This 30 day mission will help our researchers learn how isolation and close quarters affect individual and group behavior. This study at our Johnson Space Center prepares us for long duration space missions, like a trip to an asteroid or even to Mars.
The Human Research Exploration Analog (HERA) that the crew members will be living in is one 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. So no checking social media kids!
The only people they will talk with regularly are mission control and each other.
The crew member selection process is based on a number of criteria, including the same criteria for astronaut selection.
What will they be doing?
Because this mission simulates a 715-day journey to a Near-Earth asteroid, the four crew members will complete activities similar to what would happen during an outbound transit, on location at the asteroid, and the return transit phases of a mission (just in a bit of an accelerated timeframe). This simulation means that even when communicating with mission control, there will be a delay on all communications ranging from 1 to 10 minutes each way. The crew will also perform virtual spacewalk missions once they reach their destination, where they will inspect the asteroid and collect samples from it.
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.
But beware! While we do all we can to avoid crises during missions, crews need to be able to respond in the event of an emergency. The HERA crew will conduct a couple of emergency scenario simulations, including one that will require them to maneuver through a debris field during the Earth-bound phase of the mission.
Throughout the mission, researchers will gather information about cohabitation, teamwork, team cohesion, mood, performance and overall well-being. The crew members will be tracked by numerous devices that each capture different types of data.
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.
In total, this mission will include 19 individual investigations across key human research elements. From psychological to physiological experiments, the crew members will help prepare us for future missions.
Mission success! After a simulated mission to an asteroid, the crew “splashed down” around 10:30 p.m. EST on Wednesday, Feb. 24 and exited the habitat for the first time in 30 days.
Want a full, 360 degree look at HERA? Check out and explore the inside of the habitat.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Does space have a standard time or do you rely on the time zones on Earth while you are in space?
Great question. Really it is up to the particular space agency/mission which time zone they use. For example, since the International Space Station is a collaboration between NASA, the Russian Space Agency, the European Space Agency, the Japanese Space Agency, and the Canadian Space Agency, we came up with the compromise of operating on Greenwich Mean Time (GMT). So, Space Station time is the same as London time! The International Space Station orbits our planet every 90 minutes, so of course we’re transiting across multiple time zones constantly.
A quiet, starry night sky might not seem like a very eerie spectacle, but space can be a creepy place! Monsters lurk in the shadowy depths of the universe, sometimes hidden in plain sight. Many of them are invisible to our eyes, so we have to use special telescopes to see them. Read on to discover some of these strange cosmic beasts, but beware — sometimes fact is scarier than fiction.
You know those nightmares where no matter how fast you try to run you never seem to get anywhere? Black holes are a sinister possible version of that dream — especially because they’re real! If you get too close to a black hole, there is no possibility of escape.
Just last year our Fermi Gamma-ray Space Telescope traced an otherworldly ghost particle back to one of these monster black holes, providing additional insight into the many signals we’re picking up from some of the most feared creatures in the cosmic deep.
But it gets worse. Our Hubble Space Telescope revealed that these things are hidden in the hearts of nearly every galaxy in the universe. That means supermassive black holes lurk in the shadows of the night sky in every direction you look!
This fiendish specter lives in the center of the Milky Way, haunting our galaxy’s supermassive black hole. But it’s not as scary as it looks! Our SOFIA observatory captured streamlines tracing a magnetic field that appears to be luring most of the material quietly into orbit around the black hole. In other galaxies, magnetic fields seem to be feeding material into hungry black holes — beware! Magnetic fields might be the answer to why some black holes are starving while others are feasting.
The universe has bats in the attic! Hubble spotted the shadow of a giant cosmic bat in the Serpens Nebula. Newborn stars like the one at the center of the bat, called HBC 672, are surrounded by disks of material, which are hard to study directly. The shadows they cast, like the bat, can clue scientists in on things like the disk’s size and density. Our solar system formed from the same type of disk of material, but we can only see the end result of planet building here — we want to learn more about the process!
