SARP East 2025 Ecohydrology Group

SARP East 2025 Ecohydrology Group

9 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

A group of eight people stand together inside a hangar with a somewhat shiny floor. In the background is a small white plane with a blue stripe, and large windows behind that.
The 2025 SARP East Ecohydrology Group poses in front of the Dynamic Aviation B-200 aircraft, parked in a hangar at NASA’s Wallops Flight Facility in Virgina. During the internship, students spend a week engaged in Earth science data collection and learning from instruments specialists while flying onboard both the B-200 and NASA’s P-3 aircraft.
NASA/Milan Loiacono

Faculty Advisor:

Dom Ciruzzi, William & Mary

Graduate Mentor:

Sarah Payne, University of California, Santa Barbara

Ecohydrology Group Introduction

Faculty Advisor Dom Ciruzzi and Graduate Mentor Sarah Payne

Ethan Bledsoe

Uncovering Hidden Green to Reveal Water: Can Spectral Unmixing of Vegetation Reduce Evapotranspiration Bias in Semi-Arid Landscapes? 

Ethan Bledsoe, Northwestern University 

Deserts push life to its limits, presenting sparse vegetation and scarce water that challenge traditional methods for accurately capturing evapotranspiration (ET). Current satellite ET estimates often struggle in dryland areas. These estimates typically rely on vegetation indices like the Normalized Difference Vegetation Index (NDVI), which can be distorted by bright desert soils and sparse vegetation. This distortion leads to inaccurate ET estimates, affecting crucial decisions related to drought management and water resource planning. To address this problem, we used a technique called Multiple Endmember Spectral Mixture Analysis (MESMA), which classifies pixels into percentages of green vegetation, soil, and shade based on unique spectral signatures. We created a spectral library using high-resolution (1 m) hyperspectral images collected from the NEON Airborne Observation Platform (AOP) over the Santa Rita Experimental Range (SRER). This library was then applied to imagery at different resolutions—medium-resolution (30 m) Landsat 8 Operational Land Imager (OLI) satellite imagery and lower-resolution (500 m) Moderate Resolution Imaging Spectroradiometer (MODIS) satellite imagery—to produce more accurate fractional vegetation maps. We integrated these detailed vegetation maps into OpenET’s Priestley-Taylor Jet Propulsion Laboratory (PT-JPL) ET model and compared the results to ground-based ET measurements from the SRER flux tower near Tucson, Arizona. On August 20, 2021, all models underestimated ET compared to flux tower observations. Among them, the standard PT-JPL model produced the closest estimate, while MESMA-based ET values were lower and generally declined further with decreasing spatial resolution. Because our method uses publicly available imagery and a remotely collected spectral library, it can be applied to other desert regions, enhancing our understanding of modeling ET and, in-turn, improving our water management in an increasingly arid world. 

Rylee Chafin 

Examining Changes in Vegetation Moisture Indices and Biodiversity Estimates at the San Clemente Dam Removal Site in California 

Rylee Chafin, University of North Georgia 

With dam removal becoming a more widespread practice, it is important to understand how riparian ecosystems respond to these hydrological changes. Airborne Visible Infrared Imaging Spectrometer (AVIRIS) flights over the San Clemente Dam near Carmel, California provide an ideal opportunity to understand changes in hydrology and biodiversity across an entire watershed, rather than at small vegetation plots. This case study investigates the only large dam in the nation that has had sufficient AVIRIS data to understand these changes. This study processed AVIRIS data from August 2015 and October 2019 and examined how the Normalized Difference Moisture Index (NDMI) changes between the two flights. This data was then compared with two stream gauges located downstream of the dam to better understand the hydrology of this watershed and the effects of dam removal on streamflow. Then, I used the AVIRIS data to create estimated alpha diversity maps using the biodivMapR R package. This study found that NDMI and alpha diversity estimates were correlated in the riparian area. This indicates that moisture and plant biodiversity have changed across the riparian ecosystem, possibly as a result of dam removal, and helps us understand the ecological implications of this practice. Future AVIRIS (or other hyperspectral) flights over other dam removal sites can help expand this research to evaluate the effectiveness of these methods and better establish correlation between dam removal, moisture, and biodiversity. 

Sumaya Tandon

Tracking Tree Emissions from the Sky: Improving Isoprene Estimates with MEGAN 

Sumaya Tandon, Trinity University 

Isoprene, a biogenic volatile organic compound, is emitted from tree species and contributes to the formation of secondary pollutants such as formaldehyde and ozone. With its short atmospheric life span of up to an hour and complex emissions dynamics, it is hard to quantify, and therefore predict, how much of it is in the atmosphere. This study employs the Model of Emissions of Gases and Aerosols from Nature (MEGAN) to estimate isoprene emissions in California and Missouri, two regions with contrasting vegetation types, during the summer of 2013. The predictions were compared to airborne data, specifically whole air sampling, from the flight campaign SEAC4RS to evaluate MEGAN’s accuracy. Specifically, to parameterize MEGAN this study utilizes the North American Data Assimilation System (NDLAS) to compile a list of meteorological and surface variables. Two different models were run, one with consideration of drought stress and one without, to evaluate the impact of water stress on modeled isoprene emissions. The results of this study show MEGAN consistently underpredicted isoprene in both regions with and without water stress consideration. However, including drought stress can potentially improve predictions for areas with very low-emissions suggesting that accounting for water stress may improve MEGAN. With these findings in mind, it’s beneficial to integrate ecohydrological understanding into emissions models. Isoprene emissions from airborne data has rarely been used in the context of studying drought with MEGAN, therefore this work highlights the importance of understanding and refining stress response parameters- a crucial step towards improving predictions of biogenic emissions for future climate scenarios. 

