Is the earth really as beautiful as they say from space?
May the fifth be with you because history is about to be made: As early as May 5, 2018, we’re set to launch Mars InSight, the very first mission to study the deep interior of Mars. We’ve been roaming the surface of Mars for a while now, but when InSight lands on Nov. 26, 2018, we’re going in for a deeper look. Below, 10 things to know as we head to the heart of Mars.
Coverage of prelaunch and launch activities begins Thursday, May 3, on NASA Television and our homepage.
"Insight" is to see the inner nature of something, and the InSight lander—a.k.a. Interior Exploration using Seismic Investigations, Geodesy and Heat Transport—will do just that. InSight will take the "vital signs" of Mars: its pulse (seismology), temperature (heat flow) and reflexes (radio science). It will be the first thorough check-up since the planet formed 4.5 billion years ago.
You read that right: earthquakes, except on Mars. Scientists have seen a lot of evidence suggesting Mars has quakes, and InSight will try to detect marsquakes for the first time. By studying how seismic waves pass through the different layers of the planet (the crust, mantle and core), scientists can deduce the depths of these layers and what they're made of. In this way, seismology is like taking an X-ray of the interior of Mars.
Want to know more? Check out this one-minute video.
InSight is a Mars mission, but it’s also so much more than that. By studying the deep interior of Mars, we hope to learn how other rocky planets form. Earth and Mars were molded from the same primordial stuff more than 4.5 billion years ago, but then became quite different. Why didn’t they share the same fate? When it comes to rocky planets, we’ve only studied one in great detail: Earth. By comparing Earth's interior to that of Mars, InSight's team hopes to better understand our solar system. What they learn might even aid the search for Earth-like planets outside our solar system, narrowing down which ones might be able to support life.
InSight looks a bit like an oversized crane game: When it lands on Mars this November, its robotic arm will be used to grasp and move objects on another planet for the first time. And like any crane game, practice makes it easier to capture the prize.
Want to see what a Mars robot test lab is like? Take a 360 tour.
InSight will be traveling with a number of instruments, from cameras and antennas to the heat flow probe. Get up close and personal with each one in our instrument profiles.
InSight has three major parts that make up the spacecraft: Cruise Stage; Entry, Descent, and Landing System; and the Lander. Find out what each one does here.
Mars has weak sunlight because of its long distance from the Sun and a dusty, thin atmosphere. So InSight’s fan-like solar panels were specially designed to power InSight in this environment for at least one Martian year, or two Earth years.
Our scientists have found evidence that Mars’ crust is not as dense as previously thought, a clue that could help researchers better understand the Red Planet’s interior structure and evolution. “The crust is the end-result of everything that happened during a planet’s history, so a lower density could have important implications about Mars’ formation and evolution,” said Sander Goossens of our Goddard Space Flight Center in Greenbelt, Maryland.
InSight won’t be flying solo—it will have two microchips on board inscribed with more than 2.4 million names submitted by the public. "It's a fun way for the public to feel personally invested in the mission," said Bruce Banerdt of our Jet Propulsion Laboratory, the mission's principal investigator. "We're happy to have them along for the ride."
The rocket that will loft InSight beyond Earth will also launch a separate NASA technology experiment: two mini-spacecraft called Mars Cube One, or MarCO. These suitcase-sized CubeSats will fly on their own path to Mars behindInSight. Their goal is to test new miniaturized deep space communication equipment and, if the MarCOs make it to Mars, may relay back InSight data as it enters the Martian atmosphere and lands. This will be a first test of miniaturized CubeSat technology at another planet, which researchers hope can offer new capabilities to future missions.
Check out the full version of ‘Solar System: 10 Thing to Know This Week’ HERE.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.
What exactly happens to the human body during spaceflight? The Twins Study, a 340-day investigation conducted by NASA’s Human Research Program , sought to find answers. Scientists had an opportunity to see how conditions on the International Space Station translated to changes in gene expression by comparing identical twin astronauts: Scott Kelly who spent close to a year in space and Mark Kelly who remained on Earth.
From high above the skies, for almost a year, astronaut Scott Kelly periodically collected his own blood specimens for researchers on the ground during his One-Year Mission aboard the Space Station. These biological specimens made their way down to Earth onboard two separate SpaceX Dragon vehicles. A little bit of Scott returned to Earth each time and was studied by scientists across the United States.
Totaling 183 samples from Scott and his brother, Mark, these vials helped scientists understand the changes Scott’s body underwent while spending a prolonged stay in low Earth orbit.
Because identical twins share the same genetic makeup, they are very similar on a molecular level. Twin studies provide a way for scientists to explore how our health is impacted by the environment around us.
A significant finding is the variability in gene expression, which reflects how a body reacts to its environment and will help inform how gene expression is related to health risks associated with spaceflight. While in space, researchers observed changes in the expression of Scott’s genes, with the majority returning to normal after six months on Earth. However, a small percentage of genes related to the immune system and DNA repair did not return to baseline after his return to Earth. Further, the results identified key genes to target for use in monitoring the health of future astronauts and potentially developing personalized countermeasures.
