What You Need To Know About Our Space Launch System (SLS) Rocket’s Green Run Test

What is the scariest part of your job?

I love my job, and I think the scariest thing for me is making a mistake. So I work hard to learn everything I can to avoid making mistakes and be as methodical as I can to avoid that.

Solar System: Things to Know This Week

Our solar system is huge, let us break it down for you. Here are a few things to know this week:

1. The New New Horizons

Seven months after the  Pluto flyby, information and discoveries continue to flow from the New Horizons mission, as the spacecraft transmits more and more data to scientists on Earth.

2. A Longlasting Dawn

The Dawn orbiter is in good health as it carries out the ongoing reconnaissance of the dwarf planet Ceres, which is revealing some spectacular and mysterious landscapes.

3. Storm Watch: Saturn

This week the Cassini spacecraft will be watching for storms in Saturn’s turbulent atmosphere. On March 6, it will spend about 14 hours acquiring a movie of the narrow, braided F ring. Check out some past photos of Saturnian storms HERE.

4. The Next Flight to Mars Departs Soon

The ExoMars 2016 mission, a joint endeavor between the European Space Agency and the Russian space agency Roscosmos, is set to lift off in March. The 2016 mission consists of the Trace Gas Orbiter and the Schiaparelli Entry, Descent and Landing Demonstrator Module. We’re supplying some of the technology that will fly aboard the orbiter. In 2018, the ExoMars rover is slated to follow.

5. Early Encounter with a Comet

As we continue to marvel at the latest images from Rosetta, this week is a good time to remember the 30th anniversary of the Vega 1 Comet Halley flyby. This Russian spacecraft dropped off a balloon probe at Venus before continuing on to the comet, which is photographed and examined at close range by flying through its coma.

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

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Go Behind-the-Scenes at NASA

Are you active on social media? Want to go behind-the-scenes at NASA and meet our scientists, engineers, astronauts and managers? Want to see and feel a rocket launch in-person? Then you would love our NASA Social events!

A NASA Social is a program that provides opportunities for our social media followers (like you!) to learn and share information about our missions, people and programs. Formerly known as NASA Tweetups, these socials include both special in-person events and social media credentials for people who share the news in a significant way. To date, this program has brought thousands of people together for unique social media experiences of exploration and discovery.

NASA Socials range from two hours to two days in length and include a “meet and greet” session to allow participants to mingle with fellow socialites and the people behind our social media accounts. The participants are selected from those who register their interest for the event on the web.

Do you need to have a social media account to register for a NASA Social? 

Yes. The socials are designed for social media users who follow @NASA on a variety of platforms. The goal of NASA Socials is to allow people who regularly interact with each other via these platforms to meet in person and discuss one of their favorite subjects: NASA!

What types of events have we hosted in the past? Take a look:

Participants for a NASA Social surrounding the launch of a SpaceX cargo vehicle to the International Space Station met with former Deputy Administrator Lori Garver underneath the engines of the Saturn V rocket.

A participant at a NASA Social in Washington tweets as he listens to astronaut Joe Acaba answer questions about his time living aboard the International Space Station.

Juno launch Tweetup participants pose for a group photo with NASA Administrator Charles Bolden with the Vehicle Assembly Building (VAB) in the background at Kennedy Space Center.

And of course, some of our NASA Socials culminate with a rocket launch! You can experience one in-person. Apply to attend a once in a lifetime experience. 

For more information about NASA Social events, and to see upcoming opportunities, visit: http://www.nasa.gov/social

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Three Ways to Travel at (Nearly) the Speed of Light

One hundred years ago, Einstein’s theory of general relativity was supported by the results of a solar eclipse experiment. Even before that, Einstein had developed the theory of special relativity — a way of understanding how light travels through space.

Particles of light — photons — travel through a vacuum at a constant pace of more than 670 million miles per hour.

All across space, from black holes to our near-Earth environment, particles are being accelerated to incredible speeds — some even reaching 99.9% the speed of light! By studying these super fast particles, we can learn more about our galactic neighborhood. 

