Using our gravity tomography method, I can create an image of your plume at any depths in the form of vertical and horizontal sections of the density change relative to the PREM model.

For this I need the coordinates of the plume region.

Good luck.

Rudolph Greku,

Ukraine Academy,

not Chinese Academy

Dears Satyendra Kumar and Rudolf Greku:

Interesting question, interesting answer.

Saturn's moon Enceladus is the smallest body in the Solar System known today to be geologically active. Giant water plumes erupting, icy jets spew 200 kg/sec of water, with no significant variations over the Cassini´s mission. The strongest jets are more variable, though Enceladus eruptions are mostly water vapor, with a variable amount of ice grains [Hedman et al. 2018].

Please, I attached two papers to try to help you:

The composition and structure of Enceladus’ plume from the complete set of Cassini UVIS occultation observations C.J. Hansen, L.W. Esposito, J.E. Colwell, A.R. Hendrix, G. Portyankina, A.I.F. Stewart, R.A. West. Icarus 344 (2020) 113461.

Past, present, and future tectonics of Enceladus by L. Czechowski. 49th Lunar and Planetary Science Conference, 2018.

Best regards, Mario E. Sigismondi

Thank you very much for your valuable time @Rudolf Greku and @Mario Emilio Sigismondi.

I will look at both perspective and may be extend the discussion.

Thanks again!

Satyendra Kumar