Introduction of cosmic microwave background
Cosmic Microwave Background (CMB) research illuminates the early moments of our universe, providing a snapshot of its infancy merely 380,000 years after the Big Bang
Astrochemistry, a captivating interdisciplinary field, explores the chemical makeup and processes in the universe beyond Earth.
Investigating the composition of the interstellar medium, focusing on the presence of organic molecules, ions, and dust grains. Understanding these components is crucial for deciphering the formation of stars and planetary systems.
Analyzing the chemical reactions and pathways that occur in space environments, including molecular cloud cores and protoplanetary disks. Studying these reactions provides insights into the formation of complex molecules and prebiotic compounds.
Examining the processes within stars that lead to the fusion of lighter elements into heavier ones, elucidating the origin of elements essential for life. This subtopic explores nucleosynthesis in various stellar environments, contributing to our understanding of element distribution in the universe.
Investigating the atmospheres of exoplanets to identify chemical signatures indicative of habitability or even extraterrestrial life. Studying exoplanetary chemistry helps scientists assess the potential habitability of distant worlds and the conditions necessary for life to thrive.
Exploring the connection between astrochemistry and the origins of life, focusing on the synthesis of organic molecules and their role in the emergence of life. This subfield investigates the conditions under which life-supporting molecules could form in space, providing insights into the possibility of life elsewhere in the universe.