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  • Is Earth inside a huge void? ‘Sound of the Big Bang’ hints at possible solution to Hubble tension

    Is Earth inside a huge void? ‘Sound of the Big Bang’ hints at possible solution to Hubble tension

    image: 

    If we are located in a region with below-average density such as the green dot, then matter would flow away from us due to stronger gravity from the surrounding denser regions, as shown by the red arrows.


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    Credit: Moritz Haslbauer and Zarija Lukic

    Earth and our entire Milky Way galaxy may sit inside a mysterious giant hole which makes the cosmos expand faster here than in neighbouring regions of the universe, astronomers say.

    Their theory is a potential solution to the ‘Hubble tension’ and could help confirm the true age of our universe, which is estimated to be around 13.8 billion years old.

    The latest research – shared at the Royal Astronomical Society’s National Astronomy Meeting (NAM) in Durham – shows that sound waves from the early universe, “essentially the sound of the Big Bang”, support this idea.

    The Hubble constant was first proposed by Edwin Hubble in 1929 to express the rate of the universe’s expansion. It can be measured by observing the distance of celestial objects and how fast they are moving away from us.

    The stumbling block, however, is that extrapolating measurements of the distant, early universe to today using the standard cosmological model predicts a slower rate of expansion than measurements of the nearby, more recent universe. This is the Hubble tension.

    “A potential solution to this inconsistency is that our galaxy is close to the centre of a large, local void,” explained Dr Indranil Banik, of the University of Portsmouth.

    “It would cause matter to be pulled by gravity towards the higher density exterior of the void, leading to the void becoming emptier with time.

    “As the void is emptying out, the velocity of objects away from us would be larger than if the void were not there. This therefore gives the appearance of a faster local expansion rate.”

    He added: “The Hubble tension is largely a local phenomenon, with little evidence that the expansion rate disagrees with expectations in the standard cosmology further back in time.

    “So a local solution like a local void is a promising way to go about solving the problem.”

    For the idea to stand up, Earth and our solar system would need to be near the centre of a void about a billion light-years in radius and with a density about 20 per cent below the average for the universe as a whole.

    Directly counting galaxies does support the theory, because the number density in our local universe is lower than in neighbouring regions.

    However, the existence of such a large and deep void is controversial because it doesn’t mesh particularly well with the standard model of cosmology, which suggests matter today should be more uniformly spread out on such large scales.

    Despite this, new data presented by Dr Banik at NAM 2025 shows that baryon acoustic oscillations (BAOs) – the “sound of the Big Bang” – support the idea of a local void.

    “These sound waves travelled for only a short while before becoming frozen in place once the universe cooled enough for neutral atoms to form,” he explained.

    “They act as a standard ruler, whose angular size we can use to chart the cosmic expansion history.

    “A local void slightly distorts the relation between the BAO angular scale and the redshift, because the velocities induced by a local void and its gravitational effect slightly increase the redshift on top of that due to cosmic expansion.

    “By considering all available BAO measurements over the last 20 years, we showed that a void model is about one hundred million times more likely than a void-free model with parameters designed to fit the CMB observations taken by the Planck satellite, the so-called homogeneous Planck cosmology.”

    The next step for researchers is to compare their local void model with other methods to estimate the history of the universe’s expansion, such as cosmic chronometers.

    This involves looking at galaxies that are no longer forming stars. By observing their spectra, or light, it is possible to find what kinds of stars they have and in what proportion. Since more massive stars have shorter lives, they are absent in older galaxies, providing a way to establish a galaxy’s age.

    Astronomers can then combine this age with the galaxy’s redshift – how much the wavelength of its light has been stretched – which tells us how much the universe has expanded while light from the galaxy was travelling towards us. This sheds light on the universe’s expansion history.

    ENDS


    Media contacts

    Sam Tonkin

    Royal Astronomical Society

    Mob: +44 (0)7802 877 700

    press@ras.ac.uk

     

    Dr Robert Massey

    Royal Astronomical Society

    Mob: +44 (0)7802 877 699

    press@ras.ac.uk

     

    Megan Eaves

    Royal Astronomical Society

    press@ras.ac.uk


    Science contacts

    Dr Indranil Banik

    University of Portsmouth

    indranilbanik1992@gmail.com


    Images & captions

    Inside a void

    Caption: If we are located in a region with below-average density such as the green dot, then matter would flow away from us due to stronger gravity from the surrounding denser regions, as shown by the red arrows.

