Follow-up observations of a gravitational microlensing event show the source to be a 10-Earth-mass exoplanet orbiting an M-dwarf star, consistent with the discovery article.

A chance alignment between the Parker Solar Probe and Solar Orbiter at 0.11 and 0.88 au from the Sun allowed researchers a rare glimpse into how solar wind turbulence evolves with distance from the Sun.

Disk outflows from a newly formed black hole are shown to produce a bright signal that could power the first peak of certain double-peaked supernova light curves or another kind of transient altogether.

Researchers have performed in an in-depth study of two tidal disruption events that were selected via their radio emission and are visible at optical wavelengths, showing unprecedented intermediate-width spectral lines.

Simulations suggest that impacts between planetesimals can produce chondrules — round inclusions of once-melted silicates — similar to what is seen in meteorites.

The Vera C. Rubin Observatory will discover ~129 candidate near-Earth objects each night, necessitating careful consideration of which objects should be followed up on with other facilities.