List of comets by type

• Hyperbolic comet list—Comets that are hyperbolic
• Near-parabolic comet list—Comets that have a period of over 1000 years
• Long-period comet list—Comets with a period between 200 and 1000 years
• List of periodic comets—Unnumbered comets with a period of less than 200 years
• List of numbered comets—Comets numbered by the Minor Planet Center
• Sungrazing comets
  • Kreutz sungrazers
  • Meyer group (below)
  • Kracht group (below)
  • Marsden group (below)
  • Ungrouped sungrazers (below)

After Edmond Halley recognized that several apparitions of a comet every 75.3 years were the same comet, it gave way to a new designation of periodic comets, with the first being named 1P/Halley. To date, there are 503 of these periodic comets, with many more on the way to getting an official designation.

Non-periodic comets are comets that have only been seen on one occasion, and/or comets that have periods of thousands of years. The following comets are organized by their described types:

These are comets with an eccentricity of at least 1 that they only made one pass through the Solar System. These comets are further divided into near-Parabolic and Hyperbolic comets. A hypothetical true parabolic comet would have an eccentricity of exactly 1, and hyperbolic comets are any comet with an eccentricity of over 1. But to know if a comet is truly hyperbolic the orbit must be calculated when it is outside of the planetary region of the Solar System. Most of the comets marked with an X are from the material cited here^[1] and the other comets are sourced from JPL Small-Body Database.^[2] Due to their hyperbolic orbits, it is impossible to determine where they come from, but it is expected that they are from the Oort Cloud, a cloud of icy bodies several thousand Astronomical units away from the Sun. However a few of these may be Interstellar comets

Comets observed in early times, which were later found to be observations of numbered periodic comets, are marked with [periodic comet number]/[comet name]. For instance, X/-239 K1 was an appearance of Halley's comet in 239 BC, and as such is written as 1P/-239 K1. A significant portion of the comets passing closer than 0.01 AU to the Sun are fragments of the comet of 371 BC, which fractured into several pieces on the 326 AD perihelion, which further fractured into thousands of pieces on the 1106 AD perihelion, creating the cometary group now known as the Kreutz sungrazers. Due to the sheer size (2000+ known members), and the fact that none of the group members have been given a numbered designation, the members are not stated on this list, and instead are listed in a separate list further below.

Comets with a very high eccentricity (generally 0.99 or higher) and a period of over 1,000 years that don't quite have a high enough velocity to escape the Solar System. Often, these comets, due to their extreme semimajor axes and eccentricity, will have orbital interactions with planets and minor planets, and often end up with the comets orbit changing significantly in their orbital period and aphelion distance from the Sun. These comets probably come from the Oort cloud, a cloud of comets orbiting the Sun from ~10,000 to roughly 50,000 AU.

The following comets, assigned with a D before their name, were subsequently lost after their discovery, and often remain lost to this day: