Communications - Blog Posts

Calling Long-Distance: 10 Stellar Moments in 2022 for Space Communications and Navigation

Just like your phone needs Wi-Fi or data services to text or call – NASA spacecraft need communication services.

Giant antennas on Earth and a fleet of satellites in space enable missions to send data and images back to our home planet and keep us in touch with our astronauts in space. Using this data, scientists and engineers can make discoveries about Earth, the solar system, and beyond. The antennas and satellites make up our space communications networks: the Near Space Network and Deep Space Network.

Check out the top ten moments from our space comm community: 

1. Space communication networks helped the Artemis I mission on its historic journey to the Moon. From the launch pad to the Moon and back, the Near Space Network and Deep Space Network worked hand-in-hand to seamlessly support Artemis I. These networks let mission controllers send commands up to the spacecraft and receive important spacecraft health data, as well as incredible images of the Moon and Earth.

The Pathfinder Technology Demonstration 3 spacecraft with hosted TeraByte InfraRed Delivery (TBIRD) payload communicating with laser links down to Earth. Credit: NASA/Ames Research Center

2. Spacecraft can range in size – from the size of a bus to the size of a cereal box. In May 2022, we launched a record-breaking communication system the size of a tissue box. TBIRD showcases the benefits of a laser communications system, which uses infrared light waves rather than radio waves to communicate more data at once. Just like we have upgraded from 3G to 4G to 5G on our phones, we are upgrading its space communications capabilities by implementing laser comms!

3. The Deep Space Network added a new 34-meter (111-foot) antenna to continue supporting science and exploration missions investigating our solar system and beyond. Deep Space Station 53 went online in February 2022 at our Madrid Deep Space Communications Complex. It is the fourth of six antennas being added to expand the network’s capacity.

4. You’ve probably seen in the news that there are a lot of companies working on space capabilities. The Near Space Network is embracing the aerospace community’s innovative work and seeking out multiple partnerships. In 2022, we met with over 300 companies in hopes of beginning new collaborative efforts and increasing savings.

5. Similar to TBIRD, we're developing laser comms for the International Space Station. The terminal will show the benefits of laser comms while using a new networking technique called High Delay/Disruption Tolerant Networking that routes data four times faster than current systems. This year, engineers tested and proved the capability in a lab.

6. In 2021, we launched the James Webb Space Telescope, a state-of-the-art observatory to take pictures of our universe. This year, the Deep Space Network received the revolutionary first images of our solar system from Webb. The telescope communicates with the network’s massive antennas at three global complexes in Canberra, Australia; Madrid, Spain; and Goldstone, California.

7. Just like we use data services on our phone to communicate, we'll do the same with future rovers and astronauts exploring the Moon. In 2022, the Lunar LTE Studies project, or LunarLiTES, team conducted two weeks of testing in the harsh depths of the Arizona desert, where groundbreaking 4G LTE communications data was captured in an environment similar to the lunar South Pole. We're using this information to determine the best way to use 4G and 5G networking on the Moon.

8. A new Near Space Network antenna site was unveiled in Matjiesfontein, South Africa. NASA and the South African Space Agency celebrated a ground-breaking at the site of a new comms antenna that will support future Artemis Moon missions. Three ground stations located strategically across the globe will provide direct-to-Earth communication and navigation capabilities for lunar missions.

9. Quantum science aims to better understand the world around us through the study of extremely small particles. April 14, 2022, marked the first official World Quantum Day celebration, and we participated alongside other federal agencies and the National Quantum Coordination Office. From atomic clocks to optimizing laser communications, quantum science promises to greatly improve our advances in science, exploration, and technology.

10. We intentionally crashed a spacecraft into an asteroid to test technology that could one day be used to defend Earth from asteroids. The Double Asteroid Redirection Test, or DART, mission successfully collided with the asteroid Dimorphos at a rate of 4 miles per second (6.1 kilometers per second), with real-time video enabled by the Deep Space Network. Alongside communications and navigation support, the global network also supports planetary defense by tracking near-Earth objects.