Here are three ways particles can accelerate:

1) Electromagnetic Fields!

Electromagnetic fields are the same forces that keep magnets on your fridge! The two components — electric and magnetic fields — work together to whisk particles at super fast speeds throughout the universe. In the right conditions, electromagnetic fields can accelerate particles at near-light-speed.

We can harness electric fields to accelerate particles to similar speeds on Earth! Particle accelerators, like the Large Hadron Collider and Fermilab, use pulsed electromagnetic fields to smash together particles and produce collisions with immense amounts of energy. These experiments help scientists understand the Big Bang and how it shaped the universe!

2) Magnetic Explosions!

Magnetic fields are everywhere in space, encircling Earth and spanning the solar system. When these magnetic fields run into each other, they can become tangled. When the tension between the crossed lines becomes too great, the lines explosively snap and realign in a process known as magnetic reconnection. Scientists suspect this is one way that particles — for example, the solar wind, which is the constant stream of charged particles from the Sun — are sped up to super fast speeds.

When magnetic reconnection occurs on the side of Earth facing away from the Sun, the particles can be hurled into Earth’s upper atmosphere where they spark the auroras.

3) Wave-Particle Interactions!

Particles can be accelerated by interactions with electromagnetic waves, called wave-particle interactions. When electromagnetic waves collide, their fields can become compressed. Charged particles bounce back and forth between the waves, like a ball bouncing between two merging walls. These types of interactions are constantly occurring in near-Earth space and are responsible for damaging electronics on spacecraft and satellites in space.

Wave-particle interactions might also be responsible for accelerating some cosmic rays from outside our solar system. After a supernova explosion, a hot, dense shell of compressed gas called a blast wave is ejected away from the stellar core. Wave-particle interactions in these bubbles can launch high-energy cosmic rays at 99.6% the speed of light.

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

NASA Communications and Navigation in 2021: Top 10 Iconic Moments

Did you know NASA uses global networks of antennas and relay satellites to talk with astronauts and spacecraft?

Our space communications and navigation community has had an incredible year! From supporting science and exploration missions to developing cutting-edge tech, here are some of the team’s most impactful accomplishments of 2021.

1. We launched a revolutionary tech demo, the Laser Communications Relay Demonstration, which will showcase the benefits of using infrared laser links to send data from space. Laser communications systems can offer 10 to 100 times more data per second than traditional radio! You can learn more about the mission in a new season of our podcast, The Invisible Network.

2. Planetary radars observed their 1,000th near-Earth asteroid since 1968! Our Deep Space Network plays a critical role in detecting near-Earth asteroids, using radar to spot them. These radar detections help definitively predict if an asteroid is going to hit Earth, or if it’s just going to pass close by.

3. We used lessons learned developing communications services for the Moon to address digital inequality on Earth. Folks at our Glenn Research Center in Cleveland examined how lunar network approaches could address technical challenges to Wi-Fi connectivity in their local community.

4. Our Search and Rescue office participated in dress rehearsals for the Artemis I mission to the Moon! They tested critical distress technologies that will help locate Artemis astronauts in the unlikely event they need to leave the Orion capsule and enter open water before recovery teams can reach them.

5. With high international participation, we hosted a virtual workshop on cognitive communications at our Glenn Research Center in Cleveland, Ohio. Cognitive communications employs artificial intelligence and machine learning in radio systems to provide a host of benefits to user missions!

6. We celebrated the 100th birthday of the creator of Star Trek, the late Gene Roddenberry. The event featured Roddenberry’s son Rod, NASA administrator Bill Nelson, and Star Trek actor George Takei. Following the program, our Deep Space Network broadcast Gene’s 1976 remarks on diversity and inclusion toward star system 40 Eridani — home to the planet Vulcan in Star Trek lore. Signals from the broadcast will arrive there in 16.5 years.

7. We worked with the aerospace community to refine our LunaNet architecture for lunar communications and navigation services! LunaNet will leverage innovative networking techniques, standards, and an extensible framework to rapidly expand network capabilities at the Moon for Artemis. This framework will allow industry, academia, and international partners to build and operate LunaNet nodes alongside us.

8. Our Deep Space Network welcomed a brand new satellite dish into the family! Called Deep Space Station 56, or DSS-56, the 112-foot-wide (34-meter) dish is now online and ready to communicate for a variety of uses, including missions at the Moon and Mars.

9. Our Near Space Network engaged with over 200 commercial aerospace companies! They’re working toward a new paradigm where NASA missions near Earth can rely on a blend of government and commercial space communications infrastructure to meet their needs.

10. Our 10th item on the list isn’t a single moment, but the continued support our communications networks provided missions throughout 2021. Whether it was a Commercial Crew mission to the International Space Station or the Perseverance Rover’s touchdown on Mars, our Near Space Network and Deep Space Network were there to empower mission success! Make sure to follow us on Tumblr for your regular dose of space!

It was a dark and stormy flyby... ⁣⁣

Our @NASAJuno spacecraft's JunoCam captured images of the chaotic, stormy northern hemisphere of Jupiter during its 24th close pass of the giant planet on Dec. 26, 2019. Using data from the flyby, citizen scientist Kevin M. Gill created this color-enhanced image. At the time, the spacecraft was about 14,600 miles (23,500 kilometers) from the tops of Jupiter’s clouds, at a latitude of about 69 degrees north.⁣

Image Credit: Image data: NASA/JPL-Caltech/SwRI/MSSS⁣

Image processing by Kevin M. Gill, © CC BY⁣

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That's one small bite for a man, one giant leaf for mankind: Today, astronauts Scott Kelly, Kjell Lindgren and Kimiya Yui of Japan sample the fruits of their labor after harvesting a crop of "Outredgeous" red romaine lettuce from the Veggie plant growth system on the International Space Station. They are the first people to eat food grown in space.

We’re maturing Veggie technology aboard the space station to provide future pioneers with a sustainable food supplement – a critical part of our Journey to Mars. As we move toward long-duration exploration missions farther into the solar system, Veggie will be a resource for crew food growth and consumption. It also could be used by astronauts for recreational gardening activities during deep space missions. 

10 Things to Know: Massive Dust Storm on Mars

Massive Martian dust storms have been challenging—and enticing—scientists for decades. Here’s the scoop on Martian dust:

1: Challenging Opportunity

Our Opportunity rover is facing one of the greatest challenges of its 14 ½ year mission on the surface of Mars--a massive dust storm that has turned day to night. Opportunity is currently hunkered down on Mars near the center of a storm bigger than North America and Russia combined. The dust-induced darkness means the solar-powered rover can’t recharge its batteries.

2: One Tough Robot

This isn’t the first time Opportunity has had to wait out a massive storm. In 2007, a monthlong series of severe storms filled the Martian skies with dust. Power levels reached critical lows, but engineers nursed the rover back to health when sunlight returned.

3: Windswept

Martian breezes proved a saving grace for the solar-powered Mars rovers in the past, sweeping away accumulated dust and enabling rovers to recharge and get back to science. This is Opportunity in 2014. The image on the left is from January 2014. The image on the right in March 2014.

4: Dusty Disappointment

Back in 1971, scientists were eager for their first orbital views of Mars. But when Mariner 9 arrived in orbit, the Red Planet was engulfed by a global dust storm that hid most of the surface for a month. When the dust settled, geologists got detailed views of the Martian surface, including the first glimpses of ancient riverbeds carved into the dry and dusty landscape.

5: Dramatic License

As bad as the massive storm sounds, Mars isn’t capable of generating the strong winds that stranded actor Matt Damon’s character on the Red Planet in the movie The Martian. Mars’ atmosphere is too thin and winds are more breezy than brutal. The chore of cleaning dusty solar panels to maintain power levels, however, could be a very real job for future human explorers.

6: Semi-Regular Visitors

Scientists know to expect big dust storms on Mars, but the rapid development of the current one is surprising. Decades of Mars observations show a pattern of regional dust storms arising in northern spring and summer. In most Martian years, nearly twice as long as Earth years, the storms dissipate. But we’ve seen global dust storms in 1971, 1977, 1982, 1994, 2001 and 2007. The current storm season could last into 2019.

