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Supplement Numbers 3 and 4 to the ‘
USAF PHOTOGRAPHIC LUNAR ATLAS

Gerard P. Kuiper Ewen A. Whitaker
Robert G. Strom John W. Fountain

Stephen M. Larson

Photographic Reproductions
Part I: 61-in NASA Telescope, Catalina Observatory
Part II: 61-in Astrom. Telescope, US. Naval Observatory .
and
Tables and Reference Charts on Lunar Orbiter Missions

PubHshedforthe

AIR FORCE CAMBRIDGE RESEARCH LABORATORIES
Office of Aerospace Research

bythe
LUNAR AND PLANETARY LABORATORY
.S UNIVERSITY OF ARIZONA
" 1967

Contributions of the Lunar and Planetary Laboratory No. 4

 

Published by the Lunar and Planetary Laboratory, University of Arizona
for the U.S. Air Force under Contract No. AF19(628)—4332
Photographic Printing by Ray Manley Commercial Photography
Published 1967
Library of Congress Card Catalog Number 68-63335

 

CONSOLIDATED LUNAR ATLAS

1. General Concept of Atlas

In 1960 a selection of the best available lunar photogra-
phy was published in the Photographic Lunar Atlas (Kuiper,
Arthur, Moore, Tapscott, Whitaker, Univ. of Chicago Press,
1960). The reproductions were halftones. In spite of the care
and supervision given this publication, some detail, especially
of a photometric nature, was lost although the resolution was
not appreciably impaired.

Since 1960 several lunar programs have endeavored to
obtain improved photographic coverage. Among these were
the photography with the 61-in. telescope of the Lunar and
Planetary Laboratory, which was started in October 1965; the
full-moon photography on slow, fine-grained and very contrasty
plates with the 61-in. Astrometric Telescope of the US. Naval
Observatory at Flagstaff; a short series with the Lick 120-in.
telescope at the Coudé focus; and photography with the tele-
scopes at the Pic du Midi Observatory, especially with the new
43—in. By late 1966 the average gain in resolution attained over
the material available in 1960 was by a factor of 2. Further
improvement over the Photographic Lunar Atlas was achieved
by using photographic reproductions rather than printed half—
tones, thus preserving photometric detail and a range of con-
trast unobtainable in halftone printing.

On page 5 of the text accompanying the Photographic
Lunar Atlas reference is made to “Future Supplements” Nos.
1—4, of which (1) the Orthographic Atlas (Kuiper, Arthur,
Whitaker, Univ. of Arizona Press, 1961) and (2) the Recti-
fied Lunar Atlas (Whitaker, Kuiper, Hartmann, Spradley,
Univ. of Arizona Press, 1963) have appeared. The present
Consolidated Lunar Atlas combines Supplements Nos. 3 and

4, thus completing the series announced in the 1960 Atlas.

In View of the greatly enlarged interest in high-quality
lunar photography resulting from the current space program
and the now successfully completed Orbiter missions, special
emphasis is placed here on types of information where current
earth-based photography still excels: (a) low-oblique photog-
raphy, which brings out low domes, lava beds, and other struc-
tures of considerable horizontal dimension, but of low vertical
relief; and (b) full-moon photography, which presents photo-
metric information totally unavailable from even high-resolu-
tion records taken with 20° or 300 sun angles. To illustrate:
The excellent photograph, Orbiter V, M—165, shows a meander-
ing channel near the center of the record with a horizontal reso-
lution of approximately 20 m. In the Consolidated Atlas this
area is covered at low illumination on Sheet D20. The Atlas
photograph shows three large low domes (5 mm diameter on
the photograph, or 12 km on the moon), two of which are
barely recognizable on the Orbiter records, and the third of
which is quite invisible. Yet, it is this invisible dome that
apparently has caused the channel to make a major, otherwise
incomprehensible, swing toward Copernicus. Another major
dome occurs near the west edge of the Orbiter photograph of
which only the central crater or caldera is apparent. The recog—
nition of the dome and its structure requires very low illumina-
tion, such as possessed by D20 near the terminator. Also, a
very large shield-like uplift is seen on D20, southeast of the
ridge placed at the center of Orbiter V, M-165. This shield is
totally invisible on the Orbiter photograph. Many other exam-
ples could be cited. They stress the need of a large range of
sun angles, including very low obliques, for the interpretation
of lunar surface structures.

 

 

2 G. P. KUIPER, E. A. WHITAKER, R. G. STROM, J. W. FOUNTAIN, AND S. M. LARSON

Accordingly, special emphasis was placed on obtaining
for this Atlas telescopic photographs extending as close as
possible to the terminator, which for mare terrain required
comparatively long exposures; and on retaining all recorded
detail in the reproductions. To this end a fluorododging tech-
nique was used in the copying of the originals on film positives,
from which the printing negatives were made to the scale of
the present Atlas sheets. The dodging across the original nega—
tives was optimized by adjusting the separation between the
fluorescent screen and the emulsion. Sometimes unsharp masks
were used to extend the range allowed by the fluorododge
printer. The photometric relationships were thus preserved
within limited areas (up to a few centimeters on the prints),
whereas the general gradient toward the terminator was largely
removed, and the contrast between highlands and maria was
also reduced. Because of the dodging process, the local contrast
could be enhanced over the original negatives by a factor of
about 6, in spite of the limited density range of the photo-
graphic paper.

The selection for the Atlas was made in steps: Some 8000
lunar photographs were obtained by the authors with the 61-in.
NASA telescope at the Catalina Observatory by early 1967.
This program included much experimentation with emulsions
and their wavelength response, with exposure times, and with
methods of processing. We are greatly indebted to the staff
of the Product Planning Division of the Eastman Kodak Com-
pany for major assistance throughout this program, such as
supplying us with samples of new or improved emulsions not
yet commercially available, as well as technical advice on their
optimum use. This assistance has materially improved the
average resolution of the Atlas photographs.

Two F-ratios were used, F/ 13.5 giving a scale of 10”/ mm
and F/ 45 giving 3”/mm. With good seeing, the larger scale
was found to give superior records. The adopted plate size was
5 x 7 in., which at F/ 45 just fitted the fields of the Photographic
Lunar Atlas.

The photographs were graded in several stages, the first
being when the upper 20—60 percent of the records of each
night were put in the permanent plate file. Contact paper prints
were made of all photographs retained. The next grading, done
in several stages, was based on these contact paper copies,
thereby avoiding unnecessary handling of the original films.
Thereafter, 16 x 20 in. enlargements on paper were made
of the best 15—20 percent. This included many pairs of records
of comparable quality. The final selection was based on the
negatives that were clearly very good plus supplementary fields
selected on the basis of the large prints.

The 120-in. Lick photography contains several excellent
records, but because of their circular fields and limited cover-
age, their inclusion here would have complicated the Atlas
format. In no case are the records used here distinctly inferior.
The same holds for the Pic du Midi collection, of which a
substantial number were inspected at Manchester through the
courtesy of Dr. Kopal; some of the records obtained with the
43—in. telescope are quite comparable to the best records
obtained with the 61-in. telescope.

The 61-in. collection was deficient in full-moon photogra-
phy for lack of emphasis in the observing program. For this

reason, we are including copies of the excellent 61-in. US.
Naval Observatory full—moon plates obtained in a joint ACIC-
U.S. Naval Observatory program. They are found in Part II
of this Atlas. The few gaps remaining in the full-moon photog-
raphy have been covered by photographs taken with the Yerkes
40-in. and the Lick 36-in. telescopes. One 36—in. Lick photo—
graph showing a good sunrise crescent with an unusually good
libration is used in Part I.

2. Arrangement of the Photographs

In the Photographic Lunar Atlas the visible hemisphere
was divided into 44 rectangular fields, numbered A—F in longi-
tude and 1—8 in latitude (6 x 8 fields, excluding the four cor-
ners). Because of the emphasis on terminator detail in this
Atlas, it was not feasible to adopt the identical subdivisions.
Instead, the Consolidated Atlas has, like the Photographic
Lunar Atlas, eight east-west strips; but the longitude division
has been made essentially continuous to allow for a gradual
step-wise progression of the terminator in each of the eight
latitude strips. The adopted arrangement is shown in Figure
1. The basic map is the well-known AF-ACIC photographic
composite of the visible hemisphere, provided here with an
overlay showing the eight latitude strips and the number of
photographs used within each. Thus, starting at the North
Pole, the A-zone contains 16 photographs, the B—zone, extend-
ing roughly from 300—600 N, 20 photographs, etc. The total
number of photographs in Part I is 192. Since the use of the
photographs will be varied, it was not considered practical to
give their boundaries in Figure 1. The appropriate sheet num-
ber can, of course, be estimated by interpolation; but normally
several consecutive sheets will be used together, with both
sunrise and sunset illuminations.

The full-moon photographs of Part II are-treated differ-
ently since they provide uniform information over the photo-
graph. F or this reason, Figure 2 gives the central positions (not
counting overlap) of the 34 fields covering the full moon. In
order to avoid confusion with Part I, Roman numerals are used
for the arrangement in longitude in Part II. The letters for the
latitude zones are the same in Parts I and II.

The total number of photographs in Parts I and II is 226.
In addition, a special photograph was added to the beginning
of each part; (Part I) An enlarged photograph of Clavius,
which may be compared with the standard Atlas print H7,
illustrates that the full image content of Atlas photographs
may require use of a hand lens. The Clavius photograph shows
detail that had not been seen before. (Part II) The entire full
moon, undodged, allows examination of features that extend
over several fields of Part II, such as some ray systems and
maria, and records accurately the albedo dilferences over the
entire lunar disk.

The astronomical data for each photograph and the zone
designation are recorded in the margin. The C numbers refer
to the 6l-in. NASA telescope of the Catalina Observatory; N
to US. Naval Observatory; L to Lick Observatory 36-in.; Y to
Yerkes 40-in. The colongitude gives the position of the termina-
tor; l and b give the geocentric libration. The libration was
taken from the Nautical Almanac for the day of observation,
but not necessarily for the precise hour, whereas the colongi-

 

 

 

 

 

 

 

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Figure 2 Arrangement of photographs in Part II.

CONSOLIDATED LUNAR ATLAS 5

tude was in most cases interpolated for the hour. The average
scale of the photographs is about 1:2,400,000, i.e., 1 mm is
2.4 km. Because the use of the average scale would cause errors
in excess of 9 percent for plates with scales outside the limits
1:22—26 million, these are listed in Table l. The scales were

TABLE 1
SCALES FOR PHOTOGRAPHS IN KM/MM OUTSIDE THE LIMITS 2.2—2.6

 

 

 

ATLAS SCALE ATLAS SCALE
NUMBER (KM/MM) NUMBER (KM/MM)
A1 3.0 F3 3.0
A10 2 7 G1 3.0
B1 3 O BlV 2 7
B2 2 2 CV 2 7
C2 3 0 DV 2 7
C12 2 7 EV 2 7
D3 3 0 FV 2 7
E3 3 0 GIV 2 7

 

determined separately for each Sheet by one of us (E. W.) and
by Dr. Gilbert Fielder independently. We are indebted to Dr.
Fielder for his assistance.

3. Minor Defects

Except for some scratches, white specks, and marks
caused by static electricity in the plateholder, the photographs
have not been retouched. These few corrections were made
with an etching knife on the final (large-scale) contact print—
ing negative. Among the defects and imperfections remaining,
the following are noted.

(a) Static marks. Because of the frequency of low humidi-
ties at mountain observatories and the absence of an antistatic
layer on most films best suited for lunar photography, static
discharge through or above the film is a common problem.
The effect may appear as an area of lower density on the print
taking the shape of lightning, “crow’s feet,” or a diffuse spot.
A comparison of several atlas sheets showing the area of inter—
est is recommended to differentiate these defects from genuine
features. For example, on Atlas sheet A8 there is a light area
west of the crater Egede A that, when compared with sheet
A10, is seen to be spurious (a static mark).

(b) Scratches and dust marks. Dust marks, resulting from
failure to brush the plate or from dust particles being charged
so that brushing does not remove them entirely, appear as
sharp black dots and lines. Abrasion marks due to excessive
brushing, errors in manufacturing, or improper handling pro-
duce thin parallel lines that may be either light or dark.

(c) Shutter faults. Most of the Atlas frames were taken
with a focal-plane Shutter. Occasionally such a shutter will pro—
duce a double exposure at low-tension settings for part of the
field, producing a density anomaly. Although an attempt was
made to remove this through dodging, evidence of the defect
still exists, as on plate C1.

(d) Frame numbers. Many of the films and plates used
for the Atlas were numbered before exposure by writing the
frame number on the emulsion. Occasionally this extended into
the picture area. An example is found on frame D10.

(e) Newton rings. In the copying of the original plates
and films, care was taken to prevent Newton rings; however,

on a few plates it was found difficult to eliminate them entirely.
In no case does their presence lead to confusion.

(f) Contrast variation. Because of the large range in
intensities to be recorded when both terminator and high-illumi-
nation regions are present, little variation from optimum expo-
sure could be tolerated, particularly with modern aerial films,
such as Eastman 4X, that have excellent speed and contrast
but a short gradient and low saturation density. Since the termi—
nator record was considered the most important, the higher
intensities were sometimes recorded on the Shoulder of the
characteristic curve. Thus, the contrast shown in the bright
areas may be too low.

(g) Vignetting. The Catalina Observatory 61-in. tele-
scope does not quite fill the area of the 5 x 7 in. film unvi-
gnetted. Where convenient, vignetted corners were cropped
out of the Atlas prints; when not practical, however, the cor-
ners were left black and the adjacent areas shaded to restore
their proper tones. An example may be seen in frame C1.

(h) Orientation. In most cases the long dimensions of the
Atlas sheets parallel the lunar equator. However, frames B5,
F6, and G6 have the long dimension roughly parallel to the
terminator.

4. Relation to Orbiter Photography

The original concept of the Consolidated Lunar Atlas
was to provide systematic high-resolution earth-based photog-
raphy of the visible hemisphere to which would be added
Special fields photographed with exceptional resolution. With
the conclusion of the tremendously important Orbiter I—V
photography, this plan was modified to include references to
the Orbiter photographs in sufficient detail for the user of this
Atlas to decide which additional Orbiter records to consult.
To this end, charts are herewith provided showing the outlines
of the individual Orbiter fields projected onto ACIC lunar
maps; and the Orbiter coverage is listed against the Sheet num-
bers of the Consolidated Lunar Atlas in Tables 2A and 2B.

The Orbiter IV photography covers the visible hemis-
phere of the moon systematically and is considered first. Figure
3 shows the distribution of the high-resolution photography in
longitude and latitude. There is roughly 20-percent overlap in
the equatorial zones and even larger overlap toward the poles.
In the right—hand section of Figure 3, supplementary sunset
photography is shown which was taken to fill some gaps left
in the first or sunrise coverage. Since these additions were made
near apolune, their scales are reduced and their coverage cor-
respondingly wider. The approximate average resolution for
each latitude zone is indicated in the margin. The numbers
in Figure 3 refer to the high-resolution frames; each of the
medium-resolution frames taken during the same mission cov-
ers most or all of the lunar surface as seen from the spacecraft.

