Being a good friend doesn’t mean you always have all the right words to say. Sometimes it means you just know when to be a good listener.
Katrina Mayer (via quotemadness)
Later this month, a SpaceX Falcon Heavy rocket will take to the skies for the third time to launch the Department of Defense’s Space Test Program-2 (STP-2) mission. Several exciting, one-of-a-kind NASA technology and science payloads are among the two-dozen spacecraft aboard.
First, let’s talk about that Falcon Heavy rocket. Its 27 engines generate thrust at liftoff equal to that of approximately 18 airplanes, and it can lift over 140,000 pounds.
Managed by the U.S. Air Force Space and Missile Systems Center, STP-2 is the first government-contracted Falcon Heavy launch. It will reuse the two side boosters recovered after the April flight. SpaceX describes it as one of the most challenging launches in the company’s history.
It’s a big deal to us at NASA because we’re launching some pretty cool technologies. The tech will support our future exploration plans by helping improve future spacecraft design and performance. Here’s a bit about each:
Time is the heartbeat of space navigation. Today, we navigate in deep space by using giant antennas on Earth to send signals to spacecraft, which then send those signals back to Earth. Atomic clocks on Earth measure the time it takes a signal to make this two-way journey. Only then can human navigators on Earth use large antennas to tell the spacecraft where it is and where to go.
Our Jet Propulsion Laboratory has been perfecting an atomic clock fit for exploration missions. The Deep Space Atomic Clock is the first atomic clock designed to fly on a spacecraft destined for beyond Earth’s orbit. The timepiece is lighter and smaller—no larger than a toaster oven—than its refrigerator-sized, Earthly counterparts.
This miniaturized clock could enable one-way navigation: a spacecraft receives a signal from Earth and can determine its location immediately using its own, built-in navigation system. Even smaller versions of the clock are being investigated right now that could be used for the growing number of small to mid-size satellites. As we go forward to the Moon with the Artemis program, precise measurements of time are key to mission success.
The Deep Space Atomic Clock is the primary payload onboard the General Atomics Electromagnetic Systems Orbital Test Bed satellite and will perform a year-long demonstration in space.
Two tiny satellites will study how signals can be muddled as they travel through hard-to-predict bubbles in the upper atmosphere. Signals sent from satellites down to Earth (and vice versa) can be disrupted by structured bubbles that sometimes form in Earth’s upper atmosphere. Because this region is affected both by weather on Earth and conditions in space, it’s hard to predict just when these bubbles will form or how they’ll mess with signals.
The E-TBEx CubeSats (short for Enhanced Tandem Beacon Experiment) will try to shed some light on that question. As these little satellites fly around Earth, they’ll send radio signals (like the ones used by GPS) to receiving stations on the ground. Scientists will be able to look at the signals received and see if they were jumbled as they traveled through the upper atmosphere down to Earth — which will help us track when these bubbles are forming and how much they’re interfering with our signals.
For decades, we have relied on a highly toxic spacecraft fuel called hydrazine. The Green Propellant Infusion Mission (GPIM) will lay the foundation to replace conventional chemical propulsion systems with a safer and more efficient alternative for next-generation spacecraft.
GPIM will demonstrate a new propellant in space for the first time. Concocted by the U.S. Air Force Research Laboratory, this innovative, “green” fuel—which actually has more of a peach hue—is expected to improve overall spacecraft performance due to its higher density, increased thrust and lower freezing point in comparison with hydrazine.
GPIM’s propulsion system, developed by Aerojet Rocketdyne, consists of new compatible tanks, valves and thrusters. During the two-month-long demonstration on a Ball Aerospace spacecraft, engineers will conduct orbital maneuvers to demonstrate the performance of the propellant and propulsion system.
It’s not easy being a spacecraft; invisible, energetic particles zip throughout space — and while there are so few that space is considered a vacuum, what’s there still packs a punch. Tiny particles — like those seen here impacting a detector on a Sun-studying spacecraft — can wreak havoc with the electronics we send up into space.
Space Environment Testbeds — or SET, for short — is a mission to study space radiation and how it affects spacecraft and electronics in orbit. What looks like snow flurries in these animated images, for example, is actually a solar radiation storm of incredibly fast particles, unleashed by a solar eruption. Energetic particles from the Sun or deep space can spark memory damage or computer upsets on spacecraft, and over time, degrade hardware.
