NASA Drains 66-Million-Gallon Reservoir to Upgrade Critical Water System

NASA Drains 66-Million-Gallon Reservoir to Upgrade Critical Water System

A powerful but mostly unseen water system at work during rocket engine tests at NASA’s Stennis Space Center near Bay St. Louis, Mississippi, underwent an upgrade in May.

Crews brought the High Pressure Industrial Water Facility’s 66-million-gallon reservoir to its lowest level since construction in the 1960s by pumping out about 40 million gallons of water over three days.

This brought the reservoir, measuring 800 feet in diameter and about 25 feet deep, down to the level needed to replace a 3,000 gallon per minute pump that supplies water for fire suppression to the test complexes.




before
after

A wide view of the High Pressure Industrial Water Facility reservoir at Stennis Space Center on May 7, filled nearly to capacity as crews begin removing water for facility upgrades.
The High Pressure Industrial Water Facility’s 66-million-gallon reservoir is shown at NASA’s Stennis Space Center on May 7 as work gets underway to remove about 40 million gallons of water to complete upgrades.
NASA/Danny Nowlin

The reservoir at Stennis Space Center on May 11 shown at a dramatically lowered level, exposing large areas of the reservoir floor after 40 million gallons were pumped out.
The reservoir is shown at NASA’s Stennis Space Center on May 11 at its lowest level since construction in the 1960s. Crews lowered the reservoir by pumping out about 40 million gallons over three days to complete upgrades.
NASA/Danny Nowlin

A wide view of the High Pressure Industrial Water Facility reservoir at Stennis Space Center on May 7, filled nearly to capacity as crews begin removing water for facility upgrades.
The High Pressure Industrial Water Facility’s 66-million-gallon reservoir is shown at NASA’s Stennis Space Center on May 7 as work gets underway to remove about 40 million gallons of water to complete upgrades.
NASA/Danny Nowlin

The reservoir at Stennis Space Center on May 11 shown at a dramatically lowered level, exposing large areas of the reservoir floor after 40 million gallons were pumped out.
The reservoir is shown at NASA’s Stennis Space Center on May 11 at its lowest level since construction in the 1960s. Crews lowered the reservoir by pumping out about 40 million gallons over three days to complete upgrades.
NASA/Danny Nowlin


before

after

Before and After

Lowering the Reservoir

May 7, 2026 – May 11, 2026


BEFORE (SSC-20260507-s00393) The High Pressure Industrial Water Facility’s 66-million-gallon reservoir is shown at NASA’s Stennis Space Center on May 7 as work gets underway to remove about 40 million gallons of water to complete upgrades. AFTER (SSC-20260511-s00420) The reservoir is shown at NASA’s Stennis Space Center on May 11 at its lowest level since construction in the 1960s. Crews lowered the reservoir by pumping out about 40 million gallons over three days to complete upgrades.

For a typical RS-25 engine test supporting NASA’s Artemis missions, about five million gallons of water flow from the reservoir to the Fred Haise Test Stand. The water cools the engine exhaust that reaches up to 6,000 degrees Fahrenheit, supplies water to the flame deflector and helps with sound suppression during a test.

A hot fire test produces critical data to ensure an engine is safe and reliable.




before
after

View from the Thad Cochran Test Stand showing the reservoir on May 7, still mostly full as work begins to remove water for upgrades.
A view from the Thad Cochran Test Stand at NASA’s Stennis Space Center on May 7 shows the High Pressure Industrial Water Facility’s 66-milion-gallon reservoir as work gets underway to remove about 40 million gallons of water to complete upgrades.
NASA/Danny Nowlin

View from the Thad Cochran Test Stand on May 11 showing the reservoir at its lowest level since the 1960s after extensive water removal.
A view from the Thad Cochran Test Stand at NASA’s Stennis Space Center on May 11 shows the reservoir at its lowest level since construction in the 1960s. Crews lowered the reservoir by pumping out 40 million gallons over three days to complete upgrades.
NASA/Danny Nowlin

