NASA Glenn Established in Cleveland in 1941

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NASA Glenn Established in Cleveland in 1941

On January 23, 1941, local authorities, military representatives, and agency officials assembled in Cleveland to initiate construction of the National Advisory Committee for Aeronautics (NACA) new research laboratory. NACA Director of Research George Lewis stated, “I feel confident today in saying that this new aircraft engine research laboratory will be the mecca for all the world’s aircraft engine engineers and research workers.”

Today, the laboratory, now known as NASA’s John H. Glenn Research Center, is one of 10 centers and a leading economic contributor to the Cleveland area.

Exactly one year before the groundbreaking, the NACA formally proposed the creation of a new research lab dedicated to aero propulsion.  During the interim, the committee evaluated locations for the facility across the Midwest before selecting Cleveland, Ohio in November 1940.

The Cleveland Chamber of Commerce scheduled a full day of activities for that cold January Thursday in 1941. In the morning, the cadre of officials toured the Alcoa and the Cleveland Pneumatic Tool Company plants. The former was a key supplier of aluminum aircraft parts and the latter produced landing gears for the Douglas XB–19—then, the nation’s largest bomber.

Afterwards the group joined 240 local businessmen in the Hotel Cleveland’s Red Room for a luncheon hosted by Cleveland’s newly elected mayor Edward Blythin and Chamber of Commerce President Frederick Crawford. The George Worthington Hardware Company presented the NACA with a chrome-plated pick and shovel to be used for the groundbreaking.

NACA officials described the site selection activities, while Crawford reminded area businesses to maintain their pledges of support to the NACA.  Lewis told the attendees, “The future of aviation as regards to speed, efficiency, and safety, will, in a very large measure, depend on the results which come from this laboratory.”

With the war in Europe on the front pages, Edward Warner of Civil Aviation Authority added ominously, “What we are doing here today may mean the difference between America’s survival and subjugation. The difference between winning a war and losing it may be the difference between a 1,000- and 2,000-horsepower motor, or the difference between the ability to fly at 20,000 feet or 30,000 feet.”

In the afternoon the group traveled out to the construction site adjacent to Cleveland Municipal Airport. Shortly after 3 p.m., Lewis struck the ground with the chrome pick to loosen the soil, which Major General George Brett, acting chief of the Army Air Corps, then scooped up. The moment was immortalized by a local newspaper photographer.

That evening, Crawford held a dinner for the dignitaries at the Union Club. Construction of the NACA laboratory began in the ensuing days. Research commenced in May 1942.

Robert S. Arrighi
NASA’s Glenn Research Center

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Robert S. Arrighi

NASA’s IXPE Awarded Prestigious Prize in High-energy Astronomy

NASA’s IXPE (Imaging X-ray Polarimetry Explorer) team has been awarded a top prize in high-energy astronomy.

The High Energy Astrophysics Division of the American Astronomical Society (AAS) has awarded the 2024 Bruno Rossi Prize to retired NASA astrophysicist Martin Weisskopf, Italian Space Agency principal investigator Paolo Soffitta, and their team for development of IXPE, “whose novel measurements advance our understanding of particle acceleration and emission from astrophysical shocks, black holes and neutron stars,” according to the AAS announcement.

“IXPE is a realization of decades of work and belief in the importance of X-ray polarization measurements for X-ray astronomy,” said Weisskopf of NASA’s Marshall Space Flight Center in Huntsville, Alabama, who served as the principal investigator of IXPE during its development, prior to retiring from the agency in 2022. “I am honored and excited to share this prize with Paolo Soffitta and the entire IXPE team.”

“IXPE is the demonstration of how an idea pursued for more than 30 years has been transformed into a successful mission, thanks to the collaboration between the United States and Italy,” Soffitta said. “It’s incredible to receive this prize along with Martin Weisskopf and on behalf of so many people whose expertise and enthusiasm have made this breakthrough in astrophysics possible.”

Launched on Dec. 9, 2021, and developed by NASA, the Italian Space Agency, and partners in a dozen countries around the globe, IXPE orbits Earth some 340 miles up to observe X-ray emissions from powerful cosmic phenomena hundreds or thousands of light-years from Earth. In 2023 alone, its subjects of study included blazars such as Markarian 501 and Markarian 421, supernova remnants including Tycho and SN 1006, and the supermassive black hole at the center of our own galaxy.

IXPE also supports study of unanticipated cosmic events – such as the brightest pulse of high-energy radiation ever recorded, which swept through Earth’s solar system in late 2022. IXPE’s success led NASA to formally extend the mission for an additional 20 months, through at least September 2025.

“We at NASA are incredibly proud of Dr. Weisskopf and the IXPE team around the world,” said Acting Marshall Center Director Joseph Pelfrey. “IXPE allows us to look at the universe through a vantage point never seen before. It’s particularly gratifying to continue Marshall’s long association with the Rossi Prize, which identifies singular breakthroughs and unprecedented innovation in high-energy astrophysics – a field in which our researchers excel.”

