Category: 7. Science

Motty remains the only confirmed hybrid between an African elephant (Loxodonta africana) and an Asian elephant (Elephas maximus). Although the calf tragically died just days after birth, his unique descent earned him the rare distinction of being named the “world’s rarest elephant” by Guinness World Records.

Motty was born on July 11, 1978, at Chester Zoo in the UK and named after its founder, George Mottershead. As proven by tissue samples taken from the tiny male calf, this individual was the result of interbreeding between Jumbolino, a male bull African elephant, and Sheba, a female Asian elephant.

When the matriarch Sheba fell first pregnant, there wasn’t much doubt over the paternity of the individual; Jumbolino was said to be the only male elephant in the shared enclosure. However, there were still significant doubts about whether it would be possible for the two different species to produce viable offspring.

It would be impossible for these two species to mate in the wild given the vast geographical distance that separates their natural ranges on two different continents. Furthermore, these two animals are not just different species; they are different genera, meaning they are relatively distant from each other on the genetic tree too. 

African elephants and Asian elephants bear some distinct physical differences. The former species is larger, growing up to 3 to 4 meters (9.8 to 13.1 feet) from shoulder to toe, while the latter will only grow 2 to 3.5 meters (6.5 to 11.4 feet) tall. African elephants also have significantly larger ears, perfectly evolved for allowing heat to radiate away from the body in the savannah, and tend to have more wrinkly skin. 

Just as you’d expect with a hybrid of the two, Motty had features of both his mother and father. His head shape and larger ears were clearly those of an African elephant, but he also had five toenails on the front feet and four on the hind, which is a characteristic of Asian elephants.

Unfortunately, Motty had a tough start in life. Born six weeks premature, he was extremely underweight and required intensive veterinarian care from the get-go. Just 10 days after he was born, he succumbed to necrotizing enterocolitis, a serious gastrointestinal problem in newborn animals. He died on July 21, 1978. A necropsy later showed that he was suffering from a severe E. coli infection in both his colon and the umbilical cord. 

Upon his death, the body of this unique individual was reportedly preserved by a private collection and it is said to be kept at the Natural History Museum in London.

Motty is a true individual, the likes of which have never been seen since. However, there are plenty of other examples of interspecies romping and hybridization elsewhere in the animal kingdom. There is the sought-after beefalo and the uber-cute dog-fox combo, not to mention the surprising number of wholphins that swim the world’s oceans.

An earlier version of this story was published in 2023.

Solar thermal power has a great advantage over solar panels on roofs or in most solar farms: it can continue to produce electricity after the Sun has gone down. The mirrors known as heliostats at solar thermal facilities focus sunlight to heat fluids to very high temperatures to drive turbines. The more common version involves fields of heliostats reflecting light on a central tower through which the fluids move. The materials stay hot enough to continue spinning the turbines after dark, depending on the fluid and the turbine sometimes all night.

That advantage has not been sufficient to allow solar thermal to compete commercially with photovoltaics’ lower price and flexibility of location, although there are reasons to think that may change.  However, while the turbines keep working at night, the mirrors don’t, which is something Dr John Sandusky of Sandia National Labs wants to change.

“The heliostat fields don’t have a night job. They just sit there unused. The nation has an opportunity to give them a night job at a relatively low cost for finding near-Earth objects,” Sandusky told the Sandia newsletter LabNews. “If we knew ahead of time that an asteroid was coming and where it might hit, we’d have a better chance to prepare and reduce the potential damage.”

Sandusky’s first test of the idea was conducted with just one of the 212 heliostats at the National Solar Thermal Test Facility. Using software already built to move the heliostat in daylight, he had it sweep backwards and forwards around once a minute and collected the light it focused on the tower.

Current asteroid-hunting techniques produce images of areas of the sky tracked to follow the apparent motion of the stars. Asteroids, or anything else, moving relative to the stars, show up as streaks that computers can recognize.

We’ve become a lot better at detecting objects moving through the inner Solar System in recent years, which is why all three interstellar visitors we have detected have been since 2017. We already know the Vera C Rubin Observatory can take it up a notch further. Nevertheless, there is still room for further improvement, since we lack the capacity to watch the whole sky at once. Moreover, if we had a different method for finding objects like this, the giant telescopes currently used for the purpose could be redeployed to research roles.

Sandusky anticipates that the relative motion of an asteroid compared to the stars will lead to a detection when the light of one is reflected off the heliostat. 

“Solar towers collect a million watts of sunlight,” Sandusky said. “At night, we want to collect a femtowatt, which is a millionth of a billionth of a watt of power of sunlight that’s scattered off of asteroids.”

