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The Story of Supernova CSS160331:104150+314708

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)
● CSS160331:104150+314708 Explosion Site

High-magnification deep optical view into CSS160331:104150+314708'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 19.2
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
Field Transient Host
Center Coincident
🧭 Constellation
Leo Minor
The Lesser Lion
💥 Explosion Physics
Type —
Core-Collapse Supergiant
📅 Discovered On
2016/03/31
CRTS
CHAPTER I

The Iron Core Collapse of a Dying Supergiant

On 2016/03/31, astronomers scanning the heavens flagged a sudden, violent pinpoint of light that had flared into visibility. Designated CSS160331:104150+314708, it represents a catastrophic stellar explosion classified as a Type — supernova.

The progenitor of CSS160331:104150+314708 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 CSS160331:104150+314708 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 CSS160331:104150+314708 is to gaze directly into prehistoric cosmic time.

CHAPTER III

Incandescence of hundreds of millions of Suns

At the height of the outburst around 2016/03/30, CSS160331:104150+314708 surged to a peak apparent magnitude of 19.2 . 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, CSS160331:104150+314708 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. CSS160331:104150+314708 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 CSS160331:104150+314708 billions of years ago.

CHAPTER VI

Galactic Setting in Leo Minor

CSS160331:104150+314708 detonated inside an uncataloged host galaxy. In our terrestrial sky, it resides in the constellation Leo Minor (The Lesser Lion) at Right Ascension 10:41:49.67 and Declination +31:47:07.8.

CHAPTER VII

The Scientific Surveillance Campaign

Following its discovery by CRTS, observatories worldwide swung their lenses toward CSS160331:104150+314708. In the Open Supernova Catalog, CSS160331:104150+314708 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 10.5 years ago (2016/03/30). Accounting for cosmological time dilation at redshift z = 0.0000, the rest-frame age is +3835.0 days. By standard radioactive decay templates, its optical brightness has decayed by Δm ≈ 54.2 magnitudes to an estimated magnitude 73.4, rendering the transient undetectable to all ground-based observatories.

Instrument Breakdown: At its maximum brightness in 2016/03/30, it reached magnitude 19.20 (Amateur CMOS Rig). Tonight, pointing a telescope at these coordinates will reveal only the background host galaxy.

Instrument Class & Aperture Sensitivity Limit At Peak Maximum (m=19.20) Tonight (Est. m≈73.4)
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 CSS160331:104150+314708 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 CSS160331:104150+314708 in discovery time, spatial sky neighborhood, and cosmological lookback epoch:

⏱️ Closest in Time
CSS160331:112412+314347 Exploded same day
Type Transient 2016/03/31 · Mag 19.1
Gaia16ajs Exploded same day
Type Candidate 2016/03/31 · Mag 18.7
Gaia16ajx Exploded same day
Type Candidate 2016/03/31 · Mag 18.6
🔭 Closest on the Sky
AT2018ivw 9.0′ away
Type Candidate Discovered 2018/11/07
CSS101214:104318+313513 22.3′ away
Type Transient Discovered 2010/12/14
AT2022xe 33.2′ away
Type Candidate Discovered 2022/01/11
🌌 Same Cosmic Era (Redshift)
Redshift data unavailable for cosmic distance matching.

❓ Frequently Asked Questions About CSS160331:104150+314708

Scientific & observational Q&As indexed from astronomical databases & the Open Supernova Catalog
What type of supernova is CSS160331:104150+314708 and what kind of star exploded? Astrophysics & Progenitor
CSS160331:104150+314708 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 CSS160331:104150+314708? Astrophysics & Progenitor
Before detonating as CSS160331:104150+314708, 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 CSS160331:104150+314708 from Earth and how old is the light reaching us? Cosmic Distance & Time
CSS160331:104150+314708 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 CSS160331:104150+314708 tell us about the expansion of space? Cosmic Distance & Time
CSS160331:104150+314708'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 CSS160331:104150+314708 become at its peak, and how many Suns does that equal? Explosion Energetics
At peak brightness, CSS160331:104150+314708 achieved an apparent magnitude of 19.2 around 2016/03/30. 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 CSS160331:104150+314708, and where did that energy go? Explosion Energetics
The collapse of CSS160331:104150+314708'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 CSS160331:104150+314708 expanding through space? Explosion Energetics
The debris and shockwave of CSS160331:104150+314708 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 CSS160331:104150+314708 weeks and months after detonation? Radioactive Engine
While the initial flash of CSS160331:104150+314708 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 CSS160331:104150+314708 create and disperse into the universe? Nucleosynthesis & Elements
Core-collapse supernovae like CSS160331:104150+314708 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 CSS160331:104150+314708 leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
The crushing core collapse of CSS160331:104150+314708'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 CSS160331:104150+314708's explosion site look like in 1,000 to 10,000 years? Cosmic Remnant
Over the coming millennia, the explosion site of CSS160331:104150+314708 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 CSS160331:104150+314708 explode, and where is it located relative to the galactic center? Galactic Environment
CSS160331:104150+314708 is associated with an uncataloged host galaxy. High-precision astrometry from optical sky surveys pins the explosion coordinates directly to the galaxy's underlying stellar population.
Where is CSS160331:104150+314708 located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, CSS160331:104150+314708 is located at Right Ascension 10:41:49.67 and Declination +31:47:07.8, situated in the constellation Leo Minor (The Lesser Lion). Because its declination is +31:47:07.8, it is primarily placed in the Northern celestial hemisphere.
How much Milky Way interstellar dust obscures our view of CSS160331:104150+314708? Interstellar Dust
Light from CSS160331:104150+314708 passed through interstellar dust in the Milky Way, suffering a foreground color excess of E(B-V) = 0.018 magnitudes (based on Schlafly & Finkbeiner 2011 galactic recalibrations). This cosmic dust absorbs and scatters shorter blue wavelengths, dimming the transient by approximately A_V ≈ 0.06 magnitudes in visual light.
Across which photometric filter bands was CSS160331:104150+314708 monitored? Astronomical Observations
Photometric light curves for CSS160331:104150+314708 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 CSS160331:104150+314708's chemical makeup? Astronomical Observations
Spectroscopic observations of CSS160331:104150+314708 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 CSS160331:104150+314708 and how was it first detected? Discovery & History
CSS160331:104150+314708 was officially reported on 2016/03/31 by CRTS. 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 CSS160331:104150+314708? Scientific Research
Data for CSS160331:104150+314708 are compiled from international astronomical notices, the IAU Transient Name Server (TNS), and peer-reviewed astrophysical journals.
How does CSS160331:104150+314708 contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
As a core-collapse supernova, CSS160331:104150+314708 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 CSS160331:104150+314708 be detected on Earth? Multi-Messenger Astronomy
Core-collapse supernovae like CSS160331:104150+314708 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 CSS160331:104150+314708 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), CSS160331:104150+314708 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 CSS160331:104150+314708 allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see CSS160331:104150+314708 tonight with a backyard telescope or binoculars? Backyard Observation
CSS160331:104150+314708 exploded 10.5 years ago (2016/03/31). Optical transient emission has completely faded along its radioactive decay curve. Today, pointing a telescope at these coordinates reveals the expanding remnant nebula or an uncataloged host galaxy; the original optical transient is no longer detectable with amateur backyard equipment.
Does the radiation or shockwave from CSS160331:104150+314708 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 CSS160331:104150+314708 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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