Differences
This shows you the differences between two versions of the page.
Both sides previous revisionPrevious revisionNext revision | Previous revision | ||
courses:ast100:5 [2024/12/05 09:32] – asad | courses:ast100:5 [2024/12/14 12:16] (current) – [2. Periodic table] asad | ||
---|---|---|---|
Line 1: | Line 1: | ||
====== 5. Chemical Age ====== | ====== 5. Chemical Age ====== | ||
+ | |||
+ | **Juno**: Our boat is now transitioning from the Brahmaputra to the Jamuna, making this the perfect time to begin discussing the Chemical Era. The connection between Krishna of Mathura and the Taj Mahal of Agra offers a deep metaphorical link to Yamuna’s lifeblood. But to start this era, we must first revisit Earth' | ||
+ | |||
+ | **Socrates**: | ||
+ | |||
+ | **Juno**: Since the complex chemistry of only one planet is fully known to us, it makes sense to concentrate on Earth during this era. However, by the end of the discussion, we’ll also talk about ways to search for complex molecules and life on other planets within or beyond the Solar System. In fact, our approach here is quite similar to the Planetary Era. During the Planetary Era, Hermes mainly focused on the Solar System but concluded by discussing the discovery of planets around other stars. | ||
+ | |||
+ | **Socrates**: | ||
+ | |||
+ | ===== - Oceans and Atmosphere ===== | ||
+ | |||
+ | **Juno**: About 4.5 billion years ago, Earth was born. For the first 500 million years, its surface was extremely hot, dominated by volcanoes, and it rotated rapidly on its axis, completing a single rotation in just 12 hours. On top of that, leftover fragments of rocks and comets from the formation of the inner planets bombarded Earth during the Late Heavy Bombardment. This era is known as the **Hadean Era**. Some intact **zircon (ZrSiO₄)** crystals from that time indicate that oceans already existed. | ||
+ | |||
+ | **Socrates**: | ||
+ | |||
+ | **Juno**: Water vapor escaped from Earth' | ||
+ | |||
+ | **Socrates**: | ||
+ | |||
+ | {{: | ||
+ | |||
+ | **Juno**: It shows not only the rise of oxygen in the atmosphere but also significant chemical changes in the oceans. The **Archean Era** began after the Hadean, approximately 4 billion years ago. However, Earth’s crust began to stabilize around 3.8 billion years ago, when the precursors of modern continents, called **microcontinents**, | ||
+ | |||
+ | **Socrates**: | ||
+ | |||
+ | **Juno**: Yes, you can think of it that way. Today, oxygen levels are about 21%, and it started rising from near-zero around 3.2 billion years ago, as marked by the dashed line. Early photosynthesis wasn’t oxygenic, meaning it didn’t produce oxygen. During this period, bacteria combined oxygen with iron and water, forming **iron compounds** at the ocean floor. Oxygenic photosynthesis began in earnest about 3 billion years ago. Around this same time, microcontinents merged to form larger landmasses. The newly produced oxygen reacted with iron in the oceans, filling them with **iron compounds**. This is what the figure refers to as an "Iron Ocean." | ||
+ | |||
+ | **Socrates**: | ||
+ | |||
+ | **Juno**: Yes, iron was one reason. Another was the presence of many microbes in the ocean that used oxygen for metabolism. Only after the iron available for oxidation in the ocean decreased did cyanobacteria-produced oxygen start to mix into the air. In a relatively short time, atmospheric oxygen rose to nearly 1%. This oxygen then oxidized sulfur, dissolving it into the oceans, leading to what we call the **“Sulfur Ocean.”** How oxygen levels rose from 1% to 20% is a topic for the Biological Era, not now. | ||
+ | |||
+ | **Socrates**: | ||
===== - Periodic table ===== | ===== - Periodic table ===== | ||
- | < | + | < |
+ | <iframe src=" | ||
</ | </ | ||
- | ===== - Stellar oven ===== | ||
{{: | {{: | ||
- | |||
===== - Life on earth ===== | ===== - Life on earth ===== | ||
{{: | {{: | ||
- | {{: | ||
===== - Habitable zones ===== | ===== - Habitable zones ===== |
courses/ast100/5.1733416335.txt.gz · Last modified: 2024/12/05 09:32 by asad