If the length of Earth's day is determined using the Sun as reference, that day is called a solar day, and is 24 hours in length.1 If the length of a Earth's day is determined using the stars as a reference, however, that day is called a sidereal day, and is 23 hours, 56 minutes and 4.09 seconds in length. The solar day is longer, since Earth advances along its orbit approximately one degree per day. This span of time is subject to change—sometimes without notice. For instance, the 11 March 2011 earthquake in Japan has shortened the length of the day by 1.6 microseconds, according to geophysicist Richard Gross. This is because a redistribution of Earth's mass has occurred due to slippage. In addition, the length of the day varies—speeding up and slowing down—as much as 1,000 microseconds throughout the year because of seasonal changes in the jet stream.