Articles tagged with Comets
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Comets are analyzed using Swift's Ultraviolet/Optical Telescope, which separates wavelengths of ultraviolet light to study gases surrounding the icy bodies. Cometary X-ray emission is also detected, providing insights into the process of charge exchange between solar ions and comet gases.
Comet Lulin is releasing a great amount of gas, making it an ideal target for X-ray observations. Swift's UVOT detects hydroxyl molecules, revealing a cloud spanning nearly 250,000 miles, while the XRT sees X-rays from the comet's atomic cloud.
Swift's Ultraviolet/Optical Telescope (UVOT) observes the chemical composition of comet atmospheres, while its X-Ray Telescope (XRT) studies gas and solar wind interactions. This research offers clues about comets' origins and the solar system.
Comet particles from Wild 2 provide a glimpse of the solar system's early convulsions, flinging primordial material out into the cold regions. The particles contain minerals formed at high temperatures, suggesting transport from the inner to outer solar system.
Researchers analyzed oxygen isotope compositions of comet Wild 2's halo crystals, finding signatures similar to asteroids and the sun. This suggests heat-processed particles were transported outward in the young solar system, complicating theories on its early history.
A combination treatment with methotrexate and etanercept improves remission rates by 50% and radiographic non-progression by 21% compared to methotrexate alone. The treatment also increases the ability of patients to remain in employment, with significant implications for employers and society.
A Cardiff University study suggests that the sun's movement through the Milky Way causes comets to collide with Earth every 35-40 million years, coinciding with mass extinctions like the dinosaurs' extinction. This cosmic 'bounce' effect may also have helped life spread by dispersing micro-organisms into space.
New research reveals that comet Wild 2's sample is missing ingredients expected in cometary IDPs and resembles chondritic meteorites from the asteroid belt. The high-speed capture of Stardust particles may have altered the material.
The analysis of noble gases in Stardust samples indicates that some particles match a special type of carbonaceous material found in meteorites and must have spent time near the sun. The study suggests an alternative mechanism for grain incorporation into comets, contradicting earlier formation theories.
A University of Minnesota physicist analyzed comet Wild-2 dust, finding it formed close to the infant sun and bombarded by intense radiation before being flung out. The discovery sheds light on the solar system's early stages and potential impact on Earth's atmosphere.
The Deep Impact spacecraft is using its flyby of Earth to calibrate its instruments for the EPOXI mission, which will study comet Hartley 2. The team made observations of the moon to test the spacecraft's pointing and commanding systems.
The EPOXI mission will use the Deep Impact spacecraft to search for Earth-sized planets around five stars and conduct an extended flyby of Comet Hartley 2, studying its surface and composition. This new mission aims to better understand how solar systems form and evolve.
A narrow belt of moonlets as large as football stadiums has been discovered in Saturn's outermost ring, likely resulting from a larger moon being shattered by an asteroid or comet. The discovery supports the theory that Saturn's rings were initially created through a collisional cascade.
Scientists at NRL capture first images of a comet colliding with a solar hurricane, revealing the detachment of the comet's tail due to coronal mass ejection. The event is triggered by magnetic reconnection, releasing energy and detaching the plasma tail.
A NASA satellite has captured the first-ever images of a comet's plasma tail detaching from Encke's comet due to a coronal mass ejection. The event was triggered by magnetic reconnection between the comet's and solar wind fields, releasing a burst of energy that detached the tail.
A team of international researchers suggests that a comet or low-density object caused the mass extinctions at the end of the Ice Age, proposing a 'mini nuclear winter' triggered by a 10-million-megaton detonation. This impact would have destabilized a vast ice sheet, leading to rapid cooling and subsequent climate change.
Scientists at Brown University propose that an asteroid impact triggered catastrophic climate change, leading to the mass extinction of megafauna such as wooly mammoths. The theory is based on evidence of nanodiamonds and other extraterrestrial particles found in sediment samples from archeological sites.
New findings from comet probes confirm the existence of organic molecules and clay particles that could have formed early life. The Cardiff University team argues that comets' liquid interiors provide a suitable environment for life's emergence.
Researchers analyze comet Wild 2 samples, finding evidence of material formed at both cold and hot temperatures, and unusual organic molecules with oxygen and nitrogen content. The discovery raises questions about how these fragile materials survived capture and formed in the early solar system.
Researchers analyze cometary material from Stardust spacecraft, improving understanding of early solar system chemistry and mixing. ESRF's X-ray beams help determine element distribution without damaging particles.