    Credit: Moritz Haslbauer and Zarija Lukic

     

    Baryon acoustic oscillations

    Caption: Baryon acoustic oscillations (BAOs) – the “sound of the Big Bang” – support the idea of a local void.

    Credit: Gabriela Secara, Perimeter Institute

     

    Cosmic expansion

    Caption: The main techniques for charting the cosmic expansion history, such as supernovae – or standard candles – and cosmic chronometers.

    Credit: Dr Indranil Banik


    Further information

    The talk ‘Theoretical and observational approaches to the Hubble tension’ will take place at NAM at 14:15 BST on Wednesday 9 July 2025 in room OCW017. Find out more at: https://conference.astro.dur.ac.uk/event/7/sessions/90/#20250709

    If you would like a Zoom link and password to watch it online, please email press@ras.ac.uk

     

    The Hubble constant was first proposed by Edwin Hubble in 1929 to express the rate of the universe’s expansion. It can be measured by observing the distance of celestial objects and how fast they are moving away from us.

    The Hubble tension refers to the discrepancy in the measured expansion rate of the universe, specifically between the value based on observations of the early universe and value related to observations of the local universe.

    Baryon acoustic oscillations are a pattern of wrinkles in the density distribution of the clusters of galaxies spread across the universe. They provide an independent way to measure the expansion rate of the universe and how that rate has changed throughout cosmic history.


    Notes for editors

    The NAM 2025 conference is principally sponsored by the Royal Astronomical Society and Durham University.

     

    About the Royal Astronomical Society

    The Royal Astronomical Society (RAS), founded in 1820, encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science.

    The RAS organises scientific meetings, publishes international research and review journals, recognises outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 4,000 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others.

    The RAS accepts papers for its journals based on the principle of peer review, in which fellow experts on the editorial boards accept the paper as worth considering. The Society issues press releases based on a similar principle, but the organisations and scientists concerned have overall responsibility for their content.

    Keep up with the RAS on Instagram, Bluesky, LinkedIn, Facebook and YouTube.

    Download the RAS Supermassive podcast

    About the Science and Technology Facilities Council

    The Science and Technology Facilities Council (STFC), part of UK Research and Innovation (UKRI), is the UK’s largest public funder of research into astronomy and astrophysics, particle and nuclear physics, and space science. We operate five national laboratories across the UK which, supported by a network of additional research facilities, increase our understanding of the world around us and develop innovative technologies in response to pressing scientific and societal issues. We also facilitate UK involvement in a number of international research activities including the ELT, CERN, the James Webb Space Telescope and the Square Kilometre Array Observatory.

    linkedin.com/company/stfc

    ukri.org/councils/stfc

     

    About Durham University 

    Durham University is a globally outstanding centre of teaching and research based in historic Durham City in the UK. 

    We are a collegiate university committed to inspiring our people to do outstanding things at Durham and in the world. 

    We conduct research that improves lives globally and we are ranked as a world top 100 university with an international reputation in research and education (QS World University Rankings 2026). 

    We are a member of the Russell Group of leading research-intensive UK universities and we are consistently ranked as a top five university in national league tables (Times and Sunday Times Good University Guide and The Complete University Guide). 

    For more information about Durham University visit: www.durham.ac.uk/about/



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  • Green energy statecraft and Australia’s clean industry future

    Green energy statecraft and Australia’s clean industry future

    As global supply chains pivot towards low-emissions production, Australia will need to lead, or risk being left behind. The country’s challenge is not a lack of technology, capital, or ambition. It’s a gap in policy architecture. Without bankable demand, Australia’s most promising clean commodity projects – green iron, sustainable aviation fuel, and clean ammonia – remain stuck at the starting line.

    To meet that challenge, we propose a new demand-side policy model: the Clean Commodities Trading Initiative (CCTI) – a flagship example of green energy statecraft. At its heart is a new tool for national transformation: Clean Commodity Credits that reward innovation and emissions savings.

    A market-friendly mechanism to kickstart large-scale clean production.

    Green energy statecraft is a strategic approach to governance that uses the clean energy transition to simultaneously advance a nation’s economic, environmental, social, and geostrategic goals. Unlike conventional industry policy, which focuses on domestic market corrections, statecraft treats clean energy as key to national security and prosperity – used to build alliances, secure supply chains, boost productivity, and shape global rules.

    The European Union, China, Japan, and South Korea are all pursuing variations of green energy statecraft. Australia must do the same – on its own terms, with tools suited to its advantages, institutions, and budget.

    The CCTI is the tool for our times.

