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- W1979851545 abstract "I suggest an idea of primitive life creation on protocomets with sizes 100 m to 100 km at very early stages (0.1 to 100 Myr) after our Supernova explosion 4.56 Gyr before present. Dust condensation in supernova remnants develops in conditions of decreasing gas temperature. After it crosses the level of 273 K, initial comets become rich in water and organic compounds. Their surface temperature is governed by equilibrium between heat production by radioactivity and thermal radiation from the surface. (The sun began to contribute to the thermal balance only at 50 - 100 Myr). Main energy contribution at this stage is produced by the following isotopes (decay time in Myr in brackets): 41Ca(0.14), 60Fe(0.30), 26Al(0.72), 53Mn(3.70).© (1999) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only." @default.
- W1979851545 created "2016-06-24" @default.
- W1979851545 creator A5069969664 @default.
- W1979851545 date "1999-12-30" @default.
- W1979851545 modified "2023-09-23" @default.
- W1979851545 title "<title>Possibility of life origin on radioactive source of energy after our supernova explosion</title>" @default.
- W1979851545 doi "https://doi.org/10.1117/12.375080" @default.
- W1979851545 hasPublicationYear "1999" @default.
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