Sidereal Time Calculator
Work out sidereal time instantly with clear inputs, formula shown and shareable results.
About Sidereal Time Calculator
Sidereal time measures Earth's rotation against the stars rather than the Sun, so a sidereal day is 23h 56m 4s - about four minutes short. Local sidereal time equals the right ascension currently on the meridian, which is exactly what an observer needs to know which objects are highest.
Formulas
Greenwich sidereal time
GST = 18.697374558 + 24.06570982441908 x days since J2000
Local sidereal time
LST = GST + longitude / 15
Worked example
With the default values below, Sidereal Time Calculator returns Local Sidereal Time of 4.6710. Change any input above and every figure here is recalculated in your browser.
Inputs used
- Date
- 2026-01-01
- Universal timeaccepts 0–23.999 h
- 22 h
- Longitudeaccepts -180–180 deg
- -1.5 deg
Results
- Local Sidereal Time
- 4.6710 h
- Local Sidereal Time As hh:mm
- 04:40
- Greenwich Sidereal Time
- 4.7710 h
- Length Of A Sidereal Day
- 23.93447 h
Step by step
- 1Values used
- 2Greenwich sidereal time
- 3Local sidereal time
- 4Local Sidereal Time= 4.6710 h
- 5Local Sidereal Time As hh:mm= 04:40
- 6Greenwich Sidereal Time= 4.7710 h
- 7Length Of A Sidereal Day= 23.93447 h
Assumptions and limits
- The result is derived only from the 3 inputs listed above. Anything not among them is not part of the calculation.
- In particular, this calculator does not take inflation, tax, fees or charges or compounding frequency into account.
- Figures are rounded for display to 5 decimal places, so totals built from several rounded parts can differ slightly from the unrounded arithmetic.
How these calculators are built and tested is described on the Methodology page. If a figure looks wrong, please report it.
Frequently Asked Questions
Why is the sidereal day shorter?
Because Earth also advances along its orbit, so it must turn slightly more than 360 degrees to face the Sun again - about four extra minutes.
What is sidereal time used for?
Pointing telescopes. An object culminates when the local sidereal time equals its right ascension.
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