    The CCTI is a market-friendly mechanism to kickstart large-scale clean production. Its core function is simple: government acts as an early buyer of clean commodities – not to stockpile goods, but to create the conditions for investment. Clean production projects face long lead times and high capital costs. But their biggest barrier is price uncertainty. Firms can’t justify investment if they don’t know whether the market will pay a green premium to offset higher costs. The CCTI removes that uncertainty. It contracts with producers to buy a baseline volume at agreed floor prices. These offtake agreements give developers and financiers the confidence to proceed.

    Without bankable demand, Australia’s most promising clean commodity projects – such as sustainable aviation fuel – will remain stuck at the starting line (David Syphers/Unsplash)

    But the real innovation lies in what happens next.

    Upon purchasing clean commodities such as green iron, the CCTI would decouple the physical products from their clean attributes by creating Clean Commodity Credits, or Innovation Credits, since the clean attributes reflect not just lower emissions but innovation in production. This dual-market approach allows the physical commodities to be sold in conventional markets while the credits are banked or traded later.

    A clean commodity contains two price components: the base cost of the commodity; and the cost of producing it with low emissions. This second factor – the “green premium” – raises prices above conventional alternatives. Clean Commodity Credits solve that problem. They let clean commodities enter traditional markets without the higher price tag. Meanwhile, the CCTI can offset its support costs by monetising the credits in flexible ways. As we argue in our new paper, it could:

    • Bank credits for future sale as regulatory markets mature
    • Sell credits into voluntary markets to recover costs
    • Create bundled products combining physical commodities with clean attributes

    This flexibility allows the CCTI to adapt as markets evolve, maximising taxpayer value while supporting market development. 

    In effect, these credits create bankable demand for green innovation. They send a clear price signal – not just for carbon, but for the kinds of technologies, processes, and business models that will define the clean economy. They give governments a strategic mechanism to stimulate private investment and build advantage in future-facing sectors.

    If Australia continues to rely on patchwork subsidies and fragmented supply-side measures, it will fall behind.

    Traditional carbon markets, while important, work by penalising emissions. But in heavy industry, where low-carbon alternatives are still emerging, penalties alone often aren’t enough to drive change. Establishing a market for these credits flips the model. Instead of punishing laggards, it rewards leaders. Governments can set clean production targets – say, 30 per cent green steel by 2030 – and let firms meet them by innovating or buying credits from early movers. It creates a race to the top, not just a drag on the bottom line.

    This model rewards firms that act now with firm demand at a price that justifies production – not in 2030 when carbon prices bite or regulation finally arrives. And it allows government to recover its support as credit markets develop. Once established, the same principle can apply to any product the government deems strategic, regardless of its carbon value. Thus Innovation Credits may be the better name.

    Japan and South Korea, two of Australia’s key trading partners, seek long-term access to clean industrial inputs they cannot produce domestically. Australia, with its renewable energy resources and export capacity, is a natural partner. By embedding Clean Commodity or Innovation Credits into trade relationships – through joint offtake agreements, shared credit markets, or co-investment in CCTI-backed facilities – Australia can deepen economic ties and build geopolitical resilience. This is green energy statecraft in action: aligning clean industry development with alliance-building and regional stability.

    The energy transition is a global race. Other countries are moving decisively. If Australia continues to rely on patchwork subsidies and fragmented supply-side measures, it will fall behind. The CCTI offers a smarter, faster, and more strategic path forward. It reflects the kind of governance Australia now needs: bold, integrated, efficient, and effective.

    Green energy statecraft isn’t just theory. It’s practice. And with the right tools, Australia can lead.

    This article relates to a Studies in Statecraft series from the Asia-Pacific Development, Diplomacy & Defence Dialogue (AP4D).

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  • Dry Eye Awareness Month Highlights Condition Affecting Millions

    Dry Eye Awareness Month Highlights Condition Affecting Millions

    Dry eye disease (DED), a condition that is defined by disruptions to the tear film of the eye,1 has recently increased in diagnosis rate, which can be linked to increasing awareness around the condition and greater use of laptops, phones, and TVs. According to Johnson & Johnson, up to 1 in 11 people are diagnosed with DED worldwide,2 with 75% of ophthalmologists reporting more cases than 5 years prior. However, with the increased prevalence comes increased awareness and more treatments dedicated to mitigating the worst of the symptoms of DED.

