Ly@Pluto

The Alice instrument on New Horizons will perform several observations of Pluto’s far-ultraviolet (FUV) airglow emissions during its July 2015 flyby. While Pluto’s atmosphere is dominated by N2, simulations suggest that the brightest airglow signal at Pluto will actually be due to Lyman alpha (Ly α ) emissions of atomic hydrogen. This is because H atoms, produced at lower altitudes due to the photolysis of CH4 and other hydrocarbons, rise up above the homopause to become an important constituent of the atmosphere at high altitudes, and are able to scatter the very bright Ly α lines from the Sun and the interplanetary medium (IPM). The IPM Ly α signal at Earth is very much less than direct solar Ly α , but IPM Ly α falls off much more slowly than r - 2 , so that at Pluto’s distance from the Sun the two sources are of comparable strength. Detailed simulations of its Ly α emissions indicate that Pluto will appear dark against the IPM background, but that enough contrast exists for the useful extraction of H densities from the Alice observations. As viewed on approach (or from the inner solar system), the Ly α brightness of the disk of Pluto is expected to be ∼30 R, against an IPM background of ∼90 R.