NASA Teams Prepare Moon Rocket-to-Spacecraft Connector for Assembly

NASA Teams Prepare Moon Rocket-to-Spacecraft Connector for Assembly

Engineers at NASA’s Marshall Space Flight Center flip the Artemis II Orion stage adapter for installation of its diaphragm Nov. 30.
NASA/Sam Lott

The elements of the super-heavy lift SLS (Space Launch System) rocket for NASA’s Artemis II mission are undergoing final preparations before shipment to NASA’s Kennedy Space Center in Florida for stacking and pre-launch activities in 2024.

Teams at NASA’s Marshall Space Flight Center in Huntsville, Alabama, recently rotated the Orion stage adapter– a ring structure that connects NASA’s Orion spacecraft to the SLS rocket’s interim cryogenic propulsion stage (ICPS) – in preparation for the installation of its diaphragm. The installation Nov. 30 marks one of the final steps for the adapter before it is readied for shipment to Kennedy via NASA’s Super Guppy cargo aircraft.

“The diaphragm is a composite, dome-shaped structure that isolates the volume above the ICPS from that below Orion,” said Brent Gaddes, lead for the Orion stage adapter, in the Spacecraft/Payload Integration & Evolution Office for the SLS Program at Marshall. “It serves as a barrier between the two, preventing the highly flammable hydrogen gas that could escape the rocket’s propellant tanks from building up beneath the Orion spacecraft and its crew before and during launch.”

At five feet tall and weighing in at 1,800 pounds, the adapter is the smallest major element of the SLS rocket that will produce more than 8.8 million pounds of thrust to launch four Artemis astronauts inside Orion around the Moon. The adapter is fully manufactured by engineering teams at Marshall.

NASA is working to land the first woman and first person of color on the Moon under Artemis. SLS is part of NASA’s backbone for deep space exploration, along with Orion and the Gateway in orbit around the Moon, and commercial human landing systems. SLS is the only rocket that can send Orion, astronauts, and supplies to the Moon in a single launch.

For more on NASA SLS visit:

https://www.nasa.gov/sls

Corinne Beckinger
Marshall Space Flight Center, Huntsville, Ala.
256.544.0034
corinne.m.beckinger@nasa.gov

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Beth Ridgeway

NASA invita a medios al lanzamiento de misión para estudiar océanos y nubes

NASA invita a medios al lanzamiento de misión para estudiar océanos y nubes

Unos técnicos trabajan en el procesamiento del observatorio de plancton, aerosoles, nubes y ecosistemas oceánicos (PACE, por sus siglas en inglés) de la NASA en una plataforma elevada del Centro de Operaciones Espaciales Astrotech, cerca del Centro Espacial Kennedy de la agencia en Florida, el lunes 4 de diciembre de 2023.
NASA

Read this release in English here.

Ya está abierta la acreditación para los medios de comunicación para el próximo lanzamiento de la misión científica de observación de la Tierra PACE (acrónimo inglés para Plancton, Aerosoles, Nubes y Ecosistemas Oceánicos) de la NASA.

La NASA y SpaceX planean poner en órbita PACE no antes del martes 6 de febrero a bordo de un cohete Falcon 9 desde el Complejo de Lanzamiento Espacial 40 de la Estación Espacial de Cabo Cañaveral, en Florida.

Los plazos de solicitud de acreditación de medios de comunicación para el lanzamiento de PACE son los siguientes:

– Los medios de comunicación estadounidenses y los ciudadanos estadounidenses que representen a medios de comunicación internacionales deberán presentar su solicitud antes de las 5 p.m. EST 9 (hora del Este) del miércoles 17 de enero.

– Los periodistas de medios de comunicación internacionales sin ciudadanía estadounidense deberán presentar su solicitud antes de las 5 p.m. del martes 2 de enero.

Las solicitudes de acreditación de los medios de comunicación deben enviarse en línea en:

https://media.ksc.nasa.gov

La política de acreditación de medios de comunicación de la NASA está disponible en línea. Para preguntas sobre la acreditación, o para solicitar necesidades logísticas especiales, envíe un correo electrónico a: ksc-media-accreditat@mail.nasa.gov . Para otras preguntas sobre la misión, póngase en contacto con la sala de prensa de la NASA en Kennedy: 321-867-2468.

La misión PACE ampliará y mejorará el registro de 20 años de observaciones por satélite de la biología oceánica mundial, los aerosoles y las nubes. Los datos de la misión ayudarán a la NASA a entender cómo el océano y la atmósfera intercambian dióxido de carbono, medir variables atmosféricas clave asociadas con la calidad del aire y el clima de la Tierra, y vigilar la salud del océano, en parte mediante el estudio del fitoplancton, las diminutas plantas y algas que sostienen la red alimentaria marina.

La NASA publicará actualizaciones sobre los preparativos de lanzamiento para preparar la nave espacial en el blog de PACE (en inglés).

