Instant · Precise · Universal
28 units available
6 categories total
To convert years to days: multiply by 365 (or 365.25 for average including leap years). To seconds: multiply by 31,536,000.
1 yr = 365 d = 8,760 h = 525,600 min = 31,536,000 s. A leap year has 366 days (31,622,400 s).
For example, 1 Year (365 days) (yr) = 31622341.64 Second (Sidereal) (s (Sid)).
| Year (365 days) (yr) | Second (Sidereal) (s (Sid)) |
|---|---|
| 0.1 | 3162234.164 |
| 0.5 | 15811170.82 |
| 1 | 31622341.64 |
| 2 | 63244683.28 |
| 5 | 158111708.2 |
| 10 | 316223416.4 |
| 25 | 790558541 |
| 50 | 1581117082 |
| 100 | 3162234164 |
| 500 | 15811170820 |
| 1000 | 31622341640 |
The common year is a unit of time equal to 365 days, or 31,536,000 seconds.
1 yr = 365 d = 8,760 h = 525,600 min = 31,536,000 s. A leap year has 366 days (31,622,400 s).
To convert years to days: multiply by 365 (or 365.25 for average including leap years). To seconds: multiply by 31,536,000.
Age calculation, financial year reporting, contract durations, academic years, and historical timeline reference.
The year 2000 was a leap year (divisible by 400), but 1900 was not (divisible by 100 but not 400). The Gregorian rule fixes the calendar's drift to 1 day per 3,236 years.
Assuming every 4th year is a leap year — century years must be divisible by 400 (so 1900 wasn't a leap year).
Leap year rule: divisible by 4 = leap, UNLESS divisible by 100, UNLESS also divisible by 400. So 2000 was, 1900 wasn't.
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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