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A nuclear explosion in space would cause stunning auroras—and wreak havoc on satellites and space stations.

SpaceX launched 20 of its Starlink satellites from California on Tuesday night (June 18), ending a 10-day spaceflight drought for the company.

The Hubble Space Telescope has experienced ongoing problems with one of its three remaining gyroscopes, so NASA has decided to shift the telescope into single gyro mode. While the venerable space telescope has now returned to daily science operations, single gyro mode means Hubble will only use one gyro to maintain a lock on its target. This will slow its slew time and decrease some of its scientific output. But this plan increases the overall lifetime of the 34-year-old telescope, keeping one gyro in reserve. NASA is also troubleshooting the malfunctioning gyro, hoping to return it online.

Last week, NASA said that the telescope and its instruments are stable and functioning normally.

Gyroscopes help the telescope orient itself in space, keeping it stable to precisely point at astronomical targets in the distant Universe. Hubble went into safe mode back in November 2023, and then again in April and May 2024 due to the ongoing issue, where the one gyro had been increasingly returning faulty readings.

The end of a Hubble gyro reveals the hair-thin wires known as flex leads. They carry data and electricity inside the gyro. Credit: NASA

Going in to safe mode suspends science operations, and in the meantime, engineers tried to troubleshoot to figure out why the gyro experiencing the fault-producing issues and doing work-arounds to get the telescope up and running again. The most recent last safe-mode event in May led the Hubble team to transition from a three-gyro operating mode to observing with only one gyro. This enables more consistent science observations while keeping the other operational gyro available for future use.

Launched in 1990, Hubble has more than doubled its expected design lifetime, providing stunning images and scientific discoveries that have changed our understanding of the Universe and re-written astronomy textbooks.  

During its 34-year history, Hubble has had eight out of 22 gyros fail due to a corroded flex lead, which are thin (less than the width of a human hair) metal wires, that carry power in, and data out, of the gyro.  The flex leads pass through a thick fluid inside the gyro and over time, the flex leads begin to corrode and can physically bend or break.

With his feet firmly anchored on the shuttle’s robotic arm, astronaut Mike Good maneuvers to retrieve the tool caddy required to repair the Space Telescope Imaging Spectrograph during the final Hubble servicing mission in May 2009. Periodic upgrades have kept the telescope equipped with state-of-the-art instruments, which have given astronomers increasingly better views of the cosmos. Credits: NASA

Thankfully, for the first 18 years of Hubble’s life in space, the telescope had the advantage of being able to be serviced and upgraded by space shuttle astronauts. For example, in 1999, four out of six gyros had failed, with the last one failing about a month before a servicing mission was scheduled to replace them (and do other upgrades to the telescope). This meant Hubble sat in safe mode waiting for the space shuttle and astronauts to arrive.

When the final planned Hubble servicing mission was (temporarily) canceled following the space shuttle Columbia disaster, engineers developed and inaugurated a two-gyro mode to prolong Hubble’s life. The mission was reinstated after outcry from scientists and the public, and so NASA figured out a way to mitigate the risks of flying the space shuttle. Servicing Mission 4 replaced all six gyros one last time in 2009, but it has been running on three since 2018. The three gyros all quit working due to flex lead failures. The retirement of the space shuttle means Hubble has now been operating for 15 years without servicing.

The Hubble Rate Gyro Assembly contains a gyroscope and all of its associated electronics. The gyroscopes are part of Hubble’s pointing system. They provide a frame of reference for Hubble to determine where it is pointing and how that pointing changes as the telescope moves across the sky. They report any small movements of the spacecraft to Hubble’s pointing and Control System. The computer then commands the spinning reaction wheels to keep the spacecraft stable or moving at the desired rate. Credit: NASA

However, during the time it was thought no future servicing mission would happen, the team also devised a one-gyro mode, which will further extend Hubble’s life.

“We knew gyros would be a limiting factor so we started to working on a reduced gyro mode to extend their life,” the director of the Space Telescope Science Institute Ken Sembach told me back in 2015 for my book, “Incredible Stories From Space.” “As it turned out, we did need that reduced gyro mode, and now they aren’t [as big of a] limiting factor for Hubble because we now know how to use the gyro resources in a new way. That added a longer life to the mission we didn’t think we would have.”

While engineers say the difference between two-gyro mode and one gyro-mode is negligible, one-gyro mode provides the option to have one of the remaining gyros placed in reserve.

NASA says that although one-gyro mode is an excellent way to keep Hubble science operations going, it does have limitations, which include a small decrease in efficiency (roughly 12 percent) due to the added time required to slew and lock the telescope onto a science target. One gyro mode also means it takes additional time for the telescope’s fine guidance sensors to search for the guide stars. Additionally, in one-gyro mode Hubble has some restrictions on the science it can do. For example, Hubble cannot track moving objects that are closer to Earth than the orbit of Mars. Without the full complement of gyros, the motion of these objects are too fast for the telescope to track. Additionally, the reduced area of sky that Hubble can point to at any given time also reduces its flexibility to see transient events or targets of opportunity like an exploding star or an impact on Jupiter. NASA says that when combined, “these factors may yield a decrease in productivity of roughly 20 to 25 percent from the typical observing program conducted in the past using all three gyros.”

Read more about the “new normal” for Hubble’s one-gyro mode at this NASA webpage.

The post Hubble's Back, but Only Using One Gyro appeared first on Universe Today.

Slovenia signed the Accession Agreement to the ESA Convention on 18 June 2024. Upon ratification, Slovenia will become the 23rd ESA Member State.

The appearance this week of the three bright Summer Triangle stars — Vega, Deneb and Altair — marks the beginning of summer in the Northern Hemisphere. Here's how to spot them.

20 Min Read The Marshall Star for June 18, 2024 California Teams Win $1.5 Million in NASA’s Break the Ice Lunar Challenge

By Savannah Bullard

After two days of live competitions, two teams from southern California are heading home with a combined $1.5 million from NASA’s Break the Ice Lunar Challenge. 

Since 2020, competitors from around the world have competed in this challenge with the common goal of inventing robots that can excavate and transport the icy regolith on the Moon. The lunar South Pole is the targeted landing site for crewed Artemis missions, so utilizing all resources in that area, including the ice within the dusty regolith inside the permanently shadowed regions, is vital for the success of a sustained human lunar presence.

The husband-and-wife duo of Terra Engineering, Valerie and Todd Mendenhall, receive the $1 million prize June 12, for winning the final phase of NASA’s Break the Ice Lunar Challenge at Alabama A&M’s Agribition Center in Huntsville. With the Terra Engineering team at the awards ceremony are from left, Daniel K. Wims, Alabama A&M University president; Joseph Pelfrey, NASA Marshall Space Flight center director; NASA’s Break the Ice Challenge Manager Naveen Vetcha, and Majed El-Dweik, Alabama A&M University’s vice president of Research & Economic Development.NASA/Jonathan Deal

On Earth, the mission architectures developed in this challenge aim to help guide machine design and operation concepts for future mining and excavation operations and equipment for decades.

“Break the Ice represents a significant milestone in our journey toward sustainable lunar exploration and a future human presence on the Moon,” said Joseph Pelfrey, center director of NASA’s Marshall Space Flight Center. “This competition has pushed the boundaries of what is possible by challenging the brightest minds to devise groundbreaking solutions for excavating lunar ice, a crucial resource for future missions. Together, we are forging a future where humanity ventures further into the cosmos than ever before.”

