Articles tagged with Saturn
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Researchers reanalyze Cassini mission data to find that Titan's interior is more icy and slushy than previously thought, with implications for the search for life on Titan. The new findings suggest a slushy layer instead of an ocean, which could facilitate the growth of simple organisms.
Scientists have found new complex organic molecules spewing from Saturn's moon Enceladus, confirming that complex chemical reactions are taking place within its underground ocean. The discovery strengthens the case for a dedicated European Space Agency (ESA) mission to orbit and land on Enceladus.
Astronomers used Gemini South and James Webb Space Telescope to detect silane in ancient brown dwarf's atmosphere, revealing how primordial formation impacts planet atmospheres. The discovery confirms understanding of gas giant cloud formation and offers insight into the composition of distant worlds.
Amateur astronomers, led by Dr. Steven Hill, used a simple analytical method to map ammonia and cloud heights in Jupiter's atmosphere. They found that the primary clouds are likely composed of ammonium hydrosulphide, not ammonia ice, due to photochemical reactions.
Hubble's OPAL program has observed the four giant outer planets since 2018, providing long-term baseline data on their atmospheric changes. The observations have led to remarkable discoveries, including the measurement of Jupiter's wind speeds and Saturn's ring system colors.
Ravit Helled received the 2024 Paolo Farinella Prize for her work on planetary interiors, proposing a dilute core structure that was later confirmed by mission data. Her research also explores giant planet formation and evolution, with international contributions to NASA and ESA missions.
Researchers analyzed Cassini radar experiment data to estimate the composition and roughness of Titan's sea surfaces, revealing differences in hydrocarbon seas' surface layers dependent on latitude and location. The study found higher dielectric constants in southern Kraken Mare and detected tidal currents near coastal areas.
The NASA TESS-Keck Survey catalog features 126 exotic planets with detailed measurements allowing for comparisons with our solar system. Several planets stand out as touchstones for deepening astronomers' understanding of planetary formation and evolution.
A global ocean of liquid water has been found beneath Mimas' icy shell, with an estimated age of 5-15 million years, suggesting recent ocean formation and potential for life to emerge. This discovery adds Mimas to the list of moons with internal oceans, including Enceladus and Europa.
A Lancaster University PhD student used a new method to calculate the optical depth of Saturn's rings, revealing their transparency. By analyzing changes in Cassini's Langmuir Probe data during solar eclipses, the researcher determined how much sunlight passed through each ring.
New studies show that giant gas planets in nearby star systems can prevent life on smaller, rocky planet neighbors by kicking them out of orbit and wreaking havoc on their climates. Researchers found that four giant planets in the HD 141399 system are likely to destroy the chances for life on Earth-like planets.
Saturn's north pole is experiencing a cooling trend as autumn approaches, with the warm polar vortex filled with hydrocarbon gases disappearing. The new observations provide insights into the changing seasons on the massive outer planet, using data from the James Webb Space Telescope.
Researchers found long-term disruptions in Saturn's atmosphere, caused by past megastorms, which persist for hundreds of years. The study revealed that ammonia gas is being transported from the upper to lower atmosphere via precipitation and reevaporation processes.
Researchers have found high levels of phosphates in the water on Saturn's moon Enceladus, a key component of DNA and cell membranes. The discovery increases the chances of finding habitable worlds across the galaxy, as Enceladus can support life over a wider range of distances from its star.
Saturn's rings are estimated to be 400 million years old, much younger than the planet itself, according to a new study. The researchers used dust analysis to determine the age of the rings, which are composed of ice and rocky material.
Astronomers have found that Saturn's vast ring system is heating the giant planet's upper atmosphere, a phenomenon that could provide insights into the atmospheres of distant worlds. The discovery was made using archival ultraviolet-light observations from four space missions, including Hubble and Cassini.
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.
A new UCLA-led study explains that tidal heating in Enceladus' rocky core creates currents that transport silica particles to the surface. The research suggests that these flows can pick up materials from the seafloor and bring them to the ice shell, providing evidence for hydrothermal activity at the ocean floor.
NASA's Hubble Space Telescope has captured the start of Saturn's spoke season, a mysterious phenomenon that appears across the planet's rings during its equinox. The cause of the spokes remains unknown, but scientists believe they may be linked to Saturn's variable magnetic field and charged particles in the solar wind.
A new ring system has been found around the Pluto-sized dwarf planet Quaoar, which orbits beyond Neptune. The discovery is remarkable because it lies at a distance of over seven planetary radii from its parent body, posing a challenge to existing theories of ring formation.