Researchers at Washington University in St. Louis analyze comet samples and discover a unique result: the presence of 'real' stardust particles older than the sun. This finding provides key insights into the composition and origin of comets, shedding light on their role in the solar system's formation.
Researchers analyzed dust fragments from Comet Wild-2 to gain insights into the early Solar System's formation. The study found diverse mineral compositions in the comet dust, indicating extensive mixing before planet formation, and evidence of surprising variety in cometary composition.
The analysis of Stardust particles from comet Wild 2 has revealed clues about the birth of our solar system, challenging some basic theories. The particles contain osbornite, a mineral that forms at high temperatures, indicating a volatile and dynamic environment during the solar system's infancy.
Scientists have discovered material in comets that originated from the sun's inner solar system, defying a popular notion. The Stardust mission found particles with extreme properties, including one made of calcium-aluminum inclusion and another composed of magnesium olivine.
Researchers at UC Berkeley have developed techniques to pluck comet dust from the aerogel collectors used by NASA's Stardust spacecraft. The extracted samples reveal a diverse and unexpected composition of materials, including calcium/aluminum-rich inclusions similar to those found in meteorites.
Researchers at UC Davis are developing a virtual library of data from hundreds of environmental sensors to study the interconnectedness of air, water, land, and living things in California. This 'God's-eye view' will help understand how climate change affects the state, including precipitation patterns, wildfires, and ocean upwelling.
Researchers from the University of Michigan and Harvard-Smithsonian Center for Astrophysics discovered atomic nitrogen in interstellar gas clouds, suggesting pre-life molecules may be present in comets. This finding sheds new light on the early conditions that led to life on Earth.
Researchers have discovered a surprising amount of carbon in the gas surrounding a young star, Beta Pictoris. The findings may indicate that asteroids and comets in this system could contain large amounts of organic material, which could have delivered building blocks of life to early Earth.
Research on grape seed extract's potential to lower blood pressure, discovery of new elements, and studies on prostate cancer were among the topics presented at the ACS meeting. The conference also featured discussions on improving America's scientific competitiveness and food safety.
Researchers are analyzing Stardust samples to study the structure and chemistry of cometary material, providing clues about the solar system's history. The team is using advanced spectroscopic techniques to identify organic compounds and isotopic signatures in the ancient grains.
Astronomers discover high-temperature minerals in comet Wild 2, challenging the formation of crystalline materials. The Stardust mission brings back samples from the coldest spot in the solar system, providing clues about the origin of these materials.
Comet dust samples collected by the Stardust mission are being studied to determine their mineral composition, providing valuable insights into the formation of the solar system. The samples, which consist of ice, dust, and rock, were analyzed using electron microscopes and other techniques.
The study provides key insights into the composition of comets, with three pockets of thin ice detected on Tempel 1. The surface ice appears to have been exposed over time through geologically active jets, revealing an abundance of organic matter and water.
A UW astronomer has successfully collected a record-breaking amount of cosmic dust from comet Wild 2, which dates back to the formation of the solar system 4.6 billion years ago. The aerogel collector, which greatly reduced impact stress on particles, revealed tracks of larger particles visible from several feet away.
The Stardust spacecraft successfully recovered comet dust samples from Wild 2, which are believed to hold evidence about the formation of the sun and solar system. The samples will be studied using powerful instruments, including electron microscopes and nuclear accelerators.
Researchers at UC Berkeley will invite Internet users to help them search for interstellar dust grains captured by NASA's Stardust spacecraft. The 'virtual microscope' technology allows anyone with an internet connection to scan images of aerogel for tracks left by speeding dust, in hopes of discovering grains from distant stars.
The Stardust spacecraft is returning to Earth after a 2.88 billion-mile journey, carrying samples of comet Wild 2 and interstellar dust. The samples are expected to provide key information on the formation of the solar system 4.6 billion years ago.
Researchers observed the impact of a copper projectile on Comet Tempel 1, finding it released approximately 4,500 tonnes of water vapor. The comet's surface was composed of icy grains that sublimed in sunlight, producing a bright tail. These findings suggest comets are more like 'icy dust balls' than previously thought 'dirty snowballs'.
New findings from the Rosetta spacecraft suggest comets are composed primarily of dust held together by ice, contradicting the long-held 'dirty snowball' hypothesis. Cometary nuclei like Comet 9P/Tempel 1 exhibit dynamic and volatile properties, with impacts triggering outbursts of dust and gas.
