NASA Astronauts Send Independence Day Message Before Cargo Mission Launches

NASA Astronauts Send Independence Day Message Before Cargo Mission Launches

NASA’s Expedition 73 Flight Engineers Anne McClain, Nichole Ayers, and Jonny Kim called down to Earth from the International Space Station and shared an Independence Day message in this video recorded on June 16, 2025.

The NASA trio along with their Expedition 73 crewmates station Commander Takuya Onishi of JAXA (Japan Aerospace Exploration Agency) and Roscosmos Flight Engineers Sergey Ryzhikov, Alexey Zubritskiy, and Kirill Peskov relaxed the day before the U.S. holiday. Their Axiom Mission 4 (Ax-4) visitors also had an off-duty day. Ax-4 private astronauts Peggy Whitson, Shubhanshu Shukla, Sławosz Uznański-Wiśniewski, and Tibor Kapu will resume their science-packed schedule on Friday and work into the weekend.

Roscosmos’ Progress 92 resupply ship is counting down to its launch at 3:32 p.m. EDT on today from the Baikonur Cosmodrome in Kazakhstan. The Progress is scheduled to dock to the Poisk module at 5:27 p.m. on Saturday delivering about three thousand pounds of food, fuel and supplies for the orbiting lab residents. NASA+ will provide live coverage of both events.

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

Brain Research Continues on Station Ahead of Cargo Mission Launch

Brain Research Continues on Station Ahead of Cargo Mission Launch

NASA astronauts (from left) Anne McClain and Nichole Ayers, both Expedition 73 flight engineers, pose for a portrait inside the cupola while monitoring the SpaceX Dragon spacecraft carrying the Axiom Mission 4 crew as it approaches the Interntional Space Station.
NASA astronauts (from left) Anne McClain and Nichole Ayers pose for a portrait inside the cupola while monitoring the SpaceX Dragon spacecraft carrying the Axiom Mission 4 crew as it approached the International Space Station on June 26, 2025.
NASA

Brain research continued aboard the International Space Station on Wednesday as the Expedition 73 and Axiom Mission 4 (Ax-4) crews kept up their ongoing space biology studies. Meanwhile, a Progress cargo craft counts down to its launch to resupply the orbital residents this weekend.

NASA Flight Engineer Nichole Ayers took her turn today in the Columbus laboratory module wearing neck and chest electrodes measuring oscillations in the blood flow from her brain to the heart for the Drain Brain 2.0 human research experiment. Similarly, Ax-4 private astronaut Tibor Kapu wore a cap that imaged blood flow in his cerebral artery using doppler ultrasound for the Cerebral Hemodynamics investigation. Veteran astronaut and Ax-4 Commander Peggy Whitson assisted Kapu with the biomedical hardware and measured his blood pressure inside the Tranquility module. Both studies are supported by different organizations with the first seeking to prevent space-caused blood clots and the second to protect crew visual processing and perception in microgravity.

Ayers later joined her station crewmates Commander Takuya Onishi of JAXA (Japan Aerospace Exploration Agency) and NASA Flight Engineer Anne McClain for eye checks using high-resolution, near-infrared medical imaging hardware. McClain led the B Complex optical investigation in the Harmony Module as Ayers and Onishi peered into the ocular device while doctors on the ground examined their optic nerve at the back of the eye in real time. Researchers are exploring using B vitamin supplements as a method to protect crew vision in microgravity.

NASA Flight Engineer Jonny Kim began his shift inspecting portable emergency hardware including fire extinguishers and breathing masks. After his lunch period, he joined his Soyuz MS-27 crewmates Sergey Ryzhikov and Sergey Zubritskiy, both flight engineers from Roscosmos, and practiced using respirator masks in the unlikely event of a chemical leak onboard the orbital outpost.

Ryzhikov and Zubritskiy started their shift repairing a Roscosmos treadmill in the Zvezda service module. Ryzhikov also wore virtual reality glasses for a study observing how a crew member’s balance and visual perception adjust to microgravity. Zubritskiy serviced research physics hardware that measures neutron radiation. Flight Engineer Kirill Peskov spent his shift in the orbital outpost’s Roscosmos segment servicing orbital plumbing gear and activating Earth observation equipment.

