Gravity rules everything on Earth, from how our bodies develop to what our research can reveal, but what happens when we go 250 miles up to the International Space Station?
Get ready to go behind the scenes of what it takes to get science to space, and meet the people who make it happen.
Introducing Season 4 of NASA Explorers: Microgravity. Floating isn’t just fun. Microgravity could open the door to discovery.
Microgravity makes the International Space Station the perfect place to perform research that is changing the lives of people on Earth, and preparing us to go deeper into space. This season on our series NASA Explorers, we are following science into low-Earth orbit and seeing what it takes to do research aboard the space station.
Follow NASA Explorers on Facebook to catch new episodes of season 4 every Wednesday!
... and we’re ‘GO’ for launch! 🚀
NASA Flight Integration Chief and past Mission Control Flight Director, Ginger Kerrick, is here answering your questions during this Tumblr Answer Time. Tune in and join the fun!
New experiments are scheduled to arrive to the International Space Station with the launch of Orbital ATK’s Cygnus cargo spacecraft on Tuesday. These science payloads will study fires, meteors, regolith, adhesion and 3-D printing in microgravity.
What is it? What happens when you set a fire in space? The Spacecraft Fire Experiment-I (Saffire-I) will find out!
How does it work? This experiment will intentionally light a large-scale fire inside an empty Cygnus resupply vehicle after it leaves the space station and before it re-enters Earth’s atmosphere.
Why is it important? The Saffire-I investigation provides a new way to study a realistic fire on an exploration vehicle, which has not been possible in the past because the risks for performing studies on manned spacecraft are too high. Instruments on the returning Cygnus will measure flame growth, oxygen use and more.
What is it? A less heated investigation, Meteor Composition Determination (Meteor) will enable the first space-based observations of meteors entering Earth’s atmosphere from space. Meteors are somewhat rare and are difficult to monitor from the ground because of Earth’s atmosphere.
How does it work? This investigation uses high-resolution video and image analysis of the atmosphere to acquire the physical and chemical properties of the meteoroid dust, such as size, density and chemical composition.
Why is it important? Studying the elemental composition of meteors adds to our understanding of how the planets developed, and continuous measurement of meteor interactions with Earth’s atmosphere could spot previously unforeseen meteors.
What is it? A more “grounded” investigation will study the properties and behavior of regolith, the impact-shatterd “soil” found on asteroids, comets, the moon and other airless worlds.
How does it work? The Strata-1 experimental facility exposes a series of regolith simulants, including pulverized meteorite material, glass beads, and regolith simulants composed of terrestrial materials and stored in multiple transparent tubes, to prolonged microgravity on the space station. Scientists will monitor changes in regolith layers and layering, size sorting and particle migration via video images and close examination after return of the samples to Earth.
Why is it important? The Strata-1 investigation could give us new answers about how regolith behaves and moves in microgravity, how easy or difficult it is to anchor a spacecraft in regolith, how it interacts with spacecraft and spacesuit materials and other important properties.
What is it? From grounded to gripping, another investigation launching takes inspiration from small lizards. Geckos have specialized hairs on their feed called setae that let them stick to vertical surfaces without falling, and their stickiness doesn’t wear off after repeated use. The Gecko Gripper investigation tests a gecko-adhesive gripping device that can stick on command in the harsh environment of space.
How does it work? The gripping device is a material with synthetic hairs much like setae that are much thinner than a human hair. When a force is applied to make the tiny hairs bend, the positively charged part of a molecule within a slight electrical field attracts the negatively charged part of its neighbor resulting in “stickiness.” Once adhered, the gripper can bear loads up to 20 pounds. The gripper can remain in place indefinitely and can also be easily removed and reused.
Why is it important? Gecko Grippers have many applications on current and future space missions, including acting as mounting devices for payloads, instruction manuals and many other small items within the space station. In addition, this technology enables a new type of robotic inspection system that could prove vital for spacecraft safety and repair.
What is it? From adhesion to additive, the new Additive Manufacturing Facility (AMF) will also launch on the flight. Additive manufacturing (3D printing) is the process of building a part layer-by-layer, with an efficient use of the material.
How does it work? The AMF uses this technology to enable the production of components on the space station for both NASA and commercial objectives.
Why is it important? Parts, entire experiments and tools can be created on demand with this technology. The ability to manufacture on the orbiting laboratory enables on-demand repair and production capability, as well as essential research for manufacturing on long-term missions.
These sticky, stony and sizzling investigations are just a sampling of the wide range of science conducted on the orbiting laboratory that benefits future spaceflight and provides Earth-based benefits as well.
You can watch the launch of Orbital ATK’s Cygnus spacecraft online. Stream live coverage starting at 10 p.m. EDT on March 22. Launch is scheduled for 11:05 p.m., which is the start of a 30-minute launch window.
