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Universe Today

Reading the Galaxy's Past The Shape of a Black Hole Written in Rock Titan's Hidden Blanket Did Life Start When Impacts Created Vast Hydrothermal Systems in Earth's Crust? Meet REMORA: The Autonomous Space Fleet Built to Tag and Track Asteroids Watch the Moon Occult Venus in the Daytime for North America on June 17th Astrochemical Model Digs Into the Universe's Missing Sulfur Building in Space With Laser "Origami" On The Hunt For Cosmic Dawn And The Universe’s Very First Stars David Kipping Has a New Take on the Existence of Advanced Life in the Universe... and the Numbers are Not Encouraging! This is How Supermassive Black Holes Feed Themselves NASA’s Proposed EVE Mission Aims to Solve the Radius Valley Mystery Where Not to Look in the Search for ET Astronomers Find a Four-Carbon Sugar in Deep Space Why Can't the Universe Be Cyclic? 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Part 1: The Lure of the Eternal Universe A “Green” Dual-Mode Engine is About to Give CubeSats the Best of Both Worlds SETI Panel Revises Recommendations for Dealing With 'Disclosure Day' NASA Bids Farewell to MAVEN Mars Mission in Public Teleconference Astronomers Make "Live" Observation of a Nearby Protoplanetary Disk's Rotation The Cosmic Web Like You've Never Seen it Before They've Been Searching for the Milky Way's Black Hole Wind for 50 Years and Finally Found It What Happens to a Star That Captures A Primordial Black Hole? New Cloud-Detecting Method Will Help Astronomers Characterize Exoplanets Even Without A Magnetosphere, Mars Can Still Deflect Some Solar Wind The Unexpected Brightness 'Gap' in an Ancient Globular Cluster Cosmic Tryst: Venus Meets Jupiter at Dusk A Brief-ish History of SETI. Part IX: What Have We Found? 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Reading the Moon in X-rays
Mark Thompson · 2026-06-10 · via Universe Today

Here's something that might surprise you. Despite being our closest companion in space, despite the missions, the moonwalks, and the decades of study, we still don't have a complete map of what the Moon's surface is made of. We only know bits and pieces. The Apollo samples gave us remarkable chemical snapshots, but they came from just six locations. The Moon has a surface area of nearly 38 million square kilometres so that's like trying to understand an entire continent from a handful of soil samples collected within a few kilometres of each other.

Olivine basalt collected from the rim of Hadley Rille by the crew of Apollo 15 (Credit : NASA) Olivine basalt collected from the rim of Hadley Rille by the crew of Apollo 15 (Credit : NASA)

So the question has long been focussed on somehow mapping the chemistry of a whole world when you can't land everywhere? The answer, it turns out, might be in the use of X-rays.

When solar X-rays slam into the lunar surface, the atoms in the rock fire back their own characteristic X-rays in a process called X-ray fluorescence. Each element has its own unique signature, as distinctive as a fingerprint. Detect those signatures from orbit, and you can work out what's down there without ever touching the ground.

Previous missions have tried this. Apollo and Chandrayaan both made partial maps but they were always incomplete, hampered by weak solar illumination at the poles and the gradual degradation of the detectors over time. The Moon's vast polar regions, which may hold the most scientifically interesting geology, have remained blank on the map.

On August 31, 2012 a long filament of solar material that had been hovering in the sun's atmosphere, the corona, erupted out into space at 4:36 p.m. EDT. Flares like these can bathe the lunar surface in X-rays leading to X-ray fluorescence which helps to map the composition of the lunar surface (Credit : NASA) On August 31, 2012 a long filament of solar material that had been hovering in the sun's atmosphere, the corona, erupted out into space at 4:36 p.m. EDT. Flares like these can bathe the lunar surface in X-rays leading to X-ray fluorescence which helps to map the composition of the lunar surface (Credit : NASA)

Now, researchers at Tokyo Metropolitan University think they've finally cracked it. Their solution is a compact X-ray telescope weighing in at less than ten kilograms making it lightweight enough to fly on a long term satellite mission and rugged enough to survive the radiation environment of lunar orbit. Simulations show that a single telescope, catching the X-ray bursts during roughly 300 solar flares per year, could map five key elements across the entire surface in just two years. Scale that up to a five by five array of twenty five telescopes on one satellite, and the mission time drops to a year, with a finer resolution of 30 by 30 kilometres per grid square.

Five elements; oxygen, iron, magnesium, aluminium, silicon mapped globally for the first time. It doesn't sound terribly dramatic until you consider what it would tell us. The distribution of these elements is a record of how the Moon formed, how its interior evolved, and how billions of years of bombardment have churned its surface. A complete geochemical map wouldn't just fill in a gap. It would give planetary scientists an entirely new lens through which to read lunar history.

Source : X-ray telescopes on a satellite can map the Moon's surface chemistry in a few years