How Microgravity on the International Space Station Influences Bacteriophage and Host Coevolution

Microbiologists from the University of Wisconsin-Madison and Rhodium Scientific have unveiled a groundbreaking discovery aboard the International Space Station (ISS). Their latest experiment reveals that the unique near-weightless environment of space significantly alters the interactions between bacteriophages (viruses that target bacteria) and their hosts.



The International Space Station, with Earth in the background. Image credit: NASA.

In this detailed study focused on bacteriophage-host dynamics in microgravity, University of Wisconsin-Madison researcher Phil Huss and his team analyzed the interaction of T7 phages with Escherichia coli bacteria cultivated in an orbiting laboratory.

The experiments highlighted that while microgravity slows the infection rate of viruses, it does not permanently inhibit their ability to infect.

Under normal Earth conditions, T7 phages typically infect and lyse Escherichia coli within 20 to 30 minutes.

However, in the microgravity setting, no measurable growth of the bacteriophages was observed during the initial hours of culture.

After 23 days, the bacteriophage started to grow normally, effectively reducing the bacterial count. This suggests that bacteriophage activity eventually overcame the initial delays caused by the microgravity environment.

Factors unique to microgravity, such as disrupted fluid convection and changes in bacterial physiology, appear to influence how bacteriophage particles encounter and infect bacterial hosts.

In the absence of gravity, the natural mixing of fluids that typically facilitates virus-bacteria contact may be hindered, thereby slowing down the initial infection stages.

To delve deeper into the evolutionary and molecular consequences of these altered interactions, researchers sequenced the genomes of both bacteriophages and bacteria post long-term culture.

The analysis revealed numerous emerging mutations in the genomes of both organisms, indicating adaptation to their unique conditions.

Intriguingly, different mutation patterns were identified in microgravity compared to those evolving under Earth’s gravity, highlighting that the space environment exerts distinct selective pressures on both bacteriophages and their bacterial hosts.

Further scrutiny focused on the bacteriophage’s receptor-binding proteins, essential for recognizing and infecting bacterial cells effectively.

Through a deep mutational scan, significant differences in the mutational profiles of these proteins were observed between microgravity and ground-based experiments, reflecting fundamental changes in adaptive capabilities.

In a remarkable find, the researchers utilized a library of receptor-binding protein variants selected in microgravity to create bacteriophage variants that are more efficient at infecting specific drug-resistant strains of Escherichia coli on Earth. This underscores the potential of space-based research to inform biotechnology.

“Our study provides initial insights into how microgravity influences phage-host interactions,” the researchers concluded.

“Investigating phage activity in non-terrestrial settings unveils new genetic determinants of fitness, paving the way for innovative phage engineering on Earth.”

“The success of this research will establish a foundation for future phage investigations aboard the ISS.”

For more details, refer to the study published in the online journal PLoS Biology.

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P. Hass et al. 2026. Microgravity reshapes bacteriophage-host coevolution on the International Space Station. PLoS Biol 24 (1): e3003568; doi: 10.1371/journal.pbio.3003568

Source: www.sci.news

Tony Blair and Nick Clegg Host Dinner to Connect Tech Leaders with UK Ministers

Earlier this year, Tony Blair and Nick Clegg organized a private dinner where a group of technology entrepreneurs had the opportunity to meet influential ministers, as revealed by official documents.

As a long-time supporter of the tech industry, the former prime minister hosted this dinner at a high-end hotel in London, representing the Tony Blair Institute (TBI) political consultancy.

Together with former deputy prime minister Mr. Clegg, who was a senior executive at Meta at the time, they invited leaders from six tech firms, including Poppy Gustafsson, the government’s investment minister tasked with encouraging businesses to invest in the UK.

Mr. Blair is a passionate advocate for the transformative potential of technology in public services and has actively sought partnerships with industry leaders. His consultancy has produced several policy papers that advocate for placing artificial intelligence at the core of government initiatives.

However, some critics express concerns that Prime Minister Blair, known for his close ties to Keir Starmer’s administration, has been able to influence the agenda without adequate public oversight. There are also questions surrounding the reliance of Blair’s consultancy on significant contributions from Silicon Valley’s billionaire Larry Ellison, an acquaintance of Donald Trump and Elon Musk.

