ASTROPHOTOGRAPHY · STAR TRAILS

Star Trails: Rotation, Stacking and Gaps

See how total shooting time becomes angular trail length, and how frame gaps reduce stacking continuity.

Interactive trail simulator

Sky rotation—
Frames—
Capture duty—

Physical fact

The sky turns about 15° per sidereal hour because Earth rotates. Trail geometry is circular around the celestial pole; the pole altitude approximately matches your latitude.

Starting point

Try 30–90 minutes total, 15–30 s frames, and the smallest reliable interval gap. Check highlights and battery before committing to a long sequence.

Field check

Confirm the pole direction, foreground focus, intervalometer cadence and whether long-exposure noise reduction would create unwanted gaps.

Try it

Move latitude from 15° to 60° and watch the pole move. Then increase total time from 20 to 120 minutes and compare arc length.

Related

Why star trails have their shape

Earth rotation

The sky appears to rotate about 15° per sidereal hour because Earth rotates. Trails therefore curve around the celestial pole rather than moving as identical straight lines everywhere.

Declination

A star near the pole traces a small circle; one near the celestial equator covers a much larger angular path. Image trail length also depends on focal length and projection.

Stacking

Many shorter frames let you reject bad frames and protect highlights, but gaps between frames become breaks in the trail. Interval overhead matters almost as much as exposure duration.

Field workflow

Choose a pole-centered or directional composition first, estimate the total arc you want, then select frame length and interval. Avoid long-exposure processing that creates large gaps when continuous trails are the goal.