By studying radiation effects and different methods to protect satellites, SET will help future missions improve spacecraft design, engineering and operations.
Follow @NASA_Technology and @NASASun on Twitter for news about the STP-2 launch and our missions aboard.
Check out www.nasa.gov/spacex to stay up-to-date on the launch day and time. Don’t forget to tune into our launch coverage, scheduled to start about 30 minutes before liftoff!
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.
In celebration of the 50th anniversary of Apollo 11, we’ll be sharing answers to some frequently asked questions about the first time humans voyaged to the Moon. Answers have been compiled from archivists in the NASA History Office.
At the height of Apollo in 1965, about 409,900 people worked on some aspect of the program, but that number doesn’t capture it all.
It doesn’t represent the people who worked on mission concepts or spacecraft design, such as the engineers who did the wind tunnel testing of the Apollo Command Module and then moved on to other projects. The number also doesn’t represent the NASA astronauts, mission controllers, remote communications personnel, etc. who would have transferred to the Apollo program only after the end of Gemini program (1966-1967). There were still others who worked on the program only part-time or served on temporary committees. In the image above are three technicians studying an Apollo 14 Moon rock in the Lunar Receiving Laboratory at Johnson Space Center. From left to right, they are Linda Tyler, Nancy Trent and Sandra Richards.
This artwork portrait done by spaceflight historian Ed Hengeveld depicts the 12 people who have walked on the Moon so far. In all, 24 people have flown to the Moon and three of them, John Young, Jim Lovell and Gene Cernan, have made the journey twice.
But these numbers will increase.
Every successful Apollo lunar landing mission left a flag on the Moon but we don’t know yet whether all are still standing. Some flags were set up very close to the Lunar Module and were in the blast radius of its ascent engine, so it’s possible that some of them could have been knocked down. Neil Armstrong and Buzz Aldrin both reported that the flag had been knocked down following their ascent.
Our Lunar Reconnaissance Orbiter took photographs of all the Apollo lunar landing sites. In the case of the Apollo 17 site, you can see the shadow of the upright flag.
The flags appear to “wave” or “flap” but actually they’re swinging. Swinging motions on Earth are dampened due to gravity and air resistance, but on the Moon any swinging motion can continue for much longer. Once the flags settled (and were clear of the ascent stage exhaust), they remained still. And how is the flag hanging? Before launching, workers on the ground had attached a horizontal rod to the top of each flag for support, allowing it to be visible in pictures and television broadcasts to the American public. Armstrong and Aldrin did not fully extend the rod once they were on the Moon, giving the flag a ripple effect. The other astronauts liked the ripple effect so much that they also did not completely extend the rod.
Have you ever taken a photo of the night sky with your phone or camera? You likely won’t see any stars because chances are your camera’s settings are set to short exposure time only lets it quickly take in the light off the bright objects closest to you. It’s the same reason you generally don’t see stars in spacewalk pictures from the International Space Station. There’s no use for longer exposure times to get an image like this one of Bruce McCandless in 1984 as seen Space Shuttle Challenger (STS-41B).
The Hasselblad cameras that Apollo astronauts flew with were almost always set to short exposure times. And why didn’t the astronauts photograph the stars? Well, they were busy exploring the Moon!
The first giant leap was only the beginning. Work is under way to send the first woman and the next man to the Moon in five years. As we prepare to launch the next era of exploration, the new Artemis program is the first step in humanity’s presence on the the Moon and beyond.
Keep checking back for more answers to Apollo FAQs.
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May the force be with you? Much to learn you still have, padawan. In our universe it would be more appropriate to say, “May the four forces be with you.”
There are four fundamental forces that bind our universe and its building blocks together. Two of them are easy to spot — gravity keeps your feet on the ground while electromagnetism keeps your devices running. The other two are a little harder to see directly in everyday life, but without them, our universe would look a lot different!
Let’s explore these forces in a little more detail.
If you jump up, gravity brings you back down to Earth. It also keeps the solar system together … and our galaxy, and our local group of galaxies and our supercluster of galaxies.
Gravity pulls everything together. Everything, from the bright centers of the universe to the planets farthest from them. In fact, you (yes, you!) even exert a gravitational force on a galaxy far, far away. A tiny gravitational force, but a force nonetheless.
