Blast into 2025: Conquer the Astronomy Challenge – Your Cosmic Adventure Awaits!

The presence of channels, valleys, and gullies on the surface of Mars serves as the strongest evidence for the planet's history of liquid water. These geological features resemble those found on Earth, which are typically formed by the erosion and transport of material by flowing water. The intricate patterns and formations indicate that water once flowed across the Martian surface, carving out these formations over time.

This evidence aligns with various studies and observations that showcase the potential for ancient river systems and outflow channels, supporting the idea that Mars had a significantly wetter environment in its past. While ice deposits in polar regions are indicative of water presence, they do not provide evidence of liquid water flowing across the surface. Other options like current precipitation or lakes observed from orbiting satellites are either not relevant to past water history or have not been conclusively proven to exist in the context of Martian history. The geological features described in the correct answer provide compelling evidence of the presence and activity of liquid water, highlighting the planet's dynamic past.