Numerical simulations suggest that Mimas' Herschel impact basin is compatible with a thinning ice shell and geologically young ocean. The results imply that the present-day ocean within Mimas must have been warming and expanding since its formation, potentially making it an emerging ocean world.
Researchers compiled 41 solar occultation observations of Saturn's rings from the Cassini mission to inform future investigations into their formation and evolution. The study reveals new information on ring particles' sizes and compositions, shedding light on the origins of the ring system.
Scientists have discovered new evidence of phosphorus availability in Enceladus's ocean, making it a prime target in the search for extraterrestrial life. The discovery suggests that Enceladus's subsurface ocean is likely habitable due to its high levels of dissolved phosphorus.
A new study suggests that Saturn's tilted axis is due to the loss of an ancient moon, Chrysalis, which collided with the planet around 160 million years ago. The collision caused the satellite to break apart, releasing fragments that formed the planet's rings and leaving Saturn out of Neptune's gravitational resonance.
New research by UC Riverside astrophysicist Stephen Kane suggests that Jupiter's four main moons would quickly destroy any large ring formations. This prevents Jupiter from having substantial rings, unlike Saturn. The study provides evidence of catastrophic events in the past through the analysis of ring compositions and shapes.
A SwRI study examines elliptical craters on Saturn's moons Tethys and Dione, finding unique patterns that indicate the satellites' age and formation conditions. The research suggests a planetocentric impactor population, pointing to the importance of considering gravity-driven impacts when studying object ages.
A new theory offers an explanation for the formation and evolution of gas giants in our solar system, proposing that a 'rebound' effect triggered their current paths. Researchers found that the primordial gas disk dissipated from the inside out, providing a natural trigger for the instability.
Dr Henrik Melin, a researcher at the University of Leicester, has been awarded the third-ever Webb Fellowship to study the atmospheres of giant planets using the James Webb Space Telescope. He aims to understand the mechanisms driving powerful aurorae on these planets and address the 'energy crisis' in their upper atmospheres.
Researchers at the University of Leicester have discovered a new mechanism driving Saturn's massive aurorae, which are fueled by swirling winds in its upper atmosphere. This discovery answers one of NASA's Cassini mission mysteries and highlights the complex interactions between atmospheric weather and aurora creation.
Scientists recreated Titan's conditions, studying properties of organic molecules ACN and PCN on the moon's surface. The findings could provide insights into Titan's surface cracking and confirm its mineral composition.
The Dragonfly mission will investigate Titan's surface and atmosphere, searching for chemical biosignatures and exploring the moon's active methane cycle. By analyzing the prebiotic chemistry currently taking place in Titan's atmosphere and on its surface, scientists hope to gain insights into the potential for life on the moon.
Researchers simulate conditions necessary for Saturn's unique magnetic field, indicating higher temperatures at the equatorial region and lower temperatures at high latitudes. The findings advance the effort to map Saturn's hidden regions and provide insights into the planet's formation and evolution.
Recent research by CNRS scientists suggests Saturn's current tilt is due to the migration of its largest moon Titan and other satellites, causing it to interact with Neptune's orbit, leading to gradual tilting. The planet's axis could more than double in inclination over the next few billion years.
A team of scientists, led by Matt Clement, used simulations to study the formation of Jupiter and Saturn. The findings suggest that these two planets were originally closer together than previously thought, with a ratio of two Jupiter orbits to one Saturnian orbit being more consistent with the current configuration.
Researchers Jeremy Bloxham and Rakesh K. Yadav use a 3D simulation model to understand the formation of Saturn's massive hexagon storm, which has remained relatively unchanged for nearly 40 years. The study suggests that deep thermal convection plays a key role in creating the unique shape and persistence of the storm.
The latest Hubble image of Saturn reveals small atmospheric storms in the planet's northern hemisphere, with pronounced banding visible. The ringed planet's atmosphere is mostly hydrogen and helium, with seasonal changes due to increased sunlight also producing a reddish haze.
Researchers used model simulations to study Saturn's polar hexagon, discovering a potential mechanism for its formation. The simulations produced latitudinal flow jets and vortices that resembled those observed on Saturn, suggesting a possible explanation for the stable pattern.
The Cassini spacecraft captured high-resolution images of Saturn's Hexagon, revealing a multilayered haze system with particles as small as 1 micron. The team discovered that the hazes are organized by gravity waves and may be responsible for the hexagon's formation.
New analysis of data from NASA's Cassini spacecraft reveals that auroral electric currents are likely responsible for heating Saturn's upper atmosphere. The study provides the most complete mapping yet of temperature and density in a gas giant's upper atmosphere, shedding light on how heat circulates in the region.