Credit: NASA and the Advanced Visualization Laboratory at the National Center for Supercomputing and B. O'Shea, M. Norman
Despite its well-known reputation, gravity is actually the weakest of the four forces. Its strength increases with the mass of the two objects involved. And its range is infinite, but the strength drops off as the square of the distance. If you and a friend measured your gravitational tug on each other and then doubled the distance between you, your new gravitational attraction would just be a quarter of what it was. So, you have to be really close together, or really big, or both, to exert a lot of gravity.
Even so, because its range is infinite, gravity is responsible for the formation of the largest structures in our universe! Planetary systems, galaxies and clusters of galaxies all formed because gravity brought them together.
Gravity truly surrounds us and binds us together.
You know that shock you get on a dry day after shuffling across the carpet? The electricity that powers your television? The light that illuminates your room on a dark night? Those are all the work of electromagnetism. As the name implies, electromagnetism is the force that includes both electricity and magnetism.
Electromagnetism keeps electrons orbiting the nucleus at the center of atoms and allows chemical compounds to form (you know, the stuff that makes up us and everything around us). Electromagnetic waves are also known as light. Once started, an electromagnetic wave will travel at the speed of light until it interacts with something (like your eye) — so it will be there to light up the dark places.
Like gravity, electromagnetism works at infinite distances. And, also like gravity, the electromagnetic force between two objects falls as the square of their distance. However, unlike gravity, electromagnetism doesn’t just attract. Whether it attracts or repels depends on the electric charge of the objects involved. Two negative charges or two positive charges repel each other; one of each, and they attract each other. Plus. Minus. A balance.
This is what happens with common household magnets. If you hold them with the same “poles” together, they resist each other. On the other hand, if you hold a magnet with opposite poles together — snap! — they’ll attract each other.
Electromagnetism might just explain the relationship between a certain scruffy-looking nerf-herder and a princess.
Credit: Lawrence Livermore National Laboratory
The strong force is where things get really small. So small, that you can’t see it at work directly. But don’t let your eyes deceive you. Despite acting only on short distances, the strong force holds together the building blocks of the atoms, which are, in turn, the building blocks of everything we see around us.
Like gravity, the strong force always attracts, but that’s really where their similarities end. As the name implies, the force is strong with the strong force. It is the strongest of the four forces. It brings together protons and neutrons to form the nucleus of atoms — it has to be stronger than electromagnetism to do it, since all those protons are positively charged. But not only that, the strong force holds together the quarks — even tinier particles — to form those very protons and neutrons.
However, the strong force only works on very, very, very small distances. How small? About the scale of a medium-sized atom’s nucleus. For those of you who like the numbers, that’s about 10-15 meters, or 0.000000000000001 meters. That’s about a hundred billion times smaller than the width of a human hair! Whew.
Its tiny scale is why you don’t directly see the strong force in your day-to-day life. Judge a force by its physical size, do you?
If you thought it was hard to see the strong force, the weak force works on even smaller scales — 1,000 times smaller. But it, too, is extremely important for life as we know it. In fact, the weak force plays a key role in keeping our Sun shining.
But what does the weak force do? Well … that requires getting a little into the weeds of particle physics. Here goes nothing! We mentioned quarks earlier — these are tiny particles that, among other things, make up protons and neutrons. There are six types of quarks, but the two that make up protons and neutrons are called up and down quarks. The weak force changes one quark type into another. This causes neutrons to decay into protons (or the other way around) while releasing electrons and ghostly particles called neutrinos.
So for example, the weak force can turn a down quark in a neutron into an up quark, which will turn that neutron into a proton. If that neutron is in an atom’s nucleus, the electric charge of the nucleus changes. That tiny change turns the atom into a different element! Such reactions are happening all the time in our Sun, giving it the energy to shine.
The weak force might just help to keep you in the (sun)light.
All four of these forces run strong in the universe. They flow between all things and keep our universe in balance. Without them, we’d be doomed. But these forces will be with you. Always.
You can learn more about gravity from NASA’s Space Place and follow NASAUniverse on Twitter or Facebook to learn about some of the cool cosmic objects we study with light.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Hadas Cohen
Motivations are likely to be multifactorial and may be influenced by individual or organizational biases and competing interests.
An additional contributing factor is that individuals may be motivated to share information that they perceive to be both accurate and of social value.
