Work continued aboard the International Space Station. Spacewalkers Shane Kimbrough and Peggy Whitson used the station’s robotic arm to move the Pressurized Mating Adapter-3 on March 24 to move a module to accommodate U.S. commercial spacecraft carrying astronauts on future missions. They continued this work on March 30. Another spacewalk to complete the work is slated for April.
Engineers at our Goddard Space Flight Center Center complete vibration and acoustic tesing on the James Webb Space Telescope, which was subjected to earsplitting noice and shaken 50-100 times per second to simulate the rigors of launch.
Data from our MAVEN, our Mars Atmosphere and Volatile EvolutioN, and published in the journal Science, concludes that solar wind and radiation are responsible for stripping Mars of its atmosphere and turning it into the frigid desert world it is today.
Most of the gas ever in the Red Planet’s atmosphere has been lost to space. The MAVEN team focused on the gas argon, estimating that 65% of it has been stripped from the planet. In 2015, the science team determined that atmospheric gas continues to be lost to space.
We participated in a Women’s History Month celebration and the Smithsonian Air and Space Museum. The program feature NASA astronauts and engineers. The were also projects to get girls interested in sciene, technology, engineering and math, or STEM, education. There was also a screening of the film ‘Hidden Figures,’ which relates the story of African-American female mathematicians who were instrumental in the agency’s efforts to launch humans to space.
We’ve released our latest free NASA app on a whole new platform--Amazon Fire TV! The app is already available for Apple TV, iOS, and Android.Viewers can stream NASA TV, access 16,000+, download video and more!
Download the app: www.nasa.gov/nasaapp
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In July 2015, we saw Pluto up close for the first time and—after three years of intense study—the surprises keep coming. “It’s clear,” says Jeffery Moore, New Horizons’ geology team lead, “Pluto is one of the most amazing and complex objects in our solar system.”
These are combined observations of Pluto over the course of several decades. The first frame is a digital zoom-in on Pluto as it appeared upon its discovery by Clyde Tombaugh in 1930. More frames show of Pluto as seen by the Hubble Space Telescope. The final sequence zooms in to a close-up frame of Pluto taken by our New Horizons spacecraft on July 14, 2015.
Pluto’s surface sports a remarkable range of subtle colors are enhanced in this view to a rainbow of pale blues, yellows, oranges, and deep reds. Many landforms have their own distinct colors, telling a complex geological and climatological story that scientists have only just begun to decode. The image resolves details and colors on scales as small as 0.8 miles (1.3 kilometers). Zoom in on the full resolution image on a larger screen to fully appreciate the complexity of Pluto’s surface features.
July 14, 2015: New Horizons team members Cristina Dalle Ore, Alissa Earle and Rick Binzel react to seeing the spacecraft's last and sharpest image of Pluto before closest approach.
Just 15 minutes after its closest approach to Pluto, the New Horizons spacecraft captured this near-sunset view of the rugged, icy mountains and flat ice plains extending to Pluto's horizon. The backlighting highlights more than a dozen layers of haze in Pluto's tenuous atmosphere. The image was taken from a distance of 11,000 miles (18,000 kilometers) to Pluto; the scene is 780 miles (1,250 kilometers) wide.
Found near the mountains that encircle Pluto’s Sputnik Planitia plain, newly discovered ridges appear to have formed out of particles of methane ice as small as grains of sand, arranged into dunes by wind from the nearby mountains.
The vast nitrogen ice plains of Pluto’s Sputnik Planitia – the western half of Pluto’s “heart”—continue to give up secrets. Scientists processed images of Sputnik Planitia to bring out intricate, never-before-seen patterns in the surface textures of these glacial plains.
High resolution images of Pluto’s largest moon, Charon, show a surprisingly complex and violent history. Scientists expected Charon to be a monotonous, crater-battered world; instead, they found a landscape covered with mountains, canyons, landslides, surface-color variations and more.
One of two potential cryovolcanoes spotted on the surface of Pluto by the New Horizons spacecraft. This feature, known as Wright Mons, was informally named by the New Horizons team in honor of the Wright brothers. At about 90 miles (150 kilometers) across and 2.5 miles (4 kilometers) high, this feature is enormous. If it is in fact an ice volcano, as suspected, it would be the largest such feature discovered in the outer solar system.
