Comet ISON went around the sun on Nov. 28, 2013. Several solar
observatories watched the comet throughout this closest approach to the
sun, known as perihelion. While the fate of the comet is not yet
established, it is likely that it did not survive the trip. The comet
grew faint while within both the view of NASA's Solar Terrestrial
Relations Observatory, and the joint European Space Agency and NASA's
Solar and Heliospheric Observatory. The comet was not visible at all in
NASA's Solar Dynamics Observatory.
We didn't see Comet ISON in SDO," said Dean Pesnell, project scientist for SDO.
"So we think it must have broken up and evaporated before it reached perihelion."
While this means that Comet ISON will not be visible in the night sky
in December, the wealth of observations gathered of the comet over the
last year will provide great research opportunities for some time. One
important question will simply be to figure out why it is no longer
visible.
2013/11/28
Satellite Movie Shows Difficult Eastern U.S. Thanksgiving Travel
This NOAA GOES-East and GOES-West composite image from Nov. 27 at 1445 UTC/9:45 a.m. EST shows the complex storm system over the eastern United States. |
Visible and infrared images taken from NOAA's satellites were animated by the NASA GOES Project at NASA's Goddard Space Flight Center in Greenbelt, Md., to create a 28-second movie. The movie shows the progression of a low pressure area that developed in the Gulf of Mexico and cold fronts that were sweeping from west to east.
2013/11/27
Space Station Live: Circadian Rhythms
NASA Public Affairs Officer Dan Huot talks with Dr. Hans-Christian
Gunga, the principal investigator for the Circadian Rhythms study aboard
the International Space Station. This experiment examines the role of
synchronized circadian rhythms (the human body's 24-hour light-dark
cycle) and its maintenance during long duration spaceflight, and
addresses its impact and importance relative to crew health and
well-being.
Comet ISON Streams Toward the Sun
In the early hours of Nov. 27, 2013, Comet ISON entered the field of
view of the European Space Agency/NASA Solar and Heliospheric
Observatory. In this picture, called a coronagraph, the bright light of
the sun itself is blocked so the structures around it are visible. The
comet is seen in the lower right; a giant cloud of solar material,
called a coronal mass ejection or CME, is seen billowing out under the
sun.
Comet ISON, which began its trip from the Oort cloud region of our solar system, will reach its closest approach to the sun on Thanksgiving Day, skimming just 730,000 miles above the sun's surface.
Comet ISON, which began its trip from the Oort cloud region of our solar system, will reach its closest approach to the sun on Thanksgiving Day, skimming just 730,000 miles above the sun's surface.
2013/11/26
Space Station Live: Testing a New Progress Rendezvous System
Public Affairs Officer Rob Navias interviews Tom Erkenswick, Visiting
Vehicle Officer, about Russia's Progess 53 resupply craft and its new
Kurs automated rendezvous system. The Progress 53 will take a longer
route to the International Space Station so mission controllers can test
the updated Kurs which will save fuel and take up less mass inside the
spacecraft.
The Progress 53 launched Monday and will "flyby" the station Wednesday allowing Russian mission controllers to test the new Kurs system. They will review the telemetry downlinked from Progress on Thursday before giving the final go for its docking on Friday.
The Progress 53 launched Monday and will "flyby" the station Wednesday allowing Russian mission controllers to test the new Kurs system. They will review the telemetry downlinked from Progress on Thursday before giving the final go for its docking on Friday.
Space Station Live: Nov. 26, 2013
The Space Station Live recap video for Nov. 26, 2013. Watch the full
Space Station Live broadcast weekdays on NASA TV at 10 a.m. CST. http://www.nasa.gov/ntv
NASA'S STEREO Shows Comet ISON Approaching the Sun
UPDATE: The latest movie from the STEREO-A spacecraft's
Heliospheric Imager shows the comet over a five-day period from Nov. 20
to Nov. 25, 2013.
2013/11/25
Space Station Live: Nov. 25, 2013
The Space Station Live recap video for Nov. 25, 2013. Watch the full
Space Station Live broadcast weekdays on NASA TV at 10 a.m. CST. http://www.nasa.gov/ntv
Ready, Set, Space! -- NASA's GPM Satellite Begins Journey
For the past three years, the Global Precipitation Measurement (GPM)
Core Observatory has gone from components and assembly drawings to a
fully functioning satellite at NASA's Goddard Space Flight Center in
Greenbelt, Md. The satellite has now arrived in Japan, where it will
lift off in early 2014.
The journey to the launch pad has been a long and painstaking process. It began with the most basic assembly of the satellite's frame and electrical system, continued through the integration of its two science instruments, and has now culminated in the completion of a dizzying array of environmental tests to check and recheck that GPM Core Observatory will survive its new home in orbit.
"The GPM Observatory is about 3,900 kilograms (8,598 pounds)of spacecraft, fully loaded," said GPM Project Manager Art Azarbarzin at Goddard. "It's a very large spacecraft. It's a very large wing span." The satelliteleft the nest in a large white shipping container, its two solar arrays tucked neatly into its sides.Fully extended, they will spread about 12 meters (13.1 yards) in either direction. The GPM Core Observatory is the largest spacecraft ever built at Goddard, and managing its sheer size was one thing that always had to be kept in mind, said Azarbarzin.
The Core Observatory is part of an international partnership, led by NASA and the Japan Aerospace Exploration Agency, or JAXA. It will combine measurements from multiple satellites to see where and how much it's raining or snowing over 90 percent ofthe Earth every three hours. Precipitation affects everyone around the world, providing drinking water and freshwater for crops, and driving weather and storms that can cause hurricanes, landslides, and floods. Rain and snow are also part of the larger climate system for the globe.
In order to collect data on the tiny water droplets and ice particles that compose precipitation, the GPM Core Observatory has two state-of-the-art instruments – the GPM Microwave Imager or GMI and Dual-frequency Precipitation Radar or DPR.These instruments will observe more frequencies and capture a wider range of precipitation than has been done by one satellite before, from big fat drops in the tropics to drizzle or snow common in higher latitudes.
Coming Together
The Goddard team began integrating components ofthe satellite in late2010, beginning with the main spacecraft bus, or body, that contains the propulsion, navigation, power, communications, and data handling systems. In early 2012, the two science instruments arrived. Ball Aerospace Inc. of Boulder, Colo.,delivered the GMI, JAXA delivered the DPR, and the Goddard team integrated the all component pieces into a functioning satellite.
"It was very exciting to see the Observatory coming together every day," said Candace Carlisle, GPM's deputy project manager at Goddard.
FromDecember2012 through September 2013, the entire Observatory went through its environmental test program in Goddard's Integration and Test Facility to get the spacecraft ready for the ride to orbit and its life in space.
"The test program for the Observatory is pretty rigorous. And that's because when we're in space we only have one shot at it," said Azarbarzin. The antenna for the communications system, the antenna for the GPM Microwave Imager instrument, and the two solar panels all have to unfold perfectly, without any help, and then the whole satellite has survive its three-year mission life in the extremely harsh space environment.
There's a Test For That
Two hundred and fifty miles above Earth's surface the last gasp of the atmosphere blends into outer space. The region is part of the bottom edge of low Earth orbit, where a single molecule might only encounter a few other molecules in the course of an hour. It's where the rules we live by on Earth change. Earth-observing satellites and the International Space Station, also in low Earth orbit, travel in a constant free-fall around the planet, experiencing floating microgravity and bouncing between high and low temperatures while moving in and out of the sunlight in the course of a 93-minute orbit.
Survival in these harsh conditions is only slightly less difficult for machines than for humans. The electronics and the equipment to regulate temperature have to protect the electronics from the extreme hot and extreme cold.To prepare, the GPM Core Observatory entered the Thermal Vacuum chamber, a giant 12.2 meter (40-foot) chamber that looks like it came out of a gothic horror novel. The spacecraft was hoisted by crane and carefully lowered into the chamber, where all the air was pumped out. It spent a month running tests for four cycles of hot (104F / 40 C) and cold (14F / -10 C) extremes.
After thermal vacuum testing, the Core Observatoryreturned to the clean room where it went through the first of two tests to ensure the electronic systems on the spacecraft would not interfere or cause problems with each other. The engineering teambuilt its own electromagnetic interference, or EMI, testing chamber, called a "GRUBEE," in the clean room to test out the spacecraft systems.
"We built the GRUBEE because we didn't have enough height in Goddard's EMI chamber to fully deploy the high gain antenna," said Carlisle. But for the second test, the spacecraft's size didn't get in the way. With the high gain antenna stowed in launch position, the spacecraft went through its paces in Goddard's EMI chamber to check that its systems, which would be up and running during launch, wouldn't experience interference from outside sources, each other, or cause interference with the systems on the rocket taking it into space.
Then there were tests for the shaking and shock. The GPM Core Observatory will blast off on top of the Japanese H-IIA rocket, launching from Tanegashima Island, Japan, in early 2014. Encapsulated in the tip, or faring, of the rocket, the satellite will rattle and shake to the roar of a hearing-destroying 120 decibels of sound. Six minutes after launch the faring will fall away and then nine minutes later, the spacecraft will separate from the rocket with controlled explosionsthat will release the connecting bolts. The separation gives the spacecraft a jolt, called separation shock, as it flies free.
