Author/Authors :
Johnson، نويسنده , , R.E. and LeBlanc، نويسنده , , F. and Yakshinskiy، نويسنده , , B.V. and Madey، نويسنده , , T.E.، نويسنده ,
Abstract :
The sputtering and decomposition of the surface of Europa by fast ions and electrons lead to the production of an atomosphere containing sodium and potassium atoms. Here time-of-flight energy distributions are measured for Na and K sputtered from a vapor-deposited ice by 200-eV electrons. These data are then used in a Monte Carlo simulation for alkalis in Europaʹs atmosphere. Na/K ratios versus distance from Europa are calculated and compared to the recent observations in the range 6 to 18 Europan radii from the surface. Normalizing to the observations, the Na/K ratio for the loss rates is ∼27 and the ratio for the average surface source rates is ∼20. These ratios are very different from the Na/K ratio at Io and are larger than the Na/K ratio suggested for Europaʹs putative subsurface ocean, consistent with fractionation on freezing and upwelling of ocean material.