Tag Archives: Astrobiology

Microbes Might Make It Easier to Produce Rocket Fuel on Mars

A computer-generated view of Mars.
Image: NASA/JPL-Caltech

New research details a biological solution for producing rocket fuel on Mars, but significant hurdles need to be overcome to make this intriguing idea work.

With plans to visit Mars next decade, NASA is still sorting out the fuel situation; launching a rocket to the Red Planet is not the issue—it’s getting a vehicle off the surface for the return trip home that’s posing a challenge. Copious amounts of methane and liquid nitrogen will be needed to produce the required propellant, but these key components of rocket fuel are as rare on Mars as fuel refineries.

New research published in Nature Communications estimates a cost of $8 billion to ship the required 30 tons of methane and liquid oxygen to Mars. And that’s just for a single launch with a 500-ton payload! With financial support from NASA’s Innovative Advanced Concepts program, the authors of the new paper have come up with a very different solution, in which key ingredients needed to produce the propellent can be sourced directly on the Red Planet.

These ingredients include carbon dioxide, frozen water, and sunlight. Cyanobacteria, also known as blue-green algae, and a bioengineered strain of E. coli bacteria would be brought to Mars from Earth, along with the materials required to build a large array of photobioreactors. Nick Kruyer, the first author of the new study and a researcher at Georgia Tech’s School of Chemical and Biomolecular Engineering, and his colleagues have outlined a production strategy in which the cyanobacteria, powered by sunlight and carbon dioxide, produce sugars that the E. coli then converts into a viable propellant.

Artist’s conception of the possible bioreactor on Mars.
Image: BOKO mobile study

Called 2,3-butanediol, it isn’t the most energetic propellant ever invented, but in the relative low-gravity environment on Mars, this rocket fuel will get the job done, the researchers argue. As a compound, 2,3-butanediol is already well known, as it’s used in the production of rubber, but scientists have never thought to use it as a propellant until now.

Other scientists had assumed that methane was the only solution, “as it is a high-energy fuel that can be made chemically from carbon dioxide, which is abundant on Mars,” Pamela Peralta-Yahya, a co-author of the study and an associate professor in the School of Chemistry & Biochemistry at Georgia Tech, explained to Gizmodo in an email. “A key insight of this paper is that a broader range of chemicals can be considered for use as propellant because Mars has one-third of the gravity of Earth—so you can use a less energy dense rocket propellant.”

The plastic materials shipped to Mars would be assembled into a photobioreactor array the size of four football fields. Photosynthesis and carbon dioxide would enable growth of the cyanobacteria, while enzymes in a separate reactor would break down the microorganisms into sugar. As Kruyer pointed out in a press release, “biology is especially good at converting CO2 into useful products,” making it a “good fit for creating rocket fuel.” At the E. coli stage, the separation of propellant from the fermentation broth would result in 95% purity, according to the paper.

The bioproduction of Martian rocket propellant would require 32% less power than NASA’s proposed chemical solution—that is, the plan to ship copious amounts of methane to Mars. It would produce 44 tons of excess clean oxygen, which would be put to good use by astronauts. What’s more, the proposed chemical solution would generate carbon monoxide as a byproduct, “which would need to be scrubbed,” said Peralta-Yahya. “Water electrolysis is envisioned, but that chemical…strategy is at a lower technology readiness level,” she added.

As for reducing the overall cost of the endeavor, that’s less obvious, as this solution would require a 2.8-fold higher payload mass than the proposed chemical strategies, the scientists say. That’s significant. The researchers will need to reduce the weight of the equipment, such as minimizing the size of the photobioreactor.

That said, a “key contribution” of the new paper is the “identification of attainable” optimization solutions to reduce the payload mass while also using 59% less power than NASA’s methane plan, Peralta-Yahya explained. “Such optimizations include improving the cyanobacteria growth rate at cold temperatures, which would lead to smaller cyanobacteria farms,” she added.

Georgia Tech engineer and study co-author Matthew Realff said the team will need to run experiments to show that cyanobacteria can actually be grown on Mars. The team needs to “consider the difference in the solar spectrum on Mars both due to the distance from the Sun and lack of atmospheric filtering of the sunlight,” he explained in an email, while also keeping in mind that “high ultraviolet levels could damage the cyanobacteria.”