On Earth, the GPM Core Observatory went through a trial version of each physical ordeal. A giant shaker table rapidly moved the spacecraft back and forth in three vibration tests, one each for forward and back, side to side, and up and down. Next it entered the acoustic chamber where a horn nearly the size of the spacecraft blew 120 decibels of simulated rocket noise.Finally, to simulate the separation shock, the Core Observatory returned to the clean room where it was mated to a test version of the rocket payload adapter and given a jolt.
The final tests for the GPM Core Observatory were ones that were repeated several times throughout the last year: deploying all of the spacecraft's moving parts and then running the satellite through a comprehensive test of all its systems. "We re-ran the comprehensive performance test yet again to make sure that we matched all of the performance we had before we went into environmental [testing]," said Carlisle. Only then was the satellite ready to ship.
It Takes a Global Village to Build a Satellite
Building a one-of-a-kind spacecraft from scratch is a huge endeavor. "Here at Goddard we have about 300 people working on GPM," said Carlisle. That includes the electrical and mechanical technicians and the engineering teams for each subsystem. "That, in addition to a number of people at the Japan Aerospace Exploration Agency who worked on the DPR instrument and at Ball Aerospace who worked on the GMI instrument. That also does not count our science team, who worked to build the algorithms and will be developing the science products after GPM launches," she said.
"It's a very dedicated and hardworking team," said Azarbarzin. He and the Goddard team are currently getting ready for the next phase of GPM. Once the satellite arrives at the launch site on Tanegashima Island, Japan, the team will conduct a final round of performance tests before the GPM Core Observatory takes its berth on the rocket.
The journey to the launch pad has been a long and painstaking process. It began with the most basic assembly of the satellite's frame and electrical system, continued through the integration of its two science instruments, and has now culminated in the completion of a dizzying array of environmental tests to check and recheck that GPM Core Observatory will survive its new home in orbit.
"The GPM Observatory is about 3,900 kilograms (8,598 pounds)of spacecraft, fully loaded," said GPM Project Manager Art Azarbarzin at Goddard. "It's a very large spacecraft. It's a very large wing span." The satelliteleft the nest in a large white shipping container, its two solar arrays tucked neatly into its sides.Fully extended, they will spread about 12 meters (13.1 yards) in either direction. The GPM Core Observatory is the largest spacecraft ever built at Goddard, and managing its sheer size was one thing that always had to be kept in mind, said Azarbarzin.
The Core Observatory is part of an international partnership, led by NASA and the Japan Aerospace Exploration Agency, or JAXA. It will combine measurements from multiple satellites to see where and how much it's raining or snowing over 90 percent ofthe Earth every three hours. Precipitation affects everyone around the world, providing drinking water and freshwater for crops, and driving weather and storms that can cause hurricanes, landslides, and floods. Rain and snow are also part of the larger climate system for the globe.
In order to collect data on the tiny water droplets and ice particles that compose precipitation, the GPM Core Observatory has two state-of-the-art instruments – the GPM Microwave Imager or GMI and Dual-frequency Precipitation Radar or DPR.These instruments will observe more frequencies and capture a wider range of precipitation than has been done by one satellite before, from big fat drops in the tropics to drizzle or snow common in higher latitudes.
Coming Together
The Goddard team began integrating components ofthe satellite in late2010, beginning with the main spacecraft bus, or body, that contains the propulsion, navigation, power, communications, and data handling systems. In early 2012, the two science instruments arrived. Ball Aerospace Inc. of Boulder, Colo.,delivered the GMI, JAXA delivered the DPR, and the Goddard team integrated the all component pieces into a functioning satellite.
"It was very exciting to see the Observatory coming together every day," said Candace Carlisle, GPM's deputy project manager at Goddard.
FromDecember2012 through September 2013, the entire Observatory went through its environmental test program in Goddard's Integration and Test Facility to get the spacecraft ready for the ride to orbit and its life in space.
"The test program for the Observatory is pretty rigorous. And that's because when we're in space we only have one shot at it," said Azarbarzin. The antenna for the communications system, the antenna for the GPM Microwave Imager instrument, and the two solar panels all have to unfold perfectly, without any help, and then the whole satellite has survive its three-year mission life in the extremely harsh space environment.
There's a Test For That
Two hundred and fifty miles above Earth's surface the last gasp of the atmosphere blends into outer space. The region is part of the bottom edge of low Earth orbit, where a single molecule might only encounter a few other molecules in the course of an hour. It's where the rules we live by on Earth change. Earth-observing satellites and the International Space Station, also in low Earth orbit, travel in a constant free-fall around the planet, experiencing floating microgravity and bouncing between high and low temperatures while moving in and out of the sunlight in the course of a 93-minute orbit.
Survival in these harsh conditions is only slightly less difficult for machines than for humans. The electronics and the equipment to regulate temperature have to protect the electronics from the extreme hot and extreme cold.To prepare, the GPM Core Observatory entered the Thermal Vacuum chamber, a giant 12.2 meter (40-foot) chamber that looks like it came out of a gothic horror novel. The spacecraft was hoisted by crane and carefully lowered into the chamber, where all the air was pumped out. It spent a month running tests for four cycles of hot (104F / 40 C) and cold (14F / -10 C) extremes.
After thermal vacuum testing, the Core Observatoryreturned to the clean room where it went through the first of two tests to ensure the electronic systems on the spacecraft would not interfere or cause problems with each other. The engineering teambuilt its own electromagnetic interference, or EMI, testing chamber, called a "GRUBEE," in the clean room to test out the spacecraft systems.
"We built the GRUBEE because we didn't have enough height in Goddard's EMI chamber to fully deploy the high gain antenna," said Carlisle. But for the second test, the spacecraft's size didn't get in the way. With the high gain antenna stowed in launch position, the spacecraft went through its paces in Goddard's EMI chamber to check that its systems, which would be up and running during launch, wouldn't experience interference from outside sources, each other, or cause interference with the systems on the rocket taking it into space.
Then there were tests for the shaking and shock. The GPM Core Observatory will blast off on top of the Japanese H-IIA rocket, launching from Tanegashima Island, Japan, in early 2014. Encapsulated in the tip, or faring, of the rocket, the satellite will rattle and shake to the roar of a hearing-destroying 120 decibels of sound. Six minutes after launch the faring will fall away and then nine minutes later, the spacecraft will separate from the rocket with controlled explosionsthat will release the connecting bolts. The separation gives the spacecraft a jolt, called separation shock, as it flies free.
On Earth, the GPM Core Observatory went through a trial version of each physical ordeal. A giant shaker table rapidly moved the spacecraft back and forth in three vibration tests, one each for forward and back, side to side, and up and down. Next it entered the acoustic chamber where a horn nearly the size of the spacecraft blew 120 decibels of simulated rocket noise.Finally, to simulate the separation shock, the Core Observatory returned to the clean room where it was mated to a test version of the rocket payload adapter and given a jolt.
The final tests for the GPM Core Observatory were ones that were repeated several times throughout the last year: deploying all of the spacecraft's moving parts and then running the satellite through a comprehensive test of all its systems. "We re-ran the comprehensive performance test yet again to make sure that we matched all of the performance we had before we went into environmental [testing]," said Carlisle. Only then was the satellite ready to ship.
It Takes a Global Village to Build a Satellite
Building a one-of-a-kind spacecraft from scratch is a huge endeavor. "Here at Goddard we have about 300 people working on GPM," said Carlisle. That includes the electrical and mechanical technicians and the engineering teams for each subsystem. "That, in addition to a number of people at the Japan Aerospace Exploration Agency who worked on the DPR instrument and at Ball Aerospace who worked on the GMI instrument. That also does not count our science team, who worked to build the algorithms and will be developing the science products after GPM launches," she said.
"It's a very dedicated and hardworking team," said Azarbarzin. He and the Goddard team are currently getting ready for the next phase of GPM. Once the satellite arrives at the launch site on Tanegashima Island, Japan, the team will conduct a final round of performance tests before the GPM Core Observatory takes its berth on the rocket.
The Global Precipitation Measurement Core Observatory, shown here in NASA Goddard's Integration and Test Facility, had to undergo many tests to ensure it will survive the harsh space environment. |
Curiosity Resumes Science After Analysis of Voltage Issue
This artist concept features NASA's Mars Science Laboratory Curiosity rover, a mobile robot for investigating Mars' past or present ability to sustain microbial life. |
Activities over the weekend included use of Curiosity’s robotic arm to deliver portions of powdered rock to a laboratory inside the rover. The powder has been stored in the arm since the rover collected it by drilling into the target rock "Cumberland" six months ago. Several portions of the powder have already been analyzed. The laboratory has flexibility for examining duplicate samples in different ways.
The decision to resume science activities resulted from the success of work to diagnose the likely root cause of a Nov. 17 change in voltage on the vehicle. The voltage change itself did not affect the rover safety or health. The vehicle's electrical system has a "floating bus" design feature to tolerate a range of voltage differences between the vehicle's chassis -- its mechanical frame -- and the 32-volt power lines that deliver electricity throughout the rover. This protects the rover from electrical shorts.
"We made a list of potential causes, and then determined which we could cross off the list, one by one," said rover electrical engineer Rob Zimmerman of NASA's Jet Propulsion Laboratory, Pasadena, Calif. Science operations were suspended for six days while this analysis took priority.
