Thursday, 30 April 2026

US-Indian Spacecraft Captures Mexico City Subsidence

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US-Indian Spacecraft Captures Mexico City Subsidence

A satellite map of the Mexico City area shows land subsidence, with blue patches indicating the fastest rates of sinking compared to yellow and green patches. A color bar in the corner shows rate of change. The airport and a few landmarks are labeled.
PIA26709
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NASA/JPL-Caltech/David Bekaert

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US-Indian Spacecraft Captures Mexico City Subsidence

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A scientist produced this map of land subsidence (sinking) in Mexico City using data from the NISAR (NASA-ISRO Synthetic Aperture Radar) mission captured between Oct. 25, 2025, and Jan. 17, 2026. The region has been a well-known hot spot of subsidence for decades, and images like this help confirm that NISAR is performing as expected in its first year of operation.

The dark blue color indicates areas found to be subsiding by more than half an inch (more than 2 centimeters) per month, due in large part to groundwater pumping, which has led to compaction of the dry, ancient lakebed on which the city was built. The yellow and red areas are likely residual noise signals that are expected to decrease as NISAR collects more data and refines its measurements.

Two marshy ecosystems with ties to the country’s past can be seen in the image. The dark green oblong to the northeast of the airport is Nabor Carrillo, an artificial lake constructed over the now-extinct Lake Texcoco. Chalco Lake, a wetland located in a historically fertile region to the south, shares its name with a major body of water that was drained over a period of centuries to reduce flooding in the city. The ancient lake was a primary natural habitat of the Mexican Axolotl, an endangered species of salamander with the ability to regrow limbs.

Another landmark pinpointed in the image — the Angel of Independence along the Paseo de la Reforma — was built in 1910 to commemorate 100 years of Mexico’s independence. Standing over 100 feet (30 meters) tall, the monument has had 14 steps added to its base over the years as the land around it has gradually sunk.

A satellite map of the Mexico City area shows land subsidence, with blue patches indicating the fastest rates of sinking compared to yellow and green patches. A color bar in the corner shows rate of change. The airport and a few landmarks are labeled.
Figure A

Figure A is a version of the image extending further south and with no labels, scale, or compass.

The images were created with data from NISAR’s L-band radar instrument, which uses a 9-inch (24-centimeter) wavelength that enables its signal to penetrate dense vegetation such as forest canopies.

The satellite’s S-band radar, provided by the Indian Space Research Organisation’s Space Applications Centre, uses a 4-inch (10-centimeter) microwave signal that’s more sensitive to small vegetation, which makes it effective at monitoring certain types of agriculture and grassland ecosystems. Launched in 2025, NISAR is the first satellite to carry two SAR instruments at different wavelengths.

Data from NISAR will benefit humanity by helping researchers around the world better understand changes across our planet’s surface, from cities to forests and glaciers. The global and rapid coverage from NISAR will also provide unprecedented support for disaster response, producing data to assist in mitigating and assessing damage, with observations before and after catastrophic events available in short time frames.

Find more information about NISAR here: https://science.nasa.gov/mission/nisar/



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Curiosity Blog, Sols 4873-4878: Welcome to the Atacama Drill Target

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Curiosity Blog, Sols 4873-4878: Welcome to the Atacama Drill Target

A black-and-white, wide-angle photograph taken on Mars by the Curiosity rover. In the foreground, the rover's robotic arm with a complex cluster of instruments at its end reaches down, casting a dark shadow onto the ground. The terrain consists of flat, jagged, light-colored rock slabs separated by patches of dark sand with wind-blown ripples. Parts of the rover's hardware are visible in the bottom corners of the frame. In the background, a desolate, rocky landscape stretches toward a curved horizon lined with distant hills under a pale sky.
NASA’s Mars rover Curiosity acquired this image using its Front Hazard Avoidance Camera (Front Hazcam) on April 23, 2026 — Sol 4874, or Martian day 4,874 of the Mars Science Laboratory mission — at 01:12:31 UTC.
NASA/JPL-Caltech

Written by Sharon Wilson Purdy, Planetary Geologist at the Smithsonian National Air and Space Museum

Earth planning date: Friday, April 24, 2026

There was excitement in the air as the Curiosity Science Team kicked off a drill campaign at the Atacama site to characterize the first Mount Sharp layered-sulfate bedrock since leaving the boxwork terrain.

