Astrophysicists have recently made a groundbreaking discovery that is sending shockwaves through the scientific community: an immense cluster of dark matter, equivalent to the mass of 10 million suns, is moving closer to our solar system. The mysterious nature of this phenomenon and its potential consequences for Earth have sparked concern and a flurry of research efforts to understand what this means for humanity and the universe itself.

Dark matter — one of the grand enigmas of astrophysics; yet there is no radiation-emission, absorption, reflection-of light. It does make stars and galaxies rotate a lot faster than they ever did before. The only clues scientists have about what 27% of its quantity is in the cosmos versus only 5% by ordinary matter are of itself.

Explained astrophysicist Dr. Lydia Harmon: “Dark matter is like the scaffolding of the universe, holding the galaxies together. Without it, the cosmic structure as we know it wouldn’t exist. But the idea of such a massive concentration headed toward us raises unprecedented questions.”

The DESI collaboration’s latest research supports the standard model of gravity and hints at evolving dark energy, based on a detailed analysis of data from millions of galaxies and quasars. These results contribute significantly to understanding the accelerated expansion of the universe.

A physicist from the University of Texas at Dallas, alongside an international team of researchers in the Dark Energy Spectroscopic Instrument (DESI) collaboration, is conducting a multiyear mission to tackle one of astrophysics’ biggest mysteries: Why is the universe’s expansion accelerating?

Scientists have proposed competing theories to explain this phenomenon. One theory suggests that dark energy, an unknown force, is driving galaxies apart. Another theory posits that gravity—the force that binds objects together in local systems like our solar system—behaves differently on vast cosmic scales and may need to be revised to account for the accelerating expansion.

Was dark matter created some time after the Big Bang? Gravitational wave detectors could soon find the answer.

For now, the duo’s results suggest that the Dark Big Bang is far less constrained by past observations than Freese and Winkler originally anticipated. As Ilie explains, their constraints could soon be put to the test.

“We examined two Dark Big Bang scenarios in this newly found parameter space that produce gravitational wave signals in the sensitivity ranges of existing and upcoming surveys,” he says. “In combination with those considered in Freese and Winkler’s paper, these cases could form a benchmark for gravitational wave researchers as they search for evidence of a Dark Big Bang in the early universe.”