TJ Ochoa Peterson

Understanding the Relationship Between Cloud Type and Evapotranspiration in Shrubland Vegetation 

TJ Ochoa Peterson, Michigan State University 

Evapotranspiration (ET) is a key indicator of ecosystem health, representing water flux from the surface to the atmosphere. High ET values can result, in-part, from water-intensive vegetation while the inverse can indicate insufficient water for evaporation. A persistent challenge in remote sensing ET is cloud contamination. Thermal infrared sensors used to derive remote sensed ET apply cloud masking which removes affected pixels and results in data gaps. Although prior studies have examined the impact of cloud amount on ET, the influence of specific cloud types remains underexplored. This study investigates how distinct cloud types (Cumulus, Altostratus, and Cumulonimbus) affect surface-level ET over shrubland vegetation in Tucson, Arizona, during the North American Monsoon season. Cloud classification was performed using Cloud Optical Depth (COD) and Cloud Top Pressure (CTP) from GOES-18 Level 2 products, following criteria from the International Satellite Cloud Climatology Project (ISCCP) dataset. These classifications were compared against in-situ ET observations from the Santa Rita Experimental Range NEON flux tower. Results indicate that cloud presence generally reduces instantaneous ET relative to preceding clear-sky conditions. Clouds with low altitude and low density (Cumulus, Stratocumulus) generally showed brief reductions in ET. Notable results include ET values observed under high COD and low CTP conditions, characteristic of Cumulonimbus clouds, did not differ significantly from clear-sky conditions. Future research should incorporate cloud-type into ET models to improve accuracy, particularly in regions prone to frequent cloud cover. Further work could deduce cloud-type patterns for the intent of data gap filling models that estimate ET during cloud-contaminated periods, reducing data loss and enhancing understanding of land-atmosphere interactions. 

Rachel Faessler

Comparing Tree Biodiversity in San Jose, California Using Hyperspectral Imagery and Ground Data 

Rachel Faessler, University of Wisconsin-Green Bay 

Street trees provide a myriad of ecosystem services, such as cooling air temperature, improving air quality, reducing runoff, and improving human well-being. Furthermore, having many different species of trees (high biodiversity) is important, as this improves the overall resilience of a forest community to disturbances, which increases reliable access to ecosystem services. Airborne hyperspectral data is often used to measure biodiversity or health of trees in natural forests, but rarely in urban environments. When urban ecosystems are studied, the focus is on interactions with humans or the local effects of vegetation. Uniquely, this study seeks to compare indicators of alpha and beta diversity compiled from Airborne Visible/Infrared Imaging Spectrometer (AVIRIS) hyperspectral imagery (collected in 2024) and Dryad ground-based sampling of 264,000 street trees in San Jose, California (collected in 2021). There appears to be more spatial variability in the AVIRIS estimated beta diversity than in alpha diversity. There is a modest correlation between ground and AVIRIS derived measures of alpha diversity, which is a step forward in expanding estimates of tree biodiversity in cities using hyperspectral imagery. Future work could connect spatial variation of biodiversity to city planning measures such as income, residential/business areas, income, or redlining; compare hyperspectral diversity to areas of alpha diversity with consistent sampling; or build on different measures of diversity than species diversity (e.g. isohydricity). 

Katie Wilson

How Does Antecedent Soil Moisture Influence Flooding in the Southeastern U.S.? A Case Study in Athens, Georgia 

Katie Wilson, North Carolina State University 

Floods are the most common and deadly natural disaster in the United States, known for their rapid and widespread impacts. While previous research has examined how antecedent soil moisture (ASM) affects flood severity, relatively little work has focused on the Southeastern United States. This region is especially vulnerable due to high annual rainfall and tropical systems, both of which can lead to flooding. To address this gap, this study investigates the relationship between ASM and streamflow response during rainfall events in Athens, Georgia, located within the South Atlantic-Gulf watershed. Precipitation datasets (1977–2025) were compiled from three NOAA National Centers for Environmental Information weather stations in Athens. Streamflow data was obtained from the USGS Apalachee River near Bostwick, GA (1977–2025). ASM data was gathered from the Soil Climate Analysis Network (SCAN) Watkinsville station (1997–2025) and NASA’s Soil Moisture Active Passive (SMAP) satellite (2015–2025). Precipitation events were binned by total rainfall, with maximum streamflow recorded during the event and ASM taken from the day prior. Events were grouped into four rainfall categories (0–1″, 1–2″, 3–4″, and 5–6″), and streamflow responses were compared between low (0-40%) and high (60-100%) ASM conditions using the Kruskal-Wallis H test. Results showed statistically significant differences (p < 0.05) in streamflow dependent on ASM across all rainfall bins, confirming that wetter antecedent conditions increase runoff and flood potential. Incorporating ASM into flood forecasting models, along with tools like SMAP, can improve early warning systems in the Southeast U.S. and enhance flood preparedness. 

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Milan Loiacono

NASA’s Mars Spacecraft Capture Images of Comet 3I/ATLAS

NASA’s Mars Spacecraft Capture Images of Comet 3I/ATLAS

6 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Two orbiters and a rover captured images of the interstellar object — from the closest location any of the agency’s spacecraft may get — that could reveal new details.