Weisskopf, together with Harvard astrophysicist Harvey Tananbaum, previously received the Rossi Prize in 2004 for their work to develop and fly NASA’s Chandra X-ray Observatory, which continues to study high-energy X-ray phenomena across the cosmos. NASA Marshall researchers Gerald Fishman and Colleen Wilson-Hodge also were awarded the Rossi Prize in 1994 and 2018, respectively. Fishman was honored for his contributions to the Compton Gamma-ray Observatory’s BATSE (Burst and Transient Source Experiment) mission. Wilson-Hodge received the honor for her work with the Fermi GBM (Gamma-ray Burst Monitor) in August 2017, detecting gravitational and light waves from the spectacular smashup of two neutron stars in a distant galaxy.

The Rossi Prize is awarded annually for a significant recent contribution to high-energy astrophysics. The honor includes an engraved certificate and a $1,500 award.

Learn more about NASA’s high-energy astrophysics research:

https://science.nasa.gov/astrophysics

Elizabeth Landau
NASA Headquarters
elizabeth.r.landau@nasa.gov
202-358-0845

Jonathan Deal
Marshall Space Flight Center, Huntsville, Ala.
256-544-0034
jonathan.e.deal@nasa.gov

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Hubble Glimpses a Bright Galaxy Group

This new NASA Hubble Space Telescope image shows a group of interacting galaxies known as LEDA 60847.

LEDA 60847 is classified as an active galactic nuclei, or AGN. An AGN has a supermassive black hole in the galaxy’s central region that is accreting material. The AGN emits radiation across the entire electromagnetic spectrum and shines extremely brightly. By studying powerful AGNs that are relatively nearby, astronomers can better understand how supermassive black holes grow and affect galaxies.

Galaxy mergers are relatively common occurrences. Most larger galaxies are the result of smaller galaxies merging. The Milky Way itself contains traces of other galaxies, indicating it is the product of past mergers. Astronomers believe somewhere between 5% and 25% of all galaxies are currently merging. 

This image of LEDA 60847 combines ultraviolet, visible, and near-infrared data from Hubble. The ability to see across all those wavelengths is one of the things that makes Hubble unique. Different types of light across the electromagnetic spectrum tell astronomers different things about our universe. Ultraviolet light traces the glow of stellar nurseries and is used to identify the hottest stars. Visible light shows us moderate-temperature stars and material, and also how the view would appear to our own eyes. Last but not least, near-infrared light can penetrate cold dust, allowing us to study warm gas and dust, and relatively cool stars.

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Media Contact:

Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, MD
claire.andreoli@nasa.gov

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NASA Invites Media to First Intuitive Machines, SpaceX Moon Launch

As part of NASA’s CLPS (Commercial Lunar Payload Services) initiative and Artemis campaign, media accreditation is open for Intuitive Machines’ first robotic flight to the Moon’s surface. The robotic deliveries will transport agency science and technology demonstrations to the Moon for the benefit of all.

The Intuitive Machines Nova-C lander carrying NASA science and commercial payloads will launch on a SpaceX Falcon 9 rocket. Liftoff is targeted for a multi-day launch window, which opens no earlier than mid-February, from Launch Complex 39A at NASA’s Kennedy Space Center in Florida.

Among the NASA items on its lander, the Intuitive Machines mission will carry instruments focusing on plume-surface interactions, space weather/lunar surface interactions, radio astronomy, precision landing technologies, and a communication and navigation node for future autonomous navigation technologies. A successful landing will help support the CLPS model for commercial payload deliveries to the lunar surface. As the anchor customer of CLPS, NASA is investing in lower-cost methods of Moon deliveries and aims to be one of many customers.

Media prelaunch and launch activities will take place at NASA Kennedy. Media who are U.S. citizens interested in attending in person must apply for credentials no later than 12 p.m. EST on Monday, Jan. 29, by emailing media@spacex.com.  

In May 2019, NASA awarded a task order for the delivery to Intuitive Machines. Through Artemis, commercial robotic deliveries will perform science experiments, test technologies, and demonstrate capabilities to help NASA explore the Moon in advance of Artemis Generation astronaut missions to the lunar surface, in preparation for future missions to Mars.

NASA is working with several U.S. companies to deliver science and technology to the lunar surface through the agency’s CLPS initiative. This pool of companies may bid on delivery task orders. A task order award includes payload integration and operations, as well as launching from Earth and landing on the surface of the Moon. NASA’s CLPS contracts are indefinite-delivery/indefinite-quantity contracts with a cumulative maximum contract value of $2.6 billion through 2028.

For more information about the agency’s Commercial Lunar Payload Services initiative, see:

https://www.nasa.gov/clps

-end-

Alise Fisher
Headquarters, Washington
202-358-2546
alise.m.fisher@nasa.gov  

Nilufar Ramji
Johnson Space Center, Houston
281-483-5111
nilufar.ramji@nasa.gov

Antonia Jaramillo
Kennedy Space Center, Florida
321-501-8425
antonia.jaramillobotero@nasa.gov

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Roxana Bardan