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Ethiopia Map for The higher this value, the steeper the brightness slope is. In the absence of adequate data to reine the pattern of cometary brightness development, scientists tend to assume that n=. This assumption is based on the idea that this is the average value for comets. According to recent analysis by Schmude, long-period comets can have values of n from – to over, but most are grouped between and, with the bulk of them concentrated between about and, and the approximate average being. For example, while Bennett's Comet of had a brightness slope of about, Hale- Bopp's was about Accordingly, anyone assuming that Hale-Bopp's display in the inner solar system would abide by the average brightness slope n would have been slightly but not greatly! Disappointed. In the tables accompanying my discussion of the Christ Comet's apparition, I shall offer brightness estimates based on the following values of n and It is likely that the brightness slope of the long-period Bethlehem Star comet comes within this range of values. In establishing the correct value of n, we have more to go on than merely estimates based on the comet's probable apparent magnitude at irst observation we have data regarding the comet's performance in the inner solar system. Ethiopia Map 2016.