Risk of Hydrazine Use Following Freeze–Thaw Exposure

Risk of Hydrazine Use Following Freeze–Thaw Exposure

For more information, contact Jonathan E. Jones, Langley Research Center, jonathan.e.jones@nasa.gov

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The purpose of this Technical Bulletin is to communicate the risks associated with freeze–thaw cycles in hydrazine monopropellant systems and to provide general recommendations for mitigating damage, operational hazards, and loss of system reliability in propulsion and auxiliary hydrazine systems.

Background
Hydrazine (N2H4) freezes near 1.6°C, and its phase transition is known to introduce risks to flight hardware. Multiple NASA programs have historically encountered hydrazine freeze related issues:

• Space Shuttle APU hydrazine lines were vulnerable to freeze induced contraction followed by thaw induced over expansion, capable of bursting plumbing. Shuttle flight rules permitted no more than two freeze–thaw cycles before considering the system degraded or failed.1

• Voyager propulsion systems faced mission threatening scenarios as hydrazine temperatures approached the freezing/slush formation range (0.1–1.6°C). Detailed thermal modeling was required to prevent freezing of lines, blockage, and thruster malfunction.2

• Hydrazine thermodynamic properties confirm significant changes in density and pressure across phase transitions, emphasizing the sensitivity of propellant lines to freeze–thaw stress.3

These combined lessons form the basis for risk identification and mitigation.

Problem Summary
Freeze–thaw exposure of hydrazine systems presents the following critical risks:

• Structural Damage Hydrazine contraction during freezing allows additional propellant into confined lines, producing “superpacked” conditions that cause line or fitting rupture upon thaw.2

• Valve, Seal, and Diaphragm Compromise Elastomeric components and precision valve seats may experience cracking, distortion, or loss of sealing capability due to differential thermal expansion. Voyager thermal assessments highlighted susceptibility of long stainless steel runs to asymmetric temperature profiles.2

• Line Blockage and Slush Formation Partially thawed hydrazine can remain “slushy,” restricting flow, altering mass flow rates, and causing thruster hard starts or misfires.2

• Hazardous Leaks Freeze induced damage may allow hydrazine to escape confinement, posing significant toxicity, reactivity, and ground crew exposure hazards.

• Loss of System Reliability As documented in Shuttle operations, hydrazine systems exposed to freeze–thaw cycles become life limited, reducing redundancy and mission availability.1

• Thermal Margin Uncertainty Voyager experience demonstrated that simple temperature readings cannot reliably determine true line temperature, necessitating high fidelity thermal modeling.2

Recommendations Prevention Measures
• Maintain Hydrazine Above Freezing Margin Keep all hydrazine systems above freezing, using heaters, insulation, blankets, or warm gas purge. Include uncertainty analysis in modeling and testing to ensure appropriate margins against freezing are maintained during all phases of operation.

• Avoid Uncontrolled Cooling During Ground Operations Ensure that tank, line, and valve components remain in environmentally controlled areas until integrated into the vehicle.

Post Freeze Response Protocol
If freezing cannot be ruled out:

• Suspend System Use Do not operate the hydrazine system until engineering evaluation is completed.

• Assess Number of Freeze–Thaw Cycles Treat each cycle as life limiting, an engineering assessment (static and fatigue) should be conducted based on conservative estimates of the line pressures during/after freeze/thaw cycles to understand potential line/component damage. Appropriate margin should be applied based on analysis uncertainty and/or underlying assumptions.

• Conduct Integrity Verification Perform pressure decay tests, NDE (if design allows), and valve health assessments.

• Implement Slow, Uniform Thawing To prevent thaw induced over pressure, warm hardware gradually and evenly. Shuttle experience with “superpacking” reinforces the necessity of controlled thawing.

Thruster and Valve Operational Readiness
• Ensure catalyst beds and valves reach proper thermal operating conditions before commanding any flow.

• Conduct pre start thermal stabilization periods, especially when flight readiness temperatures are marginal.

