Asteroids & Comets
Remnants from the birth of our Solar System 4.6 billion years ago. From metal-rich asteroids in the Main Belt to icy comets originating in the distant Oort Cloud.
Main Asteroid Belt
Inner Solar SystemA vast doughnut-shaped region located between Mars and Jupiter containing millions of rocky debris items. Total mass is estimated at just 4% of Earth's Moon, with Ceres comprising one-third of the total.
16 Psyche
Metal Core AsteroidA unique M-type asteroid thought to be the exposed nickel-iron core of an ancient protoplanet destroyed by violent collisions. Its metal wealth is estimated at a mind-boggling $10,000 quadrillion.
Halley's Comet
1P/HalleyThe most famous periodic comet, returning to Earth's skies every 75–76 years. When approaching the Sun, its volatile ice sublimates, producing a glowing coma and ion tail millions of kilometers long.
Near-Earth Asteroids
NEOs & DefenseAsteroids whose orbits bring them close to Earth's orbit (within 1.3 AU). Space agencies track over 30,000 NEOs (like Bennu and Apophis) to monitor potential collision risks and test planetary defense (DART mission).
The Oort Cloud
Cosmic BoundaryA theoretical giant spherical shell of icy body debris encapsulating our Solar System between 2,000 and 100,000 AU from the Sun. It is the reservoir from which long-period comets originate.