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Large intensities of hot positive ions are observed out to distances of several hundred meters from the space shuttle Challenger (Spacelab 2) with a plasma analyzer on board a small free‐flying satellite, the Plasma Diagnostics Package. This ion plasma is inferred to be generated by the charge exchange of ionospheric O+ ions with a large cloud of water molecules from the space shuttle. The measured ion density ranges from ∼30 to 104 H2O+ ions cm−3. The hot ion plasma forms an ion trail in the wake of the space shuttle. A model for the water vapor cloud provides the basis for density estimates as high as 109 H2O molecules cm−3 at a distance of 50 m from the space shuttle. Thus the space shuttle possesses a substantial coorbiting atmosphere.
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Paterson et al. (1989) studied this question.
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