Scientists found that vents on Enceladus channel water vapor from a warm, probably liquid source to the surface at supersonic speeds. This supports a theory that tidal heating causes geysers and provides implications for life in the solar system.
NASA's Hubble Space Telescope has directly observed a planet circling another star, Fomalhaut b. The exoplanet orbits Fomalhaut at a distance of 10.7 billion miles, 10 times that of Saturn from the sun.
The discovery reveals the planet's massive size and potential for a vast ring system. The images taken with Hubble Space Telescope provide direct proof of the planet's existence and orbit around star Fomalhaut.
Research on the centre of planets provides deeper insight into controlled thermonuclear fusion and improves models of Jupiter and Saturn. The study reveals that extreme matter behaves like a charged liquid at smaller distances but acts more like a gas over larger lengths.
Researchers from the University of Granada and University of Valencia have confirmed natural electric activity in Titan's atmosphere using data from the Huygens probe. This discovery increases the likelihood of organic molecules forming on Titan, which could be precursors to life.
CSIRO research scientist Dr John Bunton is to receive a NASA Space Act Board Award for his work on a novel 'beamformer' capable of providing a live video link from Mars. His design involves dividing video signal data into narrow channels and summing the data from all 400 antennas to reconstruct a broadband signal.
Researchers at UC Berkeley and University College London discovered that metallic helium is produced under extreme conditions found at the centers of Jupiter and Saturn, mixing with metal hydrogen to form a liquid metal alloy. This finding challenges previous theories about the energy source powering these planets.
Scientists confirmed a surface liquid lake on Titan, measuring approximately 235 kilometers long and filled with liquid ethane. The discovery was made using the Visual and Infrared Mapping Spectrometer (VIMS) instrument on NASA's Cassini orbiter.
A team of European astronomers has discovered a triple system of super-Earths around the star HD 40307 using the HARPS instrument. The planets have masses between 4.2 and 9.4 times that of Earth, and orbit the star with periods ranging from 4.3 to 20.4 days.
Researchers have determined the masses of the coldest class of brown dwarfs for the first time outside the solar system. The team used ultrasharp images from the Keck Telescope and Hubble Space Telescope to measure the sizes and durations of binary systems, revealing two new brown dwarf binaries with masses as low as 6% of the sun's mass.
Researchers mapped large arc-shaped depressions on Jupiter's moon Europa, indicating a shift of 80° in its rotational axis. The findings suggest the presence of an internal liquid ocean, which could support life, and provide independent evidence for this possibility.
Researchers have found evidence of small, sandy particles orbiting a newborn solar system at a distance similar to the Earth's orbit around the sun. The discovery sheds light on how Earth-like planets may form and offers new opportunities for studying the chemical composition of these particles.
Scientists have shed light on Enceladus' space enigma by explaining the dynamics of its erupting plume. The new theory suggests that dust particles and water vapor form below the moon's surface, with temperature and pressure conditions allowing for rapid water vapor eruption and slower dust particle ejection.
Astronomers have discovered a solar system nearly 5,000 light years away with scaled-down versions of Jupiter and Saturn. The planets are similar in size to our own, suggesting that planetary systems like ours may be more common than previously thought.
A new system of planets has been discovered with striking similarities to our Solar System, revealing giant planets that favour family groups over lone objects. The discovery uses a world-wide net of telescopes and challenges the single-life theory of gas-giant planets.
An international team of astronomers has discovered two planets resembling smaller versions of Jupiter and Saturn in a solar system nearly 5,000 light years away. The newly-discovered planets appear to be gaseous planets with masses similar to those of the giant planets in our own solar system.
Researchers have discovered a multi-planet system with two large planets similar to Jupiter and Saturn, suggesting that planetary systems like our own may be common in the Milky Way galaxy. This is the first discovery of its kind, using a new gravitational microlensing technique.
The discovery of the double planet system provides crucial evidence for the presence of multiple planet systems similar to our own solar system. The findings suggest that if OGLE-2006-BLG-109L is typical, it is possible that other systems have Jupiter- and Saturn-sized planets.
Saturn's rings exhibit fine-scale structures with periodic radial variation in optical depth, while daily fluctuations in streamflow can be influenced by flow velocity. Internal waves in the Pacific Ocean are also studied for their impact on oceanic mixing and energy transport.
Researchers found tholins in the disk of red dust around HR 4796A, a eight-million-year-old star with planets forming. The presence of these complex molecules suggests that basic building blocks of life may be common in planetary systems.
