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Patriot Missile System Paired With Littoral Combat Ship in Test

A Lockheed Martin test this week paired an M903 Patriot launcher with the Independence-class Littoral Combat Ship USS Montgomery (LCS 8) in a demonstration to showcase expeditionary air defense concepts that can be provided to ships at sea.

The M903 is the second type of missile launcher tested and integrated into the Littoral Combat Ship (LCS) platform. Lockheed’s integration and testing efforts for the Patriot follows the Mark 70 Payload Delivery System which can deliver traditional Standard Missile variants to the LCS platform to perform ballistic missile defense and extended range anti-air warfare with SM-3 and SM-6.

Lockheed Martin previously tested the Mark 70 PDS on LCS-class ships, with former Secretary of the Navy Carlos Del Toro asserting that “LCS is back” with the new lethality it brings to the class. The launcher, also developed by Lockheed Martin, adds Mk 41 VLS capability to the flight deck of selected LCS.

Lockheed Martin spent the week aboard Montgomery demonstrating expeditionary IAMD capabilities and concepts that could be employed, aimed towards a notional fight in the Pacific as the U.S. faces down against an increasingly hostile and armed China. Rapidly proliferating missile systems fielded in the Pacific pose a threat to lightly armed littoral combat ships that would be deployed in the region.

The Mk70 Payload Delivery System, a containerized variant of the Mk 41 vertical launching system, was present on USS Nantucket (LCS 27) during its commissioning ceremony in Nov. Screenshot from U.S. Navy video

Patriot launchers, armed with PAC-3 MSE missiles, would give the LCS another option for high-end missile defense. The PAC-3 MSE is already a capability being pursued by the U.S. Navy for its combat-proven capability and mature production line, with initial units set for purchase in FY2026 for testing evaluations. It is expected to be integrated into the Mk 41 VLS cells used across the fleet/

Naval News recently covered the U.S. Navy’s interest in PAC-3 MSE at the Surface Navy Association’s National Symposium, with coverage of the first PAC-3 MSE VLS test fire here.

A M903 Patriot missile launcher sits on the flight deck of USS Montgomery (LCS 8) while in its home port of San Diego, California. The battery is equipped with eight PAC-3 MSE missiles. (Lockheed Martin photo)

The addition of ‘traditional’ Patriot launchers for the PAC-3 MSE would give the LCS classes a proven and out-of-the-box solution for the extremely high-end missile defense requirement that stretches into the hypersonic air-breathing threat regime. Experience in Ukraine and the Red Sea has helped draw conclusions, recommendations, and changes for the fleet’s missile defense capabilities, including a new ESSM Block III variant which the Sea Sparrow Office began inquiries for this week.

Placing land-based air defense systems on surface vessels is something the Russian Navy has been doing in an attempt to increase the protection of their corvettes from Ukrainian threats in the Black Sea. One year ago, a Karakurt-class corvette belonging to the Russian Baltic Fleet was also spotted with a Tor-M2KM air defense system placed on its helicopter deck.

One former Lockheed Martin official claimed the capability shown on Montgomery was fielded as an operational asset, but Naval News was unable to verify their claims. The pairing between Patriot and the Montgomery could represent a new expeditionary air defense capability for littoral waters around the Philippines.

A highly mobile Patriot battery, exploiting the high speed characteristics of the Independence-class, could be used to follow aircraft that disperse throughout the region to various austere bases, offering a high-end air and missile defense capability to those bases quicker than driving through the less developed and potentially contested roadways in rural areas of the Philippines.

Naval News has reached out to both Lockheed Martin and the U.S. Navy for further comments on the test event.

LCS firepower enhancements and magazine depth for surface combatants are two major driving efforts for the U.S. Navy as the class takes on minesweeping, minelaying, anti-surface warfare, anti-submarine warfare, and now, with PAC-3 MSE and Mk 41 VLS containers, fleet defense missions as well. Additional experimentation and weapon integration into both LCS subclasses is will continue as the service shifts towards more heavily armed combatants for high-end combat.

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Austal USA Launches First Navy Landing Craft Utility LCU Vessel

Austal USA Launches First Navy Landing Craft Utility (LCU) Vessel

Austal USA launched the company’s first Navy Landing Craft Utility (LCU) vessel at its ship manufacturing facility in Mobile, Ala. on Aug. 22.