Sandusky’s test run using the single heliostat did not find an asteroid, but he didn’t really expect it would. Instead, he wanted to prove it could be moved at the appropriate rate and reflect starlight to the instruments, and he has claimed success. He presented the results to a conference last year and published a paper, but is now seeking wider input on whether the idea has potential and how his proposed approach could improve. “We want to hear from our peers in optics and the asteroid hunting community,” Sandusky said. “Getting peer feedback provides an opportunity to understand what the concerns are about how this technology will work.”

Ironically, the basis for this idea comes from a question Sandusky was asked twenty years ago about the potential to use heliostats for imaging. “No. They’re not high enough optical quality to form an image,” he replied at the time. Nevertheless, the question lingered and it occurred to him there were parallels between the reflections of an object moving relative to the stars and frequency shifts used in radio communication.

“We have very precise methods for measuring frequency,” Sandusky said. “Even frequency changes as small as one-one-millionth of one cycle per second are measurable thanks to frequency standards that can be commercially procured and locked to references like GPS signaling. I knew it was possible to measure the very small rate differences of an asteroid passing relative to the stars.”

“If I can map all of the stars to one frequency, anything moving relative to the stars will appear at a neighboring frequency but still be separable,” he concluded. Having demonstrated the precise speed control required is possible, and that heliostats can reflect the stars, he’s ready to move on to try to find asteroids.

A stepping stone would be to have the heliostat reflect a part of the sky where a bright suitable object is known to pass, to see if it can be found this way. From there, one could chase smaller known objects, and eventually seek those not yet known. 

Sandusky also has ideas for related tasks that could expand heliostats’ nighttime uses, such as for detecting lost spacecraft, particularly orbiting between Earth and Moon, such as the one that hit the Moon in 2022. “Orbits near the moon can be difficult to track from the ground,” he said.

It’s unlikely there will be enough of a market to use heliostats in this way to substantially shift the economics of solar thermal projects when competing against other sources of energy, but every little bit helps.

The idea was published in Unconventional Imaging, Sensing and Adaptive Optics, as part of the proceedings of the Optical Engineering and Applications conference.

Further in-depth analysis, meticulously combining data from TESS with high-precision observations from powerful ground-based instruments, led to the exciting confirmation of a fourth planet (L 98-59 e) and, most notably, a fifth planet, L 98-59 f. This newly confirmed super-Earth, estimated to be nearly three times the mass of our own planet, receives a similar amount of energy from its host star as Earth does from the Sun, placing it firmly within the zone where liquid water, a cornerstone of life as we know it, could theoretically exist.

A European Space Agency spacecraft on its way to Jupiter’s moons has tested out one of its science instruments on our own Moon.

And it’s focussed on the same patch of the lunar surface seen in one of the most iconic images in science.

The Jupiter Icy Moons Explorer (Juice) is headed to Jupiter to study its icy moons to search for signs of alien life, or conditions that could support alien life.

And as it flew past our Moon in August 2024, its Radar for Icy Moon Exploration (RIME) instrument listened to radio wave echoes bounced off the Moon to determine the height of the lunar surface.

Juice and the search for life

Scientists interested in the search for signs of life beyond Earth, and for signs of habitable worlds beyond Earth, say the icy moons of our Solar System are some of the most promising places.

That’s because moons like Enceladus at Saturn or Europa at Jupiter have liquid oceans beneath their icy, frozen surfaces.

And liquid water being a prerequisite for life on Earth as we know it, the presence of liquid water on these moons means they are potentially habitable.

Juice is on its way to study Jupiter’s moons Ganymede, Europa and Callisto.

It will arrive there in July 2031 and begin its exploration of these frozen worlds.

But in the meantime, flybys of other worlds – including our Moon – are giving science teams back on Earth the chance to test Juice’s instruments are working properly.

RIME’s radargram on the Moon

One of Juice’s instruments is the Radar for Icy Moon Exploration (RIME), which is a radar sounder that will give scientists information about what’s going on beneath the surface of the icy moons, as deep as 9km (5.5 miles) into their liquid subsurface oceans.

As Juice passed on our Moon, RIME captured this image of a section of the lunar surface.

Scientists say RIME’s first-ever radargram of a patch of lunar surface matches an elevation model of the same area captured by NASA’s Lunar Orbiter Laser Altimeter (LOLA), seen below.

The bright pink and yellow line that waves across the dark purple background shows the height of the Moon’s surface.

The bumps and dips in the RIME data match up the height of the land in LOLA’s elevation map.

The test was an important stepping stone for RIME, as electronic noise coming from the rest of the spacecraft has been disturbing its readings.

During the flyby of the Moon, all of Juice’s instruments were switched off for 8 minutes, giving RIME the chance to observe in silence.