A jack-o-lantern in space?! Our Solar Dynamics Observatory watches the Sun at all times, keeping a close eye on space weather. In October 2014, the observatory captured a chilling image of the Sun with a Halloweenish face!
On Halloween a few years ago, an eerie-looking object known as 2015 TB145 sped across the night sky. Scientists observing it with our Infrared Telescope Facility determined that it was most likely a dead comet. It’s important to study objects like comets and asteroids because they’re dangerous if they cross Earth’s path — just ask the dinosaurs!
Trick-or-treat! Add a piece of glowing cosmic candy to your Halloween haul, courtesy of Hubble! This image shows the Saturn Nebula, formed from the outer layers ejected by a dying star, destined to be recycled into later generations of stars and planets. Our Sun will experience a similar fate in around five billion years.
Massive stars are in for a more fiery fate, as the Witch's Broom Nebula shows. Hubble’s close-up look reveals wisps of gas — shrapnel leftover from a supernova explosion. Astronomers believe that a couple of supernovae occur each century in galaxies like our own Milky Way.
Supernovae usually herald the death of a star, but on a few occasions astronomers have found “zombie stars” left behind after unusually weak supernovae. Our Nuclear Spectroscopic Telescope Array (NuSTAR) has even spotted a mysterious glow of high-energy X-rays that could be the “howls” of dead stars as they feed on their neighbors.
The universe is brimming with galaxies, but it’s also speckled with some enormous empty pockets of space, too. These giant ghost towns, called voids, may be some of the largest things in the cosmos, and since the universe is expanding, galaxies are racing even farther away from each other all the time! Be grateful for your place in space — the shadowy patches of the universe are dreadful lonely scenes.
Some forces are a lot creepier than floorboards creaking or a door slamming shut unexpectedly when you’re home alone. Dark energy is a mysterious antigravity pressure that our Wide Field Infrared Survey Telescope (WFIRST) is going to help us understand. All we know so far is that it’s present everywhere in the cosmos (even in the room with you as you read this) and it controls the fate of the universe, but WFIRST will study hundreds of millions of galaxies to figure out just what dark energy is up to.
Want to learn some fun ways to celebrate Halloween in (NASA) style? Check out this link!
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Artists of all kinds were invited to apply for the chance to visit our Goddard Space Flight Center to be inspired by the giant, golden, fully-assembled James Webb Space Telescope mirror.
Art/Photo Credit: Jedidiah Dore
Webb has a mirror that is nearly 22 feet high and (to optimize it for infrared observations) is covered in a microscopic layer of actual gold.
Art/Photo Credit: Susan Lin
Because of Webb’s visually striking appearance, the project hosted a special viewing event on Wednesday, Nov. 2, 2016.
Photo Credit: Maggie Masetti
There was an overwhelming response to the event invitation and ultimately twenty-four people were selected to attend. They represented a broad range of artistic media and styles, including: watercolor, 3D printed sculpture, silk screening, acrylics, sumi-e (East Asian brush technique), comics, letterpress, woodwork, metalwork, jewelry making, fiber art, ink, mural painting, kite-making, tattooing, scientific illustration, poetry, songwriting, and video making.
Art/Photo Credit: Sue Reno
Project scientists and engineers spoke with visitors to give context to what they were seeing and explain why Webb is an engineering marvel, and how it will change our view of the universe.
Among other things, Webb will see the first stars and galaxies that formed in the early universe and help us to better understand how planetary systems form and evolve. It will help us answer questions about who we, as humans, are and where we came from.
Art Credit: Jessica Lee Photo Credit: Maggie Masetti
The artists spent several hours sitting right in front of the telescope, where they sketched, painted, took photos and even filmed a music video.
Art Credit: Joanna Barnum Photo Credit: Maggie Masetti
While some of the pieces of art are finished, most of the artists went home with their heads full of ideas and sketchbooks full of notes. Stay tuned for more info on where you can see their final works displayed!
Art/Photo Credit: Susan Lin
Finished art from the event continues to be added HERE.
