Articles tagged with Saturn
Chris Fox, a space buff since childhood, and his team discovered exoplanet Kepler 159d by analyzing the orbits of nearby planets. The exoplanet has a mass similar to Saturn's and likely consists of gases with no solid surface.
Astronomers successfully collected microscopic material streaming from Saturn's rings using Cassini's Cosmic Dust Analyzer and Radio and Plasma Wave Science instruments. The research reveals that the main component of Saturn's rings is water ice, with tiny silicates also present.
A new study reveals Saturn's innermost D ring is hurling dust grains coated in its chemical cocktail into the planet's upper atmosphere at an extraordinary rate. This infalling material may change the carbon and oxygen content of the atmosphere, prompting questions about the rings' formation and lifespan.
This special issue of Science presents research on Cassini's final transmissions to Earth, revealing new observations and insights into Saturn's atmosphere and rings. The studies found that water, methane, and organic-rich material fall into the planet's atmosphere, modifying its composition and structure.
Researchers found a tilt of less than 0.01 degrees in Saturn's magnetic field, contradicting the theory that it requires a significant tilt to form. The team also spotted interesting structures near the planet, including a secondary source of magnetism and electric currents flowing between the rings and the planet.
SwRI scientists used Cassini's final measurements to detect large influx of materials raining into Saturn's atmosphere, with water and organic compounds falling at rates of up to 10,000 kilograms per second. The discovery has implications for ring evolution and atmospheric chemistry.
Scientists synthesize a nanoscale Saturn system consisting of a spherical C60 fullerene as the planet and a flat macrocycle made of six anthracene units as the ring. The structure is confirmed by spectroscopic and X-ray analyses, enabling a new structural motif for researchers.
A study led by University of Leicester scientist Dr. Leigh Fletcher found that massive northern storms on Saturn can disrupt its equatorial atmospheric patterns, similar to those seen on Earth. The research reveals a link between distant events in a planet's climate system, known as teleconnection.
Cassini spacecraft data reveals Saturn's rings casting shadows in ionized particles, affecting the planet's ionosphere. The dynamic ionosphere is structured on small scales and shows surprising variability, with possible explanations including ring rain, solar radiation, or magnetic field interactions.
Astronomers conclude that Saturn's seven moons - Pan, Atlas, Prometheus, Pandora, Epimetheus, Mimas, and Janus - work together to contain the A ring. The moon's gravitational influence slows down the spreading ring's momentum, creating an edge.
Researchers found that extreme methane rainstorms occur frequently on Titan, creating massive floods in deserts and shaping the moon's surface. The storms are correlated with the formation of alluvial fans, similar to those on Earth.
Researchers use digital holographic microscopy to detect microorganisms and evidence of life in Enceladus water plumes. A universal biosignature is also proposed to detect biological systems on ocean worlds like Enceladus.
CU Boulder scientists, led by Professor Larry Esposito, will continue to study Saturn's rings, moons and atmosphere using the Ultraviolet Imaging Spectrograph (UVIS) instrument on the Cassini-Huygens mission. The team has made numerous discoveries, including the detection of oxygen atoms in Saturn's system and water plumes from Enceladus.
The James Webb Space Telescope will study the 'ocean worlds' of Europa and Enceladus, adding to previous observations by Galileo and Cassini orbiters. The telescope's high-resolution imagery and spectroscopic analysis will help unravel the mysteries of these moons' subsurface oceans and potential biosignatures.
Scientists detect methanol around Saturn's moon Enceladus using a ground-based telescope, suggesting complex chemical reactions occur in the plume once it's ejected into space. This finding highlights the need for further direct observations by future spacecraft to understand the chemistry of subsurface oceans.
Researchers simulated the entire ring system of Chariklo, a small body in the Solar System with rings. The simulation found that the inner ring is unstable without help, suggesting smaller particles or an undiscovered shepherd satellite may be responsible.
Cassini-Huygens mission has fostered dazzling discoveries, including in-depth studies of Saturn's rings, methane lakes on Titan, and hot water plumes from Enceladus. The spacecraft will enter Saturn's atmosphere and vaporize after final ring-dive on September 15.
Researchers measured Saturn's ring brightness and temperatures using Subaru Telescope images. The Cassini Division and C ring appeared brighter in mid-infrared due to thermal emission from warmer particles. However, seasonal changes in the ring opening angle caused variations in their apparent brightness.
Researchers suggest an unseen population of gas giant planets may exist at distances similar to Jupiter and Saturn, resolving a long-standing debate about their formation. The predicted planets could be found using NASA's Wide Field Infrared Survey Telescope.
