It’s National Composites Week! Wait, What’s A Composite?

How do you guys help with climate change?

Not Your Average Delivery Vehicle

Just like people here on Earth, astronauts get shipments too! But not in the typical sense. 8,200 pounds of cargo, including supplies and scientific experiments, is on its way to the International Space Station thanks to Northrop Grumman’s Cygnus cargo spacecraft. This ‘package’ launched out of Wallops Flight Facility on Nov. 2, 2019 at 9:59 a.m. EDT. The investigations aboard the rocket range from research into human control of robotics in space to reprocessing fibers for 3D printing. Get ready, because these new and exciting experiments are arriving soon!

THE SEARCH FOR DARK MATTER

Stars, planets and their molecules only make up 15% of our universe. The rest is dark matter. However, no one has actually ever been able to see or study it. The Alpha Magnetic Spectrometer -02 (AMS-02) has been searching for this substance since 2011. Northrop Grumman’s CRS-12 mission carries new parts for AMS-02 that will be added during a series of upcoming spacewalks so that the instrument can continue to help us shed light on this mystery.

THE REMOTE EXPLORATION OF EARTH

Rovers operated by astronauts on the International Space Station will attempt to collect geological samples on Earth as part of an investigation called ANALOG-1. The samples, however, are not the important part of the study. Humans experience degraded sensorimotor functions in microgravity that could affect their operation of a robot. This study is designed to learn more about these issues, so that one day astronauts could use robots to perform research on planets they hope to walk on.

WOAH, THAT’S RAD

The AstroRad Vest is pretty rad. So rad, in fact, that it was sent up on the launch of Northrop Grumman’s CRS-12 mission. This vest intends to protect astronauts from harmful radiation in space. While going about normal activity on the space station, astronauts will wear AstroRad and make note of things like comfort over long periods of time. This will help researchers on Earth finalize the best design for future long duration missions.

EVEN ASTRONAUTS RECYCLE

The Made in Space Recycler (MIS) looks at how different materials on the International Space Station can be turned into filament used for 3D printing. This 3D printing is done right there in space, in the Additive Manufacturing Facility. Similar studies will be conducted on Earth so that comparisons can be made.  

FASTER, CHEAPER ACCESS TO SPACE

A collaboration between Automobili Lamborghini and the Houston Methodist Research Institute will be using NanoRacks-Craig-X FTP  to test the performance of 3D-printed carbon fiber composites in the extreme environment of space. The study could lead to materials used both in space and on Earth. For example, the study may help improve the design of implantable devices for therapeutic drug delivery.

DESSERT, FRESH FROM THE OVEN

Everyone enjoys the aroma of fresh-baked cookies, even astronauts. On future long-duration space missions, fresh-baked food could have psychological and physiological benefits for crew members, providing them with a greater variety of more nutritious meals. The Zero-G Oven experiment examines heat transfer properties and the process of baking food in microgravity.

Want to learn about more investigations heading to the space station (or even ones currently under way)? Make sure to follow @ISS_Research on Twitter and Space Station Research and Technology News on Facebook. 

If you want to see the International Space Station with your own eyes, check out Spot the Station to see it pass over your town.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.

Eclipse 2017 From Space

On Aug. 21, 2017, a total solar eclipse passed over North America. People throughout the continent captured incredible images of this celestial phenomenon. We and our partner agencies had a unique vantage point on the eclipse from space. Here are a few highlights from our fleet of satellites that observe the Sun, the Moon and Earth.

Our Solar Dynamics Observatory, or SDO, which watches the Sun nearly 24/7 from its orbit 3,000 miles above Earth, saw a partial eclipse on Aug. 21.

SDO sees the Moon cross in front of the Sun several times a year. However, these lunar transits don’t usually correspond to an eclipse here on Earth, and an eclipse on the ground doesn’t guarantee that SDO will see anything out of the ordinary. In this case, on Aug. 21, SDO did see the Moon briefly pass in front of the Sun at the same time that the Moon’s shadow passed over the eastern United States. From its view in space, SDO only saw 14 percent of the Sun blocked by the Moon, while most U.S. residents saw 60 percent blockage or more.

