A leap second will be added to official timekeeping this weekend. It will happen just before midnight UTC (7 p.m. CDT) on June 30, 2012.
COORDINATED UNIVERSAL TIME (UTC) WILL SEQUENCE AS FOLLOWS:
30 JUN 2012 23 HOURS 59 MINUTES 59 SECONDS
30 JUN 2012 23 HOURS 59 MINUTES 60 SECONDS
01 JUL 2012 00 HOURS 00 MINUTES 00 SECONDS
A leap second is a one-second adjustment to the Coordinated Universal Time (UTC). It’s an extra second added in to our official timekeeping, with the previous one being December 31, 2008.
At the same time, the International Telecommunications Union (ITU), a United Nations body that governs some global issues related to time, has been contemplating the controversial idea of a leap second. They considered abolishing the practice, but in late January 2012 – with delegates from more than 150 nations meeting in Geneva – the ITU decided to defer a proposal to dump the leap second until their 2015 meeting.
Why do we need a leap second? Isn’t the length of our day set by the rotation of the Earth? Like the ancients who insisted that all motion in the heavens must be perfect, uniform and unvarying, many of us today assume that the Earth’s rotation – its spin on its axis – is perfectly steady. We learned, correctly, that the sun, moon, stars and planets parade across our sky because the Earth turns. So it is easy to understand why we assume that the Earth’s rotation is precise and unwavering. Yet Earth’s rotation does not stay perfectly steady.
Instead, compared to modern timekeeping methods such as atomic clocks, the Earth is a notoriously poor timepiece. Not only is Earth’s spin slowing down, but it also is subject to effects that cannot even be predicted well.
If you have ever been to the beach, you will be familiar with the main reason our planet is slowing down. That reason is ocean tides. As our planet rotates, it plows past the great watery bulges (raised mostly by the gravitational interaction of the Earth and moon), which serves to slow it down much like a brake on a rotating wheel. This effect is small, actually very small. According to calculations based on the timing of ancient astronomical events (eclipses), the Earth’s rotation has slowed down by about .0015 to .002 seconds per day per century. That means that the a day in 2012 is about 0.002 seconds (2 milliseconds, or two-thousandths of a second) longer than was a day in 1912.
That in itself is not much, and is not enough to justify adding a “leap second” every 18 months or so, as has been done since 1972. The length of a day today is almost imperceptibly longer than the length as the same day last year. In the 1800s, a day was defined as 86,400 seconds. Today it is 86,400.002 seconds, roughly.
The discrepancy comes by comparing the Earth’s daily rotation relative to astronomical objects (which show the planet slowing down), to a extremely high precision atomic clock (which is accurate to about a billionth of a second per day).
The Earth is slowing down, very slowly. It takes about 100 years for Earth’s rotation to add just 0.002 seconds to the time it takes Earth to spin once on its axis. What happens, though, is that the daily 0.002-second difference between the original definition of a day as being 86,400 seconds builds up. After one day is it 0.002 seconds. After two days it is 0.004 seconds. After three days it is 0.006 seconds and so on. After about a year and a half, the difference mounts to about 1 second. It is this difference that requires the addition of a leap second.
The situation is not quite that clear cut, however. The figure of 0.002 seconds per day per century is an average and it can, and does, change. For example, you might recall that the Fukushima earthquake in 2011 resulted from displacements of portions of the Earth’s crust that actually speeded up the Earth’s rotation, shortening the day by 1.6 millionth of a second! While that is not much, keep in mind that such changes are cumulative, too. Other short term and unpredictable changes can be caused by a variety of events, ranging from slight changes in the distribution of mass in the Earth’s molten outer core, to movement of large masses of ice near the poles, and even density and angular momentum variations in the Earth’s atmosphere.
The bottom line is that the actual variation day to day is not always plus 2 milliseconds. According to a U.S. Naval Observatory document, between 1973 to 2008, it has ranged from a plus 4 milliseconds to a minus 1 millisecond. Over time, that could necessitate a negative leap second, signifying an increase in the Earth’s rotation speed, but since the concept was introduced in 1973, this has never been done.
This all may seem pretty esoteric and unimportant, but not to the telecommunications industry, which is where the ITU comes in. Telecommunications relies on precise timing, and the addition of a leap second forces many systems to be turned off for a second every year of two. To get all such systems in a global industry cycled on and off in sync can be a major headache. Consider also that the global positioning system (GPS) does not use the leap second system, which causes further confusion. Many in the industry feel that the periodic addition of a “leap second” to keep the to measurements in step is cumbersome and wasteful.
Although dropping the idea of a leap second would be a convenience for telecommunication and other industries, in the long (very long) run, it would cause clocks to get out of synch with the Sun, eventually causing 12 p.m. (noon) to occur in the middle of the night, for example. But at the current rate of change in Earth’s rotation rate, it would take about 5,000 years to amass just a one-hour difference between the Earth’s actual rotation rate and the atomic clock.
For now, the issue will continue to be debated, because the ITU has put off a decision until 2015. But, as mentioned above, a leap second will be added this year on June 30, 2012.
But how, you may ask, do we even measure such small changes in the Earth’s rotation? Historically, astronomers (such as those at Britain’s famed Royal Greenwich Observatory near London) have used a telescope to watch a star pass through their eyepiece, crossing an imaginary line called the meridian. Then they time how long it takes for the Earth to bring that around star back around to cross the meridian again. This is highly accurate for everyday purposes, but for scientific use it is limited in accuracy because of the wavelengths used and the murkiness of the atmosphere. A much more accurate method is to use two or more radio telescopes separated by thousands of miles, in a technique called Very Long Baseline Interferometry. By carefully combining the data from each of the telescopes, astronomers effectively have a telescope thousands of miles in size, which provides much greater resolution (detecting fine detail) and measurement of position. This allows them to determine the planet’s rotation rate to an accuracy of less than a thousandth of a second. They do not observe stars, however, but very distant objects called quasars.
Bottom line: 2012 is a leap year, and it will also have a leap second. The next leap second will be added to the clock on June 30, 2012. Leap seconds have been added every so often since 1972. The International Telecommunications Union (ITU), a U.N. body that governs some global issues related to time, has considered abolishing the practice of inserting a leap second into official time-keeping. But in late January 2012, the ITU decided to defer a proposal to dump the leap second until their 2015 meeting.