Squaring Off With Icebergs With Operation IceBridge

High-Flying Spacecraft Finish 1000th Lap Around Earth!

The quadruplet spacecraft of the Magnetospheric Multiscale mission have just returned from their first adventure into the solar wind — sailing through the most intense winds of their journey so far.

These spacecraft were designed to study Earth’s giant magnetic system, which shields our planet from the majority of the Sun’s constant outflow of material — what we call the solar wind.

Usually, the Magnetospheric Multiscale spacecraft — MMS for short — take their measurements from inside Earth’s protective magnetic environment, the magnetosphere. But in February and March, the MMS spacecraft ventured beyond this magnetic barrier to measure that solar wind directly — a feat that meant they had to change up how they fly in a whole new way.

Outside of Earth's protective magnetic field, the spacecraft were completely immersed in the particles and magnetic fields of the solar wind. As they flew through the stream of material, the spacecraft traced out a wake behind each instrument, just like a boat in a river. To avoid measuring that wake, each spacecraft was tilted into the wind so the instruments could take clean measurements of the pristine solar wind, unaffected by the wake.

Within the magnetosphere, the MMS spacecraft fly in a pyramid-shaped formation that allows them to study magnetic fields in 3D. But to study the solar wind, the mission team aligned spacecraft in a straight line at oddly spaced intervals. This string-of-pearls formation gave MMS a better look at how much the solar wind varies over different scales.

Because the four spacecraft fly so close together, MMS relies on super-accurate navigation from GPS satellites. This venture into the solar wind took the spacecraft even farther from Earth than before, so MMS broke its own world record for highest-ever GPS fix. The spacecraft were over 116,000 miles above Earth — about halfway to the Moon — and still using GPS!

Now, just in time for the 1,000th orbit of their mission — which adds up to 163 million miles flown! — the spacecraft are back in Earth's magnetosphere, flying in their usual formation to study fundamental processes within our planet’s magnetic field.

Keep up with the latest MMS research at nasa.gov/mms, on Twitter @NASASun or with NASA Sun Science on Facebook.

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Cool Space GIFs from the Internet

There’s a lot of historical and archived space footage on the internet and we’re excited to see that the public (you!) have taken it to create many other products that teach people about exploration, space and our universe. Among those products are GIFs. Those quick videos that help you express what you’re trying to say via text, or make you laugh while surfing the web.

Are space GIFs the new cat videos of the internet? Don’t know, but we sure do like them!

Here are a few neat space GIFs from the internet…

This GIF of the Cat Eye Nebula shows it in various wavelengths…

Followed by a GIF of a cat in space…floating in front of the Antennae galaxies...

One time, a frog actually photobombed the launch of our LADEE spacecraft…someone on the internet gave him a parachute…

Want to see what it’s like to play soccer in space? There’s a GIF for that…

There are also some beautiful GIFs looking through the Cupola window on the International Space Station…

This warped footage from the International Space Station gives us ride around the Earth…

While this one encourages us to explore the unknown...

When our New Horizons spacecraft flew by dwarf planet Pluto in 2015, the internet couldn’t get enough of the Pluto GIFs...

NASA GIFs

Want to dive into a black hole of other fun space GIFs? Check out our GIPHY page HERE.

Want to use our GIFs?! You can! Our GIFs are accessible directly from the Twitter app. Just tap or click the GIF button in the Twitter tool bar, search for NASAGIF, and all NASA GIFs will appear for sharing and tweeting. Enjoy!

GIF Sources

Cat Eye GIF: https://giphy.com/gifs/astronomy-cZpDWjSlKjWPm Cat GIF: https://giphy.com/gifs/cat-HopYL0SamcCli Frog GIF: https://giphy.com/gifs/nasa-photo-rocket-NOsCSDT2rUgfK Soccer GIF: https://giphy.com/gifs/yahoo-astronauts-zerogravity-QF1ZomA11zofC Cupola 1 GIF: https://giphy.com/gifs/nasa-Mcoxp6TgvQm6A Cupola 2 GIF: https://giphy.com/gifs/timelapse-space-11f3o8D2rQWzCM Earth GIF: http://giphy.com/gifs/earth-milky-way-international-space-station-ONC6WgECm5KEw Explore GIF: https://giphy.com/gifs/text-timelapse-lapse-Vj7gwAvhgsDYs Pluto 1 GIF: https://giphy.com/gifs/l46CzjUnYFfeMXiNO Pluto 2 GIF: https://giphy.com/gifs/pluto-dbV1LkFWWob84

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Top 10 Things to Know for the Return of our Launch America Mission With SpaceX

History was made May 30 when NASA astronauts Robert Behnken and Douglas Hurley launched from American soil in a commercially built and operated American crew spacecraft on its way to the International Space Station. 