Six people saw the eclipse from the International Space Station. Viewing the eclipse from orbit were NASA’s Randy Bresnik, Jack Fischer and Peggy Whitson, the European Space Agency’s Paolo Nespoli, and Roscosmos’ Commander Fyodor Yurchikhin and Sergey Ryazanskiy. The space station crossed the path of the eclipse three times as it orbited above the continental United States at an altitude of 250 miles.

From a million miles out in space, our Earth Polychromatic Imaging Camera, or EPIC, instrument captured 12 natural color images of the Moon’s shadow crossing over North America. EPIC is aboard NOAA’s Deep Space Climate Observatory, or DSCOVR, where it photographs the full sunlit side of Earth every day, giving it a unique view of the shadow from total solar eclipses. EPIC normally takes about 20 to 22 images of Earth per day, so this animation appears to speed up the progression of the eclipse.

A ground-based image of the total solar eclipse – which looks like a gray ring – is superimposed over a red-toned image of the Sun’s atmosphere, called the corona. This view of the corona was captured by the European Space Agency and our Solar and Heliospheric Observatory, or SOHO. At center is an orange-toned image of the Sun’s surface as seen by our Solar Dynamics Observatory in extreme ultraviolet wavelengths of light.

During a total solar eclipse, ground-based telescopes can observe the lowest part of the solar corona in a way that can’t be done at any other time, as the Sun’s dim corona is normally obscured by the Sun’s bright light. The structure in the ground-based corona image — defined by giant magnetic fields sweeping out from the Sun’s surface — can clearly be seen extending into the outer image from the space-based telescope. The more scientists understand about the lower corona, the more they can understand what causes the constant outward stream of material called the solar wind, as well as occasional giant eruptions called coronal mass ejections.

As millions of Americans watched the total solar eclipse that crossed the continental United States, the international Hinode solar observation satellite captured its own images of the awe-inspiring natural phenomenon. The images were taken with Hinode's X-ray telescope, or XRT, as it flew above the Pacific Ocean, off the west coast of the United States, at an altitude of approximately 422 miles. Hinode is a joint endeavor by the Japan Aerospace Exploration Agency, the National Astronomical Observatory of Japan, the European Space Agency, the United Kingdom Space Agency and NASA.

During the total solar eclipse our Lunar Reconnaissance Orbiter, or LRO, in orbit around the Moon, turned one of its instruments towards Earth to capture an image of the Moon’s shadow over a large region of the United States.

As LRO crossed the lunar south pole heading north at 3,579 mph, the shadow of the Moon was racing across the United States at 1,500 mph. A few minutes later, LRO began a slow 180-degree turn to look back at Earth, capturing an image of the eclipse very near the location where totality lasted the longest. The spacecraft’s Narrow Angle Camera began scanning Earth at 2:25:30 p.m. EDT and completed the image 18 seconds later.

Sensors on the polar-orbiting Terra and Suomi NPP satellites gathered data and imagery in swaths thousands of miles wide. The Moderate Resolution Imaging Spectroradiometer, or MODIS, sensor on Terra and Visible Infrared Imaging Radiometer Suite, or VIIRS, on Suomi NPP captured the data used to make this animation that alternates between two mosaics. Each mosaic is made with data from different overpasses that was collected at different times.

This full-disk geocolor image from NOAA/NASA’s GOES-16 shows the shadow of the Moon covering a large portion of the northwestern U.S. during the eclipse.

Our Interface Region Imaging Spectrograph, or IRIS, mission captured this view of the Moon passing in front of the Sun on Aug. 21.  

Check out nasa.gov/eclipse to learn more about the Aug. 21, 2017, eclipse along with future eclipses, and follow us on Twitter for more satellite images like these: @NASASun, @NASAMoon, and @NASAEarth.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.