View from the Thad Cochran Test Stand showing the reservoir on May 7, still mostly full as work begins to remove water for upgrades.
A view from the Thad Cochran Test Stand at NASA’s Stennis Space Center on May 7 shows the High Pressure Industrial Water Facility’s 66-milion-gallon reservoir as work gets underway to remove about 40 million gallons of water to complete upgrades.
NASA/Danny Nowlin

View from the Thad Cochran Test Stand on May 11 showing the reservoir at its lowest level since the 1960s after extensive water removal.
A view from the Thad Cochran Test Stand at NASA’s Stennis Space Center on May 11 shows the reservoir at its lowest level since construction in the 1960s. Crews lowered the reservoir by pumping out 40 million gallons over three days to complete upgrades.
NASA/Danny Nowlin


before

after

Before and After

A View from the Thad Cochran Test Stand

May 7, 2026 – May 11, 2026


BEFORE (SSC-20260507-s00395) – A view from the Thad Cochran Test Stand at NASA’s Stennis Space Center on May 7 shows the High Pressure Industrial Water Facility’s 66-milion-gallon reservoir as work gets underway to remove about 40 million gallons of water to complete upgrades. AFTER (SSC-20260511-s00423) – A view from the Thad Cochran Test Stand at NASA’s Stennis Space Center on May 11 shows the reservoir at its lowest level since construction in the 1960s. Crews lowered the reservoir by pumping out 40 million gallons over three days to complete upgrades.

The water used during a test is recycled for future use as it flows back into the on-site canal system, before returning to the reservoir.

“The old pump that supported fire suppression for testing reached its end of life, so this project promotes reliability with the upgrade,” said Justin Lucas, NASA project manager.

In addition to a new pump, the piping has improved to a 14-inch-to-12-inch configuration.

Picture trying to drink water from a big cup using a tiny coffee stirrer. This is similar to how the previous pump relied on piping that narrowed from 14 inches down to 10 inches before reaching the pump. The water moved but required more work from the system.

“With the upgraded configuration, less velocity inside the pipe with the same amount of flow equals a longer lasting pipe, pump, and hardware,” said Lucas.

The water system upgrades have strengthened a vital system that supports NASA’s Artemis missions, along with commercial companies operating at NASA Stennis, home to America’s largest multiuser propulsion test site.

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LaToya Dean

NASA Says Farewell to MAVEN Mars Mission, Hosts Media Call Today

NASA Says Farewell to MAVEN Mars Mission, Hosts Media Call Today

Artist’s concept of NASA’s MAVEN spacecraft at Mars. The spacecraft entered orbit around the planet in 2014 and has completed over eleven years of observing the Martian upper atmosphere, ionosphere, and interactions with the Sun and solar wind to explore the loss of the Red Planet’s atmosphere to space.
Credit: NASA/Goddard/University of Colorado/Laboratory for Atmospheric and Space Physics

The first mission devoted to observing the Martian atmosphere and its evolution, NASA’s MAVEN (Mars Atmosphere and Volatile Evolution), has ended after more than 11 years in orbit at Mars and a decade beyond its primary, one-year mission. The spacecraft was heard last on Dec. 6, when it experienced an unexpected loss of signal after it passed behind the Red Planet.

NASA will host a media teleconference at 2 p.m. EDT today, Wednesday, June 3, to discuss MAVEN’s achievements.

The agency convened an anomaly review board in February to evaluate recovery efforts and assess the spacecraft’s probable current state. The review board has determined that the MAVEN spacecraft is not recoverable, and it is no longer capable of performing its science and data relay mission, which is consistent with the mission team’s findings.

Telemetry from MAVEN prior to the spacecraft’s passage behind Mars in December showed all subsystems working normally. After the spacecraft emerged, NASA’s Deep Space Network (DSN) did not observe a signal. A brief fragment of telemetry data from analysis of radio signals recorded by the DSN’s open-loop receivers indicated the spacecraft was in safe mode and rotating at an unusually high rate when it emerged from behind Mars, indicating a disruption in MAVEN’s orbit trajectory. The review board concluded that due to this rotation, the batteries on the spacecraft had drained, causing the communications system to lose power and rendering MAVEN in an unrecoverable state.