The Deep Impact mission revealed several dozen impact craters on Comet Tempel 1, with a powdery layer tens of meters deep. The comet's surface is composed of a fine-grained, loosely glued layer of organic powder and ice, sparking new questions about its composition and the formation of the solar system.
The 'Deep Impact' collision released tens of thousands of tons of material, enough to bury a football field under 30 feet of comet dust. Scientists are analyzing X-ray data to better understand the evaporation process on comets and their interaction with solar wind.
Swift detected a quick rise in ultraviolet light after the Deep Impact probe struck a hard surface on the comet, revealing secrets about the impact.
NASA's Hubble Space Telescope captured dramatic images of comet 9P/Tempel 1 before and after a 820-pound projectile impact by the Deep Impact spacecraft. The collision caused a brilliant flash and increased the size of the inner cloud of dust and gas, which expanded outward in a fan shape at speeds of up to 1,200 miles per hour.
The new Web-based modules, developed by COMET, will acquaint forecasters with the physics behind rip currents and help them use wind and wave forecasts to produce outlooks of rip-current risk. The modules include animated depictions of rip-current evolution in three dimensions.
A Brown University geologist is part of a joint space mission to study a comet's composition. The Deep Impact mission will provide a first-ever look inside a comet when an impactor hits Tempel 1, helping scientists understand how comets shaped the solar system.
Scientists have discovered minerals in comet dust similar to those found on Earth, providing insights into the solar system's formation. The Spitzer space telescope has captured detailed images of Comet Encke, helping researchers model how comets eject particles as they orbit the sun.
The Deep Impact mission aims to study the composition of Comet Tempel 1 by deploying a copper probe into its surface. The probe will capture images and spectra of the comet's interior, shedding light on the early solar system's formation.
Researchers used VLT interferometer observations to study infrared spectra of dusty discs around three young stars, finding abundant crystalline silicate grains and processed dust near the star. This suggests that building blocks for Earth-like planets are present in circumstellar discs from the start.
A team of British astronomers is tracking Near-Earth Objects (NEOs) using the Faulkes Telescope North and South in Hawaii and Australia. The UK Astrometry and Photometry Programme (UKAPP) provides crucial information to protect the Earth from potential asteroid impacts.
Comet composition can be studied for the first time using a new technique, providing insights into the early solar system. Carbon disulfide has been detected in comet 122P/De Vico, with implications for understanding the origins of life.
The discovery of a disk of dust and comets around Tau Ceti suggests that this star is likely to experience constant bombardment from asteroids, making it difficult for life to evolve. Scientists will have to rethink where they look for civilisations outside our Solar System.
Scientists discover a comet with broad mesas, craters, pinnacles, and canyons on its surface, contrary to expectations of a dark dust-covered comet. The surface's unique features suggest that most impacts were absorbed or vented into space, making it possible to clearly see the crater formations.
The Stardust mission encountered a swarm of large and small particles as it passed within 146.5 miles of the comet's nucleus, exceeding its goal of collecting at least 1,000 samples measuring one-third the width of a human hair or larger.
The UK is leading a European mission to explore comets, which are ancient bodies offering clues to the Universe's secrets. The Rosetta spacecraft will deploy a lander to study the comet's surface, analyzing its composition and search for signs of life.
Researchers from Cardiff University suggest that a large comet impact could throw material containing micro-organisms out of the planet's atmosphere, infecting hundreds of millions of nascent planetary systems. This viable bacterial outflow would survive heat and radiation, ultimately spreading Earth-life across the galaxy.
Astronomers have discovered a possible link between a comet impact in the 6th century and the 'Dark Ages.' The comet's debris caused a prolonged cold period, similar to a nuclear winter, resulting in crop failures and widespread starvation. A small comet size was needed to cause such dramatic effects.
The University of Chicago's dust instrument will help estimate particle collection during the Stardust spacecraft's rendezvous with Comet Wild 2. Scientists expect analysis to provide new insights into solar system formation, while also searching for signs of life on Mars.
A UW astronomer's spacecraft, Stardust, will capture tiny comet grains for clues on the origin of life and carbon in our planet. The encounter with Wild 2 comet is expected to provide valuable insights into the early solar system.
Scientists from the Open University and University of Kent will analyze samples from Comet Wild 2, which was brought back by NASA's STARDUST mission. The cometary particles provide a window into the past, helping to answer fundamental questions about the solar system's formation.
Astronomers have successfully detected and measured the nitrogen-15 isotope in Comet LINEAR, revealing an isotopic abundance ratio of 140 ± 30. This finding provides crucial information about the composition of comets and their connection to heavier organic molecules, which are essential for life on Earth.