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Decametre radio observations are challenging due to the presence of the ionosphere. Here Groeneveld et al. present a strategy to correct for the ionosphere that allows them to make sharp decametre radio images from the ground with the LOFAR telescope.
Phase-curve observations of the ‘hot Jupiter’ exoplanet WASP-43b, made at mid-infrared wavelengths using JWST, provide evidence that fast winds limit the formation of methane on the cooler, cloudy nightside of the planet.
Phase-resolved mid-infrared observations from JWST of the hot gas giant WASP-43b detect a day–night difference of 659 ± 19 K. Comparison with climate models shows that the observations are compatible with cloudy skies, at least on the nightside, and the lack of methane detection suggests the presence of disequilibrium chemistry.
Cassini tracking data yield a lower Love number for Titan than previous analysis. This result is compatible with a low-density internal ocean that might consist of a mix of water and ammonia.
As the eighth anniversary of Nature Astronomy’s opening to submissions nears, we say goodbye to our inaugural Chief Editor, May Chiao, and welcome her successor, Paul Woods, to the helm.
Computer simulations based on the prevailing cosmological model, ΛCDM, reproduce many observed properties of our Universe. But a study of coherent satellite motions in galaxy clusters yields discrepancies that challenge the definition of ‘today’.
Based on physical modelling and using deep-learning tools, a 3D reconstruction of a flare orbiting the black hole Sagittarius A*, at the centre of the Milky Way, provides observational clues to the formation of high-energy flares and the dynamics of black-hole accretion disks.
In situ observations reveal explosive mass ejections due to magnetic reconnection in the ionosphere of Mars, with a density cavity as direct evidence. Reconnection between strong open crustal fields can rapidly eject a large amount of mass from Mars.
Cosmic rays at petaelectronvolt energies permeate the Milky Way, but their origin is unknown. This Review Article summarizes the physics required to accelerate particles to these ultrahigh energies, and their potential astrophysical sources (‘PeVatrons’).
Although both are rocky planets in the habitable zone, Venus and Earth followed different climate evolutionary paths. This Perspective argues for the importance of Venus for understanding planetary habitability and terrestrial planet evolution.
A three-dimensional reconstruction of a bright flare orbiting the black hole Sagittarius A* is computationally recovered from ALMA light curve data by constraining a neural network with a gravitational model of black holes.
Simulated close encounters between planetary systems and other stars reveal that outer giant planets on wide orbits tend to be ejected, with a fraction of them forming bound pairs. This scenario would lead to a population of free-floating binary planets in dense stellar environments
The Earth co-orbital asteroid Kamo‘oalewa, which is a target of the Chinese Tianwen-2 mission, may have a lunar origin instead of an asteroidal one. Dynamical constraints from numerical simulations suggest that it could be an escaping fragment from the lunar Giordano Bruno crater.