The photographic equivalent of Figure 3 is found in Fig-
ure 4 (folded in four), which gives halftone reproductions of
the same fields. From Figure 4 the reader may estimate the cov—
erage of each field, as well as its quality and illumination, and
relate it to the coverage in this Atlas. The Orbiter photography
is, of course, basically unforeshortened. As stated before, the
principal value of the Consolidated Lunar Atlas is the informa-
tion on surface structures shown only under low-Oblique illumi-

 

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LUNAR ORBITER PHOTOGRAPHS IN ABC AND FGH FIELDS

TABLE 2A

OF CONSOLIDATED LUNAR ATLAS

 

 

 

FRAME NUMBERS

 

 

 

 

 

ATLAS ATLAS FRAME NUMBERS ATLAS FRAME NUMBERS
N0. ORBITER IV ORBI‘TER V N0. ORBITER IV V ORBITER V N0. ORBITER IV ORBITER V
A1 55,62, 67, — — — B4 67,74, 79, — —- —— C7 78,79, 85, 66—70, 86-93
68, 74, 79, 86 86, 90, 91,
80,165,177, 98
191,192 B5 61, 66, 67, 66-69
73,74,78, C8 90, 91,97, 90—93, 104-107
A2 68, 80, 92, — — —— 79, 86 98, 102, 103,
104,165,177, 109,110
191,192 B6 74,79, 86,91 — — —
C9 90,91,97, 90-93, 104—107,
A3 68,74, 79, _ ... _ B7 80,86,91, 86-89 98, 102,103, 120—123
80,86,91, 98,104 109,110,115
92,98
BS 79, 86, 91, 86—89 C10 97, 98,102, 90—93, 104—107,
A4 79,80, 86, 102 98,103 103,109,110, 120-123
91,92,98, 114,115
103,104,110, B9 98,103,110 86-89,102
115,116 C11 97,102,103, 90—93,104-107,
B10 98,103,110, 86—89,102, 109,110,114, 120-123, 133-136
A5 80,91, 92, 102,129-132 115,122 129-132 115,122
98,103,104,
110,115,116 B11 103,110,115, 102,105—107, C12 109,114,115, 120—123,133-136,
122,127 129-132 121,122,126, 150-157,159-162
A6 86,91,92, 88, 89, 102, 127
98,103,104, 129—132 B12 98,103,110, 86—89,102,
110,115,116, 115,122,127 105-107,129-132 C13 102,103,109, 104—107,120-123,
122 110,114,115, 133-136,150—157
B13 110,115,122, 102,129-132, 121,122
A7 92, 98,103, 88, 89,102, 127,134 159—162
104,110,115, 129—132 C14 109,110,114, 120—123, 133—136,
116,122,127, B14 110,115,122, 102,105-107, 115,121,122, 150-157,159-162
128 127, 134 129-132 126, 127
A8 92,98,103, 88,89,102, B15 127,134,139, 182—185 C15 114,121,122, 133—136, 150—157,
104,110,115, 129-132 145 126, 127,133, 159-162,164-167
116,122,127, 134,139
128 B16 134,139,140, 182—185
145,151,152, C16 121,122,126, 150-157,159-162,
A9 110,115,116, 102,129—132 159,164 127,133,134, 164—167
122,127,128, 138,139, 145
134, 139, 140 817 134,139,140, 182-185,159—162
145,151,152, C17 126,127,133, 159-162,182-185
A10 110,115,116, 102,129-132 164,176 134,138,139,
122,127,128, 144, 145
134,139,140 B18 139,145,151, 182-185, 159-162
158,163 C18 133,138,139, 164—167,186—209
A11 110,115,116, 102,129—132 144,145,151,
122,127,128, B19 151,158,163, 182-185 157,158,163
134,139,140, 170
145,152,164 C19 126, 127,133, 159—162, 182-201
B20 145,151,158, 182—185 134,138,139,
A12 110,115,116, 102,129—132 163,170,175, 144,145,151
122,127,128, 183,189
134,139,140, C20 133, 138, 139, 164—167,182-209
145,152,164 C1 54,55, 61, —— —— — 144,145,151,
62, 66, 67, 157,158,163
A13 127,128,134, — — —- 73, 74, 77,
139,140,145, 91,92 C21 133,138,139, 164-167,186-209
152 144,145,151,
C2 54,55,61, ~_ _ __ 157,158,162,
A14 145,151,152, — —— — 62, 66,67, 163
164 73,74, 80,
165,177,191, C22 138,144,145, 186-209
A15 139,140,145, — — — 192 151,157,158,
151,152,163, 162,163,169,
164 C3 54,61, 62, 66—70 170, 175
66, 67,73,
A16 140,151,152, — —— — 74, 77, 78, C23 144,145,151, 186-209
163,164,175, 91,92 157,158,162,
176,183,190 163,169,170,
C4 61, 62,66, 66—70 174, 175
B1 55, 62,67, — —— — 67,73, 74,
68, 74, 79, 78, 79,85, F1 27, 34, 39, 33—37, 40
80, 165, 177, 86,92 46, 53, 60,
191,192 65,178,184,
C5 66, 67,73, 66—70 185
B2 62, 67, 74, — — — 74, 78, 79,
79,165,177, 85,86 F2 34, 38, 39, 33-37, 40
191,192 45,46,52,
C6 73, 78,79, 66—70, 90-93 53,59, 60,
B3 62, 67,74, —— — — 85, 86,90, 64,65, 184,
79, 86,91 91,97,98 185

 

 

 

TABLE 2A — Continued

 

 

 

 

 

 

ATLAS FRAME NUMBERS ATLAS FRAME NUMBERS ATLAS FRAME NUMBERS
N0. ORBITER IV ORBITER V N0. ORBITER IV ORBITER V N0. ORBITER IV ORBITER V
F3 38, 39,45, 33—37,40 F23 143,149,156 168,177-180 G23 155,160,167, — ~— —
46,52,53, 172
59, 60, 64, F24 143,149,156, 177-180
65,71,72, 168 G24 155,160,167, —— — —
178,184,185 172
F25 143,149,156, 168,177-180
F4 52,53, 59, 33—37, 40, 54 168 ' G25 160, 167, 172, — —— —
60, 64, 65, 180
71,72,76, F26 143,149,156, 177—180
77,83,184, 168,173 G26 155,160,167, —— — —-
185 172
G1 52, 59,64, 40
F5 53, 60,65, 37 71,76,83, H1 44,58,70, 82 —— — ——
72,77 178, 184, 185
H2 44,58,70, 82 — — —
F6 60,64, 65, — —- — G2 52,59, 64, 40
71,72,76, 71,76, 83, H3 44,58, 70, —— — ——
77 184, 185 82, 94
F7 65,72, 77, 54 G3 52, 59, 64,71 40 H4 44, 58,70, — —— —
84 82,94
G4 64,71,76, — — —
F8 77,84, 89, 54, 84 83,88 H5 82,94,106 — — —-
96
G5 52, 59, 64, 40 H6 58, 70, 82, — — —
F9 76,77, 83, 54,84 71,76, 83 94,106,118
84, 88, 89,
95,96 G6 71,76, 83, — —-— — H7 82,94,106, 125—128
88,95,100 118
F10 83, 84, 88, 54,84
89,95,96, G7 71,76, 83, ~— — —— H8 82,94,106, —— —— ——
100,101 88,95,100 118,130
F11 88, 89,95, 54,84 G8 76, 83, 88, 54 H9 82,94,106, — — —
96,100,101, 95 118,130,154
107,108
G9 83,88, 95, 54 H10 106,107,112, 125—128
F12 88, 89,95, 84 100 118,119,124,
96,100,101, 130,131
107,108,112, (310 83,88,95, —— — ——
113 100,107 H11 82,94,106, 125—128
118, 130,154
F13 96,101,108, 116-119 G11 88,95, 100, —— — —-
113,120 107,112 H12 82,94,106, — — ——
118, 130,154
F14 100,101,107, 116-119 G12 95,100,107, 125—128
108,112,113, 112 H13 94,106,118, —- — ~—
119,120,125 130,154
G13 100,107,112, 125-128
F15 107,108,112, 116-119 119,124 H14 106,118,130, —-— — ~
113,119,120, 154
125 G14 100,107,112, 125—128
119,124 H15 106,118,130, — — —-
F16 119,120,124, 168,177-180 154
125,131,132, G15 119,124,131, 125-128
136,137 136 H16 106,118,130, — — ——
154
F17 120,125,132, 168 G16 107,112,119, 125—128
137 124,131,136, H17 106,118,130, —— — —
142 154
F18 124,125,131, 168,177—180
132,136,137, G17 107, 112,119, 125—128 H18 118,130,154, 125—128
142,143 124,131,136, 166
142,148
F19 124,125,131, 168,177—180 H19 130,154,166 —— — —
132,136,137, G18 131,136,142, —— — —
142,143 148,155 H20 154,166,179 — — —
F20 124,125,131, 168,177—180 G19 131,136,142, — —— — H21 130,154,166 — — -—
132,136,137, 148,155
143 H22 154, 166, 179, — — —
G20 136,142,148, —— — — 193
F21 132,137,143, 168,177—180 155,160
149 H23 154, 166, 179, —— — —
G21 142,148,155, — —— — 193
F22 131,132,136, 168,177-180 160,167
137,142,143, H24 154,166,179 — ——— —
148,149,155, G22 142,148,155, — — —~
156 160,167,172 H25 154,166,179 — —— —

 

TABLE 2B

LUNAR ORBITER PHOTOGRAPHS 1N D AND E FIELDS

OF CONSOLIDATED LUNAR ATLAS

 

 

 

 

 

ATLAS FRAME NUMBERS ATLAS FRAME NUMBERS
NO. ORBITER I ORBITER II ORBITER III ORBITER IV ORBITER V NO. ORBITER I ORBITER II ORBITER III ORBITER IV ORBITER V

D1 25-27,29, — — —— — 54,61, 66, ——~ — D17 113,114, 93,95-136, 84—107, 109,114, 108-115,

31—34 177,191, 118—135, 138—145, 112-115, 121,126 120-123,
192 137—140 162 120,122, 133—137,
124-131 142—157

D2 26, 27,29, 5-24 25—35 54,61, 66, 41, 42,

31—34, 41, 73,177, 44—51 D18 113,114, 96-112, 102—120, 109,114, 108,115,
44, 50-83 191,192 118-135, 137-145, 122, 121,126 120—123,
137—149, 162—178 124—160 133-137,

D3 5—19, 5-32, 5-21, 54, 61, 66, 38,41, 42, 157—172 142-157

25—27, 29, 35-42 25—35 73, 165, 44—51,
31-34,41, 177,191, 55—62 D19 134,135, 112, 102—107, 109,114, 133-137,
42,44, 192 137—140, 137—178 112—115, 121,126 142-157
50—83 149,151 120,
122—131,
D4 29, 31—34, 5-32, 5—20, 54, 61,66, 38, 41, 42, 137—141,
41, 42, 44, 35-42 25—35 73,78, 44—51, 145-152
46—83 192 55—63
D20 134,135, 112, 102,120, 114,121, 133-137,

D5 31, 32,41, 5—32, 5-20, 61, 66,73, 38,41,42, 137—140, 137-178 122—131 126,133 142-157,
42, 44, ' 35-58, 25-35, 42, 85 44—51, 149-151 164—167
46—83, 67-74, 44—50, 55-64,

85-100 76—91 52-70 71-78 D21 134,135, 137-194 120, 121,126, 137,
137-140, 122—160, 133,138 142-157,
D6 31,41,42, 5—58, 5-21, 61, 66,73, 38,41,42, 149-151, 171 164—167
44, 46—83, 67-74, 25-35, 78,85 44-52, 153-173,
85—100 76-91 40—72 55—64, 175-183
70—78
D22 134,135, 137, 120, 121,126, 137,

D7 41, 42, 5—32, 5-21, 66,73, 85 38,42, 137-140, 146-153, 122-131, 133,138, 142-157,
46—83, 35-42, 25-35, 44—52, 149-151, 162—212 161—170 144 164-167
85—100 67-74, 44-67, 72 55-64, 153—156

76-91 70-78
D23 137—140, 137, 120, 121,126, 150-157,

D8 41,42, 5-20, 5—20, 73, 85,90 52, 55-64, 149—151, 146—195, 122—131, 133,138, 164-167
46-49, 25—32, 40-70, 72, 70—78, 153—156 197-212 161-170 144
68-100, 35-74, 80-83 80—83
105—112 76-91,94 D24 153-156 179-195, 161-170 138,144, 210-217

197-215 150,157

D9 46,47, 43—74, 40—70, 72 78, 85,90 64, 70-78,

84-100, 76—91, 94 80-83 D25 150, 179—195, 161-170 133,138, 164-167,
105-112 153—156 197-215 144,150, 210—217
157

D10 84-100, 43—74, 40—44, 85, 90,97, 64, 70-78,

103, 76—92, 94 52—70, 72, 102 80—83, D26 150, 179—195, 161-212 138, 144, 164-167,
105-112 73, 75, 79-83 94—97 153-156, 197-215 150,157, 210—217
174—215 162

D11 84—100, 4—74, 40-44, 85, 90, 97, 64, 70-78,

103, 76-92, 94 52-70, 72, 102 80-83, D27 184—215 195, 161—170, 138, 144, 210—217
105-112 73,75, 79—83 94—97 197-215 172, 150,157,
181-212, 162,169

D12 84, 103, 43-66, 40-42, 90,97, 80—83, 214, 215
105—112, 92-111, 68—70,73, 102,109 94-97,

118—133 113-136 75,79, 108-115 D28 184—215 195, 161-170, 138,144, 210-217
80—85,86-101 197—215 172, 150,157,
181—212, 162,169,

D13 103,113, 92, 93, 73,75, 97,102, 94-97, 214,215 174
114, 95—136 83—107, 109,114 108—115,

118—133, 112-119 120-123, E1 26,27, 29, — — 21, 25—35 27, 39, 46, 38, 41,42,
141-148 133-136 33, 34, 53, 54,60, 44—51
50—67 65,66,

D14 103, 92—111, 73,75, 97,102, 94—97, 184,185
105—114, 113—136 84—101, 109,114 108—115,

118—133 103—107 120—123, E2 34,50—67 —— — 21,25-35 39, 46, 53, 37, 38, 41,
133—136 60,65, 42, 44—51
184,185
D15 113,114, 92,93, 73,75, 102,109, 94—97,
118-135, 95—136, 84—107, 114,121 108-115, E3 5-19, 5—32, 5—21, 39,46, 53, 37, 38,41,
138, 138-145 112-119 120—123, 25—27, 35—42 25—35 60,65, 72, 42.. 44-51,
141—148 133—137, 29, 31-34, 178,184, 55-62
142—149 41, 42, 44, 185
50-83

D16 113,114, 92,93, 84-107 102,109, 108—115,

118-135, 95-136, 114,121 120—123, E4 33,42, 44, — — 21,25—35 46,53,60, 38,41,42,
137—139 138-145 133-137, 50-83 65, 66,72, 44-51, 63
142—149 73

 

 

 

10

G. P. KUIPER, E. A. WHITAKER, R. G. STROM, J. W. FOUNTAIN, AND S. M. LARSON

TABLE 2B —— Continued

 

 

 

 

 