The James Webb Space Telescope is finishing environmental testing at our Goddard Space Flight Center in Greenbelt, Maryland. Next it will head to our Johnson Space Center in Houston for an end-to-end test at cryogenic temperatures. After that, it goes to Northrop Grumman to be mated with the giant tennis court-sized sunshield and the spacecraft bus. The observatory will launch in October of 2018 from a European Space Agency (ESA) launch site in French Guiana, aboard an Ariane 5 rocket. Webb is a collaboration of NASA, ESA, and the Canadian Space Agency (CSA).
Follow Webb on Facebook, Twitter and Instagram.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Today is College Signing Day and we’re working with the White House to celebrate all graduating seniors and inspire more young people to Reach Higher and enroll in higher education.
Additionally, choosing a degree within a STEM (Science, Math, Engineering and Technology) field enables the United States to remain the global economic and technological leader. We feel that it’s our duty to help inspire the next generation of scientists, technologists, engineers and astronauts.
It’s important that each and every student feels empowered and equipped with the knowledge to solve tough problems, evaluate evidence and analyze information. These are all skills students can learn through studying a subjects in STEM.
College is one of the stepping stones to many careers, including becoming an astronaut! Here are a few of our astronauts on their college graduation day, along with their astronaut portrait.
Undergraduate: California Polytechnic State University Graduate: Air University and Naval Postgraduate School Astronaut Class: 2013
Undergraduate: Rensselaer Polytechnic Institute Graduate: Johns hopkins University Astronaut Class: 2009
Undergraduate: Davidson College Graduate: University of Virginia, Wake Forest University and University of Texas medical Branch Astronaut Class: 2004
Undergraduate: University of North Dakota Graduate: University of Texas at Austin Astronaut Class: 2000
Undergraduate: Washington University Graduate: California Institute of Technology Astronaut Class: 2000
Undergraduate: Iowa Wesleyan College Graduate: Rice University Astronaut Class: 1996
Undergraduate: University of California Graduate: University of Arizona Astronaut Class: 2004
Undergraduate: University of California, Berkeley Graduate: University of Houston Astronaut Class: 1996
Here, Administrator Bolden wears the jersey of Keenan Reynolds, a scholar athlete who graduates from the Naval Academy this year. His jersey is on its way to the college football hall of fame. Bolden holds a drawing of himself as a midshipman in the Navy.
Deputy Administrator Dava Newman sports her college shirt, along with Lisa Guerra, Technical Assistant to the Associate Administrator. Both women studied aerospace engineering at Notre Dame.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Science in the field gets even more delightful. Two different missions are in the field right now, studying snow and how it affects communities around the country.
From our Wallops Flight Facility in Virginia, the IMPACTS mission is flying up and down the East Coast, investigating how snow forms inside clouds. In Grand Mesa, Colorado, SnowEx’s teams on the ground and in the air are taking a close look at how much water is stored in snow.
Hate going out in the storm? The IMPACTS mission can help with that! IMPACTS uses two planes – a P-3 Orion and an ER-2 – flying through and high above the clouds to study where intense bands of snowfall form. Better understanding where intense snow will fall can improve forecast models down the road — helping prepare communities for snowstorms.
Cameras mounted on the wings of the P3 took microscopic images of snowflakes, like this one.
At the same time, the SnowEx team is in Colorado, studying the depth and density of snow. Researchers are making radar spirals with snowmobiles and working in giant snow pits to measure things like snow water equivalent, or how much water is stored in snow.
SnowEx is helping us better understand snow’s role in ecosystems and human systems, like irrigation for agriculture. If you want to bring some corn for popping, SnowEx’s science can help grow that crop.
Follow along with our teams as they brave the cold and snow: https://twitter.com/nasaexpeditions
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
What aspect of spaceflight always blows your mind, even after all this time?
1. NASA-Funded Research
It’s all just a click way with the launch of a new public access site, which reflects our ongoing commitment to provide public access to science data.
Start Exploring!
2. Red Planet Reconnaissance
One of the top places in our solar system to look for signs of past or current life is Mars. Through our robotic missions, we have been on and around Mars for 40 years. These orbiters, landers and rovers are paving the way for human exploration.