    Advancements in dry eye disease have made it so that individuals with the condition can receive treatment to alleviate symptoms. | Image credit: 9nong – stock.adobe.com

    DED primarily affects the tear film of the eye,1 with any disruption to the tear film causing watering, itching, blurred vision, or burning sensations. Although each reason for DED is different, most cases of DED have to do with the eyes not producing enough tears or tears that evaporate too quickly, with some cases having both of these root causes. Aqueous deficient dry eye occurs when the lacrimal glands do not produce enough tears, whereas evaporative dry eye is linked to meibomian gland dysfunction causing the evaporation of the tears. To formally diagnose DED, ophthalmologists and optometrists may use the tear breakup time test, which tests how quickly tears evaporate, or the slit lamp test, which shines a light into the eye to examine the eyes and eyelids.

    Meibomian gland dysfunction accounts for 86% of those who have DED, according to Johnson & Johnson,2 making it a primary focus for treating DED, which primarily effects those 50 years and older. DED overall can be difficult to treat due to why dry eye presents itself. However, meibomian gland dysfuction does have a means of being addressed due to advances in care.

    Perfluorohexyloctane ophthalmic solution (Meibo; Bausch & Laumb) has been approved by the FDA for use in dry eye associated with meibomian gland dysfunction.3 The twice-daily drop has been found to decrease the dryness of the eye when used regularly, as it prevents evaporation and stabilizes tears. Although this is the only treatment to specifically target meibomian gland dysfunction, there are other means of addressing chronic dry eye.

    Treatments for chronic dry eye include lacrifill, 0.05% cyclosporine ophthalmic emulsion, 0.09% cyclosporine, 0.1% cyclosporine ophthalmic solution, lifitegrast, and varenicline. Lacrifill works through the injection of a hyaluronic acid-based gel into the tear duct so that natural tears are kept in the eye. The 0.05% cyclosporine ophthalmic emulsion and 0.09% cyclosporine were both created to target the inflammation of the eye through drops twice per day in each eye, although it can take 3 to 6 months before it starts to work. The 0.1% cyclosporine ophthalmic solution, by contrast, aims to increase tear production in the eye using the same active ingredient as the previous 2 medications but with a higher concentration and with a different delivery. Varenicline is a nasal spray that can be used to stimulate the production of mucin, oil, and tears, and it provides an alternative to those who would rather avoid eye drops.

    Not only are there already treatments for DED that patients can use, there are also several treatments in development that may help to pinpoint the root causes of DED and address those areas of concern.3 An ointment produced by Azura Ophthalmics is currently being tested as a means of preventing the buildup of proteins in the meibomian gland ducts, which could produce healthier amounts of oil. Alcon is currently developing a drug, Acoltremon, that targets nerve cells in the cornea and eyelid to produce a cooling sensation that produces more tears. Both of these treatments have seen positive results in early trials.

    As Dry Eye Awareness Month begins, it is important to be aware of the symptoms of dry eye so that they can be easily identified for those who may be living with DED without having a proper diagnosis. Speaking with an ophthalmologist or optometrist about any experienced symptoms can help the health care provider diagnosis the type of DED the patient has and recommend means of treating the condition that can improve overall quality of life.

    References

    1. Dry eyes. Cleveland Clinic. Updated June 20, 2025. Accessed July 7, 2025. https://my.clevelandclinic.org/health/diseases/24479-dry-eye

    2. McCarthy LF. By the numbers: understanding dry eye disease. Johnson & Johnson. July 18, 2024. Accessed July 7, 2025. https://www.jnj.com/health-and-wellness/by-the-numbers-understanding-dry-eye-disease

    3. Mukamal R. Improved dry eye drugs for 2025 and beyond. American Academy of Ophthalmology. January 24, 2025. Accessed July 7, 2025. https://www.aao.org/eye-health/tips-prevention/new-dry-eye-treatments-ocular-surface-disease

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  • Exploring The Habitability And Interior Composition Of Exoplanets Lying Within The Extended Habitable Zone

    Exploring The Habitability And Interior Composition Of Exoplanets Lying Within The Extended Habitable Zone

    Distribution of 339 planets in the stellar effective flux (𝑆eff) versus stellar temperature (𝑇eff) space. Red solid circles indicate the 17 planets orbiting within the EHZ, while gray points depict the remaining planets. Solar system planets are marked with purple circles. The green solid lines correspond to the inner and outer edges of the classical 1D habitable zone, as defined by Kopparapu et al. (2013). The blue dashed line represents the inner edge of the Extended Habitable Zone (EHZ) around M dwarf stars, assuming 30% heat transport efficiency (Wandel 2023a). The brown curve marks the outer edge of the EHZ, determined by the melting of ice sheets driven by geothermal heat (Wandel 2023b). The gray dashed line indicates the tidally locked radius around M dwarf stars. The green shaded region defines the classical HZ and the blue shaded region highlights the extended HZ for tidally locked exoplanets. — astro-ph.EP

    Studying the habitability, internal structure and composition of exoplanets is crucial for understanding their potential to sustain life beyond our solar system.

