Blue Ghost Mission 2 and LuSEE-Night, on the moon’s far side

After pulling off a major uncrewed lunar landing in March 2025, Texas-based Firefly Aerospace is due for a repeat of sorts toward the end of 2026.

From the Wikipedia page, it looks like this has now been pushed into 2027, but I'm still looking forward to it.

The spaceflight company's Blue Ghost lunar lander is scheduled to return later this year back to the far side of the moon facing away from Earth. The mission, known as Blue Ghost Mission 2, would come after the same design of lander first made it to the moon's far side to conduct surface operations for the equivalent of 14 Earth days to test the lunar environment for NASA.

This mission is "bigger and bolder," Firefly said on its website, revealing that it will carry payloads not just for NASA, but international commercial customers. And this time around, the lander will be atop Firefly's Elytra Dark vehicle, which will remain in lunar orbit for five years to image the moon.

Let's zoom in on this part of the mission:

Lunar Surface Electromagnetic Experiment at Night (LuSEE-Night)

LuSEE-Night is a NASA CLPS radio telescope, developed in collaboration with the United States Department of Energy (DOE), that is permanently attached to the top deck of the lander. It will charge an internal battery during lunar daytime for operations during lunar nights. LuSEE-Night's measurements of low frequency radio waves, returned to Earth by a communications relay in a lunar orbit, will provide information about the early history of the universe. According to DOE, LuSEE-Night will, "Attempt first-of-its-kind measurements of the so-called Dark Ages of the Universe."^\8])

https://en.wikipedia.org/wiki/Lunar_Surface_Electromagnetics_Experiment

The Lunar Surface Electromagnetics Experiment (LuSEE-Night) is a planned robotic radio telescope observatory designed to land and function on the far side of Earth's Moon. The project is under development by the U.S. Department of Energy Brookhaven National Laboratory, the DOE Office of Science, UC Berkeley’s Space Sciences Laboratory and the National Aeronautics and Space Administration.

The context:

A more recent NASA-funded project, the Network for Exploration and Space Science (NESS), is drawing up plans for lunar radio telescopes that could probe exoplanets as well as the early universe. Planets that have a magnetic field emit low-frequency radio waves when electrons spiral around the field lines. Because planetary magnetic fields require an internal dynamo, like a spinning liquid metal core, detecting a field could offer clues to an exoplanet's interior—and, Burns says, "could play a key role in assessing [its] habitability." Earth's magnetic field, for example, not only protects life from cancer-causing high energy particles, but is also thought to have shielded water in the atmosphere from being lost to space.

Earth-based radio arrays might be able to detect the radio emissions from a Jupiter-size exoplanet, with a mighty magnetic field. But a lunar observatory might pick up the fainter—and lower frequency—emission of a rocky exoplanet.

This is not that, but you have to start somewhere.