Austal USA press release

LCU 1710 is the first of 12 Navy LCUs under contract at Austal USA, part of a $91.5 million contract awarded by the Navy in 2023. Austal USA has three LCU under construction.

“I am proud of the LCU program team for the hard work they’ve put forth to reach this important milestone,” stated Michelle Kruger, Austal USA President. “LCU is an important program that plays a critical role in supporting expeditionary operations for the Navy and Marine Corps. Each milestone achieved shores up our position as a key contributor to the strength and success of the maritime industrial base.”

LCU are carried aboard amphibious assault ships to the objective area and used across a range of military operations to deliver vehicles, personnel and cargo from sea-to-shore and back. These connectors provide a heavy-lift capability and can carry about the same payload capacity as several C-17 aircraft.

LCU is one of three shipbuilding programs in serial production at Austal USA’s facility.  The company also has three Navy Navajo-class Towing, Salvage and Rescue ships (T-ATS) and two U.S. Coast Guard Heritage-class Offshore Patrol Cutters (OPC) under construction.

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Late Hand Over to Tonga

Australia delivers new landing craft to Tonga

Australia has successfully delivered a new landing craft vessel to Tonga today, with an official handover ceremony taking place at the Masefield Naval Base. 

Australian DoD press release

The ceremony was attended by His Royal Highness Crown Prince Tupouto‘a ‘Ulukalala, Tonga’s Minister for Foreign Affairs and Minister for His Majesty’s Armed Forces, who received the vessel on behalf of Tonga.

The VOEA Late, provided under the Pacific Maritime Security Program (PMSP), will enhance Tonga’s humanitarian assistance and disaster relief capabilities, as well as their ability to deter, detect and disrupt illegal maritime activities in the region.

Australia will provide a comprehensive package of through-life maintenance and sustainment for the vessel, alongside training for Tonga Royal Navy crew members. 

Defence’s First Assistant Secretary Pacific Division, Susan Bodell, said the delivery highlighted Australia’s commitment to supporting our Pacific partners’ maritime security.

“Australia and Tonga share a trusted and enduring security partnership,” Ms Bodell said.

“The delivery of the new landing craft builds on decades of partnership, and upholds our shared commitment to sovereignty, security and prosperity in the Pacific.”

The delivery follows the completion of comprehensive training undertaken by Tonga Royal Navy personnel at the Australian Maritime College in Tasmania. The training equipped the crew with the necessary skills to safely operate the vessel.

The PMSP is Australia’s 30 year commitment to increase national and regional maritime security throughout the Pacific, and builds on the three decades of success in the original Pacific Patrol Boat Program.

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Australia lays keel of 6th and final Arafura class OPV

Australia lays keel of 6th and final Arafura-class OPV

A ceremony was held August 29 to mark the laying of the keel of Arafura-class Offshore Patrol Vessel (OPV) 6, NUSHIP Carpentaria at Civmec in Henderson, Western Australia. The vessel is the final Arafura-class OPV under construction for the Royal Australian Navy.

Australian DoD press release

Rear Admiral Michael Houghton, Head of Patrol Boats and Specialist Ships represented the ceremony, honouring tradition by positioning a coin under the keel of NUSHIP Carpentaria.

“A keel laying ceremony which marks the beginning of a ship’s construction, is an important naval tradition which is believed to bring good luck for the vessel’s build and life at sea,” Rear Admiral Michael Houghton said.

“The OPV program is a major contributor to continuous naval shipbuilding in Australia, which creates and sustains local jobs and harnesses our national defence industry’s local talent and technology. 

“Defence investment in a sovereign Naval Shipbuilding and Sustainment Enterprise is expected to support around 8,500 jobs in shipbuilding and sustainment by 2030.

“OPVs help patrol and secure Australia’s maritime border alongside the Evolved Cape Class patrol boats. They also play an important role in Navy’s commitment to supporting the long-term objectives of the National Defence Strategy.”

The first two vessels were constructed at the Osborne Naval Shipyard in South Australia with the remaining four are currently under construction at the Henderson Maritime Precinct. The first ship, HMAS Arafura, was commissioned into service on 28 June 2025 with the second OPV, NUSHIP Eyre, expected to be delivered later this year. 

