Articles tagged with Protoplanets
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Scientists observe violent collisions around young star Fomalhaut, detecting the aftermath of two powerful collisions over a 20-year period. The collided objects are estimated to be at least 60 kilometers across and may have formed planets.
NASA's Hubble Space Telescope captured a cosmic fender bender, revealing two luminous clouds of debris from violent collisions between space rocks. The discovery offers insights into planet formation and asteroid composition, shedding light on the structure of asteroids crucial for planetary defense programs.
Experimental tests demonstrate that interactions between magma oceans and primitive atmospheres during early years can produce significant amounts of water. This process has major implications for the physical and chemical properties of planets' interiors, with potential effects on core development and atmospheric composition.
Researchers have created a new model that shows how planet formation timing influences planetary composition and density. The study suggests that older, rocky planets are less dense than younger ones due to the varying lifetimes of stars.
Astronomers have identified a rogue planet with a mass five to 10 times that of Jupiter, growing at an unprecedented rate of six billion tonnes per second. The discovery provides valuable insights into the formation and growth of rogue planets, suggesting they may share a similar path to star formation.
New research finds Mars' mantle preserves a record of its violent beginnings, with chunky layers containing ancient fragments up to 4km wide. This discovery offers a rare glimpse into the evolution of rocky planets and challenges current understanding of planetary formation.
Astronomers have detected a growing planet outside our solar system in a cleared gap of a multi-ringed disk of dust and gas. The discovery provides the first direct evidence that protoplanets can create these gaps, resolving a long-standing debate in the scientific community.
A study by researchers at UC Santa Barbara, Yale University and others found that a third of young stars have misaligned rotational axes with their protoplanetary disks. This challenges centuries-old assumptions about the alignment of stars and planets in our solar system and suggests that some stars may be born tilted.
Researchers have detected planet-forming 'pebbles' around two young stars, DG Tau and HL Tau, revealing large reservoirs of pebbles out to at least Neptune-like orbits. This discovery offers an early glimpse into the formation of planetary systems and may help understand how planets are formed.
Researchers analyzing the atmosphere of WASP-121b using the James Webb Space Telescope detected water, carbon monoxide and silicon monoxide in both the dayside and nightside hemispheres. This is the first conclusive identification of SiO in any planetary atmosphere.
Dr. Robin Canup, a leading expert in planetary science, has received the 2025 AAS DDA Dirk Brouwer Career Award for her groundbreaking research on planet and satellite formation, including the Earth-Moon system's origins.
Researchers use NASA's James Webb Space Telescope to investigate a protoplanetary disk around a young star in the Lobster Nebula. They found sufficient solid material to potentially form at least 10 rocky planets and detected various molecules that contribute to planetary atmospheres.
The Magellan Adaptive Optics Xtreme (MagAO-X) instrument observed two young planets orbiting PDS 70, revealing compact rings of dust and startling changes in brightness. The team believes these features are telltale signs of the planet's turbulent youth.
Advanced simulations reveal that PMOs form directly from disk interactions, inheriting material and moving synchronously with host stars. This discovery reshapes our understanding of cosmic diversity, suggesting a new class of objects born from gravitational chaos.
A new collaboration between ASU, MSU, and LLNL aims to answer the question of how planets form by analyzing the atmospheres of seven young exoplanets. The team will use the James Webb Space Telescope and powerful computers to create atmospheric models that can reveal insights into planetary formation and evolution.
A new study reveals that first-generation planetesimals in the inner solar system were rich in moderately volatile elements, which were later lost during violent cosmic collisions. This discovery reshapes our understanding of how planets acquired their ingredients.
Researchers at University of Maryland have discovered that the South Pole-Aitken basin, the moon's oldest and largest visible crater, is more circular than previously believed. The team used high-resolution data to analyze mountain formations around the basin, revealing a rounder shape indicating a more vertical impact angle.
A study published in Science Advances suggests that unmelted asteroids, or 'primitive' materials, were a crucial source of volatiles on Earth. This finding implies that the materials necessary for life to emerge may not have been readily available without these unmelted asteroids.
Two UMD Astronomy space probes, AXIS and PRIMA, have advanced to the next round of consideration for a $1 billion NASA mission. AXIS will study X-rays from stars and black holes, while PRIMA will explore far-infrared radiation to understand galaxy formation.
