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Type IIb Supernova

The Story of Supernova SN2022rls

An extraordinary stellar explosion that occurred 239.0 Million Light-Years away in deep space.

⏱️ ~7 min deep read 🔬 24 Astrophysical Q&As 🔭 Viewing Guide Included 🪐 Constellation Lacerta
🔭 Deep Field (~2.1′ FOV) · DSS2 Optical (China-VO mirror)
● SN2022rls Explosion Site

High-magnification deep optical view into SN2022rls'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
239.0 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
Lacerta
The Lizard
💥 Explosion Physics
Type IIb
Core-Collapse Supergiant
📅 Discovered On
2022/08/18
J. Tonry, L. Denneau, H. Weiland, A. Lawrence, R. Siverd (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), D. Pacheco (PUC), M. Nicholl (Birmingham), C. Stubbs (Harvard), S. Rest (JHU/QUB)
CHAPTER I

A Core-Collapse Class Transient

On 2022/08/18, astronomers scanning the heavens flagged a sudden, violent pinpoint of light that had flared into visibility. Designated SN2022rls, it represents a catastrophic stellar explosion classified as a Type IIb supernova.

SN2022rls 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 SN2022rls.

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

A Message Across Deep Cosmic Time

SN2022rls has a luminosity distance of approximately 239.0 Million Light-Years (redshift z = 0.016888). That figure is not the light-travel time: under flat ΛCDM the lookback time is ≈233 Myr, when the light set out 233.0 million years ago during the Triassic period as the earliest dinosaurs and mammals were just evolving.

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 SN2022rls, 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 IIb light curves; an object-specific nickel mass for SN2022rls 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 SN2022rls'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 SN2022rls.

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 Lacerta

No host galaxy is identified for SN2022rls in this catalog record . In our terrestrial sky, it resides in the constellation Lacerta (The Lizard) at Right Ascension 22:58:29.770 and Declination +40:25:42.69.

CHAPTER VII

The Scientific Surveillance Campaign

Following its discovery by J. Tonry, L. Denneau, H. Weiland, A. Lawrence, R. Siverd (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), D. Pacheco (PUC), M. Nicholl (Birmingham), C. Stubbs (Harvard), S. Rest (JHU/QUB), observatories worldwide swung their lenses toward SN2022rls. In the sne.space, SN2022rls 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 4.2 years ago (2022/08/18). No reliable current brightness estimate — no photometry has been published.

Planetary Safety Note: Even though SN2022rls was a titanic explosion, our planet sits safely outside the lethal 50–100 light-year kill zone. At a distance of 239.0 Million Light-Years, the blast poses zero physical hazard to Earth's biosphere.

🌌 Cosmic Neighbors & Contemporaries 105,868+ transients indexed

Cataloged transients closest to SN2022rls in discovery time, spatial sky neighborhood, and cosmological redshift:

⏱️ Closest in Time
AT2022rmk Exploded same day
Type LBV 2022/08/18
AT2022roe Exploded same day
Type CV 2022/08/18
FRB20220818A Exploded same day
Type FRB 2022/08/18
🔭 Closest on the Sky
SN2013ep 0.1′ away
Type IIb Discovered 2013/07/29
TDE2023lli 11.8′ away
Type TDE Discovered 2023/06/23
AT2018ixg 19.8′ away
Type Candidate Discovered 2018/11/06
🌌 Same Cosmic Era (Redshift)
SN2013ep z = 0.016888
Type IIb ~231.3 Mly (approx.)
SN2013gs z = 0.016888
Type Ia ~231.3 Mly (approx.)
SN2009fr z = 0.0169
Type II ~231.5 Mly (approx.)

