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28 units available
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To convert ns to seconds: multiply by 10⁻⁹. To convert ns to microseconds: divide by 1,000.
1 ns = 10⁻⁹ s = 1,000 ps = 0.001 µs. Light travels about 30 cm (1 foot) in one nanosecond.
For example, 1 Nanosecond (ns) = 1.160576e-14 Day (Sidereal) (d (Sid)).
| Nanosecond (ns) | Day (Sidereal) (d (Sid)) |
|---|---|
| 0.1 | 1.160576e-15 |
| 0.5 | 5.802881e-15 |
| 1 | 1.160576e-14 |
| 2 | 2.321153e-14 |
| 5 | 5.802881e-14 |
| 10 | 1.160576e-13 |
| 25 | 2.901441e-13 |
| 50 | 5.802881e-13 |
| 100 | 1.160576e-12 |
| 500 | 5.802881e-12 |
| 1000 | 1.160576e-11 |
The nanosecond is a unit of time equal to 10⁻⁹ seconds — one billionth of a second.
1 ns = 10⁻⁹ s = 1,000 ps = 0.001 µs. Light travels about 30 cm (1 foot) in one nanosecond.
To convert ns to seconds: multiply by 10⁻⁹. To convert ns to microseconds: divide by 1,000.
CPU clock cycles (a 3 GHz processor has ~0.33 ns per cycle), DDR memory timing, Ethernet packet gaps, and GPS signal timing.
Grace Hopper handed out 30 cm wires to explain nanoseconds: 'This is one nanosecond' — the distance light travels in that time.
Confusing nanoseconds with milliseconds — they differ by a factor of 1,000,000. In computing, ns and ms are very different.
Grace Hopper's wire trick: hold a 30 cm ruler — light crosses it in 1 ns. This makes the abstract concept tangible.
The sidereal day is the time for Earth to rotate once relative to distant stars — approximately 23 hours, 56 minutes, and 4 seconds (86,164.0905 seconds).
1 sidereal day ≈ 23 h 56 min 4.09 s = 86,164.09 s. About 3 min 56 s shorter than a solar day.
To convert sidereal days to solar days: multiply by 0.99727. To hours: multiply by 23.9345.
Telescope pointing and tracking, satellite ground track calculations, and astronomical observation scheduling.
Because of the ~4-minute difference, the night sky shifts gradually — the same star appears at the same position about 4 minutes earlier each night.
Equating sidereal day with solar day. The ~4-minute difference accumulates — after 6 months, sidereal noon is at solar midnight.
Imagine Earth spinning AND orbiting: after one full spin (sidereal day), Earth has moved in its orbit, so the Sun hasn't quite returned to the same position — that takes ~4 more minutes.



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