mercredi 21 juin 2017

Proba-V images Portuguese forest fire












ESA - Proba-5 Mission logo.

21 June 2017

ESA’s Proba-V minisatellite has captured the forest fire raging in central Portugal, revealing blackened scars and columns of smoke as well as pinpointing active fire hotspots.

Portugal fire

More than a thousand firefighters are tackling the forest fire in the Pedrógão Grande region, north east of Lisbon, which has been aflame since Saturday. Some 64 people have been reported dead and more than 130 injured.

The dammed Zêzere river is seen in the centre of the main image, with burnt scars and fires burning to its north. The village of Nodeirinho – home of many of the casualties – is situated amid the scars.

Before the blaze

The forest fire is believed to have been started by a lightning strike during an intense heatwave. Aircraft have been used to drop water over the Pedrógão Grande region.

Showing details down to 100 m in size, the main image was acquired on Tuesday by Proba-V. Among ESA’s smallest Earth-observing missions, at a cubic metre, Proba-V covers the world’s entire land surface every two days.

Proba-V satellite

Proba-V has a 2250 km-wide field of view with an overall 300 m resolution, narrowing to 100 m at the centre.  A second 330 m-resolution image acquired on Saturday provides a wider context to the blaze.

Regional view of fire

The satellite contributes to Europe’s world-monitoring Copernicus programme, which makes imagery and data freely available to authorities. The V stands for Vegetation – a lighter but fully functional redesign of the camera previously flown on France’s full-sized Spot-4 and Spot-5 satellites.

Launched on 7 May 2013, Proba-V continues the supply of this much-needed information for applications such as assessing climate impact, managing water resources and monitoring crops.

Sentinel-3 images fire

Proba-V’s wide view and polar orbit means it revisits every spot on Earth’s land every two days, building up a new global composite for researchers every 10 days.

More than 1100 registered users in 108 countries are already making use of the satellite.

The Copernicus Sentinel-3 mission has also observed the fire, showing the extent of the burnt area.

Related links:

Proba Missions: http://www.esa.int/Our_Activities/Space_Engineering_Technology/Proba_Missions

In depth: Proba-V: https://earth.esa.int/web/guest/missions/esa-operational-eo-missions/proba-v

Proba-V Mission Exploitation Platform: http://proba-v-mep.esa.int/

Sentinel-3: http://www.esa.int/Our_Activities/Observing_the_Earth/Copernicus/Sentinel-3

Images, Text, Credits: ESA/P.Carril /Belpso produced by VITO.

Greetings, Orbiter.ch

Gravitational wave mission selected, planet-hunting mission moves forward












ESA - LISA Pathfinder Mission patch.

21 June 2017

The LISA trio of satellites to detect gravitational waves from space has been selected as the third large-class mission in ESA’s Science programme, while the Plato exoplanet hunter moves into development.

These important milestones were decided upon during a meeting of ESA’s Science Programme Committee today, and ensure the continuation of ESA’s Cosmic Vision plan through the next two decades.

Merging black holes

The ‘gravitational universe’ was identified in 2013 as the theme for the third large-class mission, L3, searching for ripples in the fabric of spacetime created by celestial objects with very strong gravity, such as pairs of merging black holes.

Predicted a century ago by Albert Einstein's general theory of relativity, gravitational waves remained elusive until the first direct detection by the ground-based Laser Interferometer Gravitational-Wave Observatory in September 2015. That signal was triggered by the merging of two black holes some 1.3 billion light-years away. Since then, two more events have been detected.

Furthermore, ESA’s LISA Pathfinder mission has also now demonstrated key technologies needed to detect gravitational waves from space. This includes free-falling test masses linked by laser and isolated from all external and internal forces except gravity, a requirement to measure any possible distortion caused by a passing gravitational wave.

The distortion affects the fabric of spacetime on the minuscule scale of a few millionths of a millionth of a metre over a distance of a million kilometres and so must be measured extremely precisely.

LISA concept

LISA Pathfinder will conclude its pioneering mission at the end of this month, and LISA, the Laser Interferometer Space Antenna, also an international collaboration, will now enter a more detailed phase of study. Three craft, separated by 2.5 million km in a triangular formation, will follow Earth in its orbit around the Sun.

Following selection, the mission design and costing can be completed. Then it will be proposed for ‘adoption’ before construction begins. Launch is expected in 2034.

