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Cobertura de la NASA del lanzamiento de Europa Clipper a una luna de Júpiter
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From left to right, Dr. Peter Parker, Astronaut Victor Glover and Dr. Shih-Yung post for a photo after the 2024 Silver Snoopy Awards ceremony.NASA/Mark Knopp Two employees from NASA’s Langley Research Center in Hampton, Virginia recently earned the prestigious Silver Snoopy award, an honor given to NASA employees and contractors across the agency for outstanding achievements related to astronaut safety or mission success. Dr. Shih-Yung Lin and Dr. Peter Parker received the awards during a Space Flight Awareness (SFA) award ceremony at Langley on Nov. 21. Lin earned the award for exceptional engineering and technical leadership contributions to the Orion program. Parker earned the award for outstanding leadership and technical contributions in support of the International Space Station (ISS).
NASA astronaut Victor Glover visited Langley to present the awards. Glover is currently assigned as the pilot of NASA’s Artemis II mission to the Moon. He piloted the SpaceX Crew 1 mission to the International Space Station in 2018 and served as a flight engineer on expeditions 64 and 65.
“This, for me, feels like how I felt when I received my astronaut pin. This is us giving you our team pin,” said Glover. He later added, “This is something to wear with honor. You are a very special part of our safety and mission assurance culture.”
Astronaut Victor Glover presents the 2024 Silver Snoopy Awards to Dr. Shih-Yung at NASA Langley Research Center.NASA/Angelique Herring The Silver Snoopy is the astronauts’ personal award and is presented to less than one percent of the total NASA workforce annually. The significance of the award was not lost on the honorees, who both brought family members to share in the moment.
“I’m involved with lots of research projects, but they don’t all involve loss of human life,” said Parker. “It definitely is a more prestigious, more impactful, more consequential type of project that I’m being recognized for.”
Lin, who recently retired, echoed that sentiment.
“You set a very high standard in order to achieve the safest conditions for all the astronauts,” he said. “For me, if we get a good mission out of it, or multiple missions, I would consider that my personal lifetime goal for my career. That’s what it means to me.”
Lin and Parker each received a sterling Silver Snoopy lapel pin that has flown in space, plus a certificate of appreciation signed by Glover and an authentication letter. The pins awarded to Langley’s recipients flew aboard Space Shuttle Endeavour during an assembly mission to the International Space Station, STS-118, August 8-21, 2007. The award depicts Snoopy, a character from the “Peanuts” comic strip created by Charles Schulz.
An avid supporter of the U.S. space program, Schulz gave NASA astronauts permission to adopt Snoopy as their personal safety symbol during the Apollo era and has long served to promote excellence in every phase of space flight to help ensure the success of NASA missions. The Snoopy emblem reflects NASA and industry’s sense of responsibility and continuing concern for astronaut flight safety.
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By NASA
Credit: NASA NASA has selected Sierra Lobo, Inc. of Fremont, Ohio, to provide for test operations, test support, and technical system maintenance activities at NASA’s Stennis Space Center near Bay St. Louis, Mississippi.
The NASA Stennis Test Operations Contract is fixed-price, level-of-effort contract that has a value of approximately $47 million. The performance period begins July 1, 2025, and extends three years, with a one-year base period and two one-year option periods.
The contract will provide test operations support for customers in the NASA Stennis test complex. It also will cover the operation and technical systems maintenance of the high-pressure industrial water, high-pressure gas, and cryogenic propellant storage support areas, as well as providing welding, fabrication, machining, and component processing capabilities.
NASA Stennis is the nation’s largest propulsion test site, with infrastructure to support projects ranging from component and subscale testing to large engine hot fires. Researchers from NASA, other government agencies, and private industry utilize NASA Stennis test facilities for technology and propulsion research and developmental projects.
