ORBIT Solar System Explorer

COMET PROFILE 1P / HALLEY

Halley's Comet

A comet returning across generations

A famous periodic comet returning roughly every 76 years. It orbits retrograde, from inside Venus's orbit to beyond Neptune.

Rendered view of Halley's Comet
Illustrative surface and shape · Image credits
Model orbital period
75.8 yr
Orbital inclination
162°
Model perihelion
0.57 AU

01 / Overview

Meet Halley's Comet

Halley's comparison of historical sightings turned an apparently unpredictable apparition into a returning visitor. The comet travels backward around the Sun, with a dark nucleus of ice and dust that becomes active as it warms. Debris left along its path produces the Eta Aquariid and Orionid meteor showers.

02 / Key data

Core parameters

Model orbital period
75.8 yr
Orbital inclination
162°
Model perihelion
0.57 AU
Model aphelion
35.23 AU
Data and calculation notes

Positions use the shared date and JPL orbital elements at a reference epoch. Fixed two-body orbits omit planetary perturbations and outgassing; errors grow away from the epoch. This is not a precise return forecast. Halley and 67P use public observed shape models; Encke and Hale-Bopp use independent approximations constrained by observed sizes. Nucleus surfaces, spin, and tails remain illustrative.

03 / Further reading

A closer look

Discovery and exploration10
  • Halley's Comet was the first comet recognized as returning periodically.

  • Edmond Halley compared historical sightings and inferred they were the same comet.

  • Halley's Comet last passed perihelion in 1986.

  • Halley's Comet is expected to return near perihelion in 2061.

  • Halley's Comet orbits retrograde, opposite to most planets.

  • Giotto photographed Halley's nucleus up close in 1986.

  • Halley's nucleus is irregular and very dark, not a bright ball of ice.

  • The Eta Aquariid meteor shower comes from debris left by Halley's Comet.

  • The Orionid meteor shower also comes from Halley's debris stream.

  • Halley's orbital period is roughly 76 years, varying with planetary gravity.

Coma and tails11
  • The nucleus is a comet's solid body, made mainly of ice, dust, and rock mixed together.

  • Near the Sun, cometary ice can sublimate directly to gas and carry dust with it.

  • The diffuse envelope of gas and dust around the nucleus is the coma.

  • The solar wind influences the ion tail, directing it roughly away from the Sun.

  • Dust-tail particles have their own orbits, often producing a curved tail.

  • A comet's tail can point ahead as it moves away from the Sun; it is not exhaust trailing its motion.

  • A coma can be many times larger than its nucleus; a photo's bright cloud is not the solid body's size.

  • Meteor showers can occur when Earth crosses debris left by a comet.

  • A meteor is light produced when a small particle enters the atmosphere, not a falling star.

  • Most returning comets still require a telescope to observe.

  • Comet brightness depends on activity, not just distance from Earth.

Orbit and evolution9
  • Short-period comets generally have orbital periods under 200 years.

  • Many long-period comet orbits suggest origins in the distant Oort Cloud.

  • Comets preserve early Solar System material and help us study planetary formation.

  • Comets generally move faster at perihelion and slower at aphelion.

  • Planetary gravity, especially Jupiter's, can change comet orbits and sometimes disrupt their nuclei.

  • Cometary gas jets exert small reaction forces that precise predictions must include.

  • Orbital elements refer to an epoch; neglected perturbations can accumulate over time.

  • P in a comet designation means periodic; C is commonly used for comets that are not short-period.

  • Dark dust often coats comet nuclei; containing ice does not make their surfaces snow-white.

04 / Sources

Trusted sources

NASA Science — Halley's CometJPL — Orbital data

Image credits

Nucleus shapes use public observed models, or independent approximations constrained by observed sizes when no complete global model is available. No global comet-nucleus albedo maps are available here, so materials, coma, and tails are illustrative rather than current observations.

Surface texture:Phil Stooke / NASA PDS Small Body Shape Models V2.0 · License · Rendered by ORBIT

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