PSR J1719-1438 is believed to be a planet-sized diamond, likely a remnant core of an ultra-low mass carbon-oxygen white dwarf. The discussion highlights the need for extreme pressure and heat for carbon to crystallize into diamond, raising questions about the evidence supporting this classification. The companion planet's density is noted to be significantly higher than that of pure diamond, suggesting a complex formation process. Comparisons are made to man-made diamonds, which also require specific conditions for creation. The conversation reflects curiosity about the scientific understanding of such celestial bodies and their characteristics.