The Spacetime Metric
Lecture 137 min 18 sec

What is a metric?

Geometry as a recipe for measuring distance.

Build the mathematical vocabulary needed to understand what physicists mean when they say spacetime has geometry—and what it would mean to change it.

Season 1 · remastered lesson

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37 min 18 sec · Captions: English · Español · Português · Français · Polski

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Visual explanation

Explore the central idea

Motion is optional · static explanation always available

A field map is not a metric. This Newtonian snapshot shows acceleration directions outside spherical masses, not spacetime curvature or a change in the rule for measuring intervals.

Gravity has no universal down

Imagine small test objects all around the masses. Each arrow shows the direction in which gravity changes an object’s motion, not the path it follows.

Mass arrangement
Gravity directions in three dimensionsDots mark sample positions. Arrows point along the net gravitational acceleration. The outlined dot is the selected sample. All non-zero arrows have the same length in 3D: they show direction only. Read the strength in the sample values. An arrow can look shorter when it points toward or away from your viewpoint.

Outside one spherical mass, gravity points toward its center from every direction.

All non-zero arrows have the same length in 3D: they show direction only. Read the strength in the sample values. An arrow can look shorter when it points toward or away from your viewpoint. Paler arrows are in the farther half of the scene; pale does not mean weaker gravity.

Viewpoint

These controls move your viewpoint. They do not move the masses or change the gravitational field.

Try it: where is down?

  1. Choose one mass. Predict where the arrows on its far side point, then turn the view to check. Look from above and below: do the arrows still point toward the mass?
  2. Choose two masses and turn the view again. Each arrow now combines both pulls; it need not point at either center. The smaller mass contributes too.

Did turning the view change gravity, or only how you see it?

Check your answer

Only your view changed. The masses and the pull at each point stayed the same. There is no bottom underneath the whole scene.

Selected sample · Scaled teaching units

x, y and z are scene coordinates, not universal up or down.

Position (x, y, z)
1.25; 0.02604; 0
Acceleration (x, y, z)
-2.559; -0.05333; 0
Strength
2.56

Masses in this snapshot

  • A: Mass 4; Radius 0.64; Center (0; 0; 0)
All sample values
The same sample positions and field values used by the diagram
SamplePosition (x, y, z)Acceleration (x, y, z)Strength
11.25; 0.02604; 0-2.559; -0.05333; 02.56
2-1.25; -0.02604; 02.559; 0.05333; 02.56
3-0.9199; 0.07813; 0.84271.884; -0.16; -1.7262.56
40.9199; -0.07813; -0.8427-1.884; 0.16; 1.7262.56
50.1087; 0.1302; -1.238-0.2226; -0.2667; 2.5362.56
6-0.1087; -0.1302; 1.2380.2226; 0.2667; -2.5362.56
70.7524; 0.1823; 0.9814-1.541; -0.3733; -2.012.56
8-0.7524; -0.1823; -0.98141.541; 0.3733; 2.012.56
9-1.209; 0.2344; -0.21392.476; -0.48; 0.4382.56
101.209; -0.2344; 0.2139-2.476; 0.48; -0.4382.56
111.027; 0.2865; -0.6531-2.103; -0.5867; 1.3372.56
12-1.027; -0.2865; 0.65312.103; 0.5867; -1.3372.56
13-0.3124; 0.3385; 1.1620.6397; -0.6933; -2.382.56
140.3124; -0.3385; -1.162-0.6397; 0.6933; 2.382.56
15-0.5473; 0.3906; -1.0541.121; -0.8; 2.1582.56
160.5473; -0.3906; 1.054-1.121; 0.8; -2.1582.56
171.098; 0.4427; 0.401-2.249; -0.9067; -0.82132.56
18-1.098; -0.4427; -0.4012.249; 0.9067; 0.82132.56
19-1.061; 0.4948; 0.4382.173; -1.013; -0.8972.56
201.061; -0.4948; -0.438-2.173; 1.013; 0.8972.56
210.4764; 0.5469; -1.018-0.9757; -1.12; 2.0852.56
22-0.4764; -0.5469; 1.0180.9757; 1.12; -2.0852.56
230.3284; 0.599; 1.047-0.6725; -1.227; -2.1442.56
24-0.3284; -0.599; -1.0470.6725; 1.227; 2.1442.56
25-0.9232; 0.651; -0.5351.891; -1.333; 1.0962.56
260.9232; -0.651; 0.535-1.891; 1.333; -1.0962.56
271.009; 0.7031; -0.2219-2.067; -1.44; 0.45452.56
28-1.009; -0.7031; 0.22192.067; 1.44; -0.45452.56
29-0.5729; 0.7552; 0.81481.173; -1.547; -1.6692.56
300.5729; -0.7552; -0.8148-1.173; 1.547; 1.6692.56
31-0.1226; 0.8073; -0.94640.2512; -1.653; 1.9382.56
320.1226; -0.8073; 0.9464-0.2512; 1.653; -1.9382.56
330.6941; 0.8594; 0.585-1.422; -1.76; -1.1982.56
34-0.6941; -0.8594; -0.5851.422; 1.76; 1.1982.56
35-0.8547; 0.9115; 0.035341.75; -1.867; -0.072382.56
360.8547; -0.9115; -0.03534-1.75; 1.867; 0.072382.56
370.5644; 0.9635; -0.5617-1.156; -1.973; 1.152.56
38-0.5644; -0.9635; 0.56171.156; 1.973; -1.152.56
39-0.03366; 1.016; 0.72790.06894; -2.08; -1.4912.56
400.03366; -1.016; -0.7279-0.06894; 2.08; 1.4912.56
41-0.4165; 1.068; -0.49910.8529; -2.187; 1.0222.56
420.4165; -1.068; 0.4991-0.8529; 2.187; -1.0222.56
430.5505; 1.12; 0.07407-1.127; -2.293; -0.15172.56
44-0.5505; -1.12; -0.074071.127; 2.293; 0.15172.56
45-0.3571; 1.172; 0.24840.7313; -2.4; -0.50882.56
460.3571; -1.172; -0.2484-0.7313; 2.4; 0.50882.56
470.05571; 1.224; -0.2476-0.1141; -2.507; 0.50722.56
48-0.05571; -1.224; 0.24760.1141; 2.507; -0.50722.56
492.05; 0.04271; 0-0.9516; -0.01983; 00.9518
50-2.05; -0.04271; 00.9516; 0.01983; 00.9518
51-1.509; 0.1281; 1.3820.7005; -0.05949; -0.64170.9518
521.509; -0.1281; -1.382-0.7005; 0.05949; 0.64170.9518
530.1782; 0.2135; -2.031-0.08276; -0.09915; 0.9430.9518
54-0.1782; -0.2135; 2.0310.08276; 0.09915; -0.9430.9518
551.234; 0.299; 1.609-0.5729; -0.1388; -0.74730.9518
56-1.234; -0.299; -1.6090.5729; 0.1388; 0.74730.9518
57-1.983; 0.3844; -0.35070.9206; -0.1785; 0.16280.9518
581.983; -0.3844; 0.3507-0.9206; 0.1785; -0.16280.9518
591.684; 0.4698; -1.071-0.7817; -0.2181; 0.49730.9518
60-1.684; -0.4698; 1.0710.7817; 0.2181; -0.49730.9518
61-0.5123; 0.5552; 1.9060.2379; -0.2578; -0.88480.9518
620.5123; -0.5552; -1.906-0.2379; 0.2578; 0.88480.9518
63-0.8975; 0.6406; -1.7280.4167; -0.2974; 0.80240.9518
640.8975; -0.6406; 1.728-0.4167; 0.2974; -0.80240.9518
651.801; 0.726; 0.6576-0.8361; -0.3371; -0.30530.9518
66-1.801; -0.726; -0.65760.8361; 0.3371; 0.30530.9518
67-1.74; 0.8115; 0.71830.8079; -0.3768; -0.33350.9518
681.74; -0.8115; -0.7183-0.8079; 0.3768; 0.33350.9518
690.7813; 0.8969; -1.67-0.3628; -0.4164; 0.77520.9518
70-0.7813; -0.8969; 1.670.3628; 0.4164; -0.77520.9518
710.5385; 0.9823; 1.717-0.25; -0.4561; -0.79710.9518
72-0.5385; -0.9823; -1.7170.25; 0.4561; 0.79710.9518
73-1.514; 1.068; -0.87750.703; -0.4957; 0.40740.9518
741.514; -1.068; 0.8775-0.703; 0.4957; -0.40740.9518
751.655; 1.153; -0.3639-0.7686; -0.5354; 0.1690.9518
76-1.655; -1.153; 0.36390.7686; 0.5354; -0.1690.9518
77-0.9395; 1.239; 1.3360.4362; -0.5751; -0.62050.9518
780.9395; -1.239; -1.336-0.4362; 0.5751; 0.62050.9518
79-0.2011; 1.324; -1.5520.09339; -0.6147; 0.72070.9518
800.2011; -1.324; 1.552-0.09339; 0.6147; -0.72070.9518
811.138; 1.409; 0.9594-0.5285; -0.6544; -0.44540.9518
82-1.138; -1.409; -0.95940.5285; 0.6544; 0.44540.9518
83-1.402; 1.495; 0.057960.6508; -0.694; -0.026910.9518
841.402; -1.495; -0.05796-0.6508; 0.694; 0.026910.9518
850.9257; 1.58; -0.9212-0.4298; -0.7337; 0.42770.9518
86-0.9257; -1.58; 0.92120.4298; 0.7337; -0.42770.9518
87-0.0552; 1.666; 1.1940.02563; -0.7733; -0.55430.9518
880.0552; -1.666; -1.194-0.02563; 0.7733; 0.55430.9518
89-0.683; 1.751; -0.81850.3171; -0.813; 0.380.9518
900.683; -1.751; 0.8185-0.3171; 0.813; -0.380.9518
910.9029; 1.836; 0.1215-0.4192; -0.8527; -0.05640.9518
92-0.9029; -1.836; -0.12150.4192; 0.8527; 0.05640.9518
93-0.5856; 1.922; 0.40740.2719; -0.8923; -0.18920.9518
940.5856; -1.922; -0.4074-0.2719; 0.8923; 0.18920.9518
950.09136; 2.007; -0.4061-0.04242; -0.932; 0.18860.9518
96-0.09136; -2.007; 0.40610.04242; 0.932; -0.18860.9518

This Newtonian snapshot assumes each body's mass is distributed the same way in every direction from its center. It shows only the exterior field, not spacetime curvature. The bodies stay fixed; their motion is not simulated.

Read alongside

The Metric Tensor, Warp Drives, and Wormholes

The experiments, equations, and original papers behind the lesson.

Open the companion chapter →