title: Solid organic matter in the atmosphere and on the surface of outer Solar System bodies.
abstract: Many bodies in the outer Solar System display the presence of low albedo materials. These materials, evident on the surface of asteroids, comets, Kuiper Belt objects and their intermediate evolutionary step, Centaurs, are related to macromolecular carbon bearing materials such as polycyclic aromatic hydrocarbons and organic materials such as methanol and related light hydrocarbons, embedded in a dark, refractory, photoprocessed matrix. Many planetary rings and satellites around the outer gaseous planets display such component materials. One example, Saturn's largest satellite, Titan, whose atmosphere is comprised of around 90% molecular nitrogen N2 and less than 10% methane CH4, displays this kind of low reflectivity material in its atmospheric haze. These materials were first recorded during the Voyager 1 and 2 flybys of Titan and showed up as an optically thick pinkish orange haze layer. These materials are broadly classified into a chemical group whose laboratory analogs are termed "tholins", after the Greek word for "muddy". Their analogs are produced in the laboratory via the irradiation of gas mixtures and ice mixtures by radiation simulating Solar ultraviolet (UV) photons or keV charged particles simulating particles trapped in Saturn's magnetosphere. Fair analogs of Titan tholin are produced by bombarding a 9:1 mixture of N2:CH4 with charged particles and its match to observations of both the spectrum and scattering properties of the Titan haze is very good over a wide range of wavelengths. In this paper, we describe the historical background of laboratory research on this kind of organic matter and how our laboratory investigations of Titan tholin compare. We comment on the probable existence of polycyclic aromatic hydrocarbons in the Titan Haze and how biological and nonbiological racemic amino acids produced from the acid hydrolysis of Titan tholins make these complex organic compounds prime candidates in the evolution of terrestrial life and extraterrestrial life in our own Solar System and beyond. Finally, we also compare the spectrum and scattering properties of our resulting tholin mixtures with those observed on Centaur 5145 Pholus and the dark hemisphere of Saturn's satellite Iapetus in order to demonstrate the widespread distribution of similar organics throughout the Solar System.
authors.affiliation: MS 239-14, NASA Ames Research Center, Moffett Field, CA 94035-1000, USA.
authors.forename: B N
authors.initials: BN
authors.lastname: Khare
authors.forename: E L
authors.initials: EL
authors.lastname: Bakes
authors.forename: D
authors.initials: D
authors.lastname: Cruikshank
authors.forename: C P
authors.initials: CP
authors.lastname: McKay
mesh_terms: D000641:Ammonia / Q000737:chemistry; D001272:Atmosphere / Q000737:chemistry*; D001274:Atmospheric Pressure; D004583:Electrons; D019418:Evolution, Chemical; D005118:Extraterrestrial Environment; D020450:Heavy Ions; D006838:Hydrocarbons / Q000032:analysis* / Q000138:chemical synthesis; D008697:Methane / Q000737:chemistry; D055095:Optics and Photonics; D000069497:Origin of Life; D011108:Polymers / Q000032:analysis* / Q000138:chemical synthesis; D018539:Saturn; D016082:Solar System
chemical_list: D006838:Hydrocarbons; D011108:Polymers; D000641:Ammonia; D008697:Methane