lundi 6 octobre 2014

NASA Study Finds Earth’s Ocean Abyss Has Not Warmed











NASA - GRACE Mission patch.

October 6, 2014

The cold waters of Earth’s deep ocean have not warmed measurably since 2005, according to a new NASA study, leaving unsolved the mystery of why global warming appears to have slowed in recent years.

Scientists at NASA's Jet Propulsion Laboratory (JPL) in Pasadena, California, analyzed satellite and direct ocean temperature data from 2005 to 2013 and found the ocean abyss below 1.24 miles (1,995 meters) has not warmed measurably. Study coauthor Josh Willis of JPL said these findings do not throw suspicion on climate change itself.

"The sea level is still rising," Willis noted. "We're just trying to understand the nitty-gritty details."


Image above: While the upper part of the world’s oceans continue to absorb heat from global warming, ocean depths have not warmed measurably in the last decade. This image shows heat radiating from the Pacific Ocean as imaged by the NASA’s Clouds and the Earth's Radiant Energy System instrument on the Terra satellite. (Blue regions indicate thick cloud cover.) Image Credit: NASA.

In the 21st century, greenhouse gases have continued to accumulate in the atmosphere, just as they did in the 20th century, but global average surface air temperatures have stopped rising in tandem with the gases. The temperature of the top half of the world's oceans -- above the 1.24-mile mark -- is still climbing, but not fast enough to account for the stalled air temperatures.

Many processes on land, air and sea have been invoked to explain what is happening to the "missing" heat. One of the most prominent ideas is that the bottom half of the ocean is taking up the slack, but supporting evidence is slim. This latest study is the first to test the idea using satellite observations, as well as direct temperature measurements of the upper ocean. Scientists have been taking the temperature of the top half of the ocean directly since 2005, using a network of 3,000 floating temperature probes called the Argo array.

"The deep parts of the ocean are harder to measure," said JPL's William Llovel, lead author of the study published Sunday in the journal Nature Climate Change. "The combination of satellite and direct temperature data gives us a glimpse of how much sea level rise is due to deep warming. The answer is -- not much."


Image above: Deep sea creatures, like these anemones at a hydrothermal vent, are not yet feeling the heat from global climate change. Although the top half of the ocean continues to warm, the bottom half has not increased measurably in temperature in the last decade. Image Credit: NERC.

The study took advantage of the fact that water expands as it gets warmer. The sea level is rising because of this expansion and the water added by glacier and ice sheet melt.

To arrive at their conclusion, the JPL scientists did a straightforward subtraction calculation, using data for 2005-2013 from the Argo buoys, NASA's Jason-1 and Jason-2 satellites, and the agency’s Gravity Recovery and Climate Experiment (GRACE) satellites. From the total amount of sea level rise, they subtracted the amount of rise from the expansion in the upper ocean, and the amount of rise that came from added meltwater. The remainder represented the amount of sea level rise caused by warming in the deep ocean.

The remainder was essentially zero. Deep ocean warming contributed virtually nothing to sea level rise during this period.

Coauthor Felix Landerer of JPL noted that during the same period warming in the top half of the ocean continued unabated, an unequivocal sign that our planet is heating up. Some recent studies reporting deep-ocean warming were, in fact, referring to the warming in the upper half of the ocean but below the topmost layer, which ends about 0.4 mile (700 meters) down.

Landerer also is a coauthor of another paper in the same journal issue on 1970-2005 ocean warming in the Southern Hemisphere. Before Argo floats were deployed, temperature measurements in the Southern Ocean were spotty, at best. Using satellite measurements and climate simulations of sea level changes around the world, the new study found the global ocean absorbed far more heat in those 35 years than previously thought -- a whopping 24 to 58 percent more than early estimates.

Artist's view of GRACE satellites. Image Credit: NASA

Both papers result from the work of the newly formed NASA Sea Level Change Team, an interdisciplinary group tasked with using NASA satellite data to improve the accuracy and scale of current and future estimates of sea level change. The Southern Hemisphere paper was led by three scientists at Lawrence Livermore National Laboratory in Livermore, California.

NASA monitors Earth's vital signs from land, air and space with a fleet of satellites and ambitious airborne and ground-based observation campaigns. NASA develops new ways to observe and study Earth's interconnected natural systems with long-term data records and computer analysis tools to better see how our planet is changing. The agency shares this unique knowledge with the global community and works with institutions in the United States and around the world that contribute to understanding and protecting our home planet.