The likely cause is an internal short in Curiosity's power source, the Multi-Mission Radioisotope Thermoelectric Generator. Due to resiliency in design, this short does not affect operation of the power source or the rover. Similar generators on other spacecraft, including NASA's Cassini at Saturn, have experienced shorts with no loss of capability. Testing of another Multi-Mission Radioisotope Thermoelectric Generator over many years found no loss of capability in the presence of these types of internal shorts.
Following the decision to resume science activities, engineers learned early Nov. 23 that the rover had returned to its pre-Nov. 17 voltage level. This reversal is consistent with their diagnosis of an internal short in the generator on Nov. 17, and the voltage could change again.
The analysis work to determine the cause of the voltage change gained an advantage from an automated response by the rover's onboard software when it detected the voltage change on Nov. 17. The rover stepped up the rate at which it recorded electrical variables, to eight times per second from the usual once per minute, and transmitted that engineering data in its next communication with Earth. "That data was quite helpful," Zimmerman said.
In subsequent days, the rover performed diagnostic activities commanded by the team, such as powering on some backup hardware to rule out the possibility of short circuits in certain sensors.
NASA's Mars Science Laboratory Project is using Curiosity inside Gale Crater to assess ancient habitable environments and major changes in Martian environmental conditions. JPL, a division of the California Institute of Technology in Pasadena, built the rover and manages the project for NASA's Science Mission Directorate in Washington.
2013/11/22
Benefits for Humanity: Changing Lives
In this chapter of Benefits for Humanity: In Their Own Words, learn how a
life was drastically changed using the same technology that went into
the robotics on board the International Space Station.
For more information on how science and research is benefitting life here on Earth, visit: http://www.nasa.gov/stationbenefits
For more information on how science and research is benefitting life here on Earth, visit: http://www.nasa.gov/stationbenefits
NASA Releases Comet ISON Images from STEREO
2013/11/21
Thanksgiving Message From Station's Expedition 38 Crew
.Aboard the Earth-orbiting International Space Station, NASA astronauts
Rick Mastracchio and Mike Hopkins, both Expedition 38 flight engineers,
send down their best wishes for a happy Thanksgiving. Their Russian
crewmates, Commander Oleg Kotov and Flight Engineers Sergey Ryazanskiy
and Mikhail Tyurin, show off the station's galley where the crew will be
preparing and enjoying a Thanksgiving meal.
Space Station Live: Nov. 21, 2013
The Space Station Live recap video for Nov. 21, 2013. Watch the full
Space Station Live broadcast weekdays on NASA TV at 10 a.m. CST. http://www.nasa.gov/ntv
Asteroid Initiative Workshop Plenary Session
NASA TV coverage of the plenary
session of the NASA-hosted public workshop at the Lunar and Planetary
Institute in Houston to examine 96 of the ideas submitted to the recent
Request For Information on ways to accomplish the agency's asteroid
initiative.
NASA Sees 'Watershed' Cosmic Blast in Unique Detail
On April 27, a blast of light from a dying star in a distant galaxy
became the focus of astronomers around the world. The explosion, known
as a gamma-ray burst and designated GRB 130427A, tops the charts as one
of the brightest ever seen.
A trio of NASA satellites, working in concert with ground-based robotic telescopes, captured never-before-seen details that challenge current theoretical understandings of how gamma-ray bursts work.
Gamma-ray bursts are the most luminous explosions in the cosmos, thought to be triggered when the core of a massive star runs out of nuclear fuel, collapses under its own weight, and forms a black hole. The black hole then drives jets of particles that drill all the way through the collapsing star and erupt into space at nearly the speed of light.
Gamma-rays are the most energetic form of light. Hot matter surrounding a new black hole and internal shock waves produced by collisions within the jet are thought to emit gamma-rays with energies in the million-electron-volt (MeV) range, or roughly 500,000 times the energy of visible light. The most energetic emission, with billion-electron-volt (GeV) gamma rays, is thought to arise when the jet slams into its surroundings, forming an external shock wave.
The Gamma-ray Burst Monitor (GBM) aboard NASA's Fermi Gamma-ray Space Telescope captured the initial wave of gamma rays from GRB 130427A shortly after 3:47 a.m. EDT April 27. In its first three seconds alone, the "monster burst" proved brighter than almost any burst previously observed.
GRB 130427A is the subject of five papers published online Nov. 21. Four of these, published by Science Express, highlight contributions by Fermi, Swift and RAPTOR. The NuSTAR study is published in The Astrophysical Journal Letters.
NASA's Fermi Gamma-ray Space Telescope is an international and multi-agency astrophysics and particle physics partnership managed by NASA's Goddard Space Flight Center in Greenbelt, Md., and supported by the U.S. Department of Energy's Office of Science. Goddard also manages NASA's Swift mission, which is operated in collaboration with Pennsylvania State University in University Park, Pa., and international partners. NASA's NuSTAR mission is led by the California Institute of Technology and managed by NASA's Jet Propulsion Laboratory, both in Pasadena, with contributions from international partners.
A trio of NASA satellites, working in concert with ground-based robotic telescopes, captured never-before-seen details that challenge current theoretical understandings of how gamma-ray bursts work.
Gamma-ray bursts are the most luminous explosions in the cosmos, thought to be triggered when the core of a massive star runs out of nuclear fuel, collapses under its own weight, and forms a black hole. The black hole then drives jets of particles that drill all the way through the collapsing star and erupt into space at nearly the speed of light.
Gamma-rays are the most energetic form of light. Hot matter surrounding a new black hole and internal shock waves produced by collisions within the jet are thought to emit gamma-rays with energies in the million-electron-volt (MeV) range, or roughly 500,000 times the energy of visible light. The most energetic emission, with billion-electron-volt (GeV) gamma rays, is thought to arise when the jet slams into its surroundings, forming an external shock wave.
The Gamma-ray Burst Monitor (GBM) aboard NASA's Fermi Gamma-ray Space Telescope captured the initial wave of gamma rays from GRB 130427A shortly after 3:47 a.m. EDT April 27. In its first three seconds alone, the "monster burst" proved brighter than almost any burst previously observed.
GRB 130427A is the subject of five papers published online Nov. 21. Four of these, published by Science Express, highlight contributions by Fermi, Swift and RAPTOR. The NuSTAR study is published in The Astrophysical Journal Letters.
NASA's Fermi Gamma-ray Space Telescope is an international and multi-agency astrophysics and particle physics partnership managed by NASA's Goddard Space Flight Center in Greenbelt, Md., and supported by the U.S. Department of Energy's Office of Science. Goddard also manages NASA's Swift mission, which is operated in collaboration with Pennsylvania State University in University Park, Pa., and international partners. NASA's NuSTAR mission is led by the California Institute of Technology and managed by NASA's Jet Propulsion Laboratory, both in Pasadena, with contributions from international partners.
2013/11/20
Space Station Live: Nov. 20, 2013
The Space Station Live recap video for Nov. 20, 2013. Watch the full
Space Station Live broadcast weekdays on NASA TV at 10 a.m. CST. http://www.nasa.gov/ntv
Space Station Live: Marshall's Contributions to Station Hardware
While the team at the Payload Operations Integration Center at NASA's
Marshall Space Flight Center makes science happen every day aboard the
International Space Station, Marshall also played a key role in some of
the station's major hardware components. NASA Public Affairs Officer
Lori Meggs talks with some of the folks who helped make that hardware
happen.
Brian Mitchell, who was the element project manager for Node 1, discusses development and construction of this crucial station component at Marshall. Also known as the Unity node, Node 1 was the first U.S. piece of the station.
Mike Cole, Deputy Manager for the ISS Office at Marshall, discusses the station's science hardware. Cole was the project manager when the Microgravity Science Glovebox, one of the dedicated science facilities inside the Destiny laboratory, was delivered to the station.
Brian Mitchell, who was the element project manager for Node 1, discusses development and construction of this crucial station component at Marshall. Also known as the Unity node, Node 1 was the first U.S. piece of the station.
Mike Cole, Deputy Manager for the ISS Office at Marshall, discusses the station's science hardware. Cole was the project manager when the Microgravity Science Glovebox, one of the dedicated science facilities inside the Destiny laboratory, was delivered to the station.
Benefits for Humanity: Farming from Space
The International Space Station Agricultural Camera (ISSAC) hardware in the Destiny laboratory of the space station helps farmers monitor crop growth for disease or fertility differences. |
In Crookston, A.W.G. Farms Inc. is leveraging images from the International Space Station Agricultural Camera (ISSAC) to grow sugar beets, spring wheat, sunflowers and soybeans. The Upper Midwest Aerospace Consortium, led by the University of North Dakota, operates ISSAC from Earth to help farmers like Gary Wagner monitor crop growth for disease or fertility differences.
ISSAC, unaffected by cloud cover, captures frequent images of the Earth in visible and infrared light, which are necessary for relaying information on biomass. Biomass images provide data on crop growth, and more biomass means more crop yield potential. Delivering these images to farmers more rapidly than previous remote sensing technology, Wagner called ISSAC a “tool we can use as a reference to be able to make better decisions and by doing that, our farm is more profitable, and that to me is very important.”
This is one of the many examples of the impact of space station research on the lives of the people on Earth. With its 15-year anniversary in 2013 and continued operations until at least 2020, and likely beyond, there are many more benefits to look forward to from space station research. The space station has the potential to improve and change lives on Earth with each investigation and technology test that takes place in orbit. With collaboration from the original international partnerships to the insights of inventors and integrators of the research and technology on the ground, we can anticipate continued space station benefits for humanity.