Research led by Heidelberg University reveals that small water-rich astronomical bodies in the early solar system supplied building materials for planets, including the Earth. These planetesimals brought water to Earth through their thermal evolution and point of origin.
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.
Scientists have discovered a new planet called WASP-193b that is 50% bigger than Jupiter yet has a density comparable to cotton candy. The planet's low density makes it an outlier among the over 5,400 planets discovered so far.
A new study using the James Webb Space Telescope has captured the first-ever image of a planet-forming disk's gas dispersal, providing insights into how planets form in our solar system. The observations reveal that the inner disk of T Cha is evolving on very short timescales, differing from earlier spectra detected by Spitzer.
A team of astronomers has shed new light on the process of planet formation through a groundbreaking survey of over 80 young stars. The research provides a wealth of data and unique insights into how planets arise in different regions of our galaxy, revealing diverse patterns of planet-forming discs.
The samples from Wild 2 comet have revealed a record of the solar system's dynamic formative years, shedding light on the events that shaped its history. Researchers have found unusual carbon-iron assemblages and precursors to igneous spherules in the comet material.
Researchers found that iron meteorites from the inner and outer solar systems had similar amounts of missing iron metal, suggesting that water was present in planetesimals right from the start. This challenges current models, which predict cooler temperatures for the inner solar system or formation further out.
Researchers propose that ancient planet Theia collided with Earth billions of years ago, forming two continent-sized blobs of unusual material and the Moon. The blobs, known as large low-velocity provinces (LLVPs), are rich in iron and likely composed of different proportions of elements than the mantle surrounding them.
A new SwRI study posits that the large mounds on Kuiper Belt object Arrokoth are similar in size and shape, suggesting a common origin. This finding supports the streaming instability model of planetesimal formation, where gentle collision speeds allowed objects to accumulate and form Arrokoth.
A new study has captured the early stages of planetary evolution, observing a young gas planet's violent and erratic atmospheric shedding. The research, led by Dartmouth researchers, provides insights into the most common experiences of planets beyond our solar system.
Research suggests that larger cosmic dust aggregates are less likely to stick together after collisions. This limits the growth of planetary building blocks, complicating the process of planet formation. Simulations reveal that size is a critical factor in determining sticking probability, with larger aggregates more prone to bouncing.
Using ALMA, astronomers have found evidence of a cloud of debris that might be the building blocks of a new planet or the remnants of one already formed. This discovery would confirm the existence of Trojan planets outside our Solar System, which are rocky bodies sharing the same orbit as a planet.
A study by Caltech scientists reveals that Earth primarily consisted of dry, rocky materials during its early stages, with a major addition of life-essential volatiles occurring only in the last 15% of its formation. This finding provides crucial insights into the planet's formation process and has important implications for theories o...
A study at Europlanet Science Congress 2022 found that super-thin planet nurseries can accelerate the formation of big planets. The team observed a remarkably thin disc of dust and gas around a young star, where large particles settled into a dense midplane, creating conditions favourable for planetary growth.
Researchers have uncovered the truth behind the missing volatiles in meteorites, revealing a massive shockwave phenomenon that stripped elements from planetary building blocks. This finding has significant implications for our understanding of Earth's geochemical evolution and the Solar System's youth.
A new study found that krypton isotopes in the deep mantle reveal a clearer picture of Earth's formation, contradicting the popular theory of volatile elements arrival. The research suggests that planetesimals from the cold outer solar system bombarded the Earth early on.
Scientists have made new discoveries about the early solar system using meteorite glass beads. By analyzing the isotopic compositions of elements in these beads, researchers were able to determine that massive shockwaves passing through the nebula caused the extreme heating and cooling necessary for chondrule formation.
Researchers used TRAPPIST-1's harmonious orbits to determine the impact history of its seven Earth-sized planets. The study found that these planets could have withstood only limited late bombardment, implying a relatively small amount of water arrived on time for potential life.
A new desalination process removes nearly 100% of toxic metals, producing clean water while capturing valuable metals. An infant-warming device reduces neonatal mortality rates by threefold in Rwanda, proving safe and effective without electricity.
Researchers found a 4.565 billion-year-old meteorite with an andesite crust, unlike known asteroids, suggesting andesitic crusts may have been common in early protoplanets.
A team of researchers discovered that the early Solar System formed in two distinct steps, resulting in different planetary compositions and evolutionary paths. The study explains why the inner planets are small and dry, while the outer planets are larger and wet.
