High-magnification deep optical view into SN1992E's host environment. Pan and scroll to explore the cosmic neighborhood where this star exploded.
⚡ Quick Observer Facts & Telemetry
IAU Transients DBThe Thermonuclear Obliteration of a White Dwarf
On 1992/01/27, astronomers scanning the heavens flagged a sudden, violent pinpoint of light that had flared into visibility. Designated SN1992E, it represents a catastrophic stellar explosion classified as a Type Ia supernova.
In a binary star system located deep within A063517-5956, a dense carbon-oxygen white dwarf—the dead stellar corpse of an ancient sun—orbited its stellar companion for millions of years. As it siphoned material across the gravitational saddle point, its mass relentlessly climbed toward the Chandrasekhar limit of 1.4 solar masses. At that fateful tipping point, uncontrollable carbon fusion ignited in the degenerate core, ripping the entire star apart in a thermonuclear detonation that left behind zero remnant.
A Message Across Deep Cosmic Time
The light from SN1992E is a dispatch from an ancient past. Located approximately 913.2 Million Light-Years away
(redshift z = 0.06), the photons detected by telescopes today began their journey
913.2 million years ago during the Paleozoic era, long before the first dinosaurs appeared on Earth.
While this burst of electromagnetic radiation traversed the cold void of intergalactic space at 299,792 kilometers per second, continents on Earth drifted, mountain ranges rose, and entire ecosystems rose and fell. To look into a telescope at SN1992E is to gaze directly into prehistoric cosmic time.
Incandescence of 539.5 million Suns
At the height of the outburst around 1992/01/26, SN1992E surged to a peak apparent magnitude of 20 and an intrinsic absolute magnitude of -17. At that instant, this single dying star radiated with the collective power of approximately 539.5 million Suns combined, outshining whole dwarf galaxies and illuminating the surrounding interstellar medium.
The total energy released by the cataclysm was on the order of 10⁵¹ to 10⁵³ ergs. Virtually all of this was deposited into the kinetic shockwave and radioactive nucleosynthesis.
The Radioactive Furnace: Why Supernovae Glow for Months
Unlike a conventional terrestrial explosion that cools and goes dark in seconds, SN1992E shone brightly for weeks and months. The secret behind this prolonged celestial glow is nuclear physics: the extreme heat and pressure of detonation synthesized vast quantities of radioactive Nickel-56 (⁵⁶Ni).
With a half-life of 6.075 days, Nickel-56 decays into Cobalt-56 (⁵⁶Co), emitting gamma rays and high-energy positrons that heat the expanding ejecta from within. Cobalt-56 in turn decays with a half-life of 77.2 days into stable Iron-56 (⁵⁶Fe), powering the steady exponential radioactive tail observed in the light curve.
Cosmic Kiln: Seeding the Elements of Life
Supernovae are the premier chemical foundries of our universe. SN1992E forged and liberated tons of newly synthesized elements: rich supplies of iron, silicon, calcium, and sulfur that will one day seed the formation of rocky terrestrial worlds.
As Carl Sagan famously observed, "We are made of star-stuff." The iron atoms that carry oxygen in human hemoglobin and the calcium in our bones were originally forged in explosions identical to SN1992E billions of years ago.
Galactic Setting in Dorado
SN1992E detonated inside A063517-5956, positioned at an offset of 1.05″ (1.44 kpc) from the galactic nucleus.
In our terrestrial sky, it resides in the constellation Dorado (The Swordfish / Dolphinfish) at Right Ascension 06:35:17.09
and Declination -59:56:02.8.
The Scientific Surveillance Campaign
Following its discovery by McNaught, observatories worldwide swung their lenses toward SN1992E. In the Open Supernova Catalog, SN1992E is documented across 1 photometric measurements and 0 spectroscopic epochs. These multi-wavelength observations allow astrophysicists to model the expanding photosphere, measure shock velocities, and probe circumstellar interactions.
Stargazer's Field Guide: Can You See It Tonight?
Can I see it tonight? Only as an expanding historical remnant.
The optical supernova exploded 34 years ago (1992/01/26). The bright transient outburst has long since ceased, leaving behind an expanding gaseous shell or pulsar wind nebula emitting in radio, X-rays, and faint nebular optical lines.
Historical Maximum: At peak in 1992/01/26, it reached magnitude 20.00 (2m–3m Research Telescope). Pointing here tonight observes the host galaxy (A063517-5956).
| Instrument Class & Aperture | Sensitivity Limit | At Peak Maximum (m=20.00) | Tonight (Est. m≈200.6) |
|---|---|---|---|
| Naked Eye Dark sky site (Bortle 1–3) with no optical aid |
m ≤ 6.0 | ❌ Below limit | ❌ Below limit |
| Binoculars (50mm) Standard 7x50 or 10x50 handheld binoculars |
m ≤ 9.5 | ❌ Below limit | ❌ Below limit |
| Small Backyard Scope (4" / 100mm) Entry 4-inch (100mm) refractor / reflector |
m ≤ 12.0 | ❌ Below limit | ❌ Below limit |
| Medium Amateur Scope (8"–12") 8-inch to 12-inch Dobsonian or Schmidt-Cassegrain |
m ≤ 14.5 | ❌ Below limit | ❌ Below limit |
| Amateur CMOS Rig Cooled monochrome/color CMOS camera with multi-hour stack |
m ≤ 19.5 | ❌ Below limit | ❌ Below limit |
| 2m–3m Research Telescope University or regional observatory (e.g. Palomar 60", Calar Alto) |
m ≤ 22.0 | ✅ Detectable | ❌ Below limit |
| Giant 8m–10m Observatories Keck (10m), VLT (8.2m), Gemini, Subaru optical imaging |
m ≤ 25.0 | ✅ Detectable | ❌ Below limit |
| Space Observatories Only Hubble Space Telescope (WFC3) / JWST (NIRCam deep stack) |
m ≤ 30.0 | ✅ Detectable | ❌ Below limit |
Planetary Safety Note: Even though SN1992E was a titanic explosion, our planet sits safely outside the lethal 50–100 light-year kill zone. At a distance of 913.2 Million Light-Years, the blast poses zero physical hazard to Earth's biosphere.
Cataloged supernovae closest to SN1992E in discovery time, spatial sky neighborhood, and cosmological lookback epoch: