NASA Goddard’s ‘Spiky’ Antenna Chamber: Signaling Success for 50 Years

NASA Goddard’s ‘Spiky’ Antenna Chamber: Signaling Success for 50 Years

3 min read

NASA Goddard’s ‘Spiky’ Antenna Chamber: Signaling Success for 50 Years

a room with blue-gray polyurethane spires covering the walls, ceiling and much of the floor. A center column supports a white antenna dish
The ElectroMagnetic Anechoic Chamber, GEMAC for short, at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, has been a critical proving ground for antenna technology for more than half-a-century.
NASA

On any given day, NASA’s networks may communicate with over 100 space missions. Whether the mission keeps the lines of communication open with orbiting astronauts or peers deep into the cosmos, those dozens of satellites all have one thing in common: each needs an antenna. Without one, NASA missions and their discoveries simply would not be possible.

To ensure those antennas are up to the challenges of spaceflight, for most that means rigorous testing on the ground in a simulated space environment. The Goddard ElectroMagnetic Anechoic Chamber (GEMAC) at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, has been an integral antenna proving ground for more than 50 years.

‘Sound Booth’ for Space Signals

Rows upon rows of cobalt-blue spires in Goddard’s antenna chamber evoke a soundproof room or isolation booth from a recording studio. In some ways the chamber is similar, but instead of dampening sound waves, this facility blocks out radio signals and eliminates radio wave reflections inside the chamber – “anechoic” means no echoes.

Much like laying down tracks on a hit album, errant ambient noise picked up by the microphone can ruin an otherwise perfect take. The same is true with radio waves when engineers want to test a spacecraft antenna. The radio environment on Earth is “noisy”: AM and FM broadcasts, television signals, cell phones, even microwave ovens, all produce radio frequencies – RF. To simulate the relatively tranquil RF environment of space, engineers need a way to isolate antennas from all these other Earth-based radio waves when they run their tests.

Roman’s high-gain antenna - a large, gray dish, about the height of a refrigerator, in a test chamber that is covered in blue spiked-shaped foam. A small circle is elevated in the middle of the antenna disk by six metal strips.
Engineers at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, have finished testing the high-gain antenna for the Nancy Grace Roman Space Telescope. The antenna, shown here in Goddard’s ElectroMagnetic Anechoic Chamber in January 2023, will provide the primary communication link between the Roman spacecraft and the ground.
NASA / Chris Gunn

That’s the job of those tightly packed columns of spikes lining the floors and walls. These polyurethane foam cones are microwave absorbers. They block outside interference and noise, and within the chamber’s “quiet zone” as engineers call it, they provide a reflection-free environment like the antenna will experience in space.

Antennas Put to the Test

With this radio-proof environment, engineers at Goddard can accurately measure how efficiently antennas broadcast and receive signals. If an antenna’s signal were to go in unexpected or undesired directions during flight, it could mean the loss of mission data, or even the entire spacecraft itself if a critical command were missed.

Trying to do antenna design and testing work without a chamber like this “would be like taking a calculator away from an accountant,” said Goddard engineer Ken Hersey.

As NASA’s missions (and their antennas) have increased in sophistication over time, Goddard engineers have upgraded the anechoic chamber to follow suit. Hersey was a lead designer on the most recent major overhaul, which in 1997 expanded the range of antenna frequencies that could be accommodated in tests. The chamber can even help calibrate scientific instruments, like radars and microwave radiation sensors.

Testing of the PACE Earth Coverage Antenna. A circular white disk with a curved strip extending from its center to the edge of the disk is mounted on a stand, covered with gray foamy spikes to absorb sound. The entire room is also covered in gray foamy spikes, including the ceiling.
The Earth Coverage Antenna for NASA’s PACE – the Plankton, Aerosol, Cloud, ocean Ecosystem missionRadio frequency testing of the PACE Earth Coverage Antenna in the ElectroMagnetic Anechoic Chamber at Goddard Space Flight Center.
NASA’s Goddard Space Flight Center / Denny Henry

Most recently, the anechoic chamber certified both the Roman Space Telescope high-gain antenna and the Earth coverage antenna for PACE – the Plankton, Aerosol, Cloud, ocean Ecosystem mission. Launching by May 2027, Roman will have a field of view at least 100 times greater than Hubble’s and help settle essential questions about dark matter and dark energy. PACE launches in January 2024 on a mission to study Earth’s air quality, ocean health, and climate change.

