Indian-Led Global Study Decodes Rare Binary Black Hole OJ 287
- Lead institute: ARIES Nainital with global partners
- Target: OJ 287 binary black hole
- Primary mass: At least 3.89 billion solar masses
- Observation scope: 24 telescopes across 10 years
A decade-long international monitoring campaign has decoded the cosmic flickering of OJ 287, a rare blazar located four billion light-years away housing two supermassive black holes locked in an orbital dance. Coordinated by researchers at the Aryabhatta Research Institute of Observational Sciences in Nainital, the collaborative effort mobilized 106 scientists across 18 countries and two dozen ground and space telescopes between 2015 and 2025.
OJ 287 features a primary black hole weighing at least 3.89 billion solar masses and a smaller companion completing an orbit every 12 years. The secondary black hole punches through the primary's accretion disk twice per orbit, generating relativistic plasma jets directed toward Earth and creating predictable double-peaked optical flares observed since 1880.
The newly assembled dataset represents the most densely sampled optical time series of the blazar collected in 150 years. By mapping brightness fluctuations and spectral shifts during low-flux states, researchers have resolved the relative positions of both black holes and isolated emissions from the smaller companion.
Beyond refining orbital mechanics, the findings establish OJ 287 as a premier natural laboratory for multimessenger astrophysics. Simultaneous observations across electromagnetic wavelengths now provide critical baseline data for linking optical bursts with future gravitational-wave and neutrino detections.
Frequently Asked Questions
What is OJ 287?
OJ 287 is a blazar located four billion light-years from Earth that contains two supermassive black holes orbiting each other every 12 years.
Who coordinated the 10-year study on OJ 287?
The multi-institutional project was led by Dr. Alok C. Gupta at the Aryabhatta Research Institute of Observational Sciences (ARIES), an autonomous body under the Department of Science and Technology.
What is the mass of the primary black hole in OJ 287?
Optical spectra collected during low-flux states indicate the primary supermassive black hole has a mass of at least 3.89 billion solar masses.
Source
Press Information Bureau Release ID 2319522, Ministry of Science and Technology · 2026-10-06
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