Monday was a three-sol plan (4873-4875) where we focused on “drill sol 1” activities that included a pre-load test on our drill target as well as triage contact science. APXS assembled a set of repeated observations on the Atacama drill target, and the coordinated MAHLI images taken with different lighting will provide an opportunity to detect possible changes between the datasets. Mastcam assembled stereo mosaics to document the Atacama drill site, investigate variations in the bedrock at “Kimsa Chata,” and characterize the layering within Paniri butte.

Planning resumed Friday with another three-sol plan (4876-4878) that included the full drill and portion characterization related to “drill sols 2 and 3” activities. Mastcam planned stereo mosaics of rocks in the workspace including a laminated rock with an exposed edge named “Queen of the Andes,” a rock with polygonal fractures that was broken when the rover drove over it named “Curaco,” and more coverage of the “El Almendrillo” target.

Rounding out the plans this week, the Environmental theme group continues to monitor dust in the atmosphere, study cloud movements, and document the presence of dust devils. The rover will also autonomously select two targets to be analyzed by the ChemCam instrument.

Next week we look forward to continuing our drill campaign, where the next step will be delivering a portion of the Atacama target to the ChemMin instrument for analysis. The science team is looking forward to seeing how the mineralogy of the layered sulfate unit here compares to our last drill of the same unit at the Mineral King site, which is nearly 160 meters (525 feet) below our current location!

A rover sits on the hilly, orange Martian surface beneath a flat grey sky, surrounded by chunks of rock.
NASA’s Curiosity rover at the base of Mount Sharp
NASA/JPL-Caltech/MSSS

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Apr 29, 2026

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Curiosity Blog, Sols 4867-4872: Sand Fill In Antofagasta Crater and Finding Our Next Drill Target



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US-Indian Space Mission Maps Extreme Subsidence in Mexico City

A satellite image of the Mexico City area shows land subsidence via a vibrant heat map, with dark blue patches indicating the highest rates of sinking contrasted against more stable terrain indicated in yellow and green.
New data from NISAR shows where Mexico City and its environs subsided by up to a few centimeters per month (shown in blue) between Oct. 25, 2025, and Jan. 17, 2026. Uneven and seemingly small elevation changes have added up over the decades, fracturing roads, buildings, and water lines.
NASA/JPL-Caltech/David Bekaert

One of the most powerful radar systems ever launched into space has mapped the ground moving beneath one of fastest subsiding capitals in the world: Mexico City. The findings show how quickly and reliably the NISAR (NASA-ISRO Synthetic Aperture Radar) satellite can track real-time changes across Earth’s surface from orbit, unhindered by clouds or vegetation that impede optical sensors and higher-frequency radars.

Home to some 20 million people, the Mexico City area is built atop an aquifer. Extensive groundwater pumping, combined with the weight of urban development, has resulted in the compaction of the ancient lakebed beneath the city for more than a century. An engineer first documented the issue in 1925, and by the 1990s and 2000s, parts of the metropolitan area were sinking by around 14 inches (35 centimeters) per year, damaging infrastructure including the Metro, one of the largest rapid transit systems in the Americas.

Several generations of space-based radar have tracked Mexico City on the move. The NISAR mission, launched in July 2025, is now advancing these efforts, analyzing fast-changing areas that are challenging to survey from space. Capable of working day and night, rain or shine, NISAR’s L-band synthetic aperture radar is designed to track subtle motions such as land sinking and rising, glaciers sliding, and croplands growing, as it passes overhead multiple times a month.

“Images like this confirm that NISAR’s measurements align with expectations,” said Craig Ferguson, deputy project manager at NASA Headquarters in Washington. “NISAR’s long wavelength L-band radar will make it possible to detect and track land subsidence in more challenging and densely vegetated regions such as coastal communities where they may have the compounding effects of both land subsidence and sea level rise.”

The new analysis is based on preliminary measurements taken by NISAR between October 2025 and January 2026, during Mexico City’s dry season. Parts of the region found to be subsiding by more than half an inch (more than 2 centimeters) per month are shown in dark blue. The yellow and red areas are likely residual noise signals that are expected to decrease as NISAR collects more data. The structure near the center of the image is Benito Juarez International Airport, with Lake Nabor Carrillo visible as a dark green oblong to the northeast.

One area landmark — the Angel of Independence along the Paseo de la Reforma — is a visible indicator of subsidence. Built in 1910 to commemorate 100 years of Mexico’s independence, the towering monument stands 114 feet (36 meters) high and has had 14 steps added to its base as the land around it gradually sinks.

