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Artemis II Astronauts’ First Look at Their Lunar Spacecraft
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By NASA
Humans are returning to the Moon—this time, to stay. Because our presence will be more permanent, NASA has selected a location that maximizes line-of-sight communication with Earth, solar visibility, and access to water ice: the Lunar South Pole (LSP). While the Sun is in the lunar sky more consistently at the poles, it never rises more than a few degrees above the horizon; in the target landing regions, the highest possible elevation is 7°. This presents a harsh lighting environment never experienced during the Apollo missions, or in fact, in any human spaceflight experience. The ambient lighting will severely affect the crews’ ability to see hazards and to perform simple work. This is because the human vision system, which despite having a high-dynamic range, cannot see well into bright light and cannot adapt quickly from bright to dark or vice versa. Functional vision is required to perform a variety of tasks, from simple tasks (e.g., walking, operating simple tools) through managing complex machines (e.g., lander elevator, rovers). Thus, the environment presents an engineering challenge to the Agency: one that must be widely understood before it can be effectively addressed.
In past NASA missions and programs, design of lighting and functional vision support systems for extravehicular activity (EVA) or rover operations have been managed at the lowest program level. This worked well for Apollo and low Earth orbit because the Sun angle was managed by mission planning and astronaut self-positioning; helmet design alone addressed all vision challenges. The Artemis campaign presents new challenges to functional vision, because astronauts will be unable to avoid having the sun in their eyes much of the time they are on the lunar surface. This, combined with the need for artificial lighting in the extensive shadowing at the LSP, means that new functional vision support systems must be developed across projects and programs. The design of helmets, windows, and lighting systems must work in a complementary fashion, within and across programs, to achieve a system of lighting and vision support that enables crews to see into darkness while their eyes are light-adapted, in bright light while still dark-adapted, and protects their eyes from injury.
Many of the findings of the assessment were focused on the lack of specific requirements to prevent functional vision impairment by the Sun’s brilliance (which is different from preventing eye injury), while enabling astronauts to see well enough to perform specific tasks. Specifically, tasks expected of astronauts at the LSP were not incorporated into system design requirements to enable system development that ensures functional vision in the expected lighting environment. Consequently, the spacesuit, for example, has flexibility requirements for allowing the astronauts to walk but not for ensuring they can see well enough to walk from brilliant Sun into a dark shadow and back without the risk of tripping or falling. Importantly, gaps were identified in allocation of requirements across programs to ensure that the role of the various programs is for each to understand functional vision. NESC recommendations were offered that made enabling functional vision in the harsh lighting environment a specific and new requirement for the system designers. The recommendations also included that lighting, window, and visor designs be integrated.
The assessment team recommended that a wide variety of simulation techniques, physical and virtual, need to be developed, each with different and well-stated capabilities with respect to functional vision. Some would address the blinding effects of sunlight at the LSP (not easily achieved through virtual approaches) to evaluate performance of helmet shields and artificial lighting in the context of the environment and adaptation times. Other simulations would add terrain features to identify the threats in simple (e.g., walking, collection of samples) and complex (e.g., maintenance and operation of equipment) tasks. Since different facilities have different strengths, they also have different weaknesses. These strengths and limitations must be characterized to enable verification of technical solutions and crew training.
NESC TB 2024- discipline-focus-hfView the full article
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By European Space Agency
In a world first, ESA and Telesat have successfully connected a Low Earth Orbit (LEO) satellite to the ground using 5G Non-Terrestrial Network (NTN) technology in the Ka-band frequency range, marking a crucial step towards making space-based connections as simple as using a mobile phone.
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By NASA
From left to right, Ambassador of the Principality of Liechtenstein to the United States of America Georg Sparber, Director of the Office for Communications of the Principality of Liechtenstein Dr. Rainer Schnepfleitner, NASA Deputy Administrator Pam Melroy, and Ambassador Extraordinary and Plenipotentiary to the Swiss Confederation and to the Principality of Liechtenstein Scott Miller, pose for a group photo during an Artemis Accords signing ceremony, Friday, Dec. 20, 2024, at the Mary W. Jackson NASA Headquarters building in Washington. The Principality of Liechtenstein is the 52nd country to sign the Artemis Accords, which establish a practical set of principles to guide space exploration cooperation among nations participating in NASA’s Artemis program. Credit: NASA/Keegan Barber Liechtenstein signed the Artemis Accords Friday during a ceremony hosted by NASA Deputy Administrator Pam Melroy at the agency’s headquarters in Washington, becoming the 52nd nation to commit to the responsible exploration of space for all humanity.
