Articles tagged with Asteroids
Texas A&M University is collaborating on a research project to track objects in high Earth orbits, expanding space domain awareness capabilities. The Space University Research Initiative aims to develop new technology and systems to monitor objects influenced by the moon's gravity.
Researchers found a rare pathway allowing a moon fragment to reach Earth's quasi-satellite orbit. The study suggests that many more lunar fragments remain to be discovered among the near-Earth asteroid population.
A new SwRI study posits that the large mounds on Kuiper Belt object Arrokoth are similar in size and shape, suggesting a common origin. This finding supports the streaming instability model of planetesimal formation, where gentle collision speeds allowed objects to accumulate and form Arrokoth.
A new modeling method powered by interconnected processors removed human bias from the debate over dinosaurs' demise. The study suggests that the outpouring of climate-altering gases from the Deccan Traps alone could have been sufficient to trigger global extinction, consistent with volcanic eruptions contributing to the mass extinction.
A team of researchers has successfully tested a new asteroid detection algorithm, HelioLinc3D, which identified its first 'potentially hazardous' asteroid, 2022 SF289. The discovery confirms the algorithm's effectiveness in finding near-Earth asteroids with fewer and more dispersed observations than traditional methods.
Princeton researchers used data from NASA's Parker Solar Probe to determine that a catastrophic event, such as a high-speed collision or gaseous explosion, likely created the Geminids meteoroid stream. This is in contrast to most meteor showers, which originate from comets emitting tails of ice and dust.
Researchers found tiny salt crystals in an asteroid sample, indicating the presence of liquid water. The discovery challenges previous assumptions that ordinary chondrite asteroids lack hydrated minerals.
A new study reveals that asteroid Dinkinesh is remarkably small, making it the smallest asteroid to be approached by Lucy. It is a stony, S-type asteroid composed mainly of silicates and some metal.
The telescope has imaged three nested belts extending up to 14 billion miles from the star, with inner belts revealed for the first time. The discovery provides insights into the structure of exoplanetary systems and the formation of planets.
NASA solar observatories have discovered that asteroid Phaethon's comet-like tail is not composed of dust, but rather sodium gas. The findings contradict previous theories and suggest a new explanation for Phaethon's behavior, which is the source of the annual Geminid meteor shower.
Scientists measured and compared amino acid abundances with rocky components of Ryugu particles, demonstrating water's role in their formation. The results suggest more ice was present in the precursor of one particle than the other, which may have contributed to the high abundance of a specific amino acid.
A team of astronomers discovered a population of reddish Neptunian asteroids, which are thought to have formed beyond the transition boundary between neutral-colored and redder objects. The red coloration suggests these asteroids contain more volatile ices, providing insight into the early Solar System's conditions.
Researchers attribute unusual radar properties to coherent backscatter opposition effect (CBOE) and ice surface irregularities. The CBOE model, improved by Hofgartner and Hand, can explain all icy satellite radar properties.
Researchers Jennifer Bergner and Darryl Seligman suggest that 'Oumuamua's acceleration can be explained by the outgassing of hydrogen gas as the comet warmed up in the sunlight. The comet's small size allowed for a significant effect, with the tiny push from hydrogen spurted out of ice altering its gravitational deflection around the sun.
Researchers suggest studying well-preserved grains of space dust for potential signs of life, as they could contain fossils of microorganisms. The idea estimates that around 100,000 such grains could land on Earth every year.
Scientists have detected uracil and nicotinic acid in asteroid Ryugu samples collected by the Hayabusa2 spacecraft. The discovery suggests that important building blocks for life were created in space and delivered to Earth via meteorites, supporting current theories on the source of nucleobases.
The ESO VLT observed the aftermath of the DART impact, showing that the ejected cloud was bluer than the asteroid itself, indicating fine particles. The team found no signs of ice or DART spacecraft propellant, but detected changes in light polarization suggesting altered surface composition.
The DART mission observed a 33-minute change in the orbit of Dimorphos, indicating that ejecta escaped the system and contributed to the orbital changes. The team will use this data to understand how the entire system's orbit changes over time.
The DART mission successfully deflected the orbit of asteroid Dimorphos by 33 minutes. The team's calculations showed that the momentum transferred to Dimorphos was significantly enhanced by the recoil created from streams of particles produced by the impact, exceeding initial expectations.
The DART mission successfully demonstrates the feasibility of redirecting near-Earth objects like asteroids to prevent large-scale destruction. The spacecraft's impact on Dimorphos, a small asteroid moon, resulted in an orbital change that confirms the viability of asteroid deflection as a planetary defense strategy.
