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Extraordinarily

Exchange Review August
Crypto Trends

Solana Is the New Wall Street, Says Bitwise CIO, Calling It ‘Extraordinarily Attractive’

by admin October 4, 2025



Solana’s role in the race to capture tokenized markets won new attention this week when Bitwise CIO Matthew Hougan called it “the new Wall Street.”

Speaking with Solana Labs’ Akshay Rajan on Oct. 2, Hougan said global financial leaders increasingly recognize the disruptive potential of stablecoins and tokenization.

He noted that the heads of the SEC and Bank of England, along with BlackRock’s CEO, have all signaled that digital assets could reshape payments and securities markets. Hougan added that this narrative resonates strongly with investors who understand the scale of change such technologies could bring.

Hougan said that once audiences begin to consider how to gain exposure to blockchain, comparisons between platforms inevitably follow. In that evaluation, he argued, Solana’s combination of speed, throughput and near-instant finality makes it “extraordinarily attractive.”

He cited improvements from 400 microseconds to 150 microseconds in settlement speed, describing the feature as intuitive for those accustomed to trading environments where execution and latency are critical.

Framing Solana as “the new Wall Street,” Hougan said the blockchain’s technical edge is resonating with market participants. He said the narrative is “really resonant” and added that “you’ll see substantial flows.”

Technical Analysis of SOL’s Price Action

According to CoinDesk Research’s technical analysis data model, during the 23-hour session from Oct. 3 at 15:00 UTC to Oct. 4 at 14:00 UTC, SOL traded within a narrow $8.40 range between $228.19 and $237.04, reflecting a period of consolidation.

The high was set at $237.04 around 16:00 on Oct. 3 before steady selling pressure pushed the price lower toward the $228–$229 area, which acted as support.

Trading activity was strongest early in the session, with volumes peaking at 3.29 million units around 17:00, but gradually declined to just 42,637 by the closing hour of the analysis period. This sharp reduction in volume suggested weakening participation and a potential pause before a larger directional move.

In the final 60 minutes, from 13:11 to 14:10 UTC on Oct. 4, SOL broke below the established $228–$229 support zone. Prices fell from $229.84 to $228.94, a 0.39% drop that confirmed the bearish shift.

Within this window, the market showed two phases: an early rebound attempt that briefly lifted the price to $229.78 at 13:38, followed by renewed selling that drove the token down to $228.72.

Importantly, this breakdown coincided with a surge in volume. The single busiest minute occurred at 14:01, when 18,011 units traded — the highest one-minute reading of the session.

This pattern of falling price alongside rising volume suggested larger sellers were active, potentially increasing the likelihood that bearish momentum continues.

Disclaimer: Parts of this article were generated with the assistance from AI tools and reviewed by our editorial team to ensure accuracy and adherence to our standards. For more information, see CoinDesk’s full AI Policy.



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October 4, 2025 0 comments
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Scientists Have Identified the Origin of an Extraordinarily Powerful Outer Space Radio Wave
Product Reviews

Scientists Have Identified the Origin of an Extraordinarily Powerful Outer Space Radio Wave

by admin August 23, 2025


The Earth is constantly receiving space signals that contain vital information about extremely energetic phenomena. Among the most peculiar are brief pulses of extremely high-energy radio waves, known as fast radio bursts (FRB). Astronomers compare them to a powerful lighthouse that shines for milliseconds in the middle of a rough, distant sea. Detecting one of these signals is an achievement in itself, but identifying its origin and understanding the nature of its source remains one of the great challenges of science.

That is why recent research led by Northwestern University in the United States has captured the attention of the astronomical community. The team not only detected one of the brightest FRBs ever recorded, but also traced its origin with unprecedented precision.

The pulse, identified as RBFLOAT, arrived in March 2025, lasted just a few milliseconds, and released as much energy as the sun produces in four days. Thanks to a new method of analysis, the researchers located its origin in an arm of a spiral galaxy located 130 million light-years away, in the direction of the constellation Ursa Major. The research was published in the journal The Astrophysical Journal Letters.

The CHIME radio telescope in Canada, one of the world’s leading FRB observatories, and a subnetwork of smaller stations called Outriggers detected the anomalous outburst. CHIME characterized the signal, while the Outriggers triangulated it to a narrow region of space. Optical and X-ray telescopes then provided complementary data. The team achieved a precision of 13 parsecs, equivalent to 42 light-years, within the galaxy NGC 4141.

Astronomers had previously pinpointed other FRBs, but in those cases the signals were repeated, which made the analysis easier. “RBFLOAT was the first non-repeating source localized to such precision,” said Sunil Simha, coauthor of the study, in a university statement. “These are much harder to locate. Thus, even detecting RBFLOAT is proof of concept that CHIME is indeed capable of detecting such events and building a statistically interesting sample of FRBs.”

What Caused the RBFLOAT?

Scientists are still not sure what causes RBFs, but they have some ideas. Because of the enormous energy they release and the brevity of the phenomenon, it is likely that they originate from extreme cosmic events, such as neutron star mergers, magnetars, or pulsars.

In the case of RBFLOAT, the data indicate that it is located in a star-forming region with really massive stars. The triangulation places the signal in a galactic arm where new stars are also being born. This suggests that it could be a magnetar, a subclass of neutron star with a magnetic field billions of times stronger than that of the Earth.

The experience with RBFLOAT will allow the team to apply the same triangulation technique to future signals. The authors estimate that they could achieve about 200 accurate RBF detections per year with just the signals CHIME captures.

“For years, we’ve known FRBs occur all over the sky, but pinning them down has been painstakingly slow. Now, we can routinely tie them to specific galaxies, even down to neighborhoods within those galaxies,” said Yuxin Dong, another member of the team.

This story originally appeared on WIRED en Español and has been translated from Spanish.



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August 23, 2025 0 comments
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