For information about NASA and other agency programs, visit:
https://www.nasa.gov
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Tiernan Doyle
Headquarters, Washington
202-358-1600
tiernan.doyle@nasa.gov
C. Lacy Thompson
Stennis Space Center, Bay St. Louis, Mississippi
228-363-5499
calvin.l.thompson@nasa.gov
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Last Updated Nov 21, 2024 LocationNASA Headquarters Related Terms
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Preguntas frecuentes: La verdadera historia del cuidado de la salud de los astronautas en el espacioBy NASA
NASA Read this story in English here.
La Estación Espacial Internacional es el hogar de la humanidad en el espacio y una estación de investigación que gira en órbita sobre la Tierra a unos 400 kilómetros (250 millas) de altura. La NASA y sus socios internacionales han mantenido una presencia humana continua a bordo de la estación espacial durante más de 24 años, haciendo investigaciones que no es posible realizar en la Tierra.
La gente que vive y trabaja a bordo de este laboratorio en microgravedad también forma parte de las investigaciones que se llevan a cabo, y ellos ayudan a abordar complejos problemas de la salud humana en la Tierra y preparan a la humanidad para viajar más lejos que nunca, incluyendo la Luna y Marte.
Estas son algunas de las preguntas frecuentes sobre cómo la NASA y su equipo de médicos, psicólogos, nutricionistas, científicos del ejercicio y otros profesionales especializados garantizan la salud y la condición física de los astronautas a bordo del laboratorio orbital.
¿Cuánto dura una estadía típica a bordo de la Estación Espacial Internacional?
Una misión típica a la Estación Espacial Internacional dura unos seis meses, pero puede variar en función del calendario de visitas de naves espaciales, las prioridades de la misión y otros factores. Los astronautas de la NASA también han permanecido a bordo de la estación espacial durante períodos de tiempo más largos. Estas se conocen como misiones de larga duración, y misiones anteriores de este tipo han proporcionado a la NASA cuantiosos datos sobre los vuelos espaciales a largo plazo y sus efectos en el cuerpo humano, los cuales la agencia aplica a cualquier misión tripulada.
Durante las misiones de larga duración, el equipo de profesionales médicos de la NASA se centra en optimizar la salud física y conductual de los astronautas y su desempeño, para ayudar a garantizar el éxito de la misión. Estos esfuerzos también ayudan a la NASA a prepararse para futuras misiones humanas a la Luna, Marte y más allá.
¿Cómo mantiene la NASA saludables a los astronautas mientras están en el espacio?
La NASA tiene un equipo de médicos, psicólogos y otros especialistas en tierra que se dedican a dar apoyo a la salud y el bienestar de los astronautas antes, durante y después de cada misión espacial. La NASA asigna a cada tripulación médicos con formación especializada en medicina espacial, denominados médicos de la tripulación de vuelo, una vez que la tripulación ha sido seleccionada para una misión. Los médicos de la tripulación de vuelo supervisan la atención de salud y la capacitación médica mientras los miembros de la tripulación se preparan para su misión, y monitorean la salud de la tripulación antes, durante y después de su misión a la estación espacial.
¿Cómo apoya la NASA el bienestar mental y emocional de sus astronautas mientras están en el espacio?
El equipo de salud conductual de la NASA proporciona servicios de apoyo psicológico determinados de manera individual para los miembros de la tripulación y sus familias durante cada misión. Garantizar que los astronautas puedan mantener su vitalidad en entornos extremos comienza tan pronto se inicia el proceso de selección de astronautas, en el que los candidatos son evaluados en capacidades como su adaptabilidad y resiliencia. Los astronautas reciben una formación exhaustiva que les ayuda a utilizar herramientas y tratamientos de autoevaluación para gestionar su salud conductual. La NASA también ofrece capacitación en destrezas expedicionarias a fin de preparar a cada astronauta para las misiones en capacidades importantes, como los cuidados personales y el cuidado del equipo, las comunicaciones y las destrezas de liderazgo y colaboración.
