Articles tagged with Interstellar Medium
Researchers at Aarhus University have demonstrated that protein building blocks essential for life as we know it form readily in space. Peptides, which bond amino acids together, were found to react with each other to form proteins on dust particles.
Scientists studied the effects of two hot stars, Epsilon and Beta Canis Majoris, on the local interstellar clouds around our solar system. The team found that these stars' ultraviolet radiation ionized about 20% of the hydrogen atoms and 40% of the helium atoms in the clouds.
A study by Stockholm University revealed a planet-forming disk with an unexpectedly high abundance of carbon dioxide, challenging long-standing assumptions about planetary birthplaces. The discovery was made using the James Webb Space Telescope and suggests intense ultraviolet radiation may be reshaping the chemistry of the disk.
Researchers detected sulfur in both gas and solid phases using data from the XRISM spacecraft, providing unprecedented insight into its presence in the universe. The findings are based on measurements of X-rays from two binary star systems and suggest that sulfur can easily change between these forms.
Researchers discovered an unexpectedly complex and dynamic filamentary network within a very-high-velocity cloud (VHVC) in the Milky Way using the FAST telescope. The study found that the cloud is primarily composed of warm neutral medium (WNM), with little or no cold component, suggesting a cleaner, earlier phase in cloud evolution.
The CoDICE instrument will measure energized interstellar and solar particles to better understand the boundary of the heliosphere. The instrument will also characterize solar wind ions and the mass and composition of highly energized solar particles associated with flares and coronal mass ejections.
Researchers surveyed luminous infrared galaxies to gain insight into galaxy formation in the early universe and possibly the Milky Way. They discovered massive clumps of newborn stars, unlike anything seen in the Milky Way.
Researchers find over 500 dense star-forming cores with possible protoplanetary disks in the Milky Way's Central Molecular Zone. Dual-band observations reveal unexpected spectral reddening, suggesting the presence of these early stages of solar system formation.
A new computer model simulates magnetism and turbulence in the interstellar medium, providing unprecedented detail on the Milky Way Galaxy's overall magnetic field. The model also helps understand star formation and the propagation of cosmic rays, offering insights into astrophysical phenomenon.
The study provides a new look at the galactic region surrounding our solar system, revealing a roughly uniform background Lyman alpha sky brightness. The findings suggest hot interstellar gas bubbles may be regions of enhanced hydrogen gas emissions at a wavelength called Lyman alpha.
A team of Australian scientists has performed a CT scan of the interstellar medium using a scintillating pulsar, mapping previously unseen layers of plasma. The study reveals an unexpected abundance of compact plasma blobs within the Local Bubble and measures the three-dimensional shape of a bow shock for the first time.
Researchers from the Institute of Physical Chemistry, Polish Academy of Sciences, have identified unusual phosphorus molecules in space. These molecules, including phosphabutadiyne and vinylphosphaethyne, were studied using cryogenic techniques and infrared spectroscopy, providing new insights into their formation and properties.
Astronomers have created a detailed 3D map of dust in the Milky Way galaxy, providing new insights into the effects of dust on celestial observations. The map reveals unexpected properties of interstellar dust clouds, including a steepening extinction curve in areas of intermediate density.
Three UK researchers will receive a £100,000 (US$126,000) prize at the 2025 awards, honouring their work in Life Sciences, Chemical Sciences, and Physical Sciences & Engineering. The winners were selected from 94 nominees representing 45 academic institutions.
Adam Leroy, a professor of astronomy at Ohio State University, has been recognized with the 2025 Henry Draper Medal for his groundbreaking work on the interstellar medium and its relationship to star formation in nearby galaxies. His research has provided unprecedented detail on the physical nature of this material, advancing our under...
Astronomers studying two distant galaxies in the early universe reveal unprecedented molecular diversity, shedding light on the lives of prodigious star factories. By analyzing light from over 13 molecules, researchers gain insights into the physical and chemical conditions in these galaxies.
A young star cluster, IRS13, has been found to be significantly younger than expected, with stars only 100,000 years old, despite being near the supermassive black hole Sgr A*. The cluster's turbulent history suggests it was 'captured' by the black hole's gravity, leading to a bow shock and increased star formation.
Researchers at Breakthrough Listen project have devised a new technique for finding and vetting possible radio signals from other civilizations. The technique eliminates the possibility of signal being mere radio interference from Earth, boosting confidence in future detection of alien life.
Astronomers have developed a more accurate method to measure the composition of galaxies using data from telescopes on Earth and in space. By correcting for temperature fluctuations, researchers found that the result from collisionally excited infrared lines is still 50% less than that from recombination line method.
Scientists measured and compared amino acid abundances with rocky components of Ryugu particles, demonstrating water's role in their formation. The results suggest more ice was present in the precursor of one particle than the other, which may have contributed to the high abundance of a specific amino acid.
Researchers Jennifer Bergner and Darryl Seligman suggest that 'Oumuamua's acceleration can be explained by the outgassing of hydrogen gas as the comet warmed up in the sunlight. The comet's small size allowed for a significant effect, with the tiny push from hydrogen spurted out of ice altering its gravitational deflection around the sun.
A team of researchers has discovered a wide range of nitriles, key molecular precursors for life, in the interstellar molecular cloud G+0.693-0.027 near the Milky Way center. The study provides important insights into the chemical ingredients available in the nebula that give rise to our planetary system.
Researchers from the University of Arizona suggest that dying stars can forge carbon nanotubes in the envelopes of dust and gas surrounding them. This process involves the spontaneous formation of carbon nanotubes, which are highly structured rod-like molecules consisting of multiple layers of carbon sheets.
A new technique has identified previously hidden protoclusters that could reveal new details about galaxy evolution. The ancestors of large galaxy clusters were found to be hiding in plain sight, with some protoclusters harboring unseen galaxies that evolved differently.