For more information about NASA's Earth science activities in 2014, visit: http://www.nasa.gov/earthrightnow

For more information on ocean surface topography from space, visit: http://sealevel.jpl.nasa.gov

More information on NASA’s GRACE satellites is available at: http://grace.jpl.nasa.gov

For more information on the Argo array, visit: http://www.argo.ucsd.edu/index.html

Images (mentioned), Text, Credits: NASA / Steve Cole / JPL / Alan Buis.

Cheers, Orbiter.ch

First Copernicus satellite now operational








Copernicus logo.

6 October 2014

With the commissioning of Sentinel-1A completed and the satellite’s transfer to the team in charge of its exploitation, its data are available as of today to all users: https://sentinel.esa.int/web/sentinel/home

This marks the beginning of the satellite’s operational life, delivering radar coverage for an array of applications in the areas of oceans, ice, changing land and emergency response.

Project Manager Ramón Torres, who led the development team, formally handed over the satellite to the Mission Manager, Pierre Potin.

Handing over Sentinel-1A

“The time has arrived for the satellite to exploit its extraordinary capabilities and start helping users,” said Ramón.

“A leap forward from ESA’s earlier Envisat, the unprecedented quality of Sentinel-1A will ensure that all users’ needs are fully met.

“Of course, saying farewell is always difficult, but I am confident that it is in capable and safe hands for the next stage of its journey.”

Launched on 3 April, Sentinel-1A completed commissioning on 23 September – an important process that ensures the satellite, instruments, data acquisition and data processing procedures are working well.

Not only did Sentinel-1A pass these tests and reach its target orbit on 7 August, eight anticollision manoeuvres to avoid space debris were performed during this phase.

The satellite will now begin delivering radar scans for an array of operational services and scientific research.

“My main objective is to ensure that Sentinel-1 fulfils the high expectations from the various operational services and scientific users,” notes Pierre.

“Looking at the satellite and ground segment performance – as demonstrated during the commissioning – as well as the preliminary results achieved so far, I’m confident that the mission will be a great success.”

The satellite will continue to be monitored, operated and controlled from ESA’s Space Operations Centre in Darmstadt, Germany.

Sentinel-1

The Sentinels are a new fleet of ESA satellite poised to deliver the wealth of data and imagery that are central to Europe’s Copernicus programme.

By offering a set of key information services for a broad range of applications, this global monitoring programme is a step change in the way we manage our environment, understand and tackle the effects of climate change, and safeguard everyday lives.

Sentinel-1 – a two-satellite constellation – is the first in the series and carries an advanced radar to provide an all-weather, day-and-night supply of imagery of Earth’s surface.

Even during commissioning, Sentinel-1A demonstrated its potential in the various applications domains.

Just days after launch, its results were included in maps of the floods that hit Namibia, as well as those in the Balkans the following month. This information was then used by authorities involved in flood response.

Radar images were also used to map the rupture caused by the 24 August earthquake that shook northern California – the biggest the area has seen in 25 years.

Napa Valley quake

The towing of the Costa Concordia cruise ship off the west coast of Italy was captured by the radar, demonstrating Sentinel-1’s ability to survey the marine environment.

This and many other services will now start benefiting from Sentinel-1A’s operational status. These include services related to monitoring Arctic sea-ice extent, routine sea-ice mapping, surveillance of the marine environment, monitoring land-surface for motion risks, mapping for forest, water and soil management and mapping to support humanitarian aid and crisis situations.

The mission’s contributions will further improve once the satellite’s identical twin, Sentinel-1B, is launched in 2016.

Related links:

European Commission Copernicus site: http://www.copernicus.eu/

Interview with Ramón Torres: http://www.esa.int/Our_Activities/Observing_the_Earth/Copernicus/Sentinel-1/Ramon_Torres_Project_Manager

Interview with Pierre Potin: http://www.esa.int/Our_Activities/Observing_the_Earth/Copernicus/Sentinel-1/Pierre_Potin_Mission_Manager

Sentinel-1: http://www.esa.int/Our_Activities/Observing_the_Earth/Copernicus/Sentinel-1

Data access & technical information: https://sentinel.esa.int/web/sentinel/home

Images, Text, Credits: ESA/Copernicus data (2014)/PPO.labs/Norut/COMET-SEOM Insarap study.

Greetings, Orbiter.ch

vendredi 3 octobre 2014

Station Crew Wraps Up Week of Spacewalk Preps With Research












ISS - Expedition 41 Mission patch.

October 3, 2014

The six-person Expedition 41 crew of the International Space Station conducted a range of scientific experiments Friday to benefit life here on Earth, closing out a busy workweek primarily focused on gearing up for a series of spacewalks.

Flight Engineer Alexander Gerst of the European Space Agency worked with an experiment that’s looking for a way to repurpose a diabetes treatment drug into a cancer fighter. The Drug Metabolism experiment studies yeast cells to understand how drugs act on tumors to see if metaformin, a drug commonly used to treat type 2 diabetes, can serve as an anti-cancer drug. The German astronaut retrieved samples from the Commercial Generic Bioprocessing Apparatus and injected the test drugs into them.


Image above: European Space Agency astronaut Alexander Gerst, Expedition 41 flight engineer, is pictured in the Quest airlock of the International Space Station. Image Credit: NASA.

Gerst also transferred a seedling culture dish into the Cell Biology Experiment Facility for incubation. The Plant Gravity Sensing experiment is examining the cellular and molecular mechanisms that enable plants to sense gravity. The researchers behind this study hypothesize that the gravity sensitivity of plants here on Earth can be modified to make crops more resistant to the destructive forces of nature, thus maintaining yields even in areas struck by flooding or high winds.

Meanwhile in the Japanese Kibo laboratory, Flight Engineer Barry Wilmore of NASA performed some maintenance on the Aquatic Habitat currently housing a school of fish popularly known as zebra danios for the Zebrafish Muscle study. The goal of this experiment is to determine whether zebrafish muscles weaken in microgravity similarly to human muscles and, if so, isolate the cause. Results from the Zebrafish Muscle investigation may help identify molecular changes involved in the deterioration of muscles exposed to microgravity, which could provide benefits to patients confined to bed and astronauts on long-duration space missions.

Flight Engineer Reid Wiseman checked in on several experiments taking place aboard the orbiting laboratory. The NASA astronaut first placed test canisters from the Biological Research in Canisters-19 (BRIC-19) experiment into the Minus Eighty-degree Laboratory Freezer for ISS, or MELFI. This experiment is taking a look at the development in microgravity of Arabidopsis thaliana seedlings, commonly referred to as Mouse-ear cress.

Wiseman then transferred test samples for the Micro-8 experiment, which is investigating the Candida albicans yeast in order to help scientists better understand and control the infectious nature of this opportunistic pathogen.

After a marathon week of preparations for a pair of upcoming U.S. spacewalks, the three astronauts also had some welcome off-duty time Friday.

Station robotic arm

Image above: ESA astronaut Alexander Gerst took this image of the International Space Station’s robotic arm and the Dragon commercial supply spacecraft during his six-month Blue Dot mission. Image Credits: ESA/NASA.

During the first Expedition 41 spacewalk slated to begin around 8:10 a.m. Tuesday, Wiseman and Gerst will exit out the Quest airlock for a six-and-a-half hour excursion to transfer a degraded pump module to its long-term home on the External Stowage Platform-2. The two spacewalkers also will install the Mobile Transporter Relay Assembly that provides backup power options to the Mobile Transporter railcar system, which moves the Mobile Servicing System’s Canadarm2 and Special Purpose Dexterous Manipulator to worksites along the station’s truss.

Alexander testing spacesuit

Image above: ESA astronaut Alexander Gerst testing his spacesuit on the International Space Station in preparation for 7 October 2014 when he will venture into open space with NASA astronaut Reid Wiseman on a seven-hour spacewalk. Image Credits: ESA/NASA.

Wilmore, who will be inside the cupola to provide robotic support for the first spacewalk, will join Wiseman on Oct. 15 for another excursion outside the station. Wiseman and Wilmore will venture out to the station’s starboard truss to replace a voltage regulator, known as a sequential shunt unit, which failed back in May.

On the Russian side of the complex, Commander Max Suraev performed routine maintenance on the life-support system in the Zvezda service module. He later stowed trash and unneeded items in the ISS Progress 56 cargo craft, which is set to undock from the Pirs docking compartment on Oct. 27 to make way for the next Russian space freighter – ISS Progress 57 – launching on Oct. 29.

Flight Engineer Alexander Samokutyaev, who joined Suraev to replace a Payload Interface Monitoring Unit, also conducted a session with the Cardiovector health experiment, which takes a look at the adaptation of the heart to long-duration spaceflight.

Flight Engineer Elena Serova meanwhile manually mixed test samples within the bioreactor of the Kaskad cell cultivation experiment. Later she photographed and deployed new samples for the Calcium experiment, which examines the causes of the loss of bone density that occurs in a weightless environment. For this study, Russian researchers are looking at the solubility of calcium phosphates and bone samples in water in space.

Over the weekend, the station’s astronauts and cosmonauts will take care of weekly housekeeping chores as they wipe down surfaces and vacuum dust. They also will continue their daily 2.5-hour workouts to stay fit and to prevent the loss of muscle mass and bone density that occurs in microgravity.

The station's crew conducted scientific experiments Friday, closing out a busy week focused on gearing up for a series of spacewalks.

Related links:

Drug Metabolism experiment: http://www.nasa.gov/mission_pages/station/research/experiments/1072.html

Plant Gravity Sensing experiment: http://www.nasa.gov/mission_pages/station/research/experiments/1011.html

Zebrafish Muscle investigation: http://www.nasa.gov/mission_pages/station/research/experiments/65.html

Biological Research in Canisters-19 (BRIC-19) experiment: http://www.nasa.gov/mission_pages/station/research/experiments/1082.html

Micro-8 experiment: http://www.nasa.gov/mission_pages/station/research/news/micro_8/

For more information about the International Space Station (ISS), visit: http://www.nasa.gov/mission_pages/station/main/index.html

Images (mentioned), Text, Credits: NASA / ESA.

Cheers, Orbiter.ch

Rosetta Comet Fires Its Jets












ESA - Rosetta Mission patch.

3 October 2014

Rosetta Comet Fires Its Jets

The four images that make up this montage of comet 67P/Churyumov–Gerasimenko were taken on Sept. 26, 2014 by the European Space Agency’s Rosetta spacecraft. At the time, Rosetta was about 16 miles (26 kilometers), from the center of the comet.

In the montage, a region of jet activity can be seen at the neck of the comet. These jets, originating from several discrete locations, are a product of ices sublimating and gases escaping from inside the nucleus. 

The overlapping and slightly dissimilar angles of the four images that compose the montage are a result of the combined effect of the comet rotating between the first and last images taken in the sequence (about 10 degrees over 20 minutes), and the spacecraft movement during that same time.

Launched in March 2004, Rosetta was reactivated in January 2014 after a record 957 days in hibernation. Composed of an orbiter and lander, Rosetta's objectives since arriving at comet 67P/Churyumov-Gerasimenko earlier this month are to study the celestial object up close in unprecedented detail, prepare for landing a probe on the comet's nucleus in November, and after the landing track the comet's changes through 2015, as it sweeps past the sun.


Image above: Rosetta orbiting comet 67P/Churyumov-Gerasimenko. Photo-montage by Orbiter.ch Aerospace, the distance and sizes between the comet and the probe are not realistic. Image credits: Orbiter.ch Aerospace/ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA.

Comets are time capsules containing primitive material left over from the epoch when the sun and its planets formed. Rosetta's lander will obtain the first images taken from a comet's surface and will provide comprehensive analysis of the comet's possible primordial composition by drilling into the surface. Rosetta also will be the first spacecraft to witness at close proximity how a comet changes as it is subjected to the increasing intensity of the sun's radiation. Observations will help scientists learn more about the origin and evolution of our solar system and the role comets may have played in seeding Earth with water, and perhaps even life.

Rosetta is an ESA mission with contributions from its member states and NASA. Rosetta's Philae lander is provided by a consortium led by the German Aerospace Center, Cologne; Max Planck Institute for Solar System Research, Gottingen; National Center of Space Studies of France (CNES), Paris; and the Italian Space Agency, Rome. NASA's Jet Propulsion Laboratory in Pasadena, California, a division of the California Institute of Technology, manages the U.S. participation in the Rosetta mission for NASA's Science Mission Directorate in Washington.

For more information on the U.S. instruments aboard Rosetta, visit: http://rosetta.jpl.nasa.gov

More information about Rosetta is available at: http://www.esa.int/rosetta

Image Credit: ESA / Rosetta / NAVCAM.

Greetings, Orbiter.ch

NASA Releases Images of a Mid-level Solar Flare












NASA - Solar Dynamics Observatory (SDO) patch.

October 3, 2014

Twisting Solar Eruption and Flare

Video above: A solar flare erupted on the right side of the sun on Oct. 2, 2014, while a cloud of solar material just below was flung out into space. Video Credit: NASA/SDO/ Wiessinger.

The sun emitted a mid-level solar flare, peaking at 3:01 p.m. EDT on Oct. 2, 2014.  NASA's Solar Dynamics Observatory, which watches the sun 24-hours a day, captured images of the flare. Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however -- when intense enough -- they can disturb the atmosphere in the layer where GPS and communications signals travel.


Image above: NASA's Solar Dynamics Observatory captured this image of a solar flare on Oct. 2, 2014. The solar flare is the bright flash of light on the right limb of the sun. A burst of solar material erupting out into space can be seen just below it. Image Credit: NASA/SDO.

To see how this event may affect Earth, please visit NOAA's Space Weather Prediction Center at http://spaceweather.gov, the U.S. government's official source for space weather forecasts, alerts, watches and warnings.

This flare is classified as an M7.3 flare. M-class flares are one-tenth as powerful as the most powerful flares, which are designated X-class flares.

Updates will be provided as needed.

What is a solar flare?
For answers to this and other space weather questions, please visit the Spaceweather Frequently Asked Questions page: http://www.nasa.gov/mission_pages/sunearth/spaceweather/index.html

Related Link:

View Past Solar Activity: http://www.nasa.gov/mission_pages/sunearth/multimedia/Solar-Events.html

NASA's SDO Watches Giant Filament on the Sun

A snaking, extended filament of solar material currently lies on the front of the sun-- some 1 million miles across from end to end. Filaments are clouds of solar material suspended above the sun by powerful magnetic forces. Though notoriously unstable, filaments can last for days or even weeks.


Images above: A dark snaking line in the upper right of these images on Sept. 30, 2014, show a filament of solar material hovering above the sun's surface. NASA's SDO captured the images in extreme UV light – different colors represent different wavelengths of light and different temperatures of solar material. Image Credit: NASA/SDO.

NASA's Solar Dynamics Observatory, or SDO, which watches the sun 24 hours a day, has observed this gigantic filament for several days as it rotated around with the sun. If straightened out, the filament would reach almost across the whole sun, about 1 million miles or 100 times the size of Earth.

SDO captured images of the filament in numerous wavelengths, each of which helps highlight material of different temperatures on the sun. By looking at any solar feature in different wavelengths and temperatures, scientists can learn more about what causes such structures, as well as what catalyzes their occasional giant eruptions out into space.

Look at the images to see how the filament appears in different wavelengths. The brownish combination image was produced by blending two wavelengths of extreme UV light with a wavelength of 193 and 335 Angstroms. The red image shows the 304 Angstrom wavelength of extreme UV light.

For more information about Solar Dynamics Observatory (SDO), visit: http://www.nasa.gov/mission_pages/sdo/main/index.html

Images (mentioned), Video (mentioned), Text, Credits: NASA's Goddard Space Flight Center/Karen C. Fox/Steele Hill.

Best regards, Orbiter.ch

CryoSat unveils secrets of the deep







ESA - Cryosat 2 Mission patch.

3 October 2014

ESA’s ice mission has been used to create a new gravity map, exposing thousands of previously unchartered ‘seamounts’, ridges and deep ocean structures. This vivid new picture of the least-explored part of the ocean offers fresh clues about how continents form and breakup.

Carrying a radar altimeter, CryoSat’s main role is to provide detailed measurements of the height of the world’s ice. This allows us to see how the thickness of the ice changes, seasonally and in response to climate change.

Gravity reveals seafloor

However, CryoSat works continuously, whether there is ice below or not. This means that the satellite can also measure the height of the surface of the sea. These measurements can be used to create global marine gravity models and, from them, maps of the seafloor.

Although invisible to the eye, the sea surface has ridges and valleys that echo the topography of the ocean floor, but on a greatly reduced scale.

The effect of the slight increase in gravity caused by the mass of rock in an undersea mountain is to attract a mound of water several metres high over the seamount. Deep ocean trenches have the reverse effect.

CryoSat

These features can only be detected by using radar altimetry from space.

Scientists from Scripps Institute of Oceanography at University California San Diego in the US and colleagues tapped into two new streams of satellite data to create a new gravity map mirroring features of the ocean floor – twice as accurate as the previous version produced nearly 20 years ago.

They used measurements that CryoSat has captured over the oceans during the last four years as well as measurements from the French–US Jason-1 satellite, which was retasked to map the gravity field during the last year of its 12-year mission.

Combined with existing data, the new map, described in the journal Science, reveals details of thousands of undersea mountains rising a kilometre or more from the bottom of the ocean.

The new map offers geophysics new tools to investigate little-studied remote ocean basins and processes such as seafloor spreading.

Atlantic bed imprinted in gravity

“The kinds of things you can see very clearly now are abyssal hills, which are the most common land form on the planet,” said David Sandwell, lead scientist of the paper and a geophysics professor at Scripps.

The authors of the study say the map provides a new window into the tectonics of the deep oceans.

Previously unseen features in the map include newly exposed continental connections across South America and Africa, and new evidence for seafloor spreading ridges at the Gulf of Mexico that were active 150 million years ago and are now buried by layers of sediment more than a kilometre thick.

One of the most important uses of this new marine gravity field will be to improve the estimates of seafloor depth in the 80% of the oceans that remains uncharted or is buried beneath thick sediment.

Indian Ocean bed imprinted in gravity

The new map will also provide the foundation for the upcoming new version of Google’s ocean maps to fill large voids between shipboard depth profiles.

ESA’s Richard Francis, co-author and project manager for the development of CryoSat, said, “Although CryoSat’s primary mission is in the cryosphere, we knew as soon as we selected its orbit that it would be invaluable for marine geodesy, and this work proves the point.”

Related links:

Science: New global marine gravity model from CryoSat-2 and Jason-1 reveals buried tectonic structure: http://www.sciencemag.org/content/346/6205/65

Scripps Institution of Oceanography: http://topex.ucsd.edu/index.html

Jason-1: http://science.nasa.gov/missions/jason-1/

Access CryoSat data: https://earth.esa.int/web/guest/missions/esa-operational-eo-missions/cryosat

Introducing CryoSat: http://www.esa.int/Our_Activities/Observing_the_Earth/CryoSat/Introducing_CryoSat

Images, Text, Credits: ESA/P. Carril/Scripps Institution of Oceanography.

Greetings, Orbiter.ch

jeudi 2 octobre 2014

Station Crew Conducts Biological Research, Assembles Hardware for Spacewalk












ISS - Expedition 41 Mission patch.

October 2, 2014

The six-person Expedition 41 crew of the International Space Station focused their attention Thursday on biological research and preparations for the first of three spacewalks planned for October, while the ground team worked to bring a newly installed weather monitoring instrument up to speed.

Late Wednesday, the International Space Station-Rapid Scatterometer, or ISS-RapidScat installed on the exterior of the Columbus module was activated by payload controllers at the Marshall Space Flight Center. The radar antenna of the device, which is designed to monitor ocean winds from the station’s vantage point, began spinning as planned, but the payload controllers decided to place the system in safe mode when they noted higher than expected temperatures in the instrument’s electronics. The antenna continues to spin normally while the ground team analyzes the data and learns how to manage the temperature.


Animation above: A video camera on the International Space Station captured this view of the the ISS-Rapid Scatterometer, or RapidScat, on Wednesday. Animation Credit: NASA.

ISS-RapidScat was among the nearly two-and-a-half tons of cargo delivered to the station by the SpaceX Dragon resupply craft Sept. 23. Robotics officers at Houston’s Mission Control Center remotely commanded the Canadarm2 robotic arm to remove ISS-RapidScat from Dragon’s trunk and attach it to its adapter on the station’s Columbus laboratory on Tuesday.