Pluto's receding crescent as seen by New Horizons at a distance of 120,000 miles (200,000 kilometers). Scientists believe the spectacular blue haze is a photochemical smog resulting from the action of sunlight on methane and other molecules in Pluto's atmosphere. These hydrocarbons accumulate into small haze particles, which scatter blue sunlight—the same process that can make haze appear bluish on Earth.
On Jan. 1, 2019, New Horizons will fly past a small Kuiper Belt Object named MU69 (nicknamed Ultima Thule)—a billion miles (1.5 billion kilometers) beyond Pluto and more than four billion miles (6.5 billion kilometers) from Earth. It will be the most distant encounter of an object in history—so far—and the second time New Horizons has revealed never-before-seen landscapes.
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Ever get a random craving for a food when in space?
Over the course of several days, observatories and amateur astronomers will be able to spot the spacecraft. Below, 10 things to know about this incredible mission that will bring us the largest sample returned from space since the Apollo era.
OSIRIS-REx seeks answers to the questions that are central to the human experience: Where did we come from? What is our destiny? Asteroids, the leftover debris from the solar system formation process, can help us answer these questions and teach us about the history of the Sun and planets.
Yup. OSIRIS-REx stands for the Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer spacecraft. The gist: It will rendezvous with, study, and return a sample of the asteroid Bennu to Earth.
While all the acronyms for each instrument may be alphabet soup, each has a job/role to perform in order to complete the mission. Explore what each one will do in this interactive webpage.
Scientists chose Bennu as the mission target because of its composition, size, and proximity to Earth. Bennu is a rare B-type asteroid (primitive and carbon-rich), which is expected to have organic compounds and water-bearing minerals like clays.
Bennu had a tough life in a rough neighborhood: the early solar system. It's an asteroid the size of a small mountain born from the rubble of a violent collision, hurled through space for millions of years and dismembered by the gravity of planets—but that's exactly what makes it a fascinating destination.
In 2018, OSIRIS-REx will approach Bennu and begin an intricate dance with the asteroid, mapping and studying Bennu in preparation for sample collection. In July 2020, the spacecraft will perform a daring maneuver in which its 11-foot arm will reach out for a five-second "high-five" to stir up surface material, collecting at least 2 ounces (60 grams) of small rocks and dust into a sample return capsule.
OSIRIS-REx launched on September 8, 2016 from Cape Canaveral, Florida on an Atlas V rocket. In March 2021, the window for departure from the asteroid will open and OSIRIS-REx will begin its return journey to Earth, arriving two-and-a-half years later in September 2023.
The sample will head to Earth inside of a return capsule with a heat shield and parachutes that will separate from the spacecraft once it enters the Earth's atmosphere. The capsule containing the sample will be collected at the Utah Test and Training Range. Once it arrives, it will be transported to NASA's Johnson Space Center in Houston for examination. For two years after the sample return (from late 2023-2025) the science team will catalog the sample and conduct the analysis needed to meet the mission science goals. NASA will preserve at least 75% of the sample at NASA's Johnson Space Flight Center in Houston for further research by scientists worldwide, including future generations of scientists.
Analyzing the sample will help scientists understand the early solar system, as well as the hazards and resources of near-Earth space. Asteroids are remnants of the building blocks that formed the planets and enabled life. Those like Bennu contain natural resources such as water, organics and metals. Future space exploration and economic development may rely on asteroids for these materials.
Journey with OSIRIS-REx as it launches, cruises, and arrives to Bennu in this interactive timeline.
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Our Human Research Program is conducting a Twins Study on retired twin astronauts Scott and Mark Kelly. The study began during Scott Kelly’s One-Year Mission, which encompassed International Space Station Expeditions 43, 44, 45 and 46.
Now that Scott has returned from space, researchers are integrating data as well as taking measurements on Earth from the twins. This is the first time we have conducted Omics research on identical twins. Omics is a broad area of biological and molecular studies that, in general, means the study of the entire complement of biomolecules, like proteins; metabolites or genes.
Comparing various types of molecular information on identical individuals while one undergoes unique stresses, follows a defined diet, and resides in microgravity to one who resides on Earth, with gravity, should yield interesting results. It is hoped one day that all individuals will have access to having their Omics profiles done. This is a first step towards personalizing medicine for astronauts and hopefully for the rest of us.
