What’s Up For September 2017?

We’re Upgrading Our X-ray Vision!

Think X-ray vision is a superpower found only in comics and movies? Unlike Superman and Supergirl, NASA has it for real, thanks to the X-ray observatories we’ve sent into orbit.

Now the Imaging X-ray Polarimetry Explorer – IXPE for short – has shot into space to enhance our superpower!

Meet IXPE

When dentists take X-ray pictures of a tooth, they use a machine that makes X-rays and captures them on a device placed on the opposite side. But X-rays also occur naturally. In astronomy, we observe X-rays made by distant objects to learn more about them.

IXPE will improve astronomers’ knowledge about some of these objects, like black holes, neutron stars, and the expanding clouds made by supernova explosions.

That’s because it will capture a piece of information about X-ray light that has only rarely been measured from space!

X-ray astronomers have learned a lot about the cosmos by measuring three properties of light – when it arrives, where it’s coming from, and what energies it has (think: colors). Picture these characteristics as making up three of the four sides of a pyramid. The missing piece is a property called polarization.

Polarization tells us how organized light is. This gives astronomers additional clues about how the X-rays were made and what matter they’ve passed through on their way to us. IXPE will explore this previously hidden side of cosmic X-ray sources.

What is polarization?

All light, from microwaves to gamma rays, is made from pairs of waves traveling together – one carrying electricity and the other magnetism. These two waves always vibrate at right angles (90°) to each other, with their peaks and valleys in sync, and they also vibrate at right angles to their direction of motion.

To keep things simple, we’ll illustrate only one of these waves – the one carrying electricity. If we could zoom into a typical beam of light, we’d see something like the animation above. It’s a mess, with all the wave peaks pointing in random directions.

When light interacts with matter, it can become better organized. Its electric field can vibrate in a way that keeps all the wave crests pointing in the same direction, as shown above. This is polarized light.

The amount and type of polarization we detect in light tell us more about its origin, as well as any matter it interacted with before reaching us.

Let’s look at the kinds of objects IXPE will study and what it may tell us about them.

Exploring star wrecks

Exploded stars create vast, rapidly expanding clouds called supernova remnants – like the Jellyfish Nebula above. It formed 4,000 years ago, but even today, the remnant’s heart can tell us about the extreme conditions following the star’s explosion.

X-rays give us a glimpse of the powerful processes at work during and after these explosions. IXPE will map remnants like this, revealing how X-rays are polarized across the entire object. This will help us better understand how these celestial cataclysms take place and evolve.

Magnifying supermagnets

Some supernovae leave behind neutron stars. They form when the core of a massive star collapses, squeezing more than our Sun’s mass into a ball only as wide as a city.

The collapse greatly ramps up their spin. Some neutron stars rotate hundreds of times a second! Their magnetic fields also get a tremendous boost, becoming trillions of times stronger than Earth’s. One type, called a magnetar, boasts the strongest magnetic fields known – a thousand times stronger than typical neutron stars.

These superdense, superspinning supermagnets frequently erupt in powerful outbursts (illustrated above) that emit lots of X-rays. IXPE will tell astronomers more about these eruptions and the extreme magnetic fields that help drive them.

Closing in on black holes

Black holes can form when massive stars collapse or when neutron stars crash together. Matter falling toward a black hole quickly settles into a hot, flat structure called an accretion disk. The disk’s inner edge gradually drains into the black hole. Notice how odd the disk appears from certain angles? This happens because the black hole’s extreme gravity distorts the path of light coming from the disk’s far side.

X-rays near the black hole can bounce off the disk before heading to our telescopes, and this polarizes the light. What’s exciting is that the light is polarized differently across the disk. The differences depend both on the energies of the X-rays and on what parts of the disk they strike. IXPE observations will provide astronomers with a detailed picture of what’s happening around black holes in our galaxy that can’t be captured in any other way.

By tracking how X-ray light is organized, IXPE will add a previously unseen dimension to our X-ray vision. It’s a major upgrade that will give astronomers a whole new perspective on some of the most intriguing objects in the universe.

Keep up with what’s happening in the universe and how we study it by following NASA Universe on Twitter and Facebook.

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This animation blinks between two images of our Mars Phoenix Lander. The first – dark smudges on the planet’s surface. The second – the same Martian terrain nearly a decade later, covered in dust. Our Mars orbiter captured this shot as it surveyed the planet from orbit: the first in 2008. The second: late 2017.

In August 2008, Phoenix completed its three-month mission studying Martian ice, soil and atmosphere. The lander worked for two additional months before reduced sunlight caused energy to become insufficient to keep the lander functioning. The solar-powered robot was not designed to survive through the dark and cold conditions of a Martian arctic winter.

Read the full story HERE.

Credit: NASA/JPL-Caltech/Univ. of Arizona

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Juno: Join the Mission!

Our Juno spacecraft may be millions of miles from Earth, but that doesn’t mean you can’t get involved with the mission and its science. Here are a few ways that you can join in on the fun:

Juno Orbit Insertion

This July 4, our solar-powered Juno spacecraft arrives at Jupiter after an almost five-year journey. In the evening of July 4, the spacecraft will perform a suspenseful orbit insertion maneuver, a 35-minute burn of its main engine, to slow the spacecraft by about 1,212 miles per hour so it can be captured into the gas giant’s orbit. Watch live coverage of these events on NASA Television:

Pre-Orbit Insertion Briefing Monday, July 4 at 12 p.m. EDT

Orbit Insertion Coverage Monday, July 4 at 10:30 p.m. EDT

Join Us On Social Media

Orbit Insertion Coverage Facebook Live Monday, July 4 at 10:30 p.m. EDT

Be sure to also check out and follow Juno coverage on the NASA Snapchat account!

JunoCam

The Juno spacecraft will give us new views of Jupiter’s swirling clouds, courtesy of its color camera called JunoCam. But unlike previous space missions, professional scientists will not be the ones producing the processed views, or even choosing which images to capture. Instead, the public will act as a virtual imaging team, participating in key steps of the process, from identifying features of interest to sharing the finished images online.

After JunoCam data arrives on Earth, members of the public will process the images to create color pictures. Juno scientists will ensure JunoCam returns a few great shots of Jupiter’s polar regions, but the overwhelming majority of the camera’s image targets will be chosen by the public, with the data being processed by them as well. Learn more about JunoCam HERE.

Follow our Juno mission on the web, Facebook, Twitter, YouTube and Tumblr.

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Employee Training – It’s Kind of a Big Deal

This is what it would look like if you were training to #BeAnAstronaut! Astronaut candidates must train for two years before they become official NASA astronauts. After graduation, you can look forward to more skill building when training for upcoming missions. Let’s dive into some of the courses you can expect once you’re selected for the job: 

T-38 Jet Training 

All astronaut candidates must learn to safely operate in a T-38 jet, either as a pilot or crew. Because this is the one area of their training that is not a simulation and involves decisions with life or death consequences, it teaches them to think quickly and clearly in dynamic situations.

 Neutral Buoyancy Lab Training

The mission of the Neutral Buoyancy Lab (NBL) is to prepare astronauts for spacewalking outside the International Space Station! Astronauts are lowered into a large pool wearing full spacesuits. The pool is full of hardware that replicates what the space station is really like, so astronauts are able to practice tasks they can expect on a spacewalk such as going out the airlock, finding a good path to the work site and more! The NBL is beneficial because it gives astronauts the ability to be neutrally buoyant which simulates the effects of microgravity.

Geology Training

Geology training courses are specially tailored to the work astronauts will do from the International Space Station or on the next interplanetary mission! Astronauts learn the basic principles of geology, see rocks in their natural environment and handle samples from their class discussions. It’s less like memorizing the names of rocks and more like learning how geologists think and work. 

Wilderness Survival Training 

Before they end up in space, astronauts carry out a significant portion of their training in aircraft on Earth. It's unlikely, but possible, that one of those training planes could crash in a remote area and leave the humans on board to fend for themselves for a while. Knowing how to take care of their basic needs would be invaluable. Through the exercises, instructors hope to instill self-care and self-management skills, to develop teamwork skills, and to strengthen leadership abilities – all of which are valuable for working in the isolation of the wild or the isolation of space. 

Extreme Environment Training 

Astronauts participate in a variety of extreme environment training to prepare for the stresses of spaceflight. Pictured here, they are exploring the underground system of the Sa Grutta caves in Sardinia, Italy as a part of the European Astronaut Centre’s Cooperative Adventure for Valuing and Exercising human behavior and performance Skills (CAVES) expedition. Seasoned astronauts as well as rookies participate in the course and share experiences while learning how to improve leadership, teamwork, decision-making and problem-solving skills.

Virtual Reality Training

In our Virtual Reality Laboratory training facility at Johnson Space Center astronauts are able to immerse themselves in virtual reality to complete mission tasks and robotic operations before launching to space. The facility provides real time graphics and motion simulators integrated with a tendon-driven robotic device to provide the kinesthetic sensation of the mass and inertia characteristics of any large object (<500lb) being handled.

Want more? We’ve compiled all you need to know about what it takes to #BeAnAstronaut HERE.

Apply now, HERE!  

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Meteorites Help Answer Questions About Solar System Evolution

A team of eight scientists including our own Astromaterials Curation Chief Cindy Evans spent two-months in the frozen landscape of Antarctica as part of the Antarctic Search for Meteorites (ANSMET), a 40-year program that has helped reveal information about asteroids, other bodies of our solar system and the red planet which will assist us on our Journey to Mars.