Planet-hunter adopted

In the same meeting Plato – Planetary Transits and Oscillations of stars – has now been adopted in the Science Programme, following its selection in February 2014.

This means it can move from a blueprint into construction. In the coming months industry will be asked to make bids to supply the spacecraft platform.

Searching for exoplanetary systems

Following its launch in 2026, Plato will monitor thousands of bright stars over a large area of the sky, searching for tiny, regular dips in brightness as their planets cross in front of them, temporarily blocking out a small fraction of the starlight.

The mission will have a particular emphasis on discovering and characterising Earth-sized planets and super-Earths orbiting Sun-like stars in the habitable zone – the distance from the star where liquid surface water could exist.

It will also investigate seismic activity in some of the host stars, and determine their masses, sizes and ages, helping to understand the entire exoplanet system.

Plato will operate from the ‘L2’ virtual point in space 1.5 million km beyond Earth as seen from the Sun.

Mission opportunity

The Science Programme Committee also agreed on participation in ESA’s Proba-3 technology mission, a pair of satellites that will fly in formation just 150 m apart, with one acting as a blocking disc in front of the Sun, allowing the other to observe the Sun’s faint outer atmosphere in more detail than ever before.

Proba-3

ESA will also participate in Japan’s X-ray Astronomy Recovery Mission (XARM), designed to recover the science of the Hitomi satellite that was lost shortly after launch last year.

Related links:

ESA’s Cosmic Vision: http://sci.esa.int/cosmic-vision/

ESA’s LISA Pathfinder: http://sci.esa.int/lisa-pathfinder/

ESA’s Proba-3: http://www.esa.int/Our_Activities/Space_Engineering_Technology/Proba_Missions/Proba-3_seeing_through_shadow_to_view_Sun_s_corona

Hitomi satellite: http://sci.esa.int/hitomi/

Images, Text, Credits: ESA/C.Carreau/P. Carril/AEI/Milde Marketing/Exozet.

Best regards, Orbiter.ch

mardi 20 juin 2017

Dragon Packing and BEAM Checks Onboard Station Today










ISS - Expedition 52 Mission patch.

June 20, 2017

The Expedition 52 crew is loading the SpaceX Dragon with cargo for return back to Earth in less than two weeks. BEAM, the experimental habitat, also received a new radiation shield today that was 3D printed aboard the International Space Station.

Dragon is due to leave the International Space Station July 2 after cargo transfers with the resupply ship are complete. The crew offloaded new science experiments, spacewalking gear and station hardware shortly after it arrived on June 5. Dragon will now be packed with used station gear and research samples for analysis by NASA engineers and scientists after it splashes down in the Pacific Ocean.


Image above: NASA astronauts Peggy Whitson and Jack Fischer are pictured packing up gear inside the International Space Station. Image Credit: NASA.

Flight Engineer Jack Fischer opened up BEAM today and entered the expandable activity module for a regular checkup. He replaced an older radiation shield with a thicker shield that covers a radiation sensor inside BEAM. Fischer also sampled BEAM’s air and surfaces for microbes.

Veteran astronaut Peggy Whitson of NASA spent Tuesday sampling the air and surfaces for microbes in the station’s U.S. segment. Whitson also spent some time stowing synthetic DNA samples exposed to radiation in a science freezer and began readying rodent research gear for return next month aboard Dragon.

Related links:

BEAM: https://www.nasa.gov/content/bigelow-expandable-activity-module

Space Station Research and Technology: https://www.nasa.gov/mission_pages/station/research/index.html

International Space Station (ISS): https://www.nasa.gov/mission_pages/station/main/index.html

Image (mentioned), Text, Credits: NASA/Mark Garcia.

Best regards, Orbiter.ch

Changing How Solar Power Rolls












ISS - International Space Station logo.

June 20, 2017

Traditional solar panels used to power satellites can be bulky with heavy panels folded together using mechanical hinges. An experiment that recently arrived at the International Space Station will test a new solar array design that rolls up to form a compact cylinder for launch with significantly less mass and volume, potentially offering substantial cost savings as well as an increase in power for satellites.

Smaller and lighter than traditional solar panels, the Roll-Out Solar Array, or ROSA, consists of a center wing made of a flexible material containing photovoltaic cells to convert light into electricity. On either side of the wing is a narrow arm that extends the length of the wing to provide support, called a high strain composite boom. The booms are like split tubes made of a stiff composite material, flattened and rolled up lengthwise for launch. The array rolls or snaps open without a motor, using stored energy from the structure of the booms that is released as each boom transitions from a coil shape to a straight support arm.


Animation above: The Roll-Out Solar Array (ROSA) was deployed from the end of the Canadarm2 robotic arm Sunday, June 18 outside the International Space Station. ROSA is an experiment to test a new type of solar array that rolls open in space like a party favor and is more compact than current rigid panel designs. Animation Credits: NASA Johnson.

ROSA can be easily adapted to different sizes, including very large arrays, to provide power for a variety of future spacecraft. It also has the potential to make solar arrays more compact and lighter weight for satellite radio and television, weather forecasting, GPS and other services used on Earth. In addition, the technology conceivably could be adapted to provide solar power in remote locations. The technology of the booms has additional potential applications, such as for communications and radar antennas and other instruments.

The ROSA investigation looks at how well this new type of solar panels deploys in the microgravity and extreme temperatures of space. The investigation also measures the array’s strength and durability and how the structure responds to spacecraft maneuvers.

“When the array is attached to a satellite, that spacecraft will need to maneuver, which creates torque and causes the wing, or blanket, to vibrate,” explains principal investigator Jeremy Banik, senior research engineer at the Air Force Research Laboratory, Kirtland Air Force Base in New Mexico. “We need to know precisely when and how it vibrates so as not to lose control of the spacecraft. The only way to test that is in space.”


Image above: Deployed wing image. Image Credits: Deployable Space Systems.

The investigation will monitor the array deployed in full sun and full shade and collect data on how much it vibrates when moving from shade to light. This vibration, known as thermal snap, could present challenges in operating satellites with sensitive functions, and the researchers want to learn how to avoid those challenges with ROSA.

“This structure is very thin, only a few millimeters thick, and heats up very quickly, dozens of degrees in a few seconds,” Banik says. “That creates loads in the wing that could cause it to shudder. That would create problems, for example, if a satellite was trying to take a picture at the same time.”

The investigation will measure power produced by the array to see how ROSA’s thin, crystalline photovoltaic cells hold up during launch. In addition, researchers want to see how the array handles retraction.


Image above: Deployment of the Space Station's Roll Out Solar Array Experiment. Image Credit: NASA.

“We want to show that we can pull the wing back in in a predictable way,” Banik says. “A practical reason is that we have to pull it back for stowage after this investigation, but it will be good to know it can be done for future applications, potentially for a highly maneuverable spacecraft.”

The intent of this investigation, Banik explained, is to compare on-orbit ROSA data to model predictions previously validated by on-ground measurements in a simulated environment.

“Recognize that we are trying to learn how it behaves – this is an experiment and not a demonstration – so we’ll glean useful data even if it doesn’t behave the ways we expect,” Banik said.

Investigators on the ground will initiate video of deployment and retraction, and sensors embedded on the array will record data on photovoltaic performance, temperature, and accelerations.

Roll-Out Solar Array Experiment (ROSA) Deploys on International Space Station

Video above: The Roll-Out Solar Array (ROSA) was deployed from the end of the Canadarm2 robotic arm Sunday, June 18 outside the International Space Station. ROSA is an experiment to test a new type of solar array that rolls open in space like a party favor and is more compact than current rigid panel designs. The ROSA investigation tests deployment and retraction,characterizes changes when the Earth blocks the sun, vibration and other physical challenges to determine the array’s strength and durability. ROSA has the potential to replace solar arrays on future satellites, making them more compact and lighter weight. Satellite radio and television, weather forecasting, GPS and other services used on Earth would all benefit from high-performance solar arrays. The payload will remain deployed for seven days before retracting and will be stowed back inside the trunk of SpaceX’s Dragon cargo vehicle. Note: footage of deploy is sped up 300%. Video Credits: NASA Johnson.

“When launching into space, mass and volume are everything, and ROSA is 20 percent lighter and four times smaller in volume than rigid panel arrays,” Banik says. “You realize big cost savings from shaving off a little mass and volume, which makes it possible to raise bandwidth on a communications satellite and, for example, make GPS more accessible and reliable for everyone.”

In other words, this little array could really change how solar power rolls.

ROSA was developed as part of the Solar Electric Propulsion project sponsored by NASA’s Space Technology Mission Directorate. NASA tested the ROSA technology in vacuum chambers on Earth several years ago, and this is its first test in space. This solar array technology was developed to power large spacecraft using highly-efficient electric propulsion on missions to deep space including Mars and the moon.