The OPVs are a more versatile platform compared with previous classes of patrol vessels. They are able to operate over longer distances and can be reconfigured to perform a number of tasks and roles originally carried out by several different classes of vessels.

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Naval News comments: About Arafura-class OPV

As Naval News has previously reported, procurement of Arafura experienced significant delays and revisions. The effort, dubbed SEA 1180 saw specification changes over integration issues such as the desired main gun. The current Albanese government also cut overall procurement from twelve to six vessels. Canberra now deems the design insufficient to new requirements of the Australian Navy for more robustly armed and survivable combatants.

Nevertheless the Australian Navy arguably requires more hulls for the active and ageing fleet. RAN is pushed to maintain persistent patrols across extensive Australian territorial waters and its exclusive economic zone (EEZ). In an event receiving significant local attention, the Chinese Navy (PLAN) in earlier this year conducted a circumnavigation of Australia. The operation, including a live fire-drill, illustrates a trend of increasing naval activity near Australian waters. Such events create an increasing demand for maritime awareness with both Australia and News Zealand. Additionally the primary Australian security partner, the United States, continues to place more emphasis on burden-sharing, including in the maritime domain.

Specifications:

Length: 80 m

Beam: 13 m

Draught: 4 m

Speed: 20 knots (maximum)

Range: 7,400 kilometres

Displacement: approx. 1,640 t

Crew: 40 crew with accommodation for up to 60 personnel

Armament: 40mm gun / 2 x 50 calibre machine guns

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Low Res Butterfly Nebula NGC 6302 Hubble and Webb ALMA images side by side

James Webb Space Telescope Discovers “Cool Gemstones” and “Fiery Grime” in New Butterfly Nebula Images

New James Webb Space Telescope data is revealing new insights into the Butterfly Nebula, which may explain how rocky planets form from cosmic dust, among other discoveries, as demonstrated in a new paper published in the Monthly Notices of the Royal Astronomical Society.
The focus of the new research was NGC 6303, also known as the Butterfly Nebula, a gathering of minerals and organic material surrounding a hidden star, located roughly 3,400 light-years away in the constellation Scorpius.
Previously imaged by the Hubble Space Telescope before the recent Webb observations, NGC 6302 is one of the most comprehensively studied planetary nebulae in our galaxy, with the new images providing previously unavailable insight into the nebula’s dynamism.
The Structure of Cosmic Dust
“For years, scientists have debated how cosmic dust forms in space,” said lead researcher Dr Mikako Matsuura, of Cardiff University. “But now, with the help of the powerful James Webb Space Telescope, we may finally have a clearer picture.”
Registering at 220,000 Kelvin, the Butterfly Nebula has one of the hottest recorded temperatures of any nebula’s central stars in our galaxy. As such, it forms a powerful engine for the nebula’s brilliant glow and the surrounding torus, a dense band of dust and gas. 
Across the cosmos, dust can take on various forms, ranging from random, soot-like atomic structures to perfectly ordered crystalline ones, resembling miniature gems. The James Webb Space Telescope’s latest results show the torus to contain a mix of both types, both crystalline silicates and irregular dust grains, with some dust particles reaching unusually large sizes of one millionth of a meter due to their extended growing period.
“We were able to see both cool gemstones formed in calm, long-lasting zones and fiery grime created in violent, fast-moving parts of space, all within a single object,” Matsuura added. ”This discovery is a big step forward in understanding how the basic materials of planets come together.”
Three views of NGC 6303, the Butterfly Nebula, featuring optical and near-infrared images from Hubble (left and middle) and the new Webb/ALMA image using the MIRI instrument. Credit: ESA/Webb, NASA & CSA, M. Matsuura, J. Kastner, K. Noll, ALMA (ESO/NAOJ/NRAO), N. Hirano, J. Kastner, M. Zamani (ESA/Webb)
Unusual James Webb Space Telescope Discoveries
Planetary nebulae are among the most beautiful and mysterious structures in the cosmos, although their moniker is a misnomer, since astronomers hundreds of years ago perceived the structures to be round in shape, similar to planets.
Despite this long-standing name, the Butterfly Nebula, as seen in the new James Webb Space Telescope images, offers further proof that many planetary nebulae are not round at all, as NGC 6303’s two lobes resemble the wings of a butterfly. The central band is a donut-shaped torus, which, when viewed from the side due to our vantage point on Earth, gives the impression of a buttery’s central body, hiding the Nebula’s star.
A multilayered emission structure forms outside of the torus, as ions released from atoms and molecules order themselves in accordance with the amount of energy required for their formation. Those with the highest energetic needs congregate nearer to the central star, while those born of lesser energy expand to the perimeter. The researchers identified iron and nickel jets shooting out from the star in opposite directions, forming one of the most noteworthy observations. 
Another notable sight was the honeycomb-like shapes formed by carbon-based molecules, which were observed emitting light. The molecules, polycyclic aromatic hydrocarbons, are often found in smoke on Earth. Their location in the nebula suggests that the molecules form when a blast of space wind from the central star impacts the surrounding gas. This is the first time such molecules have been identified forming in an oxygen-rich planetary nebula.
MIRI Observations
Working in integral field unit mode, the MIRI instrument aboard the James Webb Space Telescope captured the recent image, zooming in on the nebula’s center to offer new insights into its complex structure. By combining a camera with a spectrograph, the integral field unit mode allows MIRI to image multiple wavelengths simultaneously.

Such a capability enables scientists to compare how an object’s appearance varies across different wavelengths. For their analysis, the MIRI data were collated with results from the Atacama Large Millimeter/Submillimetre Array.
The team uncovered nearly 200 spectral lines in the James Webb Space Telescope data, providing detailed information on the atoms and molecules present and how they form interconnected structures.
James Webb Space Telescope data also provided the necessary clues to finally determine the central star’s location, obscured by the torus. That star also turned out to be the illumination source for a dust cloud that had previously gone undetected, but shines brilliantly in the mid-infrared wavelengths that MIRI captures.
The new paper, “The JWST/MIRI View of the Planetary Nebula NGC 6302 I.: A UV Irradiated Torus and a Hot Bubble Triggering PAH Formation,” appeared in Monthly Notices of the Royal Astronomical Society on August 27, 2025.
Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.

James Webb Space Telescope Discovers “Cool Gemstones” and “Fiery Grime” in New Butterfly Nebula Images Read More »

megan mcarthur iss

NASA Astronaut Megan McArthur Retires

NASA astronaut Megan McArthur has retired, concluding a career spanning more than two decades. A veteran of two spaceflights, McArthur logged 213 days in space, including being the first woman to pilot a SpaceX Dragon spacecraft and the last person to “touch” the Hubble Space Telescope with the space shuttle’s robotic arm.
McArthur launched as pilot of NASA’s SpaceX Crew-2 mission in April 2021, marking her second spaceflight and her first long-duration stay aboard the International Space Station. During the 200-day mission, she served as a flight engineer for Expeditions 65/66, conducting a wide array of scientific experiments in human health, materials sciences, and robotics to advance exploration of the Moon under Artemis and prepare to send American astronauts to Mars.
Her first spaceflight was STS-125 in 2009, aboard the space shuttle Atlantis, the fifth and final servicing mission to Hubble. As a mission specialist, she was responsible for capturing the telescope with the robotic arm, as well as supporting five spacewalks to update and repair Hubble after its first 19 years in space. She also played a key role in supporting shuttle operations during launch, rendezvous with the telescope, and landing.
“Megan’s thoughtful leadership, operational excellence, and deep commitment to science and exploration have made a lasting impact,” said Steve Koerner, acting director of NASA’s Johnson Space Center in Houston. “Her contributions have helped shape the future of human space exploration, and we are incredibly grateful for her service.”
In addition to her flight experience, McArthur has served in various technical and leadership roles within NASA. In 2019, she became the deputy division chief of the Astronaut Office, supporting astronaut training, development, and ongoing spaceflight operations. She also served as the assistant director of flight operations for the International Space Station Program starting in 2017.
Since 2022, McArthur has served as the chief science officer at Space Center Houston, NASA Johnson’s official visitor center. Continuing in this role, she actively promotes public engagement with space exploration themes, aiming to increase understanding of the benefits to humanity and enhance science literacy.
“Megan brought a unique combination of technical skill and compassion to everything she did,” said Joe Acaba, chief of the Astronaut Office at NASA Johnson. “Whether in space or on the ground, she embodied the best of what it means to be an astronaut and a teammate. Her contributions will be felt by the next generation of explorers she helped train.”
McArthur was born in Honolulu and raised as a “Navy kid” in many different locations worldwide. She earned a Bachelor of Science in aerospace engineering from the University of California, Los Angeles, and a doctorate in oceanography from the Scripps Institution of Oceanography at the University of California, San Diego. Before being selected as an astronaut in 2000, she conducted oceanographic research focusing on underwater acoustics, which involved shipboard work and extensive scuba diving.
McArthur is married to former NASA astronaut Robert Behnken, who also flew aboard the Dragon Endeavour spacecraft during the agency’s SpaceX Demo-2 mission in 2020.
“It was an incredible privilege to serve as a NASA astronaut, working with scientists from around the world on cutting-edge research that continues to have a lasting impact here on Earth and prepares humanity for future exploration at the Moon and Mars,” said McArthur. “From NASA’s Hubble Space Telescope to the International Space Station, our research lab in low Earth orbit, humanity has developed incredible tools that help us answer important scientific questions, solve complex engineering challenges, and gain a deeper understanding of our place in the universe. Seeing our beautiful planet from space makes it so clear how fragile and precious our home is, and how vital it is that we protect it. I am grateful I had the opportunity to contribute to this work, and I’m excited to watch our brilliant engineers and scientists at NASA conquer new challenges and pursue further scientific discoveries for the benefit of all.”
To learn more about NASA’s astronauts and their contributions to space exploration, visit:
https://www.nasa.gov/astronauts
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Shaneequa VereenJohnson Space Center, Houston281-483-5111shaneequa.y.vereen@nasa.gov

