logo
Largest Structure in The Universe May Be 50% Larger Than We Thought

Largest Structure in The Universe May Be 50% Larger Than We Thought

Yahoo26-04-2025
The largest known structure in the Universe may be even larger than the large we thought it was.
A re-examination of the distribution of powerful space explosions suggests that the Hercules-Corona Borealis Great Wall, a cluster of galaxies previously estimated to be 10 billion light-years long, could actually be as large as 15 billion light-years in size.
That's not only mind-blowing in scale, but poses a huge challenge to our understanding of the Universe. The findings have been submitted for publication, and can be read on the preprint server arXiv.
The Hercules-Corona Borealis Great Wall (or Great Wall, for short) was discovered more than a decade ago, when astronomers noticed that gamma-ray bursts were happening in a concentration that was higher than the expected distribution.
Gamma-ray bursts are the most powerful explosions in the Universe, produced during extreme events such as the core-collapse supernova birth of a black hole and the collision of two neutron stars.
Since black holes and neutron stars both form from massive stars, gamma-ray bursts are associated with the populations of massive stars that are usually found in galaxies.
Because they are so bright, gamma-ray bursts can be observed across enormous distances, and their concentrations can be used as a proxy to map galaxy clusters. The study of 283 gamma-ray bursts is what led astronomers István Horváth, Jon Hakkila, and Zsolt Bagoly to report the discovery of the Great Wall in 2014.
Now, the three scientists have joined a larger team to conduct a more detailed study of gamma-ray bursts across the sky to try to get a more accurate sense of the scale of the Great Wall.
They have closely examined 542 gamma-ray bursts with known redshifts – that is, the extent to which their light has been stretched to redder wavelengths by the expansion of the Universe, thus providing a confident measure of distance.
Their results showed that the Great Wall may extend from a redshift of 0.33 to a redshift of 2.43 – a total distance of around 15 billion light-years (the observable Universe is around 93 billion light-years across).
It's a finding that makes the problem posed by the Great Wall even more pronounced.
This is because our standard model of the evolution of the Universe is founded on something called the cosmological principle. This states that, on large enough scales, the Universe is homogeneous, or 'smooth', in all directions.
Each section of the Universe should look more or less like every other section of the Universe, with no major inconsistencies or bumps. This has been confirmed by multiple lines of evidence.
A structure larger than around 1.2 billion light-years would be considered a major inconsistency, and we've found quite a few of those.
A super-structure called Quipu measures about 1.3 billion light-years wide, while the Sloan Great Wall spans around 1.37 billion light-years. The discovery of a similar structure called the South Pole Wall, also around 1.37 billion light-years across, was announced in 2020.
The Clowes-Campusano LQG group of galaxies is 2 billion light-years across, the Giant Arc is around 3.3 billion light-years across, and the Huge Large Quasar Group is 4 billion.
Then there's the Great Wall, which at 10 billion light-years across, was already an extreme outlier. The new results have upped the ante.
Previously, the Great Wall's entire existence was debated. The new results show that evidence of the structure is not a statistical fluctuation or a sampling bias. It appears to be very much real. What the data means beyond that – what the structure tells us about the Universe and its evolution – has not yet been explored.
However, what we do know is that there's a whole lot about the Universe that we don't know, and that we can't really make sense of yet.
Somewhere out there, the answers are waiting. It's discoveries like this that are inching us ever closer to finding them.
The team's findings have been submitted for publication, and are available on arXiv.
First Utterly Alone Black Hole Confirmed Roaming The Cosmos
Rare 'Smiley Face' Moon About to Hit The Sky With Venus And Saturn
Hubble Celebrates 35 Years by Gifting Us 4 Breathtaking Cosmic Images
Orange background

Try Our AI Features

Explore what Daily8 AI can do for you:

Comments

No comments yet...

Related Articles

Hercules Metals Completes District-Scale MT-NSIP Survey on Hercules Property, Idaho
Hercules Metals Completes District-Scale MT-NSIP Survey on Hercules Property, Idaho

Yahoo

time09-07-2025

  • Yahoo

Hercules Metals Completes District-Scale MT-NSIP Survey on Hercules Property, Idaho