For background, check out NASA’s Omics video series at https://www.nasa.gov/twins-study.
Kjell Lindgren, M.D., NASA astronaut, Expedition 44/45 Flight Engineer and medical officer
Susan M. Bailey, Ph.D., Twins Study Principal Investigator, Professor, Radiation Cancer Biology & Oncology, Department of Environmental and Radiological Health Sciences, College of Veterinary Medicine & Biomedical Sciences, Colorado State University
Christopher E. Mason, Ph.D., Twins Study Principal Investigator, WorldQuant Foundations Scholar, Affiliate Fellow of Genomics, Ethics, and Law, ISP, Yale Law School, Associate Professor, Department of Physiology and Biophysics, Weill Cornell Medicine
Brinda Rana, Ph.D., Associate Professor, Department of Psychiatry, University of California San Diego School of Medicine
Michael P. Snyder, Ph.D., M.D., FACS, Twins Study Principal Investigator, Stanford W. Ascherman, Professor in Genetics, Chair, Dept. of Genetics, Director, Center for Genomics and Personalized Medicine, Stanford School of Medicine
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📣 Attention, space explorers! Our Nancy Grace Roman Space Telescope presents: two new coloring pages! Unleash your creativity to bring these celestial scenes to life.
Nancy Grace Roman, NASA’s first chief astronomer, smiles out at us from our first coloring page. She’s considered the mother of our Hubble Space Telescope because she helped everyone understand why it was important to have observatories in space – not just on the ground. If it weren’t for her, Hubble may have never become a reality.
The Roman Space Telescope is named after her to honor the legacy she left behind when she died in 2018. Thanks to Nancy Grace Roman, we’ve taken countless pictures of space from orbiting telescopes and learned so much more about the universe than we could have possibly known otherwise!
The second coloring page illustrates some of the exciting science topics the Roman Space Telescope will explore. Set to launch in the mid-2020s, the mission will view the universe in infrared light, which is like using heat vision. We’ll be able to peer through clouds of dust and see things that are much farther away.
We anticipate all kinds of discoveries from the edge of our solar system to the farthest reaches of space. This coloring page highlights a few of the things the Roman Space Telescope will help us learn more about. The mission will find thousands of planets beyond our solar system and hundreds of millions of galaxies. It will also help us unravel the mysteries of dark matter and dark energy, represented by the gray web-like pattern in the background. With so much exciting new data, who knows what else we may learn?
Download the coloring pages here!
Learn more about the Roman Space Telescope at: https://roman.gsfc.nasa.gov/
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Here are a few things you should know about our solar system this week:
1. Beyond Pluto
The principle investigator for the New Horizons mission reports that the spacecraft is healthy and has recently completed the halfway point in its long download of 50-plus gigabits of data about the Pluto system. Now, the New Horizons team has submitted a proposal to continue the exploration. Find out more HERE.
2. A Planet of Particular Importance
April 22 is Earth Day, and we’re deeply involved in studying and understanding how to protect our one and only home world. Join us for a #24Seven celebration of Earth Day. Learn more about our missions to Earth HERE.
3. It’s True — All of It
Sci-fi meets real space exploration when BB8 the droid gets to know Maggie, the engineering model for the Mars Curiosity rover, in a short video produced by some of the people behind Star Wars. Take a look HERE. Photo credit: LucasFilm
4. Bringing Home a Piece of the Sky
Did you know that we’re planning to bring part of an asteroid to Earth? The ambitious OSIRIS-REx mission, which will retrieve a sample from the asteroid Bennu, is slated for launch later this year.
5. Catch Them — If You Can
The best time to view the Lyrids meteor shower will be just before dawn on April 23, when the constellation Lyra is overhead and the moon will be near to setting. Be aware, however, that this year the light of the full moon will make them harder to spot. Find out what else is up in this month’s night skies HERE.
Want to learn more? Read our full list of things to know this week about the solar system HERE.
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With its blue skies, puffy white clouds, warm beaches and abundant life, planet Earth is a pretty special place. A quick survey of the solar system reveals nothing else like it. But how special is Earth, really?
One way to find out is to look for other worlds like ours elsewhere in the galaxy. Astronomers using our Kepler Space Telescope and other observatories have been doing just that!