Space Station Live: Nov. 19, 2013
The Space Station Live recap video for Nov. 19, 2013. Watch the full
Space Station Live broadcast weekdays on NASA TV at 10 a.m. CST. http://www.nasa.gov/ntv
QRS 3 Mission Launches from Wallops
A Minotaur I rocket launched Nov. 19 from NASA's Wallops Flight Facility
on the U. S. Air Force's Operationally Responsive Space Office's ORS-3
mission. The ORS-3 Mission, also known as an enabler mission, will
demonstrate and validate launch and range improvements for NASA and the
military. Aside from the primary payload -- the Space Test Program
Satellite-3 (STPSat-3), ORS-3 transported about 28 small cubesat
satellites to space. Among the cubesats were NASA's PhoneSat2 and the
first cubesat built by high school students.
NASA Advances Effort to Again Launch Astronauts from U.S. Soil to Space Station
NASA took another step Tuesday to restore an American capability to
launch astronauts from U.S. soil to the International Space Station by
the end of 2017, subject to the availability of adequate funding. The
agency's Commercial Crew Program (CCP) requested proposals from U.S.
companies to complete development of crew transportation systems that
meet NASA certification requirements and begin conducting crewed flights
to the space station.
"NASA is committed to launching American astronauts from U.S. soil in the very near future, and we're taking a significant step toward achieving that goal today," NASA Administrator Charles Bolden said. "Our American industry partners have already proven they can safely and reliably launch supplies to the space station, and now we're working with them to get our crews there as well. However, we will require that these companies provide spacecraft that meet the same rigorous safety standards we had for the space shuttle program, while providing good value to the American taxpayer."
This phase of the CCP, called Commercial Crew Transportation Capability (CCtCap), will enable NASA to ensure a company's crew transportation system is safe, reliable and cost-effective. The certification process will assess progress throughout the production and testing of one or more integrated space transportation systems, which include rockets, spacecraft and ground operations. Requirements under CCtCap also will include at least one crewed flight test to the space station before certification can be granted.
"The U.S. commercial space industry has made tremendous progress designing and developing the next generation of U.S. crew transportation systems for low-Earth orbit," said William Gerstenmaier, NASA's associate administrator for human exploration and operations in Washington. "Finalizing these systems in accordance with NASA’s certification requirements will not be easy. The acquisition approach we are using is designed to leverage the innovative power of industry with the expertise, skill and hard learned lessons from NASA. This request for proposals begins the journey for a new era in U.S. human spaceflight."
As with all of NASA's human spaceflight activities, astronaut safety will be a priority. CCtCap ensures a strong emphasis on crew safety through its requirements, including NASA insight throughout development and thorough testing of the space transportation systems.
"NASA is taking its years of expertise in human spaceflight systems and partnering with industry to develop a safe and reliable crew transportation system for NASA and for the nation," said Phil McAlister, NASA's director of commercial spaceflight development. "These certification contracts are part of a strategy that will help ensure human safety."
NASA expects to award one or more CCtCap contracts no later than September 2014.
CCtCap is the second phase of a two-phased effort that began last year. It builds on the accomplishments of a first certification phase, called Certification Products Contracts (CPC). CPC required companies to deliver a range of products that establish a baseline for their integrated system certification. CCtCap is open to any company with systems at the design maturity level consistent with the completion of the first certification phase.
CCtCap contractors will plan, manage and execute long-term production and operational plans for their systems. The firm-fixed price contracts, based on the Federal Acquisition Regulations (FAR), will include at least one, crewed flight test to verify the spacecraft can dock to the space station and that all its systems perform as expected. CCtCap contracts also will include at least two and as many as six crewed, post-certification missions to enable NASA to meet its station crew rotation requirements.
While CCtCap will enable NASA to acquire a capability to transport crews to the space station, systems developed by U.S. industry can be marketed and used by other customers.
As NASA works with U.S. industry partners to develop commercial spaceflight capabilities to low Earth orbit, the agency also is developing the Orion spacecraft and the Space Launch System (SLS), a crew capsule and heavy-lift rocket to provide an entirely new capability for human exploration. Designed to be flexible for launching spacecraft for crew and cargo missions, SLS and Orion will expand human presence beyond low-Earth orbit and enable new missions of exploration across the solar system.
"NASA is committed to launching American astronauts from U.S. soil in the very near future, and we're taking a significant step toward achieving that goal today," NASA Administrator Charles Bolden said. "Our American industry partners have already proven they can safely and reliably launch supplies to the space station, and now we're working with them to get our crews there as well. However, we will require that these companies provide spacecraft that meet the same rigorous safety standards we had for the space shuttle program, while providing good value to the American taxpayer."
This phase of the CCP, called Commercial Crew Transportation Capability (CCtCap), will enable NASA to ensure a company's crew transportation system is safe, reliable and cost-effective. The certification process will assess progress throughout the production and testing of one or more integrated space transportation systems, which include rockets, spacecraft and ground operations. Requirements under CCtCap also will include at least one crewed flight test to the space station before certification can be granted.
"The U.S. commercial space industry has made tremendous progress designing and developing the next generation of U.S. crew transportation systems for low-Earth orbit," said William Gerstenmaier, NASA's associate administrator for human exploration and operations in Washington. "Finalizing these systems in accordance with NASA’s certification requirements will not be easy. The acquisition approach we are using is designed to leverage the innovative power of industry with the expertise, skill and hard learned lessons from NASA. This request for proposals begins the journey for a new era in U.S. human spaceflight."
As with all of NASA's human spaceflight activities, astronaut safety will be a priority. CCtCap ensures a strong emphasis on crew safety through its requirements, including NASA insight throughout development and thorough testing of the space transportation systems.
"NASA is taking its years of expertise in human spaceflight systems and partnering with industry to develop a safe and reliable crew transportation system for NASA and for the nation," said Phil McAlister, NASA's director of commercial spaceflight development. "These certification contracts are part of a strategy that will help ensure human safety."
NASA expects to award one or more CCtCap contracts no later than September 2014.
CCtCap is the second phase of a two-phased effort that began last year. It builds on the accomplishments of a first certification phase, called Certification Products Contracts (CPC). CPC required companies to deliver a range of products that establish a baseline for their integrated system certification. CCtCap is open to any company with systems at the design maturity level consistent with the completion of the first certification phase.
CCtCap contractors will plan, manage and execute long-term production and operational plans for their systems. The firm-fixed price contracts, based on the Federal Acquisition Regulations (FAR), will include at least one, crewed flight test to verify the spacecraft can dock to the space station and that all its systems perform as expected. CCtCap contracts also will include at least two and as many as six crewed, post-certification missions to enable NASA to meet its station crew rotation requirements.
While CCtCap will enable NASA to acquire a capability to transport crews to the space station, systems developed by U.S. industry can be marketed and used by other customers.
As NASA works with U.S. industry partners to develop commercial spaceflight capabilities to low Earth orbit, the agency also is developing the Orion spacecraft and the Space Launch System (SLS), a crew capsule and heavy-lift rocket to provide an entirely new capability for human exploration. Designed to be flexible for launching spacecraft for crew and cargo missions, SLS and Orion will expand human presence beyond low-Earth orbit and enable new missions of exploration across the solar system.
Infographic: 15 Years of the International Space Station
The first International Space Station component, the Russian Zarya
module, was launched in November 1998. In the 15 years since, NASA and
its global partners have built a world class orbiting laboratory,
establishing a continuous human presence in space since 2000 and paving
the way for future exploration beyond.
We're celebrating this milestone with an infographic showcasing some of the amazing and surprising facts about humanity's home away from Earth, but there's much more to learn. For the latest news, features and videos from orbit, visit www.nasa.gov/station. You can also find out how to see the station yourself at spotthestation.nasa.gov or watch live station video at www.nasa.gov/iss-stream.
We're celebrating this milestone with an infographic showcasing some of the amazing and surprising facts about humanity's home away from Earth, but there's much more to learn. For the latest news, features and videos from orbit, visit www.nasa.gov/station. You can also find out how to see the station yourself at spotthestation.nasa.gov or watch live station video at www.nasa.gov/iss-stream.
NASA Helps Launch Student-Built Satellites and latest PhoneSat as Part of CubeSat Launch Initiative
Nine university teams and one high school team will experience on
Tuesday a feat that few outside the aerospace industry will ever
realize: watching the nanosatellites, or cubesats, that they designed
and built launch into space. An addition to the NASA PhoneSat technology demonstration will also be aboard.
More than 300 students took part in this fourth installment of NASA’s cubesat Launch Initiative and it’s Educational Launch of Nanosatellite (ELaNa) Missions, which enables students, teachers and faculty to obtain hands-on flight hardware development experience. This launch marks the first time NASA will launch a cubesat developed by students not yet in college – high school students from Thomas Jefferson High School for Science and Technology of Alexandria, Va.
The advancements of the cubesat community are enabling an acceleration of flight-qualified technology that will ripple through the aerospace industry," said Jason Crusan, director of Advanced Exploration Systems, the office that oversees the Cubesat Launch Initiative at NASA Headquarters in Washington. "Our future missions will be standing on the developments the cubesat community has enabled."
Since 2010, the cubesat Launch Initiative has issued four announcements of opportunity and selected more than 90 cubesats from public and private institutions and government labs to launch as auxillary payloads aboard commercial rockets. The cube-shaped satellites are approximately four inches long per unit, have a volume of about one quart and weigh less than three pounds. Cubesat research addresses science, exploration, technology development, education or operations.
