Semua Kabar

Hong Kong needs more cybersecurity professionals as threats increase: report

Demand for cybersecurity professionals to grow steadily over the next three to five years, Hong Kong China Network Security Association says

The report said attackers, armed with AI, drove the number of security incidents handled by the Hong Kong Computer Emergency Response Team Coordination Centre in 2024 to 12,536, the highest in five years.

Since the Covid-19 pandemic, it said, the adoption of multi-cloud strategies had increased significantly and as a result, demand for professionals with cloud security backgrounds had grown.

“There is growing demand for companies to hire security professionals with the experience of securing cloud environments and managing associated risks on multiple cloud platforms such as [Amazon Web Services], Azure and Alibaba,” said Fiona Fung, senior manager of infrastructure and cyber at recruiter Robert Walters.

The report was put together in collaboration with Sia, a consulting firm. The study surveyed around a hundred cybersecurity professionals in Hong Kong. In addition, inquiries were made with a number of professional recruiters who possessed “a broad understanding of the talent market and can provide valuable insights”. The report showed that companies needed to improve their communication and collaboration skills to combat cybersecurity risks.

Going the Distance: Lisa Pace Leads Exploration Development Integration at Johnson

Lisa Pace knows a marathon when she sees one. An avid runner, she has participated in five marathons and more than 50 half marathons. Though she prefers to move quickly, she also knows the value of taking her time. “I solve most of my problems while running – or realize those problems aren’t worth worrying about,” she said.

She has learned to take a similar approach to her work at NASA’s Johnson Space Center in Houston. “Earlier in my career, I raced to get things done and felt the need to do as much as possible on my own,” she said. “Over time, I’ve learned to trust my team and pause to give others an opportunity to contribute. There are times when quick action is needed, but it is often a marathon, not a sprint.”

Pace is chief of the Exploration Development Integration Division within theExploration Architecture, Integration, and Science Directorateat Johnson. In that role, she leads a team of roughly 120 civil servants and contractors in providing mission-level system engineering and integration services that bring different architecture elements together to achieve the agency’s goals. Today that team supports Artemis missions, NASA’s Commercial Lunar Payload Services initiative and other areas as needed.

“The Artemis missions come together through multiple programs and projects,” Pace explained. “We stitch them together to ensure the end-to-end mission meets its intended requirements. That includes verifying those requirements before flight and ensuring agreements between programs are honored and conflicts resolved.” The division also manages mission-level review and flight readiness processes from planning through execution, up to the final certification of flight readiness.

Leading the division through the planning, launch, and landing of Artemis I was a career highlight for Pace, though she feels fortunate to have worked on many great projects during her time with NASA. “My coolest and most rewarding project involved designing and deploying an orbital debris tracking telescope on Ascension Island about 10 years ago,” she said. “The engineers, scientists, and military personnel I got to work and travel with on that beautiful island is tough to top!”

Pace says luck and great timing led her to NASA. Engineering jobs were plentiful when she graduated from Virginia Tech in 2000, and she quickly received an offer from Lockheed Martin to become a facility engineer in Johnson’s Astromaterials Research and Exploration Science Division, or ARES. “I thought working in the building where they keep the Moon rocks would be cool – and it was! Twenty-five years later, I’m still here,” Pace said.

During that time, she has learned a lot about problem-solving and team building. “I often find that when we disagree over the ‘right’ way to do something, there is no one right answer – it just depends on your perspective,” she said. “I take the time to listen to people, understand their side, and build relationships to find common ground.”

She also emphasizes the importance of getting to know your colleagues. “Relationships are everything,” she said. “They make the work so much more meaningful. I carry that lesson over to my personal life and value my time with family and friends outside of work.”

Investing time in relationships has given Pace another unexpected skill – that of matchmaker. “I’m responsible for setting up five couples who are now married, and have six kids between them,” she said, adding that she knew one couple from Johnson.

She hopes that strong relationships transfer to the Artemis Generation. “I hope to pass on a strong NASA brand and the family culture that I’ve been fortunate to have, working here for the last 25 years.”

Hubble Captures an Active Galactic Center

The light that the NASA/ESAHubble Space Telescopecollected to create this image reached the telescope after a journey of 250 million years. Its source was the spiral galaxy UGC 11397, which resides in the constellation Lyra (The Lyre). At first glance, UGC 11397 appears to be an average spiral galaxy: it sports two graceful spiral arms that are illuminated by stars and defined by dark, clumpy clouds of dust.

What sets UGC 11397 apart from a typical spiral lies at its center, where a supermassive black hole containing 174 million times the mass of our Sun grows. As a black hole ensnares gas, dust, and even entire stars from its vicinity, this doomed matter heats up and puts on a fantastic cosmic light show.

Material trapped by the black hole emits light from gamma rays to radio waves, and can brighten and fade without warning. But in some galaxies, including UGC 11397, thick clouds of dust hide much of this energetic activity from view in optical light. Despite this, UGC 11397’s actively growing black hole was revealed through its bright X-ray emission — high-energy light that can pierce the surrounding dust. This led astronomers to classify it as a Type 2 Seyfert galaxy, a category used for active galaxies whose central regions are hidden from view in visible light by a donut-shaped cloud of dust and gas.

Using Hubble, researchers will study hundreds of galaxies that, like UGC 11397, harbor a supermassive black hole that is gaining mass. The Hubble observations will help researchers weigh nearby supermassive black holes, understand how black holes grew early in the universe’s history, and even study how stars form in the extreme environment found at the very center of a galaxy.

Image credit: ESA/Hubble & NASA, M. J. Koss, A. J. Barth

NASA+ is Coming to Netflix This Summer

NASA announced Monday its latest plans to team up with a streaming service to bring space a little closer to home. Starting this summer, NASA+ live programming will be available on Netflix.

Audiences now will have another option to stream rocket launches, astronaut spacewalks, mission coverage, and breathtaking live views of Earth from the International Space Station.

“The National Aeronautics and Space Act of 1958 calls on us to share our story of space exploration with the broadest possible audience,” said Rebecca Sirmons, general manager of NASA+ at the agency’s headquarters in Washington. “Together, we’re committed to a Golden Age of Innovation and Exploration – inspiring new generations – right from the comfort of their couch or in the palm of their hand from their phone.”

Through this partnership, NASA’s work in science and exploration will become even more accessible, allowing the agency to increase engagement with and inspire a global audience in a modern media landscape, where Netflix reaches a global audience of more than 700 million people.

The agency’s broader efforts include connecting with as many people as possible through video, audio, social media, and live events. The goal is simple: to bring the excitement of the agency’s discoveries, inventions, and space exploration to people, wherever they are.

NASA+ remains available for free, with no ads, through the NASA app and on the agency’swebsite.

Additional programming details and schedules will be announced ahead of launch.

For more about NASA’s missions, visit:

Cheryl WarnerHeadquarters, Washington202-358-1600cheryl.m.warner@nasa.gov

NASA to Provide Coverage of Progress 92 Launch, Space Station Docking

NASA will provide live coverage of the launch and docking of a Roscosmos cargo spacecraft delivering approximately three tons of food, fuel, and supplies to the Expedition 73 crew aboard the International Space Station.

The unpiloted Roscosmos Progress 92 spacecraft is scheduled to launch at 3:32 p.m. EDT, Thursday, July 3 (12:32 a.m. Baikonur time, Friday, July 4), on a Soyuz rocket from the Baikonur Cosmodrome in Kazakhstan.

Live launch coverage will begin at 3:10 p.m. onNASA+. Learn how to watchNASA contentthrough a variety of platforms, including social media.

After a two-day, in-orbit journey to the station, the spacecraft will dock autonomously to the space-facing port of the orbiting laboratory’s Poisk module at 5:27 p.m. on Saturday, July 5. NASA’s rendezvous and docking coverage will begin at 4:45 p.m. onNASA+.

The Progress 92 spacecraft will remain docked to the space station for approximately six months before departing for re-entry into Earth’s atmosphere to dispose of trash loaded by the crew.

