A circumplanetary envelope surrounding a low-mass planet may be the cause of a source with emitting radius of 0.5–4 au embedded within the larger PDS 66 protoplanetary disk.

Using an automatic stellar stream detection algorithm, researchers have discovered 87 stellar streams associated with globular clusters in our galaxy, doubling the number of known stellar streams.

A survey of ultramassive white dwarfs suggests that these objects form either in a way that induces no strong magnetism, or that the magnetic fields dissipate rapidly.

Using observations from the Parker Solar Probe’s three closest approaches to the Sun, researchers have found the first firm evidence that the Sun’s 5-minute oscillations stretch into the solar wind.

Based on a recent survey of trans-Neptunian objects, researchers have proposed a new surface classification scheme that divides objects based on their infrared brightness.

Luminous red novae are estimated to contribute roughly 25% as much dust as core-collapse supernovae do, and the lower expansion velocities of luminous red novae may result in less dust destruction by shocks.