Case 1
- Refractive index of the first medium n₁
- 1
- Refractive index of the second medium n₂
- 1.33
- Angle of incidence θ₁
- 30°
22.0824°
Open with these valuesChange any value to update the result.
22.0824°
Angle of refraction: 22.0824 °Your current valid inputs, with one value varied across the range.
Held fixed: Refractive index of the first medium n₁ 1.000, Refractive index of the second medium n₂ 1.330.
| Angle of incidence θ₁ (°) | Angle of refraction (°) |
|---|---|
| 20.00 | 14.9015 |
| 30.00Your value | 22.0824 |
| 40.00 | 28.9011 |
Snell's law says n₁ × sin θ₁ = n₂ × sin θ₂, so the refraction angle is arcsin(n₁ × sin θ₁ ÷ n₂). Both angles are measured from the normal, in degrees. Past the critical angle no refracted ray exists and the calculator reads 90°, the grazing limit where total internal reflection sets in.
22.0824°
Open with these values41.6823°
Open with these values49.2682°
Open with these valuesθ₂ = arcsin(n₁ × sin θ₁ ÷ n₂)
| n₁, n₂, angle of incidence | Transition | Angle of refraction |
|---|---|---|
| 1, 1.33, 30 | Air into water, bends toward the normal | 22.0824 |
| 1, 1.5, 45 | Air into glass | 28.1255 |
| 1.33, 1, 30 | Water into air, bends away from the normal | 41.6823 |
| 1, 1, 40 | No change of medium, no bending | 40 |
| 1.33, 1.52, 60 | Water into glass | 49.2682 |
| 1.52, 1, 60 | Glass into air, past the critical angle | 90 |
Take the sine of the angle of incidence, multiply by the first index, divide by the second, then take the inverse sine. Light going from air with n₁ = 1 into water with n₂ = 1.33 at 30° gives 22.0824°.
The normal is the imaginary line perpendicular to the surface, and Snell's law is written against it. That keeps the relationship consistent and makes a ray arriving head on, at 0° from the normal, pass through without bending.
Into a denser medium with a higher index it bends toward the normal, so the refraction angle is smaller than the incidence angle. Into a less dense medium it bends away from the normal and the angle grows.
It marks total internal reflection. When light leaves a denser medium at a steep angle, the ratio n₁ × sin θ₁ ÷ n₂ passes 1 and no refracted ray exists any more — all the light reflects back, which is what keeps a signal inside an optical fibre. This calculator reports 90°, the grazing limit, rather than nothing at all.
It says how much a medium slows light compared with a vacuum, which is exactly 1. Air is about 1.00, water 1.33, ordinary glass roughly 1.50 and diamond 2.42.
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