Ahead of the spacecraft’s arrival, the Progress 90 spacecraft will undock from the Poisk module on Tuesday, July 1. NASA will not stream undocking.

The International Space Station is a convergence of science, technology, and human innovation that enables research not possible on Earth. For nearly 25 years, NASA has supported a continuous U.S. human presence aboard the orbiting laboratory, through which astronauts have learned to live and work in space for extended periods of time. The space station is a springboard for developing a low Earth economy and NASA’s next great leaps in exploration, including missions to the Moon under Artemis and, ultimately, human exploration of Mars.

Learn more about the International Space Station, its research, and crew, at:

Jimi RussellHeadquarters, Washington202-358-1100james.j.russell@nasa.gov

Sandra Jones / Joseph ZakrzewskiJohnson Space Center, Houston281-483-5111sandra.p.jones@nasa.gov/joseph.a.zakrzewski@nasa.gov

NASA Awards Electrical Utility Services Contract for Kennedy

NASA has awarded a task order to Florida Power and Light of Juno Beach, Florida, to provide electric distribution utility service at the agency’s Kennedy Space Center in Florida.

This is a fixed-price task order with an estimated value of $70 million over five years. The contract consists of a two-year base period beginning July 1, 2025, followed by a two-year and a one-year option period.

Under the contract, the awardee will provide all management, labor, transportation, facilities, materials, and equipment to provide electric distribution utility service up to and including all meters across the spaceport.

For more information about NASA Kennedy, visit:

Patti BiellingKennedy Space Center, Florida321-501-7575patricia.a.bielling@nasa.gov

Scientists reveal a spontaneous reaction that could have started life

Urea is one of the most important industrial chemicals produced worldwide. It is used as a fertiliser, for the production of synthetic resins and explosives and as a fuel additive for cleaning car exhaust gases. Urea is also believed to be a potential key building block for the formation of biological molecules such as RNA and DNA in connection with the question of the origin of life. Until now, the origin of urea itself on Early Earth has not been conclusively clarified.

A research team led by Ruth Signorell, Professor of Physical Chemistry at ETH Zurich, has discovered a previously unknown reaction pathway for the formation of urea that could provide an answer. The study has just been published in the journalScience.

Either high pressures and temperatures or chemical catalysts are needed for the industrial production of urea from ammonia (NH₃) and carbon dioxide (CO2). Enzymes enable the same reaction to take place in humans and animals, removing toxic ammonia from the breakdown of proteins such as urea. As this simple molecule contains nitrogen as well as carbon and probably existed on the uninhabited Early Earth, many researchers view urea as a possible precursor for complex biomolecules.

"In our study, we show one way in which urea could have formed on the prebiotic Earth," says Signorell – "namely where water molecules interact with atmospheric gases: on the water surface."

Reactor on the edge of a droplet

Signorell's team studied tiny water droplets such as those found in sea spray and fine mist. The researchers observed that urea can form spontaneously from carbon dioxide (CO2) and ammonia (NH₃) in the surface layer of the droplets under ambient conditions. The physical interface between air and liquid creates a special chemical environment at the water surface that makes the spontaneous reaction possible.

As a droplet has a very large surface area in relation to its volume, chemical reactions mainly take place near this surface. Chemical concentration gradients form in this area, which acts like a microscopic reactor. The pH gradient across the interfacial layer of the water droplets creates the required acidic environment, which opens unconventional pathways that would otherwise not take place in liquids.

"The remarkable aspect of this reaction is that it takes place under ambient conditions without any external energy," explains Mercede Mohajer Azizbaig, one of the two first authors. This not only makes the process interesting from a technical perspective but also provides valuable insights into processes that could be significant for evolution.

A window into the early days of the Earth

The origin of life is currently the subject of a great deal of wide-ranging research, with different approaches being explored. First author Pallab Basuri explains: "Given such a controversial field of research, it was important for us to back up our observations." Theoretical calculations by co-authors Evangelos Miliordos and Andrei Evdokimov from Auburn University supported the experimental findings and confirmed that the urea reaction on the droplets takes place without any external energy supply.

