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By NASA
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
The radio antennas of NASA’s Canberra Deep Space Communications Complex are lo-cated near the Australian capital. It’s one of three Deep Space Network facilities around the world that keep the agency in contact with dozens of space missions Located at Tidbinbilla Nature Reserve near the Australian capital city, the Canberra complex joined the Deep Space Network on March 19, 1965, with one 85-foot-wide (26-meter-wide) radio antenna. The dish, called Deep Space Station 42, was decommis-sioned in 2000. This photograph shows the facility in 1965.NASA Canberra joined the global network in 1965 and operates four radio antennas. Now, preparations have begun on its fifth as NASA works to increase the network’s capacity.
NASA’s Deep Space Network facility in Canberra, Australia celebrated its 60th anniversary on March 19 while also breaking ground on a new radio antenna. The pair of achievements are major milestones for the network, which communicates with spacecraft all over the solar system using giant dish antennas located at three complexes around the globe.
Canberra’s newest addition, Deep Space Station 33, will be a 112-foot-wide (34-meter-wide) multifrequency beam-waveguide antenna. Buried mostly below ground, a massive concrete pedestal will house cutting-edge electronics and receivers in a climate-controlled room and provide a sturdy base for the reflector dish, which will rotate during operations on a steel platform called an alidade.
Suzanne Dodd, the director for the Interplanetary Network Directorate at JPL, addresses an audience at the Deep Space Network’s Canberra complex on March 19, 2025. That day marked 60 years since the Australian facility joined the network.NASA “As we look back on 60 years of incredible accomplishments at Canberra, the groundbreaking of a new antenna is a symbol for the next 60 years of scientific discovery,” said Kevin Coggins, deputy associate administrator of NASA’s SCaN (Space Communications and Navigation) Program at NASA Headquarters in Washington. “Building cutting-edge antennas is also a symbol of how the Deep Space Network embraces new technologies to enable the exploration of a growing fleet of space missions.”
When it goes online in 2029, the new Canberra dish will be the last of six parabolic dishes constructed under NASA’s Deep Space Network Aperture Enhancement Program, which is helping to support current and future spacecraft and the increased volume of data they provide. The network’s Madrid facility christened a new dish in 2022, and the Goldstone, California, facility is putting the finishing touches on a new antenna.
Canberra’s Role
The Deep Space Network was officially founded on Dec. 24, 1963, when NASA’s early ground stations, including Goldstone, were connected to the new network control center at the agency’s Jet Propulsion Laboratory in Southern California. Called the Space Flight Operations Facility, that building remains the center through which data from the three global complexes flows.
The Madrid facility joined in 1964, and Canberra went online in 1965, going on to help support hundreds of missions, including the Apollo Moon landings.
Three eye-catching posters featuring the larger 230-foot (70-meter) antennas located at the three Deep Space Network complexes around the world.NASA/JPL-Caltech “Canberra has played a crucial part in tracking, communicating, and collecting data from some of the most momentous missions in space history,” said Kevin Ferguson, director of the Canberra Deep Space Communication Complex. “As the network continues to advance and grow, Canberra will continue to play a key role in supporting humanity’s exploration of the cosmos.”
By being spaced equidistant from one another around the globe, the complexes can provide continual coverage of spacecraft, no matter where they are in the solar system as Earth rotates. There is an exception, however: Due to Canberra’s location in the Southern Hemisphere, it is the only one that can send commands to, and receive data from, Voyager 2 as it heads south almost 13 billion miles (21 billion kilometers) through interstellar space. More than 15 billion miles (24 billion kilometers) away, Voyager 1 sends its data down to the Madrid and Goldstone complexes, but it, too, can only receive commands via Canberra.
New Technologies
In addition to constructing more antennas like Canberra’s Deep Space Station 33, NASA is looking to the future by also experimenting with laser, or optical, communications to enable significantly more data to flow to and from Earth. The Deep Space Network currently relies on radio frequencies to communicate, but laser operates at a higher frequency, allowing more data to be transmitted.
