Season 1 · Session 08

Ripples in Spacetime

Colliding black holes shake the fabric of space, and we felt it.

Lands a thread

Read along anyway. These pages stand alone.

Start with the big idea

On September 14, 2015, two detectors thousands of miles apart twitched in step. The cause was a ripple thrown off by two black holes, each about thirty times the Sun's mass, spiralling together and merging 1.3 billion light-years away. For a fraction of a second that merger poured out more energy than every star in the observable universe combined, not as light but as a wave in spacetime itself. By the time it reached Earth it stretched LIGO's four-kilometre arms by less than one-thousandth the width of a proton. It is the most delicate measurement ever made. Einstein had predicted these waves in 1916 and doubted we could ever catch one. It took a century. The point that lands is that spacetime is not an inert stage the universe sits on. It is a physical fabric that stretches, squeezes, and rings like a struck bell, and now we can hear it.

More to see

LIGO
Two 4-kilometer arms. A laser beam split in two. And a measurement one-thousandth the diameter of a proton
The Chirp
LIGO control room, September 14, 2015. The first gravitational wave from two merging black holes.
Gravitational-wave chirp (illustration)
Illustration of a LIGO-style strain-vs-time chirp, the signal of two black holes spiralling in and merging.

Key ideas

Gravitational wave
A ripple in the curvature of spacetime, set off by massive objects accelerating, that travels outward at the speed of light. It physically stretches and squeezes space as it passes.
Strain
The tiny fractional change in length a wave causes. GW150914 stretched LIGO's 4-km arms by about one part in 10²¹. That's a length change near 1/1000 the diameter of a proton.
The chirp
As the two black holes spiralled in, the wave's pitch and volume rose together over a fifth of a second, then cut off at the merger. Played as audio, the signal sounds like a chirp.
A new sense
Gravitational waves pass straight through gas, dust, and galaxies that block light. They give us a way to register events light can never show. It's like gaining hearing after a life of only sight.

On your phone

Answer along during the session.

The opening question, the dig-in prompts, and the closing question, on one short form. What you write joins everyone else's on the wall, live, under your username.

Take it further

source Abbott, B.P. et al. (LIGO Scientific Collaboration and Virgo Collaboration), "Observation of Gravitational Waves from a Binary Black Hole Merger," *Physical Review Letters* 116, 061102 (2016).
source LIGO Caltech, "GW150914," https://www.ligo.caltech.edu/detection
source Einstein, A., "Näherungsweise Integration der Feldgleichungen der Gravitation," *Sitzungsberichte der Preußischen Akademie der Wissenschaften* (1916).

In person

Date to be announced. This page stands alone, so read along any time.