Researchers have detected a massive lightning storm on Saturn, with flash rates exceeding those of Voyager 1 and intensities comparable to Earth's thunderstorms. The storm has been observed since January 23 and has varied in intensity, with some 25 episodes occurring since its initial detection.
Astronomers have calculated the density of binary asteroid Patroclus, suggesting it is composed mostly of water ice covered by a patina of dirt. The team proposes that Patroclus and other Trojan asteroids may be dirty snowballs formed in the outer reaches of the solar system.
Astronomers discover an Earth-like planet with a solid core, orbiting a red dwarf star five times less massive than the sun. The discovery, made using microlensing technique, reveals thousands of potentially habitable planets in distant parts of the galaxy.
Scientists have created a general circulation model to study Titan's climate and predict cloud distribution. The model, developed by a European team, successfully explains the formation of several types of ethane and methane clouds on Titan.
Astronomers have discovered two bright debris disks around nearby stars, similar to our own solar system's Kuiper Belt. These narrow disks are believed to be shaped by the presence of a star-like companion that continually grooms their edges.
The University of Colorado's Student Dust Counter instrument will monitor dust grain density in space as New Horizons approaches Pluto. The team hopes to identify undetected clumps of dust, shedding light on the solar system's formation and other stars' planetary systems.
Researchers discovered hundreds of auroras on Mars over six years, linked to strong magnetic field patches in the crust. These events produce ultraviolet light and are not as colorful as Earth's auroras.
The Huygens probe has revealed that Titan's surface is a barren, 'river' landscape where water ice congeals like stone. Methane plays a similar role to water on Earth, existing in solid, liquid, and gas states. The dense atmosphere has conditions similar to those early in our solar system.
The Cassini mission has released a flood of new images of Saturn's icy moons, revealing detailed features such as plumes on Enceladus and compositional variation on the surfaces of Rhea, Dione, and Hyperion. The new views include large mosaics, movies, and false-color views, providing insights into the moons' intricacies.
Recent images from NASA's Cassini spacecraft show jets of fine, icy particles emanating from Saturn's moon Enceladus' south polar region. The discovery provides unambiguous visual evidence that the moon is geologically active and has a fountain-like source of material.
Recent images from NASA's Cassini spacecraft reveal spectacular evidence of an active moon, Enceladus, with jets of fine, icy particles streaming from its south polar region. The discovery confirms the moon is geologically active and provides insight into its internal heating and possible energy sources.
Researchers have found that rivers on Titan, a moon of Saturn, share similar characteristics with those on Earth. The key parameters that differ between the two are gravity acceleration, fluid viscosity, and sediment specific gravity. These similarities suggest that fluvial processes may be more consistent than initially thought.
Researchers create an optical vortex mask that eliminates starlight, allowing for direct observation of nearby planets. The device successfully images Saturn and its rings, paving the way for future exoplanet detection projects like the Terrestrial Planet Finder.
Astronomers observed thin, parallel striations like spokes on a pinwheel within Saturn's outer rings, providing clues about ring thickness and dynamics. The findings give scientists new insights into the micro-structure of the rings and will help estimate their overall thickness.
The Cassini mission reveals that Prometheus creates regular patterns in the F ring, including channels and streamers, by gravitationally extracting material from the ring. This phenomenon poses unique challenges to understanding ring-satellite interactions.
Researchers have discovered ever-changing clusters of debris in Saturn's A ring, with cluster cores ranging from 7 feet to 43 feet in size. The clusters are periodically torn apart by gravitational tides and reassembled into new configurations.
Scientists have found that parts of the D ring have relocated and dimmed, indicating very short evolutionary lifetimes. The Cassini mission has also revealed a spiral structure in the F ring, which may be caused by moons crossing the ring and spreading particles around.
Recent Cassini findings suggest that Enceladus' south pole is the source of water vapor and fine icy particles, defying previous assumptions. The discovery sheds light on the moon's internal heat and its connection to the E ring, offering a new perspective on Saturn's complex system.
The Cassini-Huygens mission has captured the first-ever images of Saturn's auroral emissions at its poles, similar to Earth's Northern Lights. The UVIS instrument on the spacecraft shows rapid responses to changes in the solar wind and significant changes in emissions within the 'oval' of the aurora at Saturn's south pole.
Researchers Bill Kurth and Don Gurnett used Cassini data to study Saturn's kilometric radiation, a phenomenon similar to Earth's northern lights. The higher resolution instrument provided detailed information on the spectrum and its variability, shedding new light on the radio emissions above Saturn's auroras.