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auskingsound oli2 20250611 lrg

Landsat 9 Sees Buccaneer Archipelago

The Operational Land Imager on Landsat 9 captured this image of Buccaneer Archipelago on June 11, 2025. The scene encapsulates the striking interactions between land and water in the area where King Sound opens to the Indian Ocean.
The powerful tidal currents stir up sediment in shallow areas, producing the beautiful turquoise swirls visible in this image. This power, however, can be hazardous to seafarers and divers as water rips through the archipelago’s constricted passages. One infamous place of turbulence, known as “Hell’s Gate,” lies in the passage between Gerald Peninsula and Muddle Islands.
Learn more about this archipelago in Western Australia.
Text credit: Kathryn Hansen
Image credit: NASA/Michala Garrison; U.S. Geological Survey

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1 mary kays iconic pink cadillac shifts to full electric

Mary Kay’s iconic pink Cadillac shifts to fully electric

NEWYou can now listen to Fox News articles!
Nearly 60 years ago, Mary Kay Ash was turned away by a car salesman who refused to sell her a car without a man’s signature. That moment became the catalyst for a legacy, one powered by determination, lipstick, and eventually, horsepower. Now, the iconic Mary Kay pink Cadillac is entering a bold new chapter: electric mobility. Mary Kay is offering its top-performing sales reps a fully electric Cadillac Optiq wrapped in a custom “pink pearl” finish. It’s the first time the company’s legendary incentive vehicle is going fully electric, and it’s turning heads while staying true to its roots.Sign up for my FREE CyberGuy ReportGet my best tech tips, urgent security alerts, and exclusive deals delivered straight to your inbox. Plus, you’ll get instant access to my Ultimate Scam Survival Guide – free when you join my CYBERGUY.COM newsletter. A fully electric Cadillac Optiq wrapped in a custom “pink pearl” finish is parked in front of Mary Kay. (Mary Kay)A statement in pink (and green)In a press release, CEO Ryan Rogers, grandson of founder Mary Kay Ash, called the move a tribute to the company’s past and a leap into the future:”With the introduction of the all-electric OPTIQ, we’re honoring that iconic legacy while driving into a transformative future-one grounded in our commitment to sustainability and dedication to inspiring and celebrating the achievements of our independent sales force for generations to come.”THIS EV HAS A FACE, AND IT TALKS BACK WITH AIIt’s not just a change in drivetrain. It’s a shift in mindset and a signal that luxury, reward, and eco-consciousness can coexist without compromise. The Cadillac Optiq grille and logo are seen up close. (Mary Kay)Why the pink Cadillac still mattersMary Kay pink Cadillacs are more than just a flashy ride. They represent achievement, empowerment, and recognition. Only the top 1% of the company’s sales force qualify. Even then, it’s not handed out lightly; recipients can choose a $900 monthly bonus instead. But 90% take the car. What makes these cars even more exclusive is that they’re leased for just two years. When the lease ends, they’re returned and repainted to the original factory color. That makes a true pink Cadillac a rare sight outside of Mary Kay circles. And yes, they’re beautiful. That pink pearl paint is exclusive, and few people outside the company ever get to drive one.VOLKSWAGEN’S ICONIC CUTE VAN DRIVES ITSELF WITH 360-DEGREE VISION The fully electric Cadillac Optiq wrapped in a custom “pink pearl” finish drives down a road. (Mary Kay)What this means for youWhether or not you’re building an empire through lipstick sales, this shift tells a bigger story. The auto industry is changing. EVs are no longer just for tech-savvy early adopters or Silicon Valley commuters. Now, they’re reaching industries built on tradition and glamour. The Mary Kay electric Cadillac shows how companies can