mercredi 2 novembre 2016

Pillars of Destruction












ESO - European Southern Observatory logo.


2 November 2016

Colourful Carina Nebula blasted by brilliant nearby stars

Region R44 in the Carina Nebula

Spectacular new observations of vast pillar-like structures within the Carina Nebula have been made using the MUSE instrument on ESO’s Very Large Telescope. The different pillars analysed by an international team seem to be pillars of destruction — in contrast to the name of the iconic Pillars of Creation in the Eagle Nebula, which are of similar nature.

Pillars of destruction

The spires and pillars in the new images of the Carina Nebula are vast clouds of dust and gas within a hub of star formation about 7500 light-years away. The pillars in the nebula were observed by a team led by Anna McLeod, a PhD student at ESO, using the MUSE instrument on ESO’s Very Large Telescope.

Region R18 in the Carina Nebula

The great power of MUSE is that it creates thousands of images of the nebula at the same time, each at a different wavelength of light. This allows astronomers to map out the chemical and physical properties of the material at different points in the nebula.

Region R37 in the Carina Nebula

Images of similar structures, the famous Pillars of Creation [1] in the Eagle Nebula and formations in NGC 3603, were combined with the ones displayed here. In total ten pillars have been observed, and in so doing a clear link was observed between the radiation emitted by nearby massive stars and the features of the pillars themselves.

Region R45 in the Carina Nebula

In an ironic twist, one of the first consequences of the formation of a massive star is that it starts to destroy the cloud from which it was born. The idea that massive stars will have a considerable effect on their surroundings is not new: such stars are known to blast out vast quantities of powerful, ionising radiation — emission with enough energy to strip atoms of their orbiting electrons. However, it is very difficult to obtain observational evidence of the interplay between such stars and their surroundings.

Star cluster Trumpler 14

The team analysed the effect of this energetic radiation on the pillars: a process known as photoevaporation, when gas is ionised and then disperses away. By observing the results of photoevaporation — which included the loss of mass from the pillars — they were able to deduce the culprits. There was a clear correlation between the amount of ionising radiation being emitted by nearby stars, and the dissipation of the pillars.

Bok Globule in the Carina Nebula

This might seem like a cosmic calamity, with massive stars turning on their own creators. However the complexities of the feedback mechanisms between the stars and the pillars are poorly understood. These pillars might look dense, but the clouds of dust and gas which make up nebulae are actually very diffuse. It is possible that the radiation and stellar winds from massive stars actually help create denser spots within the pillars, which can then form stars.

Mystic Mountain

These breathtaking celestial structures have more to tell us, and MUSE is an ideal instrument to probe them with.

3D Animation of the Carina Nebula

Zooming in on the Carina Nebula

Notes:

[1] The Pillars of Creation are an iconic image, taken with the NASA/ESA Hubble Space Telescope, making them the most famous of these structures. Also known as elephant trunks, they can be several light-years in length.

More information:

This research was presented in a paper entitled “Connecting the dots: a correlation between ionising radiation and cloud mass-loss rate traced by optical integral field spectroscopy“, by A. F. McLeod et al., published in the Monthly Notices of the Royal Astronomical Society.

The team is composed of A. F. McLeod (ESO, Garching, Germany), M. Gritschneder (Universitäts-Sternwarte, Ludwig-Maximilians-Universität, Munich, Germany), J. E. Dale (Universitäts-Sternwarte, Ludwig-Maximilians-Universität, Munich, Germany), A. Ginsburg (ESO, Garching, Germany), P. D.Klaassen (UK Astronomy Technology Centre, Royal Observatory Edinburgh, UK), J. C. Mottram (Max Planck Institute for Astronomy, Heidelberg, Germany), T. Preibisch (Universitäts-Sternwarte, Ludwig-Maximilians-Universität, Munich, Germany), S. Ramsay (ESO, Garching, Germany), M. Reiter (University of Michigan Department of Astronomy, Ann Arbor, Michigan, USA) and L. Testi (ESO, Garching, Germany).

