You may remember that back in February, four crew members lived and worked inside our Human Research Exploration Analog (HERA). That crew, made up of 4 women, simulated a 715-day journey to a Near-Earth asteroid. Then in May, a second crew of 4 – this time, 4 men, launched on their simulated journey to that same asteroid. These 30 day missions help our researchers learn how isolation and close quarters affect individual and group behavior. Studies like this at our Johnson Space Center prepare us for long duration space missions, like a trip to an asteroid or even to Mars. We now have a third crew, living and working inside the HERA. This is the spacecraft’s 11th crew. The mission began on June 11, and will end on August 10.
The crew members are currently living inside this compact, science-making house. But unlike in a normal house, these inhabitants won’t go outside for 30 days. Their communication with the rest of planet Earth will also be very limited, and they won’t have any access to internet. The only people they will talk with regularly are mission control and each other.
The HERA XI crew is made up of 3 men and 1 woman selected from the Johnson Space Center Test Subject Screening (TSS) pool. The crew member selection process is based on a number of criteria, including the same criteria for astronaut selection. The four would-be astronauts are:
• Tess Caswell
• Kyle Foster
• Daniel Surber
• Emmanuel Urquieta
What will they be doing?
The crew will test hardware prototypes to get “the bugs worked out” before they are used in off-Earth missions. They will conduct experiments involving plants, brine shrimp, and creating a piece of equipment with a 3D printer. After their visit to an asteroid, the crew will simulate the processing of soil and rocks they collected virtually. Researchers outside of the spacecraft will collect data regarding team dynamics, conflict resolution and the effects of extended isolation and confinement.
How real is a HERA mission?
When we set up an analog research investigation, we try to mimic as many of the spaceflight conditions as we can. This simulation means that even when communicating with mission control, there will be a delay on all communications ranging from 1 to 5 minutes each way, depending on how far their simulated spacecraft is from Earth.
Obviously we are not in microgravity, so none of the effects of microgravity on the human or the vehicle can be tested. You can simulate isolation to a great degree – although the crew knows they are note really isolated from humanity, the communications delays and ban from social media help them to suspend reality. We emulate confinement and the stress that goes along with it.
Scientists and researchers use analogs like HERA to gather more data for comparison to data collected aboard the space station and from other analogs so they can draw conclusions needed for a real mission to deep space, and one day for a journey to Mars.
A few other details:
The crew follows a timeline that is similar to one used for the ISS crew.
They work 16 hours a day, Monday through Friday. This includes time for daily planning, conferences, meals and exercises.
They will be growing and taking care of plants and brine shrimp, which they will analyze and document.
Past HERA crew members wore a sensor that recorded heart rate, distance, motion and sound intensity. When crew members were working together, the sensor would also record their proximity as well, helping investigators learn about team cohesion.
Researchers also learned about how crew members react to stress by recording and analyzing verbal interactions and by analyzing “markers” in blood and saliva samples.
As with the 2 earlier missions this year, this mission will include 22 individual investigations across key human research elements. From psychological to physiological experiments, the crew members will help prepare us for future missions.
Want a full, 360 degree look at HERA? Check out and explore the inside of the habitat.
For more information on our Human Research Program, visit: www.nasa.gov/hrp.
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Astronaut Scott Kelly returned home from his year in space mission on March 1. Spending that much time in space allowed him to rack up some pretty cool milestones. Here are some of his awesome “firsts”:
While in space, Scott Kelly had the opportunity to host the first NASA TweetChat from space.
The first ever Tumblr AnswerTime from space was hosted by Scott Kelly during his One Year Mission.
Scott Kelly hosted the first NASA Reddit AMA from space.
Before leaving for his year in space, President Obama asked him to Instagram his time on orbit…a Presidential request to Instagram is a first!
During his year in space, Scott conducted his first spacewalk. He hadn’t spacewalked on any of his previous missions, but did so three times during the One Year Mission.
Most notably, Scott Kelly is the first U.S. astronaut to spend a year in space. His time on orbit also allowed us to conduct the first ever Twins Study on the space station. While Scott was in space, his twin brother Mark Kelly was on Earth. Since their genetic makeup is as close to identical as we can get, this allows a unique research perspective. We can now compare all of the results from Scott in space to his brother Mark on Earth.