RIME scientists were then able check how the electronic noise affects the performance of the instrument.

Based on the data collected, they’ve been able to create an algorithm that counteracts disturbances to RIME caused by the rest of the spacecraft.

The team are satisfied the test worked, and RIME is up to the job of providing accurate information on what’s going on beneath Jupiter’s icy moons.

Not just any old patch of the Moon

The patch of the Moon studied by RIME is the same patch that can be seen in astronaut William Anders’ ‘Earthrise’ photo, which was captured on 24 December 1968 during the Apollo 8 mission.

Anders’ Earthrise photo is considered one of the most important images in science, as it gave humanity an unprecedented glimpse of what it would be like to see our home planet from the surface of another world.

The biggest crater, seen in the foreground of the image, was later renamed from ‘Pasteur T’ to ‘Anders’ Earthrise’.

So what next for Juice? The European Space Agency says the spacecraft is due to fly by Venus in August 2025.

This is a gravity assist manoeuvre, using Venus’s gravity to give Juice a boost on its journey.

Onwards to Jupiter, and the chance to find out whether Jupiter’s icy moons do indeed have the potential to host life.

An international team of scientists has, for the first time, directly detected sulfur in both its gas and solid phases in the interstellar medium — the gas- and dust-filled space between stars. This breakthrough was made possible by the X-ray Imaging and Spectroscopy Mission (XRISM) satellite.

To detect sulfur, a team of researchers led by Lia Corrales — an assistant professor of astronomy at the University of Michigan in Ann Arbor — studied X-rays from two binary star systems, GX 340+0 and 4U 1630-472. The Resolve instrument aboard XRISM allowed the scientists to measure the energy of the X-rays, revealing sulfur signatures in both gas and solid phases.

While past missions have studied sulfur in space, they have only directly detected it in its gaseous state. Brian Williams, the XRISM project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, described XRISM’s measurements of space sulfur as “the most detailed yet.”

The solid sulfur detected by XRISM could only be accurately modeled when combined with iron, suggesting the two elements are likely mixed together in space. This finding raises further questions about how elements bond and travel through cosmic environments.

The iron-sulfur model, though needing further studies, isn’t strange; as iron-sulfur compounds are often found in meteorites. Elisa Costantini, a senior astronomer at the Space Research Organization Netherlands and the University of Amsterdam, shared that new sulfur measurements will soon be available to compare with XRISM data.

Sulfur plays a crucial role in the functioning of cells in our bodies. Hence, understanding its distribution in the galaxy holds significant importance. XRISM’s latest discovery is unraveling sulfur’s hiding place in space, providing more insights into the chemical composition of the galaxy we call home.

I have always been fascinated by technology and digital devices my entire life and even got addicted to it. I have always marveled at the intricacy of even the simplest digital devices and systems around us. I have been writing and publishing articles online for about 6 years now, just about a year ago, I found myself lost in the marvel of smartphones and laptops we have in our hands every day. I developed a passion for learning about new devices and technologies that come with them and at some point, I asked myself, “Why not get into writing tech articles?” It is useless to say I followed up the idea — it is evident. I am an open-minded individual who derives an infinite amount of joy from researching and discovering new information, I believe there is so much to learn and such a short life to live, so I put my time to good use — learning new things. I am a ‘bookworm’ of the internet and digital devices. When I am not writing, you will find me on my devices still, I do explore and admire the beauty of nature and creatures. I am a fast learner and quickly adapt to changes, always looking forward to new adventures.

This week, a Cretaceous-era trackway in Canada provides the first evidence of a dinosaur herd combining two species, scientists walked back on the claims that 10,000 is the optimal number of steps per day, and the so-called “entropy catastrophe” has been bypassed after researchers superheated gold to 14 times its melting point. Finally, we explore whether natural antidepressants are a legit alternative or just a load of nonsense.

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Missing 40 Percent Of Matter In The Universe Finally Discovered: “The Simulations Were Right All Along”

The regular matter that makes us, planets, stars, and galaxies is about 5 percent of the matter-energy content of the universe. The rest is made of dark matter and dark energy, though we are not sure what they are. There is also uncertainty around regular matter, since for a long time over one-third of it was not accounted for. Models had suggested that it would exist in the space between galaxies, and different groups using wildly different methods have now confirmed that it really is there. Read the full story here

Could We Be On Track Towards A Universal Cancer Vaccine? New Findings Say: Maybe

An experimental mRNA vaccine that supercharges existing cancer treatments could be laying the groundwork for a “universal” cancer vaccine, according to the team behind the breakthrough. Scientists at the University of Florida tested the innovation in mice and found it provoked a strong antitumor response when paired with immunotherapy. Read the full story here

