Hi Massimo,
thanks for your question;
Fenerit wrote:I wish ask to you if you have experimenticed such backscattering condition or not,
Oh, yes, I did.
With the reddish colour I associated the huge heat on the darker back of 51 Pegasi/b. Incidentally, it took some time to realize this light-scattering effect...
At first I've made this work - inspired by a ZDF-TV-documentary - with a good portion of faith and several barrels of intuition. And - look at the very first images - with John's help.
Then I spent hours and days trying to learn and understand the fine tuning of the Mie-parameters. Wasn't easy...
Sometimes the colour was right, but too dark; or the density good, but the height of the atmosphere was wrong; sometimes the cloud layer looked like a snow storm in the night or everything else turns into an absurdity; or something else... But I kept my nerves.
Encouraged by Hungry4info - I think she is very competent in "extrasolar" related things - I intend to make it publish now.
Do not misunderstand me; if someone has good arguments for a better presentation of my 51 Pegasi/b interpretation; I'm willingly to correct this or that.
I emphazised in previous posts that my work on the 51 Pegasi/b map is pure fiction (my work on the map; not the extrasolar planet 51 Pegasi/b itself). Just good for an illustrated educational view.
Because 51 Pegasi/b is too bright I think to recognize any detail on its hot surface. In addition planet "b" is outshined by its related star...
(But the stars in Celestia - our sun, too - are also "unreal". In reality you can't look at the surface of a star, it's much too bright...)
But one thing I know for sure; the real planet 51 Pegasi/b looks quite different from this...
it's just my imagination...
But I'm looking forward for the first - real - images of 51 Pegasi/b.
So, thanks for your ambitious criticism
Michael