Abstract
New equilibrium thermodynamic distribution models of organic substances important to life in giant molecular clouds are suggested. These models use the normal distribution law of the standard enthalpy and the free energy (Helmholtz energy) for various organic molecules, amino acids, and nucleic acid components. These models were used to forecast organic molecule resources in the interstellar medium of the observable universe. The resources of the main biological molecules were estimated from radio-astronomical data.
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Bains, I., Brisbin, D., Cunningham, M., Sparks, P., Wong, T.: Molecular line mapping of the giant molecular cloud associated with RCW 106 I. 13CO. Mon. Not. R. Astron. Soc. 367(4), 1609–1628 (2006)
Binney, J., Merrifield, M.: Galactic Astronom. Princeton University Press, Princeton (1998)
Book Series Cellular Origin 2000–2013: Life in extreme habitats and astrobiology. In: Seckbach, J. (ed.) (2000–2013) 24 Volumes. Springer, Berlin (2000–2013)
Cami, J., Bernard-Salas, J., Peeters, E., Elizabeth Malek, S.: Detection of C60 and C70 in a Young Planetary Nebula. Science 329(5996), 1180–1182 (2010)
Dolomatov, M.Y.: Some physical and chemical aspects of simulating properties of multicomponent systems in the conditions of extreme influences. Z. Vses. Him. Obsestva Im. D.I. Mendeleeva 35(5), 632–638 (1990)
Dolomatov, MY.: Features of equilibrium thermodynamics complex systems with chaos of chemical constitutions and allocation of organic matter in the space. In: Abstracts of International Conference on Complex Systems, USA, Florida, Texas (2004)
Dolomatov, C.Y.: Fragments of the Real Substance Theory from the Hydrocarbon Systems to the Galaxies. Chemistry, Moscow (2005)
Dolomatov, M.Y., Kostyleva, E.V.: Characteristics of the organic substances abiogenic synthesis in space natural systems and the problem of oil origin. In: Oil Refining and Petrochemical Industry: The Materials of All-Russia Scientific Practical Conference, Ufa, pp. 8–14 (2001)
Dolomatov, M.Y., Zhuravleva, N.A.: The thermodynamic models of molecular chemical compound distribution in the giant molecular clouds medium. Appl. Phys. Res. 4(4) (2012). doi:10.5539/apr.v4n4p149
Hoyle, F., Wickramasinghe, N.C.: Astronomical Origins of Life: Steps Towards Panspermia. Kluwer Academic, Dordrecht (2000)
Kolesnichenko, A.V., Marov, M.Y.: Mechanics bases of heterogeneous environments in a circumsolar protoplanetary cloud: influence of firm particles on turbulence in a disk. Sol. Syst. Res. 40(1), 2–62 (2006)
Kwok, S.: Stardust. The Cosmic Seeds of Life. Springer, Berlin Heidelberg (2013)
Landau, L.D., Lifshitz, E.M.: Statistical Physics, 3rd edn. Butterworth-Heinemann, Oxford (1996)
Lee, Y., Snell, R.L., Dickman, R.L.: The cold, massive molecular cloud G216-2.5. 2: structure and kinematics. Astrophys. J. 432(1), 167–180 (1996)
Lovas, F.: Recommended rest frequencies for observed interstellar molecular microwave transitions. J. Phys. Chem. Ref. (1992). doi: 10.1063/1.555920
Makalkin, A.B., Ziglina, I.N.: Modeling formation of self-gravitating dust condensations and original planetesimals in a protoplanetary disk. In: The Third Moscow Solar System Symposium, Moscow, Space Research Institute, 3MS3-PC-03 (2012)
Makalkin, A.B., Ziglina, I.N., Dorofeeva, V.A., Safronov, V.S.: Structure of the protoplanetary disk embedded within the infalling envelope. In: Celnikier, L., Tran Thanh Van, J. (eds.) Planetary Systems: The Long View, pp. 73–76. Editions Frontières, Singapore (1998)
Maloney, P.: Size-density relations in dark clouds: non-LTE effects. In: NASA. Ames Research Center Summer School on Interstellar Processes: Abstracts of Contributed Papers, pp. 45–46 (1986). (SEE N87-15043 06-90)
Marov, M.Y., Kolesnichenko, A.V.: Turbulence and Selforganizing: Problems Modelling of Space and Environments, p. 563. Springer, Berlin (2012)
Norman, H.: Horowitz to Utopia and Back: The Search for Life in the Solar System. W.H. Freeman, New York (1986)
Rudnitskiy, G.: Interstellar molecular clouds. Earth and Universe. (1999). http://ziv.telescopes.ru/latest.html
Sakamoto, S.: Physical conditions of molecular gas in the galaxy. Publ. Astron. Soc. Pac. 106, 1112 (1996)
Tsvetkov, A.G., Shematovich, V.I.: Kinetic Monte-Carlo method for simulating of astrochemical kinetics: trial calculations of formation of molecular hydrogen on interstellar dust particles. Sol. Syst. Res. 43(4), 315–327 (2009)
Tsvetkov, A.G., Shematovich, V.I.: Kinetic Monte-Carlo method for simulating astrochemical kinetics: hydrogen chemistry in diffusion clouds. Sol. Syst. Res. 44(3), 177–188 (2010)
Ulmschneider, P.: Intelligent Life in the Universe. Adv. Astrobiol. Biogeophys. Springer, Berlin Heidelberg (2006). doi:10.1007/11614371
Universität zu Köln: Molecules in Space. Universität zu Köln. http://www.astro.uni-koeln.de/cdms/molecules. (2013). Accessed 25 August 2013
Vasyunin, A.: Development of the theory of numerical simulation of the molecular composition of the interstellar medium. Ph.D. Dissertation, Moscow (2008)
Wickramasinghe, C.: Panspermia according to Hoyle. Astrophys. Space Sci. 285, 2:535–538 (2003)
Wickramasinghe, J.T., Wickramasinghe, N.C., Napier, W.M.: Comets and the Origins of Life. World Scientific, Singapore (2011)
Willttet, D.C.B.: Planetary and interstellar processes relevant to the origins of life. In: Research Center Summer School on Interstellar Processes: Abstracts of Contributed Papers, pp. 45–46. Springer, Dordrecht (1998) (SEE N87-15043 06-90)
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Dolomatov, M.Y., Zhuravleva, N.A. Thermodynamic models of the distribution of life-related organic molecules in the interstellar medium. Astrophys Space Sci 351, 213–218 (2014). https://doi.org/10.1007/s10509-014-1844-8
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DOI: https://doi.org/10.1007/s10509-014-1844-8