Another key finding is that Scott’s immune system responded appropriately in space. For example, the flu vaccine administered in space worked exactly as it does on Earth. A fully functioning immune system during long-duration space missions is critical to protecting astronaut health from opportunistic microbes in the spacecraft environment.
Studying protein pathways in Scott enabled researchers to look at fluid regulation and fluid shifts within his body. Shifts in fluid may contribute to vision problems in astronauts. Scientists found a specific protein associated with fluid regulation was elevated in Scott, compared with his brother Mark on Earth.
The telomeres in Scott’s white blood cells, which are biomarkers of aging at the end of chromosomes, were unexpectedly longer in space then shorter after his return to Earth with average telomere length returning to normal six months later. In contrast, his brother’s telomeres remained stable throughout the entire period. Because telomeres are important for cellular genomic stability, additional studies on telomere dynamics are planned for future one-year missions to see whether results are repeatable for long-duration missions.
Scott Kelly participated in a series of cognitive performance evaluations (such as mental alertness, spatial orientation, and recognition of emotions) administered through a battery of tests and surveys. Researchers found that during spaceflight, Scott’s cognitive function remained normal for the first half of his stay onboard the space station compared to the second half of his spaceflight and to his brother, Mark, on the ground. However, upon landing, Scott’s speed and accuracy decreased. Re-exposure to Earth’s gravity and the dynamic experience of landing may have affected the results.
In studying various measurements on Scott, researchers found that his body mass decreased during flight, likely due to controlled nutrition and extensive exercise. While on his mission, Scott consumed about 30% less calories than researchers anticipated. An increase in his folate serum (vitamin B-9), likely due to an increase of the vitamin in his pre-packaged meals, was also noted by researchers. This is bolstered by the telomeres study, which suggests that proper nutrition and exercise help astronauts maintain health while in space.
Within five months of being aboard the space station, researchers found an increase in the thickness of Scott’s arterial wall, which may have been caused by inflammation and oxidative stress during spaceflight. Whether this change is reversible is yet to be determined. They hope these results will help them understand the stresses that the human cardiovascular system undergoes during spaceflight.
In addition, the results from the Microbiome, Epigenomics, and Integrative Omics studies suggest a human body is capable of adapting to and recovering from the spaceflight environment on a molecular level.
The data from the Twins Study Investigation will be explored for years to come as researchers report some interesting, surprising, and assuring data on how the human body is able to adapt to the extreme environment of spaceflight. This study gave us the first integrated molecular view into genetic changes, and demonstrated the plasticity and robustness of a human body!
We will use the valuable data to ensure the safety and health of the men and women who go on to missions to the Moon and on to Mars.
Learn more with this video about these fascinating discoveries!
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Ariana Grande got some space at N-A-S-A. Get yours too.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.
It’s the 50th anniversary of the Apollo 13 mission! NASA’s “successful failure,”Apollo 13 was to be the third lunar landing attempt, but the mission was aborted mid-flight after the rupture of a service module oxygen tank. The crew never landed on the moon, but due to the dedication and ingenuity of Mission Control, made it back to Earth safely. We’ve put some of the most important numbers of the Apollo 13 mission in perspective. Check it out!
Listen to the mission in real time, HERE.
Follow NASA History on Twitter and Facebook for more interesting information about aerospace history!
Check out the stats of all the Apollo Missions in the free e-book Apollo by the Numbers, HERE.
Right now, there are humans living and working off the Earth on the International Space Station. They orbit our planet from 250 miles above every 90 minutes, which means the crew sees 16 sunrises and sunsets every day.
If you’re in the right place, at the right time, the space station is visible to the naked eye. It looks like a fast-moving plane, only much higher and traveling thousands of miles an hour faster. The fact that it’s the third brightest object in the sky makes it easier to spot…if you know when to look up.
That’s where we can help! Our Spot the Station site allows you to enter your location and find out when the space station will be flying overhead. You can even sign up to receive alerts that will send you email or text messages to let you know when and where to look up.
Why is the space station visible? It reflects the light of the Sun, the same reason we can see the Moon. However, unlike the Moon, the space station isn’t bright enough to see during the day.
To find out when the space station is flying over your area, visit: http://spotthestation.nasa.gov/
Learn more about the International Space Station and the crew HERE.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
A former NASA intern, Deniz Burnham started her career as an engineer on an oil rig in Prudhoe Bay, Alaska, and went on to lead operations on drilling rigs in Canada, Ohio, and Texas. https://go.nasa.gov/3wDpfBo
Make sure to follow us on Tumblr for your regular dose of space!
NASA took over the White House Instagram today in honor of Astronomy Night to share some incredible views of the universe and the world around us. Check out more updates from the astronauts, scientists, and students on South Lawn.
Here’s a nighttime view of Washington, D.C. from the astronauts on the International Space Station on October 17. Can you spot the White House?
Check out this look at our sun taken by NASA’s Solar Dynamics Observatory. The SDO watches the sun constantly, and it captured this image of the sun emitting a mid-level solar flare on June 25. Solar flares are powerful bursts of radiation. Harmful radiation from a flare can’t pass through Earth’s atmosphere to physically affect humans on the ground. But when they’re intense enough, they can disturb the atmosphere in the layer where GPS and communications signals travel.
