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SCP-06F6

Type SLSN-I ● Archived outburst (+7439d)
Aliases: J143227.42+333225.1  |  Discovered: 2006/01/03 by Survey Stream
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Host Optical Cutout 0.26″/pix
Pan-STARRS1 DR1 Optical (0.25″/pix)
SCP-06F6 cutout
Interactive Sky ↗

Core Parameters

R.A. (J2000)14:32:27.395 (218.11415°)
Dec. (J2000)+33:32:24.83 (33.54023°)
Spectral TypeSLSN-I
Redshift (z)1.189
Recession Velocity196300 km/s
Luminosity Distance8408.7 Mpc
Peak Apparent Mag21.04
Peak Absolute Mag-22.733
MW Dust E(B-V)0.0083 mag
Host Galaxy—
Host Offset—
Observations0 photometry, 0 spectra

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

🎯 14:32:27.395 +33:32:24.83 FOV: 0.15°
● SCP-06F6 (SLSN-I)
Coordinate Pointing & Airmass
⚠️ Coordinate Pointing Only: The supernova exploded 20.4 years ago (2006/05/21, rest-frame phase +3398.4d). Based on standard radioactive decay physics, it has faded to m ≈ 41.4 (beyond ground telescope limits). Telescope pointing tonight observes the host galaxy, not the vanished transient.
Multi-Band Light Curve
Calibrated Spectra Viewer

Literature & Data Provenance

IDSourceReferenceNASA ADS Bibcode
No sources recorded.

❓ Frequently Asked Questions About SCP-06F6

Scientific & observational Q&As indexed from astronomical databases & the Open Supernova Catalog
What type of supernova is SCP-06F6 and what kind of star exploded? Astrophysics & Progenitor
SCP-06F6 is a rare Superluminous Supernova (SLSN), radiating 10 to 100 times more total light than a standard core-collapse supernova. Such titanic explosions are thought to be powered by an internal central engine—such as a newborn, rapidly spinning millisecond magnetar with a magnetic field exceeding 10¹⁴ Gauss, or the violent collision of expanding blast waves with dense circumstellar gas shells ejected shortly before the star died.
What was the progenitor star doing in the millions of years leading up to SCP-06F6? Astrophysics & Progenitor
Before detonating as SCP-06F6, 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 SCP-06F6 from Earth and how old is the light reaching us? Cosmic Distance & Time
SCP-06F6 is located approximately 27425.5 Million Light-Years from Earth (cosmological redshift z = 1.189, luminosity distance d_L = 8408.7 Mpc). Because electromagnetic radiation travels at 299,792 km/s, the photons detected by modern telescopes began their cosmic voyage 27425.5 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 SCP-06F6 tell us about the expansion of space? Cosmic Distance & Time
SCP-06F6 exhibits a measured spectroscopic redshift of z = 1.1890. Under Hubble's Law, this redshift corresponds to an apparent recessional velocity of approximately 356,453.2 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 SCP-06F6 become at its peak, and how many Suns does that equal? Explosion Energetics
At peak brightness, SCP-06F6 achieved an apparent magnitude of 21.04 around 2006/05/21. Corrected for cosmic distance and foreground interstellar dust, its intrinsic absolute magnitude was -22.733. At this peak, the exploding star radiated with the incandescent brilliance of approximately 106.0 billion Suns combined, briefly outshining the cumulative starlight of entire dwarf galaxies!
How much total energy was released by SCP-06F6, and where did that energy go? Explosion Energetics
The collapse of SCP-06F6'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 SCP-06F6 expanding through space? Explosion Energetics
The debris and shockwave of SCP-06F6 erupted into space at an astounding velocity of approximately 196,300 km/s (measured spectroscopically). This corresponds to roughly 65.5% of the speed of light (Mach 572,303 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 SCP-06F6 weeks and months after detonation? Radioactive Engine
While the initial flash of SCP-06F6 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 SCP-06F6 create and disperse into the universe? Nucleosynthesis & Elements
Core-collapse supernovae like SCP-06F6 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 SCP-06F6 leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
The crushing core collapse of SCP-06F6'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 SCP-06F6's explosion site look like in 1,000 to 10,000 years? Cosmic Remnant
Over the coming millennia, the explosion site of SCP-06F6 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 SCP-06F6 explode, and where is it located relative to the galactic center? Galactic Environment
SCP-06F6 is associated with an uncataloged host galaxy. High-precision astrometry from optical sky surveys pins the explosion coordinates directly to the galaxy's underlying stellar population.
Where is SCP-06F6 located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, SCP-06F6 is located at Right Ascension 14:32:27.395 and Declination +33:32:24.83, situated in the constellation Boötes (The Herdsman). Because its declination is +33:32:24.83, it is primarily placed in the Northern celestial hemisphere.
How much Milky Way interstellar dust obscures our view of SCP-06F6? Interstellar Dust
Light from SCP-06F6 passed through interstellar dust in the Milky Way, suffering a foreground color excess of E(B-V) = 0.008 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 SCP-06F6 monitored? Astronomical Observations
Photometric light curves for SCP-06F6 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 SCP-06F6's chemical makeup? Astronomical Observations
Spectroscopic observations of SCP-06F6 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 SCP-06F6 and how was it first detected? Discovery & History
SCP-06F6 was officially reported on 2006/01/03 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 SCP-06F6? Scientific Research
Data for SCP-06F6 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 SCP-06F6? Cross-Identifications
Throughout global alert streams and survey databases, SCP-06F6 has also been designated as: J143227.42+333225.1. 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 SCP-06F6 contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
As a core-collapse supernova, SCP-06F6 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 SCP-06F6 be detected on Earth? Multi-Messenger Astronomy
Core-collapse supernovae like SCP-06F6 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 SCP-06F6 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), SCP-06F6 occurred at a distance of 27425.5 Million Light-Years. While historical naked-eye supernovae occurred within our Milky Way or its immediate satellites, modern discoveries like SCP-06F6 allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see SCP-06F6 tonight with a backyard telescope or binoculars? Backyard Observation
SCP-06F6 exploded 20.4 years ago (2006/01/03). 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 SCP-06F6 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 27425.5 Million Light-Years, the inverse-square law dilutes the radiation by quintillions of times, making SCP-06F6 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 →