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- Photobombing Asteroids: Unlocking the Mystery of Psyche
Summary
By the end of this article, you will understand how astronomers use accidental ‘photobombs’ in old telescope data to figure out if an asteroid is a solid cannonball of metal or covered in dusty rock.
Quick Facts
Surprise: There are hundreds of thousands of accidental asteroid photos hiding in public space archives
Salient Idea: Thermal inertia tells us if an object is solid metal or covered in fluffy dust based on how it holds heat
Surprise: Psyche was long thought to be pure bare metal, but new data proves its surface is highly insulating
Salient Idea: The ESASky tool acts like a time machine, matching an asteroid's past orbit to exactly where old telescopes were looking
The Discovery: The Ultimate Cosmic Photobomb
In 2010, the Herschel Space Telescope was staring deep into a distant galactic region. Unbeknownst to scientists at the time, the famous asteroid (16) Psyche was drifting through the background. Decades later, astronomers used a new pipeline called the Solar System Object Search Service (SSOSS) to hunt for these accidental ‘photobombs.’ They found a Surprise: Psyche had been captured by Herschel in far-infrared light. By analyzing these serendipitous images, they measured how the asteroid held onto the Sun’s heat. Instead of acting like a solid cannonball of bare metal, it behaved like something covered in a powdery, rocky dust. This accidental picture totally changed our expectations for NASA’s upcoming mission to visit Psyche.
ESASky SSOSS: Solar System Object Search Service and the case of Psyche
This greatly simplifies the task of searching, identifying, and retrieving such data for scientific analysis.
— Dr. E. Racero
The Science Explained Simply
This is NOT just taking a picture to see what Psyche looks like. It is about measuring its thermal inertia—how quickly a surface heats up and cools down. Think of touching a metal playground slide versus a sandbox on a hot day. The metal transfers heat instantly, while the fluffy sand traps it. The Salient Idea here is that scientists expected Psyche to act like the metal slide, rapidly conducting heat. Instead, the Herschel infrared data showed it acts more like the sandbox. It holds onto heat in a way that suggests its metallic surface is covered in a highly insulating layer of regolith (crushed rocky dust).
The Aurora Connection
Why do we care about a metallic asteroid covered in dust? Psyche is widely believed to be the exposed iron core of a dead protoplanet that was shattered in the early solar system. Earth also has a molten iron core, which acts as a giant dynamo to generate our magnetic field. This magnetic shield protects our atmosphere from the solar wind and creates the beautiful auroras at the poles. By studying Psyche, we are essentially looking at the ‘engine’ that drives planetary magnetic fields, only frozen in time. Without metallic cores, worlds would have no auroras and no protection from space weather.
By examining Psyche, we are looking at the frozen heart of a planetary dynamo.
— NorthernLightsIceland.com Team
A Peek Inside the Research
How do you find a moving asteroid in an archive of millions of stationary images? It requires computational geometry, not just looking with your eyes. The team built the SSOSS pipeline to calculate the exact orbital paths of 800,000 asteroids over decades. They then mathematically overlaid these paths onto the exact ‘footprints’ (fields of view) of space telescopes like Hubble and Herschel. If the orbit and the footprint intersected at the exact right time, the computer flagged it as a detection. Through this brilliant matching game, they found over 30,000 accidental Hubble detections alone!
We performed a geometrical cross-match of the orbital path of each object with respect to the public high-level imaging footprints stored in the ESA archives.
— The Research Team
Key Takeaways
Old astronomical data contains hidden discoveries that are completely free to uncover using computational geometry
Serendipitous (accidental) detections are crucial for mapping an asteroid's true thermal properties
Psyche's low thermal inertia matches silicate dust, proving it is not a highly conductive, bare metal world
Studying exposed metallic cores like Psyche holds the key to understanding how planetary magnetic fields form
Sources & Further Reading
Frequently Asked Questions
Q: If Psyche is covered in dust, does that mean it isn’t a metallic asteroid?
A: Not necessarily! It likely still has a massive metallic core, but millions of years of meteor impacts have pulverized surface rocks and mixed them with the metal, creating a dusty, insulating outer shell.
Q: Why didn’t scientists notice Psyche in the Herschel images back in 2010?
A: Because they weren’t looking for it. The telescope was targeted at a specific galaxy or star, and Psyche was just a tiny, slow-moving speck of infrared light in the background of the image.