These preliminary findings do not address a potential root cause for the anomaly, which still is being investigated. The review board is expected to provide its final report later this year. NASA has begun the official process of decommissioning the MAVEN mission, following standard procedures to archive the full mission dataset for the science and exploration communities.

“The science MAVEN has given us is key to informing what kind of radiation protection and safety measures we must take before sending humans to Mars,” said Louise Prockter, director of the Planetary Science Division at NASA Headquarters in Washington. “The data collected from MAVEN will continue to provide valuable insight into Mars for decades to come.”

Launched in November 2013, the MAVEN mission explored the Red Planet’s upper atmosphere, ionosphere, and interactions with the Sun to explore the loss of the Martian atmosphere to space. Understanding atmospheric loss gives scientists insight into the history of the planet’s atmosphere and climate, liquid water, and planetary habitability.

“The MAVEN mission has truly advanced our understanding of the Martian atmosphere and evolution. This dataset has had a tremendous impact on the field,” said Shannon Curry, MAVEN’s principal investigator and a researcher at the Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder. “Our science team is exceptionally proud of all of these amazing discoveries.”

Sun’s impact on Mars

One of MAVEN’s first major results was that the erosion of Mars’ atmosphere increases significantly during solar storms. The team studied how the solar wind, which is a stream of charged particles continually streaming from the Sun, and solar storms continually strip away Mars’ atmosphere, as well as how this process played a key role in altering the Martian climate from a potentially habitable world to today’s cold, arid planet. The MAVEN mission made unprecedented strides in advancing our understanding of how the Sun and space weather affect Mars, as it was the only spacecraft that could simultaneously take measurements of both the Sun and the Martian atmospheric response.

Martian light shows

The MAVEN mission discovered several types of auroras that light up when energetic particles plunge into the atmosphere, bombarding gases and making them glow. The MAVEN team showed that protons create new kinds of auroras at Mars. On Earth, proton auroras only occur in very small regions near the poles, whereas at Mars they can occur everywhere.

Mars’ atmosphere sputters into space

To better understand how Mars lost most of its atmosphere, MAVEN measured atmospheric sputtering for the first time at any planet. The team did this by observing argon, which is a noble gas, meaning it rarely reacts with other constituents in the Martian atmosphere. The only significant way it can be removed is by atmospheric sputtering, a process where ions crash into the Martian atmosphere at high enough speeds that they splash gas molecules out of the atmosphere, much like doing a cannonball into a pool. The team used 11 years of data to reveal the presence of sputtered argon at high altitudes in the exact locations that the energetic particles crashed into the atmosphere, showing sputtering in real time.

Understanding Mars’ dusty secrets

In 2018, a series of dust storms created a dust cloud so large that it enveloped the Red Planet. The MAVEN team studied how this “global” dust storm affected Mars’ upper atmosphere to understand how these events affected the escape of water to space. It confirmed that heating from dust storms can loft water molecules far higher into the atmosphere than usual, leading to a sudden surge in water lost to space.

Chasing comets

In addition to Martian science, MAVEN contributed to NASA’s effort to observe comet 3I/ATLAS at Mars. Over the course of 10 days last year, the MAVEN team designed a new observing campaign to capture 3I/ATLAS by taking multiple images of the comet in several wavelengths, much like using various filters on a camera. Then it snapped high-resolution UV images to identify the hydrogen coming from the comet. By studying a combination of these images, scientists can identify a variety of molecules and better understand the comet’s composition and history.  

During the mission’s lifetime, MAVEN’s science team produced more than 800 publications, and additional publications are planned.

In addition to science, the MAVEN spacecraft was an instrumental player in NASA’s Mars Relay Network, communicating data from Mars rovers to Earth. It also holds the solar system record for most data relayed from another planet in a single day.

Audio of today’s media teleconference will stream on the agency’s website at:

https://www.nasa.gov/live

Participants in the teleconference include:

  • Tiffany Morgan, director, Mars Exploration Program, Planetary Science Division, NASA Headquarters
  • Mike Moreau, project manager, MAVEN, NASA’s Goddard Space Flight Center, Greenbelt, Maryland
  • Greg Heckler, deputy program manager for Capability Development, SCaN (Space Communications and Navigation), NASA Headquarters
  • Shannon Curry, MAVEN principal investigator, Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder

To ask questions by phone, media must RSVP no later than 12 p.m. to: sarah.frazier@nasa.gov. NASA’s media accreditation policy is available online.

