If small comets are as numerous in the inner solar system as Frank et al. [1986a] have recently proposed, large and easily detectable amounts of hydrogen would be generated in interplanetary space. Inhibition of water vapor production by a factor of 3 × 10−9 by very thick dust mantles would be necessary to prevent excitation of a detectable interplanetary Lyman α glow. Other optical problems associated with the cometesimals are also discussed.
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T. M. Donahue (1987) studied this question.
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