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The Story of Supernova PSN J08425627-2003112

An extraordinary stellar explosion that occurred Millions of Light-Years away in deep space.

🔭 Deep Field (~2.1′ FOV) · Highest-Definition Optical Field (0.25″/pix)
● PSN J08425627-2003112 Explosion Site

High-magnification deep optical view into PSN J08425627-2003112's host environment. Pan and scroll to explore the cosmic neighborhood where this star exploded.

⚡ Quick Observer Facts & Telemetry

IAU Transients DB
🌐 Distance to Earth
Millions of Light-Years
Lookback Cosmic Time
✨ Peak Brightness
Mag 18.4
Large Observatory
☀️ Peak Radiance
Hundreds of Millions of Suns
Combined Stellar Energy
🚀 Shock Velocity
~8,500 km/s
~2.8% Speed of Light
🌌 Host Galaxy
ESO 563-14
Center Coincident
🧭 Constellation
Pyxis
The Compass
💥 Explosion Physics
Type —
Core-Collapse Supergiant
📅 Discovered On
2011/02/16
Stuart Parker
CHAPTER I

The Iron Core Collapse of a Dying Supergiant

On 2011/02/16, astronomers scanning the heavens flagged a sudden, violent pinpoint of light that had flared into visibility. Designated PSN J08425627-2003112, it represents a catastrophic stellar explosion classified as a Type — supernova.

The progenitor of PSN J08425627-2003112 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.

Astrophysical Mechanism Summary
Type: Type — • Progenitor: Massive Red/Stripped Supergiant Star • Velocity: ~8,500 km/s (~2.8% c)
CHAPTER II

A Message Across Deep Cosmic Time

The light from PSN J08425627-2003112 is a dispatch from an ancient past. Located approximately Millions of Light-Years away , the photons detected by telescopes today began their journey deep cosmic time.

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 PSN J08425627-2003112 is to gaze directly into prehistoric cosmic time.

CHAPTER III

Incandescence of hundreds of millions of Suns

At the height of the outburst around 2011/02/16, PSN J08425627-2003112 surged to a peak apparent magnitude of 18.4 . At that instant, this single dying star radiated with the collective power of approximately hundreds of millions of 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.

CHAPTER IV

The Radioactive Furnace: Why Supernovae Glow for Months

Unlike a conventional terrestrial explosion that cools and goes dark in seconds, PSN J08425627-2003112 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.

CHAPTER V

Cosmic Kiln: Seeding the Elements of Life

Supernovae are the premier chemical foundries of our universe. PSN J08425627-2003112 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 PSN J08425627-2003112 billions of years ago.

CHAPTER VI

Galactic Setting in Pyxis

PSN J08425627-2003112 detonated inside ESO 563-14. In our terrestrial sky, it resides in the constellation Pyxis (The Compass) at Right Ascension 08:42:56.27 and Declination -20:03:11.1.

CHAPTER VII

The Scientific Surveillance Campaign

Following its discovery by Stuart Parker, observatories worldwide swung their lenses toward PSN J08425627-2003112. In the Open Supernova Catalog, PSN J08425627-2003112 is documented across 0 photometric measurements and 0 spectroscopic epochs. These multi-wavelength observations allow astrophysicists to model the expanding photosphere, measure shock velocities, and probe circumstellar interactions.

CHAPTER VIII

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 15.6 years ago (2011/02/16). Accounting for cosmological time dilation at redshift z = 0.0000, the rest-frame age is +5712.0 days. By standard radioactive decay templates, its optical brightness has decayed by Δm ≈ 80.5 magnitudes to an estimated magnitude 98.9, rendering the transient undetectable to all ground-based observatories.

Instrument Breakdown: At its maximum brightness in 2011/02/16, it reached magnitude 18.40 (Amateur CMOS Rig). Tonight, pointing a telescope at these coordinates will reveal only the background host galaxy (ESO 563-14).

Instrument Class & Aperture Sensitivity Limit At Peak Maximum (m=18.40) Tonight (Est. m≈98.9)
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 PSN J08425627-2003112 was a titanic explosion, our planet sits safely outside the lethal 50–100 light-year kill zone. At a distance of Millions of Light-Years, the blast poses zero physical hazard to Earth's biosphere.

🌌 Cosmic Neighbors & Contemporaries 110,222+ Transients Indexed

Cataloged supernovae closest to PSN J08425627-2003112 in discovery time, spatial sky neighborhood, and cosmological lookback epoch:

⏱️ Closest in Time
SN2011aj +2d after
Type Ia 2011/02/18 · Mag 16.2
GRB 110213A 3d before
Type LGRB 2011/02/13
MLS110213:014203+112145 3d before
Type Candidate 2011/02/13
🔭 Closest on the Sky
PS1-13eqv 25.3′ away
Type Transient Discovered 2013/12/30
SN2020abcq 28.4′ away
Type II Discovered 2020/11/28
AT2018bbq 32.8′ away
Type Candidate Discovered 2018/02/24
🌌 Same Cosmic Era (Redshift)
Redshift data unavailable for cosmic distance matching.

❓ Frequently Asked Questions About PSN J08425627-2003112

Scientific & observational Q&As indexed from astronomical databases & the Open Supernova Catalog
What type of supernova is PSN J08425627-2003112 and what kind of star exploded? Astrophysics & Progenitor
PSN J08425627-2003112 is cataloged as a Type — transient. It represents a catastrophic stellar explosion marking the terminal evolutionary endpoint of a star, liberating immense radiant energy and dispersing newly synthesized chemical elements into the host galaxy's interstellar medium.
What was the progenitor star doing in the millions of years leading up to PSN J08425627-2003112? Astrophysics & Progenitor
Before detonating as PSN J08425627-2003112, the progenitor lived a short, furious stellar life of roughly 10 to 30 million years. In its interior, temperatures and pressures reached astronomical extremes, burning through nuclear fuel in an 'onion-skin' arrangement of concentric shells: hydrogen burning into helium for millions of years, helium into carbon for hundreds of thousands of years, carbon into neon for centuries, oxygen into silicon for months, and silicon fusing into iron in mere days! Once iron filled the core, fusion could no longer extract energy, dooming the star to sudden gravitational collapse.
How far away is PSN J08425627-2003112 from Earth and how old is the light reaching us? Cosmic Distance & Time
PSN J08425627-2003112 is located approximately Millions of Light-Years from Earth. Because electromagnetic radiation travels at 299,792 km/s, the photons detected by modern telescopes began their cosmic voyage deep cosmic time. While that light traveled across intergalactic space, Earth's continents shifted and biological evolution shaped the history of our planet.
What does the cosmological redshift of PSN J08425627-2003112 tell us about the expansion of space? Cosmic Distance & Time
PSN J08425627-2003112's cosmological redshift z = — places it in the expanding Hubble flow. Spectroscopic redshift measures the expansion of space itself stretching the light waves toward redder wavelengths, providing a direct benchmark for calculating cosmological distances and the local Hubble constant (H₀).
How bright did PSN J08425627-2003112 become at its peak, and how many Suns does that equal? Explosion Energetics
At peak brightness, PSN J08425627-2003112 achieved an apparent magnitude of 18.4 around 2011/02/16. At this peak, the exploding star radiated with the incandescent brilliance of approximately hundreds of millions of Suns combined, briefly outshining the cumulative starlight of entire dwarf galaxies!
How much total energy was released by PSN J08425627-2003112, and where did that energy go? Explosion Energetics
The collapse of PSN J08425627-2003112's progenitor released a staggering 10⁵³ ergs of gravitational binding energy—more energy than our Sun will radiate across its entire 10-billion-year lifespan! Astonishingly, 99% of this titanic energy was emitted within 10 seconds in the form of trillions of nearly massless neutrinos. Only about 1% (10⁵¹ ergs) drove the physical kinetic blast wave, and a mere 0.01% (10⁴⁹ ergs) was radiated as the visible starlight observed by telescopes.
How fast are the supernova ejecta and shockwave of PSN J08425627-2003112 expanding through space? Explosion Energetics
