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PTF11emc

Type II ● Brightness Unmeasured
Aliases: None  |  Discovered: 2011/06/01 by PTF
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Host Optical Cutout 0.26″/pix
Pan-STARRS1 DR1 Optical (0.25″/pix)
PTF11emc cutout
Interactive Sky ↗

Core Parameters

R.A. (J2000)15:18:43.72 (229.68217°)
Dec. (J2000)+33:07:56.1 (33.13225°)
Spectral TypeII
Redshift (z)0.082
Recession Velocity24000 km/s (redshift Doppler-equivalent)
Luminosity Distance385 Mpc (~1216.1 Million Light-Years, μ = 37.86)
Reported Magnitude21.1
Peak magnitude: Not established
Peak Absolute Mag-16.7
MW Dust E(B-V)0.0152 mag
Host Galaxy—
Host Offset—
Observations0 detections, 0 spectra

Interactive Sky Field (Aladin) ✨ DSS2 Optical (China-VO mirror)

🎯 15:18:43.72 +33:07:56.1 FOV: 0.15°
● PTF11emc (II)
Coordinate Pointing & Airmass
Brightness not measured: discovered 15.4 years ago (2011/06/01). No calibrated photometry is published. No reliable current brightness estimate is available.
Multi-Band Light Curve
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Calibrated Spectra Viewer

Literature & Data Provenance

IDSourceReferenceNASA ADS Bibcode
No sources recorded.

❓ Frequently Asked Questions About PTF11emc

Scientific & observational Q&As indexed from astronomical databases & the Open Supernova Catalog
What type of supernova is PTF11emc and what kind of star exploded? Astrophysics & Progenitor
PTF11emc is classified as a Type II supernova, consistent with core collapse of a massive star that retained hydrogen in its outer envelope. Typical progenitor mass ranges quoted for the class are model expectations, not a measured mass for this star.
What was the progenitor star doing in the millions of years leading up to PTF11emc? Astrophysics & Progenitor
The specific progenitor of PTF11emc 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 PTF11emc.
How far away is PTF11emc from Earth and how old is the light reaching us? Cosmic Distance & Time
PTF11emc has a luminosity distance of approximately 1255.7 Million Light-Years (redshift z = 0.082, d_L = 385 Mpc). Under a flat ΛCDM cosmology (H₀≈70 km/s/Mpc, Ωₘ≈0.3), the corresponding lookback time is ≈1080 Myr — when the light set out 1080.5 million years ago in deep Precambrian time, well before multicellular animals dominated Earth. 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 PTF11emc tell us about the expansion of space? Cosmic Distance & Time
PTF11emc exhibits a measured spectroscopic redshift of z = 0.0820. The cockpit reports a user-facing recession velocity of 23,578.2 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 (≈24,583 km/s) is a different low-z approximation and is not mixed here.
How bright did PTF11emc become at its peak, and how many Suns does that equal? Explosion Energetics
At peak brightness, PTF11emc achieved an apparent magnitude of 21.1 around 2011/05/31. Corrected for cosmic distance and foreground interstellar dust, its intrinsic absolute magnitude was -16.7. At this peak, the exploding star radiated with the incandescent brilliance of approximately 409.3 million Suns combined, briefly outshining the cumulative starlight of entire dwarf galaxies!
How much total energy was released by PTF11emc, 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 PTF11emc.
How fast are the supernova ejecta and shockwave of PTF11emc expanding through space? Explosion Energetics
Spectroscopic line blueshifts imply an ejecta velocity of approximately 24,000 km/s (~8.0% of c) for PTF11emc. This is distinct from cosmological recession velocity inferred from redshift.
What powers the prolonged glow of PTF11emc 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 PTF11emc. 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 PTF11emc create and disperse into the universe? Nucleosynthesis & Elements
Events of PTF11emc's broad spectroscopic class are discussed in galactic chemical evolution as sources of oxygen-group and intermediate-mass elements (and, for some channels, iron-peak material). No measured elemental yields are published for PTF11emc.
Did PTF11emc leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
A core-collapse explosion associated with PTF11emc'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 PTF11emc'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 PTF11emc. 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 PTF11emc explode, and where is it located relative to the galactic center? Galactic Environment
No host galaxy is identified for PTF11emc in this catalog record. A blank host field means the association is unresolved here—it does not establish that the host is uncataloged, resolved in imaging, or securely linked by astrometry. Possible states (unidentified, hostless candidate, imaging detection without a catalog name, or a securely matched cataloged galaxy) require separate evidence that is not present in this field.
Where is PTF11emc located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, PTF11emc is located at Right Ascension 15:18:43.72 and Declination +33:07:56.1, situated in the constellation Corona Borealis (The Northern Crown). Because its declination is +33:07:56.1, it is primarily placed in the Northern celestial hemisphere.
How much Milky Way interstellar dust obscures our view of PTF11emc? Interstellar Dust
Along this line of sight, the catalog records a Milky Way foreground color excess of E(B−V) = 0.0152 mag (source: published extinction estimate), corresponding to roughly A_V ≈ 0.05 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 PTF11emc monitored? Astronomical Observations
No calibrated photometry is published for PTF11emc. 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 PTF11emc's chemical makeup? Astronomical Observations
No spectrum has been published for PTF11emc. 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 PTF11emc and how was it first detected? Discovery & History
PTF11emc was officially reported on 2011/06/01 by PTF. 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 PTF11emc? Scientific Research
Data for PTF11emc are compiled from international astronomical notices, the IAU Transient Name Server (TNS), and peer-reviewed astrophysical journals.
How does PTF11emc contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
As a core-collapse supernova, PTF11emc 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 PTF11emc be detected on Earth? Multi-Messenger Astronomy
Core-collapse supernovae like PTF11emc 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 PTF11emc 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), PTF11emc occurred at a distance of 1255.7 Million Light-Years. While historical naked-eye supernovae occurred within our Milky Way or its immediate satellites, modern discoveries like PTF11emc allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see PTF11emc tonight with a backyard telescope or binoculars? Backyard Observation
Unknown — no measured brightness. PTF11emc was discovered 5636 days ago (2011/06/01), 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 PTF11emc 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 1255.7 Million Light-Years, the inverse-square law dilutes the radiation by quintillions of times, making PTF11emc 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 →