As part of that effort, NASA is flying the laser-based Deep Space Optical Communications experiment with the agency’s Psyche mission. Since the October 2023 launch, it has demonstrated high data rates over record-breaking distances and downlinked ultra-high definition streaming video from deep space.
“These new technologies have the potential to boost the science and exploration returns of missions traveling throughout the solar system,” said Amy Smith, deputy project manager for the Deep Space Networkat JPL, which manages the network. “Laser and radio communications could even be combined to build hybrid antennas, or dishes that can communicate using both radio and optical frequencies at the same time. That could be a game changer for NASA.”
For more information about the Deep Space Network, visit:
https://www.nasa.gov/communicating-with-missions/dsn/
NASA’s New Deep Space Network Antenna Has Its Crowning Moment NASA’s New Experimental Antenna Tracks Deep Space Laser VIDEO: How Do We Know Where Faraway Spacecraft Are? News Media Contact
Ian J. O’Neill
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-2649
ian.j.oneill@jpl.nasa.gov
2024-048
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By European Space Agency
A capacity increase by almost 80%! In late July 2024, the Malargüe deep-space communication station completed an important upgrade of its antenna feed that will allow missions to send much more data back to Earth.
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By European Space Agency
New research, partially funded by ESA, reveals that the cool ‘ocean skin’ allows oceans to absorb more atmospheric carbon dioxide than previously thought. These findings could enhance global carbon assessments, shaping more effective emission-reduction policies.
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By NASA
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
Water piping is installed near the Thad Cochran Test Stand (B-1/B-2) at NASA’s Stennis Space Center in December 2014. The project to replace and upgrade the center’s high pressure industrial water system was a key milestone in preparations to test the SLS (Space Launch System) core stage ahead of the successful Artemis I launch.NASA/Danny Nowlin Employees install a 96-inch valve near the Thad Cochran Test Stand (B-1/B-2) at NASA’s Stennis Space Center as part of a high-pressure industrial water upgrade project in March 2015.NASA/Danny Nowlin In this March 2022 photo, crews use a shoring system to hold back soil as they install new 75-inch piping leading from the NASA Stennis High Pressure Industrial Water Facility to the valve vault pit serving the Fred Haise Test Stand.NASA/Danny Nowlin Crews use a specially designed tool to place a new pipeline liner inside the existing carrier pipe near the Fred Haise Test Stand in 2024 in the last phase of updating the original test complex industrial water system at NASA’s Stennis Space Center.NASA/Danny Nowlin Crews prepare new pipeline liner sections for installation near the Fred Haise Test Stand in 2024 in the last phase of updating the original test complex industrial water system at NASA’s Stennis Space Center.NASA/Danny Nowlin For almost 60 years, NASA’s Stennis Space Center has tested rocket systems and engines to help power the nation’s human space exploration dreams. Completion of a critical water system infrastructure project helps ensure the site can continue that frontline work moving forward.
“The infrastructure at NASA Stennis is absolutely critical for rocket engine testing for the agency and commercial companies,” said NASA project manager Casey Wheeler. “Without our high pressure industrial water system, testing does not happen. Installing new underground piping renews the lifespan and gives the center a system that can be operated for the foreseeable future, so NASA Stennis can add to its nearly six decades of contributions to space exploration efforts.”
The high pressure industrial water system delivers hundreds of thousands of gallons of water per minute through underground pipes to cool rocket engine exhaust and provide fire suppression capabilities during testing. Without the water flow, the engine exhaust, reaching as hot as 6,000 degrees Fahrenheit, could melt the test stand’s steel flame deflector.
Each test stand also features a FIREX system that holds water in reserve for use in the event of a mishap or fire. During SLS (Space Launch System) core stage testing, water also was used to create a “curtain” around the test hardware, dampening the high levels of noise generated during hot fire and lessening the video-acoustic impact that can cause damage to infrastructure and the test hardware.