OMG! Ice is Melting from Below

Oceans Melting Greenland (OMG) scientists are heading into the field this week to better understand how seawater is melting Greenland’s ice from below. (Yes, those black specks are people next to an iceberg.) While NASA is studying ocean properties (things like temperature, salinity and currents), other researchers are eager to incorporate our data into their work. In fact, University of Washington scientists are using OMG data to study narwhals – smallish whales with long tusks – otherwise known as the “unicorns of the sea.”

 Our researchers are also in the field right now studying how Alaska’s ice is changing. Operation IceBridge, our longest airborne campaign, is using science instruments on airplanes to study and measure the ice below.

What happens in the Arctic doesn’t stay in the Arctic (or the Antarctic, really). In a warming world, the greatest changes are seen in the coldest places. Earth’s cryosphere – its ice sheets, sea ice, glaciers, permafrost and snow cover – acts as our planet’s thermostat and deep freeze, regulating temperatures and storing most of our freshwater. Next month, we’re launching ICESat-2, our latest satellite to study Earth’s ice!

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.

Our Asteroid-Bound Mission is Set to Slingshot Around Earth

NASA’s first spacecraft to travel to an asteroid will get a boost from Earth tomorrow, Sept. 22. 

Earth's gravity is going to slingshot OSIRIS-REx toward its target, an asteroid named Bennu.

Asteroids are relatively small, inactive, rocky bodies that orbit around the Sun. Scientists think asteroids like Bennu may have collided with Earth a long time ago, seeding our planet with the organic compounds that made life possible. That means that there's a good chance Bennu contains answers to fundamental questions about the origins of life and how our solar system came to be. We sent OSIRIS-REx on a journey to investigate.

One of the best ways to change the trajectory of a spacecraft is by using the gravity of a planet or large moon to catapult it. It sounds like science fiction, but this type of maneuver, called a gravity assist, is a fuel-efficient way of traveling through space.

We’re not using the slingshot to speed the spacecraft, we’re doing it to change its direction. That’s because the asteroid’s orbit is tilted six degrees in comparison to Earth's orbit. When OSIRIS-REx swings by, Earth's gravity will lift it up and sling it toward Bennu.

Spot the spacecraft

Because at its closest approach OSIRIS-REx will only be 11,000 miles above Earth, you can see it with a backyard telescope. For most observers, the spacecraft will appear between the constellations Cetus and Pisces, but its exact position in the sky will vary by location.

For specifics on locating and photographing OSIRIS-REx, visit our Spot the Spacecraft page.

Wave to OSIRIS-REx

After its closest approach, OSIRIS-REx flip around and look back at Earth, so here's your chance to say hello! Take a picture of yourself or your group waving to OSIRIS-REx. Then share your photo using the hashtag #HelloOSIRISREx and tag the mission account on Twitter @OSIRISREx or Instagram @OSIRIS_REx.

To Bennu and back

In about a year from now, OSIRIS-REx will arrive at asteroid Bennu.

After it surveys and maps Bennu, OSIRIS-REx will "high-five" the asteroid with its robotic arm to collect a sample, which it will send to Earth. This asteroid sample will be the largest amount of space material transported to Earth since we brought back rocks from the Moon. High-fives all around!

If everything goes according to plan, on Sept. 24, 2023, the capsule containing the asteroid sample will make a soft landing in the Utah desert. That’s the end of the spacecraft’s seven-year-long journey to Bennu and back.

But the mission doesn't stop there. On Earth, the sample material collected by OSIRIS-REx will be analyzed to determine the asteroid's chemical composition. Scientists will look for organic compounds like amino acids and sugars — the building blocks for life. 

Bennu is approximately 4.5 billion years old. Our solar system is 4.6 billion years old. That means that Bennu is made up of some of the oldest stuff in our solar system. So samples from Bennu could tell us more about how our solar system evolved and possibly even how life began on Earth! Learn more about asteroid Bennu, the OSIRIS-REx mission and the Earth gravity assist. 

Follow the mission on Facebook and Twitter for the latest updates. 

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.

Solar System: Things to Know This Week

We've been up close and personal with Saturn for 13 years now, thanks to the Cassini mission. 

