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The silent deaths: stars that collapse into black holes without exploding

The silent deaths: stars that collapse into black holes without exploding

New Capabilities
By Newzino Staff |

Astronomers catch massive stars vanishing in real-time, filling a gap in our understanding of stellar death

August 13th, 2025: AI-Assisted Analysis Advances Failed Supernova Detection

Overview

For decades, astronomers assumed all massive stars end their lives in spectacular supernova explosions. But a quiet revolution in observations has revealed that some stars simply vanish—collapsing directly into black holes without the cosmic fireworks. Two confirmed cases, one in the Fireworks Galaxy and another in Andromeda, now suggest that 10 to 30 percent of massive stars may meet this silent end.

The discovery matters beyond astrophysics. The black holes that LIGO detects merging across the cosmos are often too massive to have formed from standard supernova explosions, which blow away much of a star's mass. Failed supernovae offer a cleaner path to creating these heavyweight black holes, potentially solving one of gravitational-wave astronomy's persistent puzzles.

Key Indicators

2
Confirmed failed supernovae
N6946-BH1 (2009) and M31-2014-DS1 (2014) are the only two confirmed observations worldwide
10-30%
Estimated fraction of massive stars
Survey data suggests up to three in ten massive stars may die this way
98%
Mass collapse in M31-2014-DS1
The Andromeda star retained almost all its mass, forming a 6.5 solar mass black hole
17 M☉
Theoretical mass threshold
Stars born above roughly 17 solar masses may be too massive to explode conventionally

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People Involved

Christopher Kochanek
Christopher Kochanek
Professor of Astronomy, Ohio State University (Leading ongoing Large Binocular Telescope survey)
Kishalay De
Kishalay De
Postdoctoral Scholar, MIT Kavli Institute (Lead author on M31-2014-DS1 discovery paper)
Stephen Smartt
Stephen Smartt
Professor of Astrophysics, Queen's University Belfast (Pioneer of supernova progenitor studies)

Organizations Involved

Large Binocular Telescope Observatory
Large Binocular Telescope Observatory
Astronomical Observatory
Status: Primary facility for failed supernova survey

Twin 8.4-meter telescope on Mount Graham, Arizona, conducting the only systematic failed supernova search.

MIT Kavli Institute for Astrophysics and Space Research
MIT Kavli Institute for Astrophysics and Space Research
Research Institute
Status: Leading M31-2014-DS1 investigation

MIT research center coordinating multi-telescope observations of the Andromeda failed supernova candidate.

Timeline

  1. AI-Assisted Analysis Advances Failed Supernova Detection

    Analysis

    Machine learning techniques increasingly applied to transient surveys help identify disappearing stars and distinguish failed supernovae from supernova impostors.

  2. Follow-up Analysis Refines Black Hole Picture

    Publication

    New paper models M31-2014-DS1 remnant as dust-enshrouded. No X-ray emission detected, complicating accretion-powered luminosity hypothesis.

  3. JWST Observes M31-2014-DS1 Remnant

    Observation

    JWST MIRI and NIRSpec observations reveal an extremely red source with strong molecular absorption, probing the aftermath of the collapse.

  4. M31-2014-DS1 Announced as Second Candidate

    Publication

    MIT-led team publishes analysis concluding the Andromeda star collapsed into a 6.5 solar mass black hole, retaining 98% of its mass.

  5. VFTS 243 Confirms Silent Collapse Is Possible

    Publication

    Study of binary system VFTS 243 in Large Magellanic Cloud shows its black hole formed without a supernova kick, providing independent evidence stars can collapse silently.

  6. JWST Reveals Complex Picture at N6946-BH1

    Publication

    New JWST observations show the original source was actually at least three blended objects. Failed supernova hypothesis not ruled out, but situation more complex than thought.

  7. M31-2014-DS1 Becomes Undetectable

    Observation

    Deep optical and near-infrared imaging fails to detect the Andromeda star, which has now fully vanished from view.

  8. First Failed Supernova Confirmed

    Publication

    Kochanek's team publishes definitive analysis of N6946-BH1, establishing it as the first strong failed supernova candidate.

  9. M31-2014-DS1 Begins Rapid Fading

    Observation

    The Andromeda star's luminosity drops dramatically over the next 1,000 days, fading more than tenfold in total light.

  10. N6946-BH1 Vanishes From Optical View

    Discovery

    Hubble and Spitzer observations confirm the star has disappeared without a supernova. A faint infrared source remains.

  11. M31-2014-DS1 Detected Brightening

    Observation

    A 20 solar mass supergiant in Andromeda begins mid-infrared brightening, maintaining constant luminosity for approximately 1,000 days.

  12. N6946-BH1 Begins Brightening

    Observation

    A 25 solar mass star in NGC 6946 brightens to over 1 million solar luminosities, entering what appears to be early supernova stages.