First Evidence Of A Dinosaur Herd Combining Two Species Revealed In Cretaceous Tracks

A Late Cretaceous trackway in Canada contains the footprints of at least nine dinosaurs from four species. Two of the trackmakers were large tyrannosaurs, which may have sparked the motions of the other dinosaurs. However, while that part of the puzzle remains unsolved, the presence of both ceratopsians and an ankylosaurid moving together appears far more certain, suggesting multi-species herding similar to zebras and wildebeests during their great migration. Read the full story here

Here’s The Actual Number Of Steps You Should Walk Per Day (It’s Not 10,000)

We’re often told we need to walk “X number” of steps every day in order to stay healthy, although most of these claims are made by people who talk the talk but can’t walk the walk. With little or no scientific evidence to back up these daily benchmarks, it has until now remained unclear exactly how many times we should be putting one foot in front of the other. Read the full story here

Solid Gold Superheated To 14 Times Its Melting Point, Bypassing The “Entropy Catastrophe”

Researchers have been able to heat up a sample of solid gold to over 14 times its melting temperature for a fraction of a second, bypassing a theoretical limit known as the entropy catastrophe. The approach, known as superheating, might lead to a better understanding of how substances change phase at a fundamental level and even to improved production of materials. Read the full story here

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Feature of the week: 

Natural Antidepressants: Legit Alternative Or A Load Of Nonsense?

What do zinc, bitter orange, lavender, saffron, and vitamin D all have in common? No, they’re not the ingredients to a bizarre-sounding salad, but they are all products that have been touted as natural antidepressants. The real question is – do any of them actually work? Read the full story here

More content:

Have you seen our e-magazine, CURIOUS? Issue 36 (July 2025) is available now. This month we asked, “How To Fake A Fossil” – check it out for exclusive interviews, book excerpts, long reads, and more.

PLUS, the We Have Questions podcast – an audio version of our coveted CURIOUS e-magazine column – continues. In episode 11, we ask, “Why Are Yawns Contagious?”

The Big Questions podcast has returned, and we’re continuing season 5 with episode 3’s big question: How Do Black Holes Shape The Universe?

Why is Microcarb important?

Rüdiger Lang: 2024 was the hottest year ever recorded, both globally and across Europe – a stark reminder of the urgency of tackling the climate crisis driven by human greenhouse gas emissions. While we know how much carbon dioxide is accumulating in the atmosphere overall, we still lack detailed information about exactly where emissions come from.

The Paris Agreement created momentum to invest in better ways to monitor emissions, and as the first dedicated European CO2 mission, Microcarb is a vital part of Europe’s efforts to track greenhouse gases, hold emitters accountable, and guide climate action. To build a complete picture, we need to separate natural flows of carbon dioxide from those caused by humans and identify sources that remain underrepresented or undetected. If countries can pinpoint emissions more accurately, they can implement targeted policies and, crucially, see whether those measures are working.

Measuring emissions this precisely is extremely challenging, but Microcarb’s sensors achieve accuracy close to 99.98%, making it possible to detect and distinguish both natural and human contributions. Microcarb will quantify how much carbon dioxide is released from both natural and human-made sources and how CO2 moves between the Earth surface, the oceans, the forests, and the atmosphere. The satellite can also zoom in to capture high-resolution snapshots of specific targets such as cities or farming regions.

There is a real need for consistent, reliable data to fill gaps in our understanding, and Microcarb will play an important role in that effort, support more effective climate policies, as well as helping to lay the foundation for larger systems like the Copernicus CO2M constellation.

The largest interstellar comet discovered could be an alien technology. The newly found Manhattan-sized object, named 3I/ATLAS, is approximately 7 miles wide and racing through our solar system.

Avi Loeb, a Harvard scientist, considering the size of the object, gave a hypothesis that it could be an alien probe or artificial technology.

“The hypothesis in question is that 3I/ATLAS is a technological artifact, and has active intelligence. If this is the case, then two possibilities follow,” he said.

The experts opined that, “First, that its intentions are entirely benign and second, they are malign.”

Scientists are investigating the composition and direction of the activity. NASA classified this object as a comet. There is a lack of consensus that 3I/ATLAS poses an alien threat. It will come closer to the sun in October 2025.

This is the third time an object entering our solar system has been detected.

The International Astronomical Union called it a comet and designated it the largest detected object. 

The new object is “moving considerably faster than the other two extra-solar objects that we previously detected”, said Mark Norris, an astronomer at the University of Central Lancashire, UK.

The first interstellar visitor was Oumuamua, discovered in 2017, and the second was 21/Borisov, found in 2019.

How many interstellar objects have been discovered?

As for now, three interstellar objects have been detected: 3I/ATLAS, Oumuamua, and 21/Borisov.