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Gassendi and Dome Gassendi
Ga1 - Moon age
11.6 days (84 %)
Gassendi (101
km) is one of the most interesting FF-crater and is located at the northern rim
of Mare Humorum. Gassendi clearly shows the tilt towards the Mare-center. The
craters at the southern rim, Doppelmayer and Lee, are also clearly tilted to
the center of the Mare. All three craters were flooded by lava which filled the
Mare. To the west there is the dome Gassendi ( type C2) with a diameter of
nearly 8 km and an height of just 100 meters. It is a bisected dome which is
devidedby a narrow rille with a length of about 56 km.
Just south
of Gassendi there is the Rima Herigonius. It is a sinusoidal rille which was a
lava channel in its active time. Rima Herigonius is difficult to observe, it is
only 1 to 2 kilometers wide at the widest points. |
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Liebig 1
- Moon age 11.6 days (84
%)
Doppelmayer (64 km) and Lee
are beautiful examples of so called tilted craters which have been tilted due
to the subsidence of the Mare surface and then flooded by lava. Doppelmayer and
Vitello (to the east) are also floor fractured crater. Doppelmayer has a
strange pyramidal massive central mountain. In the northwest is the Dome Liebig
1 which can be easily observed because of its relatively large height of about
365 meters. Its diameter is about 10 kilometers. A similar dome is Yangel1 in
Sinus Fidei.
The dome seems to be
located on an intrusive upwarp with a rough surface. To the west the Rima
Doppelmayer can be found. It is surrounded by a large area of pyroclastic ash
deposits on both sides. |
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Just southof
Liebig 1 there are the two effusive domes Doppelmayer 1 and 2. Both domes are
classified as type C1. Do 1 has a diameter of almost 17 kilometer with a height
of 400 meters and shows structures on its surface. Do 2 has a diameter of 12.5
kilometers and a height of 160 meters. That feature what looks in our image
like a narrow rille turns out to be an elongated caldera in a LRO
image. |
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LRO Liebig 1
The image to the left shows the Liebig 1 area in
a LRO image with a resolution of 125 m/px. |
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Liebig 1 - Moon age 11.5 days (83
%)
See description
above. |
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Doppelmayer
- Moon age 11.5 days (83
%)
The Doppelmayer 1 and 2
domes, imaged a few hours before the picture above. With this illumination the
domes are better visible than above. The "strange" central mountain of
Doppelmayer arises more plastically. In the top left egde of the image there is
the concentric double crater Marth, see Segment 9
C |
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Moon age 12.1 days - 13.1 days (87 - 95
%) |
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Gassendi and Dome Gassendi Ga
1 - Moon age 12.1
days (87 %)
See description of
Gassendi and Ga 1 above.
With an illumination of 87 % a slightly higher
area becomes visible south of Gassendi 1. we would classify it as a putative
dome. |
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Doppelmayer and Palmieri
- Moonage 12.1 days (87
%)
At the marked position
in this image should be an intrusive dome with a diameter of 13.5 kilometers
and a height of 60 meters. On our image there is nothing to see except for a
small bright and young impact crater. Even on the
LRO image of Palmierithe dome is very hard to
see.
The whole area in the west
of Mare Humorum is full of linear rilles. Many of it are certainly associated
with the Mare. North of Palmieri 1 there is the crater Palmieri with two
intersecting rilles on the floor. |
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Mons Hansteen and Hansteen Ha 1
- Moon age 12.1 days (87
%)
Hansteen 1 (also
Hansteen alpha) is classified as an intrusive structure. Its diameter is just
below 19 km at the height is only 85 meters. It can be learly seen on our
image. To the south there is an upwarp, which can be a putative
dome.
Mons Hansteen with its size of 29 x 27 kilometers reaches a height of
just over 1000 meters. It is classified as a volcanic structure formed by very
slow-moving lava. The spectral reflectance measurements of the surface show
strong similarities with those of the Gruithuisen domes. |
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Gassendi
- Mon age 13.1 days (95
%)
East of Gassendi there
is an intrusive megadome plateau with the unofficial name "The Helmet".
Officially it is called Agatharchides Plateau. For details see
Segment 09 C. |
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Putative Lohrmann A
- Moon age 13.1 days (95
%)
When having a look at the
terminator near the crater Lohrmann A (12 km) at an illumination of 95 % there
is a small upwarp which can be a putative lunar dome. |
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Putative Cavalerius
- Moon age 13.1 days (95
%)
Another putative plateau lies
further north, near the crater Cavalerius (7 km). It is a flat upwarp, which
seems to be crossed by rilles. Directly east of it there is the mysterious
structure Reiner Gamma, a so-called "Swirl". On the bottom left a part of the
Marius Hills are visible (see Segment
12)
Reiner Gamma is
neither a depression nor a bulge of the surrounding countryside. It is a
flat, bright oval of 35 kilometers in length with a long tail which extends
into the region of the Marius Hills. The oval is the center of a magnetic
anomaly. At this point there is the center of a strong magnetic field which is
much stronger than the normal lunar magnetic field. It is an absolutely
untypical object and the only one on the front of the Moon. |
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On the back
side of the Moon there are a small number of Swirls, which position is
antipodal to the big Mare of the front side of the Moon. It is not clear if
this is coincidence or not. In any case there is no antipodal Mare on the far
side of the moon for Reiner Gamma.
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Mondalter 12.8 Tage + 14.2 Tage (93 + 99
%) |
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Grimaldi Gr 1
- Moon age 12.8 days (93
%)
Grimaldi (222 km) is probably
rather a small impact basin than a large crater. In the northern area there is
a large intrusive plateau with a lenghth of about 30 km and a height of 160
meters. It has a clearly triangular shape. |
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Grimaldi Gr 1
- Moon age 14.2 days (99
%)
At a moon age of about 14
days, the triangular structure is clearly visible. On the surface of the dome
are at least 6 very small effusive structures visible. The shape of the whole
plateau is similar to Mons Rümker. |
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All Images - otherwise marked - and all Content are
© by Franz Hofmann + Wolfgang Paech |