Scenarios

1

JWST Confirms Both Candidates as Genuine Failed Supernovae

Discussed by: MIT Kavli Institute researchers, Large Binocular Telescope team

Continued JWST monitoring shows both N6946-BH1 and M31-2014-DS1 fading in predictable patterns consistent with fallback accretion onto black holes. Combined with non-detection of surviving stars or merger signatures, the failed supernova hypothesis becomes the consensus explanation, establishing this as a confirmed stellar death pathway.

2

N6946-BH1 Revealed as Stellar Merger, M31-2014-DS1 Stands Alone

Discussed by: JWST observation teams, stellar merger theorists

Ongoing JWST monitoring of N6946-BH1 shows the infrared source brightening or stabilizing, consistent with a surviving merged star clearing its dust envelope. The three blended objects complicate interpretation. M31-2014-DS1 remains the stronger candidate, but with only one confirmed case, statistical estimates of failed supernova rates require revision.

3

Gravitational Wave Detection Confirms Failed Supernova in Real-Time

Discussed by: LIGO-Virgo-KAGRA collaboration, neutrino observatory teams

A nearby massive star collapse produces a gravitational wave burst detectable by LIGO, combined with neutrino detection from Super-Kamiokande or similar facilities, while optical surveys catch the star vanishing. This multi-messenger detection would definitively confirm the failed supernova mechanism and enable precise mass measurements.

4

Survey Expansion Finds Dozens of Failed Supernova Candidates

Discussed by: Vera Rubin Observatory planners, Zwicky Transient Facility team

The Vera Rubin Observatory's Legacy Survey of Space and Time, beginning operations, monitors millions of stars across thousands of galaxies with AI-assisted detection. The dramatically expanded survey volume identifies numerous disappearing massive stars, enabling population-level studies of which stellar properties predict silent collapse versus explosive death.

Historical Context

SN 1987A: The Last Nearby Supernova (1987)

February 1987

What Happened

A blue supergiant in the Large Magellanic Cloud exploded 168,000 light-years from Earth—the closest supernova since Kepler's in 1604. Neutrino detectors in Japan and the US captured about two dozen particles from the collapsing core, confirming decades of theoretical predictions about supernova physics.

Outcome

Short Term

The 19 detected neutrinos proved that core collapse releases most energy as neutrinos, not light. The star's unusual blue color challenged supernova models.

Long Term

SN 1987A established neutrino astronomy as a field and motivated construction of larger detectors like Super-Kamiokande, which could detect neutrinos from a failed supernova within our galaxy.

Why It's Relevant Today

A failed supernova would produce a neutrino burst without the optical supernova. Detecting such a signal would provide smoking-gun evidence. Current detectors could catch a galactic failed supernova, but M31-2014-DS1 at 2.5 million light-years is too distant.

Eta Carinae's Great Eruption (1837-1858)

1837-1858

What Happened

Eta Carinae, a massive binary system 7,500 light-years away, underwent a decades-long outburst that briefly made it the second-brightest star in the sky. The star ejected 10-40 solar masses of material but survived, creating the spectacular Homunculus Nebula visible today.

Outcome

Short Term

The eruption was initially mistaken for a supernova. The star's survival established 'supernova impostors' as a distinct phenomenon.

Long Term

Eta Carinae remains unstable and is expected to explode as a true supernova within the next million years. Its eruption demonstrated that massive stars can have violent outbursts short of complete destruction.

Why It's Relevant Today

Failed supernovae must be distinguished from supernova impostors like Eta Carinae's eruption. The key difference: impostors leave a surviving star, while failed supernovae leave a black hole. Careful long-term monitoring is required to tell them apart.

First Gravitational Wave Detection GW150914 (2015)

September 2015

What Happened

LIGO detected gravitational waves from two black holes of 36 and 29 solar masses merging 1.3 billion light-years away. The final black hole was 62 solar masses—meaning 3 solar masses of energy radiated as gravitational waves in a fraction of a second.

Outcome

Short Term

The detection confirmed Einstein's century-old prediction and opened gravitational-wave astronomy. The unexpectedly large black hole masses puzzled theorists.

Long Term

LIGO has now detected over 300 black hole mergers. Many involve black holes too massive to have formed from standard supernovae, which blow away significant stellar mass.

Why It's Relevant Today

Failed supernovae offer a solution to the massive black hole puzzle. If a star collapses without exploding, it retains nearly all its mass, creating heavier black holes than supernova-producing stars. The 10-30% failed supernova rate could explain LIGO's heavy black hole population.

10 Sources:
+4
arXiv NASA Science Science News Monthly Notices of the Royal Astronomical Society Live Science ScienceDaily Phys.org LIGO Caltech arXiv/Astrophysical Journal arXiv