

Thursday, May 14, 2020

Military X-37B ready for sixth flight in space

A United Launch Alliance Atlas V 501 rocket is scheduled to launch the USSF-7 mission for the U.S. Space Force from Space Launch Complex-41 on Sunday at 9:14 a.m. EDT. This launch will mark the sixth flight of the X-37B Orbital Test Vehicle (OTV-6).

Along with OTV-6, the mission will deploy FalconSat-8, a small satellite developed by the U.S. Air Force Academy and sponsored by the Air Force Research Laboratory to conduct experiments on orbit. The mission also carries two NASA experiments, including a material sample plate to determine the results of radiation and other space effects on various materials. Another NASA experiment will assess space effects on seeds used to grow food. Another experiment sponsored the Naval Research Laboratory will examine the ability to transform solar power into radio frequency microwave energy which could be transmitted to the ground.

The Atlas V 501 rocket will use a five-meter-diameter payload fairing for this mission. The Atlas is powered by the RD AMROSS RD-180 engine, and the Centaur upper stage is powered by the Aerojet Rocketdyne RL10C-1 engine. This will be the 84th launch of an Atlas V rocket and the seventh launch of the 501 configuration. The Atlas V 501 has been used exclusively for national security missions.

Saturday, May 9, 2020

The mighty RS-25 rocket engine

NASA's Marshall Space Flight Center intends to buy 18 additional RS-25 rocket engines from Aerojet Rocketdyne in Canoga Park, Calif., to support the agency's new Space Launch System (SLS). The estimated value of this proposed action is $2.2 billion with an estimated period of performance from date of execution through July 15, 2028.

“RS-25” is the generic designation for the staged combustion, liquid hydrogen/liquid oxygen rocket engine system previously known as the Space Shuttle Main Engine (SSME) and it is the established core stage engine for the new SLS rocket. This proposed effort will be based on a previously existing production line for an engine system with thirty years of human spaceflight history. It is not a new engine development effort. The purchase of 18 additional RS-25s will fullfill the SLS Program engine requirements that are beyond the scope and the period of performance of the current contract, which provides six RS-25 flights engines with a period of performance through Sept. 30, 2024.

The new SLS vehicle uses a “stage-and-a-half” configuration that ignites the four core stage engines seconds before liftoff and then ignites the solid motors (boosters) at liftoff. The boosters burn out approximately two minutes into the flight while the core stage engines continue to burn until the desired cutoff point is achieved. This basic configuration is flexible for both early demonstration flights and for ultimately evolving the SLS vehicle to a configuration with a capability to lift 130 metric tons to low-earth orbit in support of future exploration missions.

NASA's strategy for minimizing the cost for development of the new SLS vehicle is to leverage the assets, capabilities and experience of the Space Shuttle Program. Early SLS flights will utilize 16 RS-25 engines from the Space Shuttle Program with necessary refurbishment and adaptations for SLS. The availability of 16 flights assets was one factor in selecting the RS-25 for the SLS architecture along with the demonstrated performance and extensive experience with this engine. These 16 assests can be used for the first four flights of SLS, with four engines per stage.

In addition to the 16 engines, six new engines were previously procured under the current contract to provide engines for the fifth SLS flight and two risk mitigation spare engines.

For the additional 18 RS-25 engines, it is estimated that each unit will take five years to fabricate and assemble. While it will be the goal of this procurement action to reduce this cycle time, the timeline of five years matches the documents Aerojet Rocketdyne historical norm for this engine.

Aerojet Rocketdyne designed, developed, and matured the RS-25 engine system as the SSME over the past forty-plus years, and has been the only source utilized for the design, development, manufacture, refurbishment, recycle, testing, and flight operations of the RS-25 for the life of the Space Shuttle Program. Further, Aerojet Rocketdyne is the contractor currently responsible for adapting the residual Space Shuttle RS-25 hardware for use as part of the SLS Program. No other contractor has this accumulated knowledge with respect to hands-on technical experience and programmatic history of this engine.