preserve their legacy while embracing innovation. If you’re considering switching to an electric vehicle, this proves that style and sustainability don’t have to be at odds.Take my quiz: How safe is your online security?Think your devices and data are truly protected? Take this quick quiz to see where your digital habits stand. From passwords to Wi-Fi settings, you’ll get a personalized breakdown of what you’re doing right – and what needs improvement. Take my Quiz here: Cyberguy.com.Kurt’s key takeawaysThis move isn’t just a flex. It’s a smart pivot that aligns Mary Kay with modern values while still honoring its founder’s bold spirit. And frankly, it’s refreshing to see a legacy brand walk the talk when it comes to sustainability and do it in such an eye-catching shade of pink.How do you see the integration of electric vehicles by legacy brands like Mary Kay impacting attitudes towards sustainability in industries rooted in tradition? Let us know by writing to us at Cyberguy.com.CLICK HERE TO GET THE FOX NEWS APPSign up for my FREE CyberGuy ReportGet my best tech tips, urgent security alerts, and exclusive deals delivered straight to your inbox. Plus, you’ll get instant access to my Ultimate Scam Survival Guide – free when you join my CYBERGUY.COM newsletter.Copyright 2025 CyberGuy.com.  All rights reserved.

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Hubble M96 2025 potw2534a

Hubble Homes in on Galaxy’s Star Formation

This NASA/ESA Hubble Space Telescope image features a galaxy whose asymmetric appearance may be the result of a galactic tug of war. Located 35 million light-years away in the constellation Leo, the spiral galaxy Messier 96 is the brightest of the galaxies in its group. The gravitational pull of its galactic neighbors may be responsible for Messier 96’s uneven distribution of gas and dust, asymmetric spiral arms, and off-center galactic core.

This asymmetric appearance is on full display in the new Hubble image that incorporates data from observations made in ultraviolet, near infrared, and visible/optical light. Earlier Hubble images of Messier 96 were released in 2015 and 2018. Each successive image added new data, building up a beautiful and scientifically valuable view of the galaxy.

The 2015 image combined two wavelengths of optical light with one near infrared wavelength. The optical light revealed the galaxy’s uneven form of dust and gas spread asymmetrically throughout its weak spiral arms and its off-center core, while the infrared light revealed the heat of stars forming in clouds shaded pink in the image.

The 2018 image added two more optical wavelengths of light along with one wavelength of ultraviolet light that pinpointed areas where high-energy, young stars are forming.

This latest version offers us a new perspective on Messier 96’s star formation. It includes the addition of light that reveals regions of ionized hydrogen (H-alpha) and nitrogen (NII). This data helps astronomers determine the environment within the galaxy and the conditions in which stars are forming. The ionized hydrogen traces ongoing star formation, revealing regions where hot, young stars are ionizing the gas. The ionized nitrogen helps astronomers determine the rate of star formation and the properties of gas between stars, while the combination of the two ionized gasses helps researchers determine if the galaxy is a starburst galaxy or one with an active galactic nucleus.

The bubbles of pink gas in this image surround hot, young, massive stars, illuminating a ring of star formation in the galaxy’s outskirts. These young stars are still embedded within the clouds of gas from which they were born. Astronomers will use the new data in this image to study how stars are form within giant dusty gas clouds, how dust filters starlight, and how stars affect their environments.

Media Contact:

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

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