Cosmic Dust
A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "Space Science".
Deadline for manuscript submissions: closed (15 July 2022) | Viewed by 331
Special Issue Editor
Interests: comets: nucleus structure and surface evolution, activity, dust and gas coma, dust, ion and neutral gas tails; trans neptunian objects; Oort cloud; interplanetary dust; trail and meteoric streams; structure and chemistry of the protoplanetary disk; accretion, early evolution and structure of planetesimals; pebbles; space missions to small bodies; spacecraft instrumentation
Special Issue Information
Dear Colleagues,
Space missions to comets and Kuiper Belt Objects have confirmed that planets were probably born by the gravitational collapse of pebble clouds triggered by streaming instability processes in the protoplanetary disk. In this Special Issue, we will review the physical processes forming dust in the interstellar medium, how dust evolved in the protosolar nebula, and how it accreted into pebbles in the protoplanetary disk, according to laboratory experiments of collisions among dust particles. We will review dust data collected on comets, supporting structural models of these objects, i.e., the most pristine bodies in our solar system. We will compare cometary dust to that collected on asteroids, bodies that underwent heavy collisional processes. Finally, we will follow how dust released by cometary activity and asteroidal collisions feed the interplanetary dust cloud today, observed as zodiacal light.
Dr. Marco Fulle
Guest Editor
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Keywords
- dust
- interstellar dust
- cometary dust
- asteroidal dust
- interplanetary dust
- pebbles
- protoplanetary disk
- laboratory experiments
- dust collisions
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