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Record Details

Record 96 of 558
Laboratory Studies of Optical Characteristics and Condensation Processes of Cosmic Dust Particles
Author and Affiliation:
Spann, J. F., Jr.(NASA Marshall Space Flight Center, Huntsville, AL United States)
Abbas, M. M.(NASA Marshall Space Flight Center, Huntsville, AL United States)
Venturini, C. C.(Alabama Univ., Huntsville, AL United States)
Abstract: Information about the optical characteristics and physical processes involving cosmic dust particles is vital for interpretation of astronomical observations and an understanding of the formation and processing of dust in the evolutionary cycle of matter in the interstellar medium. Cosmic dust particles are formed in a variety of astrophysical environments such as in cool stellar outflows and circumstellar envelopes. Definitive knowledge of the nature, composition, and physical processes of cosmic dust grains, however, can only be inferred from astronomical observations through laboratory experiments on the analogs of hypothesized dust particles and with modeling calculations. Laboratory investigations of the nature, composition, and optical characteristics of cosmic dust particles are being, carried out at many institutions with a variety of experimental techniques. Despite a wealth of available data, however, many basic issues remain unresolved. An experimental facility based on suspension of dust particles in electrodynamic balance in a pressure/temperature controlled environment in a cavity has been operational at the NASA Marshall Space Flight Center, and is currently being employed for studies of dust particle charging mechanisms using electron beams and with UV radiation. In this paper, we discuss two general classes of experiments under planning stages that may be simultaneously carried out on this facility for cosmic dust investigations (i) Infrared optical characteristics (extinction coefficients and scattering phase functions) of the analogs of hypothesized of cosmic dust particles, such as natural and synthetic amorphous silicates with varying compositions, amorphous carbon grains, polycyclic aromatic hydrocarbons (PAHs), and icy core-mantle particles etc. The initial spectral range under consideration is 1-25 micrometers, to be extended to the far infrared region in the future (ii) Condensation of volatile gases on nucleus dust particles to be investigated for planetary and astrophysical environments.
Publication Date: Jan 01, 2000
Document ID:
20000067652
(Acquired Jul 21, 2000)
Subject Category: ASTROPHYSICS
Document Type: Preprint
Meeting Information: Physics of Dusty Plasma; 8th; 26-28 Apr. 2000; Santa Fe, NM; United States
Financial Sponsor: NASA Marshall Space Flight Center; Huntsville, AL United States
Organization Source: NASA Marshall Space Flight Center; Huntsville, AL United States
Description: 1p; In English
Distribution Limits: Unclassified; Publicly available; Unlimited
Rights: No Copyright
NASA Terms: CONDENSING; COSMIC DUST; OPTICAL PROPERTIES; ASTROPHYSICS; PARTICLES; ELECTRON BEAMS; ULTRAVIOLET RADIATION; STELLAR ENVELOPES; INTERSTELLAR MATTER; PLANETARY ENVIRONMENTS; INFRARED RADIATION
Availability Source: Other Sources
Availability Notes: Abstract Only
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