Convert degrees to arc-seconds, arc-minutes, radians, milliradians, and gradians with ground distance equivalents and resolution reference.
The degrees to seconds converter transforms angular measurements from degrees into arc-seconds and related angle units such as arc-minutes, radians, milliradians, and gradians. Arc-seconds are the smallest part of the familiar DMS angle format and are useful whenever a decimal degree is not precise enough. A value that looks tiny in degrees can still matter when you are aligning equipment, comparing coordinates, or reading a high-precision survey note.
One degree equals exactly 3,600 arc-seconds. That makes arc-seconds a natural unit for astronomy, geodesy, surveying, map projections, and precision alignment work where a tiny angular change still matters in practice. The calculator keeps the alternate angular formats visible so you can move between fields that prefer radians, mrad, or DMS-style notation without redoing the math.
The converter also shows approximate ground-distance meaning at the equator, which helps connect an abstract angle unit to a real-world scale when you are working with coordinates or pointing accuracy. That side reference is especially useful when you want to sanity-check whether a small angular change would matter on the ground.
It is useful when a coordinate, telescope setting, or surveying value needs more precision than degrees alone provide. Seeing arc-seconds, radians, and distance equivalents together makes it easier to avoid unit mix-ups and compare one value across several common engineering formats, especially when the result has to be copied into another tool or report.
Arc-Seconds = Degrees × 3600. Arc-Minutes = Degrees × 60. Radians = Degrees × π / 180. Milliradians = Radians × 1000. Gradians = Degrees × 10/9.
Result: 1° = 3,600 arc-seconds = 60 arc-minutes = 0.017453 radians
One degree equals 3,600 arc-seconds. At the equator, this corresponds to approximately 111.32 km of ground distance.
Arc-seconds are a standard way to describe the apparent size or separation of objects in the sky. Telescope resolution, atmospheric seeing, and stellar parallax are all commonly expressed in arc-seconds or smaller units such as milliarcseconds.
Coordinate systems are often displayed in decimal degrees, but high-precision location work still maps cleanly into degrees, arc-minutes, and arc-seconds. At that scale, even a small fraction of an arc-second can correspond to noticeable distance on the ground, which is why the unit remains useful in surveying and GIS workflows.
Radians and milliradians are often preferred in engineering calculations, while arc-seconds are easier to interpret in observational and geospatial contexts. Converting between them helps when formulas, software, and field instruments do not use the same angular convention.
There are exactly 3,600 arc-seconds in one degree because each degree contains 60 arc-minutes and each arc-minute contains 60 arc-seconds. That fixed ratio is what makes the conversion straightforward.
At the equator, one arc-second of latitude equals approximately 30.87 meters, or 101.3 feet. The value changes for longitude as you move toward the poles because the circles of latitude get smaller.
A milliarcsecond, or mas, is 0.001 arc-seconds. The unit is used when even an arc-second is too coarse, such as in very precise astronomy measurements.
Arc-seconds measure angles, where one arc-second is 1/3600 of a degree. Time seconds measure duration, where one second is 1/60 of a minute, so the same word refers to different physical quantities.
A parsec is the distance at which one astronomical unit subtends one arc-second. It equals about 3.26 light-years and remains a standard unit for stellar distances.
Total stations and theodolites in surveying, CCD cameras in astronomy, and inertial navigation systems all measure in arc-seconds or finer. Those instruments need the extra precision because a fraction of a degree can matter a lot in practice.