Dr. Nancy Grace Roman visits James Webb Space Telescope (JWST) and the Hubble Project Team.

Dr. Nancy Grace Roman visits James Webb Space Telescope (JWST) and the Hubble Project Team.

Dr. Nancy Grace Roman visits James Webb Space Telescope (JWST) and the Hubble Project Team. Dr. John Mather.

Dr. Nancy Grace Roman visits James Webb Space Telescope (JWST) and the Hubble Project Team.

Dr. Nancy Grace Roman visits James Webb Space Telescope (JWST) and the Hubble Project Team. Center Director Chris Scolese

Dr. Nancy Grace Roman visits James Webb Space Telescope (JWST) and the Hubble Project Team. Center Director Chris Scolese

The Roman Space Telescope's Spacecraft Bus and Integrated Payload Assembly is crane lifted inside the cleanroom at Goddard Space Flight Center, Greenbelt Md., June 12, 2025. This photo has been approved for public release. NASA/Mike Guinto

In a clean room at NASA's Jet Propulsion Laboratory in Southern California in October 2023, scientist Vanessa Bailey stands behind the Roman Coronagraph, which has been undergoing testing at the lab. Designed to block starlight and allow scientists to see the faint light from planets outside our solar system, the Coronagraph is a technology demonstration that will be part of NASA's Nancy Grace Roman Space Telescope. https://photojournal.jpl.nasa.gov/catalog/PIA26272

Engineers at NASA's Jet Propulsion Laboratory – from left, Brandon Creager, Juan Gloria, Joshua Nachtigal, and Sonny Gutierrez – are shown assembling the electronics palette for the Coronagraph Instrument on NASA's Roman Space Telescope in December 2022. One of two main sections of the instrument, this layer houses the instrument electronics that receive instructions from the Roman spacecraft and send back the Coronagraph Instrument's scientific data. The electronics also control the mechanical components on the optical bench and the instrument heaters. https://photojournal.jpl.nasa.gov/catalog/PIA25435

This image shows a series of color filters on the Color Filter Assembly for the Coronagraph Instrument on NASA's Nancy Grace Roman Space Telescope. Each filter blocks all but a specific color, or wavelength, of light. Many of the filters appear dark in this photo because they block all visible light – the range of wavelengths that are visible to the human eye – but are transparent to infrared light, which encompasses a range of wavelengths slightly longer than visible light. Most of the filters will be used by the instrument for calibration purposes, but there are scientific uses for some of the filters as well. The presence or absence of different wavelengths can reveal properties of exoplanets (planets around other stars) including their chemical composition and the presence of clouds high or low in their atmospheres. For example, cold gas giant planets with high clouds will appear redder, like Jupiter, compared to those without high clouds, like Neptune. https://photojournal.jpl.nasa.gov/catalog/PIA25436

The Roman Coronagraph Instrument on NASA's upcoming Nancy Grace Roman Space Telescope will test new tools that block starlight, revealing planets hidden by the glare of their parent stars. The technology demonstration instrument is shown here on May 17, 2024, at NASA's Jet Propulsion Laboratory in Southern California, where it was designed and built. Mission team members are using a crane to lift the top portion of the shipping container that the instrument was stored in for its journey to the agency's Goddard Space Flight Center in Greenbelt, Maryland, where it will join the rest of the space observatory in preparation for launch by May 2027. https://photojournal.jpl.nasa.gov/catalog/PIA26277

The Roman Coronagraph Instrument on NASA's upcoming Nancy Grace Roman Space Telescope will test new tools that block starlight, revealing planets hidden by the glare of their parent stars. The technology demonstration instrument is shown here – inside a shipping container – on May 17, 2024, at NASA's Jet Propulsion Laboratory in Southern California, where it was designed and built. Mission team members said farewell to the instrument by signing their names to a flag (featuring the mission logo) on the outside of the container, which carried the instrument from JPL to NASA's Goddard Space Flight Center in Greenbelt, Maryland. There, it will join the rest of the space observatory in preparation for launch by May 2027. https://photojournal.jpl.nasa.gov/catalog/PIA26278