The researchers will also need to be wary about contaminating Mars with our microbes. Securely containing the cyanobacteria and E. coli will be a necessary step in ensuring that astrobiologists can keep looking for signs of past life on Mars without interference from Earthly organisms.

NASA’s current planetary protection guidelines explicitly prohibit the sending of microbes to the surface of another planet, but as Peralta-Yahya explained, “biotechnology applications on Mars have the potential to provide distinct advantages over chemical processes.” To keep their solution safe, the team would develop and test a number of containment strategies, such as physical barriers, kill switches, and engineered microbes incapable of surviving outside of the reactor.

The scientists have proposed a fascinating solution to a serious problem. Yes, plenty of work remains, but it’s a good start. Mars may be a barren desert, but it’s not completely without resources. We just have to find ways of using them to our best advantage.

More: Martian Colonists Could Use Their Own Blood to Produce Concrete, New Research Suggests.

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Biosignature Spotted on Venus Could Be From Volcanoes, Not Life

A team of planetary scientists said that if there is phosphine on Venus, it could have geological—not biological—origins. Their findings suggest that phosphine, a chemical often associated with microbes, could come from a reaction in the Venusian sky kicked off by volcanic eruptions on the planet’s surface.

Last year, a scientific debate began when a team of scientists announced they had detected phosphine, a gas that is produced by some microorganisms and thus considered a biosignature, in Venus’s atmosphere. Further studies immediately complicated that result, and earlier this year another team said the gas wasn’t phosphine at all but sulfur dioxide. The recent team’s findings, published today in the Proceedings of the National Academy of Sciences, indicate that Venus could have active volcanoes, something planetary scientists have long been unsure about.

The principle is this: Venus’s deep mantle could contain phosphorus compounds, called phosphides, which could be belched into the atmosphere by the planet’s volcanoes in the form of volcanic dust. With enough explosive force—the researchers described the necessary force as that of Earth’s Krakatoa or even the Yellowstone supervolcano—that dust could be blasted high into the planet’s sulfuric acid-clouded atmosphere. There, the phosphides would react with the sulfuric acid to produce phosphine.

A 1991 simulated-color radar image of Maat Mons, a Venusian volcano, taken by the Magellan spacecraft.
Image: NASA/JPL

“The phosphine is not telling us about the biology of Venus,” said Jonathan Lunine, a planetary scientist at Cornell University and co-author of the paper, in a university press release. “It’s telling us about the geology. Science is pointing to a planet that has active explosive volcanism today or in the very recent past.”

But the mystery of whether Venus has phosphine or not, and what might have produced it, is far from settled. “I sadly remain unconvinced by this latest argument,” said Clara Sousa-Silva, a quantum astrochemist at the Center for Astrophysics | Harvard and Smithsonian, in an email. “The reaction of mineral phosphides with concentrated sulfuric acid will not necessarily generate phosphine. ... A likely outcome of reacting phosphides with concentrated sulfuric acid would be an oxidation reaction and not production of phosphine.”

Sousa-Silva’s previous work has examined the atmospheres of Venus and other planets for potential signs of life like phosphine. She added, “we have known (and stated as much, repeatedly) that there are abiotic routes for the formation of phosphine, including volcanism. It’s just that these routes are extremely rare and inefficient.”

Venus’s tectonics are difficult to observe because of the planet’s dense atmosphere, which conceals its surface. The few images we have of the planet’s surface come from the Soviet Venera program of the 1970s and 80s and radar scans taken by the Magellan Orbiter, which can pierce through Venus’s cloud cover. The data that Lunine’s team drew their conclusions from was collected using the James Clerk Maxwell Telescope on Mauna Kea and the ALMA telescope array in Chile. Some images collected by Magellan indicated geological features capable of explosive volcanism, the researchers said. Previously, data from Europe’s Venus Express orbiter indicated that the planet may have active volcanoes.

Thankfully, three upcoming missions are set to tell us a whole lot more about this scorching-hot planet. Around 2030, NASA’s DAVINCI+ probe and VERITAS orbiter and the European Space Agency’s EnVision orbiter will all head to Venus to study its atmospheric makeup and surface tectonics, among other features of our nearest planetary neighbor.