Tablets, smart appliances, and other technologies that are an indispensable part of daily life are no longer state-of-the-art compared to the research and technology development going on over our heads. As we celebrate 20 years of humans continuously living and working in space aboard the International Space Station, we’re recapping some of the out-of-this-world tech development and research being done on the orbiting lab too.
Our Space Technology Mission Directorate (STMD) helps redefine state-of-the-art tech for living and working in space. Here are 10 technologies tried and tested on the space station with helping hands from its astronaut occupants over the years.
Astronauts on the space station are responsible for everything from conducting science experiments and deploying satellites to tracking inventory and cleaning. While all are necessary, the crew can delegate some jobs to the newest robotic inhabitants – Astrobees.
These cube-shaped robots can work independently or in tandem, carrying out research activities. Once they prove themselves, the bots will take on some of the more time-consuming tasks, such as monitoring the status of dozens of experiments. The three robots – named Bumble, Honey, and Queen – can operate autonomously following a programmed set of instructions or controlled remotely. Each uses cameras for navigation, fans for propulsion, and a rechargeable battery for power. The robots also have a perching arm that lets them grip handrails or hold items. These free-flying helpers take advantage of another STMD technology called Gecko Grippers that “stick” to any surface.
We wanted to develop tools for grabbing space junk, and something strong and super-sticky is necessary to collect the diverse material orbiting Earth. So, engineers studied the gecko lizard, perhaps the most efficient “grabber” on this planet. Millions of extremely fine hairs on the bottom of their feet make an incredible amount of contact with surfaces so the gecko can hold onto anything. That inspired our engineers to create a similar material.
Now the Gecko Gripper made by OnRobot is sold on the commercial market, supporting industrial activities such as materials handling and assembly. The NASA gecko adhesive gripper that’s being tested in microgravity on the Astrobee robots was fabricated on Earth. But other small plastic parts can now be manufactured in space.
Frequent resupply trips from Earth to the Moon, Mars, and other solar system bodies are simply not realistic. In order to become truly Earth-independent and increase sustainability, we had to come up with ways to manufacture supplies on demand.
A demonstration of the first 3D printer in space was tested on the space station in 2014, proving it worked in microgravity. This paved the way for the first commercial 3D printer in space, which is operated by Made In Space. It has successfully produced more than 150 parts since its activation in 2016. Designs for tools, parts, and many other objects are transmitted to the station by the company, which also oversees the print jobs. Different kinds of plastic filaments use heat and pressure in a process that’s similar to the way a hot glue gun works. The molten material is precisely deposited using a back-and-forth motion until the part forms. The next logical step for efficient 3D printing was using recycled plastics to create needed objects.
To help fragile technology survive launch and keep food safe for consumption, NASA employs a lot of single-use plastics. That material is a valuable resource, so we are developing a number of ways to repurpose it. The Refabricator, delivered to the station in 2018, is designed to reuse everything from plastic bags to packing foam. The waste plastic is super-heated and transformed into the feedstock for its built-in 3D printer. The filament can be used repeatedly: a 3D-printed wrench that’s no longer needed can be dropped into the machine and used to make any one of the pre-programmed objects, such as a spoon. The dorm-fridge-sized machine created by Tethers Unlimited Inc. successfully manufactured its first object, but the technology experienced some issues in the bonding process likely due to microgravity’s effect on the materials. Thus, the Refabricator continues to undergo additional testing to perfect its performance.
An upcoming hardware test on the station will try out a new kind of 3D printer. The on-demand digital manufacturing technology is capable of using different kinds of materials, including plastic and metals, to create new parts. We commissioned TechShot Inc. to build the hardware to fabricate objects made from aerospace-grade metals and electronics. On Earth, FabLab has already demonstrated its ability to manufacture strong, complex metal tools and other items. The unit includes a metal additive manufacturing process, furnace, and endmill for post-processing. It also has built-in monitoring for in-process inspection. When the FabLab is installed on the space station, it will be remotely operated by controllers on Earth. Right now, another printer created by the same company is doing a different kind of 3D printing on station.
Today scientists are also learning to 3D print living tissues. However, the force of gravity on this planet makes it hard to print cells that maintain their shape. So on Earth, scientists use scaffolding to help keep the printed structures from collapsing.
