Host Optical Cutout
0.26″/pix
Pan-STARRS1 DR1 Optical (0.25″/pix)
Core Parameters
| R.A. (J2000) | 14:20:24.200 (215.10083°) |
|---|---|
| Dec. (J2000) | +53:03:37.50 (53.06042°) |
| Spectral Type | — |
| Redshift (z) | 1.4 |
| Recession Velocity | 210000 km/s |
| Luminosity Distance | 10300 Mpc |
| Peak Apparent Mag | — |
| Peak Absolute Mag | — |
| MW Dust E(B-V) | 0.0089 mag |
| Host Galaxy | — |
| Host Offset | 0.00″ (0.00 kpc) |
| Observations | 0 photometry, 0 spectra |
Interactive Sky Field (Aladin) ✨ Highest-Definition Optical (0.25″/pix)
🎯 14:20:24.200 +53:03:37.50
FOV: 0.15°
● EGS13Cha (—)
Coordinate Pointing & Airmass
⚠️ Coordinate Pointing Only: The supernova exploded 13.7 years ago (2013, rest-frame phase +2091.2d). Based on standard radioactive decay physics, it has faded to m ≈ 47.8 (beyond ground telescope limits). Telescope pointing tonight observes the host galaxy, not the vanished transient.
Multi-Band Light Curve
Calibrated Spectra Viewer
🌌 Cosmic Neighbors & Contemporaries
110,222+ Transients Indexed
Cataloged supernovae closest to EGS13Cha in discovery time, spatial sky neighborhood, and cosmological lookback epoch:
⏱️ Closest in Time
CLY13Gal
Exploded same day
Type Transient
2013
CLY13Hos
Exploded same day
Type Transient
2013
CLY13Pup
Exploded same day
Type Transient
2013
Literature & Data Provenance
| ID | Source | Reference | NASA ADS Bibcode |
|---|---|---|---|
| No sources recorded. | |||
❓ Frequently Asked Questions About EGS13Cha
Scientific & observational Q&As indexed from astronomical databases & the Open Supernova Catalog
What type of supernova is EGS13Cha and what kind of star exploded? Astrophysics & Progenitor
EGS13Cha is cataloged as a Type — 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 EGS13Cha? Astrophysics & Progenitor
Before detonating as EGS13Cha, 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 EGS13Cha from Earth and how old is the light reaching us? Cosmic Distance & Time
EGS13Cha is located approximately 33594.1 Million Light-Years from Earth (cosmological redshift z = 1.4, luminosity distance d_L = 10300 Mpc). Because electromagnetic radiation travels at 299,792 km/s, the photons detected by modern telescopes began their cosmic voyage 33594.1 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 EGS13Cha tell us about the expansion of space? Cosmic Distance & Time
EGS13Cha exhibits a measured spectroscopic redshift of z = 1.4000. Under Hubble's Law, this redshift corresponds to an apparent recessional velocity of approximately 419,709.4 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 EGS13Cha become at its peak, and how many Suns does that equal? Explosion Energetics
At peak brightness, EGS13Cha achieved an apparent magnitude of —. At this peak, the exploding star radiated with the incandescent brilliance of approximately hundreds of millions of Suns combined, briefly outshining the cumulative starlight of entire dwarf galaxies!
How much total energy was released by EGS13Cha, and where did that energy go? Explosion Energetics
The collapse of EGS13Cha'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 EGS13Cha expanding through space? Explosion Energetics
The debris and shockwave of EGS13Cha erupted into space at an astounding velocity of approximately 210,000 km/s (measured spectroscopically). This corresponds to roughly 70.0% of the speed of light (Mach 612,245 in air)! At this blistering speed, the expanding debris shell traverses the entire diameter of planet Earth in just 0.06 seconds, carving a giant bubble in the interstellar medium.
What powers the prolonged glow of EGS13Cha weeks and months after detonation? Radioactive Engine
While the initial flash of EGS13Cha 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 EGS13Cha create and disperse into the universe? Nucleosynthesis & Elements
Core-collapse supernovae like EGS13Cha 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 EGS13Cha leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
The crushing core collapse of EGS13Cha'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 EGS13Cha's explosion site look like in 1,000 to 10,000 years? Cosmic Remnant
Over the coming millennia, the explosion site of EGS13Cha 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 EGS13Cha explode, and where is it located relative to the galactic center? Galactic Environment
EGS13Cha occurred in an uncataloged host galaxy, located at an offset of 0.00″ (0.00 kpc) from the galactic nucleus. In optical and infrared imaging, this positions the explosion within the galaxy's active stellar disk or spiral arms, where ongoing star formation constantly generates massive short-lived stellar progenitors.
Where is EGS13Cha located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, EGS13Cha is located at Right Ascension 14:20:24.200 and Declination +53:03:37.50, situated in the constellation Canes Venatici (The Hunting Dogs). Because its declination is +53:03:37.50, it is primarily placed in the Northern celestial hemisphere.
How much Milky Way interstellar dust obscures our view of EGS13Cha? Interstellar Dust
Light from EGS13Cha passed through interstellar dust in the Milky Way, suffering a foreground color excess of E(B-V) = 0.009 magnitudes (based on Schlafly & Finkbeiner 2011 galactic recalibrations). This cosmic dust absorbs and scatters shorter blue wavelengths, dimming the transient by approximately A_V ≈ 0.03 magnitudes in visual light.
Across which photometric filter bands was EGS13Cha monitored? Astronomical Observations
Photometric light curves for EGS13Cha were acquired through standard astronomical alert streams and survey programs, measuring flux across optical passbands to map its peak magnitude and fading rate.
What did astronomical spectroscopy reveal about EGS13Cha's chemical makeup? Astronomical Observations
Spectroscopic observations of EGS13Cha 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 EGS13Cha and how was it first detected? Discovery & History
EGS13Cha was officially reported on 2013 by an automated robotic transient sky survey. 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 EGS13Cha? Scientific Research
Data for EGS13Cha are compiled from international astronomical notices, the IAU Transient Name Server (TNS), and peer-reviewed astrophysical journals.
How does EGS13Cha contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
As a core-collapse supernova, EGS13Cha 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 EGS13Cha be detected on Earth? Multi-Messenger Astronomy
Core-collapse supernovae like EGS13Cha 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 EGS13Cha 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), EGS13Cha occurred at a distance of 33594.1 Million Light-Years. While historical naked-eye supernovae occurred within our Milky Way or its immediate satellites, modern discoveries like EGS13Cha allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see EGS13Cha tonight with a backyard telescope or binoculars? Backyard Observation
EGS13Cha exploded 13.7 years ago (2013). Optical transient emission has completely faded along its radioactive decay curve. Today, pointing a telescope at these coordinates reveals the expanding remnant nebula or an uncataloged host galaxy; the original optical transient is no longer detectable with amateur backyard equipment.
Does the radiation or shockwave from EGS13Cha 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 33594.1 Million Light-Years, the inverse-square law dilutes the radiation by quintillions of times, making EGS13Cha 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.
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