Numerical simulations reveal a 'safety zone' where warmer gas pushes satellites away from their parent planets, explaining the presence of single large moons like Titan. The findings support the idea that many large moons formed along with their parent planets.
Researchers analyze Cassini data to study Saturn's ultraviolet auroras and their dynamic processes. The new observations provide unique views of the small-scale structures behind these auroras, revealing similarities with Jupiter's magnetosphere.
The study investigates the physical forces acting on Enceladus that allow the tiger stripe fissures to form and remain in place. The researchers found that the fissures could have formed on either pole, but the south pole's unique deformation led to their formation.
Scientists have discovered that the unique tiger stripes on Enceladus are caused by tidal forces from Saturn's gravity, which release pressure and prevent the cracks from freezing shut. This allows water to erupt from the fissures, creating a regular spacing pattern.
Researchers studied Titan's energy budget over 14 years and found significant seasonal variations. The findings suggest the distance between the sun and Earth may play a role in Earth's energy balance.
Researchers have discovered a complex storm system in Saturn's north polar atmosphere, with features suggesting they are caused by convection in deep water clouds. The storms were found to be long-lived and high-intensity, unlike those on Earth, and appear to have formed at a rate of one every 30-60 years.
The latest Hubble image of Saturn reveals a planet with a dynamic atmosphere, featuring turbulent storms and subtle changes in its banded structure. The iconic hexagon at Saturn's north pole remains unchanged, while the mysterious six-sided pattern continues to intrigue scientists.
Astronomers have measured the temperature of Uranus' rings for the first time, finding a cool 77 Kelvin. The new images also reveal differences in ring composition compared to Saturn's rings, including lower albedo and narrower widths.
Researchers used Cassini's closest observations to study Saturn's rings, revealing three distinct textures and tiny moons within the rings. The study also found streaky textures and large boulders, which may be fragments of broken objects or formed through accretion processes.
Researchers found that Mimas' migration into the Cassini Division pushed apart ice particles, creating the 4500 km wide band. The moon's orbit may have been driven by orbital resonance with Saturn, causing it to lose energy and migrate inwards.
A team of researchers led by Caitlin Griffith discovered a mysterious linear ice corridor on Titan's surface, which suggests the presence of past volcanic activity. The find sheds new light on Titan's unique atmospheric chemistry and potential for life
Researchers from UCL and University of Arizona developed a 'deep learning' approach called PlanetNet to detect storms on Saturn. The algorithm accurately maps the components and features in turbulent regions, revealing previously undetected atmospheric features such as ammonia ice clouds.
A new study using the PlanetNet algorithm provides unprecedented precision in analyzing Saturn's storm clouds, revealing features previously undetected. The analysis of Cassini data reveals atmospheric processes driving the storms, including dark cloud material swept up from lower atmosphere.
The Cassini spacecraft gathered data on five small moons close to Saturn's rings, revealing no volatiles other than water ice. The moons' geology was shaped by complex processes, including tidal stresses, with optical properties influenced by contamination from the main rings and ring material.
The latest data from Juno and Cassini spacecraft has challenged existing theories on planetary formation and behavior, revealing new insights into Jupiter and Saturn's magnetic fields and atmospheres. Surprisingly, the atmosphere is evenly mixed, contradicting conventional predictions.
Saturn's ring system acts as a sensitive seismograph to measure the giant planet's vibrations, enabling scientists to determine its rotation rate. Researchers used wave patterns in the rings to probe Saturn's interior, obtaining the first precise determination of its rotation rate.
A recent study using Cassini data estimates Saturn's ring mass to be around 40 percent of the moon Mimas' mass, indicating a relatively young age for the rings. The discovery also provides insight into Saturn's internal structure and atmospheric circulation patterns.
New gravity field data reveal Saturn's rings are significantly younger than the planet, with ages estimated at 10-100 million years. The findings contradict previous assumptions and shed light on the formation of Saturn's ring system.
Researchers found that Saturn's iconic rings are losing ice particles at a maximum rate, draining an Olympic-sized pool in half an hour. The entire ring system is expected to vanish in 300-100 million years.
Saturn's iconic rings are being pulled into the planet by gravity, draining an Olympic-sized swimming pool in half an hour. The research suggests the ring system will be gone in 300 million years, with some particles also falling onto Saturn's geysers from moon Enceladus.
A team of scientists has found a new way to explain the formation of Saturn's radiation belts, which challenges current theories on electron acceleration. They suggest that Z-mode waves are responsible for energizing electrons in the belt, rather than radial diffusion.