We look forward to many more special moments connecting Earth to space in the coming year.

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NASA Communications and Navigation in 2021: Top 10 Iconic Moments

Did you know NASA uses global networks of antennas and relay satellites to talk with astronauts and spacecraft?

Our space communications and navigation community has had an incredible year! From supporting science and exploration missions to developing cutting-edge tech, here are some of the team’s most impactful accomplishments of 2021.

1. We launched a revolutionary tech demo, the Laser Communications Relay Demonstration, which will showcase the benefits of using infrared laser links to send data from space. Laser communications systems can offer 10 to 100 times more data per second than traditional radio! You can learn more about the mission in a new season of our podcast, The Invisible Network.

2. Planetary radars observed their 1,000th near-Earth asteroid since 1968! Our Deep Space Network plays a critical role in detecting near-Earth asteroids, using radar to spot them. These radar detections help definitively predict if an asteroid is going to hit Earth, or if it’s just going to pass close by.

3. We used lessons learned developing communications services for the Moon to address digital inequality on Earth. Folks at our Glenn Research Center in Cleveland examined how lunar network approaches could address technical challenges to Wi-Fi connectivity in their local community.

4. Our Search and Rescue office participated in dress rehearsals for the Artemis I mission to the Moon! They tested critical distress technologies that will help locate Artemis astronauts in the unlikely event they need to leave the Orion capsule and enter open water before recovery teams can reach them.

5. With high international participation, we hosted a virtual workshop on cognitive communications at our Glenn Research Center in Cleveland, Ohio. Cognitive communications employs artificial intelligence and machine learning in radio systems to provide a host of benefits to user missions!

6. We celebrated the 100th birthday of the creator of Star Trek, the late Gene Roddenberry. The event featured Roddenberry’s son Rod, NASA administrator Bill Nelson, and Star Trek actor George Takei. Following the program, our Deep Space Network broadcast Gene’s 1976 remarks on diversity and inclusion toward star system 40 Eridani — home to the planet Vulcan in Star Trek lore. Signals from the broadcast will arrive there in 16.5 years.

7. We worked with the aerospace community to refine our LunaNet architecture for lunar communications and navigation services! LunaNet will leverage innovative networking techniques, standards, and an extensible framework to rapidly expand network capabilities at the Moon for Artemis. This framework will allow industry, academia, and international partners to build and operate LunaNet nodes alongside us.

8. Our Deep Space Network welcomed a brand new satellite dish into the family! Called Deep Space Station 56, or DSS-56, the 112-foot-wide (34-meter) dish is now online and ready to communicate for a variety of uses, including missions at the Moon and Mars.

9. Our Near Space Network engaged with over 200 commercial aerospace companies! They’re working toward a new paradigm where NASA missions near Earth can rely on a blend of government and commercial space communications infrastructure to meet their needs.

10. Our 10th item on the list isn’t a single moment, but the continued support our communications networks provided missions throughout 2021. Whether it was a Commercial Crew mission to the International Space Station or the Perseverance Rover’s touchdown on Mars, our Near Space Network and Deep Space Network were there to empower mission success! Make sure to follow us on Tumblr for your regular dose of space!

Around the World in Seven Ground Stations

Happy Birthday, Jules Verne!

Considered by many to be the father of science fiction, French novelist Jules Verne takes his readers on a “From the Earth to the Moon,” “Twenty Thousand Leagues Under the Sea” and “Around the World in Eighty Days.” In his honor, let’s take our own journey around the world, exploring seven far-flung ground stations and the communications networks they support. These ground stations downlink data from science and exploration missions, maintaining the critical link from space to ground.

Our Deep Space Network supports far-out missions like Voyager 1, a spacecraft that's now over 13 billion miles from Earth. To communicate that far, the Network uses antennas as large as 230 feet in diameter. The network has ground stations in Pasadena, California; Madrid, Spain; and this one in Canberra, Australia. The ground stations are strategically placed for maximum coverage of the night sky, ensuring that deep space missions can communicate their data back to Earth. Check out that lizard!

Our Space Network uses relay satellites in conjunction with ground stations to provide continuous communications coverage for satellites in low-Earth orbit like the International Space Station, enabling 24/7 connection with astronauts onboard. Spacecraft using the Space Network beam their data to the constellation of Tracking and Data Relay Satellites, which forward that data to the ground. This is a photo of a Space Network ground station in Guam, a U.S. territory. The spherical structures around the antennas are called “radomes” and protect the antennas from the tropical storms!

Optical communications uses lasers to provide missions with higher data rates than radio communications. Optical terminals also offer missions reduced size, weight and power requirements over comparable radio antennas. A smaller system leaves more room for science instruments, a weight reduction can mean a less expensive launch and reduced power allows batteries to last longer. This ground station in Haleakalā, Hawaii, will relay data to California through a groundbreaking optical communications satellite, the Laser Communications Relay Demonstration. The demonstration will show the power and promise of optical communications to support the next generation of science missions.

Antarctica may seem like an odd place for radio antennas, but McMurdo Ground Station is vitally important to our networks. In 2017, we used the McMurdo ground station to demonstrate a new technology called Disruption Tolerant Networking (DTN), sending a selfie from McMurdo to the space station through numerous DTN nodes. DTN protocols allow data to be stored at points along its route that do not have an open connection to the next intermediary, preventing data loss and improving data returns.

This Near Earth Network ground station in Santiago, Chile, might not be our only South American ground station for long. The Near Earth Network is considering Punta Arenas, Chile, as a possible location for Ka-band antennas, which would provide missions with higher data rates. The Near Earth Network is also experimenting with Ka-band arraying, which uses multiple smaller antennas to provide the same capabilities of a larger, Ka-band antenna. Ka-band services will greatly increase the amount of science data we can gather!

If the space station ever has communications trouble, we could communicate with our astronauts through emergency very high frequency (VHF) communications ground stations like this one in Wallops Island, Virginia. VHF offers voice-only, contingency communications for the station and the Soyuz spacecraft, which ferries astronauts to and from the station. We maintain two VHF stations strategically placed to maximize contact with the space station as it orbits above North America. International partners operate VHF stations that provide contacts as the station orbits above Asia and Europe. NASA’s segment of the VHF network recently underwent critical upgrades that improve the reliability and durability of the system.

This beautiful photo captures Near Earth Network antennas in Svalbard, Norway, beneath the glow of the Northern lights, a phenomenon that occurs when charged particles from the Sun interact with various gasses in Earth’s atmosphere. If one were to visit Iceland, one could see these same lights above Snæfellsjökull volcano, featured in Jules Verne’s “A Journey to the Center of the Earth” as the imaginary entrance to a subterranean world.

A lot has changed in the nearly two centuries since Jules Verne was born. Verne’s 1865 novel “From the Earth to the Moon” and its 1870 sequel “Around the Moon” imagine a giant cannon capable of launching three men into lunar orbit. These imaginary astronauts used opera glasses to survey the lunar surface before returning safely to Earth.

Such a story may seem ridiculous in an age where humanity has occupied space for decades and satellites explore distant worlds with increasing regularity, but Verne’s dreams of spaceflight were novel ­– if not revolutionary – at the time. This change in worldview reflects humanity’s inexorable technological progress and our mission at NASA to turn science fiction into science fact.

As the next generation of exploration commences, our ever-evolving communications capabilities rise to meet the demands of missions that dreamers like Verne could hardly imagine.

The seven ground stations featured here were just a taste of our communications infrastructure. To learn more about space communications, visit: https://www.nasa.gov/SCaN

Optical Communications: Explore Lasers in Space

When we return to the Moon, much will seem unchanged since humans first arrived in 1969. The flags placed by Apollo astronauts will be untouched by any breeze. The footprints left by man’s “small step” on its surface will still be visible across the Moon’s dusty landscape.

Our next generation of lunar explorers will require pioneering innovation alongside proven communications technologies. We’re developing groundbreaking technologies to help these astronauts fulfill their missions.

In space communications networks, lasers will supplement traditional radio communications, providing an advancement these explorers require. The technology, called optical communications, has been in development by our engineers over decades.

Optical communications, in infrared, has a higher frequency than radio, allowing more data to be encoded into each transmission. Optical communications systems also have reduced size, weight and power requirements. A smaller system leaves more room for science instruments; a weight reduction can mean a less expensive launch, and reduced power allows batteries to last longer.

On the path through this “Decade of Light,” where laser joins radio to enable mission success, we must test and demonstrate a number of optical communications innovations.

The Laser Communications Relay Demonstration (LCRD) mission will send data between ground stations in Hawaii and California through a spacecraft in an orbit stationary relative to Earth’s rotation. The demo will be an important first step in developing next-generation Earth-relay satellites that can support instruments generating too much data for today’s networks to handle.

The Integrated LCRD Low-Earth Orbit User Modem and Amplifier-Terminal will provide the International Space Station with a fully operational optical communications system. It will communicate data from the space station to the ground through LCRD. The mission applies technologies from previous optical communications missions for practical use in human spaceflight.

In deep space, we’re working to prove laser technologies with our Deep Space Optical Communications mission. A laser’s wavelength is smaller than radio, leaving less margin for error in pointing back at Earth from very, very far away. Additionally, as the time it takes for data to reach Earth increases, satellites need to point ahead to make sure the beam reaches the right spot at the right time. The Deep Space Optical Communications mission will ensure that our communications engineers can meet those challenges head-on.

An integral part of our journey back to the Moon will be our Orion spacecraft. It looks remarkably similar to the Apollo capsule, yet it hosts cutting-edge technologies. NASA’s Laser Enhanced Mission Communications Navigation and Operational Services (LEMNOS) will provide Orion with data rates as much as 100 times higher than current systems.

LEMNOS’s optical terminal, the Orion EM-2 Optical Communications System, will enable live, 4K ultra-high-definition video from the Moon. By comparison, early Apollo cameras filmed only 10 frames per second in grainy black-and-white. Optical communications will provide a “giant leap” in communications technology, joining radio for NASA’s return to the Moon and the journey beyond.

NASA’s Space Communications and Navigation program office provides strategic oversight to optical communications research. At NASA’s Goddard Space Flight Center in Greenbelt, Maryland, the Exploration and Space Communications projects division is guiding a number of optical communications technologies from infancy to fruition. If you’re ever near Goddard, stop by our visitor center to check out our new optical communications exhibit. For more information, visit nasa.gov/SCaN and esc.gsfc.nasa.gov.

The Invisible Network: A New NASA Podcast

We sit on the precipice of a golden age of space exploration — a renaissance of space science and technology. Every day, our missions send millions of bits of data to Earth, unraveling long-held mysteries about the universe, our solar system and even our own planet. But what makes it all possible?

Today we debut a new, limited edition podcast called “The Invisible Network.” It brings you a side of NASA you may have never seen or heard of before — oft overlooked technologies crucial to spaceflight and humanity’s ambitions among the stars.

Communications is the vital link between Earth and space. A collection of far-flung ground stations enabled the Apollo missions: our first steps on the Moon; the Voyager missions: our first brushes with interstellar space; and supported the earliest space and Earth science missions, expanding our knowledge of the stars and of ourselves.

Today, our communications networks are vastly different than those that supported Apollo. Tomorrow’s networks will be even more advanced.

