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By NASA
3 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
Students celebrate after a successful performance in the 2024 Student Launch competition at Bragg Farms in Toney, Alabama.NASA NASA has selected 71 teams from across the U.S. to participate in its 25th annual Student Launch Challenge, one of the agency’s Artemis Student Challenges. The competition is aimed at inspiring Artemis Generation students to explore science, technology, engineering, and math (STEM) for the benefit of humanity.
As part of the challenge, teams will design, build, and fly a high-powered amateur rocket and scientific payload. They also must meet documentation milestones and undergo detailed reviews throughout the school year.
The nine-month-long challenge will culminate with on-site events starting on April 30, 2025. Final launches are scheduled for May 3, at Bragg Farms in Toney, Alabama, just minutes north of NASA’s Marshall Space Flight Center in Huntsville, Alabama. Teams are not required to travel for their final launch, having the option to launch from a qualified site. Details are outlined in the Student Launch Handbook.
Each year, NASA updates the university payload challenge to reflect current scientific and exploration missions. For the 2025 season, the payload challenge will again take inspiration from the Artemis missions, which seek to land the first woman and first person of color on the Moon, and pave the way for future human exploration of Mars.
As Student Launch celebrates its 25th anniversary, the payload challenge will include reports from STEMnauts, non-living objects representing astronauts. The STEMnaut crew must relay real-time data to the student team’s mission control via radio frequency, simulating the communication that will be required when the Artemis crew achieves its lunar landing.
University and college teams are required to meet the 2025 payload requirements set by NASA, but middle and high school teams have the option to tackle the same challenge or design their own payload experiment.
Student teams will undergo detailed reviews by NASA personnel to ensure the safety and feasibility of their rocket and payload designs. The team closest to their target will win the Altitude Award, one of multiple awards presented to teams at the end of the competition. Other awards include overall winner, vehicle design, experiment design, and social media presence.
In addition to the engineering and science objectives of the challenge, students must also participate in outreach efforts such as engaging with local schools and maintaining active social media accounts. Student Launch is an all-encompassing challenge and aims to prepare the next generation for the professional world of space exploration.
The Student Launch Challenge 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.
For more information about Student Launch, visit:
Student Launch Website Taylor Goodwin
Marshall Space Flight Center, Huntsville, Ala.
256.544.0034
taylor.goodwin@nasa.gov
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Last Updated Oct 04, 2024 EditorBeth RidgewayLocationMarshall Space Flight Center Related Terms
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2 min read NASA Announces Teams to Compete in International Rover Challenge
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By NASA
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
NASA MSFC HERC is the annual engineering competition – one of NASA’s longest standing challenges – held its concluding event April 19 and April 20, at the U.S. Space & Rocket Center in Huntsville, near NASA’s Marshall Space Flight Center.NASA NASA has selected 75 student teams to begin an engineering design challenge to build rovers that will compete next spring at the U.S. Space and Rocket Center near the agency’s Marshall Space Flight Center in Huntsville, Alabama. The competition is one of the agency’s Artemis Student Challenges, encouraging students to pursue degrees and careers in science, technology, engineering, and mathematics (STEM).
Recognized as NASA’s leading international student challenge, the 31st annual Human Exploration Rover Challenge (HERC) aims to put competitors in the mindset of NASA’s Artemis campaign as they pitch an engineering design for a lunar terrain vehicle which simulates astronauts piloting a vehicle, exploring the lunar surface while overcoming various obstacles.
Participating teams represent 35 colleges and universities, 38 high schools, and two middle schools from 20 states, Puerto Rico, and 16 other nations from around the world. The 31st annual Human Exploration Rover Challenge (HERC) is scheduled to begin on April 11, 2025. The challenge is managed by NASA’s Southeast Regional Office of STEM Engagement at NASA Marshall.
Following a 2024 competition that garnered international attention, NASA expanded the challenge to include a remote-control division, Remote-Operated Vehicular Research, and invited middle school students to participate. The 2025 HERC Handbook includes guidelines for the new remote-control division and updates for the human-powered division.
NASA’s Artemis Student Challenges reflects the goals of the Artemis campaign, which seeks to land the first woman and first person of color on the Moon while establishing a long-term presence for science and exploration.
More than 1,000 students with 72 teams from around the world participated in the 2024 challenge as HERC celebrated its 30th anniversary as a NASA competition. Since its inception in 1994, more than 15,000 students have participated in HERC – with many former students now working at NASA, or within the aerospace industry.
To learn more about HERC, please visit:
HERC Website Taylor Goodwin
Marshall Space Flight Center, Huntsville, Ala.
256.544.0034
taylor.goodwin@nasa.gov
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Last Updated Oct 04, 2024 EditorBeth RidgewayLocationMarshall Space Flight Center Related Terms
Marshall Space Flight Center Explore More
20 min read The Marshall Star for October 2, 2024
Article 2 days ago 29 min read The Marshall Star for September 25, 2024
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NASA Student Launch Challenge
Middle/high school and college-level student teams design, build, test, and launch a high-powered rocket carrying a scientific or engineering payload.
NASA Human Exploration Rover Challenge
Teams of high school and college students design, develop, build, and test human-powered rovers capable of traversing challenging terrain.
NASA STEM Opportunities and Activities For Students
Marshall Space Flight Center
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By NASA
5 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
Two NASA employees, Howard Chang and Bradley Williams, were named as two of the “20 under 35 of 2024” by the Space and Satellite Professionals International. The award recognizes outstanding young professionals in the space industry.
Photos courtesy of Bradley Williams and Howard Chang The annual list of “20 Under 35” features 20 employees and entrepreneurs to keep your eye on in coming years. They were selected from nominations submitted by the membership and evaluated by the same panel of judges who name winners of the Promise Awards.
Howard Chang is an Assistant Chief Counsel at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Bradley (Brad) Williams is the Acting Associate Director for Flight, Heliophysics Division, NASA Science Mission Directorate at NASA Headquarters, Washington.
“I’m honored to be named in this year’s cohort,” Chang said. “I saw how SSPI connects people across the space and satellite industry—across generations, countries, and even disciplines—to build up the space economy of the future. And I can’t express enough thanks to all my NASA colleagues for their support and kindness—especially Deputy Chief Counsel Amber Hufft for her time and mentorship this year.”
“It is an absolute honor to be recognized by SSPI on the 20 under 35 list of 2024,” said Williams. “I feel privileged to have benefitted from the opportunities I’ve had so far in my career. I want to thank the numerous mentors through the years who have provided me guidance and lessons learned and especially my colleagues and the leaders at NASA who have recognized my contributions and supported my growth potential as a leader.”
About Howard Chang
Howard Chang serves as the lead attorney for NASA’s Wallops Flight Facility’s commercial, nonprofit, and interagency partnerships in Wallops Island, Virginia. He also focuses on legal issues involving Unmanned Aircraft Systems (UAS), small UAS, real property transactions, government contracts litigation and administration supporting NASA Goddard, and partnerships involving the Goddard Institute for Space Studies located at Columbia University, New York, NASA commended Chang with an individual merit award in recognition of his superior support to the Goddard Space Flight Center during his first six months.
In addition to his legal work, Chang contributes substantially to thought leadership in space law and policy. He has authored articles for The Federalist and the International Institute of Space Law on topics from the Apollo 8 mission to the travaux preparatoires of the Principles Declaration of 1963—the precursor to the Outer Space Treaty. He is a frequent speaker on matters of space law. He will be presenting at the 2024 International Astronautical Congress in Milan, Italy on the Wolf Amendment and the future of the International Space Station. In Milan, he will present in his capacity as an Advisor for the Georgetown University Space Initiative. He continues to serve as a guest lecturer on space policy for law schools and undergraduate space courses as well.
Chang previously worked at an international firm in its aerospace finance and space law practices, engaging in litigation, transactional, regulatory, and policy work for aerospace and space companies. In addition, he worked on white-collar criminal defense, internal corporate investigations, congressional investigations, trial litigation, appellate litigation, and national security matters.
About Bradley Williams
Bradley Williams is the acting Associate Director for Flight Programs in the Heliophysics Division of the Science Mission Directorate at NASA Headquarters, Washington where he oversees more than a dozen missions in operations and approximately another dozen missions in different stages of development.
Previously, Williams was a Program Executive in the Heliophysics Division where his assignments included IMAP, TRACERS, HelioSwarm, the Solar Cruiser solar sail technology project, and Senior Program Executive of the NASA Space Weather Program.
Before joining NASA, he was the Director of Civil Space Programs at Terran Orbital Corporation, where he led the spacecraft development for both commercial and NASA technology demonstration missions and assisted with the growth of the science mission portfolio.
Previously at the University of Arizona, he worked with faculty and research teams to identify proposal opportunities and develop spaceflight proposals. Williams was a vital member of the OSIRIS-REx Camera Suite (OCAMS) team. He also served as the Deputy Payload Manager on GUSTO, the first of its kind, balloon-borne observatory.
He has been recognized for his achievements being named a Via Satellite Rising Star in 2024 and has been awarded the Robert H. Goddard Engineering Team Award, NASA Group Achievement Award, and asteroid (129969) Bradwilliams named in his honor.
The “20 Under 35“ are honored each year at SSPI’s Future Leaders Dinner. At the Dinner, SSPI presents the three top-ranked members of the 20 Under 35 with a Promise Award, recognizing them as leaders of their year’s cohort, and honors the Mentor of the Year for fostering young talent, both within his or her organization and throughout the industry. The 2024 “20 Under 35” will be honored at the Future Leaders Celebration on October 21, 2024 during Silicon Valley Space Week.
Rob Gutro
NASA’s Goddard Space Flight Center
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Last Updated Oct 03, 2024 EditorJamie AdkinsContactRob Garnerrob.garner@nasa.gov Related Terms
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By NASA
Concepto artístico de la nave espacial Europa Clipper de la NASA.
Créditos: NASA/JPL-Caltech. Read this release in English here.
La NASA ofrecerá cobertura en directo, en inglés y en español, de las actividades previas al lanzamiento y del lanzamiento de Europa Clipper, la misión de la agencia para explorar Europa, una luna helada de Júpiter. La cobertura del lanzamiento se ofrecerá también en español. La NASA prevé que el lanzamiento se dé a las 12:31 p.m. EDT (hora del este) del jueves, 10 de octubre, a bordo de un cohete SpaceX Falcon Heavy desde el Complejo de Lanzamiento 39A en el Centro Espacial Kennedy de la NASA en Florida.
Más allá de la Tierra, Europa, una luna de Júpiter, es considerada uno de los entornos con más potencial para la habitabilidad del sistema solar. Tras un viaje de aproximadamente 1.800 millones de millas (unos 2.900 millones de kilómetros), Europa Clipper entrará en órbita alrededor de Júpiter en abril de 2030. Desde ahí, la nave espacial llevará a cabo un estudio detallado de Europa para determinar si este mundo helado podría presentar condiciones adecuadas para la vida. Europa Clipper es la mayor nave espacial que la NASA ha desarrollado para una misión planetaria. Transporta un conjunto de nueve instrumentos y un experimento gravitatorio, los cuales investigarán un océano bajo la superficie de Europa que los científicos creen que contiene el doble de agua líquida que los océanos de la Tierra.
Para consultar el calendario de eventos en directo y las plataformas en las que se retransmitirán, visita:
https://go.nasa.gov/europaclipperlive
El plazo para la acreditación de los medios de comunicación para la cobertura presencial de este lanzamiento ya finalizó. La política de acreditación de medios de la NASA está disponible en línea (en inglés). Si tienes preguntas sobre la acreditación de los medios de comunicación, envía un correo electrónico a: ksc-media-accreditat@mail.nasa.gov.
La cobertura de la misión de la NASA es la siguiente (todas las horas son del este y están sujetas a cambios en función de las operaciones a tiempo real):
Martes, 8 de octubre
1 p.m. – Entrevistas presenciales, abiertas a los medios de comunicación acreditados para este lanzamiento.
3:30 p.m. – Sesión informativa científica de Europa Clipper de la NASA con los siguientes participantes:
Gina DiBraccio, directora en funciones, División de Ciencias Planetarias, Sede de la NASA Robert Pappalardo, científico de proyecto, Europa Clipper, Laboratorio de Propulsión a Chorro de la NASA (NASA JPL) Haje Korth, científico adjunto de proyecto, Europa Clipper, Laboratorio de Física Aplicada de la Universidad Johns Hopkins Cynthia Phillips, científica de proyecto, Europa Clipper, NASA JPL La cobertura de la conferencia de prensa científica se retransmitirá en directo en NASA+ y en el sitio web de la agencia, Aprende cómo ver contenidos de la NASA a través de diversas plataformas, incluidas las redes sociales.
Los representantes de los medios de comunicación podrán formular preguntas tanto presencialmente como por teléfono. El espacio disponible en el auditorio para la participación en persona será limitado. Para obtener el número de teléfono y el código de acceso a la conferencia, los medios de comunicación deberán ponerse en contacto con la sala de prensa de la NASA en Kennedy a más tardar una hora antes del comienzo del acto: ksc-newsroom@mail.nasa.gov.
Miércoles, 9 de octubre
2 p.m. – Panel social del NASA Social en el centro Kennedy, con los siguientes participantes:
Kate Calvin, científica jefe y asesora principal sobre el clima, sede de la NASA Caley Burke, analista de diseño de vuelos, Programa de Servicios de Lanzamiento de la NASA Erin Leonard, científica del proyecto Europa Clipper, NASA JPL Juan Pablo León, ingeniero de banco de pruebas de sistemas, Europa Clipper, NASA JPL (León es hispanohablante) Elizabeth Turtle, investigadora principal, instrumento de sistema de imágenes de Europa, Europa Clipper, APL Esta mesa redonda se transmitirá en directo a través de las cuentas de la NASA en YouTube, X y Facebook. Los miembros del público pueden hacer preguntas en línea publicando en las transmisiones en vivo de YouTube, X y Facebook o usando el hashtag #AskNASA.
3:30 p.m. – Conferencia de prensa de la NASA previa al lanzamiento de Europa Clipper (tras la finalización de la revisión del estado de preparación para el lanzamiento), con los siguientes participantes:
Administrador asociado de la NASA Jim Free Sandra Connelly, administradora adjunta, Dirección de Misiones Científicas, Sede de la NASA Tim Dunn, director de lanzamiento, Programa de Servicios de Lanzamiento de la NASA Julianna Scheiman, directora para misiones científicas de la NASA, SpaceX Jordan Evans, gerente de proyecto, Europa Clipper, NASA JPL Mike McAleenan, meteorólogo de lanzamiento, 45º Escuadrón Meteorológico, Fuerza Espacial de EE.UU. La conferencia de prensa previa al lanzamiento se retransmitirá en directo en NASA+, el sitio web de la agencia, la aplicación de la NASA, y YouTube.
Los representantes de los medios de comunicación podrán formular preguntas tanto presencialmente como por teléfono. El espacio disponible en el auditorio para la participación en persona será limitado. Para obtener el número de teléfono y el código de acceso a la conferencia, los medios de comunicación deberán ponerse en contacto con la sala de prensa de la NASA en Kennedy a más tardar una hora antes del comienzo del acto: ksc-newsroom@mail.nasa.gov.
5:30 p.m. – Transmisión del despliegue de Europa Clipper de la NASA a la plataforma de lanzamiento. La retransmisión en vivo (en inglés) estará disponible en NASA+, el sitio web de la agencia, la aplicación de la NASA, y YouTube.
Jueves, 10 de octubre
11:30 a.m. – La cobertura en inglés del lanzamiento empezará en NASA+ y el el sitio web de la agencia.
11:30 a.m. – La cobertura en español del lanzamiento empezará en NASA+ y el canal de YouTube en español de la NASA.
12:31 p.m. – Lanzamiento.
Cobertura de audio
El audio de las conferencias de prensa y de la cobertura del lanzamiento, ambos en inglés, se transmitirá por los circuitos «V» de la NASA, a los que se puede acceder marcando 321-867-1220, -1240 o -7135. El día del lanzamiento, el «audio de la misión», es decir, las actividades de la cuenta atrás sin los comentarios de los medios de NASA+ sobre el lanzamiento, se retransmitirá por el 321-867-7135.
Cobertura de vídeo en directo previa al lanzamiento
La NASA proporcionará una conexión de vídeo en directo del Complejo de Lanzamiento 39A aproximadamente 18 horas antes del despegue previsto de la misión en el canal de YouTube de la sala de prensa de la NASA en Kennedy. La transmisión será ininterrumpida hasta que comience la emisión del lanzamiento en NASA+.
Cobertura del lanzamiento en el sitio web de la NASA
La cobertura de la misión el día del lanzamiento estará disponible en el sitio web de la agencia. La cobertura incluirá enlaces a retransmisiones en directo (en español e inglés) y actualizaciones del blog que comenzarán no antes de las 10 a.m. del 10 de octubre, a medida que se cumplan los hitos de la cuenta regresiva. Poco después del despegue se podrá acceder a vídeos y fotos del lanzamiento en streaming a demanda.
Siga la cobertura de la cuenta regresiva en el blog de Europa Clipper (en inglés). Si tiene alguna pregunta sobre la cobertura de la cuenta atrás, póngase en contacto con la sala de prensa Kennedy llamando al 321-867-2468.
Para obtener información sobre cobertura en español en el Centro Espacial Kennedy o si desea solicitar entrevistas en español, comuníquese con María José Viñas: maria-jose.vinasgarcia@nasa.gov, Antonia Jaramillo: antonia.jaramillobotero@nasa.gov o Messod Bendayan: messod.c.bendayan@nasa.gov
Asistencia virtual al lanzamiento
Los miembros del público pueden registrarse para asistir virtualmente a este lanzamiento. El programa de invitados virtuales (en inglés) de la NASA para esta misión también incluye recursos curados de lanzamiento, notificaciones sobre oportunidades o cambios relacionados, y un sello para el pasaporte de invitado virtual de la NASA después del lanzamiento.
Observación y participación en redes sociales
Haz que la gente sepa que estás siguiendo la misión en X, Facebook e Instagram utilizando los hashtags #EuropaClipper y #NASASocial. También puedes mantenerte conectado siguiendo y etiquetando estas cuentas:
X: @NASA, @EuropaClipper, @NASASolarSystem, @NASAJPL, @NASAKennedy, @NASA_LSP, @NASA_ES (en español)
Facebook: NASA, NASA’s Europa Clipper, NASA’s JPL, NASA’s Launch Services Program, NASA en español
Instagram: @NASA, @nasasolarsystem, @NASAKennedy, @NASAJPL, @NASA_ES (en español)
Para más información en español sobre la misión:
https://ciencia.nasa.gov/europaclipper
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Karen Fox / Molly Wasser/ María José Viñas
Sede, Washington
202-358-1600
karen.c.fox@nasa.gov / molly.l.wasser.nasa.gov / maria-jose.vinasgarcia@nasa.gov
Leejay Lockhart
Centro Espacial Kennedy, Florida
321-747-8310
leejay.lockhart@nasa.gov
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Last Updated Oct 03, 2024 LocationKennedy Space Center Related Terms
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By NASA
5 min read
NASA’s LRO: Lunar Ice Deposits are Widespread
Deposits of ice in lunar dust and rock (regolith) are more extensive than previously thought, according to a new analysis of data from NASA’s LRO (Lunar Reconnaissance Orbiter) mission. Ice would be a valuable resource for future lunar expeditions. Water could be used for radiation protection and supporting human explorers, or broken into its hydrogen and oxygen components to make rocket fuel, energy, and breathable air.
Prior studies found signs of ice in the larger permanently shadowed regions (PSRs) near the lunar South Pole, including areas within Cabeus, Haworth, Shoemaker and Faustini craters. In the new work, “We find that there is widespread evidence of water ice within PSRs outside the South Pole, towards at least 77 degrees south latitude,” said Dr. Timothy P. McClanahan of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and lead author of a paper on this research published October 2 in the Planetary Science Journal.
The study further aids lunar mission planners by providing maps and identifying the surface characteristics that show where ice is likely and less likely to be found, with evidence for why that should be. “Our model and analysis show that greatest ice concentrations are expected to occur near the PSRs’ coldest locations below 75 Kelvin (-198°C or -325°F) and near the base of the PSRs’ poleward-facing slopes,” said McClanahan.
This illustration shows the distribution of permanently shadowed regions (in blue) on the Moon poleward of 80 degrees South latitude. They are superimposed on a digital elevation map of the lunar surface (grey) from the Lunar Orbiter Laser Altimeter instrument on board NASA’s Lunar Reconnaissance Orbiter spacecraft. NASA/GSFC/Timothy P. McClanahan “We can’t accurately determine the volume of the PSRs’ ice deposits or identify if they might be buried under a dry layer of regolith. However, we expect that for each surface 1.2 square yards (square meter) residing over these deposits there should be at least about five more quarts (five more liters) of ice within the surface top 3.3 feet (meter), as compared to their surrounding areas,” said McClanahan. The study also mapped where fewer, smaller, or lower-concentration ice deposits would be expected, occurring primarily towards warmer, periodically illuminated areas.
Ice could become implanted in lunar regolith through comet and meteor impacts, released as vapor (gas) from the lunar interior, or be formed by chemical reactions between hydrogen in the solar wind and oxygen in the regolith. PSRs typically occur in topographic depressions near the lunar poles. Because of the low Sun angle, these areas haven’t seen sunlight for up to billions of years, so are perpetually in extreme cold. Ice molecules are thought to be repeatedly dislodged from the regolith by meteorites, space radiation, or sunlight and travel across the lunar surface until they land in a PSR where they are entrapped by extreme cold. The PSR’s continuously cold surfaces can preserve ice molecules near the surface for perhaps billions of years, where they may accumulate into a deposit that is rich enough to mine. Ice is thought to be quickly lost on surfaces that are exposed to direct sunlight, which precludes their accumulations.
The team used LRO’s Lunar Exploration Neutron Detector (LEND) instrument to detect signs of ice deposits by measuring moderate-energy, “epithermal” neutrons. Specifically, the team used LEND’s Collimated Sensor for Epithermal Neutrons (CSETN) that has a fixed 18.6-mile (30-kilometer) diameter field-of-view. Neutrons are created by high-energy galactic cosmic rays that come from powerful deep-space events such as exploding stars, that impact the lunar surface, break up regolith atoms, and scatter subatomic particles called neutrons. The neutrons, which can originate from up to about a 3.3-foot (meter’s) depth, ping-pong their way through the regolith, running into other atoms. Some get directed into space, where they can be detected by LEND. Since hydrogen is about the same mass as a neutron, a collision with hydrogen causes the neutron to lose relatively more energy than a collision with most common regolith elements. So, where hydrogen is present in regolith, its concentration creates a corresponding reduction in the observed number of moderate-energy neutrons.
“We hypothesized that if all PSRs have the same hydrogen concentration, then CSETN should proportionally detect their hydrogen concentrations as a function of their areas. So, more hydrogen should be observed towards the larger-area PSRs,” said McClanahan.
The model was developed from a theoretical study that demonstrated how similarly hydrogen-enhanced PSRs would be detected by CSETNs fixed-area field-of-view. The correlation was demonstrated using the neutron emissions from 502 PSRs with areas ranging from 1.5 square miles (4 km2) to 417 square miles (1079 km2) that contrasted against their surrounding less hydrogen-enhanced areas. The correlation was expectedly weak for the small PSRs but increased towards the larger-area PSRs.
The research was sponsored by the LRO project science team, NASA’s Goddard Space Flight Center’s Artificial Intelligence Working Group, and NASA grant award number 80GSFC21M0002. The study was conducted using NASA’s LRO Diviner radiometer and Lunar Orbiter Laser Altimeter instruments. The LEND instrument was developed by the Russian Space Agency, Roscosmos by its Space Research Institute (IKI). LEND was integrated to the LRO spacecraft at the NASA Goddard Space Flight Center. LRO is managed by NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for the Science Mission Directorate at NASA Headquarters in Washington.
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Last Updated Oct 03, 2024 Editor wasteigerwald Contact wasteigerwald william.a.steigerwald@nasa.gov Location Goddard Space Flight Center Related Terms
Earth’s Moon Lunar Reconnaissance Orbiter (LRO) Uncategorized Explore More
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