More: Why Venus Is Soon to Be the Most Exciting Place in the Solar System

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Hear Lasers Zap Rocks on Mars in Perseverance’s Latest Dispatch

Mosaic view of a Martian rock dubbed “Yeehgo,” captured by the SuperCam instrument on the Perseverance rover.
Image: NASA/JPL-Caltech/LANL/CNES/CNRS/ASU/MSSS

Unprecedented audio recordings taken by NASA’s Perseverance rover are transporting us to the surface of the Red Planet, allowing us to hear the sound of a gentle alien breeze, and the click-clicking of lasers zapping a Martian rock.

We’re exactly three weeks into the Perseverance mission, so it’s still early days. The project is in the deployment phase, with the Mars 2020 team systematically deploying each of the rover’s many instruments to make sure they’re working properly and configured for the science phase of the mission. Perseverance will spend the next two years or more exploring Jezero crater, so there’s no need to rush things along.

The team recently rolled out the rover’s aptly named SuperCam, in an early showcase of the instrument’s tremendous potential. Affixed to the rover’s mast, the 12-pound (5.4kilogram) SuperCam can perform five different types of geological analysis, allowing the team to select the best rocks for sampling.

Close-up SuperCam image of a rock dubbed “Máaz,” which means Mars in the Navajo language.
Image: NASA/JPL-Caltech/LANL/CNES/CNRS

These explorations are important from a geological perspective, but also from an astrobiological perspective. Rocks in Jezero crater—a former lake—could contain fossils or other biomarkers indicative of former microbial life. Whereas the key goal of the ongoing Curiosity mission was to determine if Mars was once habitable (it apparently was), the Perseverance rover is actually looking for evidence of ancient aliens (to be clear, habitability is different than inhabited; Mars may have once fostered the conditions for life, but that doesn’t mean life actually took root on the Red Planet).

The SuperCam instrument was developed by the Los Alamos National Laboratory in New Mexico and a consortium of French labs headed by the Centre National d’Etudes Spatiales. The first data packet from SuperCam was recently received at the French Space Agency’s control center in Toulouse, according to a NASA statement. Newly released SuperCam images show a pair of rocks, dubbed Yeehgo and Máaz, in exquisite detail.

“It is amazing to see SuperCam working so well on Mars,” Roger Wiens, the principal investigator for SuperCam, said in the statement. “When we first dreamed up this instrument eight years ago, we worried that we were being way too ambitious. Now it is up there working like a charm.”

Perseverance is also unique in that it’s capable of recording sounds on Mars. NASA has provided three different audio samples, and they include the first acoustic recording of laser shots on Mars, and the sound of Martian winds.

Perseverance recorded the laser sounds at a distance of 10 feet (3.1 meters) from the target rock. The clicking sounds produced by the laser pulses vary, allowing scientists to infer various physical characteristics of the target, such as hardness.

“SuperCam truly gives our rover eyes to see promising rock samples and ears to hear what it sounds like when the lasers strike them,” explained Thomas Zurbuchen, associate administrator for science at NASA headquarters in Washington, DC, in the statement. “This information will be essential when determining which samples to cache and ultimately return to Earth through our groundbreaking Mars Sample Return Campaign, which will be one of the most ambitious feats ever undertaken by humanity.”

The future mission Zurbuchen is referring to will be quite historic, as the samples cached by Perseverance would represent the first Martian materials returned to Earth for analysis.

The Mars 2020 team has also rolled out and received data from the rover’s visible and infrared sensor, one of the SuperCam sensors. This instrument gathers reflected sunlight, exposing the mineral content of rocks and sediments.

SuperCam’s Raman spectrometer is also producing data, an achievement that now represents the first time that spectroscopy has been done somewhere other than Earth, Olivier Beyssac, CNRS research director at the Institute of Mineralogy, Materials Physics and Cosmochemistry in Paris, pointed out in the NASA statement. Raman spectroscopy works by shooting light—specifically green laser beams—at a target object, like a rock. This non-destructive technique shows how light is interacting with chemical bonds in the target, providing information about the object’s chemical structure, internal levels of stress, and other information.

“Raman spectroscopy is going to play a crucial role in characterizing minerals to gain deeper insight into the geological conditions under which they formed and to detect potential organic and mineral molecules that might have been formed by living organisms,” said Beyssac.

