(1) Contact timings, including first visibility of the penumbra
(2) Danjon scale estimates of the umbra
brightness
(3) Crater contact timings (see table of predictions below)
(4) Light curve, either of the Moon (through reversed binoculars) or
the Naked Eye Limiting magnitude during the eclipse (see below).
(5) Visual impressions.
Predicted timings
First contact with umbra –
Start of totality
–
End of totality
–
End of eclipse –
Danjon scale estimates
L=0 Very dark eclipse. Moon
almost invisible, especially at mid-totality.
L=1 Dark eclipse, grey or brownish in
coloration. Details distinguishable only with difficulty.
L=2 Deep red or rust-coloured
eclipse. Very dark central shadow, while outer umbra is relatively bright.
L=3 Brick-red eclipse. Umbral
shadow usually has a bright or yellow rim.
L=4 Very bright copper-red or orange eclipse. Umbral shadow has a bluish, very bright rim.
Naked eye limiting magnitude
during the eclipse
The following is a list of crater contact timing predictions from the Royal Astronomical Society of Canada. However, the exact size of the umbra and hence the times of contacts are unpredictable.
Crater |
Immersion |
Observed |
Crater |
Emersion |
Observed |
Grimaldi |
|
|
Grimaldi |
|
|
Billy |
|
|
Aristarchus |
|
|
Campanus |
|
|
Kepler |
|
|
Kepler |
|
|
Billy |
|
|
Tycho |
|
|
Plato |
|
|
Aristarchus |
|
|
Pytheas |
|
|
Copernicus |
|
|
Timocharis |
|
|
Pytheas |
|
|
Copernicus |
|
|
Timocharis |
|
|
Campanus |
|
|
Dionysius |
|
|
Aristoteles |
|
|
Manilius |
|
|
Eudoxus |
|
|
Menelaus |
|
|
Tycho |
|
|
Plinius |
22:21 |
|
Manilius |
00:37 |
|
Goclenius |
22:22 |
|
Menelaus |
00:41 |
|
Plato |
22:23 |
|
Dionysius |
00:45 |
|
Taruntius |
22:27 |
|
Plinius |
00:45 |
|
Langrenus |
22:27 |
|
Proclus |
00:56 |
|
Eudoxus |
22:28 |
|
Taruntius |
00:59 |
|
Aristoteles |
22:31 |
|
Goclenius |
01:01 |
|
Proclus |
|
|
Langrenus |
|
|