7: Science in the Dust

Dust is hard on machines, but can be a boon to science. A study of the 2007 storm published earlier this year suggests such storms play a role in the ongoing process of gas escaping from the top of Mars' atmosphere. That process long ago transformed wetter, warmer ancient Mars into today's arid, frozen planet. Three of our orbiters, the Curiosity rover and international partners are already in position to study the 2018 storm.

8: Adjusting InSight

Mission controllers for Mars InSight lander--due to land on Mars in November--will be closely monitoring the storm in case the spacecraft’s landing parameters need to be adjusted for safety. 

Once on the Red Planet, InSight will use sophisticated geophysical instruments to delve deep beneath the surface of Mars, detecting the fingerprints of the processes of terrestrial planet formation, as well as measuring the planet's "vital signs": Its "pulse" (seismology), "temperature" (heat flow probe), and "reflexes" (precision tracking).

9: Martian Weather Report

One saving grace of dust storms is that they can actually limit the extreme temperature swings experienced on the Martian surface. The same swirling dust that blocks out sunlight also absorbs heat, raising the ambient temperature surrounding Opportunity.

Track the storm and check the weather on Mars anytime.

10: Dust: Not Just a Martian Thing

A dust storm in the Sahara can change the skies in Miami and temperatures in the North Atlantic. Earth scientists keep close watch on our home planet’s dust storms, which can darken skies and alter Earth’s climate patterns.

Read the full web version of this article HERE. 

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Our Planet: 8 Stunning Views of Earth from Space

Swirling clouds, deep blue oceans and textured land- and icescapes are among the many faces of our planet revealed in NASA’s new photo-essay book: Earth. This collection of 69 images captured by satellites tells a story of a 4.5-billion-year-old planet where there is always something new to see. Earth is a beautiful, awe-inspiring place, and it is the only world most of us will ever know. It is your planet. It is NASA’s mission. The book is available now in hardcover and ebook, and online with interactive features.

Here are eight of those breathtaking images for your viewing pleasure. 

Channel Country, Australia

These wide floodplains in Queensland, Australia are unique on the planet. Scientists think they are caused by the extreme variation in water and sediment discharges from the rivers. In many years there is no rainfall at all, and the rivers are effectively non-existent. In years of modest rainfall, the main channels will carry some water, sometimes spilling over into narrow water holes known as billabongs.

Every few decades, the floodplain carries extremely high discharges of water. For instance, tropical storms to the north can lead to great water flows that inundate the entire width of the floodplain. On such occasions, the floodplain appears as series of brown and green water surfaces with only tree tops indicating the location of the islands. Such is the case in this image taken from the International Space Station in September 2016.

Grounded in the Caspian, Kazakhstan

A wide variety of ice forms in the Caspian Sea, which stretches from Kazakhstan to Iran. Just offshore, a well-developed expanse of consolidated ice appears bright white. Farther offshore, a gray-white field of chunky, hummocked ice has detached and is slowly drifting around a polynya, an area of open water surrounded by sea ice. That darker patch is actually growing young, thin ice and nilas, a term that designates sea ice crust up to 10 centimeters (4 inches) in thickness.

The close-up shows nilas and a white, diamond-shaped piece of ice. It might look like this chunk is on the move, cutting a path through thinner ice. But it’s more likely that the “diamond” was stuck to the sea bottom and the wind pushed ice around it.

Tsauchab River Bed, Namibia

The Tsauchab River is a famous landmark for the people of Namibia and tourists. Yet few people have ever seen the river flowing with water. In December 2009, an astronaut on the International Space Station caught this glimpse of the Tsauchab River bed jutting into the sea of red dunes. It ends in a series of light-colored, silty mud holes on the dry lake floor.

Like several other rivers around the Namib Desert, the Tsauchab brings sediment down from the hinterland toward the coastal lowland. This sediment is then blown from the river beds, and over tens of millions of years it has accumulated as the red dunes of the Namib Sand Sea.

