NASA Glenn Looking to Lease Facilities

As NASA advances its aviation and spaceflight missions, its facilities and infrastructure need to evolve along with them. NASA centers, including Glenn Research Center in Cleveland, must find ways to reduce the cost of maintaining assets they aren’t currently using.

Toward this goal, NASA Glenn is offering opportunities to lease assets it no longer uses. These Enhanced Use Lease (EUL) agreements will allow space, aeronautics, and other related industry to use Glenn land and facilities in direct support of NASA’s mission. It’s an arrangement that could bring some of the best minds in aerospace closer together, spurring innovation.

“We want to strategically align Glenn’s unique aircraft and spacecraft testing assets with the aviation industry and emerging commercial market,” said Carlos Flores, NASA Glenn’s Strategic Planning Branch chief. “Our hope is to expand partnerships, accelerate innovation, and create regional economic opportunities.”

Flores said there are many advantages for commercial entities to lease NASA facilities. These partners will have more access to resources—such as other facilities and technical expertise— than those outside the gate.

“Once a company or university gets a foot in the door, it is very possible they will discover other assets and expertise they can leverage,” Flores said.

Glenn identified four facilities in Cleveland and one in Sandusky, Ohio, that will be considered under the EUL authority. They include:

• Cryogenics Component Lab
• Altitude Combustion Stand
• Administration Building
• 2.2 Second Drop Tower
• Flight Research Building

In March, Glenn released an Announcement for Proposal, or AFP, to the public soliciting offers for the use of the Cryogenics Components Laboratory at NASA’s Neil Armstrong Test Facility in Sandusky. An AFP is expected for the Altitude Combustion Stand in Cleveland within a couple of months.

Glenn and other NASA centers continually work to align their facilities and infrastructure with the Agency Master Plan, which serves as a roadmap for future development and redevelopment of agency property.

To align with the Agency Master Plan, Glenn must reduce its “maintenance gap,” which is the amount of property owned versus the amount of property the center can afford to maintain.

“The maintenance gap is one of the realities we face in an environment of current and future budget constraints,” Flores said. 

While demolition is sometimes the easiest way to reduce square footage and maintenance costs, leasing can be a viable option for buildings that do not fit the demolition criteria.

“EULs will not only reduce the maintenance gap and the square footage we are responsible to maintain, but they will also enable us to create strategic partnerships and utilize revenue from the base rent for repairs to infrastructure,” Flores said.

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Kelly M. Matter

Hubble Glimpses a Star-Forming Factory

The celestial object showcased in this image from the NASA/ESA Hubble Space Telescope is the spiral galaxy UGC 9684, which lies around 240 million light-years from Earth in the constellation Boötes. This image shows an impressive example of several classic galactic features, including a clear bar in the galaxy’s center, and a halo surrounding its disk.

The data for this Hubble image came from a study of Type-II supernovae host galaxies. These cataclysmic stellar explosions take place throughout the universe, and are of great interest to astronomers, so automated surveys scan the night sky and attempt to catch sight of them. The supernova which brought UGC 9684 to Hubble’s attention occurred in 2020. It has since faded from view and is not visible in this image, which was taken in 2023.

Remarkably, the 2020 supernova isn’t the only one that astronomers have seen in this galaxy – UGC 9684 has hosted four supernova-like events since 2006, putting it up there with the most active supernova-producing galaxies. It turns out that UGC 9684 is a quite active star-forming galaxy, calculated as producing one solar mass worth of stars every few years! The most massive of these stars are short-lived, a few million years, and end their days as supernova explosions. This high level of star formation makes UGC 9684 a veritable supernova factory, and a galaxy to watch for astronomers hoping to examine these exceptional events.

Text Credit: European Space Agency (ESA)

Media Contact:

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

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NASA Invites Social Creators for Launch of NOAA Weather Satellite 

Registration is open for digital content creators to attend the launch of NOAA’s (National Oceanic and Atmospheric Administration) GOES-U (Geostationary Operational Environmental Satellite U) satellite, a mission to help improve weather observing and environmental monitoring capabilities on Earth, as well as improve space weather observations.