Aerojet Rocketdyne manufacturing is performed at three facilities; machining, welding, assembly and test of subassemblies at the Canoga Park California Strategic Fabrication Center, turbopump assembly operations at the West Palm Beach, Florida facility, and final assembly and test at the NASA Stennis Space Center in Mississippi. While the NASA Stennis Space Center is a Government-owned facility, the other two facilities are Aerojet Rocketdyne facilities.

Aerojet Rocketdyne (and its predecessor companies) is the only contractor in this country to design and build large liquid hydrogen/liquid oxygen rocket engines for human spaceflight. They designed and built the first liquid hydrogen/liquid oxygen engines to ever fly, the RL10, first launched in 1963. They designed and built the J-2 engine used for the second stage of the Saturn IB vehicle and the second and third stage of the Saturn V vehicle. Furthermore, they designed and built the world's largest liquid hydrogen/liquid oxygen production engine, the RS-68, for the Delta IV vehicle in support of the Department of Defense. And most recently, they restarted production of six new RS-25 flight engines for the SLS Program.

For the past forty-plus years the RS-25 was, and remains today, the highest performing large staged combustion liquid hydrogen engine in the world. It is a unique engine with unique capabilities that took substantial and prolonged effort to develop and certify for human spaceflight. An attempt to develop a new engine with a new contractor (or the RS-25 engine with a new contractor) would require significantly more engine hot fire testing to certify for flight.

The RS-25 engine design carries with it four decades of development and production activity and three decades of flight experience. As a staged-combustion liquid hydrogen engine, the RS-25 engine design is also the most advanced and complex engine ever built and flown. With over one million seconds of accumulated hot-fire test time and the equivalent of over four hundred human spaceflights, the RS-25 design, production processes, and operational procedures have incorporated within them thousands of lessons learned.

The overall period of performance for the proposed activity in support of the current SLS Program flight manifest is approximately nine years. To support an August 2025 launch of a fifth mission, the first four engines must be delivered no later than July 2025. Based on historical data it takes a lead-time of approximately five years to fabricate and assemble the engine. Based on an ATP of July 2019, the first of four engines would need to be delivered in July 2024. Assuming the engines are delivered every three months, the fourth engine would be delivered in April 2025, with about three months contingency in the schedule. The last of the 18 engines would deliver in the first quarter of fiscal year 2028.

Wednesday, March 18, 2020

NASA begins work on four new astrophysics missions

NASA has selected proposals for four missions that would study cosmic explosions and the debris they leave behind, as well as monitor how nearby stellar flares may affect the atmospheres of orbiting planets.

Following detailed evaluations, the agency intends to select two proposals in 2021 to be the next astrophysics missions under the Explorers Program. The selected missions will be targeted for launch in 2025.

"From studying stars and planets outside our solar system to seeking answers to the largest cosmic mysteries, I look forward to the breakthrough science from these modest size missions,” said Thomas Zurbuchen, associate administrator of the agency's Science Mission Directorate in Washington, D.C.

Two astrophysics Small Explorer (SMEX) missions and two Missions of Opportunity (MO) proposals were competitively selected.

Excluding the cost of launch, SMEX mission costs are capped at $145 million each, and MO costs are capped at $75 million each.

Each SMEX proposal will receive $2 million to conduct a nine-month mission concept study. The selected proposals are:

The Extreme-ultraviolet Stellar Characterization for Atmospheric Physics and Evolution (ESCAPE) Mission
  • ESCAPE would study nearby stars, watching for rapid, strong ultraviolet flares. It aims to determine how likely such flares are to strip the atmosphere from a rocky planet orbiting the star, affecting conditions for habitability.
  • Principal investigator: Kevin France at the University of Colorado at Boulder.
The Compton Spectrometer and Imager (COSI)
  • COSI would scan our Milky Way galaxy, measuring gamma rays from radioactive elements produced during stellar explosions to map the recent history of star death and element production. It would also measure polarization, to improve our understanding of how distant energetic cosmic explosions produce gamma rays.
  • Principal investigator: John Tomsick at the University of California, Berkeley.
MO proposals will each receive $500,000 to conduct a nine-month implementation concept study. The selected proposals are:

The Gravitational-wave Ultraviolet Counterpart Imager Mission
  • The Gravitational-wave Ultraviolet Counterpart Imager consists of two independent small satellites, each scanning the sky in a different ultraviolet band. It would detect the light from hot gas in the explosion that follows a burst of gravitational waves caused by merging neutron stars or a neutron star merging with a black hole. Between these events, the mission would map the sky in ultraviolet light, finding other bright objects such as exploding stars.
  • Principal investigator: Stephen (Brad) Cenko at NASA's Goddard Space Flight Center in Greenbelt, Md.
LEAP – A LargE Area burst Polarimeter
  • Mounted on the International Space Station, LEAP would study the energetic jets launched during the explosive death of a massive star, or the merger of compact objects such as neutron stars. LEAP's measurements of polarization in gamma-ray bursts could distinguish between competing theories for the nature of the jets, which move out at close to the speed of light. LEAP would complement NASA's Imaging X-ray Polarimetry Explorer, scheduled to launch in 2021.
  • Principal investigator: Mark McConnell at the University of New Hampshire in Durham.

Tuesday, October 22, 2019

Virginia rocket launch may be visible in Chesapeake Bay region

Several space technologies will be put to the test with the launch of a suborbital rocket at 8 p.m. EDT on Thursday from NASA’s Wallops Flight Facility in Virginia.

Called Suborbital Technology Experiment Carrier-8 or SubTec-8, the launch is designed to test new technologies to improve the capability of conducting suborbital science missions. Some of these technologies also may be applied to orbital spacecraft. The launch may be visible in the Chesapeake Bay region.

SubTec-8 will fly on a Terrier-Improved Malemute sounding rocket and is predicted to reach an altitude of 128 miles before descending by parachute and landing in the Atlantic Ocean. The first SubTec launch occurred in 2005.

SubTec-8 technologies include distributed payload communications that will allow multipoint measurements for scientists to study multiple regions in space simultaneously; a low cost star tracker for assisting in pointing the rocket when taking astronomical observations; and a high data rate encoder that will provide the ability to transmit data from the rocket to the ground four times faster than currently available.

Friday, August 30, 2019

NASA celebrates 20th anniversary of the Chandra X-ray Observatory

NASA's Marshall Space Flight Center and the U.S. Space & Rocket Center in Alabama are celebrating the 20th anniversary of the Chandra X-ray Observatory -- the world's most powerful X-ray telescope.

Since its launch on July 23, 1999, Chandra has been NASA's flagship mission for X-ray astronomy. Astronomers around the world use Chandra's X-ray vision to explore cosmic mysteries -- from distant galaxies and an expanding universe to black holes, dark energy and supernovas.















Thursday, April 26, 2018

Study looks at commercialization of low Earth orbit

In May, NASA will be releasing a NASA Research Announcement (NRA) for low Earth orbit (LEO) commercialization, according to contract documents released Tuesday.

The purpose of this NRA is to inform NASA's strategy for enabling the commercialization of human spaceflight in LEO and meeting NASA's long-term LEO needs. The NRA will solicit industry concepts, business plans and viability for habitable platforms, whether using the International Space Station (ISS) or free-flying, that would enable a commercial marketplace in LEO where NASA is one of many customers. Additionally, the study seeks industry input on the role of government and evolution of ISS in the roadmap to commercialization of LEO.

NASA anticipates awarding multiple four-month, fixed priced contracts, up to $1 million per award. Participation is open to U.S. organizations, including industry, educational institutions, and nonprofit institutions, the agency said in documents.

A Pre-Proposal Conference to discuss the study objectives and proposal instructions with prospective respondents is planned for May 1 in the Gilruth Center at Johnson Space Center, Houston, Texas.

Wednesday, March 8, 2017

NASA orders avionics and autopilot upgrade for research aircraft

NASA's Armstrong Flight Research Center operates a Beechcraft B200 aircraft, tail number N801NA, serial number BB-1164. The current avionics and autopilot suite, a critical aircraft system that projects rely on for accuracy, on the aircraft has been problematic for reliable operation and have been known to cause issues during research flight campaigns. Additionally, the aircraft needs RVSM capability, ADS-B In/Out, and TCAS/TAWS capabilities. “These are requirements for future projects, and they need to be addressed,” NASA officials said in contract documents released Wednesday.

The avionics and autopilot upgrade to N801NA will include:
  • G1000 Platinum Package with Synthetic Vision, including RVSM capabilities. Includes standby ADI, airspeed indicators and altimeter. Headset compatible, tie-in to audio panel.
  • Weather Radar upgrade (GWX-70).
  • ADS-B In/Out upgrade.
  • TCAS/TAWS upgrade, replace Skywatch 497 with Garmin GTW 825.
  • ADF compatible (currently ADF-60, upgrade to ADF-60A for compatibility with G1000).
  • Tie in the existing UHF radio to the G1000 suite.
  • Update the current DME-40s and Radio Altimeter (not compatible with G1000) to a DME-42 and Garmin Radio Altimeter and tie-in to G1000 package.
  • Retain the existing equipment that was removed to keep as spares for other B200 aircraft.
The work necessary to complete the avionics and autopilot upgrades shall be completed at a contractor’s facility.

All work should be completed within 20 business days of the arrival of N801NA to the contractor.

Wednesday, September 7, 2016

Video: Asteroid-sampling spacecraft ready for launch

NASA’s OSIRIS-REx spacecraft will be boosted into orbit aboard a United Launch Alliance Atlas V rocket from Space Launch Complex 41 at Cape Canaveral Air Force Station in Florida. OSIRIS-REx stands for Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer. The U.S.'s first mission to sample an asteroid, OSIRIS-REx will travel to the near-Earth asteroid Bennu. Learn how this pioneering spacecraft and the Atlas V were readied for flight.

Video: Cassini image shows dunes on Saturn's moon Titan

NASA's Cassini spacecraft has radar vision that allows it to peer through the haze that surrounds Saturn's largest moon Titan. This video focuses on Shangri-la, a large, dark area on Titan filled with dunes. The long, linear dunes are thought to be comprised of grains derived from hydrocarbons that have settled out of Titan's atmosphere. Cassini has shown that dunes of this sort encircle most of Titan's equator. Scientists can use the dunes to learn about winds, the sands they're composed of, and highs and lows in the landscape.

The radar image was obtained by the Cassini Synthetic Aperture radar on July 25, during the mission's 122nd targeted Titan encounter.


Saturday, August 27, 2016

The study of Jupiter and Jupiter-like planets

Astronomers say that in our galaxy alone, a billion or more such Jupiter-like worlds could be orbiting stars other than our sun. And we can use them to gain a better understanding of our solar system and our galactic environment, including the prospects for finding life.

It turns out the inverse is also true -- we can turn our instruments and probes to our own backyard, and view Jupiter as if it were an exoplanet to learn more about those far-off worlds. The best-ever chance to do this is now, with Juno, a NASA probe the size of a basketball court, which arrived at Jupiter in July to begin a series of long, looping orbits around our solar system's largest planet. Juno is expected to capture the most detailed images of the gas giant ever seen. And with a suite of science instruments, Juno will plumb the secrets beneath Jupiter's roiling atmosphere.

It will be a very long time, if ever, before scientists who study exoplanets -- planets orbiting other stars -- get the chance to watch an interstellar probe coast into orbit around an exo-Jupiter, dozens or hundreds of light-years away. But if they ever do, it's a safe bet the scene will summon echoes of Juno.

"The only way we're going to ever be able to understand what we see in those extrasolar planets is by actually understanding our system, our Jupiter itself," said David Ciardi, an astronomer with NASA's Exoplanet Science Institute at Caltech.

Juno's detailed examination of Jupiter could provide insights into the history, and future, of our solar system. The tally of confirmed exoplanets so far includes hundreds in Jupiter's size-range, and many more that are larger or smaller.