Prior to the system upgrade, the water flow was delivered by the site’s original piping infrastructure built in the 1960s. However, that infrastructure had well exceeded its expected 30-year lifespan.
Scope of the Project
The subsequent water system upgrade was planned across multiple phases over a 10-year span. Crews worked around ever-changing test schedules to complete three major projects representing more than $50 million in infrastructure investment.
“Many people working the construction jobs for these projects are from the Gulf Coast area, so it has created jobs and work for the people doing the construction,” Wheeler said. “Some of the specialty work has had people coming in from all over the country, as well as vendors and suppliers that are supplying the materials, so that has an economic impact here too.”
Crews started by replacing large sections of piping, including a 96-inch line, from the 66-million-gallon onsite reservoir to the Thad Cochran (B-1/B-2) Test Stand. This phase also included the installation of a new 25,000-gallon electric pump at the High Pressure Industrial Water Facility to increase water flow capacity. The upgrades were critical for NASA Stennis to conduct Green Run testing of the SLS core stage in 2020-21 ahead of the successful Artemis I launch.
Work in the A Test Complex followed with crews replacing sections of 75-inch piping from the water plant and installing several new 66-inch gate valves.
In the final phase, crews used an innovative approach to install new steel liners within existing pipes leading to the Fred Haise Test Stand (formerly A-1 Test Stand). The work followed NASA’s completion of a successful RS-25 engine test campaign last April for future Artemis missions to the Moon and beyond. The stand now is being prepared to begin testing of new RS-25 flight engines.
Overall, the piping project represents a significant upgrade in design and materials. The new piping is made from carbon steel, with protective linings to prevent corrosion and gate valves designed to be more durable.
Importance of Water
It is hard to overstate the importance of the work to ensure ongoing water flow. For a typical 500-second RS-25 engine test on the Fred Haise Test Stand, around 5 million gallons of water is delivered from the NASA Stennis reservoir through a quarter-of-a-mile of pipe before entering the stand to supply the deflector and cool engine exhaust.
“Without water to cool the deflector and the critical parts of the test stand that will get hot from the hot fire itself, the test stand would need frequent corrective maintenance,” Wheeler said. “This system ensures the test stands remain in a condition where continuous testing can happen.”
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Last Updated Sep 26, 2024 EditorNASA Stennis CommunicationsContactC. Lacy Thompsoncalvin.l.thompson@nasa.gov / (228) 688-3333LocationStennis Space Center Related Terms
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By NASA
NASA’s Cold Atom Lab, shown where it’s installed aboard the International Space Station, recently demonstrated the use of a tool called an atom interferometer that can precisely measure gravity and other forces — and has many potential applications in space.NASA/JPL-Caltech Future space missions could use quantum technology to track water on Earth, explore the composition of moons and other planets, or probe mysterious cosmic phenomena.
NASA’s Cold Atom Lab, a first-of-its-kind facility aboard the International Space Station, has taken another step toward revolutionizing how quantum science can be used in space. Members of the science team measured subtle vibrations of the space station with one of the lab’s onboard tools — the first time ultra-cold atoms have been employed to detect changes in the surrounding environment in space.
The study, which appeared in Nature Communications on Aug. 13, also reports the longest demonstration of the wave-like nature of atoms in freefall in space.
The Cold Atom Lab science team made their measurements with a quantum tool called an atom interferometer, which can precisely measure gravity, magnetic fields, and other forces. Scientists and engineers on Earth use this tool to study the fundamental nature of gravity and advance technologies that aid aircraft and ship navigation. (Cell phones, transistors, and GPS are just a few other major technologies based on quantum science but do not involve atom interferometry.)
Physicists have been eager to apply atom interferometry in space because the microgravity there allows longer measurement times and greater instrument sensitivity, but the exquisitely sensitive equipment has been considered too fragile to function for extended periods without hands-on assistance. The Cold Atom Lab, which is operated remotely from Earth, has now shown it’s possible.