Para obtener información sobre cobertura en español en el Centro Espacial Kennedy o si desea solicitar entrevistas en español, comuníquese con Antonia Jaramillo at: antonia.jaramillobotero@nasa.gov, 321-501-8425, o Messod Bendayan, 256-930-1371.

Para más información sobre PACE (en inglés), visite:

https://science.nasa.gov/mission/pace

-fin-

María José Viñas
Sede, Washington
240-458-0248
maria-jose.vinasgarcia@nasa.gov

Laura Aguiar / Leejay Lockhart
Centro Espacial Kennedy, Florida
321-867-2468
laura.aguiar@nasa.gov / leejay.lockhart@nasa.gov

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Dec 11, 2023

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Roxana Bardan

NASA Invites Media to Launch of New Mission to Study Oceans, Clouds

NASA Invites Media to Launch of New Mission to Study Oceans, Clouds

Technicians work to process NASA’s Plankton, Aerosol, Cloud, ocean Ecosystem (PACE) observatory on an Aronson Tilt Table in a high bay at the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida on Monday, Dec. 4, 2023.
NASA

Lee esta nota de prensa en español aquí.

Media accreditation is open for the upcoming launch of NASA’s PACE (Plankton, Aerosol, Cloud ocean Ecosystem) Earth observing science mission.

NASA and SpaceX are targeting no earlier than Tuesday, Feb. 6, for a Falcon 9 rocket to launch PACE to orbit from Space Launch Complex 40 at Cape Canaveral Space Force Station in Florida.

Media accreditation application deadlines for the PACE launch are as follows:

  • U.S. media and U.S. citizens representing international media must apply by 5 p.m. EST on Wednesday, Jan. 17.
  • International media without U.S. citizenship must apply by 5 p.m. on Tuesday, Jan. 2.

Media accreditation requests must be submitted online at:

https://media.ksc.nasa.gov

NASA’s media accreditation policy is available online. For questions about accreditation, or to request special logistical needs, please email: ksc-media-accreditat@mail.nasa.gov. For other mission questions, please contact NASA Kennedy’s newsroom: 321-867-2468.

The PACE mission will continue and improve NASA’s 20-year record of satellite observations of global ocean biology, aerosols, and clouds. Data from the mission will help NASA understand how the ocean and atmosphere exchange carbon dioxide, measure key atmospheric variables associated with air quality and Earth’s climate, and monitor ocean health, in part by studying phytoplankton, tiny plants and algae that sustain the marine food web.

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

Para obtener información sobre cobertura en español en el Centro Espacial Kennedy o si desea solicitar entrevistas en español, comuníquese con Antonia Jaramillo at: antonia.jaramillobotero@nasa.gov, 321-501-8425, o Messod Bendayan, 256-930-1371.

For more information about PACE, visit:

https://science.nasa.gov/mission/pace

-end-

Alise Fisher / Erin Morton
Headquarters, Washington
202-358-2546 / 202-805-9393
alise.m.fisher@nasa.gov / erin.morton@nasa.gov

Laura Aguiar / Leejay Lockhart
Kennedy Space Center, Florida
321-867-2468
laura.aguiar@nasa.gov / leejay.lockhart@nasa.gov

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Roxana Bardan

Astronaut Kathryn Thornton Works on Hubble Space Telescope

Astronaut Kathryn Thornton Works on Hubble Space Telescope

Astronaut Kathryn Thornton works with instruments while on a spacewalk. A small part of Earth is visible behind her on the right.)
NASA

In this image from Dec. 8, 1993, astronaut Kathryn C. Thornton works with equipment during a spacewalk. The spacewalk was part of an 11-day mission, Servicing Mission 1, to service the Hubble Space Telescope. Shortly after Hubble was launched in 1990, NASA discovered a flaw in the observatory’s primary mirror that affected the clarity of the telescope’s early images. Fortunately, Hubble’s design allowed astronauts to perform repairs, replace parts, and update its technology with new instruments while in orbit.

Watch an exclusive interview with Thornton, where she shares a firsthand account of the groundbreaking mission, unveiling the challenges, triumphs, and the incredible journey that revitalized Hubble.

Image credit: NASA

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Monika Luabeya

NASA Sensor Produces First Global Maps of Surface Minerals in Arid Regions

NASA Sensor Produces First Global Maps of Surface Minerals in Arid Regions

NASA’s EMIT produced its first global maps of hematite, goethite, and kaolinite in Earth’s dry regions using data from the year ending November 2023. The mission collected billions of measurements of the three minerals and seven others that may affect climate when lofted into the air as dust storms.
NASA/JPL-Caltech

EMIT delivers first-of-a-kind maps of minerals in Earth’s dust-source areas, enabling scientists to model the fine particles’ role in climate change and more.

NASA’s EMIT mission has created the first comprehensive maps of the world’s mineral dust-source regions, providing precise locations of 10 key minerals based on how they reflect and absorb light. When winds loft these substances into the air, they either cool or warm the atmosphere and Earth’s surface, depending on their composition. Understanding their abundance around the globe will help researchers predict future climate impacts.

