Today, we revealed the four astronauts who will fly around the Moon during the Artemis II mission, scheduled to launch in 2024. Get to know them:
Meet the first member of our Artemis II crew: mission specialist Christina Koch. Koch visited the International Space Station in 2019, where she participated in the first all-woman spacewalk with Jessica Meir. She began her NASA career as an electrical engineer at Goddard Space Flight Center.
Representing the Canadian Space Agency is Jeremy Hansen from London, Ontario. Col. Hansen was a fighter pilot with Canadian Armed Forces before joining the Canadian Space Agency, and currently works with NASA on astronaut training and mission operations. This will be Col. Hansen’s first mission in space.
Victor Glover is our Artemis II pilot. Glover is part of our 2013 class of NASA astronauts and was the pilot for NASA’s SpaceX Crew-1 mission. He’s logged 3,000 flight hours in more than 40 different aircraft.
...and rounding out our Artemis II crew: mission commander Reid Wiseman. Wiseman lived and worked aboard the International Space Station as a flight engineer in 2014. He also commanded the undersea research mission NEEMO21, and most recently served as Chief of the NASA astronauts.
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Astronauts train all over the world, including at Johnson Space Center. Here, they learn not just how to live aboard the International Space Station, but also how to conduct science in microgravity.
Astronauts serve as the eyes and hands of researchers while their experiments are in space, so they must be trained in everything from using a microscope, to maintaining the equipment for combustion experiments.
Check out this week’s episode of NASA Explorers as we go to class with an astronaut.
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Location: In the constellation Ursa Major
Type: Flocculent spiral galaxy
Discovered by: William Herschel
NGC 2841 is a beautiful example of a flocculent spiral galaxy – a type with discontinuous, featherlike, and patchy arms. A bright cusp of starlight distinguishes the galaxy's center from the dust lanes that outline the group of almost white middle-aged stars. The far younger blue stars trace the spiral arms.
Find out more information about NGC 2841 here.
Right now, the Hubble Space Telescope is exploring #GalaxiesGalore! Find more galaxy content and spectacular new images by following along on Hubble’s Twitter, Facebook, and Instagram.
Credit: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration; Acknowledgment: M. Crockett and S. Kaviraj (Oxford University, UK), R. O'Connell (University of Virginia), B. Whitmore (STScI), and the WFC3 Scientific Oversight Committee
What type of planning goes into ensuring a successful launch, and how easily is it decided?
This dwarf planet sure knows how to get a BIG reaction because we’re stunned by the latest images from our New Horizons spacecraft!
Back on July 14, the spacecraft completed it’s historic Pluto flyby, and is now in an intensive downlink phase. During this time, New Horizons will send us some of the best data and images we’ve seen!
These latest images were taken just 15 minutes after New Horizons’ closest approach to Pluto. The spacecraft looked back toward the sun and captured this near-sunset view. Icy mountains, flat plains and the horizon can all be seen in detail.
When we take a closer look, these features truly begin to stand out. Mountains up to 11,000 feet high are met by flat icy plains that extend out to Pluto’s horizon. There, more than a dozen layers of haze in the dwarf planet’s atmosphere can be seen. It’s almost as if we’re flying over the surface with the New Horizons spacecraft.
Speaking of flyover, this new animation of Pluto has been created from images returned from the spacecraft this month. This view shows us what it might be like to take an aerial tour through Pluto’s thin atmosphere and soar above the surface.
These images and videos are not only stunning, but also provide us with important information about the dwarf planet. So far, scientists can tell that the weather changes from day to day on Pluto. These images, combined with others that have been downloaded, provide evidence for a remarkably Earth-like “hydrological” cycle on Pluto.
For updates on the data and images received by the New Horizons spacecraft, check our blog: https://blogs.nasa.gov/pluto/
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Happy #MoonDay! To celebrate the 49th anniversary of Apollo 11 landing on the Moon, we present you with “Moonlight,” a video by our Goddard science visualizer Ernie Wright set to Debussy’s Clair de Lune. The Apollo missions were a landmark in lunar exploration. The visit and the samples that our Moon walkers collected transformed our understanding of the Moon and the solar system. Now, our Lunar Reconnaissance Orbiter’s high-resolution data gives an incredibly detailed view of our closest neighbor.
This visualization captures the mood of Claude Debussy's best-known composition, Clair de Lune (which means moonlight in French). The piece was published in 1905 as the third of four movements in the composer's Suite Bergamasque, and unlike the other parts of this work, Clair is quiet, contemplative, and slightly melancholy, evoking the feeling of a solitary walk through a moonlit garden.
“Moonlight” uses a digital 3D model of the Moon built from Lunar Reconnaissance Orbiter global elevation maps and image mosaics. The lighting is derived from actual Sun angles during lunar days in 2018. Enjoy and read more HERE.
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This is what it would look like if you were training to #BeAnAstronaut! Astronaut candidates must train for two years before they become official NASA astronauts. After graduation, you can look forward to more skill building when training for upcoming missions. Let’s dive into some of the courses you can expect once you’re selected for the job:
All astronaut candidates must learn to safely operate in a T-38 jet, either as a pilot or crew. Because this is the one area of their training that is not a simulation and involves decisions with life or death consequences, it teaches them to think quickly and clearly in dynamic situations.
