Light and waves

April 2019

The first image of a black hole

Event Horizon Telescope Collaboration

How do you build a telescope as big as the Earth?

Radio dishes across the Earth observed together, acting like one telescope the size of the planet. They imaged the glowing ring of gas around the black hole at the centre of galaxy M87, about 55 million light-years away.

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How they figured it out

The sharpness of a telescope depends on its size compared with the wavelength it sees. To see the shadow of the black hole in M87, as small in our sky as an orange on the Moon, you would need a dish the size of the Earth.

So astronomers linked radio dishes around the world, each recording signals stamped by atomic clocks onto hard drives: petabytes of data. The drives from the South Pole had to wait months for the end of the Antarctic winter before they could be flown out. The 2017 observations became the first image of a black hole, released on 10 April 2019.

The equation

V(u,v)=∬I(x,y) e−2πi(ux+vy) dx dyV(u,v) = \iint I(x,y)\, e^{-2\pi i (ux + vy)}\, dx\,dy

Each pair of dishes measures one wave-pattern ingredient of the image; together they rebuild it.

Everyday echoPhone cameras store photos by their wave ingredients too (that is what JPEG does).

See it in real life

Phones at a concert

Imagine reconstructing a concert stage from photos taken by fans in seats all over the stadium: more seats, sharper picture. Hospital MRI scanners build images from frequency measurements in the same way.

Where engineers use it

  • Radio astronomy and MRI

    Rebuilding images from measured Fourier components is how MRI scanners work too.

  • Atomic clocks

    Each dish recorded data stamped by atomic clocks so it could be combined later.