Stars, Cool Dwarfs, Brown Dwarfs
Brown dwarfs are substances which are too big to be called planets and too minor to be stars. They have crowds that range between twice the mass of Jupiter and the lower mass limit for nuclear reactions. An ultra-cool dwarf is a stellar or sub-stellar object of spectral class M that has an effective temperature under 2,700 K. TRAPPIST-1 is a widely known example of an ultra-cool dwarf star. Stars are enormous celestial bodies made mostly of hydrogen and helium that produce light and heat from the mixing nuclear forges inside their cores. Aside from our sun, the dots of bright we see in the sky are all light-years from Earth.
- Deuterium fusion
- Sub-brown dwarf
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Stars, Cool Dwarfs, Brown Dwarfs Conference Speakers
Recommended Sessions
- Aeronautical and Aerospace Engineering
- Astrochemistry and Spectroscopy
- Astronomical Computing and Applications
- Astrophysics and Gravitational Waves
- Cosmic Microwave Background and Radiation
- Cosmology and Gravitational Physics
- Dark Matter, Dark Energy, and Black Holes
- Earth and Atmospheric science
- Electromagnetic radiation
- Exoplanets and Planetary Physics
- Galaxies and Big Bang Theory
- Neutrino and Nuclear Astrophysics
- Optical Astronomy and Optoelectronics
- Particle Physics and Higgs Boson
- Physics and Astronomy
- Planets, Comets, Asteroids and Dust
- Space Missions and Satellites
- Stars, Cool Dwarfs, Brown Dwarfs
- Stellar Evolution, Atmospheres and Winds
- Sun, Solar System and Extrasolar Planetary Systems
- Supernovae, Planetary Nebulae and Supernova Remnants
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