Looking ahead, the Mars 2020 team will continue to test the rover’s driving capabilities (it’s already clocked 21.3 feet [6.5 meters]), and choose an aerial field from which to deploy the Ingenuity helicopter.

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Recovery of Rare Meteorite a ‘Dream Come True’ for Scientists

The rare meteorite, which fell to Earth on Feb. 28, 2021.
Image: The University of Manchester

A chunk of black rock dating back to the earliest days of the solar system has fallen onto a residential driveway in the UK.

Late last month, a rock weighing around 10.6 ounces (300 grams) pinged onto a driveway belonging to Rob and Cathryn Wilcock, who live in the small town of Winchcombe, UK.

“When I heard it drop, I stood up and looked out the window to see what was there. But because it was dark I couldn’t see anything,” Hannah, the daughter of the couple, told the BBC. “It was only the next morning when we went out that we saw it on the drive—a bit like a kind of splatter. And in all honesty, my original thought was—has someone been driving around the Cotswolds lobbing lumps of coal into people’s gardens?”

A lump of coal, it is not. Rather, it’s a meteorite. And not just any kind of meteorite—it’s a piece of carbonaceous chondrite which, at an estimated 4.5 billion years old, dates back to the formation of the solar system, according to a statement from the University of Manchester.

“Nearly all meteorites come to us from asteroids, the leftover building blocks of the solar system that can tell us how planets like the Earth formed,” Ashley King, UK Research and Innovation Future Leaders Fellow in the Department of Earth Sciences at the Natural History Museum, said in the statement. “The opportunity to be one of the first people to see and study a meteorite that was recovered almost immediately after falling is a dream come true!”

The fireball, as seen over the UK and northern Europe on Feb. 28, 2021.
Image: Ben Stanley/Markus Kempf/AllSky7 network via the University of Manchester

The rare sample arrived in a blaze of glory, as the rock lit the skies above the UK and northern Europe on Feb. 28, 2021. The fireball, which entered Earth’s atmosphere at speeds reaching 8.7 miles per second (14 kilometers per second), was spotted by thousands of witnesses, many of whom reported the spectacle to the UK Meteor Observation Network.

Extensive camera footage taken of the event from different angles allowed scientists to triangulate a landing spot, and to also recreate its flight path through the solar system, according to the University of Manchester statement. Other remnants of the shattered asteroid are believed to have fallen either in the region known as the Cotswold, and a search for these valuable pieces continues.

Along with the main piece, there are other smaller fragments from the meteorite hitting the driveway. Despite being a dusty, shattered mess, the pieces are in excellent condition, and they’re being compared to pristine samples returned from space missions.

“I was in shock when I saw it and immediately knew it was a rare meteorite and a totally unique event,” Richard Greenwood, a research fellow at the Open University, said in the statement. “It’s emotional being the first one to confirm to the people standing in front of you that the thud they heard on their driveway overnight is in fact the real thing.”

Carbonaceous chondrites are formed from a combination of minerals and organic compounds, such as amino acids. By studying such ancient objects, scientists can peer back to the earliest days of the solar system, allowing them to better understand the origin of planets and water, and how the basic building blocks of life reached Earth.

“We’re absolutely thrilled that something that’s going to be so valuable to science, to the human understanding of the world and of the Solar System has happened, and that we can be a small part in it,” Rob Wilcock told BBC.

The meteorite will be moved the Natural History Museum, allowing for a formal investigation of the object.

Of the tens of thousands of known meteorites on Earth, only 51 are carbonaceous chondrites. The meteorite from Feb. 28 is the first carbonaceous chondrite to be found in the UK, and the first meteorite sample to be retrieved in the county since 1991.

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Bad Astronomy | Titan haze particles made in a lab and photographed in extreme detail

Titan is the largest moon of Saturn, and the second largest moon in the solar system, about the same size as Mercury. Unique among moons, it has a thick atmosphere — despite the lower gravity, the surface pressure is 1.5 times Earth’s at sea level.

Its atmosphere is 95% nitrogen (Earth’s is 78%) and 5% methane. Normally that would be transparent, but Titan’s air is loaded with haze — tiny particles about a micron across (one-millionth of a meter; a human hair is roughly 50–100 microns wide). These particles are suspended in the atmosphere, making it opaque.

The haze particles are formed when ultraviolet light from the Sun and/or subatomic particles zipping around space slam into the nitrogen and methane, breaking it down into elements that then rearrange themselves into more complex molecules. Some of them are simple rings of carbon, and some are far more complex molecules called PAHs — polycyclic aromatic hydrocarbons. It’s not been clear how the simple ones link up to form the bigger ones, but now, for the first time, this process has been simulated in a lab and the results examined using a powerful type of microscope that reveals the basic atomic configurations of the molecules.

That’s amazing. Those are individual molecules you’re seeing in those images. The scalebar is 0.5 nanometers, half of a billionth of a meter. They’re not images like a photograph, though. It’s literally impossible to do this with visible light; the wavelength of light is hundreds of nanometers, too long to see structures this small. Instead, they used what’s called atomic force microscopy*.

This uses a technique analogous to the way phonographs work, by using a needle at the end of an arm that traces the grooves in a record. In this case though, a molecule at the tip of a microscopic needle runs along a molecule and can detect the change in the shape due to atomic forces holding the molecule together. It’s like running your fingers over an object to feel its shape.

The samples of molecules were created in a lab to simulate Titan’s atmosphere. Scientists filled a stainless steel vessel with a gaseous mixture that’s the same as Titan’s air and used an electric discharge (a spark maker, essentially) to simulate the UV and cosmic rays hitting the gas. It’s not exactly like Titan: They did this at room temperature, which is much warmer than Titan, but the reactions aren’t very sensitive to temperature. They also used a gas pressure of about 0.001 Earth’s, which, though very thin, is much higher than the top of Titan’s atmosphere where the reactions take place. However, the higher pressure allows the reaction rate to be much higher, so they aren’t waiting weeks to get a decent sample.

They found over a hundred different molecules, a dozen or so of which they could examine using their microscope. Many are simple carbon rings and more complex PAHs, as expected. But they also found that many of the PAHs had a nitrogen atom embedded in them, making what are called N-PAHs. These molecules were detected in Titan’s atmosphere by the Cassini mission, which orbited Saturn for 13 years and made over 100 passes of Titan during that time, examining its surface and atmosphere. The simulations in the lab confirm this result.

Moreover, the lab experiment created molecules made of many connected rings, up to seven of them, which will help atmospheric scientists understand how the more complex PAHs are made from simpler molecules.

This work is important for many reasons. Titan’s atmosphere is loaded with this stuff, collectively called tholins (Greek for “mud”, since they make molecules which color the environment yellow, orange, and reddish-brown), and they’re also seen on other worlds; Pluto’s reddish colored landscape is due to tholins.

Titan doesn’t have a water cycle like Earth, but it does have a methane cycle: Liquid methane in vast lakes at its north pole evaporates into the atmosphere, rains down on the hills nearby, then flows back into the lakes. Methane vapor may condense on the suspended tholins, helping it rain out, and then the tholins can coat the moon’s surface. That’s very interesting, because nitrogen and carbon molecules are important in prebiotic chemistry, making up amino acids, which in turn are the building blocks of proteins.

Earth’s early atmosphere was likely very similar to Titan’s, before the Great Oxygenation Event about 3 billion years ago which gave us the atmosphere, more or less, we have today. Studying Titan is like studying ancient Earth. Not to be too broad, but life evolved on Earth in that early atmosphere, so it’s not too silly to wonder if something similar is occurring on Titan. We certainly don’t know if life is brewing or thriving there, but it’s certainly within the realm of science to look into it.

Titan is an alien world over a billion kilometers from the Sun, and drier than any desert on our own planet. Yet there are aching similarities, ones we can study in the lab. NASA is already in the early stages of planning a mission to Titan called Dragonfly — a lander and quadcopter drone that will fly over the surface and examine regions likely to have or have had conditions conducive to life.

What will it find there? These lab results are an important step in figuring that out.


*Just typing those words makes me feel like a scientist in an old black-and-white sci-fi movie.

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Intriguing ‘Life’ Signal on Venus Was Plain Old Sulphur Dioxide, New Research Suggests

The night side of Venus as seen in thermal infrared.
Image: JAXA/ISAS/DARTS/Damia Bouic

Scientists stunned the world last year by claiming to have discovered traces of phosphine in the Venusian clouds. New research suggests this gas—which, excitingly, is produced by microbes—was not actually responsible for the signal they detected. Instead, it was likely sulfur dioxide, a not-so-thrilling chemical.

