λ=190゚Ls,
(ω=075°- 082°W,
φ=20°S),
δ=11.5",
ι=43°
Seeing: 2-3 /10. Observation at a break in the clouds.
Note:
Ophir-Candor looks whitish bright (so in B) affected by the evening mist from Xanthe. Compared with Ophir, the brightness of the Syria Planum (the area following Solis L) is not definite. Phasis is apparent.
Use is made of an f /7.7 Newtonian extended to f /50 having a 25 cm speculum equipped with an ST-5C (at -5゚C).
Image data are
30 IR images each exposed with 0.5~0.8secs
30~50 R + IR Rejection images each with 0.4~1 secs
10~30 G + IR Rejection images each with 0.8~1.2 secs
10 B + IR Rejection images each with 10 secs
Filters: Koh-Ei-Sha's interference RGB filter of Type 3.
The Morita Observatory is located (132.3°E, 34.3°N) at Hatsuka-ichi, Hiroshima, Japan.