The results suggest that this natural reaction could also have been possible in the atmosphere of the Early Earth — an atmosphere that was rich in CO2 and probably contained small traces of ammonia. In such environments, aqueous aerosols or fog droplets could have acted as natural reactors in which precursor molecules such as urea were formed. "Our study shows how seemingly mundane interfaces can become dynamic reaction spaces, suggesting that biological molecules may have a more common origin than was previously thought," says Signorell.

In the long term, the direct reaction of CO2 and ammonia under ambient conditions could also have potential for the climate-friendly production of urea and downstream products.

Materialsprovided byETH Zurich.Note: Content may be edited for style and length.

JWST unlocks 10-billion-year mystery of how galaxies shape themselves

Many galaxies, including our own Milky Way, are characterized by a flat, extended, rotating stellar disk. These disk galaxies commonly contain two main parts: a thin disk and a thick disk. The thin disk contains younger, metal-rich stars, while the thick disk contains older, metal-poor stars. These distinct components hold fossil records that help astronomers understand how galaxies form stars, build up elements like oxygen and carbon, essential for life, and evolve into their present shapes.

Until now, thin and thick disks have only been identified in the Milky Way and nearby galaxies. It has been impossible with previous telescopes to distinguish the thin edge of a distant galaxy when viewed from the side.

That changed with the launching of the James Webb Space Telescope (JWST) in 2021, which is currently the largest telescope in space.

An international team of researchers has examined 111 JWST images of distant edge-on galaxies, ones where the alignments enabled the researchers to observe the galaxies' vertical disk structures.

Takafumi Tsukui (formerly of the Australian National University and now based at Tohoku University), who led the research team, says that observing distant galaxies is like using a time machine, allowing us to see how galaxies have built their disks over cosmic history.

"Thanks to the JWST's sharp vision, we were able to identify thin and thick disks in galaxies beyond our local universe, some going as far back as 10 billion years ago."

The study revealed a consistent trend: in the earlier universe, more galaxies appear to have had a single thick disk, while in later epochs, more galaxies showed a two-layered structure with an additional thin disk component. This suggests that galaxies first formed a thick disk, followed by the formation of a thin disk within it. In more massive galaxies, this thin disk appears to have formed earlier.

The study estimated the thin disk formation time for Milky Way-sized galaxies to be around 8 billion years ago. This figure aligns with formation timelines for the Milky Way itself, where stellar ages can be measured.

To understand the revealed sequential formation from thick to thin disks and the corresponding formation timelines, the team not only examined the stellar structure but also the motion of gas, direct ingredients of stars obtained from the Atacama Large Millimeter/submillimeter Array (ALMA) and ground-based surveys in the literature. These observations supported a coherent formation scenario:

Tsukui emphasizes that the images provided by JWST help answer one of the biggest questions in astronomy: was our galaxy's formation typical or unique? "The JWST images provided a window into galaxies that resemble the Milky Way's early state, bringing us valuable insights from galaxies far away."

The team hopes that their study will help bridge studies of nearby galaxies with far away ones and refine our understanding of disk formation. The study was published in the journalMonthly Notices of the Royal Astronomical Societyon June 26, 2025.

Materialsprovided byTohoku University.Note: Content may be edited for style and length.

This brain scan sees Alzheimer’s coming—but only in some brains

A team of researchers from the Keck School of Medicine of USC's Mark and Mary Stevens Neuroimaging and Informatics Institute (Stevens INI) has identified a new brain imaging benchmark that may improve how researchers classify biologically meaningful changes associated with Alzheimer's disease, especially in Hispanic and non-Hispanic White populations. The new study, published inImaging Neuroscience, is part of the Health and Aging Brain Study-Health Disparities (HABS-HD), a multi-university collaboration led by the University of North Texas Health Science Center and supported by the National Institute on Aging.

