In this scenario, the binary system consists of two rogue planets, which are planets that are not bound to a star and instead roam freely through space. These rogue planets are orbiting each other in a binary system, gravitationally bound to one another. In addition to the two rogue planets, there is also a brown dwarf in the system. A brown dwarf is a type of failed star that is not massive enough to sustain nuclear fusion in its core. This brown dwarf is larger and more massive than the rogue planets and acts as a powerful gravitational force in the system. One of the rogue planets is a gas giant, with a large mass and thick atmosphere of hydrogen and helium. The brown dwarf begins to consume the gas giant, slowly devouring its outer layers and pulling it towards itself with its strong gravitational pull. As the gas giant is consumed, its mass adds to the brown dwarf, making it even larger and more powerful in the system. Meanwhile, the other rogue planet orbits the brown dwarf and gas giant system, witnessing the dramatic events unfolding before it. The interactions between the three objects create a dynamic and chaotic environment in this binary system of rogue planets and a brown dwarf devouring a mass of gas giant.