Europa - Ultraviolet emissions and the possibility of atomic oxygen and hydrogen clouds

Details Europa - Ultraviolet emissions and the possibility of atomic oxygen and hydrogen clouds Europa - Ultraviolet emissions and the possibility of atomic oxygen and hydrogen clouds

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...225..325w&link_type=abstract

Astrophysical Journal, Part 1, vol. 225, Oct. 1, 1978, p. 325-334.

Astronomy and Astrophysics

Astronomy

5

Emission Spectra, Europa, Hydrogen Clouds, Oxygen Atoms, Ultraviolet Astronomy, Ion Production Rates, Pioneer 10 Space Probe, Ultraviolet Photometry, Data Reduction, Europa, Ultraviolet, Emissions, Ice, Oxygen, Hydrogen, Clouds, Pioneer 10, Density, Radius, Jupiter, Satellites, Water, Radiation, Particles, Impacts

Scientific paper

Emission signals from Europa with wavelength below 800 A were detected by the Pioneer 10 ultraviolet photometer. In the present paper, improved procedures for data reduction are used to determine the spatial region as well as the intensity of the suggested emission sources. The observations indicate a cloud with a radius of about 1.5 Jupiter radii and an apparent brightness of approximately 10 rayleighs for a wavelength of 500 A. It is argued that neutral oxygen atoms, along with neutral hydrogen, are produced through dissociation of water ice on the surface of Europa by particle impact. Electron impact ionization excitation of oxygen atoms in the resulting cloud then gives rise to the observed emission. The present source brightness and cloud radius results are used to estimate an oxygen column density of the order of 10 trillion per sq cm, while the density of atomic hydrogen is at most 100 billion per sq cm and 1 trillion per sq cm for molecular hydrogen.

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