The MAVEN mission is part of NASA’s Mars Exploration Program portfolio. The mission’s principal investigator is based at the Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder, which also is responsible for managing science operations and public outreach and communications. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the MAVEN mission. Lockheed Martin Space built the spacecraft and is responsible for mission operations. NASA’s Jet Propulsion Laboratory in Southern California provides navigation and Deep Space Network support.  

For more information about NASA’s Mars Exploration Program, visit:

https://science.nasa.gov/planetary-science/programs/mars-exploration

-end-

Karen Fox / Alana Johnson
Headquarters, Washington
240-285-5155 / 202-672-4780
karen.c.fox@nasa.gov / alana.r.johnson@nasa.gov

Sarah Frazier
Goddard Space Flight Center, Greenbelt, Md.
202-853-7191
sarah.frazier@nasa.gov

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Jessica Taveau

Typhoon Jangmi

Typhoon Jangmi

A nighttime satellite image highlights the structure of a typhoon’s large eye and surrounding eyewall.

From late May into early June 2026, a broad, slow-spinning storm churned north-northwest over the Philippine Sea toward southern Japan. Typhoon Jangmi’s rainbands unleashed torrential rainfall across a vast swath of the region, triggering flooding concerns in several areas.

The VIIRS (Visible Infrared Imaging Radiometer Suite) on the Suomi NPP satellite captured this nighttime image (above) of the storm at about 16:40 Universal Time on May 30 (1:40 a.m. Japan Standard Time on May 31). Around that time, the typhoon produced sustained winds of 120 kilometers (75 miles) per hour, based on 1-minute averages reported by the Joint Typhoon Warning Center (JTWC). That’s equivalent to a category 1 storm on the Saffir-Simpson hurricane wind scale.

The image shows a detailed view of the eyewall and eye, with a diameter that is on the larger end of the spectrum, according to Scott Braun, a research meteorologist at NASA’s Goddard Space Flight Center. There also appears to be some low-level rotation on the eastern side of the eye, producing features known as “mesocyclones” that are partially obscured by high-level clouds. Though they appear striking, the features are fairly typical, Braun noted.

A nighttime satellite image shows a wide view of the typhoon with its outer cloud bands extending over southern Japan.

The second image shows a wider view of the same storm one day later. The VIIRS on the NOAA-20 satellite acquired this image at about 16:40 Universal Time on May 31 (1:40 a.m. Japan Standard Time on June 1), when the storm was a slightly stronger typhoon with sustained winds of 130 kilometers (80 miles) per hour.

In both images, Jangmi’s eye was still located south of Okinawa. However, the storm’s outer cloud bands already reached over land as the storm moved north. Forecasts called for the storm to make a close approach to Okinawa and then turn northeast toward the Amami region around June 1-2. It was expected to continue delivering large amounts of rain, especially along the nation’s Pacific coast, according to news reports.

NASA Earth Observatory images by Michala Garrison, using VIIRS day-night band data from NASA EOSDIS LANCEGIBS/Worldview, and the Joint Polar Satellite System (JPSS). Story by Kathryn Hansen.

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Bacteria, Cartilage, and Metal Tops Tuesday’s Research Aboard Station

Bacteria, Cartilage, and Metal Tops Tuesday’s Research Aboard Station

NASA astronaut and Expedition 74 Flight Engineer Chris Williams replaces sample hardware inside the Destiny laboratory module’s Microgravity Science Glovebox aboard the International Space Station to support semiconductor crystal research. Growing crystals in weightlessness may enable future large-scale semiconductor manufacturing, advancing the commercial space economy and supporting Earth-based industries.
NASA astronaut replaces sample hardware inside the Destiny laboratory module’s Microgravity Science Glovebox aboard the International Space Station to support semiconductor crystal research.
NASA/Jack Hathaway

Microbiology,  biotechnology, and physics were the dominant research themes aboard the International Space Station on Tuesday as the Expedition 74 crew explored how microgravity affects bacteria, cartilage growth, and metallic structure. Scientific hardware maintenance rounded out the schedule for the orbital residents to ensure continuous experimental operations.

