Finn's Take· TL;DRThirty years ago, we knew of not a single confirmed planet orbiting another star. Not one. Today, that tally has surpassed 6,000 — and it keeps climbing week by week. That alone would be a remarkable scientific achievement. But the number itself isn't even the most astonishing part of the story. The real surprise is what all those planets turned out to be.
The sheer count is striking on its own, but the number is not the most interesting part. The surprise is what these worlds turned out to be like — because the most common kind of planet in the galaxy is one our own solar system does not contain. We spent centuries assuming our cosmic neighborhood was a reasonable template for the rest of the universe. It isn't.
Super-Earths and sub-Neptunes — worlds larger than Earth but smaller than Neptune — account for roughly 3,300 of the confirmed exoplanets, representing more than half of everything discovered so far. Within the growing exoplanet population, the sub-Neptune has emerged as the most common planet type in the Milky Way. And yet, our solar system has nothing like them.
Our solar system features a distinct gap between Earth, at roughly one Earth-radius, and Neptune at nearly four times that size, leaving no local example of a sub-Neptune. The solar system gives us a familiar catalogue: small rocky worlds close to the Sun, then gas and ice giants farther out. For a long time, that local inventory shaped the imagination — a planet could be Earth-like, Mars-like, Jupiter-like, Neptune-like. Then exoplanet surveys began finding something that sits awkwardly between those categories.
NASA describes super-Earths as planets unlike anything in our solar system: larger than Earth, smaller than Neptune, and common among worlds found so far in the galaxy. Closely related mini-Neptunes or sub-Neptunes occupy the same "missing middle," often with thick hydrogen, helium, or water-rich atmospheres over heavier interiors. These aren't exotic edge cases. They're the norm.
The modern era of exoplanet discovery began in 1995, when Michel Mayor and Didier Queloz confirmed a gas giant orbiting the Sun-like star 51 Pegasi — a feat that later earned them a share of the 2019 Nobel Prize in Physics. From that single confirmed world, the field exploded. As NASA's Kepler and TESS missions got going, the number of confirmed exoplanets continued to rise. By 2015, Kepler had discovered its 1,000th exoplanet, and 2016 was a banner year with nearly 1,500 detections in that year alone.
The firmest conclusion from all this data is simply that planets are the rule rather than the exception. Kepler and its successors indicate that most stars host planets of some kind, which means our galaxy contains planets in the hundreds of billions. Our solar system, once the only model we had, now looks like a statistical outlier — unusually sparse in the very size range the galaxy appears to produce most readily.
The absence of sub-Neptunes in our solar system forces researchers to build every inference from light-years away, relying on atmospheric data captured by instruments like the James Webb Space Telescope. Prior to JWST, the study of sub-Neptune atmospheres was typically thwarted by low signal-to-noise measurements and pervasive cloud layers. JWST, with its large aperture and broad infrared wavelength coverage, promised to finally open the door to characterizing planets smaller than Neptune — and it has delivered.
The discovery of thousands of worlds between Earth and Neptune has quietly inverted a very old assumption. The solar system once looked like the obvious pattern because it was the only one visible. Now it looks unusually sparse in the very size range the galaxy appears to produce most readily. That does not make our solar system defective. It makes it informative. Its missing planets are data too. Every world we catalog is another clue in a puzzle that, just three decades ago, we didn't even know existed.