Planets, Comets, Asteroids and Dust
Asteroids and comets are considered remnants from the huge cloud of gas and dust that condensed to generate the sun, planets, and moons certain 4.5 billion years ago. Today, most asteroids orbit the sun in a tightly packed belt located between Mars and Jupiter. And when detected through a telescope, comets appear fuzzier.
- Hyperbolic comets
- The C-type asteroids
- The S-types asteroids
- The M-types asteroids
- Massive planet
- Extrasolar planet
- Metallic dusts
- Mineral dusts
- Chemical dusts
- Organic and vegetable dusts
Related Conference of Planets, Comets, Asteroids and Dust
December 12-13, 2024
4th International Conference on Applied Physics and Materials Science
Rome, Italy
June 19-20, 2025
8th International Conference on Astronomy, Astrophysics and Space Science
Budapest, Hungary
Planets, Comets, Asteroids and Dust 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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