From a tour of Saturn's many enthralling moons to an incredible view of Earth through its rings, the planet continues to captivate the imagination. This week, here are 10 things you need to know about our fascinating ringed neighbor.

1. Strange Sighting

When Galileo Galilei was observing Saturn in the 1600s, he noticed strange objects on each side of the planet. He drew in his notes a triple-bodied planet system with ears. These "ears" were later discovered to be the rings of Saturn.

2. Solar System Status

Saturn orbits our sun and is the sixth planet from the sun at an average distance of about 886 million miles or 9.5 AU.

3. Short Days

Time flies when you're on Saturn. One day on Saturn takes just 10.7 hours (the time it takes for Saturn to rotate or spin once). The planet makes a complete orbit around the sun (a year in Saturnian time) in 29 Earth years, or 10,756 Earth days. saturn.jpl.nasa.gov/news/2955/measuring-a-day

4. No Shoes Necessary

That's because you can't stand on Saturn—it's a gas-giant planet and doesn't have a solid surface. But you might want a jacket. The planet's temperatures can dip to -220 degrees F.

5. Few visitors

Only a handful of missions have made their way to Saturn: Pioneer 11, Voyager 1 and 2, and Cassini-Huygens, which is there now. Since 2004, Cassini has been exploring Saturn and its moons and rings—but will complete its journey on Sept. 15, 2017.

6. Saturn's Close-Up

This month is a great time to observe Saturn from Earth. Check out June's "What's Up?" video for a how-to guide.

7. Daring Dives

Saturn's spectacular ring system is made up of seven rings with several gaps and divisions between them. From now until September, the Cassini spacecraft is performing a set of daring dives every week between the planet and the rings. No other mission has ever explored this unique region before, and what we learn from these final orbits will help us understand of how giant planets—and planetary systems everywhere—form and evolve.

8. Many, Many Moons 

Saturn has a total of 62 moons: 53 known moons, with an additional nine moons awaiting confirmation.

9. Curious Shapes 

Saturn's moon Atlas looks like a flying saucer. See for yourself.

10. Would You Live on a Moon? 

Saturn can't support life as we know it, but some of its moons have conditions that might support life. Ocean worlds could be the answer to life in space and two of Saturn's moons—Titan and Enceladus—are on that list.

Want to learn more? Read our full list of the 10 things to know this week about the solar system HERE.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com

NASA Day of Remembrance

Every year at this time, we take a moment to reflect as the NASA Family on the very broad shoulders on which we stand: the shoulders of those women and men of NASA who gave their lives so that we could continue to reach for new heights for the benefit of all humankind.

To honor our fallen heroes and friends, NASA Administrator Charles Bolden and Deputy Administrator Dava Newman spoke at a wreath-laying ceremony at Arlington National Cemetery, at the grave sites of the fallen crew.

The crew aboard the International Space Station also payed tribute with a moment of silence. 

President Barack Obama recognized the day with the release of an official statement that honors the legacy of the heroes who lost their lives helping America touch the stars.

To view the President’s full statement, visit HERE. 

Visit our Day of Remembrance page to learn about the crews & missions we've lost: http://www.nasa.gov/externalflash/DOR2016/index.html

Thank you for keeping our fallen colleagues in your hearts and for honoring their legacy.

Stars Make Firework Supplies!

The next time you see fireworks, take a moment to celebrate the cosmic pyrotechnics that made them possible. From the oxygen and potassium that help fireworks burn to the aluminum that makes sparklers sparkle, most of the elements in the universe wouldn’t be here without stars.

From the time the universe was only a few minutes old until it was about 400 million years old, the cosmos was made of just hydrogen, helium and a teensy bit of lithium. It took some stellar activity to produce the rest of the elements!

Stars are element factories

Even after more than 13 billion years, the hydrogen and helium that formed soon after the big bang still make up over 90 percent of the atoms in the cosmos. Most of the other elements come from stars.

Stars began popping into the universe about 400 million years after the big bang. That sounds like a long time, but it’s only about 3% of the universe’s current age!

Our Nancy Grace Roman Space Telescope will study the universe’s early days to help us learn more about how we went from a hot, soupy sea of atoms to the bigger cosmic structures we see today. We know hydrogen and helium atoms gravitated together to form stars, where atoms could fuse together to make new elements, but we're not sure when it began happening. Roman will help us find out.

The central parts of atoms, called nuclei, are super antisocial – it takes a lot of heat and pressure to force them close together. Strong gravity in the fiery cores of the first stars provided just the right conditions for hydrogen and helium atoms to combine to form more elements and generate energy. The same process continues today in stars like our Sun and provides some special firework supplies.

Carbon makes fireworks explode, helps launch them into the sky, and is even an ingredient in the “black snakes” that seem to grow out of tiny pellets. Fireworks glow pink with help from the element lithium. Both of these elements are created by average, Sun-like stars as they cycle from normal stars to red giants to white dwarfs.

Eventually stars release their elements into the cosmos, where they can be recycled into later generations of stars and planets. Sometimes they encounter cosmic rays, which are nuclei that have been boosted to high speed by the most energetic events in the universe. When cosmic rays collide with atoms, the impact can break them apart, forming simpler elements. That’s how we get boron, which can make fireworks green, and beryllium, which can make them silver or white!

Since massive stars have even stronger gravity in their cores, they can fuse more elements – all the way up to iron. (The process stops there because instead of producing energy, fusing iron is so hard to do that it uses up energy.)

That means the sodium that makes fireworks yellow, the aluminum that produces silver sparks (like in sparklers), and even the oxygen that helps fireworks ignite were all first made in stars, too! A lot of these more complex elements that we take for granted are actually pretty rare throughout the cosmos, adding up to less than 10 percent of the atoms in the universe combined!

Fusion in stars only got us through iron on the periodic table, so where do the rest of our elements come from? It’s what happens next in massive stars that produces some of the even more exotic elements.

Dying stars make elements too!

Once a star many times the Sun’s mass burns through its fuel, gravity is no longer held in check, and its core collapses under its own weight. There, atoms are crushed extremely close together – and they don’t like that! Eventually it reaches a breaking point and the star explodes as a brilliant supernova. Talk about fireworks! These exploding stars make elements like copper, which makes fireworks blue, and zinc, which creates a smoky effect.

Something similar can happen when a white dwarf star – the small, dense core left behind after a Sun-like star runs out of fuel – steals material from a neighboring star. These white dwarfs can explode as supernovae too, spewing elements like the calcium that makes fireworks orange into the cosmos.

When stars collide

White dwarfs aren’t the only “dead” stars that can shower their surroundings with new elements. Stars that are too massive to leave behind white dwarfs but not massive enough to create black holes end up as neutron stars.

If two of these extremely dense stellar skeletons collide, they can produce all kinds of elements, including the barium that makes fireworks bright green and the antimony that creates a glitter effect. Reading this on a phone or computer? You can thank crashing dead stars for some of the metals that make up your device, too!

As for most of the remaining elements we know of, we've only seen them in labs on Earth so far.

Sounds like we’ve got it all figured out, right? But there are still lots of open questions. Our Roman Space Telescope will help us learn more about how elements were created and distributed throughout galaxies. That’s important because the right materials had to come together to form the air we breathe, our bodies, the planet we live on, and yes – even fireworks!

So when you’re watching fireworks, think about their cosmic origins!

Learn more about the Roman Space Telescope at: https://roman.gsfc.nasa.gov/

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com

@tinyscoop: What's the strangest experiment you've ever had to carry out up there?

Is there any other way to actually look at the eclipse (besides television/streams) without using the special eclipse glasses?

Unfortunately, you can not directly look at the eclipse without the proper eye protection https://eclipse2017.nasa.gov/safety. But there are lots of fun indirect methods that you can use. The GIF shows how you can make a pin hole projector with your hands. We also have patterns for 3D printers to make your own pin hole projector in the shape of the US or your state https://eclipse2017.nasa.gov/2d3d-printable-pinhole-projectors