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Japan’s ispace suffers second lunar landing failure

The Japanese firm ispace has suffered another setback after its second attempt to land on the Moon ended in failure yesterday. The Hakuto-R Mission 2, also known as Resilience, failed to touch down near the centre of Mare Frigoris (sea of cold) in the far north of the Moon after a sensor malfunctioned during descent.

Launched on 15 January from the Kennedy Space Center, Florida, aboard a SpaceX Falcon 9 rocket, the craft spent four months travelling to the Moon before it entered lunar orbit on 7 May. It then spent the past month completing several lunar orbital manoeuvres.

During the descent phase, the 2.3 m-high lander began a landing sequence that involved firing its main propulsion system to gradually decelerate and adjust its attitude. ispace says that the lander was confirmed to be nearly vertical but then the company lost communication with the craft.

The firm concludes that the laser rangefinder experienced delays attempting to measure the distance to the lunar surface during descent, meaning that it was unable to decelerate sufficiently to carry out a soft landing.

“Given that there is currently no prospect of a successful lunar landing, our top priority is to swiftly analyse the telemetry data we have obtained thus far and work diligently to identify the cause,” noted ispace founder and chief executive officer Takeshi Hakamada in a statement. “We strive to restore trust by providing a report of the findings.”

The mission was planned to have operated for about two weeks. Resilience featured several commercial payloads, worth $16m, including a food-production experiment and a deep-space radiation probe. It also carried a rover, dubbed Tenacious, which was about the size of a microwave oven and would have collected and analysed lunar regolith.

The rover would have also delivered a Swedish artwork called The Moonhouse – a small red cottage with white corners – and placed it at a “symbolically meaningful” site on the Moon.

Lunar losses

The company’s first attempt to land on the Moon also ended in failure in 2023 when the Hakuto-R Mission 1 crash landed despite being in a vertical position as it carried out the final approach to the lunar surface.

The issue was put down to a software problem that incorrectly assessed the craft’s altitude during descent.

If the latest attempt was a success, ispace would have joined the US firms Intuitive Machines and Firefly Aerospace, which both successfully landed on the Moon last year and in March, respectively.

The second lunar loss casts doubt on ispace’s plans for further lunar landings and its grand aim of establishing a lunar colony of 1000 inhabitants by the 2040s.

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Leinweber Foundation ploughs $90m into US theoretical physics

The Leinweber Foundation has awarded five US institutions $90m to create their own theoretical research institutes. The investment, which the foundation says is the largest ever for theoretical physics research, will be used to fund graduate students and postdocs at each institute as well as several Leinweber Physics Fellows.

The Leinweber Foundation was founded in 2015 by the software entrepreneur Larry Leinweber. In 1982 Leinweber founded the software company New World Systems Corporation, which provided software to the emergency services. In 2015 he sold the company to Tyler Technologies for $670m.

Based in Michigan, Leinweber Foundation supports research, education and community endeavours where it has provided Leinweber Software Scholarships to undergraduates at Michigan’s universities.

A Leinweber Institute for Theoretical Physics (LITP) will now be created at the universities of California, Berkeley, Chicago and Michigan as well as at the Massachusetts Institute of Technology (MIT) and at Princeton’s Institute for Advanced Study (IAS), where the institute will instead be named the Leinweber Forum for Theoretical and Quantum Physics.

The MIT LIPT, initially led by Washington Taylor before physicist Tracy Slatyer takes over later this year, will receive $20m from the foundation and will provide support for six postdocs, six graduate students as well as visitors, seminars and “other scholarly activities”.

“This landmark endowment from the Leinweber Foundation will enable us to support the best graduate students and postdoctoral researchers to develop their own independent research programmes and to connect with other researchers in the Leinweber Institute network,” says Taylor.

Spearing innovation

UC Berkeley, meanwhile, will receive $14.4m from the foundation in which the existing Berkeley Center for Theoretical Physics (BITP) will be renamed LITP at Berkeley and led by physicist Yasunori Nomura.

The money will be used for four postdoc positions to join the existing 15 at the BITP as well as to support graduate students and visitors. “This is transformative,” notes Nomura. “The gift will really have a huge impact on a wide range of research at Berkeley, including particle physics, quantum gravity, quantum information, condensed matter physics and cosmology.”