The final round of the Break the Ice competition featured six finalist teams who succeeded in an earlier phase of the challenge. The competition took place at the Alabama A&M Agribition Center in Huntsville on June 11 and 12, where each team put their diverse solutions to the test in a series of trials, using terrestrial resources like gravity-offloading cranes, concrete slabs, and a rocky track with tricky obstacles to mimic the environment on the Moon.

The husband-and-wife duo of Terra Engineering took home the top prize for their “Fracture” rover. Team lead Todd Mendenhall competed in NASA’s 2007 Regolith Excavation Challenge, facilitated through NASA’s Centennial Challenges, which led him and Valerie Mendenhall to continue the pursuit of solutions for autonomous lunar excavation.

A small space hardware business, Starpath Robotics, earned the second-place prize for its four-wheeled rover that can mine, collect, and haul material. The team, led by Saurav Shroff and lead engineer Mihir Gondhalekar, developed a robotic mining tool that features a drum barrel scraping mechanism for breaking into the tough lunar surface. This allows the robot to mine material quickly and robustly without sacrificing energy.

“This challenge has been pivotal in advancing the technologies we need to achieve a sustained human presence on the Moon,” said Kim Krome, the Acting Program Manager for NASA’s Centennial Challenges. “Terra Engineering’s rover, especially, bridged several of the technology gaps that we identified – for instance, being robust and resilient enough to traverse rocky landscapes and survive the harsh conditions of the lunar South Pole.”

Starpath Robotics earned the second place prize for its four-wheeled rover that can mine, collect, and haul material during the final phase of NASA’s Break the Ice Lunar Challenge. From left, Matt Kruszynski, Saurav Shroff, Matt Khudari, Alan Hsu, David Aden, Mihir Gondhalekarl, Joshua Huang, and Aakash Ramachandran.NASA/Jonathan Deal

Beyond the $1.5 million in prize funds, three teams will be given the chance to use Marshall Space Flight Center’s thermal vacuum (TVAC) chambers to continue testing and developing their robots. These chambers use thermal vacuum technologies to create a simulated lunar environment, allowing scientists and researchers to build, test, and approve hardware for flight-ready use.

The following teams performed exceptionally well in the excavation portion of the final competition, earning these invitations to the TVAC facilities:

• Terra Engineering (Gardena, California)
• Starpath Robotics (Hawthorne, California)
• Michigan Technological University – Planetary Surface Technology Development Lab (Houghton, Michigan)

“We’re looking forward to hosting three of our finalists at our thermal vacuum chamber, where they will get full access to continue testing and developing their technologies in our state-of-the-art facilities,” said Break the Ice Challenge Manager Naveen Vetcha, who supports NASA’s Centennial Challenges through Jacobs Space Exploration Group. “Hopefully, these tests will allow the teams to take their solutions to the next level and open the door for opportunities for years to come.”

NASA’s Break the Ice Lunar Challenge is a NASA Centennial Challenge led by the agency’s Marshall Space Flight Center, with support from NASA’s Kennedy Space Center. Centennial Challenges are part of the Prizes, Challenges, and Crowdsourcing program under NASA’s Space Technology Mission Directorate. Ensemble Consultancy supports challenge competitors. Alabama A&M University, in coordination with NASA, supports the final competitions and winner event for the challenge.

Bullard, a Manufacturing Technical Solutions Inc. employee, supports the Marshall Office of Communications.

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NASA Announces Winners of 2024 Student Launch Competition

Over 1,000 students from across the U.S. and Puerto Rico launched high-powered, amateur rockets on April 13, just north of NASA’s Marshall Space Flight Center, as part of the agency’s annual Student Launch competition.

Teams of middle school, high school, college, and university students were tasked to design, build, and launch a rocket and scientific payload to an altitude between 4,000 and 6,000 feet, while making a successful landing and executing a scientific or engineering payload mission.

High school and collegiate student teams gathered just north of NASA’s Marshall Space Flight Center to participate in the agency’s annual Student Launch competition April 13.Credits: NASA/Charles Beason

“These bright students rise to a nine-month challenge that tests their skills in engineering, design, and teamwork,” said Kevin McGhaw, director of NASA’s Office of STEM Engagement Southeast Region. “They are the Artemis Generation, the future scientists, engineers, and innovators who will lead us into the future of space exploration.”

NASA announced the University of Notre Dame is the overall winner of the agency’s 2024 Student Launch challenge, followed by Iowa State University, and the University of North Carolina at Charlotte. A complete list challenge winners can be found on the agency’s student launch web page. NASA presented the 2024 Student Launch challenge award winners in a virtual award ceremony June 7.

Each year NASA implements a new payload challenge to reflect relevant missions. This year’s payload challenge is inspired by the Artemis missions, which seek to land the first woman and first person of color on the Moon.

The complete list of award winners are as follows:

2024 Overall Winners

• First place: University of Notre Dame, Indiana
• Second place: Iowa State University, Ames
• Third place: University of North Carolina at Charlotte

3D Printing Award:

College Level:

• First place: University of Tennessee Chattanooga

Middle/High School Level:

• First place: First Baptist Church of Manchester, Manchester, Connecticut

Altitude Award

College Level:

• First place: Iowa State University, Ames

Middle/High School Level:

• First place: Morris County 4-H, Califon, New Jersey

Best-Looking Rocket Award:

College Level:

• First place: New York University, Brooklyn, New York

Middle/High School Level:

• First place: Notre Dame Academy High School, Los Angeles

American Institute of Aeronautics and Astronautics Reusable Launch Vehicle Innovative Payload Award:

College Level:

• First place: University of Colorado Boulder
• Second place: Vanderbilt University, Nashville, Tennessee
• Third place: Carnegie Mellon, Pittsburgh, Pennsylvania

Judge’s Choice Award:

Middle/High School Level:

• First place: Cedar Falls High School, Cedar Falls, Iowa
• Second place: Young Engineers in Action, LaPalma, California
• Third place: First Baptist Church of Manchester, Manchester, Connecticut

Project Review Award:

College Level:

• First place: University of Florida, Gainesville

AIAA Reusable Launch Vehicle Award:

College Level:

• First place: University of Florida, Gainesville
• Second place: University of North Carolina at Charlotte
• Third place: University of Notre Dame, Indiana

AIAA Rookie Award:

College Level:

• First place: University of Colorado Boulder

Safety Award:

College Level:

• First place: University of Notre Dame, Indiana
• Second place: University of Florida, Gainesville
• Third place: University of North Carolina at Charlotte

Social Media Award:

College Level:

• First place: University of Colorado Boulder

Middle/High School Level:

• First place: Newark Memorial High School, Newark, California

STEM Engagement Award:

College Level:

• First place: University of Notre Dame, Indiana
• Second place: University of North Carolina at Charlotte
• Third place: New York University, Brooklyn, New York

Middle/High School Level:

• First place: Notre Dame Academy High School, Los Angeles, California
• Second place: Cedar Falls High School, Cedar Falls, Iowa
• Third place: Thomas Jefferson High School for Science and Technology, Alexandria, Virginia

Service Academy Award:

First place: United States Air Force Academy, USAF Academy, Colorado

Vehicle Design Award:

Middle/High School Level:

• First place: First Baptist Church of Manchester, Manchester, Connecticut
• Second place: Explorer Post 1010, Rockville, Maryland
• Third place: Plantation High School, Plantation, Florida

Payload Design Award:

Middle/High School Level:

• First place: Young Engineers in Action, LaPalma, California
• Second place: Cedar Falls High School, Cedar Falls, Iowa
• Third place: Spring Grove Area High School, Spring Grove, Pennsylvania

Student Launch is one of NASA’s nine Artemis Student Challenges, activities which connect student ingenuity with NASA’s work returning to the Moon under Artemis in preparation for human exploration of Mars.

