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Type removed Supernova

The Story of Supernova AT2018bme

An extraordinary stellar explosion that occurred 938.2 Million Light-Years away in deep space.

⏱️ ~6 min deep read 🔬 24 Astrophysical Q&As 🔭 Viewing Guide Included 🪐 Constellation Canes Venatici
🔭 Deep Field (~2.1′ FOV) · DSS2 Optical (China-VO mirror)
● AT2018bme Explosion Site

High-magnification deep optical view into AT2018bme'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
938.2 Million Light-Years
Lookback Cosmic Time
✨ Peak Brightness
Mag 18.7
Large Observatory
☀️ Peak Radiance
2.2 billion Suns
Combined Stellar Energy
🚀 Shock Velocity
~18,041 km/s
~6.0% Speed of Light
🌌 Host Galaxy
2MASX J12524868+4544335
Offset: 0.53″ (0.65 kpc)
🧭 Constellation
Canes Venatici
The Hunting Dogs
💥 Explosion Physics
Type removed
Core-Collapse Supergiant
📅 Discovered On
2018/01/20
ATLAS
CHAPTER I

A Core-Collapse Class Transient

On 2018/01/20, astronomers scanning the heavens flagged a sudden, violent pinpoint of light that had flared into visibility. Designated AT2018bme, it represents a catastrophic stellar explosion classified as a Type removed supernova.

AT2018bme 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 AT2018bme.

Astrophysical Mechanism Summary
Type: Type removed • Progenitor: Massive Red/Stripped Supergiant Star • Velocity: ~18,041 km/s (~6.0% c)
CHAPTER II

A Message Across Deep Cosmic Time

AT2018bme has a luminosity distance of approximately 938.2 Million Light-Years (redshift z = 0.062103). That figure is not the light-travel time: under flat ΛCDM the lookback time is ≈830 Myr, when the light set out 829.8 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

Incandescence of 2.2 billion Suns

At the height of the outburst around 2018/01/20, AT2018bme surged to a peak apparent magnitude of 18.7 and an intrinsic absolute magnitude of -18.529. At that instant, this single dying star radiated with the collective power of approximately 2.2 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 removed light curves; an object-specific nickel mass for AT2018bme 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 AT2018bme'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 AT2018bme.

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 Canes Venatici

AT2018bme is associated with cataloged host 2MASX J12524868+4544335 , at an offset of 0.53″ (0.65 kpc) from the reported galactic center. In our terrestrial sky, it resides in the constellation Canes Venatici (The Hunting Dogs) at Right Ascension 12:52:48.730 and Declination +45:44:33.45.

CHAPTER VII

The Scientific Surveillance Campaign

Following its discovery by ATLAS, observatories worldwide swung their lenses toward AT2018bme. In the sne.space, AT2018bme 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 8.8 years ago (2018/01/20). No reliable current brightness estimate — no photometry has been published.

Planetary Safety Note: Even though AT2018bme was a titanic explosion, our planet sits safely outside the lethal 50–100 light-year kill zone. At a distance of 938.2 Million Light-Years, the blast poses zero physical hazard to Earth's biosphere.

🌌 Cosmic Neighbors & Contemporaries 105,868+ transients indexed

Cataloged transients closest to AT2018bme in discovery time, spatial sky neighborhood, and cosmological redshift:

⏱️ Closest in Time
AT2018ahh Exploded same day
Type Candidate 2018/01/20 · Mag 18.2
AT2018blx Exploded same day
Type removed 2018/01/20 · Mag 18.7
AT2018boe Exploded same day
Type Candidate 2018/01/20 · Mag 19.7
🔭 Closest on the Sky
SN2018bvg 29.0′ away
Type Ia Discovered 2018/05/19
SN2019ari 33.4′ away
Type Ia Discovered 2019/02/08
PS1-14uy 39.0′ away
Type Transient Discovered 2014/03/20
🌌 Same Cosmic Era (Redshift)
AT2020ktj z = 0.062104
Type Candidate ~850.7 Mly (approx.)
PTF10elk z = 0.062113
Type Ia ~850.9 Mly (approx.)
SN2020kee z = 0.06212
Type Ia ~851.0 Mly (approx.)

