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By NASA
1 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
NASA Glenn Research Center’s Frank Kaufhold discuses next-generation technologies for turbofan engines with the public during EAA AirVenture. Credit: NASA/Andrew Carlsen The first “A” in NASA stands for aeronautics, and NASA’s Glenn Research Center helped bring that message to thousands of people at major airshows in Wisconsin and Ohio this summer.
In July, NASA Glenn subject matter experts and outreach professionals landed in Oshkosh, Wisconsin, to participate in EAA AirVenture Oshkosh 2024. Thousands of aircraft arrived at Wittman Regional Airport in Oshkosh and other airports in east-central Wisconsin to attend the event.
Under the large NASA tent, staff shared information on both agencywide and center-specific projects, missions, and technology. NASA Glenn employees also assisted NASA Administrator Bill Nelson through tours and presentations.
NASA Glenn Research Center’s Amber Waid, left, discusses the wing-like shape of the truss of the X-66 Sustainable Flight Demonstrator with NASA Administrator Bill Nelson during EAA AirVenture. Credit: NASA/Andrew Carlsen Over Labor Day weekend, NASA Glenn’s experts traveled down the road to the Cleveland National Air Show at Burke Lakefront Airport. A main attraction, NASA Glenn’s newest aircraft — the Pilatus PC-12 — garnered enthusiasm from visitors who met NASA’s aircrew and learned about how this aircraft helps test innovative communications technology.
NASA Glenn Research Center interns Nikhita Kalluri, left, and Divya Nagireddy share fun facts about NASA and aviation with guests at the Cleveland National Air Show. Credit: NASA Inside the NASA tent, guests experienced virtual reality simulators, watched wind tunnel demonstrations, and learned about Quesst, NASA’s mission to make quiet, faster-than-sound air travel a reality.
NASA Glenn Research Center’s research pilot James Demers talks with guests about airplanes and flight research at the Cleveland National Air Show. Credit: NASA Return to Newsletter Explore More
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By NASA
3 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
While astronaut Gene Cernan was on the lunar surface during the Apollo 17 mission, his spacesuit collected loads of lunar dust. The gray, powdery substance stuck to the fabric and entered the capsule causing eye, nose, and throat irritation dubbed “lunar hay fever.” Credit: NASACredit: NASA Moon dust, or regolith, isn’t like the particles on Earth that collect on bookshelves or tabletops – it’s abrasive and it clings to everything. Throughout NASA’s Apollo missions to the Moon, regolith posed a challenge to astronauts and valuable space hardware.
During the Apollo 17 mission, astronaut Harrison Schmitt described his reaction to breathing in the dust as “lunar hay fever,” experiencing sneezing, watery eyes, and a sore throat. The symptoms went away, but concern for human health is a driving force behind NASA’s extensive research into all forms of lunar soil.
The need to manage the dust to protect astronaut health and critical technology is already beneficial on Earth in the fight against air pollution.
Working as a contributor on a habitat for NASA’s Next Space Technologies for Exploration Partnerships (NextSTEP) program, Lunar Outpost Inc. developed an air-quality sensor system to detect and measure the amount of lunar soil in the air that also detects pollutants on Earth.
Originally based in Denver, the Golden, Colorado-based company developed an air-quality sensor called the Space Canary and offered the sensor to Lockheed Martin Space for its NextSTEP lunar orbit habitat prototype. After the device was integrated into the habitat’s environmental control system, it provided distinct advantages over traditional equipment.
Rebranded as Canary-S (Solar), the sensor is now meeting a need for low-cost, wireless air-quality and meteorological monitoring on Earth. The self-contained unit, powered by solar energy and a battery, transmits data using cellular technology. It can measure a variety of pollutants, including particulate matter, carbon monoxide, methane, sulfur dioxide, and volatile organic compounds, among others. The device sends a message up to a secure cloud every minute, where it’s routed to either Lunar Outpost’s web-based dashboard or a customer’s database for viewing and analysis.
The oil and gas industry uses the Canary-S sensors to provide continuous, real-time monitoring of fugitive gas emissions, and the U.S. Forest Service uses them to monitor forest-fire emissions.
“Firefighters have been exhibiting symptoms of carbon monoxide poisoning for decades. They thought it was just part of the job,” explained Julian Cyrus, chief operating officer of Lunar Outpost. “But the sensors revealed where and when carbon monoxide levels were sky high, making it possible to issue warnings for firefighters to take precautions.”
The Canary-S sensors exemplify the life-saving technologies that can come from the collaboration of NASA and industry innovations.
