Experimental indication of a naphthalene-base molecular aggregate for the carrier of the 2175 angstroms interstellar extinction feature.
Experiments where the simple polycyclic aromatic hydrocarbon (PAH) naphthalene (C10H8) is subjected to the energetic environment of a plasma have resulted in the synthesis of a molecular aggregate that has ultraviolet spectral characteristics that suggest it provides insight into the nature of the carrier of the 2175 angstroms interstellar extinction feature and may be a laboratory analog. Ultraviolet, visible, infrared, and mass spectroscopy, along with gas chromatography, indicate that it is a molecular aggregate in which an aromatic double ring ("naphthalene") structural base serves as the electron "box" chromophore that gives rise to the envelope of the 2175 angstroms feature. This chromophore can also provide the peak of the feature or function as a mantle in concert with another peak provider such as graphite. The molecular base/chromophore manifests itself both as a structural component of an alkyl-aromatic polymer and as a substructure of hydrogenated PAH species. Its spectral and molecular characteristics are consistent with what is generally expected for a complex molecular aggregate that has a role as an interstellar constituent.
Beegle
L W
LW
Department of Physics, The University of Alabama at Birmingham 35294-1170, USA.
Wdowiak
T J
TJ
Robinson
M S
MS
Cronin
J R
JR
McGehee
M D
MD
Clemett
S J
SJ
Gillette
S
S
D055580:Astronomical Phenomena; D001256:Astronomy; D005118:Extraterrestrial Environment; D008401:Gas Chromatography-Mass Spectrometry; D005740:Gases / Q000032:analysis*; D009281:Naphthalenes / Q000032:analysis / Q000737:chemistry*; D013055:Spectrophotometry, Infrared; D013056:Spectrophotometry, Ultraviolet
D005740:Gases; D009281:Naphthalenes; C031721:naphthalene