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Type II Supernova

The Story of Supernova SN2022mgz

An extraordinary stellar explosion that occurred 385.0 Million Light-Years away in deep space.

⏱️ ~7 min deep read 🔬 24 Astrophysical Q&As 🔭 Viewing Guide Included 🪐 Constellation Leo
🔭 Deep Field (~2.1′ FOV) · DSS2 Optical (China-VO mirror)
● SN2022mgz Explosion Site

High-magnification deep optical view into SN2022mgz'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
385.0 Million Light-Years
Lookback Cosmic Time
✨ Peak Brightness
Mag —
Research Scope
☀️ Peak Radiance
~1.0 to 5.0 Billion Suns
Combined Stellar Energy
🚀 Shock Velocity
Not measured
No spectral ejecta velocity
🌌 Host Galaxy
Field Transient Host
Center Coincident
🧭 Constellation
Leo
The Lion
💥 Explosion Physics
Type II
Core-Collapse Supergiant
📅 Discovered On
2022/06/06
J. Tonry, L. Denneau, H. Weiland (IfA, University of Hawaii), N. Erasmus, W. Koorts (South African Astronomical Observatory), J. Anderson (ESO), A. Jordan, V. Suc (UAI, Obstech), K. W. Smith, S. Srivastav, D. R. Young, S. J. Smartt, J. Gillanders, M. Fulton, M. McCollum, T. Moore (Queen's University Belfast), L. Shingles (GSI/QUB), A. Rest (STScI), T.-W. Chen (Stockholm), M. Nicholl (Birmingham), D. Pacheco (PUC), C. Stubbs (Harvard)
CHAPTER I

A Core-Collapse Class Transient

On 2022/06/06, astronomers scanning the heavens flagged a sudden, violent pinpoint of light that had flared into visibility. Designated SN2022mgz, it represents a catastrophic stellar explosion classified as a Type II supernova.

SN2022mgz 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 SN2022mgz.

Astrophysical Mechanism Summary
Type: Type II • Progenitor: Massive Red/Stripped Supergiant Star • Velocity: Not measured
CHAPTER II

A Message Across Deep Cosmic Time

SN2022mgz has a luminosity distance of approximately 385.0 Million Light-Years (redshift z = 0.027). That figure is not the light-travel time: under flat ΛCDM the lookback time is ≈370 Myr, when the light set out 369.9 million years ago during the Paleozoic era, long before the first dinosaurs appeared on Earth.

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

CHAPTER III

Brightness Record

No calibrated peak magnitude is published for SN2022mgz, so neither its apparent brightness nor an equivalent solar luminosity can be stated.

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 II light curves; an object-specific nickel mass for SN2022mgz 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 SN2022mgz'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 SN2022mgz.

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 Leo

No host galaxy is identified for SN2022mgz in this catalog record . In our terrestrial sky, it resides in the constellation Leo (The Lion) at Right Ascension 09:41:40.680 and Declination +16:57:07.27.

CHAPTER VII

The Scientific Surveillance Campaign

Following its discovery by J. Tonry, L. Denneau, H. Weiland (IfA, University of Hawaii), N. Erasmus, W. Koorts (South African Astronomical Observatory), J. Anderson (ESO), A. Jordan, V. Suc (UAI, Obstech), K. W. Smith, S. Srivastav, D. R. Young, S. J. Smartt, J. Gillanders, M. Fulton, M. McCollum, T. Moore (Queen's University Belfast), L. Shingles (GSI/QUB), A. Rest (STScI), T.-W. Chen (Stockholm), M. Nicholl (Birmingham), D. Pacheco (PUC), C. Stubbs (Harvard), observatories worldwide swung their lenses toward SN2022mgz. In the Open Supernova Catalog, SN2022mgz 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 4.4 years ago (2022/06/06). No reliable current brightness estimate — no photometry has been published.

Planetary Safety Note: Even though SN2022mgz was a titanic explosion, our planet sits safely outside the lethal 50–100 light-year kill zone. At a distance of 385.0 Million Light-Years, the blast poses zero physical hazard to Earth's biosphere.

🌌 Cosmic Neighbors & Contemporaries 105,768+ transients indexed

Cataloged transients closest to SN2022mgz in discovery time, spatial sky neighborhood, and cosmological redshift:

⏱️ Closest in Time
FRB20220606A Exploded same day
Type FRB 2022/06/06
SN2022mdz Exploded same day
Type Ia 2022/06/06
SN2022meq Exploded same day
Type Ia 2022/06/06
🔭 Closest on the Sky
AT2020aens 21.8′ away
Type Candidate Discovered 2020/12/22
MLS130215:093953+165516 25.8′ away
Type Ia Discovered 2013/02/07
AT2020uwe 26.7′ away
Type Candidate Discovered 2020/10/04
🌌 Same Cosmic Era (Redshift)
SN1992ak z = 0.027
Type Transient ~369.9 Mly (approx.)
SN1993D z = 0.027
Type Ia ~369.9 Mly (approx.)
SN1998cv z = 0.027
Type Ic ~369.9 Mly (approx.)

❓ Frequently Asked Questions About SN2022mgz

Scientific & observational Q&As indexed from astronomical databases & the Open Supernova Catalog
🔍 24 of 24
What type of supernova is SN2022mgz and what kind of star exploded? Astrophysics & Progenitor
SN2022mgz is classified as a Type II supernova, consistent with core collapse of a massive star that retained hydrogen in its outer envelope. Typical progenitor mass ranges quoted for the class are model expectations, not a measured mass for this star.
What was the progenitor star doing in the millions of years leading up to SN2022mgz? Astrophysics & Progenitor
The specific progenitor of SN2022mgz 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 SN2022mgz.
How far away is SN2022mgz from Earth and how old is the light reaching us? Cosmic Distance & Time
SN2022mgz has a luminosity distance of approximately 385.0 Million Light-Years (redshift z = 0.027, d_L = 118.03). Under a flat ΛCDM cosmology (H₀≈70 km/s/Mpc, Ωₘ≈0.3), the corresponding lookback time is ≈370 Myr — when the light set out 369.9 million years ago during the Paleozoic era, long before the first dinosaurs appeared on 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 SN2022mgz tell us about the expansion of space? Cosmic Distance & Time
SN2022mgz exhibits a measured spectroscopic redshift of z = 0.0270. The cockpit reports a user-facing recession velocity of 7,985.2 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 (≈8,094 km/s) is a different low-z approximation and is not mixed here.
How bright did SN2022mgz become at its peak, and how many Suns does that equal? Explosion Energetics
The peak brightness of SN2022mgz is not recorded. No peak apparent magnitude and no calibrated photometry are published for this transient, so neither its apparent brightness nor its intrinsic luminosity can be stated. Any figure quoted here would be an estimate from a template rather than a measurement of this object. Follow-up photometry would establish the light curve and the peak.
How much total energy was released by SN2022mgz, and where did that energy go? Explosion Energetics
Core-collapse events of this broad class are often discussed with a ~10⁵³ erg gravitational binding energy of which ~99% may escape as neutrinos—again a class scale, not a measured budget for SN2022mgz.
How fast are the supernova ejecta and shockwave of SN2022mgz expanding through space? Explosion Energetics
No ejecta velocity is measured for SN2022mgz. Blast-wave speed is obtained from Doppler shifts of spectral absorption features (e.g. Si II λ6355 for Type Ia), not from cosmological redshift. Any recession velocity derived from z describes Hubble flow, not the explosion debris. Type II events typically show ejecta speeds of order ~8,500 km/s near maximum, but that class scale is not a measurement of SN2022mgz.
What powers the prolonged glow of SN2022mgz weeks and months after detonation? Radioactive Engine
Classified core-collapse light curves are often sustained after peak by radioactive ⁵⁶Ni → ⁵⁶Co → ⁵⁶Fe decay, with typical nickel yields of order 0.05–0.15 solar masses—again a class scale, not a measured yield for SN2022mgz. Shock-breakout heating may dominate the earliest optical flash; without a published bolometric fit, neither nickel mass nor the dominant power source is established for this event.
What chemical elements did SN2022mgz create and disperse into the universe? Nucleosynthesis & Elements
Events of SN2022mgz'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 SN2022mgz.
Did SN2022mgz leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
A core-collapse explosion associated with SN2022mgz'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 SN2022mgz'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 SN2022mgz. 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 SN2022mgz explode, and where is it located relative to the galactic center? Galactic Environment
No host galaxy is identified for SN2022mgz 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 SN2022mgz located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, SN2022mgz is located at Right Ascension 09:41:40.680 and Declination +16:57:07.27, situated in the constellation Leo (The Lion). Because its declination is +16:57:07.27, it is primarily placed in the Northern celestial hemisphere.
How much Milky Way interstellar dust obscures our view of SN2022mgz? Interstellar Dust
Along this line of sight, the catalog records a Milky Way foreground color excess of E(B−V) = 0.0467 mag (source: Analytical Galactic Disk Model (IAU)), corresponding to roughly A_V ≈ 0.14 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 SN2022mgz monitored? Astronomical Observations
No calibrated photometry is published for SN2022mgz. 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 SN2022mgz's chemical makeup? Astronomical Observations
No spectrum has been published for SN2022mgz. 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 SN2022mgz and how was it first detected? Discovery & History
SN2022mgz was officially reported on 2022/06/06 by J. Tonry, L. Denneau, H. Weiland (IfA, University of Hawaii), N. Erasmus, W. Koorts (South African Astronomical Observatory), J. Anderson (ESO), A. Jordan, V. Suc (UAI, Obstech), K. W. Smith, S. Srivastav, D. R. Young, S. J. Smartt, J. Gillanders, M. Fulton, M. McCollum, T. Moore (Queen's University Belfast), L. Shingles (GSI/QUB), A. Rest (STScI), T.-W. Chen (Stockholm), M. Nicholl (Birmingham), D. Pacheco (PUC), C. Stubbs (Harvard). 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 SN2022mgz? Scientific Research
Data for SN2022mgz 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 SN2022mgz? Cross-Identifications
Throughout global alert streams and survey databases, SN2022mgz has also been designated as: 2022mgz, PS22mex, AT2022mgz, Gaia22cpe, ATLAS22qib, SN 2022mgz. 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 SN2022mgz contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
As a core-collapse supernova, SN2022mgz 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 SN2022mgz be detected on Earth? Multi-Messenger Astronomy
Core-collapse supernovae like SN2022mgz 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 SN2022mgz 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), SN2022mgz occurred at a distance of 385.0 Million Light-Years. While historical naked-eye supernovae occurred within our Milky Way or its immediate satellites, modern discoveries like SN2022mgz allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see SN2022mgz tonight with a backyard telescope or binoculars? Backyard Observation
Unknown — no measured brightness. SN2022mgz was discovered 1613 days ago (2022/06/06), 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 SN2022mgz 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 385.0 Million Light-Years, the inverse-square law dilutes the radiation by quintillions of times, making SN2022mgz 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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