Para ayudar a mantener la motivación y la moral a bordo de la estación espacial, los astronautas pueden enviar correos electrónicos, hacer llamadas y videoconferencias con sus familiares y amigos, recibir paquetes personales enviados a bordo de las misiones de reabastecimiento de carga de la NASA y sostener teleconferencias con un psicólogo, si es necesario.
¿Cómo afecta la microgravedad a la salud física de los astronautas?
En microgravedad, sin la carga continua de la gravedad de la Tierra, se producen muchos cambios en el cuerpo humano. La NASA entiende muchas de las respuestas del sistema humano al entorno espacial, entre las que se cuentan las adaptaciones a la densidad ósea, la salud muscular, sensitivomotora y cardiovascular, pero todavía queda mucho por aprender. Estos efectos de los vuelos espaciales varían de uno a otro astronauta, por lo que los médicos de la tripulación de vuelo de la NASA monitorean regularmente la salud de cada miembro de la tripulación durante una misión e individualizan las rutinas de dieta y acondicionamiento físico para dar prioridad a la salud y el estado físico durante su permanencia en el espacio.
¿Por qué los astronautas hacen ejercicio en el espacio?
Todos los astronautas a bordo del laboratorio en órbita participan en planes de ejercicio específicamente diseñados y similares a los de la Tierra. Para mantener su fuerza y resistencia, los miembros de la tripulación tienen programadas dos horas y media de ejercicio diario para sustentar su salud muscular, ósea, aeróbica y sensitivomotora. El equipo actual a bordo de la estación espacial incluye el Dispositivo Avanzado de Ejercicio Resistivo (ARED, por sus siglas en inglés), que imita el levantamiento de pesas; una cinta de correr, llamada T2; y el Cicloergómetro con Sistema de Aislamiento y Estabilización de Vibraciones (CEVIS, por sus siglas en inglés) para el ejercicio cardiovascular.
¿Qué función cumplen la alimentación y la nutrición en el apoyo a la salud de los astronautas?
La nutrición desempeña un papel fundamental en el mantenimiento de la salud y el rendimiento óptimo de un astronauta antes, durante y después de su misión. La alimentación también cumple un rol psicosocial durante la prolongada estancia de un astronauta a bordo de la estación espacial. Los expertos que trabajan en el Laboratorio de Sistemas de Alimentación Espacial de la NASA en el Centro Johnson en Houston desarrollan alimentos nutritivos y apetitosos. Los miembros de la tripulación tienen pueden complementar las opciones del menú estándar con sus platos favoritos personales, que pueden brindar un sabor hogareño.
NASA ¿Cómo sabe la NASA si los astronautas están recibiendo los nutrientes adecuados?
Los nutricionistas y científicos de bioquímica nutricional de la NASA determinan los nutrientes (vitaminas, minerales, calorías) que los astronautas necesitan mientras están en el espacio. Este equipo lleva el registro de lo que come cada miembro de la tripulación mediante un programa de seguimiento basado en computadoras de tableta, que cada astronauta completa a diario. Los datos de la aplicación se envían semanalmente a los nutricionistas para controlar la ingesta dietética. El análisis de las muestras de sangre y orina de los astronautas que son tomadas antes, durante y después de las misiones espaciales es una parte crucial del estudio de cómo responden sus cuerpos a las condiciones únicas de los vuelos espaciales. Estas muestras proporcionan información valiosa sobre cómo cada astronauta se adapta a la microgravedad, la radiación y otros factores que afectan la fisiología humana en el espacio.
¿Cómo se entrenan los astronautas para trabajar juntos mientras están en el espacio?
Además de su capacitación técnica, los astronautas participan en la formación de destrezas de trabajo en equipo. Aprenden destrezas eficaces para la vida en grupo y cómo cuidarse y apoyarse unos a otros. Debido a su naturaleza remota y aislada, los vuelos espaciales de larga duración pueden dificultar el trabajo en equipo. Los astronautas deben mantener la conciencia situacional e implementar el programa de vuelo en un entorno en constante cambio. Por lo tanto, la comunicación efectiva es fundamental cuando se trabaja en equipo a bordo de la estación y con diferentes equipos de soporte en tierra. Los astronautas también deben ser capaces de comunicar información compleja a personas con diferente formación profesional. En última instancia, los astronautas son personas que viven y trabajan juntas a bordo de la estación y deben ser capaces de llevar a cabo un trabajo altamente técnico y resolver cualquier problema interpersonal que pueda surgir.