The samples returned from the Hayabusa2 mission provide valuable insights into the formation and evolution of our solar system. The study found that Ryugu contains hydrated minerals and evidence of freeze-thawing, indicating that it experienced both liquid and frozen water in its past.
Recent studies suggest that cosmic rays, originating from supernova remnants and pulsars, have a significant impact on galactic dynamics and star formation. The streaming instability triggered by cosmic rays in the interstellar medium can create plasma waves that heat and scatter gas, influencing the formation of planets and stars.
Researchers have discovered a persistent signature of plasma waves in the interstellar medium using Voyager 1's Plasma Wave System. The detection allows scientists to understand how the solar wind interacts with the interstellar environment.
Researchers directly observed C+S2 product channel from CS2 photodissociation using Dalian Coherent Light Source. The study provided evidence for the origin of interstellar medium S2 fragments and demonstrated that they could be generated from CS2 photodissociation
A research team from Friedrich Schiller University Jena has proven that dust particles and ice are mixed in the interstellar medium. This finding suggests complex organic molecules may be present on dust particles, which can contribute to planetary formation. The study also reveals a hidden reservoir of oxygen in solid-state water.
Researchers at Princeton Plasma Physics Laboratory have developed the first fully kinetic model of plasma behavior, demonstrating that fast magnetic reconnection can occur in partially ionized systems. This finding has implications for understanding auroras and the formation of stars.
Researchers observe intense gas motions at filament junctions, indicating strong acceleration gradients and massive core formation. The study reveals that interstellar filaments and hub systems are privileged locations for forming the most massive stars in the Galaxy.
Astronomers observe how massive forces create shock waves in interstellar medium, leading to X-ray and radio emissions. The study provides insight into galactic proportions, allowing researchers to see event across electromagnetic spectrum.
A study by an international team solves the origin of successive generations of stars in globular clusters. The most massive, evolved AGB stars are found to contaminate the interstellar medium, giving rise to new generations of stars.
Researchers have found a unique triple-bubble structure in the interstellar medium of galaxy M33, consisting of three concentric supernova shells. This discovery provides insights into the complex feedback processes that govern star formation and the dissemination of metals produced in massive stars.
Scientists from the University of Tokyo have detected silicon and nitrogen-terminated carbon chain molecules in interstellar space using laboratory experiments. The discovery provides valuable information on the formation mechanisms of these molecules and their potential impact on understanding the chemical composition of the universe.
Researchers from Max Planck Institute and Cornell University detect iso-propyl cyanide, a branched carbon molecule, in a giant gas cloud called Sagittarius B2. The discovery opens a new frontier in the complexity of molecules found in regions of star formation.
Researchers at Lund University found that toothpaste fluorine is formed in stars similar to our sun, supporting a theory about its origins. By analyzing light emitted by stars, they calculated the amount of fluorine present and compared it with predictions.
The study found that the heliosphere moves through the interstellar medium at about 52,000 miles per hour, slow enough to create a bow wave rather than a shock. This new data contradicts previous theories and has implications for how galactic cosmic rays propagate around the solar system.
Researchers using IBEX data measure neutral 'alien' particles entering our solar system, revealing their speed, direction, and interaction with the heliosphere. The findings provide insights into the local interstellar medium, galaxy distribution of elements like oxygen and neon, and the future trajectory of the Sun's planetary system.
Researchers at UH Manoa have discovered a novel chemical route to form PAHs, challenging conventional wisdom that they only occur at high temperatures. The study suggests that low-temperature chemistry can initiate the synthesis of the first PAH in interstellar space.
Researchers from Johns Hopkins University present a new view of the region of the sun's influence, suggesting that the heliosphere may not have a comet-like shape. The Cassini spacecraft's images reveal that particle pressure and magnetic field energy density control the shape of the heliosphere.
UNH's Space Science Center played a crucial role in the Interstellar Boundary Explorer (IBEX) mission, which has provided groundbreaking maps of the boundary between our solar system and the interstellar medium. The mission's data reveals new insights into the interactions between the solar wind and interstellar gas, including the form...
Researchers aim to understand the structure and dynamics of the heliosphere using cosmic rays to probe its outer environment. The project has potential implications for space weather forecasting and keeping astronauts safe from hazardous space radiation.
Researchers use twin STEREO spacecraft to detect neutral atoms and map the energized particles at the edge of the solar system. The findings clear up a discrepancy in energy dumped into space by decelerating solar wind, and provide new insights into the heliosheath and its structure.
Scientists have identified a new type of massive stellar death, where stars may collapse into black holes without exploding in supernova explosions. This discovery was made using data from two long-duration Gamma-ray bursts detected by NASA's Swift satellite.
Researchers at the University of Illinois created composite images of optical, radio, infrared, ultraviolet and X-ray wavelengths to understand massive stars' impact on their galactic surroundings. The study reveals that massive stars energize and enrich the interstellar medium with strong ultraviolet radiation and fast stellar winds.
Researchers from Lawrence Livermore National Laboratory have detected a unique 2175 Å wavelength feature in interstellar grains within interplanetary dust particles. The feature is carried by carbon and amorphous silicate grains, abundant in IDPs, which may help explain how some IDPs formed from interstellar materials.
The Cosmic Hot Interstellar Plasma Spectrometer satellite will study the bubble of hot gas between nearby stars, helping scientists understand local galaxy regions and supernova origins. With its high resolution, CHIPSat will measure individual lines to determine physical conditions in the hot gas.
A team of astronomers has found convincing evidence for a key tenet of the three-phase model of the interstellar medium. The study of a supernova remnant in the Large Magellanic Cloud reveals the features of evaporating gas and shocked cloudlets, supporting the theory.