NASA and SpaceX are targeting a two-hour launch window opening at 5:16 p.m. EDT Tuesday, June 25, for the GOES-U launch on a SpaceX Falcon Heavy rocket from Launch Complex 39A at NASA’s Kennedy Space Center in Florida. NOAA’s GOES-U satellite will carry a suite of instruments for advanced imagery, atmospheric measurements, real-time mapping of lightning activity, and detecting approaching space weather hazards, including a new compact coronagraph that will image the outer layer of the Sun’s atmosphere to detect and characterize coronal mass ejections.

If your passion is to communicate and engage the world online, then this is the event for you! Seize the opportunity to see and share the #ReadyToGOES mission launch.

A maximum of 50 social media users will be selected to attend this two-day event and will be given access similar to news media.

NASA Social participants will have the opportunity to:

• View the launch of the GOES-U satellite on a SpaceX Falcon Heavy rocket.
• Tour NASA facilities at Kennedy Space Center.
• Meet and interact with GOES-U subject matter experts.
• Meet fellow space enthusiasts who are active on social media.

NASA Social registration for the GOES-U launch opens on Thursday, May 9, and the deadline to apply is 3 p.m. EDT Tuesday, May 14. All social applications will be considered on a case-by-case basis. 

APPLY NOW

Do I need to have a social media account to register?

Yes. This event is designed for people who: 

• Actively use multiple social networking platforms and tools to disseminate information to a unique audience. 
• Regularly produce new content that features multimedia elements. 
• Have the potential to reach a large number of people using digital platforms, or reach a unique audience, separate and distinctive from traditional news media and/or NASA audiences. 
• Must have an established history of posting content on social media platforms. 
• Have previous postings that are highly visible, respected, and widely recognized. 

Users on all social networks are encouraged to use the hashtag #NASASocial and #ReadyToGOES. Updates and information about the event will be shared via @NASASocial and @NASAKennedy on X and via posts to Facebook and Instagram. 

How do I register?

Registration for this event opens Thursday, May 9, and closes at 3 p.m. EDT on Tuesday, May 14. Registration is for one person only (you) and is nontransferable. Each individual wishing to attend must register separately. Each application will be considered on a case-by-case basis. 

Can I register if I am not a U.S. citizen?

Because of the security deadlines, registration is limited to U.S. citizens. If you have a valid permanent resident card, you will be processed as a U.S. citizen. 

When will I know if I am selected?

After registrations have been received and processed, an email with confirmation information and additional instructions will be sent to those selected. We expect to send the acceptance notifications by May 31. 

What are NASA Social credentials?

All social applications will be considered on a case-by-case basis. Those chosen must prove through the registration process that they meet specific engagement criteria. 

If you do not make the registration list for this NASA Social, you still can attend the launch offsite and participate in the conversation online. Find out about ways to experience a launch here. 

What are the registration requirements?

Registration indicates your intent to travel to NASA’s Kennedy Space Center in Florida and attend the two-day event in person. You are responsible for your own expenses for travel, accommodations, food, and other amenities. 

Some events and participants scheduled to appear at the event are subject to change without notice. NASA is not responsible for loss or damage incurred as a result of attending. NASA, moreover, is not responsible for loss or damage incurred if the event is cancelled with limited or no notice. Please plan accordingly. 

Kennedy is a government facility. Those who are selected will need to complete an additional registration step to receive clearance to enter the secure areas. 

IMPORTANT: To be admitted, you will need to provide two forms of unexpired government-issued identification; one must be a photo ID and match the name provided on the registration. Those without proper identification cannot be admitted. 

For a complete list of acceptable forms of ID, please visit: NASA Credentialing Identification Requirements. 

All registrants must be at least 18 years old. 

What if the launch date changes?

Many different factors can cause a scheduled launch date to change multiple times. If the launch date changes, NASA may adjust the date of the NASA Social accordingly to coincide with the new target launch date. NASA will notify registrants of any changes by email. 

