ORBIT Solar System Explorer

COMET PROFILE 2P / ENCKE

Encke's Comet

Frequent returns, repeated solar heating

A short-period comet orbiting the Sun in about 3.3 years, with a nucleus roughly 4.8 km across. It returns much more often than Halley's Comet.

Rendered view of Encke's Comet
Illustrative surface and shape · Image credits
Model orbital period
3.3 yr
Orbital inclination
11.4°
Model perihelion
0.34 AU

01 / Overview

Meet Encke's Comet

Encke circles the Sun in about 3.3 years, frequently crossing the inner Solar System. Its elongated orbit brings it from a cooler outer reach to intense perihelion sunlight, repeatedly driving activity and material loss. Debris associated with the Taurid complex links this comet to a wider interplanetary dust environment.

02 / Key data

Core parameters

Model orbital period
3.3 yr
Orbital inclination
11.4°
Model perihelion
0.34 AU
Model aphelion
4.10 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
  • Encke's Comet orbits the Sun in only about 3.3 years.

  • Encke's Comet is named for Johann Encke, who calculated its periodic orbit.

  • Pierre Méchain first observed Encke's Comet in 1786.

  • Encke linked observations from different years to confirm they described the same body.

  • Encke's official designation is 2P, among the earliest numbered periodic comets.

  • Encke's nucleus is about 4.8 km across, far smaller than a major planet.

  • Encke's Comet is associated with the Taurid meteoroid complex.

  • Encke's perihelion lies inside Mercury's orbit; its far end reaches beyond Mars.

  • Encke's highly eccentric orbit causes large changes in its distance from the Sun.

  • Frequent returns expose Encke repeatedly to solar heating and material loss.

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 — Encke'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:JPL SBDB physical constraints; no public global nucleus model; ORBIT shape approximation · License · Rendered by ORBIT

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