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) = 8783.984181 Hour (Sidereal) (h (Sid)).
| Year (365 days) (yr) | Hour (Sidereal) (h (Sid)) |
|---|---|
| 0.1 | 878.3984181 |
| 0.5 | 4391.99209 |
| 1 | 8783.984181 |
| 2 | 17567.96836 |
| 5 | 43919.9209 |
| 10 | 87839.84181 |
| 25 | 219599.6045 |
| 50 | 439199.209 |
| 100 | 878398.4181 |
| 500 | 4391992.09 |
| 1000 | 8783984.181 |
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 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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