A new study led by University of Southampton researchers suggests that ocean acidification may not have caused the mass extinction of ammonites and other planktonic calcifiers. The research found that the asteroid impact was the primary cause of the extinctions, but not due to ocean acidification levels being too weak.
New research published by the University of Warwick finds evidence that water-rich asteroids or comets are common around other stars than the Sun. The study suggests that water can be delivered to planets like Earth via these bodies, potentially creating a suitable environment for life to form.
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Asteroids formed by capturing millimeter-sized chondrules with gravitational force, which then accumulated like sand in a storm. This process could also explain the formation of protoplanets and terrestrial planets, including Earth.
Scientists have found a record of the ancient Moon-forming giant impact observable in stony meteorites. The team used data analysis and numerical modeling work to infer the Moon formed about 4.47 billion years ago.
A NASA-funded SwRI-led research team independently estimated the Moon's age as 4.47 billion years based on shock signatures found in stony meteorites originating from the Main Asteroid Belt. This study provides insights into the last stages of planet formation in the inner solar system.
Researchers from CSIC have determined the orbit of Annama, a new characterized meteorite, and found similarities with a potentially dangerous asteroid. The study suggests that Annama may be linked to an asteroid of about 400 meters in diameter, posing a potential threat to Earth.
A team of scientists plans to take core samples from the Chicxulub impact crater, 65.5 million years old and associated with the mass extinction event that wiped out dinosaurs. The expedition will aim to uncover details about the impact and shed light on the mechanisms of large impacts on Earth and other rocky planets.
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A research team at the University of Arizona has discovered sulfide chondrules in meteorites, providing evidence for a new type of environment in the early solar system. The discovery sheds light on the formation of elements essential for life, such as carbon and oxygen.
Researchers have discovered tiny magnetic particles in meteorites that retain a faithful record of the magnetic fields generated by their parent bodies. By analyzing these particles, scientists were able to reconstruct the history of magnetic activity on the meteorite parent body and capture the moment when the core finished solidifying.
Researchers capture asteroid magnetic field moments, revealing extended lifetimes and creating mechanisms similar to the Earth's own magnetic field. Ancient meteorites provide a cosmic archaeological mission, shedding light on the magnetic history of asteroids and their impact on the Earth's core future.
A team of scientists found that collisions helped transform initially porous materials into solid asteroids and meteorites by absorbing energy in the porous matrix. This process likely occurred due to electrostatics and shock waves generated by high-velocity collisions, resulting in a cosmic speed limit for colliding objects.
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Research suggests asteroid material originated from impacts between embryo planets, resolving long-standing mystery of chondrule formation. Chondrules are abundant in meteorites and similar to spherules formed by impact on Earth and moon.
A new study reveals that dinosaurs remained diverse in European ecosystems until the end of the Cretaceous period. Fossils from Spain, France, and other countries show that meat-eating and plant-eating species were present and thriving during the final few hundred thousand years before the asteroid impact.
Scientists at the University of Nottingham used magnetic levitation to manufacture wax models of tektites, which are tiny glass objects formed by asteroid impacts. The research validates numerical models of spinning droplets and provides new information on tektite formation.
A recent study reveals that many metatherian mammals, including marsupials like opossums, nearly went extinct alongside the dinosaurs. This allowed advanced placental mammals to rise to dominance and become ubiquitous across the globe today.
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Scientists created a global geologic and tectonic map of asteroid Vesta, revealing a history of large impacts from massive meteorites. The oldest surviving crust predates the largest impact event, the Veneneia impact, which occurred around 2.1 billion years ago.
Researchers have discovered an unexpected tail on asteroid 62412, which was previously known as a typical asteroid. The discovery reveals that there may be up to 100 active asteroids in the main asteroid belt, shedding light on the processes that cause some asteroids to become active.
Asteroid Patroclus-Menoetius has been found to have a non-spherical shape, with axial ratios indicating a mostly oblate shape. The team's analysis also revealed the asteroid pair's spins were faster when they formed, currently in a doubly synchronous state.
Researchers used super high-speed cannon to simulate collisions on celestial bodies. They found that damage from the impact starts where one would expect, but fails in opposite direction and propagates outward like a blooming flower. The study suggests Vesta's 'belt' formed by an oblique impact.
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Researchers from MIT and other institutions found the Procellarum region on the moon's near side was formed by a large plume of magma deep within the moon's interior. The angular outline of the basin could not have been created by an asteroid impact, according to the team.