Enhanced survey method enables imaging at depths of up to 6 km Toronto, Ontario--(Newsfile Corp. - July 9, 2025) - Hercules Metals Corp. (TSXV: BIG) (OTCQB: BADEF) (FSE: C0X) ("Hercules" or the "Company") is pleased to announce the successful completion of a large-scale (>100 square kilometre) magnetotelluric and natural-source induced polarization ("MT-NSIP") geophysical survey by Moombarriga USA ("M-Geo") over the Company's Hercules Property in western Idaho (the "Property"), including its flagship Leviathan porphyry copper discovery and newly-added claims. An additional 20 square kilometres was surveyed on the adjacent Cuddy Mountain property1, held by Scout Discoveries Corp. ("Scout"), as part of a collaborative survey initiative. The combined 120 km² dataset is now being processed and inverted as a single contiguous block, which allows resistivity to be reliably modelled to depths of up to six (6) kilometres, significantly beyond the ~800-metre penetration achieved from the conventional DC-IP survey completed in 2023. Survey Highlights Expanded Coverage: The 120 km² MT-NSIP survey expands upon the previous 12 km² and 11 km² DC-IP grids completed by Hercules and Scout, respectively. Superior Depth Penetration: By utilizing long-wavelength natural currents, MT-NSIP enables imaging at depths an order of magnitude greater than the previous active-source DC-IP methods. MT Resistivity Applications: Mapping of regional fault structures and structural intersections. Advanced interpretation of alteration zonation. Porphyry centres often present as a conductive phyllic halo surrounding a resistive potassic core. NSIP Innovation: NSIP is a novel emerging method to derive deep chargeability data, up to two (2) kilometres depth, using the same natural-source input as MT. Partially funded by a third party, this survey may serve as a pioneering industry case study if its results prove successful. The survey aims to explore for extensions of the Leviathan porphyry and potentially identify other centres associated with disseminated sulfide mineralization, which may occur within the project area. Figure 1: MT-NSIP stations relative to previous conventional active-source DC-IP surveys on the Hercules Property and adjacent Cuddy Mountain project. To view an enhanced version of this graphic, please visit: Discussion and Preliminary Analysis The decision to collaborate with Scout on a broader regional survey served two strategic purposes: Regional Fault Targeting: Modelling at this scale enhances the ability to interpret large structural corridors, which often serve as conduits for porphyry emplacement. With Hercules' significantly expanded land position (see Hercules March 4, 2025 news release), the potential for additional concealed centres can now be further unlocked. Enhanced Depth Resolution: The broader survey area increases the effective survey aperture (area), which enables significantly deeper geophysical imaging. Preliminary Resistivity Results and Insight M-Geo has delivered a preliminary resistivity dataset ahead of the inversion modelling, revealing several key insights: Regional fault structures cut northeast and northwest across the Property, indicating potential district-scale structural controls. A conductivity anomaly associated with the Leviathan Porphyry indicates expansion potential along trend, and provides a baseline for evaluating the prospectivity of other new anomalies across the Property. A prominent resistivity high has emerged beneath a multi-kilometre soil and rock chip anomaly in the Eastern Block Zone. The anomaly appears consistent with a potential buried intrusive stock. New surface mapping demonstrates a folding pattern consistent with doming, which may support the presence of an underlying intrusive stock. Ongoing inversion of the resistivity data will better define the anomaly's geometry, and if successful, chargeability data may indicate the presence of disseminated sulfides. Next Steps With field acquisition complete, inversion modelling is underway. Results will be integrated with the Company's existing geological, geophysical and geochemical datasets. The Company anticipates that this integration will yield targets for additional porphyry centres on the expanded Hercules land package. Qualified Person The scientific and technical information in this news release has been reviewed and approved for disclosure by Dillon Hume, and Vice President, Exploration for the Company. Mr. Hume is a "Qualified Person" for Hercules Metals within the meaning of National Instrument 43-101 - Standards of Disclosure for Mineral Projects. About Hercules Metals Corp. Hercules Metals Corp. (TSXV: BIG) (OTCQB: BADEF) (FSE: C0X) is an exploration Company focused on developing America's newest porphyry copper district, in Idaho. The 100% owned Hercules Project located northwest of Cambridge, hosts the newly discovered Leviathan porphyry copper system, one of the most important new discoveries in the region to date. The Company is well positioned for growth through continued drilling, supported by a strategic investment from Barrick Mining Corporation. With the potential for significant scale, the Company's management and board of directors aims to build on its proven track record which includes the discovery and development of numerous precious metals projects worldwide. For further information please contact: Chris PaulCEO & DirectorTelephone +1 (604) 670-5527Email: chris@ Dillon HumeVP, ExplorationTelephone: +1 (604) 283-2043Email: dhume@ This news release does not constitute an offer to sell or a solicitation of an offer to buy any of the securities in the United States. Any securities referred to herein have not and will not be registered under the United States Securities Act of 1933, as amended (the "U.S. Securities Act") or any state securities laws and may not be offered or sold within the United States or to U.S. Persons unless registered under the U.S. Securities Act and applicable state securities laws of an exemption from such registration is available. Disclaimer for Forward-Looking Information This news release contains certain information that may be deemed "forward-looking information" with respect to the Company within the meaning of applicable securities laws. Such forward-looking information involves known and unknown risks, uncertainties and other factors that may cause the Company's actual results, performance or achievements, or developments in the industry to differ materially from the anticipated results, performance or achievements expressed or implied by such forward-looking information. Forward-looking information includes statements that are not historical facts and are generally, but not always, identified by the words "expects," "plans," "anticipates," "believes," "intends," "estimates," "projects," "potential" and similar expressions, or that events or conditions "will," "would," "may," "could" or "should" occur. Forward-looking information contained in this press release may include, without limitation, the expected execution of future exploration programs on the Property; assay results of future drill holes; results of operations, and the expected financial performance of the Company. Although the Company believes the forward-looking information contained in this news release is reasonable based on information available on the date hereof, by its nature, forward-looking information involves assumptions and known and unknown risks, uncertainties and other factors which may cause our actual results, level of activity, performance or achievements, or other future events, to be materially different from any future results, performance or achievements expressed or implied by such forward-looking information. Examples of such assumptions, risks and uncertainties include, without limitation, assumptions, risks and uncertainties associated with general economic conditions; the Covid-19 pandemic; adverse industry events; the receipt of required regulatory approvals and the timing of such approvals; that the Company maintains good relationships with the communities in which it operates or proposes to operate, future legislative and regulatory developments in the mining sector; the Company's ability to access sufficient capital from internal and external sources, and/or inability to access sufficient capital on favorable terms; mining industry and markets in Canada and generally; the ability of the Company to implement its business strategies; competition; the risk that any of the assumptions prove not to be valid or reliable, which could result in delays, or cessation in planned work, risks associated with the interpretation of data, the geology, grade and continuity of mineral deposits, the possibility that results will not be consistent with the Company's expectations, as well as other assumptions risks and uncertainties applicable to mineral exploration and development activities and to the Company, including as set forth in the Company's public disclosure documents filed on the SEDAR+ website at THE FORWARD-LOOKING INFORMATION CONTAINED IN THIS PRESS RELEASE REPRESENTS THE EXPECTATIONS OF HERCULES METALS AS OF THE DATE OF THIS PRESS RELEASE AND, ACCORDINGLY, IS SUBJECT TO CHANGE AFTER SUCH DATE. READERS SHOULD NOT PLACE UNDUE IMPORTANCE ON FORWARD-LOOKING INFORMATION AND SHOULD NOT RELY UPON THIS INFORMATION AS OF ANY OTHER DATE. WHILE HERCULES METALS MAY ELECT TO, IT DOES NOT UNDERTAKE TO UPDATE THIS INFORMATION AT ANY PARTICULAR TIME EXCEPT AS REQUIRED IN ACCORDANCE WITH APPLICABLE LAWS. Neither the TSX Venture Exchange nor its Regulation Services Provider (as that term is defined in the policies of the TSX Venture Exchange) accepts responsibility for the adequacy or accuracy of this press release. ________________________1 This news release contains information about adjacent properties on which Hercules has no right to explore or mine. Readers are cautioned that mineral deposits on adjacent properties are not indicative of mineral deposits on the Company's properties. To view the source version of this press release, please visit Error in retrieving data Sign in to access your portfolio Error in retrieving data Error in retrieving data Error in retrieving data Error in retrieving data

