Explosive Intensification for Hurricane Polo

Explosive Intensification for Hurricane Polo




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Hurricane Polo, with a well-defined eye, swirls over the Pacific Ocean off the coast of Mexico. The storm was positioned just south of Acapulco, with its outer cloud bands extending inland toward Mexico City.
NASA Earth Observatory/Michala Garrison

A map depicts sea surface temperature anomalies off Mexico's Pacific coast on September 23. Deep red areas highlight areas 3°C above the norm for that date. A dotted line traces the storm's path from September 20 to September 23 as it moved through the unusually warm waters.
NASA Earth Observatory/Michala Garrison

Hurricane Polo, with a well-defined eye, swirls over the Pacific Ocean off the coast of Mexico. The storm was positioned just south of Acapulco, with its outer cloud bands extending inland toward Mexico City.
NASA Earth Observatory/Michala Garrison
A map depicts sea surface temperature anomalies off Mexico's Pacific coast on September 23. Deep red areas highlight areas 3°C above the norm for that date. A dotted line traces the storm's path from September 20 to September 23 as it moved through the unusually warm waters.
NASA Earth Observatory/Michala Garrison

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mur sst


After rapidly intensifying, Hurricane Polo spins off Mexico’s Pacific coast on September 23, 2026 (left), over unusually warm waters (right). NASA Earth Observatory images by Michala Garrison, using data from the MODIS (Moderate Resolution Imaging Spectroradiometer) on NASA’s Aqua satellite and the MUR SST (Multiscale Ultrahigh Resolution Sea Surface Temperature) project.

In mid-September 2026, Hurricane Polo began as a tropical disturbance off the Pacific coast of Mexico. By September 20, it was organized enough to qualify as a tropical depression, and by the next day it was a tropical storm.

From there, Polo launched into a period of rapid intensification that left meteorologists searching for adjectives strong enough to convey what was happening. Some described the storm’s rate of intensification and strength as “jaw-dropping,” others as “astonishing,” and others as “absolute insanity.”  

“Polo went through a period of what can only be described as explosively rapid intensification,” said Gary Partyka, an atmospheric scientist with the Global Modeling and Assimilation Office (GMAO) at NASA’s Goddard Space Flight Center, in an email. “This was RAPID, rapid intensification.”

The storm was in an environment that was “near perfect” for strengthening, Partyka said, characterized by weak wind shear, high moisture, warmer ocean temperatures, and high levels of atmospheric instability.

Several observers leaned on extreme rapid intensification—a technical classification meaning the storm’s wind speeds increased at least 60 knots (111 kilometers or 69 miles per hour) within a 24-hour period. By September 22, the storm’s maximum sustained wind speed had risen by 90 knots (167 kilometers per hour or 104 miles per hour) within 24 hours, hitting category 5 strength. In its normally staid forecast discussions, the National Hurricane Center called the intensification “truly remarkable.”

When NOAA’s Hurricane Hunter aircraft flew over the storm on September 22, researchers estimated winds of nearly 285 kilometers (180 miles) per hour. That would make it the third-strongest storm on record in the eastern Pacific by maximum sustained winds and the fastest on record to go from a tropical depression to a category 5 storm, according to some analysts.

On the afternoon of September 23, when the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite captured this image (left), Polo was churning off the coast of Guerrero, southwest of Acapulco. With maximum sustained winds of 230 kilometers (145 miles) per hour, the storm was category 4 strength when the image was acquired, having undergone an eyewall replacement cycle that weakened it slightly.

“The satellite imagery of Polo is very impressive, with the storm’s large, clear eye and extensive outflow pattern,” said Kristen Corbosiero, an atmospheric scientist at the State University of New York at Albany, who is working on a NASA project that uses satellite data to study tropical cyclone ventilation. “Weak winds above the system and good outflow at the top of the system also contributed to Polo’s rapid intensification.”

As Polo developed, it moved over areas where sea surface temperatures were as high as 32 degrees Celsius (90 degrees Fahrenheit)—2 to 3 degrees warmer than usual for September 23. Surface waters across much of the region were above 27.8°C (82°F), the temperature generally required to sustain and intensify hurricanes.

The map above (right) is based on data from the Multiscale Ultrahigh Resolution Sea Surface Temperature (MUR SST) project at NASA’s Jet Propulsion Laboratory, which blends satellite measurements from NASA, NOAA, and international missions with observations from ships and buoys. Rather than absolute temperatures, the map shows anomalies—how much warmer or cooler the ocean surface was on September 23, 2026, than the project’s 2003-2014 average for that date.

While the map above conveys temperatures at the water surface, the presence of warm water deeper in the column has likely contributed to the storm’s staying power, Corbosiero added. Sometimes hurricanes churn up cooler water from deep in the column that can slow a storm’s intensification, but in this case the cool water wake behind the storm appears minimal, and measurements and models show high ocean heat content at considerable depths.

Both Partyka and Corbosiero cautioned against attributing Polo’s rapid intensification directly to El Niño’s unusually warm surface temperatures in the central and eastern Pacific Ocean. Several hurricanes in this region have undergone rapid intensification in the past during La Niña and neutral conditions, Corbosiero noted, including Hurricane Otis in 2023 and Patricia in 2015, both category 5 storms.  

However, the overall amount of tropical cyclone activity in the eastern Pacific does typically increase during El Niño due to changes in large-scale ocean and atmospheric circulation patterns, and that’s what has happened so far in 2026. As of September 24, the accumulated cyclone energy in the region was nearly twice the norm, according to data from Colorado State University.

People tracking sea surface temperature anomalies or other aspects of the storm can do so using NASA’s Worldview browser, a near real-time data viewer from the Short-term Prediction Research and Transition (SPoRT) project, and the FLUID tool from GMAO. Forecasters expect Polo to stay over the Pacific until next week, when it may curve toward the northeast and approach Baja California.

NASA Earth Observatory images by Michala Garrison, using sea surface temperature data from the Multiscale Ultrahigh Resolution (MUR) project, MODIS data from NASA EOSDIS LANCE and GIBS/Worldview, and storm track data from NOAA’s National Hurricane Center. Story by Adam Voiland.

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NASA Welcomes Côte d’Ivoire as Newest Artemis Accords Signatory

NASA Welcomes Côte d’Ivoire as Newest Artemis Accords Signatory

Credit: NASA

Côte d’Ivoire signed the Artemis Accords on Thursday as the 75th signatory during a signing ceremony in the nation’s largest city Abidjan, marking the largest milestone yet for the international coalition of like-minded countries committed to peaceful and responsible space exploration.

“The United States and Côte d’Ivoire already cooperate on Earth,” said NASA’s Deputy Administrator Matt Anderson. “Today, we expand that partnership beyond it. Joining the Artemis Accords opens new opportunities for our scientists, engineers, and institutions to work together as humanity returns to the Moon and prepares for what comes next. We’ve aligned on the principles. The opportunities are in front of us. And now we can get to work.”

The nation’s Minister of Higher Education and Scientific Research Adama Diawara signed on behalf of the country in a ceremony held during Africa Space Expo ASPEX 2026. Chargé d’affaires Junaid Munir from the U.S. Department of State witnessed the ceremony.

“This is a great achievement, and important for Côte d’Ivoire’s ambitions and for the rest of the African Union members,” said Director General of the Space Agency of Côte d’Ivoire Tidiane Outtara.

Côte d’Ivoire has expanded its involvement in space science and technology through years of international cooperation. Since 2019, the National Office of Technical Development of Côte d’Ivoire and NASA have collaborated on Earth observation and geodesy, a field that measures Earth’s shape, gravity, and movement. Together, the partners have advanced global geodetic networks, improved space‑based measurement techniques, and increased understanding of how Earth’s systems interact.

The country later established the Space Agency of Côte d’Ivoire in 2025 to coordinate national efforts in Earth observation, space weather, astronomy, satellite navigation, and communications.

In 2020, NASA and the State Department joined with seven other founding nations to establish the Artemis Accords, responding to the growing interest in lunar activities by both governments and private companies. The Artemis Accords are the first set of practical principles aimed at enhancing transparency, safety, and coordination among nations as they explore the Moon, Mars, and beyond, committing nations to:

  • Explore peaceably and transparently
  • Render aid to those in need
  • Enable access to scientific data
  • Ensure activities do not interfere with those of others
  • Preserve historically significant sites and artifacts by developing best practices

By signing the Artemis Accords, nations open the door to opportunities for future lunar exploration with NASA, advancing humanity’s return to the Moon, and shaping the Golden Age of exploration and innovation.

Learn more about the Artemis Accords at: 

https://www.nasa.gov/artemis-accords

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Sep 24, 2026

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Jennifer M. Dooren

NASA Shares SpaceX Crew-14 Assignments for Space Station Mission

NASA Shares SpaceX Crew-14 Assignments for Space Station Mission

NASA’s SpaceX Crew-14 crew members during preflight training at SpaceX’s facility in Hawthorne, California (from left, Roscosmos cosmonaut Arutyun Kiviryan, NASA astronaut Chris Birch, NASA astronaut Kayla Barron, and JAXA (Japan Aerospace Exploration Agency) astronaut Makoto Suwa).        
Credit: SpaceX

Four crew members from three space agencies will launch to the International Space Station no earlier than spring 2027 for a long-duration science expedition as part of NASA’s SpaceX Crew-14 mission.

NASA astronauts Kayla Barron and Chris Birch will serve as spacecraft commander and pilot, with JAXA (Japan Aerospace Exploration Agency) astronaut Makoto Suwa, and Roscosmos cosmonaut Arutyun Kiviryan as mission specialists. After docking, Crew-14 will join the space station’s Expedition 75/76.

This mission is the 14th commercial crew rotation with SpaceX under NASA’s Low Earth Orbit Program. The crew will conduct scientific investigations and technology demonstrations to help prepare humans for future exploration missions to the Moon and Mars and to benefit people on Earth.

This will be Barron’s second flight to the space station. She was selected as a NASA astronaut in 2017. Barron earned a bachelor’s degree in systems engineering from the U.S. Naval Academy in Annapolis, Maryland and a master’s degree in nuclear engineering from the University of Cambridge in England. A commander in the U.S. Navy, Barron earned her submarine warfare officer qualification, deploying three times aboard the USS Maine. She first launched to the space station in 2021 aboard NASA’s SpaceX Crew-3 mission, spending a total of 177 days in space across space station Expeditions 66/67. She completed two spacewalks and served as lead robotics operator for another. Most recently, Barron supported the development of new technologies and operational concepts for NASA’s Artemis program.

Selected as a NASA astronaut in 2021, Birch graduated from the University of Arizona in Tucson with degrees in mathematics and biochemistry and molecular biophysics. She earned a doctorate in biological engineering from the Massachusetts Institute of Technology, and later taught bioengineering at the University of California, Riverside, and scientific writing and communication at the California Institute of Technology in Pasadena. Birch competed as a decorated track cyclist on the U.S. National Team and was named to the Olympic Long Team for the 2020 Tokyo Games. She has served as a capsule communicator, supporting crews aboard the space station and during the Artemis II mission. Birch was crew lead for Expedition 72, working with flight control teams to help manage daily operations, and served as a crew representative for NASA’s Orion Program, supporting Artemis II mission development and operations. This will be her first spaceflight.

The Crew-14 mission also is the first spaceflight assignment for Suwa. Before JAXA selected him as an astronaut candidate in 2023, Suwa spent nearly a decade with the World Bank Group. Previously, he served in Rwanda as a Japan Overseas Cooperation Volunteer before joining the United Nations World Meteorological Organization. Suwa holds a doctorate in geosciences from Princeton University and completed basic training to become certified as an astronaut in 2024.

This mission will be Kiviryan’s first trip to the space station. He graduated from Saint Petersburg Suvorov Military School in 2010 and later studied at the Baltic State Technical University. He graduated in 2015 as an engineer specializing in rocket science and completed training in the operation of computer-controlled machines. Kiviryan was selected for the Gagarin Research and Test Cosmonaut Training Center Cosmonaut Corps in 2021 and has served as a test cosmonaut since 2023.  

For more than 25 years, people have lived and worked continuously aboard the International Space Station, advancing scientific knowledge and making research breakthroughs that aren’t possible on Earth. The space station helps NASA understand and overcome the challenges of human spaceflight, expand commercial opportunities in low Earth orbit, and build on the foundation for long-duration missions to the Moon, as part of the Artemis program, and to Mars.

Learn more about International Space Station research and operations at:

https://www.nasa.gov/station

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Lauren E. Low

Advanced Health Tech Research Continues to Protect Astronaut Health

Advanced Health Tech Research Continues to Protect Astronaut Health

NASA astronaut and Expedition 75 flight engineer Jack Hathaway carries the Advanced Space Experiment Processer-4 (ADSEP-4) and relocates it for installation inside the International Space Station's Destiny laboratory module. ADSEP-4 houses research samples for processing in microgravity, can be launched aboard a SpaceX Dragon or Northrop Grumman's Cygnus XL spacecraft for powered science, and installed in EXPRESS racks aboard the orbital outpost for experimentation.
NASA astronaut Jack Hathaway relocates sample processing hardware and prepares it for installation inside the International Space Station’s Destiny laboratory module.
NASA/Jessica Meir

Advanced health research, including ultrasound scans, blood tests, and exercise studies, using the latest technology in microgravity was on Thursday’s schedule for the Expedition 75 crew. The orbital residents also continued their ongoing cargo operations and maintenance tasks aboard the International Space Station.

Station commander Jessica Meir conducted the EchoFinder-2 space health study for a second day, this time with NASA flight engineer Jack Hathaway. The duo took turns inside the Columbus laboratory module scanning each other’s organs with the Echo ultrasound hardware as a technician on the ground monitored in real time. The investigation uses a computer tablet and a combination of augmented reality and artificial intelligence to correctly position the probe then detect and visualize the organs. Results may enable future crews to use medical monitoring tools without guidance from doctors on the ground as they travel farther away from Earth.

An immune system study was under way for a third day inside the Harmony module as NASA flight engineer Anil Menon processed blood samples after a 24-hour incubation period. Menon first retrieved tubes, specially designed for use in microgravity, containing blood samples from the Kubik incubator. Next, he spun the sample tubes in a centrifuge separating the blood into red and white blood cells, platelets, and plasma. At the completion of the experiment, he placed the sample tubes in a science freezer for preservation and later analysis. The samples will be analyzed aboard the orbital complex to learn how living in space affects an astronaut’s ability to fight infections and disease.

Flight engineer Sophie Adenot of ESA (European Space Agency) strapped on the sensor-packed Bio-Monitor vest and headband then pedaled for an hour on the Destiny laboratory module’s exercise cycle. The wearable sensors comfortably monitored Adenot’s blood pressure, heart rate, and breathing rate during her workout. Afterward, she prepared her biomedical data for downloading to give doctors insight into space-influenced physiological changes and how lunar and planetary gravity environments may affect crew health.

Adenot later took turns with Menon and transferred cargo in and out of the Cygnus XL cargo spacecraft from Northrop Grumman. Cygnus XL launched on April 14 carrying over 11,000 pounds of science and supplies for the crew. It arrived at the station two days later for a capture with the Canadarm2 robotic arm and installation to the Unity module’s Earth-facing port.

The Progress 96 cargo spacecraft, which arrived with nearly three tons of food, fuel, and supplies on Sept. 19, is still being unloaded by Roscosmos flight engineers Pyotr Dubrov, Anna Kikina, and Andrey Fedyaev. The three cosmonauts also split their Thursday shift jogging on a treadmill for a fitness assessment, replacing power system components inside the Zvezda service module, and synchronizing neutron radiation detection hardware with mission controllers on Earth.

Learn more about station activities by following the space station blog, @space_station on X, as well as the ISS Facebook and ISS Instagram accounts.

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Mark A. Garcia

NASA’s Machines for Mars Make Beer Bubbly 

NASA’s Machines for Mars Make Beer Bubbly 

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Preparations for Next Moonwalk Simulations Underway (and Underwater)

A woman controls an Earthly Labs-branded machine in a factory setting; a tank that says “carbon dioxide” is in the foreground.
A brewer makes adjustments to the Earthly Labs carbon-capture unit, which purifies carbon dioxide from the beer brewing process for use in carbonation.
Credit: Chart Industries Inc.

In 2021, Maine Beer Company’s carbon dioxide supplier ran short on carbon dioxide.

“There was potential for our beer to go stale in the tanks,” said Dave Love, the brewery’s sustainability manager. “We wouldn’t be able to use CO2 for any of our bottling, kegging, or centrifuge operations.”

The solution the company settled on originated on Mars — or more specifically, in NASA’s plans for harvesting resources from the Red Planet. Now it’s saving money and reducing emissions for wineries, distilleries, power companies, helium producers, and more.

Beginning in the 1990s, the company Pioneer Astronautics won multiple Small Business Innovation Research (SBIR) contracts from Johnson Space Center in Houston to build systems that could generate resources on Mars. The technology could, for example, capture carbon dioxide from the Martian atmosphere and combine it with hydrogen to produce water for life support and methane for rocket fuel. These capabilities weren’t entirely new, but Pioneer’s systems were compact, efficient, and automated.

Later, Pioneer Astronautics founder Robert Zubrin created Pioneer Energy to rearrange these subsystems into technology for the oil and gas industry (Spinoff 2015, 2020). He soon realized technology for capturing and purifying carbon dioxide on Mars could do the same in a brewery, capturing CO2 from the brewing process for use in carbonation. By 2015, the Craft Brewery Recovery System was in production (Spinoff 2016). In the end, though, the company put the system up for licensing.

Amy George founded Earthly Labs of Austin, Texas, in 2016 to develop small-scale carbon capture. She discovered the Craft Brewery Recovery System and obtained an exclusive license. 

Since the pandemic reduced its availability, carbon dioxide has continued experiencing shortages and volatility, and George said these have emerged as major drivers of interest in the technology. 

And it isn’t just helping brewers. After expanding into wineries and distilleries, Earthly Labs started discovering other markets. Energy companies often generate carbon dioxide as a by-product, which they can sell if it’s captured. Several are now customers.

Another application finding new customers is helium production. Helium, which is used to make microchips and fiber-optic cables, among other applications, is found in underground deposits, mixed with other gases, such as methane and carbon dioxide, that need to be separated. 

In 2021, Earthly Labs was acquired by Chart Industries Inc., which specializes in cryogenic equipment engineering and has helped scale up the technology for applications like power plants.

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Andrew Wagner