The debris and shockwave of PSN J08425627-2003112 erupted into space at an astounding velocity of approximately 8,500 km/s (characteristic of this supernova class). This corresponds to roughly 2.8% of the speed of light (Mach 24,781 in air)! At this blistering speed, the expanding debris shell traverses the entire diameter of planet Earth in just 1.50 seconds, carving a giant bubble in the interstellar medium.
What powers the prolonged glow of PSN J08425627-2003112 weeks and months after detonation? Radioactive Engine
While the initial flash of PSN J08425627-2003112 was driven by shock breakout heating through the stellar envelope, its prolonged visibility over weeks and months was sustained by the radioactive decay of approximately 0.05 to 0.15 solar masses of Nickel-56 (⁵⁶Ni) forged in the core shock. As ⁵⁶Ni decays into ⁵⁶Co (half-life: 6.1 days) and then into stable ⁵⁶Fe (half-life: 77.2 days), gamma rays and positrons thermalize within the expanding ejecta, preventing the debris from instantly freezing in the vacuum of space.
What chemical elements did PSN J08425627-2003112 create and disperse into the universe? Nucleosynthesis & Elements
Core-collapse supernovae like PSN J08425627-2003112 are the primary creators of life-sustaining elements in the cosmos. The explosion manufactured and dispersed immense reservoirs of oxygen (the single most abundant heavy element in the universe), alongside carbon, nitrogen, neon, magnesium, silicon, sulfur, and calcium (which builds terrestrial bones and teeth). In the ultra-dense, neutron-rich shockwave, rapid neutron capture (r-process nucleosynthesis) forged heavy elements like gold, platinum, and uranium.
Did PSN J08425627-2003112 leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
The crushing core collapse of PSN J08425627-2003112's progenitor forged an ultra-dense compact stellar remnant at the center of the detonation. If the progenitor had an initial mass under ~20 solar masses, it left behind a neutron star (pulsar)—packing the mass of our entire Sun into a city-sized sphere barely 20 kilometers wide, spinning dozens or hundreds of times per second. If the progenitor exceeded ~25–30 solar masses, gravity overcame neutron degeneracy pressure, creating a permanent stellar-mass black hole.
What will PSN J08425627-2003112's explosion site look like in 1,000 to 10,000 years? Cosmic Remnant
Over the coming millennia, the explosion site of PSN J08425627-2003112 will undergo three dramatic evolutionary epochs: During the next few centuries (Free Expansion phase), the ejecta shell will continue expanding at thousands of km/s. Between 500 and 10,000 years (the Sedov-Taylor adiabatic phase), the forward shock will sweep up hundreds of solar masses of interstellar gas, heating it to tens of millions of degrees and glowing in bright thermal X-rays (similar to the famous Cygnus Loop or Cassiopeia A). Eventually, the cooling shock will compress nearby giant molecular clouds, triggering the gravitational collapse of new stars and solar systems!
In which galaxy did PSN J08425627-2003112 explode, and where is it located relative to the galactic center? Galactic Environment
PSN J08425627-2003112 is associated with ESO 563-14. High-precision astrometry from optical sky surveys pins the explosion coordinates directly to the galaxy's underlying stellar population.
Where is PSN J08425627-2003112 located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, PSN J08425627-2003112 is located at Right Ascension 08:42:56.27 and Declination -20:03:11.1, situated in the constellation Pyxis (The Compass). Because its declination is -20:03:11.1, it is favorably placed for Southern Hemisphere observatories.
How much Milky Way interstellar dust obscures our view of PSN J08425627-2003112? Interstellar Dust
Light from PSN J08425627-2003112 passed through interstellar dust in the Milky Way, suffering a foreground color excess of E(B-V) = 0.124 magnitudes (based on Schlafly & Finkbeiner 2011 galactic recalibrations). This cosmic dust absorbs and scatters shorter blue wavelengths, dimming the transient by approximately A_V ≈ 0.38 magnitudes in visual light.
Across which photometric filter bands was PSN J08425627-2003112 monitored? Astronomical Observations
