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Type Ia Supernova

The Story of Supernova SN2016fij

An extraordinary stellar explosion that occurred 577.9 Million Light-Years away in deep space.

⏱️ ~8 min deep read 🔬 24 Astrophysical Q&As 🔭 Viewing Guide Included 🪐 Constellation Sculptor
🔭 Deep Field (~2.1′ FOV) · Highest-Definition Optical Field (0.25″/pix)
● SN2016fij Explosion Site

High-magnification deep optical view into SN2016fij'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
577.9 Million Light-Years
Lookback Cosmic Time
✨ Peak Brightness
Mag 16.8
Astro Camera (CCD)
☀️ Peak Radiance
4.9 billion Suns
Combined Stellar Energy
🚀 Shock Velocity
~11,400 km/s
~3.8% Speed of Light
🌌 Host Galaxy
2dFGRS S501Z101
Offset: 10.20″ (8.12 kpc)
🧭 Constellation
Sculptor
The Sculptor
💥 Explosion Physics
Type Ia
Thermonuclear White Dwarf
📅 Discovered On
2016/08/15
ASAS-SN
CHAPTER I

The Thermonuclear Obliteration of a White Dwarf

On 2016/08/15, astronomers scanning the heavens flagged a sudden, violent pinpoint of light that had flared into visibility. Designated SN2016fij, it represents a catastrophic stellar explosion classified as a Type Ia supernova.

In a binary star system located deep within 2dFGRS S501Z101, 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.

Astrophysical Mechanism Summary
Type: Type Ia • Progenitor: Carbon-Oxygen White Dwarf (Binary System) • Velocity: ~11,400 km/s (~3.8% c)
CHAPTER II

A Message Across Deep Cosmic Time

The light from SN2016fij is a dispatch from an ancient past. Located approximately 577.9 Million Light-Years away (redshift z = 0.0389), the photons detected by telescopes today began their journey 577.9 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 SN2016fij is to gaze directly into prehistoric cosmic time.

CHAPTER III

Incandescence of 4.9 billion Suns

At the height of the outburst around 2016/08/24, SN2016fij surged to a peak apparent magnitude of 16.8 and an intrinsic absolute magnitude of -19.4. At that instant, this single dying star radiated with the collective power of approximately 4.9 billion 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.

CHAPTER IV

The Radioactive Furnace: Why Supernovae Glow for Months

Unlike a conventional terrestrial explosion that cools and goes dark in seconds, SN2016fij 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. SN2016fij 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 SN2016fij billions of years ago.

CHAPTER VI

Galactic Setting in Sculptor

SN2016fij detonated inside 2dFGRS S501Z101, positioned at an offset of 10.20″ (8.12 kpc) from the galactic nucleus. In our terrestrial sky, it resides in the constellation Sculptor (The Sculptor) at Right Ascension 00:46:56.320 and Declination -33:47:35.59.

CHAPTER VII

The Scientific Surveillance Campaign

Following its discovery by ASAS-SN, observatories worldwide swung their lenses toward SN2016fij. In the Open Supernova Catalog, SN2016fij 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.

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 10.1 years ago (2016/08/24). Accounting for cosmological time dilation at redshift z = 0.0389, the rest-frame age is +3548.9 days. By standard radioactive decay templates, its optical brightness has decayed by Δm ≈ 54.6 magnitudes to an estimated magnitude 71.4, rendering the transient undetectable to all ground-based observatories.

Instrument Breakdown: At its maximum brightness in 2016/08/24, it reached magnitude 16.80 (Amateur CMOS Rig). Tonight, pointing a telescope at these coordinates will reveal only the background host galaxy (2dFGRS S501Z101).

Instrument Class & Aperture Sensitivity Limit At Peak Maximum (m=16.80) Tonight (Est. m≈71.4)
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 SN2016fij was a titanic explosion, our planet sits safely outside the lethal 50–100 light-year kill zone. At a distance of 577.9 Million Light-Years, the blast poses zero physical hazard to Earth's biosphere.

🌌 Cosmic Neighbors & Contemporaries 110,222+ Transients Indexed

Cataloged supernovae closest to SN2016fij in discovery time, spatial sky neighborhood, and cosmological lookback epoch:

⏱️ Closest in Time
DES16X1ge Exploded same day
Type Ia 2016/08/15 · Mag 21.1
Gaia16bbc Exploded same day
Type Candidate 2016/08/15 · Mag 18.64
Gaia16bbd Exploded same day
Type Candidate 2016/08/15 · Mag 18.16
🔭 Closest on the Sky
AT2017frn 27.3′ away
Type Candidate Discovered 2017/07/18
SN2024abqq 38.3′ away
Type Ia Discovered 2024/11/21
SN2010ma 52.5′ away
Type Ic BL Discovered 2010/12/19
🌌 Same Cosmic Era (Redshift)
SN2008O z = 0.0389
Type Ia ~532.9 Mly lookback
PTF11byi z = 0.0389
Type Ia ~532.9 Mly lookback
SN2010cy z = 0.0389
Type Ia ~532.9 Mly lookback