Chicago will receive $18.4m where the existing Kadanoff Center for Theoretical Physics will be merged into a new LITP at the University of Chicago and led by physicist Dam Thanh Son.

The remaining $37.2m will be split between the Leinweber Forum for Theoretical and Quantum Physics at the IAS and at Michigan, in which the existing Leinweber Center for Theoretical Physics will expand and become an institute.

“Theoretical physics may seem abstract to many, but it is the tip of the spear for innovation. It fuels our understanding of how the world works and opens the door to new technologies that can shape society for generations,” says Leinweber in a statement. “As someone who has had a lifelong fascination with theoretical physics, I hope this investment not only strengthens U.S. leadership in basic science, but also inspires curiosity, creativity, and groundbreaking discoveries for generations to come.”

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China launches Tianwen-2 asteroid sample-return mission

China has launched its first mission to retrieve samples from an asteroid. The Tianwen-2 mission launched at 01:31 a.m. local time on 28 May from the Xichang satellite launch centre, south-west China, aboard a Long March B rocket.

Tianwen-2’s target is a small near-Earth asteroid called 469219 Kamoʻoalewa, which is 15–39 million km away and is known as a “quasi-satellite” of Earth.

The mission is set to reach the body, which is 40–100 m wide, in July 2026. It will first study it up close using a suite of 11 instruments including cameras, spectrometers and radar, before aiming to collect about 100 g of material.

This will be achieved via three possible methods. One is via hovering close to the asteroid; another is using a robotic arm to collect samples from the body; while a third is dubbed “touch and go”, which involves gently landing on the asteroid and using drills at the end of each leg to retrieve material.

The collected samples will then be stored in a module that is released and returned to Earth in November 2027. If successful, it will make China the third nation to retrieve asteroid material behind the US and Japan.

Next steps

The second part of the 10-year mission involves using Earth for a gravitational swing-by to spend six year travelling to another target – 311P/PanSTARRS. The body lies in the main asteroid belt between Mars and Jupiter and at its closest distance is about 140 million km away from Earth.

The 480 m-wide object, which was discovered in 2013, has six dust tails and has characteristics of both asteroids and comets. Tianwen-2 will not land on 311P/PanSTARRS but instead use its instruments to study the “active asteroid” from a distance.

Tianwen-2’s predecessor, Tianwen-1, was China’s first mission to Mars, successfully landing on Utopia Planitia – a largely flat impact basin but scientifically interesting with potential water-ice underneath – following a six-month journey.

China’s third interplanetary mission, Tianwen-3, will aim to retrieve sample from Mars and could launch as soon as 2028. If successful, it would make China the first country to achieve the feat.

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Former IOP president Cyril Hilsum celebrates 100th birthday

Cyril Hilsum, a former president of the Institute of Physics (IOP), celebrated his 100th birthday last week at a special event held at the Royal Society of Chemistry.

Born on 17 May 1925, Hilsum completed a degree in physics at University College London in 1945. During his career he worked at the Services Electronics Research Laboratory and the Royal Radar Establishment and in 1983 was appointed chief scientist of GEC Hirst Research Centre, where he later became research director before retiring aged 70.

Hilsum helped develop commercial applications for the semiconductor gallium arsenide and is responsible for creating the UK’s first semiconductor laser as well as developments that led to modern liquid crystal display technologies.

Between 1988 and 1990 he was president of the IOP, which publishes Physics World, and in 1990 was appointed a Commander of the Order of the British Empire (CBE) for “services to the electrical and electronics industry”.

Hilsum was honoured by many prizes during his career including IOP awards such as the Max Born Prize in 1987, the Faraday Medal in 1988 as well as the Richard Glazebrook Medal and Prize in 1998. In 2007 he was awarded the Royal Society’s Royal Medal “for his many outstanding contributions and for continuing to use his prodigious talents on behalf of industry, government and academe to this day”.

Cyril Hilsum at an event to mark his 100th birthday
Looking back: Hilsum examines photographs that form an exhibition charting his life. (Courtesy: Lindey Hilsum)

Despite now being a centenarian, Hilsum still works part-time as chief science officer for Infi-tex Ltd, which produces force sensors for use in textiles.

