Monday, March 23, 2026

Giant Craters May Reveal if Psyche is a Lost Planetary Core

Artist's illustration of asteroid 16 Psyche. (Credit: Maxar/ASU/P.Rubin/NASA/JPL-Caltech)

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 protoplanet’s core that didn’t build into a full-fledged planet. But how did such a unique asteroid form?



Parabolic Flight Experiments Delve into Planetary Formation

Planets are thought to grow from dust grains in a protoplanetary disk to form larger and larger objects, eventually creating planets. This illustration from European Southern Observatory is an artist's concept of a typical disk of gas and dust around a newborn star.

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.



Rubin Alert Leads to First Follow-Up Observations and Detection of Four Supernovae

The NSF-NOIRLab Cerro Tololo Inter-American Observatory (CTIO), located high in the mountains of Chile, studies the southern night sky. Credit: CTIO/NOIRLab/NSF/AURA/P. Horálek (Institute of Physics in Opava)

NSF NOIRLab has completed end-to-end runs of its ecosystem for following up on alerts from NSF–DOE 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.



This Ancient Star In A Low-Mass Galaxy Is A Precious Find

This image shows stars in Pictor II, an ultra-faint dwarf galaxy. It's an ancient galaxy, more than 10 billion years old. One of the stars is named PicII-503, and it's a Population II star, known for their low metallicities. Astronomers have been searching for these ancient stars because they hold clues to the evolution of the Universe. Image Credit: CTIO/NOIRLab/DOE/NSF/AURA

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.



Black Hole Mergers Test the Limits of General Relativity

Discoveries made by the LIGO-Virgo-KAGRA (LVK) network since LIGO's first detection of gravitational waves emanating from pairs of colliding black holes. Credit: LIGO/Caltech/MIT/R. Hurt (IPAC)

We can now use the gravitational waves of black holes to test general relativity and look for evidence of alternative theories of gravity.



Saturday, March 21, 2026

How Will Martian Gravity Affect Skeletal Muscle?

Astronauts working outside a habitat on the surface of Mars. Credit: NASA

Marie Mortreux, an assistant professor in the University of Rhode Island’s College of Health Sciences, is part of an international team of researchers studying how the Mars’s gravity would affect astronauts’ skeletal muscle.



Friday, March 20, 2026

Saturn-mass world discovered orbiting two low-mass stars

Artist's illustration of an exoplanet orbiting two stars. (Credit: NASA/JPL-Caltech/T. Pyle)

You just established a settlement on an Earth-like planetary body far from our solar system. You did your evening chores after eating dinner, and you want to go out for the evening view, which consists of two setting stars, reminiscent of the infamous scene in Star Wars. However, there’s one major difference: a large planetary body is in the sky. As you were aware before arriving, you’re on an exomoon orbiting a Saturn-sized exoplanet, both of which orbits two stars.