Category: 7. Science

  • Mineralogy, Geochemistry And Morphology Of Arctic Gossans On Axel Heiberg Island, NU, Canada: Spectroscopic Investigation And Implications For Mars

    Mineralogy, Geochemistry And Morphology Of Arctic Gossans On Axel Heiberg Island, NU, Canada: Spectroscopic Investigation And Implications For Mars

    (A) Map of the study area on Axel Heiberg Island, Nunavut, Canada. The north arrow is valid for every panel. (B) Geological map of the region modified from Harrison and Jackson (2010) with the sampling sites (yellow dots) selected for the study grouped by sector. CR: Colour ridge, WG: White glacier, GH: Gypsum Hill. The ArcticDEM was used to highlight the topography of the area. (C) Sampling sites (yellow dots) with ESRI imagery used as a basemap. The scale is the same as in panel b. (For interpretation of the references to color in this figure legend, the reader is referred to the Web version of this article.) — Science Direct

    Gossans are formed through the oxidation of sulfide ore deposits by fluids, such as meteoric water or hydrothermal solutions, leading to locally acidic conditions.

    In permafrost regions, gossans undergo seasonal chemical weathering after their initial formation (reactive gossans), potentially providing a sustained energy source for microbial activity.

    Arctic gossans are therefore considered valuable analogs for Martian paleo-hydrothermal systems and promising astrobiological targets. While hundreds of gossans have been identified in the Arctic, few have been studied in detail and even fewer using rover-compatible remote sensing techniques.

    This study aims to characterize the morphological profile of seven Arctic gossans located at Expedition Fiord (Axel Heiberg Island, Nunavut), as well as their geochemistry, mineralogy and organic carbon content using X-ray fluorescence, X-ray diffraction (XRD), Visible (VNIR) to thermal infrared (MIR-TIR) reflectance and Raman spectroscopy.

    Results showed a dominance of silicon, calcium and iron. Mineralogical analyses revealed gypsum and quartz as major phases, with variable amounts of silicates, sulfates, iron sulfides and iron oxyhydroxides.

    Raman spectroscopy detected organic carbon in most samples, up to 50 cm deep, in various organo-mineral complexes. XRD was the only technique to detect iron sulfides. VNIR-MIR-TIR reflectance and Raman spectroscopy provided mineralogical results consistent with XRD. All gossans displayed classical profiles, with alteration zones overlying primary sulfides, but showed diverse color and compositional stratification patterns.

    These variations suggest local mechanisms influence mineral and associated organic carbon distribution. Further investigations should focus on better understanding these local variations, which could guide the search for biosignatures in gossan-like features on Mars.

    Mineralogy, geochemistry And Morphology Of Arctic Gossans On Axel Heiberg Island, NU, Canada: Spectroscopic Investigation And Implications For Mars, Science Direct (open access)

    Astrobiology

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  • Inferring And Interpreting The Visual Geometric Albedo and Phase Function of Earth

    Inferring And Interpreting The Visual Geometric Albedo and Phase Function of Earth

    Phase-dependent measurements of Earth’s broadband visual apparent albedo, including historic observations from Danjon (1928). Mission or observing technique is indicated by datapoint color and shape. Uncertainties are indicated, which are sometimes smaller than the point size. — astro-ph.EP

    Understanding reflectance-related quantities for worlds enables effective comparative planetology and strengthens mission planning and execution.

    Measurements of these properties for Earth, especially its geometric albedo and phase function, have been difficult to achieve due to our Terrestrial situation — it is challenging to obtain planetary-scale brightness measurements for the world we stand on.

    Using a curated dataset of visual phase-dependent, disk-averaged observations of Earth taken from the ground and spacecraft, alongside a physical-statistical model, this work arrives at a definitive value for the visual geometric albedo of our planet: 0.242 (+0.005/-0.004).

    This albedo constraint is up 30–40% smaller than earlier, widely-quoted values. The physical-statistical model enables retrieval-like inferences to be performed on phase curves, and includes contributions from optically thick clouds, optically thin aerosols, Rayleigh scattering, ocean glint, gas absorption, and Lambertian surface reflectance.

