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Type IIn Supernova

The Story of Supernova SN2024jem

An extraordinary stellar explosion that occurred 620.3 Million Light-Years away in deep space.

⏱️ ~6 min deep read 🔬 24 Astrophysical Q&As 🔭 Viewing Guide Included 🪐 Constellation Pavo
🔭 Deep Field (~2.1′ FOV) · DSS2 Optical (China-VO mirror)
● SN2024jem Explosion Site

High-magnification deep optical view into SN2024jem'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
620.3 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
Pavo
The Peacock
💥 Explosion Physics
Type IIn
Core-Collapse Supergiant
📅 Discovered On
2024/05/20
M. Magee, G. Ramsay, K. Ackley, M. Dyer, F. Jiménez-Ibarra, J. Lyman, K. Ulaczyk, D. Steeghs, D. Galloway, V. Dhillon, P. O'Brien, K. Noysena, R. Kotak, R. Breton, L. Nuttall, E. Pallé, D. Pollacco, T. Killestein, A. Kumar, D. O'Neill, on behalf of GOTO collaboration
CHAPTER I

A Core-Collapse Class Transient

On 2024/05/20, astronomers scanning the heavens flagged a sudden, violent pinpoint of light that had flared into visibility. Designated SN2024jem, it represents a catastrophic stellar explosion classified as a Type IIn supernova.

SN2024jem 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 SN2024jem.

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

A Message Across Deep Cosmic Time

SN2024jem has a luminosity distance of approximately 620.3 Million Light-Years (redshift z = 0.043). That figure is not the light-travel time: under flat ΛCDM the lookback time is ≈582 Myr, when the light set out 582.4 million years ago during the Neoproterozoic, hundreds of millions of years before complex animal life diversified.

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 SN2024jem, 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 IIn light curves; an object-specific nickel mass for SN2024jem 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 SN2024jem'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 SN2024jem.

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 Pavo

No host galaxy is identified for SN2024jem in this catalog record . In our terrestrial sky, it resides in the constellation Pavo (The Peacock) at Right Ascension 20:21:39.406 and Declination -65:24:30.47.

CHAPTER VII

The Scientific Surveillance Campaign

Following its discovery by M. Magee, G. Ramsay, K. Ackley, M. Dyer, F. Jiménez-Ibarra, J. Lyman, K. Ulaczyk, D. Steeghs, D. Galloway, V. Dhillon, P. O'Brien, K. Noysena, R. Kotak, R. Breton, L. Nuttall, E. Pallé, D. Pollacco, T. Killestein, A. Kumar, D. O'Neill, on behalf of GOTO collaboration, observatories worldwide swung their lenses toward SN2024jem. In the Open Supernova Catalog, SN2024jem 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 2.5 years ago (2024/05/20). No reliable current brightness estimate — no photometry has been published.

Planetary Safety Note: Even though SN2024jem was a titanic explosion, our planet sits safely outside the lethal 50–100 light-year kill zone. At a distance of 620.3 Million Light-Years, the blast poses zero physical hazard to Earth's biosphere.

🌌 Cosmic Neighbors & Contemporaries 105,768+ transients indexed

Cataloged transients closest to SN2024jem in discovery time, spatial sky neighborhood, and cosmological redshift:

⏱️ Closest in Time
SN2024jdi Exploded same day
Type Ia 2024/05/20
SN2024jfe Exploded same day
Type Ia 2024/05/20
SN2024jef Exploded same day
Type Ia 2024/05/20
🔭 Closest on the Sky
GRB 131226A 1.78° away
Type LGRB Discovered 2013/12/26
GRB 920414A 2.28° away
Type LGRB Discovered 1992/04/14
FRB20240316B 2.68° away
Type FRB Discovered 2024/03/16
🌌 Same Cosmic Era (Redshift)
SN1991aw z = 0.043
Type Transient ~589.0 Mly (approx.)
SN2001bk z = 0.043
Type II ~589.0 Mly (approx.)
SN2002ez z = 0.043
Type Ia ~589.0 Mly (approx.)

