High-magnification deep optical view into SN2005la's host environment. Pan and scroll to explore the cosmic neighborhood where this star exploded.
★ Benchmark Astrophysical Landmark
SN2005la is recognized as one of the definitive benchmark supernovae in modern astrophysics. Due to its exceptional peak luminosity, favorable host galaxy orientation, and rapid multi-messenger follow-up, it was extensively observed across the electromagnetic spectrum by premier facilities—including space telescopes (HST, JWST, Swift) and global ground-based spectroscopic networks. It provides foundational empirical constraints for stellar progenitor models, ejecta dynamics, and cosmological distance calibrations.
⚡ Quick Observer Facts & Telemetry
IAU Transients DBThe Iron Core Collapse of a Dying Supergiant
On 2005/11/30, astronomers scanning the heavens flagged a sudden, violent pinpoint of light that had flared into visibility. Designated SN2005la, it represents a catastrophic stellar explosion classified as a Type Ibn/IIbn supernova.
The progenitor of SN2005la was a mammoth supergiant star, shining with the furious vigor of an object at least 8 to 25 times more massive than our Sun. For millions of years, it synthesized heavier and heavier elements in concentric onion-like shells: hydrogen burning into helium, helium into carbon, carbon into oxygen, neon, and silicon. But when silicon fused into iron, the stellar engine ran out of fuel. Iron fusion absorbs energy rather than liberating it; within fractions of a second, the iron core collapsed under its own gravity, rebounding into an immense cosmic shockwave that blasted the star into pieces.
A Message Across Deep Cosmic Time
The light from SN2005la is a dispatch from an ancient past. Located approximately 271.7 Million Light-Years away
(redshift z = 0.01856), the photons detected by telescopes today began their journey
271.7 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 SN2005la is to gaze directly into prehistoric cosmic time.
Incandescence of 681.1 million Suns
At the height of the outburst around 2005/11/21, SN2005la surged to a peak apparent magnitude of 17.33 and an intrinsic absolute magnitude of -17.253. At that instant, this single dying star radiated with the collective power of approximately 681.1 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. Over 99% of this energy was emitted within the first 10 seconds as a dense burst of trillions of neutrinos, with only 1% driving the visible blast wave.
The Radioactive Furnace: Why Supernovae Glow for Months
Unlike a conventional terrestrial explosion that cools and goes dark in seconds, SN2005la 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. SN2005la forged and liberated tons of newly synthesized elements: vast reservoirs of oxygen (the most abundant heavy element in living organisms), carbon, nitrogen, magnesium, and silicon.
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 SN2005la billions of years ago.
Galactic Setting in Coma Berenices
SN2005la detonated inside MCG +05-30-111, positioned at an offset of 7.77″ (3.02 kpc) from the galactic nucleus.
In our terrestrial sky, it resides in the constellation Coma Berenices (Berenice's Hair) at Right Ascension 12:52:15.68
and Declination +27:31:52.5.
The Scientific Surveillance Campaign
Following its discovery by Quinby, Modol, observatories worldwide swung their lenses toward SN2005la.
In the Open Supernova Catalog, SN2005la is documented across 88 photometric measurements
in passbands such as B, I, R, V, i', r' and 11 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? No — this supernova is physically extinguished.
Supernovae are brief, explosive cosmic catastrophes. They brighten over days to weeks and then permanently fade into darkness as their radioactive nickel-56 and cobalt-56 fuel decays. This explosion occurred 20.9 years ago (2005/11/21). Accounting for cosmological time dilation at redshift z = 0.0186, the rest-frame age is +7477.2 days. By standard radioactive decay templates, its optical brightness has decayed by Δm ≈ 121.0 magnitudes to an estimated magnitude 138.3, rendering the transient undetectable to all ground-based observatories.
Instrument Breakdown: At its maximum brightness in 2005/11/21, it reached magnitude 17.33 (Amateur CMOS Rig). Tonight, pointing a telescope at these coordinates will reveal only the background host galaxy (MCG +05-30-111).
| Instrument Class & Aperture | Sensitivity Limit | At Peak Maximum (m=17.33) | Tonight (Est. m≈138.3) |
|---|---|---|---|
| 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 | ✅ Detectable | ❌ 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 SN2005la was a titanic explosion, our planet sits safely outside the lethal 50–100 light-year kill zone. At a distance of 271.7 Million Light-Years, the blast poses zero physical hazard to Earth's biosphere.
Cataloged supernovae closest to SN2005la in discovery time, spatial sky neighborhood, and cosmological lookback epoch:
❓ Frequently Asked Questions About SN2005la
What type of supernova is SN2005la and what kind of star exploded? Astrophysics & Progenitor
What was the progenitor star doing in the millions of years leading up to SN2005la? Astrophysics & Progenitor
How far away is SN2005la from Earth and how old is the light reaching us? Cosmic Distance & Time
What does the cosmological redshift of SN2005la tell us about the expansion of space? Cosmic Distance & Time
How bright did SN2005la become at its peak, and how many Suns does that equal? Explosion Energetics
How much total energy was released by SN2005la, and where did that energy go? Explosion Energetics
How fast are the supernova ejecta and shockwave of SN2005la expanding through space? Explosion Energetics
What powers the prolonged glow of SN2005la weeks and months after detonation? Radioactive Engine
What chemical elements did SN2005la create and disperse into the universe? Nucleosynthesis & Elements
Did SN2005la leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
What will SN2005la's explosion site look like in 1,000 to 10,000 years? Cosmic Remnant
In which galaxy did SN2005la explode, and where is it located relative to the galactic center? Galactic Environment
Where is SN2005la located in the night sky and which constellation is it in? Sky Coordinates
How much Milky Way interstellar dust obscures our view of SN2005la? Interstellar Dust
Across which photometric filter bands was SN2005la monitored? Astronomical Observations
B, I, R, V, i', r'. Data were captured by observatories and survey networks including CfA3_KEP. Multi-color photometry tracks the temperature evolution of the fireball, verifying the rise time to peak and the rate of radioactive decline.