Exploration: How We Know About Small Bodies

The tools, the methods and the people behind every number you read about asteroids and comets.

Almost everything we know about small bodies comes from indirect measurements. A dwarf planet at the edge of the Solar System is a faint dot. A comet's nucleus hides inside its own cloud. Astronomers learn the size, shape, makeup and path of these objects by combining many kinds of observations, and each guide in this category explains one of those tools.

Discovery comes first. Sky surveys photograph the same patches of sky night after night, and software looks for points of light that move against the stars. Candidates are reported to the Minor Planet Center, which collects the measurements, assigns a provisional designation and publishes the orbit. Names come later, and only after an orbit is well known. The International Astronomical Union has rules for them.

Orbits are the language of the field. A few numbers, such as eccentricity and inclination, describe the whole path of an asteroid or comet. One guide shows how to read them and how to look up any object in NASA's Small-Body Database.

Telescopes on the ground and in space measure brightness, color and heat. When a distant body passes in front of a star, the star's light blinks out, and the timing gives a precise size. Spacecraft then confirm or overturn those estimates. A timeline guide lists the missions that have visited asteroids, comets and dwarf planets, and another explains how scientists work out what an asteroid is made of.

You can also take part. Several projects accept help from the public, from classifying images to timing occultations, and one guide lists what is open and what you need to start.

Begin with how minor planets are discovered or jump to the mission timeline.

The nine guides

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