“Reaching this milestone was incredibly challenging, and our success was not always a given,” said Jason Williams, the Cold Atom Lab project scientist at NASA’s Jet Propulsion Laboratory in Southern California. “It took dedication and a sense of adventure by the team to make this happen.”
Power of Precision
Space-based sensors that can measure gravity with high precision have a wide range of potential applications. For instance, they could reveal the composition of planets and moons in our solar system, because different materials have different densities that create subtle variations in gravity.
This type of measurement is already being performed by the U.S.-German collaboration GRACE-FO (Gravity Recovery and Climate Experiment Follow-on), which detects slight changes in gravity to track the movement of water and ice on Earth. An atom interferometer could provide additional precision and stability, revealing more detail about surface mass changes.
Precise measurements of gravity could also offer insights into the nature of dark matter and dark energy, two major cosmological mysteries. Dark matter is an invisible substance five times more common in the universe than the “regular” matter that composes planets, stars, and everything else we can see. Dark energy is the name given to the unknown driver of the universe’s accelerating expansion.
“Atom interferometry could also be used to test Einstein’s theory of general relativity in new ways,” said University of Virginia professor Cass Sackett, a Cold Atom Lab principal investigator and co-author of the new study. “This is the basic theory explaining the large-scale structure of our universe, and we know that there are aspects of the theory that we don’t understand correctly. This technology may help us fill in those gaps and give us a more complete picture of the reality we inhabit.”
A Portable Lab
NASA’s Cold Atom Lab studies the quantum nature of atoms, the building blocks of our universe, in a place that is out of this world – the International Space Station. This animated explainer explores what quantum science is and why NASA wants to do it in space. Credit: NASA/JPL-Caltech About the size of a minifridge, the Cold Atom Lab launched to the space station in 2018 with the goal of advancing quantum science by putting a long-term facility in the microgravity environment of low Earth orbit. The lab cools atoms to almost absolute zero, or minus 459 degrees Fahrenheit (minus 273 degrees Celsius). At this temperature, some atoms can form a Bose-Einstein condensate, a state of matter in which all atoms essentially share the same quantum identity. As a result, some of the atoms’ typically microscopic quantum properties become macroscopic, making them easier to study.
Quantum properties include sometimes acting like solid particles and sometimes like waves. Scientists don’t know how these building blocks of all matter can transition between such different physical behaviors, but they’re using quantum technology like what’s available on the Cold Atom Lab to seek answers.
In microgravity, Bose-Einstein condensates can reach colder temperatures and exist for longer, giving scientists more opportunities to study them. The atom interferometer is among several tools in the facility enabling precision measurements by harnessing the quantum nature of atoms.
Due to its wave-like behavior, a single atom can simultaneously travel two physically separate paths. If gravity or other forces are acting on those waves, scientists can measure that influence by observing how the waves recombine and interact.
“I expect that space-based atom interferometry will lead to exciting new discoveries and fantastic quantum technologies impacting everyday life, and will transport us into a quantum future,” said Nick Bigelow, a professor at University of Rochester in New York and Cold Atom Lab principal investigator for a consortium of U.S. and German scientists who co-authored the study.
More About the Mission
A division of Caltech in Pasadena, JPL designed and built Cold Atom Lab, which is sponsored by the Biological and Physical Sciences (BPS) division of NASA’s Science Mission Directorate at the agency’s headquarters in Washington. BPS pioneers scientific discovery and enables exploration by using space environments to conduct investigations that are not possible on Earth. Studying biological and physical phenomena under extreme conditions allows researchers to advance the fundamental scientific knowledge required to go farther and stay longer in space, while also benefitting life on Earth.
To learn more about Cold Atom Lab, visit:
https://coldatomlab.jpl.nasa.gov/
News Media Contact
Calla Cofield
Jet Propulsion Laboratory, Pasadena, Calif.
626-808-2469
calla.e.cofield@jpl.nasa.gov
2024-106
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Last Updated Aug 13, 2024 Related Terms
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