Free online angle converter. Convert degrees to radians, gradians, arcminutes, arcseconds, and turns instantly — for trigonometry, engineering, CNC machining, and navigation. Accurate, instant, no sign-up.
degrees • radians • gradians • arcmin • arcsec
Convert degrees to radians for sin, cos, tan in calculus, where radians are required for derivatives and series.
JavaScript, Python, and C use radians in Math.sin(). CNC and CAD often use degrees. Convert to avoid errors.
Telescopes and star positions use arcminutes and arcseconds — 1 degree = 60 arcmin = 3,600 arcsec.
Angles can be measured in several units, and the most common conversion is between degrees and radians. A full circle is 360 degrees, 2π radians (approximately 6.2832), 400 gradians, or 1 turn. The key relationship: 1 radian = 180/π ≈ 57.2958 degrees, and 1 degree = π/180 ≈ 0.01745 radians. Degrees are intuitive for everyday use (a right angle is 90°), but radians are the natural unit in higher mathematics because they make calculus formulas clean — the derivative of sin(x) is cos(x) only when x is in radians.
Common angles convert to memorable radian values: 30° = π/6, 45° = π/4, 60° = π/3, 90° = π/2, 180° = π, and 360° = 2π. Gradians (also called gons) divide a right angle into 100 parts and are used in surveying and some European engineering. For precise work in astronomy and navigation, degrees are subdivided into arcminutes (1° = 60′) and arcseconds (1′ = 60″), so 1 degree = 3,600 arcseconds. Milliradians (mrad) are used in ballistics and optics for fine angular adjustments.
30° = 0.5236 rad = π/6. 45° = 0.7854 rad = π/4. 60° = 1.0472 rad = π/3. 90° = 1.5708 rad = π/2. 180° = 3.1416 rad = π.
Radians are dimensionless (arc length ÷ radius), making trig derivatives and Taylor series work cleanly. d/dx sin(x) = cos(x) requires radians. This is why programming Math functions use radians.
1 gradian = 1/400 of a circle = 0.9°. A right angle = 100 gon. Used in continental European surveying and some calculators (GRAD mode).
1° = 60 arcmin = 3,600 arcsec. The full Moon spans ~30 arcmin. Hubble resolves ~0.05 arcsec. Star coordinates use arcsec precision.