The 3D BioFabrication Facility (BFF) created by TechShot Inc. could provide researchers a gamechanger that sidesteps the need to use scaffolds by bioprinting in microgravity. This first American bioprinter in space uses bio-inks that contain adult human cells along with a cell-culturing system to strengthen the tissue over time. Eventually, that means that these manufactured tissues will keep their shape once returned to Earth’s gravity! While the road to bioprinting human organs is likely still many years away, these efforts on the space station may move us closer to that much-needed capability for the more than 100,000 people on the wait list for organ transplant.
Conditions in space are hard on the human body, and they also can be punishing on food. Regular deliveries of food to the space station refresh the supply of nutritious meals for astronauts. But prepackaged food stored on the Moon or sent to Mars in advance of astronauts could lose some nutritional value over time.
That’s why the BioNutrients experiment is underway. Two different strains of baker’s yeast which are engineered to produce essential nutrients on demand are being checked for shelf life in orbit. Samples of the yeast are being stored at room temperature aboard the space station and then are activated at different intervals, frozen, and returned to Earth for evaluation. These tests will allow scientists to check how long their specially-engineered microbes can be stored on the shelf, while still supplying fresh nutrients that humans need to stay healthy in space. Such microbes must be able to be stored for months, even years, to support the longer durations of exploration missions. If successful, these space-adapted organisms could also be engineered for the potential production of medicines. Similar organisms used in this system could provide fresh foods like yogurt or kefir on demand. Although designed for space, this system also could help provide nutrition for people in remote areas of our planet.
Everything from paints and container seals to switches and thermal protection systems must withstand the punishing environment of space. Atomic oxygen, charged-particle radiation, collisions with meteoroids and space debris, and temperature extremes (all combined with the vacuum) are just some conditions that are only found in space. Not all of these can be replicated on Earth. In 2001, we addressed this testing problem with the Materials International Space Station Experiment (MISSE). Technologists can send small samples of just about any technology or material into low-Earth orbit for six months or more. Mounted to the exterior of the space station, MISSE has tested more than 4,000 materials. More sophisticated hardware developed over time now supports automatic monitoring that sends photos and data back to researchers on Earth. Renamed the MISSE Flight Facility, this permanent external platform is now owned and operated by the small business, Alpha Space Test & Research Alliance LLC. The woman-owned company is developing two similar platforms for testing materials and technologies on the lunar surface.
Small satellites could provide a cheaper, faster way to deliver small payloads to Earth from the space station. To do just that, the Technology Education Satellite, or TechEdSat, develops the essential technologies with a series of CubeSats built by college students in partnership with NASA. In 2017, TechEdSat-6 deployed from the station, equipped with a custom-built parachute called exo-brake to see if a controlled de-orbit was possible. After popping out of the back of the CubeSat, struts and flexible cords warped the parachute like a wing to control the direction in which it travelled. The exo-brake uses atmospheric drag to steer a small satellite toward a designated landing site. The most recent mission in the series, TechEdSat-10, was deployed from the station in July with an improved version of an exo-brake. The CubeSat is actively being navigated to the target entry point in the vicinity of the NASA’s Wallops Flight Facility on Wallops Island, Virginia.
Independent navigation for spacecraft in deep space is challenging because objects move rapidly and the distances between are measured in millions of miles, not the mere thousands of miles we’re used to on Earth. From a mission perched on the outside of the station, we were able to prove that X-rays from pulsars could be helpful. A number of spinning neutron stars consistently emit pulsating beams of X-rays, like the rotating beacon of a lighthouse. Because the rapid pulsations of light are extremely regular, they can provide the precise timing required to measure distances.
The Station Explorer for X-Ray Timing and Navigation (SEXTANT) demonstration conducted on the space station in 2017 successfully measured pulsar data and used navigation algorithms to locate the station as it moved in its orbit. The washing machine-sized hardware, which also produced new neutron star science via the Neutron star Interior Composition Explorer (NICER), can now be miniaturized to develop detectors and other hardware to make pulsar-based navigation available for use on future spacecraft.
As NASA continues to identify challenges and problems for upcoming deep space missions such as Artemis, human on Mars, and exploring distant moons such as Titan, STMD will continue to further technology development on the space station and Earth.
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The planets beyond our solar system – exoplanets – are so far away, often trillions of miles, that we don’t have the technology to truly see them. Even the best photos show the planets as little more than bright dots. We’ve confirmed more than 5,000 exoplanets, but we think there are billions. Space telescopes like Hubble aren’t able to take photos of these far-off worlds, but by studying them in different wavelengths of light (colors), we’ve learned enough about conditions on these planets that we can illustrate them.