Bio-Rad Expands Droplet Digital PCR Offering Through Strategic Acquisition and Platform Rollout
Bio-Rad Expands Droplet Digital PCR Offering Through Strategic Acquisition and Platform Rollout

Yahoo

time07-07-2025

  • Yahoo

Bio-Rad Expands Droplet Digital PCR Offering Through Strategic Acquisition and Platform Rollout

HERCULES, Calif., July 07, 2025--(BUSINESS WIRE)--Bio-Rad Laboratories, Inc. (NYSE: BIO and BIO.B), a global leader in life science research and clinical diagnostics products, today announced the launch of four new Droplet Digital™ PCR (ddPCR™) platforms. The newly introduced instruments include Bio-Rad's QX Continuum™ ddPCR system along with the QX700™ series of ddPCR platforms acquired as part of the company's recently completed acquisition of digital PCR developer Stilla Technologies. Together with Bio-Rad's existing line of QX200™ and QX600™ ddPCR systems, the expanded product portfolio, including over 400,000 assays, offers the most comprehensive line of digital PCR products for life science research and diagnostic applications. The end-to-end solutions feature industry-leading absolute quantification, high precision, and advanced multiplexing capabilities, combined with streamlined and simplified workflows. "With this launch, our expanded portfolio of instruments, reagents, software, and services extends Bio-Rad's presence in the genomics research and applied science markets and strengthens our leadership in droplet digital PCR solutions," said Jim Barry, EVP and President of Bio-Rad's Life Science Group. "The newly introduced platforms complement Bio-Rad's existing QX ddPCR portfolio and offer our customers unparalleled workflow simplicity and throughput capabilities across the full spectrum of digital PCR applications including oncology, infectious disease, and genetic research." The QX Continuum™ ddPCR system is designed for translational research applications. It features qPCR-like workflow offering simplicity, performance and flexibility in an all-in-one configuration with four-color multiplexing and up to eight discrete thermal profiles per plate. The QX700™ series consists of three new ddPCR instruments designed for academic research, environmental testing, cell and gene therapy, and biopharma quality control workflows. The systems enable seven-color multiplexing, capacity to process over 700 samples per day, with minimal input volume, continuous loading capability, and easy-to-use software for streamlined data interpretation. To learn more about the new QX Continuum and QX700 series, as well as Bio-Rad's comprehensive portfolio of digital PCR instruments, consumables, and assays visit: BIO-RAD, QX CONTINUUM, QX700, QX600, QX200, DROPLET DIGITAL, and DDPCR are trademarks of Bio-Rad Laboratories, Inc. in certain jurisdictions. About Bio-Rad Bio-Rad Laboratories, Inc. (NYSE: BIO and BIO.B) is a leader in developing, manufacturing, and marketing a broad range of products for the life science research and clinical diagnostics markets. Based in Hercules, California, Bio-Rad operates a global network of research, development, manufacturing, and sales operations with approximately 7,700 employees and $2.6 billion in revenues in 2024. Our customers include universities, research institutions, hospitals, and biopharmaceutical companies, as well as clinical, food safety and environmental quality laboratories. Together, we develop innovative, high-quality products that advance science and save lives. To learn more, visit Forward-Looking Statements This release may be deemed to contain certain forward-looking statements within the meaning of the Private Securities Litigation Reform Act of 1995. These forward-looking statements include, without limitation, statements we make regarding our products and our expectations about our products. Forward-looking statements generally can be identified by the use of forward-looking terminology such as "plan", "believe," "expect," "anticipate," "may," "will," "intend," "estimate," "continue," or similar expressions or the negative of those terms or expressions, although not all forward-looking statements contain these words. Such statements involve risks and uncertainties, which could cause actual results to vary materially from those expressed in or indicated by the forward-looking statements. These risks and uncertainties include risks relating to our international operations, global economic and geopolitical conditions, tariffs or other trade barriers, reductions in government funding or capital spending of our customers, our ability to develop and market new or improved products, our ability to compete effectively, international legal and regulatory risks, supply chain risks, and product quality and liability issues. For further information regarding our risks and uncertainties, please refer to the "Risk Factors" and "Management's Discussion and Analysis of Financial Condition and Results of Operation" in Bio-Rad's public reports filed with the Securities and Exchange Commission, including our most recent Annual Report on Form 10-K and our Quarterly Reports on Form 10-Q. Bio-Rad cautions you not to place undue reliance on forward-looking statements, which reflect an analysis only and speak only as of the date hereof. We disclaim any obligation to update these forward-looking statements. View source version on Contacts Investor Contact: Edward Chung, Investor Relations510-741-6104ir@ Media Contact: Anna Gralinska, Corporate Communications510-741-6643cc@

Wyoming Skies: Long, deepening colors of twilight make July a month to remember
Wyoming Skies: Long, deepening colors of twilight make July a month to remember