Pictured above is the SpaceX Dragon Endeavour spacecraft that lifted off on the company’s Falcon 9 rocket from Launch Complex 39A at Kennedy Space Center in Florida and docked with the space station on May 31. Now, Behnken and Hurley are ready to return home in Endeavour for a splashdown off the coast of Florida, closing out a mission designed to test SpaceX’s human spaceflight system, including launch, docking, splashdown, and recovery operations. Undocking is targeted for 7:34 p.m. ET on August 1, with splashdown back to Earth slated for 2:42 p.m. on August 2. Watch our continuous live coverage HERE. 

1. Where will Behnken and Hurley splash down?

Image: SpaceX’s Crew Dragon is guided by four parachutes as it splashes down in the Atlantic on March 8, 2019, after the uncrewed spacecraft's return from the International Space Station on the Demo-1 mission.

Together with SpaceX, we are capable of supporting seven splashdown sites off the coast of Florida. The seven potential splashdown sites for the Dragon Endeavor are off the coasts of Pensacola, Tampa, Tallahassee, Panama City, Cape Canaveral, Daytona, and Jacksonville.

2. How will a splashdown location be chosen?

Splashdown locations are selected using defined priorities, starting with selecting a station departure date and time with the maximum number of return opportunities in geographically diverse locations to protect for weather changes. Teams also prioritize locations which require the shortest amount of time between undocking and splashdown based on orbital mechanics, and splashdown opportunities that occur in daylight hours.

Check out the Departure and Splashdown Criteria Fact Sheet for an in-depth look at selecting return locations, decision points during return, and detailed weather criteria.

3. How long will it take for Behnken and Hurley to return to Earth?

Return time for Behnken and Hurley will vary depending on the undock and splashdown opportunities chosen, with the primary opportunity taking between six and 30 hours.

4. What does the return look like? What are the major milestones?

Crew Dragon’s return home will start with undocking from the International Space Station. At the time of undock, Dragon Endeavour and its trunk weigh approximately 27,600 pounds. We will provide live coverage of the return from undocking all the way through splashdown.

There will be two very small engine burns immediately after hooks holding Crew Dragon in place retract to actually separate the spacecraft from the station. Once flying free, Dragon Endeavour will autonomously execute four departure burns to move the spaceship away from the space station and begin the flight home. Several hours later, one departure phasing burn, lasting about six minutes, puts Crew Dragon on the proper orbital path to line it up with the splashdown zone.

Shortly before the final deorbit burn, Crew Dragon will separate from its trunk, which will burn up in Earth’s atmosphere. The spacecraft then executes the deorbit burn, which commits Crew Dragon to return and places it on an orbit with the proper trajectory for splashdown. After trunk separation and the deorbit burn are complete, the Crew Dragon capsule weighs approximately 21,200 pounds.  

5. How fast will Dragon Endeavour be going when it re-enters the Earth’s atmosphere? How hot will it get?

Crew Dragon will be traveling at orbital velocity prior to re-entry, moving at approximately 17,500 miles per hour. The maximum temperature it will experience on re-entry is approximately 3,500 degrees Fahrenheit. The re-entry creates a communications blackout between the spacecraft and Earth that is expected to last approximately six minutes.

6. When do the parachutes deploy?

Image: SpaceX’s final test of Crew Dragon’s Mark 3 parachute system on Friday, May 1, 2020, that will be used during the Demo-2 splashdwon mission. 

Dragon Endeavour has two sets of parachutes will that deploy once back inside Earth’s atmosphere to slow down prior to splashdown. Two drogue parachutes will deploy at about 18,000 feet in altitude while Crew Dragon is moving approximately 350 miles per hour. Four main parachutes will deploy at about 6,000 feet in altitude while Crew Dragon is moving approximately 119 miles per hour.

