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Protoplanetary Disk

All articles tagged with #protoplanetary disk

Isotopes Trace Interstellar Visitor 3I/ATLAS to Ancient, Metal-Poor Disk
astronomy4 days ago

Isotopes Trace Interstellar Visitor 3I/ATLAS to Ancient, Metal-Poor Disk

Astronomers using ESO's Very Large Telescope measured carbon and nitrogen isotope ratios in the interstellar comet 3I/ATLAS, finding carbon-12/carbon-13 ~151 and nitrogen-14/nitrogen-15 ~363. These values are higher than typical solar-system comets, suggesting formation in the cold outer disk around an older, metal-poor star, consistent with isotope-selective chemistry in such environments. The results, published online July 6, 2026 in Nature Astronomy, provide a rare glimpse into material from another planetary system and the efficiency of planetesimal formation around ancient stars.

Interstellar comet 3I/ATLAS reveals outer-disk isotopic fingerprints
space4 days ago

Interstellar comet 3I/ATLAS reveals outer-disk isotopic fingerprints

Astronomers measuring CN isotopologues in the interstellar comet 3I/ATLAS find unusually high 12C/13C (~151) and 14N/15N (~363) ratios, higher than Solar System comets and closer to interstellar/outer-disk values, implying 3I formed in the outer disk around an old, low-metallicity star and offering rare clues about planetesimal formation under different stellar environments.

Ancient interstellar comet 3I/Atlas reveals alien chemistry
science8 days ago

Ancient interstellar comet 3I/Atlas reveals alien chemistry

Astronomers using JWST spectroscopy found that interstellar comet 3I/Atlas has a chemical makeup unlike any solar-system object, with high CO2 and low NH3 and distinctive isotope fingerprints (D/H and 12C/13C) indicating formation in a very cold protoplanetary disk around an ancient star roughly 12 billion years ago; as only the third known interstellar object, 3I/Atlas provides a fossil record of planetary systems in the early Milky Way, and upcoming surveys (like NEO Surveyor and the Rubin Observatory) are expected to uncover more such visitors.

Astronomers Spot a Ring That Could Be a Cosmic Planet Factory
space1 month ago

Astronomers Spot a Ring That Could Be a Cosmic Planet Factory

Astronomers have detected a prominent ring in the disk around a young star, seen as a likely site where planets form. The ring’s structure and gaps suggest ongoing planet-building activity within a protoplanetary disk, offering new clues about how planetary systems originate, though follow-up observations are needed to confirm active planet formation inside the ring.

Hubble Reveals the Biggest Chaotic Planet-Forming Disk Yet
space2 months ago

Hubble Reveals the Biggest Chaotic Planet-Forming Disk Yet

NASA's Hubble Space Telescope captured the sharpest visible-light images yet of a colossal, highly irregular protoplanetary disk around a young star about 1,000 light-years away, nicknamed Dracula’s Chivito. The disk spans roughly 400 billion miles (about 40 times the solar system’s diameter to the Kuiper Belt) and is filled with massive, uneven filaments and wisps, suggesting turbulent accretion or external influences. With a mass estimated at 10–30 Jupiter masses, it could form several giant planets, underscoring that planet formation can be far more chaotic and dynamic than traditional models suggest. Future observations may reveal whether the central star is single or binary and shed light on how such extreme environments shape emerging planetary systems.

JWST Uncovers Clues to the Birth of a Giant Exoplanet
space2 months ago

JWST Uncovers Clues to the Birth of a Giant Exoplanet

Using JWST imaging of 29 Cygni b, a ~15-Jupiter-mass exoplanet about 133 light-years away, researchers find the planet is unusually metal-rich and its orbit aligns with its star, suggesting it may have formed in a protoplanetary disk via bottom-up accretion rather than simple direct collapse. This links the formation of some of the Milky Way’s most massive planets to the same disk-based processes that birth smaller worlds.