Mr. Ellison, who briefly claimed the title of the world’s richest person this year, has donated or committed over $300 million to Mr. Blair’s consultancy.

Documents obtained by the Guardian through freedom of information laws reveal that 12 attendees discussed the government’s evolving stand on artificial intelligence at a gathering deemed a “salon dinner.”

Do you have any information about this story? Email henry.dyer@theguardian.com or message (using your non-work phone) Signal or WhatsApp to +44 7721 857348. For the most secure communications, visit theguardian.com/tips.

The dinner took place at the luxurious Corinthia Hotel in late January and featured Ron Jaffe, managing director of Insight Partners, a US venture capital firm investing in tech companies.

Also present was Alex Kendall, CEO of Wave, focused on self-driving cars, along with Nigel Thune, head of Graphcore, a computer chip manufacturer, and Mark Warner, CEO of Faculty AI, who last year collaborated with TBI to produce a document on leveraging AI to enhance public services.

A representative for Mr. Clegg noted, “During his tenure at Meta, Nick Clegg frequently interacted with government ministers and other tech CEOs, which is standard for his role in policy and global affairs.”

According to a TBI spokesperson, “The event featured discussions with ministers about various issues among tech leaders. No companies were charged to attend.”

Companies that participated asserted they do not contribute to or employ TBI.

This dinner illustrates how Prime Minister Blair’s consultancy is advancing pro-technology policies. The rapidly growing TBI is active in 45 countries and employs over 900 staff members. Its most recent financial statement reported revenues of $145 million in 2022 from advisory services and donations, although many donors and clients remain undisclosed.

The consultancy faces criticism for potentially allowing donor interests to influence its policy positions, a claim it disputes. It has also been criticized for continuing financial ties with Saudi Arabia following the murder of journalist Jamal Khashoggi in 2018. Blair is anticipated to play a significant role in the reconstruction of Gaza following the war.

Weeks prior to the dinner, the government confidentially provided an outline of an AI action plan to TBI shortly before it was set to be publicly released. On January 9, Ferial Clark, then Minister of Science, Innovation and Technology (DSIT), made this request at the prompting of TBI’s Director of Science Policy, Jacob Mokander.

The following day, an aide to Mr. Clark reached out to Mr. Mokander stating, “It was a pleasure speaking with you. As a follow-up, here’s the top-secret action plan summary. Thank you for expanding the plan through your networks and supportive quotes on Monday.” Mr. Mokander replied, “Thanks for sharing the action plan (confidentiality).” Blair endorsed the action plan on January 13, which aims to bolster the UK’s role in AI development and deployment.

When asked why this document was shared with TBI so early, a DSIT spokesperson stated, “We cannot apologize for our regular engagement with stakeholders. It’s standard to share embargoed information with them ahead of publication.”

A spokesperson for TBI remarked, “It’s typical for governments to consult experts and engage various stakeholders when crafting policy. As indicated in the footnotes, the AI Opportunity Action Plan accurately references our published work.”

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Observations Indicate OJ 287 Galaxy May Host an Ultra-Massive Black Hole Binary at Its Core

Utilizes data from 10m space-based wireless telescopes, including Radioastron. Astronomers have formed a network of 27 ground observation stations focused on OJ 287, a galaxy approximately 5 billion light-years distant from the Cancer constellations.



This image of OJ 287 reveals the sharply curved ribbon-like structure of the plasma jet emitted from its center. Image credits: Efthalia Traianou / Heidelberg University / IWR.

“Among the different types of active galactic nuclei, BL Lacertae (BL LAC) objects are notable for their rapid, large-amplitude variability and significant polarization across multiple wavelengths due to relativistic jets aligned closely with our line of sight.”

“A standout example of this subclass is OJ 287, characterized by a redshift of z = 0.306.”

Optical observations of OJ 287 have yielded an extensive light curve extending back to the 1880s, covering nearly 150 years.