Using an advanced brain imaging scan called tau PET, the research team studied over 675 older adults from HABS-HD, aiming to identify the optimal brain signal that distinguishes individuals with clinically-relevant biological markers of AD from those who are aging normally.

Tau PET enables researchers to visualize abnormal proteins in the brain which contribute to Alzheimer's disease, known as tau, by using a small amount of a special radioactive tracer that highlights areas where tau has accumulated. With these scans, researchers can establish tau cut-points, a new type of biomarker used to determine whether a scan shows an amount of tau protein in the brain high enough to suggest possible early signs of Alzheimer's disease or related conditions. This new benchmark could eventually inform the way clinicians interpret tau PET scans and better identify who may be at risk for AD.

In this study, researchers compared tau PET scans of study participants who were cognitively impaired with those who were not impaired based on cognitive tests to establish a tau cut-point that would indicate a higher risk for Alzheimer's disease. They found one — but it was only effective in certain circumstances.

"Our tau cut-point was able to distinguish whether study participants had cognitive impairment – but only when another abnormal protein, amyloid, was also present in those with cognitive impairment, and only in Hispanic and non-Hispanic White participants," said senior author Meredith N. Braskie, PhD, assistant professor of neurology. "In non-Hispanic Black participants, the tau cut-point did not perform as expected. This suggests that other pathologies or conditions may be driving cognitive decline in this group. Our study is an important step toward better understanding how tau relates to cognition in diverse populations and has important implications for future clinical trials that aim to target tau."

The team used a new imaging tracer called 18F-PI-2620, to measure tau protein buildup in the brain. They found that when tau levels in the medial temporal lobe­ — a region deep in the brain — exceeded a certain threshold, it strongly indicated cognitive impairment related to AD.

"While our findings support prior research linking medial temporal lobe tau to cognitive impairment, establishing a cut-point in this region using 18F-PI-2620, marks an important step toward defining tau positivity for both research and clinical applications. At the same time, the limited reliability of tau as an indicator of cognitive impairment in non-Hispanic Black participants highlights the need for more diverse populations in research and for future studies to examine both biological and social determinants of Alzheimer's disease," said lead author Victoria R. Tennant, a PhD candidate in USC's Neuroscience Graduate Program.

The findings reflect a growing focus in AD research on making sure diagnostic tools work for everyone — not just in narrow clinical trial populations. Alzheimer's disease is known to affect the brain in stages. While amyloid plaques often build up early, tau tangles are more closely tied to memory loss and other symptoms.

"This type of imaging is critical for understanding who is at risk and how the disease develops," said Stevens INI director Arthur W. Toga, PhD. "These findings are just the latest to come from HABS-HD, which is the most comprehensive study of Alzheimer's disease and related dementias in diverse communities. HABS-HD has already produced key findings related to ethnic variations in AD biomarkers, the influences of social determinants on cognitive health, and vascular contributions to dementia, just to name a few. We hope this work will lead to more personalized care and better outcomes for all communities."

In addition to Tennant and Braskie, the study's other authors are Koral V. Wheeler, Noelle N. Lee, Jamie A. Terner, Maxwell W. Hand, Suchita Ganesan, Patrick Walsh, Aisha Greene, Tyler Berkness, Tiantian Lei, Arthur W. Toga from the Mark and Mary Stevens Neuroimaging and Informatics Institute, Keck School of Medicine of USC, University of Southern California; Rema Raman and Robert A. Rissman from the Alzheimer's Therapeutic Research Institute, Keck School of Medicine of USC, University of Southern California; Bradley T. Christian from the Waisman Center, University of Wisconsin-Madison; Melissa Petersen, Ann D. Cohen, Karin L. Meeker, Zhengyang Zhou, Rajesh R. Nandy and Sid E. O'Bryant from the University of North Texas Health Science Center at Fort Worth; Beau M. Ances from the Washington University School of Medicine in St. Louis; and Kristine Yaffe from the Department of Psychiatry, Neurology, and Epidemiology/Biostatistics, University of California, San Francisco.

