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Record #00428Space archive

Most Massive Known Black Hole

TON 618 is an ultramassive black hole associated with a luminous quasar, often estimated at about 66 billion solar masses. Its ranking and mass remain dependent on indirect estimation methods.

Verification status
Evidence-backedView verification details ↗
Last updated
2026-11-07
Category index
Space

ARCHIVE VISUAL / 01

NOT TO SCALE

Current Record

about66 billionsolar masses

Current record value

Holder
TON 618
Location
—
Start date
—
Record status
Evidence-backedView verification details ↗Report an issue
OverviewRecord historyRelated recordsSources

Overview

Archive Note

TON 618's mass is inferred indirectly from quasar emission-line properties and assumptions about the broad-line region rather than direct dynamical weighing.

Published calibrations differ. A 2024 study discusses an estimate near 40.7 billion solar masses, so the commonly quoted 66-billion figure should not be treated as exact.

Key information

Object
Black hole powering a luminous quasar
Often-cited mass estimate
About 66 billion solar masses
Alternative model estimate
About 40.7 billion solar masses

Record history

1 Milestones
  1. —about 66 billion solar massesTON 618Current Record

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Sources

Evidence & References

Verification basis and limitations

Evidence-backed

Credible sources support core facts; the comparison scope or corroboration remains incomplete.

Basis: corroborating reliable secondary materials

NASA cites an estimate of roughly 66 billion solar masses for TON 618; another academic study discusses a model estimate near 40.7 billion. The mass is inferred from quasar emission-line methods, not direct dynamical weighing, and its ranking depends on adopted estimates.

Comparison boundaries still under review

Mass is model-dependent; published estimates discussed here range from roughly 40.7 to 66 billion solar masses, and the ranking may change.

Verification assessment
2026-11-07
Last editorial review
2026-11-07

Current Entry identifies the current entry in this archive; it does not establish that the record is still held today.

Source IDSourcePublisherLink
SRC-001Deciphering the origins and growth of supermassive black holesAcademicENCurrent recordMonthly Notices of the Royal Astronomical SocietySRC-002Black HolesOfficialENCurrent recordNASASRC-003Constraints on stupendously large black holesAcademicENCurrent recordMonthly Notices of the Royal Astronomical Society

The record value on this page is organized from the public sources above. Measurement methods may differ; JiLuDB follows the unified method described for each entry.

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