Research from NASA's Cassini mission data implies Saturn's moons may have formed from the planet's rings rather than being captured by it, with some moons migrating away at an unexpected rate
Researchers discovered the presence of a white spot on Saturn's equator moving at speeds of 1,600 km/h. The study found that winds increase dramatically with depth, reaching up to 1,650 km/h at 150 km below the surface.
A team of researchers presented a new model for the origin of Saturn's rings based on computer simulations. The study found that Kuiper belt objects were destroyed by tidal forces when passing close to giant planets, forming icy ring systems. This process explains the compositional differences between Saturn and Uranus' rings.
Dr. John Spencer has received the AGU's Whipple Award for his outstanding contributions to planetary science, including deciphering Enceladus' internal ocean and discovering oxygen on Jupiter's moons.
Researchers have discovered a chemical trail on Saturn's moon Titan that could indicate the presence of prebiotic conditions. The trail was found in the form of hydrogen cyanide, an organic chemical that can react with itself or other molecules to form long chains called polyimine.
Scientists have pinpointed a mechanism for cyclical tidal stresses to drive and sustain Enceladus's long-lived eruptions. The Cassini spacecraft has observed geysers erupting continuously along the south pole for decades.
A team of scientists led by UH professor Liming Li analyze Cassini spacecraft data to understand the seasonal changes on Saturn. They also examine the energy budget for Jupiter and Saturn to better comprehend planetary climate evolution.
Researchers found that water ions escape from Saturn's magnetosphere at a reconnection point, where magnetic fields disconnect and reconnect. This discovery helps scientists understand the physics of rapid rotators like Jupiter and how they expel materials.
Scientists have successfully simulated 3D models of deep jet streams and storms on Jupiter and Saturn, revealing their dynamics and providing clues to Earth's weather patterns. The study helps clarify the origin and behavior of these features, which remain debated among researchers.
Researchers capture first image of a debris ring orbiting a white dwarf star, revealing a spiral-like structure and 'inside-out' structure. The ring system is formed by the star's gravity tearing apart asteroids, emitting a dark red glow from gas produced by collisions.
Researchers reveal that Saturn's F ring and its shepherd satellites, Prometheus and Pandora, formed from the collision of small satellites with a dense core. This study sheds light on the formation process of satellite systems in our solar system and beyond.
Dr. Martin Duncan's new model proposes that gas giants like Jupiter and Saturn formed through the accumulation of small 'pebbles', allowing cores to form rapidly enough to capture their atmosphere. The successful model predicts the formation of one to four gas giant planets, consistent with the observed outer solar system configuration.
Researchers suggest planetary pebbles, icy objects about a foot in diameter, were the building blocks for Jupiter and Saturn. This new model improves solar system formation models, producing the observed structure of the solar system with two gas giants, two ice giants, and a pristine Kuiper belt.
Scientists discovered that the size of particles doesn't matter for ring formation and that the abundance of larger particles drops off due to surface forces. The team's model showed that the size distribution in planetary rings is universal, supporting a hypothesis that it follows the same laws as Saturn's rings.
A breakthrough study by the University of Leicester team, led by Professor Nikolai Brilliantov, reveals that planetary rings have a universally similar particle distribution. The researchers solved the 'amazing' mathematical inverse cubes law of particle size distribution, suggesting that Saturn's rings are in a steady state that does ...
Scientists used Sandia's Z machine to verify the metallic phase of hydrogen, solving a long-standing discrepancy in Saturn's age. The experiment found that dense hydrogen can become atomic, releasing energy that could explain Saturn's temperature.
Researchers at MIT propose that Saturn's polar cyclones are caused by small thunderstorms building up angular momentum, leading to the formation of large and long-lasting vortices. The team developed a model that predicts which planets would form such cyclones based on two parameters: atmospheric energy and storm size.
Researchers mimicked the conditions of distant planets and stars using a laboratory technique, revealing how noble gases behave under extreme pressures and temperatures. This discovery sheds light on the atmospheric and internal chemistry of celestial objects, including the mystery of Saturn's internal heat emission.
A new system devised by Dr. Ravit Helled measures Saturn's rotation period, offering a more accurate determination of the planet's internal structure, weather patterns, and formation process. The method applies to other gas planets in the solar system, including Uranus and Neptune.
A new study by a team of Cassini mission scientists led by the University of Colorado Boulder has found evidence of hydrothermal activity on Enceladus, a Saturn moon with remarkable geologic activity. The tiny grains of rock detected near Saturn imply that seawater infiltrates and reacts with a rocky crust, emerging as a heated, minera...
