Laboratory comparisons of organic materials to interstellar dust and the murchison meteorite

Abstract

Spectra of objects which lie along several lines of sight through the diffuse interstellar medium (DISM) reveal an absorption feature near 3.4 μm, which has been attributed to saturatedaliphatic hydrocarbons on interstellar grains. The similarity of the absorption bands near 3.4μm (2950 cm −1) along different lines of sight indicates that the carrier of this band lies in the diffuse dust. Several materials have been proposed as “fits” to the 3.4 μm feature over the years. A comparison of these identifications is presented. These comparisons illustrate the need for high resolution, high signal-to-noise observational data as a means of distinguishing between laboratory organics as matches to the interstellar material. Although any material containing hydrocarbons will produce features in the 3.4 μm region, the proposed “matches” to the DISM do differ in detail. These differences may help in the analyses of the chemical composition and physical processes which led to the production of the DISM organics, although ISO Observations through the 5–8 μm spectral region are essential for a definitive identification. A remarkable similarity between the spectrum of the diffuse dust and an organic extract from the Murchison meteorite suggests that some of the interstellar organic material may be preserved in primitive solar system bodies. The 3.4 μ absorption feature (in the rest frame) has recently been detected in external galaxies, indicating the widespread availability of organic material for incorporation into planetary systems.