Category Astronomy/Space

Spiral galaxy Messier 61, picture taken with the Hubble Space Telescope. Our Milky Way might look like this galaxy. Credit: ESA/Hubble & NASA. Acknowledgements: G. Chapdelaine, L. Limatola, and R. Gendler

How does the gas in the centre of the Milky Way behave? Researchers from Heidelberg University, in collaboration with colleagues from the University of Oxford, recently investigated the motion of gas clouds in a comprehensive computer simulation. The new model finally makes it possible to conclusively explain this complex gas motion.

Our solar system is located in the outer regions of the Milky Way, a disk-shaped galaxy with an approximate diameter of 100,000 light years...

Simulation of the interior of a solar-type star. Credit: University of Montréal – DAp/CEA – AIM

Resolving an ongoing controversy about whether the star at the center of our Solar System exhibits the same cyclic behavior as other nearby, solar-type stars the new study results also advance scientists’ understanding of how stars generate their magnetic fields. The Sun’s activity – including changes in the number of sunspots, levels of radiation and ejection of material – varies on an eleven-year cycle, driven by changes in its magnetic field.

Understanding this cycle is one of the biggest outstanding problems in solar physics, in part because it does not appear to match magnetic cycles observed on other solar-type stars – leading some to suggest the Sun is fundamentally different.

Here, by c...