SolarExplorer

Small Solar System Bodies

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 System

A 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.

2.2 – 3.2 AU
1.1 – 1.9 Million
Ceres (940 km)
Silicates / Metals

16 Psyche

Metal Core Asteroid

A 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.

~220 km
85%+ Iron & Nickel
En Route (Psyche)
5.0 Years

Halley's Comet

1P/Halley

The 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.

15 x 8 km
75–76 Years
1986
Mid-2061

Near-Earth Asteroids

NEOs & Defense

Asteroids 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).

33,000+
~2,300
Bennu, Ryugu
NASA DART (2022)

The Oort Cloud

Cosmic Boundary

A 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.

2,000–100,000 AU
Trillions
Halfway to Proxima Centauri
Water, Methane, Ammonia Ice