Geology training courses are specially tailored to the work astronauts will do from the International Space Station or on the next interplanetary mission! Astronauts learn the basic principles of geology, see rocks in their natural environment and handle samples from their class discussions. It’s less like memorizing the names of rocks and more like learning how geologists think and work.
Before they end up in space, astronauts carry out a significant portion of their training in aircraft on Earth. It's unlikely, but possible, that one of those training planes could crash in a remote area and leave the humans on board to fend for themselves for a while. Knowing how to take care of their basic needs would be invaluable. Through the exercises, instructors hope to instill self-care and self-management skills, to develop teamwork skills, and to strengthen leadership abilities – all of which are valuable for working in the isolation of the wild or the isolation of space.
Astronauts participate in a variety of extreme environment training to prepare for the stresses of spaceflight. Pictured here, they are exploring the underground system of the Sa Grutta caves in Sardinia, Italy as a part of the European Astronaut Centre’s Cooperative Adventure for Valuing and Exercising human behavior and performance Skills (CAVES) expedition. Seasoned astronauts as well as rookies participate in the course and share experiences while learning how to improve leadership, teamwork, decision-making and problem-solving skills.
In our Virtual Reality Laboratory training facility at Johnson Space Center astronauts are able to immerse themselves in virtual reality to complete mission tasks and robotic operations before launching to space. The facility provides real time graphics and motion simulators integrated with a tendon-driven robotic device to provide the kinesthetic sensation of the mass and inertia characteristics of any large object (<500lb) being handled.
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With tumultuous winds peaking at 400 mph, the Great Red Spot has been swirling wildly over Jupiter’s skies for at least 150 years and possibly much longer. People saw a big spot on Jupiter as early as the 1600s when they started stargazing through telescopes, though it’s unclear whether they were looking at a different storm. Today, scientists know the Great Red Spot has been there for a while, but what causes its swirl of reddish hues remains to be discovered. More >
Despite its unofficial name, the Little Red Spot is about as wide as Earth. The storm reached its current size when three smaller spots collided and merged in the year 2000. More >
The planet’s rings might get most of the glory, but another shape’s been competing for attention: the hexagon. This jet stream is home to a massive hurricane tightly centered on the north pole, with an eye about 50 times larger than the average hurricane eye on Earth. Numerous small vortices spin clockwise while the hexagon and hurricane spin counterclockwise. The biggest of these vortices, seen near the lower right corner of the hexagon and appearing whitish, spans about 2,200 miles, approximately twice the size of the largest hurricane on Earth. More>
A tempest erupted in 2010, extending approximately 9,000 miles north-south large enough to eventually eat its own tail before petering out. The storm raged for 200 days, making it the longest-lasting, planet-encircling storm ever seen on Saturn. More >
Better cover your eyes. Dust storms are a frequent guest on the Red Planet, but one dust storm in 2001 larger by far than any seen on Earth raised a cloud of dust that engulfed the entire planet for three months. As the Sun warmed the airborne dust, the upper atmospheric temperature rose by about 80 degrees Fahrenheit. More >
Several large, dark spots on Neptune are similar to Jupiter’s hurricane-like storms. The largest spot, named the “Great Dark Spot” by its discoverers, contains a storm big enough for Earth to fit neatly inside. And, it looks to be an anticyclone similar to Jupiter’s Great Red Spot. More >
Not to be confused with Earth’s tornadoes, a stalk-like prominence rose up above the Sun, then split into about four strands that twisted themselves into a knot and dispersed over a two-hour period. This close-up shows the effect is one of airy gracefulness. More >
The storm blew across the equatorial region of Titan, creating large effects in the form of dark and likely “wet” from liquid hydrocarbons areas on the surface of the moon. The part of the storm visible here measures 750 miles in length east-to-west. The wings of the storm that trail off to the northwest and southwest from the easternmost point of the storm are each 930 miles long. More >
On March 9, 1989, a huge cloud of solar material exploded from the sun, twisting toward Earth. When this cloud of magnetized solar material called a coronal mass ejection reached our planet, it set off a chain of events in near-Earth space that ultimately knocked out an entire power grid area to the Canadian province Quebec for nine hours. More >
Back on Earth, Typhoon Tip of 1979 remains the biggest storm to ever hit our planet, making landfall in Japan. The tropical cyclone saw sustained winds peak at 190 mph and the diameter of circulation spanned approximately 1,380 miles. Fortunately, we now have plans to better predict future storms on Earth. NASA recently launched a new fleet of hurricane-tracking satellites, known as the Cyclone Global Navigation Satellite System (CYGNSS), which will use the same GPS technology you and I use in our cars to measure wind speed and ultimately improve how to track and forecast hurricanes. More >
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When humans launch to the International Space Station, they are members of expeditions. An expedition is long duration stay on the space station. The first expedition started when the crew docked to the station on Nov. 2, 2000.
Expedition 52 began in June 2017 aboard the orbiting laboratory and will end in September 2017.
FUN FACT: Each Expedition begins with the undocking of the spacecraft carrying the departing crew from the previous Expedition. So Expedition 52 began with the undocking of the Soyuz MS-03 spacecraft that brought Expedition 51 crew members Oleg Novitskiy and Thomas Pesquet back to Earth, leaving NASA astronauts Peggy Whitson and Jack Fischer and Roscosmos cosmonaut Fyodor Yurchikhin aboard the station to await the arrival of the rest of the Expedition 52 crew in July.
This expedition includes dozens of out of this world science investigations and a crew that takes #SquadGoals to a whole new level.
Take a look below to get to know the crew members and some of the science that will occur during the space station’s 52nd expedition.
Born: Batumi, Adjar ASSR, Georgian SSR Interests: collecting stamps and space logos, sports, history of cosmonautics and reading Spaceflights: STS-112, Exps. 15, 24/25, 36/37, 51 Bio: https://go.nasa.gov/2o9PO9F
Born: Louisville, Colorado. Interests: spending time with my family, flying, camping, traveling and construction Spaceflights: Expedition 51 Twitter: @Astro2Fish Bio: https://go.nasa.gov/2o9FY7o
Born: Mount Ayr, Iowa Interests: weightlifting, biking, basketball and water skiing Spaceflights: STS-111, STS – 113, Exps. 5, 16, 50, 51, 52 Twitter: @AstroPeggy Bio: https://go.nasa.gov/2rpL58x
Born: Fort Knox, Kentucky Interests: travel, music, photography, weight training, sports, scuba diving, motorcycling, and flying warbirds Spaceflights: STS-129 and STS-135 Twitter: @AstroKomrade Bio: https://go.nasa.gov/2rq5Ssm
Born: Moscow, Soviet Union Interests: Numismatics, playing the guitar, tourism, sport games Spaceflights: Exps. 37/38 Twitter: @Ryazanskiy_ISS Bio: https://go.nasa.gov/2rpXfOK
Born: Milan, Italy Interests: scuba diving, piloting aircraft, assembling computer hardware, electronic equipment and computer software Spaceflights: STS-120, Exps. 26/27 Bio: https://go.nasa.gov/2rq0tlk
In addition to one tentatively planned spacewalk, crew members will conduct scientific investigations that will demonstrate more efficient solar arrays, study the physics of neutron stars, study a new drug to fight osteoporosis and study the adverse effects of prolonged exposure to microgravity on the heart.
Roll-Out Solar Array (ROSA)
Solar panels are an efficient way to generate power, but they can be delicate and large when used to power a spacecraft or satellites. They are often tightly stowed for launch and then must be unfolded when the spacecraft reaches orbit.
The Roll-Out Solar Array (ROSA), is a solar panel concept that is lighter and stores more compactly for launch than the rigid solar panels currently in use. ROSA has solar cells on a flexible blanket and a framework that rolls out like a tape measure.
Neutron Star Interior Composition Explored (NICER)
Neutron stars, the glowing cinders left behind when massive stars explode as supernovas, are the densest objects in the universe, and contain exotic states of matter that are impossible to replicate in any ground lab.
The Neutron Star Interior Composition Explored (NICER) payload, affixed to the exterior of the space station, studies the physics of these stars, providing new insight into their nature and behavior.
Systemic Therapy of NELL-1 for Osteoporosis (Rodent Research-5)
When people and animals spend extended periods of time in space, they experience bone density loss. The Systemic Therapy of NELL-1 for osteoporosis (Rodent Research-5) investigation tests a new drug that can both rebuild bone and block further bone loss, improving health for crew members.
Fruit Fly Lab-02
Exposure to reduced gravity environments can result in cardiovascular changes such as fluid shifts, changes in total blood volume, heartbeat and heart rhythm irregularities, and diminished aerobic capacity. The Fruit Fly Lab-02 study will use the fruit fly (Drosophila melanogaster) to better understand the underlying mechanisms responsible for the adverse effects of prolonged exposure to microgravity on the heart.
Watch their progress HERE!
Our planet is shown surrounded by an imaginary constellation shaped like a house, depicting the theme of the patch: “The Earth is our home.” It is our precious cradle, to be preserved for all future generations. The house of stars just touches the Moon, acknowledging the first steps we have already taken there, while Mars is not far away, just beyond the International Space Station, symbolized by the Roman numeral “LII,” signifying the expedition number.
The planets Saturn and Jupiter, seen orbiting farther away, symbolize humanity’s exploration of deeper space, which will begin soon. A small Sputnik is seen circling the Earth on the same orbit with the space station, bridging the beginning of our cosmic quest till now: Expedition 52 will launch in 2017, sixty years after that first satellite. Two groups of crew names signify the pair of Soyuz vehicles that will launch the astronauts of Expedition 52 to the Station.
Click here for more details about the expedition and follow @ISS_Research on Twitter to stay up to date on the science happening aboard YOUR orbiting laboratory!
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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.
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Jack Hathaway, a distinguished naval aviator, was born and raised in South Windsor, Connecticut. An Eagle Scout, Hathaway volunteers as an assistant scoutmaster for the Boy Scouts. https://go.nasa.gov/4bU8QbI
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