NASA flight engineer Jack Hathaway reviewed procedures ahead of an investigation to explore how bacteria adapt to the space environment. Hathaway familiarized himself with the tools and steps he will use to study how two sets of bacterial samples respond to weightlessness. One set will be treated with an antibiotic and the second set will be left alone. After the samples are incubated for five days their DNA will be sequenced for more insight into microbial adaptation to microgravity. Results may lead to advanced efforts to reduce the risk of bacterial infection and help protect an astronaut’s immune system during a spaceflight.

NASA flight engineer Jessica Meir nourished cartilage tissue samples inside the Kibo laboratory module’s Life Science Glovebox that are growing to gain a better understanding of the function of cartilage cells and tissue in microgravity. The tissue samples are being engineered aboard the orbiting lab to understand how cartilage develops and repairs itself possibly improving astronaut fitness regimens and promoting the development of advanced implants on Earth.

NASA flight engineer Chris Williams inserted StarSteel samples, a high‑performance engineered metal or alloy, into the Mochii electron microscope to observe space-caused changes to the advanced material’s surface and structure. The physics research work may lead to the development of stronger, lighter, or more durable materials for Earth and space applications.

Flight engineer Sophie Adenot of ESA (European Space Agency) replaced a computer chip inside a research incubator located inside Kibo. Afterward, she updated the incubator’s network settings for the main internal memory chip that performs startup, runs experiments, stores data, and communicates with ground systems.

Roscosmos cosmonauts Sergey Kud-Sverchkov and Sergei Mikaev took turns on Tuesday studying how living in space affects blood pressure. The duo wore a set of cuffs attached to their arms, wrist, and fingers measuring their cardiac data helping doctors keep an eye on crew health and understand how weightlessness affects the circulatory system. Next, they joined Williams and tested the custom-fitted seat liners they will sit in next month when they return to Earth inside the Soyuz MS-28 spacecraft.

Roscosmos flight engineer Andrey Fedyaev spent the first half of his shift inside the Nauka science module working on orbital plumbing and ventilation maintenance. Afterward, Fedyaev cleaned gas-liquid heat exchangers, devices that ensure the space station’s temperature and humidity remain safe and comfortable, inside the Zarya module.

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

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Mark A. Garcia

NASA Space Roboticist Challenge

NASA Space Roboticist Challenge

Fly Foundational Robots (FFR) mission
Image Credit: Motiv Space Systems

The Fly Foundational Robots (FFR) mission will launch a robotic arm, with seven degrees of freedom, to low Earth orbit. NASA is opening access to the robotic arm to a select group of U.S. researchers — principal investigators, post-doctoral researchers, professors, and highly qualified graduate students — who have a compelling experiment and the capability to execute it.

All participants must submit eligibility documentation at registration. Once your eligibility is reviewed and confirmed, you will receive access to the Phase 1 submission portal.

  • Phase 0 — Eligibility Registration
    Begin by completing your eligibility registration. Submission documentation is required at this stage as part of federal competition requirements. Registration closes at 12:59 p.m. ET (11:59 p.m. CT) on Sept. 23.
  • Phase 1 — White Paper Submission
    Submit a white paper proposing a short, focused experiment using the FFR robotic arm. Up to 15 teams advance to Phase 2. Submission closes at 12:59 p.m. ET (11:59 p.m. CT) on Oct. 2.
  • Phase 2 — Simulation & Validation
    Invited participants conduct simulation and validation testing, including visits to Goddard Space Flight Center in Greenbelt, Maryland.

Prize: Teams that pass validation will receive an offer of on-orbit experiment time on the FFR Mission

Challenge Registration Open Date: May 20, 2026

Challenge Registration Close Date: September 23, 2026

For more information, visit: https://spaceroboticistchallenge.com/

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Bailey G. Light