ESO is the foremost intergovernmental astronomy organisation in Europe and the world’s most productive ground-based astronomical observatory by far. It is supported by 16 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Poland, Portugal, Spain, Sweden, Switzerland and the United Kingdom, along with the host state of Chile. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world’s most advanced visible-light astronomical observatory and two survey telescopes. VISTA works in the infrared and is the world’s largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is a major partner in ALMA, the largest astronomical project in existence. And on Cerro Armazones, close to Paranal, ESO is building the 39-metre European Extremely Large Telescope, the E-ELT, which will become “the world’s biggest eye on the sky”.

Links:

Research paper: http://www.eso.org/public/archives/releases/sciencepapers/eso1639/eso1639a.pdf

Photos of the VLT: http://www.eso.org/public/images/archive/category/paranal/

ESO’s Very Large Telescope (VLT): http://eso.org/vlt

MUSE instrument: https://www.eso.org/public/teles-instr/vlt/vlt-instr/muse/?lang

NASA/ESA Hubble Space Telescope: http://spacetelescope.org/

Images, Text, Credits: ESO/A. McLeod/Videos: ESO/M. Kornmesser/Nick Risinger (skysurvey.org)/Digitized Sky Survey 2 . Music: John Dyson (from the album Moonwind). Acknowledgement: VPHAS+ Consortium/Cambridge Astronomical Survey Unit.

Best regards, Orbiter.ch

Launch success of the satellite "Himawari-9"








JAXA - Japan Aerospace Exploration Agency logo.

November 2, 2016


Image above: Launch success of the H-IIA Launch Vehicle No. 31 (H-IIA F31) with the geostationary meteorological satellite "Himawari-9" on board.

Mitsubishi Heavy Industries, Ltd. and the Japan Aerospace Exploration Agency (JAXA) successfully launched the H-IIA Launch Vehicle No. 31 (H-IIA F31) with the geostationary meteorological satellite "Himawari-9" on board at 3:20 p.m. on November 2, 2016 (JST) from the Tanegashima Space Center.

The live broadcast of the Himawari-9/H-IIA F31 launch

The launch vehicle flew as planned, and at approximately 27 minutes and 51 seconds after liftoff, the separation of Himawari-9 was confirmed.

Geostationary meteorological satellite "Himawari-9"

At the time of the launch, the weather was fine, a wind speed was 6.1 meters/second from the north-east and the temperature was 21.3 degrees Celsius.

About Geostationary Meteorological Satellite "Himawari" (GMS):

The Japanese Geostationary Meteorological Satellite (GMS) series, also known as its nickname, "Himawari" (meaning a "sunflower"), is on the geostationary orbit at 140 degrees of east longitude to carry out weather observation from space being part of the World Weather Watch (WWW) project of the World Meteorological Organization. The images of the earth and clouds sent from this satellite series have been used in many areas such as weather forecasts in TV or newspaper; therefore, it is strongly connected to our daily life.

After the "Himawari-6", the GMS series was replaced by a Multifunctional Transport Satellite series to broaden its scope of operation. It is operated by the Japan Meteorological Agency for climatic observation.

H-IIA Launch Vehicle No. 31 Flight Sequence (Quick Estimation) PDF: http://global.jaxa.jp/press/2016/11/files/20161102_h2af31.pdf

Reference:

Geostationary Meteorological Satellite "Himawari" (GMS): http://global.jaxa.jp/projects/sat/gms/index.html

MHI Launch Services: http://h2a.mhi.co.jp/en/index.html

H-IIA Launch Vehicle: http://global.jaxa.jp/projects/rockets/h2a/

Images, Video, Text, Credits: Japan Aerospace Exploration Agency (JAXA)/National Research and Development Agency/Mitsubishi Heavy Industries, Ltd.

Greetings, Orbiter.ch

mardi 1 novembre 2016

New, Space-Based View of Human-Made Carbon Dioxide












NASA - OCO-2 Mission logo.

Nov. 1, 2016

Orbiting Carbon Observatory (OCO-2) satellite. Image Credit: NASA

Scientists have produced the first global maps of human emissions of carbon dioxide ever made solely from satellite observations of the greenhouse gas. The maps, based on data from NASA's Orbiting Carbon Observatory-2 (OCO-2) satellite and generated with a new data-processing technique, agree well with inventories of known carbon dioxide emissions.

No satellite before OCO-2 was capable of measuring carbon dioxide in fine enough detail to allow researchers to create maps of human emissions from the satellite data alone. Instead, earlier maps also incorporated estimates from economic data and modeling results.

The team of scientists from the Finnish Meteorological Institute, Helsinki, produced three main maps from OCO-2 data, each centered on one of Earth's highest-emitting regions: the eastern United States, central Europe and East Asia. The maps show widespread carbon dioxide across major urban areas and smaller pockets of high emissions.


Image above: Human carbon dioxide emissions from fossil fuel burning and other sources have been mapped from OCO-2's global dataset. Image Credits: World Bank/Kim Eun Yeul.

"OCO-2 can even detect smaller, isolated emitting areas like individual cities," said research scientist Janne Hakkarainen, who led the study. "It's a very powerful tool that gives new insight."

The results appear in a paper titled published Nov. 1 in the journal Geophysical Research Letters.

Human emissions of carbon dioxide have grown at a significant rate since the Industrial Revolution, and the greenhouse gas lingers in the atmosphere for a century or more. This means that recent human output is only a tiny part of the total carbon dioxide that OCO-2 records as it looks down toward Earth's surface. "Currently, the background level of carbon dioxide in the atmosphere is about 400 parts per million, and human emissions within the past year may add only something like three parts per million to that total," said Hakkarainen. The data-processing challenge, he noted, was to isolate the signature of the recent emissions from the total amount.

The team's new data-processing technique accounts for seasonal changes in carbon dioxide, the result of plant growth and dormancy, as well as the background carbon dioxide level. To be sure their method was correct, they compared the results with measurements of nitrogen dioxide -- another gas emitted from fossil fuel combustion -- from the Ozone Monitoring Instrument, a Dutch-Finnish instrument on NASA's Aura satellite. OMI and OCO-2 are both in the A-Train satellite constellation, so the two measurements cover the same area of Earth and are separated in time by only 15 minutes.

The two measurements correlated well, giving the researchers confidence that their new technique produced reliable results.


Image above: Human carbon dioxide emissions over Europe, the Middle East and northern Africa. Values range from 3 parts per million CO2 below background levels (navy blue) to 3 parts per million above (pale yellow). High emissions over Germany and Poland (top center) and Kuwait and Iraq (right) mostly come from fossil fuel burning, but over sub-Saharan Africa they mostly come from fires. Image Credit: FMI.

Coauthor Johanna Tamminen, head of the atmospheric remote sensing group at the Finnish Meteorological Institute, noted that with its comparison of OCO-2 and OMI data, "The research demonstrates the possibility of analyzing joint satellite observations of carbon dioxide and other gases related to combustion processes to draw out information about the emissions sources."

OCO-2 Deputy Project Scientist Annmarie Eldering of NASA's Jet Propulsion Laboratory, Pasadena, California, said, "We are very pleased to see this research group make use of the OCO-2 data. Their analysis is a great demonstration of discovery with this new dataset." Eldering was not involved in the study.

NASA uses the vantage point of space to increase our understanding of our home planet, improve lives and safeguard our future. NASA develops new ways to observe and study Earth's interconnected natural systems with long-term data records. The agency freely shares this unique knowledge and works with institutions around the world to gain new insights into how our planet is changing.

For more information about OCO-2: https://oco2.jpl.nasa.gov/

Images (mentioned), Text, Credits: NASA Earth Science News Team, written by Carol Rasmussen/JPL/Alan Buis.

Greetings, Orbiter.ch

Gemini XII Crew Masters the Challenges of Spacewalks












NASA - Gemini XII Mission patch.

Nov. 1, 2016

In the 20 months following the first piloted Gemini mission, NASA astronauts demonstrated the ability to change orbits, perform rendezvous and docking, along with spending up to two weeks in space. Spacewalking, on the other hand, remained an enigma. With only one more Gemini flight on the schedule, solving the problems of working outside a spacecraft would be the primary goal for Gemini XII.

As was the case on the previous four missions, the Gemini XII flight plan called for rendezvous and docking with a target vehicle. But, according to Dr. George Mueller, NASA’s associate administrator for Manned Spaceflight, mastering what NASA called an extravehicular activity (EVA) or spacewalk would be crucial in proving the agency was ready to move ahead with Apollo and achieving the goal of landing a man on the moon before the end of the decade.


Image above: Gemini XII pilot Buzz Aldrin, left, and command pilot Jim Lovell stand in a Gemini mockup during training at NASA's Manned Spacecraft Center (now Johnson Space Center) in Houston. Image Credit: NASA.

“I feel that we must devote the last EVA period in the Gemini Program to a basic investigation of EVA fundamentals,” he said.

To take on the challenges of this crucial flight, NASA assigned a veteran of the longest spaceflight to date and the astronaut who helped “write the book” on orbital rendezvous.

The command pilot was Jim Lovell who served on the 14-day Gemini VII mission in December 1965. A Naval aviator, he went on to be a member of the Apollo 8 crew, the first mission to orbit astronauts around the moon in 1968. As commander of Apollo 13 in 1970, Lovell became the first person to travel in space four times.


Image above: On Oct. 29, 1966, Gemini XII astronaut Buzz Aldrin practices installing a telescoping handrail between a mockup of a Gemini spacecraft docked to an Agena. The spacewalk training took place in a large pool at Environmental Research Associates facility in Randallstown, Maryland near Baltimore. Additional hand holds and the underwater training were keys to adequately preparing for the challenges of spacewalks. Image Credit: NASA.

Flying with Lovell was U.S. Air Force pilot, Buzz Aldrin, the first astronaut to have earned a doctorate. In 1963, he was awarded a doctorate in astronautics from the Massachusetts Institute of Technology. His graduate thesis was "Line-of-sight guidance techniques for manned orbital rendezvous.” Aldrin went on to serve as lunar module pilot on Apollo 11 in 1969, during which he and Neil Armstrong become the first humans to walk on the moon.

To make lunar EVAs possible, spacewalking during Gemini flights was a crucial learning experience in Gemini. Ed White’s spacewalk on Gemini IV made it look easy. But the experiences of Gene Cernan, Mike Collins and Dick Gordon on three later missions demonstrated a new approach was needed for both training and performing spacewalks.

Through Gemini XI, EVA training focused on use of the KC-135 aircraft flying parabolas. During the dives, astronauts experienced up to 30 seconds of weightlessness. But this was followed by the aircraft climbing and the astronauts having a period of rest. Consequently, spacewalkers in training were not facing the types of continued strenuous work and fatigue experienced by Cernan, Collins and Gordon.


Image above: At Cape Kennedy (now Cape Canaveral) Air Force Station, the crew for Gemini XII arrive at Launch Complex 19. Command pilot Jim Lovell is followed by pilot Buzz Aldrin. The signs on their backs note that this mission is the final flight of the Gemini Program. Image Credit: NASA.

Dr. Robert Gilruth, director of the Manned Spacecraft Center (now Johnson Space Center) in Houston, ordered a new approach.

“I have given a great deal of thought recently to the subject of how best to simulate and train for extravehicular activities,” Gilruth said in memo to Deke Slayton, director of Flight Crew Operations. “Both zero ‘g’ trajectories in the KC-135 and underwater simulations should have a definite place in our training programs.”

The alternate approach uses a large pool of water for “neutral buoyancy.” In this method special weights are added to the astronaut’s spacesuit creating buoyancy to offset gravity so the astronaut neither rises nor sinks.

Aldrin spent several sessions of more than two hours each working with a Gemini mockup in the pool at the Environmental Research Associates facility near Baltimore, Maryland.


Image above: “We're taking pictures of the beautiful Agena here,” said command pilot Jim Lovell as Gemini XII closed to within 50 feet of its Agena target vehicle after liftoff on Nov. 11, 1966. Image Credit: NASA.

This approach became so successful, underwater training has become the primary spacewalk training method used by the United State, Russia and China. Today, NASA's Neutral Buoyancy Laboratory in Houston is large enough to include mockups of major sections of the International Space Station. As such, it is the largest indoor body of water in the world, with 6.2 million gallons of water.

With the additional training behind them, Lovell and Aldrin lifted off aboard their Gemini XII spacecraft atop a Titan II rocket on Nov. 11, 1966. They followed one hour, 39 minutes after their Agena was placed in orbit by an Atlas launch vehicle.

