@SciAm @scientific-american-SciAm

#BhupendraMishra +2026: "Our approximate model suggests that #AGN dust tori host the largest populations of #planets in the universe."

https://arxiv.org/abs/2605.19241

#ArXiv_2605_192541

Active Galactic Nucleus Tori: Potential Birthplace to Millions of Planets

The outer regions of AGN disks have temperatures similar to those of circumstellar disks, permitting dust condensation. Therefore, planet formation and growth could be active in these dust tori through similar mechanisms. We aim at quantifying the parameter space for the occurrence of streaming instability, and its outcomes in terms of the masses of the objects formed, their total number, and their continued growth via pebble accretion. We use a a recently proposed disk model with strong magnetization to keep the disk gravitationally stable. We find that the dust grain sizes required for streaming instability are easily attained through coagulation; the dust filaments it produces can contain solar masses, collapsing into tens of millions of planetesimals ranging from Earth to super-Jupiter masses. These planets are usually born in the 3D Bondi regime of pebble accretion, and have mass-doubling times from 10^3 to 10^7 yrs, though 3D Hill and geometric accretion are also realized. Gas accretion occurs concurrently, and crossover mass can be attained while still in the planetary mass range. As a result, vigorous accretion can occur, leading to objects with stellar masses -- defining a core accretion channel for star formation. The pebble isolation mass is beyond the hydrogen burning limit, so accretion is limited by stellar feedback instead of gap carving. Our model also predicts a population of exotic objects directly formed above the hydrogen burning limit, yet of pure dust. Our approximate model suggests that AGN dust tori host the largest populations of planets in the universe.

arXiv.org

Changing-Look Quasars

Figure 1a: The quasar 3C 273, which resides in a giant elliptical galaxy in the constellation of Virgo. Credit: ESA/Hubble & NASA

How do they fit into a biblical creationist model?

Quasars are very high redshift astronomical objects with broad emission line (BEL) spectra. The latter is very different to that in the usual humdrum galaxies. This means the objects redshifts and BEL spectra can be used to identify them. And because of their high redshifts they are assumed to be very distant, very luminous active galaxies with super-massive black holes at their hearts, powering them to emit prodigious amounts of radiation over all wave-bands of the electromagnetic spectrum.

Figure 1b: Spectra of quasar 3C 273 compared to the star Vega. Spectral lines are shifted towards the red end of the spectrum, from which its distance is determined using the standard LCDM cosmology.

Most of the high redshift objects in the universe are quasars. The redshifts of galaxies and quasars when interpreted within big bang cosmology—the greater the redshift the greater the distance—means that the most distant objects are seen at a time when the Universe was youngest.1

Following big bang thinking, quasars are then considered to be just galaxies in some early stage of development—back closer in time to the big bang—than the usual spiral and elliptical galaxies we might see with much lower redshifts. The quasar 3C 273, shown in Fig. 1a, the first to be identified (discovered in the early 1960s by astronomer Allan Sandage), has been shown to reside in a giant elliptical galaxy in the constellation of Virgo. According to standard cosmology its redshift puts it at a distance of 2.5 billion light-years from Earth.

Quasar to galaxy transitions

According to the big bang theory, how long should a quasar remain in the form of a quasar before transitioning into a normal galaxy and how long should that transition take? Quite obviously the answer to that question depends on one having a correct understanding of what quasars actually are and an accurate model describing their evolution. It would be no underestimate to state that an accurate model for galaxy formation, let alone a transition from a quasar to a normal field galaxy, is far from being known. The formation of a galaxy alone requires the invoking of a very large dark matter content, and often ‘jumping over’ the important details of star formation just to obtain something that looks like a galaxy. This means that there are physical laws in this Universe that create barriers in computer simulations preventing the formation of stars and hence galaxies. It is these that must be ‘jumped over’ in order that the simulations may proceed.2

We can assume that quasars have masses comparable to that of most galaxies. From that is follows then that naturalistic changes—that is, uniformitarian changes—can be expected to be of the order of a billion years.3 Without any real model for the changes expected in quasars, it may not be too unreasonable to expect any changes in their luminosity to be over uniformitarian timescales, and fuelled by growth of their supermassive black-holes, as some propose.

