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FRIDAY, FEBRUARY 6, 2026
Humanoids2 min read

Moon Telescope Aims to Uncover Cosmic Dark Ages

By Sophia Chen

Close-up of robotic exoskeleton mechanism

Image / Photo by Josh Riemer on Unsplash

A radio telescope destined for the moon’s far side may finally unlock secrets from the universe's infancy.

The LuSEE-Night telescope, designed by a team at NASA and the University of California, Berkeley, is set to launch aboard Firefly Aerospace’s Blue Ghost Mission 2, with an anticipated landing in 2024. This spacecraft aims to be the third successful mission to the moon's far side, following China's Chang’e 4 and upcoming Chang’e 6 missions.

The far side of the moon offers a unique advantage: it's free from the radio frequency (RF) noise that plagues terrestrial observatories. This interference complicates the detection of faint signals, particularly those from the cosmic Dark Ages—an era that began approximately 380,000 years after the Big Bang and lasted up to 400 million years. During this time, neutral hydrogen was the predominant element in the universe, but signals from this epoch have yet to be detected from Earth due to atmospheric noise and urban RF interference.

LuSEE-Night aims to detect these elusive signals by operating in the low-frequency range of 1 to 10 MHz, a challenging task given the physical constraints of lunar operations. The technical specifications reveal that the telescope will consist of a 4-meter dipole antenna array, allowing it to effectively sample the faint RF emissions. By positioning the instrument on the moon, scientists hope to access a clear line of sight to the universe’s earliest moments, potentially reshaping our understanding of cosmic evolution.

The mission is ambitious, yet it highlights the incremental achievements that define modern space exploration. Unlike many previous attempts at lunar exploration, the LuSEE-Night project is grounded in the lessons learned from earlier missions. Engineering documentation shows that the team has taken care to address the limitations faced by its predecessors, particularly in terms of power supply and data transmission. The telescope will be powered by solar panels, with a runtime designed to last through the lunar day, which lasts about 14 Earth days, before entering a low-power state during the lunar night.

However, challenges remain. The moon's harsh environment, including temperature extremes and radiation exposure, poses risks to the integrity of the equipment. The design must account for these factors to ensure that the antenna array remains operational throughout its mission. Furthermore, the radio signals of interest are exceedingly faint, making detection a formidable task, even under optimal conditions.

The LuSEE-Night mission is not just about uncovering ancient cosmic signals; it also sets a precedent for future lunar exploration. As the first of its kind to attempt this specific scientific inquiry, it operates at a Technology Readiness Level (TRL) of 6, indicating that while it has proven its functionality in a lab setting, its field readiness will be tested upon lunar deployment. The results from this mission could inform subsequent missions, both to the moon and beyond, as humanity seeks to answer fundamental questions about the universe.

As we look forward to the launch, the LuSEE-Night mission encapsulates the spirit of exploration and the relentless pursuit of knowledge. It serves as a reminder that, while the road to discovery is often fraught with setbacks, each incremental step brings us closer to understanding our place in the cosmos.

Sources

  • LuSEE-Night: See You on the Far Side of the Moon

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