Earth's Center of Mass Drifts Less Than We Thought

Earth's center of mass isn't stationary. It drifts seasonally and over the course of years. A new study measures this down to the scale of millimeters and finds the seasonal drift is smaller than we thought.

Solar Orbiter Catches the Sun’s Missing High-Speed Vibrations

The Sun’s magnetic fields are a twisty, curvy, ever changing mess. In particular, our star’s polar regions host regions called polar coronal holes that host invisible magnetic highways that stretch out into interplanetary space. But there’s a lot we don’t know about how those highways actually work, and in particular how they give the particles that form the fast solar wind an extra “kick” that sends them zooming at hundreds of kilometers per second. A new paper from a team led by Dr. Yuhang Gao and Prof. Hui Tian at Peking University, and published recently in the journal National Science Review, thinks they might have found an answer by using high-speed shots from Solar Orbiter to detect never-before seen rapid, high-frequency magnetic waves in those areas.

Astronomers Uncover "Hypersoft" X-ray Sources

X-rays showcase some of the most unique astronomical objects in the universe. Neutron stars and black holes siphoning gas from companion stars stick out like sore thumbs at this level of radiation. However, according to a new paper by Mustafa Muhibullah and Jimmy Irwin from the University of Alabama and Rosanne Di Stefano from the Center for Astrophysics at Harvard & the Smithsonian, there appears to be another group of ultra-bright X-ray emitters that we’ve completely missed until now. They call them Hypersoft X-ray Sources (HSSs) and, according to a press release accompanying the paper, might answer two long-standing astronomical questions.

The Sun Is Physically Capable of Producing a "Superflare" According To A New Study

We have long known that the Sun is active. It “flares” quite often, sending huge amounts of energy off in a certain direction - sometimes directly at Earth. But we also know that, compared to other Sun-like stars, it seems relatively quiet, and not capable of producing the “superflares” we sometimes see in its stellar equivalents. That sounds like great news for humanity, and some scientists have even argued that lack of superflares was a critical impetus for the development of complex life on Earth. But a new paper from Natalie Krivova of the Max Planck Institute for Solar System Research and her co-authors in the journal Philosophical Transactions A calls the assumption that our Sun is incapable of such dramatic outbursts into question. That also means that, eventually, our highly technological society could bear the brunt of one of them.

MIT Research Could Lead to Refueling Depots on Mars

MIT PhD candidate Lanie McKinney is developing technology to convert the chemicals in the Martian atmosphere into propellant to bring astronauts home.

Researchers Measure the Environment Where the First Supermassive Black Holes Formed

Scientists theorize that the rapid emergence of supermassive black holes (SMBHs) in the early Universe can be explained by the direct-collapse black hole (DCBH) scenario. In a recent study, astronomers investigated the potential host environments of DCBHs and found that this scenario is a plausible explanation for how the "seeds" of SMBH formed.

BepiColombo Makes Up-Close Measurement of Mercury's Solar Bombardment

BepiColombo's measurements of particle bombardment at Mercury will help assess the impact of space storms on Mercury's surface and on Earth's atmosphere.