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plasma tail

astronomy
Also known as: Type I tail, ion tail

Quick Summary

A plasma tail, also known as a Type I tail, is one of two tails that can form around a comet. This tail is composed of ionized molecules and radicals that are released from the comet's coma. These ions interact with the solar wind and the Sun's magnetic field, causing them to flow away from the Sun at high speeds, typically exceeding 400 km per second.1

The plasma tail points almost directly away from the Sun because the solar wind's velocity is much greater than the orbital velocities of most comets. These tails often appear blue due to the presence of CO+ molecules, though H2O+ is the major ion. Occasionally, a comet's plasma tail can disconnect and fade, with a new one forming, which can happen when the comet crosses magnetic sector boundaries in the Sun's field.1

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2 Britannica Sources
  1. comet - Tails
  2. comet

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