Ultra Thin Moon at noontime Just over a day from New Moon with the Orion 10" f/3.9 Newtonian Astrograph July 2, 2016 Uploaded 7/3/16 Left: daytime moon very close to the Sun. Right: Telescope setup required to image this encounter.

 This was certainly one of the most difficult lunar imaging sessions I have ever done! With the thin crescent moon only 24 hours from new, the only time I could actually image the crescent was at noon at the zenith. Even if I had a perfect eastern horizon, the seeing down that low would have been excruciating. Fortunately the seeing I had at the zenith permitted some details to be resolved, and the transparency was good for a typical monsoon high humidity afternoon. To be able to image with the high sun blasting my black telescope tube, I wrapped the scope with a huge silver mylar space blanket. Next I had to add a big black internally carpeted baffle on the front of the tube so that the direct sunlight would not enter the focuser from the side. By removing only the two inch dust cap on the front scope cover, I could then safely point the scope at the sun and center it by its projected beam on a white paper. An interesting trick when you do this, is to project the sun about four feet away onto a white card. Then the beam is nearly parallel coming out of the eyepiece. When you point away from the sun in a featureless blue sky, the view is in infinity focus. The setting circles (manual mind you) were dialed in to the RA of the Suns current position. (DEC is always right on a permanently mounted base) Next the moons current position was dialed up using a planetarium program Stellarium to get the current lunar coordinates.

When a wide field ocular was inserted, the moon was just barely visible in very brilliant light blue sky! Fortunately, the camera is much better at seeing low contrast objects like this, and using the IR filter to cut through the bad daytime seeing made it easy to see the moon and some surprising features! The whole idea here was to see if there was a contrast boost using the IR filter vs just visible light. The result of THAT experiment will surprise you...

Note: Conventional usage of South is up in all images, more info below. (So Rik, stand on your head please.)
Here you can see the difference between a normally exposed image on the left with no filters, and the image on the right with an IR pass filter. While the signal to noise is the same, the sharpness in IR is 2 - 3x better! To compare the S/N, the brightness of the same bright patch on the moon was measured. Then the background sky in each image. The Delta B indicates the contrast. It was the same - 21 ADU. So next to the Sun, where the sky is really more white than blue, and with tons of dust and vapor back scatter, there is no contrast boost. Select size for enlarged view: 1290 x 960
Here is a two part panorama at prime focus with the 10 inch and IR pass filter. You can just start to see the unusual black shadow filled craters on the limb. Mind you, the sky was VERY bright when I took this image! So bright in fact that it was very difficult to get an evenly lit shot. Ive darkened the sky here to improve the contrast in what was a very low contrast barely there kind of image. Select size for enlarged view: 1290 x 960
Same image as above but colorized with RGB data. This is NOT what I was seeing in the eyepiece. What I saw was an almost invisible crescent, that was shaking violently in the very bad seeing at noon, with the sun baking the observatory and telescope. Select size for enlarged view: 1290 x 960
This image is the combined montage with the 2.5x Barlow. It is large sized and you will have to scroll up and down the image to see it all. It is about half the size of the original. Look about in the middle for the black filled craters. Wild! Select size for enlarged view: 2400 tall
Individual close ups at 75% scale for intricate details: These are with the 2.5x Televue Powermate, yielding about 2500mm EFL On the left is the original image, on the right Ive labeled the features I could identify with the Virtual Moon Atlas.
Select size for enlarged view: 1290 x 960
Select size for enlarged view: 1290 x 960
Select size for enlarged view: 1290 x 960
Select size for enlarged view: 1290 x 960
Note the black craters with shadowed rims! Select size for enlarged view: 1290 x 960
Select size for enlarged view: 1290 x 960
Select size for enlarged view: 1290 x 960
Select size for enlarged view: 1290 x 960
Select size for enlarged view: 1290 x 960
Select size for enlarged view: 1290 x 960
Select size for enlarged view: 1290 x 960
Select size for enlarged view: 1290 x 960
Very difficult to identify anything in this image! Select size for enlarged view: 1290 x 960
One closer view with the 5x Powermate is here.
5x close up in pretty bad seeing. But the black dark shadow filled craters Cardanus and Krafft that are backlit with dark shadowed rims are pretty outrageous. Along the limb we see more smaller black craters. I have never seen anything quite like this ever in my lunar images! Select size for enlarged view: 1290 x 960
Processing: 25/1200 best frames, alignment in Autostakkert, USM, Levels and Contrast Masking In Photoshop CS2.
Instrument: Orion (GSO) 10" f/3.9 with 2.5x and 5x Powermates Platform: Astrophysics AP1200 CCD Camera: Image Source DMK 51 Filter: Orion IR Pass Exposure: 1/30 sec 12fps for 2.5x, 1/13 sec for 5x. Location: Payson, Arizona Elevation: 5150 ft. Sky: Seeing 1.5/5, Transparency 7/10 Outside Temperature: 75F