Extraordinary research published in Nature last September is being challenged by a paper set to be published in The Astrophysical Journal, a preprint of which is currently available at the arXiv. This is not the first paper to critique the apparent discovery of phosphine on Venus, and it’s probably not going to be the last.

That phosphine might be present on Venus was a revelation that blew our minds, and that’s because living organisms are one of the only known sources of the stinky gas. The team responsible for the apparent discovery, led by astronomer Jane Greaves from Cardiff University, found the evidence in spectral signals collected by two radio dishes: the James Clerk Maxwell Telescope (JCMT) and the Atacama Large Millimeter/submillimeter Array (ALMA). Spectral lines at certain wavelengths indicate the presence of specific chemicals, and in this case they implied the presence of phosphine in the Venusian cloud layer.

The authors of the Nature study were not claiming that life exists on Venus. Rather, they were asking the scientific community to explain their rather bizarre observation. Indeed, it was an exceptional claim, as it implied that Venus—one of the most inhospitable planets in the solar system—might actually be habitable, with microscopic organisms floating through the clouds.

Alas, this doesn’t appear to be the case.

“Instead of phosphine in the clouds of Venus, the data are consistent with an alternative hypothesis: They were detecting sulfur dioxide,” Victoria Meadows, a co-author of the new study and an astronomy professor at the University of Washington, explained in a statement. “Sulfur dioxide is the third-most-common chemical compound in Venus’ atmosphere, and it is not considered a sign of life.”

Meadows, along with researchers from NASA, the Georgia Institute of Technology, and the University of California, Riverside, reached this conclusion by modeling conditions inside the Venusian atmosphere, which they did to re-interpret the radio data gathered by the original team.

“This is what’s known as a radiative transfer model, and it incorporates data from several decades’ worth of observations of Venus from multiple sources, including observatories here on Earth and spacecraft missions like Venus Express,” explained Andrew Lincowski, a researcher with the UW Department of Astronomy and the lead author of the paper, in the statement.

Equipped with the model, the researchers simulated spectral lines produced by phosphine and sulphur at multiple atmospheric altitudes on Venus, as well as how those signatures were received by ALMA and JCMT. Results showed that the shape of the signal, detected at 266.94 gigahertz, likely came from the Venusian mesosphere—an extreme height where sulphur dioxide can exist but phosphine cannot owing to the harsh conditions there, according to research. In fact, so extreme is this environment that phosphine wouldn’t last for more than a few seconds.

As the authors argue, the original researchers understated the amount of sulphur dioxide in the Venusian atmosphere and instead attributed the 266.94 gigahertz signal to phosphine (both phosphine and sulphur dioxide absorb radio waves around this frequency). This happened, according to the researchers, due to an “undesirable side-effect” known as spectral line dilution, study co-author and NASA JPL scientist Alex Akins explained in the statement.

“They inferred a low detection of sulfur dioxide because of [an] artificially weak signal from ALMA,” added Lincowski. “But our modeling suggests that the line-diluted ALMA data would have still been consistent with typical or even large amounts of Venus sulfur dioxide, which could fully explain the observed JCMT signal.”

This new result could prove devastating for the Nature paper, and it’ll be interesting to hear how the authors respond to this latest critique. That said, some scientists believe the writing is already on the wall, or more accurately, the trash bin.

“Already quickly after publication of the original work, we and others have put strong doubts on their analysis,” wrote Ignas Snellen, a professor at Leiden University, in an email. “Now, I personally think that this is the final nail in the coffin of the phosphine hypothesis. Of course, one can never prove that Venus is completely phosphine-free, but at least there is now no remaining evidence to suggest otherwise. I am sure that others will keep on looking though.”

Back in December, Snellen and his colleagues challenged the Nature study, arguing that the method used by the Greaves team resulted in a “spurious” high signal-to-noise ratio and that “no statistical evidence” exists for phosphine on Venus.

The apparent absence of phosphine on Venus, and thus the absence of any hints of microbial life, is far less interesting than the opposite, but that’s how it goes sometimes. Science makes no claims or promises about the interestingness of all things, and we, as defenders of the scientific method, must come to accept our unfolding universe as we find it.

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