❓ Frequently Asked Questions About SN2016fij

Scientific & observational Q&As indexed from astronomical databases & the Open Supernova Catalog
🔍 24 of 24
What type of supernova is SN2016fij and what kind of star exploded? Astrophysics & Progenitor
SN2016fij is classified as a Type Ia Supernova—the complete thermonuclear detonation of an ultra-dense carbon-oxygen white dwarf star. In a binary system, the white dwarf siphoned material from a companion star (or merged with a second white dwarf) until reaching the Chandrasekhar limit (~1.4 solar masses). At this critical threshold, uncontrollable carbon and oxygen fusion detonated through the stellar interior in less than a second with supersonic speeds exceeding 10,000 km/s. Because their peak absolute luminosities follow remarkably consistent empirical relations (the Phillips relation), Type Ia supernovae serve as 'Standard Candles' for measuring cosmological distances and the accelerated expansion of the universe.
What was the progenitor star doing in the millions of years leading up to SN2016fij? Astrophysics & Progenitor
The progenitor of SN2016fij began billions of years ago as a modest intermediate-mass star (1 to 8 solar masses). After exhausting its core hydrogen and helium, it expelled its outer envelope as a glowing planetary nebula, leaving behind a dense carbon-oxygen white dwarf the size of Earth but with the mass of the Sun. For millions or billions of years, it orbited in a close binary system, gradually accreting hydrogen- and helium-rich gas from its stellar companion until gravitational compression pushed its core temperature past the threshold of runaway carbon ignition.
How far away is SN2016fij from Earth and how old is the light reaching us? Cosmic Distance & Time
SN2016fij is located approximately 577.9 Million Light-Years from Earth (cosmological redshift z = 0.0389, luminosity distance d_L = 177.2). Because electromagnetic radiation travels at 299,792 km/s, the photons detected by modern telescopes began their cosmic voyage 577.9 million years ago during the Paleozoic era, long before the first dinosaurs appeared on Earth. 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 SN2016fij tell us about the expansion of space? Cosmic Distance & Time
SN2016fij exhibits a measured spectroscopic redshift of z = 0.0389. Under Hubble's Law, this redshift corresponds to an apparent recessional velocity of approximately 11,661.9 km/s away from our Milky Way galaxy. This redshift is not motion through space alone, but the stretching of light waves as the fabric of the universe itself expanded during the millions of years the photons traveled to our telescopes.
How bright did SN2016fij become at its peak, and how many Suns does that equal? Explosion Energetics
At peak brightness, SN2016fij achieved an apparent magnitude of 16.8 around 2016/08/24. Corrected for cosmic distance and foreground interstellar dust, its intrinsic absolute magnitude was -19.4. At this peak, the exploding star radiated with the incandescent brilliance of approximately 4.9 billion Suns combined, briefly outshining the cumulative starlight of entire dwarf galaxies!
How much total energy was released by SN2016fij, and where did that energy go? Explosion Energetics
The thermonuclear explosion of SN2016fij released approximately 10⁵¹ ergs of energy (1 Bethe or 1 foe), equivalent to 10²⁸ megatons of TNT! Virtually all of this energy was converted into the kinetic blast wave and the radioactive synthesis of heavy isotopes. Because Type Ia supernovae lack a gravitational core collapse into a neutron star, neutrino emission was minimal (~1%), and the blast converted its full binding energy into the kinetic destruction of the white dwarf.
How fast are the supernova ejecta and shockwave of SN2016fij expanding through space? Explosion Energetics
The debris and shockwave of SN2016fij erupted into space at an astounding velocity of approximately 11,400 km/s (measured spectroscopically). This corresponds to roughly 3.8% of the speed of light (Mach 33,236 in air)! At this blistering speed, the expanding debris shell traverses the entire diameter of planet Earth in just 1.12 seconds, carving a giant bubble in the interstellar medium.
What powers the prolonged glow of SN2016fij weeks and months after detonation? Radioactive Engine
The brilliant light curve of SN2016fij is energized by the radioactive decay of heavy isotopes synthesized during detonation. The blast produced approximately 0.5 to 0.7 solar masses of radioactive Nickel-56 (⁵⁶Ni). ⁵⁶Ni decays with a half-life of 6.075 days into Cobalt-56 (⁵⁶Co), emitting energetic gamma rays that heat the opaque expanding fireball to power the optical peak. Subsequently, ⁵⁶Co decays into stable Iron-56 (⁵⁶Fe) with a half-life of 77.2 days, governing the smooth, exponential decline tail observed over the following year.
What chemical elements did SN2016fij create and disperse into the universe? Nucleosynthesis & Elements
As a thermonuclear Type Ia explosion, SN2016fij functioned as a premier cosmic foundry for iron-peak elements. The detonation synthesized over half a solar mass of Iron-56 (⁵⁶Fe)—the exact element that forms Earth's dense metallic core and binds oxygen in human red blood cells! It also forged substantial quantities of silicon (producing the hallmark Si II λ6355 absorption dip), sulfur, calcium, argon, and titanium, enriching the interstellar clouds that condense into future planetary systems.
Did SN2016fij leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