The so-called hot Jupiters acquired their name for a reason: They are in tight orbits around their stars that make them sizzling-hot, completing a full revolution -- the planet's entire year -- in what would be a few days on Earth. And they're charbroiled along the way.

But why does our solar system lack a "hot Jupiter?" Or is this, perhaps, the fate awaiting our own Jupiter billions of years from now -- could it gradually spiral toward the sun, or might the swollen future sun expand to engulf it?

Not likely, Ciardi says; such planetary migrations probably occur early in the life of a solar system.

"In order for migration to occur, there needs to be dusty material within the system," he said. "Enough to produce drag. That phase of migration is long since over for our solar system."

Jupiter itself might already have migrated from farther out in the solar system, although no one really knows, he said.

If Juno's measurements can help settle the question, they could take us a long way toward understanding Jupiter's influence on the formation of Earth -- and, by extension, the formation of other "Earths" that might be scattered among the stars.

"Juno is measuring water vapor in the Jovian atmosphere," said Elisa Quintana, a research scientist at the NASA Ames Research Center in Moffett Field, Calif. "This allows the mission to measure the abundance of oxygen on Jupiter. Oxygen is thought to be correlated with the initial position from which Jupiter originated."

Measuring the water is a key step in understanding how and where Jupiter formed.

"If Juno detects a high abundance of oxygen, it could suggest that the planet formed farther out," Quintana said.

A probe dropped into Jupiter by NASA's Galileo spacecraft in 1995 found high winds and turbulence, but the expected water seemed to be absent. Scientists think Galileo's one-shot probe just happened to drop into a dry area of the atmosphere, but Juno will survey the entire planet from orbit.




Where Jupiter formed, and when, also could answer questions about the solar system's "giant impact phase," a time of crashes and collisions among early planet-forming bodies that eventually led to the solar system we have today.

"It definitely was a violent time," Quintana said. "There were collisions going on for tens of millions of years. For example, the idea of how the moon formed is that a proto-Earth and another body collided; the disk of debris from this collision formed the moon. And some people think Mercury, because it has such a huge iron core, was hit by something big that stripped off its mantle; it was left with a large core in proportion to its size.

"For a long time, people thought Jupiter was essential to habitability because it might have shielded Earth from the constant influx of impacts [during the solar system's early days] which could have been damaging to habitability," she said. "What we've found in our simulations is that it's almost the opposite. When you add Jupiter, the accretion times are faster and the impacts onto Earth are far more energetic. Planets formed within about 100 million years; the solar system was done growing by that point," Quintana said.

"If you take Jupiter out, you still form Earth, but on timescales of billions of years rather than hundreds of millions. Earth still receives giant impacts, but they're less frequent and have lower impact energies," she said.

Another critical Juno measurement that could shed new light on the dark history of planetary formation is the mission's gravity science experiment. Changes in the frequency of radio transmissions from Juno to NASA's Deep Space Network will help map the giant planet's gravitational field.

Knowing the nature of Jupiter's core could reveal how quickly the planet formed, with implications for how Jupiter might have affected Earth's formation.

And the spacecraft's magnetometers could yield more insight into the deep internal structure of Jupiter by measuring its magnetic field.

"We don't understand a lot about Jupiter's magnetic field," Ciardi said. "We think it's produced by metallic hydrogen in the deep interior. Jupiter has an incredibly strong magnetic field, much stronger than Earth's."

Mapping Jupiter's magnetic field also might help pin down the plausibility of proposed scenarios for alien life beyond our solar system.

Earth's magnetic field is thought to be important to life because it acts like a protective shield, channeling potentially harmful charged particles and cosmic rays away from the surface.

"If a Jupiter-like planet orbits its star at a distance where liquid water could exist, the Jupiter-like planet itself might not have life, but it might have moons which could potentially harbor life," he said.

An exo-Jupiter's intense magnetic field could protect such life forms, he said.

