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AT2019cd

Type Candidate ● Archived outburst (+2827d)
Aliases: ZTF19aaahrff  |  Discovered: 2019/01/04 by ZTF
⚡ Re-Enrich Data 📥 Download JSON 📊 Photometry CSV
Host Optical Cutout 0.26″/pix
DESI DR10 Optical (0.26″/pix)
AT2019cd cutout
Interactive Sky ↗

Core Parameters

R.A. (J2000)03:12:46.621 (48.19425°)
Dec. (J2000)+01:11:28.80 (1.19133°)
Spectral TypeCandidate
Redshift (z)0.049186
Recession Velocity14383 km/s
Luminosity Distance225.758 Mpc
Peak Apparent Mag19.4
Peak Absolute Mag-17.3161
MW Dust E(B-V)—
Host GalaxyKUG 0310+010
Host Offset—
Observations1 photometry, 0 spectra

Interactive Sky Field (Aladin) ✨ Highest-Definition Optical (0.25″/pix)

🎯 03:12:46.621 +01:11:28.80 FOV: 0.15°
● AT2019cd (Candidate)
Coordinate Pointing & Airmass
⚠️ Coordinate Pointing Only: The supernova exploded 7.7 years ago (2019/01/03, rest-frame phase +2694.5d). Based on standard radioactive decay physics, it has faded to m ≈ 57.6 (beyond ground telescope limits). Telescope pointing tonight observes the host galaxy (KUG 0310+010), not the vanished transient.
Multi-Band Light Curve
Calibrated Spectra Viewer

Literature & Data Provenance

IDSourceReferenceNASA ADS Bibcode
[1]2016A&A...594A..13PPlanck Collaboration et al. (2016)2016A&A...594A..13P
[2]Transient Name Server—
[3]Latest Supernovae—
[4]The Open Supernova CatalogGuillochon et al. (2017)2017ApJ...835...64G