    Detailed application of this inverse model to Earth’s phase curve quantifies contributions of these different processes to the phase-dependent brightness of the Pale Blue Dot. Model selection identifies a scenario where aerosol forward scattering results in a false negative for surface habitability detection.

    Observations of phase curves for Earth at redder-optical or near-infrared wavelengths could disentangle ocean glint effects from aerosol forward scattering and would help with understanding the utility of phase curve observations for the under-development Habitable Worlds Observatory.

    Tyler D. Robinson

    Comments: Submitted to PSJ; comments welcome and appreciated!
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
    Cite as: arXiv:2507.22258 [astro-ph.EP] (or arXiv:2507.22258v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2507.22258
    Focus to learn more
    Submission history
    From: Tyler Robinson
    [v1] Tue, 29 Jul 2025 22:14:50 UTC (8,184 KB)
    https://arxiv.org/abs/2507.22258

    Astrobiology,

    Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻

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  • 700,000 years ahead of their teeth: The carbs that made us human

    700,000 years ahead of their teeth: The carbs that made us human

    As early humans spread from lush African forests into grasslands, their need for ready sources of energy led them to develop a taste for grassy plants, especially grains and the starchy plant tissue hidden underground.

    But a new Dartmouth-led study shows that hominins began feasting on these carbohydrate-rich foods before they had the ideal teeth to do so. The study provides the first evidence from the human fossil record of behavioral drive, wherein behaviors beneficial for survival emerge before the physical adaptations that make it easier, the researchers report in Science.

    The study authors analyzed fossilized hominin teeth for carbon and oxygen isotopes left behind from eating plants known as graminoids, which includes grasses and sedges. They found that ancient humans gravitated toward consuming these plants far earlier than their teeth evolved to chew them efficiently. It was not until 700,000 years later that evolution finally caught up in the form of longer molars like those that let modern humans easily chew tough plant fibers.

    The findings suggest that the success of early humans stemmed from their ability to adapt to new environments despite their physical limitations, says Luke Fannin, a postdoctoral researcher at Dartmouth and lead author of the study.

    “We can definitively say that hominins were quite flexible when it came to behavior and this was their advantage,” Fannin says. “As anthropologists, we talk about behavioral and morphological change as evolving in lockstep. But we found that behavior could be a force of evolution in its own right, with major repercussions for the morphological and dietary trajectory of hominins.”

    Nathaniel Dominy, the Charles Hansen Professor of Anthropology at Dartmouth and senior author of the study, says isotope analysis overcomes the enduring challenge of identifying the factors that caused the emergence of new behaviors — behavior doesn’t fossilize.

    “Anthropologists often assume behaviors on the basis of morphological traits, but these traits can take a long time — a half-million years or more–to appear in the fossil record,” Dominy says.

    “But these chemical signatures are an unmistakable remnant of grass-eating that is independent of morphology,” he says. “They show a significant lag between this novel feeding behavior and the need for longer molar teeth to meet the physical challenge of chewing and digesting tough plant tissues.”

    The team analyzed the teeth of various hominin species, beginning with the distant human relative Australopithecus afarensis, to track how the consumption of different parts of graminoids progressed over millennia. For comparison, they also analyzed the fossilized teeth of two extinct primate species that lived around the same time — giant terrestrial baboon-like monkeys called theropiths and small leaf-eating monkeys called colobines.

    All three species veered away from fruits, flowers, and insects toward grasses and sedges between 3.4 million to 4.8 million years ago, the researchers report. This was despite lacking the teeth and digestive systems optimal for eating these tougher plants.

    Hominins and the two primates exhibited similar plant diets until 2.3 million years ago when carbon and oxygen isotopes in hominin teeth changed abruptly, the study found. This plummet in both isotope ratios suggests that the human ancestor at the time, Homo rudolfensis, cut back on grasses and consumed more oxygen-depleted water.

