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Type SLSN-I Supernova

The Story of Supernova SN2022czy

An extraordinary stellar explosion that occurred 1.72 Billion Light-Years away in deep space.

⏱️ ~6 min deep read 🔬 24 Astrophysical Q&As 🔭 Viewing Guide Included 🪐 Constellation Coma Berenices
🔭 Deep Field (~2.1′ FOV) · DSS2 Optical (China-VO mirror)
● SN2022czy Explosion Site

High-magnification deep optical view into SN2022czy'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
1.72 Billion Light-Years
Lookback Cosmic Time
✨ Peak Brightness
Mag 19
Large Observatory
☀️ Peak Radiance
5.4 billion Suns
Combined Stellar Energy
🚀 Shock Velocity
~31,000 km/s
~10.3% Speed of Light
🌌 Host Galaxy
Field Transient Host
Center Coincident
🧭 Constellation
Coma Berenices
Berenice's Hair
💥 Explosion Physics
Type SLSN-I
Core-Collapse Supergiant
📅 Discovered On
2022/02/22
ATLAS
CHAPTER I

A Core-Collapse Class Transient

On 2022/02/22, astronomers scanning the heavens flagged a sudden, violent pinpoint of light that had flared into visibility. Designated SN2022czy, it represents a catastrophic stellar explosion classified as a Type SLSN-I supernova.

SN2022czy is classified in a core-collapse spectroscopic family. Events of this class are generally linked to the death of a massive star after successive nuclear burning stages, but no unique progenitor mass, lifetime, or pre-explosion identification is established for this object. The narrative of onion-shell fusion ending in iron-core collapse describes the class model, not a measured biography of SN2022czy.

Astrophysical Mechanism Summary
Type: Type SLSN-I • Progenitor: Massive Red/Stripped Supergiant Star • Velocity: ~31,000 km/s (~10.3% c)
CHAPTER II

A Message Across Deep Cosmic Time

SN2022czy has a luminosity distance of approximately 1.72 Billion Light-Years (redshift z = 0.11). That figure is not the light-travel time: under flat ΛCDM the lookback time is ≈1422 Myr, when the light set out 1421.6 million years ago in deep Precambrian time, well before multicellular animals dominated Earth.

Luminosity distance incorporates cosmic expansion and exceeds the light-travel distance. The two quantities must be reported separately.

CHAPTER III

Incandescence of 5.4 billion Suns

At the height of the outburst around 2022/02/21, SN2022czy surged to a peak apparent magnitude of 19 and an intrinsic absolute magnitude of -19.5. At that instant, this single dying star radiated with the collective power of approximately 5.4 billion Suns combined, outshining whole dwarf galaxies.

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

After peak, many supernovae are powered by the radioactive chain ⁵⁶Ni → ⁵⁶Co → ⁵⁶Fe. That is the standard model for Type SLSN-I light curves; an object-specific nickel mass for SN2022czy is not published here.

Nickel-56 decays to Cobalt-56 (half-life ≈6.1 days), then to stable Iron-56 (half-life ≈77.2 days), heating the ejecta from within. Typical class yields must not be quoted as measured values for this event.

CHAPTER V

Cosmic Kiln: Seeding the Elements of Life

Supernovae enrich galaxies with heavy elements. Events of SN2022czy's class are associated with oxygen-group and intermediate-mass products (O, C, Ne, Mg, Si) in galactic chemical-evolution models. No measured elemental yields are published for SN2022czy.

As Carl Sagan observed, "We are made of star-stuff" — a statement about nucleosynthesis in general, not a claim that atoms from this specific remnant are identified in the Solar System.

CHAPTER VI

Galactic Setting in Coma Berenices

No host galaxy is identified for SN2022czy in this catalog record . In our terrestrial sky, it resides in the constellation Coma Berenices (Berenice's Hair) at Right Ascension 12:22:01.154 and Declination +16:59:44.55.

CHAPTER VII

The Scientific Surveillance Campaign

Following its discovery by ATLAS, observatories worldwide swung their lenses toward SN2022czy. In the Open Supernova Catalog, SN2022czy 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? Unknown — no measured brightness.

Discovered 4.7 years ago (2022/02/22). No reliable current brightness estimate — no photometry has been published.

Planetary Safety Note: Even though SN2022czy was a titanic explosion, our planet sits safely outside the lethal 50–100 light-year kill zone. At a distance of 1.72 Billion Light-Years, the blast poses zero physical hazard to Earth's biosphere.

