Julian Date
& Sidereal Time Converter
High-precision astronomical timekeeping. Convert standard calendar dates to Julian Days and calculate Local Sidereal Time for telescope synchronization.
Julian Date (JD)
Modified Julian (MJD)
Greenwich Sidereal
Local Sidereal (LST)

The Astronomer’s Chronometer
In standard civil life, we measure time using the Gregorian calendar. However, for the study of celestial mechanics and the tracking of the moon phase today, more precise systems are required.
What is the Julian Date (JD)?
The Julian Day system was introduced in 1583. It is a simple, continuous count of days and fractions of days since noon on January 1, 4713 BC. Because it is a simple decimal number, it allows scientists to calculate the exact duration between two astronomical events—like two solar eclipses thousands of years apart—without worrying about month lengths or leap year corrections.
Modified Julian Date (MJD)
For modern computing, astronomers often use the Modified Julian Date. This is simply the Julian Date minus 2,400,000.5. It reduces the size of the numbers and aligns the day-change with midnight UTC rather than noon.
Technical Note: Our converter uses the J2000.0 epoch, the current standard reference frame for the positions of stars and planets.
Understanding Sidereal Time
Sidereal time is “star time.” While a solar day is 24 hours, a Sidereal Day is approximately 23 hours, 56 minutes, and 4 seconds. This is the time it takes for the Earth to complete one full rotation relative to the distant “fixed” stars. Local Sidereal Time (LST) is essential for anyone using an equatorial telescope mount; it tells you exactly which part of the celestial sphere is crossing your local meridian at this moment.