Juno's findings will be important not only to understanding how exo-Jupiters might influence the formation of exo-Earths, or other kinds of habitable planets. They'll also be essential to the next generation of space telescopes that will hunt for alien worlds. The Transiting Exoplanet Survey Satellite will conduct a survey of nearby bright stars for exoplanets beginning in June 2018, or earlier. The James Webb Space Telescope, expected to launch in 2018, and WFIRST (Wide-Field Infrared Survey Telescope), with launch anticipated in the mid-2020s, will attempt to take direct images of giant planets orbiting other stars.

"We're going to be able to image planets and get spectra," or light profiles from exoplanets that will reveal atmospheric gases, Ciardi said. Juno's revelations about Jupiter will help scientists to make sense of these data from distant worlds.

"Studying our solar system is about studying exoplanets," he said. "And studying exoplanets is about studying our solar system. They go together."

Monday, March 14, 2016

Video: Student scientists help NASA build spacecraft to explore asteroid

College students in Boston are getting the chance to help NASA explore an asteroid. These student scientists have built an instrument called REXIS, which will fly on the OSIRIS-REx spacecraft that is scheduled to launch later this year. This video puts a spotlight on a group of these students and their experience on the REXIS project.




Friday, February 19, 2016

Video: Cargo ship departs International Space Station

The Cygnus cargo craft, built by Orbital/ATK in Dulles, Va., departed the International Space Station on Friday, a little over two months after delivering almost four tons of supplies to the station’s residents. Dubbed the “SS Deke Slayton II”, the resupply vehicle, now loaded with trash, will be commanded to deorbit on Saturday, for a destructive re-entry into the Earth’s atmosphere over the Pacific Ocean.



Monday, January 4, 2016

Ball Aerospace names new vice president roles

Ball Aerospace & Technologies Corp. has promoted Mike Gazarik, Technology Director, to the position of Vice President for Engineering and named Jeff Osterkamp Vice President for Mission Assurance.

Gazarik joined Ball in March from NASA where he was the Associate Administrator for the Space Technology Mission Directorate at NASA headquarters. Since then, he has worked to align Ball's technology development with business development and growth strategies. As the vice president of engineering, he will provide overall strategic and operational leadership of the organization, which includes all disciplines of engineering as well as manufacturing, testing, supply chain management, facilities, IRAD and intellectual property.

Gazarik earned a bachelor's degree in Electrical Engineering from the University of Pittsburgh and a master's and Ph.D. from the Georgia Institute of Technology, also in Electrical Engineering.

In transitioning from the role as VP for Engineering to VP of Mission Assurance, Osterkamp replaces Sherri Fike who retired in December. Osterkamp has more than 30 years of experience at Ball Aerospace. His previous roles include executive leadership of the company's component technologies business area; the National Defense strategic business unit; the Program Management Office; Sensor and Video Technologies; and Advanced Antenna and Video Systems.

Osterkamp earned his B.S. in Electrical Engineering from the University of Idaho and an M.S. in Engineering Management from the University of Colorado.

Friday, November 13, 2015

NASA seeks new director at Marshall Space Flight Center

NASA has named Todd May acting director of NASA's Marshall Space Flight Center in Huntsville, Ala., as the agency continues the process of looking for a permanent director.

Patrick Scheuermann, who served as the Marshall director since September 2012, is retiring from the agency, effective Friday. His retirement caps a 27-year career with NASA that began in 1988 as a propulsion test engineer at the agency's Stennis Space Center near Bay St. Louis, Miss.

May was appointed Marshall deputy director in August, and previously served as manager of the Space Launch System (SLS) Program since August 2011. May led the SLS Program through a series of milestones, including engine tests and a successful, in-depth critical design review. SLS, now under development, will be the most powerful rocket ever built, able to carry astronauts in NASA's Orion spacecraft on deep space missions, including to an asteroid and ultimately on a journey to Mars.

May's NASA career began in 1991, working in the Materials and Processes Laboratory at Marshall. He was deputy program manager of the Russian Integration Office in the International Space Station Program at NASA's Johnson Space Center in Houston in 1994, and worked on the team at Marshall that developed and launched the Gravity Probe B mission to test Einstein's Theory of Relativity in 2004. That same year he assumed management of the Discovery and New Frontiers Programs, created to explore the solar system with frequent unmanned spacecraft missions.

May moved to NASA Headquarters in Washington in 2007 as a deputy associate administrator in the Science Mission Directorate. Returning to Marshall in June 2008, May was named Marshall's associate director, Technical, a post he held until being named SLS program manager.

The SLS Program is managed at Marshall, one of NASA's largest field installations, with almost 6,000 civil service and contractor employees, an annual budget of approximately $2.5 billion and a broad spectrum of science and technological missions.

Friday, October 16, 2015

Potential habitability of Saturn's icy moon Enceladus

NASA's Cassini spacecraft has begun returning its best-ever views of the northern extremes of Saturn's icy, ocean-bearing moon Enceladus. The spacecraft obtained the images during its Wednesday flyby, passing 1,142 miles (1,839 kilometers) above the moon's surface. Mission controllers say the spacecraft will continue transmitting images and other data from the encounter for the next several days.

Scientists expected the north polar region of Enceladus to be heavily cratered, based on low-resolution images from the Voyager mission, but the new high-resolution Cassini images show a landscape of stark contrasts. "The northern regions are crisscrossed by a spidery network of gossamer-thin cracks that slice through the craters," said Paul Helfenstein, a member of the Cassini imaging team at Cornell University, Ithaca, N.Y. "These thin cracks are ubiquitous on Enceladus, and now we see that they extend across the northern terrains as well."

Cassini's next encounter with Enceladus is planned for Oct. 28, when the spacecraft will come within 30 miles (49 km) of the moon's south polar region. During the encounter, Cassini will make its deepest-ever dive through the moon's plume of icy spray, sampling the chemistry of the extraterrestrial ocean beneath the ice. Mission scientists are hopeful data from that flyby will provide evidence of how much hydrothermal activity is occurring in the moon's ocean, along with more detailed insights about the ocean's chemistry -- both of which relate to the potential habitability of Enceladus.

Cassini's final close Enceladus flyby will take place on Dec. 19, when the spacecraft will measure the amount of heat coming from the moon's interior. The flyby will be at an altitude of 3,106 miles (4,999 km).

The Cassini-Huygens mission is a cooperative project of NASA, European Space Agency and the Italian Space Agency. NASA's Jet Propulsion Laboratory in Pasadena, Calif., manages the mission for the agency's Science Mission Directorate in Washington. JPL is a division of the California Institute of Technology in Pasadena. The Cassini imaging operations center is based at the Space Science Institute in Boulder, Colo.

Tuesday, September 29, 2015

Video: NASA Langley Director, 'Get out of people's way'

Dave Bowles took over as NASA Langley Research Center Director in March. He recently sat down for a chat that touched on everything from his background to his leadership style.



Thursday, September 24, 2015

Xtronaut: The game of solar system exploration

A University of Arizona professor has combined his expertise in space mission planning and technology with his passion for strategy gaming to create Xtronaut: The Game of Solar System Exploration.
 
The Xtronaut game, developed by Professor Dante Lauretta, captures the various challenges and excitement of planning a space mission. Lauretta co-founded Xtronaut Enterprises with space entrepreneur Michael Lyon to increase awareness of NASA's asteroid sample return mission named OSIRIS-REx.

In 2011, NASA selected the asteroid sample return mission, OSIRIS-REx – a $1 billion mission to send a robotic spacecraft to an asteroid named "Bennu", collect a sample of the asteroid, and return to Earth. Unfortunately, the education outreach budget for OSIRIS-REx was eliminated in 2013. In response, mission leader Dante Lauretta and space entrepreneur Michael Lyon founded Xtronaut Enterprises to develop innovative activities associated with space exploration.

Xtronaut gives two to four players ages seven and up the chance to develop space missions and explore the solar system. The game is based on real planetary missions and rocket science. It also contains elements of politics and strategy that are inspired by the real-life situations that space missions face. The game has been tested with players that range from elementary school students to graduate students in planetary sciences and mission scientists.