By contrast, according to the Genesis 1 narrative, God took one 24-hour day to create all astronomical objects, therefore we expect at creation that the youngest sources (which could include quasars) have very quickly changing observable features, such as luminosity. Yet very rapid changes, even down to timescales of days and weeks, in the observed luminosity of quasars have been recorded.4,5 One suggestion is that those variations are caused by microlensing6 and another is obscuration by dust but these mechansims are considered to be too long.7 Another is the rapid consumption of a passing star or gas and dust by the central supermassive black hole. Such proposals are offered because changes on such short timescales are not expected from the growth of the alleged supermassive black-holes at the heart of the quasars.

Changing-look quasars

Now we read in an online news report8 that astronomers think that they have detected a dozen quasars in a disappearing act—the so-called “changing-look quasars.” Or they have been caught transitioning into their quiescent and dimmer counterparts—galaxies with starving black holes at their cores. This fact has left astronomers asking whether these objects are shutting down permanently or simply flickering out for the time being.

Last year Stephanie LaMassa from NASA Goddard Space Flight Center (then at Yale University) discovered the greatest change in luminosity ever detected in a quasar. She was digging through data from the Sloan Digital Sky Survey when she found that a quasar had dimmed in brightness by a factor of six in just 10 years. Its spectrum changed, too, from that of a classic quasar to a regular galaxy.8 (my emphasis added)

Figure 2: The image shows an artist’s conception of the ‘changing-look quasar’ as is appeared in early 2015. The glowing blue region shows the last of the gas being swallowed by the central black hole as it shuts off. The spectrum is the previous one obtained by the SDSS in 2003. Credit: Dana Berry / SkyWorks Digital, Inc.; SDSS collaboration.

Because astronomers believe in the very long time scale big bang paradigm they are forced to suggest any rapid dimming in the luminosity of any quasar must be either a transient effect or the very rare chance of observing the fuel exhausted from a supermassive black hole.  One report states that,

“Astronomers can’t find any sign of the black hole at the center of the quasar SDSS J1011+5442, and they couldn’t be happier.”9

In the case of this quasar (see Fig. 2) it is alleged that,

“… over the past ten years, it appears to have swallowed all the gas in its vicinity. With the gas fallen into the black hole, astronomers from the Sloan Digital Sky Survey (SDSS) were unable to detect the spectroscopic signature of the quasar, which now appears as an otherwise normal galaxy.”9 (my emphasis added)

The dimming was very significant and now appears like a normal humdrum galaxy.

“The difference was stunning and unprecedented,” said John Ruan of the University of Washington, lead author of a related paper ….. “The hydrogen-alpha emission dropped by a factor of 50 in less than twelve years, and the quasar now looks like a normal galaxy.” The change was so great that throughout the SDSS collaboration and astronomy community, the quasar became known as a “changing-look quasar.”9 (my emphasis added)

However, one of the newly discovered rapidly dimming quasar did re-brighten.

“And one of the 12 newly discovered objects did not just disappear but reappear. Krolik thinks that this lonely quasar blazed back into existence for the same reason that it flickered out: a variation in the gas and dust flowing onto the black hole.”8 (my emphasis added)

Certainly it is possible that the standard interpretation for quasars as AGNs10 powered by a supermassive black-hole is one possible explanation. The next step then will be to see if any of the other newly discovered dozen or so quasars re-brighten over the coming years.

A different explanation

A different explanation is one consistent with the work of the late Halton Arp11 where he suggested that quasars are born from the hearts of active parent galaxies. Over time, which he had no measure of, the ejected quasars transitioned from active highly luminous high redshift objects with BEL line spectra to the usual field galaxies with much lower redshifts and typical spectra.  This is illustrated in Fig. 3. Quasars are ejected in opposite directions from the nucleus of an active galaxy and over time they change their internal state including redshift, which decreases with finite discrete steps towards the commonly observed low redshift in field galaxies. Thus quasars and active galactic nuclei become normal galaxies.

Figure 3: Arp’s model of ejection of quasars from active parent galaxies and their eventual change to normal galaxies. Reproduced from Ref. 11 after Arp’s original in his book “Seeing Red.”