In many cases, student teams are able to connect with mentors in the aerospace industry to help them develop their cubesats. Twyman Clements of Kentucky Space LLC, is mentor to the ELaNa IV KySat-2 team comprising students from the University of Kentucky and Morehead State University. “There’s an enormous sense of accomplishment,” he says, “Not just in designing with a great team but also encouraging the students to take the initiative and learn their areas of strength to become better students – and much more importantly, better professionals. There’s nothing like an impending satellite launch to motivate you.”
Success of the ELaNa missions has also helped universities to secure funding for future projects. According to Craig Kief, Deputy Director of the Configurable Space Microsystems Innovations & Applications Center (COSMIAC), "ELaNa has proven to be a game-changing endeavor. It has allowed us to be able to show past performance in the areas of nanosatellite development. This achievement has easily resulted in over $1M in future research projects for the University of New Mexico.”
The 11 ELaNa IV cubesats are scheduled to launch aboard the Orbital Sciences Corporation’s Minotaur-1 rocket on Nov. 19, between 7:30-9:30 p.m. EST. Over the next few months, they will receive data from their satellites in space. As part of their agreement with NASA, they will provide NASA a report on their outcomes and scientific findings.
More than 300 students took part in this fourth installment of NASA’s cubesat Launch Initiative and it’s Educational Launch of Nanosatellite (ELaNa) Missions, which enables students, teachers and faculty to obtain hands-on flight hardware development experience. This launch marks the first time NASA will launch a cubesat developed by students not yet in college – high school students from Thomas Jefferson High School for Science and Technology of Alexandria, Va.
The advancements of the cubesat community are enabling an acceleration of flight-qualified technology that will ripple through the aerospace industry," said Jason Crusan, director of Advanced Exploration Systems, the office that oversees the Cubesat Launch Initiative at NASA Headquarters in Washington. "Our future missions will be standing on the developments the cubesat community has enabled."
Since 2010, the cubesat Launch Initiative has issued four announcements of opportunity and selected more than 90 cubesats from public and private institutions and government labs to launch as auxillary payloads aboard commercial rockets. The cube-shaped satellites are approximately four inches long per unit, have a volume of about one quart and weigh less than three pounds. Cubesat research addresses science, exploration, technology development, education or operations.
In many cases, student teams are able to connect with mentors in the aerospace industry to help them develop their cubesats. Twyman Clements of Kentucky Space LLC, is mentor to the ELaNa IV KySat-2 team comprising students from the University of Kentucky and Morehead State University. “There’s an enormous sense of accomplishment,” he says, “Not just in designing with a great team but also encouraging the students to take the initiative and learn their areas of strength to become better students – and much more importantly, better professionals. There’s nothing like an impending satellite launch to motivate you.”
Success of the ELaNa missions has also helped universities to secure funding for future projects. According to Craig Kief, Deputy Director of the Configurable Space Microsystems Innovations & Applications Center (COSMIAC), "ELaNa has proven to be a game-changing endeavor. It has allowed us to be able to show past performance in the areas of nanosatellite development. This achievement has easily resulted in over $1M in future research projects for the University of New Mexico.”
The 11 ELaNa IV cubesats are scheduled to launch aboard the Orbital Sciences Corporation’s Minotaur-1 rocket on Nov. 19, between 7:30-9:30 p.m. EST. Over the next few months, they will receive data from their satellites in space. As part of their agreement with NASA, they will provide NASA a report on their outcomes and scientific findings.
University of New Mexico Students inspect their CubeSat, Trailblazer. |
2013/11/18
Space Station Live: Nov. 18, 2013
Mike Hopkins conducts a session with the Capillary Flow Experiment -- a suite of fluid physics experiments that investigate how fluids move up surfaces in microgravity |
Mission Managers Hail Successful MAVEN Launch
Officials Celebrate MAVEN Separation from Centaur
MAVEN Spacecraft Launches to Mars
2013/11/17
MAVEN Launch #NASASocial
Segment: 150 of NASA's social media followers were given an insider's look at America's space program and the opportunity to learn about the upcoming launch of NASA's Mars Atmosphere and Volatile EvolutioN (MAVEN) from Kennedy Space Center in Florida. Participants heard first-hand accounts of the mission development and research goals from the MAVEN science and engineering teams from NASA Kennedy, Goddard and other organizations.
2013/11/16
NASA Begins First Antarctic Airborne Campaign from McMurdo Station
NASA's Operation IceBridge has begun its 2013 Antarctic field campaign with the arrival of the agency's aircraft and scientists at the National Science Foundation's McMurdo Station in Antarctica.
The IceBridge mission will conduct daily survey flights through Nov. 26 on a NASA P-3 research aircraft from a base of operations at McMurdo Station. The P-3 usually is based at the agency's Wallops Flight Facility in Virginia. As part of a multi-year project, researchers are collecting data on Antarctic land and sea ice. Previous IceBridge Antarctic missions were conducted out of Punta Arenas, Chile.
"Flying from Antarctica will allow us to survey areas that had been unreachable from Chile," said Michael Studinger, IceBridge project scientist at NASA's Goddard Space Flight Center in Greenbelt, Md. "There are many scientifically important areas we can now reach from McMurdo."
One such area is the Siple Coast on the edge of Antarctica's Ross Ice Shelf. The ice streams there are of particular interest. "We know from spaceborne ice surface velocity measurements that some of the Siple Coast ice streams are changing," said Studinger. "But since 2009, we have had no laser altimeter measurements of ice surface elevations in this area."
In 2009, NASA's ice-monitoring satellite, the Ice, Cloud and Land Elevation Satellite (ICESat) reached the end of its life and stopped collecting data. IceBridge was started the same year and will keep an eye on changing polar ice until NASA launches the ICESat successor (ICESat-2) in three years.
IceBridge also plans to fly over areas of sea ice in and around the Ross Sea where there have been no airborne ice thickness measurements. The scientists will also survey beneath the Ross Ice Shelf using a gravimeter, an instrument that can detect minute changes in gravitational fields below the aircraft. These small changes help researchers determine the depth and shape of water cavities beneath floating ice.
The P-3 left Wallops Nov. 11 carrying a suite of instruments, including laser altimeters, radars, cameras and gravity and magnetic field sensors. The IceBridge team also has set up ground stations at McMurdo to collect global positioning system data.
Mission planners worked with the National Science Foundation and the U.S. Antarctic Program for more than a year laying the groundwork for this campaign. The IceBridge project science office is located at Goddard.
Space Station Live: Nov. 15, 2013
The Space Station Live recap video for Nov. 15, 2013. Watch the full
Space Station Live broadcast weekdays on NASA TV at 10 a.m. CST. http://www.nasa.gov/ntv
Exploring the Third Dimension of Cassiopeia A
One of the most famous objects in the sky - the Cassiopeia A
supernova remnant - will be on display like never before, thanks to
NASA's Chandra X-ray Observatory and a new project from the Smithsonian
Institution. A new three-dimensional (3D) viewer, being unveiled this
week, will allow users to interact with many one-of-a-kind objects from
the Smithsonian as part of a large-scale effort to digitize many of the
Institutions objects and artifacts.
Scientists have combined data from Chandra, NASA's Spitzer Space Telescope, and ground-based facilities to construct a unique 3D model of the 300-year old remains of a stellar explosion that blew a massive star apart, sending the stellar debris rushing into space at millions of miles per hour. The collaboration with this new Smithsonian 3D project will allow the astronomical data collected on Cassiopeia A, or Cas A for short, to be featured and highlighted in an open-access program -- a major innovation in digital technologies with public, education, and research-based impacts.
To coincide with Cas A being featured in this new 3D effort, a specially-processed version of Chandra's data of this supernova remnant is also being released. This new image shows with better clarity the appearance of Cas A in different energy bands, which will aid astronomers in their efforts to reconstruct details of the supernova process such as the size of the star, its chemical makeup, and the explosion mechanism. The color scheme used in this image is the following: low-energy X-rays are red, medium-energy ones are green, and the highest-energy X-rays detected by Chandra are colored blue.
Cas A is the only astronomical object to be featured in the new Smithsonian 3D project. This and other objects in the collection - including the Wright brothers plane, a 1,600-year-old stone Buddha, a gunboat from the Revolutionary War, and fossil whales from Chile -- were being showcased in the Smithsonian X 3D event, taking place on November 13th and 14th at the Smithsonian in Washington, DC. In addition to new state-of-the-art 3D viewer, the public will be able to explore these objects through original videos, online tours, and other supporting materials.
Cas A is the only supernova remnant to date to be modeled in 3D. In order to create this visualization, unique software that links the fields of astrophysics and medical imaging (known as "astronomical medicine") was used. Since its initial release in 2009, the 3D model has proven a rich resource for scientists as well as an effective tool for communicating science to the public. Providing this newly formatted data in an open source framework with finely-tuned contextual materials will greatly broaden awareness and participation for general public, teacher, student and researcher audiences.
NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory controls Chandra's science and flight operations from Cambridge, Mass.
Scientists have combined data from Chandra, NASA's Spitzer Space Telescope, and ground-based facilities to construct a unique 3D model of the 300-year old remains of a stellar explosion that blew a massive star apart, sending the stellar debris rushing into space at millions of miles per hour. The collaboration with this new Smithsonian 3D project will allow the astronomical data collected on Cassiopeia A, or Cas A for short, to be featured and highlighted in an open-access program -- a major innovation in digital technologies with public, education, and research-based impacts.
To coincide with Cas A being featured in this new 3D effort, a specially-processed version of Chandra's data of this supernova remnant is also being released. This new image shows with better clarity the appearance of Cas A in different energy bands, which will aid astronomers in their efforts to reconstruct details of the supernova process such as the size of the star, its chemical makeup, and the explosion mechanism. The color scheme used in this image is the following: low-energy X-rays are red, medium-energy ones are green, and the highest-energy X-rays detected by Chandra are colored blue.
Cas A is the only astronomical object to be featured in the new Smithsonian 3D project. This and other objects in the collection - including the Wright brothers plane, a 1,600-year-old stone Buddha, a gunboat from the Revolutionary War, and fossil whales from Chile -- were being showcased in the Smithsonian X 3D event, taking place on November 13th and 14th at the Smithsonian in Washington, DC. In addition to new state-of-the-art 3D viewer, the public will be able to explore these objects through original videos, online tours, and other supporting materials.
Cas A is the only supernova remnant to date to be modeled in 3D. In order to create this visualization, unique software that links the fields of astrophysics and medical imaging (known as "astronomical medicine") was used. Since its initial release in 2009, the 3D model has proven a rich resource for scientists as well as an effective tool for communicating science to the public. Providing this newly formatted data in an open source framework with finely-tuned contextual materials will greatly broaden awareness and participation for general public, teacher, student and researcher audiences.
NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory controls Chandra's science and flight operations from Cambridge, Mass.
2013/11/13
Space Station Live: Nov. 13, 2013
The Space Station Live recap video for Nov. 13, 2013. Watch the full
Space Station Live broadcast weekdays on NASA TV at 10 a.m. CST. http://www.nasa.gov/ntv
NASA Hails Success of Commercial Space Program
NASA Administrator Charles Bolden Wednesday hailed the success of the agency’s public-private partnership with American companies to resupply the International Space Station and announced the next phase of contracting with U.S. companies to transport astronauts is set to begin next week.
A little more than two years after the end of the Space Shuttle Program, the United States now has two space transportation systems capable of delivering science experiments and supplies from U.S. soil to the International Space Station. Under an ambitious plan funded by the Obama Administration, the agency is seeking to partner with American companies to send NASA astronauts to the space station as soon as 2017.
Bolden provided remarks at NASA Headquarters in Washington as agency officials announced the successful conclusion of the Commercial Orbital Transportation Services (COTS) program, an initiative that aimed to achieve safe, reliable and cost-effective commercial transportation to and from the space station and low-Earth orbit.
The rockets and spacecraft developed by NASA's partners Space Exploration Technologies Corp. (SpaceX) and Orbital Sciences Corp. under COTS have significantly increased NASA's ability to conduct new scientific investigations aboard the orbiting laboratory. All current and planned U.S. experiments aboard the station will be facilitated in some way by a SpaceX or Orbital Sciences resupply mission.
"America’s best days in space exploration are ahead of us thanks to the grit and determination of those in government, and the private sector, who dare to dream big dreams and have the skills to turn them into reality," Bolden said. "We’ve ended the outsourcing of space station resupply work and brought those jobs back home to America. The commercial space industry will be an engine of 21st century American economic growth and will help us carry out even more ambitious deep space exploration missions."
SpaceX was selected as a NASA partner in 2006 to develop its Dragon spacecraft and Falcon 9 rocket. SpaceX completed its COTS development with a demonstration mission to the space station in 2012, restoring an American capability to deliver and return cargo for the first time since the retirement of the space shuttle in 2011.
SpaceX has since flown the first two of 12 contracted cargo resupply flights to the space station through a $1.6 billion Commercial Resupply Services (CRS) contract with NASA.
The COTS program was a great success -- not only for NASA and the commercial space industry, but also the American taxpayer," said Gwynne Shotwell, SpaceX president and COO. "Together, NASA and SpaceX restored cargo transport capabilities to the United States and also laid the foundation for the future transport of American astronauts. SpaceX appreciates NASA’s ongoing support and is honored to partner with them in these efforts."
Orbital Sciences was selected as a NASA partner in 2008 and completed development of its Cygnus spacecraft and Antares rocket in October with a successful demonstration mission to the space station. The final review of the mission by NASA this month marked the beginning of closeout activities for the COTS program. Orbital Sciences is poised to launch the first of its eight cargo resupply missions to the space station in December through its $1.9 billion CRS contract with NASA.
"Orbital’s successful completion of the COTS program, including two launches of the new Antares rocket and the first mission to the International Space Station by the Cygnus cargo logistics spacecraft, was the direct result of the outstanding collaboration between the NASA and Orbital engineering and program management teams," said Frank Culbertson, Executive Vice President and General Manager of Orbital’s Advanced Programs Group. "The unique structure of the COTS initiative, under which NASA’s technical expertise, experienced human spaceflight workforce, and well-honed safety operations standards provided the overall framework, enabled Orbital to bring the energy, innovation and discipline of the commercial sector to the program, resulting in a reliable and cost-effective resupply service."
Orbital Sciences and SpaceX offer some similar capabilities to resupply cargo, ensuring NASA can maintain continuity in delivering critical supplies for space station crews. Each company also offers unique capabilities of importance to NASA. Orbital Sciences' Cygnus spacecraft can carry a large pressurized volume of cargo. Cygnus burns up in Earth's atmosphere on reentry, which allows astronauts to discard items no longer needed aboard the station by loading them inside the spacecraft before its departure. SpaceX's Dragon is the only spacecraft in the world capable of returning large amounts of cargo from space, which includes science experiments conducted aboard the station that can be delivered to researchers on Earth. Dragon also can carry unpressurized cargo, destined for the exterior of the space station, underneath the spacecraft.
Throughout the COTS program, NASA's partners achieved a number of important spaceflight firsts for the U.S. commercial space industry. This included the first commercial spacecraft to orbit and return to Earth, achieved by SpaceX. The company also was the first commercial provider to resupply the space station. Orbital Sciences was the first company to launch to the space station from Virginia, beginning its mission from the new Mid-Atlantic Regional Spaceport Pad-0A at NASA's Wallops Flight Facility in Wallops Island, Va.
NASA and its Commercial Crew Program partners also are working to develop the next generation of U.S. spacecraft and rockets capable of transporting humans to and from low-Earth orbit from American soil. NASA intends to use new commercial capabilities to fly U.S. astronauts to and from the International Space Station within the next four years. On Nov. 19, the agency will issue a final Request for Proposals for the new Commercial Crew Transportation Capability (CCTCap) contract, designed to ensure commercial companies meet NASA’s safety requirements for transporting NASA crews to the space station. This procurement phase is expected to include crewed demonstration missions to the space station before 2017.
MAVEN Spacecraft Positioned Atop Atlas V Rocket
NASA's MAVEN (Mars Atmosphere and Volatile EvolutioN) spacecraft,
inside a payload fairing, is hoisted to the top of a United Launch
Alliance Atlas V rocket at the Vertical Integration Facility at Cape
Canaveral Air Force Station's Space Launch Complex 41. The move and
hoisting operations mark another major milestone for the launch team as
everything proceeds on schedule to launch Nov. 18, when the Atlas V will
lift MAVEN into space and on to Mars. The two-hour launch window
extends from 1:28 to 3:28 p.m. EST.
MAVEN is the first spacecraft devoted to exploring and understanding the Martian upper atmosphere. It will orbit the planet in an elliptical orbit that allows it to pass through and sample the entire upper atmosphere on every orbit. The spacecraft will investigate how the loss of Mars' atmosphere to space determined the history of water on the surface.
MAVEN is the first spacecraft devoted to exploring and understanding the Martian upper atmosphere. It will orbit the planet in an elliptical orbit that allows it to pass through and sample the entire upper atmosphere on every orbit. The spacecraft will investigate how the loss of Mars' atmosphere to space determined the history of water on the surface.
Expedition 38/39 Mission Overview
Commander Oleg Kotov, veteran of two previous station missions, leads
Expedition 38 as the six-member crew conducts advanced microgravity
research aboard the International Space Station. Flight Engineers Mike
Hopkins and Sergey Ryazanskiy, who launched with Kotov Sept. 25, are
both on their first spaceflight missions.
Flight Engineers Rick Mastracchio, Koichi Wakata and Mikhail Tyurin delivered the Olympic torch to the station Nov. 6. Kotov and Ryazanskiy carried the torch outside the station during a spacewalk Nov. 9.
Expedition 36/37 crew members Fyodor Yurchikhin, Karen Nyberg and Luca Parmitano returned the torch when they landed in Kazakhstan Nov. 10 as part of the traditional relay leading up to to the 2014 Winter Olympics in Sochi, Russia.
Flight Engineers Rick Mastracchio, Koichi Wakata and Mikhail Tyurin delivered the Olympic torch to the station Nov. 6. Kotov and Ryazanskiy carried the torch outside the station during a spacewalk Nov. 9.
Expedition 36/37 crew members Fyodor Yurchikhin, Karen Nyberg and Luca Parmitano returned the torch when they landed in Kazakhstan Nov. 10 as part of the traditional relay leading up to to the 2014 Winter Olympics in Sochi, Russia.
Space Station Live: Nov. 12, 2013
The Space Station Live recap video for Nov. 12, 2013. Watch the full
Space Station Live broadcast weekdays on NASA TV at 10 a.m. CST. http://www.nasa.gov/ntv
NASA Satellites Track Typhoon Haiyan's Second Landfall and Flood Potential
NASA satellites provided data to meteorologists at the Joint Typhoon Warning Center who were updating forecasts for Tropical Storm Haiyan as it weakened from a typhoon and made a second landfall in northern Vietnam.
NASA's Tropical Rainfall Measuring Mission or TRMM satellite can measure rainfall from space and estimate potential flooding and landslides. An animation of TRMM rainfall data was created at NASA's Goddard Space Flight Center in Greenbelt, Md. to map that rainfall. A TRMM animation of flood potential from Nov. 2 to Nov. 12 showed the movement of Tropical Storm 30W, Typhoon Krosa and Super-Typhoon Hainan in the western North Pacific Ocean. The animation showed the Tropical Storm 30W drenched the central Philippines days before Super-Typhoon Haiyan made landfall and increased flood potential to "high."
Haiyan made landfall in northeastern Vietnam and on Nov. 11 at 2100 UTC/4 p.m. EDT with maximum sustained winds of 75 miles/120 km per hour, and continued moving northeast through southern China. Satellite data showed the extent of the tropical storm's cloud cover that stretched from northeastern Vietnam over southeastern China.
On Nov. 10 at 03:30 UTC/Nov. 9 at 10:30 p.m. EDT, the Moderate Resolution Imaging Spectroradiometer or MODIS instrument aboard NASA's Terra satellite showed the center of Typhoon Haiyan was just south of Hainan Island, China in the South China Sea. Later in the day, Haiyan moved north of Hainan Island and headed for a landfall in extreme northeastern Vietnam. Haiyan's maximum sustained winds were near 75 knots/86 mph/138.9 kph. At 1500 UTC/10 a.m. EDT on Nov. 10. At that time it was centered near 19.8 north and 107.9 east, about 160 nautical miles southeast of Hanoi, Vietnam, and moving to the north-northwest at 17 knots/19/5 mph/31.48 kph.
According to RT news.com more than 174,000 households were evacuated, which is about 600,000 people. Haiyan was forecast to make landfall on Nov. 11 at 0000 UTC/8 a.m. Nov 8 local time/(7 p.m. EST Nov. 10), near the Cam Pha District, which is over 100 miles east of Hanoi. Early on Nov. 11, Haiyan made landfall in extreme northeastern Vietnam, as predicted.
On Nov. 11 at 0300 UTC/10 a.m. Vietnam local time/Nov. 10 at 9 p.m. EDT Haiyan was moving over land and its maximum sustained winds were still near 60 knots/69 mph/111.1 kph. The center of the tropical storm was located near 22.2 north and 107.4 east, just 87 nautical miles northeast of Hanoi, Vietnam. Haiyan was moving to the north at 13 knots/14.9 mph/24.0 kph.
Animated enhanced infrared satellite imagery showed the storm was weakening quickly while over land and that bulk of the thunderstorms (and convection) had been pushed north of the center as a result of increasing winds shear from the southwest. On Nov. 11 at 05:45 UTC, the Moderate Resolution Imaging Spectroradiometer or MODIS instrument aboard NASA's Aqua satellite captured an image of Tropical Storm Haiyan over mainland China. The MODIS image showed the extent of cloud cover from northeastern Vietnam over the Guangxi, Guangdong, Hunan, Guizhou, Sichuan, Chongqing, Hubei, Shaanxi, Henan, Anhui and Jaingxi provinces.
Mid-latitude westerly winds moving over China helped weaken the storm. Haiyan is forecast to turn to the east and dissipate in the next day.
Typhoon Haiyan Pounding Hainan Island, China
The Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Terra satellite captured this image of Typhoon Haiyan just south of Hainan Island, China and approaching Vietnam on November 10, 2013. The storm was tracking northwest and slowly weakening prior to landfall in northern Vietnam on Sunday evening (Monday morning, local time). As of early Sunday morning, the storm had maximum sustained winds of about 90 miles (145 kilometers) per hour, the equivalent of a category 1 storm. Haiyan crossed the Philippines as a Super-Typhoon and headed for Indochina in early November 2013.
Spitzer and ALMA Reveal a Star's Bubbly Birth
It's a bouncing baby . . . star! Combined observations from NASA's
Spitzer Space Telescope and the newly completed Atacama Large
Millimeter/submillimeter Array (ALMA) in Chile have revealed the throes
of stellar birth as never before in the well-studied object known as HH
46/47.
Herbig-Haro (HH) objects form when jets shot out by newborn stars collide with surrounding material, producing small, bright, nebulous regions. To our eyes, the dynamics within many HH objects are obscured by enveloping gas and dust. But the infrared and submillimeter wavelengths of light seen by Spitzer and ALMA, respectively, pierce the dark cosmic cloud around HH 46/47 to let us in on the action.
The Spitzer observations show twin supersonic jets emanating from the central star that blast away surrounding gas and set it alight into two bubbly lobes. HH 46/47 happens to sit on the edge of its enveloping cloud in such a way that the jets pass through two differing cosmic environments. The rightward jet, heading into the cloud, is plowing through a "wall" of material, while the leftward jet's path out of the cloud is relatively unobstructed, passing through less material. This orientation serves scientists well by offering a handy compare-and-contrast setup for how the outflows from a developing star interact with their surroundings.
"Young stars like our sun need to remove some of the gas collapsing in on them to become stable, and HH 46/47 is an excellent laboratory for studying this outflow process," said Alberto Noriega-Crespo, a scientist at the Infrared Processing and Analysis Center at the California Institute of Technology, Pasadena, Calif. "Thanks to Spitzer, the HH 46/47 outflow is considered one of the best examples of a jet being present with an expanding bubble-like structure."
Noriega-Crespo led the team that began studying HH 46/47 with Spitzer nearly 10 years ago when the telescope first began observing the heavens. Now, using a new image processing technique developed in the past few years, he and his colleagues have been able to render HH 46/47 in higher resolution.
Meanwhile, the fresh views of HH 46/47 by ALMA have revealed that the gas in the lobes is expanding faster than previously thought. This faster expansion has an influence on the overall amount of turbulence in the gaseous cloud that originally spawned the star. In turn, the extra turbulence could have an impact on whether and how other stars might form in this gaseous, dusty, and thus fertile, ground for star-making.
A team led by Hector Arce at Yale University, New Haven, Conn., carried out the ALMA observations and their analysis was published recently in The Astrophysical Journal.
NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology in Pasadena. Spacecraft operations are based at Lockheed Martin Space Systems Company, Littleton, Colorado. Data are archived at the Infrared Science Archive housed at the Infrared Processing and Analysis Center at Caltech. Caltech manages JPL for NASA. For more information about Spitzer, visit http://spitzer.caltech.edu and http://www.nasa.gov/spitzer.
The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of Europe, North America and East Asia in cooperation with the Republic of Chile.
Herbig-Haro (HH) objects form when jets shot out by newborn stars collide with surrounding material, producing small, bright, nebulous regions. To our eyes, the dynamics within many HH objects are obscured by enveloping gas and dust. But the infrared and submillimeter wavelengths of light seen by Spitzer and ALMA, respectively, pierce the dark cosmic cloud around HH 46/47 to let us in on the action.
The Spitzer observations show twin supersonic jets emanating from the central star that blast away surrounding gas and set it alight into two bubbly lobes. HH 46/47 happens to sit on the edge of its enveloping cloud in such a way that the jets pass through two differing cosmic environments. The rightward jet, heading into the cloud, is plowing through a "wall" of material, while the leftward jet's path out of the cloud is relatively unobstructed, passing through less material. This orientation serves scientists well by offering a handy compare-and-contrast setup for how the outflows from a developing star interact with their surroundings.
"Young stars like our sun need to remove some of the gas collapsing in on them to become stable, and HH 46/47 is an excellent laboratory for studying this outflow process," said Alberto Noriega-Crespo, a scientist at the Infrared Processing and Analysis Center at the California Institute of Technology, Pasadena, Calif. "Thanks to Spitzer, the HH 46/47 outflow is considered one of the best examples of a jet being present with an expanding bubble-like structure."
Noriega-Crespo led the team that began studying HH 46/47 with Spitzer nearly 10 years ago when the telescope first began observing the heavens. Now, using a new image processing technique developed in the past few years, he and his colleagues have been able to render HH 46/47 in higher resolution.
Meanwhile, the fresh views of HH 46/47 by ALMA have revealed that the gas in the lobes is expanding faster than previously thought. This faster expansion has an influence on the overall amount of turbulence in the gaseous cloud that originally spawned the star. In turn, the extra turbulence could have an impact on whether and how other stars might form in this gaseous, dusty, and thus fertile, ground for star-making.
A team led by Hector Arce at Yale University, New Haven, Conn., carried out the ALMA observations and their analysis was published recently in The Astrophysical Journal.
NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology in Pasadena. Spacecraft operations are based at Lockheed Martin Space Systems Company, Littleton, Colorado. Data are archived at the Infrared Science Archive housed at the Infrared Processing and Analysis Center at Caltech. Caltech manages JPL for NASA. For more information about Spitzer, visit http://spitzer.caltech.edu and http://www.nasa.gov/spitzer.
