After exceeding her 90-day mission and design parameters many times over, our plucky little rover Opportunity turns 13 years old on the Red Planet. She’s officially a teenager!
The public contributes so much wonderful art that we decided to make a place to share it. Enjoy!
Our Juno spacecraft recently got a closer look at Jupiter’s Little Red Spot. The craft’s JunoCam imager snapped this shot of Jupiter's northern latitudes on December 2016, as the spacecraft performed a close flyby of the gas giant. The spacecraft was at an altitude of 10,300 miles above Jupiter's cloud tops.
A simple chemistry method could vastly enhance how scientists search for signs of life on other planets. The test uses a liquid-based technique known as capillary electrophoresis to separate a mixture of organic molecules into its components. It was designed specifically to analyze for amino acids, the structural building blocks of all life on Earth.
Our NEOWISE mission recently discovered some celestial objects traveling through our neighborhood, including one on the blurry line between asteroid and comet. An object called 2016 WF9 was detected by the NEOWISE project in November 2016 and it's in an orbit that takes it on a scenic tour of our solar system. A different object, discovered by NEOWISE a month earlier, is more clearly a comet, releasing dust as it nears the sun.
Discover the full list of 10 things to know about our solar system this week HERE.
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Pew. Pew. Lasers in space!
Iconic movie franchises like Star Wars and Star Trek feature futuristic laser technologies, but space lasers aren’t limited to the realm of science fiction. In fact, laser communications technologies are changing the way missions transmit their data. The Laser Communications Relay Demonstration (LCRD) blasts into space this weekend, demonstrating the unique – and totally awesome – capabilities of laser communications systems.
Currently, NASA missions rely on radio frequency to send data to Earth. While radio has served the agency well since the earliest days of spaceflight, there are significant benefits to laser systems. Just as the internet has gone from dial-up to high-speed connections, lasers communications’ higher frequency allows missions to send much more information per second than radio systems. With laser communications, it would only take nine days to transmit a complete map of Mars back to Earth, compared to nine weeks with radio frequency systems.
LCRD will demonstrate these enhanced capabilities from 22,000 miles above Earth’s surface. And although the mission uses lasers, these lasers are not visible to the human eye. Once in orbit, the mission will perform experiments using two telescopes on Earth that will relay data through the spacecraft from one site to the other over an optical communications link. These experiments will help NASA and the aerospace community understand the operational challenges of using lasers to communicate to and from space.
On Earth, there are ground stations telescopes that will capture LCRD’s laser signal and send the data to the mission operations center in New Mexico. The two ground stations are located on Haleakalā, Hawaii and Table Mountain, California. These picturesque locations weren’t chosen because they’re beautiful, but rather for their mostly clear skies. Clouds – and other atmospheric disturbances – can disrupt laser signals. However, when those locations do get cloudy, we’ve developed corrective technologies to ensure we receive and successfully decode signals from LCRD.
This demonstration will help NASA, researchers, and space companies learn more about potential future applications for laser communications technologies. In the next few years, NASA will launch additional laser missions to the Moon on Artemis II and to the asteroid belt, even deeper into space. These missions will give us insight on the use of laser communications further in space than ever before.
Ultimately, laser systems will allow us to glean more information from space. This means more galaxy pics, videos of deep space phenomena, and live, 4K videos from astronauts living and working in space.
Laser communications = more data in less time = more discoveries.
If laser communications interests you, check out our Space Communications and Navigation (SCaN) Internship Project. This program provides high school, undergrad, graduate, and even Ph.D. candidates with internship opportunities in space communications areas – like laser comm.
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On Monday, August 21, 2017, our nation will be treated to a total eclipse of the Sun. The eclipse will be visible – weather permitting – across all of North America. The entire continent will experience at least a partial eclipse lasting two to three hours. Halfway through the event, anyone within a 60 to 70 mile-wide path from Oregon to South Carolina will experience a total eclipse. During those brief moments when the moon completely blocks the Sun's bright face for 2+ minutes, day will turn into night, making visible the otherwise hidden solar corona, the Sun's outer atmosphere. Bright stars and planets will become visible as well. This is truly one of nature's most awesome sights. The eclipse provides a unique opportunity to study the Sun, Earth, Moon and their interaction because of the eclipse's long path over land coast to coast.