This comprehensive dataset has uncovered periodic brightness variations, featuring marked 60-year cycles and notable high-brightness flares with recurrent double peaks occurring approximately every 12 years.

These periodic changes can be attributed to the presence of a binary supermassive black hole system, where secondary supermassive black holes follow eccentric precession paths around the more massive primary.

“The level of detail in the new images allows us to see the structure of the OJ 287 Galaxy like never before,” stated Dr. Traianou.

“The images penetrate deep into the galaxy’s center, revealing the jet’s sharply curved ribbon-like structure.”

“This also provides new insights into the composition and dynamics of plasma jets.”

“Certain regions exceed temperatures of 10 trillion Kelvin, indicating the release of extreme energy and movement near the black hole.”

Astronomers have also monitored the development, dispersion, and interactions of new shock waves along the jet, linking them to energies in the range of trillions of electron volts from rare gamma-ray observations made in 2017.

Using Radioastron and 27 terrestrial observatories, they captured images of OJ 287 across the radio spectrum.

The imaging relies on measurement techniques that utilize overlapping waves related to the properties of light waves.

“Interference measurement images bolster the hypothesis that a binary supermassive black hole resides within OJ 287,” the researchers commented.

“This also offers critical insights on how these black holes influence the shape and direction of the emitted plasma jet.”

“These unique characteristics position the galaxy as an ideal candidate for further studies on black hole mergers and associated gravitational waves.”

Survey results will be published in the journal Astronomy and Astrophysics.

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E. Traianou et al. 2025. Reveal ribbon-like jets on OJ 287 via Radioastron. A&A 700, A16; doi: 10.1051/0004-6361/202554929

Source: www.sci.news

Recently Discovered Exoplanet Triggers Flares on Its Host Star

The Hot-Jupiter exoplanet HIP 67522b revolves around its star, HIP 67522, frequently triggering flares from the star’s surface, which seem to heat and penetrate the planet’s atmosphere.

Artistic impression of the HIP 67522 young planetary system. Image credit: J. Fohlmeister, AIP.

HIP 67522 is a G0 star located approximately 417 light-years away in the constellation Centaurus.

This star is part of the Scorpius-Centaurus Stellar Association and is also known as HD 120411, 2Mass J13500627-4050090, and TYC 7794-2268-1.

At about 17 million years old, HIP 67522 is home to two young exoplanets.

The inner planet, HIP 67522b, completes an orbit around the star every seven days and has a diameter roughly ten times that of Earth, making it similar in size to Jupiter.

Using five years of data from NASA’s TESS and ESA’s CHEOPS telescopes, astronomer Ekaterina Ilin and her team studied the HIP 67522 system in detail.

They uncovered that the planet and its host star share a powerful yet destructive connection.

Although not completely understood, the planet becomes ensnared in the star’s magnetic field, resulting in eruptions on the star’s surface that transfer energy back to the planet.

When combined with other high-energy radiation from the star, these flares appear to significantly enhance the rapid inflation of the planet’s atmosphere.

This indicates that the planet might not remain within the size range of Jupiter for much longer.

Continuous exposure to intense radiation can lead to atmospheric loss over time.

In about 100 million years, this could change the planet into a hot Neptune state or even result in more severe atmospheric reductions, with sub-Neptunes commonly observed in our galaxies, but lacking smaller planetary types than Neptune in our solar system.

“We found the first definitive evidence of the interaction between the flare star and the planet, demonstrating that the planet induces energy eruptions in the host star,” remarked Dr. Ilin, lead author of a paper published in the journal Nature.

“What is particularly thrilling is that this interaction persists for at least three years, allowing for in-depth study.”

“Such planetary interactions have long been anticipated, but these observations were made possible with this extensive spatial telescope dataset,” stated Dr. Katja Poppenhäger, an astronomer at Leibniz-Institut für Astrophysik Potsdam and Potsdam University.

“The planets are essentially subjected to intense bursts of radiation and particles from these induced flares,” explained Astron astronomer Dr. Harish Vedantum.

“The conditions in this self-inflicted environment are likely to expand the planet’s atmosphere and can significantly accelerate the rate at which the planet is losing its atmosphere.”