Meanwhile, Flight Engineers Reid Wiseman and Alexander Gerst spent much of Thursday assembling hardware and reviewing procedures for a spacewalk scheduled to begin on Tuesday around 8:10 a.m. EDT. During the six-and-a-half-hour excursion, Wiseman and Gerst will transfer a degraded pump module from its temporary stowage location to its long-term home on the External Stowage Platform-2. The two spacewalkers also will install the Mobile Transporter Relay Assembly (MTRA) that provides backup power options to the Mobile Transporter railcar system, which moves the Mobile Servicing System’s Canadarm2 and Special Purpose Dexterous Manipulator to worksites along the station’s truss.


Image above: Inside the International Space Station's Quest airlock, Flight Engineer Reid Wiseman works on the spacesuit that Flight Engineer Alexander Gerst will wear during Tuesday's spacewalk. Image Credit: NASA TV.

Flight Engineer Barry Wilmore, who will be at the controls of Canadarm2 inside the station cupola to provide support for Tuesday’s spacewalk, joined his astronaut crewmates for a review of the robotic operations.

Wilmore will be joining Wiseman on the second Expedition 41 spacewalk set for Oct. 15, to replace a voltage regulator that failed back in May. And on Oct. 22, Commander Max Suraev and Flight Engineer Alexander Samokutyaev will conduct the first Russian spacewalk of Expedition 41.

Wilmore performed some maintenance on the Aquatic Habitat currently housing a school of fish popularly known as zebra danios for the Zebrafish Muscle study. The goal of this experiment is to determine whether zebrafish muscles weaken in microgravity similarly to human muscles and, if so, isolate the cause. Results from the Zebrafish Muscle investigation may help identify molecular changes involved in the deterioration of muscles exposed to microgravity and could provide benefits to patients on extended bed rest and astronauts on long-duration missions in space.


Image above: One of the Expedition 41 crew members aboard the International Space Station, flying at an altitude of 222 nautical miles above a point in the Atlantic Ocean several hundred miles off the coast of Africa near the Tropic of Cancer, photographed this eye-catching panorama of the night sky on Sept. 27. Image Credit: NASA.

Gerst participated in a periodic fitness evaluation as he worked out on the station’s exercise bike – the Cycle Ergometer with Vibration Isolation and Stabilization. Wilmore assisted his German crewmate by initiating blood pressure and electrocardiogram measurements to help the flight surgeons benchmark the crew’s cardiovascular and musculoskeletal health.

Gerst also donned monitors to track his body’s core temperature over a 36-hour period for the Circadian Rhythms study. Because the station orbits the Earth every 92 minutes and experiences 16 sunrises and sunsets every day, the astronauts do not have the same day/night cues that people have on Earth. Results from this investigation will provide insights into the adaptations of the human autonomic nervous system in space and will help optimize crew schedules and workplace illumination.

Wiseman activated a botanical study known as Biological Research in Canisters-19, or BRIC-19. This experiment is taking a look at the development in microgravity of Arabidopsis thaliana seedlings, commonly referred to as Mouse-ear cress. The seedlings will be preserved and returned to Earth for genetic analysis and comparison with a control set of seedlings germinated in normal gravity.

On the Russian side of the complex, Flight Engineer Elena Serova participated in the Cardiovector experiment, which takes a look at the adaptation of the heart to long-duration spaceflight. Samokutyaev meanwhile performed the Virtual study, a Russian investigation into the human body’s sensory adaptations to weightlessness.

Commander Suraev spent part of his day transferring water from the Progress 56 cargo ship attached to the Pirs docking compartment. Progress 56, which is set to depart in late October, delivered nearly three tons of supplies when it docked to the station on July 23.

Related links:

International Space Station-Rapid Scatterometer, or ISS-RapidScat: http://www.jpl.nasa.gov/missions/iss-rapidscat/

Zebrafish Muscle study: http://www.nasa.gov/mission_pages/station/research/experiments/65.html

Circadian Rhythms study: http://www.nasa.gov/mission_pages/station/research/experiments/892.html

Biological Research in Canisters-19, or BRIC-19: http://www.nasa.gov/mission_pages/station/research/experiments/1082.html

For more information about the International Space Station (ISS), visit: http://www.nasa.gov/mission_pages/station/main/index.html

Images (mentioned), Animation (mentioned), Text, Credits: NASA.

Greetings, Orbiter.ch