Abiotic Production of Primitive Protein and Formed Microparticles
Polymerization of amino acids to give proteins and formed microparticles
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Polymerization of amino acids to give proteins and formed microparticles
Thermal polymerizations of amino acids and production of formed microparticles on lava
Design study for 2MV microparticle accelerator
Single stage prototype microparticle accelerator design study
Penetration of thin films by hypervelocity impact microparticles
Criticism of article on microparticle impact effect on metal optical properties
Sensors used in cosmic dust experiments studied for response to microparticle hypervelocity impacts, noting relationship to velocity
Hydrodynamic model of micrometeoroid impact - calculations for impact of spherical aluminum microparticle on semi-infinite aluminum target
Sensors used in cosmic dust experiments studied for response to microparticle hypervelocity impacts, noting relationship to velocity
Electrostatic acceleration system for hypervelocity microparticles with selected kinematic properties
Filamentary crystal growth associated with hypervelocity microparticle impacts on copper foil
Microparticle collection experiments during 1966 Orionid and Leonid meteor showers accomplished by Luster and ALARR /air launched-air recovered rocket/ instruments
Filamentary crystal growth associated with hypervelocity microparticles impact upon Cu foil
Thin film penetration by hypervelocity microparticles of carbonyl iron
Microparticles composed of each of four enzymically synthesized homopolynucleotides and the same lysine-rich proteinoid have been found to influence the condensation of the AMP-anhydrides of each of four amino acids. The conditions of preparation of the particles and other variables of the experiments control the types of reaction. When a period set of conditions was identified empirically, the incorporation favored the amino acids whose present-day codons are related to the homopolynucleotide in the particle.
The design of a three element piezoelectric microparticle impact sensing diaphragm is described which is sensitive to the detection of momentum propagated by the bending wave. The design achieves a sensitivity of .03 microdyn/sec and optimizes the detection of the direct-path pulse from impact relative to secondary reflections and interference from discontinuities. Measurement of the relative arrival times and the maximum amplitudes of the outputs from the three piezoelectric sensors leads to the determination of the impact position and the normally resolved impact momentum exchange. Coincidence of the signals and a partial redundancy of data leads to a very high noise discrimination.
By application of Lyttleton's theory for the formation of comets, it is shown that a possible mechanism for the origin and formation of a concentration of cosmic particles around the earth and the other planets of the solar system exists. In the vicinity of the neutral point, where the velocity of colliding particles is not greater than 6 km/s, it is found that if the solid particles after collision must remain in a solid state, there can be no possibility of accretion for Mercury, Mars, and the Moon, where the maximum value of the distance of the center of the planet to the asymptotic trajectory is less than the radius of the planet. On the other hand, the capture radii of microparticles in solid form varies from a minimum of 2.95 planetary radii for Venus and 3.47 for the Earth, to about 986 for Jupiter.
A microparticle accelerator has been devised for micrometeoroid impact and cratering simulation; the device produces high-velocity (0.5-15 km/sec), micrometer-sized projectiles of any cohesive material. In the source, an electrodynamic levitator, single particles are charged by ion bombardment in high vacuum. The vertical accelerator has four drift tubes, each initially at a high negative voltage. After injection of the projectile, each tube is grounded in turn at a time determined by the voltage and charge/mass ratio to give four acceleration stages with a total voltage equivalent to about 1.7 MV.