Citizen scientists from Unistellar network observe and analyze NASA's DART impact, supporting the efficiency of kinetic impactor technique to deflect asteroids. The study confirms the success of planetary defense methods, making significant contributions to humanity's quest to understand the universe.
The Politecnico di Milano has successfully contributed to the DART mission, a historic planetary defense test that deflected an asteroid's trajectory. The mission's scientific results reveal the effectiveness of kinetic impact technology in planetary defense and provide insights into the structure and evolution of binary asteroids.
The Hubble movie reveals surprising hour-by-hour changes as dust and chunks of debris were flung into space. The dynamic interaction within the binary system starts to distort the ejecta pattern, forming rotating pinwheel-shaped features tied to the gravitational pull of Didymos.
Researchers at Tohoku University analyzed samples from Japan's Hayabusa2 spacecraft and identified what they believe may be the oldest solids from the solar system. The grains were likely transported outward from the inner regions of the early solar system to their current location in the outer reaches.
A team from Heidelberg University discovered a new class of asteroids rich in water, similar to dwarf planet Ceres. The small bodies are thought to have formed in a cold region at the edge of the Solar System before being impacted by gravitational disruptions.
Scientists at the University of Jena have solved a decades-long puzzle by studying quartz samples under extreme pressure. They discovered that characteristic lamellae, which are often used to detect asteroid impacts, form when quartz transforms into a more tightly packed phase under high pressure.
Researchers at Imperial College London found that around half of Earth's zinc inventory came from asteroids in the outer Solar System, contributing to the emergence of life on Earth. The study suggests that this material supplied other important volatiles like water, crucial for sustaining life.
Researchers discovered that asteroid Itokawa is resistant to collision and has survived for nearly 4.2 billion years due to its rubble pile composition. This finding could lead to more effective defense strategies against potentially hazardous asteroids, including the use of nuclear blasts to nudge them off course.
Researchers analyzing Ryugu asteroid samples found minerals produced through water reactions over 4.5 billion years ago, providing insight into the solar system's infancy. The discovery sheds light on asteroid accretion and the formation of planets like Earth.
An international team of scientists suggests that an outward, fast migration of Jupiter can distort the configuration of Trojan swarms, resulting in more stable orbits in one swarm than the other. This new mechanism provides a natural explanation for the observed asymmetry in the number of asteroids in the L4 and L5 swarms.
Scientists at NASA's Goddard Space Flight Center simulated the formation of amino acids and amines in laboratory conditions, similar to those found in interstellar clouds. The results suggest that these precursors to life can survive their journey to asteroids and potentially form the basis of life on Earth.
Researchers recreated interstellar cloud and asteroid conditions to understand how carbonaceous chondrites acquired amino acids, finding that interstellar cloud conditions are resilient to asteroid processing but influence the amount of amino acids present.
Researchers studied asteroid Ryugu's surface composition using X-ray Absorption Near Edge Spectroscopy and electron microscopy. They found dehydrated serpentine minerals and a water-rich interior, suggesting space weathering plays a key role in asteroid evolution.
A new study suggests that comet impacts can transport oxidants from Europa's surface to its ocean, increasing the probability of finding life. The research model shows that if an impact reaches halfway through the moon's icy shell, meltwater sinks to the ocean, bringing critical chemicals.
New research on asteroid samples from Ryugu reveals similarities to Ivuna-like carbonaceous chondrites, providing a better understanding of the early solar system. The study also sheds light on the accretion of volatiles during planetary formation and finds that Ryugu-like material accounts for ~5-6% of Earth's mass.
Researchers developed a new lidar technique using 3D flash lidar combined with super-resolution algorithm for hazard avoidance during landing. The technique improved the precision and safety of robotic vehicles on Mars, enabling them to navigate through challenging environments.
A Martian megatsunami was likely triggered by an asteroid collision similar to the Chicxulub impact that led to mass extinctions on Earth. The crater formed as a result of this impact may have caused a tsunami that reached over 1,500 kilometres from the center, measuring up to 250 meters tall on land.
A study published in Nature Communications suggests that small asteroids are probably young because of their loose internal structure and low cohesion. This finding has important implications for understanding the geological development of asteroids.
A recent study from the University of Copenhagen reveals that Mars was once covered in a 300-metre-deep ocean, filled with water and icy asteroids carrying biologically important molecules. This finding suggests that conditions allowing the emergence of life were present on Mars long before Earth.
Researchers from Osaka University have successfully detected carbon, nitrogen, and oxygen in samples from near-Earth asteroid Ryugu using muon non-destructive analysis. The findings suggest that CI chondrites may be contaminated with terrestrial materials, challenging previous understanding of the solar system's chemical compositions.
