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Type II Supernova

The Story of Supernova SN2024kee

An extraordinary stellar explosion that occurred 561.5 Million Light-Years away in deep space.

⏱️ ~6 min deep read 🔬 24 Astrophysical Q&As 🔭 Viewing Guide Included 🪐 Constellation Ursa Minor
🔭 Deep Field (~2.1′ FOV) · DSS2 Optical (China-VO mirror)
● SN2024kee Explosion Site

High-magnification deep optical view into SN2024kee'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
561.5 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
Ursa Minor
The Little Bear
💥 Explosion Physics
Type II
Core-Collapse Supergiant
📅 Discovered On
2024/06/01
Nabeel Rehemtulla (CIERA, NU), Christoffer Fremling (Caltech), Daniel Perley (LJMU), Theophile du Laz (Caltech) on behalf of ZTF
CHAPTER I

A Core-Collapse Class Transient

On 2024/06/01, astronomers scanning the heavens flagged a sudden, violent pinpoint of light that had flared into visibility. Designated SN2024kee, it represents a catastrophic stellar explosion classified as a Type II supernova.

SN2024kee 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 SN2024kee.

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

A Message Across Deep Cosmic Time

SN2024kee has a luminosity distance of approximately 561.5 Million Light-Years (redshift z = 0.039037). That figure is not the light-travel time: under flat ΛCDM the lookback time is ≈530 Myr, when the light set out 530.2 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 SN2024kee, 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 SN2024kee 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 SN2024kee'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 SN2024kee.

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 Ursa Minor

No host galaxy is identified for SN2024kee in this catalog record . In our terrestrial sky, it resides in the constellation Ursa Minor (The Little Bear) at Right Ascension 16:01:26.402 and Declination +71:24:10.49.

CHAPTER VII

The Scientific Surveillance Campaign

Following its discovery by Nabeel Rehemtulla (CIERA, NU), Christoffer Fremling (Caltech), Daniel Perley (LJMU), Theophile du Laz (Caltech) on behalf of ZTF, observatories worldwide swung their lenses toward SN2024kee. In the Open Supernova Catalog, SN2024kee 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 2.4 years ago (2024/06/01). No reliable current brightness estimate — no photometry has been published.

Planetary Safety Note: Even though SN2024kee was a titanic explosion, our planet sits safely outside the lethal 50–100 light-year kill zone. At a distance of 561.5 Million Light-Years, the blast poses zero physical hazard to Earth's biosphere.

🌌 Cosmic Neighbors & Contemporaries 105,768+ transients indexed

Cataloged transients closest to SN2024kee in discovery time, spatial sky neighborhood, and cosmological redshift:

⏱️ Closest in Time
AT2024kby Exploded same day
Type CV 2024/06/01
SN2024kan Exploded same day
Type II 2024/06/01
SN2024kbl Exploded same day
Type Ia 2024/06/01
🔭 Closest on the Sky
SN2018bax 15.7′ away
Type Ia Discovered 2018/04/11
FRB20231123B 19.2′ away
Type FRB Discovered 2023/11/23
FRB20230626A 19.8′ away
Type FRB Discovered 2023/06/26
🌌 Same Cosmic Era (Redshift)
SN2018heh z = 0.039037
Type II ~534.8 Mly (approx.)
SN1990Y z = 0.039034
Type Ia ~534.7 Mly (approx.)
SN2018hoi z = 0.03903
Type Ia ~534.7 Mly (approx.)

❓ Frequently Asked Questions About SN2024kee

Scientific & observational Q&As indexed from astronomical databases & the Open Supernova Catalog
🔍 24 of 24
What type of supernova is SN2024kee and what kind of star exploded? Astrophysics & Progenitor
SN2024kee 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 SN2024kee? Astrophysics & Progenitor
The specific progenitor of SN2024kee 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 SN2024kee.
How far away is SN2024kee from Earth and how old is the light reaching us? Cosmic Distance & Time
SN2024kee has a luminosity distance of approximately 561.5 Million Light-Years (redshift z = 0.039037, d_L = 172.17). Under a flat ΛCDM cosmology (H₀≈70 km/s/Mpc, Ωₘ≈0.3), the corresponding lookback time is ≈530 Myr — when the light set out 530.2 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 SN2024kee tell us about the expansion of space? Cosmic Distance & Time
SN2024kee exhibits a measured spectroscopic redshift of z = 0.0390. The cockpit reports a user-facing recession velocity of 11,474.7 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 (≈11,703 km/s) is a different low-z approximation and is not mixed here.
How bright did SN2024kee become at its peak, and how many Suns does that equal? Explosion Energetics
The peak brightness of SN2024kee 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 SN2024kee, 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 SN2024kee.
How fast are the supernova ejecta and shockwave of SN2024kee expanding through space? Explosion Energetics
No ejecta velocity is measured for SN2024kee. 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 SN2024kee.
What powers the prolonged glow of SN2024kee 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 SN2024kee. 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 SN2024kee create and disperse into the universe? Nucleosynthesis & Elements
Events of SN2024kee'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 SN2024kee.
Did SN2024kee leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
A core-collapse explosion associated with SN2024kee'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 SN2024kee'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 SN2024kee. 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 SN2024kee explode, and where is it located relative to the galactic center? Galactic Environment
No host galaxy is identified for SN2024kee 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 SN2024kee located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, SN2024kee is located at Right Ascension 16:01:26.402 and Declination +71:24:10.49, situated in the constellation Ursa Minor (The Little Bear). Because its declination is +71:24:10.49, it is primarily placed in the Northern celestial hemisphere.
How much Milky Way interstellar dust obscures our view of SN2024kee? Interstellar Dust
Along this line of sight, the catalog records a Milky Way foreground color excess of E(B−V) = 0.0527 mag (source: Analytical Galactic Disk Model (IAU)), corresponding to roughly A_V ≈ 0.16 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 SN2024kee monitored? Astronomical Observations
No calibrated photometry is published for SN2024kee. 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 SN2024kee's chemical makeup? Astronomical Observations
No spectrum has been published for SN2024kee. 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 SN2024kee and how was it first detected? Discovery & History
SN2024kee was officially reported on 2024/06/01 by Nabeel Rehemtulla (CIERA, NU), Christoffer Fremling (Caltech), Daniel Perley (LJMU), Theophile du Laz (Caltech) on behalf of ZTF. 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 SN2024kee? Scientific Research
Data for SN2024kee 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 SN2024kee? Cross-Identifications
Throughout global alert streams and survey databases, SN2024kee has also been designated as: 2024kee, AT2024kee, GOTO24cqd, SN 2024kee, ZTF24aaqiqpw. 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 SN2024kee contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
As a core-collapse supernova, SN2024kee 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 SN2024kee be detected on Earth? Multi-Messenger Astronomy
Core-collapse supernovae like SN2024kee 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 SN2024kee 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), SN2024kee occurred at a distance of 561.5 Million Light-Years. While historical naked-eye supernovae occurred within our Milky Way or its immediate satellites, modern discoveries like SN2024kee allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see SN2024kee tonight with a backyard telescope or binoculars? Backyard Observation
Unknown — no measured brightness. SN2024kee was discovered 886 days ago (2024/06/01), 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 SN2024kee 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 561.5 Million Light-Years, the inverse-square law dilutes the radiation by quintillions of times, making SN2024kee 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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