Dodoma City Guide

Dodoma City Guide

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Dodoma City Guide for Could it have been a Halley-type meteoroid stream? Since Halley-type meteoroids tend to peak just before dawn, whereas Jupiter-family meteoroids tend to peak just after midnight, and since the velocity and inclination of the meteoroid stream responsible for the Hydrid meteor storm are on or over the upper threshold of typical Jupiter-family meteoroid streams approximately ? km/second and ? degrees respectively, a good case for the parent being a Halley-type comet, like C/ F Mellish, can be made. Actually, the orbit of the Hydrid meteoroid stream, assuming that the radiant of the meteors was two-thirds of the way from Gamma Hydrae to HIP or from Gamma Hydrae itself, is reminiscent of Comet Mellish in perihelion distance and eccentricity table David Asher, perceiving the similarity, backtracked the orbit of this comet to see if it matched, but found that Mellish’s argument of perihelion and ascending node did not evolve in a way that realistically permitted it itself to be the parent of the meteoroid stream. A comparison of the orbit of Comet C/ F Mellish to the orbit of the meteoroid stream responsible for the BC Hydrids, assuming that the meteors radiated from two-thirds of the way from Gamma Hydrae to HIP and that Vinf= Hydrids A or from Gamma and that Vinf Hydrids B. FIG Possible orbits of the meteoroid stream responsible for the meteor storm of October , BC. Apollo asteroid-type orbits fall within the pink zone, Jupiter-family orbits within the green zone, and Halley-type orbits within the yellow zone. The more elongated the orbit, the more steeply inclined it is. The outermost planetary orbit is that of Uranus. Dodoma City Guide 2016.

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