Space News & Blog Articles

While the Universe may appear serene and inspiring at first glance, it is actually filled with particles traveling at nearly the speed of light that possess immense energy. These consist primarily of atomic nuclei and subatomic particles, such as protons, electrons, and neutrinos, which constantly bombard Earth. The origin of these particles remains one of the longest-standing mysteries in modern astrophysics. A leading theory is that they are created by extreme events, such as supernovae and tidal disruption events (TDEs), which occur when stars are ripped apart by black holes.

The case for habitability in Enceladus' warm, ice-capped ocean is growing. Ever since Cassini found evidence of hydrothermal activity in the moon's ocean, and detected life's building blocks in the plumes of material ejected from the ocean, scientists have worked to put this data into context.

Last time I wrote about new data that overturns the standard cosmological model. Before anyone starts dusting off their fringe cosmological models, we should note what this new study doesn't overturn. It doesn't say the Big Bang model is wrong, nor does it say that the Universe isn't expanding or that Hubble's redshift-distance relation needs to be thrown out. It really only says that our Hubble constant model is wrong. But we already knew that thanks to a little thing known as the Hubble tension. These new results could solve that mystery as well.

Iron rusts. On Earth, this common chemical reaction often signals the presence of something far more interesting than just corroding metal for example, living microorganisms that make their living by manipulating iron atoms. Now researchers argue these microbial rust makers could provide some of the most promising biosignatures for detecting life on Mars and the icy moons of the outer Solar System.

Astronomers using the Keck Observatory on Maunakea in Hawaii have captured the closest ever view of a protoplanetary disk, the swirling cloud of gas and dust where planets form from interstellar debris. Their target, a young star called HD 34282 located 400 light years away, offers a front row seat to planetary birth.

You come for the king, you best not miss.

Tracking time is one of those things that seems easy, until you really start to get into the details of what time actually is. We define a second as 9,192,631,770 oscillations of a cesium atom. However, according to Einstein’s theory of general relativity, mass slows down these oscillations, making time appear to move more slowly for objects in large gravity wells. This distinction becomes critical as we start considering how to keep track of time between two separate gravity wells of varying strengths, such as on the Earth and the Moon. A new paper pre-print on arXiv by Pascale Defraigne at the Royal Observatory of Belgium and her co-authors discusses some potential frameworks for solving that problem and settles on using the new Lunar Coordinate Time (TCL) suggested by the International Astronomical Union (IAU).

The ESA's Euclid space telescope has been in space for just over a year, investigating some of the deepest mysteries of the cosmos. By observing cosmic structures up to a distance of 10 billion light-years, the observatory will chart the evolution of the Universe, attempt to constrain the influence of Dark Energy, and study the morphology of galaxies. In terms of galaxies, Euclid will attempt to answer the question of why the Universe contains such a variety of galaxies, characterized by size, shape, and colours.