This research was supported by the National Institute on Aging of the National Institutes of Health [R01AG054073, R01AG058533, R01AG070862, P41EB015922, and U19AG078109], and by the Office of the Director, the National Institutes of Health, [S10OD032285].

Materials provided byKeck School of Medicine of USC.Note: Content may be edited for style and length.

Brain scan breakthrough reveals why Parkinson’s drugs don’t always work

Simon Fraser University researchers are using a new approach to brain imaging that could improve how drugs are prescribed to treat Parkinson's disease.

The new study, published in the journalMovement Disorders, looks at why levodopa – the main drug used in dopamine replacement therapy – is sometimes less effective in patients.

The drug is typically prescribed to help reduce the movement symptoms associated with the neurodegenerative disorder.

While it is effective in improving symptoms for the vast majority of patients, not everyone experiences the same level of benefit.

In order to find out why this is the case, an SFU collaboration with researchers in Sweden has used magnetoencephalography (MEG) technology to determine how the drug affects signals in the brain.

"Parkinson's is the second most prevalent neurodegenerative disease worldwide and it is the most rapidly increasing, in terms of incidence," says Alex Wiesman, assistant professor in biomedical physiology and kinesiology at SFU.

"Treating this disease, both in terms of helping people with their symptoms, but also trying to find ways to reverse the effects, is becoming more and more important.

"If clinicians can see how levodopa activates certain parts of the brain in a patient, it can help to inform a more personalised approach to treatment."

The study was a collaboration with researchers at Karolinska Institute in Sweden, who used MEG to collect data from 17 patients with Parkinson's disease – a relatively small sample size.

Researchers mapped participants' brain signals before and after taking the drug, in order to see how and where the drug impacted brain activity.

MEG is an advanced non-invasive technology that measures the magnetic fields produced by the brain's electrical signals.

It can help clinicians and researchers to study brain disorders and diseases, including brain injuries, tumors, epilepsy, autism, mental illness and more.

Using this rare brain imaging technology, Wiesman and team developed a new analysis that lets them "search" the brain for off-target drug effects.

"With this new way of analyzing brain imaging data, we can track in real time whether or not the drug is affecting the right brain regions and helping patients to manage their symptoms," says Wiesman.

"What we found was that there's sometimes 'off target' effects of the drug. In other words, we could see the drug activating brain regions we don't want to be activating and that's getting in the way of the helpful effects.

"We found that those people who showed 'off target' effects are still being helped by the drug, but not to the same extent as others."

Parkinson's disease is a neurodegenerative disorder, meaning parts of the brain become progressively damaged over time. It affects predominately the dopamine-producing neurons in a specific area of the brain called the substantia nigra.

People with Parkinson's disease may experience a range of movement-related symptoms, such as tremors, slow movement, stiffness and balance problems.

Wiesman hopes that a better understanding of how levodopa affects an individual's brain signals could improve how drugs are prescribed to treat Parkinson's.

"This might be really helpful for tracking individualized responses to these types of drugs and helping with prescribing and therapeutics," he says.

"So maybe we try different medications, maybe we adjust dosages differently. And this helps clinicians get at that question of how we prescribe personalized medicine in a way that really helps the patient.

"The more we can personalize that approach, make it more expedient, make it a bit more specific to that person, the better."

This new type of brain imaging analysis is not only for studying Parkinson's disease; any medications that affect brain signaling can be studied using the method developed by Wiesman and colleagues.

SFU's ImageTech Lab, at the Surrey Memorial Hospital, is home to the only MEG in western Canada.

"We have this really fantastic technology right here at SFU, and combined with the new analysis approaches that we're developing, it gives us a really unprecedented look into what's happening in the brain," says Wiesman.

"We can use this technology moving forward to study Parkinson's disease in ways that no one has ever done before worldwide.

"Our next step is to take our new approach and apply it to a larger patient group. We also need to translate this research to more accessible brain imaging methods, like electroencephalogram (EEG).

"Ultimately, we want to make sure this technology is useful for a diverse population and more widely accessible to patients with Parkinson's disease."

Materialsprovided bySimon Fraser University.Note: Content may be edited for style and length.