Yahoo

time29-06-2025

  • Yahoo

Wyoming Skies: Long, deepening colors of twilight make July a month to remember

Stargazing in July hopefully promises warm nights in Wyoming. The highlight of July evenings is the prominent band of the Milky Way arcing across the dark skies. Along the Milky Way, you'll spot the Summer Triangle and the Teapot of Sagittarius and Scorpius hovering over the southern horizon. Additionally, there are numerous deep-sky objects to study in a single night. To enhance the summer skies, two of the strongest meteor showers of the year streak overhead. While I consider July nights my favorite, as a student once pointed out, 'you always say that,' I can't deny it. Begin your July evening by enjoying the long, deepening colors of twilight. As darkness falls, the first stars start to appear. Arcturus and Vega are the brightest stars overhead, followed by Altair and Deneb. Finally, ruddy Antares sparkles to the south. Less bright stars soon appear, allowing you to identify some constellations. This month, eight objects in the evening sky shine at first magnitude or brighter. In order of brightness, they are Arcturus, Vega, Altair, Antares, Spica, Regulus, Deneb and Mars. In July, the constellation Hercules is high overhead. The four stars forming the top of Hercules are known as the Keystone. If you point a telescope or binoculars to the west side of the Keystone, you'll discover a magnificent globular star cluster called M13. West of Hercules, you'll spot a semi-circle of stars called Corona Borealis. Keep an eye on it this summer, as astronomers have been predicting since last fall that the 'Blaze Star' will briefly appear. This star typically undergoes an outburst, known as a nova, approximately every 80 years, but it's almost a year overdue. Right next to Corona Borealis lies Bootes, a kite-shaped group of stars easily identifiable due to the brilliant star Arcturus. To find Arcturus, use a handy sky key that guides you to follow the handle of the Big Dipper and then 'arc to Arcturus, then speed on to Spica.' This direct path leads you to the two bright stars, with Spica being the brightest star in Virgo. East of Hercules, you'll find Lyra, home to the bright star Vega, and Cygnus, which contains the well-known asterism known as the Northern Cross. The brightest star in Cygnus is Deneb. You'll easily spot a large pattern of stars called the Summer Triangle. This triangle comprises the three brightest stars in three different constellations. Deneb, the most northern star, is in Cygnus, Altair, the most southern star, is in Aquila, and Vega, the star that forms the third star of the triangle, is in Lyra. Looking south, you'll spot the 'Teapot' of Sagittarius and a fishhook-shaped group of stars forming the constellation of Scorpius. Both are situated along a prominent band of the Milky Way. If you follow the Milky Way upward in the sky, you'll pass by Aquila, Cygnus, and end up at Cassiopeia in the northeast. Cassiopeia is easily recognizable, consisting of five moderately bright stars that appear as an M or W shape in the sky. Returning to the Teapot above the southern horizon, you'll quickly understand its name. It resembles an old-fashioned teapot, and the 'steam' emanating from the spout is the Milky Way. Its spout also points in the direction of the center of our Milky Way galaxy. What is the Milky Way, the radiant glow across a dark sky? When you gaze upon the Milky Way, you're witnessing a spiral arms of our galaxy. It contains an immense number of stars, along with gas and dust, which blend together, creating a subtle, milky glow across the sky. The summer Milky Way is particularly prominent in a dark sky on summer evenings. If you use binoculars and follow along the Milky Way, you'll discover a treasure trove of stars, star clusters and nebulae. Most of the planets visible this month are found in the morning sky. Mars descends more each evening, traversing the stars of Leo. The moon will visit Mars on July 28. Mercury will be low in the western twilight until mid-month. Keep an eye out for it about 30 to 40 minutes after sunset. Early morning risers will have delightful spectacle this month. The brilliant planet Venus will be easily visible before dawn, with the bright planet Jupiter below it, and it'll ascend higher each morning. Venus and Jupiter will pair up on Aug. 12. Saturn blends in with the first magnitude stars and is found in the southern sky at dawn. On July 16, the moon will pass by Saturn. Near Venus will be the glittering star cluster Pleiades, also known as the Seven Sisters. It's a beautiful group of stars resembling a tiny dipper. Additionally, a thin crescent moon will be near Venus on July 21 and visit Jupiter on July 23. On the morning of July 20, the moon passes in front of — and blots out — some of the stars of the Pleiades. They are best observed through binoculars. And on July 3, Earth reaches its farthest point from the sun, known as aphelion. This distance is approximately 3 million miles greater than when we were closest to the sun, during perihelion, on Jan. 3, 2025. The tilt of the Earth plays a crucial role in determining our warmest months. In July, the Northern Hemisphere tilts toward the sun, allowing us to receive direct sunlight. On the other hand, in January, we are tilted away from the sun, resulting in reduced direct sunlight. The Southern Hemisphere experiences the opposite pattern, with summer being the time when they are closest to the sun and winter when they are farthest.

DOWNLOAD THE APP

Get Started Now: Download the App

Ready to dive into a world of global content with local flavor? Download Daily8 app today from your preferred app store and start exploring.
app-storeplay-store