7. Who recovers the crew and the Dragon Endeavour capsule from the water? What vehicles and personnel are involved?

Image: SpaceX’s Crew Dragon is loaded onto the company’s recovery ship, Go Searcher, in the Atlantic Ocean, about 200 miles off Florida’s east coast, on March 8, after returning from the International Space Station on the Demo-1 mission.Credits: SpaceX

For splashdown at any of the seven potential sites, SpaceX personnel will be on location to recover the capsule from the water. Two recovery ships, the Go Searcher and the Go Navigator, split locations between the Gulf of Mexico and the Atlantic Ocean off the coast of Florida. On either ship will be more than 40 personnel from SpaceX and NASA, made up of spacecraft engineers, trained water recovery experts, medical professionals, the ship’s crew, NASA cargo experts, and others to assist in the recovery.

8. How long after splashdown until Behnken and Hurley are out of the capsule?

Image: NASA astronaut Doug Hurley, along with teams from NASA and SpaceX, rehearse crew extraction from SpaceX’s Crew Dragon, on August 13, 2019. Credits: NASA/Bill Ingalls

Immediately after splashdown has occurred, two fast boats with SpaceX personnel deploy from the main recovery ship. The first boat checks capsule integrity and tests the area around the Crew Dragon for the presence of any hypergolic propellant vapors. Once cleared, the personnel on the boats begin preparing the spaceship for recovery by the ship. The second fast boat is responsible for safing and recovering Crew Dragon’s parachutes, which have at this point detached from the capsule and are in the water.

At this point the main recovery vessel can move in and begin to hoist the Crew Dragon capsule onto the main deck. Once the capsule is on the recovery vessel, it is moved to a stable location for the hatch to be opened for waiting medical professionals to conduct initial checks and assist Behnken and Hurley out of Dragon Endeavour.

This entire process is expected to take approximately 45 to 60 minutes, depending on spacecraft and sea state conditions.

9. Where do Behnken and Hurley go after they are out of the capsule?

Immediately after exiting the Crew Dragon capsule, Behnken and Hurley will be assisted into a medical area on the recovery ship for initial assessment. This is similar to procedures when welcoming long-duration crew members returning home on Soyuz in Kazakhstan.

After initial medical checks, Behnken and Hurley will be returned to shore either by traveling on the primary recovery ship or by helicopter. Helicopter returns from the recovery ship are the baseline for all splashdown zones except for the Cape Canaveral splashdown site, with travel times ranging from approximately 10 minutes to 80 minutes. The distance from shore will be variable depending on the splashdown location, ranging from approximately 22 nautical miles to 175 nautical miles.

Once returned to shore, both crew members will immediately board a waiting NASA plane to fly back to Ellington field in Houston.

10. What happens next?

Image: NASA astronauts Shannon Walker, Victor Glover Jr. and Mike Hopkins and Japan’s Soichi Noguchi train in a SpaceX Crew Dragon capsule. Credit: SpaceX

Meanwhile, Dragon Endeavour will be returned back to the SpaceX Dragon Lair in Florida for inspection and processing. Teams will examine the data and performance of the spacecraft throughout the test flight to complete the certification of the system to fly operational missions for our Commercial Crew and International Space Station Programs. The certification process is expected to take about six weeks. Following successful certification, the first operational mission will launch with Crew Dragon commander Michael Hopkins, pilot Victor Glover, and mission specialist Shannon Walker – all of NASA – along with Japan Aerospace Exploration Agency (JAXA) mission specialist Soichi Noguchi will launch on the Crew-1 mission from Launch Complex 39A at NASA’s Kennedy Space Center in Florida. The four crew members will spend six months on the space station.

The launch is targeted for no earlier than late-September.

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There’s Going to Be an Outburst!

Watch the Perseid Meteor Shower at Its Peak Tonight

The last time we had an outburst, that is a meteor shower with more meteors than usual, was in 2009. This year’s Perseid meteor shower is predicted to be just as spectacular starting tonight!

Plan to stay up late tonight or set your alarm clock for the wee morning hours to see this cosmic display of “shooting stars” light up the night sky. Known for it’s fast and bright meteors, tonight’s annual Perseid meteor shower is anticipated to be one of the best meteor viewing opportunities this year.

For stargazers experiencing cloudy or light-polluted skies, a live broadcast of the Perseid meteor shower will be available via Ustream overnight tonight and tomorrow, beginning at 10 p.m. EDT.