❓ Frequently Asked Questions About AT2018bme

Scientific & observational Q&As indexed from astronomical databases & the sne.space
🔍 24 of 24
What type of supernova is AT2018bme and what kind of star exploded? Astrophysics & Progenitor
AT2018bme is cataloged as a Type removed 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 AT2018bme? Astrophysics & Progenitor
The specific progenitor of AT2018bme 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 AT2018bme.
How far away is AT2018bme from Earth and how old is the light reaching us? Cosmic Distance & Time
AT2018bme has a luminosity distance of approximately 938.2 Million Light-Years (redshift z = 0.062103, d_L = 287.663). Under a flat ΛCDM cosmology (H₀≈70 km/s/Mpc, Ωₘ≈0.3), the corresponding lookback time is ≈830 Myr — when the light set out 829.8 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 AT2018bme tell us about the expansion of space? Cosmic Distance & Time
AT2018bme exhibits a measured spectroscopic redshift of z = 0.0621. The cockpit reports a user-facing recession velocity of 18,040.9 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 (≈18,618 km/s) is a different low-z approximation and is not mixed here.
How bright did AT2018bme become at its peak, and how many Suns does that equal? Explosion Energetics
At peak brightness, AT2018bme achieved an apparent magnitude of 18.7 around 2018/01/20. Corrected for cosmic distance and foreground interstellar dust, its intrinsic absolute magnitude was -18.529. At this peak, the exploding star radiated with the incandescent brilliance of approximately 2.2 billion Suns combined, briefly outshining the cumulative starlight of entire dwarf galaxies!
How much total energy was released by AT2018bme, 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 AT2018bme.
How fast are the supernova ejecta and shockwave of AT2018bme expanding through space? Explosion Energetics
Spectroscopic line blueshifts imply an ejecta velocity of approximately 18,041 km/s (~6.0% of c) for AT2018bme. This is distinct from cosmological recession velocity inferred from redshift.
What powers the prolonged glow of AT2018bme 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 AT2018bme. 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 AT2018bme create and disperse into the universe? Nucleosynthesis & Elements
The nucleosynthetic products of AT2018bme are unknown because its type is unresolved. Element yields depend directly on the explosion mechanism: a thermonuclear Type Ia produces mostly iron-peak elements such as 56Ni and 56Fe, whereas a core-collapse event produces large quantities of oxygen, neon, magnesium and silicon from successive burning shells. No spectrum has been published for this transient, so which of these occurred is not established.
Did AT2018bme leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
A core-collapse explosion associated with AT2018bme'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 AT2018bme'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 AT2018bme. 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 AT2018bme explode, and where is it located relative to the galactic center? Galactic Environment
AT2018bme is associated with cataloged host 2MASX J12524868+4544335 at an angular/physical offset of 0.53″ (0.65 kpc) from the reported galactic center. That offset places the transient in the host's projected light distribution; it does not by itself prove which stellar population produced the progenitor.
Where is AT2018bme located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, AT2018bme is located at Right Ascension 12:52:48.730 and Declination +45:44:33.45, situated in the constellation Canes Venatici (The Hunting Dogs). Because its declination is +45:44:33.45, it is primarily placed in the Northern celestial hemisphere.
How much Milky Way interstellar dust obscures our view of AT2018bme? Interstellar Dust
Along this line of sight, the catalog records a Milky Way foreground color excess of E(B−V) = 0.0262 mag (source: published extinction estimate), corresponding to roughly A_V ≈ 0.08 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 AT2018bme monitored? Astronomical Observations
No calibrated photometry is published for AT2018bme. 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 AT2018bme's chemical makeup? Astronomical Observations
No spectrum has been published for AT2018bme. 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 AT2018bme and how was it first detected? Discovery & History
AT2018bme was officially reported on 2018/01/20 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 AT2018bme? Scientific Research
Data for AT2018bme 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 AT2018bme? Cross-Identifications
Throughout global alert streams and survey databases, AT2018bme has also been designated as: ATLAS18omp. 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 AT2018bme contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
AT2018bme 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 AT2018bme be detected on Earth? Multi-Messenger Astronomy
No neutrino or gravitational-wave counterpart has been reported for AT2018bme, 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 AT2018bme 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), AT2018bme occurred at a distance of 938.2 Million Light-Years. While historical naked-eye supernovae occurred within our Milky Way or its immediate satellites, modern discoveries like AT2018bme allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see AT2018bme tonight with a backyard telescope or binoculars? Backyard Observation
Unknown — no measured brightness. AT2018bme was discovered 3220 days ago (2018/01/20), 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 AT2018bme 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 938.2 Million Light-Years, the inverse-square law dilutes the radiation by quintillions of times, making AT2018bme 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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