The event horizon of a black hole does not form solely along the equatorial plane; it actually encompasses the entire black hole. Animated depictions simplify this concept into 2D representations, which can be misleading. Most black holes are modeled using the Schwarzschild solution, but many may actually be Kerr black holes due to their common rotation. The understanding of black hole formation, particularly regarding angular momentum loss, remains incomplete, leading to uncertainty about the prevalence of rotating black holes. Overall, the event horizon's formation is a complex topic that extends beyond simplistic visualizations.