At the start of October, three of NASA’s Mars spacecraft had front row seats to view 3I/ATLAS, only the third interstellar object so far discovered in our solar system. The Mars Reconnaissance Orbiter (MRO) snapped a close-up of the comet, while the MAVEN (Mars Atmosphere and Volatile EvolutioN) orbiter captured ultraviolet images and the Perseverance rover caught a faint glimpse as well.  

Imagery from MRO will allow scientists to better estimate the comet’s size, and MAVEN’s images are unique among all observations this year in determining the chemical makeup of the comet and how much water vapor is released as the Sun warms the comet. These details will help scientists better understand the past, present, and future of this object.

HiRISE 

The comet will be at its closest approach to Earth on Friday, Dec. 19. On Oct. 2, MRO observed 3I/ATLAS from 19 million miles (30 million kilometers) away, with one of the closest views that any NASA spacecraft or Earth-based telescopes are expected to get.  

The orbiter’s team viewed the comet with a camera called HiRISE (the High Resolution Imaging Science Experiment), which normally points at the Martian surface. By rotating, MRO can point HiRISE at celestial objects as well — a technique used in 2014, when HiRISE joined MAVEN in studying another comet, called Siding Spring

Captured at a scale of roughly 19 miles (30 kilometers) per pixel, 3I/ATLAS looks like a pixelated white ball on the HiRISE imagery. That ball is a cloud of dust and ice called the coma, which the comet shed as it continued its trajectory past Mars. 

“Observations of interstellar objects are still rare enough that we learn something new on every occasion,” said Shane Byrne, HiRISE principal investigator at the University of Arizona in Tucson. “We’re fortunate that 3I/ATLAS passed this close to Mars.” 

Further study of the HiRISE imagery could help scientists estimate the size of the comet’s nucleus, its central core of ice and dust. More study also may reveal the size and color of particles within its coma. 

“One of MRO’s biggest contributions to NASA’s work on Mars has been watching surface phenomena that only HiRISE can see,” said MRO’s project scientist Leslie Tamppari of NASA’s Jet Propulsion Laboratory in Southern California. “This is one of those occasions where we get to study a passing space object as well.” 

MAVEN  

Over the course of 10 days starting Sept. 27, MAVEN captured 3I/ATLAS in two unique ways with its Imaging Ultraviolet Spectrograph (IUVS) camera. First, IUVS took multiple images of the comet in several wavelengths, much like using various filters on a camera. Then it snapped high-resolution UV images to identify the hydrogen coming from 3I/ATLAS. Studying a combination of these images, scientists can identify a variety of molecules and better understand the comet’s composition.  

“The images MAVEN captured truly are incredible,” said Shannon Curry, MAVEN’s principal investigator and research scientist at the Laboratory for Atmospheric and Space Physics (LASP) at the University of Colorado Boulder. “The detections we are seeing are significant, and we have only scraped the surface of our analysis.” 

The IUVS data also offers an estimated upper limit of the comet’s ratio of deuterium (a heavy isotope of hydrogen) to regular hydrogen, a tracer of the comet’s origin and evolution. When the comet was at its closest to Mars, the team used more sensitive channels of IUVS to map different atoms and molecules in the comet’s coma, such as hydrogen and hydroxyl. Further study of the comet’s chemical makeup could reveal more about its origins and evolution. 

“There was a lot of adrenaline when we saw what we’d captured,” said MAVEN’s deputy principal investigator, Justin Deighan, a LASP scientist and the lead on the mission’s comet 3I/ATLAS observations. “Every measurement we make of this comet helps to open up a new understanding of interstellar objects.” 

A predominantly black view of space is dotted with stars, seen as short white streaks, in an animated image that consists of two observations. In the right half of the image, interstellar comet 3I/ATLAS is a barely visible white smudge that becomes slightly more distinct in the second observation.
Interstellar comet 3I/ATLAS is seen as a faint smudge against a background starfield in two images taken by the Mastcam-Z instrument aboard NASA’s Perseverance Mars rover on Oct. 4, 2025. At the time it was imaged, the comet was about 19 million miles (30 million kilometers) from the rover, which was exploring the rim of the Red Planet’s Jezero Crater.
NASA/JPL-Caltech/ASU/MSSS

Perseverance 

Far below the orbiters, on the Martian surface, NASA’s Perseverance rover also caught sight of 3I/ATLAS. On Oct. 4, the comet appeared as a faint smudge to the rover’s Mastcam-Z camera. The exposure had to be exceptionally long to detect such a faint object. Unlike telescopes that track objects as they move, Mastcam-Z is fixed in place during long exposures. This technique produces star trails that appear as streaks in the sky, though the comet itself is barely perceptible. 

More about MRO, MAVEN, Perseverance 

A division of Caltech in Pasadena, California, JPL manages MRO for NASA’s Science Mission Directorate in Washington as part of NASA’s Mars Exploration Program portfolio. The University of Arizona in Tucson operates MRO’s HiRISE, which was built by BAE Systems in Boulder, Colorado. Lockheed Martin Space in Denver built MRO and supports its operations. 

The MAVEN mission, also part of NASA’s Mars Exploration Program portfolio, is led by the Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder. It’s managed by NASA’s Goddard Space Flight Center in Greenbelt, Maryland. MAVEN was built and operated by Lockheed Martin Space in Littleton, Colorado, with navigation and network support from JPL. 

JPL built and manages operations of the Perseverance rover on behalf of the agency’s Science Mission Directorate as part of NASA’s Mars Exploration Program portfolio. 