During his year in space, Scott had the opportunity to be one of the first astronauts to harvest and eat lettuce grown in the space station’s VEGGIE facility.
Space flowers! Scott was also one of the firsts to help grow and harvest zinnia flowers in the VEGGIE facility. Growing flowering plants in space will help scientists learn more about growing crops for deep-space missions and our journey to Mars.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
What does it feel like to float?? Do you have trouble adjusting to walking on the earth after that ??
What was your favourite NASA mission or project?
Follow our Mars 2020 rover, named Perseverance or “Percy,” on Twitter to keep up with all its progress and discoveries!
Percy: https://twitter.com/NASAPersevere
People always say that space is a vacuum. That’s true – space is about a thousand times emptier than even the best laboratory vacuums on Earth. Even so, space contains lots of stuff we can’t see. We study this invisible space stuff because we need to understand it to safely send technology and astronauts into space.
The stuff that fills space is mostly plasma, which is gas where particles have separated into positive ions and negative electrons, creating a sea of electrically-charged particles. This plasma also contains something else – magnetic fields.
The particles in space can reach very high speeds, creating radiation. One of the main engines that drives that acceleration to high speeds is called magnetic reconnection. But what is magnetic reconnection?
Magnetic reconnection happens when two oppositely-aligned magnetic fields pinch together and explosively realign. As the lines snap into their new configuration – as in the animation below – the sudden change sends electrons and ions flying at incredible speeds.
Magnetic reconnection releases energy. We can't see the energy itself, but we can see the results: It can set off solar explosions – such as solar flares and coronal mass ejections – or disturbances near Earth that cause auroras.
In March 2015, we launched the four Magnetospheric Multiscale, or MMS, spacecraft on a mission to study magnetic reconnection. Magnetic reconnection only happens in a vacuum with ionized gas. These conditions are vanishingly rare on Earth, so we went to space to study this explosive process.
Because MMS has four separate – but essentially identical – spacecraft, it can watch magnetic reconnection in three dimensions.
The below animation shows what MMS sees – the magnetic fields are magenta, positive ions are purple, and electrons are yellow. The arrows show which the direction the fields and particles are moving.
Like how a research plane flies through a hurricane, MMS flew directly through a magnetic reconnection event in October 2015.
In the data visualization below, you can see the magnetic reconnection happening as the yellow arrows (which represent electrons) explode in all directions. You’ll notice that the magnetic field (represented by magenta arrows) changes direction after the magnetic reconnection, showing that the magnetic field has reconfigured.
Magnetic reconnection transfers energy into Earth’s atmosphere – but it’s not inherently dangerous. Sometimes, the changes in Earth’s magnetic field caused by magnetic reconnection can create electric currents that put a strain on power systems. However, the energy released is more often channeled into auroras, the multicolored lights that most often appear near the North and South Poles.
As the MMS mission continues the four spacecraft can be moved closer together or farther apart, letting us measure magnetic reconnection on all different scales. Each set of observations contributes to explaining different aspects of this invisible phenomenon of magnetic reconnection. Together, the information will help scientists better map out our space environment — crucial information as we journey ever farther beyond our home planet.
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You are seeing the culmination of almost twenty years of rain and snow, all at once.
For the first time, we have combined and remastered the satellite measurements from two of our precipitation spacecraft to create our most detailed picture of our planet’s rain and snowfall. This new record will help scientists better understand normal and extreme rain and snowfall around the world and how these weather events may change in a warming climate.
Using this new two-decade record, we can see the most extreme places on Earth.
The wettest places on our planet occur over oceans. These extremely wet locations tend to be very concentrated and over small regions.
A region off the coast of Indonesia receives on average 279 inches of rain per year.
An area off the coast of Colombia sees on average 360 inches of rain per year.
The driest places on Earth are more widespread. Two of the driest places on Earth are also next to cold ocean waters. In these parts of the ocean, it rains as little as it does in the desert -- they’re also known as ocean deserts!
Just two thousand miles to the south of Colombia is one of the driest areas, the Atacama Desert in Chile that receives on average 0.64 inches of rain per year.
Across the Atlantic Ocean, Namibia experiences on average 0.49 inches of rain a year and Egypt gets on average 0.04 inches of rain per year.
As we move from January to December, we can see the seasons shift across the world.
During the summer in the Northern Hemisphere, massive monsoons move over India and Southeast Asia.
We can also see dynamic swirling patterns in the Southern Ocean, which scientists consider one of our planet’s last great unknowns.
This new record also reveals typical patterns of rain and snow at different times of the day -- a pattern known as the diurnal cycle.
As the Sun heats up Earth’s surface during the day, rainfall occurs over land. In Florida, sea breezes from the Gulf of Mexico and Atlantic Ocean feed the storms causing them to peak in the afternoon. At night, storms move over the ocean.
In the winter months in the U.S. west coast, the coastal regions generally receive similar amounts of rain and snow throughout the day. Here, precipitation is driven less from the daily heating of the Sun and more from the Pacific Ocean bringing in atmospheric rivers -- corridors of intense water vapor in the atmosphere.
This new record marks a major milestone in the effort to generate a long-term record of rain and snow. Not only does this long record improve our understanding of rain and snow as our planet changes, but it is a vital tool for other agencies and researchers to understand and predict floods, landslides, disease outbreaks and agricultural production.
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Sit back, relax, and get ready to learn some science and engineering! Experts Sarah Stewart Johnson and Lauren DuCharme are here to talk about the July 30 launch of our Perseverance mission, women in STEM, and much more.
Our Answer Time starts now!
What led you to this job? (what’s your degree in/what are your passions)
It’s only Tuesday and this week is already filled with news about our solar system. Here are the top five things to know this week:
1) Mars!
With five spacecraft in orbit and two rovers exploring the ground, there’s always something new and interesting about the Red Planet. Yesterday things got even more exciting when we released the most compelling evidence yet that liquid water sometimes flows on Mars today.
2) HTV-5 Cargo Ship
On Monday, the HTV-5 cargo ship was released from the International Space Station to burn up as it reenters Earth’s atmosphere. The HTV-5 carried a variety of experiments and supplies to the space station, and was docked for five weeks.
3) Pluto Continues to Excite
If you haven’t been keeping up with the weekly releases of newly downloaded pictures from our New Horizons spacecraft, you are definitely missing out. But don’t worry, we have you covered. The latest updates can be found HERE, be sure to follow along as new information is released. More images are scheduled to be featured on Oct. 1.
4) Cassini Mission
This week on Sept. 30, our Cassini spacecraft will reach the closest point to Saturn in it’s latest orbit around the planet. Just to put things in perspective, that will be Cassini’s 222nd orbit around Saturn! Learn more about this mission HERE.
5) What Happened to Mars’ Atmosphere?
Believe it or not, the Martian atmosphere we see today used to be much more substantial many years ago. What happened? Our Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft has been in orbit around Mars for one Earth year, searching for the answers. Learn more HERE.
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A human journey to Mars, at first glance, offers an inexhaustible amount of complexities. To bring a mission to the Red Planet from fiction to fact, NASA’s Human Research Program has organized some of the hazards astronauts will encounter on a continual basis into five classifications.
A spacecraft is not only a home, it’s also a machine. NASA understands that the ecosystem inside a vehicle plays a big role in everyday astronaut life.
Important habitability factors include temperature, pressure, lighting, noise, and quantity of space. It’s essential that astronauts are getting the requisite food, sleep and exercise needed to stay healthy and happy. The space environment introduces challenges not faced on Earth.
Technology, as often is the case with out-of-this-world exploration, comes to the rescue! Technology plays a big role in creating a habitable home in a harsh environment and monitoring some of the environmental conditions.
Astronauts are also asked to provide feedback about their living environment, including physical impressions and sensations so that the evolution of spacecraft can continue addressing the needs of humans in space.
Exploration to the Moon and Mars will expose astronauts to five known hazards of spaceflight, including hostile and closed environments, like the closed environment of the vehicle itself. To learn more, and find out what NASA’s Human Research Program is doing to protect humans in space, check out the "Hazards of Human Spaceflight" website. Or, check out this week’s episode of “Houston We Have a Podcast,” in which host Gary Jordan further dives into the threat of hostile and closed environments with Brian Crucian, NASA immunologist at the Johnson Space Center.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.
as flight directors, you are in charge of a lot of the operations, but do you ever get to experience handling controls or zero gravity simulation? do you have to know every aspect of everyone's job?
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