AI challenges astrophysics on the direction of research
Never before in history has so much data been received from space. Researchers are debating how to use artificial intelligence
Key points
For years, NASA has had satellites observing the Moon with extremely high precision, producing a vast amount of data that is now virtually limitless.
The LRO (Lunar Reconnaissance Orbiter) satellite, which has been in orbit around the Moon since 2009, has a resolution of up to 0.5 metres per pixel, thus making it possible to see boulders and smaller craters; it also measures the relative heights of the individual regions imaged, with a vertical accuracy of 10 centimetres.
It has produced well over a petabyte of scientific data, and its homogeneous dataset seems ideal for testing the application of AI to planetary astrophysics. For this reason, NASA and IBM have jointly developed an open-source artificial intelligence model.
The aim is to help engineers and researchers map craters, identify volcanic features and study the polar regions, where water ice may be found. The other objective is to understand whether we are already able to use AI – if not to make new discoveries, then at least to reduce the time, costs and repetitive work involved for researchers.
The world’s most important telescope
It should be noted that, in the case of LRO, the data are all homogeneous. In the case of the most important space telescope currently in operation, the James Webb Space Telescope (JWST), an average of up to sixty gigabytes of scientific data is generated each day, which amounts to around 20 terabytes a year. On the other hand, the brand-new Vera Rubin Observatory, which operates using the largest camera in existence, with a resolution of 3,200 megapixels – that is, 3.2 billion pixels – generates around 20 terabytes per night – roughly 5 petabytes (Pb) a year — and over the course of a decade, the Rubin Observatory’s telescope will produce between 60 Pb of raw images and up to 500 Pb when all processed data is taken into account.