The competition is managed by Marshall’s Office of STEM Engagement (OSTEM). Additional funding and support are provided by NASA’s OSTEM via the Next Gen STEM project, NASA’s Space Operations Mission Directorate, Northrup Grumman, National Space Club Huntsville, American Institute of Aeronautics and Astronautics, National Association of Rocketry, Relativity Space, and Bastion Technologies.

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Keith Savoy Named Deputy Director at Michoud Assembly Facility

Keith Savoy has been named deputy director of NASA’s Michoud Assembly Facility, effective June 16.

Savoy will assist in managing the day-to-day operations of one of the world’s largest manufacturing facilities, where key elements of NASA’s Space Launch System (SLS), and Orion spacecraft are built. Michoud, a multi-tenant manufacturing site sitting on 829 acres with over 2 million square feet of manufacturing space, is managed by NASA’s Marshall Space Flight Center and provides facility infrastructure and capacity for federal, state, academic, and technology-based industry partners.

Keith Savoy has been named deputy director of NASA’s Michoud Assembly Facility.NASA

Savoy was the chief operating officer of Michoud Assembly Facility from 2022-2024, where he oversaw the day-to-day administrative and operational functions of the NASA-owned facility, helping sustain SLS and Orion production efforts and coordinating requirements and logistics with Michoud tenant leadership for approximately 3,500 Michoud employees.

He previously served as manager of the Office of Center Operations of Michoud from 2016-2022. His responsibilities included managing the facility’s planning, maintenance, design, construction, and engineering. Savoy also oversaw energy and water conservation, environmental permitting and compliance, industrial hygiene, and medical, security, and logistics services, where he was responsible for managing over $350 million of supplemental funding projects sitewide.

Savoy also held the position of lead engineer, Logistics and Operation Planning for NASA from 2007-2016 at Michoud as an expert consultant for all engineering aspects of the facility. He managed multi-phase projects and helped advance aerospace manufacturing at Michoud to meet the complex requirements of SLS and Orion multi-purpose crew vehicle programs, ensuring environmental compliance. Savoy worked closely with local, state, and federal environmental regulatory agencies to identify and resolve engineering and environmental issues. His expertise was a key contributor to ensuring NASA’s sustainable and environmental goals were achieved.

Prior to working for NASA, Savoy held several positions of increasing responsibility with Lockheed Martin from 1988-2007. As manager of Operational Planning and Layout, he was responsible for managing the Construction of Facilities. This required developing and implementing plans, outlining scope-of-work, overseeing large-scale project budgets, and Project Definition Rating assessment/score and 1509 development. Savoy implemented Six Sigma & Lean principles concepts to achieve many successes and identified innovative solutions and best practices to satisfy customer requirements. Savoy was also the manager of the Infrastructure Enhancement Team where he managed over 160 personnel and a $10 million budget.

Savoy has a Master of Science in environmental management from National Technological University in Fort Collins, Colorado, a bachelor of science in electrical engineering from the University of Louisiana-Lafayette, and a technical degree in industrial instrumentation from International Technical Institute in Baton Rouge, Louisiana.

Throughout his career, Savoy has received various awards including the NASA Honor Award Outstanding Leadership Medal, Director’s Commendation Honor Award, Safety Flight Awareness Awards, and several Silver Medal Group Achievement Awards.

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‘NASA in the Park’ Returns to Rocket City June 22

NASA in the Park is coming back to Big Spring Park East in Huntsville, Alabama, on June 22, from 10 a.m. to 2 p.m. CDT. The event is free and open to the public.

NASA’s Marshall Space Flight Center, its partners, and collaborators will fill the park with space exhibits, music, food vendors, and hands-on activities for all ages. Marshall is teaming up with Downtown Huntsville Inc. for this unique celebration of space and the Rocket City.

“NASA in the Park gives us the opportunity to bring our work outside the gates of Redstone Arsenal and thank the community for their continuing support,” Marshall Director Joseph Pelfrey said. “It’s the first time we’ve held the event since 2018, and we look forward to sharing this experience with everyone.”

Pelfrey will kick the event off with local leaders on the main stage. NASA speakers will spotlight topics ranging from space habitats to solar sails, and local rock band Five by Five will perform throughout the day.

“NASA Marshall is leading the way in this new era of space exploration, for the benefit of all humankind,” Pelfrey said. “We are proud members of the Rocket City community, which has helped us push the boundaries of science, technology, and engineering for nearly 65 years.”

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Mission Success is in Our Hands: Baraka Truss

By Wayne Smith

Mission Success is in Our Hands is a safety initiative collaboration between NASA’s Marshall Space Flight Center and Jacobs. As part of the initiative, eight Marshall team members are featured in testimonial banners placed around the center. This is the last in a Marshall Star series profiling team members featured in the testimonial banners. The Mission Success team also awards the Golden Eagle Award on a quarterly basis to Marshall and contractor personnel who are nominated by their peers or management. Candidates for this award have made significant, identifiable contributions that exceed normal job expectations to advance flight safety and mission assurance. Nominations for 2024 are open now online on Inside Marshall.

Baraka Truss is the Avionics and Software Branch chief at NASA’s Marshall Space Flight Center. NASA/Charles Beason

Baraka Truss is the Avionics and Software Branch chief in the Safety and Mission Assurance Organization, Vehicle Systems Department, at NASA’s Marshall Space Flight Center. Her key responsibilities include being viewed as a leadership role model, “demonstrating commitment to the mission and NASA’s core values, creating the most impact for the greater agency, and engaging in activities that promote supervisory excellence and value beyond the immediate organization.”

Truss has worked at Marshall for 28 years. Her previous roles have been software engineer, Software Engineering Process Group lead, special assistant to the center director, Independent Assessment Team lead, Software Quality Discipline lead engineer, Software Assurance Team lead, and     SLS (Space Launch System) Software chief safety officer.

A native of Montgomery, Alabama, Truss earned a bachelor’s and master’s degree in computer science from Alabama A&M University in Huntsville.

Question: How does your work support the safety and success of NASA and Marshall missions?

Truss: My work involves daily managing and interactions with the avionics and software team members whose mission is to ensure the safety of hardware and software for various programs and projects at Marshall and NASA.

Question: What does the initiative campaign “Mission Success is in Our Hands” mean to you?

Truss: That when risks arise, we should be sure to listen to all sides and make informed decisions, be held accountable, and speak up for what is safe when we need to do so.

Question: Do you have a story or personal experience you can share that might help others understand the significance of mission assurance or flight safety? What did you learn from it?

Truss: In my experience, mission assurance requires you to “believe the unlikely.” I have learned that believing what you have never seen requires you to stretch your imagination, because we are prone to discount and devalue things that we have not seen. We are skeptical about things that have never been seen, never been done, never been achieved, or never been accomplished.

Because according to our limited logic if it’s never been seen, never been done, never been achieved, or never been accomplished, then it’s not likely to be seen, not likely to be done, not likely to be achieved, and not likely to be accomplished. Therefore, we see no need to attempt it, try it, believe it, or invest in it because while we’ll acknowledge that it’s possible, we quickly add it’s not probable, because our idea of likelihood is limited by our experience. My experiences working for NASA have stretched me to an amazing place of accountability, assurance, and mission success.

Question: How can we work together better to achieve mission success?

Truss: Again, by listening to all sides and making informed decisions, being held accountable, and speaking up for what is safe when we need to do so.

Smith, a Media Fusion employee and the Marshall Star editor, supports the Marshall Office of Communications.

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That’s the Spirit: Marshall Team Members Show Support at Community Softball Game

NASA shows its team spirit during the Armed Forces Celebration Community Softball Game on June 12 at Toyota Field. Marshall Space Flight Center’s Robert Champion and Jason Adam joined Team Redstone to take on the North Alabama Rockets, made up of community leaders. (Huntsville Sports Commission)

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Coming in Hot: NASA’s Chandra Checks Habitability of Exoplanets

This graphic shows a three-dimensional map of stars near the Sun. These stars are close enough that they could be prime targets for direct imaging searches for planets using future telescopes. The blue haloes represent stars that have been observed with NASA’s Chandra X-ray Observatory and ESA’s XMM-Newton. The yellow star at the center of this diagram represents the position of the Sun. The concentric rings show distances of 5, 10, and 15 parsecs (one parsec is equivalent to roughly 3.2 light-years).

Astronomers are using these X-ray data to determine how habitable exoplanets may be based on whether they receive lethal radiation from the stars they orbit, as described in a press release. This type of research will help guide observations with the next generation of telescopes aiming to make the first images of planets like Earth.

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This video shows a three-dimensional map of stars near the Sun on the left side of the screen and a dramatic illustration of a star with a planet orbiting around it on the right side.Movie: Cal Poly Pomona/B. Binder; Illustration: NASA/CXC/M.Weiss

Researchers examined stars that are close enough to Earth that telescopes set to begin operating in the next decade or two – including the Habitable Worlds Observatory in space and Extremely Large Telescopes on the ground – could take images of planets in the stars’ so-called habitable zones. This term defines orbits where the planets could have liquid water on their surfaces.

There are several factors influencing what could make a planet suitable for life as we know it. One of those factors is the amount of harmful X-rays and ultraviolet light they receive, which can damage or even strip away the planet’s atmosphere.

Based on X-ray observations of some of these stars using data from Chandra and XMM-Newton, the research team examined which stars could have hospitable conditions on orbiting planets for life to form and prosper. They studied how bright the stars are in X-rays, how energetic the X-rays are, and how much and how quickly they change in X-ray output, for example, due to flares. Brighter and more energetic X-rays can cause more damage to the atmospheres of orbiting planets.

The researchers used almost 10 days of Chandra observations and about 26 days of XMM observations, available in archives, to examine the X-ray behavior of 57 nearby stars, some of them with known planets. Most of these are giant planets like Jupiter, Saturn or Neptune, while only a handful of planets or planet candidates could be less than about twice as massive as Earth.

These results were presented at the 244th meeting of the American Astronomical Society meeting in Madison, Wisconsin, by Breanna Binder (California State Polytechnic University in Pomona).

NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science from Cambridge, Massachusetts and flight operations from Burlington, Massachusetts.

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NASA Announces New System to Aid Disaster Response

In early May, widespread flooding and landslides occurred in the Brazilian state of Rio Grande do Sul, leaving thousands of people without food, water, or electricity. In the following days, NASA teams provided data and imagery to help on-the-ground responders understand the disaster’s impacts and deploy aid.

Building on this response and similar successes, on June 13, NASA announced a new system to support disaster response organizations in the U.S. and around the world.

Members of the Los Angeles County Fire Department’s Urban Search and Rescue team in Adiyaman, Turkey, conducting rescue efforts in the wake of powerful earthquakes that struck the region in February 2023. NASA provided maps and data to support USAID and other regional partners during these earthquakes.USAID

“When disasters strike, NASA is here to help – at home and around the world,” said NASA Administrator Bill Nelson. “As challenges from extreme weather grow, so too does the value of NASA’s efforts to provide critical Earth observing data to disaster-response teams on the frontlines. We’ve done so for years. Now, through this system, we expand our capability to help power our U.S. government partners, international partners, and relief organizations across the globe as they take on disasters – and save lives.”

The team behind NASA’s Disaster Response Coordination System gathers science, technology, data, and expertise from across the agency and provides it to emergency managers. The new system will be able to provide up-to-date information on fires, earthquakes, landslides, floods, tornadoes, hurricanes, and other extreme events.

“The risk from climate-related hazards is increasing, making more people vulnerable to extreme events,” said Karen St. Germain, director of NASA’s Earth Science Division. “This is particularly true for the 10% of the global population living in low-lying coastal regions who are vulnerable to storm surges, waves and tsunamis, and rapid erosion. NASA’s disaster system is designed to deliver trusted, actionable Earth science in ways and means that can be used immediately, to enable effective response to disasters and ultimately help save lives.”

Agencies working with NASA include the Federal Emergency Management Agency, the National Oceanic and Atmospheric Administration (NOAA), the U.S. Geological Survey, and the U.S. Agency for International Development – as well as international organizations such as World Central Kitchen.

“With this deliberate and structured approach, we can be even more effective in putting Earth science into action,” said Josh Barnes, at NASA’s Langley Research Center. Barnes manages the Disaster Response Coordination System.

NASA Administrator Bill Nelson delivers remarks June 13 during an event launching a new Disaster Response Coordination System that will provide communities and organizations around the world with access to science and data to aid disaster response. NASA/Bill Ingalls

NASA Disasters Team Aiding Brazil

When the floods and landslides ravaged parts of Brazil in May, officials from the U.S. Southern Command – working with the U.S. Space Force and Air Force, and regional partners – reached out to NASA for Earth-observing data.

NASA’s response included maps of potential power outages from the Black Marble project at NASA’s Goddard Space Flight Center. Disaster response coordinators at NASA Goddard also reviewed high-resolution optical data – from the Commercial Smallsat Data Acquisition Program – to map more than 4,000 landslides.

Response coordinators from NASA’s Jet Propulsion Laboratory and the California Institute of Technology produced flood extent maps using data from the NASA and U.S. Geological Survey Landsat mission and from ESA’s (the European Space Agency) Copernicus Sentinel-2 satellite. Response coordinators at NASA’s Johnson Space Center also provided photographs of the flooding taken by astronauts aboard the International Space Station.

Building on Previous Work

The Brazil event is just one of hundreds of responses NASA has supported over the past decade. The team aids decision-making for a wide range of natural hazards and disasters, from hurricanes and earthquakes to tsunamis and oil spills. 

“NASA’s Disasters Program advances science for disaster resilience and develops accessible resources to help communities around the world make informed decisions for disaster planning,” said Shanna McClain, manager of NASA’s Disasters Program. “The new Disaster Response Coordination System significantly expands our efforts to bring the power of Earth science when responding to disasters.”

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2 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater) Artist concept of a high-speed point-to-point vehicle.NASA Langley

Owing to NASA’s Quesst mission and Commercial Supersonic Technology project, there is growing industry interest in commercial aircraft that fly faster than the speed of sound. In 2020, NASA funded two independent studies to investigate the economic viability of this potential market for high-speed commercial flight. Since then, NASA has funded additional studies to investigate the technology developments needed for these aircraft, as well as the regulatory and certification barriers that currently exist for aircraft that break the sound barrier.