❓ Frequently Asked Questions About SN2024jem

Scientific & observational Q&As indexed from astronomical databases & the Open Supernova Catalog
🔍 24 of 24
What type of supernova is SN2024jem and what kind of star exploded? Astrophysics & Progenitor
SN2024jem is cataloged as a Type IIn transient. Mechanism-specific claims (progenitor mass, nickel yield, remnant type) require more than this label and are not asserted here as object-specific measurements.
What was the progenitor star doing in the millions of years leading up to SN2024jem? Astrophysics & Progenitor
The specific progenitor of SN2024jem 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 SN2024jem.
How far away is SN2024jem from Earth and how old is the light reaching us? Cosmic Distance & Time
SN2024jem has a luminosity distance of approximately 620.3 Million Light-Years (redshift z = 0.043, d_L = 190.20). Under a flat ΛCDM cosmology (H₀≈70 km/s/Mpc, Ωₘ≈0.3), the corresponding lookback time is ≈582 Myr — when the light set out 582.4 million years ago during the Neoproterozoic, hundreds of millions of years before complex animal life diversified. 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 SN2024jem tell us about the expansion of space? Cosmic Distance & Time
SN2024jem exhibits a measured spectroscopic redshift of z = 0.0430. The cockpit reports a user-facing recession velocity of 12,614.2 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 (≈12,891 km/s) is a different low-z approximation and is not mixed here.
How bright did SN2024jem become at its peak, and how many Suns does that equal? Explosion Energetics
The peak brightness of SN2024jem 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 SN2024jem, 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 SN2024jem.
How fast are the supernova ejecta and shockwave of SN2024jem expanding through space? Explosion Energetics
No ejecta velocity is measured for SN2024jem. 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 IIn events typically show ejecta speeds of order ~8,500 km/s near maximum, but that class scale is not a measurement of SN2024jem.
What powers the prolonged glow of SN2024jem 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 SN2024jem. 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 SN2024jem create and disperse into the universe? Nucleosynthesis & Elements
Events of SN2024jem'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 SN2024jem.
Did SN2024jem leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
A core-collapse explosion associated with SN2024jem'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 SN2024jem'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 SN2024jem. 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 SN2024jem explode, and where is it located relative to the galactic center? Galactic Environment
No host galaxy is identified for SN2024jem 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 SN2024jem located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, SN2024jem is located at Right Ascension 20:21:39.406 and Declination -65:24:30.47, situated in the constellation Pavo (The Peacock). Because its declination is -65:24:30.47, it is favorably placed for Southern Hemisphere observatories.
How much Milky Way interstellar dust obscures our view of SN2024jem? Interstellar Dust
Along this line of sight, the catalog records a Milky Way foreground color excess of E(B−V) = 0.0587 mag (source: Analytical Galactic Disk Model (IAU)), corresponding to roughly A_V ≈ 0.18 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 SN2024jem monitored? Astronomical Observations
No calibrated photometry is published for SN2024jem. 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 SN2024jem's chemical makeup? Astronomical Observations
No spectrum has been published for SN2024jem. 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 SN2024jem and how was it first detected? Discovery & History
SN2024jem was officially reported on 2024/05/20 by M. Magee, G. Ramsay, K. Ackley, M. Dyer, F. Jiménez-Ibarra, J. Lyman, K. Ulaczyk, D. Steeghs, D. Galloway, V. Dhillon, P. O'Brien, K. Noysena, R. Kotak, R. Breton, L. Nuttall, E. Pallé, D. Pollacco, T. Killestein, A. Kumar, D. O'Neill, 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 SN2024jem? Scientific Research
Data for SN2024jem 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 SN2024jem? Cross-Identifications
Throughout global alert streams and survey databases, SN2024jem has also been designated as: 2024jem, AT2024jem, GOTO24bwz, SN 2024jem. 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 SN2024jem contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
As a core-collapse supernova, SN2024jem 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 SN2024jem be detected on Earth? Multi-Messenger Astronomy
Core-collapse supernovae like SN2024jem 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 SN2024jem 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), SN2024jem occurred at a distance of 620.3 Million Light-Years. While historical naked-eye supernovae occurred within our Milky Way or its immediate satellites, modern discoveries like SN2024jem allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see SN2024jem tonight with a backyard telescope or binoculars? Backyard Observation
Unknown — no measured brightness. SN2024jem was discovered 900 days ago (2024/05/20), 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 SN2024jem 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 620.3 Million Light-Years, the inverse-square law dilutes the radiation by quintillions of times, making SN2024jem 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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