The Lunar 100 was created by Charles A. Wood who states: "The
Lunar 100 list is an attempt to provide Moon lovers with
something akin to what deep-sky observers enjoy with the Messier
catalog: a selection of telescopic sights to ignite interest and
enhance understanding. [It is]... a selection of the Moon's 100
most interesting regions, craters, basins, mountains, rilles,
and domes."
Woods challenges "...observers to find and observe them all and,
more important, to consider what each feature tells us about
lunar and Earth history."
The Lunar 100 features are arranged from the easiest to view to
the most difficult. The Moon itself is L1. L2 is Earthshine, and
L3 represents the dichotomy between the Lunar highlands and the
Lunar Maria. While the Lunar 100 are concentrated all on the
nearside of the Moon, they can not be seen in a single night or
a single month. Some of them require special lighting conditions
or phases of the Moon, and others, in addition, require very
favorable librations of the Moon to bring them into view. The
Lunar 100 is an observing list. However, the equipment at the
3towers Observatory was used to image the Lunar 100, mainly
using the
web cam techniques detailed.
The bright crater
at bottom center is Menelaus. North of it is Bessel.
Sulpicius Gallus is the crater West of Menelaus and half
shadowed. Most of Mare Serenitatis is seen in this
image.
71. Sulpicius
Gallus dark mantel
9.7 days
71. Sulpicius
Gallus dark mantle
18 days
72. Atlas
dark-halo craters
4.5 days
72. Atlas
dark-halo craters
7.6 days
72. Atlas
dark-halo craters
9.7 days
72. Atlas dark-halo
craters
16 day
Hercules is the
crater with a small inner crater. Atlas is next to
Hercules and has dark spots. Endymion is the
large, flat crater Northeast of Atlas.
73. Smythii basin
4
days
73. Smythii basin
5
days
Mare Smythii is on
the Eastern edge of the Moon. Langrenus is the large
crater with central peaks.
73. Smythii basin
14.3 days
Mare Smythii at
Full Moon.
74. Copernicus H dark-halo impact crater
10
days
The tiny crater
Southeast of Copernicus with a dark halo around it is
Copernicus H. Directly South of Copernicus is the double
crater Fauth and Fauth A.
74. Copernicus H
dark-halo impact crater
11.7 days
74. Copernicus H
dark-halo impact crater
21.7 days
75. Ptolemaeus B
8
days
The largest
craters are from top to bottom, right to left are
Hipparchus, Albategnius, Ptolemaeus, and Alphonsus. In
the floor of Ptolemaeus is the small crater Ammonius and
North of Ammonius is a saucer like depression which is
Ptolemaeus B.
75. Ptolemaeus B
8.0
days
76. W. Bond
8.1
days
W. Bond is the
large flat crater with a small inner crater.
77. Sirsalis Rille
13
days
77. Sirsalis Rille
13.1 days
78. Lambert R
22
days
Below center is
the crater Pytheas and above center is Lambert. Lambert
R is a "ghost" crater South of Lambert. Euler is
near the left edge, Timocharis is East of Lambert, and
Eratosthenes is at the lower right hand corner.
78. Lambert R
23
days
Lambert is below
center with a large "ghost" crater just South of
Lambert.
79. Sinus Aestuum dark-mantle deposit
9
days
79. Sinus Aestumm
dark-mantle deposit
21.7 days
80. Orientale basin
14.7 days
80. Orientale basin
and Western Limb of the Moon at Full Moon
14.7 days
LA - Lacus Autumni; MC - Montes Cordillera; LAe -
Lacus Aestatis; MR - Montes Rook