The third known interstellar object — a comet from beyond our Solar System
Let me put that eccentricity number in context. Every comet we've ever seen from another star system — all three of them in human history — arrived with an eccentricity barely above 1. 'Oumuamua came through at 1.20, just barely unbound. Borisov at 3.36, clearly a visitor. Then Atlas arrived at 6.139. It wasn't sneaking through our solar system. It was blazing through at an angle that says: I came from very, very far away, and I'm not staying.
What drew me to this research is the rarity. In the entire history of astronomy, we have identified exactly three objects from outside our solar system. Three data points. And yet each one has rewritten something we thought we understood. 'Oumuamua challenged our assumptions about shape and composition. Borisov proved interstellar comets could look like our own. Atlas — with JWST detecting water, CO₂, and CO in its coma — gave us the first chemical fingerprint of ices forged around another star. We are, quite literally, reading the chemistry of another solar system's birth.
With Voyager, we sent a message out. With Atlas, the universe sent one back.
3I/ATLAS (C/2025 N1) is the third confirmed interstellar object to pass through our Solar System, following 1I/'Oumuamua (2017) and 2I/Borisov (2019). Discovered by the ATLAS survey in July 2025, this object travels on a strongly hyperbolic orbit (e = 6.139) with a nearly retrograde inclination of 175.1°, unambiguously confirming its extrasolar origin. Unlike 'Oumuamua, 3I/ATLAS displays clear cometary activity — JWST spectroscopy has detected H₂O, CO₂, and CO volatiles, providing our first direct measurement of interstellar cometary composition. With 4,267 observations over a 180-day arc and a dramatic 4-magnitude brightening observed from ground-based and space-based telescopes, 3I/ATLAS represents an unprecedented opportunity to study material from another planetary system as it passes through our own.
With an eccentricity of 6.139 — far exceeding the e = 1 threshold for unbound orbits — 3I/ATLAS is gravitationally unbound from the Sun. Its nearly retrograde inclination (175.1°) further distinguishes it from any Solar System population. This is the most hyperbolic trajectory ever observed for a small body passing through our Solar System, surpassing both 1I/'Oumuamua (e = 1.20) and 2I/Borisov (e = 3.36).
The James Webb Space Telescope detected water (H₂O), carbon dioxide (CO₂), and carbon monoxide (CO) in the coma of 3I/ATLAS — the first direct spectroscopic measurement of volatile species in an interstellar comet. These detections provide direct constraints on ice chemistry in an extrasolar protoplanetary disk, offering a window into planet formation conditions around another star.
3I/ATLAS brightened by approximately 4 magnitudes (a factor of ~40× in flux) between discovery and perihelion, from V ≈ 14.0 to V ≈ 10.0. This brightening is consistent with increasing solar heating driving sublimation of volatile ices, confirming the object's cometary nature and distinguishing it from the inert appearance of 1I/'Oumuamua.
3I/ATLAS was characterized by both the Hubble Space Telescope (UV/optical morphology, coma structure) and the James Webb Space Telescope (infrared spectroscopy, volatile composition). This marks the first interstellar object observed across the full UV-to-IR wavelength range by flagship space observatories, enabling comprehensive physical and chemical characterization.
3I/ATLAS approaches the Sun traveling in nearly the opposite direction to the planets — its orbital inclination of 175.1° places it just 4.9° from perfectly retrograde. This extreme geometry results in very high encounter velocities relative to solar-orbiting bodies and indicates arrival from far above or below the ecliptic plane.
With 1I/'Oumuamua (2017, inert, ambiguous morphology), 2I/Borisov (2019, clearly cometary), and now 3I/ATLAS (2025, cometary with volatile detections), we are building the first statistical sample of interstellar visitors. Each object reveals new aspects of extrasolar planetary system chemistry, with 3I providing the richest compositional data to date.