Host Optical Cutout
0.26″/pix
DESI DR10 Optical (0.26″/pix)
Core Parameters
| R.A. (J2000) | 23:23:08.01 (350.78337°) |
|---|---|
| Dec. (J2000) | +13:02:39.2 (13.04422°) |
| Spectral Type | II |
| Redshift (z) | 0.042636 |
| Recession Velocity | 12510 km/s (redshift Doppler-equivalent) |
| Luminosity Distance | 194.776 Mpc (~614.9 Million Light-Years, μ = 36.38) |
| Reported Magnitude | 19.59 Peak magnitude: Not established |
| Peak Absolute Mag | -16.8124 |
| MW Dust E(B-V) | 0.0484 mag |
| Host Galaxy | PGC 71280 |
| Host Offset | — |
| Observations | 0 detections, 0 spectra |
Interactive Sky Field (Aladin) ✨ DSS2 Optical (China-VO mirror)
🎯 23:23:08.01 +13:02:39.2
FOV: 0.15°
● PTF10pjg (II)
Coordinate Pointing & Airmass
Brightness not measured: discovered 16.3 years ago (2010/07/11). No calibrated photometry is published. No reliable current brightness estimate is available.
Multi-Band Light Curve
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Calibrated Spectra Viewer
🌌 Cosmic Neighbors & Contemporaries
105,768+ transients indexed
Cataloged transients closest to PTF10pjg in discovery time, spatial sky neighborhood, and cosmological redshift:
⏱️ Closest in Time
PSc060157
Exploded same day
Type Ia
2010/07/11 · Mag 21.65
PSc060199
Exploded same day
Type Ia
2010/07/11 · Mag 21.93
PSc060238
Exploded same day
Type Ia
2010/07/11 · Mag 21.89
Literature & Data Provenance
| ID | Source | Reference | NASA ADS Bibcode |
|---|---|---|---|
| No sources recorded. | |||
❓ Frequently Asked Questions About PTF10pjg
Scientific & observational Q&As indexed from astronomical databases & the Open Supernova Catalog
What type of supernova is PTF10pjg and what kind of star exploded? Astrophysics & Progenitor
PTF10pjg 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 PTF10pjg? Astrophysics & Progenitor
The specific progenitor of PTF10pjg 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 PTF10pjg.
How far away is PTF10pjg from Earth and how old is the light reaching us? Cosmic Distance & Time
PTF10pjg has a luminosity distance of approximately 635.3 Million Light-Years (redshift z = 0.042636, d_L = 194.776 Mpc). Under a flat ΛCDM cosmology (H₀≈70 km/s/Mpc, Ωₘ≈0.3), the corresponding lookback time is ≈578 Myr — when the light set out 577.6 million years ago during the Neoproterozoic, hundreds of millions of years before complex animal life diversified. 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 PTF10pjg tell us about the expansion of space? Cosmic Distance & Time
PTF10pjg exhibits a measured spectroscopic redshift of z = 0.0426. The cockpit reports a user-facing recession velocity of 12,509.7 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 (≈12,782 km/s) is a different low-z approximation and is not mixed here.
How bright did PTF10pjg become at its peak, and how many Suns does that equal? Explosion Energetics
At peak brightness, PTF10pjg achieved an apparent magnitude of 19.59 around 2010/08/29. Corrected for cosmic distance and foreground interstellar dust, its intrinsic absolute magnitude was -16.8124. At this peak, the exploding star radiated with the incandescent brilliance of approximately 453.9 million Suns combined, briefly outshining the cumulative starlight of entire dwarf galaxies!
How much total energy was released by PTF10pjg, 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 PTF10pjg.
How fast are the supernova ejecta and shockwave of PTF10pjg expanding through space? Explosion Energetics
Spectroscopic line blueshifts imply an ejecta velocity of approximately 12,510 km/s (~4.2% of c) for PTF10pjg. This is distinct from cosmological recession velocity inferred from redshift.
What powers the prolonged glow of PTF10pjg 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 PTF10pjg. 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 PTF10pjg create and disperse into the universe? Nucleosynthesis & Elements
Events of PTF10pjg'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 PTF10pjg.
Did PTF10pjg leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
A core-collapse explosion associated with PTF10pjg'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 PTF10pjg'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 PTF10pjg. 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 PTF10pjg explode, and where is it located relative to the galactic center? Galactic Environment
PTF10pjg is cataloged with host galaxy PGC 71280. No secure nuclear offset is published in this record.
Where is PTF10pjg located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, PTF10pjg is located at Right Ascension 23:23:08.01 and Declination +13:02:39.2, situated in the constellation Pegasus (The Winged Horse). Because its declination is +13:02:39.2, it is primarily placed in the Northern celestial hemisphere.
How much Milky Way interstellar dust obscures our view of PTF10pjg? Interstellar Dust
Along this line of sight, the catalog records a Milky Way foreground color excess of E(B−V) = 0.0484 mag (source: published extinction estimate), corresponding to roughly A_V ≈ 0.15 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 PTF10pjg monitored? Astronomical Observations
No calibrated photometry is published for PTF10pjg. 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 PTF10pjg's chemical makeup? Astronomical Observations
No spectrum has been published for PTF10pjg. 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 PTF10pjg and how was it first detected? Discovery & History
PTF10pjg was officially reported on 2010/07/11 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 PTF10pjg? Scientific Research
Data for PTF10pjg are compiled from international astronomical notices, the IAU Transient Name Server (TNS), and peer-reviewed astrophysical journals.
How does PTF10pjg contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
As a core-collapse supernova, PTF10pjg 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 PTF10pjg be detected on Earth? Multi-Messenger Astronomy
Core-collapse supernovae like PTF10pjg 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 PTF10pjg 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), PTF10pjg occurred at a distance of 635.3 Million Light-Years. While historical naked-eye supernovae occurred within our Milky Way or its immediate satellites, modern discoveries like PTF10pjg allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see PTF10pjg tonight with a backyard telescope or binoculars? Backyard Observation
Unknown — no measured brightness. PTF10pjg was discovered 5959 days ago (2010/07/11), 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 PTF10pjg 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 635.3 Million Light-Years, the inverse-square law dilutes the radiation by quintillions of times, making PTF10pjg 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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