    Characterizing planetary structures and atmospheric evolution provides valuable insights into surface conditions and the long-term habitability of these planets. In this study, we present a comprehensive analysis of exoplanets spanning from super-Earths to mini-Neptunes (Rp ≤ 4 R and Mp ≤ 15 M) located within the extended habitable zone, along with parameterization of their host stars.

    We find that the planets in our sample orbit M dwarf stars and are tidally locked to them. Using archival photometric data from Gaia, Pan-STARRS1, 2MASS, and WISE, we estimate the atmospheric and physical parameters of the host stars.

    We also model the interior structure of these planets to infer their possible compositions. Additionally, under the assumption that these exoplanets can accrete a gaseous layer, we model the envelope fraction of the habitable exoplanets.

    With an Earth-like rocky composition, LHS 1140 b and TOI-1452 b can hold onto negligible amount of their initial gas layer. However, sustaining a sufficient amount of atmosphere over time, the planets LP 791-18 c, LTT 3780 c and K2-18 b are likely to be water worlds.

    The models suggest a water rich composition for TOI-1266 c without any significant amount of atmosphere. Modeling interior compositions and atmospheric escape scenarios allow us to assess the potential habitability of these planets by evaluating the likelihood of surface liquid water and the retention of stable atmospheres.

    Sushmita Deb, Kaushal Sharma, Samrat Biswas, Biman Jyoti Medhi

    Comments: 15 pages, 6 figures
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
    Cite as: arXiv:2507.04440 [astro-ph.EP] (or arXiv:2507.04440v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2507.04440
    Focus to learn more
    Related DOI:
    https://doi.org/10.1093/mnras/staf1057
    Focus to learn more
    Submission history
    From: Sushmita Deb
    [v1] Sun, 6 Jul 2025 15:58:53 UTC (15,164 KB)
    https://arxiv.org/abs/2507.04440
    Astrobiology,

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  • BIKE CHECK: Anna Henderson’s Pink Madone

    BIKE CHECK: Anna Henderson’s Pink Madone

    Lidl-Trek’s mechanics have been hard at work to prepare a beautiful pink Trek Madone to celebrate Anna Henderson’s lead of the Giro d’Italia. Anna took the race lead, along with an excellent stage win, on the second day of the Italian Grand Tour. After a bold 40km attack, Anna outsprinted her breakaway companion, to win her first Grand Tour stage and move into the race lead by 15 seconds.

    I felt super proud to wear the Maglia Rosa today. The Team gave me special things to wear: I had pink glasses, helmet and bike. I was dressed in Pink from head to toe and it felt super special. It’s a day I will remember.

    Team mechanic Vincent gets to work after the stage

    Final touches put together with Union Tools

    And it’s Time to get this bike to its rightful owner

    Special delivery!

    The golden hour sun hits different on a pink Madone

    No bike build is complete without a SRAM groupset and Pirelli tires

    BAAW

    And on the road to Stage 3!


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  • Was Earth’s Water Acquired Locally During The Earliest Phases Of The Solar System Formation?

    Was Earth’s Water Acquired Locally During The Earliest Phases Of The Solar System Formation?

    Water-equivalent content by weight in the Solar System and model predictions. Left upper panel: Midplane temperature of the disk using T1au = 145, 180, 200 and 300 K (from light blue to dark blue respectively) in Eq. 2. Left lower panel: The solid curves show the snowlines calculated using the Tinacci et al. (2023) BE distribution for the different temperature profiles (colours code as above). The data points show the median values of the water-equivalent content by weight for different objects of the Solar System (Sec. 3), where vertical bars represent the minimum and maximum range. Please note that the values reported in Tab. 1 are considered upper limits (see text). The uncertainty of the formation region of the various objects are shown as ellipses, distinguishing NC, CC, and comet populations. Right: Computed snowlines using T1au = 200 K in Eq. 2 and different models (see text): BE distribution (solid line), single BE (dashed) and condensation at 180 K (dotted). The right and left panels share the same vertical axis. — astro-ph.EP

    The origin of the terrestrial water remains debated, as standard Solar System formation models suggest that Earth formed from dry grains, inside the snowline of the Proto-Solar Nebula (PSN).

