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Type CV Supernova

The Story of Supernova AT2025qzw

An extraordinary stellar explosion that occurred 0 Light-Years away in deep space.

⏱️ ~8 min deep read 🔬 24 Astrophysical Q&As 🔭 Viewing Guide Included 🪐 Constellation Vulpecula
🔭 Deep Field (~2.1′ FOV) · Highest-Definition Optical Field (0.25″/pix)
● AT2025qzw Explosion Site

High-magnification deep optical view into AT2025qzw'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
0 Light-Years
Lookback Cosmic Time
✨ Peak Brightness
Mag 17.63 (L)
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
Vulpecula
The Fox
💥 Explosion Physics
Type CV
Core-Collapse Supergiant
📅 Discovered On
2025/07/13
D. O'Neill, G. Ramsay, K. Ackley, M. Dyer, J. Lyman, K. Ulaczyk, D. Steeghs, D. Galloway, V. Dhillon, P. O'Brien, K. Noysena, R. Kotak, R. Breton, J. Casares, L. Nuttall, B. Godson, T. Killestein, A. Kumar, M. Pursiainen, on behalf of GOTO collaboration
CHAPTER I

The Iron Core Collapse of a Dying Supergiant

On 2025/07/13, astronomers scanning the heavens flagged a sudden, violent pinpoint of light that had flared into visibility. Designated AT2025qzw, it represents a catastrophic stellar explosion classified as a Type CV supernova.

The progenitor of AT2025qzw 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 CV • 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 AT2025qzw is a dispatch from an ancient past. Located approximately 0 Light-Years away (redshift z = 0), 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 AT2025qzw is to gaze directly into prehistoric cosmic time.

CHAPTER III

Incandescence of hundreds of millions of Suns

At the height of the outburst around 2025/07/13 (MJD 60869.1), AT2025qzw surged to a peak apparent magnitude of 17.63 (L) . 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, AT2025qzw 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. AT2025qzw 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 AT2025qzw billions of years ago.

CHAPTER VI

Galactic Setting in Vulpecula

AT2025qzw detonated inside an uncataloged host galaxy. In our terrestrial sky, it resides in the constellation Vulpecula (The Fox) at Right Ascension 21:06:38.509 and Declination +24:54:15.67.

CHAPTER VII

The Scientific Surveillance Campaign

Following its discovery by D. O'Neill, G. Ramsay, K. Ackley, M. Dyer, J. Lyman, K. Ulaczyk, D. Steeghs, D. Galloway, V. Dhillon, P. O'Brien, K. Noysena, R. Kotak, R. Breton, J. Casares, L. Nuttall, B. Godson, T. Killestein, A. Kumar, M. Pursiainen, on behalf of GOTO collaboration, observatories worldwide swung their lenses toward AT2025qzw. In the Open Supernova Catalog, AT2025qzw is documented across 1 photometric measurements in passbands such as L 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? The outburst is recent, and the flash has faded.

This is one of the newer supernovae in the catalog, discovered 471 days ago (2025/07/13 (MJD 60869.1)). It is not an ancient explosion. The radioactive tail has dropped the estimated brightness by Δm ≈ 7.1 to about magnitude 24.7, which is past the window of binoculars and small backyard telescopes.

What that brightness means: Giant 8m–10m Observatories. Coordinates tonight still point at the host galaxy.

Instrument Class & Aperture Sensitivity Limit At Peak Maximum (m=17.63) Tonight (Est. m≈24.7)
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 ✅ Detectable
Space Observatories Only
Hubble Space Telescope (WFC3) / JWST (NIRCam deep stack)
 m ≤ 30.0 ✅ Detectable ✅ Detectable

Planetary Safety Note: Even though AT2025qzw was a titanic explosion, our planet sits safely outside the lethal 50–100 light-year kill zone. At a distance of 0 Light-Years, the blast poses zero physical hazard to Earth's biosphere.

🌌 Cosmic Neighbors & Contemporaries 110,222+ Transients Indexed

Cataloged supernovae closest to AT2025qzw in discovery time, spatial sky neighborhood, and cosmological lookback epoch:

⏱️ Closest in Time
SN2025rao Exploded same day
Type II 2025/07/13
SN2025rby Exploded same day
Type Ia 2025/07/13
SN2025rcl Exploded same day
Type Ia 2025/07/13
🔭 Closest on the Sky
AT2021yes 26.4′ away
Type Candidate Discovered 2021/09/01
iPTF14goa 31.0′ away
Type Ia Discovered 2014/10/13
SN2023umn 54.5′ away
Type Ia Discovered 2023/10/09
🌌 Same Cosmic Era (Redshift)
SN1987A z = 9.51e-06
Type II Pec ~0.1 Mly lookback
AT2021bgj z = 1.13e-05
Type Candidate ~0.2 Mly lookback
Gaia20dff z = 1.13e-05
Type Be ~0.2 Mly lookback