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Last Updated Sep 17, 2024 Related Terms
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By Space Force
As Delivered by Chief of Space Operations U.S. Space Force Gen. Chance Saltzman on September 17, 2024
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By NASA
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
Urban air mobility means a safe and efficient system for vehicles, piloted or not, to move passengers and cargo within a city.NASA As the aviation industry evolves, new air vehicles and operators are entering the airspace. NASA is working to ensure these new diverse set of operations can be safely integrated into the current airspace. The agency is researching how traditional and emerging aircraft operations can efficiently operate in a shared airspace.
NASA’s Air Traffic Management-eXploration (ATM-X) project is a holistic approach to advancing a digital aviation ecosystem through research, development and testing. To accommodate the growing complexity and scale of new operations in Advanced Air Mobility (AAM), ATM-X leverages technologies that contribute to transforming the national airspace, improving airspace access, and making operations safer and more efficient for all users.
ATM-X fosters access to data by enhancing the availability of digital information and predictive services – including flight traffic predictions – for airspace operations.
ATM-X works closely with the Federal Aviation Administration (FAA), commercial partners, industry experts, and stakeholders in evaluating the sustainable impacts of emerging mobility solutions. ATM-X is conducting research to augment current key stakeholders that enable safe operations today such as pilots and air traffic controllers. Through these cooperations, ATM-X researches and validates technological advances in computing, communications, and increasingly automated technologies to support the continued evolution of aviation operations.
ATM-X supports the modernization of today’s air transportation system through a diverse portfolio of core capabilities, which include remotely supervised missions up through high-altitude operations. The four research subprojects under ATM-X work collaboratively to enable a robust transformation of the National Airspace System (NAS).
NASA/Maria Werries Unmanned Aircraft System Traffic Management Beyond-Visual-Line-of Sight (UTM-BVLOS)
UTM BVLOS is supporting the future of aviation by operationalizing UTM for safe use of drones in our everyday lives. UTM BVLOS is part of a new traffic management paradigm called Extensible Traffic Management (xTM) that will use digital information exchange, cooperative operating practices, and automation to provide air traffic management for remotely piloted operations for small UAS beyond an operator’s visual line of sight. This project focuses on enabling operations in a low- altitude airspace, including drone package delivery and public safety operations.
As the FAA works to authorize these types of flights, NASA’s UTM BVLOS team is working with industry to ensure these operations can be routine, safe, and efficient. One such effort is the industry-driven “Key Site Operational Evaluation” out of North Texas, where UTM BVLOS is helping to test UTM tools and services in an operational context.
Digital Information Platform (DIP)
DIP is focused on increasing access to digital information to enable increasingly sustainable and efficient operations for today and future airspace systems. DIP is prototyping a digital service-oriented framework that uses machine learning to provide information, including traffic predictions, weather information, and in-time flight trajectory updates. DIP tests and validates key services for end-to-end trajectory planning and surface operations.
DIP is engaging with the FAA, industry, flight operators, and relevant stakeholders, in a series of Sustainable Flight National Partnership – Operations demonstrations to support the United States Climate Action Plan objective of net-zero emissions by 2050. Through these types of collaborations, DIP tests and validates key services and capabilities for end-to-end trajectory planning and surface operations.
Pathfinding for Airspace with Autonomous Vehicles (PAAV)
PAAV is focused on enabling remotely piloted operations in today’s airspace, which includes assessing increasingly automated capabilities to allow safe operations across all phases of flight.
PAAV is working with key stakeholders, including the FAA, industry standards organizations, and industry partners to develop an ecosystem which helps validate standards, concepts, procedures, and technology. This research will help test and validate a broad range of tools and services that could provide critical information and functions necessary for remotely piloted operations at lower complexity airspace shared with conventional aircrafts. This includes ground-based surveillance to detect and avoid hazards, command and control communications, and relevant weather information, which is critical for safe, seamless, and scalable UAS cargo operations.
NAS Exploratory Concepts & Technologies (NExCT)
Advancements in aircraft design, power, and propulsion systems are enabling high-altitude long-endurance vehicles, such as balloons, airships, and solar aircraft to operate at altitudes of 60,000 feet and above. This airspace is referred to as “Upper Class E” airspace in the United States, or ETM. These advancements open doors to benefits ranging from increased internet coverage, improved disaster response, expanded scientific missions, to even supersonic flight. To accommodate and foster this growth, NExCT is developing a new traffic management concept in this airspace.
NExCT is working with the FAA and industry partners to extend a new concept for safely integrating and scaling air traffic across UTM, UAM, and ETM, collectively referenced as the Extensible Traffic Management (xTM) domain. Together, this research project will enable, test, and validate a common xTM framework that is efficient and safe.