We know, thanks to the now-retired Spitzer Space Telescope, that there is a thick atmosphere on a planet called 55 Cancri e about 40 light-years away. And Hubble found silicate vapor in the atmosphere of this rocky world. We also know it’s scorching-close to its Sun-like star, so … lava. Lots and lots of lava. This planet is just one of the many that the James Webb Space Telescope will soon study, telling us even more about the lava world!
You can take a guided tour of this planet (and others) and see 360-degree simulations at our new Exoplanet Travel Bureau.
Travel to the most exotic destinations in our galaxy, including:
Kepler-16b, a planet with two suns.
Then there’s PSO J318.5-22, a world with no sun that wanders the galaxy alone. The nightlife would never end on a planet without a star.
TRAPPIST-1e, which will also be studied by the Webb Space Telescope, is one of seven Earth-sized planets orbiting a star about 40 light-years from Earth. It’s close enough that, if you were standing on this exoplanet, you could see our Sun as a star in the Leo constellation! You can also see it on the poster below: look for a yellow star to the right of the top person’s eye.
We haven’t found life beyond Earth (yet) but we’re looking. Meanwhile, we can imagine the possibility of red grass and other plants on Kepler-186f, a planet orbiting a red dwarf star.
We can also imagine what it might be like to skydive on a super-Earth about seven times more massive than our home planet. You would fall about 35% faster on a super-Earth like HD 40307g, making for a thrilling ride!
Any traveler is going to want to pick up souvenirs, and we have you covered. You can find free downloads of all the posters here and others! What are you waiting for? Come explore with us!
Make sure to follow us on Tumblr for your regular dose of space!
Image credits: NASA/JPL-Caltech
We judge ourselves by what we feel capable of doing, while others judge us by what we have already done.
Henry Wadsworth Longfellow (via quotemadness)
After completing more than two years of basic training, our graduating class of astronauts is eligible for spaceflight. Assignments include the International Space Station, Artemis missions to the Moon, and ultimately, missions to Mars.
The class includes 11 astronauts, selected in 2017 from a record-setting pool of more than 18,000 applicants. This was more than double the previous record of 8,000 applicants set in 1978.
Meet the graduates:
“If you don’t love what you’re doing, you’re not going to be good at it. I think it’s a combination of finding things that you really love that will also be really challenging and will force you to grow along the way.”
This Washington native graduated from the U.S. Naval Academy with a bachelor’s degree in systems engineering. As a Gates Cambridge Scholar, which offers students an opportunity to pursue graduate study in the field of their choice at the University of Cambridge. Barron earned a master’s degree in nuclear engineering.
As a Submarine Warfare Officer, Barron was part of the first class of women commissioned into the submarine community, completing three strategic deterrent patrols aboard the USS Maine.
“Every STEM opportunity that I have ever gone down is because of some mentor who inspired me or some student who was ahead of me in school who inspired me.”
Zena Cardman is a native of Virginia and completed a bachelor’s degree in biology and master’s degree in marine sciences at The University of North Carolina, Chapel Hill. Her research has focused on microorganisms in subsurface environments, ranging from caves to deep sea sediments.
An intrepid explorer, Cardman’s field experience includes multiple Antarctic expeditions, work aboard research vessels as both scientist and crew, and NASA analog missions in British Columbia, Idaho, and Hawaii.
“I grew up with the mentality that education is truly a gift not to be taken for granted.”
This Iowa native graduated from the U.S. Air Force Academy in 1999 with bachelor’s degrees in astronautical engineering and engineering science. He continued on to earn a master’s degree in aeronautics and astronautics from Massachusetts Institute of Technology (MIT) and graduated from the U.S. Naval Test Pilot School.
Chari served as the Commander of the 461st Flight Test Squadron and the Director of the F-35 Integrated Test Force. He has accumulated more than 2,000 hours of flight time in the F-35, F-15, F-16 and F-18 including F-15E combat missions in Operation Iraqi Freedom.
“I get to work with incredible people that want to solve problems and are passionate about it. I really want to contribute to the world and this is how I want to do it.”
This Colorado native earned a bachelor’s degree in electrical engineering from the University of San Diego and a master’s degree in systems engineering from the Naval Postgraduate School. He also graduated from U.S. Naval Test Pilot School.