The first order of business was rendezvous with the Agena. Things were going well when Lovell confirmed they spotted their target 98 miles away. But minutes later there was trouble.

“We seem to have lost our radar lock-on at about 74 miles,” Aldrin said. “We don't seem to be able to get anything through the computer.”

Aldrin pulled out a sextant and his slide rule and put his MIT doctoral research to work. With the sextant, Aldrin measured the angle between the horizon and the Agena. Aldrin confirmed the information with his rendezvous chart, then calculated corrections with the spacecraft’s computer.


Image above: Gemini XII command pilot Jim Lovell maneuvers his spacecraft into position to dock with the Agena target vehicle. Image Credits: NASA/Buzz Aldrin.

“How are you doing up there?” asked fellow astronaut Pete Conrad during the third orbit. He was serving as capsule communicator, known as capcom, in Mission Control.

“We're taking pictures of the beautiful Agena here,” Lovell said as Gemini XII closed in on its target.

“We're giving you a GO for docking,” Conrad said.

“We are docked,” Lovell reported four minutes later as the combined spacecraft orbited south of Japan in range of the tracking ship Coastal Sentry Quebec.

During flight day two, Aldrin began practicing some of the new processes for spacewalks. This would be a two-hour, 18 minute EVA limited to standing in the hatch to familiarize himself with the environment, as well as conducting Earth and ultraviolet astronomical photography.

“The hatch is coming open,” he said. “Man, look at that.”


Image above: Buzz Aldrin installs a handrail between the Gemini and Agena spacecraft during his first stand-up spacewalk. This was something he had practiced in underwater training. Gemini XII is docked to the Agena in the background. Image Credit: NASA.

Aldrin expressed amazement seeing so much of Earth and the universe once outside the confines of the spacecraft.

One of his first jobs was to install a handrail between his hatch and the docking collar of the Agena. This would aid his movements during a full spacewalk the next day. As Aldrin took pictures of landmarks on Earth, he offered the usual photographer’s “suggestion.”

“Okay, tell everybody down there to smile,” he said to capcom Conrad.

Having set up a camera on the edge of his hatch, Aldrin pointed the camera in his direction.

“Now let me raise my visor and I'll smile,” he said taking what Aldrin now describes as “the first space selfie.”

With the space stand-up EVA completed, the next day came the crucial test of a new approach to spacewalking.

“I'm free now and the only thing that's holding me is the one hand on the handrail,” Aldrin said as he used the aid he installed the day before.


Image above: During his first stand-up spacewalk on Nov. 12, 1966, Buzz Aldrin photographed landmarks on Earth. While doing so, he set his camera on the edge of the hatch, pointing it in his direction. He then took what he now describes as “the first space selfie.” Image Credits: NASA/Buzz Aldrin.

In addition to revised preflight training techniques, more handrails and handholds were added along with a waist tether giving the spacewalker the ability to turn wrenches and retrieve experiment packages without undue effort.

Aldrin’s approach was to go about his work slowly and deliberately. He would work for a while then rest, even if a reminder was needed.

“Now do you know what you're going to do?” Lovell asked.

“Go ahead, clue me in,” Aldrin said.

“You'll get a rest for two minutes,” Lovell said.

Aldrin then attached a tether from the Agena for the gravity-gradient experiment. With the handholds, he did not experience the problems Gordon encountered on the previous flight.


Image above: During a spacewalk on Nov. 13, 1966, Gemini XII pilot Buzz Aldrin works at a box attached to Agena. He pulled electrical connectors apart and put them together again, then tried out a torque wrench designed for the Apollo Program. With all his work successfully completed and with no fatigue, Aldrin return to his Gemini seat after two hours, nine minutes outside, experiencing none of the problems that had plagued the previous three Gemini missions. Image Credits: NASA/Jim Lovell.

Next, Aldrin moved to the spacecraft’s aft adapter where he placed his feet in overshoe restraints and attached waist tethers. With these supports in place, he was able to fasten rings and hooks, connect and disconnect electrical and fluid connections, tighten bolts and cut cables.

“I've got the cutters,” Aldrin said. “They're cutting the strap seam quite nicely.”

Aldrin again went forward to a box attached to the Agena. Lovell photographed him as he pulled electrical connectors apart and put them together again, then tried out a torque wrench designed for the Apollo program.

With all his work successfully competed and with no fatigue, Aldrin returned to his Gemini seat after two hours, nine minutes outside.

The riddle of spacewalking was solved.

The next task for Gemini XII was to undock from the Agena and maneuver their craft to keep taut the tether attached by Aldrin during his spacewalk. By firing their thrusters to slowly rotate the combined spacecraft, they, like Gemini XI, were able to use centrifugal force to generate a small amount of gravity during the four hour, 20 minute exercise.

Aldrin’s third time outside Gemini XII and his second stand-up on the seat spacewalk, was on the fourth flight day. He took numerous ultraviolet photographs of stars and constellations during one hour, 11 minutes outside.


Image above: While orbiting above the Gulf of California and Baja California, a 100-foot tether connects the Agena with the Gemini XII spacecraft. While firing their side thrusters to slowly rotate the combined spacecraft, Jim Lovell and Buzz Aldrin used centrifugal force to generate a small amount of artificial gravity. Image Credit: NASA.

After the mission, NASA’s “Summary of Gemini Extravehicular Activity” noted that Gemini XII’s spacewalks demonstrated all the tasks attempted were feasible when body restraints were used to maintain position. But, “the most significant result was that underwater simulation duplicated the actual extravehicular actions and reactions with a high degree of fidelity.”

Another repeat of a test on Gemini XI was a computer controlled re-entry on Nov. 15, 1966.

“Gemini XII, Houston,” capcom Conrad said. “Our data shows you right on the money.”

In fact, Lovell and Aldrin splashed down just three miles from their target, near the recovery aircraft carrier USS Wasp sailing 600 miles east of Cape Kennedy.

The next day, Lovell and Aldrin were flown from the USS Wasp to the Cape’s skid strip where they were welcomed by Kennedy’s center director, Dr. Kurt Debus.

“We feel everyone here did an outstanding job in getting us into space,” Lovell said to those in attendance. “It takes a lot of people to fulfill a program. It’s the untiring efforts of thousands who got us up to there and back.”

Gemini Program Manager Walt Williams looked ahead to Apollo.

“It is now time to go on,” he said. “We will be able to go on with confidence because there was this program and it was called Gemini.”

President Lyndon B. Johnson also had high praise for those who made the Gemini Program possible.

“Today's flight was the culmination of a great team effort, stretching back to 1961,” he said. ”It directly involved more than 25,000 people in the National Aeronautics and Space Administration, the Department of Defense, other government agencies, universities, other research centers and in American industry.”

The President then looked forward to Apollo.


Image above: Following the Gemini XII splashdown on Nov. 15, 1966, astronauts Buzz Aldrin, left, and Jim Lovell are welcomed aboard the recovery aircraft carrier, USS Wasp, concluding their four-day mission. Image Credit: NASA.

“The months ahead will not be easy, as we reach toward the moon,” he said, ”but with Gemini as the forerunner, I am confident that we will overcome the difficulties and achieve another success.”

EDITOR'S NOTE: This is the final article in a series of features marking the 50th anniversary of Project Gemini. The program was designed as a steppingstone toward landing on the moon. The investment also provided technology now used in NASA's work aboard the International Space Station and planning for the Journey to Mars. For more, see "On the Shoulders of Titans: A History of Project Gemini." If you missed any of the features in this series, click on any of the links below.

Gemini III: Gemini Pioneered the Technology Driving Today's Exploration: http://www.nasa.gov/content/gemini-pioneered-the-technology-driving-todays-exploration

Gemini IV: Learning to Walk in Space: http://www.nasa.gov/feature/gemini-iv-learning-to-walk-in-space

Gemini V: Paving the Way for Long Duration Spaceflight: http://orbiterchspacenews.blogspot.ch/2015/08/gemini-v-paving-way-for-long-duration.html

Gemini VII & Gemini IV: Dual Gemini Flights Achieved Crucial Spaceflight Milestones: http://orbiterchspacenews.blogspot.ch/2015/12/dual-gemini-flights-achieved-crucial.html

Gemini VIII: Gemini's First Docking Turns to Wild Ride in Orbit: http://www.nasa.gov/feature/geminis-first-docking-turns-to-wild-ride-in-orbit

Gemini IX Crew Found 'Angry Alligator' in Earth Orbit: http://orbiterchspacenews.blogspot.ch/2016/06/gemini-ix-crew-found-angry-alligator-in.html

Gemini X Sets Records for Rendezvous, Altitude Above Earth: http://www.nasa.gov/feature/gemini-x-set-records-for-rendezvous-altitude-above-earth

Gemini XI: Demanding Mission Flies on Top of the World: http://www.nasa.gov/feature/demanding-gemini-xi-mission-flies-on-top-of-the-world

Gemini XII: Crew Masters the Challenges of Spacewalks: http://www.nasa.gov/feature/gemini-xii-crew-masters-the-challenges-of-spacewalks

Gemini Program: https://www.nasa.gov/mission_pages/gemini/index.html

Images (mentioned), Text, Credits: NASA's Kennedy Space Center, by Bob Granath.

Best regards, Orbiter.ch

Home is Where the Astronaut Is












ISS - International Space Station logo.

Nov. 1, 2016


Image above: ISS photographed by an STS-130 crew member. Image Credit: NASA.

The International Space Station serves as home, office and recreation room for astronauts. They share this confined space far above the Earth with crew members from different countries and cultures for as long as six months or more. At the same time, maintaining individual well-being and crew harmony is important for the crew and mission success.

The Culture, Values, and Environmental Adaptation in Space (At Home In Space) investigation, sponsored by the Canadian Space Agency, looks at changes in perceptions about home in space and the ways a unique culture may develop aboard the station during a mission.

Participants answer a series of questionnaires before, during and after flight, enabling researchers to see whether perceptions and the relative importance of values change over the course of a mission. Questions explore individual and culturally related differences, family functioning and relationships, personal values and coping with stress.


Image above: Astronaut Karen Nyberg helped create a quilt while aboard the space station. Image Credit: NASA.

“This is the first study to look at the extent to which a unique, shared space culture develops, whether crews develop customs and celebrations that are part of being on the station and different from what they would do on Earth,” explains Phyllis Johnson, principal investigator, Department of Sociology at the University of British Columbia in Vancouver, Canada.

Researchers expect to see a relationship between creation of a space culture and how crew members respond to different situations.

“They might be more of a team because of that culture and it might be a way to decrease stress,” Johnson said.

The investigation also takes the first look at how crew members adapt their living quarters to make them feel like home. Historically, astronauts have taken into space personal items such as photographs, children’s drawings and hobby activities. But no one has asked crew members how important it is to have these things with them.

The study also examines the effects on astronauts of their prolonged absence from family and familiar life on Earth.


Image above: The Expedition 43 crew gathers aboard the International Space Station to affix their mission patch to the vehicle. Commander Terry Virts (center left), Scott Kelly (top left), Gennady Padalka (top center), Anton Shkaplerov (top right), Mikhail Kornienko (bottom right), Samantha Cristoforetti (bottom center). Image Credit: NASA.

Investigators note that this work goes beyond traditional space psychology’s emphasis on problems, though. 

“It is important to recognize and measure positive effects of being in a challenging environment such as space,” said co-investigator and psychologist Peter Suedfeld, also at the University of British Columbia. “We look at personal change in attitudes and perspectives once back on Earth to see the effects on an individual’s life after such a dramatic experience.”

For multi-year missions, such as voyages to Mars, this work could lead to more effective ways for astronauts to feel at home and to integrate with fellow crew members.

“If we can help them be comfortable and happy, it helps morale and the success of the mission, and reduces potential problems,” Johnson said.


Image above: Crewmembers pose in the Zvezda Service Module (SM) during a meal. Clockwise, from left, flight engineers (FEs) Anatoly Ivanishin, Oleg Skripochka, Kate Rubins, commander Jeff Williams, and FEs Alexey Ovchinin and Takuya Onishi. Ivanishin, Skripochka and Ovchinin are Roscosmos cosmonauts; Onishi is a Japan Aerospace Exploration Agency (JAXA) astronaut. Image Credit: NASA.

Some communities on Earth experience conditions similar to those in space, including oil rig workers, crews on long-voyage tankers and cargo ships, researchers in remote locations such as the Antarctic and those on long military deployments. Older Americans in group housing also experience similar limits on living space, privacy, autonomy and control over their social and physical environment. This work could help make these groups feel more at home as well.

By helping to identify the most effective ways to make astronauts feel comfortable, this research will ultimately lead to happier and more productive crews on long missions where stress and tension are unavoidable.

“I compare a Mars mission to Earth’s early explorers, historic expeditions where people were isolated, confined to a vessel, in a dangerous outside environment and limited communication with home,” said Suedfeld. “What do we do to make the similar experience of long duration spaceflight better?”

The answer: help astronauts feel more at home in space.

Related links:

At Home In Space study: http://www.nasa.gov/mission_pages/station/research/experiments/1988.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), Text, Credits: NASA Johnson Space Center/Melissa Gaskill/Kristine Rainey.

Greetings, Orbiter.ch

lundi 31 octobre 2016

NASA’s SDO Catches a Lunar Transit












NASA - Solar Dynamics Observatory (SDO) patch.

Oct. 31, 2016

On Oct. 30, 2016, NASA’s Solar Dynamics Observatory, or SDO, experienced a partial solar eclipse in space when it caught the moon passing in front of the sun. The lunar transit lasted one hour, between 3:56 p.m. and 4:56 p.m. EDT, with the moon covering about 59 percent of the sun at the peak of its journey across the face of the sun. The moon’s shadow obstructs SDO’s otherwise constant view of the sun, and the shadow’s edge is sharp and distinct, since the moon has no atmosphere which would distort sunlight.


Animation above: On Oct. 30, 2016, NASA’s Solar Dynamics Observatory, or SDO, experienced a partial solar eclipse in space when it caught the moon passing in front of the sun. The lunar transit lasted one hour, between 3:56 p.m. and 4:56 p.m. EDT, with the moon covering about 59 percent of the sun at the peak of its journey across the face of the sun. Animation above: Credits: NASA’s Goddard Space Flight Center/SDO/Joy Ng.

From SDO’s point of view, the sun appears to be shaking slightly – but not because the solar observatory was spooked by this near-Halloween sight. Instead, the shaking results from slight adjustments in SDO’s guidance system, which normally relies upon viewing the entire sun to center the images between exposures. SDO captured these images in extreme ultraviolet light, a type of light invisible to human eyes. The imagery here is colorized in red.

Related Links:

NASA's SDO website: http://www.nasa.gov/sdo

NASA's eclipses and transits website: http://www.nasa.gov/eclipse

Animation (mentioned), Text, Credits: NASA’s Goddard Space Flight Center, by Lina Tran/Rob Garner.

Greetings, Orbiter.ch

View from Above












NASA - Cassini Mission to Saturn patch.

Oct. 31, 2016


Saturn appears as a serene globe amid tranquil rings in this view from NASA's Cassini spacecraft. In reality, the planet's atmosphere is an ever-changing scene of high-speed winds and evolving weather patterns, punctuated by occasional large storms (see PIA14901). The rings, consist of countless icy particles, which are continually colliding. Such collisions play a key role in the rings' numerous waves and wakes, which are the manifestation of the subtle influence of Saturn's moons and, indeed, the planet itself.

The long duration of the Cassini mission has allowed scientists to study how the atmosphere and rings of Saturn change over time, providing much-needed insights into this active planetary system.

The view looks toward the sunlit side of the rings from about 41 degrees above the ring plane. The image was taken with the Cassini spacecraft wide-angle camera on July 16, 2016 using a spectral filter which preferentially admits wavelengths of near-infrared light centered at 752 nanometers.

The view was acquired at a distance of approximately 1 million miles (2 million kilometers) from Saturn. Image scale is 68 miles (110 kilometers) per pixel.

The Cassini mission is a cooperative project of NASA, ESA (the European Space Agency) and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colorado.

PIA14901: http://photojournal.jpl.nasa.gov/catalog/PIA14901

For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov and http://www.nasa.gov/cassini. The Cassini imaging team homepage is at http://ciclops.org and ESA's website http://www.esa.int/Our_Activities/Space_Science/Cassini-Huygens

Image. Text, Credits: NASA/JPL-Caltech/Space Science Institute/Tony Greicius.

Greetings, Orbiter.ch