    The researchers lay out three possible explanations for this spike, including that these hominins drank far more water than other primates and savanna animals, or that they suddenly adopted a hippopotamus-like lifestyle of being submerged in water all day and eating at night.

    The explanation most consistent with what’s known about early-human behavior, they report, is that later hominins gained regular access to underground plant organs known as tubers, bulbs, and corms. Oxygen-depleted water also is found in these bulging appendages that many graminoids use for storing large amounts of carbohydrates safely away from plant-eating animals.

    The transition from grasses to these high-energy plant tissues would make sense for a species growing in population and physical size, Fannin says. These underground caches were plentiful, less risky than hunting, and provided more nutrients for early humans’ expanding brains. Having already adopted stone tools, ancient humans could dig up tubers, bulbs, and corms while facing little competition from other animals.

    “We propose that this shift to underground foods was a signal moment in our evolution,” Fannin says. “It created a glut of carbs that were perennial — our ancestors could access them at any time of year to feed themselves and other people.”

    Measurements of hominin teeth showed that while they became consistently smaller — shrinking about 5% every 1,000 years — molars grew longer, the researchers report. Hominins’ dietary shift toward graminoids outpaced that physical change for most of their history.

    But the study found that the ratio flipped about 2 million years ago with Homo habilis and Homo ergaster, whose teeth exhibited a spurt of change in shape and size more suited to eating cooked tissues, such as roasted tubers.

    Graminoids are ubiquitous across many ecosystems. Wherever they were, hominins would have been able to maximize the nutrients derived from these plants as their teeth became more efficient at breaking them down, Dominy says.

    “One of the burning questions in anthropology is what did hominins do differently that other primates didn’t do? This work shows that the ability to exploit grass tissues may be our secret sauce,” Dominy says.

    “Even now, our global economy turns on a few species of grass–rice, wheat, corn, and barley,” he says. “Our ancestors did something completely unexpected that changed the game for the history of species on Earth.”

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  • How Close Can the Juno Spacecraft Get to the Interstellar Object 3I/ATLAS? | by Avi Loeb | Aug, 2025

    How Close Can the Juno Spacecraft Get to the Interstellar Object 3I/ATLAS? | by Avi Loeb | Aug, 2025

    Zoom image will be displayed

    Thrust impulse ∆V (left vertical axis) and propellant mass (right vertical axis) needed for Juno to come within a range of distances from 3I/ATLAS (horizontal axis). The launch date is assumed to be September 15, 2025. (Image credit: Loeb, Hibberd & Crowl 2025)

    In my latest paper with Adam Hibberd and Adam Crowl from July 28, 2025, I proposed using the Juno spacecraft, currently in orbit around Jupiter, to probe the newly discovered interstellar object 3I/ATLAS, which will pass on March 16, 2026 within a distance of 53.6 million kilometers from Jupiter.

    This is a story of scientific redemption. The Juno mission was destined to crash into Jupiter in mid-September 2025. Instead of giving the spacecraft a push into the abyss of Jupiter’s atmosphere, our paper proposes to extend its scientific lifespan by giving it a push away from Jupiter — so that by mid-March 2026 Juno will get close to 3I/ATLAS as it comes near Jupiter. If the remaining propellant is insufficient for a zero-distance intercept (a physical collision!), then a milder burn of Juno’s engine in mid-September 2025 could still bring Juno closer to the path of 3I ATLAS by mid-March 2026.

    How close can Juno get to 3I/ATLAS as a function of the available fuel mass?

    This question became timely after a phone call that I received from Congresswoman Anna Paulina Luna, who on July 31, 2025 sent a letter to NASA’s leadership encouraging the use of Juno as a probe of 3I/ATLAS.

    A close encounter between Juno and 3I/ATLAS will provide a once-in-a-lifetime opportunity to bring a human-made spacecraft within a short distance from a large interstellar object. The event will also be an unprecedented public outreach opportunity for NASA.

    The next step is for NASA to assess the remaining amount of fuel left in Juno’s engine. Once the fuel reservoir will be known, it would be possible to optimize the timing for applying thrust impulses to Juno’s trajectory so as to bring it closest to 3I/ATLAS in mid-March 2026.

    In anticipation of NASA’s study, we have added new figures to our paper that show the distance of closest approach between Juno and 3I/ATLAS as a function of the remaining propellant mass that its engine can use.

    The above figure suggests that burning a small propellant mass of just 110 kilograms — which is merely 5.4% of Juno’s initial fuel mass — on September 15, 2026, will allow Juno to get within a distance of 25 million kilometers from 3I/ATLAS by March 16, 2026. With more propellant burnt, the minimum distance could shrink significantly.

    There fuel requirement can be further minimized with the application of more than one impulse. The best propulsion strategy can be finalized after the exact quantity of propellant remaining in Juno is determined. Corrections to Juno’s path might be needed if cometary activity of 3I/ATLAS will be intensified as it comes closer to the Sun and its non-gravitational acceleration will change its expected trajectory.

    The instruments on Juno, namely a near-infrared spectrometer, magnetometer, microwave radiometer, gravity science instrument, energetic particle detector, radio and plasma wave sensor, UV spectrograph and visible light camera/telescope, can all be used to probe the nature of 3I/ATLAS from a close distance, far better than any observatories on Earth.

    Here’s hoping that NASA with attend to the visionary letter and tweet (accessible here with about 300k views within a day) from Congresswoman Luna. The resulting benefits will be great to space science and to understanding our place in our cosmic neighborhood.

    ABOUT THE AUTHOR

    Zoom image will be displayed

    (Image Credit: Chris Michel, National Academy of Sciences, 2023)

    Avi Loeb is the head of the Galileo Project, founding director of Harvard University’s — Black Hole Initiative, director of the Institute for Theory and Computation at the Harvard-Smithsonian Center for Astrophysics, and the former chair of the astronomy department at Harvard University (2011–2020). He is a former member of the President’s Council of Advisors on Science and Technology and a former chair of the Board on Physics and Astronomy of the National Academies. He is the bestselling author of “Extraterrestrial: The First Sign of Intelligent Life Beyond Earth” and a co-author of the textbook “Life in the Cosmos”, both published in 2021. The paperback edition of his new book, titled “Interstellar”, was published in August 2024.

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  • Can A Convecting Magma Ocean Offer A Solution To The Puzzling Case Of Core Convection In Early Earth? – astrobiology.com

    1. Can A Convecting Magma Ocean Offer A Solution To The Puzzling Case Of Core Convection In Early Earth?  astrobiology.com
    2. Invariance of dynamo action in an early-Earth model  Nature
    3. How Earth’s ancient magnetic shield may have sparked life  Earth.com
    4. Earth’s magnetic field: how the liquid core protected life a billion years ago  Universe Space Tech
    5. Geophysicists Ran Simulations And Found That Earth’s Liquid Core May Have Released a Magnetic Field in the Past  Knewz

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  • ‘It’s the signal that initiates healing’

    ‘It’s the signal that initiates healing’

    Scientists at the University of Helsinki have found that plants use gas movement to heal their protective outer layers.

    When a plant’s outer cork layer gets damaged, gases shift. Ethylene escapes while oxygen flows in through the wound. This simple gas exchange tells the plant to start repairs.

    The protective cork layer, called the periderm, normally blocks gases from moving in or out, which creates conditions where ethylene (a plant hormone) builds up inside while oxygen levels drop due to the plant’s natural growth processes. 

    When damage occurs, this balance gets disrupted.

    “Gas diffusion through a wound isn’t just a consequence of injury — it’s the signal that initiates healing,” explained Dr. Hiroyuki Iida, the lead scientist on the project.

    The team first noticed ethylene’s role in healing, then worked with University of Oxford Professor Francesco Licausi to confirm oxygen’s importance, too.







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    Once repairs finish and the barrier seals back up, gases again accumulate inside the plant, which signals that healing can stop and normal growth can resume. This elegant detection system works without complex sensors, using basic physics to monitor barrier integrity.