The SwRI experiment helped predict the effects of NASA's DART impact on asteroid Dimorphos. The study assessed ejecta momentum enhancement created by the space probe's collision, measuring a 3.4-fold increase in momentum transfer.
An international team has discovered three near-Earth asteroids, including one that is 1.5 kilometers wide and may someday threaten Earth's path. The observations were made possible by the unique capabilities of the Dark Energy Camera mounted on the Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory.
The study includes 191 asteroids' radar cross sections and Doppler-frequency broadening, offering clues to asteroids' spin periods and sizes. The research also discovered two metal-rich near-Earth asteroids and five possible enstatite-rich asteroids, shedding new light on the formation and evolution of the solar system.
Researchers have developed a method to map an asteroid's interior structure based on its spin changes during close encounters with Earth. This technique, called AIME, could help scientists plan more effective defense strategies for asteroids like Apophis, which poses a significant hazard if it were to make impact.
A new surveillance constellation concept aims to detect and track near-Earth asteroids, providing early warning and tracking capabilities. The system consists of six space-based surveyors and a mothership, which work together to monitor the orbits of potentially hazardous asteroids.
Researchers have identified a potential source of shock-darkened meteorites, which could explain discrepancies in how near-Earth asteroids are classified. The asteroid, 1998 OR2, is about 1.5 miles wide and shows characteristics that suggest it has undergone shock darkening.
A Curtin-led research team found asteroid impacts on the Moon millions of years ago coincide with large meteorite impacts on Earth, such as the one that wiped out dinosaurs. The study also reveals that major impact events on Earth were accompanied by smaller impacts, providing new insights into asteroid dynamics.
Scientists from the University of Rochester have provided a more accurate simulation of the impact that formed Earth’s largest crater two billion years ago. The new research suggests the impactor was much larger, about 20 to 25 kilometers in diameter, and traveling at a velocity of 15 to 20 kilometers per second.
Researchers used the Advanced Photon Source to study asteroid fragments from Ryugu, finding they were made of water and carbon dioxide ice. The analysis suggests the asteroid formed over 4 billion years ago in the outer solar system, with a hydrated interior and dryer surface.
Researchers used muon beams to analyze Asteroid Ryugu samples, finding essential elements like carbon, nitrogen, and oxygen. However, the oxygen abundance relative to silicon was 25% less than expected, suggesting contamination after atmospheric entry.
Julie Castillo-Rogez and Martin Jutzi have made significant contributions to understanding asteroids, including their origins and dynamical evolution. Their work has advanced our knowledge of asteroids, from small bodies to planetary scales, with implications for ongoing space missions.
Researchers located four new craters created by impacts on Mars' surface using data from a seismometer and visuals acquired from the Mars Reconnaissance Orbiter. This is the first time that researchers have captured the dynamics of an impact on Mars.
A new study suggests that massive volcanic eruptions were the primary cause of mass extinctions, including the one that wiped out the dinosaurs. The research found a strong temporal connection between flood basalt eruptions and significant climatic events.
Scientists have developed a new method to distinguish between normal land structures and small asteroid craters by analyzing charcoal samples, revealing 30% of impact sites remain unlocated. The study found unique characteristics in impact charcoals that differ from wildfire charcoals.
Researchers found compact fragments in the Aguas Zarcas meteorite that wouldn't break apart, leading to CT scans revealing deformed rocks with the same orientation. The team proposed a hypothesis that asteroids 'spit out' pebbles due to high-speed collisions and thermal cycling, which can cause rock brittleness.
Research on asteroid 2008 TC3 reveals that larger meteorites survived to the ground, contradicting previous assumptions about interior shielding. The study's findings provide new insights into asteroid fragmentation and the origins of space rocks.
A NASA scientist will lead a team in characterizing and understanding Potentially Hazardous Asteroids (PHAs) with a $848,013 grant. The project aims to predict PHA close approaches and issue warnings to prevent asteroid impacts.
A global team led by researchers from Curtin University used a supercomputer-powered technology to explore the geology of Mars without leaving home. They found that the ancient Martian meteorite NWA 7034 was ejected 5-10 million years ago from the north-east of the Terra Cimmeria - Sirenum province, in the southern hemisphere of Mars.
Asteroids like Bennu and Ryugu appear rough due to the loss of fine-grained regolith caused by tiny space dust grains hopping around on their surfaces. This process may help small asteroids migrate faster through space, affecting their orbits.
Asteroid Bennu's surface is characterized as loosely bound, with a near-subsurface layer composed of weakly bound rock fragments containing twice the void space as the overall asteroid. The study provides new insights into the physical properties of rubble-pile asteroids, with implications for their long-term evolution.