Instant · Precise · Universal
28 units available
6 categories total
To convert seconds to minutes: divide by 60. To convert to hours: divide by 3,600. To milliseconds: multiply by 1,000.
1 s = 1,000 ms = 10⁶ µs = 10⁹ ns. There are 60 seconds in a minute and 86,400 in a day.
For example, 1 Second (s) = 0.00001160576284 Day (Sidereal) (d (Sid)).
| Second (s) | Day (Sidereal) (d (Sid)) |
|---|---|
| 0.1 | 0.000001160576284 |
| 0.5 | 0.000005802881422 |
| 1 | 0.00001160576284 |
| 2 | 0.00002321152569 |
| 5 | 0.00005802881422 |
| 10 | 0.0001160576284 |
| 25 | 0.0002901440711 |
| 50 | 0.0005802881422 |
| 100 | 0.001160576284 |
| 500 | 0.005802881422 |
| 1000 | 0.01160576284 |
The second is the SI base unit of time, defined by the fixed value of the cesium-133 hyperfine transition frequency: exactly 9,192,631,770 cycles.
1 s = 1,000 ms = 10⁶ µs = 10⁹ ns. There are 60 seconds in a minute and 86,400 in a day.
To convert seconds to minutes: divide by 60. To convert to hours: divide by 3,600. To milliseconds: multiply by 1,000.
All timekeeping — clocks, timers, stopwatches, cooking, traffic lights, music tempo (BPM), and heartbeat monitoring.
Cesium atomic clocks are accurate to about 1 second in 300 million years. The 2019 SI redefinition preserved the second's cesium-based definition.
Using 'sec' instead of 's' in scientific writing. Also, assuming all seconds are exactly equal — leap seconds exist to correct for Earth's slowing rotation.
A heartbeat lasts about 0.8 seconds. Counting 'one Mississippi' is a classic way to estimate one second.
The sidereal day is the time for Earth to rotate once relative to distant stars — approximately 23 hours, 56 minutes, and 4 seconds (86,164.0905 seconds).
1 sidereal day ≈ 23 h 56 min 4.09 s = 86,164.09 s. About 3 min 56 s shorter than a solar day.
To convert sidereal days to solar days: multiply by 0.99727. To hours: multiply by 23.9345.
Telescope pointing and tracking, satellite ground track calculations, and astronomical observation scheduling.
Because of the ~4-minute difference, the night sky shifts gradually — the same star appears at the same position about 4 minutes earlier each night.
Equating sidereal day with solar day. The ~4-minute difference accumulates — after 6 months, sidereal noon is at solar midnight.
Imagine Earth spinning AND orbiting: after one full spin (sidereal day), Earth has moved in its orbit, so the Sun hasn't quite returned to the same position — that takes ~4 more minutes.



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