To learn more about NASA’s observations of comet 3I/ATLAS, visit: 

https://go.nasa.gov/3I-ATLAS

News Media Contacts

Andrew Good 
Jet Propulsion Laboratory, Pasadena, Calif. 
818-393-2433 
andrew.c.good@jpl.nasa.gov 

Alise Fisher / Molly Wasser 
NASA Headquarters, Washington 
202-617-4977 / 240-419-1732 
alise.m.fisher@nasa.gov / molly.l.wasser@nasa.gov 

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Presencia el lanzamiento de Artemis II

Presencia el lanzamiento de Artemis II

9 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Los miembros de la tripulación de Artemis II (de izquierda a derecha: el astronauta de la CSA o Agencia Espacial Canadiense Jeremy Hansen, y los astronautas de la NASA Christina Koch, Victor Glover y Reid Wiseman) salen de las instalaciones de alojamiento de astronautas en el Edificio de Operaciones y Verificación Neil Armstrong, dirigiéndose hacia los vehículos de transporte de la tripulación Artemis para ir a la Plataforma de Lanzamiento 39B como parte de una prueba integrada de sistemas terrestres en el Centro Espacial Kennedy en Florida el miércoles 20 de septiembre, para poner a prueba el horario de la tripulación para el día del lanzamiento.
NASA/Kim Shiflett

Los creadores digitales y usuarios de redes sociales están invitados a inscribirse para asistir al lanzamiento de la misión Artemis II de la NASA. El cohete Sistema de Lanzamiento Espacial (SLS, por sus siglas en inglés) de la agencia lanzará al espacio la nave espacial Orion desde el complejo de lanzamientos 39B en el Centro Espacial Kennedy de la NASA en Florida. Cuatro astronautas a bordo de la nave volarán alrededor de la Luna y regresarán a la Tierra tras permanecer unos 10 días en el espacio.

¿Eres un apasionado de las redes sociales y las comunicaciones? ¿Te entusiasma crear contenido para su público? ¿Eres fanático de experiencias nuevas y únicas? Si la respuesta a todo es sí, ¡este evento de NASA Social es para ti! Esta es tu oportunidad de tener un asiento de primera fila para presenciar esta misión histórica de Artemis que sentará la bases para futuros aterrizajes en la Luna y futuras misiones tripuladas a Marte.

Este evento de NASA Social tendrá lugar durante dos días, incluyendo el día del lanzamiento. Está previsto que la misión Artemis II sea lanzada a más tardar en abril de 2026, con posibles oportunidades desde febrero. Un máximo de 50 creadores digitales serán seleccionados para asistir a este evento de dos días, y tendrán un acceso similar al de los medios de comunicación.

Los participantes de este NASA Social tendrán la oportunidad de:

  • Recorrer el Centro Espacial Kennedy de la NASA
  • Aprender directamente de nuestros expertos
  • Conocer a otros creadores digitales y usuarios de redes sociales
  • Compartir con las personas que integran el equipo de redes sociales de la NASA
  • Ver el lanzamiento de la misión Artemis II

El plazo de inscripción a este evento de NASA Social para el lanzamiento de Artemis II comienza en esta página el miércoles 19 de noviembre y la fecha límite para presentar la solicitud es el lunes 24 de noviembre a las 5 p.m., hora del este. Todas las solicitudes serán consideradas individualmente.

INSCRÍBETE YA

¿Necesito tener una cuenta de redes sociales para inscribirme?
Sí. Este evento está diseñado para personas que:

  • Utilizan activamente diferentes plataformas y herramientas de redes sociales para difundir información a una audiencia determinada.
  • Producen con regularidad nuevos contenidos que contienen elementos multimedia.
  • Tienen el potencial de alcanzar un gran número de personas utilizando las plataformas digitales.
  • Conectan con una audiencia específica, independiente y diferente de la de los medios de comunicación tradicionales o la de la NASA.
  • Tienen un historial acreditado de publicación de contenido en plataformas de redes sociales.
  • Tienen publicaciones anteriores que han logrado una gran visibilidad y que son respetadas y ampliamente reconocidas.

Se anima a los usuarios a seguir @NASAArtemis para las actualizaciones de la campaña Artemis en X, Facebook e Instagram (en inglés), así como las cuentas de la NASA en español en X, Facebook e Instagram. Las actualizaciones y la información sobre el evento se compartirán (en inglés) en X a través de la cuenta @NASA_Events.

¿Cómo me inscribo?
El  plazo de inscripción para este evento comienza el 19 de noviembre y termina el 24 de noviembre a las 5 p. m., hora del este de Estados Unidos. La inscripción es solo para una persona (tú) y no es transferible. Cada persona que desee asistir debe inscribirse por separado. Cada solicitud será considerada individualmente.

¿Puedo inscribirme si no tengo ciudadanía estadounidense?
Sí, este evento está abierto para todos los que lo soliciten.

¿Cuándo sabré si he sido seleccionado?
Después de que se hayan recibido y procesado las inscripciones, se enviará a la gente seleccionada un correo electrónico con información de confirmación e instrucciones adicionales. Esperamos enviar las primeras notificaciones el lunes 8 de diciembre, y las notificaciones de lista de espera el lunes 15 de diciembre.

¿Cuáles son las credenciales de NASA Social?
Todas las solicitudes para el evento de NASA Social serán consideradas individualmente. Aquellas personas elegidas deben demostrar a través del proceso de inscripción que cumplen con los criterios específicos de participación.