Scientists will be able to take ground-based and airborne observations over a period of about 90 minutes to complement the wealth of data provided by NASA assets.
Watch this and other eclipse videos on our YouTube channel: https://youtu.be/8jaxiha8-rY?list=PL_8hVmWnP_O2oVpjXjd_5De4EalioxAUi
To learn all about the 2017 Total Eclipse: https://eclipse2017.nasa.gov/
Music credit: Ascending Lanterns by Philip Hochstrate
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Ten years ago, on March 6, 2009, a rocket lifted off a launch pad at Cape Canaveral Air Force Station in Florida. It carried a passenger that would revolutionize our understanding of our place in the cosmos--NASA’s first planet hunter, the Kepler space telescope. The spacecraft spent more than nine years in orbit around the Sun, collecting an unprecedented dataset for science that revealed our galaxy is teeming with planets. It found planets that are in some ways similar to Earth, raising the prospects for life elsewhere in the cosmos, and stunned the world with many other first-of-a-kind discoveries. Here are five facts about the Kepler space telescope that will blow you away:
NASA retired the Kepler spacecraft in 2018. But to this day, researchers continue to mine its archive of data, uncovering new worlds.
*All images are artist illustrations. Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
There’s a lot of historical and archived space footage on the internet and we’re excited to see that the public (you!) have taken it to create many other products that teach people about exploration, space and our universe. Among those products are GIFs. Those quick videos that help you express what you’re trying to say via text, or make you laugh while surfing the web.
Are space GIFs the new cat videos of the internet? Don’t know, but we sure do like them!
This GIF of the Cat Eye Nebula shows it in various wavelengths…
Followed by a GIF of a cat in space…floating in front of the Antennae galaxies...
One time, a frog actually photobombed the launch of our LADEE spacecraft…someone on the internet gave him a parachute…
Want to see what it’s like to play soccer in space? There’s a GIF for that…
There are also some beautiful GIFs looking through the Cupola window on the International Space Station…
This warped footage from the International Space Station gives us ride around the Earth…
While this one encourages us to explore the unknown...
When our New Horizons spacecraft flew by dwarf planet Pluto in 2015, the internet couldn’t get enough of the Pluto GIFs...
Want to use our GIFs?! You can! Our GIFs are accessible directly from the Twitter app. Just tap or click the GIF button in the Twitter tool bar, search for NASAGIF, and all NASA GIFs will appear for sharing and tweeting. Enjoy!
GIF Sources
Cat Eye GIF: https://giphy.com/gifs/astronomy-cZpDWjSlKjWPm Cat GIF: https://giphy.com/gifs/cat-HopYL0SamcCli Frog GIF: https://giphy.com/gifs/nasa-photo-rocket-NOsCSDT2rUgfK Soccer GIF: https://giphy.com/gifs/yahoo-astronauts-zerogravity-QF1ZomA11zofC Cupola 1 GIF: https://giphy.com/gifs/nasa-Mcoxp6TgvQm6A Cupola 2 GIF: https://giphy.com/gifs/timelapse-space-11f3o8D2rQWzCM Earth GIF: http://giphy.com/gifs/earth-milky-way-international-space-station-ONC6WgECm5KEw Explore GIF: https://giphy.com/gifs/text-timelapse-lapse-Vj7gwAvhgsDYs Pluto 1 GIF: https://giphy.com/gifs/l46CzjUnYFfeMXiNO Pluto 2 GIF: https://giphy.com/gifs/pluto-dbV1LkFWWob84
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What's a SPOC? Isn't that a star trek character?
How visible will the stars be compared to a normal night sky if I'm in the path of totality? (Sun completely covered)
I’m not entirely sure, but you will be able to see some stars that you normally wouldn’t see. https://eclipse2017.nasa.gov/sites/default/files/publications/Eclipse_brochure-bookmark_508.pdf In fact, during the 1919 eclipse, Sir Arthur Eddington and others used our ability to see stars close to the Sun during the eclipse to help confirm Einstines’ theory of general relativity. https://eclipse2017.nasa.gov/testing-general-relativity
“At a glacial pace” used to mean moving so slowly the movement is almost imperceptible. Lately though, glaciers are moving faster. Ice on land is melting and flowing, sending water to the oceans, where it raises sea levels.