🌌 Cosmic Neighbors & Contemporaries 105,768+ transients indexed

Cataloged transients closest to SN2022czy in discovery time, spatial sky neighborhood, and cosmological redshift:

⏱️ Closest in Time
AT2022cye Exploded same day
Type Candidate 2022/02/22 · Mag 19
AT2022cyf Exploded same day
Type Candidate 2022/02/22 · Mag 18.8
AT2022cyg Exploded same day
Type Candidate 2022/02/22 · Mag 18.8
🔭 Closest on the Sky
TDE2022czy 0.0′ away
Type TDE Discovered 2022/02/22
PSN J12204403+1650448 20.5′ away
Type Transient Discovered 2015/05/12
SN2022zzz 26.2′ away
Type II Discovered 2022/11/12
🌌 Same Cosmic Era (Redshift)
SN1996aj z = 0.11
Type Ia ~1518.0 Mly (approx.)
SN1998ep z = 0.11
Type Ia ~1518.0 Mly (approx.)
SN1996S z = 0.11
Type II ~1518.0 Mly (approx.)

❓ Frequently Asked Questions About SN2022czy

Scientific & observational Q&As indexed from astronomical databases & the Open Supernova Catalog
🔍 24 of 24
What type of supernova is SN2022czy and what kind of star exploded? Astrophysics & Progenitor
SN2022czy is classified as a superluminous supernova (SLSN). Proposed power sources include magnetar spin-down and ejecta–CSM interaction; which engine applies to this object is not established from the classification label alone.
What was the progenitor star doing in the millions of years leading up to SN2022czy? Astrophysics & Progenitor
The specific progenitor of SN2022czy has not been observed. Events of this spectroscopic class are generally associated with massive-star core collapse after successive nuclear burning stages (hydrogen → helium → carbon → neon → oxygen → silicon → iron). Typical lifetimes of such progenitors are tens of millions of years, but that is a class expectation—not a measured age or evolutionary track for this star. No pre-explosion imaging identification is cited in the available record for SN2022czy.
How far away is SN2022czy from Earth and how old is the light reaching us? Cosmic Distance & Time
SN2022czy has a luminosity distance of approximately 1.72 Billion Light-Years (redshift z = 0.11, d_L = 526). Under a flat ΛCDM cosmology (H₀≈70 km/s/Mpc, Ωₘ≈0.3), the corresponding lookback time is ≈1422 Myr — when the light set out 1421.6 million years ago in deep Precambrian time, well before multicellular animals dominated Earth. Luminosity distance is larger than the light-travel distance because cosmic expansion stretches the path; the two must not be equated.
What does the cosmological redshift of SN2022czy tell us about the expansion of space? Cosmic Distance & Time
SN2022czy exhibits a measured spectroscopic redshift of z = 0.1100. The cockpit reports a user-facing recession velocity of 31,173.3 km/s, computed as the redshift Doppler-equivalent v = c·((1+z)²−1)/((1+z)²+1). Cosmological redshift is not generally equivalent to special-relativistic motion through space; this number is a convenient velocity label for z, not a measured peculiar velocity and not supernova ejecta speed. Bare c·z (≈32,977 km/s) is a different low-z approximation and is not mixed here.
How bright did SN2022czy become at its peak, and how many Suns does that equal? Explosion Energetics
At peak brightness, SN2022czy achieved an apparent magnitude of 19 around 2022/02/21. Corrected for cosmic distance and foreground interstellar dust, its intrinsic absolute magnitude was -19.5. At this peak, the exploding star radiated with the incandescent brilliance of approximately 5.4 billion Suns combined, briefly outshining the cumulative starlight of entire dwarf galaxies!
How much total energy was released by SN2022czy, and where did that energy go? Explosion Energetics
SLSN radiated energies can exceed ordinary supernovae by large factors, but the power source (magnetar, CSM interaction, or other) is model-dependent. No object-specific energy release is published for SN2022czy.
How fast are the supernova ejecta and shockwave of SN2022czy expanding through space? Explosion Energetics
Spectroscopic line blueshifts imply an ejecta velocity of approximately 31,000 km/s (~10.3% of c) for SN2022czy. This is distinct from cosmological recession velocity inferred from redshift.
What powers the prolonged glow of SN2022czy weeks and months after detonation? Radioactive Engine
SLSN light curves may be powered by magnetar spin-down, CSM interaction, or (in some models) large ⁵⁶Ni masses. Which engine powers SN2022czy is not established here, and no object-specific nickel mass is published.
What chemical elements did SN2022czy create and disperse into the universe? Nucleosynthesis & Elements
Events of SN2022czy's broad spectroscopic class are discussed in galactic chemical evolution as sources of oxygen-group and intermediate-mass elements (and, for some channels, iron-peak material). No measured elemental yields are published for SN2022czy.
Did SN2022czy leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
A core-collapse explosion associated with SN2022czy's class forges 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 SN2022czy's explosion site look like in 1,000 to 10,000 years? Cosmic Remnant
Supernova remnants in general evolve through free-expansion, Sedov–Taylor, and radiative phases over centuries to millennia, sometimes becoming bright X-ray shells and occasionally compressing nearby molecular clouds. These are standard remnant-evolution models, not forecasts measured for SN2022czy. Whether this site will trigger star formation, reach particular X-ray temperatures, or match Cassiopeia A depends on local density and magnetic field—none of which are constrained by the data shown here.
In which galaxy did SN2022czy explode, and where is it located relative to the galactic center? Galactic Environment
No host galaxy is identified for SN2022czy in this catalog record. A blank host field means the association is unresolved here—it does not establish that the host is uncataloged, resolved in imaging, or securely linked by astrometry. Possible states (unidentified, hostless candidate, imaging detection without a catalog name, or a securely matched cataloged galaxy) require separate evidence that is not present in this field.
Where is SN2022czy located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, SN2022czy is located at Right Ascension 12:22:01.154 and Declination +16:59:44.55, situated in the constellation Coma Berenices (Berenice's Hair). Because its declination is +16:59:44.55, it is primarily placed in the Northern celestial hemisphere.
How much Milky Way interstellar dust obscures our view of SN2022czy? Interstellar Dust
Along this line of sight, the catalog records a Milky Way foreground color excess of E(B−V) = 0.0344 mag (source: Analytical Galactic Disk Model (IAU)), corresponding to roughly A_V ≈ 0.11 mag for R_V = 3.1. Band-specific corrections (e.g. A_r) differ from A_V and should be applied when available. Map-based values (IRSA / Schlafly & Finkbeiner 2011) must not be claimed unless that map was actually queried.
Across which photometric filter bands was SN2022czy monitored? Astronomical Observations
No calibrated photometry is published for SN2022czy. Without multi-epoch flux measurements, neither a light curve nor a peak magnitude can be established. Follow-up imaging from survey alert streams would be required to map its brightness evolution.
What did astronomical spectroscopy reveal about SN2022czy's chemical makeup? Astronomical Observations
No spectrum has been published for SN2022czy. Without spectroscopy, its chemical composition, expansion velocity, and physical classification cannot be established. Classification spectra from follow-up observatories would be required to identify diagnostic absorption and emission lines.
Who discovered SN2022czy and how was it first detected? Discovery & History
SN2022czy was officially reported on 2022/02/22 by ATLAS. 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 SN2022czy? Scientific Research
Data for SN2022czy are compiled from international astronomical notices, the IAU Transient Name Server (TNS), and peer-reviewed astrophysical journals.
What other names and survey identifiers exist for SN2022czy? Cross-Identifications
Throughout global alert streams and survey databases, SN2022czy has also been designated as: AT2022czy, ATLAS22gtw. 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 SN2022czy contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
SN2022czy cannot currently be used for cosmological distance work because its classification is unresolved. The distance ladder relies on type-specific techniques: Type Ia supernovae use the Phillips relation between peak absolute magnitude and decline rate, while Type II events use the Expanding Photosphere Method or SCM-II. An unclassified transient fits neither, so no Hubble-constant constraint can be derived from it until a spectrum establishes its type.
Could gravitational waves or neutrinos from SN2022czy be detected on Earth? Multi-Messenger Astronomy
No neutrino or gravitational-wave counterpart has been reported for SN2022czy, and none is expected to be identifiable without a classification. The multi-messenger signature differs sharply by type: core-collapse events emit a neutrino burst at shock breakout (detected once, for SN 1987A), while thermonuclear Type Ia events produce negligible neutrinos and gravitational waves. Searching for a counterpart before knowing which mechanism applies would be unfocused.
How does SN2022czy 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), SN2022czy occurred at a distance of 1.72 Billion Light-Years. While historical naked-eye supernovae occurred within our Milky Way or its immediate satellites, modern discoveries like SN2022czy allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see SN2022czy tonight with a backyard telescope or binoculars? Backyard Observation
Unknown — no measured brightness. SN2022czy was discovered 1716 days ago (2022/02/22), but no calibrated photometry is published for it, so its current apparent magnitude cannot be stated. Without a magnitude there is no basis for a telescope-aperture recommendation. Use the coordinates and airmass chart above to plan a follow-up observation and report what you measure.
Does the radiation or shockwave from SN2022czy 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 1.72 Billion Light-Years, the inverse-square law dilutes the radiation by quintillions of times, making SN2022czy 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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