Thermal Modeling and Monitoring
• Utilize high fidelity thermal line modeling, emulating Voyager’s detailed propellant line modeling approach.2

• Avoid relying solely on bulk plate or tank temperatures to infer line readiness.

• Use thermal analysis and test to guide instrumentation placement on of the flight systems to monitor key temperatures set points.

Documentation and Incident Tracking
• Record all freeze exposures as reportable anomalies.

•Assign engineering disposition and track hardware life reduction accordingly.

Conclusion
Hydrazine freeze–thaw cycles present significant structural, operational, and safety risks for propulsion and auxiliary systems. Historical NASA programs show that prevention of hydrazine freezing is the most effective mitigation, with freeze exposure requiring formal engineering assessment, life limit adjustments, and controlled recovery procedures. Adhering to these recommendations will reduce risk to personnel, flight hardware, and mission success.

References
1. Space Shuttle Operational Flight Rules, Vol. A. All Flights, Mission Operations Diretorate, 20 June 2002. 2. W. C. Ledeboer, “Creating a Voyager Thermal Model 39 Years Into the Flight Mission, Along With Model Correlation and Application,” 8 July 2018. 3. J. L. Haws and B. G. Harden, “Thermodynamic Properties of Hydrazine,” Nov 1965.

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Meagan Chappell

NASA’s Hubble Seeks Lensed Supernova, Marks 200,000 Orbits

NASA’s Hubble Seeks Lensed Supernova, Marks 200,000 Orbits

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NASA’s Hubble Seeks Lensed Supernova, Marks 200,000 Orbits

Several galaxies shine against black space, with a large cluster near center-left.
An image from NASA’s Hubble Space Telescope of galaxy cluster MACS J0417 is part of repeated observations to monitor for the reappearance of supernova Athena, which can help astronomers measure the expansion rate of the universe.
NASA, ESA, STScI, M. Pascale (UCLA); Image Processing: J. DePasquale (STScI)

NASA’s Hubble Space Telescope completed its 200,000th orbit around Earth on Sept. 19, marking another new milestone for an observatory that continues to transform our understanding of the universe.

Hubble has traveled more than 5 billion miles around Earth over its 36-year lifetime, exceeding 1.7 million total observations. An observation completed on the day of the 200,000th orbit pertains to one of Hubble’s defining scientific legacies: measuring the expansion rate of the universe, or the Hubble Constant. The image takes advantage of the telescope’s ability to return to the same regions of the sky over time to monitor for the reappearance of a supernova, or explosion of a star, called Athena.

Massive galaxy cluster MACS J0417, located at the left center of the image, acts as a gravitational lens, bending and magnifying light from objects far behind it. Light from a supernova can reach Earth along multiple paths, causing the same stellar explosion to appear more than once at times separated by months or even years depending on the path it took. Supernova Athena, discovered by NASA’s James Webb Space Telescope in 2025, is predicted to reappear between now and early March 2027. Measuring the timing of Athena’s reappearances can help researchers map the mass of MACS J0417, which acts as a magnifying, foreground lens for distant objects, and refine our understanding of the expansion rate of the universe.

After more than 36 years in space, Hubble still is reaching new heights of scientific productivity and impact. Hubble’s unique ability to observe and analyze light in ultraviolet and visible wavelengths complements NASA’s James Webb and Roman Space Telescopes’ capabilities. As a result, demand for Hubble observing time remains high as astronomers request about seven times as much observing time as is available each year.

Hubble continues to observe targets across every area of astronomy around the clock, with real-time tracking of those observations available on NASA’s website.

Media Contact:

Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, MD
claire.andreoli@nasa.gov

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Sep 23, 2026
Editor
Michelle Belleville

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APOD: 2026 September 23 – A New Lunar Crater: McGetchin

APOD: 2026 September 23 – A New Lunar Crater: McGetchin

APOD

Astronomy Picture of the Day

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

An image of the lunar surface with a large depression at the center surrounded by raised ridges that slope down back to the surface.An image of the lunar surface speckled wth impressions (craters) of various small sizes.