In recent years they’ve been finding other planets increasingly similar to Earth, but still none that appear as hospitable as our home world. For those researchers, the search goes on.
Another group of researchers have taken on an entirely different approach. Instead of looking for Earth-like planets, they’ve been looking for Earth-like ingredients. Consider the following:
Our planet is rich in elements such as carbon, oxygen, iron, magnesium, silicon and sulfur…the stuff of rocks, air, oceans and life. Are these elements widespread elsewhere in the universe?
To find out, a team of astronomers led by the Japanese Aerospace Exploration Agency (JAXA), with our participation, used Suzaku. This Japanese X-ray satellite was used to survey a cluster of galaxies located in the direction of the constellation Virgo.
The Virgo cluster is a massive swarm of more than 2,000 galaxies, many similar in appearance to our own Milky Way, located about 54 million light years away. The space between the member galaxies is filled with a diffuse gas, so hot that it glows in X-rays. Instruments onboard Suzaku were able to look at that gas and determine which elements it’s made of.
Reporting their findings in the Astrophysical Journal Letters, they reported findings of iron, magnesium, silicon and sulfur throughout the Virgo galaxy cluster. The elemental ratios are constant throughout the entire volume of the cluster, and roughly consistent with the composition of the sun and most of the stars in our own galaxy.
When the Universe was born in the Big Bang 13.8 billon years ago, elements heavier than carbon were rare. These elements are present today, mainly because of supernova explosions.
Massive stars cook elements such as, carbon, oxygen, iron, magnesium, silicon and sulfur in their hot cores and then spew them far and wide when the stars explode.
According to the observations of Suzaku, the ingredients for making sun-like stars and Earth-like planets have been scattered far and wide by these explosions. Indeed, they appear to be widespread in the cosmos. The elements so important to life on Earth are available on average and in similar relative proportions throughout the bulk of the universe. In other words, the chemical requirements for life are common.
Earth is still special, but according to Suzaku, there might be other special places too. Suzaku recently completed its highly successful mission.
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Did you miss it? Astronaut Scott Kelly answered questions over the weekend on People Magazine’s Facebook page! Anything and everything from his favorite food in space to his year aboard the International Space Station.
Here are a few highlights from the conversation:
Follow Astronaut Scott Kelly during the remainder of his year in space: Facebook, Twitter, Instagram
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Not since 1977 has a full moon dawned in the skies on Christmas. But this year, a bright full moon will be an added gift for the holidays.
This full moon, the last of the year, is called the Full Cold Moon because it occurs during the beginning of winter.
Make sure you get outside to check out this rare event because it won’t happen again until 2034!
Here are a few fun facts about the event and our moon:
The moon’s peak this year will occur at 6:11 a.m. EST
As you gaze up at the Christmas moon, take note that we have a spacecraft currently orbiting Earth’s moon. Our Lunar Reconnaissance Orbiter (LRO) mission has been investigating the lunar surface since 2009
More than 100 spacecraft have been launched to explore the moon
Our moon is the only celestial body beyond Earth that has been visited by human beings..so far!
Twelve human beings have walked on the surface of the moon
The moon makes a complete orbit around Earth in 27 Earth days and rotates or spins at the same rate. This causes the moon to keep the same side, or face, towards Earth during the course of its orbit
The moon is the brightest and largest feature in the night sky. Venus is second
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Peering deep into the core of the Crab Nebula, this close-up image reveals the beating heart of one of the most historic and intensively studied remnants of a supernova, an exploding star. The inner region sends out clock-like pulses of radiation and tsunamis of charged particles embedded in magnetic fields.
The neutron star at the very center of the Crab Nebula has about the same mass as the sun but compressed into an incredibly dense sphere that is only a few miles across. Spinning 30 times a second, the neutron star shoots out detectable beams of energy that make it look like it's pulsating.
The Hubble Space Telescope snapshot is centered on the region around the neutron star (the rightmost of the two bright stars near the center of this image) and the expanding, tattered, filamentary debris surrounding it. Hubble's sharp view captures the intricate details of glowing gas, shown in red, that forms a swirling medley of cavities and filaments. Inside this shell is a ghostly blue glow that is radiation given off by electrons spiraling at nearly the speed of light in the powerful magnetic field around the crushed stellar core.
Read more about this image HERE.
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