SOOT LINES | The new parameter that could help us locate new type of ALIENS in the Universe.
When we look for habitable planets, we usually focus on the habitable zone, the region around a star where liquid water can exist on a rocky world. But there might be another important factor that we have overlooked: the soot line, the boundary where solid carbon molecules are destroyed by heat and radiation. In this video, we explore how the soot line could affect the formation and evolution of planets, and what that means for our search for life in the universe. We will learn how Earth is water-poor and carbon-poor because it formed inside the soot line, and how planets that form between the soot line and the water-ice line could be rich in organic carbon but water-poor. We will also discuss how these sooty worlds could have different atmospheric compositions and surface environments than Earth, and whether they could support life as we know it or not. Join us as we discover a new way to expand the search for habitable planets beyond the soot line.
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