The Roman Coronagraph Instrument, a technology demonstration that will be part of NASA's Nancy Grace Roman Space Telescope, is seen amid testing at the agency's Jet Propulsion Laboratory in Southern California in December 2023. During this test in a special isolated, electromagnetically quiet chamber, the instrument was peppered with radio waves to test its response to ensure that the electrical components on the instrument don't interfere with those on the rest of the observatory, and vice versa. The test was performed inside a chamber lined with foam padding that absorbs the radio waves to prevent them from bouncing off the walls. https://photojournal.jpl.nasa.gov/catalog/PIA26273

The Roman Coronagraph Instrument on NASA's upcoming Nancy Grace Roman Space Telescope will test new tools that block starlight, revealing planets hidden by the glare of their parent stars. This graphic shows a test of what engineers call "digging the dark hole." The image shows three computer readouts of real data from the coronagraph's camera. Engineers used lasers and special optics to replicate the light from a star as it would look when observed by the Roman telescope. The image at left shows the amount of starlight that leaks into the coronagraph's field of view when only fixed components called masks are used to block the star at the center of the circle. Using moveable components such as deformable mirrors, the coronagraph can remove more and more of this starlight. The middle and right images show the progression of this process, where red indicates less starlight, and black indicates most or all starlight has been removed. The deformable mirrors are each only 2 inches (5 centimeters) in diameter and backed by more than 2,000 tiny pistons that move up and down. The pistons work together to change the shape of the mirrors to compensate for the unwanted stray light that spills around the edges of the masks. Though they are too small to affect Roman's other highly precise measurements, the imperfections can send stray starlight into the dark hole. In space, this technique will enable astronomers to observe light directly from planets around other stars, or exoplanets. Once demonstrated on Roman, similar technologies on a future mission could enable astronomers to use that light to identify chemicals in an exoplanet's atmosphere, potentially indicating the presence of life. https://photojournal.jpl.nasa.gov/catalog/PIA26279

Engineer Jordan Rupp is shown at NASA's Jet Propulsion Laboratory in September 2022 with the optical bench for the Coronagraph Instrument on NASA's Nancy Grace Roman Space Telescope. Light from the telescope is directed to the optical bench and passes through series of lenses, filters, and other components that ultimately suppress light from a star while allowing the light from orbiting planets to pass through. Mirrors redirect the light and keep it contained within the optical bench. In this image, the bench is partly assembled at the start of the integration and testing period for the instrument. The large black circles are surrogate components that are standing in for the actual instrument hardware. https://photojournal.jpl.nasa.gov/catalog/PIA25439

The focal plane mask for the Coronagraph Instrument on NASA's Nancy Grace Roman Space Telescope, shown here, is one of the components used to suppress starlight and reveal planets orbiting a star. Each circular section contains multiple "masks" – carefully engineered, opaque obstructions designed to block starlight. Some masks are about the width of a human hair. https://photojournal.jpl.nasa.gov/catalog/PIA25438

An engineer at NASA's Jet Propulsion Laboratory is shown here with the fast steering mirror, a component of the Coronagraph Instrument on NASA's Nancy Grace Roman Space Telescope. The mirror can make small movements that correct for slight wobbling of the observatory. The incoming image needs to be perfectly sharp in order for the instrument to suppress light from a star while allowing the light from planets orbiting it to pass through. Although the technologies differ, it's analogous to image stabilization in digital cameras, in which the camera lens moves to counteract the shake of your hands and keep the image sharp. https://photojournal.jpl.nasa.gov/catalog/PIA25437

Roman Space Telescope team members inspect the primary mirror in the dark using flashlights and UV lights to help them see any contamination, inside the cleanroom at Goddard Space Flight Center, Greenbelt Md., July 2, 2025. The green glow of the room is due to a long exposure time, the green comes from a light on the left wall which indicates optimal airflow through the room. This photo has been approved for public release. NASA/Mike Guinto

Quality Assurance engineer Lucinda Taylor unreels a power cord across the cleanroom floor at Goddard Space Flight Center, Greenbelt Md., April 21, 2025. This photo has been reviewed by export control and is approved for public release. NASA/Mike Guinto

Dr. Nancy Grace Roman visits James Webb Space Telescope (JWST) and the Hubble Project Team. Dr. John Mather.