“Today, as Liechtenstein signs the Artemis Accords, we take another step forward together, united by the promise of international cooperation and discovery,” said Melroy. “Liechtenstein’s commitment strengthens our vision, where space is explored with peace, transparency, and sustainability as guiding principles. With each new signatory, the Artemis Accords community adds fresh energy and capabilities to ensure the benefits of space reach the entire world.”
Director of Liechtenstein’s Office for Communications Rainer Schnepfleitner signed the Artemis Accords on behalf of Liechtenstein. The Ambassador of the Principality of Liechtenstein to the United States Georg Sparber and U.S. Ambassador to the Swiss Confederation and the Principality of Liechtenstein Scott Miller also participated in the event.
“With its participation in the Artemis Accords, Liechtenstein looks forward to advancing space exploration among a strong group of like-minded countries committed to the peaceful use of space for the benefit of all humanity,” Sparber said.
The United States, led by NASA and the U.S. Department of State, and seven other initial signatory nations established the Artemis Accords in 2020, identifying a set of principles promoting the beneficial use of space for humanity. Since then, signatories have expanded to represent a quarter of the world’s countries, with 19 countries signing in 2024.
In addition to an increase in numbers, the Artemis Accords signatories, representing every region of the world, continued to build consensus this year and make significant progress in implementing the accords principles.
NASA co-chaired the Artemis Accords Principals’ Meeting in October, which brought together 42 nations and furthered discussions on the safe and responsible use of space. They agreed on recommendations for non-interference, interoperability, release of scientific data, long-term sustainability guidelines, and registration of space objects to advance implementation.
The Artemis Accords are grounded in the Outer Space Treaty and other agreements including the Registration Convention, the Rescue and Return Agreement, as well as best practices for responsible behavior that NASA and its partners have supported, including the public release of scientific data.
Learn more about the Artemis Accords at:
https://www.nasa.gov/artemis-accords
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Amber Jacobson / Elizabeth Shaw
Headquarters, Washington
202-358-1600
amber.c.jacobson@nasa.gov / elizabeth.a.shaw@nasa.gov
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Last Updated Dec 20, 2024 LocationNASA Headquarters Related Terms
Office of International and Interagency Relations (OIIR) View the full article
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By NASA
1 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
NASA’s X-59 quiet supersonic research aircraft completed its first maximum afterburner test at Lockheed Martin’s Skunk Works facility in Palmdale, California. This full-power test, during which the engine generates additional thrust, validates the additional power needed for meeting the testing conditions of the aircraft. The X-59 is the centerpiece of NASA’s Quesst mission, which aims to overcome a major barrier to supersonic flight over land by reducing the noise of sonic booms.Lockheed Martin Corporation/Garry Tice NASA completed the first maximum afterburner engine run test on its X-59 quiet supersonic research aircraft on Dec. 12. The ground test, conducted at Lockheed Martin’s Skunk Works facility in Palmdale, California, marks a significant milestone as the X-59 team progresses toward flight.
An afterburner is a component of some jet engines that generates additional thrust. Running the engine, an F414-GE-100, with afterburner will allow the X-59 to meet its supersonic speed requirements. The test demonstrated the engine’s ability to operate within temperature limits and with adequate airflow for flight. It also showed the engine’s ability to operate in sync with the aircraft’s other subsystems.
The X-59 is the centerpiece of NASA’s Quesst mission, which seeks to solve one of the major barriers to supersonic flight over land by making sonic booms quieter. The X-59’s first flight is expected to occur in 2025.
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Last Updated Dec 20, 2024 EditorDede DiniusContactMatt Kamletmatthew.r.kamlet@nasa.gov Related Terms
Aeronautics Aeronautics Research Mission Directorate Armstrong Flight Research Center Commercial Supersonic Technology Integrated Aviation Systems Program Low Boom Flight Demonstrator Quesst (X-59) Supersonic Flight Explore More
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