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The pursuit of understanding dark matter, which comprises 85 percent of the universe’s mass, could take a significant leap forward with a nearby supernova. Researchers at the University of California, Berkeley, led by Associate Professor of Physics Benjamin Safdi, have theorised that the elusive particle known as the axion might be detected within moments of gamma rays being emitted from such an event. Axions, predicted to emerge during the collapse of a massive star’s core into a neutron star, could transform into gamma rays in the presence of intense magnetic fields, offering a potential breakthrough in physics.

Potential Role of Gamma-Ray Telescopes

The study was published in Physical Review Letters and revealed that the gamma rays produced from axions could confirm the particle’s mass and properties if detected. The Fermi Gamma-ray Space Telescope, currently the only gamma-ray observatory in orbit, would need to be pointed directly at the supernova, with the likelihood of this alignment estimated at only 10 percent. A detection would revolutionise dark matter research, while the absence of gamma rays would constrain the range of axion masses, rendering many existing dark matter experiments redundant.

Challenges in Catching the Event

For detection, the supernova must occur within the Milky Way or its satellite galaxies—an event averaging once every few decades. The last such occurrence, supernova 1987A, lacked sensitive enough gamma-ray equipment. Safdi emphasised the need for preparedness, proposing a constellation of satellites, named GALAXIS, to ensure 24/7 sky coverage.

Axion’s Theoretical Importance

The axion, supported by theories like quantum chromodynamics (QCD) and string theory, bridges gaps in physics, potentially linking gravity with quantum mechanics. Unlike neutrinos, axions could convert into photons in strong magnetic fields, providing unique signals. Laboratory experiments like ABRACADABRA and ALPHA are also probing for axions, but their sensitivity is limited compared to the scenario of a nearby supernova. Safdi expressed urgency, noting that missing such an event could delay axion detection by decades, underscoring the high stakes of this astrophysical endeavour.

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Oak Trees: A Journey Through Time, From Fossils to the Forests We Know

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Oak Trees: A Journey Through Time, From Fossils to the Forests We Know

Rising global temperatures and shifting tectonic plates are believed to have shaped the development of one of Earth’s most iconic trees, the oak (Quercus). According to reports, the Paleocene-Eocene Thermal Maximum (PETM), a significant climatic event approximately 56 million years ago, created extreme conditions that influenced the evolution of diverse plant species, including the ancestors of modern oaks. This event occurred during a time of volcanic activity that released massive amounts of carbon into the atmosphere, leading to an average temperature increase of 8 degrees Celsius globally.

The Impact of the PETM on Early Ecosystems

It has been documented that the PETM caused dramatic changes in both terrestrial and marine ecosystems. According to sources, tropical forests expanded across South America, while plant and animal species migrated vast distances in response to rising temperatures. The fossil record suggests that during this period, the ancestors of today’s oaks began to emerge, though evidence such as acorns and pollen remains sparse.

First Oak Fossils Discovered in Austria

Fossilised oak pollen was first identified in Oberndorf, Austria, near the site of the Church of Saint Pankraz. Reports indicate that this discovery provides the earliest evidence of oaks dating back to the PETM. The surrounding forests, a mosaic of subtropical and temperate species, were home to plants that later contributed to modern biodiversity.

The Evolutionary Split of Oaks

As the Atlantic Ocean widened, dividing North America and Europe, reports suggest that the ancestral oak population split into two major lineages. One evolved in the Americas, while the other adapted to regions in Eurasia and North Africa. This separation is attributed to tectonic activity and natural barriers, which likely played a critical role in the diversification of oak species. The history of oaks exemplifies the gradual process of evolution driven by environmental factors, with their legacy continuing into today’s temperate forests.

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NASA’s Parker Solar Probe Achieves Closest Sun Flyby Ever on December 24

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NASA’s Parker Solar Probe Achieves Closest Sun Flyby Ever on December 24

NASA’s Parker Solar Probe is set to perform its closest flyby of the sun on December 24, 2024, at 6:53 a.m. EST. The spacecraft, which launched in 2018, will approach within 3.8 million miles (6.1 million kilometres) of the solar surface, setting a record for the nearest distance a human-made object has travelled to a star. Travelling at an extraordinary speed of 430,000 mph (692,000 kph), the probe will traverse the sun’s corona, collecting data on its high-temperature environment.

Mission Details and Flyby Preparations

The Parker Solar Probe, managed by NASA and designed at the Johns Hopkins Applied Physics Laboratory (JHUAPL), has completed 21 previous solar encounters and seven flybys of Venus, as per a report by Parker Solar Space. The upcoming event marks the 22nd solar approach in its mission to deepen the understanding of the sun’s outer atmosphere. According to Nick Pinkine, mission operations manager at JHUAPL, the probe will provide unprecedented data from regions no spacecraft has explored before.

As part of its preparations, the probe sent a final transmission to Earth on December 20, signalling all systems are functioning normally, according to reports. Contact with the spacecraft will remain offline until December 27, when it is expected to send a health status update. Comprehensive science data, including telemetry, will begin to arrive in January 2025, as per reports.

Engineering to Withstand Extreme Temperatures

During the flyby, the spacecraft will endure temperatures reaching 1,800 degrees Fahrenheit (980 degrees Celsius). Its advanced heat shield, constructed from carbon foam, ensures the probe’s instruments remain at near room temperature while withstanding up to 1,377 degrees Celsius.

Future of the Mission

As per reports, two additional close solar flybys are planned for March 22 and June 19, 2025. Decisions regarding the spacecraft’s trajectory and continued operations are expected after the primary mission concludes. The Parker Solar Probe’s findings aim to address critical questions about the sun’s behaviour, contributing to the broader understanding of solar phenomena.

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NASA’s discovery of a sideways black hole in NGC 5084 raises questions

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NASA's discovery of a sideways black hole in NGC 5084 raises questions

In findings shared through The Astrophysical Journal, NASA scientists have uncovered an extraordinary black hole in galaxy NGC 5084. Located around 80 million light-years away in the constellation Virgo, the black hole has been observed lying at a 90-degree tilt relative to the galactic plane. Using archival data from the Chandra X-ray Observatory and imagery from the Hubble Space Telescope, the research team identified twin plasma plumes forming a striking “X” shape, an unprecedented phenomenon in astronomical observations, as per reports.

Unusual Discovery Sparks Investigation

The discovery was attributed to a novel image analysis method, known as Selective Amplification of Ultra Noisy Astronomical Signal (SAUNAS), enabling researchers to detect faint X-ray emissions. The study team noted this departure from the typical spherical distribution of X-rays, indicating a significant and previously undetected event in the galaxy’s history.

Dr Pamela Marcum, an astrophysicist at NASA’s Ames Research Center, explained in a statement, that the unusual cross-shaped structure of the X-ray plumes, coupled with the tilted dusty disk, provides unique insights into the galaxy’s past.

A Cosmic Collision Hypothesised

Further analysis through the Atacama Large Millimeter/submillimeter Array (ALMA) confirmed the presence of a dusty ring at the galactic core, rotated in alignment with the black hole’s tilt. The alignment and structural anomalies suggest that NGC 5084 may have experienced a collision with another galaxy, generating plasma outflows above and below its plane.

Dr Alejandro Serrano Borlaff, also from Ames Research Center, stated that the combination of observations across multiple wavelengths revealed the dynamic and transformative events that have shaped this galaxy.

This discovery underscores the potential of archived data, dating back decades, when combined with modern processing techniques. Researchers anticipate that ongoing studies will unravel more details about the violent event that altered NGC 5084’s structure and orientation.

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