Year and Day Measurement

Calculation of Year, Day and Time

Sidereal Year

  • Sidereal year the duration taken for one revolution of the earth around the sun with distant star at infinity as datum reference
  • Time taken for one sidereal year is equal to 365 days and 6 hours

Tropical Year

  • Tropical year is duration taken for one revolution of the earth around the sun with sun as the datum reference
  • Duration of tropical year is 365 days, 5 hours, 48 minutes and 45 seconds

Calendar Year

  • Calendar year is made to keep whole number of days in a year to 365 days instead of 365 days, 5 hours, 48 minutes and 45 seconds
  • Leap years have 29 days in February to cater for ¼ day short every year
  • The adjustment to make a usable calendar year is done in three phases
  • Every fourth year is a leap year while Centuries are not leap years but Fourth centuries are leap years

Sidereal Day

  • Sidereal day is the time between two meridian transits of the earth with a distant star at infinity as datum
  • A day is the time taken for one rotation of earth around its axis using any celestial body for measurement
  • Sidereal day is not related to periods of daylight or darkness and is not usable in day-to-day life
  • Revolution of earth does not affect sidereal day since the Meridian transit referenced to infinity will remain constant

Apparent Solar Day

  • Apparent solar day is the time taken between successive meridian transits with the Real sun which is apparent to us as datum
  • Earth revolves as well as rotates anti-clockwise from north celestial pole requiring additional distance between two meridian transits
  • Observers’ meridian shift its position between two meridian transits making the apparent solar day longer than the sidereal day
  • Apparent solar day varies from day to day due to speeds of revolution which in turn varies depending on the distance from the sun
  • Therefore, Apparent solar day is also unusable for practical purposes

Mean Solar Day

  • Civil day or Mean Solar Day is the time taken between successive meridian transits with the mean sun as datum
  • Mean sun is an imaginary sun assumed to circle the earth every 24 hours
  • Mean solar day is obtained by dividing total length of a year by 365 ¼ days
  • Since 360 degrees of rotation will take 24 hours, 15 degrees of rotation will take 1 hour and 1 degree of rotation will take 4 minutes

Equation of Time

  • Equation of time is the time difference between mean and apparent time
  • Mean solar day is taken as the basis of measurement for mean time which is constant throughout the year
  • Apparent time depends on the visible sun or the real sun which varies with distance between earth and sun
  • Equation of Time differs with position of earth in the orbit
  • Mean time of 12 noon does not mean that the real sun is overhead meridian
  • Maximum difference between mean and apparent time is 16 minutes in mid-November which means that the real sun is 16 minutes behind the meridian transit
  • Similarly, the second maximum is 14 minutes in mid-February which means that the real sun is 14 minutes ahead of meridian transit

Best of luck