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

Source: science.nasa.gov

Risk of Hydrazine Use Following Freeze–Thaw Exposure

For more information, contact Jonathan E. Jones, Langley Research Center, [email protected]

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.

Source: www.nasa.gov

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.

Source: science.nasa.gov

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.

References & Resources

You may also be interested in:

Stay up-to-date with the latest content from NASA as we explore the universe and discover more about our home planet.

Bountiful Roebuck Bay 

4 min read

Tidal and seasonal shifts leave their mark on this crescent-shaped, productive bay in Western Australia’s Kimberley region.

Article

An Epic View of the Seasons

6 min read

The tilt in Earth’s axis of rotation makes the apparent position of continents shift with the seasons in imagery from…

Article

Great Balls of Fire

4 min read

An astronaut on the International Space Station was surprised to photograph a shower of light streaking through the darkness while…

Article

Source: science.nasa.gov

Curiosity Blog, Sols 5010-5015: Checking out the Bands

3 min read

Curiosity Blog, Sols 5010-5015: Checking out the Bands

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.
NASA’s Mars rover Curiosity acquired this image, showing the path ahead. The subtle banding can be picked out here in tonal differences. Curiosity captured the image using its Right Navigation Camera on Sept. 14, 2026 — Sol 5014, or Martian day 5,014 of the Mars Science Laboratory mission — at 02:05:20 UTC.
NASA/JPL-Caltech

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

Earth planning date: Friday, Sept. 11, 2026

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.”

On Friday, after a drive of about 60 meters (nearly 200 feet), we found ourselves with mostly sand close to the rover and just one small rough-textured outcrop close enough for contact science and LIBS. Fortunately, the block was extremely interesting, with abundant small flakes and chips incorporated and laminated areas that are a bit smoother. We will investigate the rougher textures with MAHLI (“Yungay” and “Chiu Chiu”), APXS (Chiu Chiu) and ChemCam LIBS (“Puya Raimondii”) and a smoother area with LIBS (“Liolaemus Tacnae”).

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.

In parallel to all the geology activities, the environmental team planned their usual full schedule of monitoring activities, such as dust-devil movies, suprahorizon movies looking at the crater rim, and tau images, which look at dust in the atmosphere.

Navcam and Mastcam acquired images of the path ahead in our drive direction. The subtle bands can just about be picked out here, by looking at tonal differences. It will be very interesting to see how these look and vary from each other when we get close enough to each one.

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

Details

Last Updated

Sep 22, 2026

Related Terms

Source: science.nasa.gov

Embracing the Equinox

3 Min Read

Embracing the Equinox

illustration of equinoxes and solstices on Earth in relation to the Sun

Illustration showing how Earth’s tilt leads to the Northern and Southern Hemispheres receiving changing amounts of sunlight over the course of the year. At the equinoxes, neither hemisphere is more tilted toward the Sun, so both hemispheres receive the same amount of sunlight.

Credits:
NASA/JPL-Caltech

Depending on your locale, equinoxes can be seen as harbingers of longer nights and gloomy weather, or promising beacons of nicer temperatures and more sunlight. Observing and predicting equinoxes is one of the earliest skills in humanity’s astronomical toolkit. Many ancient observatories around the world observed equinoxes along with the more pronounced solstices. These days, you don’t need your own observatory to know when an equinox occurs, since you’ll see it marked on your calendar twice a year! The word “equinox” originates from Latin, and translates to equal (equi-) night (-nox). But what exactly is an equinox?

An equinox occurs twice every year, in March and September. In 2026, the equinoxes will occur on March 20, at exactly 14:46 UTC (or 7:46 AM EDT), and again on September 23, at 00:05 UTC (or September 22, 2026, at 5:05 PM PDT). The equinox marks the exact moment when the center of the Sun crosses the plane of our planet’s equator. The day of an equinox, observers at the equator will see the Sun directly overhead at noon. After the March equinox, observers anywhere on Earth will see the Sun’s path in the sky continue its movement further north every day until the June solstice, after which it begins traveling south. The Sun crosses the equatorial plane again during the September equinox, and continues traveling south until the December solstice, when it heads back north once again. This movement is why some refer to the March equinox as the northward equinox and the September equinox as the southward equinox.