Taranaki and Egmont, New Zealand

The circular pattern of New Zealand’s Egmont National Park stands out from space as a human fingerprint on the landscape. The park protects the forested and snow-capped slopes around Mount Taranaki (Mount Egmont to British settlers). It was established in 1900, when officials drew a radius of 10 kilometers around the volcanic peak. The colors differentiate the protected forest (dark green) from once-forested pasturelands (light- and brown-green).

Named by the native Maori people, Taranaki stands 2,518 meters (8,260 feet) tall, and it is one of the world’s most symmetric volcanoes. It first became active about 135,000 years ago. By dating lava flows, geologists have figured out that small eruptions occur roughly every 90 years and major eruptions every 500 years. Landsat 8 acquired this image of Taranaki and the park in July 2014.

Storms Stir Up Sediment in Bermuda

In October 2014, the eye of Hurricane Gonzalo passed right over Bermuda. In the process, the potent storm stirred up the sediments in the shallow bays and lagoons around the island, spreading a huge mass of sediment across the North Atlantic Ocean. This Landsat 8 image shows the area after Gonzalo passed through.

The suspended sediments were likely a combination of beach sand and carbonate sediments from around the shallows and reefs. Coral reefs can produce large amounts of calcium carbonate, which stays on the reef flats (where there are coralline algae that also produce carbonate) and builds up over time to form islands.

Framing an Iceberg in the South Atlantic Ocean

In June 2016, the Suomi NPP satellite captured this image of various cloud formations in the South Atlantic Ocean. Note how low stratus clouds framed a hole over iceberg A-56 as it drifted across the sea.

The exact reason for the hole in the clouds is somewhat of a mystery. It could have formed by chance, although imagery from the days before and after this date suggest something else was at work. It could be that the relatively unobstructed path of the clouds over the ocean surface was interrupted by thermal instability created by the iceberg. In other words, if an obstacle is big enough, it can divert the low-level atmospheric flow of air around it, a phenomenon often caused by islands.

Lofted Over Land in Madagascar

Along the muddy Mania River, midday clouds form over the forested land but not the water. In the tropical rainforests of Madagascar, there is ample moisture for cloud formation. Sunlight heats the land all day, warming that moist air and causing it to rise high into the atmosphere until it cools and condenses into water droplets. Clouds generally form where air is ascending (over land in this case), but not where it is descending (over the river). Landsat 8 acquired this image in January 2015.

A Lava Lamp Look at the Atlantic Ocean 

Stretching from tropical Florida to the doorstep of Europe, the Gulf Stream carries a lot of heat, salt, and history. This river of water is an important part of the global ocean conveyor belt, moving water and heat from the Equator toward the far North Atlantic. It is one of the strongest currents on Earth and one of the most studied. Its discovery is often attributed to Benjamin Franklin, though sailors likely knew about the current long before they had a name for it.

This image shows a small portion of the Gulf Stream off of South Carolina as it appeared in infrared data collected by the Landsat 8 satellite in April 2013. Colors represent the energy—heat—being emitted by the water, with cooler temperatures in purple and the warmest water being nearly white. Note how the Gulf Stream is not a uniform band but instead has finer streams and pockets of warmer and colder water.

These images are just a few from our new book called Earth. Explore the other 61 images here.

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What was the hardest part in training to go to space?

One of the most challenging parts of space training was learning how to use the space suit.  We weigh over 400 pounds in the space suit, and since it is pressurized, each movement of your hands is like working against an exercise ball.  Since the suit needs to be quite bulky in order to protect us from the environment of space (vacuum, radiation, micrometeoroids, extreme temperature) while doing a spacewalk, it makes body movements a bit awkward.  Dexterity is quite compromised with the bulky gloves as well.  Although it is challenging, however, it is likely also the most rewarding, because, well, you are in a SPACE SUIT!!!  Hopefully I’ll get to do a spacewalk and look down on the our planet from above on a mission to the International Space Station in a few years.