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Turbulence plays a key role in space and astrophysical plasmas. The study reports evidence of the weak-to-strong transition when Alfvénic turbulence cascades from large to small scales revealed from the Cluster observation of space plasma.
JWST observations of GRB 221009A reveal the associated supernova, confirming that the GRB resulted from the collapse of a rapidly rotating massive star. The lack of r-process emission suggests that these extreme events are not key sources of the heaviest elements.
Venus lacks a magnetic field, leading to interactions between the solar wind and its atmosphere. During its Venus fly-by, BepiColombo observed planetary C+ and O+ escape into space due to this interaction, which is important for understanding atmospheric evolution.
An outstanding discrepancy between observations and models of stellar limb darkening is resolved here by the inclusion of stellar surface magnetism in models. This will enable an improved characterization of transiting exoplanets.
In response to concerns raised by the Navajo Nation on treating the Moon as a grave, NASA has a unique opportunity to advance the conversation with Indigenous communities regarding how we interact with space environments, and who gets to decide.
The Vesta anorthosite meteorite discovery suggests Vesta experienced a lunar magma ocean-like process. Anorthite formed during magma crystallization could have floated to the surface of Vesta, creating a primary anorthositic crust.
Radio pulses from a rare, radio-loud magnetar, XTE J1810−197, are seen to have undergone a conversion in their polarization state. This change can be linked to the magnetar’s magnetic field geometry, and has commonalities with an effect also seen in fast radio bursts.
A state-of-the-art simulation reveals that the long-lasting 10 MK plasma in solar active regions can be heated by magnetic reconnections driven by continuous flux emergence that repeatedly deposit impulsive heating into the coronal plasma.
A radio-loud magnetar, XTE J1810–197, has been observed to precess shortly after an X-ray outburst. The precession decayed over the subsequent few months, which probably rules out freely precessing magnetars as the source of the fast radio bursts.
Micrometeorite impacts are an important process in forming several Ti oxides, including rutile (TiO2) and new Ti minerals (trigonal Ti2O and triclinic Ti2O). These Ti oxides can alter the photocatalytic properties and reflectance spectra of regolith on the Moon and other airless planetary bodies in the Solar System.
Ten stars in the Large Magellanic Cloud exhibit very low elemental abundances, suggesting that they have experienced enrichment by the earliest generations of stars only. These stars provide a window into a distant region of the high-redshift universe.
A joint analysis of the diffuse γ-ray and neutrino emissions in the Galaxy shows that there is a non-negligible leptonic component in the diffuse γ-ray emission below 100 TeV that is contributed by pulsar halos.
The successful impact of NASA’s DART on Dimorphos, the moon of asteroid Didymos, has been analysed using advanced numerical simulations. The results reveal the asteroid’s low surface cohesion and rubble-pile structure, similar to what has been observed on asteroids Ryugu and Bennu.
JWST detections of Si, C and Fe absorption lines in a bright z = 9.31 galaxy with a two-component clump structure suggest that mergers contributed to the rapid build-up of mass and chemical enrichment soon after the Big Bang.
Water molecules in Europa’s icy surface are split into hydrogen and oxygen by charged particle bombardment. NASA’s Juno spacecraft flew near Europa and constrained the production of oxygen in Europa’s surface ice, thus providing only a narrow range to support habitability in its subsurface ocean.