ATLAS FRAME NUMBERS ATLAS FRAME NUMBERS
No. ORBITER I ORBITER II ORBITER III ORBITER IV ORBITER V No. VORBITER I ORBITER II ORBITER III ORBITER IV ORBITER V
E5 44, 50—83, 76—91 21, 25—35, 53, 60, 65, 37, 38,41, E17 149, 151, 163—178 107, 113,120, 138—141
85—100 44-70, 72, 73, 77, 42, 44-51, 157—173 112-120, 125, 132
72,78 78,84, 85 63, 64, 124—160
71—78
E18 149,151, 171-178 120, 113,120, 138-141,
E6 44, 50-83, 76-91 21, 25-35, 65, 72, 73, 38, 41,42, 157-173 124-160 125,132 169-176
85—100 44—70, 72, 77,78, 44—51,63,
78,79 84, 85 64, 61—78 E19 134,135, 163—178 120, 120,125, 138-141,
137—139, 124-160, 132, 137 169-180
E7 44, 46—83, 35—42, 25-35, 65, 66,72, 38,42, 149—151, 171,
85-100 67—74, 44—67, 73,77, 44—52, 153-173, 173—180
76—91 72,78 78, 84 55-64,71-78 175—183
E8 46—100, 35-42, 40—70, 72, 72, 73,77, 55-64, E20 139, 163—178, 120, 125, 132, 169—180
103, 67-74, 78, 79—83 78, 84,85, 71-78, 149—151, 205-212 124-131, 137, 143
105—112 76—91, 94 89, 90, 80-84 153—173, 136—160,
96,97 175-215 171-212
E9 46—100, 35-58, 5—20, 72, 73, 77, 55—64, E21 140, 146-161, 120, 122, 125, 132, 169—176,
103, 67—74, 40—70, 72, 78, 84,85, 71—78, 149—151, 163-195, 124-131, 137,143 178—180
105—1 12 76—91, 94 78—83 89,90, 96, 80—84 153—173, 197—212 136—161,
97 175-215 163—184
E10 85-100, 76—91, 94 44-70, 72, 77,84, 85, 64, 71-78, E22 149—151, 163-178 136—160, 125, 132, 169-180
105-112 78-83, 89, 90, 96, 84, 98—101 153—173, 171—212 137,143
108—111 97,101 175-215
E11 85-100, 76-91, 94 52-70, 72, 84, 85, 89, 64, 71-78, E23 149,151, — — 136-160, 125, 132, 169-176,
105—112 79, 80-83, 90,96,97, 84,98-101 153—173, 171-212 137,143, 178-180
108-111 101 175—215 149
E12 84, 103, 93, 94, 79—84, 84, 89,96, 80-84, E24 153—156, 187-194, 161, 132, 137, 169-176,
105-112, 113—136 88-101, 97,101, 98-101, 175-215 197—212 163-212 143,149 178-180
118-133, 108-111, 102,108. 108-119
141-148 116-119 109 E25 153—156, — — 171-213 132,137, 169-180
175—215 143, 149,
E13 118-133, 93,129—136 107—119, 96,101, 98-101, 156,161
141—148 138-145 108,113 116—119
E26 176—215 —— — 171—213 143,149, 177-180
E14 118—135, 93,113-136 84,86—101, 96,101, 98-101, 156,161,
137—139, 103—119, 108,113, 108-119, 168
141—148 132—135 120 138—141
E27 176—215 — — 171-213, 137,143, 177-180
E15 118-135, 93,113—136, 84,86—101, 101,108, 108—119, 215 149,156,
137-148 138-145, 103-120, 113,120 138—141 161,168
163-178 124-131
E28 176-215 195, 161—170, 137,143, — ——
E16 118-133, 129—136, 107, 108,113, 116-119, 197-212, 172-215 149,156,
141-148, 163-178 112-120, 120,125 138—141 214,215 161,168,
157-173 124—160 173

 

nations or near full moon; and on the photometric relationships
over larger areas in both morning and afternoon illuminations.

The coverage by the other four Orbiter missions is given
in Table 3 and shown for the visible hemisphere in Figure 5,
also folded in four. Here the area designations are approxi-
mately arranged in lunar longitude. To separate and clarify
the Orbiter photography that falls within a strip along the
equator approximately 160 wide, where often more than one
Orbiter has photographed a given area, each mission was
plotted separately on six AClC LAC Charts. The resulting
maps, Figures 6—26, have been arranged by section from east
to west. For each area and each mission, the frame numbers
are given with only the first and last of a block of consecutive
and overlapping frames listed. If only a single frame number

is given, it was the only one taken on that mission. In nearly all
cases, the outlines of the areas refer to the medium-resolution
coverage. The high-resolution frames with the same numbers,
taken concurrently with another camera, fall within the same
outlines but cover only a fraction of the area. The number of
such high-resolution frames within a given medium-resolution
block may be 1, 4, 8, or 16. Occasionally, and only for Orbiter
III, some high-resolution frames were obtained without a cor-
responding medium-resolution frame. These exceptions are
frames 40, 42, 72, and 75 of Orbiter III, which are included in
our figures. On the other hand, the Orbiter I medium-resolution
frames do not normally have accompanying high-resolution
frames.

As is seen on Figure 5, three types of Orbiter coverage

TABLE 3

LUNAR ORBITER PHOTOGRAPHS REPRESENTED BY
THE AREAS SHOWN 1N FIGURE 5

 

 

NASA SITE ( ) AND FRAME NUMBERS

 

 

AREA ORBITER I ORBITER II ORBITER III ORBITER V

1 (A0)5—24 __~__ ___.— ___.

2 25—27 _ _ _ _ _ _ __ _ _

3 29,33,34 ___ ___. ___

4 ___ “___“ ___. (V1)33—36

5 ——— ——— ___ (V2)37

6 ___ ___ ___ (V4)40

7 31,32 __ __ _._ _ _ _ _ _ _

8 ___— ___ ___ (V3)38

9 ___ ___— _—— (V5)41

'10 ___._ ___ _——— (V6)42

11 44;(A1) 50-67 __ __ _ (P2) 25—36 (V8) 44—51

12 ___—— (S1)21—24 ___— __—

13 41 _ _. _ __ _ _ __ _ _—

14 ____ ——— ——— (V9)52

15 (B2) 48-49; (P1) 5—20; (S2) 25-32; (P1) 5—20 (V11) 55—62
(A2) 68-83 (P2) 3542 (V12) 63

16 42 _ _ _ __ __ _ _— —— _

17 46,47 __—— __—_ ___—

18 — — __ — — —— — — —— (V14) 66-69

19 ___— __—.— ___ (V15)70

20 ————— ___. (SS)78 __—

21 ___ ___ ___ (V10)54

22 ___ ___ __# (V13)64

23 (A3) 85-100 (P5) 67-74; (P5) 52-67; (55) 72; (V16) 71-78

(P6) 76—91 (P6) 68-71; (P4) 44—50

24 — _ __ (P3) 43—58 — —— — — — —

25 (B4) 84 —_ _ _ __ _ __ (V18) 80-83

26 _— — — (P4) 59-66 — — — — —— _—

27 _____ ——- (S9)79 ___—-

28 (A4) 105—112 (S8) 94 (510) 80—83 —— — —

29 ___ ___ ___. (V19)84

30 ___— _.—_ ___—_- (V21)86-89

31 _— _ __ _ — —— _ — _ (V22) 9093

32 ———— ___ (S6)73 __—

33 _— _ — —— — _— _ — — (V23) 9497

34 ___ (S6)92 ___ __—

35 (Bs)103 ———— ___— ————

36 — — — _ _ _ (S17) 108-111 (V24) 98—101

37 H__ ___ ____ (V25)102

38 — _— —— — — — — _— — (V31) 129—132

39 _ _ __ _ _ _ _ _— _ (V26) 104-107

 

 

TABLE 3 — Continued

 

 

NASA SITE ( ) AND FRAME NUMBERS

 

ORBITER l

ORBITER I I

ORBITER III

ORBITER V

 

45
46
47

48
49
50
51
52
53
54
55A
558
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70

(A5) 118—133

(A6) 141—148
(BS) 113,114

(B8) 134,135

138

139,140

137

(B9) 149,151
(A7) 157-173

(B10) 150

(B11) 153—156
(A8) 175—183

(S7) 93

(S9) 95; (P7) 96-111;

(P8) 113-136

(812) 162
($10) 112
(P9) 138—145

(P11)163—178'

(811)137;
(P10) 146-161

(P12) 179—194

(813) 85
(s11) 84

(P7) 86-101

(819)116-119

(815)103-106;
($16) 107

(S18) 112-115

(814) 102

(S23) 132—135

(S21) 120
(P8) 124—131

(S22) 122

(P9)137—160
(S24) 136

(S20) 123

(P11)173-180

(V29) 120—123

(V28) 116-119
(V30) 125—128
(V32) 133-136
(V33) 137

(V35) 142—145
(V36) 146—149
(V37) 150—157

(V34) 138-141

(V38) 159—162

(V42) 169—176

 

