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  1. Home
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  4. /Spacetime Interval Calculator

Spacetime Interval Calculator

Last updated: March 18, 2026

Calculator

Results

Spacetime Interval (s²)

—

m²

|s|

—

m

Proper Time (τ)

0.0000e+0

s

Proper Distance (σ)

0.0000e+0

m

Interval Type

—

Results

Spacetime Interval (s²)

—

m²

|s|

—

m

Proper Time (τ)

0.0000e+0

s

Proper Distance (σ)

0.0000e+0

m

Interval Type

—

The Spacetime Interval Calculator computes the Lorentz-invariant spacetime interval between two events in special relativity. The interval is defined as:

$$s^2 = c^2 \Delta t^2 - \Delta x^2 - \Delta y^2 - \Delta z^2$$

Unlike spatial distances or time intervals alone — which change depending on the observer's reference frame — the spacetime interval $$s^2$$ is the same for all inertial observers. This invariance makes it one of the most fundamental quantities in relativity, encoding the causal structure of spacetime itself.

The sign of $$s^2$$ classifies the relationship between two events: timelike ($$s^2 > 0$$) means a massive particle could travel between them; spacelike ($$s^2 < 0$$) means no signal can connect them; lightlike ($$s^2 = 0$$) means only light can bridge the gap. This classification is absolute — all observers agree on it.

Visual Analysis

How It Works

In Minkowski spacetime, the geometry is described by the metric:

$$ds^2 = c^2\,dt^2 - dx^2 - dy^2 - dz^2$$

This is the flat-spacetime analog of the Pythagorean theorem, but with a crucial sign difference: the time component enters with a positive sign and spatial components with negative signs (using the +−−− convention). For finite separations between two events:

$$s^2 = c^2(\Delta t)^2 - (\Delta x)^2 - (\Delta y)^2 - (\Delta z)^2$$

The three interval types have distinct physical meanings:

  • Timelike ($$s^2 > 0$$): The time separation dominates. There exists a reference frame where both events occur at the same location but at different times. The proper time between them is $$\tau = \sqrt{s^2}/c = \sqrt{\Delta t^2 - \Delta r^2/c^2}$$, which is the time measured by a clock traveling between the events.
  • Spacelike ($$s^2 < 0$$): The spatial separation dominates. There exists a frame where both events are simultaneous but at different locations. The proper distance is $$\sigma = \sqrt{|s^2|}$$. No causal influence can travel between spacelike-separated events.
  • Lightlike / Null ($$s^2 = 0$$): The events are connected by a light ray. This defines the light cone — the boundary between causal and non-causal regions of spacetime.

The invariance of $$s^2$$ under Lorentz transformations is the geometric foundation of special relativity. Just as rotations preserve spatial distance $$d^2 = x^2 + y^2 + z^2$$, Lorentz boosts preserve the spacetime interval. This is why the Minkowski metric is sometimes called a "pseudo-Euclidean" metric — it measures a generalized "distance" in 4D spacetime.

Understanding Your Results

The Interval Type tells you the causal relationship between the two events. For timelike intervals, the Proper Time gives the elapsed time on a clock moving inertially between the events — this is the shortest possible time separation. For spacelike intervals, the Proper Distance gives the spatial separation measured in a frame where both events are simultaneous. A lightlike interval means the events lie on each other's light cone. These classifications are observer-independent and form the backbone of causality in relativity.

Worked Examples

Timelike: Two Events Connected by a Slow Signal

Inputs

delta t2
delta x100000000
delta y0
delta z0

Results

s squared349200000000000000
s value590900000
proper time1.972
proper distance0
interval typeTimelike (causal connection possible)

With Δt = 2 s and Δx = 100,000 km, the interval is timelike (s² > 0). A massive particle could travel between these events, with proper time τ ≈ 1.97 s.

Spacelike: Simultaneous Distant Events

Inputs

delta t0.5
delta x300000000
delta y0
delta z0

Results

s squared-67500000000000000
s value259800000
proper time0
proper distance259800000
interval typeSpacelike (no causal connection)

With Δt = 0.5 s and Δx = 300,000 km (≈ 1 light-second), the spatial separation exceeds what light can traverse. No signal can connect these events.

Frequently Asked Questions

The spacetime interval $$s^2 = c^2\Delta t^2 - \Delta x^2 - \Delta y^2 - \Delta z^2$$ is the relativistic generalization of distance. Unlike ordinary distance or time, which change between reference frames, the spacetime interval is Lorentz invariant — every inertial observer computes the same value. It encodes both the separation and the causal relationship between two events.

A timelike interval ($$s^2 > 0$$) means the two events are close enough in space (relative to their time separation) that a massive particle traveling slower than light could be present at both. There exists a frame where both events happen at the same place, separated only by time. The proper time $$\tau = \sqrt{s^2}/c$$ is the time elapsed on a clock traveling between them.

A spacelike interval ($$s^2 < 0$$) means the spatial separation exceeds what any signal — even light — could traverse in the given time. No causal influence can pass between the events. There exists a frame where both events are simultaneous, separated only by space. The ordering (which happened first) is frame-dependent.

A lightlike interval ($$s^2 = 0$$) means $$c\Delta t = \sqrt{\Delta x^2 + \Delta y^2 + \Delta z^2}$$ — the events are exactly connected by a light signal. Light cones, formed by all null intervals from a given event, divide spacetime into causally connected (timelike) and disconnected (spacelike) regions.

The invariance follows from the postulates of special relativity: the laws of physics are the same in all inertial frames, and the speed of light is constant. Mathematically, Lorentz transformations mix space and time coordinates while preserving the quantity $$c^2\Delta t^2 - \Delta x^2 - \Delta y^2 - \Delta z^2$$, just as rotations mix x and y while preserving $$x^2 + y^2$$.

The sign convention determines whether $$s^2 = c^2\Delta t^2 - \Delta r^2$$ (+−−−, used here) or $$s^2 = -c^2\Delta t^2 + \Delta r^2$$ (−+++). Both are standard in physics. With +−−−, timelike intervals are positive and spacelike are negative. Particle physicists often use −+++. The physics is identical; only the sign of $$s^2$$ flips.

Sources & Methodology

Misner, C.W., Thorne, K.S. & Wheeler, J.A. (1973). Gravitation. W.H. Freeman. Taylor, E.F. & Wheeler, J.A. (1992). Spacetime Physics, 2nd Ed. W.H. Freeman. Carroll, S.M. (2004). Spacetime and Geometry. Addison-Wesley.
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