If the launch is postponed, attendees will be invited to attend a later launch date. NASA cannot accommodate attendees for delays beyond 72 hours. 

NASA Social attendees are responsible for any additional costs they incur related to any launch delay. We strongly encourage participants to make travel arrangements that are refundable and/or flexible. 

What if I cannot come to the Kennedy Space Center?

If you cannot come to the Kennedy Space Center and attend in person, you should not register for the NASA Social. You can follow the conversation online using #NASASocial.  

You can watch the launch on NASA Television or www.nasa.gov/nasatv/. NASA will provide regular launch and mission updates on @NASA and @NASAKennedy. 

If you cannot make this NASA Social, don’t worry; NASA is planning many other Socials in the near future at various locations! Check back here for updates.

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Michelle Zajac

NASA Invites Media to NOAA’s Advanced Weather Satellite Launch

NASA is preparing to launch NOAA’s (National Oceanic and Atmospheric Administration) GOES-U (Geostationary Operational Environmental Satellite U), a mission to help improve weather observing and environmental monitoring capabilities on Earth, as well as advance space weather observations.

NASA and SpaceX are targeting a two-hour launch window opening at 5:16 p.m. EDT Tuesday, June 25. The mission will launch on a SpaceX Falcon Heavy rocket from Launch Complex 39A at NASA’s Kennedy Space Center in Florida.

The satellite will carry a suite of instruments for advanced imagery, atmospheric measurements, real-time mapping of lightning activity, and detecting approaching space weather hazards, including a new compact coronagraph that will image the outer layer of the Sun’s atmosphere to detect and characterize coronal mass ejections.

Media interested in covering the GOES-U launch must apply for media accreditation. Deadlines for accreditation are as follows:

• U.S. media and U.S. citizens representing international media must apply for accreditation by 11:59 p.m., Friday, June 7.
• International media without U.S. citizenship must apply by 11:59 p.m., Tuesday, May 28.

Media requiring special logistical arrangements, such as space for satellite trucks, tents, or electrical connections, should email ksc-media-accreditat@mail.nasa.gov by May 28.

A copy of NASA’s media accreditation policy is available online. For questions about accreditation, please email: ksc-media-accreditat@mail.nasa.gov. For other mission questions, please contact NASA Kennedy’s newsroom at: 321-867-2468.

Accredited media will have the opportunity to participate in a series of prelaunch briefings and interviews with key mission personnel. Details regarding the media event schedule will be communicated to accredited members as the launch date approaches.

NASA will post updates on launch preparations to prepare the spacecraft on the GOES blog.

As the fourth and final satellite in the GOES-R Series, GOES-U will enhance the nation’s ability to monitor and forecast weather, ocean, and environmental dynamics in real-time. The satellite has seven instruments that will provide advanced imagery and atmospheric measurements of Earth’s Western Hemisphere, real-time mapping of lightning activity, and advanced monitoring of solar activity and space weather. Following a successful launch and on-orbit checkout, NOAA will redesignate GOES-U as GOES-19. Working in tandem with GOES-18, the satellites will continuously observe Earth from the west coast of Africa to New Zealand, providing data for weather forecasting, severe storm tracking, and environmental monitoring. The GOES constellation helps protect the one billion people who live and work in the Americas.

NASA and NOAA collaborate on various missions to enhance our understanding of Earth, its climate, and its environment, enhancing the safety and well-being of all humanity. NASA’s Launch Services Program, based at Kennedy, manages the launch service for the GOES-U mission. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, oversees the acquisition of the spacecraft and instruments. Lockheed Martin designs, builds, and tests the GOES-R series satellites. L3Harris Technologies provides the primary instrument, the Advanced Baseline Imager, along with the ground system, which includes the antenna system for data reception.

