Sextant to Revolution

A sextant uses two mirrors to superimpose the image of a celestial body onto the horizon. The navigator looks through the eyepiece and sees the horizon directly through a half-silvered mirror, while a second mirror on a movable arm reflects the Sun or star down into the same field of view. You swing the arm until the star appears to sit exactly on the horizon, then read the angle off the graduated arc. The double-reflection design means the arc only needs to span 60° (one sextant) to measure angles up to 120°.

The name refers to the arc of the instrument, not its measurement range. A sextant's arc is one-sixth of a circle (60°), but thanks to the double-reflection principle — where the angle of reflection doubles the arc angle — it can actually measure angles up to 120°. Similarly, an octant (one-eighth of a circle, 45° arc) measures up to 90°. The naming convention describes the physical shape of the tool, not its capability.

Yes, and navies worldwide still require it. The US Naval Academy reintroduced mandatory celestial navigation in 2015 after a decade-long hiatus, citing concerns about GPS vulnerability to jamming, spoofing, and satellite failure. A skilled celestial navigator with a sextant, an accurate clock, and a nautical almanac can determine position to within about 1–2 nautical miles — good enough to make port safely. Several solo round-the-world sailors carry sextants as backup specifically because they have no electronics to fail.

The sextant itself couldn't solve longitude — that required an accurate clock (John Harrison's marine chronometer, completed in 1761). But the sextant was the other half of the solution. A navigator used it to measure the Sun's altitude at local noon to find the exact time of solar noon at their position. Comparing this to Greenwich time on the chronometer gave the time difference, and since Earth rotates 15° per hour, that time difference directly yielded longitude. Sextant + chronometer = position anywhere on Earth.

Sixty degrees is the interior angle of an equilateral triangle — the simplest regular polygon after the square. Honeycomb cells are hexagons (six 120° angles, each the supplement of 60°) because hexagonal packing is the most efficient way to tile a plane. Carbon atoms in graphene and diamond form 60° and 109.5° angles respectively. The 60° angle appears everywhere in nature because it's the geometric consequence of close-packing equal-sized spheres or circles.

RPM (revolutions per minute) counts how many full 360° rotations an object completes each minute. It dominates because it maps directly to what you can see and feel — a wheel either goes around or it doesn't. Degrees per second would produce absurdly large numbers: an engine at 3,000 RPM is spinning at 18,000 degrees per second, which is meaningless to a mechanic. RPM is intuitive, and that's why every tachometer, drill spec sheet, and turntable rating uses it.

Earth completes one revolution on its axis every 23 hours 56 minutes (a sidereal day). At the equator, that's a surface speed of about 1,670 km/h. If it suddenly stopped, everything not bolted to bedrock would continue moving eastward at that speed — winds would scour the surface, oceans would slosh into continental-scale tsunamis, and the atmosphere would take years to settle. Thankfully, Earth is decelerating by only about 2.3 milliseconds per century due to tidal friction with the Moon.

A vinyl record plays at 33⅓ or 45 RPM. A washing machine spin cycle hits 1,000–1,400 RPM. A car engine idles at 600–900 RPM and redlines at 6,000–9,000 RPM (F1 cars reached 20,000 RPM before regulations capped them). A dentist's drill spins at 250,000–400,000 RPM. Hard drive platters rotate at 5,400 or 7,200 RPM. A jet engine's high-pressure turbine reaches 10,000–15,000 RPM. The fastest man-made spinning object — a nanorotor in a lab — reached 300 billion RPM in 2018.

In strict usage, "revolution" is orbital (Earth revolves around the Sun) while "rotation" is axial (Earth rotates on its axis). But colloquially the two words get swapped constantly, even by scientists. The key distinction: an orbit traces a path around an external point, while a spin is about an internal axis. The Moon is tidally locked, meaning its rotation period equals its revolution period — which is why we always see the same face.

Conservation of angular momentum. When a skater pulls their arms inward, they reduce their moment of inertia (the rotational equivalent of mass). Since angular momentum (L = Iω) must stay constant, decreasing I forces ω (angular velocity in revolutions per second) to increase. A skater can go from 2 revolutions per second with arms out to 5–7 revolutions per second with arms tucked. It's the same physics that makes neutron stars spin at hundreds of revolutions per second after a massive star collapses.