Next up is this incredible view of Saturn’s rings, seen in ultraviolet by NASA’s Cassini spacecraft. Hinting at the origin of the rings and their evolution, this ultraviolet view indicates that there’s more ice toward the outer part of the rings than in the inner part.
Take a look at the millions of galaxies that populate the patch of sky known as the COSMOS field, short for Cosmic Evolution Survey. A portion of the COSMOS field is seen here by NASA’s Spitzer Space Telescope. Even the smallest dots in this image are galaxies, some up to 12 billion light-years away. The picture is a combination of infrared data from Spitzer (red) and visible-light data (blue and green) from Japan’s Subaru telescope atop Mauna Kea in Hawaii. The brightest objects in the field are more than ten thousand times fainter than what you can see with the naked eye.
This incredible look at the Cat’s Eye nebula was taken from a composite of data from NASA’s Chandra X-ray Observatory and Hubble Space Telescope. This famous object is a so-called planetary nebula that represents a phase of stellar evolution that the Sun should experience several billion years from now. When a star like the Sun begins to run out of fuel, it becomes what is known as a red giant. In this phase, a star sheds some of its outer layers, eventually leaving behind a hot core that collapses to form a dense white dwarf star. A fast wind emanating from the hot core rams into the ejected atmosphere, pushes it outward, and creates the graceful filamentary structures seen with optical telescopes.
This view of the International Space Station is a composite of nine frames that captured the ISS transiting the moon at roughly five miles per second on August 2. The International Space Station is a unique place—a convergence of science, technology, and human innovation that demonstrates new technologies and makes research breakthroughs not possible on Earth. As the third brightest object in the sky, the International Space Station is easy to see if you know when to look up. You can sign up for alerts and get information on when the International Space Station flies over you at spotthestation.nasa.gov. Thanks for following along today as NASA shared the view from astronomy night at the White House. Remember to look up and stay curious!
The Japan Aerospace Exploration Agency H-IIB rocket is zooming toward the International Space Station carrying NASA’s Life Sciences Glovebox, a state-of-the-art microgravity research facility.
JAXA’s HTV3, taken during Expedition 32
NASA's Marshall Space Flight Center in Huntsville, Alabama, and their partners around the world are excited to initiate new, high-value biological research in low-Earth orbit.
The Japanese rocket, hauling the research facility and other cargo via the HTV-7 transfer vehicle, successfully lifted off at 1:52 p.m. EDT from Tanegashima Space Center off the coast of Japan.
Its launch marks a first for hauling bulky equipment to space. Roughly the size of a large fish tank, the Life Sciences Glovebox comes in at 26 inches high, 35 inches wide and 24 inches deep, with 15 cubic feet of available workspace.
"The Life Sciences Glovebox is on its way to the space station to enable a host of biological and physiological studies, including new research into microgravity's long-term impact on the human body," said Yancy Young, project manager at Marshall. "This versatile facility not only will help us better protect human explorers on long voyages into deep space, but it could aid medical and scientific advances benefiting the whole world."
Boeing engineers at Marshall modified a refrigerator-freezer rack to house the core facility, using state-of-the-art, 3D-printing technology to custom design key pieces of the rack to secure the unit in its protective foam clamshell.
NASA is now determining the roster of science investigations lined up to make use of the facility, beginning as early as late 2018. "We've already got more than a dozen glovebox experiments scheduled in 2019, with many more to follow," said Chris Butler, payload integration manager for the glovebox at Marshall.
The Life Sciences Glovebox will be transferred to a zero-gravity stowage rack in the station's Kibo module, where up to two crew members can conduct experiments simultaneously, overseen in real-time by project researchers on Earth.
Check out more pictures of the Glovebox HERE!
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.
And that’s a wrap! Thank you for all the great questions. We hope you learned a little bit about what it takes to work in mission control as a flight director.
If you’re hungry for more, you can read the latest installment of our First Woman graphic novel series, where fictional character Commander Callie Rodriguez embarks on the next phase of her trailblazing journey and leaves the Moon to take the helm at Mission Control.
Keep up with the flight directors, the Space Station, and the Artemis missions at the links below.
Flight directors: X
Artemis: Facebook: Facebook, Instagram, X
Space Station: Facebook, Instagram, X (@Space_Station), X( @ISS_Research)
Make sure to follow us on Tumblr for your regular dose of space!
This unprocessed image shows features in Saturn's atmosphere from closer than ever before. The view was captured by our Cassini spacecraft during its first Grand Finale dive between the planet and its rings on April 26, 2017.
As Cassini dove through the gap, it came within about 1,900 miles (3,000 kilometers) of Saturn's cloud tops (where the air pressure is 1 bar -- comparable to the atmospheric pressure of Earth at sea level) and within about 200 miles (300 kilometers) of the innermost visible edge of the rings.
See all the unprocessed images from Cassini: https://saturn.jpl.nasa.gov/galleries/raw-images/
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