Scientists have discovered eerie-sounding radio emissions from Saturn's auroras using Cassini spacecraft data. The study provides high-resolution measurements allowing audio recordings of the radio waves, offering clues about the source of the emissions.
A University of Chicago instrument has discovered dust particles around Saturn's moon Enceladus, sparking interest in a possible dust cloud or connection to the E-ring. The findings could help scientists better understand Enceladus' role as a source of water ice particles in the E-ring.
The National Science Board has awarded Cornell University a $70 million contract to manage the Arecibo Observatory until March 31, 2010. This renewal will enable further scientific research capabilities at the observatory, with plans to develop new instruments and expand user access.
The Cassini Imaging Team report on Titan reveals that the moon's winds blow faster than its surface rotates, with speeds of up to 34 meters per second. The discovery suggests that meteorology works similarly on slowly rotating planets like Venus.
Tim Appenzeller wins AGU's Sullivan Award for his article 'The Case of the Missing Carbon', while Jeffrey Kluger receives the Perlman Award for 'Secrets of the Rings'. Both articles are praised for their scientific accuracy, clarity and engaging storytelling.
Cassini mission data reveals the formation of molecular oxygen atmospheres in Saturn's rings without life present. This finding suggests that oxygen can be produced through non-biological means, complicating the search for life beyond Earth.
A massive gamma-ray flare from a magnetar was detected by the RHESSI satellite, emitting as much energy in two-tenths of a second as the sun gives off in 250,000 years. The event's immense power suggests a solution to the origins of short-duration gamma ray bursts.
Researchers at the University of Iowa have discovered a link between Saturn's radio emissions and its bright auroras. The findings indicate that strong radio emissions from Saturn's aurora are similar to those on Earth, suggesting a connection between the two.
A team of astronomers led by Clarke gathered data on Saturn's aurora using Cassini and Hubble spacecraft. Their observations revealed that Saturn's aurora differ in character from day to day, with varying lengths and behaviors compared to Earth's and Jupiter's.
NASA's Mars Exploration Rovers and the Cassini-Huygens Mission will be discussed, highlighting new discoveries and future exploration plans. The AAAS annual meeting also features presentations on climate change, urban decision-making, and revolutionary engine architectures.
Scientists have detected a 'whiff' of methane evaporating off the surface of Saturn's moon Titan, revealing insights into its geology and weather systems. The data from the Huygens probe also suggests that beneath the thin crust lies a material made of water ice grains.
The Huygens probe will parachute onto Titan's surface on January 14, studying its thick atmosphere and clouds with six science experiments. DISR will take images of the surface for over two hours, creating panoramic views of the ground and horizon.
The Cassini spacecraft detected a massive cloud of escaping oxygen atoms on the dark side of Saturn's rings in January 2004. Scientists believe that the sudden release could be caused by a collision between ice particles and material in one of the main ring systems, or an eruption of icy slush on Enceladus.
Researchers have discovered Cassini findings on Saturn's rings, dust impacts, and radio rotation rate variations. The study found that Saturn's lightning is one million times stronger than Earth's, with some signals linked to storm systems.
Scientists have found that Saturn's system is composed of ice and oxygen atoms, which are produced by collisions between small icy moons and the planet's magnetosphere. The research suggests that these collisions have been occurring for millions of years, adding fresh material to the ring system.
A nuclear-powered space mission to Neptune, expected to launch between 2016 and 2018, aims to gather data on the planet's atmosphere and its largest moon Triton. The mission will employ electrical and optical sensors to study Neptune's atmospheric elemental ratios, gravity, and magnetic fields.
The Huygens probe will encounter a mysterious surface of seven-kilometer-high ice mountains and liquid methane seas. Scientists expect the Cassini spacecraft to improve the current sketchy picture of Titan's surface.
Using the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory, researchers observed the Kepler's supernova remnant, uncovering a bubble-shaped shroud of gas and dust expanding at 4 million miles per hour. The observations revealed distinct features, including heated interstellar dust and regions of hot gas.
Scientists used computer models to analyze the internal structures of Jupiter and Saturn, finding that heavy elements like iron are concentrated in Saturn's core. The research uses data from shock compression experiments and helps improve models of the planets' formation.
Researchers from University of Colorado Boulder analyze Cassini mission data, revealing compositional variation in Saturn's A, B, and C rings. The study suggests that the outer part of the rings contains more ice, shedding light on their origin and evolution.
The Cassini-Huygens spacecraft has successfully landed at Saturn, providing unprecedented insights into the planet's rings, moons, and atmosphere. The four-year mission will explore Titan, Saturn's largest moon, and shed light on the origin and evolution of planetary systems.