ATM-X
AOSP
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Last Updated Sep 11, 2024 EditorJim BankeContactHillary Smithhillary.smith@nasa.gov Related Terms
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By NASA
5 min read
NASA, ESA Missions Help Scientists Uncover How Solar Wind Gets Energy
Since the 1960s, astronomers have wondered how the Sun’s supersonic “solar wind,” a stream of energetic particles that flows out into the solar system, continues to receive energy once it leaves the Sun. Now, thanks to a lucky lineup of a NASA and an ESA (European Space Agency)/NASA spacecraft both currently studying the Sun, they may have discovered the answer — knowledge that is a crucial piece of the puzzle to help scientists better forecast solar activity between the Sun and Earth.
A paper published in the Aug. 30, 2024, issue of the journal Science provides persuasive evidence that the fastest solar winds are powered by magnetic “switchbacks,” or large kinks in the magnetic field, near the Sun.
“Our study addresses a huge open question about how the solar wind is energized and helps us understand how the Sun affects its environment and, ultimately, the Earth,” said Yeimy Rivera, co-leader of the study and a postdoctoral fellow at the Smithsonian Astrophysical Observatory, part of Center for Astrophysics | Harvard & Smithsonian. “If this process happens in our local star, it’s highly likely that this powers winds from other stars across the Milky Way galaxy and beyond and could have implications for the habitability of exoplanets.”
This artist’s concept shows switchbacks, or large kinks in the Sun’s magnetic field. NASA’s Goddard Space Flight Center/Conceptual Image Lab/Adriana Manrique Gutierrez Previously, NASA’s Parker Solar Probe found that these switchbacks were common throughout the solar wind. Parker, which became the first craft to enter the Sun’s magnetic atmosphere in 2021, allowed scientists to determine that switchbacks become more distinct and more powerful close to the Sun. Up to now, however, scientists lacked experimental evidence that this interesting phenomenon actually deposits enough energy to be important in the solar wind.
“About three years ago, I was giving a talk about how fascinating these waves are,” said co-author Mike Stevens, astrophysicist at the Center for Astrophysics. “At the end, an astronomy professor stood up and said, ‘that’s neat, but do they actually matter?’”
To answer this, the team of scientists had to use two different spacecraft. Parker is built to fly through the Sun’s atmosphere, or “corona.” ESA’s and NASA’s Solar Orbiter mission is also on an orbit that takes it relatively close to the Sun, and it measures solar wind at larger distances.
The discovery was made possible because of a coincidental alignment in February 2022 that allowed both Parker Solar Probe and Solar Orbiter to measure the same solar wind stream within two days of each other. Solar Orbiter was almost halfway to the Sun while Parker was skirting the edge of the Sun’s magnetic atmosphere.
This conceptual image shows Parker Solar Probe about to enter the solar corona. NASA/Johns Hopkins APL/Ben Smith An artist’s concept shows Solar Orbiter near the Sun. NASA’s Goddard Space Flight Center Conceptual Image Lab
“We didn’t initially realize that Parker and Solar Orbiter were measuring the same thing at all. Parker saw this slower plasma near the Sun that was full of switchback waves, and then Solar Orbiter recorded a fast stream which had received heat and with very little wave activity,” said Samuel Badman, astrophysicist at the Center for Astrophysics and the other co-lead of the study. “When we connected the two, that was a real eureka moment.”
Scientists have long known that energy is moved throughout the Sun‘s corona and the solar wind, at least in part, through what are known as “Alfvén waves.” These waves transport energy through a plasma, the superheated state of matter that makes up the solar wind.
However, how much the Alfvén waves evolve and interact with the solar wind between the Sun and Earth couldn’t be measured — until these two missions were sent closer to the Sun than ever before, at the same time. Now, scientists can directly determine how much energy is stored in the magnetic and velocity fluctuations of these waves near the corona, and how much less energy is carried by the waves farther from the Sun.
The new research shows that the Alfvén waves in the form of switchbacks provide enough energy to account for the heating and acceleration documented in the faster stream of the solar wind as it flows away from the Sun.
“It took over half a century to confirm that Alfvenic wave acceleration and heating are important processes, and they happen in approximately the way we think they do,” said John Belcher, emeritus professor from the Massachusetts Institute of Technology who co-discovered Alfvén waves in the solar wind but was not involved in this study.
In addition to helping scientists better forecast solar activity and space weather, such information helps us understand mysteries of the universe elsewhere and how Sun-like stars and stellar winds operate everywhere.
“This discovery is one of the key puzzle pieces to answer the 50-year-old question of how the solar wind is accelerated and heated in the innermost portions of the heliosphere, bringing us closer to closure to one of the main science objectives of the Parker Solar Probe mission,” said Adam Szabo, Parker Solar Probe mission science lead at NASA.
By Megan Watzke
Center for Astrophysics | Harvard & Smithsonian
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Last Updated Aug 30, 2024 Related Terms
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