Dr. Sofia Sheikh from the SETI Institute led a study that sheds new light on how pulsar signals—the spinning remnants of massive stars—distort as they travel through space. This study, published in The Astrophysical Journal, was performed by a multi-year cohort of undergraduate researchers in the Penn State branch of the Pulsar Search Collaboratory student club. Maura McLaughlin, Chair, Eberly Distinguished Professor of Physics and Astronomy, West Virginia University, created the Pulsar Search Collaboratory to engage high schoolers and undergraduates in pulsar science, and she helped facilitate access to the data used in this study. Using archival data from the Arecibo Observatory, the student team found patterns that show how pulsar signals change as they move through the interstellar medium (ISM), the gas and dust that fills the space between stars. The team measured scintillation bandwidths for 23 pulsars, including new data for six pulsars not previously studied. The results showed that in almost all cases, measured bandwidths were higher than predictions by widely used models of the galaxy, highlighting a need for updates to current ISM density models.

“This work demonstrates the value of large, archived datasets,” said Dr. Sofia Sheikh, SETI Institute researcher and lead author. “Even years after the Arecibo Observatory's collapse, its data continues to unlock critical information that can advance our understanding of the galaxy and enhance our ability to study phenomena like gravitational waves.”

While NASA’s NEOWISE telescope ended its journey through space on Nov. 1, 2024, the team at IPAC, a science center at Caltech, was working on one further gift from the prolific mission. 

A paper published in Gravitational and Space Research unveils insights gained from International Space Station (ISSInternational Space Station) National Laboratory-sponsored research on transport phenomena, fundamental physical processes involving momentum, energy, and mass transfer. Transport phenomena describe the ways in which heat and matter move through their surroundings, for example, how heat radiates from a stove or how a scent fills the room. Exploring these dynamics outside Earth’s gravitational forces could lead to revolutionary advances in pharmaceuticals and other commercial applications.

Dark ovals in Jupiter's polar haze, visible only at UV wavelengths, were first noticed 25 years ago, then ignored. A UC Berkeley study shows that these dark UV ovals are common, appearing at the south pole in 75% of Hubble Space Telescope images taken since 2015. They appear less often at the north pole. The scientists theorize that a magnetic vortex generated in the ionosphere stirs up and concentrates the hydrocarbon haze that blankets the poles.

Researchers from the Curtin node of the International Centre for Radio Astronomy Research (ICRAR) have made a record-breaking astrophysical discovery while simultaneously uncovering a possible explanation for the rare and extreme astrophysical event known as long-period radio transients.

Researchers at the University of Science and Technology of China have discovered that gamma rays can convert aqueous-phase methane into complex organic molecules, including glycine, at room temperature. This process mimics the potential formation of organic molecules in space and could have implications for understanding the origins of life. The study also suggests that gamma rays could be a sustainable energy source for converting methane into valuable products.

A new computer model developed by the University of Texas Institute for Geophysics can be used to detect and measure interior oceans on the ice covered moons of Uranus. The model works by analyzing orbital wobbles that would be visible from a passing spacecraft. The research gives engineers and scientists a sliderule to help them design NASA's upcoming Uranus Orbiter and Probe mission.