![Gamma-ray burst [GRB]. Credit: Cruz Dewilde/ NASA SWIFT.](https://nasaspacenews.com/wp-content/uploads/2025/05/gamma-ray-burst-credit-nasa-swift-cruz-dewilde-1-75x75.jpg)
One of the most profound mysteries in modern astronomy is what happened between the Big Bang and the birth of the first stars. This vast period—known as the Cosmic Dark Ages—remains mostly unobserved due to the lack of light and the limitations of Earth-based instruments. Today, a group of European astronomers and engineers has proposed a bold mission to break this cosmic silence: the Dark Ages Explorer (DEX).
What Are the Cosmic Dark Ages and Why They Matter
The Cosmic Dark Ages span from around 380,000 years after the Big Bang—when the Universe cooled enough for neutral hydrogen to form—to about one billion years later, when the first stars and galaxies began to shine. During this time, space was filled with cold, dark hydrogen gas that emitted faint radio waves. Among the few detectable signals from this era is the 21-centimeter line, a specific wavelength of light produced by neutral hydrogen atoms.
This signal is one of the few tools scientists have to study the time before stars and galaxies existed. Unlike starlight, which can be blocked or scattered by matter, this long-wavelength radio emission travels across the cosmos largely untouched, preserving a detailed record of the early Universe’s structure.
The DEX Telescope and Its Mission Objectives
The Dark Ages Explorer (DEX) is designed to overcome Earth’s radio interference by placing the telescope on the Moon’s far side—a location naturally shielded from terrestrial radio noise. The mission, led by researchers from Radboud University, ASTRON, and several other European institutes, involves deploying a large array of antennas over a flat area, ideally a crater floor, spanning 200 by 200 meters.
This setup would allow DEX to observe extremely faint hydrogen signals across a wide range of frequencies, corresponding to different redshifts—distances in time—spanning from the Cosmic Dawn to the earlier Dark Ages. DEX would essentially create a three-dimensional time-lapse of how matter began to clump together, forming the large-scale structure of the Universe. Unlike optical telescopes like Hubble or Webb, which observe galaxies after they’ve formed, DEX would peer further back—to the moment before the light switched on.
Why the Far Side of the Moon Is Ideal
Observing the 21-cm hydrogen line from Earth is nearly impossible. Our planet’s atmosphere blocks many radio frequencies, and the explosion of human-made signals—from cell towers to satellites—pollutes the radio spectrum. The far side of the Moon, however, offers the quietest environment in the Solar System for low-frequency radio astronomy.
With no atmosphere and complete shielding from Earth’s noise, the lunar far side provides an undisturbed view of the radio sky. It’s the perfect natural observatory. This location would enable DEX to detect signals from a time when the Universe was still in its silent, starless phase, capturing data that has never been seen before.
Facing the Engineering Challenges Head-On
Operating a telescope on the Moon comes with substantial technical challenges. The surface environment is extreme: temperatures can swing between boiling and freezing during each lunar day and night cycle. The terrain is rocky and uneven, and there is no existing infrastructure to rely on.
To address these challenges, the DEX team proposes using ultra-light, foil-based antennas that can be rolled out or inflated to minimize mass and complexity. Powering the array also poses difficulties. Running traditional electrical cables across the site would increase mass and complexity. Alternatives like wireless data transmission or optical fiber are being explored to avoid interference and reduce deployment constraints.
Additionally, precise antenna placement is critical. Any deviation in positioning would degrade the quality of the data by introducing noise or distortion in the frequency patterns. A reliable, autonomous deployment system must ensure a consistent and predictable grid layout across the harsh lunar terrain.
Connecting DEX to Other Cosmic Missions
DEX is part of a broader global push to explore the early Universe using radio telescopes. NASA’s LuSEE-Night mission, expected to launch in 2025, will be a test platform for low-frequency radio science from the Moon’s far side. China’s Hongmeng Project proposes a satellite-based system to explore the same wavelength ranges from lunar orbit. And NASA’s visionary Lunar Crater Radio Telescope (LCRT) concept imagines building a massive dish inside a lunar crater using robotic systems.
These efforts reflect growing international interest in studying the Dark Ages and the Cosmic Dawn. Together, they form a global ecosystem of complementary missions that will collect overlapping data and help cross-validate theories about the early Universe’s structure and evolution.
What DEX Could Reveal About the Cosmos
What makes DEX so compelling is its potential to resolve long-standing puzzles. The James Webb Space Telescope has already surprised scientists by spotting galaxies and black hole candidates that seem too mature for their age—just a few hundred million years after the Big Bang. Similarly, the EDGES experiment detected a stronger-than-expected hydrogen absorption signal around 70 MHz, suggesting unexpected cooling or additional radiation sources in the early Universe.
DEX would be uniquely equipped to test these anomalies by directly measuring how neutral hydrogen evolved over time and space. Its high-resolution maps of matter distribution could confirm or challenge existing models about the formation of the first stars and galaxies. It could help clarify the timeline of reionization, identify the origins of early black hole seeds, and even shed light on dark matter’s role in cosmic structure formation.
Spin-Off Benefits for Earth and Space
Beyond astronomy, DEX could yield valuable technological advancements. The development of temperature-resistant electronics, ultra-light antennas, and autonomous deployment systems could benefit satellite communications, remote sensing, and planetary exploration.
These technologies may also assist future Moon missions, space-based infrastructure, and even defense and communication systems on Earth. Historically, space exploration has often driven innovation in unrelated sectors—from medical imaging to solar panels. DEX continues this tradition by pushing boundaries in hardware design and deployment.
A Cosmic Time Machine in the Making
The Dark Ages Explorer isn’t just another space telescope—it’s a window into the Universe’s forgotten past. By listening to the quiet whispers of neutral hydrogen from billions of years ago, DEX could finally fill in the missing chapter between the Big Bang and the first starlight.
If it succeeds, it will help answer fundamental questions about where we come from, how the Universe built its first structures, and what unknown physics may still be out there, waiting to be discovered. As space agencies and scientists worldwide prepare for a new era of lunar exploration, DEX stands at the intersection of scientific ambition and technological innovation—ready to turn the Moon into a gateway to the deepest parts of the cosmos.
Reference:
An absorption profile centred at 78 MHz in the sky-averaged
spectrum