Dominick served on the USS Ronald Reagan as department head for Strike Fighter Squadron 115. He has more than 1,600 hours of flight time in 28 aircraft, 400 carrier-arrested landings and 61 combat missions.
“As you get older, other things become important to you, like being a part of something that’s bigger than yourself. This human endeavor of exploration is something that’s really exciting.”
Bob Hines is a Pennsylvania native and earned a bachelor’s degree in aerospace engineering from Boston University. He is a graduate of the U.S. Air Force Test Pilot School, where he earned a master’s degree in flight test engineering. He continued on to earn a master’s degree in aerospace engineering from the University of Alabama.
Hines served in the U.S. Air Force and Air Force Reserves for 18 years. He also served as a research pilot at our Johnson Space Center. He has accumulated more than 3,500 hours of flight time in 41 different types of aircraft and has flown 76 combat missions in support of contingency operations around the world.
“It was back in high school that I realized that I was really interested in engineering. I always liked taking things apart and understanding how things work and then I also really enjoy solving problems.”
Nicknamed “Woody”, this Pennsylvania native earned a bachelor’s degree in aeronautics and astronautics from MIT and a doctorate in electrical engineering and computer science from the University of California, Berkeley.
Hoburg was leading a research group at MIT at the time of his selection and is a two-time recipient of the AIAA Aeronautics and Astronautics Teaching Award in recognition of outstanding teaching.
“I fundamentally believed in the NASA mission of advancing our space frontier, all while developing innovation and new technologies that would benefit all of humankind.”
This California native trained and operated as a Navy SEAL, completing more than 100 combat operations and earning a Silver Star and Bronze Star with Combat “V”. Afterward, he went on to complete a degree in mathematics at the University of San Diego and a doctorate of medicine at Harvard Medical School.
Kim was a resident physician in emergency medicine with Partners Healthcare at Massachusetts General Hospital.
“Surround yourself with good people that have the characteristics that you want to grow in yourself. I think if you surround yourself with people like that you kind of bring each other up to a higher and higher level as you go.”
Jasmin Moghbeli, a U.S. Marine Corps major, considers Baldwin, New York, her hometown. She earned a bachelor’s degree in aerospace engineering with information technology at MIT, followed by a master’s degree in aerospace engineering from the Naval Postgraduate School.
She is a distinguished graduate of the U.S. Naval Test Pilot School and has accumulated more than 1,600 hours of flight time and 150 combat missions.
“I’m one of those people who have wanted to be an astronaut since I was a little kid, and I think that came from an early obsession with flying – birds, airplanes, rockets.”
This Houston native earned a bachelor’s degree in aerospace engineering at the University of Kansas and a Master of Science degree in aeronautics and astronautics from Purdue University. As a student, she participated in multiple NASA internship programs, including the Reduced Gravity Student Flight Opportunities Program, the NASA Academy at Goddard Space Flight Center, and the internship program at the Jet Propulsion Laboratory.
O’Hara was a research engineer at Woods Hole Oceanographic Institution, where she worked on the engineering, test and operations of deep-ocean research submersibles and robots. She is also a private pilot and certified EMT and wilderness first responder.
“I just figured it was time to take the plunge and try it. And so, I did and beyond all dreams, it came true.”
Dr. Francisco “Frank” Rubio, a U.S. Army lieutenant colonel, is originally from Miami. He earned a bachelor’s degree in international relations from the U.S. Military Academy and earned a doctorate of medicine from the Uniformed Services University of the Health Sciences.
Rubio served as a UH-60 Blackhawk helicopter pilot and flew more than 1,100 hours, including more than 600 hours of combat and imminent danger time during deployments to Bosnia, Afghanistan, and Iraq. He is also a board certified family physician and flight surgeon.
“I’ve always been interested in exploring space. What’s out there and how can we as humans reach those outer stars and how can we learn more information about who we are through that process.”
This Colorado native earned a bachelor’s degree in geological and environmental sciences at Stanford University, and a doctorate in geology from the University of California, Los Angeles. Watkins has worked at Ames Research Center and the Jet Propulsion Laboratory.
Watkins was a postdoctoral fellow at the California Institute of Technology, where she collaborated on the Mars Curiosity rover, participating in daily planning of rover activities and investigating the geologic history of the Red Planet.
Learn more about the new space heroes right here: https://www.nasa.gov/newastronauts
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