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) = 0.0002785383112 Hour (Sidereal) (h (Sid)).
| Second (s) | Hour (Sidereal) (h (Sid)) |
|---|---|
| 0.1 | 0.00002785383112 |
| 0.5 | 0.0001392691556 |
| 1 | 0.0002785383112 |
| 2 | 0.0005570766223 |
| 5 | 0.001392691556 |
| 10 | 0.002785383112 |
| 25 | 0.006963457779 |
| 50 | 0.01392691556 |
| 100 | 0.02785383112 |
| 500 | 0.1392691556 |
| 1000 | 0.2785383112 |
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 hour is 1/24 of a sidereal day — approximately 3,590.17 seconds (59 minutes and 50.17 seconds in solar time).
1 sidereal hour = 3,590.17 solar seconds ≈ 59 min 50.17 s in solar time. 24 sidereal hours = 1 sidereal day.
To convert sidereal hours to solar seconds: multiply by 3,590.17. To solar hours: multiply by 0.99727.
Right ascension in celestial coordinates is measured in hours (0–24 h of sidereal time), directly using sidereal hours.
Right ascension is measured in hours: 1 h of RA = 15° of sky. The entire sky is 24 sidereal hours in rotation.
Treating sidereal hours as exactly 60 solar minutes. The ~10-second difference matters for precision tracking.
If you use a star-tracking telescope, it rotates once per sidereal day (23h 56m). Each sidereal hour, it covers 15° of sky.



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