Instant · Precise · Universal
28 units available
6 categories total
To convert days to hours: multiply by 24. To convert days to seconds: multiply by 86,400.
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.
For example, 1 Day (d) = 86636.55244 Second (Sidereal) (s (Sid)).
| Day (d) | Second (Sidereal) (s (Sid)) |
|---|---|
| 0.1 | 8663.655244 |
| 0.5 | 43318.27622 |
| 1 | 86636.55244 |
| 2 | 173273.1049 |
| 5 | 433182.7622 |
| 10 | 866365.5244 |
| 25 | 2165913.811 |
| 50 | 4331827.622 |
| 100 | 8663655.244 |
| 500 | 43318276.22 |
| 1000 | 86636552.44 |
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.
The sidereal second is 1/60 of a sidereal minute — approximately 0.99727 solar seconds.
1 sidereal second ≈ 0.99727 solar seconds. 86,400 sidereal seconds = 1 sidereal day.
To convert sidereal seconds to solar seconds: multiply by 0.99727. One solar second ≈ 1.00274 sidereal seconds.
Telescope tracking motors rotate at sidereal rate (1 revolution per sidereal day) to follow stars across the sky.
The difference between sidereal and solar seconds (2.73 ms) seems tiny, but over a day it adds up to the full ~236 s difference.
Assuming sidereal seconds equal solar seconds. The ~0.27% difference is critical in precision astronomy.
Multiply any sidereal time interval by 0.99727 to get the solar equivalent. This ratio stays constant at all time scales.



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