Once these missions take flight, their groundbreaking observations will become the latest in an ongoing legacy of discoveries made possible with help from a battery of polyurethane cones and Goddard’s anechoic antenna chamber.

By Lauren Saloio
NASA’s Goddard Space Flight Center, Greenbelt, Md.

Media Contact:
Rob Garner
NASA’s Goddard Space Flight Center, Greenbelt, Md.

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Last Updated

Nov 02, 2023

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Rob Garner

Workshop to Highlight NASA’s Support for Mobility, In-Space Servicing

Workshop to Highlight NASA’s Support for Mobility, In-Space Servicing

September's full Moon, the Harvest Moon, is photographed from the International Space Station, perfectly placed in between exterior station hardware.
September’s full Moon, the Harvest Moon, is photographed from the International Space Station, perfectly placed in between exterior station hardware.

NASA leadership, including Deputy Administrator Pam Melroy, will participate in a workshop on space mobility and in-space servicing on Tuesday, Nov. 7, at the University of Maryland in College Park.

Beginning at 8:30 a.m. EST, the Consortium for Space Mobility and ISAM Capabilities (COSMIC) workshop runs through Wednesday, Nov. 8. NASA announced the consortium in April, aiming to create a nationwide aerospace community alliance that provides global leadership in space mobility and in-space servicing, assembly, and manufacturing (ISAM) for use in Earth orbit, lunar orbit, deep space, and on planetary surfaces.

Following welcome remarks from Prasun Desai, acting associate administrator, Space Technology Mission Directorate at NASA Headquarters in Washington, Melroy will provide a keynote on NASA’s support for ISAM.

Other leaders from The White House Office of Science and Technology Policy, the U.S. Department of Defense, the defense and aerospace industry, and academia, also will participate. The conference features panel discussions and breakout workshops for COSMIC’s three caucuses ­– U.S. government, industry, and academia ­– and the Consortium’s five focus areas.

Media interested in attending the opening day, either in person or virtually, should RSVP by 12 p.m. on Monday, Nov. 6, to Parker Wishik at 708-391-7806 or parker.wishik@aero.org. NASA and COSMIC experts will be available for interview opportunities upon request. Other COSMIC plenary sessions will be recorded and later published to the COSMIC YouTube channel.

NASA funds COSMIC, creating a nationwide alliance around the capability areas, and it will support the ISAM National Strategy and National ISAM Implementation Plan, released in 2022, which define a national approach to build on existing investments and emerging capabilities to realize future opportunities enabled by ISAM. The Consortium aims to accelerate ISAM’s universal adoption and support its utilization as a routine part of space architectures and mission lifecycles.  

The Aerospace Corporation leads COSMIC as the management entity contracted by NASA’s Space Technology Mission Directorate to ensure coordination among members, caucuses, and focus areas and to execute COSMIC initiative-focused events.  

For information on the COSMIC kickoff meeting, including the full agenda, visit:

https://cosmicspace.org/2023/08/cosmics-kickoff-meeting

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Jimi Russell
Headquarters, Washington
216-704-2412
james.j.russell@nasa.gov

Parker Wishik
COSMIC
708-391-7806
parker.wishik@aero.org

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Jennifer M. Dooren

Details from Webb’s Cameras Reveal Crabby Composition

Details from Webb’s Cameras Reveal Crabby Composition

The Crab Nebula is an oval nebula with complex structure against a black background. On the nebula’s exterior, particularly at the top left and bottom left, lie curtains of glowing red and orange fluffy material. Its interior shell shows large-scale loops of mottled filaments of yellow-white and green, studded with clumps and knots. Translucent thin ribbons of smoky white lie within the remnant’s interior, brightest toward its center. The white material follows different directions throughout, including sometimes sharply curving away from certain regions within the remnant. A faint, wispy ring of white material encircles the very center of the nebula. Around and within the supernova remnant are many points of blue, red, and yellow light.
NASA, ESA, CSA, STScI, T. Temim (Princeton University)

The James Webb Space Telescope captures new details of the Crab Nebula, 6,500 light-years away, in this image released on Oct. 30, 2023. While these remains of an exploded star have been well-studied by multiple observatories, including the Hubble Space Telescope, Webb’s infrared sensitivity and resolution offer new clues into the makeup and origins of this scene.