“Mexico City is a well-known hot spot when it comes to subsidence, and images like this are just the beginning for NISAR,” said David Bekaert, a project manager at the Flemish Institute for Technological Research and a member of the NISAR science team. “We’re going to see an influx of new discoveries from all over the world, given the unique sensing capabilities of NISAR and its consistent global coverage.”

A joint mission developed by NASA and the Indian Space Research Organisation (ISRO), NISAR launched from Satish Dhawan Space Centre on India’s southeastern coast. Managed by Caltech, NASA’s Jet Propulsion Laboratory in Southern California leads the United States component of the project and provided the satellite’s L-band SAR and antenna reflector. The spacecraft bus and its S-band SAR were provided by ISRO.

The NISAR satellite is the first to carry two SAR instruments at different wavelengths and is monitoring Earth’s land and ice surfaces twice every 12 days, collecting data using the spacecraft’s giant drum-shaped reflector, which measures 39 feet (12 meters) wide — the largest radar antenna reflector NASA has ever sent into space. 

To learn more about NISAR, visit:

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

Media Contacts

Andrew Wang / Andrew Good
Jet Propulsion Laboratory, Pasadena, Calif.
626-379-6874 / 818-393-2433
andrew.wang@jpl.nasa.gov / andrew.c.good@jpl.nasa.gov

Written by Sally Younger

2026-027

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Wednesday, 29 April 2026

NASA Connects Little Red Dots with Chandra, Webb

This image of a special object, dubbed the “X-ray dot,” represent a discovery from Chandra that could help explain the nature of a mysterious class of sources in the early Universe. The optical and infrared image from Hubble show the region around the X-ray dot, while the Chandra X-ray image shows the close up. Prior to this discovery, “little red dots” seen by the Webb telescope had not been known to emit X-rays. This one does, which leads researchers to propose that the X-ray dot represents a previously unknown transition phase of growing supermassive black holes.
This image of a special object, dubbed the “X-ray dot,” represents a discovery from Chandra that could help explain the nature of a mysterious class of sources in the early Universe. The optical and infrared image from Hubble show the region around the X-ray dot, while the Chandra X-ray image shows the close up. Prior to this discovery, “little red dots” seen by the Webb telescope had not been known to emit X-rays. This one does, which leads researchers to propose that the X-ray dot represents a previously unknown transition phase of growing supermassive black holes.
X-ray: NASA/CXC/Max Plank Inst./R. Hviding et al.; Optical/IR; NASA/ESA/STScI/HST; Image Processing: NASA/CXC/SAO/N. Wolk

A newly discovered object may be a key to unlocking the true nature of a mysterious class of sources that astronomers have found in the early universe in recent years.

A “X-ray dot” found by NASA’s Chandra X-ray Observatory could explain what the hundreds or potentially thousands of these objects are. A paper describing the results published in The Astrophysical Journal Letters.

Shortly after NASA’s James Webb Space Telescope started its science observations, reports of a new class of mysterious objects emerged. Astronomers found small, red objects about 12 billion light-years from Earth or farther, which became known as “little red dots” (LRDs).

Many scientists think LRDs are supermassive black holes embedded in clouds of dense gas, which mask some of the typical signatures in different kinds of light – including X-rays – that astronomers usually use to identify them. This would make them different from typical growing supermassive black holes, which are not embedded in dense gas, allowing bright ultraviolet light and X-rays from material orbiting the black holes to escape.

Because of this and their potential similarities to stellar atmospheres, astronomers have called this the “black hole star” scenario for LRDs.

This new “X-ray dot” (officially known as 3DHST-AEGIS-12014), which is located about 11.8 billion light-years from Earth, may provide a crucial bridge between black hole stars and typical growing supermassive black holes. It exhibits most of the features of an LRD, including being small, red, and located at a vast distance, but it glows in X-ray light, unlike other LRDs.

“Astronomers have been trying to figure out what little red dots are for several years,” said lead author Raphael Hviding of the Max Planck Institute for Astronomy in Germany. “This single X-ray object may be – to use a phrase – what lets us connect all of the dots.”

Artist's Illustration of a Close-Up View of X-ray Dot, 3DHST-AEGIS-12014.
Artist’s Illustration of a Close-Up View of X-ray Dot, 3DHST-AEGIS-12014.
NASA/CXC/SAO/M. Weiss; adapted by K. Arcand & J. Major

The team found this one special object after comparing new data from Webb with a deep survey previously performed by Chandra.

“If little red dots are rapidly growing supermassive black holes, why do they not give off X-rays like other such black holes?” said co-author Anna de Graaff of the Center for Astrophysics | Harvard & Smithsonian, in Cambridge, Massachusetts. “Finding a little red dot that looks different from the others gives us important new insight into what could power them.”

The researchers suggest that the X-ray dot represents a transition phase from an LRD to a typical growing supermassive black hole. As the black hole star consumes its surrounding gas, patchy holes in the clouds of gas appear. This allows X-rays from material falling onto the black hole to poke through, which are observed by Chandra. Eventually all the gas is consumed, and the black hole star ceases to exist.

There are also hints in the Chandra data of the X-ray dot that there are variations in X-ray brightness, which supports the idea that the black hole is partly obscured. As the cloud of gas rotates, patches of denser and less dense gas can move across the black hole, causing changes in X-ray brightness.

“If we confirm the X-ray dot as a little red dot in transition, not only would it be the first of its kind, but we may be seeing into the heart of a little red dot for the first time,” said co-author Hanpu Liu of Princeton University in New Jersey. “We would also have the strongest piece of evidence yet that the growth of supermassive black holes is at the center of some, if not all, of the little red dot population.”

An alternate idea for the X-ray dot is that it is a more common type of growing supermassive black hole but is veiled in an exotic type of dust that astronomers have not seen before. Future observations are planned that should be able to shed light on the truth.

“The X-ray dot had been sitting in our Chandra survey data for over ten years, but we had no idea how remarkable it was before Webb came along to observe the field,” said co-author Andy Goulding of Princeton. “This is a powerful example of collaboration between two great observatories.”

NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.

Read more from NASA’s Chandra X-ray Observatory

Learn more about the Chandra X-ray Observatory and its mission here:

https://science.nasa.gov/chandra

https://chandra.si.edu

News Media Contact

Megan Watzke
Chandra X-ray Center
Cambridge, Mass.
617-496-7998
mwatzke@cfa.harvard.edu

Joel Wallace
Marshall Space Flight Center, Huntsville, Alabama
256-544-0034
joel.w.wallace@nasa.gov



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There’s No Place Like NASA’s New X-59 Hangar Home 

4 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

A white and blue jet airplane is parked in front of a building with large sliding doors and a NASA logo centered on the forward wall. The building is the new X-59 hangar.
NASA’s X-59 quiet supersonic airplane sits parked in front of its new hangar home at the agency’s Armstrong Flight Research Center in California. The facility originally was constructed in 1968 and for nearly 60 years has hosted a number of research aircraft and programs.
NASA/Christopher LC Clark

There’s no sign reading “home sweet home” in the hangar where the X‑59 now sits, but the sentiment is unmistakable among those tending to the quiet supersonic aircraft.

Located at NASA’s Armstrong Flight Research Center in Edwards, California, the X-59 hangar was built in 1968 but looks like new thanks to a full renovation and modernization. While the X-59 was being assembled in Palmdale, California, workers at NASA Armstrong gutted the hangar, adding new electrical wiring, a fire suppression system, office space, air conditioning, and other safety features.

“The whole team is incredibly proud of what we’ve accomplished in preparing this new home for the X-59,” said Bryan Watters, the NASA project manager at Armstrong who led the renovation effort. “The fact we could take a 1960s hangar and modernize it for use by a 2020’s X-plane is very special.”

The X-59 is the centerpiece of NASA’s Quesst mission to enable a new era of commercial supersonic air travel over land by reducing the sound of typically loud sonic booms to a much quieter sonic thump.

Home hunting

When NASA test pilot Nils Larson successfully took the X-59 into the air for the first time on Oct. 28, 2025, he flew from the Lockheed Martin Skunk Works assembly site in Palmdale to nearby NASA Armstrong, from where test flights have continued to make progress.

From the beginning of the program, knowing the X-59 would eventually need a new residence at NASA Armstrong, Quesst managers were on the hunt for somewhere to house the quiet supersonic demonstrator.

Like anyone looking for the ideal place to call home, the team made sure there would be enough space for the airplane and all its support equipment. But with the experimental jet measuring at just under 100 feet long and 30 feet wide, there were few options.

“We had to find a hangar that was long enough so that part of the X-59 wouldn’t hang outside, exposed to the elements,” Watters said.

Building 4826, as the hangar is officially designated, turned out to be the choice spot. “It was basically stripped down and gutted so that essentially it was just structural steel with siding. From that state it was rebuilt,” Watters said.

The feature they are perhaps most proud of is the hangar’s new floor. Covering more than 32,000 square feet, it is coated with epoxy that prevents any spills from seeping into the concrete.

From the hangar’s office windows, the view of the hangar floor can include the F-15 research jets that will be used as chase planes to support X-59 flights in the coming months. The renovation faced challenges along the way, chief among them being supply chain issues stemming from the COVID-19 pandemic. But there were some incredible, unforgettable moments too.

Circa 1990
Nov. 2025
A white fighter jet turned into a research aircraft with red and blue trim is parked inside a NASA hangar.
On loan to NASA from the Air Force, an F-15 Eagle fighter jet was the focus of the Short Takeoff and Landing/Maneuver Technology Demonstrator research program, which concluded in 1991. The aircraft is seen here inside Building 4826, a hangar at NASA’s Armstrong Flight Research Center that was renovated and began use in 2025 as home for the X-59 quiet supersonic technology demonstrator.
NASA
A blue and white supersonic jet with red trim sits inside a newly renovated hangar.
NASA’s X-59 quiet supersonic technology demonstrator aircraft is seen parked inside its new hangar home at the agency’s Armstrong Flight Research Center in California.
NASA/Christopher LC Clark
A white fighter jet turned into a research aircraft with red and blue trim is parked inside a NASA hangar.
On loan to NASA from the Air Force, an F-15 Eagle fighter jet was the focus of the Short Takeoff and Landing/Maneuver Technology Demonstrator research program, which concluded in 1991. The aircraft is seen here inside Building 4826, a hangar at NASA’s Armstrong Flight Research Center that was renovated and began use in 2025 as home for the X-59 quiet supersonic technology demonstrator.
NASA
A blue and white supersonic jet with red trim sits inside a newly renovated hangar.
NASA’s X-59 quiet supersonic technology demonstrator aircraft is seen parked inside its new hangar home at the agency’s Armstrong Flight Research Center in California.
NASA/Christopher LC Clark
Circa 1990
Nov. 2025

past and present

Hangar Updated to Continue Hosting Historic Research

This NASA hangar at Armstrong Flight Research Center originally was constructed in 1968 and since then has hosted a number of history-making programs. Compare the two images above to see how the hangar looked during the late 1980s when it hosted an F-15 research aircraft (left), and beginning in 2025 after it had been renovated and modernized to host the X-59 quite supersonic technology demonstrator aircraft.

Moved in

With X-59 now flying regularly and comfortably settled into its new digs, the Quesst team is gauging its performance on the way to quiet supersonic flight.

“This is truly a great time for Quesst and the X-59,” said Cathy Bahm, NASA’s project manager for the Low Boom Flight Demonstrator. “It’s also still a little surreal to be able to just walk down from your office and see the airplane in our hangar.”

For more than a year, the hangar refurbishment team worked through every detail of the X-59’s new home to make sure it would be safe and sound. But actually seeing the aircraft occupy that space is an adjustment for them, too.

“We’ve looked at X-59 models on our desk for years and then, you know, there’s the real thing right in front of us, in a hangar that we renovated,” Watters said.

A real thing in the hangar – and streaking across the California desert sky. The X-59’s transition from an idea into a working aircraft is a testament to the teams that help build out every aspect of its infrastructure.  

NASA’s X-59 is supported under the agency’s Aeronautics Research Mission Directorate.

About the Author

Jim Banke

Jim Banke

Managing Editor/Senior Writer

Jim Banke is a veteran aviation and aerospace communicator with more than 40 years of experience as a writer, producer, consultant, and project manager based at Cape Canaveral, Florida. He is part of NASA Aeronautics' Strategic Communications Team and is Managing Editor for the Aeronautics topic on nasa.gov. In 2007 he was recognized with a Distinguished Public Service Medal, NASA's highest honor for a non-government employee.

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US-Indian Spacecraft Captures Mexico City Subsidence

3 Min Read US-Indian Spacecraft Captures Mexico City Subsidence PIA26709 Credits: NASA/JPL-Caltech/David Bekaert ...