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Segment 5
A FF - crater Posidonius, Lava borders in Mare
Tranquilitatis, The Apollo 17 region with its pyroclastic deposits and the
lunar cones Isis and Osiris. Segment 5 B Gardner megaplateau,
Domefield Cauchy west, Jansen and Carrel, Menelaus and Arago Segment 5 C
Hyginus, Murchinson, Manilius and Yangel (Sinus Fidei) Segment 5 D Aristillus,
Autolycus, Theaetetus, Rima Hadley (Apollo 15), Palus Putredinus, Valentine
Dome |
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Valentine domes 1 and 2 - Moon age 7.1 days (39 %)
Valentine 1 and 2 Valentine are on the eastern
side of the gap between the mountains Apennines and Caucasus. Both are
extremely flat intrusive domes. Valentine 1 has a diameter of about 30 km at an
height of 130 meters. Valentine 2 is significantly smaller and has a lower
height. The domes remember at the domes Laplace 5 and 6 in the Sinus Iridium.
The name "Valentine" is inofficial and can not be found on any map of
the Moon or lunar atlas. Both domes are difficult to observe because of their
size and low height and the observation requires a very flat solar
illumination. |
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LRO - Valentine domes 1 and
2
The image to the left
shows the two domes in a LRO image with a resolution of 125 m/px. Here, a
narrow rille is visible which crosses the dome in approximately east-west
direction.
Such systems of rilles (probably fracture zones, caused by
the upwarp of the area) are typical of large intrusive domes, see the
Aristillus domes below. |
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Aristillus - Autolycus - Theaetetus - Moon age 7.5 days (44 %)
At a lunar age of about 7.5 days three large
domes become visisble near the craters Autolycus (39 km), Theaetetus (25 km)
and Aristillus (55 km). Autolycus is classified as effusive (no systems of
rilles). Theaetetus and Aristillus are classified as intrusive (extended
systems of rilles). Autolycus' diameter is about 28 kilometers and it only
reaches a height of 75 meters.
Aristillus has a size 58 kilometers and
is one of the largest intrusive domes. It is with 85 meters only marginally
higher than the Autolycus dome. Theaetetus is a complex structure (see LRO
image below) and is similar in structure to the amazingly dome Yerkes 1 in Mare
Crisium. |
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Aristillus - Autolycus - Putredinis
Moon age 7.7 days (46 %)
The large Valentine dome is getting invisible, the
dome Aristillus and Autolycus are clearly visible.
On the top right
side on the image there is the dome Palus Putredinus between the shadow of two
mountains. |
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NEW 2016 Aristillus - Autolycus - Moon age 7.8 days
(49 %)
The
large domes Autolycus and Aristillus at a moon age of 7.8 days. The Valentine
Dome is barely visible. The peaks of the Montes Caucasus cast spectacular
shadows. |
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Moon age
8.5 days - Illumination 54 % |
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Aristillus - Theaetetus - Moon age 8.4 days
(54 %)
The domes
Aristillus and Theaetetus at a Moon age of 8.4 days.
The crater Cassini
(57 km) resembles a crater form that can be often found on Mars and have the
name "Rampart craters". |
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LRO -
Theaetetus
High resolution
LRO image of the Theaetetus dome with 125 m/px. Morphological it is similar to
Yerkes 1 in Mare Crisium, see Segment 1. The
upwarp and the system of rilles is clearly visible. |
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Rima Hadley - Putredinis and Beer - Moon age 8.4 days (54 %)
Rima Hadley is on of the best known and best
explored sinousoidal rilles on the Moon. Besides the rille there is the landing
site of Apollo 15. The rille has a lenght of 116 km. It arises from a caldera
in the arched region to the southwest (in the shadow). The caldera is named
Jomo, a male African first name. Hadley C, the crater in the middle of the
rille has a diameter of 5.8 kilometers.
Further to the west the small
effusive dome Putredinus 1 can be found. It has a summit caldera, a diameter of
7 kilomters and a height of 90 meters. Another effusive dome is visible south
of the small crater Beer (10 km) on the right side of the image. |
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Valentine domes 1 and 2 - Moon age 8.4 days (53 %)
At this Moon age the Valentine domes are not
detectable any more. |
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Moon age
9.5 days - Illumination 65 % |
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Rima Hadley - Putredinis -
Beer - Moonage 9.5 days (65
%)
Now the sun is
completely risen over Rima Hadley at this Moon age. The elongated caldera of
the sinusoidal rillee becomes visible and is marked in our image. This lighting
situation is also very good to observe craterlets in Archimedes (83 km) . In
our image about 30 of these small craters are detectable. |
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All Images - otherwise marked - and all Content are
© by Franz Hofmann + Wolfgang Paech |