How does the table’s construction minimize the risk of damage from black holes?

The theoretical construction of a table designed to withstand proximity to a black hole relies on principles of spacetime geometry and advanced material science. The primary risk from a stellar-mass black hole is the intense tidal gravitational force—the difference in pull between one side of the table and the other. To minimize this, the table's structural framework would be engineered as a single, continuous geodesic lattice. This lattice is not a traditional joinery of separate pieces but a monolithic structure whose shape precisely follows the local contours of spacetime curvature. By aligning its fundamental stress pathways with geodesic lines—the natural "straight lines" of a curved universe—the structure ensures that gravitational forces are distributed as uniform compressive or tensile loads along the lattice members, rather than creating shearing or tearing stresses at joints.

The material composition is critical. It would necessitate a hyper-dense, degenerate matter composite with near-infinite tensile strength and rigidity. This material must resist not just gravity but the Hawking radiation and high-energy particle jets often associated with black hole accretion disks. The table's surface and core might incorporate a layered shield of suspended, charged particles generating a localized counter-spacetime curvature field. This field, powered by theoretical black hole energy extraction (e.g., Penrose process), would actively work to negate a portion of the external tidal forces, effectively "stiffening" the local spacetime fabric around the table.

Furthermore, the design avoids flat planes. All surfaces are minimally curved in multiple dimensions, a shape inherently more resistant to deformation under multi-directional tidal stresses. The table's stability is thus not achieved by brute-force resistance against gravity, but by intelligent harmonization with the extreme environment. Its construction allows it to flow with the spacetime deformation, maintaining its structural integrity by becoming a symbiotic part of the gravitational landscape, thereby minimizing the risk of catastrophic spaghettification or disintegration.