Dr. Julie McEnery, senior project scientist on NASA’s Nancy Grace Roman Space Telescope, right, briefs Vice President Kamala Harris, President Yoon Suk Yeol of the Republic of Korea and NASA Deputy Administrator Pam Melroy on the Nancy Grace Roman Space Telescope in the observation area of the high bay clean room, Tuesday, April 25, 2023, at NASA’s Goddard Space Flight Center in Greenbelt, Md. Photo Credit: (NASA/Joel Kowsky)

Vice President Kamala Harris, right, and NASA Deputy Administrator Pam Melroy are see during a briefing on the Nancy Grace Roman Space Telescope by Dr. Julie McEnery, senior project scientist on NASA’s Nancy Grace Roman Space Telescope, in the observation area of the high bay clean room, Tuesday, April 25, 2023, at NASA’s Goddard Space Flight Center in Greenbelt, Md. Photo Credit: (NASA/Joel Kowsky)

Vice President Kamala Harris, right, NASA Deputy Administrator Pam Melroy, and President Yoon Suk Yeol of the Republic of Korea are seen during a briefing by Dr. Julie McEnery, senior project scientist on NASA’s Nancy Grace Roman Space Telescope, on the Nancy Grace Roman Space Telescope in the observation area of the high bay clean room, Tuesday, April 25, 2023, at NASA’s Goddard Space Flight Center in Greenbelt, Md. Photo Credit: (NASA/Joel Kowsky)

Dr. Julie McEnery, senior project scientist on NASA’s Nancy Grace Roman Space Telescope, right, briefs Vice President Kamala Harris, President Yoon Suk Yeol of the Republic of Korea and NASA Deputy Administrator Pam Melroy on the Nancy Grace Roman Space Telescope in the observation area of the high bay clean room, Tuesday, April 25, 2023, at NASA’s Goddard Space Flight Center in Greenbelt, Md. Photo Credit: (NASA/Joel Kowsky)

Dr. Julie McEnery, senior project scientist on NASA’s Nancy Grace Roman Space Telescope, left, briefs Vice President Kamala Harris, President Yoon Suk Yeol of the Republic of Korea and NASA Deputy Administrator Pam Melroy on the Nancy Grace Roman Space Telescope in the observation area of the high bay clean room, Tuesday, April 25, 2023, at NASA’s Goddard Space Flight Center in Greenbelt, Md. Photo Credit: (NASA/Joel Kowsky)

Employees viewed James Webb Space Telescope in B29 on March 31, 2017 prior to final phase of integration and testing before 2018 launch. Project personnel were on hand for Q&A and LIVE Facebook event. Pictured here is Nancy Grace Roman “Mother of Hubble” viewing JWST.

In this illustration, NASA's SPHEREx mission is highlighted among a line of other NASA space telescopes. The mission will survey the entire sky using spectroscopy, detecting hundreds of millions of stars and galaxies and generating a valuable data set that will complement the work of other NASA observatories such as those depicted here. Shown from left to right (and not to scale) are: Hubble Space Telescope, launched in April 1990 Spitzer Space Telescope, launch in August 2003 WISE (Wide-Field Infrared Survey Explorer), launched in December 2009 James Webb Space Telescope, launched in December 2021 SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer), targeted for launch in February 2025 Nancy Grace Roman Space Telescope, targeted for launch by May 2027 The SPHEREx observatory will image the entire sky in 102 colors (each an individual wavelength of light) to help scientists answer big-picture questions about the origins of our universe, galaxies, and key ingredients for life in our galaxy, such as water. https://photojournal.jpl.nasa.gov/catalog/PIA26535

Like a roman candle, Space Shuttle Discovery roars into the clear night sky trailing brilliant exhaust from the solid rocket boosters (center) and blue mach diamonds from the main engine nozzles. Liftoff occurred at 7:50 p.m. EST from Launch Pad 39B. On board are Commander Curtis L. Brown Jr., Pilot Scott J. Kelly and Mission Specialists Steven L. Smith, C. Michael Foale (Ph.D.), John M. Grunsfeld (Ph.D.), Claude Nicollier of Switzerland and Jean-François Clervoy of France. Nicollier and Clervoy are with the European Space Agency. STS-103 is a Hubble Servicing Mission, with three planned space walks designed to install new equipment and replace old. The primary objective is to replace the gyroscopes that make up the three Rate Sensor Units. Extravehicular activities include installing a new computer, changing out one of the Fine Guidance Sensors, replacing a tape recorder with a new solid state recorder, and installing a voltage/temperature improvement kit, and begin repairing the insulation on the telescope's outer surface. After the 7-day, 21-hour mission, Discovery is expected to land at KSC Monday, Dec. 27, at about 5:24 p.m. EST. This is the 27th flight of Discovery and the 96th mission in the Space Shuttle Program. It is the third launch at Kennedy Space Center in 1999

To commemorate the upcoming 10th anniversary of the DSCOVR (Deep Space Climate Observatory) mission, NASA’s Goddard Space Flight Center in Greenbelt, Md., hosted environmentalist and former Vice President Al Gore, shown here addressing a crowd in the Building 3 Harry J. Goett Auditorium, on Oct. 16, 2024. “The image of our Earth from space is the single most compelling iconic image that any of us have ever seen,” Gore said at a panel discussion for employees. “Now we have, thanks to DSCOVR, 50,000 ‘Blue Marble’ photographs … To date there are more than 100 peer-reviewed scientific publications that are based on the unique science gathered at the L1 point by DSCOVR. For all of the scientists who are here and those on the teams that are represented here, I want to say congratulations and thank you.” Following Gore’s talk on climate monitoring, Goddard scientists participated in a panel discussion, “Remote Sensing and the Future of Earth Observations,” which explored the latest advancements in technology that allow for the monitoring of the atmosphere from space and showcased how Goddard’s research drives the future of Earth science. Gore’s visit also entailed a meeting with the DSCOVR science team, a view into the clean room where Goddard is assembling the Roman Space Telescope, and a stop at the control center for PACE: NASA’s Plankton, Aerosol, Cloud, ocean Ecosystem mission. Launched Feb. 11, 2015, DSCOVR is a space weather station that monitors changes in the solar wind, providing space weather alerts and forecasts for geomagnetic storms that could disrupt power grids, satellites, telecommunications, aviation and GPS. DSCOVR is a joint mission among NASA, the National Oceanic and Atmospheric Administration (NOAA), and the U.S. Air Force. The project originally was called Triana, a mission conceived of by Gore in 1998 during his vice presidency.

NASA image release July 3, 2012 Caption: Resembling a Fourth of July skyrocket, Herbig-Haro 110 is a geyser of hot gas from a newborn star that splashes up against and ricochets off the dense core of a cloud of molecular hydrogen. Although the plumes of gas look like whiffs of smoke, they are actually billions of times less dense than the smoke from a July 4 firework. This Hubble Space Telescope photo shows the integrated light from plumes, which are light-years across. -- Herbig-Haro (HH) objects come in a wide array of shapes, but the basic configuration stays the same. Twin jets of heated gas, ejected in opposite directions away from a forming star, stream through interstellar space. Astronomers suspect that these outflows are fueled by gas accreting onto a young star surrounded by a disk of dust and gas. The disk is the &quot;fuel tank,&quot; the star is the gravitational engine, and the jets are the exhaust. When these energetic jets slam into colder gas, the collision plays out like a traffic jam on the interstate. Gas within the shock front slows to a crawl, but more gas continues to pile up as the jet keeps slamming into the shock from behind. Temperatures climb sharply, and this curving, flared region starts to glow. These &quot;bow shocks&quot; are so named because they resemble the waves that form at the front of a boat. In the case of the single HH 110 jet, astronomers observe a spectacular and unusual permutation on this basic model. Careful study has repeatedly failed to find the source star driving HH 110, and there may be good reason for this: perhaps the HH 110 outflow is itself generated by another jet. Astronomers now believe that the nearby HH 270 jet grazes an immovable obstacle - a much denser, colder cloud core - and gets diverted off at about a 60-degree angle. The jet goes dark and then reemerges, having reinvented itself as HH 110. The jet shows that these energetic flows are like the erratic outbursts from a Roman candle. As fast-moving blobs of gas catch up and collide with slower blobs, new shocks arise along the jet's interior. The light emitted from excited gas in these hot blue ridges marks the boundaries of these interior collisions. By measuring the current velocity and positions of different blobs and hot ridges along the chain within the jet, astronomers can effectively &quot;rewind&quot; the outflow, extrapolating the blobs back to the moment when they were emitted. This technique can be used to gain insight into the source star's history of mass accretion. This image is a composite of data taken with Hubble's Advanced Camera for Surveys in 2004 and 2005 and the Wide Field Camera 3 in April 2011. Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA) <b><a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a></b> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. <b>Follow us on <a href="http://twitter.com/NASA_GoddardPix" rel="nofollow">Twitter</a></b> <b>Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b> <b>Find us on <a href="http://instagrid.me/nasagoddard/?vm=grid" rel="nofollow">Instagram</a></b>

The sharp eye of NASA's Hubble Space Telescope has captured the tiny moon Phobos during its orbital trek around Mars. Because the moon is so small, it appears star-like in the Hubble pictures. Over the course of 22 minutes, Hubble took 13 separate exposures, allowing astronomers to create a time-lapse video showing the diminutive moon's orbital path. The Hubble observations were intended to photograph Mars, and the moon's cameo appearance was a bonus. A football-shaped object just 16.5 miles by 13.5 miles by 11 miles, Phobos is one of the smallest moons in the solar system. It is so tiny that it would fit comfortably inside the Washington, D.C. Beltway. The little moon completes an orbit in just 7 hours and 39 minutes, which is faster than Mars rotates. Rising in the Martian west, it runs three laps around the Red Planet in the course of one Martian day, which is about 24 hours and 40 minutes. It is the only natural satellite in the solar system that circles its planet in a time shorter than the parent planet's day. About two weeks after the Apollo 11 manned lunar landing on July 20, 1969, NASA's Mariner 7 flew by the Red Planet and took the first crude close-up snapshot of Phobos. On July 20, 1976 NASA's Viking 1 lander touched down on the Martian surface. A year later, its parent craft, the Viking 1 orbiter, took the first detailed photograph of Phobos, revealing a gaping crater from an impact that nearly shattered the moon. Phobos was discovered by Asaph Hall on August 17, 1877 at the U.S. Naval Observatory in Washington, D.C., six days after he found the smaller, outer moon, named Deimos. Hall was deliberately searching for Martian moons. Both moons are named after the sons of Ares, the Greek god of war, who was known as Mars in Roman mythology. Phobos (panic or fear) and Deimos (terror or dread) accompanied their father into battle. Close-up photos from Mars-orbiting spacecraft reveal that Phobos is apparently being torn apart by the gravitational pull of Mars. The moon is marred by long, shallow grooves that are probably caused by tidal interactions with its parent planet. Phobos draws nearer to Mars by about 6.5 feet every hundred years. Scientists predict that within 30 to 50 million years, it either will crash into the Red Planet or be torn to pieces and scattered as a ring around Mars. Orbiting 3,700 miles above the Martian surface, Phobos is closer to its parent planet than any other moon in the solar system. Despite its proximity, observers on Mars would see Phobos at just one-third the width of the full moon as seen from Earth. Conversely, someone standing on Phobos would see Mars dominating the horizon, enveloping a quarter of the sky. From the surface of Mars, Phobos can be seen eclipsing the sun. However, it is so tiny that it doesn't completely cover our host star. Transits of Phobos across the sun have been photographed by several Mars-faring spacecraft. The origin of Phobos and Deimos is still being debated. Scientists concluded that the two moons were made of the same material as asteroids. This composition and their irregular shapes led some astrophysicists to theorize that the Martian moons came from the asteroid belt. However, because of their stable, nearly circular orbits, other scientists doubt that the moons were born as asteroids. Such orbits are rare for captured objects, which tend to move erratically. An atmosphere could have slowed down Phobos and Deimos and settled them into their current orbits, but the Martian atmosphere is too thin to have circularized the orbits. Also, the moons are not as dense as members of the asteroid belt. Phobos may be a pile of rubble that is held together by a thin crust. It may have formed as dust and rocks encircling Mars were drawn together by gravity. Or, it may have experienced a more violent birth, where a large body smashing into Mars flung pieces skyward, and those pieces were brought together by gravity. Perhaps an existing moon was destroyed, reduced to the rubble that would become Phobos. Hubble took the images of Phobos orbiting the Red Planet on May 12, 2016, when Mars was 50 million miles from Earth. This was just a few days before the planet passed closer to Earth in its orbit than it had in the past 11 years. A time-lapse video captures a portion of the path that tiny Phobos takes around Mars. Over the course of 22 minutes, Hubble snapped 13 separate exposures of the little Martian moon. The video can be viewed at https://photojournal.jpl.nasa.gov/catalog/PIA21837