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Key Points

5 points
1

Decade‑long optical campaign captured OJ 287’s brightness and spectrum.

2

Binary supermassive black holes with a 12‑year period.

3

Relativistic jets produce variable emissions from radio to gamma rays.

4

Collaboration of 106 scientists, 48 institutions, 18 nations, using ~24 telescopes.

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Results advance knowledge of jet physics and multimessenger signals.

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Summary

OJ 287 hosts a binary system of two supermassive black holes with a twelve‑year orbital period.

The blazar emits relativistic jets directed toward Earth, causing rapid variations across the electromagnetic spectrum.

More than one hundred scientists from 48 institutions across 18 nations contributed data from dozens of ground‑based and space telescopes.

Findings improve understanding of black‑hole dynamics, jet emission mechanisms, and multimessenger astronomy.

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New Words to Learn

8 words
blazar
an active galactic nucleus with a jet aimed toward Earth, producing variable emissions
plasma
ionized gas consisting of free electrons and ions, common in space jets
electromagnetic spectrum
range of all electromagnetic radiation, from low‑frequency radio to high‑frequency gamma rays
binary black hole system
two supermassive black holes gravitationally bound and orbiting each other
relativistic jets
narrow streams of particles ejected at speeds close to light speed
multimessenger astronomy
study that combines different signals like light, gravitational waves, neutrinos, and cosmic rays
polarisation
the direction in which light waves vibrate
light‑year
distance light travels in one year, about 9.5 trillion kilometres
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