Degree to Second

The Babylonians used base-60 arithmetic and noticed the year was close to 360 days — convenient because 360 divides evenly by 2, 3, 4, 5, 6, 8, 9, 10, 12, 15, 18, 20, and more. That ridiculous number of factors makes slicing a circle into halves, thirds, quarters, fifths, sixths, and eighths all come out to whole numbers. A base-100 system would only divide cleanly by 2, 4, 5, 10, 20, 25, and 50 — far less flexible for geometry and land surveying.

Navigation requires quick mental arithmetic with headings, bearings, and wind corrections. "Turn right to heading 270" is instantly understood in a cockpit; "turn right to 4.712 radians" would get someone killed. Compass roses, runway numbers (which are headings divided by 10), and nautical charts all assume a 360° circle. The entire global aviation and maritime infrastructure — from VOR stations to AIS transponders — is calibrated in degrees.

The degree symbol is a small raised circle placed immediately after the number with no space (45°, not 45 °). On Windows, hold Alt and type 0176 on the numpad. On Mac, press Option+Shift+8. On phones, long-press the zero key. In HTML, use ° or °. A common mistake is using a superscript letter "o" or the ring-above diacritic — these look similar but are different Unicode characters and can break search or data parsing.

One degree equals 60 arcminutes, and one arcminute equals 60 arcseconds — so 1° = 3,600″. To convert DMS to decimal, divide minutes by 60 and seconds by 3,600, then add them to the degree value. For example, 40°26′46″N becomes 40 + 26/60 + 46/3600 = 40.4461°. Google Maps uses decimal degrees internally but lets you enter either format. At the equator, one degree of longitude spans about 111 km.

Yes — the French Revolutionary government introduced the gradian (grad), dividing a circle into 400 parts to match the metric system. A right angle became exactly 100 grad. They also tried decimal time (10-hour days) and a decimal calendar. The time and calendar experiments died within a few years, but gradians survived and are still used in French and German surveying. Every scientific calculator has a GRAD mode because of this 230-year-old French experiment.

One arcsecond of latitude corresponds to roughly 31 meters (about 101 feet) on the ground. This is why high-precision GPS coordinates are quoted to fractions of arcseconds — a shift of just 0.01″ means about 30 cm. Longitude arcseconds cover less ground as you move toward the poles because the meridians converge; at 45° latitude, one arcsecond of longitude spans about 22 meters.

Stellar parallax is the tiny apparent shift of a nearby star against distant background stars as Earth orbits the Sun. Even the closest star, Proxima Centauri, shifts by only 0.768 arcseconds over six months — far too small for the naked eye. The parsec (parallax-arcsecond) is defined as the distance at which a star would show exactly 1″ of parallax. No star is close enough to reach that threshold, which gives you a sense of how mind-bogglingly far away even our nearest neighbors are.

Hubble resolves details down to about 0.05 arcseconds — roughly the angular size of a coin seen from 80 km away. At that resolution it can distinguish individual stars in nearby galaxies, spot the discs of Pluto and large asteroids, and detect gravitational lensing arcs. Ground-based telescopes are blurred to about 0.5–1″ by atmospheric turbulence unless they use adaptive optics, which is why space telescopes remain essential for sharp imaging.

Arcseconds per pixel is the standard metric for imaging sensors in astronomy because it directly links detector geometry to sky coverage. A telescope with 0.3″/pixel resolution can separate objects that close together on the sky. Photographers encounter this too — the resolving power of any long telephoto lens is ultimately limited by atmospheric seeing (typically 1–2″), which is why even a perfect 600 mm lens produces soft images of distant objects on a hazy day.

The average human eye resolves about 60 arcseconds (1 arcminute) under good conditions, though some people with exceptional vision reach 30″. This is why the standard eye test chart (Snellen chart) defines 20/20 vision as the ability to resolve details that subtend 1 arcminute. For comparison, Jupiter at its brightest subtends about 50″, just below that threshold — which is why it looks like a bright dot to the naked eye, not a disc.