Apparently the idea that quasars or active galactic nuclei could become inactive is not controversial in the big bang universe. But the expected timescale is not less than tens of thousands of years. What LaMassa and her colleagues doubted was that a quasar could go from active to inactive in just 10 years.  But this is what these newly discovered rapidly dimming quasars have established. Rapid changes in the emission properties of the quasars, on timescales very much in line with a creation scenario, are observed. Even their spectra changing from that of a classic quasar to a regular galaxy.9

A biblical creation explanation

So this discovery is consistent with a creation scenario where we expect that processes in astronomical sources to be well less than seven thousand years. In the case of a creation process of galaxies formed from AGNs—the parent galaxies—and the ejected galaxies in the form of quasars, it would be essential that the quasars (at least some of them) have changed to normal humdrum galaxies in a period less than the time since Creation, that is less than about six thousand years.

However, it is also expected that many galaxies were created in their current forms, but if Arp’s evidence for quasars and active galactic nuclei transitioning to normal galaxies is correct, then this is what would be expected in the biblical creation model. Here we have an opportunity to see if these rapidly dimmed quasars, remain dim or re-brighten. Time will tell.

References

  • This claim I dispute as there is evidence that puts this idea in doubt.  There is strong evidence, even in the very large galaxy surveys that suggests a very high probability of high redshift quasars being associated with low redshift parent galaxies.
  • Hartnett, J.G., Stars just don’t form naturally—‘dark matter’ the ‘god of the gaps’ is needed, September 1, 2015.
  • Back of the envelope calculation for the formation of a typical sized galaxy and hence quasar from the free collapse of a proto-Galactic cloud is of order 1 billion years. See B.W. Carroll & D.A. Ostlie, An Introduction to Modern Astrophysics, 1st Edition. pp. 1074-75, 1996.
  • M.R.S. Hawkins, Time dilation and quasar variability, Astrophys. J. 553:L97–L100, 2001.
  • M.R.S. Hawkins, On time dilation in quasar light curves, MNRAS 405:1940–1946, 2010.
  • When a quasar is sufficiently aligned with a massive compact foreground object the bending of light due to its gravitational field is distorted, resulting in an observable magnification. The timescale of the transient brightening depends on the mass of the foreground object as well as on the relative proper motion between the background ‘source’ and the foreground ‘lens’ object.
  • C.L. MacLeod, et al., A systematic search for changing-look quasars in SDSS, MNRAS, 457(1): 389-404, 2016.
  • S. Hall, The Case of the Disappearing Quasars, Scientific American, November 23, 2015
  • J. Raddick, The Case of the Missing Quasar, SDSS, January 6, 2015.
  • AGN = Active Galactic Nucleus
  • J.G. Hartnett, The heavens declare a different story, May 3, 2014; Journal of Creation 17(2):94–97, August 2003.
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    Weekly Update from the Open Journal of Astrophysics – 02/05/2026

    Here we are, on schedule, with another update of activity at the Open Journal of Astrophysics. Since the last update we have published a further seven papers, bringing the number in Volume 9 (2026) to 94 and the total so far published by OJAp up to 542. I checked the corresponding update for last year (on 3rd May 2025), and we’ve had an increase from 54 to 94 in papers published (about 74%) between the first four months of 2025 and the first four months of 2026.

    I will continue to include the posts made on our Mastodon account (on Fediscience) to encourage you to visit it. Mastodon is a really excellent service, and a more than adequate replacement for X/Twitter (which nobody should be using); these announcements also show the DOI for each paper.

    The first paper to report this week is “DESI-DR1 3 × 2-pt analysis: consistent cosmology across weak lensing surveys” by Anna Porredon (CIEMAT, Madrid, Spain) and 72 others (DESI Colllaboration). This paper was published on Tuesday 28th April in the folder Cosmology and Nongalactic Astrophysics. This paper presents a joint cosmological analysis of galaxy clustering and gravitational lensing observations, providing consistent constraints on cosmological parameters. The analysis also introduces a new blinding procedure to prevent confirmation bias. See this post for news of an important DESI milestone.

