samedi 10 août 2019

Hubble Catches 2 Galaxies at Play













NASA - Hubble Space Telescope patch.

Aug. 10, 2019


The pair of strange, luminescent creatures at play in this image are actually galaxies — realms of millions upon millions of stars.

This galactic duo is known as UGC 2369. The galaxies are interacting, meaning that their mutual gravitational attraction is pulling them closer and closer together and distorting their shapes in the process. A tenuous bridge of gas, dust and stars can be seen connecting the two galaxies, created when they pulled material out into space across the diminishing divide between them.

Interaction with others is a common event in the history of most galaxies. For larger galaxies like the Milky Way, the majority of these interactions involve significantly smaller so-called dwarf galaxies. But every few billion years, a more momentous event can occur. For our home galaxy, the next big event will take place in about four billion years, when it will collide with its bigger neighbor, the Andromeda galaxy. Over time, the two galaxies will likely merge into one — already nicknamed Milkomeda.

Hubble Space Telescope (HST)

For more information about Hubble, visit:

http://hubblesite.org/

http://www.nasa.gov/hubble

http://www.spacetelescope.org/

Text Credits: ESA (European Space Agency)/NASA/Rob Garner/Image, Animation,  Credits: ESA/Hubble & NASA, A. Evans.

Greetings, Orbiter.ch

vendredi 9 août 2019

Satellite Software Contest on Station as Crew Tests Organ Printing













ISS - Expedition 60 Mission patch.

August 9, 2019

The International Space Station is the setting today for a student competition to control tiny, free-floating satellites aboard the orbiting lab. Meanwhile, the Expedition 60 crewmembers conducted a variety of research operations and continued configuring a pair of spacesuits.

Middle school students are competing to design algorithms that autonomously control basketball-sized SPHERES satellites aboard the station. The student-written software tests rendezvous and docking maneuvers that simulate scenarios such as retrieving an inoperable satellite. Flight Engineers Andrew Morgan and Alexander Skvortsov were on hand monitoring the SPHERES contest inside the Kibo laboratory module.


Image above: The Milky Way lights up an orbital night pass as the International Space Station orbited 257 miles above the Coral Sea in between Australia and Papua New Guinea. The atmospheric glow highlights Earth’s limb. Image Credit: NASA.

NASA astronaut Christina Koch is helping scientists learn how to print and grow human organs in space. She printed tissue samples using the BioFabrication Facility in the Columbus lab module. The samples are housed for several weeks inside a specialized incubator to promote cellular growth. Earth’s gravity inhibits 3-D bioprinters and incubators from recreating and growing complex organic structures.

Flight Engineers Nick Hague and Luca Parmitano continued working on U.S. spacesuits and spacewalking tools during the afternoon. Hague started the day configuring a fluorescence microscope that can observe cellular changes in microgravity. Parmitano serviced Europe’s Fluid Science Laboratory to continue researching the physics of fluids in microgravity.

International Space Station (ISS). Animation Credit: NASA

Commander Alexey Ovchinin worked in the Russian segment of the space lab today readying obsolete gear for return to Earth aboard a Soyuz spacecraft. The veteran cosmonaut spent the rest of the afternoon servicing life support gear and inspecting biology research hardware.

Related links:

Expedition 60: https://www.nasa.gov/mission_pages/station/expeditions/expedition60/index.html

SPHERES: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7591

Kibo laboratory module: https://www.nasa.gov/mission_pages/station/structure/elements/japan-kibo-laboratory

BioFabrication Facility: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=7599

Columbus lab module: https://www.nasa.gov/mission_pages/station/structure/elements/europe-columbus-laboratory

Specialized incubator: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=369

Fluorescence microscope: https://www.nasa.gov/mission_pages/station/research/news/ISS_Shrinks_Tool

Fluid Science Laboratory: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=258

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

NASA’s MMS Finds First Interplanetary Shock













NASA - Magnetospheric Multiscale Mission (MMS) patch.

Aug. 9, 2019

The Magnetospheric Multiscale mission — MMS — has spent the past four years using high-resolution instruments to see what no other spacecraft can. Recently, MMS made the first high-resolution measurements of an interplanetary shock.

Magnetospheric Multiscale Mission or MMS. Image Credit: NASA

These shocks, made of particles and electromagnetic waves, are launched by the Sun. They provide ideal test beds for learning about larger universal phenomena, but measuring interplanetary shocks requires being at the right place at the right time. Here is how the MMS spacecraft were able to do just that.

What’s in a Shock?

Interplanetary shocks are a type of collisionless shock — ones where particles transfer energy through electromagnetic fields instead of directly bouncing into one another. These collisionless shocks are a phenomenon found throughout the universe, including in supernovae, black holes and distant stars. MMS studies collisionless shocks around Earth to gain a greater understanding of shocks across the universe.

Interplanetary shocks start at the Sun, which continually releases streams of charged particles called the solar wind.

Animation of Solar Wind

Video above: Animation of the solar wind. Video Credits: NASA's Goddard Space Flight Center/Conceptual Image Lab.

The solar wind typically comes in two types — slow and fast. When a fast stream of solar wind overtakes a slower stream, it creates a shock wave, just like a boat moving through a river creates a wave. The wave then spreads out across the solar system. On Jan. 8, 2018, MMS was in just the right spot to see one interplanetary shock as it rolled by. 

Catching the Shock

MMS was able to measure the shock thanks to its unprecedentedly fast and high-resolution instruments. One of the instruments aboard MMS is the Fast Plasma Investigation. This suite of instruments can measure ions and electrons around the spacecraft at up to 6 times per second. Since the speeding shock waves can pass the spacecraft in just half a second, this high-speed sampling is essential to catching the shock.

Looking at the data from Jan. 8, the scientists noticed a clump of ions from the solar wind. Shortly after, they saw a second clump of ions, created by ions already in the area that had bounced off the shock as it passed by. Analyzing this second population, the scientists found evidence to support a theory of energy transfer first posed in the 1980s.

MMS consists of four identical spacecraft, which fly in a tight formation that allows for the 3D mapping of space. Since the four MMS spacecraft were separated by only 12 miles at the time of the shock (not hundreds of kilometers as previous spacecraft had been), the scientists could also see small-scale irregular patterns in the shock. The event and results were recently published in the Journal of Geophysical Research.


Animation above: Data from the Fast Plasma Investigation aboard MMS shows the shock and reflected ions as they washed over MMS. The colors represent the amount of ions seen with warmer colors indicating higher numbers of ions. The reflected ions (yellow band that appears just above the middle of the figure) show up midway through the animation, and can be seen increasing in intensity (warmer colors) as they pass MMS, shown as a white dot. Animation Credits: Ian Cohen.

Going Back for More

Due to timing of the orbit and instruments, MMS is only in place to see interplanetary shocks about once a week, but the scientists are confident that they’ll find more. Particularly now, after seeing a strong interplanetary shock, MMS scientists are hoping to be able to spot weaker ones that are much rarer and less well understood. Finding a weaker event could help open up a new regime of shock physics.

Related Link:

Learn more about NASA’s MMS Mission: http://www.nasa.gov/mms

Image (mentioned), Video (mentioned),  Animation (mentioned), Text, Credits: NASA/Rob Garner/Goddard Space Flight Center, by Mara Johnson-Groh.

Greetings, Orbiter.ch

Space Station Science Highlights: Week of August 5, 2019













ISS - Expedition 60 Mission patch.

Aug. 9, 2019

Astronauts aboard the International Space Station conducted new and ongoing scientific experiments this week, including studies of time perception and microgravity’s effects on brain proteins associated with neurodegenerative diseases and testing a 3D biological printer. The only laboratory that allows scientists to manipulate every variable including gravity, the space station also provides a platform for commercial research and investigations that support Artemis, NASA’s program to return humans to the Moon as a stepping stone to Mars.

Here are details on some of the science conducted on the orbiting laboratory during the week of August 5:

Does anybody really know what time it is?


Image above: NASA astronaut Christina Koch photographs Earth landmarks from the U.S. Destiny laboratory module's Window Observation Research Facility (WORF). Koch is wearing specialized goggles to protect her eyes from the Sun's rays. Image Credit: NASA.

The accurate perception of objects in the environment is critical for a person’s spatial orientation and reliable performance of motor tasks. Time perception in microgravity also is fundamental to motion perception, sound localization, speech, and fine motor coordination. The Time Perception experiment uses a laptop program that induces visual and audio stimuli and measures a subject's response to spatial and time perception. The goal is to quantify subjective changes in time perception that people experience during and after long-duration exposure to microgravity. Crew members performed experiment sessions using a head-mounted Oculus Rift display and headphones and a finger trackball.

Making printing a pancreas a possibility


Image above: NASA astronaut Andrew Morgan works on setting up the BioFabrication Facility to test-print tissues as part of an investigation into whether human organs can be 3D printed in the weightless environment of space. Image Credit: NASA.

The crew performed cassette installations, swaps and removals to test the new BioFabrication Facility (BFF) and encountered some difficulties with several of the smart pumps. To address these issues, the crew manually adjusted, inspected and cleaned the pumps and the ground team reported the activity appears to have been successful. Science and medicine envision using 3D biological printers to produce usable human organs, but printing complex structures inside organs, such as capillary structures, has proven difficult in Earth’s gravity. The BFF is designed to print organ-like tissues in microgravity as a step toward manufacturing human organs in space using refined biological 3D printing techniques.

A bank for something better than money

The crew collected samples for the NASA Repository investigation. A storage bank that maintains biological specimens over extended periods of time and under well-controlled conditions, Repository supports scientific discovery of fundamental knowledge about human physiological changes in and adaptation to microgravity. The samples provide unique opportunities for longitudinal studies of changes in human physiology spanning many missions and are a resource for future space flight-related research. Samples collected from crew members, including blood and urine, are processed and archived before, during and after flight.

The brain on microgravity


Animation above: NASA astronauts Nick Hague and Christina Koch work in the Life Sciences Glovebox on the Cell Science-02 investigation, which examines how microgravity affects healing, tissue regeneration and agents that induce healing. Animation Credit: NASA.

The Amyloid Aggregation investigation assesses whether microgravity affects formation of amyloid fibrils, which could represent a possible risk to astronauts on long flights. Amyloid fibrils are self-assembled fibrous protein aggregates that are associated with a number of neurodegenerative diseases such as Alzheimer’s and Parkinson’s. Better understanding of the mechanism underlying amyloid aggregation could protect astronauts on long missions and contribute to design of treatments for these diseases on Earth. The crew activated samples for the investigation and returned them to cold stowage.

Other investigations on which the crew performed work:

- ACME Flame Design, which studies the production and control of soot to optimize oxygen-enriched combustion and the design of robust, soot-free flames, is part of a series of independent ACME experiments using the orbiting laboratory’s Combustion Integrated Rack (CIR):
https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=1651

https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=317

- The European Space Agency’s GRIP experiment tests the ability of astronauts to manipulate items and control their arm motions in space: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=1188

- Lighting Effects studies the effects that replacing fluorescent light bulbs on the space station with solid-state light-emitting diodes (LEDs) has on crew member circadian rhythms, sleep, and cognitive performance:
https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=2013

- The ISS Experience creates short virtual reality videos from footage taken during the yearlong investigation covering different aspects of crew life, execution of science and the international partnerships involved on the space station:
https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7877

- The Cell Science-02 investigation examines how microgravity affects healing, tissue regeneration and agents that induce healing:
https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=1676

- The Actiwatch is a wristwatch-like monitor containing an accelerometer to measure motion and color sensitive photodetectors for monitoring ambient lighting to help analyze the crew’s circadian rhythms, sleep-wake patterns and activity:
https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=838

- Food Acceptability examines changes in the appeal of food aboard the space station during long-duration missions. “Menu fatigue” from repeatedly consuming a limited choice of foods may contribute to the loss of body mass often experienced by crew members, potentially affecting astronaut health, especially as mission length increases:
https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7562