Thanks to Webb’s Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI), scientists were able to determine the composition of the material ejected from the explosion. The supernova remnant is comprised of several different components, including doubly ionized sulfur (represented in red-orange), ionized iron (blue), dust (yellow-white and green), and synchrotron emission (white). In this image, colors were assigned to different filters from Webb’s NIRCam and MIRI: blue (F162M), light blue (F480M), cyan (F560W), green (F1130W), orange (F1800W), and red (F2100W).

Take a video tour of this image.

Image Credit: NASA, ESA, CSA, STScI, T. Temim (Princeton University)

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Monika Luabeya

Scorching, Seven-Planet System Revealed by New Kepler Exoplanet List

Scorching, Seven-Planet System Revealed by New Kepler Exoplanet List

Artist’s concept showing two of the seven planets discovered orbiting a Sun-like star. The system, called Kepler-385, was identified using data from NASA’s Kepler mission.
NASA/Daniel Rutter

A system of seven sweltering planets has been revealed by continued study of data from NASA’s retired Kepler space telescope: Each one is bathed in more radiant heat from their host star per area than any planet in our solar system. Also unlike any of our immediate neighbors, all seven planets in this system, named Kepler-385, are larger than Earth but smaller than Neptune. It is one of only a few planetary systems known to contain more than six verified planets or planet candidates. The Kepler-385 system is among the highlights of a new Kepler catalog that contains almost 4,400 planet candidates, including more than 700 multi-planet systems.

“We’ve assembled the most accurate list of Kepler planet candidates and their properties to date,” said Jack Lissauer, a research scientist at NASA’s Ames Research Center in California’s Silicon Valley and lead author on the paper presenting the new catalog. “NASA’s Kepler mission has discovered the majority of known exoplanets, and this new catalog will enable astronomers to learn more about their characteristics.”

At the center of the Kepler-385 system is a Sun-like star about 10% larger and 5% hotter than the Sun. The two inner planets, both slightly larger than Earth, are probably rocky and may have thin atmospheres. The other five planets are larger – each with a radius about twice the size of Earth’s – and expected to be enshrouded in thick atmospheres.

Artist’s concept of Kepler-385, the seven-planet system revealed in a new catalog of planet candidates discovered by NASA’s Kepler space telescope.
NASA/Daniel Rutter

The ability to describe the properties of the Kepler-385 system in such detail is testament to the quality of this latest catalog of exoplanets. While the Kepler mission’s final catalogs focused on producing lists optimized to measure how common planets are around other stars, this study focuses on producing a comprehensive list that provides accurate information about each of the systems, making discoveries like Kepler-385 possible.

The new catalog uses improved measurements of stellar properties and calculates more accurately the path of each transiting planet across its host star. This combination illustrates that when a star hosts several transiting planets, they typically have more circular orbits than when a star hosts only one or two.

Kepler’s primary observations ceased in 2013 and were followed by the telescope’s extended mission, called K2, which continued until 2018. The data Kepler collected continues to reveal new discoveries about our galaxy. After the mission already showed us there are more planets than stars, this new study paints a more detailed picture of what each of those planets and their home systems look like, giving us a better view of the many worlds beyond our solar system.

The research article, “Updated Catalog of Kepler Planet Candidates: Focus on Accuracy and Orbital Periods” is forthcoming in The Journal of Planetary Science.

Learn more:

Listen to a sonification of the orbit data of the seven planets in the Kepler-385 system: https://www.youtube.com/watch?v=2BCiOTJjcQQ

For news media:

Members of the news media interested in covering this topic should reach out to the NASA Ames newsroom.

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Frank Tavares

Una nueva aplicación de la NASA ayuda a avistar la estación espacial

Una nueva aplicación de la NASA ayuda a avistar la estación espacial

4 min read

Una nueva aplicación de la NASA ayuda a avistar la estación espacial

NASA

Read this release in English here.

La NASA está haciendo más fácil para el público avistar Estación Espacial Internacional, el hogar de la humanidad en el espacio, mientras esta sobrevuela la Tierra, así como ampliando el acceso a noticias y recursos sobre este laboratorio en microgravedad con una nueva aplicación para teléfonos móviles, o celulares, llamada Spot the Station (Avista la estación).

La aplicación para celulares ya está disponible para descargar en iOS y Android.

La aplicación se basa en el sitio web Spot the Station de la agencia y proporciona información y capacidades adicionales para mejorar la experiencia del público en el avistamiento de la estación espacial. Una interfaz de realidad aumentada facilita a los usuarios ubicar la estación y ofrece opciones para capturar y compartir imágenes y vídeos de sus avistamientos en tiempo real. Con el poder de la realidad aumentada, la brújula incorporada en la aplicación le mostrará al espectador dónde se encuentra la estación espacial, incluso si se está al otro lado del planeta. Los usuarios también pueden registrarse para recibir notificaciones de las próximas oportunidades de avistamiento en sus teléfonos móviles en función de su ubicación exacta.

“Incluso después de 23 años de presencia humana continua a bordo de la Estación Espacial Internacional, es increíblemente emocionante ver la estación cuando miras hacia arriba en el momento justo”, dijo Robyn Gatens, directora de la Estación Espacial Internacional en la sede de la NASA en Washington. “Este laboratorio orbital, que continúa proporcionando tantos beneficios únicos y tangibles para la humanidad, realmente no está tan lejos de nuestro alcance”.

La estación espacial es visible porque refleja la luz del Sol, que es la misma razón por la que podemos ver la Luna. Pero a diferencia de la Luna, la estación espacial no es lo suficientemente brillante como para poder observarla durante el día. Solo es posible verla cuando amanece o anochece en la localidad del espectador. Por lo tanto, la oportunidad de avistamiento varía de una vez al mes a varias a la semana, ya que es necesario que haya oscuridad en la localidad del espectador, y la estación espacial tiene que pasar por encima de su cabeza. Con la aplicación Spot the Station para móviles, los usuarios sabrán cuándo la estación está sobrevolando su área y cómo localizarla.

La aplicación fue desarrollada por el Programa de la Estación Espacial Internacional en la Dirección de Misiones de Operaciones Espaciales de la NASA y el Centro de Excelencia para la Innovación Colaborativa, el cual es parte del programa de Premios, Desafíos y Crowdsourcing de la Dirección de Misiones de Tecnología Espacial de la agencia. El código de la aplicación está abierto para que cualquiera pueda acceder a ella, modificarla y utilizarla en sus propios proyectos, así como ofrecer comentarios opcionales para los programadores. La NASA continuará actualizando y mejorando la aplicación para móviles de forma continua a medida que reciba los comentarios de los usuarios.

El lanzamiento de esta aplicación también se produce justo antes del 25.o aniversario del inicio de operaciones de la Estación Espacial Internacional, el cual marca la unión de los módulos Zarya y Unity, los primeros elementos de lo que hoy es un enorme complejo orbital, el 6 de diciembre de 1998. La estación espacial permite el avance del conocimiento científico en las ciencias de la Tierra, del espacio, físicas y biológicas para el beneficio de los habitantes de nuestro planeta natal. Además, la estación espacial sirve como el laboratorio líder mundial para las investigaciones de vanguardia y el desarrollo de la tecnología que respalda la exploración humana y robótica de destinos más allá de la órbita baja de la Tierra, incluyendo la Luna y Marte.

Aprende más sobre la estación espacial, sus investigaciones y su tripulación en el sitio web (en inglés):

https://www.nasa.gov/station

-end-

News Media Contacts:

Julian Coltre / María José Viñas
Sede, Washington
202-358-1100 / 240-458-0248
julian.n.coltre@nasa.gov / maria-jose.vinasgarcia@nasa.gov

Leah Cheshier / Kenna Pell
Johnson Space Center, Houston
281-483-5111
leah.d.cheshier@nasa.gov / kenna.m.pell@nasa.gov

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Claire A. O’Shea