A full disk view of the earth from GOES 16, GOES East on the vernal Equinox.
A full disk view of the earth from GOES 16, GOES East on the vernal Equinox.
NOAA/NASA

Our Sun shines equally on both the Northern and Southern Hemispheres during equinoxes, which is why they are the only times of the year when the Earth’s North and South Poles are simultaneously lit by sunlight. Notably, the length of day and night on the equinox isn’t precisely equal; the date for that split depends on your latitude, and may occur a few days earlier or later than the equinox itself. The complicating factors? Our Sun and atmosphere! The Sun itself is a sphere and not a point light source, so its edge is refracted by our atmosphere as it rises and sets, which adds several minutes of light to every day. The Sun doesn’t neatly wink on and off at sunrise and sunset like a light bulb, and so there isn’t a perfect split of day and night on the equinox – but it’s very close.

Equinoxes are associated with the changing seasons. In March, Northern Hemisphere observers welcome the longer, warmer days heralded by their vernal, or spring, equinox, but Southern Hemisphere observers note the shorter days – and longer, cooler nights – signaled by their autumnal, or fall, equinox. Come September, the reverse is true.

Originally posted by Dave Prosper: February 2022

Last Updated by Kat Troche: March 2026

Source: science.nasa.gov

NASA Welcomes Albania as Newest Artemis Accords Signatory  

U.S. Deputy Assistant Secretary of State for Space and Environment Connor Tomlinson, left, NASA Deputy Administrator Matt Anderson, Albania’s Minister for Europe and Foreign Affairs Ferit Hoxha, and Ambassador of the Republic of Albania to the United States Ervin Bushati, right, are seen at the conclusion of an Artemis Accords signing ceremony Monday, September 21, 2026, at the Mary W. Jackson NASA Headquarters building in Washington. The Republic of Albania is the 73rd country to sign the Artemis Accords, which establish a practical set of principles to guide space exploration cooperation among nations participating in NASA’s Artemis program.
U.S. Deputy Assistant Secretary of State for Space and Environment Connor Tomlinson, left, NASA Deputy Administrator Matt Anderson, Albania’s Minister for Europe and Foreign Affairs Ferit Hoxha, and Ambassador of the Republic of Albania to the United States Ervin Bushati, right, are seen at the conclusion of an Artemis Accords signing ceremony Monday, September 21, 2026, at the Mary W. Jackson NASA Headquarters building in Washington.
NASA/Bill Ingalls

The Republic of Albania signed the Artemis Accords Monday during a ceremony hosted by NASA at the agency’s headquarters in Washington, joining the coalition of like‑minded nations committed to the responsible and transparent exploration of space.

“It is my privilege to welcome the Republic of Albania as the 73rd signatory of the Artemis Accords,” said NASA Deputy Administrator Matt Anderson. “The relationship between our nations goes back more than a century. Today, we extend that partnership into space.”

Albania’s Minister for Europe and Foreign Affairs Ferit Hoxha signed on behalf of the country. Ambassador of the Republic of Albania to the United States Ervin Bushati and the U.S. Deputy Assistant Secretary of State for Space and Environment Connor Tomlinson also participated in the event.

“It is a great honor for Albania to join the growing community of nations that have signed these important Artemis Accords,” said Hoxha in remarks during the ceremony. “By taking this step, Albania affirms its commitment to peaceful, transparent, sustainable, and cooperative exploration of space. We do so as a country deeply committed to international law, multilateral cooperation, and the belief that humanity’s greatest achievements are realized not in isolation, but through partnerships.”

Marking a significant step in Albania’s efforts to strengthen its use of space‑based data, Albania launched two dedicated Earth‑observation satellites, Albania‑1 and Albania‑2, in January 2023 aboard a SpaceX Falcon 9 rocket from NASA’s Kennedy Space Center in Florida, an example of how the United States is supporting Albania’s capabilities in space.

Albania also has played an active role in NASA’s Space Apps Challenge, hosting local events that connected students, technologists, and innovators with NASA’s openly available Earth and space science data. NASA Space Apps is the world’s largest annual global hackathon, mobilizing participants in more than 150 countries to develop creative solutions to real-world challenges using open data from NASA and partner space agencies to advance exploration for the benefit of all.

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. They introduced the first set of practical principles aimed at enhancing the safety and coordination between 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 space exploration and innovation. 

Learn more about the Artemis Accords at:  

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

Source: www.nasa.gov

NASA Kicks Off Nationwide Effort to Prepare Tomorrow’s Space Workforce

NASA kicked off its State Hubs for Skilled Technical Workforce initiative Sept. 15, 2026 with awardees at Space Center Houston. Agency leadership convened State Hub partners to align strategy and build momentum while focusing on partnerships, small business engagement, and next steps.

