- The eccentricity
of the Moon's orbit
is 0.0549 or 5.49 %.
- This means the Earth-Moon
distance varies up and down from the mean
Earth-Moon
distance by about 5.5 %. The total range of variation is 11 %.
The 11 % variation in DISTANCE causes
Moon's angular diameter
to vary by 11 % too.
Note that angular diameter
is always an "apparent" quantity.
In astro-jargon,
"apparent" means as seen from a particular vantage point which is
understood to be Earth, unless otherwise
stated.
- The variation in
angular diameter
is probably too small ever to be noticed by casual observation since we usually see the
Moon
at perigee and
apogee without a convenient
sufficiently accurate natural STANDARD OF COMPARISON.
But difference in
angular diameter
of the Moon
is striking if you directly compare
the angular diameters
at perigee and
apogee
with the correct relative apparent size
as in the image.
- On the sky,
the difference in the angular diameters
is just a bit too small to be seen by the unaided
naked eye.
However, it is easily measured with simple instruments.
- Note that the images at
perigee and
apogee both
show full moons.
In fact, only occasionally does either
apsis (pl. apsides) coincide with
a full moon.
To explicate: the
mean anomalistic month = 27.554549878 days (J2000) is the
mean period between like apsides, but
mean lunar month = 29.530588861 days (J2000).
So there is a fairly long interval before
an apsis
and full moon
cycle back into concidence after a given coincidence.
Astronomical perturbations
account for the fact that the
mean anomalistic month = 27.554549878 days (J2000)
and the
mean lunar sidereal month 27.321661547 days (J2000) ≅ 27.32166 days (to 7 digits) ≅ 27.3 days
(the true
orbital period
relative to the
observable universe)
are NOT the same.
- By the by,
a supermoon is
a near-perigee
occurrence of a full moon
or new moon---but
"supermoon" is just phony modern made-up term.
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