Nothing remains at the center. Because a Type Ia supernova involves the total thermonuclear disruption of the progenitor white dwarf, the entire star was incinerated and flung into space. There is no central neutron star, pulsar, or black hole left behind. The star's entire mass now exists as an expanding gaseous shell traveling through the host galaxy.
What will SN2016fij's explosion site look like in 1,000 to 10,000 years? Cosmic Remnant
Over the coming millennia, the explosion site of SN2016fij 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 SN2016fij explode, and where is it located relative to the galactic center? Galactic Environment
SN2016fij occurred in 2dFGRS S501Z101, located at an offset of 10.20″ (8.12 kpc) from the galactic nucleus. In optical and infrared imaging, this positions the explosion within the galaxy's active stellar disk or spiral arms, where ongoing star formation constantly generates massive short-lived stellar progenitors.
Where is SN2016fij located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, SN2016fij is located at Right Ascension 00:46:56.320 and Declination -33:47:35.59, situated in the constellation Sculptor (The Sculptor). Because its declination is -33:47:35.59, it is favorably placed for Southern Hemisphere observatories.
How much Milky Way interstellar dust obscures our view of SN2016fij? Interstellar Dust
Light from SN2016fij passed through interstellar dust in the Milky Way, suffering a foreground color excess of E(B-V) = 0.011 magnitudes (based on Schlafly & Finkbeiner 2011 galactic recalibrations). This cosmic dust absorbs and scatters shorter blue wavelengths, dimming the transient by approximately A_V ≈ 0.04 magnitudes in visual light.
Across which photometric filter bands was SN2016fij monitored? Astronomical Observations
SN2016fij was tracked across 1 photometric observations utilizing filter bands including optical filters. Data were captured by observatories and survey networks including global optical observatories. Multi-color photometry tracks the temperature evolution of the fireball, verifying the rise time to peak and the rate of radioactive decline.
What did astronomical spectroscopy reveal about SN2016fij's chemical makeup? Astronomical Observations
Spectroscopic observations of SN2016fij 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 SN2016fij and how was it first detected? Discovery & History
SN2016fij was officially reported on 2016/08/15 by ASAS-SN. 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 SN2016fij? Scientific Research
SN2016fij is documented across 7 scientific references and archival data sources in the Open Supernova Catalog. These include discovery circulars and research datasets from ATel 9407, ATel 9461, 2016A&A...594A..13P, 2011ApJ...737..103S. All raw photometry and spectroscopy points are cross-indexed to their original bibliographic records for peer-reviewed verification.
What other names and survey identifiers exist for SN2016fij? Cross-Identifications
Throughout global alert streams and survey databases, SN2016fij has also been designated as: AT2016fij, ASASSN-16jh. These cross-matched identifiers allow astronomers to cross-reference observations across the Zwicky Transient Facility (ZTF), the Asteroid Terrestrial-impact Last Alert System (ATLAS), Pan-STARRS, Gaia Photometric Science Alerts, and the IAU Transient Name Server (TNS).
How does SN2016fij contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
Because SN2016fij is a Type Ia supernova, it serves as an indispensable rung on the Cosmic Distance Ladder. Astrophysicists utilize the Phillips relation—a tight empirical correlation between peak absolute magnitude and light curve decline rate (Δm₁₅)—to standardize its luminosity. By comparing this calibrated intrinsic brightness with observed apparent magnitude, researchers calculate precise geometric distances across the universe, providing key empirical tests of the Hubble constant (H₀) and dark energy.
Could gravitational waves or neutrinos from SN2016fij be detected on Earth? Multi-Messenger Astronomy
For thermonuclear explosions like SN2016fij, gravitational wave and neutrino emissions are negligible compared to core-collapse events. However, multi-messenger radio and X-ray observations are crucial: detecting synchrotron radio emission would reveal circumstellar gas shed by a companion star, helping settle the century-old debate between single-degenerate and double-degenerate white dwarf progenitor channels.
How does SN2016fij 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), SN2016fij occurred at a distance of 577.9 Million Light-Years. While historical naked-eye supernovae occurred within our Milky Way or its immediate satellites, modern discoveries like SN2016fij allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see SN2016fij tonight with a backyard telescope or binoculars? Backyard Observation
SN2016fij exploded 10.1 years ago (2016/08/15). Optical transient emission has completely faded along its radioactive decay curve. Today, pointing a telescope at these coordinates reveals the expanding remnant nebula or 2dFGRS S501Z101; the original optical transient is no longer detectable with amateur backyard equipment.
Does the radiation or shockwave from SN2016fij 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 577.9 Million Light-Years, the inverse-square law dilutes the radiation by quintillions of times, making SN2016fij 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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