A young star, HL Tauri, is producing planets from its concentric rings made of gas and dust. Research by Mayer Humi provides a study target for protoplanetary ring theories around stars, shedding light on the creation of solar systems.
A team of scientists at MIT and elsewhere has determined that a family of oddball meteorites likely came from an early planetesimal with a magnetic core. The discovery suggests that the diversity of the earliest objects in the solar system may have been more complex than previously thought.
Researchers found evidence of internal melting and differentiation in a carbonaceous meteorite, suggesting that primitive bodies started forming core, mantle, and crust structures. The study connects this process to highly differentiated iron meteorites through isotopic signatures.
Researchers from Curtin University analyzed volcanic meteorites from Antarctica to understand Asteroid Vesta's geological history. The study found that Vesta was volcanically active for at least 30 million years after its formation, contradicting previous models and suggesting pockets of magma survived on the asteroid.
Three studies provide new insights into the composition and origin of Arrokoth. The object's binary lobes were likely formed in a local collapse cloud, with an ancient age of about 4 billion years. Its surface is uniformly red, cold, and covered with methanol ice and complex organic molecules.
Scientists modeled early impact events on Mars, revealing a heterogeneous mantle and challenging previous estimates of the planet's formation time. The new research provides insight into the Red Planet's evolution and composition.
Astronomers discovered a giant Jupiter-like exoplanet orbiting a small red dwarf star, defying standard planet formation theories. The exoplanet, GJ 5312b, is nearly half as massive as Jupiter and orbits the tiny star with an eccentric 204-day orbit.
Astronomers detected a massive planet, GJ 3512b, orbiting the small red dwarf star GJ 3512, defying predictions of theoretical models. The discovery poses questions about planetary formation mechanisms and encourages further research.
A Southwest Research Institute-led team studied the orientation of distant solar system bodies in binary pairs, providing insights into planet formation. Most Kuiper Belt objects (80%) orbit in a prograde direction, contradicting theories on binary formation and supporting the streaming instability hypothesis.
A new study reveals the first intact planetary body orbiting a white dwarf star, with a densely packed planetesimal no larger than 600 kilometers in diameter. The object's high density suggests it may be the remnant core of a planet stripped away by tidal forces.
SwRI leads largest-ever Hubble survey of the Kuiper Belt, focusing on binary populations and testing planetesimal formation theories. The Solar System Origins Legacy Survey aims to understand solar system architecture and planetary evolution.
The study confirms the evolution of transits produced by a planetesimal orbiting the white dwarf WD 1145+017. The system shows periodic transits blocking light from the star, with continuous interaction and fragmentation resulting in changes in transit depth and shape.
Melt drainage through percolation continues even with low melt fractions, suggesting all but 1-2% of melt can be drained. This process enables planetesimal core formation.
A giant gas giant planet, NGTS-1b, has been discovered orbiting a tiny star, defying conventional formation theories. The planet's proximity to its star and short orbital period pose significant challenges for understanding the origins of such massive worlds.
A group of dark asteroids with related orbits have been identified as part of a previously unknown family, estimated to be roughly 4 billion years old. The discovery provides valuable information on the size distribution of original planetesimal bodies and challenges traditional theories of asteroid formation.
A new study estimates that the asteroid that formed the Moon's Imbrium Basin was likely a protoplanet-sized object, two times larger in diameter and 10 times more massive than previous estimates. The research also sheds light on the geological features surrounding the basin, which help explain some of its puzzling characteristics.
Researchers found two gaps in the gas disk that overlap with dust gaps, suggesting infant planets carve out the gaps. The team estimates a planet mass 0.8 times Jupiter's at the inner gap, but the outer gap's origin remains unclear.
Dr. Bill Ward, a renowned planetary scientist, was elected to the National Academy of Sciences for his groundbreaking research on the origin and evolution of the Moon and other celestial bodies. His work has significantly contributed to our understanding of planetary science and the formation of our solar system.
A study suggests that Planet Mercury's unusual metal-rich composition is a result of early hit-and-run collisions with larger planets. This process could have stripped away Mercury's mantle without intense shock, leaving behind a mostly-iron body.
The discovery of HD 106906 b, a giant planet orbiting its star at 650 times the average Earth-Sun distance, has puzzled astronomers. The planet's unusual orbit and mass throw doubt on existing planet formation theories, leaving scientists searching for alternative explanations.