CONSOLIDATED LUNAR ATLAS 13

TABLE 3 — Continued

 

 

NASA SITE ( ) AND FRAME NUMBERS

 

 

AREA ORBITER I ORBITER II ORBITER III ORBITER V
77 —————— ———-—-— (S27)171 —————
78 _ _ _ _ _ _ — — —— (V43) 177-180
79 ————— ————— ———— (V41)168

80 ——— ——— (S26)162 ———
81 —-——— ————— (S25)161 ————
82 —— — — (S13) 195; (P10) 163-170 — —— —

(P13) 197—212

83 ——-4— ————- (S28)172 ———
84 (A9) 184-215 —— — — (P12) 181-212 — — ——
85 _ _ _ _ _ _ — — — (V45) 182-185
86A —— -—- — — — — — — — (V46) 186—193
86B — —— —- — — — — — — (V48) 194-201
86C —— — — — — — ~— —— —— (V49) 202—205
86D — — — — — — - —— — (V50) 206-209
87 ———— (S16)214 —-———- —————
88 ———— (S15)213 ——— ——-———
89 _ _ _ _.._ __ ._ — — —— (V51) 210-217
90 ——-—-— (S17)215 ——— ———
91 ——— ——-——-— (829)213 ———
92 174 — —— —-— — — — —- —— —
93 ——— ———— (S30)214 ————
94 ———— ——— (S3l)215 ———

 

exist: (1) systematic photography, taken almost normal to
the lunar surface; (2) oblique photography showing the lunar
landscape near the horizon and designated by V-shaped pano—
ramic sectors, outlined in red; and (3) high-altitude coverage
from Orbiter I of larger areas of the moon, outlined by dashes.

5. Additional Photography

Since the 61-in. photography in this Atlas covered a
period just over one year, it is anticipated that future low-
oblique photography will yield photographs superior to those
included. The authors and the sponsors intend to distribute a
package of substitute sheets after one or two years, to replace
Atlas sheets definitely surpassed.

Acknowledgments. The publication of this Atlas, the con-
cluding supplement of the 1960 Photographic. Lunar Atlas,
was supported, like it and the Orthographic and Rectified
Lunar Atlases, by the US. Air Force Cambridge Research

Laboratories, under Contract AF19(628)—4332. The authors
are deeply indebted to the sponsors for their agreement on
using the photographic method of reproduction, in a format
developed in the production of the five Ranger atlases. We are
indebted to the National Aeronautics and Space Administra-
tion for providing this Laboratory with the excellent 61-in.
telescope used in most of the records presented here, and for
continuing staff support in lunar and planetary photography.
We are pleased to be able to include copies of the best full-
moon photographs obtained by the Flagstaff office of the Air
Force Aeronautical Chart and Information Center in collabora-
tion with the staff of the US. Naval Observatory. As stated in
the text, the program of the 6l—in. lunar photography at the
Catalina Observatory has greatly benefited from the advice
and generous assistance of the staff of the Product Planning
Division, Eastman Kodak Company, Rochester, New York.
The production runs were made at Ray Manley Commercial
Photography, to whom we are indebted for their skill and excel—
lent liaison with the Laboratory staff.

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C 4|84 I967 Feb. I9d 2h 53".“8 UT Col. 24‘.’2 l = -7‘?4 b = -3°8

 

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C |585 I966 May 2d 3h 49”.”9 UT Col. 5294 I = +|‘.’2 b = -5‘.’4

 

C 2862 I966 OCT. 8d l2h 8W7 UT Col. I989?)

 

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C 2396 I966 Jul. l3d ||h 46m? UT Col. 2|7?| I = -6‘.’5 b = +O?4

 

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C 2499 I966 Sept. 3" 9h 24’3‘4 UT Col. |30?| | = -2‘.’7

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C 2593 I966 Sept 5“ IIh 40'T‘3 UT Col. I55?6

 

C 3897 I967 Jon. l9d 3h 3W5 UT Col. 7‘32 | = -3?6 b = +|‘.’5

 

 

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C 3902 I967 Jan. 20" Ih 46ml UT Col. l8‘35 l = -4‘.’8 b = +O?|

 

C I960 I966 May 29" 3h 46m8 UT Col. 22‘?2 = +|‘.’5 b =

 

C l9ll I966 May 28d 4h l6'I‘4 UT Col. IO‘?2 I = +O?5 b = —6‘.’4

 

C 3727 I966 Dec. 23d 4h 43”.”8 UT Col. 39‘?8 l = -3?5 b = +|‘.’3

 

C 4062 I967 Jon. 22d 3h 2036 UT Col. 43‘.’8 | = -6‘.’3 b = -2‘.’7

 

C 2928 I966 Oct 9d llh 35'93 UT Col. 2|O‘.’3

 

C I275 I966 Apr. 2" 8h 26'1‘5 UT Col. 48‘.’8

 

C 4259 I967 Feb. 22d 3h 20ml UT Col. 60‘39

 

369 I965 Dec. 6d 5h l4'F‘O UT Col. 6397 = -5‘.’8 b = +2”?

 

c 239| I966 Jul. I3d uh 44% UT Col. 2:7?0

 

C 3239 I966 Oct 28d 6h 28W3 UT Col. 79‘?3 l = -|‘.’7 b = +32

 

 

 

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C 692 I966 Jon. 9" IIh ZI'T‘O UT Col. I2090 | = +|‘.’4 b = -6‘.’4

 

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C 230 I965 Nov. l2d th 44% UT Col. l34‘34 | = -2‘.’4

 

C 257| I966 Sept 4" IOh 37”.”6 UT Col. [42‘39

 

C |4|| I966 Apr. 27" 2h 54W4 UT Col. 35l‘.’O | = -4‘.’6

 

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C |527 I966 Apr. 28d 2h SOWZ UT Col. 32 | = -3‘.’8 b = -6‘.’3

 

C 2668 I966 Sept. 6d IIh IO'F‘I UT Col. |67‘.’5

 

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C 3904 I967 Jon. 20d |h 47“.”l UT Col. |8‘?5 I: -4‘.’8 b = +O‘.’|

 

C 2439 I966 Aug. 8d llh 3’94 UT Col. I7393 | = -5‘.’|

 

C 4l95 I967 Feb. I9d 2h 56'.“8 UT Col. 24‘.’2 = -7‘.’4 b = -3‘.’8

 

Sept 7d llh 25”.”2 UT Col. |79‘.’8

 

I967 Jan. 2|d 2h 44“.”2 UT Col. 3W4 | = -5‘.’7 b = -|‘?3

 

C ”96 I966 Apr. Id 3“ 2293 UT Col. 34‘?! I = -4‘?3 b = -6‘.’3

 

C 2303 I966 Jul. lld llh 36”.”0 UT Col. l9|‘?5 l = -5‘.’O

 

 

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C 2923 I966 OCT. 9d ||h 32% UT Col. 2|O92 | =

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C 790 I966 Feb. 4" 6“ 52¢?) UT Col. 74‘.’| |= -3‘.’7 b = -5‘.’2

 

C 3|98 I966 OCT. 28d 6h 7”.“l UT Col. 7990 | = -l‘.’7 b = +392

 

 

 

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C I355 I966 Apr. 6" 8h O'T‘O UT Col. 97??) | = +4?|

 

C I726 966 May 6“ 8h II'T‘8 UT Col. |O3‘.’4 | = +592 b =

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I938 Jun. 3d 04h 00m UT Col. 32897 | = +592 b = +6?6

 

C 648 I966

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C 44|3 I967 Mar. I7d 2h 3W2 UT Col. 340??) |= -6‘.’O b = -2‘.’4

 

C 249i I966 Sept 3d 9hl9'T‘O UT Col. |30?O = -2‘.’7

 

 

 

C 2564 I966 Sept 4d IOh 35”.”4 UT Col. |42‘.’8 l = -4‘.’O b = +297 E8

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C l4|9 I966 Apr. 27d 2h 58’."3 UT Col. 35|?O |= -4‘.’6 b = -5‘.’6

 

C I850 I966 May 27d 3h 58W3 UT Col. 35799 |

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C 3355 I966 Nov. 3d 9h 4”.”6 UT Col. [5395 I: -5‘.°8 b = -5‘?O Ell

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C 3846 I967 don. l9d 2h 4|”.“8 UT Col.

 

C 2663 I966 Sept 6" llh 7W5 UT Col. |67?5

 

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C 3944 I967 3h 27’."2 UT Col. I996 l= -4‘.’8 b =

 

I966 May 29d 3h 50'T‘8 UT Col. 22‘.’2

 

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C 2720

 

C 3977 I967 Jon. 2|d 2h 42m5 UT Col. 3|?4 | = -5?7 b = -|?3

 

C ”99 I966 Apr. Id 3“ 2*..‘2 UT Col. 34?| |= -4‘.’3 b = -6‘?3

 

C 278| I966 Sept 8d IIh 52“.”? UT

 

C 2878 I966 Oct. 8Cl I2h l8’T‘3 UT

 

C 4052 I967 Jon. 22d 3h ”'90 UT Col. 43?? l = -6°3 b = -2‘.’7

 

C |262 I966 Apr. 2" 8h II'T‘7 UT Col. 48?? = -2‘.’8 b =

 

6 I662 I966 Mov 2d 5h 45”.”? UT Col. 5394 I = +I‘.’2 b = -5‘.’4

 

C 292i I966 OCT. 9d IIh 3|".‘2 UT Col. 2|O92

 

C 378 I965 Dec. 6d 5h 23'."O UT Col. 63‘?8 I = -5‘.’8 b = -2°7

 

C 2376 I966 Jul. |3d ||h 35”.”2 UT Col. 2|6‘.’9

 

C 796 I966 Feb. 4d 7h 2W3 UT Col. 7492 I: -3‘.’7 b =

 

C 3233 I966 OCT. 28d 6h 25'."3 UT Col. 7993 I: -|‘.’7 b = +3?2

 

 

 

 

.
w
n
.

 

 

 

C I354 I966 Apr. 6" 7h 58?? UT Col. 97%

 

C I732 I966 May 6d 8h I5'T‘7 UT Col. |0394

 

L I75 I938 Jun. 3d 04h 00m UT Col. 328?? I: +5?2 b = +6?6

 

C 4372

I967 Mar. I7d 2h 8'99 UT

COL

340??)

l= -6?0

b = -2?4

 

 

F4

 

I: +194 b = —6‘.’4

|20‘.’2

Col.

T
U
0
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6
2
m:
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9
n.
G
J
6
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C 70|

 

|= -4?5 b= +290

COL|2797

_.|
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2
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4
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8
d

B
d.
O
5
6
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CIOI

 

C 223 I965 Nov. l2d IOh 3W2 UT Col. |3493

 

C I430 I966 Apr. 27" 3h 3’90 UT Col. 35l‘.’| | = -4‘.’6 b =

 

C 2559 I966 SepT. 4d IOh 32m4 UT Col. |42‘.’8 | = -490 b = +27 F9

 

C I794 I966 May 27d 3h 33% UT Col. 35696 I = —O‘.’6 b = -6‘.’7

 

C 26|5 I966 Sept. 5“ l2h 2W2 UT Col. I5599

" W41" “W “M
x . , I H

a
,1

         

C 3853 I967 Jon. I9d 2h 44W? UT Col. 7?! | = -3‘.’6 b = +|‘.’5 Fl2

 

C 266| I966 Sep’r. 6d ||h 5”.”6 UT Col. |67?5

§~ ‘~

 

C 3950 I967 Jan. 20" 3h 29m9 UT Col. |9‘?6

 

C I995 I966 MCIV 29d 4h 40”.”6 UT Col. 2296 I: +|‘?5 b =

 

C 3745 I966 Dec. 23d 4“ 5338 UT Col. 39?9 | = -3‘.’5 b = +|93

 

C 23|7 I966 Jul. ||d ||h 4I'T‘O UT Col. l9|‘.’5 l = -5‘.’O

 

b = -2‘.’7

| = -6‘.’3

7
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C 4048

 

C I256 I966 Apr. 2d 8h 5'92 UT Col. 4897 I: -2‘.’8 b = -6‘.’6 F|9

/=. "
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| = -6‘.’7 b = —6€’O

l98‘.’4

Col.

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I966 May 2" 4h 5W9 UT Col. 5296

 

C 2365 I966 Jul. I2Cl ||h 37% UT Col. 20497 I: -5‘.’9

If

 

I967 Feb. 22d 3h 34”.“9 UT Col. 6I‘.’O |= —6‘.’6 b = —6‘?4

 

I966 Feb. 4" 7h 63‘? UT Col‘

 

C 2380 I966 Jul. |3d l|h 37WO UT Col. 2|699

 

b= +392

|=—|‘.’7

7990

COL

T
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8
2
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C 3205

 

  

 

a,“

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"w ”mm. ,
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L |75 I938 Jun. 3d 04h 00m UT Col. 328?? I = +5?2 b = +6?6

 

C I348 I966 Apr. 6“ 7h 3W7 UT Col. 97‘?O | = +49| b = -3‘?6 (32

 

 

 

C [735 [966 May 6d 8h I7'T‘7 UT Col. |03°4 |= +5°2 b = +095

x V a

Vb“

 

G4

-6?4

b:

I: +|95

Col. 33998

I966 Jun. 24“ 3“ 3696 UT

C 2|89

 

41,;th

C 664 I966 Jan. 9d 8h BOWO UT Col. H897 I = +|92 b = -6‘.’3

 

66

C |23 I965 OCT. l3d 9h 20”.”2 UT Col. |2894 I: -4‘.°5 b — +|99
' ‘ \J

v, ' Yul « , V U?
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fa (2:55,: ‘3" ,‘ : ., ’
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C I437 I966 Apr. 27" 3" SW? UT Col. 35l‘.’| = -4‘?6 b = -5‘.’6

 

C I856 I966 May 27" 4h 3W9 UT Col. 357?9 I = -O‘.’6 b = -6‘.’7 G9

 

b =-+297

I: —4?0

Col. |42‘.’8

T
U
2
m .
O
3
h
m
d
4
m
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S
6
6
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C 2555 A

 

C 3870 I967 Jan. I9d 2h 52".‘0 UT Col. 7‘32 |= -3‘.’6 b = +|°5 GH

 

I: —5?3 b = +03?

COL|5595

T
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2
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hl
d

5
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S
6
6
ob

C 2584

 

C 39” I967 Jan. 20“ |h 5W6 UT Col. |8‘.’5 |= -4‘.’8 b = +O‘.’|

 

C 2655 I966 SepT. 6d llh 2W7 UT Col. |6795 I: -696

 

C 1208 I966 Apr. Id 3“ 3|“.‘8 UT Col. 345’2 |= -4‘.’3 b = -6‘?3 (55

 

C 2435 I966 Aug. 8d IOh 55’.“2 UT Col. |73‘.’2 l = -5‘.’| b = +297 G|6

 

2
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6
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C 2743

 

C 4044 I967 Jon. 22d 3h 4".“3 UT Col. 43?? l = -6‘?3 b = -2‘?7

 

C 1254 I966 Apr. 2d 8h 3W3 UT Col. 4897 I: -2‘?8 b : -6‘?6 G|9

 

 

 

 

620

—690

-697

l98?4 |

COL

I966 Oct8d|2h22m7 UT

C 2885

 

C 93l I966 Mar. 53" 6h I'T‘O UT Col. 6695 I = —2‘.’5 b = -6‘?4 622

 

C 804 I966 Feb. 4d 7h 8W6 UT Col. 74‘32 |= -3‘?7 b = -5‘.’2 623

 

b= -5?6

|= -6?8

8
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C 282|

 

C 558 I966 Jon. 6d 6h 4'3‘2 UT Col. 8|?O l= -4‘.’4 b = -3‘.’| 625

 

C 2477 I966 Aug. l2d llh 40”.”3 UT Col. 22295 |= -7‘.’4 b

 

     

‘m
1: :1

 

C 666 I966 Jon. 9d 8h 32W) UT COH18‘?7 I: +l93

i ‘

6 » y ‘ \a K

 

C 2153 I966 Jun. 24d 3h |6m9 UT Col. 33937 I: +l‘?5 b = -6‘?4

A

 

C I444 I966 Apr. 27" 3h 9m8 UT Col. 35W l = -4‘.’6 b = -5‘.’6

 

H4

-6‘.’7

b:

| = -O‘.’6

Col. 356%

I966 May 27d 3h I9'T‘3 UT

C l782

 

C 2|8 I965 Nov. |2d IOh |9m8 UT Coll |3492 I: —2‘?5 b = -3‘.’O HE
C \ H ‘ - ‘ .

