NASA’s Next-Gen Exoplanet-Imaging Technology Advances Search for Extraterrestrial Life


Nancy Grace Roman Space Telescope Illustration

The Roman Space Telescope’s Coronagraph has cleared key tests, setting the stage for groundbreaking observations of exoplanets and aiding in the quest to find life beyond Earth. Credit: NASA

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NASA
Established in 1958, the National Aeronautics and Space Administration (NASA) is an independent agency of the United States Federal Government that succeeded the National Advisory Committee for Aeronautics (NACA). It is responsible for the civilian space program, as well as aeronautics and aerospace research. Its vision is "To discover and expand knowledge for the benefit of humanity." Its core values are "safety, integrity, teamwork, excellence, and inclusion." NASA conducts research, develops technology and launches missions to explore and study Earth, the solar system, and the universe beyond. It also works to advance the state of knowledge in a wide range of scientific fields, including Earth and space science, planetary science, astrophysics, and heliophysics, and it collaborates with private companies and international partners to achieve its goals.

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Roman Space Telescope
The Nancy Grace Roman Space Telescope (previously known as the Wide Field Infrared Survey Telescope, or WFIRST) is a space telescope that is being developed by NASA. It is named in honor of Nancy Grace Roman, a pioneering astrophysicist who was instrumental in the development of the Hubble Space Telescope. The Roman Space Telescope is designed to study a wide range of cosmic phenomena, including the expansion of the universe, the formation and evolution of galaxies, and the search for exoplanets. It will be equipped with a wide-field camera that will allow it to survey a large portion of the sky and study objects in the infrared part of the electromagnetic spectrum. The Roman Space Telescope is scheduled to be launched in the mid-2020s.

” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]” tabindex=”0″ role=”link”>Roman Space Telescope’s Coronagraph Instrument, designed to observe distant exoplanets by blocking stellar light, has passed essential tests, marking a significant advancement in space observation technology and the search for extraterrestrial life.

A cutting-edge tool to view planets outside our solar system has passed two key tests ahead of its launch as part of the agency’s Roman Space Telescope by 2027.

The Coronagraph Instrument on NASA’s Nancy Grace Roman Space Telescope will demonstrate new technologies that could vastly increase the number of planets outside our solar system (exoplanets) that scientists can directly observe. Designed and built at the agency’s Jet Propulsion Laboratory in Southern California, it recently passed a series of critical tests ahead of launch. That includes tests to ensure the instrument’s electrical components don’t interfere with those on the rest of the observatory and vice versa.

Key Tests and Coronagraph Technology

“This is such an important and nerve-wracking stage of building a spacecraft instrument, testing whether or not everything works as intended,” said Feng Zhao, deputy project manager for the Roman Coronagraph at <span class="glossaryLink" aria-describedby="tt" data-cmtooltip="

JPL
The Jet Propulsion Laboratory (JPL) is a federally funded research and development center that was established in 1936. It is owned by NASA and managed by the California Institute of Technology (Caltech). The laboratory's primary function is the construction and operation of planetary robotic spacecraft, though it also conducts Earth-orbit and astronomy missions. It is also responsible for operating NASA's Deep Space Network. JPL implements programs in planetary exploration, Earth science, space-based astronomy and technology development, while applying its capabilities to technical and scientific problems of national significance.

” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]” tabindex=”0″ role=”link”>JPL. “But we have an amazing team who built this thing, and it passed the electrical components tests with flying colors.”

A coronagraph blocks light from a bright cosmic object, like a star, so that scientists can observe a nearby object that would otherwise be hidden by the glare. (Think of a car’s sun visor.) The light reflected or emitted by a planet carries information about the chemicals in the planet’s atmosphere and other potential signs of habitability, so coronagraphs will likely be a critical tool in the search for life beyond our solar system.

Vanessa Bailey Behind Nancy Grace Roman Coronagraph

JPL scientist Vanessa Bailey stands behind the Nancy Grace Roman Coronagraph, which has been undergoing testing at JPL. About the size of a baby grand piano, the Coronagraph is designed to block starlight and allow scientists to see the faint light from planets outside our solar system. Credit: NASA/JPL-Caltech

Advancements in Exoplanet Observation

But if scientists were trying to obtain images of an Earth-like planet in another solar system (same size, same distance from a star similar to our Sun), they wouldn’t be able to see the planet in the star’s glare, even with the best coronagraphs and most powerful telescopes operating today.

The Roman Coronagraph aims to change that paradigm. The innovations that have gone into the instrument should make it possible to see planets similar to <span class="glossaryLink" aria-describedby="tt" data-cmtooltip="

Jupiter
Jupiter is the largest planet in the solar system and the fifth planet from the sun. It is a gas giant with a mass greater then all of the other planets combined. Its name comes from the Roman god Jupiter.

” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]” tabindex=”0″ role=”link”>Jupiter in size and distance from their star. The Coronagraph team expects these advances will help enable the leap to viewing more Earth-like planets with future observatories.

As a technology demonstration, the Roman Coronagraph’s primary goal is to test technologies that have not been flown in space before. Specifically, it will test sophisticated light-blocking capabilities that are at least 10 times better than what’s currently available. Scientists expect to push its performance even further to observe challenging targets that could yield novel scientific discoveries.

Roman Coronagraph Radio Test

The Roman Coronagraph was peppered with radio waves to test its response to stray electrical signals. The test was performed inside a chamber lined with foam padding that absorbs the radio waves to prevent them from bouncing off the walls. Credit: NASA/JPL-Caltech

Overcoming Challenges in Space Observation

Even with the Coronagraph blocking a star’s light, a planet will still be exceptionally faint, and it might take a full month of observations to get a good picture of the distant world. To make these observations, the instrument’s camera detects individual photons, or single particles of light, making it far more sensitive than previous coronagraphs.

That’s one reason the recent tests were crucial: The electrical currents that send power to the spacecraft’s components can produce faint electrical signals, mimicking light in the Coronagraph’s sensitive cameras – an effect known as electromagnetic interference. Meanwhile, signals from the Coronagraph could similarly disrupt Roman’s other instruments.

The mission needs to ensure neither will happen when the telescope is operating in an isolated, electromagnetically quiet environment 1 million miles (about 1.5 million kilometers) from Earth. So a team of engineers put the fully assembled instrument in a special isolated, electromagnetically quiet chamber at JPL and turned it on to full power.

They measured the instrument’s electromagnetic output to make sure it fell below the level required to operate aboard Roman. The team used injection clamps, transformers, and antennas to produce electrical disturbances and radio waves similar to what the rest of the telescope will generate. Then they measured the instrument’s performance, looking for excessive noise in the camera images and other unwanted responses from the optical mechanisms.

“The electric fields we generate with the antennas are about the same strength as what’s generated by a computer screen,” said Clement Gaidon, the Roman Coronagraph electrical systems engineer at JPL. “That’s a pretty benign level, all things considered, but we have very sensitive hardware onboard. Overall, the instrument did a fantastic job navigating across the electromagnetic waves. And props to the team for wrapping this test campaign in record time!”

The Broad Mission of the Roman Space Telescope

The lessons learned from the Coronagraph technology demonstration will be separate from the Roman Space Telescope’s primary mission, which includes multiple science objectives. The mission’s principal tool, the Wide Field Instrument, is designed to generate some of the largest images of the universe ever taken from space. These images will enable Roman to conduct groundbreaking surveys of cosmic objects such as stars, planets, and galaxies, and study the large-scale distribution of matter in the universe.

For example, by taking repeated images of the center of the <span class="glossaryLink" aria-describedby="tt" data-cmtooltip="

Milky Way
The Milky Way is the galaxy that contains our Solar System and is part of the Local Group of galaxies. It is a barred spiral galaxy that contains an estimated 100-400 billion stars and has a diameter between 150,000 and 200,000 light-years. The name "Milky Way" comes from the appearance of the galaxy from Earth as a faint band of light that stretches across the night sky, resembling spilled milk.

” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]” tabindex=”0″ role=”link”>Milky Way – like a multiyear time-lapse movie – the Wide Field Instrument will discover tens of thousands of new exoplanets. (This planet survey will be separate from the observations made by the Coronagraph).

Roman will also make 3D maps of the cosmos to explore how galaxies have formed and why the universe’s expansion is speeding up, measuring the effects of what astronomers call “dark matter” and “dark energy.” With these wide-ranging capabilities, Roman will help answer questions about big and small features of our universe.

More About the Mission

The Nancy Grace Roman Space Telescope is managed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, with participation by JPL and Caltech/IPAC in Southern California, the Space Telescope Science Institute in Baltimore, and a science team comprising scientists from various research institutions. The primary industrial partners are Ball Aerospace & Technologies Corp. in Boulder, Colorado; L3Harris Technologies in Melbourne, Florida; and Teledyne Scientific & Imaging in Thousand Oaks, California.

The Roman Coronagraph Instrument was designed and is being built at JPL, which manages the instrument for NASA. Contributions were made by ESA (the <span class="glossaryLink" aria-describedby="tt" data-cmtooltip="

European Space Agency
The European Space Agency (ESA) is an intergovernmental organization dedicated to the exploration and study of space. ESA was established in 1975 and has 22 member states, with its headquarters located in Paris, France. ESA is responsible for the development and coordination of Europe's space activities, including the design, construction, and launch of spacecraft and satellites for scientific research and Earth observation. Some of ESA's flagship missions have included the Rosetta mission to study a comet, the Gaia mission to create a 3D map of the Milky Way, and the ExoMars mission to search for evidence of past or present life on Mars.

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JAXA
Formed in 2003, the Japan Aerospace Exploration Agency (JAXA) was born through the merger of three institutions, namely the Institute of Space and Astronautical Science (ISAS), the National Aerospace Laboratory of Japan (NAL) and the National Space Development Agency of Japan (NASDA). JAXA performs various activities related to aerospace, from basic research in the aerospace field to development and utilization and is responsible for research, technology development, and launch of satellites into orbit, and is involved in advanced missions such as asteroid exploration and possible human exploration of the Moon.

” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]” tabindex=”0″ role=”link”>JAXA (the Japanese Aerospace Exploration Agency), the French space agency CNES (Centre National d’Études Spatiales), and the Max Planck Institute for Astronomy in Germany. Caltech, in Pasadena, California, manages JPL for NASA. The Roman Science Support Center at Caltech/IPAC partners with JPL on data management for the Coronagraph and generating the instrument’s commands.


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