“The Invisible Network” explores technological innovations guiding us into the future. These seemingly un-sexy feats of engineering will allow us to return to the Moon, journey to Mars and venture ever-further into the unknown.

Artist’s rendering of the upcoming Orion missions.

Our podcast’s title, "The Invisible Network," comes from author and former NASA engineer Sunny Tsiao’s book, “Read You Loud and Clear,” published in 2008. Tsiao notes that our communications and tracking programs are often described as “invisible.” Infrastructures, he writes, are seldom recognized, except when they fall short.

If our networks are invisible, perhaps it’s because they work so well.

We hope you’ll join us on our journey into The Invisible Network. Subscribe to the show and share us with a friend. For more information visit nasa.gov/invisible or nasa.gov/scan.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.

In Conversation with the Sun: Parker Solar Probe Communications

Our Sun powers life on Earth. It defines our days, nourishes our crops and even fuels our electrical grids. In our pursuit of knowledge about the universe, we’ve learned so much about the Sun, but in many ways we’re still in conversation with it, curious about its mysteries.

Parker Solar Probe will advance this conversation, flying through the Sun’s atmosphere as close as 3.8 million miles from our star’s surface, more than seven times closer to it than any previous spacecraft. If space were a football field, with Earth at one end and the Sun at the other, Parker would be at the four-yard line, just steps away from the Sun! This journey will revolutionize our understanding of the Sun, its surface and solar winds.

Supporting Parker on its journey to the Sun are our communications networks. Three networks, the Near Earth Network, the Space Network and the Deep Space Network, provide our spacecraft with their communications, delivering their data to mission operations centers. Their services ensure that missions like Parker have communications support from launch through the mission.

For Parker’s launch on Aug. 12, the Delta IV Heavy rocket that sent Parker skyward relied on the Space Network. A team at Goddard Space Flight Center’s Networks Integration Center monitored the launch, ensuring that we maintained tracking and communications data between the rocket and the ground. This data is vital, allowing engineers to make certain that Parker stays on the right path towards its orbit around the Sun.

The Space Network’s constellation of Tracking and Data Relay Satellites (TDRS) enabled constant communications coverage for the rocket as Parker made its way out of Earth’s atmosphere. These satellites fly in geosynchronous orbit, circling Earth in step with its rotation, relaying data from spacecraft at lower altitudes to the ground. The network’s three collections of TDRS over the Atlantic, Pacific and Indian oceans provide enough coverage for continuous communications for satellites in low-Earth orbit.

The Near Earth Network’s Launch Communications Segment tracked early stages of Parker's launch, testing our brand new ground stations’ ability to provide crucial information about the rocket’s initial velocity (speed) and trajectory (path). When fully operational, it will support launches from the Kennedy spaceport, including upcoming Orion missions. The Launch Communications Segment’s three ground stations are located at Kennedy Space Center; Ponce De Leon, Florida; and Bermuda. 

When Parker separated from the Delta IV Heavy, the Deep Space Network took over. Antennas up to 230 feet in diameter at ground stations in California, Australia and Spain are supporting Parker for its 24 orbits around the Sun and the seven Venus flybys that gradually shrink its orbit, bringing it closer and closer to the Sun. The Deep Space Network is delivering data to mission operations centers and will continue to do so as long as Parker is operational.

Near the Sun, radio interference and the heat load on the spacecraft’s antenna makes communicating with Parker a challenge that we must plan for. Parker has three distinct communications phases, each corresponding to a different part of its orbit.

When Parker comes closest to the Sun, the spacecraft will emit a beacon tone that tells engineers on the ground about its health and status, but there will be very little opportunity to command the spacecraft and downlink data. High data rate transmission will only occur during a portion of Parker’s orbit, far from the Sun. The rest of the time, Parker will be in cruise mode, taking measurements and being commanded through a low data rate connection with Earth.

