Kuiper Belt

⭐⭐ Intermediate Solar System

40 views | Updated January 19, 2026
The Kuiper Belt is a vast, doughnut-shaped region of our solar system extending from Neptune's orbit (30 AU) to approximately 50 AU from the Sun, containing thousands of icy remnants from the solar system's formation 4.6 billion years ago. Named after Dutch-American astronomer Gerard Kuiper, who predicted its existence in 1951, this cosmic "freezer" wasn't confirmed until 1992 when astronomers discovered the first Kuiper Belt Object beyond Pluto.</p><p>This frigid realm hosts fascinating celestial bodies, including dwarf planets like Pluto, Eris, and Makemake, which are composed primarily of frozen methane, ammonia, and water. The belt serves as the birthplace of short-period comets—those completing orbits in less than 200 years—such as Halley's Comet. When gravitational interactions nudge these icy bodies toward the inner solar system, they develop spectacular tails as solar radiation vaporizes their frozen surfaces.</p><p>The Kuiper Belt contains over 100,000 objects larger than 100 kilometers across, with the largest known member being Eris at 2,326 kilometers in diameter. NASA's New Horizons mission revolutionized our understanding by visiting Pluto in 2015 and the mysterious object Arrokoth in 2019, revealing these distant worlds as complex, geologically active bodies rather than simple frozen rocks. This region represents a pristine archive of the early solar system's conditions and composition.

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