Ax-4 crewmates Shubhanshu Shukla and Sławosz Uznański-Wiśniewski partnered together in Columbus and studied using near-infrared technology to record brain activity for constructing brain-computer interfaces. Uznański-Wiśniewski wore a specialized cap connected via Bluetooth to a laptop computer recording his brain activity while Shukla optimized the signal quality and calibrated the hardware. The pair also recorded and downlinked video of crew activities for the Astronaut Mental Health study. Shukla also looked at muscle cell stem cultures through a microscope to understand the muscle repair process in weightlessness.

The next uncrewed cargo mission, Progress 92, is counting down to its launch at 3:32 p.m. EDT on Thursday from the Baikonur Cosmodrome in Kazakhstan. Progress 92 is scheduled to dock to the Poisk module at 5:27 p.m. on Saturday delivering about three thousand pounds of food, fuel and supplies for the orbiting lab residents. NASA+ will provide live coverage of both events.

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 Remembers Former Johnson Director Jefferson Howell

NASA Remembers Former Johnson Director Jefferson Howell

NASA Director Howell giving a speech
Former Johnson Director Jefferson Howell

July 3, 2025

Jefferson Davis Howell, Jr., former director of NASA’s Johnson Space Center in Houston, died July 2, in Bee Cave, Texas. He was 85 years old.

Howell was a champion of the construction of the International Space Station, working on a deadline to complete the orbiting lab by 2004. He oversaw four space shuttle crews delivering equipment and hardware to reach that goal. He also served as director during a pivotal moment for the agency: the loss of STS-107 and the crew of space shuttle Columbia. He made it his personal responsibility to meet with the families, look after them, and attend memorial services, all while keeping the families informed of the accident investigation as it unfolded.

“Gen. Howell led NASA Johnson through one of the most difficult chapters in our history, following the loss of Columbia and her crew,” said acting associate administrator Vanessa Wyche. “He brought strength and steady direction, guiding the workforce with clarity and compassion. He cared deeply for the people behind the mission and shared his leadership skills generously with the team. We extend our heartfelt condolences to his family and all who knew and loved him.”

At the time of his selection as director, he was serving as senior vice president with Science Applications International Corporation (SAIC) as the program manager for the safety, reliability, and quality assurance contract at Johnson. Following the accident, he made it his mission to improve the relationship between the civil servant and contractor workforce. He left his position and the agency, in October 2005, shortly after the Return-to-Flight mission of STS-114.

“General Howell stepped into leadership at Johnson during a pivotal time, as the International Space Station was just beginning to take shape. He led and supported NASA’s successes not only in space but here on the ground — helping to strengthen the center’s culture and offering guidance through both triumph and tragedy,” said Steve Koerner, Johnson Space Center’s acting director. “On behalf of NASA’s Johnson Space Center, we offer our deepest sympathies to his family, friends, and all those who had the privilege of working alongside him. The impact of his legacy will continue to shape Johnson for decades to come.”

The Victoria, Texas, native was a retired lieutenant general in the U.S. Marine Corps with a decorated military career prior to his service at NASA. He flew more than 300 combat missions in Vietnam and Thailand.

Howell is survived by his wife Janel and two children. A tree dedication will be held at NASA Johnson’s memorial grove in the coming year.

-end-

Chelsey Ballarte

Johnson Space Center, Houston

281-483-5111

chelsey.n.ballarte@nasa.gov

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Wendy K. Avedisian

NASA Mission Monitoring Air Quality from Space Extended 

NASA Mission Monitoring Air Quality from Space Extended 

4 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Since launching in 2023, NASA’s Tropospheric Emissions: Monitoring of Pollution mission, or TEMPO, has been measuring the quality of the air we breathe from 22,000 miles above the ground. June 19 marked the successful completion of TEMPO’s 20-month-long initial prime mission, and based on the quality of measurements to date, the mission has been extended through at least September 2026. The TEMPO mission is NASA’s first to use a spectrometer to gather hourly air quality data continuously over North America during daytime hours. It can see details down to just a few square miles, a significant advancement over previous satellites.