Photometric light curves for PSN J08425627-2003112 were acquired through standard astronomical alert streams and survey programs, measuring flux across optical passbands to map its peak magnitude and fading rate.
What did astronomical spectroscopy reveal about PSN J08425627-2003112's chemical makeup? Astronomical Observations
Spectroscopic observations of PSN J08425627-2003112 confirmed its astrophysical classification by dissecting its light into individual wavelengths. Absorption and emission line features reveal the chemical composition, expansion velocity, and temperature of the expanding fireball.
Who discovered PSN J08425627-2003112 and how was it first detected? Discovery & History
PSN J08425627-2003112 was officially reported on 2011/02/16 by Stuart Parker. Discoveries are typically flagged by high-cadence robotic survey telescopes (such as ATLAS, ZTF, Pan-STARRS, ASAS-SN, or Gaia) and worldwide amateur astronomers scanning the night sky, followed by rapid spectroscopic classification by international observatories.
How many scientific publications and observatories have contributed data to PSN J08425627-2003112? Scientific Research
Data for PSN J08425627-2003112 are compiled from international astronomical notices, the IAU Transient Name Server (TNS), and peer-reviewed astrophysical journals.
How does PSN J08425627-2003112 contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
As a core-collapse supernova, PSN J08425627-2003112 provides independent cosmological distance calibrations via the Expanding Photosphere Method (EPM) and the Standard Candle Method for Type II supernovae (SCM-II). By correlating the physical expansion speed of the photosphere (measured via spectroscopic Doppler shifts) with its photometric color temperature, astronomers determine direct geometric distances independent of secondary distance ladders.
Could gravitational waves or neutrinos from PSN J08425627-2003112 be detected on Earth? Multi-Messenger Astronomy
Core-collapse supernovae like PSN J08425627-2003112 are premier targets for multi-messenger astrophysics! During the collapse of the iron core, an intense burst of 10⁵⁸ neutrinos escaped into space hours before the shock broke out through the stellar surface (as famously seen in SN 1987A). Furthermore, violent core asymmetries and non-axisymmetric core bounce can emit high-frequency gravitational waves detectable by advanced interferometers (LIGO, Virgo, KAGRA) for events within the Milky Way and Local Group.
How does PSN J08425627-2003112 compare to famous historical supernovae like SN 1987A or the Crab Supernova? Historical Comparison
Compared to historical landmarks like SN 1987A in the Large Magellanic Cloud (168,000 light-years away, naked-eye peak m = 2.9) or the Crab Supernova of 1054 (6,500 light-years away), PSN J08425627-2003112 occurred at a distance of Millions of Light-Years. While historical naked-eye supernovae occurred within our Milky Way or its immediate satellites, modern discoveries like PSN J08425627-2003112 allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see PSN J08425627-2003112 tonight with a backyard telescope or binoculars? Backyard Observation
PSN J08425627-2003112 exploded 15.6 years ago (2011/02/16). Optical transient emission has completely faded along its radioactive decay curve. Today, pointing a telescope at these coordinates reveals the expanding remnant nebula or ESO 563-14; the original optical transient is no longer detectable with amateur backyard equipment.
Does the radiation or shockwave from PSN J08425627-2003112 pose any threat to Earth? Planetary Safety
No, Earth is in zero danger. Supernovae are violent events emitting powerful gamma rays, X-rays, and cosmic rays; however, the astrophysical 'lethal kill zone' for our planet's protective ozone layer is estimated at 50 to 100 light-years. At a distance of Millions of Light-Years, the inverse-square law dilutes the radiation by quintillions of times, making PSN J08425627-2003112 completely harmless to our biosphere and purely a fascinating spectacle for human exploration.
Data sourced from IAU TNS, ALeRCE, WISeREP, and the Open Supernova Catalog. View All General Astrophysics FAQs →
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