The team recovered nearly 570 new meteorite samples from the Miller Range of the Trans-Antarctic Mountains during the expedition.

After a several-month journey from Antarctica, these samples arrived at our Johnson Space Center in Houston, Texas, on April 14 to become part of the U.S. Antarctic meteorite collection housed at Johnson and the Smithsonian Institution in Washington, D.C.

Samples recovered from recent seasons include rare and scientifically valuable pieces of Mars and Moon, as well as rocks formed very early during the formation and evolution of the solar system that hold clues to the origin of volatiles, planets and the organic compounds essential to life.

Meteorites are currently the only way to acquire samples from Mars as well as new samples of the moon that are different from – and originated far from – the Apollo landing sites, as well as a variety of asteroid bodies.

Samples from this collection (representing nearly 40 individual collection seasons) are available to researchers worldwide, and hundreds are distributed every year by the Astromaterials Curation Office.

The meteorites collected give us important clues about the early solar system, but even the thousands of meteorites recovered over the years represent a tiny part of the larger puzzle, including a find in the 1990s that produced evidence that sparked a vigorous debate about whether life could have existed on Mars more than 3.6 billion years ago.

As engineers and scientists around the country work hard to develop the technologies astronauts will use to one day live and work on Mars, and safely return home from the next giant leap for humanity, the meteorites provide critical data that enable engineers to build the right technologies.

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NASA’s View of COVID-19

#COVID19 led to changes in human activities around the globe. We can see some of these changes from space. Some bodies of water have run clearer, emissions of pollutants have temporarily declined, and transportation and shipment of goods have decreased.

Along with our partner agencies – ESA and JAXA – we’re making satellite data available on the COVID-19 Earth Observation Dashboard, where you can explore some of the changes we can see from space.

But it’s not just what we can see. When the pandemic began, NASA engineers sprang into action to build ventilators, oxygen hoods and more to help save lives.

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Hot & Steamy RS-25 Engine Test

Today, we tested the RS-25 engine at Stennis Space Center in Mississippi, and boy was it hot! Besides the fact that it was a hot day, the 6,000 degree operating temperature of the hot fire test didn’t help things. This engine is one of four that will power the core stage of our Space Launch System (SLS) into deep space and to Mars. Today’s test reached 109% power and burned 150,000 gallons of liquid oxygen and 60,000 gallons of liquid hydrogen. When SLS launches with all 4 of its engines, it will be the most powerful rocket in the world!

This engine was previously used to to fly dozens of successful missions on the space shuttle, so you might be asking, “Why are we spending time testing it again if we already know it’s awesome?” Well, it’s actually really important that we test them specifically for use with SLS for a number of reasons, including the fact that we will be operating at 109% power, vs. the 104% power previously used.

If you missed the 535-second, ground rumbling test today -- you’re in luck. We’ve compiled all the cool stuff (fire, steam & loud noises) into a recap video. Check it out here:

Six Science-y Shipments Sent to the Space Station

Northrop Grumman launched its Cygnus spacecraft into orbit to the International Space Station at 4:01 a.m. EST on Nov. 17 from Wallops Flight Facility in Virginia. Cygnus launched on an Antares rocket carrying crew supplies, equipment and scientific research to crewmembers aboard the station. The spacecraft is named after NASA astronaut and U.S. Navy officer John Young, who walked on the Moon during Apollo 16 and commanded the first space shuttle mission. Throughout his lifetime, Young logged 835 hours in space over the course of six missions.

Antares launched the S.S. John Young from the Mid-Atlantic Regional Spaceport’s Pad-0A on Wallops Island, carrying tons of cargo, including scientific investigations that will study 3D printing and recycling, cement solidification, and crystals that may fight Parkinson’s disease.

Here’s a look at six science-y experiments and research this mission will deliver to the space station.

1. 3D printing and recycling

Refabricator demonstrates an integrated 3D printer and recycler for the first time aboard the space station.

It recycles waste plastic materials into high-quality 3D-printer filament, which could enable sustainable fabrication, repair, and recycling on long-duration space missions.

2. Sensory input in microgravity

Changes in sensory input in microgravity may be misinterpreted and cause a person to make errors in estimation of velocity, distance or orientation.

VECTION, a Canadian Space Agency (CSA) investigation, examines this effect as well as whether people adapt to altered sensory input on long-duration missions and how that adaptation changes upon return to Earth.

3. Solidifying cement in space

The MVP-Cell 05 investigation uses a centrifuge to provide a variable gravity environment to study the complex process of cement solidification, a step toward eventually making and using concrete on extraterrestrial bodies.

4. From stardust to solar systems

Much of the universe was created when dust from star-based processes clumped into intermediate-sized particles and eventually became planets, moons and other objects. Many questions remain as to just how this worked, though.

The EXCISS investigation seeks answers by simulating the high-energy, low gravity conditions that were present during formation of the early solar system. Scientists plan to zap a specially formulated dust with an electrical current, then study the shape and texture of pellets formed.

5. Growing crystals to fight Parkinson’s disease

The CASIS PCG-16 investigation grows large crystals of an important protein, Leucine-rich repeat kinase 2, or LRRK2, in microgravity for analysis back on Earth.

This protein is implicated in development of Parkinson’s disease, and defining its shape and morphology may help scientists better understand the pathology of the disease and develop therapies to treat it. Crystals of LRRK2 grown in gravity are too small and too compact to study, making microgravity an essential part of this research.

6. Better gas separation membranes

Membranes represent one of the most energy-efficient and cost-effective technologies for separating and removing carbon dioxide from waste gases, thereby reducing greenhouse gas emissions. CEMSICA tests membranes made from particles of calcium-silicate (C-S) with pores 100 nanometers or smaller. Producing these membranes in microgravity may resolve some of the challenges of their manufacture on Earth and lead to development of lower-cost, more durable membranes that use less energy. The technology ultimately may help reduce the harmful effects of CO2 emissions on the planet.

For daily updates, follow @ISS_Research.

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Water, Water Everywhere; We Track Drops to Drink!

When we think about what makes a planet habitable, we’re often talking about water. With abundant water in liquid, gas (vapor) and solid (ice) form, Earth is a highly unusual planet. Almost 70% of our home planet’s surface is covered in water!

But about 97% of Earth’s water is salty – only a tiny amount is freshwater: the stuff humans, pets and plants need to survive.

Water on our planet is constantly moving, and not just geographically. Water shifts phases from ice to water to vapor and back, moving through the planet’s soils and skies as it goes.

That’s where our satellites come in.

Look at the Midwestern U.S. this spring, for example. Torrential rain oversaturated the soil and overflowed rivers, which caused severe flooding, seen by Landsat.

Our satellites also tracked a years-long drought in California. Between 2013 and 2014, much of the state turned brown, without visible green.  

It’s not just rain. Where and when snow falls – and melts – is changing, too. The snow that falls and accumulates on the ground is called snowpack, which eventually melts and feeds rivers used for drinking water and crop irrigation. When the snow doesn’t fall, or melts too early, communities go without water and crops don’t get watered at the right time.

Even when water is available, it can become contaminated by blooms of phytoplankton, like cyanobacteria . Also known as blue-green algae, these organisms can make humans sick if they drink the water. Satellites can help track algae from space, looking for the brightly colored blooms against blue water.

Zooming even farther back, Earth’s blue water is visible from thousands of miles away. The water around us makes our planet habitable and makes our planet shine blue among the darkness of space.

Knowing where the water is, and where it’s going, helps people make better decisions about how to manage it. Earth’s climate is changing rapidly, and freshwater is moving as a result. Some places are getting drier and some are getting much, much wetter. By predicting droughts and floods and tracking blooms of algae, our view of freshwater around the globe helps people manage their water.

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Scott Kelly Was the First To…

Astronaut Scott Kelly returned home from his year in space mission on March 1. Spending that much time in space allowed him to rack up some pretty cool milestones. Here are some of his awesome “firsts”:

Firsts on Social Media

While in space, Scott Kelly had the opportunity to host the first NASA TweetChat from space.

The first ever Tumblr AnswerTime from space was hosted by Scott Kelly during his One Year Mission.

Scott Kelly hosted the first NASA Reddit AMA from space.

Before leaving for his year in space, President Obama asked him to Instagram his time on orbit…a Presidential request to Instagram is a first!

Firsts for Scott

During his year in space, Scott conducted his first spacewalk. He hadn’t spacewalked on any of his previous missions, but did so three times during the One Year Mission.

Firsts for an American Astronaut

Most notably, Scott Kelly is the first U.S. astronaut to spend a year in space. His time on orbit also allowed us to conduct the first ever Twins Study on the space station. While Scott was in space, his twin brother Mark Kelly was on Earth. Since their genetic makeup is as close to identical as we can get, this allows a unique research perspective. We can now compare all of the results from Scott in space to his brother Mark on Earth.

During his year in space, Scott had the opportunity to be one of the first astronauts to harvest and eat lettuce grown in the space station’s VEGGIE facility. 

Space flowers! Scott was also one of the firsts to help grow and harvest zinnia flowers in the VEGGIE facility. Growing flowering plants in space will help scientists learn more about growing crops for deep-space missions and our journey to Mars.

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