“My birthday event was an amazing opportunity for me to greet old colleagues and friends,” Hilsum told Physics World. “Many had not seen each other since they had worked together in the distant past. It gave me a rare opportunity to acknowledge the immense contributions they had made to my career.”

Hilsum says that while the IOP gives much support to applied physics, there is still a great need for physicists “to give critical contributions to the lives of society as a whole”.

“As scientists, we may welcome progress in the subject, but all can get pleasure in seeing the results in their home, on their iPhone, or especially in their hospital!” he adds.

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Ray Dolby Centre opens at the University of Cambridge

A ceremony has been held today to officially open the Ray Dolby Centre at the University of Cambridge. Named after the Cambridge physicist and sound pioneer Ray Dolby, who died in 2013, the facility is the new home of the Cavendish Laboratory and will feature 173 labs as well as lecture halls, workshops, cleanrooms and offices.

Designed by the architecture and interior design practice Jestico + Whiles (who also designed the UK’s £61m National Graphene Institute) and constructed by Bouygues UK, the centre has been funded by £85m from Dolby’s estate as well as £75m from the UK’s Engineering and Physical Sciences Research Council (EPSRC).

Spanning 33 000 m² across five floors, the new centre will house 1100 staff members and students.

The basement will feature microscopy and laser labs containing vibration-sensitive equipment as well as 2500 m² of clean rooms.

The Dolby centre will also serve as a national hub for physics, hosting the Collaborative R&D Environment – a EPSRC National Facility – that will foster collaboration between industry and university researchers and enhance public access to new research.

Parts of the centre will be open to the public, including a café as well as outreach and exhibition spaces that are organised around six courtyards.

The centre also provides a new home for the Cavendish Museum, which includes the model of DNA created by James Watson and Francis Crick as well as the cathode ray tube that was used to discover the electron.

The ceremony today was attended by Dagmar Dolby, president of the Ray and Dagmar Dolby Family Fund, Deborah Prentice, vice-chancellor of the University of Cambridge and physicist Mete Atatüre, who is head of the Cavendish Laboratory.

“The greatest impacts on society – including the Cavendish’s biggest discoveries – have happened because of that combination of technological capability and human ingenuity,” notes  Atatüre. “Science is getting more complex and technically demanding with progress, but now we have the facilities we need for our scientists to ask those questions, in the pursuit of discovering creative paths to the answers – that’s what we hope to create with the Ray Dolby Centre.”

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General Fusion lays off staff due to ‘unexpected and urgent financing constraints’

The Canadian firm General Fusion is to lay off about 25% of its 140-strong workforce and reduce the operation of its fusion device dubbed Lawson Machine 26 (LM26). The announcement was made in an open letter published on 5 May by the company’s chief executive Greg Twinney. The moves follows what the firm says is an “unexpected and urgent financing constraint”.

Founded in 2002 by the Canadian plasma physicist Michel Laberge, General Fusion is based in Richmond, British Columbia. It is one of the first private fusion companies and has attracted more than $325m of funding from both private investors, including Amazon boss Jeff Bezos and the Canadian government.

The firm is pursuing commercial fusion energy via Magnetized Target Fusion (MTF) technology, based on the concept of an enclosed, liquid-metal vortex. Plasma is injected into the centre of the vortex before numerous pistons hammer on the outside of the enclosure, compressing the plasma and sparking a fusion reaction, with the resulting heat being absorbed by the liquid metal.

LM26 switched on in 2023 and is designed to achieve fusion conditions of over 100 million kelvin. Over the past couple of years, the machine has claimed a number of milestones, including generating a magnetised plasma in the machine’s target chamber in March. Last week, General Fusion also said that LM26 had successfully compressed a large-scale magnetized plasma with lithium.

The firm was hoping to achieve “scientific breakeven equivalent” in the coming years with the aim of potentially building a commercial-scale machine with the technology in the 2030s. But that timescale now looks unlikely as General Fusion announces plans to downscales its efforts due to funding issues. In his letter, Twinney said the firm has “proven a lot with a lean budget”.

