The mass of the Earth is approximately 5.9 x 10^24 kg, a value that has remained relatively constant over time despite increases in population and biodiversity. This stability is due to the conservation of mass; new living organisms are formed from existing atoms rather than creating new mass. The Earth gains a small amount of mass from space debris, estimated at over 100 tons daily, but it loses more mass than it gains due to atmospheric escape from solar wind. The universal gravitational constant, G, which is crucial for calculating Earth's mass, does not change, and the variations in local gravitational acceleration (g) are minor and influenced by geographical features. Overall, the mass of the Earth is a reflection of the recycling of matter rather than a net increase, and significant changes in total mass would require extraordinary cosmic events.