Articles tagged with Planetary Rings
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.
Astronomers have discovered a new insight into how planets form, using high-powered telescopes to target the star V1247 Orionis. The team found a dust-trapping vortex that could protect sites of planet formation, allowing dust particles to clump together and grow.
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.
An international team of astronomers led by University of Warwick discovered a giant gas planet up to 50x Jupiter's mass with rings, causing regular eclipses of the young star PDS 110 in Orion constellation. The next eclipse is predicted for September, allowing amateur astronomers to witness and gather new data.
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 propose that debris from an asteroid impact could have formed Mars' rings, which would then break apart and re-form into moons. The model suggests that this cycle may repeat, potentially explaining sedimentary deposits found on Mars.
The supernova has continued to fascinate astronomers with its spectacular light show, located in the nearby Large Magellanic Cloud. Recent studies using NASA's Hubble Space Telescope and Chandra X-ray Observatory have provided unique insight into the early stages of gas dispersal after a star's death.
Researchers have mapped gases in three dark rings around a distant star, indicating the presence of planets that are clearing dust and gas from the outer rings. However, one inner ring remains mysterious, with more carbon monoxide than expected, leaving scientists to investigate alternative explanations for its formation.
Researchers have discovered complex systems of concentric rings surrounding young stars, formed by the interaction between protoplanetary discs and growing planets. These findings provide new insights into planet formation, shedding light on the dynamics of innermost disc regions.
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.
A team of citizen scientists and professional astronomers have discovered an unusual exoplanet hunting ground, finding the oldest known circumstellar disk orbiting a young star. The discovery, led by Steven Silverberg, reveals a red dwarf star with a warm disk that has sustained its disk for an exceptionally long time.
A team of researchers has shed light on the origin of centaur rings, revealing a scenario where tidal disruptions lead to disc formation and ring creation. The study suggests that rings around centaurs are more common than previously thought, with many awaiting discovery.
Astronomers have discovered a ring structure of complex organic molecules around a Solar-type protostar, providing direct evidence that interstellar materials are fed into the rotating disk structure. The distribution of these molecules reveals new perspectives on planetary system formation and chemical composition.
Researchers create synthetic ring teeth proteins with varying repeats to achieve programmable materials with improved strength and flexibility. These self-healing polymers can be tailored for specific properties, such as elasticity and plasticity, making them suitable for various applications in textiles, cosmetics, and medicine.
A newly discovered exoplanet, HD 106906 b, may have been violently ejected from its birthplace close to its star due to a recent gravitational disturbance. The planet is surrounded by a large dust ring or shroud, which could be evidence of the violent episode.
Phobos will likely break apart and form a ring around Mars due to tidal forces. The debris from Phobos will continue to orbit Mars for millions of years before eventually colliding with the planet.
A team of astronomers used data from the VLT to study the remains of an asteroid around a stellar remnant -- a white dwarf. They discovered an orbiting disc of gaseous material and found that it is lopsided and has not yet become circular.
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.
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 ...
Astronomers using NASA's Swift satellite have discovered concentric X-ray rings centered on a black hole, which form due to the 'echo' effect of light traveling through dust layers. The findings provide insights into the normally invisible interstellar dust and allow for better understanding of the black hole's behavior.
Researchers have developed a new method to estimate distances to X-ray sources using the geometry of light echoes and dust clouds. By analyzing the timing and deflection of X-rays as they pass through interstellar space, astronomers can calculate the distance to Circinus X-1, a binary system located in the plane of the galaxy.
Researchers have discovered a young planetary system with a ring-like disk of debris surrounding a Sun-like star, sharing similarities with the formation of our own early solar system. The disk is roughly the same size as our solar system's Kuiper Belt and may contain dust and icy particles.
A team of researchers from MIT has detected optical features around Chiron that may signal the presence of a ring system, jets, or a shell of dust. The findings are based on observations of a stellar occultation in 2011, which revealed symmetrical and sharp features near the start and end of the event.
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.
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.
Researchers find that debris disks can produce narrow rings on their own, without the presence of a planet. Gas and dust interactions lead to clumping and pattern formation, making it harder for astronomers to detect planets.
The TWINS mission has provided three-dimensional images and global characterization of the magnetosphere, tracking how it responds to space weather storms. The stereo imaging has revealed details on ion movement and escape patterns, helping scientists understand the ring current's behavior.
Astronomers discovered a mysterious planet circling the nearby star Fomalhaut with an unusual elliptical orbit. The team hypothesizes that another undetected planet may have gravitationally ejected Fomalhaut B, sending it on a collision course with a vast dust ring.
A new analysis of Hubble observations suggests Fomalhaut b is a rare, uniquely massive planet shrouded by dust. The team found the planet remained at constant brightness, contradicting earlier interpretations of it as a transient dust cloud.
Astronomers have discovered an extraordinary amount of dust around a nearby star that has mysteriously disappeared. The dusty disc was bigger and more massive than Saturn's rings and would have extended from the sun halfway out to Earth if it were in our solar system.
Scientists have discovered strange half-mile-sized objects leaving glittering trails behind them as they punch through parts of Saturn's F ring. These 'mini-jets' fill in a missing link in our understanding of the curious behavior of the F ring, showing that smaller snowballs can survive and strike through the ring on their own.
Astronomers at the University of Florida have discovered two low-mass planets orbiting the nearby star Fomalhaut. Using ALMA's superior resolution and sensitivity, they found that the ring of dust surrounding the star is shaped by two planets working together to maintain its narrow width.
The ALMA observatory has discovered a nearby planetary system with sharp-edged dust ring, indicating 'shepherding' planets that keep the disk within their gravitational effect. The planets are smaller than previously thought, about the size of Mars to a few times the Earth, and are among the coldest planets found orbiting a normal star.
A team of astrophysicists discovered a ring system in the constellation Centaurus that is similar to Saturn's. The system consists of four thin rings of dust debris, with each ring having a mass similar to Earth's moon, and orbits tens of millions of kilometers from the central star.
Voyager 1 has sailed to the edge of the solar system and is expected to punch its way into interstellar space in the coming months or years. The spacecraft was launched in 1977 and completed the Grand Tour of the Solar System, making numerous groundbreaking discoveries about the outer planets and their moons.
Physicists have found that supersolid helium has liquid-like characteristics, contradicting previous assumptions of a solid state. The researchers attribute this behavior to moving defects in the crystal structure, which relax at higher temperatures.
Simulations suggest Saturn's rings and inner moons formed after a massive satellite collided with the planet. The resulting debris formed the icy rings and ice-rich inner moons.
An international team of astrophysicists has created the most complete atlas of nuclear rings, which are enormous star-forming ring-shaped regions that circle certain galactic nuclei. The catalogue includes 113 such rings in 107 galaxies and provides insights into their properties and relationships with galaxy structure.
The Cassini spacecraft has provided stunning insights into Saturn's ring system, showing routine collisions and debris trails. The rings are composed mostly of water ice, with a mysterious reddish contaminant that could be rust or small organic molecules.
During Saturn's equinox, light hits the ring particles at low angles, giving a three-dimensional view of the rings. The CIRS instrument on board the Cassini spacecraft observed record-low temperatures of 382 degrees below zero Fahrenheit in the A-ring.
The Swift satellite has acquired the highest-resolution view of the Andromeda Galaxy in ultraviolet light, capturing over 20,000 ultraviolet sources. The galaxy's star-formation processes can now be studied in greater detail than previously possible with the help of three ultraviolet filters.
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.
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.
Researchers used NASA's Thunderhead supercomputer to simulate dusty disks around sunlike stars, finding that planets as small as Mars can create detectable ring structures. The models provide a way to infer a planet's mass and orbital distance based on dust particle simulations.
Researchers from the University of Maryland and Max-Planck Institute found that Jupiter's outermost ring is extended beyond Thebe's orbit due to dust particles' electric charges interacting with the planet's magnetic field. This phenomenon affects any planet's rings, shedding light on planetary formation.
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.
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.
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.
The New Horizons spacecraft provided detailed observations of Jupiter's atmosphere, revealing new insights into cloud structure and composition. The mission also explored the planet's four largest moons, including Io, which showed over 20 geological changes since the last close-up look.
For the first time since their discovery in 1977, astronomers have observed a Uranus ring crossing and detected significant changes in the rings' arrangement. The observations used advanced telescopes and revealed new details about the fine dust that permeates the rings, including a previously unseen outer ring.
Astronomers have discovered a young star with an elliptical ring that is likely caused by the presence of an undiscovered Neptune-sized planet. The ring is offset by 1.4 billion miles, more than 15 times the distance from Earth to the Sun.
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 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.
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.