❓ Frequently Asked Questions About AT2025qzw

Scientific & observational Q&As indexed from astronomical databases & the Open Supernova Catalog
🔍 24 of 24
What type of supernova is AT2025qzw and what kind of star exploded? Astrophysics & Progenitor
AT2025qzw is cataloged as a Type CV 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 AT2025qzw? Astrophysics & Progenitor
Before detonating as AT2025qzw, 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 AT2025qzw from Earth and how old is the light reaching us? Cosmic Distance & Time
AT2025qzw is located approximately 0 Light-Years from Earth (cosmological redshift z = 0, luminosity distance d_L = 0.00). 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 AT2025qzw tell us about the expansion of space? Cosmic Distance & Time
AT2025qzw exhibits a measured spectroscopic redshift of z = 0.0000. Under Hubble's Law, this redshift corresponds to an apparent recessional velocity of approximately 0.0 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 AT2025qzw become at its peak, and how many Suns does that equal? Explosion Energetics
At peak brightness, AT2025qzw achieved an apparent magnitude of 17.63 (L) around 2025/07/13 (MJD 60869.1). 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 AT2025qzw, and where did that energy go? Explosion Energetics
The collapse of AT2025qzw'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 AT2025qzw expanding through space? Explosion Energetics
The debris and shockwave of AT2025qzw 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 AT2025qzw weeks and months after detonation? Radioactive Engine
While the initial flash of AT2025qzw 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 AT2025qzw create and disperse into the universe? Nucleosynthesis & Elements
Core-collapse supernovae like AT2025qzw 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 AT2025qzw leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
The crushing core collapse of AT2025qzw'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 AT2025qzw's explosion site look like in 1,000 to 10,000 years? Cosmic Remnant
Over the coming millennia, the explosion site of AT2025qzw 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 AT2025qzw explode, and where is it located relative to the galactic center? Galactic Environment
AT2025qzw 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 AT2025qzw located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, AT2025qzw is located at Right Ascension 21:06:38.509 and Declination +24:54:15.67, situated in the constellation Vulpecula (The Fox). Because its declination is +24:54:15.67, it is primarily placed in the Northern celestial hemisphere.
How much Milky Way interstellar dust obscures our view of AT2025qzw? Interstellar Dust
Light from AT2025qzw passed through interstellar dust in the Milky Way, suffering a foreground color excess of E(B-V) = 0.136 magnitudes (based on Schlafly & Finkbeiner 2011 galactic recalibrations). This cosmic dust absorbs and scatters shorter blue wavelengths, dimming the transient by approximately A_V ≈ 0.42 magnitudes in visual light.
Across which photometric filter bands was AT2025qzw monitored? Astronomical Observations
AT2025qzw was tracked across 1 photometric observations utilizing filter bands including L. Data were captured by observatories and survey networks including GOTO. 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 AT2025qzw's chemical makeup? Astronomical Observations
Spectroscopic observations of AT2025qzw 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 AT2025qzw and how was it first detected? Discovery & History
AT2025qzw was officially reported on 2025/07/13 by D. O'Neill, G. Ramsay, K. Ackley, M. Dyer, J. Lyman, K. Ulaczyk, D. Steeghs, D. Galloway, V. Dhillon, P. O'Brien, K. Noysena, R. Kotak, R. Breton, J. Casares, L. Nuttall, B. Godson, T. Killestein, A. Kumar, M. Pursiainen, on behalf of GOTO collaboration. 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 AT2025qzw? Scientific Research
AT2025qzw is documented across 3 scientific references and archival data sources in the Open Supernova Catalog. These include discovery circulars and research datasets from Transient Name Server, 2025TNSTR2675....1O, The Open Supernova Catalog. 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 AT2025qzw? Cross-Identifications
Throughout global alert streams and survey databases, AT2025qzw has also been designated as: 2025qzw, GOTO25etu, SN2025qzw, AT 2025qzw. 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 AT2025qzw contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
As a core-collapse supernova, AT2025qzw 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 AT2025qzw be detected on Earth? Multi-Messenger Astronomy
Core-collapse supernovae like AT2025qzw 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 AT2025qzw 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), AT2025qzw occurred at a distance of 0 Light-Years. While historical naked-eye supernovae occurred within our Milky Way or its immediate satellites, modern discoveries like AT2025qzw allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see AT2025qzw tonight with a backyard telescope or binoculars? Backyard Observation
Discovered 471 days ago (2025/07/13), AT2025qzw has passed peak maximum and is fading along its radioactive Co-56 decay tail at an estimated apparent magnitude of m ≈ 24.7. It is accessible with sensitive amateur astrophotography rigs or larger research telescopes, depending on local sky darkness.
Does the radiation or shockwave from AT2025qzw 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 0 Light-Years, the inverse-square law dilutes the radiation by quintillions of times, making AT2025qzw 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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