¿Qué sucede si hay una emergencia médica a bordo de la estación espacial?
Todos los astronautas reciben capacitación médica y tienen contacto regular con un equipo de médicos que vigilan de cerca su salud desde tierra. La NASA también mantiene una farmacia bien surtida y un conjunto de equipamientos médicos a bordo de la estación espacial para atender diversas afecciones y lesiones. Si una emergencia médica requiere volver a la Tierra, la tripulación regresará en la nave espacial que fue llevada a bordo para recibir atención médica urgente en tierra.
NASA/Bill Ingalls Puedes obtener más información sobre la Dirección de Salud y Desempeño Humano de la NASA (en inglés) en:
www.nasa.gov/hhp
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By NASA
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
The mystery of why life uses molecules with specific orientations has deepened with a NASA-funded discovery that RNA — a key molecule thought to have potentially held the instructions for life before DNA emerged — can favor making the building blocks of proteins in either the left-hand or the right-hand orientation. Resolving this mystery could provide clues to the origin of life. The findings appear in research recently published in Nature Communications.
Proteins are the workhorse molecules of life, used in everything from structures like hair to enzymes (catalysts that speed up or regulate chemical reactions). Just as the 26 letters of the alphabet are arranged in limitless combinations to make words, life uses 20 different amino acid building blocks in a huge variety of arrangements to make millions of different proteins. Some amino acid molecules can be built in two ways, such that mirror-image versions exist, like your hands, and life uses the left-handed variety of these amino acids. Although life based on right-handed amino acids would presumably work fine, the two mirror images are rarely mixed in biology, a characteristic of life called homochirality. It is a mystery to scientists why life chose the left-handed variety over the right-handed one.
A diagram of left-handed and right-handed versions of the amino acid isovaline, found in the Murchison meteorite.NASA DNA (deoxyribonucleic acid) is the molecule that holds the instructions for building and running a living organism. However, DNA is complex and specialized; it “subcontracts” the work of reading the instructions to RNA (ribonucleic acid) molecules and building proteins to ribosome molecules. DNA’s specialization and complexity lead scientists to think that something simpler should have preceded it billions of years ago during the early evolution of life. A leading candidate for this is RNA, which can both store genetic information and build proteins. The hypothesis that RNA may have preceded DNA is called the “RNA world” hypothesis.
If the RNA world proposition is correct, then perhaps something about RNA caused it to favor building left-handed proteins over right-handed ones. However, the new work did not support this idea, deepening the mystery of why life went with left-handed proteins.
The experiment tested RNA molecules that act like enzymes to build proteins, called ribozymes. “The experiment demonstrated that ribozymes can favor either left- or right-handed amino acids, indicating that RNA worlds, in general, would not necessarily have a strong bias for the form of amino acids we observe in biology now,” said Irene Chen, of the University of California, Los Angeles (UCLA) Samueli School of Engineering, corresponding author of the Nature Communications paper.
In the experiment, the researchers simulated what could have been early-Earth conditions of the RNA world. They incubated a solution containing ribozymes and amino acid precursors to see the relative percentages of the right-handed and left-handed amino acid, phenylalanine, that it would help produce. They tested 15 different ribozyme combinations and found that ribozymes can favor either left-handed or right-handed amino acids. This suggested that RNA did not initially have a predisposed chemical bias for one form of amino acids. This lack of preference challenges the notion that early life was predisposed to select left-handed-amino acids, which dominate in modern proteins.
