Whyarium Keeping Time
Shadow and Sun · from 1500 BC

Sundial

The oldest clock in the world has no moving parts at all. It is the Earth that moves; the shadow simply writes it down.

01 · A shadow for a hand

A stick, the Sun and patience

Egyptian scribes set a bar with a crosspiece on the ground and counted how many marks its shadow crossed. They split the day into twelve parts, so a summer "hour" was longer than a winter one.

Move the pointer over the drawing on the right: the Sun will travel across the sky and the gnomon's shadow across the dial.

02 · The gnomon

Tilted by the latitude

The triangle on the dial is called the gnomon. Its sloping edge rises above the horizon by exactly the latitude of the place, 38.97° for Gandia, and points at the Pole Star.

That makes the edge parallel to the Earth's axis. The Sun goes round that axis once a day, so the edge's shadow turns evenly at any time of year.

03 · Hour lines

Why the spacing is uneven

The Sun crosses the sky at exactly 15° an hour, but a horizontal dial catches the shadow at a slant. The lines crowd together around noon and spread apart toward morning and evening.

angle = arctan(sin φ · tan 15°t)

That is why you can't move a sundial to another town: at a different latitude it would tell the wrong time.

04 · Summer

A long day, a short shadow

In June the Sun climbs to 74.5° over Gandia. The shadow is short and the day lasts nearly 15 hours, so the dial needs lines from five in the morning to seven in the evening.

05 · Winter

The same hour, a different shadow

In December the Sun never rises above 27.6°. The shadow is longer and the day shorter, but the gnomon's edge still lands on the same hour line. That is the whole point of the tilt.

06 · Solar time and clock time

Why noon comes at two

Gandia sits almost on the Greenwich meridian, yet since 1940 Spain has kept Central European Time. Add an hour for summer time and solar noon arrives at about 14:00 by the clock.

There is a second correction too, the equation of time: the Earth's orbit is an ellipse, so solar days are sometimes longer and sometimes shorter. The difference reaches 16 minutes.

38°58′ NVVIVIIVIIIIXXXIXIIIIIIIIIVVVIVII
Gnomon: its sloping edge is parallel to the Earth's axisDial with hour lines laid out for latitude 38.97°The hour lines fan out unevenly: a line's angle from noon is arctan(sin 38.97° · tan 15°·t). That is why a sundial only tells the right time at its own latitude.