“y― ALPO-Japan Latest

Saturn Image 2025/11/06(UT)
ŠFμL–η,ˆΙ“‘—ΉŽj,—ι–Ψ —²,X“cŒυŽ‘,’ίŠC•q‹v,ŒFXΖ–Ύ,”φθŒφˆκ
Mike Wolle,Vincenzo della Vecchia,Laurent Dulbecco,Paul G. Abel
N.Minagawa,S.Ito,M.Wolle,T.Suzuki,M.Morita,T.Tsurumi,V.della Vecchia,T.Kumamori,L.Dulbecco,K.Ozaki,P.Abel

Nobuya Minagawa

α“Œ‹ž“s  —§μŽs  ŠFμL–ηβ[Nobuya Minagawa:Tokyo Japan]

Satoshi Ito
ƒV[ƒCƒ“ƒO‚ͺˆ«‚­‚ΔƒJƒ‰[‚Ν’ϊ‚߁AΤŠO‚Μ‚έŽB‰e‚΅‚ά‚΅‚½B

αˆ€’mŒ§  t“ϊˆδŽs  ˆΙ“‘—ΉŽjβ[Satoshi Ito. Kasugai City,Aichi,Japan]

Mike Wolle

[Mike Wolle : Austria ]

Takashi Suzuki

[Takashi  Suzuki  (Hachiouji-City Tokyo  Japan)]
α“Œ‹ž“s”ͺ‰€ŽqŽs  —ι–Ψ  —²β

Mitsuji Morita
‹C—¬‚ͺŒƒ‚΅‚­ƒsƒ“ƒg‚ͺ‡‚ν‚Ή‚Γ‚η‚’‚Ω‚Η‚ΜƒV[ƒCƒ“ƒO‚Ε‚΅‚½B

αŽ ‰κŒ§ŽηŽRŽs  X“cŒυŽ‘β[Mitsuji Morita:Siga Japan]

Toshihisa Tsurumi

α‰ͺŽRŒ§‰ͺŽRŽs  ’ίŠC•q‹vβ[Toshihisa Tsurumi:Okayama-City Okayama-Prefecture Japan]

Vincenzo della Vecchia

[Vincenzo della Vecchia : [Aversa,Italy]

Teruaki Kumamori
—‚‰ΊŒƒ‚΅‚’ƒV[ƒCƒ“ƒO‚Ε‚΅‚½‚ͺ‰½‚Ζ‚©‚ά‚Ζ‚ά‚θ‚ά‚΅‚½B

α‘εγ•{δŽs ŒFXΖ–Ύβ[Teruaki Kumamori:Ohsaka Japan]

Laurent Dulbecco

[Laurent Dulbecco : Dusseldorf,Germany]

Kimikazu Ozaki
”–‚’Œ¦‘w‰_‚ͺ‚ ‚θA‹C—¬‚ΰˆ«‚­AΧ‚’—Φ‚ͺƒ‚ƒjƒ^[γ‚Ε–\‚κ‚Δ‚’‚āEEEEB

[Ki.Ozaki,Sobue Inazawa Aichi JAPAN]
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Paul G. Abel
After 30 years of amateur astronomy I finally managed to see a transit of Titan.  Conditions were not good, there was frequent passing cloud and seeing was only average at best.  Nevertheless, I was able to see Titan pass on to the disk.  One thing I did notice, just to the left of Titan there seemed to be a bright spot (see drawings 2 and 3).  Rhea was in transit but much further away so I'm unsure if this was a contrast effect or a real bright spot in the EZ.  Also:
The Globe:
 ESPR: A vague greyish region- no sign of a SPB.
 ESSTB-STB: Two light brown belts visible, the regions around them still retain a subtle greenish tint.
 ESEB: A broad band and again I could see two components although the SEB(N) was the darkest
 EEZ: A light zone and there seemed to be an EBV in the EZ(S) and the ShRG can be seen in the EZ(N)
 ENEB: Another broad band with two components.  Titan can be seen moving along the NEB(S).
 ENNTB-N3TB: Two faint belts that seem to have a bluish colour to them.
 ESPR: A vague region again with little detail.
The Rings: These are very narrow now but there is a faint dark patch in the rings which indicate the Cassini Division.  The rings appear to be of uniform thickness and I observed no condensations along the ansae.  
By 2125UT the planet was getting low to the roofs and the seeing became quite impossible and observations were concluded.

[Paul G. Abel:Leicester:United Kingdom]

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