Space News & Blog Articles

Dark Matter (DM) remains one of the most daunting mysteries for astronomers, astrophysicists, and cosmologists. Six decades ago, the theory that the Universe was filled with mass that did not interact with normal matter in visible light became an accepted part of our cosmological models. And yet, all efforts to detect this mysterious matter in space or its constituent particles in a lab have produced null results. However, scientists have developed several promising methods that are helping them narrow the search for DM and measure its influence on the cosmos.

One of the critical aspects of exoplanet habitability is the long-term stability of the stars they orbit. Some stars are extremely massive and blast through their hydrogen fuel in only a few million years. Rigel, the blue supergiant in Orion, is an example of one of these. It will shine for only about 10 million years. That's not much time for life to arise on planets.

It feels like every time we publish an article about an exciting discovery of a potential biosignature on a new exoplanet, we have to publish a follow-up one a few months later debunking the original claims. That is exactly how science is supposed to work, and part of our job as science journalists is to report on the debunking as well as the original story, even if it might not be as exciting. In this particular case, it seems the discovery of dimethyl sulfide in the atmosphere of exoplanet K2-18 b was a false alarm, according to a new paper available in pre-print form on arXiv by Luis Welbanks of Arizona State University and his co-authors.

Jupiter enters the evening sky and dominates the night.

This is Part 1 in a series on the physics of free will.

Gravitational Lensing is a vital tool for astronomers to observe objects that are too distant or faint (or both) to be resolved by current instruments. This method leverages a prediction from Einstein's Theory of General Relativity, namely that massive objects alter the curvature of spacetime. When a "lens" comes into view, its gravitational field bends and amplifies light from more distant objects. In a recent study, a team of astronomers used a combination of ground-based telescopes to discover the first spatially resolved, gravitationally lensed supernova.