The eclipse postings on RASC discussion lists to date have been of images - both still and time-lapse. They have been phenomenal! However, on March 14, 2025, I chose 10x42 IS binoculars, a pre-printed map of the Moon and my SQM* as my observing tools of choice.

We were in our backyard where we had full view of the orb during our observing session 1am-4am. With battery operated gloves and socks and sandwiched between two sleeping bags on our park bench, we enjoyed the show the Solar System offered. 

I drew the lines as the Moon's surface was darkened by the Earth’s shadow up until 3:30am. However, in totality at 4 am, there was still what we referred to as a ‘polar cap’ on the N-NE limb. We did not observe past 4am to determine the timing of the re-illumination of the lunar surface.

From my rough notes:
  • 3:03am: SW limb showing hints of pink visually and in binoculars 
  • 3:30am: ‘polar cap’ still looked to be illuminated on its limb but no features could be discerned in binoculars.
  • 3:38am: ‘polar cap’ now turned pinkish but not as bright.
I also measured the darkening of the skies as the Moon was eclipsed. Here is the summary of my readings.
 
Time
(AM ADT)
SQM

Temp. (° C)

1:25 17.64 not taken
2:14 18.14 not taken
2:29 18.50 -5
2:47 18.57 -6
3:01 19.02 -7
3:11 19.15 -7
3:19 19.15 -7
3:30 19.18 -7
4:00 19.22
-8℃

Sometime between 3:30am and 3:50am we noticed that stars were visible in Jerry’s telescope and now my binoculars.

In looking up, I saw several stars and quickly confirmed I had correctly identified the stars of Leo’s tail NW of the Moon. In binoculars, I could easily see 4 stars in a slight curve within the 6.5° FOV - p4 Leo, 58 Leo, c Leo, and x Leo. Gienah Corvi (𝜸 Corvus) was to the SW; I didn’t seek out the remaining stars of that constellation as I was so enthralled with Leo still being observable and so high in the sky.
 

* The Sky Quality Meter (SQM) is a handheld device used to measure the luminance of the night sky. It is
typically used by amateur astronomers to quantify the sky glow aspect of light pollution, and uses units of "magnitudes per square arcsecond" favoured by astronomers.