“Forecasters are predicting a Perseid outburst this year with double normal rates on the night of Aug. 11-12,” said Bill Cooke with NASA’s Meteoroid Environments Office in Huntsville, Alabama. “Under perfect conditions, rates could soar to 200 meteors per hour.”

Every Perseid meteor is a tiny piece of the comet Swift-Tuttle, which orbits the sun every 133 years. When Earth crosses paths with Swift-Tuttle’s debris, specks of comet-stuff hit Earth’s atmosphere and disintegrate in flashes of light. These meteors are called Perseids because they seem to fly out of the constellation Perseus.

Most years, Earth might graze the edge of Swift-Tuttle’s debris stream, where there’s less activity. Occasionally, though, Jupiter’s gravity tugs the huge network of dust trails closer, and Earth plows through closer to the middle, where there’s more material.

This is predicted be one of those years!

Learn more about the Perseids!

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TESS: The Planet Hunter

So you’re thinking...who’s TESS? But, it’s more like: WHAT is TESS? 

The Transiting Exoplanet Survey Satellite (TESS) is an explorer-class planet finder that is scheduled to launch in April 2018. This mission will search the entire sky for exoplanets — planets outside our solar system that orbit sun-like stars.

In the first-ever space borne all-sky transit survey, TESS will identify planets ranging from Earth-sized to gas giants, orbiting a wide range of stellar types and orbital distances.

The main goal of this mission is to detect small planets with bright host stars in the solar neighborhood, so that we can better understand these planets and their atmospheres.

TESS will have a full time job monitoring the brightness of more than 200,000 stars during a two year mission. It will search for temporary drops in brightness caused by planetary transits. These transits occur when a planet’s orbit carries it directly in front of its parent star as viewed from Earth (cool GIF below).

TESS will provide prime targets for further, more detailed studies with the James Webb Space Telescope (JWST), as well as other large ground-based and space-based telescopes of the future.

What is the difference between TESS and our Kepler spacecraft?

TESS and Kepler address different questions: Kepler answers "how common are Earth-like planets?" while TESS answers “where are the nearest transiting rocky planets?”

What do we hope will come out of the TESS mission?

The main goal is to find rocky exoplanets with solid surfaces at the right distance from their stars for liquid water to be present on the surface. These could be the best candidates for follow-up observations, as they fall within the “habitable zone” and be at the right temperatures for liquid water on their surface.

TESS will use four cameras to study sections of the sky’s north and south hemispheres, looking for exoplanets. The cameras would cover about 90 percent of the sky by the end of the mission. This makes TESS an ideal follow-up to the Kepler mission, which searches for exoplanets in a fixed area of the sky. Because the TESS mission surveys the entire sky, TESS is expected to find exoplanets much closer to Earth, making them easier for further study.

Stay updated on this planet-hunting mission HERE.

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We asked real life astronauts YOUR questions! Was your submission sent to space?

Astronauts Drew Feustel & Ricky Arnold recently recorded answers to your questions in a Video Answer Time session. We collected your questions and sent them to space to be answered by the astronauts on Friday, May 18. We recorded their answers and will post them tomorrow, May 30, here on our Tumblr. 

Was your question selected to be sent to the International Space Station? Check our Tumblr tomorrow, starting at noon EDT to find out!

About the astronauts:

Andrew J. Feustel was selected by NASA in 2000.  He has been assigned to Expedition 55/56, which launched in March 2018. The Lake Orion, Michigan native has a Ph.D. in the Geological Sciences, specializing in Seismology, and is a veteran of two spaceflights. Follow Feustel on Twitter and Instagram.

Richard R. Arnold II was selected as an astronaut by NASA in May 2004. The Maryland native worked in the marine sciences and as a teacher in his home state, as well as in countries such as Morocco, Saudi Arabia, and Indonesia. Follow Arnold on Twitter and Instagram.

Don’t forget check our Tumblr tomorrow at noon EDT to see if your question was answered by real-life astronauts in space. 

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

Question: would you rather be on the beach or would you rather gawk at it from space? For some, it’s a tough choice.

Astronaut Soichi Noguchi of the Japan Space Agency recently took this image of Andros Island, the largest island in the Bahamas. He and his three crew mates, NASA astronauts Victor Glover, Mike Hopkins and Shannon Walker, are currently living and working aboard the International Space Station for a six-month science mission. The crew launched on Nov. 15 from Kennedy Space Center and are conducting a number of scientific research, including Earth observation.

