Instant · Precise · Universal
28 units available
6 categories total
To convert ms to seconds: divide by 1,000. To convert seconds to ms: multiply by 1,000.
1 ms = 0.001 s = 1,000 µs = 10⁶ ns. There are 1,000 milliseconds in one second.
For example, 1 Millisecond (ms) = 1.157407e-8 Day (d).
| Millisecond (ms) | Day (d) |
|---|---|
| 0.1 | 1.157407e-9 |
| 0.5 | 5.787037e-9 |
| 1 | 1.157407e-8 |
| 2 | 2.314815e-8 |
| 5 | 5.787037e-8 |
| 10 | 1.157407e-7 |
| 25 | 2.893519e-7 |
| 50 | 5.787037e-7 |
| 100 | 0.000001157407407 |
| 500 | 0.000005787037037 |
| 1000 | 0.00001157407407 |
The millisecond is a unit of time equal to 10⁻³ seconds — one thousandth of a second.
1 ms = 0.001 s = 1,000 µs = 10⁶ ns. There are 1,000 milliseconds in one second.
To convert ms to seconds: divide by 1,000. To convert seconds to ms: multiply by 1,000.
Web page load times, video game frame timing (16.67 ms = 60 fps), network ping times, and heartbeat intervals (~800 ms).
Human reaction time to visual stimuli is about 250 ms. A housefly's wing beats once every 4 ms. A humming bird's wing: ~12 ms per beat.
Confusing ms (milliseconds) with Mb/s (megabits per second). In networking, ms measures latency while Mb/s measures throughput.
Your eye blink = ~300 ms. A 60 fps game = 16.67 ms per frame. These are great millisecond benchmarks.
The day is a unit of time equal to 24 hours, or 86,400 seconds, representing one full rotation of the Earth on its axis.
1 d = 24 h = 1,440 min = 86,400 s. A mean solar day is ~86,400.002 s due to Earth's slowing rotation.
To convert days to hours: multiply by 24. To convert days to seconds: multiply by 86,400.
Calendar systems, hospital stays, travel itineraries, project deadlines, and food expiration dates.
Earth's day was only about 6 hours long 4.5 billion years ago. It's gradually getting longer — days grow about 2.3 ms per century.
Assuming all days are exactly 86,400 s — some days have leap seconds (86,401 s). Also, confusing calendar days with 24-hour periods.
A solar day (noon to noon) differs slightly from a sidereal day (star to star) by about 4 minutes, due to Earth's orbital motion.



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