Host Optical Cutout
0.26″/pix
DESI DR10 Optical (0.26″/pix)
Core Parameters
| R.A. (J2000) | 16:30:24.55 (247.60229°) |
|---|---|
| Dec. (J2000) | +23:38:25.0 (23.64028°) |
| Spectral Type | SLSN-I |
| Redshift (z) | 0.5015 |
| Recession Velocity | 115600 km/s (redshift Doppler-equivalent) |
| Luminosity Distance | 2928.8 Mpc (~9273.1 Million Light-Years, μ = 42.27) |
| Reported Magnitude | 19.91 Peak magnitude: Not established |
| Peak Absolute Mag | -21.982 |
| MW Dust E(B-V) | 0.0409 mag |
| Host Galaxy | — |
| Host Offset | — |
| Observations | 0 detections, 0 spectra |
Interactive Sky Field (Aladin) ✨ DSS2 Optical (China-VO mirror)
🎯 16:30:24.55 +23:38:25.0
FOV: 0.15°
● PTF09atu (SLSN-I)
Coordinate Pointing & Airmass
Brightness not measured: discovered 17.3 years ago (2009/07/14). 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
105,868+ transients indexed
Cataloged transients closest to PTF09atu in discovery time, spatial sky neighborhood, and cosmological redshift:
⏱️ Closest in Time
GRB 090715A
+1d after
Type LGRB
2009/07/15
GRB 090715B
+1d after
Type LGRB
2009/07/15
GRB 090712A
2d before
Type LGRB
2009/07/12
Literature & Data Provenance
| ID | Source | Reference | NASA ADS Bibcode |
|---|---|---|---|
| No sources recorded. | |||
❓ Frequently Asked Questions About PTF09atu
Scientific & observational Q&As indexed from astronomical databases & the sne.space
What type of supernova is PTF09atu and what kind of star exploded? Astrophysics & Progenitor
PTF09atu is classified as a superluminous supernova (SLSN). Proposed power sources include magnetar spin-down and ejecta–CSM interaction; which engine applies to this object is not established from the classification label alone.
What was the progenitor star doing in the millions of years leading up to PTF09atu? Astrophysics & Progenitor
The specific progenitor of PTF09atu 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 PTF09atu.
How far away is PTF09atu from Earth and how old is the light reaching us? Cosmic Distance & Time
PTF09atu has a luminosity distance of approximately 9552.5 Million Light-Years (redshift z = 0.5015, d_L = 2928.8 Mpc). Under a flat ΛCDM cosmology (H₀≈70 km/s/Mpc, Ωₘ≈0.3), the corresponding lookback time is ≈5051 Myr — when the light set out 5051.3 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 PTF09atu tell us about the expansion of space? Cosmic Distance & Time
PTF09atu exhibits a measured spectroscopic redshift of z = 0.5015. The cockpit reports a user-facing recession velocity of 115,560.0 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 (≈150,346 km/s) is a different low-z approximation and is not mixed here.
How bright did PTF09atu become at its peak, and how many Suns does that equal? Explosion Energetics
At peak brightness, PTF09atu achieved an apparent magnitude of 19.91 around 2009/08/18. Corrected for cosmic distance and foreground interstellar dust, its intrinsic absolute magnitude was -21.982. At this peak, the exploding star radiated with the incandescent brilliance of approximately 53.1 billion Suns combined, briefly outshining the cumulative starlight of entire dwarf galaxies!
How much total energy was released by PTF09atu, and where did that energy go? Explosion Energetics
SLSN radiated energies can exceed ordinary supernovae by large factors, but the power source (magnetar, CSM interaction, or other) is model-dependent. No object-specific energy release is published for PTF09atu.
How fast are the supernova ejecta and shockwave of PTF09atu expanding through space? Explosion Energetics
Spectroscopic line blueshifts imply an ejecta velocity of approximately 115,600 km/s (~38.6% of c) for PTF09atu. This is distinct from cosmological recession velocity inferred from redshift.
What powers the prolonged glow of PTF09atu weeks and months after detonation? Radioactive Engine
SLSN light curves may be powered by magnetar spin-down, CSM interaction, or (in some models) large ⁵⁶Ni masses. Which engine powers PTF09atu is not established here, and no object-specific nickel mass is published.
What chemical elements did PTF09atu create and disperse into the universe? Nucleosynthesis & Elements
Events of PTF09atu'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 PTF09atu.
Did PTF09atu leave behind a black hole, a neutron star, or nothing at all? Cosmic Remnant
A core-collapse explosion associated with PTF09atu'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 PTF09atu'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 PTF09atu. 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 PTF09atu explode, and where is it located relative to the galactic center? Galactic Environment
No host galaxy is identified for PTF09atu 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 PTF09atu located in the night sky and which constellation is it in? Sky Coordinates
In the celestial sphere, PTF09atu is located at Right Ascension 16:30:24.55 and Declination +23:38:25.0, situated in the constellation Hercules (Hercules). Because its declination is +23:38:25.0, it is primarily placed in the Northern celestial hemisphere.
How much Milky Way interstellar dust obscures our view of PTF09atu? Interstellar Dust
Along this line of sight, the catalog records a Milky Way foreground color excess of E(B−V) = 0.0409 mag (source: published extinction estimate), corresponding to roughly A_V ≈ 0.13 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 PTF09atu monitored? Astronomical Observations
No calibrated photometry is published for PTF09atu. 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 PTF09atu's chemical makeup? Astronomical Observations
No spectrum has been published for PTF09atu. 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 PTF09atu and how was it first detected? Discovery & History
PTF09atu was officially reported on 2009/07/14 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 PTF09atu? Scientific Research
Data for PTF09atu are compiled from international astronomical notices, the IAU Transient Name Server (TNS), and peer-reviewed astrophysical journals.
How does PTF09atu contribute to measuring the Hubble Constant and the scale of the cosmos? Cosmology & Distance Ladder
PTF09atu cannot currently be used for cosmological distance work because its classification is unresolved. The distance ladder relies on type-specific techniques: Type Ia supernovae use the Phillips relation between peak absolute magnitude and decline rate, while Type II events use the Expanding Photosphere Method or SCM-II. An unclassified transient fits neither, so no Hubble-constant constraint can be derived from it until a spectrum establishes its type.
Could gravitational waves or neutrinos from PTF09atu be detected on Earth? Multi-Messenger Astronomy
No neutrino or gravitational-wave counterpart has been reported for PTF09atu, and none is expected to be identifiable without a classification. The multi-messenger signature differs sharply by type: core-collapse events emit a neutrino burst at shock breakout (detected once, for SN 1987A), while thermonuclear Type Ia events produce negligible neutrinos and gravitational waves. Searching for a counterpart before knowing which mechanism applies would be unfocused.
How does PTF09atu 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), PTF09atu occurred at a distance of 9552.5 Million Light-Years. While historical naked-eye supernovae occurred within our Milky Way or its immediate satellites, modern discoveries like PTF09atu allow astrophysicists to probe diverse galactic environments, metallicities, and stellar populations across the broader universe.
Can I see PTF09atu tonight with a backyard telescope or binoculars? Backyard Observation
Unknown — no measured brightness. PTF09atu was discovered 6333 days ago (2009/07/14), 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 PTF09atu 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 9552.5 Million Light-Years, the inverse-square law dilutes the radiation by quintillions of times, making PTF09atu completely harmless to our biosphere and purely a fascinating spectacle for human exploration.
Data sourced from IAU TNS, ALeRCE, WISeREP, and the sne.space.
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