“NASA satellites have a long history of missions lasting well beyond the primary mission timeline. While TEMPO has completed its primary mission, the life for TEMPO is far from over,” said Laura Judd, research physical scientist and TEMPO science team member at NASA’s Langley Research Center in Hampton, Virginia. “It is a big jump going from once-daily images prior to this mission to hourly data. We are continually learning how to use this data to interpret how emissions change over time and how to track anomalous events, such as smoggy days in cities or the transport of wildfire smoke.” 

By measuring nitrogen dioxide (NO2) and formaldehyde (HCHO), TEMPO can derive the presence of near-surface ozone. On Aug. 2, 2024 over Houston, TEMPO observed exceptionally high ozone levels in the area. On the left, NO2 builds up in the atmosphere over the city and over the Houston Ship Channel. On the right, formaldehyde levels are seen reaching a peak in the early afternoon. Formaldehyde is largely formed through the oxidation of hydrocarbons, an ingredient of ozone production, such as those that can be emitted by petrochemical facilities found in the Houston Ship Channel.
Trent Schindler/NASA’s Scientific Visualization Studio

When air quality is altered by smog, wildfire smoke, dust, or emissions from vehicle traffic and power plants, TEMPO detects the trace gases that come with those effects. These include nitrogen dioxide, ozone, and formaldehyde in the troposphere, the lowest layer of Earth’s atmosphere.

“A major breakthrough during the primary mission has been the successful test of data delivery in under three hours with the help of NASA’s Satellite Needs Working Group. This information empowers decision-makers and first responders to issue timely air quality warnings and help the public reduce outdoor exposure during times of higher pollution,” said Hazem Mahmoud, lead data scientist at NASA’s Atmospheric Science Data Center located at Langley Research Center.

…the substantial demand for TEMPO’s data underscores its critical role…

hazem mahmoud

hazem mahmoud

NASA Data Scientist

TEMPO data is archived and distributed freely through the Atmospheric Science Data Center. “The TEMPO mission has set a groundbreaking record as the first mission to surpass two petabytes, or 2 million gigabytes, of data downloads within a single year,” said Mahmoud. “With over 800 unique users, the substantial demand for TEMPO’s data underscores its critical role and the immense value it provides to the scientific community and beyond.” Air quality forecasters, atmospheric scientists, and health researchers make up the bulk of the data users so far.

On April 14, strong winds triggered the formation of a huge dust storm in the U.S. central plains and fueled the ignition of grassland fires in Oklahoma. On the left, the NO2 plumes originating from the grassland fires are tracked hour-by-hour by TEMPO. Smoke can be discerned from dust as a source since dust is not a source of NO2. The animation on the right shows the ultraviolet (UV) aerosol index, which indicates particulates in the atmosphere that absorb UV light, such as dust and smoke.
Trent Schindler/NASA’s Scientific Visualization Studio

The TEMPO mission is a collaboration between NASA and the Smithsonian Astrophysical Observatory, whose Center for Astrophysics Harvard & Smithsonian oversees daily operations of the TEMPO instrument and produces data products through its Instrument Operations Center.

Datasets from TEMPO will be expanded through collaborations with partner agencies like the National Oceanic and Atmospheric Administration (NOAA), which is deriving aerosol products that can distinguish between smoke and dust particles and offer insights into their altitude and concentration.

On May 5, TEMPO measured NO2 emissions over the Twin Cities in the center of Minnesota during morning rush hour. The NO2 increases seen mid-day through the early evening hours are illustrated by the red and black shaded areas at the Red River Valley along the North Dakota state line. These levels are driven by emissions from the soils in agriculturally rich areas. Agricultural soil emissions are influenced by environmental factors like temperature and moisture as well as fertilizer application. Small fires and enhancements from mining activities can also be seen popping up across the region through the afternoon.
Trent Schindler/NASA’s Scientific Visualization Studio

“These datasets are being used to inform the public of rush-hour pollution, air quality alerts, and the movement of smoke from forest fires,” said Xiong Liu, TEMPO’s principal investigator at the Center for Astrophysics Harvard & Smithsonian. “The library will soon grow with the important addition of aerosol products. Users will be able to use these expanded TEMPO products for air quality monitoring, improving forecast models, deriving pollutant amounts in emissions and many other science applications.”

