Instant · Precise · Universal
28 units available
6 categories total
To convert sidereal years to days: multiply by 365.25636. To tropical years: multiply by 365.25636/365.24219.
1 sidereal year ≈ 365.25636 days ≈ 365 d 6 h 9 min 10 s. About 20 min 24 s longer than the tropical year.
For example, 1 Year (Sidereal) (yr (Sid)) = 31644552.05 Second (Sidereal) (s (Sid)).
| Year (Sidereal) (yr (Sid)) | Second (Sidereal) (s (Sid)) |
|---|---|
| 0.1 | 3164455.205 |
| 0.5 | 15822276.02 |
| 1 | 31644552.05 |
| 2 | 63289104.1 |
| 5 | 158222760.2 |
| 10 | 316445520.5 |
| 25 | 791113801.2 |
| 50 | 1582227602 |
| 100 | 3164455205 |
| 500 | 15822276020 |
| 1000 | 31644552050 |
The sidereal year is the time for Earth to complete one orbit relative to the fixed stars — approximately 365.25636 days (31,558,149.7632 seconds).
1 sidereal year ≈ 365.25636 days ≈ 365 d 6 h 9 min 10 s. About 20 min 24 s longer than the tropical year.
To convert sidereal years to days: multiply by 365.25636. To tropical years: multiply by 365.25636/365.24219.
Tracking stellar positions, calculating satellite orbital decay, and determining long-term star catalog corrections.
The ~20-minute difference between sidereal and tropical years is caused by axial precession — Earth's axis traces a full circle every ~25,772 years.
Using sidereal year when tropical year is intended (or vice versa) in calendar calculations.
Think of it this way: the sidereal year measures Earth's orbit relative to stars. The tropical year measures relative to seasons. Precession makes them differ.
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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