    This discovery holds promise for the future of food waste and crop resilience. Potatoes, carrots, fruits, and other produce with damaged outer layers tend to lose water and become more susceptible to disease, ultimately leading to spoilage. 

    By studying and improving this natural repair system, farmers might grow plants that handle dry conditions better, while picked produce could stay fresh for longer in stores.

    With warming temperatures and growing populations putting pressure on global food systems, this finding creates promising paths for more sustainable farming. Improving how plants heal could help feed more people while cutting waste throughout the food supply chain.

    Researchers are now exploring practical uses that could reach farms and food storage facilities within the next few years.

    Join our free newsletter for good news and useful tips, and don’t miss this cool list of easy ways to help yourself while helping the planet.


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  • Innovative mRNA Therapy Emerges as a Potential Heart Regeneration Solution Post-Heart Attack

    Innovative mRNA Therapy Emerges as a Potential Heart Regeneration Solution Post-Heart Attack

    Sat 2nd Aug, 2025

    Heart attacks are a significant contributor to mortality and disability globally, primarily due to the irreversible loss of cardiomyocytes, which leads to chronic heart failure. Traditional treatments focus on symptom management rather than addressing the underlying cardiac damage.

    Researchers at the Lewis Katz School of Medicine at Temple University have pioneered a novel approach aimed at repairing damaged cardiac tissue by reactivating a crucial developmental gene. Their findings, published in Theranostics, detail how the gene PSAT1 can be delivered through synthetic modified messenger RNA (modRNA) to stimulate heart muscle regeneration and enhance cardiac function following a heart attack.

    Dr. Raj Kishore, the lead researcher and a prominent figure in cardiovascular research at Temple University, explained that PSAT1 is significantly expressed during early heart development but becomes inactive in adult hearts. The research team sought to determine if reactivating this gene could trigger regenerative processes in adult cardiac tissue following injury.

    To explore this hypothesis, the team synthesized PSAT1-modRNA and administered it directly into the hearts of adult mice immediately after inducing a heart attack. Their goal was to reinitiate regenerative signaling pathways that promote cell survival, proliferation, and angiogenesis–processes typically active during early development but dormant in adult tissues.

    The outcomes were compelling. Mice receiving the PSAT1-modRNA treatment exhibited notable increases in cardiomyocyte proliferation, decreased tissue scarring, enhanced blood vessel formation, and improved heart function and survival rates compared to untreated controls.

    Investigations into the mechanisms revealed that PSAT1 activates the serine synthesis pathway (SSP), a critical metabolic network linked to nucleotide synthesis and cellular stress resistance. The activation of SSP resulted in reduced oxidative stress and DNA damage, both of which contribute to cardiomyocyte death following myocardial infarction.

    Furthermore, the study established that PSAT1 is transcriptionally regulated by YAP1, a known promoter of regenerative signaling. PSAT1 also facilitates the nuclear movement of ?-catenin, a protein essential for cardiomyocyte cell cycle re-entry. Notably, inhibiting SSP negated the positive effects of PSAT1, underscoring the pathway’s vital role in cardiac repair.

    The implications of these findings are significant. The modRNA technology, which has recently revolutionized vaccine development, offers a flexible and efficient means of delivering genes like PSAT1 with high specificity and minimal side effects. Unlike traditional viral gene therapies, modRNA does not integrate into the host genome, thereby reducing the risk of long-term complications.

    This research opens a new therapeutic pathway for ischemic heart disease, signaling a shift towards mRNA-based strategies aimed at regenerating damaged organs. The team plans to further investigate the safety, durability, and delivery optimization of PSAT1-based therapies in larger animal models. They also intend to refine the timing and localization of gene expression, crucial factors for clinical implementation.

    Although still in preclinical stages, this work represents a significant advancement toward therapies that not only address heart failure but also aim to repair the heart at its fundamental level.

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  • SpaceX delivers four astronauts to the International Space Station

    SpaceX delivers four astronauts to the International Space Station

    CAPE CANAVERAL, Fla. (AP) — SpaceX delivered a fresh crew to the International Space Station on Saturday, making the trip in a quick 15 hours.

