Sidereal Time Calculator (Local Sidereal Time)
Local and Greenwich sidereal time for any date, time and longitude — the right ascension crossing your meridian, for pointing a telescope.
Results
What this tool does
Sidereal time follows the stars instead of the Sun. Because the Earth also moves around the Sun, a sidereal day is about 3 min 56 s shorter than a solar day, so the stars rise four minutes earlier each night. Local sidereal time equals the right ascension of the stars on your meridian right now: a star with RA 5h 35m is highest in the sky when the LST reads 5:35. Enter the time in UTC, not local clock time; the formula is the one in Meeus's Astronomical Algorithms and is good to a fraction of a second.
Formula
GMST = 280.46061837° + 360.98564736629° × (JD − 2451545.0) + 0.000387933 T² − T³ ÷ 38 710 000 · LST = GMST + longitude (Meeus)
Variables
| Symbol | Meaning | Unit |
|---|---|---|
yr | Year | — |
mo | Month (1–12) | — |
dy | Day of the month | — |
hu | Time (UTC, decimal hours) | h |
lo | Longitude (east positive) | ° |
LH | Local sidereal time — hours | h |
LM | Local sidereal time — minutes | min |
LS | Local sidereal time — seconds | s |
LD | Local sidereal time in decimal hours | h |
GM | Greenwich mean sidereal time | h |
Worked example
- Year2026
- Month (1–12)10
- Day of the month10
- Time (UTC, decimal hours)21 h
- Longitude (east positive)-9.14 °
- Local sidereal time — hours21 h
- Local sidereal time — minutes41 min
- Local sidereal time — seconds21 s
- Local sidereal time in decimal hours21.68906 h
- Greenwich mean sidereal time22.29839 h
Limitations
- The default values are typical reference figures, not measurements of your situation. Replace them with your own data whenever you have it.
- The calculation runs at full precision and only the display is rounded. If you copy an intermediate value and retype it, small differences can appear.