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’ ’ 3““: ~-
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C 675

I966 Jan. 9" 8h 39%) UT

Col. Il8‘.’7

|=+l93

b = -6‘.’3

 

 

‘

H6

C 39|2 I967 Jon. 20d |h 52”.”3 UT Col. |8‘.’5 |= -4‘.’8 b = +O‘.’| H7

 

C 3912 I967 Jon. 20d |h 52”.”3 UT Col. I895 |= —4‘.’8 b = +O?| CLAVIUS (H7)

 

C 749 I966 Jon. IOd 9h 46".“0 UT Col. |3| ‘.’O I: +3?2 b = -636 H8

 

c 2:4 I965 Nov. 12d 10h 10m? UT Col. 134?: I: —2?5 b = —390 H9

' ‘V‘

WM;

    

r

    

‘.

C 26|8 I966 Sep1.5d I2h 25m?) UT

 

C 3968 I967 Jon. 2|d 2h 35'95 UT Col. 3P3 |= -5‘.’7 b = -l‘.’3

 

C |2|4 I966 Apr. Id 3“ 37’."2 UT Col. 3492 |= -4‘.’3 b =

 

C 3372 I966 Nov. 3" 9h 30".“7 UT Col. l5397 I = -5‘.’8 b = -5‘?O H|3

 

 

C 3437 I966 Nov. 4d IOh 24'.“8 UT Col. |6694 l= -5‘.’7 b = —5‘.’9 Hl4

 

C I62 I965 OCT. l9d I2h I2'T‘9 UT Col. 20298 | = -O‘.’5 b =

 

C 2653 I966 Sept 6d I!h I’T‘E UT Col‘ |6794

 

C 4036 I967 Jon. 22d 2h 53”.”7 UT Col. 43‘?6 I = -6‘.’3 b = —2‘.’7

 

b = -6‘?6

|= -2‘.°8

5090

Col.

T
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C |3|8

 

C 268! I966 Sept 7d ||h I4'T‘O UT Col. |79‘?8 l = ~75’3 b = -2‘.’O Hl8

' I * 5;”, I% ’4‘

&

 

C 2849 I966 OCT. 8d ||h 56m5 UT Col. I985?
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C I42 I965 OCT. I9d ||h 47% UT Col. 20296

 

C 432| 1967 Feb. 22d 3h 42m9 UT Col. 6|9O |= ~696 b = -6‘.’4

 

C 2827 I966 Sept IOd l2h 6W0 UT

 

C 543 I966 Jon. 6d 5“ 45'90 UT Col. 805’9 |= -4‘.’4 b = -5‘.’| H24

 

H25

210?3

I966 OCT. 9d llh 45m2 UT Col.

C 2933

 

 

 

Y 842 I960 Mar. |3d 5h I6m6 UT Col. 93??) I = -5‘.’2 b = +O‘.’5

 

v.

 

\0‘
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N 58l8 I965 OCT. 9d 6h 29ml UT Col. 7890

 

N-l6 3|7l-A I965 Jon. l7d 7h 25“.“3 UT Cdl. 8597

 

I: -O?| b= -3?4

COL 8597

T
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N%6 BYN-A

 

P9
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BI

b = -3‘?6

+693

Col. 78‘?O

I965 OCT. 9d 6h 29'?! UT

N 58|8

 

 

N 58|8 |965 OCT. 9" 6h 29ml UT Col; 78‘?O I = +65% b

 

N 58|8 I965 OCT. 9“ 6h 29ml UT Col. 78‘?O l = +63 b = -3‘.’6

 

N 9547C I966 Dec. |d 8h 7”.”8 UT Col. |3398 | = -4‘.’6 b = -5‘.’9

 

     

1"
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N 58|8 I965 OCT. 9" 6h 29ml UT Col. 7890 l = +693 b = -3‘.’6 CI

 

N 58|8 I965 OCT. 9" 6h 29ml UT Col. 7890 | = +693 b = -3‘.’6

 

N 58|8 I965 Oct ‘3" 6h 29ml UT Col. 78‘.’O | = +65 b = -3‘.’6

 

b = -3‘.’6

+693

Col. 7890

T
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W
9
2
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6
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9
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6
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N 58|8

 

N 9547C I966 Dec. |d 8h 7W8 UT Col. |3398

 

 

 

 

 

a»,

.u.

-3‘.’6

b:

= +693

.0

0

Col. 78

T
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I965 OCT. 9“ 6“

N 58|8

 

N 58|8 I965 OCT. 9d 6h 29ml UT Col. 78‘.’O I = +6?3 b = -3‘.’6

.. .9374-

 

l = +6.33 b = -3‘.’6

Col. 7890

T
U
W
9
2
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6
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9
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N 58|8

 

N 58|8 I965 OCT. 9d 6h 29ml UT Col. 7890

 

N 9547C I966 Dec. |d 8h 72“.”8 UT Col. |33‘?8

 

 

 

 

. :55! .313.

N 58|8 I965 OCT. 9" 6h 29ml UT Col. 78‘?O I = +69?) b = -3‘.’6

 

I
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N 58|8 I965 Oct 9d 6h 29ml UT
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N 58|8 I965 Oct. 9d 6h 29ml UT Col. 78‘?O I = +693 b = -3‘.’6

. ’9
O

o
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N 5818 I965 OCT. 9" 6h 29ml UT Col. 78‘?O | = +6?3 b = —3‘.’6

 

N 9547C I966 Dec. |d 8h 7”.“8 UT Col. B398

 

N 58|8 1965 OCT. 9d 6h 29”.”! UT Col. 7890 | = +693 b = -3‘.’6

 

 

 

N 58|8 I965 OCT. 9" 6h 29ml UT Col. 7890 | = +693 b = -3‘.’6

 

b = —3‘.’6

+6?3

Col. 78‘?O

T
U
W.
9
2
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6
d

9
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6
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N 58|8

 

b = -3‘?6

+6?3

Col. 7890

T
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9
2
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6
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9
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N 58|8

 

N 9547C I966 Dec. |d 8h 7”.”8 UT Col. |3398 | = -4‘.’6 b = -5‘.’9

 

 

 

 

 

2

O

b=-2

|= +397

2
o .
8
7
0
C

6UT

m

I946 Jon. l7d O7h 50

L 224

 

GIY

b = —599

|= -496

8

O

W8IJT Cm.B3

I966 Dec W 8h'?

N 9547C

 

| = -3‘.’O b = +O?|

Col. 24‘.’O

T
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7
5
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0
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2
2
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9
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Y |06

 

= +63 b = —3‘?6

Col. 78530

T
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9
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6
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9
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0
5
6
old

N 5818

 

     

S'fl

 

|= +396 b = +|9|

Col. 33592

I959 Sept. 18" 08h I2m UT

Y 482

 

I = -3‘.’O b = +09|

CoI. 2490

T
U
m
7
5
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3
0
d
2
2
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0.
A
9
5
B

Y |06

 

I: -390 b =

Cd.2490

Tl
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7
5
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2
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A
9
5
B

YIOB