--click on name below--
Overview
Untitled Near Side
Mare Nectaris
Arzachel
Mare Orientale
Unknown Topography
Deslandres Crater
Theopholis Crater
Einstein-Bohr Crater
Mare Crisium
Ptolemaeus Crater
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Lunar Topographies Overview
These carvings represent segments of the moon's surface as found in the topograhical data from NASA's LRO and JAXA's KAGUYA missions.
Painstaking attention is paid to the relationship of crater groups in the composition of each carving.
Areas of special interest have a natural balance of crater to sea; rough to gentle in texture.
"On the moon we will develop technologies to survive in the infinite frontier of space, because the moon presents
the same challenges we will encounter throughout the universe: harmful radiation, electrified dust, and extreme
temperatures.
Just as a scout finds the safest way for expeditions on Earth, NASA will first send a robotic scout,
called the Lunar Reconnaissance Orbiter (LRO), to gather crucial data on the lunar environment that
will help astronauts prepare for long-duration lunar expeditions.
LRO will spend at least a year in a low polar orbit approximately 50 kilometers (31 miles)
above the lunar surface, while its seven instruments find safe landing sites, locate potential resources,
characterize the radiation environment and test new technology."
from NASA
"The Japan Aerospace Exploration Agency (JAXA) launched "KAGUYA (SELENE)" by the H-IIA
Launch Vehicle at 10:31:01 a.m. on September 14, 2007 (JST) from Tanegashima Space Center (TNSC).
The major objectives of the "KAGUYA" mission are to obtain scientific data of the lunar origin and
evolution and to develop the technology for the future lunar exploration. "KAGUYA" consists of a main
orbiting satellite at about 100km altitude and two small satellites (Relay Satellite and VRAD Satellite)
in polar orbit. The orbiters will carry instruments for scientific investigation of the Moon, on the Moon,
and from the Moon."
from JAXA
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Untitled Near Side
This carving represents a large segment of the moon's visible side. The scale and grandure of the Montes Apenninus is juxtaposed with the details of Ptolemaeus and its neighbors to the south.
It is carved in purple heart. This wood has a dynamic coloration that produces strata that interact with the topography of the carving.
14" X 65" X 1"
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Mare Nectaris
Mare Nectaris and associated topography, south of the sea of tranquility
It is carved in redgum, the wood of Liquidambar styraciflua. This wood has a dynamic coloration that produces strata that interact with the topography of the carving.
29" diameter X 1"
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Arzachel Crater
Arzachel Crater and surrounding topography.
It is carved in padauk, an African wood of rich, deep orange color.
5" X 11" x 2"
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Mare Orientale Triptych
This 3 panel work is of the north eastern quadrant of Mare Orientale and its surrounding area
It is carved in Sapele, another African wood.
It's almost flesh-colored and has an opalescent grain. The highlights of the carving shimmer as the viewer passes by
38" X 15" x 1"
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Unknown Crater Set
This work is of an unknown region of the moon
It is carved from Black Walnut, a common North American wood.
It's it is rich and dark brown and has a subtle grain.
6.5" X 25" x 2"
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Deslandres Crater
Deslandres Crater and its neighboring topography
It is carved from Purpleheart (Peltogyne,).
It's it is a rich purple and has a subtle, even grain.
4" X 13" x 2"
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Theopholis
Theopholis its mate, south of the sea of tranquility.
This is another redgum carving
6" X 11" x 1"
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Einstein-Bohr Craters
Einstein had personality, so does the crater of his namesake. It shares a region with another famous physicist, Neils Bohr.
This is another Purpleheart carving
11" diameter x 1"
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Mare Crisium
Another large-format carving in redgum. Mare Crisium is a large sea north-east of the sea of tranquility
9" x 32" x 1"
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Ptolemaeus Crater
Anothe large-format carving in Sapele. Ptolemaeus is a large crater south of the sea of vapor and the bay of billows
7" x 38" x 1"
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