❓ Frequently Asked Questions About SN2022rls

Scientific & observational Q&As indexed from astronomical databases & the sne.space
🔍 24 of 24
What type of supernova is SN2022rls and what kind of star exploded? Astrophysics & Progenitor
SN2022rls is a stripped-envelope supernova (Type IIb), consistent with core collapse after loss of the outer hydrogen (and for Ic, helium) envelope. The specific progenitor channel for this object is not uniquely determined by the spectral type alone.
What was the progenitor star doing in the millions of years leading up to SN2022rls? Astrophysics & Progenitor
The specific progenitor of SN2022rls 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 SN2022rls.
How far away is SN2022rls from Earth and how old is the light reaching us? Cosmic Distance & Time
SN2022rls has a luminosity distance of approximately 239.0 Million Light-Years (redshift z = 0.016888, d_L = 73.27). Under a flat ΛCDM cosmology (H₀≈70 km/s/Mpc, Ωₘ≈0.3), the corresponding lookback time is ≈233 Myr — when the light set out 233.0 million years ago during the Triassic period as the earliest dinosaurs and mammals were just evolving. 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 SN2022rls tell us about the expansion of space? Cosmic Distance & Time
SN2022rls exhibits a measured spectroscopic redshift of z = 0.0169. The cockpit reports a user-facing recession velocity of 5,020.1 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 (≈5,063 km/s) is a different low-z approximation and is not mixed here.
How bright did SN2022rls become at its peak, and how many Suns does that equal? Explosion Energetics
The peak brightness of SN2022rls 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 SN2022rls, 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 SN2022rls.
How fast are the supernova ejecta and shockwave of SN2022rls expanding through space? Explosion Energetics
No ejecta velocity is measured for SN2022rls. 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 IIb events typically show ejecta speeds of order ~12,500 km/s near maximum, but that class scale is not a measurement of SN2022rls.
What powers the prolonged glow of SN2022rls 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 SN2022rls. 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 SN2022rls create and disperse into the universe? Nucleosynthesis & Elements
Events of SN2022rls'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 SN2022rls.
Did SN2022rls leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
A core-collapse explosion associated with SN2022rls'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 SN2022rls'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 SN2022rls. 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 SN2022rls explode, and where is it located relative to the galactic center? Galactic Environment
No host galaxy is identified for SN2022rls 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 SN2022rls located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, SN2022rls is located at Right Ascension 22:58:29.770 and Declination +40:25:42.69, situated in the constellation Lacerta (The Lizard). Because its declination is +40:25:42.69, it is primarily placed in the Northern celestial hemisphere.
How much Milky Way interstellar dust obscures our view of SN2022rls? Interstellar Dust
Along this line of sight, the catalog records a Milky Way foreground color excess of E(B−V) = 0.1026 mag (source: Analytical Galactic Disk Model (IAU)), corresponding to roughly A_V ≈ 0.32 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 SN2022rls monitored? Astronomical Observations
No calibrated photometry is published for SN2022rls. 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 SN2022rls's chemical makeup? Astronomical Observations
No spectrum has been published for SN2022rls. 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 SN2022rls and how was it first detected? Discovery & History
SN2022rls was officially reported on 2022/08/18 by J. Tonry, L. Denneau, H. Weiland, A. Lawrence, R. Siverd (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), D. Pacheco (PUC), M. Nicholl (Birmingham), C. Stubbs (Harvard), S. Rest (JHU/QUB). 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 SN2022rls? Scientific Research
Data for SN2022rls 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 SN2022rls? Cross-Identifications
Throughout global alert streams and survey databases, SN2022rls has also been designated as: 2022rls, PS22hfl, AT2022rls, SN 2022rls, ATLAS22baaw, ZTF22abbtzfm. 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 SN2022rls contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
As a core-collapse supernova, SN2022rls 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 SN2022rls be detected on Earth? Multi-Messenger Astronomy
Core-collapse supernovae like SN2022rls 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 SN2022rls 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), SN2022rls occurred at a distance of 239.0 Million Light-Years. While historical naked-eye supernovae occurred within our Milky Way or its immediate satellites, modern discoveries like SN2022rls allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see SN2022rls tonight with a backyard telescope or binoculars? Backyard Observation
Unknown — no measured brightness. SN2022rls was discovered 1546 days ago (2022/08/18), 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 SN2022rls 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 239.0 Million Light-Years, the inverse-square law dilutes the radiation by quintillions of times, making SN2022rls completely harmless to our biosphere and purely a fascinating spectacle for human exploration.
Data sourced from IAU TNS, ALeRCE, WISeREP, and the sne.space. View All General Astrophysics FAQs →
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