Launched to the International Space Station in 2022, EMIT – short for Earth Surface Mineral Dust Source Investigation – is an imaging spectrometer developed by NASA’s Jet Propulsion Laboratory in Southern California. The mission fills a crucial need among climate scientists for more detailed information on surface mineral composition.

Surveying Earth’s surface from about 250 miles (410 kilometers) above, EMIT scans broad areas that would be impossible for a geologist on the ground or instruments carried by aircraft to survey, yet it does this while achieving effectively the same level of detail.

EMIT, a NASA mission launched to the International Space Station in 2022, mapped hematite, goethite, and kaolinite in North Africa and the Arabian Peninsula. The three minerals are among 10 key substances the mission studied that are thought to influence climate change.
NASA/JPL-Caltech

To date, the mission has captured more than 55,000 “scenes” – 50-by-50-mile (80-by-80-kilometer) images of the surface – in its study area, which includes arid regions within a 6,900-mile-wide (11,000-kilometer-wide) belt around Earth’s mid-section. Taken together, the scenes comprise billions of measurements – more than enough to create detailed maps of surface composition.

The mission has also demonstrated a range of additional capabilities in its 17 months in orbit, including detecting plumes of methane and carbon dioxide being emitted by landfills, oil facilities, and other infrastructure.

“Wherever we need chemistry to understand something on the surface, we can do that with imaging spectroscopy,” said Roger Clark, an EMIT science team member and senior scientist at the Planetary Science Institute in Tucson, Arizona. “Now, with EMIT, we’re going to see the big picture, and that’s certainly going to open some eyes.” 

Dust and Climate

Scientists have long known that airborne mineral dust affects the climate. They know that darker, iron oxide-rich substances absorb the Sun’s energy and warm the surrounding air, while non-iron-based, brighter substances reflect light and heat, cooling the air. Whether those effects have a net warming or cooling impact, however, has remained uncertain.

Researchers have an idea of how dust travels through the atmosphere, but the missing piece has been the composition – the color, essentially – of the surface in the places dust typically originates, which until now was derived from fewer than 5,000 sample sites around the world. Based on billions of samples, EMIT’s maps offer much more detail.

“We’ll take the new maps and put them into our climate models,” said Natalie Mahowald, EMIT’s deputy principal investigator and an Earth system scientist at Cornell University in Ithaca, New York. “And from that, we’ll know what fraction of aerosols are absorbing heat versus reflecting to a much greater extent than we have known in the past.”

Dust and Ecosystems

Beyond harnessing EMIT’s mineral data to improve Earth climate modeling, scientists can use the information to study dust’s impact on the ecosystems where it lands. There’s strong evidence that particles settling in the ocean can spur phytoplankton blooms, which can have implications for aquatic ecosystems and the planet’s carbon cycle. Scientists also have shown that dust originating in the Andes of South America, as well as in parts of northern and sub-Saharan Africa, provides nutrients for rainforest growth in the Amazon basin.

EMIT data can enable researchers to pinpoint the sources of mineral dust and get a more detailed look at its composition, helping estimate the travel of key elements such as phosphorus, calcium, and potassium, which are thought to factor into this long-distance fertilization.

“EMIT could help us to build more intricate and finely resolved dust-transport models to track the movement of those nutrients across long distances,” said Eric Slessarev, a soil researcher at Yale University in New Haven, Connecticut. “That will help us to better understand the chemistry of soils in places very far from the dust-generating regions.” 

A New Generation of Science

Aside from tracking 10 key minerals that are part of its primary mission, EMIT data is being used to identify a range of other minerals, types of vegetation, snow and ice, and even human-produced substances at or near Earth’s surface. And with vastly more measurements at their disposal, researchers will be able to find statistical relationships between surface characteristics and other features of interest.

For example, they might spot signals in EMIT data that correspond with the presence of rare-earth elements and lithium-bearing minerals, said Robert Green, a senior research scientist at JPL and EMIT’s principal investigator. This new information could be used to look for those substances in previously unknown places.

“To this point we simply haven’t known the distribution of surface minerals over huge swaths of the planet,” said Phil Brodrick, a JPL data scientist who spearheaded the creation of the mineral maps. With the EMIT data, “there will likely be a new generation of science that comes out that we don’t know about yet, and that’s a really cool thing.”

More About the Mission

EMIT was selected from the Earth Venture Instrument-4 solicitation under the Earth Science Division of NASA’s Science Mission Directorate and was developed at NASA’s Jet Propulsion Laboratory, which is managed for the agency by Caltech in Pasadena, California. The instrument’s data is available at the NASA Land Processes Distributed Active Archive Center for use by other researchers and the public.

To learn more about the mission, visit:

https://earth.jpl.nasa.gov/emit/

News Media Contacts

Andrew Wang / Jane J. Lee
Jet Propulsion Laboratory, Pasadena, Calif.
626-379-6874 / 818-354-0307
andrew.wang@jpl.nasa.gov / jane.j.lee@jpl.nasa.gov

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Naomi Hartono