Related links:

Roll-Out Solar Array, or ROSA: https://www.nasa.gov/mission_pages/station/research/experiments/2139.html

Solar Electric Propulsion project: https://www.nasa.gov/mission_pages/tdm/sep/index.html

Space Station Research and Technology: https://www.nasa.gov/mission_pages/station/research/index.html

International Space Station (ISS): https://www.nasa.gov/mission_pages/station/main/index.html

Images (mentioned), Animation (mentioned), Video (mentioned), Text, Credits: NASA/Jennifer Harbaugh/JSC/Melissa Gaskill.

Best regards, Orbiter.ch

NASA Mars Orbiter Views Rover Climbing Mount Sharp












NASA - Mars Reconnaissance Orbiter (MRO) logo.

June 20, 2017


Image above: The feature that appears bright blue at the center of this scene is NASA's Curiosity Mars rover amid tan rocks and dark sand on Mount Sharp, as viewed by the HiRISE camera on NASA's Mars Reconnaissance Orbiter on June 5, 2017. The rover is about 10 feet long and not really as blue as it looks here. Image Credits: NASA/JPL-Caltech/Univ. of Arizona.

Using the most powerful telescope ever sent to Mars, NASA's Mars Reconnaissance Orbiter caught a view of the Curiosity rover this month amid rocky mountainside terrain.

The car-size rover, climbing up lower Mount Sharp toward its next destination, appears as a blue dab against a background of tan rocks and dark sand in the enhanced-color image from the orbiter's High Resolution Imaging Science Experiment (HiRISE) camera. The exaggerated color, showing differences in Mars surface materials, makes Curiosity appear bluer than it really looks.

The image was taken on June 5, 2017, two months before the fifth anniversary of Curiosity's landing near Mount Sharp on Aug. 5 PDT (Aug. 6, 2017, EDT and Universal Time).

When the image was taken, Curiosity was partway between its investigation of active sand dunes lower on Mount Sharp, and "Vera Rubin Ridge," a destination uphill where the rover team intends to examine outcrops where hematite has been identified from Mars orbit.

The rover's location that day is shown at https://mars.nasa.gov/multimedia/images/2017/curiositys-traverse-map-through-sol-1717 as the point labeled 1717. Images taken that day by Curiosity's Mast Camera (Mastcam) are at https://mars.nasa.gov/msl/multimedia/raw/?s=1717&camera=MAST%5F.

HiRISE obtains images of Curiosity a few times each year. The University of Arizona, Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., Boulder, Colorado. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project and Mars Science Laboratory Project for NASA's Science Mission Directorate, Washington.

For more information about NASA's Mars Reconnaissance Orbiter, visit:

https://mars.nasa.gov/mro/

For more information about NASA's Mars Science Laboratory Project and Curiosity, visit:

https://mars.nasa.gov/msl/

Image, Text, Credits: NASA/Laurie Cantillo/Dwayne Brown/Tony Greicius/JPL/Guy Webster.

Best regards, Orbiter.ch

NASA Completes Study of Future ‘Ice Giant’ Mission Concepts











NASA logo.

June 20, 2017

A NASA-led and NASA-sponsored study of potential future missions to the mysterious “ice giant” planets Uranus and Neptune has been released—the first in a series of mission studies NASA will conduct in support of the next Planetary Science Decadal Survey. The results of this and future studies will be used as the Decadal Survey deliberates on NASA’s planetary science priorities from 2022-2032. The study identifies the scientific questions an ice giant mission should address, and discusses various instruments, spacecraft, flight-paths and technologies that could be used.


Image above: Left: Arriving at Uranus in 1986, Voyager 2 observed a bluish orb with subtle features. A haze layer hid most of the planet's cloud features from view. Right: This image of Neptune was produced from Voyager 2 and shows the Great Dark Spot and its companion bright smudge. Image Credits: Left: NASA/JPL-Caltech - Right: NASA.

"This study argues the importance of exploring at least one of these planets and its entire environment, which includes surprisingly dynamic icy moons, rings, and bizarre magnetic fields," said Mark Hofstadter of NASA's Jet Propulsion Laboratory in Pasadena, California, one of the two co-chairs of the science team that produced the report. The European Space Agency (ESA) also participated in the study.