NASA's Asteroid Initiative aims to protect Earth from potentially hazardous impacts. Citizens participate in forums to discuss detection strategies, planetary defense, and asteroid exploration. The initiative seeks to balance costs, risks, and benefits of human exploration in space.
Researchers at the University of Tennessee discovered that near-Earth asteroid 1950 DA is held together by van der Waals forces, which defy traditional assumptions about asteroid composition. This finding has implications for defending against massive asteroid impacts and may inform strategies for space exploration.
A Curtin University study of a WA meteorite has shed light on the solar system's bombardment history, revealing that asteroid collisions ceased after 3.4 billion years ago due to asteroids being too small or protected by regolith. The research suggests that impacts stopped occurring after this period and remain unchanged until now.
Asteroid impacts were a key factor in shaping early Earth's surface, with large collisions melting and burying the crust. The Hadean eon's geography was heavily reprocessed, with impact-generated melt contributing to the formation of the Moon.
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Research suggests that giant asteroid impacts significantly altered the early Earth, mixing and melting its surface. The findings provide new insights into the role of asteroid bombardments in shaping the Hadean Earth's surface.
A new study suggests that dinosaurs' demise was partly due to the perfect storm of environmental upheaval, including volcanic activity, changing sea levels, and varying temperatures. This weakened their food chain, making them vulnerable to extinction.
Leaf-mining insects completely disappeared after the dinosaur extinction event, only to reappear a million years later with diverse damage patterns. The researchers found nine different mine-damage types at Mexican Hat attributable to moths, wasps, and flies, suggesting an influx of novel insect herbivores during the early Paleocene.
Researchers have redefined the asteroid Vesta's internal structure based on Dawn data and simulations, questioning previous models of rocky planet formation. The study found that Vesta's crust is 3 times thicker than expected and lacks olivine, a mineral common in planetary mantles.
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A NASA model can predict and visualize the interaction between solar wind, solar radiation, and asteroid surfaces in unprecedented detail. The model adapts to complex activities and provides highly efficient simulations, potentially identifying hazards for human explorers.
Researchers David Trilling and Michael Mommert found asteroid 2011 MD to be 65% empty, consisting of a cloud of rocks or dust with a solid rock at its nucleus. This challenges long-held assumptions about the nature of small asteroids.
A new analysis by NASA-funded researchers suggests that vitamin B3 could have originated from carbon-rich meteorites. The team found high levels of vitamin B3 and related molecules in eight different meteorites, which support the theory that extraterrestrial sources may have assisted the origin of life.
The OSIRIS-REx mission aims to find answers about the early solar system and organic materials that made life possible. The spacecraft will collect at least 2 ounces of asteroid samples and return them to Earth for scientists to study.
A French, American team of researchers has discovered that the regolith of small asteroids is formed by thermal fatigue, a process caused by temperature cycling. This finding challenges previous theories that suggested impacts and micrometeoroid impacts were responsible for creating the asteroid's surface.
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Asteroid P/2013 R3 broke apart into 10 smaller pieces as it approached the sun, with fragments drifting away at a leisurely pace. Scientists believe the asteroid's weak interior and gradual rotation rate may be responsible for its disintegration.
Astronomers have witnessed the first-ever breakup of an asteroid into as many as 10 smaller pieces using NASA's Hubble Space Telescope. The discovery suggests that sunlight may be responsible for this type of disintegration, which is a subtle effect known as YORP torque.
The Hubble Space Telescope has photographed an asteroid, P/2013 R3, breaking apart into as many as ten smaller pieces. The fragments are drifting away from each other at a leisurely 1.5 kilometers per hour, likely due to the Yarkovsky-O'Keefe-Radzievskii-Paddack effect.
Researchers found a massive asteroid around PSR J0738-4042, which is being pounded by asteroids and could form planets. The asteroid's mass is about a billion tonnes, and its formation is linked to the star's intense radiation.
A new asteroid map reveals that rogue asteroids, once considered anomalous, are actually diverse and widespread throughout the main asteroid belt. The study suggests that the early solar system underwent dramatic changes, potentially affecting planetary migration and Earth's water development.
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The asteroid belt's diverse composition suggests that giant planets' migrations reshaped the solar system, potentially delivering water to Earth and influencing its habitability. Small asteroids show particularly varied compositions, suggesting a complex history of collisions and re-deposition.
Students used a privately owned telescope to observe and photograph asteroids 3905 Doppler, orbiting two smaller rocky bodies that block each other's light. The discovery provides an unprecedented opportunity to learn about the physical properties and orbital evolution of these objects.