In 2018, we launched the Ice, Cloud and Land Elevation Satellite-2 (ICESat-2) to continue a global record of ice elevation. Now, the results are in. Using millions of measurements from a laser in space and quite a bit of math, researchers have confirmed that Earth is rapidly losing ice.
ICESat-2 was a follow-up mission to the original ICESat, which launched in 2003 and took measurements until 2009. Comparing the two records tells us how much ice sheets have lost over 16 years.
During those 16 years, melting ice from Antarctica and Greenland was responsible for just over a half-inch of sea level rise. When ice on land melts, it eventually finds its way to the ocean. The rapid melt at the poles is no exception.
One gigaton of ice holds enough water to fill 400,000 Olympic swimming pools. It’s also enough ice to cover Central Park in New York in more than 1,000 feet of ice.
Between 2003 and 2019, Greenland lost 200 gigatons of ice per year. That’s 80 million Olympic swimming pools reaching the ocean every year, just from Greenland alone.
During the same time period, Antarctica lost 118 gigatons of ice per year. That’s another 47 million Olympic swimming pools every year. While there has been some elevation gain in the continent’s center from increased snowfall, it’s nowhere near enough to make up for how much ice is lost to the sea from coastal glaciers.
ICESat-2 sends out 10,000 pulses of laser light a second down to Earth’s surface and times how long it takes them to return to the satellite, down to a billionth of a second. That’s how we get such precise measurements of height and changing elevation.
These numbers confirm what scientists have been finding in most previous studies and continue a long record of data showing how Earth’s polar ice is melting. ICESat-2 is a key tool in our toolbox to track how our planet is changing.
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At the bottom of a very dark swimming pool, divers are getting ready for missions to the Moon. Take a look at this a recent test in the Neutral Buoyancy Laboratory at NASA’s Johnson Space Center. NASA astronauts are no strangers to extreme environments. We best prepare our astronauts by exposing them to training environments here on Earth that simulate the 1/6th gravity, suit mobility, lighting and lunar terrain they'll expect to see on a mission to the Moon. Practice makes perfect.
The Neutral Buoyancy Laboratory at NASA's Johnson Space Center is where astronauts train for spacewalks, and soon, moonwalks.
When astronauts go to the Moon’s South Pole through NASA’s Artemis program, the Sun will only be a few degrees over the horizon, creating long, dark shadows. To recreate this environment, divers at the lab turned off the lights, put up black curtains on the pool walls to minimize reflection, and used powerful underwater lamps to simulate the environment astronauts might experience on lunar missions.
These conditions replicate the dark, long shadows astronauts could see and lets them evaluate the different lighting configurations. The sand at the bottom is common pool filter sand with some other specialized combinations in the mix.
This was a test with divers in SCUBA gear to get the lighting conditions right, but soon, NASA plans to conduct tests in this low-light environment using spacesuits.
Neutral buoyancy is the equal tendency of an object to sink or float. Through a combination of weights and flotation devices, an item is made to be neutrally buoyant and it will seem to "hover" under water. In such a state, even a heavy object can be easily manipulated, much as it is in the zero gravity of space, but will still be affected by factors such as water drag.
The Neutral Buoyancy Laboratory is 202 ft in length, 102 ft in width and 40 ft in depth (20 ft above ground level and 20 ft below) and holds 6.2 million gallons of water.
Instead of traditional chemical rockets, the spacecraft uses sophisticated ion engines for propulsion. This enabled Dawn to become the first mission to orbit not one, but two different worlds — first the giant asteroid Vesta and now the dwarf planet Ceres. Vesta and Ceres formed early in the solar system's history, and by studying them, the mission is helping scientists go back in time to the dawn of the planets. To mark a decade since Dawn was launched on Sept. 27, 2007, here are 10 things to know about this trailblazing mission.
Most rocket engines use chemical reactions for propulsion, which tend to be powerful but short-lived. Dawn's futuristic, hyper-efficient ion propulsion system works by using electricity to accelerate ions (charged particles) from xenon fuel to a speed seven to 10 times that of chemical engines. Ion engines accelerate the spacecraft slowly, but they're very thrifty with fuel, using just milligrams of xenon per second (about 10 ounces over 24 hours) at maximum thrust. Without its ion engines, Dawn could not have carried enough fuel to go into orbit around two different solar system bodies. Try your hand at an interactive ion engine simulation.
