The phase cycle
A moon is
full when it stands on Jupiter’s night side, opposite the Sun, and
new
when it crosses between Jupiter and the Sun. The Sun scarcely shifts against Jupiter’s sky
in a few days, so each phase cycle is simply the orbit, reckoned against the Sun:
1.7699d for Io,
3.5541d Europa,
7.1664d Ganymede,
16.7536d Callisto.
Every full moon is eclipsed
Jupiter’s axis leans only
3.1°, so the shadow never strays far
from the orbits. Io, Europa and Ganymede fall into it at
every full phase without exception.
Callisto alone, at
26 Jupiter radii, can ride clear — it passes years
untouched, then keeps a season of eclipses near Jupiter’s equinox, once in about six years.
Jupiter-shine
The unlit face is not black. Jupiter fills
19.5° of Io’s sky,
some
38 times the width of our own full Moon, and floods the night side
with reflected light. That glow is brightest at new phase — when Jupiter, seen from the moon,
is itself full — and it is drawn here.
Authorities & accuracy
Satellite positions follow Meeus,
Astronomical Algorithms, ch. 44 (low precision),
reproducing his worked example to within
0.04 Jupiter radii and good
to about
0.1 throughout. Contacts are refined by bisection against the
true umbral cone and the oblate disk. Codes follow the
Astronomical Almanac:
Ec eclipse,
Sh shadow,
D disappearance,
R reappearance,
I ingress,
E egress.
Good for planning, not for occultation timing.