Challenging environment 

“Today’s funding landscape is more challenging than ever as investors and governments navigate a rapidly shifting and uncertain political and market climate,” says Twinney. “We are ready to execute our plan but are caught in an economic and geopolitical environment that is forcing us to wait.” But he insists that General Fusion, which his seeking new investors, remains an “attractive opportunity”.

Andrew Holland, chief executive of the non-profit Fusion Industry Association, told Physics World that the “nature of private enterprise is that business cycles go up and go down” and claims that excitement about fusion is growing around the world. “I hope that business cycles and geopolitics don’t interrupt the good work of scientific advancement,” he says. “I’m hopeful investors see the value being created with every experiment.”

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The mechanics behind rose petal shapes revealed

Roses have been cultivated for thousands of years, admired for their beauty. Despite their use in fragrance, skincare and even in teas and jams, there are some things, however, that we still don’t know about these symbolic flowers.

And that includes the physical mechanism behind the shape of rose petals.

The curves and curls of leaves and flower petals arise due to the interplay between their natural growth and geometry.

Uneven growth in a flat sheet, in which the edges grow quicker than the interior, gives rise to strain and in plant leaves and petals, for example, this can result in a variety of shapes such as saddle and ripple shapes.

Yet when it comes to rose petals, the sharply pointed cusps – a point where two curves meet — that form at the edge of the petals set it apart from soft, wavy patterns seen in many other plants.

While young rose petals have smooth edges, as the rose matures the petals change to a polygonal shape with multiples cusps.

To investigate this intriguing difference, researchers from The Hebrew University of Jerusalem carried out theoretical modelling and conducted a series of experiments with synthetic disc “petals”.

They found that the pointed cusps that form at the edge of rose petals are due to a type of geometric frustration called a Mainardi-Codazzi-Peterson (MCP) incompatibility.

This type of mechanism results in stress concentrating in a specific area, which go on to form cusps to avoid tearing or forming unnatural folding.

When the researchers supressed the formation of cusps, they found that the discs reverted to being smooth and concave.

The researchers say that the findings could be used for applications in soft robotics and even the deployment of spacecraft components.

And it also goes some way to deepen our appreciation of nature’s ability to juggle growth and geometry.

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Spectacular images of the cosmos released to celebrate Hubble’s 35 years in orbit

A series of spectacular images of the cosmos has been released to celebrate the Hubble Space Telescope‘s 35 years in space. The images include pictures of Mars, planetary nebulae and a spiral galaxy.

Hubble was launched into low-Earth orbit in April 1990, stowed in the payload bay of the space shuttle Discovery. The telescope experienced a difficult start as its 2.4 m primary mirror suffered from spherical aberration – a fault that caused the curvature of the mirror to not bring light to focus at the same point. This was fixed three years later during a daring space walk in which astronauts successfully installed the COSTAR instrument.

During Hubble’s operational life, the telescope has made nearly 1.7 million observations, studying approximately 55,000 astronomical targets. Its discoveries have resulted in over 22,000 papers and over 1.3 million citations.

Operating for three decades, Hubble has allowed astronomers to see astronomical changes such as seasonal variability on the planets in our solar system, black-hole jets travelling at nearly the speed of light as well as stellar convulsions, asteroid collisions and expanding supernova bubbles.

Despite being 35 years in orbit around the Earth, Hubble is still one of the most sought after observatories with demand for observing time oversubscribed by 6:1.

“[Hubble’s] stunning imagery inspired people across the globe, and the data behind those images revealed surprises about everything from early galaxies to planets in our own solar system,” notes Shawn Domagal-Goldman, acting director of NASA’s astrophysics division. “The fact that it is still operating today is a testament to the value of our flagship observatories.”

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Fusion industry meets in London to discuss ‘one of the economic opportunities of the century’

“Fusion is now within reach” and represents “one of the economic opportunities of the century”. Not the words of an optimistic fusion scientist but from Kerry McCarthy, parliamentary under-secretary of state at the UK’s Department for Energy Security and Net Zero.

She was speaking on Tuesday at the inaugural Fusion Fest by Economist Impact. Held in London, the day-long event featured 400 attendees and more than 60 speakers from around the world.

McCarthy outlined several initiatives to keep the UK at the “forefront of fusion”. That includes investing £20m into Starmaker One, a £100m endeavour announced in early April to kickstart UK investment fusion fund.