    The four U.S., Russian and Japanese astronauts pulled up in their SpaceX capsule after launching from NASA’s Kennedy Space Center. They will spend at least six months at the orbiting lab, swapping places with colleagues up there since March. SpaceX will bring those four back as early as Wednesday.

    READ MORE: Astronaut crew launches to ISS after being sidelined by Boeing’s troubled Starliner

    Moving in are NASA’s Zena Cardman and Mike Fincke, Japan’s Kimiya Yui and Russia’s Oleg Platonov — each of whom had been originally assigned to other missions. “Hello, space station!” Fincke radioed as soon as the capsule docked high above the South Pacific.

    Cardman and another astronaut were pulled from a SpaceX flight last year to make room for NASA’s two stuck astronauts, Boeing Starliner test pilots Butch Wilmore and Suni Williams, whose space station stay went from one week to more than nine months. Fincke and Yui had been training for the next Starliner mission. But with Starliner grounded by thruster and other problems until 2026, the two switched to SpaceX.

    Platonov was bumped from the Soyuz launch lineup a couple of years ago because of an undisclosed illness.

    Their arrival temporarily puts the space station population at 11.

    “It was such an unbelievably beautiful sight to see the space station come into our view for the first time,” Cardman said once on board.

    While their taxi flight was speedy by U.S. standards, the Russians hold the record for the fastest trip to the space station — a lightning-fast three hours.

    The Associated Press Health and Science Department receives support from the Howard Hughes Medical Institute’s Department of Science Education and the Robert Wood Johnson Foundation. The AP is solely responsible for all content.

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  • SpaceX astronauts International Space Station

    SpaceX astronauts International Space Station

    A SpaceX Falcon Nine rocket lifts off from Launch Complex 39A carrying NASA’s Crew-11 mission to the International Space Station in Cape Canaveral, Florida, U.S., August 1, 2025.

    Steve Nesius | Reuters

    SpaceX delivered a fresh crew to the International Space Station on Saturday, making the trip in a quick 15 hours.

    The four U.S., Russian and Japanese astronauts pulled up in their SpaceX capsule after launching from NASA’s Kennedy Space Center. They will spend at least six months at the orbiting lab, swapping places with colleagues up there since March. SpaceX will bring those four back as early as Wednesday.

    Moving in are NASA’s Zena Cardman and Mike Fincke, Japan’s Kimiya Yui and Russia’s Oleg Platonov — each of whom had been originally assigned to other missions. “Hello, space station!” Fincke radioed as soon as the capsule docked high above the South Pacific.

    Cardman and another astronaut were pulled from a SpaceX flight last year to make room for NASA’s two stuck astronauts, Boeing Starliner test pilots Butch Wilmore and Suni Williams, whose space station stay went from one week to more than nine months. Fincke and Yui had been training for the next Starliner mission. But with Starliner grounded by thruster and other problems until 2026, the two switched to SpaceX.

    Platonov was bumped from the Soyuz launch lineup a couple of years ago because of an undisclosed illness.

    Their arrival temporarily puts the space station population at 11.

    “It was such an unbelievably beautiful sight to see the space station come into our view for the first time,” Cardman said once on board.

    While their taxi flight was speedy by U.S. standards, the Russians hold the record for the fastest trip to the space station — a lightning-fast three hours.

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  • A Discovery That Could Rewrite Astronomy

    A Discovery That Could Rewrite Astronomy

    Astronomers have made a groundbreaking discovery that defies the conventional understanding of planetary formation in binary star systems. A planet orbiting in a retrograde direction—opposite to its binary stars’ movement—has been confirmed in the nu Octantis system. This discovery, published in Nature on May 21, 2025, challenges existing theories and opens new doors for studying planetary systems in tight binary star environments. The research was led by Professor Man Hoi Lee and his team from the University of Hong Kong, shedding light on how such a planet might have formed. A critical piece of the puzzle was the precise radial velocity data gathered using the European Southern Observatory’s HARPS spectrograph, which helped confirm the planet’s unusual orbit.

