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CLA11Tib

Type — ● Epoch Uncataloged
Aliases: None  |  Discovered: — by Survey Stream
⚡ Re-Enrich Data 📥 Download JSON 📊 Photometry CSV
Host Optical Cutout 0.26″/pix
DESI DR10 Optical (0.26″/pix)
CLA11Tib cutout
Interactive Sky ↗

Core Parameters

R.A. (J2000)02:48:01.27 (42.00529°)
Dec. (J2000)-03:33:16.9 (-3.55469°)
Spectral Type—
Redshift (z)1.143
Recession Velocity192600 km/s
Luminosity Distance8009.1 Mpc
Peak Apparent Mag—
Peak Absolute Mag—
MW Dust E(B-V)0.0263 mag
Host Galaxy—
Host Offset—
Observations0 photometry, 0 spectra

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

🎯 02:48:01.27 -03:33:16.9 FOV: 0.15°
● CLA11Tib (—)
Coordinate Pointing & Airmass
Target Ephemeris: Plots nightly altitude and airmass for target coordinates. Verify transient brightness before observing.
Multi-Band Light Curve
Calibrated Spectra Viewer
🌌 Cosmic Neighbors & Contemporaries 110,222+ Transients Indexed

Cataloged supernovae closest to CLA11Tib in discovery time, spatial sky neighborhood, and cosmological lookback epoch:

⏱️ Closest in Time
No contemporary transients indexed.
🔭 Closest on the Sky
AT2019jhu 2.7′ away
Type Candidate Discovered 2019/01/02
Nero 5.3′ away
Type Transient Discovered 2010
CLA10Cal 6.1′ away
Type Transient Discovered 2010
🌌 Same Cosmic Era (Redshift)
SN2002ki z = 1.141
Type Ia ~15745.8 Mly lookback
HST04Gre z = 1.14
Type Ia ~15732.0 Mly lookback
GRB 071122A z = 1.14
Type LGRB ~15732.0 Mly lookback

Literature & Data Provenance

IDSourceReferenceNASA ADS Bibcode
No sources recorded.

❓ Frequently Asked Questions About CLA11Tib

Scientific & observational Q&As indexed from astronomical databases & the Open Supernova Catalog
What type of supernova is CLA11Tib and what kind of star exploded? Astrophysics & Progenitor
CLA11Tib 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 CLA11Tib? Astrophysics & Progenitor
Before detonating as CLA11Tib, 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 CLA11Tib from Earth and how old is the light reaching us? Cosmic Distance & Time
CLA11Tib is located approximately 26122.2 Million Light-Years from Earth (cosmological redshift z = 1.143, luminosity distance d_L = 8009.1 Mpc). Because electromagnetic radiation travels at 299,792 km/s, the photons detected by modern telescopes began their cosmic voyage 26122.2 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 CLA11Tib tell us about the expansion of space? Cosmic Distance & Time
CLA11Tib exhibits a measured spectroscopic redshift of z = 1.1430. Under Hubble's Law, this redshift corresponds to an apparent recessional velocity of approximately 342,662.8 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 CLA11Tib become at its peak, and how many Suns does that equal? Explosion Energetics
At peak brightness, CLA11Tib 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 CLA11Tib, and where did that energy go? Explosion Energetics
The collapse of CLA11Tib'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 CLA11Tib expanding through space? Explosion Energetics
The debris and shockwave of CLA11Tib erupted into space at an astounding velocity of approximately 192,600 km/s (measured spectroscopically). This corresponds to roughly 64.2% of the speed of light (Mach 561,516 in air)! At this blistering speed, the expanding debris shell traverses the entire diameter of planet Earth in just 0.07 seconds, carving a giant bubble in the interstellar medium.
What powers the prolonged glow of CLA11Tib weeks and months after detonation? Radioactive Engine
While the initial flash of CLA11Tib 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 CLA11Tib create and disperse into the universe? Nucleosynthesis & Elements
Core-collapse supernovae like CLA11Tib 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 CLA11Tib leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
The crushing core collapse of CLA11Tib'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 CLA11Tib's explosion site look like in 1,000 to 10,000 years? Cosmic Remnant
Over the coming millennia, the explosion site of CLA11Tib 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 CLA11Tib explode, and where is it located relative to the galactic center? Galactic Environment
CLA11Tib 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 CLA11Tib located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, CLA11Tib is located at Right Ascension 02:48:01.27 and Declination -03:33:16.9, situated in the constellation Cetus (The Sea Monster). Because its declination is -03:33:16.9, it is favorably placed for Southern Hemisphere observatories.
How much Milky Way interstellar dust obscures our view of CLA11Tib? Interstellar Dust
Light from CLA11Tib passed through interstellar dust in the Milky Way, suffering a foreground color excess of E(B-V) = 0.026 magnitudes (based on Schlafly & Finkbeiner 2011 galactic recalibrations). This cosmic dust absorbs and scatters shorter blue wavelengths, dimming the transient by approximately A_V ≈ 0.08 magnitudes in visual light.
Across which photometric filter bands was CLA11Tib monitored? Astronomical Observations
Photometric light curves for CLA11Tib 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 CLA11Tib's chemical makeup? Astronomical Observations
Spectroscopic observations of CLA11Tib 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 CLA11Tib and how was it first detected? Discovery & History
CLA11Tib was officially reported on — 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 CLA11Tib? Scientific Research
Data for CLA11Tib are compiled from international astronomical notices, the IAU Transient Name Server (TNS), and peer-reviewed astrophysical journals.
How does CLA11Tib contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
As a core-collapse supernova, CLA11Tib 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 CLA11Tib be detected on Earth? Multi-Messenger Astronomy
Core-collapse supernovae like CLA11Tib 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 CLA11Tib 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), CLA11Tib occurred at a distance of 26122.2 Million Light-Years. While historical naked-eye supernovae occurred within our Milky Way or its immediate satellites, modern discoveries like CLA11Tib allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see CLA11Tib tonight with a backyard telescope or binoculars? Backyard Observation
Discovered None days ago (—), CLA11Tib has passed peak maximum and is fading along its radioactive Co-56 decay tail at an estimated apparent magnitude of m ≈ 20.0. It is accessible with sensitive amateur astrophotography rigs or larger research telescopes, depending on local sky darkness.
Does the radiation or shockwave from CLA11Tib 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 26122.2 Million Light-Years, the inverse-square law dilutes the radiation by quintillions of times, making CLA11Tib 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 →