The usual cliché is that fusion is always being 20 years away, perhaps not helped by large international projects such as the ITER experimental fusion reactor that is currently being built in Cadarache, France, which has struggling with delays and cost hikes.

Yet many delegates at the meeting were optimistic that significant developments are within reach with private firms racing to demonstrate “breakeven” – generating more power out than needed to fuel the reaction. Some expect “a few” private firms to announce breakeven by 2030.

And these aren’t small ventures. Commonwealth Fusion Systems, based in Massachusetts, US, for example, has 1300 people. Yet large international companies are, for the moment, only dipping their toe into the fusion pool.

While some $8bn has already been spent by private firms on fusion, many expect the funding floodgates to open once breakeven has been achieved in a private lab.

Most stated that a figure of about $50-60bn, however, would be needed to make fusion a real endeavour in terms of delivering power to the grid, something that could happen in the 2040s. But it was reiterated throughout the day that fusion must provide energy at a price that consumers would be willing to pay.

On target

It is not only private firms that are making progress. Many will point out that ITER has laid much of the groundwork in terms of fostering a fusion “ecosystem” – a particular buzzword of the day – that was demonstrated, in part, by the significant attendence at the event.

And developments are not just being confined to magnetic fusion. Kim Budil, director of the Lawrence Livermore National Laboratory, which is home to the National Ignition Facility, noted that the machine had recently achieved a fusion gain for the eighth time.

In a recent shot, she said that the device had produced 7 MJ with about 2 MJ having been delivered to the small capsule target. This represents a gain of about 3.4 – much more than its previous record of 2.4.

NIF, which is based on inertial confinement fusion rather than magnetic confinement, is currently undergoing refurbishment and upgrades. It is hoped that this will increase the energy input to about 2.6 MJ but gains of between 10-15 will be demonstrated if the technique can go anywhere.

Despite the number of fusion firms ballooning from a handful in the early 2010s to some 30 today, the general feeling at the meeting was that only a few will likely go on to build power plants, with the remainder using fusion for other sectors.

The issue is that no-one knew what technology would likely succeed, so all to play for.

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CERN releases plans for the ‘most extraordinary instrument ever built’

The CERN particle-physics lab near Geneva has released plans for the 15bn SwFr (£13bn) Future Circular Collider (FCC) – a huge 91 km circumference machine. The three-volume feasibility study, released on 31 March, calls for the giant accelerator to collide electrons with positrons to study the Higgs boson in unprecedented detail. If built, the FCC would replace the 27 km Large Hadron Collider (LHC), which will come to an end in the early 2040s.

Work on the FCC feasibility study began in 2020 and the report examines the physics objectives, geology, civil engineering, technical infrastructure and territorial and environmental impact. It also looks at the R&D needed for the accelerators and detectors as well as the socioeconomic benefits and cost.

The study, involving some 150 institutes in over 30 countries, took into account some 100 different scenarios for the collider before landing on a ring circumference of 90.7 km that would be built underground at a depth of about 200 m, on average.

The FCC would also contain eight surface sites to access the tunnel with seven in France and one in Switzerland, and four main detectors. “The design is such that there is minimal impact on the surface, but with the best possible physics output,” says FCC study leader Michael Benedikt.

The funding model for the FCC is still a work in progress, but it is estimated that at least two-thirds of the cost of building the FCC-ee will come from CERN’s 24 member states.

Four committees will now review the feasibility study, beginning with CERN’s scientific committee in July. It will then go to a cost-review panel before being reviewed by the CERN council’s scientific and finance committees. In November, the CERN council will then examine the proposal with a decision to go ahead taken in 2028.

If given the green light, construction on the FCC electron-positron machine, dubbed FCC-ee, would begin in 2030 and it would start operations in 2047, a few years after the High Luminosity LHC (HL-LHC) closes down, and run for about 15 years.  It’s main aim would be to study the Higgs boson with a much better precision that the LHC.