Researchers found large patches of trace gases shining brightly near Titan's poles, with unexpected east-to-west variations. These findings are consistent with observations made by NASA's Cassini spacecraft, which found cloud caps and high concentrations of gases over the poles.
Scientists have found intriguing zones of organic molecules shifted away from Titan's north and south poles, contradicting expectations. The discovery may provide insights into the complex chemistry of Titan's atmosphere and its potential connection to Earth's early atmosphere.
Astronomers using Cassini data infer the presence of a potentially rugby ball-shaped rocky core or sloshing sub-surface ocean in Mimas. The moon's unusual wobble reveals surface displacement of up to 6 kilometers, contradicting predictions of uniform interior structure.
University of Leicester researchers captured stunning images of Saturn's auroras, providing evidence for the theory that Saturn's magnetic tail collapse causes auroral displays. The findings support a similar process on Earth.
Scientists studied the persistence of a hexagon-shaped atmospheric phenomenon on Saturn, which remains constant despite large radiative forcing in its atmosphere. The findings suggest that the hexagon is deeply rooted within Saturn's atmosphere and could reveal the planet's internal rotational period.
A recent discovery in Saturn's outer A ring has provided insight into the formation of moons. The 'Peggy' object, a small icy body, may be migrating out of the ring and becoming a new moon.
Researchers studied Saturn's northern polar region and confirmed the hexagon's stability and unchanged jet stream. They suggest it's a manifestation of a Rossby wave similar to those on Earth, with implications for understanding Saturn's atmosphere.
Astronomers have observed a miniature planet, Chariklo, with two rings of ice and pebbles located between Saturn and Uranus. The discovery was made using a new camera at the Danish telescope in Chile, which revealed two thin rings separated by 14 km.
Scientists have observed water ice and ammonia ice in Saturn's atmosphere for the first time. The new findings suggest that clouds of different chemical compositions can coexist, with water ice making up 22% and ammonia ice 55%.
Researchers found a negative correlation between gravity and topography signals on Titan, attributed to large roots extending into the ocean beneath the ice shell. The study suggests that Titan's ice shell is rigid and at least 40 kilometers thick.
Researchers have explained the behavior of Saturn's giant storms for the first time, using computer models and high-resolution images from the Cassini space probe. The storms are characterized by intense winds of up to 500 km/h and a turbulent ring with an enormous surface area.
A University of Iowa undergraduate student has discovered that Saturn's magnetosphere changes with the seasons, helping to clarify the planet's day length. The findings may alter our understanding of the Earth's magnetosphere and Van Allen radiation belts.
New research published in Nature Geoscience reveals how Saturn keeps itself looking young and hot due to gas layers preventing heat from escaping. This unique layering effectively insulates the planet, preventing heat radiating out efficiently.
Theoretical models demonstrate that gas giant planets can survive periodic outbursts of mass transfer from the gas disk onto the young star. These models show that Jupiter and Saturn could have formed through this process, supporting the presence of 20% of sun-like stars with gas giants.
A new analysis of Titan's topography and gravity data reveals the moon's icy outer crust is significantly thicker than previously estimated. This finding has significant implications for understanding Titan's ocean and internal structure.
Data from NASA's Cassini spacecraft show a shift in seasonal sunlight causing a sudden change in atmospheric circulation on Saturn's moon Titan. This unexpected turn reveals the key factor in Titan's atmosphere circulation is the slant of light, which led to sinking air at altitudes previously thought to be upwelling.
The Cassini mission has discovered a second feature shaped like the video game icon PAC-MAN on Saturn's moon Tethys. This finding confirms that high-energy electrons can dramatically alter icy satellite surfaces, and suggests that such anomalies may be widespread in the Saturn system.
Scientists have spotted a second Pac-Man thermal shape on Tethys, confirming that high-energy electrons can dramatically alter an icy moon's surface. The discovery suggests a more complex and varied process in the Saturn system.
Scientists have discovered a giant oval vortex on Saturn persisting long after the visible effects of the 'Great Springtime Storm' subsided. The vortex is characterized by high temperatures and unique chemistry, unlike Jupiter's famous Great Red Spot.
Researchers at NASA's Goddard Space Flight Center detected a massive release of ethylene gas during a rare storm on Saturn, with temperatures soaring 150 degrees Fahrenheit above normal. The storm was observed using Cassini's composite infrared spectrometer and revealed unprecedented disturbances in the planet's upper atmosphere.
A new model proposes that the Saturn system originated from giant impacts in which several major satellites merged to form Titan, resulting in the formation of Saturn's middle-sized moons. The model suggests these moons were formed from ice-rich material similar to Titan's mantle and have active geology and dynamics.