木星 ALPO-Japan Latest

Jupiter Image 2020/07/21(UT)
大田 聡
Guilherme Grassmann,Bruce Macdonald,Christofer Mauricio Baez Jim,Vincenzo della Vecchia,Lucas Magalhaes Teixeira Gon,Michel Jacquesson,Pericles Enache,Trevor Barry,Vlamir da Silva Junior,Peter Edwards,Constantin Sprianu,Michael Wong,Andy Casely
G.Grassmann,B.Macdonald,S.Ota,C.Baez,V.della Vecchia,L.Magalhaes,Michel.J,P.Enache,T.Barry,V.da Silva Jr.,P.Edwards,C.Sprianu,M.Wong,A.Casely

Guilherme Grassmann

[Guilherme Grassmann,Americana-San Paulo,Brasil]

Bruce Macdonald

(Bruce Macdonald : Punta Gorda,Florida USA)

Satoshi Ota

[Tomigusuku city Okinawa Japan]
≪沖縄県  豊見城市  大田 聡≫

Christofer Mauricio Baez Jimenez
15 images de-rotated using WinJUPOS.

[Christofer Mauricio Baez Jimenez :Santo Domingo,Dominican Republic.]

Vincenzo della Vecchia

[Vincenzo della Vecchia : [Aversa,Italy]

Lucas Magalhaes Teixeira Goncalves


[Lucas Magalhaes Teixeira Goncalves :Sao Bernardo do Campo,SP,Brazil]

Michel Jacquesson



[Michel Jacquesson : Sevigny-Waleppe (Ardennes) France]

Pericles Enache




[Pericles Enache,Sao Paulo,Brazil]

Trevor Barry
Imaged Jupiter July 21st in good seeing but poor transparency.
All data was captured through a veil of cloud which dropped the histogram 30 to 40% lower than normal.
Even though the live feed was dimmer than normal very fine detail was still quite apparent.
Have a small bright elongated oval well resolved in the NNTB.
Several tiny dark spots are resolved along the NTB with quite intricate structure resolved within the NEB.
A prominent dark festoon extends back into the EZ from the Northern edge of the NEB.
Fine detail is resolved in a band along the Northern edge of the SEB.
Two small bright ovals are resolved in the SSTB. Quite surprising to see this level of detail through the cloud.

[Trevor Barry:Broken Hill:Australia]

Vlamir da Silva Junior
GRS is setting here,followed by Oval BA. Note the STZ-AWO,it's very close to the CM at the time of the IR image.
A1,A2 and A3 on SSTB are well visible on the following side.
The sequence of favorable seeing together with the close proximity of the recently occured oposition of the planet helped to find hard to see spots and ovals like S4-LRS-1 and N5-AWO
(using BAA maps to help identifying it) and also moving from one image to another to see movement,
like a gif. WS-4 is well seen on NNTB.










[Vlamir da Silva Junior : Sao Paulo,Brazil]

Peter Edwards

[Peter Edwars: West Sussex United Kingdom]

Constantin Sprianu



[Constantin Sprianu,Otopeni,Romania]

Michael Wong



[Michael Wong,Hong Kong,China]

Andy Casely










[Andy Casely,Sydney,Australiaa]

ALPO-Japan Latest Jupiter Section
2020/07/22
2020/07/20