WISPIT 2: A Young Solar System Taking Shape
space3 months ago

WISPIT 2: A Young Solar System Taking Shape

Astronomers directly observed two planets forming around the very young star WISPIT 2, about 437 light-years away. A distant giant, WISPIT 2b, sits at 57 AU with ~5 Jupiter masses, while a closer planet, WISPIT 2c, lies at 14 AU with 8–12 Jupiter masses. The system’s disk shows multiple rings and gaps, hinting at a possible third planet and offering a rare glimpse into how our Solar System may have formed; future imaging with the Extremely Large Telescope could reveal more.

Budding planets around a newborn star reveal early solar-system formation
space3 months ago

Budding planets around a newborn star reveal early solar-system formation

Astronomers studying the young star WISPIT 2, located about 437 light-years away and ~5.4 million years old, have directly detected two forming planets—WISPIT 2b and WISPIT 2c—in the star’s surrounding protoplanetary disk, carving gaps as they grow. Hints of a third planet farther out have researchers hopeful, and the system offers a rare look at how solar systems like our own form; observations via the VLT (with SPHERE and GRAVITY+ upgrades) suggest future clues may be revealed by the ELT.

Hubble Spots Giant, Turbulent Planet-Forming Disk 40 Times Wider Than Our Solar System
astronomy5 months ago

Hubble Spots Giant, Turbulent Planet-Forming Disk 40 Times Wider Than Our Solar System

NASA’s Hubble Space Telescope has captured the largest known protoplanetary disk around the young star IRAS 23077+6707 (nicknamed Dracula’s Chivito), extending about 400 billion miles—roughly 40 times the Solar System’s diameter. Seen nearly edge-on in visible light, the disk is unusually turbulent and asymmetric, with filament-like features on one side and a sharp edge on the other, hinting at dynamic infall of material and environmental interactions. With an estimated mass 10–30 times Jupiter’s, the system may host a large planetary system and provides a valuable laboratory for understanding planet formation in extreme conditions.

JWST traces crystal seeds from a newborn star to its outer disk
space5 months ago

JWST traces crystal seeds from a newborn star to its outer disk

NASA’s James Webb Space Telescope mapped where crystalline silicates form around the young star EC 53 in the Serpens Nebula and showed these minerals being carried outward by winds into the outer, planet-forming disk. EC 53 undergos ~18-month bursts lasting about 100 days, forging silicates in hot regions and launching them into cooler outer regions, effectively seeding the outer disk with components that icy comets may carry—providing a direct link between crystal formation and distribution in early planetary systems. The findings, published in Nature, help explain how comets at the solar system’s edge could form.

Webb Discovers Crystalline Silicates Forged in Inner Disk of Young Star, Flung to Disk Edges
space5 months ago

Webb Discovers Crystalline Silicates Forged in Inner Disk of Young Star, Flung to Disk Edges

NASA’s James Webb Space Telescope observed protostar EC 53 in the Serpens Nebula and confirmed that crystalline silicates form in the hot inner disk, with MIRI spectra identifying minerals like forsterite and enstatite. The star’s strong disk winds and periodic outbursts appear to launch these crystals outward toward the disk’s edges, offering a mechanism for crystalline silicates found in comets and potentially seeding planet formation during the system’s ongoing evolution.

Cosmic Hamburger Disk Reveals Birthplace of Distant Giant Planets
space5 months ago

Cosmic Hamburger Disk Reveals Birthplace of Distant Giant Planets

Astronomers using ALMA have imaged Gomez’s Hamburger (GoHam), one of the largest edge-on protoplanetary disks, finding a stratified arrangement of gas and dust and signs of ongoing planet formation, including a potential giant-planet core or clump dubbed GoHam b in the outer disk. The disk’s sheer size and uneven features—such as a bright, lopsided region and a northern wind—make it an ideal laboratory to study how giant planets can form far from their star and how such planets shape their surroundings.