Session
2023 poster session
Location
Weber State University
Start Date
5-8-2023 10:00 AM
Description
Brown dwarfs are celestial bodies outside the solar system that are more massive than planets, but less massive than stars. Since they are less massive than stars, they do not fuse hydrogen in their core, but rather cool slowly over time. However, brown dwarfs still emit light. We can measure this light by taking its spectra. From this spectra, we can learn many characteristics and properties of brown dwarfs, such as their temperature, chemical composition, and much more. Brown dwarfs can be categorized by their spectra into M,L,T and Y spectral types.
Atmospheric Modeling of Brown Dwarfs
Weber State University
Brown dwarfs are celestial bodies outside the solar system that are more massive than planets, but less massive than stars. Since they are less massive than stars, they do not fuse hydrogen in their core, but rather cool slowly over time. However, brown dwarfs still emit light. We can measure this light by taking its spectra. From this spectra, we can learn many characteristics and properties of brown dwarfs, such as their temperature, chemical composition, and much more. Brown dwarfs can be categorized by their spectra into M,L,T and Y spectral types.