- Rodent Research-17 (RR-17) uses young and old mice to evaluate the physiological, cellular and molecular effects of microgravity and spaceflight:
https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7992

Space to Ground: A New Mission: 08/09/2019

Related links:

Expedition 60: https://www.nasa.gov/mission_pages/station/expeditions/expedition60/index.html

Artemis: https://www.nasa.gov/artemis

Time Perception: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7504

BioFabrication Facility (BFF): https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=7599

Repository: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=954

Amyloid Aggregation: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7902

Spot the Station: https://spotthestation.nasa.gov/

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 (NASA), Text, Credits: NASA/Michael Johnson/Vic Cooley, Lead Increment Scientist Expedition 60.

Best regards, Orbiter.ch

jeudi 8 août 2019

Meet the Promising New Researchers Making Waves on the Space Station













ISS - International Space Station logo.

Aug. 8, 2019

Each year, the president of the United States selects an elite group of scientists and engineers at the beginning of their independent research careers to receive the Presidential Early Career Award for Scientists and Engineers. This is the highest honor given by the U.S. government to outstanding science, technology, engineering and mathematics (STEM) professionals at this point in their professions.

This year’s selection of 314 scientists includes 18 NASA researchers. Although these scientists are, as the award’s name indicates, early in their career, they have already built up impressive resumes. The list of accomplishments for three of them includes important contributions to research aboard the International Space Station.

International Space Station (ISS). Animation Credit: NASA

“The work of these three scientists is helping NASA enable human spaceflight exploration while making scientific discoveries. We benefit greatly from their research,” said Craig Kundrot, director of the Space Life and Physical Sciences Research and Applications division at NASA Headquarters. “Congratulations to Dr. Massa, Dr. Smith, and Dr. Barrila, and we look forward to them advancing the frontiers of knowledge in space biology.”

We sat down to chat with these three awardees, Jennifer Barrila, Ph.D., Gioia Massa, Ph.D. and David J. Smith, Ph.D., to learn more about how the orbiting laboratory has shaped their work.


Image above: Presidential Early Career Award for Scientists and Engineers recipient and International Space Station researcher Jennifer Barrila. Photo courtesy of Jennifer Barrila.

Jennifer Barrila grew up in the 80s during the Space Shuttle Program. Her admiration for the people she saw flying to space inspired Barrila to pursue a career goal that most kids only dream of: becoming an astronaut. Many who share this daunting ambition focus on becoming aerospace engineers or pilots. But Barrila’s fascination for biology led her to a different path. “As I was finishing high school, the space station was being constructed,” says Barrila. “I knew when it was complete they would need scientists to perform experiments, so I decided to follow my passion and train in the biological sciences.”

While Barrila, who now works at Arizona State University, hasn’t yet gone to space, her research has made the trip. She has played integral roles in several experiments aboard the space station and a shuttle mission that studied how microgravity may alter infectious disease risks. Barrila co-led the first study to profile how human cells respond to Salmonella infection in space, served as a co-investigator on the first full-duration virulence study performed in space and is working on two experiments that could launch to the orbiting laboratory later this year.

She also was also part of a study that examined the impact of microgravity on Salmonella’s ability to infect a 3D cell culture model of the human colon. Barrila is now working to advance these models by incorporating fecal microbes collected from astronauts before, during and after spaceflight. “We're looking to see whether changes that occurred to the astronaut microbiome could possibly change their susceptibility to infection with Salmonella,” Barrila says. “I'm pretty excited about this study because we just don't know what we will see.”

While Barrila would still love to go to space, it is no longer her primary goal. “I went into this field wanting to become an astronaut, but doing the research has been so incredibly rewarding,” says Barrila. “Even if I never get to go into space, it’s been exciting to have the opportunity to contribute to the human spaceflight program.”


Image above: Presidential Early Career Award for Scientists and Engineers recipient and International Space Station researcher Gioia Massa. Photo courtesy of Gioia Massa.

Gioia Massa grew up in Florida about an hour away from NASA’s Kennedy Space Center in Cape Canaveral. After her middle school agriculture teacher was invited to Kennedy to learn about plant production for astronauts, he shared what he learned with Massa. “He brought back hours and hours of video. I was just completely captivated,” says Massa. “I think I watched all of it.”

From that springboard she chose to learn about hydroponics in high school, interned at Kennedy Space Center in the space life sciences training program and eventually earned her Ph.D. in Plant Biology from Penn State University. When a role for a NASA scientist opened up in 2013, Massa jumped at the opportunity.

Her work at NASA has built on her middle school passion of growing plants in space, looking at numerous aspects of agriculture in microgravity, specifically on the space station.


Image above: View of VEG-04 plant check, watering and weighing of harvested leaves in the Columbus Module. Image Credit: NASA.

She is studying the perfect conditions for plant growth in space and what species grow most effectively there. She is even getting feedback from the astronauts currently on board the station on which crops taste best. “Plants are very adaptable. They can really respond to the environment,” says Massa. “But getting that environment right is truly our hardest challenge. The biology is not as challenging as the physics to overcome.”

Right now, Massa and her team are focused on perfecting the cultivation of lettuce plants and a few other basic crops that they have learned to grow effectively. They hope to continue with their experiments on the space station and build on this knowledge to learn to grow more fruiting crops such as tomatoes and peppers. “To have an orbiting laboratory up there with astronauts continuously available to do science gives you a lot of power that you would otherwise not have. If you just do things one time, it leaves so many open questions,” says Massa. “Being able to do repeated evolutionary work on a platform like the space station is really the only way to advance these exploration systems.”


Image above: Presidential Early Career Award for Scientists and Engineers recipient and International Space Station researcher David J. Smith. Photo courtesy of David J. Smith.

David J. Smith got a surprise call while in graduate school. On the other end was Crystal Jaing Ph.D., a researcher from Lawrence Livermore National Laboratory. “I couldn't believe my luck,” says Smith. “It was hard to believe, after having read all of her team’s literature, that she wanted to collaborate on something. She put together the dream team in microbiology.”

Jaing was recruiting a team for a new investigation of microbiology on the space station called Microbial Tracking-2. “Our goal is to identify any correlations of the microbiome community between what is in the space station versus what's on the astronauts to see if there is any microbial transfer and the potential impacts to crew health,” says Jaing.

While Smith’s previous research was based within our atmosphere, he shared an interest with Jaing in detecting microorganisms in challenging environments. “My work in graduate school was finding microbial signals in the upper atmosphere,” says Smith. “When Crystal put together this proposal, we knew that some of those microbes would also be floating around in spacecraft air. We thought we would bring some of the methodology from the open atmosphere here on Earth to the station.”

The year after finishing graduate school, Smith got a job working at Kennedy Space Center and helped finalize the proposal for Microbial Tracking-2.


Image above: Microbial Tracking-2 hardware aboard the International Space Station, where it collects samples of the microbes and viruses floating in the air. Image Credit: NASA.

The Microbial Tracking team now has almost completed the sample collection period. Crew samples taken before, during and after flight, as well as environmental samples from station surfaces and air, make up the data. Smith and the research team will use this information to identify microbes and viruses on the orbital outpost and crew, and assess their disease-causing potential.

Smith sees this research in low-Earth orbit as a crucial step towards more than just preventing disease in space. He says it is needed to produce safe water, air and food systems on longer space missions to destinations like the Moon or Mars. “It’s going to be a whole different ball game when we go to deep space,” says Smith. “And it’s not going to be just macrosystems we have to be mindful of. It’s the invisible little passengers we bring along with us.”

The Space Life and Physical Sciences Research and Applications Division (SLPSRA) of NASA’s Human Exploration and Operations Mission Directorate at NASA Headquarters in Washington funds the research of these three outstanding scientists.

Relate links:

How human cells respond to Salmonella infection in space: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=790

First full-duration virulence study performed in space: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=792

Plant growth in space: https://www.nasa.gov/content/growing-plants-in-space

Microbial Tracking-2: https://www.nasa.gov/ames/research/space-biosciences/microbial-tracking-2

Previous research: https://aem.asm.org/content/aem/79/4/1134.full.pdf

Space Life and Physical Sciences Research and Applications Division (SLPSRA): https://www.nasa.gov/directorates/heo/slpsra#_blank

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), Text, Credits: NASA/Michael Johnson/JSC/International Space Station Program Science Office/Erin Winick.

Best regards, Orbiter.ch

Cloaked Black Hole Discovered in Early Universe Using NASA’s Chandra













NASA - Chandra X-ray Observatory patch.

Aug. 8, 2019

Astronomers have discovered evidence for the farthest "cloaked" black hole found to date, using NASA's Chandra X-ray Observatory. At only about 6% of the current age of the universe, this is the first indication of a black hole hidden by gas at such an early time in the history of the cosmos.


Image above: Data from NASA’s Chandra X-ray Observatory have revealed what may be the most distant shrouded black hole. Image Credits: X-ray: NASA/CXO/Pontificia Universidad Catolica de Chile/F. Vito; Radio: ALMA (ESO/NAOJ/NRAO); optical: Pan-STARRS.

Supermassive black holes, which are millions to billions of times more massive than our Sun, typically grow by pulling in material from a disk of surrounding matter. Rapid growth generates large amounts of radiation in a very small region around the black hole. Scientists call this extremely bright, compact source a "quasar."

According to current theories, a dense cloud of gas feeds material into the disk surrounding a supermassive black hole during its period of early growth, which "cloaks" or hides much of the quasar's bright light from our view. As the black hole consumes material and becomes more massive, the gas in the cloud is depleted, until the black hole and its bright disk are uncovered.

“It’s extraordinarily challenging to find quasars in this cloaked phase because so much of their radiation is absorbed and cannot be detected by current instruments,” said Fabio Vito CAS-CONICYT Fellow at the Pontificia Universidad Católica de Chile, in Santiago, Chile, who led the study. “Thanks to Chandra and the ability of X-rays to pierce through the obscuring cloud, we think we’ve finally succeeded.”

The new finding came from observations of a quasar called PSO167-13, which was first discovered by Pan-STARRS, an optical-light telescope in Hawaii. Optical observations from these and other surveys have detected about 200 quasars already shining brightly when the universe was less than a billion years old, or about 7 percent of its present age. These surveys were only considered effective at finding unobscured black holes, because the radiation they detect is suppressed by even thin clouds of gas and dust. Since PSO167-13 was part of those observations, this quasar was expected to be unobscured, too.

Vito’s team tested this idea by using Chandra to observe PSO167-13 and nine other quasars discovered with optical surveys. After 16 hours of observation, only three X-ray light photons were detected from PSO167-13, all with relatively high energies. Since low-energy X-rays are more easily absorbed than higher energy ones, the likely explanation is that the quasar is highly obscured by gas, allowing only high-energy X-rays to be detected.

“This was a complete surprise”, said co-author Niel Brandt of Penn State University in University Park, Pennsylvania. “It was like we were expecting a moth but saw a cocoon instead. None of the other nine quasars we observed were cloaked, which is what we anticipated.”

An interesting twist for PSO167-13 is that the galaxy hosting the quasar has a close companion galaxy, visible in data previously obtained with the Atacama Large Millimeter Array (ALMA) of radio dishes in Chile and NASA’s Hubble Space Telescope. Because of their close separation and the faintness of the X-ray source, the team was unable to determine whether the newly-discovered X-ray emission is associated with the quasar PSO167-13 or with the companion galaxy.

If the X-rays come from the known quasar, then astronomers need to develop an explanation for why the quasar appeared highly obscured in X-rays but not in optical light. One possibility is that there has been a large and rapid increase in cloaking of the quasar during the three years between when the optical and the X-ray observations were made.

Chandra X-ray Observatory. Animation Credits: NASA/CXC

On the other hand, if instead the X-rays arise from the companion galaxy, then it represents the detection of a new quasar in close proximity to PSO167-13. This quasar pair would be the most distant yet detected.

In either of these two cases, the quasar detected by Chandra would be the most distant cloaked one yet seen, at 850 million years after the Big Bang. The previous record holder was observed 1.3 billion years after the Big Bang.

The authors plan to follow up with more observations to learn more.

“With a longer Chandra observation we'll be able to get a better estimate of how obscured this black hole is,” said co-author Franz Bauer, also from the Pontificia Universidad Católica de Chile and associate member of the Millenium Institute of Astrophysics, “and make a confident identification of the X-ray source with either the known quasar or the companion galaxy.”

The authors also plan to search for more examples of highly obscured black holes.

“We suspect that the majority of supermassive black holes in the early universe are cloaked: it’s then crucial to detect and study them to understand how they could grow to masses of a billion suns so quickly,” said co-author Roberto Gilli of INAF in Bologna, Italy.

A paper describing these results is accepted for publication in Astronomy and Astrophysics and is available online. NASA's Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science and flight operations from Cambridge, Massachusetts.

Astronomy and Astrophysics: https://arxiv.org/abs/1906.04241

Read more from NASA's Chandra X-ray Observatory: http://chandra.harvard.edu/photo/2019/cloaked/

For more Chandra images, multimedia and related materials, visit: http://www.nasa.gov/chandra

Image (mentioned), Animation (mentioned), Text, Credits: NASA/Lee Mohon/Chandra X-ray Center/Megan Watzke/Marshall Space Flight Center/Molly Porter.

Greetings, Orbiter.ch

Crew Gears Up for Spacewalk, Scans Eyes and Practices Medical Emergency













ISS - Expeition 60 Mission patch.

August 8, 2019

The Expedition 60 crew is gearing up for an upcoming spacewalk to prepare the International Space Station for more commercial crew missions. Biomedical science also took up a portion of the astronauts’ day as they help researchers understand what happens to the human body in microgravity.

NASA astronauts Nick Hague and Andrew Morgan are reviewing their tasks planned for Aug. 21 when they conduct the fifth spacewalk of the year at the orbiting lab. The duo will take about six-and-a-half hours to install the International Docking Adapter-3 (IDA-3) on top of the Harmony module. The IDA-3, delivered inside the Dragon cargo craft’s trunk, will be the second port at the station designed to receive the new Boeing and SpaceX crew ships.


Image above: NASA astronaut Nick Hague, in his white U.S. spacesuit, is contrasted by the blackness of space during a six-hour, 39-minute spacewalk that took place in March 2019. Image Creddit: NASA.

Flight Engineers Christina Koch and Luca Parmitano are helping the spacewalkers get ready for the upcoming excursion. They are configuring spacesuit components today and will continue assisting the pair before, during and after the next spacewalk.

Morgan first joined Koch and Parmitano during the morning for ultrasound eye exams. Koch took charge of the eye scans in the Columbus lab module with real-time inputs from doctors on the ground. She observed her crewmates’ retina, cornea, lens and optic nerve to maintain eye health in space.

International Space Station (ISS). Animation Creit: NASA

Koch and Parmitano later split up feeding the station’s mice and cleaning their habitats in the Destiny laboratory module. Observing the rodents, which are genetically similar to humans, in the weightless environment of microgravity gives scientists critical therapeutic insights that can benefit Earthlings and astronauts.

The most recent trio to arrive at the station gathered at the end of the day to train for a medical emergency. Morgan, Parmitano and cosmonaut Alexander Skvortsov practiced cardiopulmonary resuscitation (CPR), checked out medical gear and reviewed emergency communications.

Related links:

Expedition 60: https://www.nasa.gov/mission_pages/station/expeditions/expedition60/index.html

Spacewalk: https://www.nasa.gov/mission_pages/station/spacewalks/

International Docking Adapter-3 (IDA-3): https://www.nasa.gov/feature/meet-the-international-docking-adapter

Harmony module: https://www.nasa.gov/mission_pages/station/structure/elements/harmony

Rodents: https://go.nasa.gov/2YojzZO

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

Best regards, Orbiter.ch