A New Lunar Crater: McGetchin

Explanation: A once-in-a-lifetime crater has appeared on the Moon! A comet or asteroid roughly the size of a humpback whale (approximately 10-20 meters, 30-60 feet) crashed into the Moon sometime between April and May of 2024. The Lunar Reconnaissance Orbiter (LRO), with its monthly monitoring of the Moon, captured today’s images of the lunar surface before and after the event. The resulting crater, named after Apollo-era lunar scientist McGetchin, is two soccer fields across. Craters of this size are only expected once every 132 years! Follow up thermal imaging revealed a large cold spot that surrounds the warm crater. Surface impacts will puff up the loose lunar sediment, or regolith, making it less dense and harder to retain heat. This event affected an area much larger than the visible crater, which will inform humanity’s understanding of surface impacts and the evolution of the Moon’s surface. It also reminds us all to be thankful for Earth’s atmosphere.

APOD’s submission email has changed. Please see APOD Submissions.
APOD’s main NASA site is moving: From apod.nasa.gov to science.nasa.gov/apod
Tomorrow’s picture: the great unknown

Date: September 23, 2026
Credit: NASA/GSFC/Intuitive Machines
Authors & editors: Keighley Rockcliffe, Robert Nemiroff, Jerry Bonnell, Cecilia Chirenti
A service of: ASD at NASA / GSFC,
NASA Science Activation & Michigan Tech. U.

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Boom Year for Desert Blooms

Boom Year for Desert Blooms




August 19, 2025
August 30, 2026

Branching riverbeds and roads cut through rusty orange land in the Western Australian outback.
Branching riverbeds and roads cut through rusty orange land in the Western Australian outback.
NASA Earth Observatory / Lauren Dauphin

Land in the Western Australian outback appears mostly rusty orange but contains areas of green, especially in riverbeds.
Land in the Western Australian outback appears mostly rusty orange but contains areas of green, especially in riverbeds.
NASA Earth Observatory / Lauren Dauphin

Branching riverbeds and roads cut through rusty orange land in the Western Australian outback.
Branching riverbeds and roads cut through rusty orange land in the Western Australian outback.
NASA Earth Observatory / Lauren Dauphin
Land in the Western Australian outback appears mostly rusty orange but contains areas of green, especially in riverbeds.
Land in the Western Australian outback appears mostly rusty orange but contains areas of green, especially in riverbeds.
NASA Earth Observatory / Lauren Dauphin

August 19, 2025

August 30, 2026


Arid shrublands in Western Australia were bursting with life in late austral winter 2026, when a profusion of wildflowers brought vivid colors to the rusty ochre landscape. After several wetter-than-normal months earlier in the year, dormant seeds in the soil awoke to produce carpets of blooms. Local experts think the display could be the best the area has seen in nearly two decades.

The images above, captured with the OLI (Operational Land Imager) on the NASA-USGS Landsat 8 satellite, compare the more verdant landscape of late August 2026 (right) with a similar time in 2025 (left), when it was drier. This area is located about 600 kilometers (370 miles) north of Perth in the Murchison region, one of Western Australia’s main areas for grazing sheep and cattle. The local vegetation includes grasses, saltbush, and the slow-growing evergreen mulga tree.

White flowers cover the ground amid sparsely spaced shrubby trees.
White flowers carpet the Western Australian outback.
© CSIRO Australia, September 16, 2026

Every so often, a variety of wildflowers makes an appearance, too. In 2026, rainfall totals were above average in June and very much above average in August due to several cold fronts moving through the area, according to Australia’s Bureau of Meteorology. The rains helped rouse a diverse mix of flowers to bloom across the outback, including on a radio astronomy site managed by the Commonwealth Scientific and Industrial Research Organisation (CSIRO), Australia’s national science agency. The flower show included some threatened species, which the observatory has helped monitor on its formerly pastoral land.

Though the spectacle underfoot might have momentarily stolen the show, Inyarrimanha Ilgari Bundara, the CSIRO Murchison Radio-astronomy Observatory, is primarily focused on what’s overhead and the exploration of deep space. At the Murchison site, CSIRO operates several antenna arrays that observe and catalog objects in the southern sky. The remote facility is situated within a “radio quiet” zone, where terrestrial communications and electronic devices are controlled to limit electromagnetic interference with the instruments.

A field of pink wildflowers occupies the foreground. Four white dish antennas, part of a radio astronomy observatory, are out of focus in the background.
Mulla mulla flowers appear in front of CSIRO’s Australian Square Kilometre Array Pathfinder (ASKAP) radio telescope.
© CSIRO Australia, September 16, 2026

Other telescopes in CSIRO’s purview in Australia have played crucial roles in NASA missions from the agency’s early years to today. The Murriyang radio telescope in Parkes, New South Wales, tracked Mariner 2—the first successful planetary science mission—in 1962 and was an important receiving station for the Apollo 11 mission to the Moon in 1969. CSIRO also manages and operates the Canberra Deep Space Communication Complex, one of three facilities in NASA’s global Deep Space Network that supports interplanetary spacecraft missions and collects radar and radio astronomy observations. Both supported the Artemis II mission in April 2026.

NASA Earth Observatory images by Lauren Dauphin, using Landsat data from the U.S. Geological Survey. Photos © CSIRO Australia, September 16, 2026. Story by Lindsey Doermann.

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A grayscale image of the Martian surface taken by the Curiosity rover. The immediate foreground features a dense field of jagged, light-colored, thinly-layered rock fragments resting on a bed of darker sand or dust. The barren terrain gently slopes upward toward the horizon, where a cluster of dark, rugged hills and a larger, rounded mountain peak on the far right stand out against a smooth, featureless sky.
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NASA/JPL-Caltech

Catherine O’Connell-Cooper, APXS Strategic Planner and Payload Uplink/Downlink Lead, University New Brunswick, NB, Canada

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This week we had two planning days (Tuesday and Friday), as Monday was Labor Day in North America, where many of the Curiosity team are based. Labor Day (the first Monday in September) marks the end of summer holidays and thrills, and the return to more typical routines and back to school.

The MSL team has marked several important milestones within the past few weeks — marking our 14th “Landiversary” on Aug. 6 and surpassing the 1-kilometer elevation mark and our 5000th sol (Martian day) in early September. Our next big date is not until Nov. 26, the 15th anniversary of launch, and so it feels like Curiosity is also back to a more routine schedule at this point.

We are moving up the valley known informally as “Valle Grande.” In recent weeks, we climbed up over what we interpreted as an “erosional supersurface” (which marks a gap in the usual rock record) and are now traversing through a subtly banded area. Bands are 25-200 meters (about 80-650 feet) in diameter, with morphological changes, such as bands with more sand and less rocky outcrops (which often appear darker from a distance because there is more sand) and others where outcrops seem more continuous that allow us to mark out rough contacts between them.  

The terrain this week was characterized by sparse outcrops with a rough texture, often nodular, surrounded by lots of sand and coarse pebbly sand. On Tuesday APXS and MAHLI investigated brushed nodular bedrock at “Cerro Armazones” and “Monte Melimoyu.” ChemCam acquired LIBS on a knot of dark-toned nodules at “Tuta Huallpas” and the dark-toned float rock “Acllahuasi.”

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Across both plans, the ChemCam long-distance imager and camera teams were hard at work. In addition to near-field images, which focus on areas close to the rover, both Mastcam and ChemCam acquired several larger mosaics on the buttes on either side of us (“Mishe Mokwa” and “Cordillera”) and looking back to the small butte “La Linea.” Mastcam also took some mosaics documenting the “Chocolatal” scuff, which we analyzed last week, and a larger mosaic of the “Sullivan Field” sand field where Chocolatal is located. Sullivan Field contains sand ripples, mega ripples, and transverse aeolian ridges, and was named by the team in honor of the late Robert Sullivan, a world expert on Martian sands and cherished member of the Curiosity science team.

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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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Last Updated
Sep 22, 2026

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