Artist impression of the FCC-hh
To the energy frontier: if built, the FCC-hh would begin operation in 2073 and run to the end of the century (courtesy: PIXELRISE)

The FCC feasibility study then calls for a hadron machine, dubbed FCC-hh, to replace the FCC-ee in the existing 91 km tunnel. It would be a “discovery machine”, smashing together protons at high energy with the aim of creating new particles. If built, the FCC-hh will begin operation in 2073 and run to the end of the century.

The original design energy for the FCC-hh was to reach 100 TeV but that has now been reduced to 85 TeV.  That is mostly due to the uncertainty in magnet technology. The HL-LHC will use 12 T superconducting quadrupole magnets made from niobium-tin (Nb3Sn) to squeeze the beams to boost the luminosity.

CERN engineers think it is possible to increase that to 14 T and if this was used for the FCC it would result in a collision centre-of-mass energy of about 85 TeV. “It’s a prudent approach at this stage,” noted Fabiola Gianotti, current CERN director-general, adding that the FCC would be “the most extraordinary instrument ever built.”

The original design called for high-temperature superconducting magnets, such as so-called ReBCO tapes, and CERN is looking into such technology. If it came to fruition in the necessary timescales and was implemented in the FCC-hh then it could push the energy to 120 TeV.

China plans

One potential spanner in the works is China’s plans for a very similar machine called the Circular Election-Positron Collider (CEPC). A decision on the CEPC could come this year with construction beginning in 2027.

Yet officials at CERN are not concerned. They point to the fact that many different colliders have been built by CERN, which has the expertise as well as infrastructure to build such a huge collider.  “Even if China goes ahead, I hope the decision is to compete,” says CERN council president Costas Fountas. “Just like Europe did with the LHC when the US started to build the [cancelled] Superconducting Super Collider.”

If the CERN council decides, however, not to go ahead with the FCC, then Gianotti says that other designs to replace the LHC are still on the table such as a linear machine or a demonstrator muon collider.

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Disabled people in science need paradigm shift in support, says report

Disabled people in science must be recognized and given better support to help reverse the numbers of such people dropping out of science. That is the conclusion of a new report released today by the National Association of Disabled Staff Networks (NADSN). It also calls for funders to stop supporting institutions that have toxic research cultures and for a change in equality law to recognize the impact of discrimination on disabled people including neurodivergent people.

About 22% of working-age adults in the UK are disabled. Yet it is estimated that only 6.4% of people in science have a disability, falling to just 4% for senior academic positions. What’s more, barely 1% of research grant applications to UK Research and Innovation – the umbrella organization for the UK’s main funding councils – are from researchers who disclose being disabled. Disabled researchers who do win grants receive less than half the amount compared to non-disabled researchers.

NADSN is an umbrella organization for disabled staff networks, with a focus on higher education. It includes the STEMM Action Group, which was founded in 2020 and consists of nine people at universities across the UK who work in science and have lived experience of disability, chronic illness or neurodivergence. The group develops recommendations to funding bodies, learned societies and higher-education institutions to address barriers faced by those who are marginalised due to disability.

In 2021 the group published a “problem statement” that identified issues facing disabled people in science. They range from digital problems, such as the need for accessible fonts in reports and presentations, to physical concerns such as needing access ramps for people in wheelchairs or automatic doors to open heavy fire doors. Other issues include the need for adjustable desks in offices and wheelchair accessible labs.

“Many of these physical issues tend to be afterthoughts in the planning process,” says Francesca Doddato, a physicist from Lancaster University, who co-wrote the latest report. “But at that point they are much harder, and more costly, to implement.”

We need to have this big paradigm shift in terms of how we see disability inclusion

Francesca Doddato

Workplace attitudes and cultures can also be a big problem for disabled people in science, some 62% of whom report having been bullied and harassed compared to 43% of all scientists. “Unfortunately, in research and academia there is generally a toxic culture in which you are expected to be hyper productive, move all over the world, and have a focus on quantity over quality in terms of research output,” says Doddato. “This, coupled with society-wide attitudes towards disabilities, means that many disabled people struggle to get promoted and drop out of science.”

The action group spent the past four years compiling their latest report – Towards a fully inclusive environment for disabled people in STEMM – to present solutions to these issues. They hope it will raise awareness of the inequity and discrimination experienced by disabled people in science and to highlight the benefits of having an inclusive environment.