Meet the Mars robots
3. Three Moons and a Planet that Could Have Alien Life
In a presentation at TED Talks Live, our director of planetary science, Jim Green, discusses the best places to look for alien life in our solar system.
Watch the talk
4. Setting Free a Dragon
Tune in to NASA TV on Friday, Aug. 26 at 5:45 a.m. EDT for coverage of the release of the SpaceX Dragon CRS-9 cargo ship from the International Space Station.
Watch live
5. Anniversary Ring(s)
Aug. 26 marks 35 years since Voyager probe flew by Saturn, delighting scientists with rich data and images. Today, thanks to our Cassini spacecraft, we know much more about the ringed planet.
Learn more about Cassini’s mission to Saturn
Learn more about Voyager 2
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Twenty-five years ago, an object roughly the size of an oven made space history when it plunged into the clouds of Jupiter, the largest planet in our solar system. On Dec. 7, 1995, the 750-pound Galileo probe became the first probe to enter the gas giant. Traveling at a blistering speed of 106,000 miles per hour, the probe’s protective heat shield experienced temperatures as hot as the Sun’s surface generated by friction during entry. As the probe parachuted through Jupiter’s dense atmosphere, its science instruments made measurements of the planet’s chemical and physical makeup. The probe collected data for nearly an hour before its signal was lost. Its data was transmitted to Earth via the Galileo spacecraft, an orbiter that carried the probe to Jupiter and stayed within contact during the encounter. Learn more about the mission.
The Galileo probe was managed by NASA’s Ames Research Center in California’s Silicon Valley.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
There are many paths to a career at NASA. Here are 10 amazing people on the frontlines of deep space exploration.
“I was running a pub in the North of England after dropping out of college, and as fate would have it, I met a lovely American physics lecturer Dr. Jim Gotaas,” said Abi Rymer (shown above in the bottom right of the group photo). Abi works on the Europa Clipper mission.
“I was sold on a course he ran on Observational Astronomy and Instrumentation at the University of Central Lancashire in Preston, Lancashire and I went from there to join the second year of the Physics and Astronomy at Royal Holloway, part of London University. I loved theoretical physics but never imagined I was talented enough to do a PhD. When I graduated, I was shocked to be top of the year.”
“Within seven months of being at NASA’s Jet Propulsion Laboratory,” says Brent Buffington, a mission design manager, “I figured out we could modify the Cassini Prime Mission trajectory to fly very close to the moon Tethys—a moon that didn’t have any close flybys in the original Prime Mission—and simultaneously lower a planned 621-mile (1,000-kilometer) targeted flyby of Hyperion down to 311 miles (500 kilometers). To be this young buck fresh out of grad school standing in front of a room full of seasoned engineers and scientists, trying to convince them that this was the right thing to do with a multi-billion dollar asset, and ultimately getting the trajectory modification approved was extremely rewarding.”
“Geochemical evidence suggests that between 4 and 2.5 billion years ago, there may have been an intermittent haze in the atmosphere of Earth similar to the haze in the atmosphere of Saturn’s moon Titan,” says astrobiologist Giada Arney. “It's a really alien phase of Earth's history —our planet wouldn't have been a pale blue dot, it would have been a pale orange dot. We thought about questions like: What would our planet look like if you were looking at it as an exoplanet? How you might infer biosignatures—the signs of life—from looking at such an alien planet?”
“I spent the summer after graduating from studying Mars' remnant magnetic field in the Planetary Magnetospheres Lab at NASA Goddard Space Flight Center,” says planetary geophysicist Lynnae Quick. “My advisor, Mario Acuña, showed me how to bring up Mars Global Surveyor (MGS) images of the Martian surface on my computer. This was the first time I'd ever laid eyes, firsthand, on images of another planet's surface returned from a spacecraft. I remember just being in awe.
“My second favorite moment has to be pouring over mosaics of Europa and learning to identify and map chaos regions, impact craters and other surface units during my first summer at APL. Once again, I felt that there was a whole other alien world at my fingertips.”
“A few months after NASA was formed I was asked if I knew anyone who would like to set up a program in space astronomy,” says Nancy Roman, a retired NASA astronomer. “I knew that taking on this responsibility would mean that I could no longer do research, but the challenge of formulating a program from scratch that I believed would influence astronomy for decades to come was too great to resist.”
“I took Planetary Surfaces with Bruce Murray (whom I later found out had been JPL’s fifth director) and did a presentation on Europa's chaos terrains,” say Serina Diniega, an investigation scientist on the Europa Clipper mission. “I was fascinated to learn about the different models proposed for the formation of these enigmatic features and the way in which scientists tried to discriminate between the models while having very limited observational data. In this, I realized I’d found my application: modeling the evolution of planetary landforms."
“I admire people who dedicate themselves 110 percent to what they do,” says Warren Kaye, a software engineer. “People like the recently deceased Stephen Hawking, who rose above his own physical limitations to develop new scientific theories, or Frank Zappa, who was able to produce something like 50 albums worth of music over a 20-year span.”
“I got to pick what the camera took pictures of in a given week, and then analyze those pictures from the standpoint of a geologist,” says Tanya Harrison, a planetary scientist. “There aren't many people in the world who get paid to take pictures of Mars every day! Seeing the first images...It was almost surreal -- not only are you picking what to take pictures of on Mars, you're also typically the first person on Earth to see those pictures when they come back from Mars.”
As a child, what did you want to be when you grew up?
“A scientist,” says Casey Lisse, a scientist on our New Horizons mission to Pluto and the Kuiper Belt.
At what point did you determine that you would become a scientist?
“Age 5.”
“Throughout my life, I’ve gone from being an extremely shy introvert to more of an outgoing extrovert,” says science writer Elizabeth Landau. “It’s been a gradual uphill climb. I used to be super shy. When I was really young, I felt like I didn't know how to talk to other kids. I was amazed by how people fluidly spoke to each other without thinking too hard about it, without appearing to have any kind of embarrassment or reservation about what they were saying. I've definitely developed confidence over time—now I can very quickly and comfortably switch from talking about something like physics to personal matters, and be totally open to listening to others as well.”
Check out the full version of “Solar System: 10 Things to Know This Week” HERE.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.
The total solar eclipse on August 21 will trace a narrow path across the nation, although most of the U.S. will see a partial eclipse. Here's what to do before, during and after the eclipse, plus how you can become a citizen scientist helping us with eclipse observations.
Not everyone can travel to the path of totality, so here are some things you can do whether you see totality or a partial eclipse.
Want to be a citizen scientist?
Before the eclipse, make and pack your very own eclipse toolkit, containing a notebook, pen, a clock, a stopwatch, the front page of a newspaper, a thermometer, and a stick with a piece of crepe paper tied to it. Don’t forget your assistant, who will help conduct science observations.
Practice using a citizen scientist phone app, like our GLOBE app to study clouds, air and surface temperatures and other observations. Go to the location where you plan to observe the eclipse and check for any obstructions. You may want to focus on only one activity as the eclipse will last less than 3 minutes ... or just really experience the eclipse.
Cell phones don’t take eclipse video! And plan to have your safe eclipse-viewing glasses within reach for before and after totality. Just before totality, if you have a good view of the horizon, look west to see the approaching shadow. After totality, look east low on the horizon for the departing shadow.
During totality, look for stars. You should be able to see the star Regulus in the solar corona or the stars of Orion.
During totality, we may see moving bands of shadows, like on the bottom of a swimming pool.
How dark does it get at totality? Look at the newspaper you brought with you. What is the smallest print you can read?
How much does the temperature drop? Does the wind stop or change direction?
Use your hands, a sheet of paper with a hole in it, a kitchen colander or any other object with one or more holes to use as a pinhole projector. You’ll be able to see the crescent shape of the sun projected through the holes.
Find out more about the eclipse, including eclipse safety, at https://eclipse2017.nasa.gov
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Explore the universe and discover our home planet with the official NASA Tumblr account
1K posts