Although the initial studies found an economically feasible market may exist for aircraft that fly between 2-4 times the speed of sound, additional studies have shown the most profitable market is at the lower end of this speed range. In addition, current restrictions on overland sonic booms, landing and takeoff noise, and engine emissions currently prohibit the operation of high-speed commercial aircraft. NASA’s Commercial Supersonic Technology and Hypersonic Technology projects are working to overcome the technological and regulatory barriers by partnering with industry and other government agencies. In addition, NASA hosts industry workshops to discuss high-speed commercial flight and to understand this evolving industry.

Presentations and reports from the market studies are available on the NASA Technical Reports Server:

SAIC Report

SAIC Presentation

Deloitte Report

Deloitte Presentation

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Details Last Updated Jun 18, 2024 EditorJim BankeContactShannon Eichornshannon.eichorn@nasa.gov Related Terms

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• Advanced Air Vehicles Program

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NASA Releases Hubble Image Taken in New Pointing Mode This NASA Hubble Space Telescope features the galaxy NGC 1546.NASA, ESA, STScI, David Thilker (JHU)

NASA’s Hubble Space Telescope has taken its first new images since changing to an alternate operating mode that uses one gyro.

The spacecraft returned to science operations June 14 after being offline for several weeks due to an issue with one of its gyroscopes (gyros), which help control and orient the telescope.

This new image features NGC 1546, a nearby galaxy in the constellation Dorado. The galaxy’s orientation gives us a good view of dust lanes from slightly above and backlit by the galaxy’s core. This dust absorbs light from the core, reddening it and making the dust appear rusty-brown. The core itself glows brightly in a yellowish light indicating an older population of stars. Brilliant-blue regions of active star formation sparkle through the dust. Several background galaxies also are visible, including an edge-on spiral just to the left of NGC 1546.

Hubble’s Wide Field Camera 3 captured the image as part of a joint observing program between Hubble and NASA’s James Webb Space Telescope. The program also uses data from the Atacama Large Millimeter/submillimeter Array, allowing scientists to obtain a highly detailed, multiwavelength view of how stars form and evolve.

The image represents one of the first observations taken with Hubble since transitioning to the new pointing mode, enabling more consistent science operations. The NASA team expects that Hubble can do most of its science observations in this new mode, continuing its groundbreaking observations of the cosmos.

“Hubble’s new image of a spectacular galaxy demonstrates the full success of our new, more stable pointing mode for the telescope,” said Dr. Jennifer Wiseman, senior project scientist for Hubble at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “We’re poised now for many years of discovery ahead, and we’ll be looking at everything from our solar system to exoplanets to distant galaxies. Hubble plays a powerful role in NASA’s astronomical toolkit.”

Launched in 1990, Hubble has been observing the universe for more than three decades, recently celebrating its 34th anniversary. Read more about some of Hubble’s greatest scientific discoveries.

Resources Download the image above NASA’s Hubble Restarts Science in New Pointing Mode Operating Hubble with Only One Gyroscope Hubble Pointing and Control Hubble Science Highlights Hubble Images Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble

Media Contact:

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

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Details Last Updated Jun 18, 2024 EditorAndrea GianopoulosLocationNASA Goddard Space Flight Center Related Terms

• Astrophysics
• Astrophysics Division
• Galaxies
• Goddard Space Flight Center
• Hubble Space Telescope
• Missions
• The Universe

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Humans may have shaped the development of aromatic herbs like lavender and mint, but did herbs also shape our own evolution?

Humans may have shaped the development of aromatic herbs like lavender and mint, but did herbs also shape our own evolution?

3 min read

Artemis, Architecture, and Lunar Science: SMD and ESDMD Associate Administrators visits Tokyo

June 18, 2024

At NASA we always say that exploration enables science, and science enables exploration. During a recent, quick trip to Tokyo, Japan with our Associate Administrator for the Exploration Systems Development Mission Directorate (ESDMD), Cathy Koerner, I had an opportunity to share this message with our partners at the Japanese Aerospace Exploration Agency (JAXA).

We explore for several reasons but primarily to benefit humanity. How exactly does exploration benefit humanity? By accepting audacious challenges like retuning to the Moon and venturing on to Mars, we inspire and motivate current and future generations of scientists, engineers, problem solvers, and communicators to contribute to our mission and other national priorities. By conducting scientific investigations in deep space, on the Moon, and on Mars, we enhance our understanding of the universe and our place in it. And finally, what we achieve when we explore, how it’s accomplished, and who participates benefits international partnerships and global cooperation that are essential for enhancing the quality of life for all.

NASA Associate Administrator for the Science Mission Directorate, Dr. Nicky Fox, and Associate Administrator for the Exploration systems Development Mission Directorate, Cathy Koerner, meet with the Japanese Aerospace Exploration Agency (JAXA) in Tokyo, Japan on June 11, 2024. Credits: NASA

In addition to bi-lateral meetings with our JAXA partners, Cathy and I co-presented at the International Space Exploration Symposium where I shared how every NASA Science division has a stake in Artemis. Cathy provided updates on the Orion spacecraft, SLS rocket, Gateway, human landing systems, and advanced spacesuits, and I talked about all of the incredible science we will conduct along the way. The Artemis campaign is a series of increasingly complex missions that provide ever-growing capabilities for scientific exploration of the Moon. From geology to solar, biological, and fundamental physics phenomena, exploration teaches about the earliest solar system environment: whether and how the bombardments of nascent worlds influenced the emergence of life, how the Earth and Moon formed and evolved, and how volatiles (like water) and other potential resources were distributed and transported throughout the solar system.

Together with our partners like JAXA, NASA is working towards establishing infrastructure for long-term exploration in lunar orbit and on the surface. For example, on Artemis III, JAXA will provide the Lunar Dielectric Analyzer instrument, which once installed near the lunar South Pole, will help collect valuable scientific data about the lunar environment, it’s interior, and how to sustain a long-duration human presence on the Moon. In April, the U.S. and Japan were proud to make a historic announcement for cooperation on the Moon. Japan will design, develop, and operate a pressurized rover for crewed and uncrewed exploration on the Moon. NASA will launch and deliver the rover, and provide two opportunities for Japanese astronauts to travel to the lunar surface. This historic agreement was highlighted by President Biden and Prime Minister Kishida and is an example of the strong relationship between the United States and Japan. The enclosed and pressurized rover will be able to accommodate two astronauts on the lunar surface for 30 days, and will have a lifespan of about 10 years, enabling it to be used for multiple missions. It will enable longer-duration expeditions, so that astronauts can conduct more moonwalks and perform more science in geographically diverse areas near the lunar South Pole.

Artemis is different than anything humanity has ever done before. The Artemis campaign will bring the world along for this historic journey, forever changing humanity’s perspective of our place in the universe. This is the start of a lunar ecosystem, where we’ll do more science than we can dream of, together.

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Credits: NASA

NASA has awarded the Goddard Logistics Services Contract to TRAX International Corporation of Las Vegas to provide logistics services and management for NASA missions.

The cost-plus-fixed-fee contract includes a base period and up to five options with a potential contract value of approximately $265 million if all options are exercised. The basic period of performance is from Thursday, Aug. 1, 2024, to July 21, 2025. The five option periods, if exercised, would extend the contract through Jan. 31, 2030.

Under this contract, TRAX will provide disposal operations, export control, equipment management, mail, supply, materials, and transportation for NASA. The work will be performed at the agency’s Goddard Space Flight Center in Greenbelt, Maryland, Wallops Flight Facility in Virginia, and NASA Headquarters in Washington.