    The overlay for this paper is here

    You can find the officially accepted version on arXiv here and the announcement on Fediverse here:

    https://fediscience.org/@OJ_Astro/116480407578621011

    The second paper for this week, also published on Tuesday 28th April but in the folder High-Energy Astrophysical Phenomena is “Masers and Broad-Line Mapping Favor Magnetically-Dominated AGN Accretion Disks” by Philip F. Hopkins (Caltech, USA), Dalya Baron (Stanford U., USA) and Joanna M. Piotrowska (Caltech). This one presents a new constraint on supermassive black hole accretion disks physics, suggesting that outer regions are likely in a ‘hyper-magnetized’ state, as thermal or radiation pressure models appear inconsistent.

    The overlay for this one is here:

    The official version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/116480505354195181

    Next one up, the third paper of the week, is “Galaxy mergers and disk angular momentum evolution: stellar halos as a critical test” by Eric F. Bell (U. Michigan, Ann Arbor, USA), Richard D’Souza (Vatican Observatory), Monica Valluri & Katya Gozman (U. Michigan). This was published on Wednesday 29th April in the folder Astrophysics of Galaxies. The paper argues that satellite accretion impacts the angular momentum evolution of galaxies, often causing significant reorientation. This process is detectable in Milky Way-mass galaxies so the idea is testable observationally.

    The overlay for this one is here:

    The final, accepted version can be found on arXiv here and the Mastodon announcement is here:

    https://fediscience.org/@OJ_Astro/116486649450860283

    The fourth paper this week, published on Thursday April 30th, is “Time-Dilation Methods for Extreme Multiscale Timestepping Problems” by Philip F. Hopkins and Elias R. Most (Caltech, USA). This paper is in the folder Instrumentation and Methods for Astrophysics: it presents a new method for astrophysical simulations that modulates time evolution with a variable dilation/stretch factor, improving efficiency and accuracy in modeling processes across different scales.

    The overlay is here:

    The finally accepted version of this paper can be found here and the Mastodon announcement follows:

    https://fediscience.org/@OJ_Astro/116492226856595031

    The fifth article of this week was also published on Thursday 30th April, but in the folder Astrophysics of Galaxies. The title is “Cosmic Rays on Galaxy Scales: Progress and Pitfalls for CR-MHD Dynamical Models” and the author is Philip F. Hopkins (Caltech, USA) who has three papers featured this week. The paper presents an overview of cosmic ray (CR) modeling, highlighting its influence on galactic physics and star formation. It addresses previous modeling errors and presents new methods for full-spectrum dynamics.

    The overlay is here:

    You can find the authorized version of this paper on arXiv here and the Fediverse announcement is here:

    https://fediscience.org/@OJ_Astro/116492282488422075

    The sixth paper of the week is “Baryonification III: An accurate analytical model for the dispersion measure probability density function of fast radio bursts” by MohammadReza Torkamani (Universität Bonn, Germany) and 8 others based in Germany, Switzerland, UK and Sweden. This article was also published on Thursday April 30th in the folder Cosmology and Nongalactic Astrophysics. It presents a framework for predicting dispersion measures of fast radio bursts using the baryonification model, providing a cost-effective alternative to hydrodynamical simulations. The model’s accuracy is validated through full numerical simulations. The overlay is here:

    You can find the officially-accepted version on arXiv here and the Mastodon announcement here:

    https://fediscience.org/@OJ_Astro/116492403170125062

    Seventh and finally for this week we have “The stellar and dark matter distributions in early-type galaxies measured by stacked weak gravitational lensing” by Momoka Fujikawa and Masamune Oguri (Chiba University, Japan). This study uses weak gravitational lensing to investigate stellar mass and dark matter density in red galaxies, suggesting a stronger feedback effect than current simulations predict. This was published on Friday 1st May 2026 in the folder Astrophysics of Galaxies. The overlay is here:

    You can find the officially-accepted version on arXiv here and the Fediverse announcement is here:

    https://fediscience.org/@OJ_Astro/116497987401632687

    And that concludes this week’s update. I’ll do another one at the end of next week. Will Vol. 9 have reached a hundred by then?

    P.S. Just a reminder that, thanks to the efforts of a member of our Editorial Board, the Open Journal of Astrophysics now has a Wikipedia page.

