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Selena Buzzard (SB)
Lunar Exploration Project
Focused on South Pole
Shackleton Crater
SB 3D Interactive Model
The Selena Buzzard (SB) is a cutting-edge tethered exploration system designed to navigate and map the interior of Shackleton Crater at the lunar south pole. This cable-car-based concept employs a robust cable system supported by strategically placed ground-based anchors, ensuring stability and precise data collection even in extreme lunar conditions, such as perpetual shadow and cryogenic temperatures. With a continuous multi-functional tether, SB facilitates reliable power transmission and uninterrupted data to the base station, enhancing operational efficiency. Equipped with advanced instrumentation, the system gathers essential thermal, spectroscopic, and topographic data, providing invaluable insights into the Moon's surface and subsurface composition.
SB Animation
Traversability conditions and landing site assessment map for the lunar south polar region. The percentage of time that the surface will be illuminated and visible to the Earth is modeled for the expected Artemis timeframe (July 9, 2024 - June 11, 2025) at 500 m/pixel. Ideal conditions for surface activities (45% sunlight (SUN) and Earth (E) line-of-sight) are indicated by light yellow. Areas indicative of potential water ice on the surface are shown in light pink. (Source: https://www.lroc.asu.edu/images/1255)
Shackleton Crater, located at the lunar south pole, is a fascinating and unique place due to its extreme environmental conditions. The crater is about 21 kilometers (13 miles) in diameter and 4.2 kilometers (2.6 miles) deep, and it's notable because of the permanent shadow and the possibility of water ice trapped in these regions.
Sunlight at Shackleton Crater:
Rim of the Crater:
The rim of Shackleton Crater does receive sunlight for long periods, but it is never continuously illuminated. Because the Moon's axial tilt is only 1.5 degrees (compared to Earth’s 23.5 degrees), the poles experience very low solar angles. This causes the high points, like the crater’s rim, to be bathed in sunlight for extended durations throughout the lunar day. In some locations, sunlight might be received for up to 80–90% of the lunar day, although not continuously.
Crater Floor (Permanently Shadowed Region):
The interior floor of Shackleton Crater is in almost constant darkness. Since the sun is so low on the horizon near the lunar poles, the crater’s steep walls block sunlight from reaching the bottom. This lack of sunlight creates an environment where temperatures remain extremely cold, with estimates showing that the crater's floor can be as low as 40-50 K (-233 to -223°C or -387 to -369°F).
The permanently shadowed regions (PSRs) of Shackleton Crater are of great interest because they may harbor water ice deposits that have accumulated over billions of years. These deposits could be incredibly valuable for future lunar exploration as a source of water for drinking, creating oxygen, or even producing fuel (by splitting water into hydrogen and oxygen).
Why Shackleton Crater Is Important:
Water Ice Exploration: The permanently shadowed regions are prime candidates for ice accumulation. These areas are cold traps, meaning they can hold water ice without it sublimating into space. Discovering accessible water ice would be a game-changer for long-term lunar exploration and future missions to Mars, as it could be used for life support and fuel.
Continuous Power Supply on the Rim: The fact that the rim of Shackleton Crater receives nearly continuous sunlight makes it an ideal location for setting up solar-powered equipment and infrastructure. This provides a significant advantage for building bases or scientific outposts.
Extreme Conditions for Science: The extreme cold and shadowed environment offer opportunities for scientific research on materials and phenomena that might not exist in other regions of the Moon. It's an analog for studying other icy bodies in the solar system, such as moons of Jupiter and Saturn.
Shackleton Crater represents a compelling target for exploration, balancing the challenges of darkness and cold with the promise of resources that could support sustained human presence on the Moon.
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