Elaine Ho, associate administrator for NASA’s Office of STEM Engagement in Washington, addresses NASA State Hubs project leaders and agency, state, and federal partners at Space Center Houston on Sept. 15, 2026
Credit: NASA

“The NASA State Hubs initiative is a top priority for the agency, because we know the space economy is really accelerating across the country,” said Elaine Ho, associate administrator for NASA’s Office of STEM Engagement at NASA Headquarters in Washington. “It’s energizing to watch our partners come together to put real plans into action to help students advance into well paying, rewarding technical jobs. I am excited about what’s ahead.”

NASA State Hubs project leaders and agency, state, and federal partners gathered in Houston to connect with peers, hear presentations from each State Hub, and explore workforce needs, skillsets, credentials, and hiring trends.

NASA State Hubs project leaders pause for a photo with Joe Acaba, center left, NASA astronaut and associate director for Mission and Strategy at Johnson Space Center in Houston, and Elaine Ho, associate administrator for NASA’s Office of STEM Engagement, center right.
Credit: NASA

In August, the agency selected seven projects representing states across the country: California, Colorado, Florida, Georgia, Minnesota, Texas, and Utah. Each Hub will offer programs tailored to its state’s unique aerospace industry and workforce priorities, ensuring students get opportunities that meet those needs.

During the meeting, NASA leadership and awardees discussed challenges impacting the STEM workforce pipeline, including limited coordination between industry, community colleges, and state economic development entities, difficulty scaling job programs, and misconceptions about manufacturing jobs.

In the coming months, NASA State Hub awardees will finalize approaches and begin delivering programming, tools, and resources that connect students across their state with the technical skills and hands-on experiences that prepare them to join the aerospace workforce.

Together, NASA and its State Hubs partners are mapping out the path to a future aerospace landscape powered by career ready workers who can build what comes next, advance NASA’s missions, and sustain America’s leadership in space.

For more information on NASA State Hubs, visit:
https://www.nasa.gov/learning-resources/nasa-state-hubs

Source: www.nasa.gov

Perseverance’s View of ‘Turquoise Bay’

1 Min Read

Perseverance’s View of ‘Turquoise Bay’

A panoramic view of a barren, reddish-orange Martian landscape stretching toward distant hills, partially obscured by the jagged black silhouettes of a rover in the foreground.

PIA26815

Credits:
NASA/JPL-Caltech/MSSS

Description

NASA’s Perseverance Mars rover used its Mastcam-Z camera to capture this 360-degree panorama of “Turquoise Bay,” a geologic area of interest in the “Margin Unit.” The 818 images used to create the natural-color panorama were captured between Oct. 5 and Oct. 16, 2023, the 933rd to 944th Martian days, or sols, of the mission.

A panoramic view of a barren, reddish-orange Martian landscape stretching toward distant hills, partially obscured by the jagged black silhouettes of a rover in the foreground.
Figure A (low resolution)

Figure A is an enhanced-color version, in which color bands were processed to improve visual contrast and accentuate color differences.

NASA’s Jet Propulsion Laboratory, which is managed for the agency by Caltech in Pasadena, California, built and manages operations of the Perseverance rover. Arizona State University leads the operations of the Mastcam-Z instrument, working in collaboration with Malin Space Science Systems in San Diego, on the design, fabrication, testing, and operation of the cameras, and in collaboration with the Niels Bohr Institute of the University of Copenhagen on the design, fabrication, and testing of the calibration targets.

For more about Perseverance: science.nasa.gov/mission/mars-2020-perseverance/

Source: science.nasa.gov

NASA’s Chandra Finds Unusual Objects in Pinwheel Galaxy

Researchers found 84 so-called hypersoft X-ray sources in M101, Messier 31, and four elliptical galaxies. This newly-discovered class of objects give off very low-energy X-rays and likely high levels of ultraviolet light. Their existence may help explain questions around Type Ia supernova explosions and the intergalactic medium. These images of the face-on spiral galaxy M101 show X-ray data from Chandra and an optical image from the Hubble Space Telescope.
X-ray: NASA/CXC/Univ. of Alabama/M. Muhibullah et al.; Optical: NASA/ESA/STScI; Image Processing: NASA/CXC/SAO/N. Wolk

Using NASA’s Chandra X-ray Observatory, researchers found mysterious objects that give off unusually low-energy X-rays but intense levels of ultraviolet radiation. One of the galaxies they studied, M101, is pictured here in this image released on Sept. 9, 2026. Astronomers suggest these newly spotted objects in other galaxies may help solve not one, but two long-standing questions in astrophysics.

Read more about this discovery.

Image description: X-ray: NASA/CXC/Univ. of Alabama/M. Muhibullah et al.; Optical: NASA/ESA/STScI; Image Processing: NASA/CXC/SAO/N. Wolk

Source: www.nasa.gov