    Here, we revisit this issue through the lens of computational chemistry. While the classically used snowline relies on a single condensation temperature, recent work in quantum chemistry shows that the binding energy of water on icy grains has a gaussian distribution, which implies a gradual sublimation of water rather than a sharp transition. We use the computed distribution of binding energies to estimate the radial distribution of adsorbed ice on the dust grains across the PSN protoplanetary disk.

    Our model reproduces the full range of estimated water abundances on Earth and matches the hydration trends observed in chondrite groups at their predicted formation distances. Thus, we suggest that a significant fraction of Earth’s water may have been acquired locally at early stages of the Solar System formation, without requiring delivery from beyond the classical snowline.

    Lise Boitard-Crépeau, Cecilia Ceccarelli, Pierre Beck, Lionel Vacher, Piero Ugliengo

    Comments: 7 pages, 2 figures, published in ApJL
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
    Cite as: arXiv:2507.03968 [astro-ph.EP] (or arXiv:2507.03968v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2507.03968
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    Journal reference: ApJL 987 (2025) L25
    Related DOI:
    https://doi.org/10.3847/2041-8213/ade5aa
    Focus to learn more
    Submission history
    From: Lise Boitard-Crépeau
    [v1] Sat, 5 Jul 2025 09:17:34 UTC (740 KB)
    https://arxiv.org/abs/2507.03968
    Astrobiology,

    Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻

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  • Some stomach cancer cases can be prevented by targeting bacteria – NewsNation

    1. Some stomach cancer cases can be prevented by targeting bacteria  NewsNation
    2. Global lifetime estimates of expected and preventable gastric cancers across 185 countries  Nature
    3. A common bacteria could cause 12 million cases of stomach cancer  Euronews.com
    4. Study projects over 15 million people born during 2008-2017 could develop gastric cancer in life  The Hindu
    5. Simple Treatment Could Prevent 75% of Stomach Cancer Cases, Doctors Reveal  NDTV

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  • Yaamava’ Resort & Casino Giving Away the Holy Grail of Comics: Action Comics #1

    Yaamava’ Resort & Casino Giving Away the Holy Grail of Comics: Action Comics #1

    Hollywood Stars and Comic Legends Align at Yaamava’ with Special Appearances by Dean Cain, Kevin Smith and Ralph Garman

    HIGHLAND, Calif., July 8, 2025 /PRNewswire/ –The top-ranked, most valuable comic book in the world is up for grabs at Yaamava’ Resort & Casino at San Manuel: a graded copy of Action Comics #1, the 1938 issue that launched the superhero era. Considered a cornerstone of pop culture history, only 78 graded copies of this legendary comic are known to exist, and one lucky Club Serrano member will win it in the grand finale of the Holy Grail of Comics promotion on August 5.

    “This isn’t just a giveaway—it’s a once-in-a-lifetime opportunity to own the most iconic comic ever published,” said Kenji Hall, General Manager, Yaamava’ Resort & Casino at San Manuel. “At Yaamava’, our guests are the real superheroes, and we can’t wait to bring them yet another epic moment.”

    To celebrate the final stretch of the Holy Grail of Comics promotion, Yaamava’ will host two star-studded events.

    On July 11 at 6 p.m., filmmaker, actor and author Kevin Smith and actor/comedian Ralph Garman will bring their hit podcast, Hollywood Babble-On, to Tukut Lounge at Yaamava’ Resort & Casino for a fan-focused night of comic-culture celebration. Limited tickets available online at Yaamava.com/HollywoodBabbleOn.

    On August 5, Dean Cain, known for his role as Clark Kent/Superman in the ABC television series Lois & Clark: The New Adventures of Superman, will unveil the lucky winner who gets to take home the coveted Action Comics #1.

    Club Serrano members began earning entries for the Holy Grail of Comics giveaway on June 1, 2025. Entries can be earned through August 5 until 8:50 p.m.

    In addition to earning entries, visitors can pose for photos in the specially designed “fortress” display housing the comic or receive surprise “cape drops”—instant entry into the grand finale drawing.

    The Holy Grail of Comics is a historic celebration of comics, collectors and pop culture.

    For full promotion details, visit Yaamava.com. 