    The nu Octantis system, which is located about 2.9 billion years old, features two stars: nu Oct A, a subgiant roughly 1.6 times the mass of the Sun, and nu Oct B, which is about half the Sun’s mass. These stars orbit each other once every 1,050 days. Though evidence for a planet orbiting in this system was first noticed in 2004, it was only with recent high-precision observations that the team was able to firmly confirm the planet’s presence and its unusual retrograde orbit.

    The Strange Nature of Retrograde Orbits in Binary Systems

    In most planetary systems, planets tend to orbit in the same direction as their host stars’ motion. This is typically a product of the way these systems form, with the material surrounding the stars coalescing in the same direction. However, the nu Octantis planet’s retrograde orbit—one that moves in the opposite direction of the stars’ orbit—presents an anomaly that has puzzled scientists for years. Such planets are incredibly rare and theoretically difficult to form or maintain, particularly in binary star systems where the gravitational influence of both stars can make stable planetary orbits highly improbable.

    To confirm the retrograde nature of the orbit, the research team performed a thorough analysis of both archival and new radial velocity data, which tracks a star’s motion towards or away from Earth. These observations, collected over 18 years, confirmed that the planet’s orbit not only is retrograde but is also nearly aligned with the plane of the binary stars’ orbit. This discovery was further supported by additional high-precision data gathered using the HARPS spectrograph.

    The team’s work adds to a growing body of evidence suggesting that retrograde planets could be more common than previously thought, especially in systems with evolved stellar components like white dwarfs. In fact, the research raises the possibility that planets like the one in nu Octantis could offer a new window into the formation and evolution of planetary systems in a variety of cosmic environments.

    Unveiling the History of nu Octantis: A White Dwarf and a Unique Planet

    Understanding the full history of the nu Octantis system is essential to explaining the unusual planet’s existence. Nu Oct B, the system’s secondary star, has undergone significant evolution over billions of years. Originally, it had a mass about 2.4 times that of the Sun. However, it eventually evolved into a white dwarf after exhausting its nuclear fuel. As a result of this transformation, nu Oct B now has only about 25% of its original mass.

    The research team found that nu Oct B‘s transition into a white dwarf was likely responsible for the material surrounding it, which could have influenced the planet’s formation. One theory suggests that the planet might have formed from a retrograde disc of material expelled from nu Oct B as it transitioned to a white dwarf. Alternatively, the planet could have been captured from a prograde orbit into its current retrograde orbit around nu Oct A.

    In an effort to clarify the origins of the system, the team examined the initial configurations of the stars and their evolution over time. Their analysis suggested that the planet could not have formed around nu Oct A simultaneously with the stars. The evolution of nu Oct B and its transformation into a white dwarf played a key role in shaping the system’s current state. Ho Wan Cheng, the first author of the paper, explained: “We found that the system is about 2.9 billion years old and that nu Oct B was initially about 2.4 times the mass of the Sun and evolved to a white dwarf about 2 billion years ago. Our analysis showed that the planet could not have formed around nu Oct A at the same time as the stars.”

    A New Perspective on Second-Generation Planets

    This study introduces the fascinating possibility that the nu Octantis planet is a second-generation planet. Dr. Trifon Trifonov, a co-author of the study, suggests that the planet could have either been captured from a prograde orbit around the binary system or formed from material expelled by nu Oct B. In his words, “We might be witnessing the first compelling case of a second-generation planet; either captured, or formed from material expelled by nu Oct B, which lost more than 75% of its primordial mass to become a white dwarf.” This insight opens up new avenues for studying the evolution of planets, especially those formed in unusual circumstances or captured from other orbits.

    The discovery of retrograde planets challenges the traditional models of planetary formation. In a typical star system, planets are expected to move in the same direction as their host star, aligning with the general angular momentum of the system. The existence of a retrograde planet in such a tightly bound binary system could indicate that these systems are capable of fostering unique planetary environments, offering insights into planetary migration, capture, and secondary planetary formation.

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