Scientists have long wanted to study Vesta and Ceres up close. Vesta is a large, complex and intriguing asteroid. Ceres is the largest object in the entire asteroid belt, and was once considered a planet in its own right after it was discovered in 1801. Vesta and Ceres have significant differences, but both are thought to have formed very early in the history of the solar system, harboring clues about how planets are constructed. Learn more about Ceres and Vesta—including why we have pieces of Vesta here on Earth.
This view of Ceres built from Dawn photos is centered on Occator Crater, home of the famous "bright spots." The image resolution is about 460 feet (140 meters) per pixel.
Take a closer look.
Craters on Ceres are named for agricultural deities from all over the world, and other features carry the names of agricultural festivals. Ceres itself was named after the Roman goddess of corn and harvests (that's also where the word "cereal" comes from). The International Astronomical Union recently approved 25 new Ceres feature names tied to the theme of agricultural deities. Jumi, for example, is the Latvian god of fertility of the field. Study the full-size map.
Thanks to Dawn, evidence is mounting that Ceres hides a significant amount of water ice. A recent study adds to this picture, showing how ice may have shaped the variety of landslides seen on Ceres today.
Ahuna Mons, a 3-mile-high (5-kilometer-high) mountain, puzzled Ceres explorers when they first found it. It rises all alone above the surrounding plains. Now scientists think it is likely a cryovolcano — one that erupts a liquid made of volatiles such as water, instead of rock. "This is the only known example of a cryovolcano that potentially formed from a salty mud mix, and that formed in the geologically recent past," one researcher said. Learn more.
The brightest area on Ceres, located in the mysterious Occator Crater, has the highest concentration of carbonate minerals ever seen outside Earth, according to studies from Dawn scientists. Occator is 57 miles (92 kilometers) wide, with a central pit about 6 miles (10 kilometers) wide. The dominant mineral of this bright area is sodium carbonate, a kind of salt found on Earth in hydrothermal environments. This material appears to have come from inside Ceres, and this upwelling suggests that temperatures inside Ceres are warmer than previously believed. Even more intriguingly, the results suggest that liquid water may have existed beneath the surface of Ceres in recent geological time. The salts could be remnants of an ocean, or localized bodies of water, that reached the surface and then froze millions of years ago. See more details.
Dawn's chief engineer and mission director, Marc Rayman, provides regular dispatches about Dawn's work in the asteroid belt. Catch the latest updates here.
Another cool way to retrace Dawn's decade-long flight is to download NASA's free Eyes on the Solar System app, which uses real data to let you go to any point in the solar system, or ride along with any spacecraft, at any point in time—all in 3-D.
Send a postcard from one of these three sets of images that tell the story of dwarf planet Ceres, protoplanet Vesta, and the Dawn mission overall.
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This month, in honor of Valentine's Day, we'll focus on celestial star pairs and constellation couples.
Let's look at some celestial pairs!
The constellations Perseus and Andromeda are easy to see high overhead this month.
According to lore, the warrior Perseus spotted a beautiful woman--Andromeda--chained to a seaside rock. After battling a sea serpent, he rescued her.
As a reward, her parents Cepheus and Cassiopeia allowed Perseus to marry Andromeda.
The great hunter Orion fell in love with seven sisters, the Pleiades, and pursued them for a long time. Eventually Zeus turned both Orion and the Pleiades into stars.
Orion is easy to find. Draw an imaginary line through his belt stars to the Pleiades, and watch him chase them across the sky forever.
A pair of star clusters is visible on February nights. The Perseus Double Cluster is high in the sky near Andromeda's parents Cepheus and Cassiopeia.
Through binoculars you can see dozens of stars in each cluster. Actually, there are more than 300 blue-white supergiant stars in each of the clusters.
There are some colorful star pairs, some visible just by looking up and some requiring a telescope. Gemini's twins, the brothers Pollux and Castor, are easy to see without aid.
Orion's westernmost, or right, knee, Rigel, has a faint companion. The companion, Rigel B, is 500 times fainter than the super-giant Rigel and is visible only with a telescope.
Orion's westernmost belt star, Mintaka, has a pretty companion. You'll need a telescope.
Finally, the moon pairs up with the Pleiades on the 22nd and with Pollux and Castor on the 26th.
Watch the full What’s Up for February Video:
There are so many sights to see in the sky. To stay informed, subscribe to our What’s Up video series on Facebook.
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