NASA's Goddard Space Flight Center researchers are part of a new virtual institute focusing on space science and human exploration. They will apply models to understand plasma interactions with asteroids, small bodies, and the effects of solar wind and radiation.
Scientists have found that Mars can also stir up asteroid surfaces, refreshing them over time. The research suggests that the Red Planet plays a key role in altering the chemical nature of asteroids' surfaces, changing their reddish hue.
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Astronomers using the Hubble Space Telescope have observed a unique asteroid with six comet-like tails, challenging current understanding of asteroids and comets. The asteroid's rotation rate may have caused its surface to fly apart, ejecting dust into space.
Astronomers have discovered an unusual asteroid with six comet-like tails, which change dramatically over just 13 days. The object's rotation rate may be causing its surface to fly apart, ejecting dust in episodic eruptions.
Astronomers have observed an asteroid, P/2013 P5, spouting six comet-like tails of dust, defying the typical appearance of asteroids. The unusual tail structures change dramatically in just 13 days, sparking debate over their origin and suggesting a possible rotational breakup.
The Chelyabinsk meteorite was analyzed by an international team of researchers, revealing its composition and origin. The study found that the meteoroid entered Earth's atmosphere at 19 km/s and broke up 30 kilometers above ground, causing widespread damage.
The SwRI-led ISET team will study the origin, evolution, and physical properties of near-Earth asteroids and their moons, aiming to better understand their potential for cost-effective human exploration. The research will also investigate minimoons, small bodies with the potential to provide insights into the history of the Solar System.
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Astronomers found a water-rich asteroid orbiting an exhausted star, indicating the presence of Earth-like exoplanets. The discovery suggests that the star GD 61 had the potential to contain habitable planets, with water and rocky surfaces being key ingredients.
A Northern Arizona University-led team used the Spitzer Space Telescope to detect cometary activity in asteroid (3552) Don Quixote, a near-Earth object that was previously thought to be dead. The discovery suggests that water and carbon dioxide ice deposits may still exist on other near-Earth asteroids.
A University of Tennessee professor helped discover that a near-Earth object is actually a comet, not an asteroid. The body, 3552 Don Quixote, contains water ice and has a coma and tail, suggesting it may be the source of Earth's water.
The OSIRIS-REx mission will study asteroid Bennu in detail before returning with a sample of material from its surface. The spacecraft will map the asteroid's composition from orbit using spectrometers to identify key elements like water, metals, and organic carbon.
Dolores H. Hill, a NASA scientist, has been selected by the White House as a Citizen Science Champion of Change for her work on the Target Asteroids project. The project aims to engage amateur astronomers in tracking near-Earth objects and improve our understanding of asteroids.
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A Purdue University-led team has mapped the location and development of mass concentrations, or mascons, on the lunar surface, resolving a decades-long mystery. The findings provide valuable insights into the moon's origin and evolution and will aid in navigating future lunar missions.
Astronomers have found signs of rocky material in the atmospheres of two dead stars, suggesting that terrestrial planets may still exist. The debris detected around these white dwarfs is thought to be the remains of asteroids that were shredded by the star's gravity.
Researchers have found evidence of building blocks for Earth-sized planets in the atmospheres of two burned-out stars called white dwarfs. The silicon and low levels of carbon in these dead stars suggest that asteroid-like debris is falling onto them, potentially creating rocky planet assembly around stars.
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Researchers have devised a way to detect and track asteroid collisions in interplanetary space using a new method to measure the mass of magnetic clouds created by impacts. This technique could help scientists better understand where to find new meteoroid debris that poses a threat.
Researchers found lower than expected levels of iridium and osmium at the K-Pg boundary, contradicting the asteroid impact theory. A comet explanation reconciles this with evidence of a massive crater.
Researchers found a new class of dust motion on the moon, where charged particles swarm like bees around partially shaded regions. This phenomenon creates oscillations over 1-10 meter-sized shaded regions, with dust bouncing back and forth between sunlit areas.
Iowa State University engineers are working on a $500 million test launch of an asteroid intercept system, which could use nuclear devices to break apart incoming asteroids. The system, developed by Bong Wie's Asteroid Deflection Research Center, has the potential to save Earth from devastating asteroid impacts.
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The University of Calgary has launched a satellite to track near-Earth asteroids, enabling researchers to study these rare and difficult-to-detect objects. The NEOSSat satellite will enable scientists to take hundreds of sensitive images daily to search for moving dots of light that represent asteroids.