    About Yaamava’ Resort & Casino at San Manuel:
    Yaamava’ Resort & Casino at San Manuel is the only AAA Five-Diamond rated entertainment destination in the West, featuring a Forbes Travel Guide Four-Star hotel with spacious suites, an elevated pool deck, a Forbes Five-Star spa, and a state-of-the-art theater. Recently named the 2024 USA TODAY 10Best Readers’ Choice Award for Best Casino Outside of Las Vegas and Best Casino Restaurant for its Pines Modern Steakhouse as well as Best Native American Casino and Best Overall Casino Outside of Las Vegas by the Newsweek Readers’ Choice Awards, Yaamava’ is located just 70 miles from downtown Los Angeles in Highland, CA. The Casino has more than 7,400 slots, five high-limit gaming rooms, luxury retail shops, a wide variety of award-winning dining options, and more than a dozen bars and lounges, including IE’s premiere sports bar, The 909 Food Hall. The San Manuel Entertainment Authority owns and operates Yaamava’ Resort & Casino.

    For more information, visit www.yaamava.com or follow us on Instagram, TikTok, Facebook, Threads and X (formally known as Twitter).

    SOURCE Yaamava’ Resort & Casino


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  • Billie Eilish & UMG Upcycle 400K Tees in Bold Move for Sustainable Merch

    Billie Eilish & UMG Upcycle 400K Tees in Bold Move for Sustainable Merch

    Key Takeaways

    Merch Recycling Initiative: Thanks to a project spearheaded by Billie Eilish, Universal Music Group is repurposing over 400,000 unsold T-shirts into new garments through a textile recycling partnership.


    Sustainability in Music: The project reflects a broader industry trend toward sustainable merchandise, especially among artists with younger, eco-conscious audiences.

    More than 400,000 unsold concert tees are getting a second life.

    Singer Billie Eilish and her mother, Maggie Baird, have been working with Universal Music Group (UMG) – which represents Eilish – to find a more sustainable solution for the thousands of pounds of unsold concert merchandise the label has in its massive Nashville warehouse. Bravado, UMG’s merch arm, has stored unsold apparel there for years, if not decades, President Matt Young told Fast Company.

    Eilish’s concert stop in Quebec last year broke the venue’s record for most single-day merch sales.

    Rather than simply donating them – which can, in some sectors, just lead to apparel ending up in landfills or incinerated – Bravado partnered with Spanish clothing designer and textile manufacturer Hallotex to upcycle the old concert merch into new.

    The company is shipping more than 400,000 old T-shirts to Morocco, where Hallotex will unspool them into cotton yarn and then respin them into more than 280,000 new 100% cotton tees that UMG artists will use in the fall. Shirts that can’t be recycled will be shredded and turned into housing insulation.

    “We are drowning in clothes on this planet, much of which is in landfills, much of which is shipped to other countries to pollute their waters and their land,” Baird – Eilish’s mother – told Fast Company. “I think we have to be extremely thoughtful about what merch gets put out in the world – why does it exist, how is it made and what happens to it in its second life?”

    UMG warehouse

    UMG’s Nashville warehouse has thousands of pounds of old, unused concert merch that will now be upcycled into new cotton tees. (Courtesy of UMG/Bravado)

    Music merch has long been an essential part of the concert experience, with high demand from fans of all ages at events from Taylor Swift’s mega Eras Tour to the Oasis reunion. It’s an industry expected to reach $16.3 billion in global sales within the next five years.

    And Eilish is already no stranger to incorporating sustainable merch into that demand. She has a section of her online merch store dedicated to apparel made from recycled materials, including from a recent Earth Day partnership with three sustainable businesses. On her HIT ME HARD AND SOFT tour last year, she played a video before each show about her choice to offer sustainable merch options and what that looks like.

    Her push for sustainable concert merch, though, is particularly impactful because of her heavily Gen Z audience. A recent ASI Research study on promotional products consumers found that more than 70% of Gen Z consumers said it was important for promo they receive to be environmentally friendly, more than other generations.

    Young – Bravado’s president – said that it’s been Eilish, Baird and several other young artists that have pushed UMG and Bravado toward more sustainable merch options, including the upcycling program, since he’s been at the helm of the company.

    And Eilish’s project is yet another indicator that sustainability is becoming more of a “must-have” than a “nice-to-have” for promo firms and beyond. Is now the time to make a joke about giving these tees a “Happier Than Ever” ending?

    Promo for the Planet is your destination for the latest news, biggest trends and best ideas to help build a more sustainable and socially-responsible industry.


