Astronomical Sidereal Time Tracker: Local Sidereal Time Clock

Track Greenwich Mean Sidereal Time (GMST) and Local Sidereal Time (LST) with an artistic astronomical astrolabe watch face and real-time stellar drift simulator.

MERIDIAN URSA MAJOR CASSIOPEIA CYGNUS XXIV II IV VI VIII X XII XIV XVI XVIII XX XXII 12 3 6 9
Coordinated Universal Time (UTC) 00:00:00
Local Sidereal Time (LST) 00:00:00
Stellar-Solar Drift 0m 00s
Julian Date 0.0
Cosmic Chime Ticks
Astronomical Drift
Adjust your local Longitude to see Local Sidereal Time shift in real-time.
Toggle the speed multiplier to watch the standard solar hour hand and the sidereal star sphere drift.
Enable Cosmic Chimes to hear the difference between a standard tick and an astronomical hour crossing.
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Frequently Asked Questions

What is the difference between solar time and sidereal time?

Solar time is based on the Sun's position relative to the local meridian (takes 24 hours), whereas sidereal time is based on the Earth's rotation relative to distant background stars (takes 23 hours, 56 minutes, 4.09 seconds).

Why is a sidereal day shorter than a solar day?

As the Earth rotates on its axis, it also travels along its orbit around the Sun. To face the Sun again, the Earth has to rotate slightly more than 360 degrees, which adds about 3 minutes and 56 seconds to the day compared to a simple star-aligned rotation.

How does longitude affect local sidereal time?

Local Sidereal Time is calculated by adding the observer's longitude (converted to hours: 15 degrees per hour) to Greenwich Mean Sidereal Time (GMST). Every degree east adds 4 minutes to your local sidereal clock.

# What is Sidereal Time?

Sidereal time is a timekeeping system astronomers use to locate celestial objects. A sidereal day is approximately 23 hours, 56 minutes, and 4.09 seconds. It is the time it takes the Earth to make one complete rotation on its axis relative to the vernal equinox or the distant stars, rather than the Sun.

# Solar Day vs. Sidereal Day

A solar day measures the time between consecutive transits of the Sun across the local meridian. Because the Earth travels about 1/365th of its orbital path around the Sun each day, it must rotate slightly more than 360 degrees to realign with the Sun. A sidereal day is a true 360-degree rotation relative to the stars, making it 3 minutes and 56 seconds shorter.

# Why Astronomers and Watchmakers Care

For astronomers, a star is always at the same position in the sky at the same Sidereal Time. To track stars, telescope mounts must rotate exactly once per sidereal day. High-end watchmaking brands (like Patek Philippe, Vacheron Constantin, and IWC) create ultra-complicated astronomical watches featuring sidereal gear trains to track LST directly on the wrist.

# Stellar vs. Solar Drift Reference Table

Elapsed Days Sidereal Time Ahead By Degrees of Rotation Shift Stellar Constellation Drift
1 Day3m 56s0.986°Slight shift west
15 Days59m 0s14.79°Half a zodiac sign shift
30 Days1h 58m29.58°One full zodiac constellation shift
90 Days5h 54m88.74°One full season constellation shift
180 Days11h 48m177.48°Opposite constellations visible at midnight
365 Days24h 0m360.00°Complete cycle, star alignment reset

Calculated from J2000 Epoch

COMPUTATION
Local Sidereal Time is computed by converting UTC time to Julian Date (days since -4712), finding the Greenwich Mean Sidereal Time, and applying your longitude (15 degrees per hour). Our tool uses the high-precision IAU J2000 linear model for real-time tracking.

Bibliographic References