For information about NASA and agency programs, visit:

https://www.nasa.gov

-end-

Abbey Donaldson
Headquarters, Washington
202-358-1600
Abbey.a.donaldson@nasa.gov

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Details Last Updated Jun 18, 2024 LocationNASA Headquarters Related Terms

• Goddard Space Flight Center
• NASA Centers & Facilities
• NASA Headquarters
• Wallops Flight Facility

Earth’s protective atmosphere has sheltered life for billions of years, creating a haven where evolution produced complex lifeforms like us. The ozone layer plays a critical role in shielding the biosphere from deadly UV radiation. It blocks 99% of the Sun’s powerful UV output. Earth’s magnetosphere also shelters us.

But the Sun is relatively tame. How effective are the ozone and the magnetosphere at protecting us from powerful supernova explosions?

Every million years—a small fraction of Earth’s 4.5 billion-year lifetime—a massive star explodes within 100 parsecs (326 light-years) of Earth. We know this because our Solar System sits inside a massive bubble in space called the Local Bubble. It’s a cavernous region of space where hydrogen density is much lower than outside the bubble. A series of supernovae explosions in the previous 10 to 20 million years carved out the bubble.

Supernovae are dangerous, and the closer a planet is to one, the more deadly its effects. Scientists have speculated on the effects that supernova explosions have had on Earth, wondering if it triggered mass extinctions or at least partial extinctions. A supernova’s gamma-ray burst and cosmic rays can deplete Earth’s ozone and allow ionizing UV radiation to reach the planet’s surface. The effects can also create more aerosol particles in the atmosphere, increasing cloud coverage and causing global cooling.

A new research article in Nature Communications Earth and Environment examines supernova explosions and their effect on Earth. It is titled “Earth’s Atmosphere Protects the Biosphere from Nearby Supernovae.” The lead author is Theodoros Christoudias from the Climate and Atmosphere Research Center, Cyprus Institute, Nicosia, Cyprus.

The Local Bubble isn’t the only evidence of nearby core-collapse supernovae (SNe) in the last few million years. Ocean sediments also contain 60Fe, a radioactive isotope of iron with a half-life of 2.6 million years. SNe expel 60Fe into space when they explode, indicating that a nearby supernova exploded about 2 million years ago. There’s also 60Fe in sediments that indicate another SN explosion about 8 million years ago.

This graphic from the research article shows the potential atmospheric and climate impacts of a nearby supernova. Gamma rays can deplete the ozone, allowing more UV radiation to reach Earth’s surface. Some UV radiation is ionizing, meaning it can damage DNA. Cosmic rays can also create more condensation nuclei, meaning more clouds and potential global cooling, Image Credit: Christoudias et al. 2024

Researchers have correlated an SN explosion with the Late Devonian extinction about 370 million years ago. In one paper, researchers found plant spores burned by UV light, an indication that something powerful depleted Earth’s ozone layer. In fact, Earth’s biodiversity declined for about 300,000 years prior to the Late Devonian extinction, suggesting that multiple SNe could’ve played a role.

Earth’s ozone layer is in constant flux. As UV energy reaches it, it breaks ozone molecules (O3) apart. That dissipates the UV energy, and the oxygen atoms combine into O3 again. The cycle repeats. That’s a simplified version of the atmospheric chemistry involved, but it serves to illustrate the cycle. A nearby supernova could overwhelm the cycle, depleting the ozone column density and allowing more deadly UV to reach Earth’s surface.

But in the new paper, Christoudias and his fellow authors suggest that Earth’s ozone layer is much more resilient than thought and provides ample protection against SNe within 100 parsecs. While previous researchers have modelled Earth’s atmosphere and its response to a nearby SN, the authors say that they’ve improved on that work.

They modelled Earth’s atmosphere with an Earth Systems Model with Atmospheric Chemistry (EMAC) model to study the impact of nearby SNe explosions on Earth’s atmosphere. Using EMAC, the authors say they’ve modelled “the complex atmospheric circulation dynamics, chemistry, and process feedbacks” of Earth’s atmosphere. These are needed to “simulate stratospheric ozone loss in response to elevated ionization, leading to ion-induced nucleation and particle growth to CCN” (cloud condensation nuclei.)

“We assume a representative nearby SN with GCR (galactic cosmic ray) ionization rates in the atmosphere that are 100 times present levels,” they write. That correlates with a supernova explosion about 100 parsecs or 326 light-years away.

These panels from the research letter show the ozone column percentage decrease from a 100-fold increase in GCR intensity over nominal. The left vertical axis represents Earth’s latitude, and the x-axis shows the time of year. Ozone loss is more pronounced over the poles due to the effect of Earth’s magnetosphere, where it’s weaker. a is present-day Earth, while b represents an ancient Earth with only 2% oxygen during the pre-Cambrian. Image Credit: Christoudias et al. 2024

“The maximum ozone depletion over the poles is less than the present-day anthropogenic ozone hole over Antarctica, which amounts to an ozone column loss of 60–70%,” the authors explain. “On the other hand, there is an increase of ozone in the troposphere, but it is well within the levels resulting from recent anthropogenic pollution.”

But let’s cut to the chase. We want to know if Earth’s biosphere is safe or not.

The maximum mean stratospheric ozone depletion from 100 times more ionizing radiation than normal, representative of a nearby SN, is about 10% globally. That’s about the same decrease as our anthropogenic pollution causes. It wouldn’t affect the biosphere very much.

“Although significant, it is unlikely that such ozone changes would have a major impact on the biosphere, especially because most of the ozone loss is found to occur at high latitudes,” the authors explain.

But that’s for modern Earth. During the pre-Cambrian, before life exploded in a multiplication of forms, the atmosphere had only about 2% oxygen. How would an SN affect that? “We simulated a 2% oxygen atmosphere since this would likely represent conditions where the emerging biosphere on land would still be particularly sensitive to ozone depletion,” the authors write.

“Ozone loss is about 10–25% at mid-latitudes and an order of magnitude lower in the tropics,” the authors write. At minimum ozone levels at the poles, ionizing radiation from an SN could actually end up increasing the ozone column. “We conclude that these changes of atmospheric ozone are unlikely to have had a major impact on the emerging biosphere on land during the Cambrian,” they conclude.

What about global cooling?

Global cooling would increase, but not to a dangerous extent. Over the Pacific and Southern oceans, CCN could increase by up to 100%, which sounds like a lot. “These changes, while climatically relevant, are comparable to the contrast between the pristine pre-industrial atmosphere and the polluted present-day atmosphere.” They’re saying that it would cool the atmosphere by about the same amount as we’re heating it now.

These two panels from the research help illustrate the global cooling effect from a nearby SN exposing Earth to 100 times more ionizing radiation. b shows the fractional change in CCN relative to the present day. d shows the fractional change in outgoing solar radiation relative to the present day due to increased cloud albedo. Image Credit: Christoudias et al. 2024

The researchers point out that their study concerns the entire biosphere, not individuals. “Our study does not consider the direct health risks to humans and animals resulting from exposure to elevated ionizing radiation,” they write. Depending on individual circumstances, individuals could be exposed to dangerous levels of radiation over time. But overall, the biosphere would hum along despite a 100-fold increase in UV radiation. Our atmosphere and magnetosphere can handle it.

“Overall, we find that nearby SNe are unlikely to have caused mass extinctions on Earth,” the authors write. “We conclude that our planet’s atmosphere and geomagnetic field effectively shield the biosphere from the effects of nearby SNe, which has allowed life to evolve on land over the last hundreds of million years.”