    #32PtAnalysis #ActiveGalacticNuclei #AGN #arXiv250907104v2 #arXiv251009756v2 #arXiv251209342v2 #arXiv251215960v3 #arXiv260106253v2 #arXiv260118784v2 #arXiv260424965v1 #AstrophysicsOfGalaxies #baryonification #ComputationalAstrophysics #cosmicRays #CosmologyAndNonGalacticAstrophysics #DarkEnergySpectroscopicInstrument #DESI #DiamondOpenAccess #DiamondOpenAccessPublishing #DispersionMeasures #fastRadioBursts #galacticCosmicRays #galaxyEvolution #galaxyFormation #galaxyMergers #HighEnergyAstrophysicalPhenomena #InstrumentationAndMethodsForAstrophysics #magnetohydrodynamics #masers #MilkyWay #OpenAccess #OpenAccessPublishing #SolarAndStellarAstrophysics #SolarCorona #supermassiveBlackHoles #VeraCRubinObservatory #weakGravitationalLensing #wikipedia
    Une galaxie a perdu 95% de sa lumière en 20 ans… son trou noir semble “s’éteindre”. Un phénomène rare qui bouscule nos modèles www.techno-science.net/actualite/ga... #Space #Science #Innovation #Astrophysics #BlackHole #Galaxies #AGN #NewSpace

    🔆 Une galaxie perd 95% de sa l...
    🔆 Une galaxie perd 95% de sa luminosité en 20 ans: pourquoi ?

    En comparant des images archivées sur vingt ans, des astronomes ont observé un phénomène inhabituel. Grâce à des...

    Techno-Science.net
    Une galaxie a perdu 95% de sa lumière en 20 ans… son trou noir semble “s’éteindre”. Un phénomène rare qui bouscule nos modèles
    https://www.techno-science.net/actualite/galaxie-perd-95-sa-luminosite-20-ans-pourquoi-N28611.html #Space #Science #Innovation #Astrophysics #BlackHole #Galaxies #AGN #NewSpace
    🔆 Une galaxie perd 95% de sa luminosité en 20 ans: pourquoi ?

    En comparant des images archivées sur vingt ans, des astronomes ont observé un phénomène inhabituel. Grâce à des...

    Techno-Science.net

    @MPIfR_Bonn Spannende Sache. Dass Markarian 501 eventuell ein binäres supermassereiches Schwarzes Loch im Zentrum hat, wurde schon 2003 von Rieger und Mannheim vorgeschlagen.
    https://ui.adsabs.harvard.edu/abs/2003A%26A...397..121R/abstract

    #SMBH #Astrophysics #Mrk501 #AGN

    On the central black hole mass in Mkn 501

    We analyse the apparent disagreement between the mass estimates of the central black hole(s) in Mkn 501 based on (i) the observations of the host galaxy, (ii) the high energy (HE) emission mechanism, and (iii) the modulation of the beamed radiation by a black hole (BH) binary system. While method (i) seems to imply a central mass ga 5x 10<SUP>8</SUP> M<SUB>sun</SUB>, method (ii) suggests a BH mass less than =~ 6 x 10<SUP>7</SUP> M<SUB>sun</SUB>. We critically discuss the estimates inferred from (i) showing that current uncertainties may permit a central mass as low as =~ (2-3)x 10<SUP>8</SUP> M<SUB>sun</SUB>. We demonstrate that in this case the estimates (i) and (ii) might be brought into agreement by assuming a binary BH system where the jet dominating the HE emission originates from the less massive (secondary) BH as suggested by method (iii). On the other hand, if Mkn 501 has in fact a high central BH mass of order 10<SUP>9</SUP> M<SUB>sun</SUB>, a change of fundamental assumptions seems to be required in the context of several HE emission models. We show, that in this case a binary scenario following (iii) may be still possible if the jet which dominates the emission emerges from the more massive (primary) BH and if the binary evolution passes through phases of super-Eddington accretion and/or decreased conversion efficiency.

