Cosmology is the study of the origin, evolution, and eventual fate of the universe. It is a branch of astronomy that seeks to understand the large-scale structure and dynamics of the universe as a whole.
Key Concepts in Cosmology
Big Bang Theory: This is the prevailing cosmological model for the observable universe from the earliest known periods through its subsequent large-scale evolution.
Dark Matter: This is a form of matter that is thought to account for approximately 85% of the matter in the universe and about a quarter of its total energydensity.
Dark Energy: This is an unknown form of energy that is hypothesized to permeate all of space, tending to accelerate the expansion of the universe.
Cosmic Microwave Background Radiation (CMB): This is electromagnetic radiation as a remnant from an early stage of the universe and it is considered the oldest light in the universe.
Investigating the different types of galaxies and their role in the structure of the universe.
Examining the expansion of the universe and the various cosmological models that seek to explain it.
Remember to also familiarize yourself with key scientists and astronomers who have contributed to the field of cosmology, such as Edwin Hubble, George Lemaitre, and Vera Rubin.
Keep in mind that cosmology is a dynamic and evolving field, so staying updated on the latest research and discoveries is essential for a comprehensive understanding of the universe.
Identify the distribution of freshwater and salt water on Earth (e.g., oceans, lakes, rivers, glaciers, ground water, polar ice caps) and construct a graphical representation depicting the amounts and percentages found in different reservoirs.