Watch online: nasa.gov/nasatv
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We have had an active robotic presence there ever since—in fact, no one under 20 has experienced a day without NASA at Mars—but the Pathfinder mission was the first-ever robotic rover to explore the Red Planet. Below are 10 things to know about this iconic mission as we celebrate two decades of unprecedented science and discovery.
Pathfinder launched from Cape Canaveral, Florida on Dec. 4, 1996, and landed at Mars' Ares Vallis on July 4, 1997. The landing site, an ancient flood plain in Mars' northern hemisphere, is among the rockiest parts of the planet. Scientists chose it because they believed it was a relatively safe surface to land on and contained a wide variety of rocks deposited during a catastrophic flood.
Pathfinder delivered to Mars a tiny, 23-pound (11.5 kilogram) rover named Sojourner, which carried scientific instruments to analyze the Martian atmosphere, climate and geology. To put its small size in perspective, the mechanisms at the end of the Curiosity Rover's robotic arm are heavier than all of Sojourner. You can check out a 360 video of Pathfinder and Sojourner here.
The name Sojourner was chosen after a year-long, worldwide competition in which students up to 18 years old were invited to write about a historical heroine and how she would translate their accomplishments to the Martian environment. Twelve-year-old Valerie Ambroise of Bridgeport, Connecticut, submitted the winning essay on Sojourner Truth, a Civil War-era abolitionist who made it her mission to "travel up and down the land" advocating for the rights of all people to be free and participate fully in society.
Pathfinder's landing was innovative and unprecedented. It entered the thin Martian atmosphere assisted by parachute to slow its descent and with a giant system of airbags to cushion the impact. This mission marked the first time this airbag technique was used. Spirit and Opportunity later used the same method successfully.
The wireless modem between Pathfinder and Sojourner was a commercial, off-the-shelf product. The project team acquired several and stress-tested them until they found the best ones to send off to Mars.
Sojourner had bumpers—actual mechanical fenders—painted with black and white stripes. It also had two forward-facing black-and-white cameras, and one rear-facing camera (all one-third of a Megapixel). And Sojourner's tiny wheels measured just 12.5 centimeters in diameter.
Pathfinder was widely regarded as one of the first "internet sensations." There was so much web traffic from around the world, the entire internet backbone of France crashed under the load.
Among the many scientific discoveries from Pathfinder and Sojourner: Rounded pebbles and cobbles at the landing site suggested that Mars might have had running water during a warmer past when liquid water was stable on the planet. Early morning water ice clouds also were seen in the lower atmosphere.
The lander and the rover both outlived their design lives—the lander by nearly three times, and the rover by 12 times.
Go back in time and see historical photographs of Pathfinder's assembly process here.
Simply put, an exoplanet is a planet that orbits another star.
All of the planets in our solar system orbit around the Sun. Planets that orbit around other stars outside our solar system are called exoplanets.
Just because a planet orbits a star (like Earth) does not mean that it is automatically stable for life. The planet must be within the habitable zone, which is the area around a star in which water has the potential to be liquid…aka not so close that all the water would evaporate, and not too far away where all the water would freeze.
Exoplanets are very hard to see directly with telescopes. They are hidden by the bright glare of the stars they orbit. So, astronomers use other ways to detect and study these distant planets by looking at the effects these planets have on the stars they orbit.
One way to search for exoplanets is to look for "wobbly" stars. A star that has planets doesn’t orbit perfectly around its center. From far away, this off-center orbit makes the star look like it’s wobbling. Hundreds of planets have been discovered using this method. However, only big planets—like Jupiter, or even larger—can be seen this way. Smaller Earth-like planets are much harder to find because they create only small wobbles that are hard to detect.
In 2009, we launched a spacecraft called Kepler to look for exoplanets. Kepler looked for planets in a wide range of sizes and orbits. And these planets orbited around stars that varied in size and temperature.
Kepler detected exoplanets using something called the transit method. When a planet passes in front of its star, it’s called a transit. As the planet transits in front of the star, it blocks out a little bit of the star's light. That means a star will look a little less bright when the planet passes in front of it. Astronomers can observe how the brightness of the star changes during a transit. This can help them figure out the size of the planet.
By studying the time between transits, astronomers can also find out how far away the planet is from its star. This tells us something about the planet’s temperature. If a planet is just the right temperature, it could contain liquid water—an important ingredient for life.
So far, thousands of planets have been discovered by the Kepler mission.
We now know that exoplanets are very common in the universe. And future missions have been planned to discover many more!
Next month, we’re launching an explorer-class planet finder — the Transiting Exoplanet Survey Satellite (TESS). This mission will search the entire sky for exoplanets — planets outside our solar system that orbit sun-like stars.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.
