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Astronomical Alignment

At a little after midday on the 7th of August, humankind will experience a remarkable moment, if for a fleeting second, as the clock ticks over to show 12:34:56, 7/8/9. Depending on your clock, you may have even captured a rehearsal event in the wee hours of the morning. But if you do want to catch the show, be sure to get in today. It's a performance that's unlikely to appear again for another 100 years. If you can't wait that long, fear not, because in less than 80 years today's alignment well be spectacularly surpassed, when all 10 digits will align in perfect order: 01:23:45, 6/7/89.

But how did we arrive at this extraordinary moment? With a great deal of rigmarole, as it turns out. When Jesus was walking the Earth 2000 years ago the world had not yet thought to count years anno domini (AD), and Augustus had only recently been honoured in the calendar system, renaming Sextilis to August. But the calendar of the time, the Julian calendar (named for Julius Caesar), was quite accurate by today's measures - astronomers had correctly approximated the period of seasonal variation over the year to 365 days and even accounted for most of the inaccuracy by adding an extra day to February every four years. And this was 1600 years before Galileo Galilei managed to get himself arrested by vehemently arguing that the Earth revolves around the sun!

In fact it took until Galilei's time for the Julian calendar to be surpassed. On the 24th of February, 1582 (by our current calendar), Pope Gregory XIII decreed the Gregorian calendar and it became the internationally accepted civil calendar we still use today (although there are plenty of creative variations on how to present it). Most of Europe at that time was already using the Incarnation of Jesus as an epoch for counting the years, and the main reform introduced by the Gregorian calendar was to further refine the inaccuracy of leap years by specifying the "don't leap if divisible 100, except if also divisible by 400" condition we use today. So in a world that still mostly believed the sun revolved around the Earth, astronomers were able to measure the yearly period to 365.2425 days. Not bad, considering we now know that the earth actually takes between 365.2421 and 365.2596 days to orbit the sun, depending on which of the several possible points of reference are used.

That brings us to 2008 AD, which is actually 2007 lots of 365 or 366 days since Jesus was born, because his first year is denoted 1 AD - and even then scholars generally agree that the historical evidence is too unclear to be sure that 1 AD wasn't off by at least a few years. But let's stick with the status quo, which places us at day 733407, and move on to the month.

The origin of a month is suggested by its cognate, Moon. Indeed, a month arose as a measure of the cycle of moon phases. The irregular lengths of the months we use today however, are less a measure of astronomical behaviour and more a product of variously motivated adjustments over a long and vague history. The variation from astronomical behaviour is particularly evident in February, which can pass without a single full moon occurring. Our modern month lengths were set way back in 45 BC with the introduction of the Julian calendar, and August became the eighth month instead of the sixth several hundred years prior. August 2008 places us at day 733619.

Even before it was well understood that the Earth undergoes rotation, it was clear to astronomers that the pattern of stars above them repeated with some regularity, and the period of a day could be measured. The day then, has historically formed a useful fundamental measure of time, from which other units such as the year and the hour, could be defined. The 8th day of August brings us to day 733627.

The hour was chosen in ancient civilisations as a convenient way to section a day, and the most logical division of the time was twelve. The period between sunrise and sunset was therefore split into twelve hours, and a full day became 24 hours. Most people these days would assume that dividing by ten would have been a more logical choice. Perhaps it would have been, but when it's clear to you that the seasonal variations of the year are marked by twelve cycles of moon phases, and all your life you've been counting to twelve on one hand by tapping your thumb against each of the phalanges of your other four fingers, you may well think otherwise. The 12th hour on the 8th day puts us at hour 17606867 AD.

The Babylonians recognised the number 60 as being particularly suitable for arithmetic, given it is divisible by 2, 3, 4, 5, 6 and 10, and did their astronomical calculations in the sexagesimal (base-60) system. It is from them that our divisions of the hour - the minute and the second - arise. The 34th minute of the 12th hour puts us at minute 1056412028 AD, and finally, the 56th second of the 34th minute places the historical event of 12:34:56 on the 7th August, 2009 at the 63384721712th second, anno domini.

But what does 63384721712 represent? Well, substituting dots for seconds might give you a pictorial representation. Or consider that that many 5 cent coins would weigh more than four and half Sydney Harbour Bridges, yet if you placed all those coins end to end you'd still only be one hundredth the way to the Sun. In other words, large numbers are terribly hard to comprehend, and that's why scientists use a variety of units - instead of the Sun being 6338472171200 coins away, it's 1 AU (astronomical unit) away. Instead of the Sydney Harbour bridge weighing 14085493713 coins, it weighs 36 kilotons. The units we use to tell the date might be a hodge-podge of millennia old decisions, but they sure are a great deal nicer than keeping track of 63384721712 seconds!

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