Communications infrastructure is vital to any mission. As Parker journeys ever closer to the center of our solar system, each byte of downlinked data will provide new insight into our Sun. It’s a mission that continues a conversation between us and our star that has lasted many millions of years and will continue for many millions more.

For more information about NASA’s mission to touch the Sun: https://www.nasa.gov/content/goddard/parker-solar-probe

For more information about our satellite communications check out: http://nasa.gov/SCaN

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.

Going for GOLD

On Jan. 25, we’re going for GOLD!

We’re launching an instrument called Global-scale Observations of the Limb and Disk, GOLD for short. It’s a new mission that will study a complicated — and not yet fully understood — region of near-Earth space, called the ionosphere.

Space is not completely empty: It’s teeming with fast-moving energized particles and electric and magnetic fields that guide their motion. At the boundary between Earth’s atmosphere and space, these particles and fields — the ionosphere — co-exist with the upper reaches of the neutral atmosphere.

That makes this a complicated place. Big events in the lower atmosphere, like hurricanes or tsunamis, can create waves that travel all the way up to that interface to space, changing the wind patterns and causing disruptions.

It’s also affected by space weather. The Sun is a dynamic star, and it releases spurts of energized particles and blasts of solar material carrying electric and magnetic fields that travel out through the solar system. Depending on their direction, these bursts have the potential to disrupt space near Earth.

This combination of factors makes it hard to predict changes in the ionosphere — and that can have a big impact. Communications signals, like radio waves and signals that make our GPS systems work, travel through this region, and sudden changes can distort them or even cut them off completely.

Low-Earth orbiting satellites — including the International Space Station — also fly through the ionosphere, so understanding how it fluctuates is important for protecting these satellites and astronauts.  

GOLD is a spectrograph, an instrument that breaks light down into its component wavelengths, measuring their intensities. Breaking light up like this helps scientists see the behavior of individual chemical elements — for instance, separating the amount of oxygen versus nitrogen. GOLD sees in far ultraviolet light, a type of light that’s invisible to our eyes.

GOLD is a hosted payload. The instrument is hitching a ride aboard SES-14, a commercial communications satellite built by Airbus for SES Government Solutions, which owns and operates the satellite.

Also launching this year is the Ionospheric Connection Explorer, or ICON, which will also study the ionosphere and neutral upper atmosphere. But while GOLD will fly in geostationary orbit some 22,000 miles above the Western Hemisphere, ICON will fly just 350 miles above Earth, able to gather close up images of this region.

Together, these missions give us an unprecedented look at the ionosphere and upper atmosphere, helping us understand the very nature of how our planet interacts with space.

To learn more about this region of space and the GOLD mission, visit: nasa.gov/gold.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.  

How Humans Change Space Itself

It’s no surprise that humans influence the surface of our planet, but our reach can go farther than that. Humans affect space, too.

We know storms from the sun can naturally change the space environment around Earth, which can have an impact on satellites and power grids.

Scientists now know that Cold War era nuclear tests in the 1950s caused similar effects.

Particles around Earth are organized into layers known as radiation belts. These 1950s tests created a temporary extra layer of radiation closer to Earth. 

The effects of this could be seen all around the world. Aurora appeared at the equator instead of the poles, utility grids in Hawaii were strained, and in some cases, satellites above test sites were affected. 

Some types of communications signals can also affect Earth’s radiation belts. 

Very low-frequency waves, or VLFs, are used for radio communications. They are often used to communicate with submarines, because these waves can penetrate deep into the ocean. 

The waves can also travel far into the space environment around Earth. When these waves are in space, they affect how high-energy particles move, creating a barrier against natural radiation.

The outer edge of this radio-wave barrier corresponds almost exactly the inner edge of Earth’s natural radiation belts – meaning it could be human activity that at least partly shapes this natural radiation around Earth.  

For more NASA sun and space research, visit www.nasa.gov/sunearth and follow us on Twitter and Facebook.

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