The report identifies three main areas that will have to be reformed to make science fully inclusive for disabled scientists: enabling inclusive cultures and practices; enhancing accessible physical and digital environments; and accessible and proactive funding.

In the short term, it calls on people to recognize the challenges and barriers facing disabled researchers and to improve work-based training for managers. “One of the best things is just being willing to listen and ask what can I do to help?” notes Doddato. “Being an ally is vitally important.”

Doddato says that sharing meeting agendas and documents ahead of time, ensuring that documents are presented in accessible formats, or acknowledging that tasks such as getting around campus can take longer are some aspects that can be useful.“All of these little things can really go a long way in shifting those attitudes and being an ally, and those things they don’t need policies that people need to be willing to listen and be willing to change.”

Medium- and long-term goals in the report involve holding organisations responsible for their working practice polices and to stop promoting and funding toxic research cultures. “We hope that report encourages funding bodies to put pressure on institutions if they are demonstrating toxicity and being discriminatory,” adds Doddato. The report also calls for a change to equality law to recognize the impact of intersectional discrimination, although it admits that this will be a “large undertaking” and will be the subject of a further NADSN report.

Doddato adds that disabled people’s voices need to be hear “loud and clear” as part of any changes. “What we are trying to address with the report is to push universities, research institutions and societies to stop only talking about doing something and actually implement change,” says Doddato. “We need to have a big paradigm shift in terms of how we see disability inclusion. It’s time for change.”

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Ants’ hairy jaws help robots to get a grip

Researchers at the University of Edinburgh in the UK have built a prototype “hairy robotic gripper” that is inspired by the hairs found on ant jaws.

Ants are not only excellent nest builders but are also expert foragers, able to carry food and other items that can be many times their own weight.

Part of that ability lies in their powerful jaws, with snap-jaw ants able to close their mandibles at a top speed of 400 kmph.

Ant jaws also feature small hairs that are used to sense items but also to mechanically stabilise their grip on the objects.

Edinburgh researchers filmed ants and the sequence of movements they do when picking up seeds and other things. They then used this to build a robot gripper.

The device consists of two aluminium plates that each contain four rows of “hairs” made from thermoplastic polyurethane.

The hairs are 20 mm long and 1 mm in diameter, protruding in a v-shape. This allowing the hairs to surround circular objects, which can be particularly difficult to grasp and hold onto using parallel plates.

In tests picking up 30 different household items including a jam jar and shampoo bottle (see video), adding hairs to the gripper increased the prototype’s grasp success rate from 64% to 90%.

The researchers think that such a device could be used in environmental clean-up as well as in construction and agriculture.

Barbara Webb from the University of Edinburgh, who led the research, says the work is “just the first step”.

“Now we can see how [ants’] antennae, front legs and jaws combine to sense, manipulate, grasp and move objects – for instance, we’ve discovered how much ants rely on their front legs to get objects in position,” she adds. “This will inform further development of our technology.”

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James Webb Space Telescope spots spectacular auroras on Neptune

The first direct evidence for auroras on Neptune has been spotted by the James Webb Space Telescope (JWST) and the Hubble Space Telescope.

Auroras happen when energetic particles from the Sun become trapped in a planet’s magnetic field and eventually strike the upper atmosphere with the energy released creating a signature glow.

Auroral activity has previously been seen on Jupiter, Saturn and Uranus but not on Neptune despite hints in a flyby of the planet by NASA’s Voyager 2 in 1989.

“Imaging the auroral activity on Neptune was only possible with [the JWST’s] near-infrared sensitivity,” notes Henrik Melin from Northumbria University. “It was so stunning to not just see the auroras, but the detail and clarity of the signature really shocked me.”

The data was taken by JWST’s Near-Infrared Spectrograph as well as Hubble’s Wide Field Camera 3. The cyan on the image above represent auroral activity and is shown together with white clouds on a multi-hued blue orb that is Neptune.

While auroras on Earth occur at the poles, on Neptune they happen elsewhere. This is due to the nature of Neptune’s magnetic field, which is tilted by 47 degrees from the planet’s rotational axis.

As well as the visible imagery, the JWST also detected an emission line from trihydrogen cation (H3+), which can be created in auroras.

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