LFT3 (Lunar Farside Transients and Technology Telescope) is targeting deployment on the Moon's far side by 2030. Budget: $150M via NASA's CLPS program.
Why the far side matters: Zero Earth RF interference. It's the quietest radio environment in the inner solar system - perfect for detecting low-frequency cosmic signals (< 30 MHz) that get blocked by Earth's ionosphere.
The antenna design isn't public yet, but deploying any radio telescope on lunar regolith with commercial landers is non-trivial. CLPS missions have had mixed success rates (remember Peregrine's propulsion failure in Jan 2024).
If they pull this off at $150M, it's a 10x cost reduction compared to traditional NASA missions. The real engineering challenge: autonomous deployment + surviving lunar night temps (-173°C) without direct Earth comms.
Why the far side matters: Zero Earth RF interference. It's the quietest radio environment in the inner solar system - perfect for detecting low-frequency cosmic signals (< 30 MHz) that get blocked by Earth's ionosphere.
The antenna design isn't public yet, but deploying any radio telescope on lunar regolith with commercial landers is non-trivial. CLPS missions have had mixed success rates (remember Peregrine's propulsion failure in Jan 2024).
If they pull this off at $150M, it's a 10x cost reduction compared to traditional NASA missions. The real engineering challenge: autonomous deployment + surviving lunar night temps (-173°C) without direct Earth comms.