Researchers analyzed Cassini's Visual and Infrared Mapping Spectrometer data, revealing water ice, minerals, and unidentifiable materials on Phoebe's surface. This suggests a possible connection between Phoebe and comets, supporting the idea that it may be similar to Kuiper Belt Objects.
A team of astronomers using a novel camera will hunt for planets orbiting other stars, aiming to directly image faint gas-giants. The SDI camera has already made stunning images of Saturn's moon Titan and discovered an object near Jupiter in solar systems beyond our own.
The Cassini orbiter is equipped with 12 scientific instruments to study Saturn's rings and moons. The UVIS instrument will measure UV light reflected by or emitted from Saturn's atmosphere, its rings, and moon atmospheres.
The University of Chicago High Rate Detector will study the physical, chemical and dynamical properties of trapped Saturnian dust. The instrument is capable of detecting 100,000 particles per second, measuring particles ranging from human hair to smaller particles.
Researchers create tholins in lab experiments to understand Titan's chemistry and potential for life. They analyze spectroscopic properties and react with molten water to form oxygenated compounds.
Jonathan I. Lunine, a renowned planetary scientist, will testify before the President's Commission on Implementation of U.S. Space Exploration Policy about detecting other Earths around nearby stars. He suggests developing medium-sized optical and infrared space telescopes, the Terrestrial Planet Finder, which could discover habitable ...
Scientists plan to deploy the Huygens probe to study Titan's lakes, seas, and climate. The moon's thick atmosphere and liquid hydrocarbons will provide a unique environment to understand oceanographic processes and predict climate changes.
A new study published in Icarus reveals that planet formation simulations indicate a high probability of finding Earthlike planets near other stars. The research suggests that the presence and orbits of giant planets like Jupiter can greatly impact the amount of water on terrestrial planets.
New calculations suggest that recycling of material through small moons can lengthen the lifetime of rings and moons. This process, known as cosmic recycling, allows for the re-accretion of fragments into new moons, extending the persistence of ring systems.
The cloud's mass indicates that Europa faces more severe radiation consequences than previously thought, wielding significant influence on Jupiter's magnetosphere. The discovery uses innovative ENA imaging technique to visualize the three-dimensional structure of planetary space environments.
Individuals with reduced functional Artemis protein are prone to mild immunodeficiency and increased risk of developing lymphomas. This finding suggests that mutations in Artemis or other DNA repair genes may be responsible for immune deficiency and/or lymphoma cases.
New theory explains why circumstellar Keplerian disks are stable around Be stars, contradicting previous model's predictions. The Magnetically Torqued Disk model suggests a narrow range of star types can form detectable disks.
A new kind of cruise missile engine, called a scramjet, has been tested to achieve Mach 6.5 speeds in simulated hypersonic conditions, outperforming traditional ramjets. The engine is being developed for use in the HyFly joint DARPA/ONR Flight Demo program, aiming to launch missiles at speeds up to Mach 6 and ranges of 600 nautical miles.
Researchers are using computer simulations to determine if the 47 Ursae Majoris system can contain an Earth-like planet. The system's asteroid belt is in the habitable zone, increasing the likelihood of finding a terrestrial planet.
The Cassini spacecraft's Magnetospheric Imaging Instrument (MIMI) has captured the first images of Jupiter's magnetosphere and surrounding particles. These images reveal the presence of a huge nebula enveloping Jupiter, extending out to 13 million miles from the planet.
A search for lightning on Venus in 1998 and 1999 using the Cassini spacecraft failed to detect high-frequency radio waves commonly associated with lightning. Donald Gurnett, a space physicist at the University of Iowa, suggests that if lightning exists on Venus, it may be extremely rare or very different from terrestrial lightning.
The University of Colorado-built UVIS instrument package has produced the first spectral images of Jupiter, capturing its aurora and a gigantic glowing ring of gas encircling the planet. The image reveals temperatures of over 100,000 degrees Fahrenheit and a torus density so low that it would fit inside Fenway Park if compressed to sol...
Researchers at Case Western Reserve University have developed a technique to simulate various gravitational environments using a magnetic levitation method. This allows them to study the behavior of liquids and solids in conditions ranging from Earth's gravity to zero-G environments, providing new insights into fluid dynamics.
The Marshall Space Flight Center is developing innovative solutions to reduce costs and increase reliability in space transportation. The team aims to make space accessible to the general public, enabling adventure travel, business ventures, and scientific research.