In March, Jupiter, it’s moons and moon shadows will all be visible in the sky. Find out when and where to look up:
Jupiter dominates the evening sky this month, rising at sunset and setting at dawn. On March 8, Jupiter reaches what is called “opposition”. Imagine that Jupiter and the sun are at opposite ends of a straight line, with the Earth in between. This brings Jupiter its closest to Earth, so it shines brighter and appears larger in telescopes.
On the nights of March 14 – 15, March 21 – 22 and March 29, two of Jupiter’s moons will cross the planet’s disk.
When the planet is at opposition and the sun shines on Jupiter’s moons, we can see the moon’s shadow crossing the planet. There are actually 11 of these double shadow transits in March!
The next six months will be awesome times for you to image Jupiter when it’s highest in the sky; near midnight now, and a little earlier each night through the late summer.
Even through the smallest telescopes or binoculars, you should be able to see the two prominent belts on each side of Jupiter’s equator made up of the four Galilean moons: Io, Europa Ganymede and Calisto. If you have a good enough view, you may even see Jupiter’s Red Spot!
Our Juno spacecraft will arrive at Jupiter on July 4th of this year and will go into orbit around the giant planet. Right now, the Juno mission science team is actively seeking amateur and professional images of the planet. These images are uploaded to a Juno website, and the public is invited to discuss points of interest in Jupiter’s atmosphere.
Locations will later be voted on and the favorites will be targets for JunoCam, the spacecraft’s imaging camera. Once JunoCam has taken the images, they’ll be posted online. Imaging participants can then process these raw mission images and re-upload them for others to view.
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Will ordinary sunglasses suffice?
Unfortunately not. Sunglasses are not sufficient to ever look directly at the Sun. You can find glasses and filters that are safe here https://eclipse2017.nasa.gov/safety And if you can’t find any that will get to you in time for the eclipse on Monday (you can always use them to look at the Sun at a later time to see sunspots), you can make a pin hole projector! https://eclipse.aas.org/eye-safety/projection I think those are fantastic fun!
Did you hear? Astronaut applications are open! Here are a few signs that might mean you’re ready to apply:
1. You Don’t Mind Having Roommates
When you’re an astronaut, you have to work and live with your crew mates for extended periods of time. It’s important to the mission and your safety that everyone can collaborate and work together.
2. You LOVE Space
If the Milky Way, planets and space travel doesn’t excite you then this might not be the perfect job for you. But if you love galaxies, space station research and deep space exploration, then maybe you should take a look at our application.
3. Adventure Doesn’t Scare You
Being an astronaut means that you get to take part in adventures that most people will never experience. Imagine: sitting on the launch pad in the Orion spacecraft, atop a rocket that’s getting ready to launch. You’ll travel farther into space than any other humans have been and help push the boundaries of technology in the proving ground of deep space lunar orbits, leading the way for future missions to Mars.
4. You Want to be on the Cutting Edge of Science
Not only do astronauts get to travel to space, but they also get to conduct really cool research in microgravity. Did you know that right now they’re growing Zinnia flowers on the International Space Station? This research could help with our future deep space exploration and could teach us a few things about growing plants on Earth. Learn more about all the awesome research on the space station HERE.
5. You’re Not Afraid of Heights
One of the coolest things about being an astronaut, is that you get to go to SPACE! At the very least, you’ll travel to the International Space Station, which is 250 miles above Earth. Or, you could be one of the first astronauts to travel to a distant asteroid or even Mars!
Interested in applying to become an astronaut? You’re in luck, applications open Dec. 14! Learn about some common myths about becoming an astronaut HERE.
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Nora AlMatrooshi, the first Emirati woman astronaut, worked as a piping engineer before becoming an astronaut candidate for the United Arab Emirates. https://mbrsc.ae/team/nora/
Make sure to follow us on Tumblr for your regular dose of space!
What exactly did you do during your time as a flight surgeon? I guess im just trying to ask, what does that job include?
Our solar system is littered with asteroids and comets, and sometimes they get a little close to Earth. But no need to worry! This happens all the time. When an asteroid or comet could come close to our planet, it’s known as a near-Earth object – aka NEO.
But how close is “close”?
A near-Earth object is defined as an object that could pass by our Earth within 30 million miles. We begin to keep close watch on objects that could pass within 5 million miles of our planet.
To put that into perspective, our Moon is only 238,900 miles away.
However unlikely an impact is, we want to know about all near-Earth objects. Our Planetary Defense Coordination Office maintains watch for asteroids and comets coming close to Earth. Along with our partners, we discover, catalog and characterize these bodies.
But what if one of these objects posed a threat?
We want to be prepared. That is why we are working on several deflection techniques and technologies to help protect our planet.
So next time that you hear of an asteroid passing “close” to Earth, know that it’s just one of many that we are tracking.
Here are 10 more things you should know about Planetary Defense.
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