“The findings suggest that life’s eventual homochirality might not be a result of chemical determinism but could have emerged through later evolutionary pressures,” said co-author Alberto Vázquez-Salazar, a UCLA postdoctoral scholar and member of Chen’s research group.
Earth’s prebiotic history lies beyond the oldest part of the fossil record, which has been erased by plate tectonics, the slow churning of Earth’s crust. During that time, the planet was likely bombarded by asteroids, which may have delivered some of life’s building blocks, such as amino acids. In parallel to chemical experiments, other origin-of-life researchers have been looking at molecular evidence from meteorites and asteroids.
“Understanding the chemical properties of life helps us know what to look for in our search for life across the solar system,” said co-author Jason Dworkin, senior scientist for astrobiology at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and director of Goddard’s Astrobiology Analytical Laboratory.
Dworkin is the project scientist on NASA’s OSIRIS-REx mission, which extracted samples from the asteroid Bennu and delivered them to Earth last year for further study.
“We are analyzing OSIRIS-REx samples for the chirality (handedness) of individual amino acids, and in the future, samples from Mars will also be tested in laboratories for evidence of life including ribozymes and proteins,” said Dworkin.
The research was supported by grants from NASA, the Simons Foundation Collaboration on the Origin of Life, and the National Science Foundation. Vázquez-Salazar acknowledges support through the NASA Postdoctoral Program, which is administered by Oak Ridge Associated Universities under contract with NASA.
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Last Updated Nov 21, 2024 EditorWilliam SteigerwaldContactNancy N. Jonesnancy.n.jones@nasa.govLocationGoddard Space Flight Center Related Terms
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By NASA
Hubble Space Telescope Home NASA’s Hubble Finds… Hubble Space Telescope Hubble Home Overview About Hubble The History of Hubble Hubble Timeline Why Have a Telescope in Space? Hubble by the Numbers At the Museum FAQs Impact & Benefits Hubble’s Impact & Benefits Science Impacts Cultural Impact Technology Benefits Impact on Human Spaceflight Astro Community Impacts Science Hubble Science Science Themes Science Highlights Science Behind Discoveries Hubble’s Partners in Science Universe Uncovered Explore the Night Sky Observatory Hubble Observatory Hubble Design Mission Operations Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts News Hubble News Hubble News Archive Social Media Media Resources Multimedia Multimedia Images Videos Sonifications Podcasts E-books Lithographs Fact Sheets Glossary Posters Hubble on the NASA App More Online Activities 5 Min Read NASA’s Hubble Finds Sizzling Details About Young Star FU Orionis
An artist’s concept of the early stages of the young star FU Orionis (FU Ori) outburst, surrounded by a disk of material. Credits:
NASA-JPL, Caltech In 1936, astronomers saw a puzzling event in the constellation Orion: the young star FU Orionis (FU Ori) became a hundred times brighter in a matter of months. At its peak, FU Ori was intrinsically 100 times brighter than our Sun. Unlike an exploding star though, it has declined in luminosity only languidly since then.
Now, a team of astronomers has wielded NASA’s Hubble Space Telescope‘s ultraviolet capabilities to learn more about the interaction between FU Ori’s stellar surface and the accretion disk that has been dumping gas onto the growing star for nearly 90 years. They find that the inner disk touching the star is extraordinarily hot — which challenges conventional wisdom.
The observations were made with the telescope’s COS (Cosmic Origins Spectrograph) and STIS (Space Telescope Imaging Spectrograph) instruments. The data includes the first far-ultraviolet and new near-ultraviolet spectra of FU Ori.
“We were hoping to validate the hottest part of the accretion disk model, to determine its maximum temperature, by measuring closer to the inner edge of the accretion disk than ever before,” said Lynne Hillenbrand of Caltech in Pasadena, California, and a co-author of the paper. “I think there was some hope that we would see something extra, like the interface between the star and its disk, but we were certainly not expecting it. The fact we saw so much extra — it was much brighter in the ultraviolet than we predicted — that was the big surprise.”