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  • Fact check: Rana Sanaullah said Pakistan should follow the Muslim world’s position on the Abraham Accords – World

    Fact check: Rana Sanaullah said Pakistan should follow the Muslim world’s position on the Abraham Accords – World

    Posts from users on social media platform X on July 3 shared a post from digital media outlet Siasat.pk that attributed a statement to Adviser to the Prime Minister Rana Sanaullah that Pakistan should follow the Arab position on the Abraham Accords. However, the PML-N leader actually said that Pakistan should follow the position of the Muslim world on the issue.

    The Israeli offensive, which began in response to Hamas’s unprecedented attack on October 7, 2023, has killed more than 57,000 Palestinians and destroyed much of the housing and hospital infrastructure in the enclave.

    The Abraham Accords, brokered by the United States in 2020, are landmark agreements for diplomatic relations between Israel and several Arab nations, including the United Arab Emirates, Bahrain, Morocco and Sudan. These accords paved the way for formal ties, such as embassies and trade deals, underpinned by mutual interests in security, economic collaboration, and technology exchange. While celebrated as a diplomatic shift in the Middle East, the accords also sparked debate and resistance in Pakistan. Foreign Minister Ishaq Dar and Defence Minister Khawaja Asif have both affirmed that Pakistan will not join, asserting that any recognition of Israel would contradict its longstanding support for a two‑state solution and could only be considered if it served Pakistan’s national interest.

    On July 3, a post from Siasat.pk on X shared a visual with the following quote attributed to Sanaullah: “Pakistan, Saudi Arabia, Turkey, and Iran should make a joint decision regarding the Abraham Accords, Pakistan should align with Arab countries on the Abraham Accords.”

    The post gained 15,000 views.

    The same visual was also shared by former anchorpersons Imran Riaz and Sabir Shakir, both criticising it and racking up over 100,000 and 7,000 views, respectively.

    It was reposted by a user, who, according to his X bio, is a journalist, with the caption: “Why have the ministers suddenly caught the fever of the Abraham Accords?”

    It was shared on X by a user who is known for criticising PTI and, more recently, the PML-N.

    The caption of the post questioned its authenticity, asking: “Did Rana sahib really make this statement, or is it just a stunt?”

    The post was viewed by more than 29,000 users.

    A fact-check was initiated to determine the veracity of the claim due to keen public interest in the Abraham Accords and because many PML-N supporters were observed contesting the post.

    Scanning the QR code in Siasat.pk’s post redirected to a July 2 X post by journalist Nadeem Malik, who had shared a 4:30-minute clip from his show ‘Nadeem Malik Live’, which featured Sanaullah as a guest.

    The caption of his X post also attributed the same quote to the official as the post from Siasat.pk.

    The transcript of the clip is provided below:

    Nadeem Malik: “Rana Sahib, what is your opinion on the Abraham Accords? How should Pakistan move forward?”

    Rana Sanaullah: “Look, the party or the government currently can’t have an opinion on the matter because this issue has not been presented or discussed at that level. As my two respected [fellow guests] have shared their personal opinion, I can share mine too. In my personal opinion … there has been a lot of bloodshed and injustice in Palestine. All Muslim countries and the world should establish peace there and the daily bloodshed must stop.

    “For this purpose, if there is any kind of accord there, whether it is the Abraham [Accords] or any other kind of agreement between those forces and people directly involved there … and if it is acceptable to the group (Hamas) representing the Palestinians and the Arab countries sharing the border and then are agreed then I think Pakistan, Saudi Arabia, Turkiye and if Iran is included as well, these are major countries, there is Malaysia too, then they should make a joint decision and Pakistan should go with the Muslim world.

    “If Saudi Arabia, Turkiye and Iran make a decision, and the Arab states directly impacted by this matter make a decision, then Pakistan should go along with it.”

    Reviewing the clip makes it clear that Sanaullah said Pakistan should go along with what the majority of the Muslim world and its major regional players in the Middle East decide regarding the Abraham Accords.

    Therefore, the fact-check determined that the claim that PM aide Rana Sanaullah said that Pakistan should follow the Arab position on the Abraham Accords is misleading.

    The official said that Pakistan should follow the position of the Muslim world on the issue, including countries such as Saudi Arabia, Iran, Turkiye, Malaysia and the Arab states directly impacted by the situation in the Middle East. To omit the names of the other countries or the mention of the Muslim world has the potential to misguide the public into thinking he said Pakistan should follow the Arab position on the matter, making it seem as if he was arguing for Pakistan’s subservience to its Arab allies.


    This fact check was originally published by iVerify Pakistan — a project of CEJ-IBA and UNDP.

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