In a separate paper published in Astronomy and Astrophysics, astronomers confirmed that HIP 67522 is a magnetically active star emitting strong radio radiation along with a magnetic field.

They monitored the star at low radio frequencies for approximately 135 hours using the Australian Telescope Compact Array (ATCA), revealing it as a bright and explosive source of radio waves.

However, there were no indications of radio wave flares resulting from star-planet interactions.

“The lack of detection aligns with the notion that planet-driven flares may be too faint for ATCA to observe, corroborating the conclusions on magnetic star-planet interactions presented in our Nature paper,” they noted.

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Ekaterina Ilin et al. Nearby planets induce flares in their host star. Nature, published online July 2, 2025. doi:10.1038/s41586-025-09236-z

Ekaterina Ilin et al. 2025. Search for planetary-induced radio signals from the young exoplanet-host star HIP 67522. A&A, in press; doi: 10.1051/0004-6361/202554684

Source: www.sci.news

Hubble captures Type IA Super Shinsei and its host galaxy in stunning detail

Two years ago, a type IA supernova event called SN 2022ABVVT was discovered in Spiral Galaxy LEDA 132905.



This Hubble image LEDA 132905, a spiral galaxy over 400 million light years in sculptor constellation. Image credit: NASA / ESA / Hubble / RJ Foley, UC Santa cruz.

LEDA 132905 in the sculptor’s constellation is over 400 million light years away.

“The galaxy’s spiral structure, resembling a bright blue star patch, appears faint,” said members of the Hubble team.

“The bright white dot between the bright center of the galaxy and the faint left end is the SN 2022ABVVT supernova.”

The supernova SN 2022ABVT was discovered in 2022 by astronomers of the asteroid landlady impacted alert system (ATLAS).

About two months later, the NASA/ESA Hubble Space Telescope observed the star explosion.

“Atlas, designed to track faint-moving signals from asteroids near Earth, also detects objects that suddenly become brighter or fade, like supernovae in the centers of galaxies, various stars, and hungry black holes,” astronomers explained.

This Hubble image of LEDA 132905 was captured using the Hubble wide field camera 3 (WFC3) in the infrared part of the spectrum.

Astronomers are interested in studying type IA supernovae, which occur when the exposed core of ancient stars ignites in a sudden and destructive nuclear fusion burst.

These supernovae are valuable for measuring accurate distances to other galaxies.

“The universe is vast, and supernova explosions are faint,” researchers stated.

“How can we be in the right place at the right time to observe a supernova?”

“Today, most supernovae are discovered by robot telescopes constantly scanning the night sky.”

“However, some are still found the traditional way, with diligent observers taking repeated images of the sky and searching for any changes.”

Source: www.sci.news

Consumer Affairs: Airbnb host raises prices by 39% following reservation

My daughter used my credit card to book a 5-month stay using Airbnb after taking an internship in Toronto. After the host accepted the booking, she received an email saying the entire stay had increased by £4,000 for her (plus 39% for her).

In a panic, she canceled because she couldn’t afford to pay the extra fee. Airbnb took it. There is a £1,962 handling fee plus £682 cleaning fee and tax. Her daughter canceled immediately, so it is unlikely that your reservation will be lost.

Airbnb endlessly cites its terms of service. I asked the host to give me the money back, but he said he wouldn’t give it back. Feels as if it helped this guy perpetuate something. Seems like a scam.

JS,

on mail

I’m surprised Airbnb didn’t resolve this issue in your favor before I got involved. You were asked to pay an additional 39% after booking – seriously? Fortunately, the company has now refunded you the full amount.

I was told that I should have declined the host’s request for additional fees. In that case, it was up to the host to decide whether to proceed at the original rate or cancel.

You wonder who at the company came up with the terms and conditions that allow for such a request, but all’s well that ends well. I hope your daughter enjoys Toronto.

We welcome letters, but cannot respond individually. Email us at Consumer.champions@theguardian.com or write to Consumer Champions, Money, the Guardian, 90 York Way, London N1 9GU. Please enter a phone number where you can be reached during the day. Submission and publication of all letters is subject to our Terms of Use.

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