ES-02
Solar, apparent and mean solar day
Learning outcomes & permitted supports
- Explain why a solar day depends on Earth's rotation plus orbital advance.
- Distinguish the apparent and mean Sun, LAT and LMT, and use the equation of time with correct sign.
- Predict meridian-passage timing and convert it through LMT → GMT → ZT.
Supports in this lab: live physical model, engine readouts, EoT curve. No almanac needed; all values computed and validated.
The physical system
Two suns, two clocks
Engine readout (lon 0°)
| Equation of time | −4m 21s |
|---|---|
| Sun transits at (LMT) | 12:04:21 |
| Sun declination | 13° 42.9′ N |
| Sun GHA | 268° 54.7′ |
| Semidiameter | 15.8′ |
| Earth–Sun distance | 1.0127 AU |