Detecting gravitational waves has always demanded enormous machines; kilometre scale instruments capable of sensing distortions smaller than a proton. But a new theoretical study suggests the universe may have been leaving its calling card in the light emitted by individual atoms. If the idea holds up, the future of gravitational wave detection might not be sprawling observatories carved into the landscape, but something you could hold in the palm of your hand.

Heat shield design is one of the most critical aspects of missions that plan to either land on a planets (or moons) surface or return to our own. Spacecraft that have to survive the fiery, hypersonic plunge through an atmosphere require these systems. For decades, heat shields have been designed to slowly burn away in a process called ablation, which is intended to dissipate the incredible thermal energy or reentry. But, theres another, less understood phenomenon that affects them too - spallation, where a heat shield sheds material in violent, unpredictable bursts. This second mode of destruction seems to be particularly prevalent in oxygen-deprived atmospheres, like that of Titan, where the Dragonfly helicopter plans to land in the not too distant future. A new paper published in Carbon from researchers at the University of Illinois Urbana-Champaign (UIUC) performed some tests showing just how different those heat shields might need to be.

When we think of asteroids, we almost immediately think of giant rocks bouncing around like the iconic chase scene in Empire Strikes Back, and we often hear how they are remnants from the birth of the solar system. While the asteroids that comprise the Main Asteroid Belt of our solar system are not only spread far apart from each other, they are also not all made of rock. One asteroid approximately the size of the State of Massachusetts called 16 Psyche is made of metal, which planetary scientists hypothesize could be the remnants of a protoplanets core that didnt build into a full-fledged planet. But how did such a unique asteroid form?

What happens in a protoplanetary disk to create planetesimals around a star? We know the general story -- the material begins to clump together and eventually grows from dust grains to rocky bodies capable of sticking together to make planets. But, how does that dust begin the aggregation journey? That's what a research team from the Switzerland wanted to know. So, they did experiments aboard parabolic micro-gravity flights to find an answer.

NSF NOIRLab has completed end-to-end runs of its ecosystem for following up on alerts from NSFDOE Vera C. Rubin Observatory. The runs demonstrated how multiple NOIRLab-developed software tools, plus a network of telescopes around the globe, will enable quick follow-up observations of the countless transient objects that Rubin will uncover during its ten-year survey.

To understand the Universe we see around us today, we have to understand its past. Some hard-to-find ancient stars, called Population II stars, preserve evidence from the ancient Universe. Astronomers finally found one.

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