    ADS
    ReveaLLAGN 1 - JWST Emission-Line Spectra Reveal Low-Luminosity #AGN with UV-Deficient SEDs and Warm Molecular Gas: https://arxiv.org/abs/2601.16977 -> James Webb Space Telescope uncovers secret supermassive black holes that escape traditional detection: https://www.space.com/astronomy/james-webb-space-telescope/james-webb-space-telescope-uncovers-secret-supermassive-black-holes-that-escape-traditional-detection
    ReveaLLAGN 1: JWST Emission-Line Spectra Reveal Low-Luminosity AGN with UV-Deficient SEDs and Warm Molecular Gas

    We present near- and mid-infrared spectra of eight Low-Luminosity Active Galactic Nuclei (LLAGN), spanning nearly four orders of magnitude in black hole mass and Eddington ratio, obtained with JWST/NIRSpec and MIRI as part of the ReveaLLAGN program along with identical archival data of Cen A. The high spatial resolution of JWST cleanly separates AGN emission from host-galaxy contamination, enabling detections of high-ionization potential lines more than an order of magnitude fainter than previously measured. Emission-line diagnostics reveal a transition at log($L_{bol}/L_{Edd}$) ~ -3.5, where the spectral energy distribution becomes increasingly deficient in ultraviolet photons. We find that rotational H$_2$ excitation temperatures are elevated (~500 K higher) compared to both higher-luminosity AGN and star-forming galaxies, while the H$_2$(0-0)S(3)/PAH$_{11.3 μm}$ ratios are consistent with those observed in the AGN population. We discuss the possible roles of outflows, jets, and X-ray dominated regions in shaping the interstellar medium surrounding LLAGN. Silicate emission at ~10 $μ$m, localized to the nuclear region, is detected in most ReveaLLAGN targets. This dataset offers the first comprehensive JWST-based characterization of infrared emission lines in the nuclear regions of LLAGN.

    arXiv.org

    #TachyonBeam #astronomy #galaxies #SMBH #AGN

    A rare example of three active galactic nuclei in three merging galaxies has been discovered using two radio telescopes: the VLA and the VLBA. The triple system is cataloged as J1218/1219+1035. This targeted study, conducted by a team of researchers at various radio frequencies, has identified only the third case of a triple active galactic nucleus, the first confirmed through radio observations.

    https://english.tachyonbeam.com/2025/12/31/a-rare-case-of-three-active-galactic-nuclei-in-three-merging-galaxies-has-been-discovered/

    A rare case of three active galactic nuclei in three merging galaxies has been discovered

    A rare example of three active galactic nuclei in three merging galaxies has been discovered using two radio telescopes: the VLA and the VLBA. The triple...

    The First Triple Radio Active Galactic Nucleus in an Ongoing Galaxy Merger: https://iopscience.iop.org/article/10.3847/2041-8213/ae2002 -> A unique discovery - astronomers identify the first triple radio #AGN / Radio Black Hole Trio Lights Up in Rare Galaxy Merger: https://www.dvidshub.net/news/555300/unique-discovery-astronomers-identify-first-triple-radio-agn / https://public.nrao.edu/news/radio-black-hole-trio-lights-up-in-rare-galaxy-merger/ - first confirmed system of three radio-bright active galactic nuclei reveals how supermassive black holes grow as galaxies collide.
    The First Triple Radio Active Galactic Nucleus in an Ongoing Galaxy Merger

    The First Triple Radio Active Galactic Nucleus in an Ongoing Galaxy Merger, Schwartzman, Emma, Pfeifle, Ryan W., Clarke, Tracy E., Weaver, Kimberly A., Secrest, Nathan J., Rothberg, Barry, McCarthy, Miranda, Stern, Daniel, Boorman, Peter G., Piotrowska, Joanna

    La Revista del Archivo General de la Nación, publicación especializada en historia, archivística, patrimonio documental y disciplinas afines, se complace en invitar a la convocatoria para el próximo volumen de nuestra revista, enviando sus artículos originales para evaluación y eventual publicación.

    👉 https://revista.agn.gob.pe/ojs/index.php/ragn/about

    Instructivo:
    👉 https://revista.agn.gob.pe/.../ragn/information/authors

    Consultas:
    [email protected]

    #Revista #AGN #Cultura