A hot spot on Enceladus's south pole generates enough heat to eject ice and vapor plumes, indicating geological activity. The presence of water vapor and lack of sodium suggest a different mechanism may be at play, fueling questions about the moon's habitability.
New research suggests Saturn's rings have been present since the solar system was formed 4.5 billion years ago, with different ring features varying in age and material being continually recycled. The recycling process helps explain why the rings appear brighter than expected, despite ongoing pollution.
The Voyager 2 spacecraft has detected a strong magnetic field in the interstellar region, distorting the bubble of outflowing gas from the sun. Additionally, the temperature was found to be ten times cooler than expected just outside the boundary, sparking new explanations.
A mathematical algorithm has been developed to determine the most efficient path for a spacecraft's journey from point A to point B, regardless of distance or time. The algorithm was tested and validated on the 1997 Cassini Mission, which required numerous gravity assists and complex maneuvers.
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.
A new study published in Journal of Adolescent Health found that random drug and alcohol testing among high school athletes did not reduce past month or year use. In fact, students at schools with regular testing reported feeling less athletically competent and believed less in the benefits of drug testing.
Astronomers have found persistent morning drizzle of methane over the western foothills of Titan's major continent, Xanadu. The discovery suggests that moisture-laden clouds pushed upslope by winds condense to form a coastal rain, with the drizzle dissipating after local mid-morning.
A team of astronomers at UC Berkeley reports a nearly global cloud cover and morning drizzle of methane over Titan's western foothills. The drizzle may be caused by processes similar to those on Earth, with moisture-laden clouds pushed upslope by winds condensing to form a coastal rain.
Scientists at the University of Chicago have found that Titan's climate is analogous to Earth's tropics, with methane clouds and a tropical weather system. The moon's slow rotation rate and atmosphere produce an updraft that lifts evaporated methane into clouds, similar to Earth's ITCZ.
Researchers propose a new model, Frigid Faithful, which explains the formation of fractures and ridges on Saturn's moon Enceladus without requiring liquid water. The model describes how heat from a shallow source beneath the surface could lead to geyser-like activity and complex tectonic features.
Recent findings indicate a trend of increasing water content in the atmospheres of planets, from Jupiter (depleted) to Uranus and Neptune (water-rich). Computer models provide insights into planetary atmospheric chemistry, predicting the composition of Earth-like planets in other solar systems.
Researchers mapped Saturn's rings using a 'CAT scan' method, confirming the presence of clumps and empty gaps. The discovery may help explain the origin and age of Saturn's rings.
The Cassini spacecraft has mapped the structure of Saturn's rings, revealing densely packed particle clumps that are constantly forming and colliding. The findings suggest the mass of the rings may be twice or more previous estimates, with implications for understanding the origin and age of Saturn's ring system.
Researchers found that tidal forces caused by Saturn's gravity can control the timing of eruptions from cracks in Enceladus' southern hemisphere. The study suggests that these cracks, known as Tiger Stripes, are warmer than their surroundings and may be the source of eruptions.
A new study suggests that frictional heating is the most likely explanation for the plumes and features observed on Enceladus. The process occurs when tidal forces cause fault lines in the moon's icy shell to rub back and forth, producing enough heat to transform ice into water vapor and ice crystals.
The University of Central Florida professor has made a groundbreaking discovery that the hottest known extrasolar planet, HD 149026b, is approaching temperatures of 3,700 degrees. This unprecedented finding indicates that the planet's surface must be incredibly black to absorb all the starlight it receives.
Researchers found evidence of magnetic reconnection in turbulent plasma around Earth using ESA's Cluster satellites. This discovery has significant implications for understanding the behavior of turbulent plasma and its role in fundamental processes such as energy dissipation and particle acceleration.
A new study published in PLoS Biology found that cells change size and shape to form the heart's chambers, with blood flow and cardiac contractility influencing cell shape. The researchers propose a balance of internal and external forces necessary for optimal chamber curvature, potentially underlying some types of heart disease.
According to ASU researcher Ronald Greeley, Europa is the most promising candidate among four worlds beyond Earth that might contain life. The moon has a thick layer of water and organic minerals, making it an ideal target for NASA's next mission. Scientists hope to measure the ice shell's thickness using tidal flexing measurements.
Researchers found that Enceladus's geysers spray ice particles, creating reflective surfaces on other Saturn moons and altering their appearance. The study suggests that Enceladus's geological activity supports the possibility of liquid water beneath its surface.
Researchers found that gas giants either form within the first 10 million years of a sun-like star's life or not at all. The study suggests that gas giant planets must form early in a star's history, offering insights into planet formation.
Researchers propose a new model explaining the giant plume on Enceladus by dissolving gases in clathrate ice under the water ice cap. This environment allows for a Frigid Faithful plume, which produces nitrogen, methane, and carbon dioxide gases.
The Cassini spacecraft has imaged the tallest mountains ever seen on Saturn's moon Titan, with peaks reaching nearly a mile high. The mountains are topped with bright, white material that may be methane or other organic 'snow,' suggesting a unique geology and potential for life.
Scientists explore factors that pulled Earth out of its 'Snowball Earth' state and study seismic wave speed in the lower mantle. Researchers also investigate water vapor in Saturn's upper atmosphere using Cassini radio occultation data.
A new study suggests that early Earth haze could have provided a substantial source of organic material useful for emerging life on the planet. The researchers found that hazy conditions could have produced a similar organic haze over a wide range of methane and carbon dioxide concentrations.
Researchers have directly imaged a faint brown dwarf companion to the star HD 3651, which hosts a planet. The discovery provides valuable information on planetary formation and offers a unique insight into the co-formation of planets and brown dwarfs around the same star.
Scientists have observed a continuously changing feature in Saturn's innermost ring, the D ring, which indicates a recent comet or asteroid collision. The findings suggest that Saturn's rings are not eternal but dynamic systems that can change over time.
The Cassini spacecraft has found additional faint ring structures formed by processes acting on and within Saturn's moons and main rings. The newly discovered rings are created by impacts onto larger bodies, releasing material that creates diffuse rings.
The Cassini spacecraft has detected a massive ethane cloud surrounding Titan's north pole, contradicting previous assumptions of extensive ethane clouds and surface liquids. The discovery suggests that ethane may be 'snowing' onto the surface, forming methane lakes below.
The IAU defined a planet as a celestial body in orbit around the Sun with sufficient mass to assume hydrostatic equilibrium. The new definition includes our solar system's eight recognized planets and a distinct class of dwarf planets, including Pluto.
Recent observations from the Cassini spacecraft and Huygens probe suggest massive methane storms on Titan, creating a 'methane cycle' similar to Earth's water cycle. These storms produce dense clouds of methane and copious precipitation of liquid drops, generating rivers and canals on Titan's surface.
Astronomers have observed a massive nuclear explosion on the surface of a white dwarf star, sending gas into space and creating a blast wave that accelerates electrons to nearly the speed of light. The European VLBI Network tracked the outburst using telescopes around the world, revealing a cigar-like shape in the blast wave.
Researchers propose that Enceladus' reorientation could be caused by a low-density blob beneath its surface, leading to a hot spot at the pole and explaining the moon's striking surface features. The study suggests testable predictions for future observations of Enceladus.
A new model for the capture of planetary satellites involving a three-body gravitational encounter between a binary and a planet suggests that Triton was originally part of a binary pair orbiting the Sun. This mechanism introduces a new pathway for satellite capture by planets, which may be relevant to other objects in the solar system.
The new movies released by NASA's Cassini mission provide a realistic experience of the Titan landing. The images taken by Huygens' Descent Imager/Spectral Radiometer (DISR) during its plunge into Titan's atmosphere have been converted into movie format, showcasing the probe's descent and the changes it observed in the environment.
Research papers highlight the influence of Himalayan topography on monsoon rainfall and reveal self-gravity wakes in Saturn's A ring. Additionally, studies show complex ion chemistry on Titan's nightside and suggest ammonia ions in Titan's ionosphere.
Scientists discovered massive sand dunes on Saturn's moon Titan, formed by tidal winds and unique atmospheric conditions. The dunes, similar to those in Namibian Deserts, suggest that Titan's atmosphere can create surface winds powerful enough to sculpt sand.
The discovery of a blue ring around Uranus reveals similarities with Saturn's E ring, both associated with small moons. Researchers attribute the blue color to gravitational forces acting on dust particles that allow smaller ones to survive while larger ones are recaptured by the moon.
Astronomers have found a blue ring around Uranus, similar to Saturn's blue ring in Enceladus' orbit, attributed to submicron-sized material and subtle forces acting on dust particles. The discovery suggests that the two outer rings share a common explanation for their blue color.
Astronomers discover that Uranus' blue ring is predominantly made of submicron-sized material, unlike most other rings which appear red. The similarity between the outer rings suggests an in-kind explanation for their blue color.