Every 90 minutes, the International Space Station completes one orbit around Earth. Because Earth rotates below them while they orbit, the crew get to see most of their beautiful blue marble of a planet from the unique vantage point of space. By photographing Earth from about 250 miles above the surface, astronauts can record phenomena such as storms in real time, and even provide input to ground teams. Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.

What do you do when things don't go according to plan?

Gamma-ray Bursts: Black Hole Birth Announcements

Gamma-ray bursts are the brightest, most violent explosions in the universe, but they can be surprisingly tricky to detect. Our eyes can't see them because they are tuned to just a limited portion of the types of light that exist, but thanks to technology, we can even see the highest-energy form of light in the cosmos — gamma rays.

So how did we discover gamma-ray bursts? 

Accidentally!

We didn’t actually develop gamma-ray detectors to peer at the universe — we were keeping an eye on our neighbors! During the Cold War, the United States and the former Soviet Union both signed the Nuclear Test Ban Treaty of 1963 that stated neither nation would test nuclear weapons in space. Just one week later, the US launched the first Vela satellite to ensure the treaty wasn’t being violated. What they saw instead were gamma-ray events happening out in the cosmos!

Things Going Bump in the Cosmos

Each of these gamma-ray events, dubbed “gamma-ray bursts” or GRBs, lasted such a short time that information was very difficult to gather. For decades their origins, locations and causes remained a cosmic mystery, but in recent years we’ve been able to figure out a lot about GRBs. They come in two flavors: short-duration (less than two seconds) and long-duration (two seconds or more). Short and long bursts seem to be caused by different cosmic events, but the end result is thought to be the birth of a black hole.

Short GRBs are created by binary neutron star mergers. Neutron stars are the superdense leftover cores of really massive stars that have gone supernova. When two of them crash together (long after they’ve gone supernova) the collision releases a spectacular amount of energy before producing a black hole. Astronomers suspect something similar may occur in a merger between a neutron star and an already-existing black hole.

Long GRBs account for most of the bursts we see and can be created when an extremely massive star goes supernova and launches jets of material at nearly the speed of light (though not every supernova will produce a GRB). They can last just a few seconds or several minutes, though some extremely long GRBs have been known to last for hours!

A Gamma-Ray Burst a Day Sends Waves of Light Our Way!

Our Fermi Gamma-ray Space Telescope detects a GRB nearly every day, but there are actually many more happening — we just can’t see them! In a GRB, the gamma rays are shot out in a narrow beam. We have to be lined up just right in order to detect them, because not all bursts are beamed toward us — when we see one it's because we're looking right down the barrel of the gamma-ray gun. Scientists estimate that there are at least 50 times more GRBs happening each day than we detect!

So what’s left after a GRB — just a solitary black hole? Since GRBs usually last only a matter of seconds, it’s very difficult to study them in-depth. Fortunately, each one leaves an afterglow that can last for hours or even years in extreme cases. Afterglows are created when the GRB jets run into material surrounding the star. Because that material slows the jets down, we see lower-energy light, like X-rays and radio waves, that can take a while to fade. Afterglows are so important in helping us understand more about GRBs that our Neil Gehrels Swift Observatory was specifically designed to study them!

Last fall, we had the opportunity to learn even more from a gamma-ray burst than usual! From 130 million light-years away, Fermi witnessed a pair of neutron stars collide, creating a spectacular short GRB. What made this burst extra special was the fact that ground-based gravitational wave detectors LIGO and Virgo caught the same event, linking light and gravitational waves to the same source for the first time ever!

For over 10 years now, Fermi has been exploring the gamma-ray universe. Thanks to Fermi, scientists are learning more about the fundamental physics of the cosmos, from dark matter to the nature of space-time and beyond. Discover more about how we’ll be celebrating Fermi’s achievements all year!

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Get to Know the 5 College Teams Sending Their Experiments to Space!

Did you know that YOU (yes you!), can send science experiments to the International Space Station? 

To celebrate 20 years of continuous human presence on the International Space Station, NASA STEM on Station is sending five student experiments to the space station through Student Payload Opportunity with Citizen Science (SPOCS). Selected teams will also engage K-12 students as a part of their experiment through citizen-science.

Get to know the 5 college teams sending their experiments to space!

Arkansas State University 

Team: A-State Science Support System

Experiment Title: Microgravity Environment Impact on Plastic Biodegradation by Galleria mellonella

Experiment Description: Discover the ability of wax worms to degrade plastics in space.

Why did you propose this experiment?

Our team’s passion for sustainability developed into novel ideas for space travel through biodegradation of plastics. 

How will the experiment benefit humankind or future space exploration?

If our experiment is successful, it will “launch” us closer to understanding how to reduce humankind’s plastic footprint on Earth and allow us to safely push farther into unknown planetary habitats.

How have you worked together as a team during the pandemic?

Unknown to each other before the project, our interdisciplinary team formed through virtual communication.

What science fiction character best represents your team and why?

The sandworms of Dune represent our team perfectly considering their importance in space travel, the natural ecological service they provide, and their sheer awesomeness

Columbia University

Team: Columbia Space Initiative

Experiment Title: Characterizing Antibiotic Resistance in Microgravity Environments (CARMEn)

Experiment Description: Discover the impact of mutations on bacteria in microgravity when grown into a biofilm with fungus.

Why did you propose this experiment?

As a highly interdisciplinary team united by our love of outer space, SPOCS was the perfect opportunity to fuse biology, engineering, and education into a meaningful team project.

How will the experiment benefit humankind or future space exploration?

Studying how different microorganisms interact with each other to develop bacterial resistance in space will help improve antibiotic treatments for future Artemis astronauts.

How have you worked together as a team during the pandemic?

Most of our team actually hasn’t ever met in person—we’ve been videoconferencing weekly since May!

What science fiction character best represents your team and why?

Our team is definitely Buzz Lightyear from Toy Story, because we strive to reach infinity (or at least the International Space Station) and beyond!

Stanford University

Team: Stanford Student Space Initiative

Experiment Title: Biopolymer Research for In-Situ Capabilities (BRIC)

Experiment Description: Determine how microgravity impacts the solidification of biobricks.

Why did you propose this experiment?

We have an ongoing project to design and build a machine that turns lunar or Martian soil into bricks, and we want to learn how reduced gravity will impact the process.

How will the experiment benefit humankind or future space exploration?

We are studying an environmentally-friendly concrete alternative that can be used to make structures on Earth and other planets out of on-site, readily available resources.

How have you worked together as a team during the pandemic?

We transitioned our weekly meetings to an online format so that we could continue at our planned pace while maintaining our community.

What science fiction character best represents your team and why?

Like our beloved childhood friend WALL-E, we craftily make inhospitable environments suitable for life with local resources.

University of Idaho

Team: Vandal Voyagers I

Experiment Title: Bacteria Resistant Polymers in Microgravity

Experiment Description: Determine how microgravity impacts the efficacy of bacteria resistant polymers.

Why did you propose this experiment?

The recent emphasis on surface sterility got us thinking about ways to reduce the risk of disease transmission by surfaces on the International Space Station.

How will the experiment benefit humankind or future space exploration?

If successful, the application of proposed polymers can benefit humankind by reducing transmission through high contact surfaces on and off Earth such as hand rails and door handles.

How have you worked together as a team during the pandemic?

We are allowed to work collaboratively in person given we follow the current university COVID guidelines.

What science fiction character best represents your team and why?

Mark Watney from The Martian because he is willing to troubleshoot and problem solve on his own while collaborating with NASA from afar.

University of New Hampshire at Manchester

Team: Team Cooke

Experiment Title: Novel Methods of Antibiotic Discovery in Space (NoMADS)

Experiment Description: Determine how microgravity impacts the amount of bacterium isolates that produce antibiotic metabolites.

Why did you propose this experiment?

To contribute to the limited body of knowledge regarding bacterial resistance and mutations in off-Earth conditions.

How will the experiment benefit humankind or future space exploration?

Understanding how bacteria in the human microbiome and on spacecraft surfaces change can ensure the safe and accurate treatment of bacterial infections in astronauts.

How have you worked together as a team during the pandemic?

Our team continued to evolve our communication methods throughout the pandemic, utilizing frequent remote video conferencing, telecommunications, email, and in-person conferences.

What science fiction character best represents your team and why?

Professor Xavier, the founder of the X-Men, because he also works with mutants and feels that while they are often misunderstood, under the right circumstances they can greatly benefit the world.

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