The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of Europe, North America and East Asia in cooperation with the Republic of Chile.
2013/11/10
Expedition 37 heads home
Expedition 37 Commander Fyodor Yurchikhin, NASA Flight Engineer Karen
Nyberg and European Space Agency Flight Engineer Luca Parmitano undocked
from the International Space Station to begin their journey back to
Earth. The trio completed 166 days in space since launching in late May.
Expedition 37 Crew, Olympic Torch Returning to Earth
Three Expedition 37 crew members are on their way back to Earth after 166 days aboard the International Space Station.
Soyuz Commander Fyodor Yurchikhin and Flight Engineers Karen Nyberg and Luca Parmitano undocked their Soyuz TMA-09M spacecraft from aft end the Zvezda service module at 6:26 p.m. EST Sunday to begin the journey home. At the time of the undocking, the complex was orbiting 262 miles over northeast Mongolia.
A deorbit burn at 8:55 p.m. will put the Soyuz on track for a parachute-assisted landing in the steppe of Kazakhstan southeast of Dzhezkazgan at 9:49 p.m. (8:49 a.m. Monday, Kazakh time).
NASA Television will air live coverage of the Soyuz landing activities beginning at 8:30 p.m.
› Watch NASA TV
The undocking marked the end of Expedition 37 and the start of
Expedition 38 under the command of Oleg Kotov. Yurchikhin passed the
helm of the station over to Kotov during a change of command ceremony
Sunday. After making their final farewells, Yurchikhin, Parmitano and
Nyberg boarded their Soyuz, and the crews closed the hatches between
the vehicles at 3:09 p.m.
› Watch change of command ceremony
› Watch crew farewell and hatch closing
Returning to Earth along with Yurchikhin, Nyberg and Parmitano is the torch that will be used to light the Olympic flame at the Feb. 7 opening ceremonies of the 2013 Winter Olympic Games in Sochi, Russia.
The Olympic torch arrived at the space station Thursday aboard the Soyuz TMA-11M spacecraft carrying three new crew members – Expedition 38 Flight Engineers Mikhail Tyurin, Rick Mastracchio and Koichi Wakata. To accommodate their arrival, Yurchikhin, Nyberg and Parmitano relocated their Soyuz spacecraft on Nov. 1 from the Rassvet module where it had been docked since May 28 over to Zvezda. The arrival of Mastracchio, Wakata and Tyurin marked the first time since October 2009 that nine people have served together aboard the station without the presence of a space shuttle.
› Read more about the Expedition 38 launch and docking
› Read more about the Soyuz relocation
Kotov and Flight Engineer Sergey Ryazanskiy relayed the torch outside the station Saturday during a spacewalk to continue setting up a combination extravehicular activity workstation and biaxial pointing platform and deactivate a completed experiment.
› Read more about the spacewalk
Kotov, Ryazanskiy and Flight Engineer Mike Hopkins, who launched and docked to the station aboard the Soyuz TMA-10M vehicle on Sept. 25, will return to Earth on March 12. Their departure will signify the beginning of Expedition 39 under the command of Wakata, the first Japan Aerospace Exploration Agency astronaut entrusted with that position
Soyuz Commander Fyodor Yurchikhin and Flight Engineers Karen Nyberg and Luca Parmitano undocked their Soyuz TMA-09M spacecraft from aft end the Zvezda service module at 6:26 p.m. EST Sunday to begin the journey home. At the time of the undocking, the complex was orbiting 262 miles over northeast Mongolia.
A deorbit burn at 8:55 p.m. will put the Soyuz on track for a parachute-assisted landing in the steppe of Kazakhstan southeast of Dzhezkazgan at 9:49 p.m. (8:49 a.m. Monday, Kazakh time).
NASA Television will air live coverage of the Soyuz landing activities beginning at 8:30 p.m.
› Watch NASA TV
› Watch crew farewell and hatch closing
Returning to Earth along with Yurchikhin, Nyberg and Parmitano is the torch that will be used to light the Olympic flame at the Feb. 7 opening ceremonies of the 2013 Winter Olympic Games in Sochi, Russia.
The Olympic torch arrived at the space station Thursday aboard the Soyuz TMA-11M spacecraft carrying three new crew members – Expedition 38 Flight Engineers Mikhail Tyurin, Rick Mastracchio and Koichi Wakata. To accommodate their arrival, Yurchikhin, Nyberg and Parmitano relocated their Soyuz spacecraft on Nov. 1 from the Rassvet module where it had been docked since May 28 over to Zvezda. The arrival of Mastracchio, Wakata and Tyurin marked the first time since October 2009 that nine people have served together aboard the station without the presence of a space shuttle.
› Read more about the Expedition 38 launch and docking
› Read more about the Soyuz relocation
Kotov and Flight Engineer Sergey Ryazanskiy relayed the torch outside the station Saturday during a spacewalk to continue setting up a combination extravehicular activity workstation and biaxial pointing platform and deactivate a completed experiment.
› Read more about the spacewalk
Kotov, Ryazanskiy and Flight Engineer Mike Hopkins, who launched and docked to the station aboard the Soyuz TMA-10M vehicle on Sept. 25, will return to Earth on March 12. Their departure will signify the beginning of Expedition 39 under the command of Wakata, the first Japan Aerospace Exploration Agency astronaut entrusted with that position
2013/11/09
Expedition 37 flight controllers on console with Flight Director Courtenay McMillan during grapple
PHOTO DATE: 10-22-13
LOCATION: Bldg. 30 - FCR-1 (30M/231)
SUBJECT: Expedition 37 flight controllers on console with Flight Director Courtenay McMillan during grapple and unberthing of the Orbital Sciences/Cygnus cargo ship from the nadir port of the Harmony module on ISS.
PHOTOGRAPHER: BILL STAFFORD
LOCATION: Bldg. 30 - FCR-1 (30M/231)
SUBJECT: Expedition 37 flight controllers on console with Flight Director Courtenay McMillan during grapple and unberthing of the Orbital Sciences/Cygnus cargo ship from the nadir port of the Harmony module on ISS.
PHOTOGRAPHER: BILL STAFFORD
Olympic Torch Highlights Station Spacewalk
Two Russian cosmonauts clad in Orlan spacesuits conducted an out-of-this-world hand-off of the Olympic torch at the start of Saturday’s 5-hour, 50-minute spacewalk to perform maintenance on the International Space Station.
Expedition 37 Flight Engineers Oleg Kotov and Sergey Ryazanskiy opened the hatch to the Pirs docking compartment at 9:34 a.m. EST and floated outside to begin a photo opportunity with the unlit torch.
› View video of spacewalkers with Olympic torch
An icon of international cooperation through sports competition, the Olympic torch arrived at the space station Thursday aboard a Soyuz spacecraft carrying three new crew members – Expedition 38 Flight Engineers Mikhail Tyurin, Rick Mastracchio and Koichi Wakata. On Sunday, the torch will return to Earth aboard another Soyuz spacecraft vehicle along with Expedition 37 Commander Fyodor Yurchikhin and Flight Engineers Karen Nyberg and Luca Parmitano.
The spacewalk was a high-flying extension of a relay that will culminate with the torch being used to light the Olympic flame at the Feb. 7 opening ceremonies of the 2014 Winter Olympic Games in Sochi, Russia.
After Kotov and Ryazanskiy completed their photo and video session with the torch outside the station, they stowed it back inside the airlock and proceeded with the remainder of their chores 260 miles above the Earth.
The two spacewalkers translated out to the hull of the Zvezda service module to continue the set up of a combination extravehicular activity workstation and biaxial pointing platform that was installed during an Expedition 36 spacewalk on Aug. 22.
After installing some handrails on the workstation, Kotov and Ryazanskiy loosened a trio of bolts and removed a launch bracket from the pointing platform. A high resolution camera system will be installed on the platform during a spacewalk targeted for December.
The installation of a foot restraint on the mounting seat of the workstation was deferred to a future spacewalk after the spacewalkers noticed some issues with its alignment.
For their final planned task, Kotov and Ryazanskiy deactivated the Radiometria experiment package on Zvezda. Designed to collect information useful in seismic forecasts and earthquake predictions, Radiometria was installed on the station during an Expedition 26 spacewalk in February 2011. After securing the experiment's cables, the spacewalkers headed back to the airlock to wrap up the excursion. The task to fold down and restrain Radiometria's antenna was deferred to a future spacewalk.
The duo closed the Pirs hatch at 3:24 p.m., marking the official end of the spacewalk.
During the spacewalk, Yurchikhin, Parmitano and Nyberg were isolated to their Soyuz TMA-09M spacecraft and Zvezda, while Flight Engineer Mike Hopkins was restricted to the Poisk module and his Soyuz TMA-10M craft. The remaining three crew members -- Mastracchio, Wakata and Tyurin – had access to much of the remaining area of the station, including the Zarya module, their Soyuz TMA-11M vehicle and the Rassvet module to which it is docked, as well as the entirety of the U.S. segment of the station.
Saturday’s spacewalk was the 174th in support of space station assembly and maintenance, the fourth in Kotov's career and the first for Ryazanskiy. Kotov, who was designated EV1 for the spacewalk wore the suit with red stripes. Ryazanskiy, EV2, wore the suit marked with blue stripes.
This was the eighth spacewalk conducted at the station this year. In December, Tyurin will accompany Kotov on his fifth spacewalk.
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