For further details about the GOES-U mission and updates on launch preparations, visit:

https://go.nasa.gov/48httvm

-end-

Liz Vlock
Headquarters, Washington
202-358-1600
elizabeth.a.vlock@nasa.gov

Peter Jacobs
Goddard Space Flight Center, Greenbelt, Maryland
301-286-0535
peter.jacobs@nasa.gov

Leejay Lockhart
Kennedy Space Center, Florida
321-747-8310
leejay.lockhart@nasa.gov

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Abbey A. Donaldson

NASA Field Geology Training Prepares Artemis Mission Support Teams  

NASA engineers, managers, and flight directors recently traded their cubicles and conference rooms for an ancient volcanic field in the northern Arizona desert to participate in a field geology course aimed at arming them with first-hand experience in what Artemis astronauts will do when they explore the Moon. 

The two-and-a-half-day exercise for Artemis mission support teams was a condensed version of the rigorous training astronauts receive to prepare for Artemis missions to the lunar South Pole region, but shares an important purpose.  

“We are building a common language and a common understanding of what it will be like to do field geology on the surface of the Moon,” said Cindy Evans, Artemis geology training lead at NASA’s Johnson Space Center in Houston. “This is so the people who are building spacesuits, building tools, building software systems, the people who will be flight controllers, and the managers who direct and fund all of this, can all understand the interlocking parts of surface exploration.” 

We are building a common language and a common understanding of what it will be like to do field geology on the surface of the Moon.

Cindy Evans

Artemis Geology Training Lead at NASA’s Johnson Space Center

Small teams led by geology experts from NASA, the USGS (U.S. Geological Survey), and academia studied maps, built hypotheses about the geologic history of the area, and trekked for miles to test whether those hypotheses match reality. This field test required smashing rocks with hammers to study their mineral makeup, and carefully selecting a few to examine further after returning from the field in the same way Artemis astronauts will return samples from the Moon.  

Geology studies help uncover the rich physical history of an area. Each rock type represents a process and the order of layering of those rocks reveals a story that could unlock a planet’s secrets, offering clues for how it was formed and evolved over time.  

“The Moon doesn’t have an atmosphere or flowing water like we have here on Earth, and doesn’t have plate tectonics, which are processes that erase a lot of the evidence from the early Earth,” said Jacob Bleacher, chief exploration scientist in the Exploration Systems Development Mission directorate at NASA Headquarters in Washington. “The Moon still has that evidence, so we can go to the Moon and learn lessons about our home planet that we can’t learn here on the Earth.”  

In the desert, as the mission support team members practiced the fundamental methods used by geologists to study an environment, they pieced together the story of the region. The planned walking paths, known as traverses, frequently changed based on what they were finding. Teams embraced the principle of “flexecution” – or flexible execution – a practice that could come into play as astronauts explore the lunar surface and report findings to a backroom of scientists supporting the mission in the Mission Control Center at Johnson, referred to as the science evaluation room.  

“The geologists will be the science evaluation room during Artemis missions, assimilating real-time mission data to understand the observations, tracking the samples, going back to the maps that they’ve built trying to understand how all those pieces fit together on a day-by-day and traverse-by-traverse basis,” said Evans. “When the astronauts return home with the samples and with their full observations, the scientists can hit the ground running to address key science questions.” 

With Artemis, NASA will study the history of the Moon and its relationship with Earth and build a blueprint for deeper space exploration. 

“What we’re doing now is laying the groundwork for long-term exploration at the Moon,” Bleacher said. “Laying that groundwork will then help us explore other destinations like Mars. The Moon is a part of everything that we understand here on the Earth. It’s also an anchor point to help us understand how to interpret everything else in the solar system.” 

NASA conducts field tests in locations on Earth that have lunar-like landscapes to test a variety of operations and procedures, as well as new technologies, before leaving Earth for Artemis missions on the Moon. In addition to this geology training to build a foundation for mission support teams, another team will conduct simulated moonwalks in the Arizona desert this spring with mockup spacesuits to test hardware and new capabilities, like a heads-up display using augmented reality, for future Artemis missions.  

Through Artemis, NASA will send astronauts – including the first woman, first person of color, and its first international partner astronaut – to explore more of the lunar surface than ever before prepare for human missions to Mars for the benefit of all. 

Rachel Barry  
Johnson Space Center 

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Andrea Lloyd