❓ Frequently Asked Questions About AT2019cd

Scientific & observational Q&As indexed from astronomical databases & the Open Supernova Catalog
What type of supernova is AT2019cd and what kind of star exploded? Astrophysics & Progenitor
AT2019cd is cataloged as a Type Candidate transient. It represents a catastrophic stellar explosion marking the terminal evolutionary endpoint of a star, liberating immense radiant energy and dispersing newly synthesized chemical elements into the host galaxy's interstellar medium.
What was the progenitor star doing in the millions of years leading up to AT2019cd? Astrophysics & Progenitor
Before detonating as AT2019cd, the progenitor lived a short, furious stellar life of roughly 10 to 30 million years. In its interior, temperatures and pressures reached astronomical extremes, burning through nuclear fuel in an 'onion-skin' arrangement of concentric shells: hydrogen burning into helium for millions of years, helium into carbon for hundreds of thousands of years, carbon into neon for centuries, oxygen into silicon for months, and silicon fusing into iron in mere days! Once iron filled the core, fusion could no longer extract energy, dooming the star to sudden gravitational collapse.
How far away is AT2019cd from Earth and how old is the light reaching us? Cosmic Distance & Time
AT2019cd is located approximately 736.3 Million Light-Years from Earth (cosmological redshift z = 0.049186, luminosity distance d_L = 225.758 Mpc). Because electromagnetic radiation travels at 299,792 km/s, the photons detected by modern telescopes began their cosmic voyage 736.3 million years ago during the Paleozoic era, long before the first dinosaurs appeared on Earth. While that light traveled across intergalactic space, Earth's continents shifted and biological evolution shaped the history of our planet.
What does the cosmological redshift of AT2019cd tell us about the expansion of space? Cosmic Distance & Time
AT2019cd exhibits a measured spectroscopic redshift of z = 0.0492. Under Hubble's Law, this redshift corresponds to an apparent recessional velocity of approximately 14,745.6 km/s away from our Milky Way galaxy. This redshift is not motion through space alone, but the stretching of light waves as the fabric of the universe itself expanded during the millions of years the photons traveled to our telescopes.
How bright did AT2019cd become at its peak, and how many Suns does that equal? Explosion Energetics
At peak brightness, AT2019cd achieved an apparent magnitude of 19.4 around 2019/01/03. Corrected for cosmic distance and foreground interstellar dust, its intrinsic absolute magnitude was -17.3161. At this peak, the exploding star radiated with the incandescent brilliance of approximately 721.8 million Suns combined, briefly outshining the cumulative starlight of entire dwarf galaxies!
How much total energy was released by AT2019cd, and where did that energy go? Explosion Energetics
The collapse of AT2019cd's progenitor released a staggering 10⁵³ ergs of gravitational binding energy—more energy than our Sun will radiate across its entire 10-billion-year lifespan! Astonishingly, 99% of this titanic energy was emitted within 10 seconds in the form of trillions of nearly massless neutrinos. Only about 1% (10⁵¹ ergs) drove the physical kinetic blast wave, and a mere 0.01% (10⁴⁹ ergs) was radiated as the visible starlight observed by telescopes.
How fast are the supernova ejecta and shockwave of AT2019cd expanding through space? Explosion Energetics
The debris and shockwave of AT2019cd erupted into space at an astounding velocity of approximately 14,383 km/s (measured spectroscopically). This corresponds to roughly 4.8% of the speed of light (Mach 41,933 in air)! At this blistering speed, the expanding debris shell traverses the entire diameter of planet Earth in just 0.89 seconds, carving a giant bubble in the interstellar medium.
What powers the prolonged glow of AT2019cd weeks and months after detonation? Radioactive Engine
While the initial flash of AT2019cd was driven by shock breakout heating through the stellar envelope, its prolonged visibility over weeks and months was sustained by the radioactive decay of approximately 0.05 to 0.15 solar masses of Nickel-56 (⁵⁶Ni) forged in the core shock. As ⁵⁶Ni decays into ⁵⁶Co (half-life: 6.1 days) and then into stable ⁵⁶Fe (half-life: 77.2 days), gamma rays and positrons thermalize within the expanding ejecta, preventing the debris from instantly freezing in the vacuum of space.
What chemical elements did AT2019cd create and disperse into the universe? Nucleosynthesis & Elements
Core-collapse supernovae like AT2019cd are the primary creators of life-sustaining elements in the cosmos. The explosion manufactured and dispersed immense reservoirs of oxygen (the single most abundant heavy element in the universe), alongside carbon, nitrogen, neon, magnesium, silicon, sulfur, and calcium (which builds terrestrial bones and teeth). In the ultra-dense, neutron-rich shockwave, rapid neutron capture (r-process nucleosynthesis) forged heavy elements like gold, platinum, and uranium.
Did AT2019cd leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
The crushing core collapse of AT2019cd's progenitor forged 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 AT2019cd's explosion site look like in 1,000 to 10,000 years? Cosmic Remnant
Over the coming millennia, the explosion site of AT2019cd will undergo three dramatic evolutionary epochs: During the next few centuries (Free Expansion phase), the ejecta shell will continue expanding at thousands of km/s. Between 500 and 10,000 years (the Sedov-Taylor adiabatic phase), the forward shock will sweep up hundreds of solar masses of interstellar gas, heating it to tens of millions of degrees and glowing in bright thermal X-rays (similar to the famous Cygnus Loop or Cassiopeia A). Eventually, the cooling shock will compress nearby giant molecular clouds, triggering the gravitational collapse of new stars and solar systems!
In which galaxy did AT2019cd explode, and where is it located relative to the galactic center? Galactic Environment
AT2019cd is associated with KUG 0310+010. High-precision astrometry from optical sky surveys pins the explosion coordinates directly to the galaxy's underlying stellar population.
Where is AT2019cd located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, AT2019cd is located at Right Ascension 03:12:46.621 and Declination +01:11:28.80, situated in the constellation Aries (The Ram). Because its declination is +01:11:28.80, it is primarily placed in the Northern celestial hemisphere.
Across which photometric filter bands was AT2019cd monitored? Astronomical Observations
AT2019cd was tracked across 1 photometric observations utilizing filter bands including optical filters. Data were captured by observatories and survey networks including global optical observatories. Multi-color photometry tracks the temperature evolution of the fireball, verifying the rise time to peak and the rate of radioactive decline.
What did astronomical spectroscopy reveal about AT2019cd's chemical makeup? Astronomical Observations
Spectroscopic observations of AT2019cd confirmed its astrophysical classification by dissecting its light into individual wavelengths. Absorption and emission line features reveal the chemical composition, expansion velocity, and temperature of the expanding fireball.
Who discovered AT2019cd and how was it first detected? Discovery & History
AT2019cd was officially reported on 2019/01/04 by 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 AT2019cd? Scientific Research
AT2019cd is documented across 4 scientific references and archival data sources in the Open Supernova Catalog. These include discovery circulars and research datasets from 2016A&A...594A..13P, Transient Name Server, Latest Supernovae, The Open Supernova Catalog. All raw photometry and spectroscopy points are cross-indexed to their original bibliographic records for peer-reviewed verification.
What other names and survey identifiers exist for AT2019cd? Cross-Identifications
Throughout global alert streams and survey databases, AT2019cd has also been designated as: ZTF19aaahrff. 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 AT2019cd contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
As a core-collapse supernova, AT2019cd 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 AT2019cd be detected on Earth? Multi-Messenger Astronomy
Core-collapse supernovae like AT2019cd 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 AT2019cd 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), AT2019cd occurred at a distance of 736.3 Million Light-Years. While historical naked-eye supernovae occurred within our Milky Way or its immediate satellites, modern discoveries like AT2019cd allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see AT2019cd tonight with a backyard telescope or binoculars? Backyard Observation
AT2019cd exploded 7.7 years ago (2019/01/04). Optical transient emission has completely faded along its radioactive decay curve. Today, pointing a telescope at these coordinates reveals the expanding remnant nebula or KUG 0310+010; the original optical transient is no longer detectable with amateur backyard equipment.
Does the radiation or shockwave from AT2019cd 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 736.3 Million Light-Years, the inverse-square law dilutes the radiation by quintillions of times, making AT2019cd 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 →