To date, Uranus and Neptune have been visited briefly by one spacecraft, Voyager 2.  Voyager rapidly flew by Uranus in 1986 and Neptune in 1989, as part of its grand tour of discovery that previously took it by Jupiter and Saturn.

Said co-chair Amy Simon of NASA's Goddard Space Flight Center in Greenbelt, Maryland, "We do not know how these planets formed and why they and their moons look the way they do. There are fundamental clues as to how our solar system formed and evolved that can only be found by a detailed study of one, or preferably both, of these planets." 

A variety of potential mission concepts are discussed in the study, including orbiters, flybys, and probes that would dive into Uranus’ atmosphere to study its composition. A narrow-angle camera would send data back to Earth about the ice giants and their moons. Uranus has 27 known moons, while Neptune has 14.

Collectively, Uranus and Neptune are referred to as ice giant planets. In spite of that name, relatively little solid ice is thought to be in them today, but it is believed there is a massive liquid ocean beneath their clouds, which accounts for about two-thirds of their total mass. This makes them fundamentally different from the gas giant planets, Jupiter and Saturn (which are approximately 85 percent gas by mass), and terrestrial planets like Earth or Mars, which are basically 100 percent rock. It’s not clear how or where ice giant planets form, why their magnetic fields are strangely oriented, and what drives geologic activity on some of their moons. These mysteries make them scientifically important, and this importance is enhanced by the discovery that many planets around other stars appear to be similar to our own ice giants.


Image above: Illustration of compositional differences among the giant planets and their relative sizes. Earth is shown for comparison. Jupiter and Saturn are primarily made of hydrogen and helium, the terrestrial planets are almost pure rock, while Uranus and Neptune are thought to be largely supercritical liquid water. Image Credits: JPL/Caltech, based on material from the Lunar and Planetary Institute.

It is now up to the next decadal survey to recommend science priorities for NASA for the next decade. NASA will then determine if and when to fly a mission that is responsive to those priorities.

The full study (529 pages), as well as a short summary are available at:

http://www.lpi.usra.edu/icegiants/mission_study

Related link:

Voyager: https://www.nasa.gov/mission_pages/voyager/index.html

Images (mentioned), Text, Credits: NASA/Tricia Talbert.

Greetings, Orbiter.ch

lundi 19 juin 2017

Station Kicks off Week with Solar Array Study and Biological Research










ISS - Expedition 52 Mission patch.

June 19, 2017

Flying over the Earth. Animation Credit: NASA

Robotics controllers completed the unloading and set up of the third and final external experiment delivered last week aboard the SpaceX Dragon resupply ship. Inside the International Space Station, the Expedition 52 crew studied a variety of life science including plant growth, bone loss and cardiac biology.

Over the weekend, engineers on the ground remotely operated the Canadarm2 to extract the Roll Out Solar Array from Dragon.  The experiment, also known as ROSA, will remain attached to the Canadarm2 over seven days to test the effectiveness of the advanced, flexible solar array that rolls out like a tape measure.


Image above: The Roll Out Solar Array, also known as ROSA, was deployed June 18 from the tip of the Canadarm2. Image Credit: NASA.

Flight Engineer Jack Fischer and Peggy Whitson set up the Seedling Growth-3 botany study today that is researching how plant cells respond to lighting conditions in microgravity. Fischer also installed samples in a NanoRacks facility for an educational research project that is studying the effects of radiation damage on synthetic DNA.

Whitson measured bone loss in mice for the Rodent Research-5 study. Results may improve the health of astronauts living in space and humans on Earth with bone diseases. Whitson later moved onto the Cardiac Stem Cells experiment that seeks to understand the accelerated aging process that takes place in space.

Related links:

Roll Out Solar Array: https://www.nasa.gov/mission_pages/station/research/experiments/2139.html

Seedling Growth-3: https://www.nasa.gov/mission_pages/station/research/experiments/1189.html

Rodent Research-5: https://www.nasa.gov/mission_pages/station/research/experiments/2283.html

Cardiac Stem Cells: https://www.nasa.gov/mission_pages/station/research/experiments/2436.html

Expedition 52: https://blogs.nasa.gov/spacestation/category/expedition-52/

Space Station Research and Technology: https://www.nasa.gov/mission_pages/station/research/index.html

International Space Station (ISS): https://www.nasa.gov/mission_pages/station/main/index.html

Image (mentioned), Animation (mentioned), Text, Credits: NASA/Mark Garcia.

Best regards, Orbiter.ch