A map of North America shows several wide swaths of purple illustrating smoke in the atmosphere as measured by NASA's TEMPO instrument during wildfires in Manitoba from June 2, 2025.
The TEMPO mission detects and highlights movement of smoke originating from fires burning in Manitoba on June 2. Seen in purple hues are observations made by TEMPO in the ultraviolet spectrum compared to Advanced Baseline Imagers (ABIs) on NOAA’s GOES-R series of weather satellites that do not have the needed spectral coverage. The NOAA GOES-R data paired with NASA’s TEMPO data enhance state and local agencies’ ability to provide near-real-time smoke and dust impacts in local air quality forecasts.
NOAA/NESDIS/Center for Satellite Applications and Research

“The TEMPO data validation has truly been a community effort with over 20 agencies at the federal and international level, as well as a community of over 200 scientists at research and academic institutions,” Judd added. “I look forward to seeing how TEMPO data will help close knowledge gaps about the timing, sources, and evolution of air pollution from this unprecedented space-based view.”

An agency review will take place in the fall to assess TEMPO’s achievements and extended mission goals and identify lessons learned that can be applied to future missions.

The TEMPO mission is part of NASA’s Earth Venture Instrument program, which includes small, targeted science investigations designed to complement NASA’s larger research missions. The instrument also forms part of a virtual constellation of air quality monitors for the Northern Hemisphere which includes South Korea’s Geostationary Environment Monitoring Spectrometer and ESA’s (European Space Agency) Sentinel-4 satellite. TEMPO was built by BAE Systems Inc., Space & Mission Systems (formerly Ball Aerospace). It flies onboard the Intelsat 40e satellite built by Maxar Technologies. The TEMPO Instrument Operations Center and the Science Data Processing Center are operated by the Smithsonian Astrophysical Observatory, part of the Center for Astrophysics | Harvard & Smithsonian in Cambridge.

For more information about the TEMPO instrument and mission, visit:

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

About the Author

Charles G. Hatfield

Charles G. Hatfield

Science Public Affairs Officer, NASA Langley Research Center

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Charles G. Hatfield

Hubble Observations Give “Missing” Globular Cluster Time to Shine

Hubble Observations Give “Missing” Globular Cluster Time to Shine

2 min read

Hubble Observations Give “Missing” Globular Cluster Time to Shine

Bright stars cluster against a black background. The stars are more densely concentrated in the center of the image. The stars appear mostly white, but bright red and blue stars are also visible sprinkled throughout the image.
This NASA Hubble Space Telescope image features a dense and dazzling array of blazing stars that form globular cluster ESO 591-12.
NASA, ESA, and D. Massari (INAF — Osservatorio di Astrofisica e Scienza dello Spazio); Processing: Gladys Kober (NASA/Catholic University of America)

A previously unexplored globular cluster glitters with multicolored stars in this NASA Hubble Space Telescope image. Globular clusters like this one, called ESO 591-12 or Palomar 8, are spherical collections of tens of thousands to millions of stars tightly bound together by gravity. Globular clusters generally form early in the galaxies’ histories in regions rich in gas and dust. Since the stars form from the same cloud of gas as it collapses, they typically hover around the same age. Strewn across this image of ESO 591-12 are a number of red and blue stars. The colors indicate their temperatures; red stars are cooler, while the blue stars are hotter.

Hubble captured the data used to create this image of ESO 591-12 as part of a study intended to resolve individual stars of the entire globular cluster system of the Milky Way. Hubble revolutionized the study of globular clusters since earthbound telescopes are unable to distinguish individual stars in the compact clusters. The study is part of the Hubble Missing Globular Clusters Survey, which targets 34 confirmed Milky Way globular clusters that Hubble has yet to observe.

The program aims to provide complete observations of ages and distances for all of the Milky Way’s globular clusters and investigate fundamental properties of still-unexplored clusters in the galactic bulge or halo. The observations will provide key information on the early stages of our galaxy, when globular clusters formed.

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Media Contact:

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

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