Aún si no consigues participar en este evento de NASA Social, puedes observar el lanzamiento fuera de las instalaciones de la NASA y participar en la conversación en línea. Descubre las formas en que puedes presenciar un despegue visitando el sitio web (en inglés)
http://www.nasa.gov/centers/kennedy/launchingrockets/viewing.html

¿Cuáles son los requisitos para la inscripción?
La inscripción debe indicar tu intención de viajar al Centro Espacial Kennedy de la NASA en Florida y de asistir en persona a este evento de dos días de duración. Tú serás responsable de tus propios gastos de viaje, alojamiento, comida y otros servicios.

La programación de los eventos y la participación de invitados especiales están sujetas a cambios sin previo aviso. La NASA no se hace responsable de las pérdidas o daños ocasionados como resultado de tu visita. Además, la NASA no se hace responsable de las pérdidas o daños ocasionados si el evento es cancelado con una anticipación limitada o sin previo aviso. Por favor, planifica tu asistencia como corresponda.

El centro Kennedy es una instalación del gobierno. Aquellas personas seleccionadas podrían tener que completar algunos pasos de inscripción adicionales para recibir autorización para ingresar a áreas de acceso protegido.

IMPORTANTE: No se admitirá a personas sin la debida identificación.

Para ciudadanos estadounidenses:

  • Se te pedirá que presentes la identificación de REAL ID o un pasaporte válido de Estados Unidos MÁS uno de los siguientes documentos:
  • Documentos aceptables para acompañar la identificación federal o estatal:
  • Pasaporte estadounidense
  • Tarjeta de autorización de empleo no vencida (formulario I-688A)
  • Documento de autorización de empleo no vencido emitido por el Departamento de Seguridad Nacional (DHS) que contenga una fotografía (formulario I-688B)
  • Licencia de conducir o tarjeta de identificación expedida por un estado o territorio de Estados Unidos, siempre que contenga una fotografía o información como nombre, fecha de nacimiento, sexo, estatura, color de ojos y dirección
  • Tarjeta de identificación expedida por organismos o entidades gubernamentales federales, estatales o locales, siempre que contenga una fotografía o información como nombre, fecha de nacimiento, sexo, estatura, color de ojos y dirección
  • Tarjeta de identificación académica con fotografía
  • Tarjeta de registro electoral
  • Tarjeta de identificación como dependiente de militar
  • Tarjeta militar o registro de reclutamiento de Estados Unidos
  • Tarjeta de miembro de la Marina Mercante de la Guardia Costera de Estados Unidos
  • Documento tribal de identificación de nativo estadounidense
  • Tarjeta del Seguro Social de Estados Unidos emitida por la Administración del Seguro Social (que no sea una tarjeta que indique que no es válida para el empleo)
  • Original o copia certificada de la partida de nacimiento expedida por un estado, condado, autoridad municipal o territorio de Estados Unidos que contenga un sello oficial
  • Tarjeta de identificación de ciudadanía estadounidense (formulario I-197)
  • Tarjeta de identificación para uso de ciudadanos residentes en Estados Unidos (formulario I-179)
  • Documento de autorización de empleo no vencido emitido por el DHS que contenga una fotografía (que sea diferente de los documentos indicados anteriormente)

Para ciudadanos extranjeros:

  • Se permiten los mismos documentos indicados para los ciudadanos estadounidenses (la tarjeta del seguro social, SSN, solo será solicitada cuando corresponda)
  • Pasaporte extranjero no vencido, con sello I-551 o formulario I-94 adjunto que indique autorización de empleo no vencida
  • Número de pasaporte y fecha de registro
  • Documento de ciudadanía
  • Licencia de conducir emitida por una autoridad gubernamental canadiense
  • Para extranjeros con residencia legal en Estados Unidos:
  • Se permiten los mismos documentos indicados para los ciudadanos estadounidenses y:
  • Tarjeta de residencia permanente o tarjeta de recibo de registro de extranjero con fotografía (formulario I-551)
  • Tarjeta de residente temporal no vencida (formulario I-688)
  • Certificado de nacimiento en el extranjero expedido por el Departamento de Estado (formulario FS-545 o formulario DS-1350)

La Ley de REAL ID fue aprobada por el Congreso en 2005 para establecer estándares mínimos de seguridad para las licencias de conducir y tarjetas de identificación emitidas por los estados.
Todas las personas inscritas deben tener al menos 18 años de edad.

¿Qué sucede si cambia la fecha de lanzamiento?
Cientos de factores diferentes pueden hacer que una fecha de lanzamiento programada cambie varias veces. La fecha de lanzamiento no será oficial hasta después de la revisión de aptitud para el vuelo. Si la fecha de lanzamiento cambia antes de esta revisión, la NASA puede ajustar la fecha del evento de NASA Social en consecuencia para que coincida con la nueva fecha de lanzamiento objetiva, y notificará a las personas inscritas por correo electrónico acerca de cualquier cambio que tenga lugar.

Si el lanzamiento se pospone, se invitará a las personas seleccionadas a asistir a una fecha de lanzamiento posterior. Si el lanzamiento se pospone por más de 72 horas, el evento de NASA Social podría ser cancelado.
Los asistentes al evento de NASA Social son responsables de todos los gastos adicionales ocasionados en relación con cualquier retraso en el lanzamiento. Recomendamos encarecidamente a los participantes que hagan reservas de viaje reembolsables y/o flexibles.