This study shows that Earth’s biosphere will not suffer greatly as long as supernova explosions keep their distance.

The post Earth’s Atmosphere is Our Best Defence Against Nearby Supernovae appeared first on Universe Today.

Conceptualization of the GeoXO constellation.Credits: NOAA

NASA, on behalf of the National Oceanic and Atmospheric Administration (NOAA), has selected Lockheed Martin Corp. of Littleton, Colorado, to build the spacecraft for NOAA’s Geostationary Extended Observations (GeoXO) satellite program.

This cost-plus-award-fee contract is valued at approximately $2.27 billion. It includes the development of three spacecraft as well as four options for additional spacecraft. The anticipated period of performance for this contract includes support for 10 years of on-orbit operations and five years of on-orbit storage, for a total of 15 years for each spacecraft. The work will take place at Lockheed Martin’s facility in Littleton and NASA’s Kennedy Space Center in Florida.

The GeoXO constellation will include three operational satellites — east, west and central. Each geostationary, three-axis stabilized spacecraft is designed to host three instruments. The centrally-located spacecraft will carry an infrared sounder and atmospheric composition instrument and can also accommodate a partner payload. Spacecraft in the east and west positions will carry an imager, lightning mapper, and ocean color instrument. They will also support an auxiliary communication payload for the NOAA Data Collection System relay, dissemination, and commanding.

The contract scope includes the tasks necessary to design, analyze, develop, fabricate, integrate, test, evaluate, and support launch of the GeoXO satellites; provide engineering development units; supply and maintain the ground support equipment and simulators; and support mission operations at the NOAA Satellite Operations Facility in Suitland, Maryland.

NASA and NOAA oversee the development, launch, testing, and operation of all the satellites in the GeoXO program. NOAA funds and manages the program, operations, and data products. On behalf of NOAA, NASA and commercial partners develop and build the instruments and spacecraft and launch the satellites.

As part of NOAA’s constellation of geostationary environmental satellites to protect life and property across the Western Hemisphere, the GeoXO program is the follow-on to the Geostationary Operational Environmental Satellites – R (GOES-R) Series Program.

The GeoXO satellite system will advance Earth observations from geostationary orbit. The mission will supply vital information to address major environmental challenges of the future in support of weather, ocean, and climate operations in the United States. The advanced capabilities from GeoXO will help assess our changing planet and the evolving needs of the nation’s data users. Together, NASA and NOAA are working to ensure GeoXO’s critical observations are in place by the early 2030s when the GOES-R Series nears the end of its operational lifetime.

For more information on the GeoXO program, visit:

https://www.nesdis.noaa.gov/geoxo

-end-

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

Jeremy Eggers
Goddard Space Flight Center, Greenbelt, Md.
757-824-2958
jeremy.l.eggers@nasa.gov

John Leslie
NOAA’s National Environmental Satellite, Data, and Information Service
202-527-3504
nesdis.pa@noaa.gov

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Details Last Updated Jun 18, 2024 LocationNASA Headquarters Related Terms

• GOES (Geostationary Operational Environmental Satellite)
• Earth Observatory
• Earth Science Division
• NOAA (National Oceanic and Atmospheric Administration)
• Science Mission Directorate

NOAA's GOES-R series constellation will be complete in space with the launch of its GOES-U satellite at the end of June. This will mark the first time a NOAA satellite will be transported to space using a SpaceX Falcon Heavy rocket.

Crews transport NOAA’s (National Oceanic and Atmospheric Administration) Geostationary Operational Environmental Satellite (GOES-U) from the Astrotech Space Operations facility to the SpaceX hangar at Launch Complex 39A at NASA’s Kennedy Space Center in Florida beginning on Friday, June 14, 2024, with the operation finishing early Saturday, June 15, 2024. The fourth and final weather-observing and environmental monitoring satellite in NOAA’s GOES-R Series will assist meteorologists in providing advanced weather forecasting and warning capabilities. The two-hour window for liftoff opens 5:16 p.m. EDT Tuesday, June 25, aboard a SpaceX Falcon Heavy rocket from Launch Complex 39A at NASA’s Kennedy Space Center in Florida. (NASA/Ben Smegelsky)

NASA will provide live coverage of prelaunch and launch activities for the National Oceanic and Atmospheric Administration’s (NOAA) GOES-U (Geostationary Operational Environmental Satellite U) mission. The two-hour launch window opens at 5:16 p.m. EDT Tuesday, June 25, for the satellite’s launch on a SpaceX Falcon Heavy rocket from Launch Complex 39A at NASA’s Kennedy Space Center in Florida. 

The GOES-U satellite, the final addition to GOES-R series, will help to prepare for two kinds of weather — Earth and space weather. The GOES satellites serve a critical role in providing continuous coverage of the Western Hemisphere, including monitoring tropical systems in the eastern Pacific and Atlantic oceans. This continuous monitoring aids scientists and forecasters in issuing timely warnings and forecasts to help protect the one billion people who live and work in the Americas. Additionally, GOES-U carries a new compact coronagraph that will image the outer layer of the Sun’s atmosphere to detect and characterize coronal mass ejections. 

The deadline for media accreditation for in-person coverage of this launch has passed. NASA’s media credentialing policy is available online. For questions about media accreditation, please email: ksc-media-accreditat@mail.nasa.gov. 

NASA’s mission coverage is as follows (all times Eastern and subject to change based on real-time operations): 

Monday, June 24 

9:30 a.m. – NASA EDGE GOES-U prelaunch show on NASA+, the NASA app, and the agency’s website. 

11 a.m. – GOES-U science briefing with the following participants: 

• Charles Webb, deputy director, Joint Agency Satellite Division, NASA 

• Ken Graham, director, NOAA’s National Weather Service 
• Dan Lindsey, chief scientist, GOES-R Program, NOAA 
• Elsayed Talaat, director, NOAA’s Office of Space Weather Observations 
• Chris Wood, NOAA Hurricane Hunter pilot 

Coverage of the science news conference will stream live on NASA+, the NASA app, YouTube, and the agency’s website. 

Media may ask questions in person and via phone. Limited auditorium space will be available for in-person participation. For the dial-in number and passcode, media should contact the Kennedy newsroom no later than one hour before the start of the event at ksc-newsroom@mail.nasa.gov. 

3:15 p.m. – NASA Social panel at Kennedy with the following participants: 

• Jade Zsiros, telemetry engineer, NASA’s Launch Services Program 
• Ellen Ramirez, deputy division chief, Mission Operations Division, National Environmental Satellite, Data, and Information Service Office of Satellite and Product Operations, NOAA 
• Dakota Smith, satellite analyst and communicator, NOAA’s Cooperative Institute for Research in the Atmosphere 
• Allana Nepomuceno, senior manager, GOES-U Assembly, Test, and Launch Operations, Lockheed Martin 
• Chris Reith, program manager, Advanced Baseline Imager, L3Harris Technologies 

The panel will stream live on NASA Kennedy’s YouTube, X and Facebook accounts. Members of the public may ask questions online by posting to the YouTube, X, and Facebook live streams or using #AskNASA. 

5 p.m. – Prelaunch news conference at Kennedy (following completion of the Launch Readiness Review), with the following participants: 

• Denton Gibson, launch director, Launch Services Program, NASA 
• Steve Volz, assistant administrator, NOAA’s Satellite and Information Service 
• Pam Sullivan, director, GOES-R Program, NOAA 
• John Gagosian, director, Joint Agency Satellite Division 
• Julianna Scheiman, director, NASA Science Missions, SpaceX 
• Brian Cizek, launch weather officer, 45th Weather Squadron, U.S. Space Force 

Coverage of the prelaunch news conference will stream live on NASA+, the NASA app, YouTube, and the agency’s website. 

Media may ask questions in person and via phone. Limited auditorium space will be available for in-person participation. For the dial-in number and passcode, media should contact the Kennedy newsroom no later than one hour before the start of the event at ksc-newsroom@mail.nasa.gov. 

Tuesday, June 25 

1 p.m. – Media one-on-one interviews with the following: 

• Michael Morgan, Assistant Secretary of Commerce for Environmental Observation and Prediction, NOAA 
• Michael Brennan, director, NOAA’s National Hurricane Center 
• James Spann, senior scientist, Office of Space Weather Observations, NOAA 
• John Gagosian, director, Joint Agency Satellite Division 
• Krizia Negron, language program lead, National Weather Service Office of Science and Technology Integration, NOAA (bilingual, available for Spanish interviews) 

• Dan Lindsey, chief scientist, GOES-R Program, NOAA 
• Jagdeep Shergill, program director, GEO Weather, Lockheed Martin 
• Chris Reith, program manager, Advanced Baseline Imager, L3Harris Technologies 

4:15 p.m. – NASA launch coverage begins on NASA+, the agency’s website, and other digital channels.  

5:16 p.m. – Two-hour launch window opens 

Audio Only Coverage 

Audio only of the news conferences and launch coverage will be carried on the NASA “V” circuits, which may be accessed by dialing 321-867-1220, -1240 or -7135. On launch day, “mission audio,” countdown activities without NASA Television media launch commentary, will be carried on 321-867-7135. 

Live Video Coverage Prior to Launch 

NASA will provide a live video feed of Launch Complex 39A approximately 24 hours prior to the planned liftoff of the mission on NASA Kennedy’s YouTube: https://youtube.com/kscnewsroom. The feed will be uninterrupted until the prelaunch broadcast begins on NASA Television media channel. 

NASA Website Launch Coverage 

Launch day coverage of the mission will be available on the agency’s website. Coverage will include live streaming and blog updates beginning no earlier than 3 p.m., June 25, as the countdown milestones occur. On-demand streaming video and photos of the launch will be available shortly after liftoff. 

For questions about countdown coverage, contact the Kennedy newsroom at 321-867-2468. Follow countdown coverage on the GOES blog. 

Para obtener información sobre cobertura en español en el Centro Espacial Kennedy o si desea solicitar entrevistas en español, comuníquese con Antonia Jaramillo: antonia.jaramillobotero@nasa.gov o Messod Bendayan: messod.c.bendayan@nasa.gov 

Attend the Launch Virtually 

Members of the public can register to attend this launch virtually. NASA’s virtual guest program for this mission also includes curated launch resources, notifications about related opportunities or changes, and a stamp for the NASA virtual guest passport following launch. 

Watch, Engage on Social Media 

Let people know you’re following the mission on X, Facebook, and Instagram by using the hashtags #ReadyToGOES and #NASASocial. You can also stay connected by following and tagging these accounts: 

X: @NASA, @NASA_LSP, @NASAKennedy, @NOAASatellites, @NASAGoddard 

Facebook: NASA, NASA LSP, NASA Kennedy, NOAA Satellites, NASA Goddard 

Instagram: NASA, NASA Kennedy, NOAA Satellites 

For more information about the mission, visit: 

https://www.nasa.gov/goes-u

-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 

NASA has rescheduled last week's EVA, which was called off only an hour before the astronauts were set to exit the station.

Boeing's Starliner will come back to Earth with its two astronauts no earlier than June 26. The four-day extension will allow for more thruster testing at the ISS.

NASA’s OSIRIS-REx mission has been immortalized at the Smithsonian’s National Air and Space Museum in Washington as the latest awardee of the Robert J. Collier Trophy. Bestowed annually by the National Aeronautic Association, the trophy recognizes groundbreaking aerospace achievements.

Members of the OSIRIS-REx team at the Smithsonian Institute’s National Air and Space Museum in Washington, D.C., with the Collier trophy on June 13, 2024. From left to right: Nayi Castro, mission operations manager, NASA’s Goddard Space Flight Center, Greenbelt, Md.; Nicole Lunning, curator, NASA’s Johnson Space Center, Houston; Anjani Polit, mission implementation systems engineer, University of Arizona, Tucson; Coralie Adam, OSIRIS-REx optical navigation lead, KinetX Inc.; Michael Moreau, OSIRIS-REx deputy project manager, NASA Goddard; Dennis Reuter, OVIRS instrument scientist, NASA Goddard; Ronald Mink, OSIRIS-REx missions systems engineer, NASA Goddard; Joshua Wood, system design lead, Lockheed Martin Space; Peter Antreasian, OSIRIS-REx navigation team chief, KinetX Inc.; Sandy Freund, program manager, Lockheed Martin Space; Eric Sahr, optical navigation engineer, KinetX Inc.NASA/Rani Gran

OSIRIS-REx, formally the Origins, Spectral Interpretation, Resource Identification, and Security – Regolith Explorer, was honored “for successfully executing the first American retrieval of an asteroid sample and its return to Earth,” according to the award citation. The award was announced in March, and the OSIRIS-REx team visited the museum on June 13, 2024, to see the mission’s name engraved in brass at the base of the statue.

“It just blows me away to see the OSIRIS-REx team engraved on the Collier trophy, next to names like Orville Wright, the Apollo 8 crew, and the Voyager Mission Team,” said Michael Moreau, OSIRIS-REx deputy project manager at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.  “I’m so proud of our amazing team that their excellence and sacrifice to make the OSIRIS-REx mission so successful have been recognized with this prestigious award.”

While NASA’s accomplishments have been honored with the Collier award many times, this is one of just a handful of instances that NASA Goddard has been a major partner on a winning team. NASA Goddard most recently claimed a share of the award in 2022 for the James Webb Space Telescope. Previous wins also include 1993 honors for the Hubble Space Telescope and the 1974 prize for a NASA–U.S. Geological Survey satellite that began the long-running Landsat program that studies and monitors changes to Earth’s land masses.

The OSIRIS-REx team includes NASA’s Goddard Space Flight Center in Greenbelt, Maryland; Lockheed Martin in Littleton, Colorado; the University of Arizona, Tucson; and KinetX in Tempe, Arizona. NASA’s Johnson Space Center is responsible for the curation of the Bennu sample material that OSIRIS-REx returned to Earth in September 2023.

The Collier Trophy resides in a glass case in the “America by Air” section on the museum’s first floor. The century-old trophy stands at over 7 feet tall and weighs 525 pounds. The bronze sculpture depicts a globe, with three figures emerging from it. The sculpture rests on two walnut bases, each adorned with an engrave brass plaque bearing the names of the recipients.

Baltimore sculptor Ernest Wise Keyser designed the Trophy in 1910 for Robert J. Collier, the publisher of Collier’s Weekly magazine and president of the Aero Club of America.

By Rani Gran
NASA’s Goddard Space Flight Center, Greenbelt, Md.

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Details Last Updated Jun 18, 2024 EditorRob GarnerContactRani Gran Related Terms

• Goddard Space Flight Center
• OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer)