NASA’s Hubble Telescope Reaches Milestone, Looks for Elusive Supernova

NASA’s Hubble Telescope Reaches Milestone, Looks for Elusive Supernova

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 captured this image of massive galaxy cluster MACS J0417 (left of center) on Sept. 19, 2026. This galaxy cluster acts as a gravitational lens, bending and magnifying light from objects far behind it. 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.

Hubble also 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.

Read more about Hubble and this recent milestone.

Image credit: NASA, ESA, STScI, M. Pascale (UCLA); Image Processing: J. DePasquale (STScI)

Powered by WPeMatico

Get The Details…
HQ Web Team

Arctic Sea Ice Reaches 2026 Annual Minimum Extent

Arctic Sea Ice Reaches 2026 Annual Minimum Extent

Daily images of ice cover in the Arctic Ocean show sea ice melting around the pole from March 15, 2026 to Sept. 12, 2026.
Trent Schindler/NASA’s Scientific Visualization Studio

Arctic sea ice reached its annual minimum extent on Sept. 12, according to NASA and the National Snow and Ice Data Center (NSIDC) at the University of Colorado Boulder. The ice covered an estimated 1.78 million square miles (4.6 million square kilometers), tying 2008, 2010, and 2025 for the 10th-lowest minimum in the satellite record.

The 2026 minimum is consistent with patterns observed in the satellite record. The past 20 years, from 2007 through 2026, have produced the 20 lowest annual Arctic sea ice minimum extents observed since continuous satellite measurements began in late 1978.

Arctic sea ice grows during the dark, cold autumn and winter and retreats as temperatures rise during spring and summer, typically reaching its lowest extent in September. Weather conditions can cause substantial differences in the amount of ice that melts from one summer to another.

Over the last decade, for example, increased cloud cover has prevented solar radiation from further accelerating the melt of sea ice, according to Linette Boisvert, a sea ice scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

That has contributed to relatively stable September sea ice extent in recent years. “We’ve plateaued, but we’re still low relative to the earlier part of the record,” said Walt Meier, a senior research scientist at NSIDC.

Antarctic sea ice extent approaches annual maximum

At the opposite end of the planet, Antarctic sea ice is approaching its annual maximum following a fluctuation during August.

Sea ice around Antarctica declined by roughly 116,000 square miles (300,000 square kilometers) over a six-day period before resuming its seasonal growth. Meier said the decline appeared to be associated with weather conditions that pushed and compacted the thin, mobile ice near its outer edge.

“Those types of things happen all the time,” Meier said. “But the magnitude of it certainly is unusual.”

Antarctic sea ice varies more from year to year than Arctic sea ice because, in contrast to the Arctic, it is not surrounded by land and can respond more freely to changing wind and weather conditions. But Antarctic sea ice extent at its annual maximum has generally been lower in recent years. Because of this large year-to-year variability, Boisvert and Meier remain cautious about characterizing the change as a long-term trend.

Scientists have tracked polar sea ice from space for nearly five decades. During that time, NASA and the National Oceanic and Atmospheric Administration (NOAA) used a series of satellite instruments to maintain a continuous sea ice record, beginning with NASA’s Nimbus-7 satellite, which began observations in October 1978. The record continued with instruments aboard Defense Meteorological Satellite Program satellites beginning in 1987 and NASA’s Aqua satellite from 2002 to 2011. Today, scientists continue the record using data from the Advanced Microwave Scanning Radiometer 2 (AMSR2), launched in 2012 aboard JAXA’s (Japan Aerospace Exploration Agency) GCOM-W satellite.

Antarctic sea ice typically reaches its annual maximum in late September or early October. NASA and NSIDC will announce the 2026 maximum after scientists confirm that seasonal ice growth has ended.

Media contact: Elizabeth Vlock
NASA Headquarters

Powered by WPeMatico

Get The Details…

Shannon Lucid’s Record-Setting Mission Aboard Mir

Shannon Lucid’s Record-Setting Mission Aboard Mir

Shannon Lucid on Mir looking at wheat growing in a small greenhouse
Astronaut Shannon W. Lucid checked on wheat plants aboard Russia’s Mir Space Station on Sept. 23, 1996. Lucid left Mir later that day along with the rest of the STS-79 crew except for John E. Blaha, who was beginning a four-month stay aboard the station.
NASA

Shannon Lucid’s Record-Setting Mission Aboard Mir 

Three days before returning to Earth, Shannon W. Lucid—who joined NASA in 1978 as one of its first six female astronauts—checked in on wheat growing in the Svet greenhouse aboard the Russian space station Mir. For six months, Lucid lived and worked alongside two Russian cosmonauts conducting life science studies and other experiments in microgravity.

Lucid returned to Earth aboard space shuttle Atlantis on Sept. 26, 1996, completing a 188-day mission—a new record for both a woman and for an American. Lessons from her time on Mir helped NASA prepare for the psychological and cultural challenges of long-duration missions on the International Space Station.  

In December 1996, President Bill Clinton awarded Shannon Lucid the Congressional Space Medal of Honor for her achievement. She was the tenth person and the first woman to receive this award.

After her mission on Mir, Lucid continued to serve NASA in key roles on the ground. She worked as a CAPCOM in Mission Control, where she was the primary voice communicating with astronauts in orbit. Later, she served as NASA’s Chief Scientist, helping guide the agency’s science priorities. Lucid retired from NASA in 2012 after a career that spanned more than three decades.

Share

Details

Last Updated

Sep 23, 2026

Powered by WPeMatico

Get The Details…
Michele Ostovar

FFA 2026 Hyperwall Schedule

FFA 2026 Hyperwall Schedule

FFA 2026

Join NASA in the Exhibit Hall (Booth #648) for Hyperwall Storytelling by NASA experts. Full Hyperwall Agenda below.

TUESDAY, OCTOBER 20

10:00 AM NISAR Updates, One Year After Launch Paul Rosen, Marco Lavelle 
10:15 AM NOAA Geostationary Satellites: Valuable Data for both Research and Operational Use Dan Lindsey
3:00 PM  Discovering Mineral Resources with NASA Imaging Spectroscopy Robert O. Green
3:15 PM 
The Importance of Satellite Ocean Observations at NOAA
Paul Chang

Powered by WPeMatico

Get The Details…

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

Download the PDF version

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.

Powered by WPeMatico

Get The Details…
Meagan Chappell