¿Qué sucede si no puedo acudir al Centro Espacial Kennedy?
Si no puedes venir al Centro Espacial Kennedy y asistir en persona, no debes inscribirte en el evento de NASA Social. Únete a la conversación siguiendo las cuentas de @NASAArtemis (en inglés) en X, Facebook e Instagram, o las cuantas de la NASA en español en X, Facebook e Instagram y mira el lanzamiento en nasa.gov/live (ofreceremos retransmisiones en inglés y en español). La NASA proporcionará actualizaciones periódicas sobre el lanzamiento y la misión en sus cuentas @NASA y @NASAArtemis y @NASA_ES.

Si no puedes asistir a este evento de NASA Social, no te preocupes: ¡la NASA está planeando muchos otros eventos de NASA Social en el futuro cercano que se llevarán a cabo en diferentes lugares! Sigue nuestras noticias en las redes sociales de la NASA, o en nuestro boletín semanal en español: https://www.nasa.gov/suscribete.

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Andres D. Almeida

Experience the Launch of Artemis II

Experience the Launch of Artemis II

Artemis II crew members (from left) CSA (Canadian Space Agency) astronaut Jeremy Hansen, and NASA astronauts Christina Koch, Victor Glover, and Reid Wiseman walk out of Astronaut Crew Quarters inside the Neil Armstrong Operations and Checkout Building to the Artemis crew transportation vehicles prior to traveling to Launch Pad 39B as part of an integrated ground systems test at Kennedy Space Center in Florida on Wednesday, Sept. 20, to test the crew timeline for launch day.
NASA/Kim Shiflett

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Digital creators and social media users are invited to register to attend the launch of the NASA’s Artemis II mission. The agency’s SLS (Space Launch System) rocket will launch the Orion spacecraft from Launch Complex 39B at NASA’s Kennedy Space Center in Florida. Four astronauts aboard will fly around the Moon and return to Earth after about 10 days in space.

Are you passionate about social media and communications? Do you love to create content for an audience? Are you a fan of new, unique experiences? If you said yes, this NASA Social event is for you! This is your opportunity to be on the front lines of this historic Artemis mission that will lay the groundwork for future Moon landings and crewed missions to Mars.

The NASA Social event will take place over two days, including the day of launch. Artemis II is targeted to launch no later than April 2026, with potential opportunities as soon as February. A maximum of 50 digital creators will be selected to attend this two-day event and will be given access similar to news media.

NASA Social participants will have the opportunity to:

  • Tour NASA’s Kennedy Space Center
  • Learn directly from subject matter experts
  • Meet fellow digital creators and social media users
  • Spend time with members of NASA’s social media team
  • View the launch of the Artemis II mission

NASA Social registration for the Artemis II launch opens on this page on Wednesday, Nov. 19 and the deadline to apply is 5 p.m. EST on Monday, Nov. 24. All applications will be considered on a case-by-case basis.

APPLY NOW

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

Yes. This event is designed for people who:

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

Users are encouraged to follow @NASAArtemis for Artemis updates on X, Facebook, and Instagram. Updates and information about the event will be shared on X via @NASA_Events.

How do I register?

Registration for this event opens Nov. 19 and closes at 5 p.m. EST on Nov. 24. Registration is for one person only (you) and is non-transferable. Each individual wishing to attend must register separately. Each application will be considered on a case-by-case basis.

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

Yes, this event is open for all to apply.

When will I know if I am selected?

After registrations have been received and processed, an email with confirmation information and additional instructions will be sent to those selected. We expect to send the first notifications on Monday, Dec. 8, and waitlist notifications on Monday, Dec. 15.

What are NASA Social credentials?

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

If you do not make the registration list for this NASA Social, you still can attend the launch off site and participate in the conversation online. Find out about ways to experience a launch at http://www.nasa.gov/centers/kennedy/launchingrockets/viewing.html

What are the registration requirements?

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

The schedule of events and special guest appearances are subject to change without notice. NASA is not responsible for loss or damage incurred as a result of attending. NASA, moreover, is not responsible for loss or damage incurred if the event is canceled with limited or no notice. Please plan accordingly.

Kennedy is a government facility. Those who are selected may need to complete additional steps to receive clearance to enter the secure areas.

Kennedy is a government facility. Those who are selected may need to complete additional steps to receive clearance to enter the secure areas.

IMPORTANT: Those without proper identification cannot be admitted.

For United States Citizens:

You will be required to present a REAL ID compliant identification or valid U.S. passport PLUS one of the following:

Acceptable documents to accompany federal or state identification:

  • U.S. Passport
  • Unexpired Employment Authorization Card (Form I-688A)
  • Unexpired Employment Authorization Document issued by DHS that contains a photograph (Form I-688B)
  • Driver’s license or ID card issued by a state or outlying possession of the United States provided it contains a photograph or information such as name, date of birth, gender, height, eye color, and address
  • ID card issued by federal, state or local government agencies or entities, provided it contains a photograph or information such as name, date of birth, gender, height, eye color and address
  • School ID card with a photograph
  • Voter’s Registration Card
  • Military Dependent’s ID Card
  • U.S. Military card or draft record
  • U.S. Coast Guard Merchant Mariner Card
  • Native American Tribal Document
  • U.S. Social Security Card issued by the Social Security Administration (other than a card stating it is not valid for employment)
  • Original or Certified copy of birth certificate issued by a state, county, municipal authority or outlying possessions of the United States bearing an official seal
  • U.S. Citizen ID Card (Form I-197)
  • ID Card for use of Resident Citizens of the United States (Form I-179)
  • Unexpired employment authorization document issued by DHS (other than those listed previously)

For Foreign Nationals:

  • Same items required of U.S. Citizens (SSN only when applicable)
  • Unexpired foreign passport, with I-551 stamp or attached Form I-94 indicating unexpired employment authorization
  • Passport number and registration date
  • Citizenship
  • Driver’s license issued by a Canadian Government authority

For Legal Resident Aliens:

  • Same items required of U. S. Citizens, and:
  • Permanent Resident Card or Alien Registration Receipt Card with photograph (Form I-551)
  • Unexpired Temporary Resident Card (Form I-688)
  • Certification of Birth Abroad issued by the Department of State (Form FS-545 or Form DS-1350)

The REAL ID Act was passed by Congress in 2005 to establish minimum security standards for state-issued driver’s licenses and identification cards.

All registrants must be at least 18 years old.

What if the launch date changes?

Hundreds of different factors can cause a scheduled launch date to change multiple times. The launch date will not be official until after the Flight Readiness Review. If the launch date changes prior to the review, NASA may adjust the date of the NASA Social accordingly to coincide with the new target launch date, and will notify registrants of any changes via email.

If the launch is postponed, attendees will be invited to attend a later launch date. If the launch is postponed beyond 72 hours, the NASA Social event may be canceled.

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

What if I cannot come to the Kennedy Space Center?

If you cannot come to the NASA Kennedy and attend in person, you should not register for the NASA Social. Join the conversation by following @NASAArtemis on X, Facebook, and Instagram, and watch the launch at nasa.gov/live. NASA will provide regular launch and mission updates on @NASA and @NASAArtemis.

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

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Gary Daines

Station Nation: Meet Alyssa Yockey, Neutral Buoyancy Laboratory Flight Lead 

Station Nation: Meet Alyssa Yockey, Neutral Buoyancy Laboratory Flight Lead 

Alyssa Yockey supports the International Space Station from NASA’s Johnson Space Center in Houston as a flight lead at the Neutral Buoyancy Laboratory. The Neutral Buoyancy Laboratory is one of the world’s largest indoor pools where astronauts and support teams conduct trainings and other large-scale operations, both in the water and on the pool deck. 

In this role, Yockey guides teams through integration efforts, including test readiness reviews to ensure all requirements are met, and helps prepare for suited or other testing events. She ensures smooth planning and execution of each mission-focused activity. Yockey also serves as a safety diver during astronaut suited testing events, giving her a unique perspective on both the planning and execution of Neutral Buoyancy Laboratory operations. 

Read on to learn about Yockey’s career with NASA and more! 

Alyssa Yockey, flight lead at the Neutral Buoyancy Laboratory in the Sonny Carter Training Facility in Houston.
Alyssa Yockey

Where are you from? 

Friendswood, Texas. 

How long have you been working for NASA? 

Eleven and a half years. 

What was your path to NASA? 

My path to NASA has been a unique blend of science and hands-on experience. I grew up in Friendswood, Texas, surrounded by the influence of NASA and the space community. While many around me were drawn to engineering, I knew early on that wasn’t the path I wanted to take. Instead, I followed my curiosity for the natural world and earned a master’s degree in marine biology, which gave me a strong foundation in research, problem-solving, and working in challenging environments. From there, I pursued opportunities that built on those skills, including completing offshore water survival training at the Neutral Buoyancy Laboratory for the job I held at the time. This role also allowed me to learn more about the wide range of opportunities at the facility. In addition, I became a certified scuba diver during college, which strengthened my capability and confidence in underwater and extreme environments. Together, these experiences combined my academic background with practical training, and ultimately guided me toward my role at NASA. 

Alyssa Yockey and her younger brother with Space Shuttle Columbia at Ellington Field, early 1990s.
Alyssa Yockey

How would you describe your job to family or friends that may not be familiar with NASA? 

When I explain my job to family and friends, I usually say I help make sure “astronaut pool days” go smoothly. I work with different teams to get their projects ready for NASA’s giant pool – the Neutral Buoyancy Laboratory – where astronauts practice for spacewalks both on the International Space Station and on the lunar surface. That means taking care of the paperwork, preparing checklists for mock-up setup, and ensuring everything’s ready before anyone puts on a suit and hops in the water. When I am not doing that, I sometimes have the opportunity to jump in myself as a safety diver, which essentially makes me an underwater lifeguard for the astronauts. 

Two divers pose underwater. The diver on the left is wearing a spacesuit.
Alyssa Yockey (right) supporting NASA astronaut Chris Cassidy (left) as a safety diver during his last suited event in the Neutral Buoyancy Laboratory prior to his retirement.
NASA

What advice would you give to young individuals aspiring to work in the space industry or at NASA? 

The space field is built on innovation and problem-solving, so don’t be afraid to ask questions, explore different disciplines, and step outside your comfort zone.

Alyssa Yockey

Alyssa Yockey

Neutral Buoyancy Laboratory Flight Lead 

Stay curious, be resilient, and never stop learning. Seek internships, research opportunities, and mentorships, as they can open doors and give you hands-on experience. Most importantly, remember that there is no single path into this industry. Whether you come from engineering, science, business, policy, or even the arts, your unique perspective can contribute to pushing the boundaries of what’s possible in space exploration. 

Is there a space figure you’ve looked up to or someone that inspires you?  

For me, it hasn’t been about looking up to one individual but rather being inspired by the collective effort it takes to make space exploration possible. What inspires me most is seeing how different disciplines and perspectives unite toward a single goal, often under intense pressure. That kind of teamwork and dedication motivates me to give my best and reminds me that every role, no matter how big or small, contributes to the larger success of the space program. 

