Make an illustration for this: Here's a timeline showing how elements form

Make an illustration for this: Here's a timeline showing how elements form, with a focus on their atomic numbers: --- ### **1. The Big Bang (13.8 Billion Years Ago)** - **Atomic Numbers:** 1 (Hydrogen), 2 (Helium) - **Description:** Right after the Big Bang, the universe cooled down, leading to the formation of the simplest elements: hydrogen (Atomic Number 1) and helium (Atomic Number 2). ### **2. Stellar Nucleosynthesis Begins (13.5 Billion Years Ago)** - **Atomic Numbers:** 1 to 2 (Hydrogen to Helium) - **Description:** In the cores of the first stars, nuclear fusion starts converting hydrogen into helium, producing energy and beginning the process of stellar nucleosynthesis. ### **3. Heavier Elements Form in Stars (13.5 Billion Years Ago - Present)** - **Atomic Numbers:** 3 to 26 (Lithium to Iron) - **Description:** Over time, stars fuse helium and other light elements to create heavier elements like carbon (Atomic Number 6), oxygen (Atomic Number 8), and up to iron (Atomic Number 26). ### **4. Supernova Explosions (13.4 Billion Years Ago - Present)** - **Atomic Numbers:** Greater than 26 (Iron) - **Description:** When massive stars explode in supernovae, the intense energy allows for the formation of elements heavier than iron, such as gold (Atomic Number 79) and uranium (Atomic Number 92). ### **5. Formation of the Solar System (4.6 Billion Years Ago)** - **Atomic Numbers:** Various (Including 6, 8, 14, 26) - **Description:** The remnants of earlier stars come together to form the Sun and planets. Elements like carbon, oxygen, silicon (Atomic Number 14), and iron become key building blocks of the planets, including Earth. ### **6. Earth's Crust Forms (4.5 Billion Years Ago)** - **Atomic Numbers:** 8, 14, 26 (Oxygen, Silicon, Iron) - **Description:** As Earth cools, its crust forms, rich in elements like oxygen, silicon, and iron, which are crucial for its structure. ### **7. Life Begins on Earth (4 Billion Years Ag