A Better Understanding of Stellar Accretion
Originally deemed to be a unique case among stars, FU Ori exemplifies a class of young, eruptive stars that undergo dramatic changes in brightness. These objects are a subset of classical T Tauri stars, which are newly forming stars that are building up by accreting material from their disk and the surrounding nebula. In classical T Tauri stars, the disk does not touch the star directly because it is restricted by the outward pressure of the star’s magnetic field.
The accretion disks around FU Ori objects, however, are susceptible to instabilities due to their enormous mass relative to the central star, interactions with a binary companion, or infalling material. Such instability means the mass accretion rate can change dramatically. The increased pace disrupts the delicate balance between the stellar magnetic field and the inner edge of the disk, leading to material moving closer in and eventually touching the star’s surface.
This is an artist’s concept of the early stages of the young star FU Orionis (FU Ori) outburst, surrounded by a disk of material. A team of astronomers has used the Hubble Space Telescope’s ultraviolet capabilities to learn more about the interaction between FU Ori’s stellar surface and the accretion disk that has been dumping gas onto the growing star for nearly 90 years. They found that the inner disk, touching the star, is much hotter than expected—16,000 kelvins—nearly three times our Sun’s surface temperature. That sizzling temperature is nearly twice as hot as previously believed. NASA-JPL, Caltech
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The enhanced infall rate and proximity of the accretion disk to the star make FU Ori objects much brighter than a typical T Tauri star. In fact, during an outburst, the star itself is outshined by the disk. Furthermore, the disk material is orbiting rapidly as it approaches the star, much faster than the rotation rate of the stellar surface. This means that there should be a region where the disk impacts the star and the material slows down and heats up significantly.
“The Hubble data indicates a much hotter impact region than models have previously predicted,” said Adolfo Carvalho of Caltech and lead author of the study. “In FU Ori, the temperature is 16,000 kelvins [nearly three times our Sun’s surface temperature]. That sizzling temperature is almost twice the amount prior models have calculated. It challenges and encourages us to think of how such a jump in temperature can be explained.”
To address the significant difference in temperature between past models and the recent Hubble observations, the team offers a revised interpretation of the geometry within FU Ori’s inner region: The accretion disk’s material approaches the star and once it reaches the stellar surface, a hot shock is produced, which emits a lot of ultraviolet light.
Planet Survival Around FU Ori
Understanding the mechanisms of FU Ori’s rapid accretion process relates more broadly to ideas of planet formation and survival.
“Our revised model based on the Hubble data is not strictly bad news for planet evolution, it’s sort of a mixed bag,” explained Carvalho. “If the planet is far out in the disk as it’s forming, outbursts from an FU Ori object should influence what kind of chemicals the planet will ultimately inherit. But if a forming planet is very close to the star, then it’s a slightly different story. Within a couple outbursts, any planets that are forming very close to the star can rapidly move inward and eventually merge with it. You could lose, or at least completely fry, rocky planets forming close to such a star.”
Additional work with the Hubble UV observations is in progress. The team is carefully analyzing the various spectral emission lines from multiple elements present in the COS spectrum. This should provide further clues on FU Ori’s environment, such as the kinematics of inflowing and outflowing gas within the inner region.
“A lot of these young stars are spectroscopically very rich at far ultraviolet wavelengths,” reflected Hillenbrand. “A combination of Hubble, its size and wavelength coverage, as well as FU Ori’s fortunate circumstances, let us see further down into the engine of this fascinating star-type than ever before.”
These findings have been published in The Astrophysical Journal Letters.
The observations were taken as part of General Observer program 17176.
The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.
Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contacts:
Claire Andreoli (claire.andreoli@nasa.gov)
NASA’s Goddard Space Flight Center, Greenbelt, MD
Abigail Major, Ray Villard
Space Telescope Science Institute, Baltimore, MD
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Last Updated Nov 21, 2024 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms
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Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
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This e-book highlights the mission’s recent discoveries and observations related to the birth, evolution, and death of stars.
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