Every mission is the result of countless people—engineers, divers, scientists, technicians, trainers, flight controllers, and more—all bringing their expertise together to solve complex problems.

Alyssa Yockey

Alyssa Yockey

Neutral Buoyancy Laboratory Flight Lead 

What is your favorite NASA memory or the most meaningful project you’ve worked on during your time with NASA? 

My favorite NASA memory is getting to witness, over multiple years, the collaboration of various NASA groups in developing the choreography for the four Alpha Magnetic Spectrometer (AMS) spacewalks. It was incredible to be part of that process from the very beginning. I was lucky enough to see the very first development run at the Neutral Buoyancy Laboratory, and then later watch as ESA (European Space Agency) astronaut Luca Parmitano and NASA astronaut Drew Morgan performed those same spacewalks on orbit. Being able to see all that preparation, teamwork, and problem-solving come full circle was both rewarding and unforgettable. 

A woman smiles and gives a thumbs up underwater in a spacesuit.
Alyssa Yockey in the Extravehicular Mobility Unit during a suited egress training at the Neutral Buoyancy Laboratory.
NASA

What do you love sharing about station? 

I love sharing how the space station connects directly back to life on Earth. People often think of it only as a place for astronauts to live and work in space, but it’s really a one-of-a-kind laboratory that helps us solve problems here at home. From medical research that leads to new treatments, to technology that improves clean water and sustainability, to international cooperation that shows what we can achieve when we work together—the station is a powerful reminder that exploration drives innovation and benefits everyone on Earth. 

November 2, 2025, marks 25 years of continuous human presence. What does this milestone mean to you? 

This milestone is inspiring – it represents the innovation, persistence, and teamwork required to make the extraordinary seem routine. Personally, it reminds me why exploration matters: it connects us across nations, pushes the limits of what’s possible, and builds the foundation for the next steps in our journey beyond Earth. 

If you could have dinner with any astronaut, past or present, who would it be? 

I would choose Karen Nyberg. Not only did she contribute significantly as a NASA astronaut and engineer, but she also brought a very human and creative element to her time in space. I admire how she combined her professional expertise with her passion for sewing and quilting, even creating a quilt block while aboard the space station. As someone who enjoys quilting myself, I think it would be fascinating to hear about how she balanced technical work with creative expression in such a unique environment. I imagine our conversation would cover both science and stitching, which is the perfect blend of my own interests. 

Do you have a favorite space-related memory or moment that stands out to you? 

One of my favorite space-related memories is getting to meet and chat with former NASA flight director Gene Kranz during a book signing. It was fun to hear stories firsthand from someone who played such a pivotal role in NASA’s history, and to gain insight into the dedication, teamwork, and problem-solving that make spaceflight possible. Meeting him brought history to life and reinforced why I’m grateful to be part of this field. 

A man at a desk signs autographs. Two people stand in front of him as he shaked
Alyssa Yockey (center) and her husband (left) meeting Gene Kranz (right) at a book signing event.
Alyssa Yockey

What are some of the key projects you have worked on during your time at NASA? What have been your favorite? 

During my time at NASA, I first served as a dive operations training officer, where I was responsible for training and supporting divers in the Neutral Buoyancy Laboratory. From there, I took on the role of flight lead, supporting a range of projects including Axiom Space’s integration into the Neutral Buoyancy Laboratory, working with the Micro-G Neutral Buoyancy Experiment Design Teams (Micro-G NExT) student experiment design teams, and participating in various lunar operations testing events. Each of these projects has been rewarding in different ways, whether through helping commercial partners prepare for their missions, mentoring and guiding students as they see their concepts come to life, or contributing to the future of lunar exploration. I especially enjoy the challenges each project brings, as they push me to adapt, collaborate across disciplines, and continuously grow in my role. 

What are your hobbies/things you enjoy doing outside of work? 

Outside of work, I enjoy spending time outdoors with my husband and our pups, traveling and camping in different state and national parks. Hiking is one of our favorite ways to explore new places and take in the scenery together. At home, I like to unwind with a good book or by sewing and quilting. Quilting has become a truly rewarding creative outlet for me — I love selecting fabrics, experimenting with patterns, and watching a design come to life piece by piece. Each quilt has its own story, whether it’s made for a friend, a family member, or simply for the joy of creating something new. 

Left: “One Giant Stitch” quilt, crafted by Alyssa Yockey with unique modifications. Original pattern by Kelli Fannin Quilt Designs.
Right: Signature Quilt made by Alyssa Yockey featuring fabric from retired astronaut Karen Nyberg’s “Earth Views” line, created from her favorite photos taken from space. 
Alyssa Yockey

Day launch or night launch? 

Night launch! 

Favorite space movie? 

Hidden Figures. 

NASA Worm or Meatball logo? 

Worm! 

NASA spelled out in red letters.

NASA and its partners have supported humans continuously living and working in space since November 2000. After 25 years of continuous human presence, the space station remains a training and proving ground for the future of commercial space stations, deep space missions, enabling NASA’s Artemis campaign, lunar exploration, and future Mars missions. 

Every day, we are conducting exciting research aboard our orbiting laboratory that will help us explore farther into space and bring benefits back to people on Earth. You can keep up with the latest news, videos, and pictures about space station science on the Station Research & Technology news page. It is a curated hub of space station research digital media from Johnson and other centers and space agencies.  

Sign up for our weekly email newsletter to get the updates delivered directly to you.  

Follow updates on social media at @Space_Station on X, and on the space station accounts on Facebook and Instagram.  

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Mary Pfister