Snippets

compiled by Arlene & David Kaplan

-NYT

Fighting for ‘The Right to Night’ Under Starry, Rural Skies On a Saturday in September in Michigan’s Upper Peninsula, a dozen people navigated through the woods to the shore of Lake Superior, where the waves licked softly against the land. Above, a wash of stars filled the blue-black sky, cut in half by the haze of the Milky Way…more

-NASA
-NYT

Why the Rings of Saturn Seem as if They’re About to Disappear If you head into your backyard this weekend and set up your telescope, the giant planet Saturn will be there for you to see. “Saturn is a spectacular object to look at,” said Damian Peach, an English astrophotographer who frequently observes the giant planet. “Even with small telescopes, you can see the rings.”….more

-NYT

The Moon Was an Inside Job Not long after Earth formed, it received an almighty sucker punch when an object roughly the size of Mars slammed right into it. The interloper, known as Theia, was destroyed, and parts of it and Earth were sprayed into space. The result was the moon….more

-NASA

Almost Everything About NASA’s Latest Mission to Mars Is Unusual NASA’s latest robotic mission to Mars, ESCAPADE, should perhaps have been named the Great Escape, given how many times it has eluded doom. The data that the mission eventually collects will provide clues about why Mars, which once possessed a thick atmosphere and flowing water on its surface, is today cold, dry and almost airless…..more

-NYT

The ‘Lost Sisters’ of the Pleiades Fill the Entire Night Sky Look to the east after sunset on a clear winter night and you’ll spot a bright, tightly packed collection of stars. That’s the Pleiades, a star cluster 445 light-years from Earth that has inspired both myth and measurement for centuries….more

-NYT

Northern Lights Bring Dazzling Views to Northeast The northern lights could be seen in skies as far south as Texas late Tuesday and early Wednesday after the sun emitted masses of charged particles that disrupted the Earth’s magnetic field — and created a dazzling display. Aurora borealis, or northern lights, are most common over locations closer to the North Pole…more

-Livescience

New ‘nearly interstellar’ comet — wrongly linked to 3I/ATLAS A never-before-seen comet that shares some minor similarities with the infamous interstellar object 3I/ATLAS is about to make its closest approach to our planet just a few days after it was first spotted speeding toward us…more

-NYT

What Can Cosmic Dust Tell Us About the Changing Arctic? Scientists have reconstructed 30,000 years of changes to sea ice in several locations across the Arctic Ocean by looking for traces of cosmic dust embedded in the seafloor, according to a study published Thursday. Scientists analyzed sediment samples from the Arctic Ocean by looking for traces of space particles,..more

-NYT

2 Spooky Flashes Lit Up the Moon. Here’s What Made Them Early November, a handful of watching telescopes captured something crashing into the moon. Then over the weekend, a second object punctured its silvery surface. The two incidents were a reminder that the moon is not so much the serene orb we clearly see in night skies a few nights a month but rather a noisy battleground constantly gaining new craters….more

-NYT

NASA Rover Makes a Shocking Discovery: Lightning on Mars It is shocking but not surprising. Lightning crackles on Mars, scientists reported on Wednesday. What they observed, however, were not jagged, high-voltage bolts like those on Earth, arcing thousands of feet from cloud to ground…more

Posted in December 2025, Sidereal Times | Tagged , | Leave a comment

From The Director

by Rex Parker, PhD director@princetonastronomy.org

November 11, 2025, Meeting on Campus.  With the close of a very successful season of public observing nights at Washington Crossing Observatory, our main venue for several months will be the evening meetings at Peyton Hall on campus the second Tuesday each month (7:30pm).  Our guest speaker Nov 11 will be Romain Teyssier, Professor of Astrophysical Sciences and Applied and Computational Mathematics at Princeton University.  Dr Teyssier studies cosmology and galaxy and star formation. He is the main author of the RAMSES code, a massively parallel open-source code used to model large scale astronomical structures using supercomputers.  This has inspired an international community of researchers to employ RAMSES for cosmology with high spatial resolution.  This presentation will provide AAAP members with insights to how cosmology is being practiced today.  The Nov 11 meeting will also be run via Zoom as usual, but it’s better to attend in person at Peyton Hall if you can.  Please see Victor’s article in this issue for more information.  I hope to see you on Nov 11!

Be Part of the Unjournal Club.  We’ve developed the tradition of the member “10 min talk”, which I like to call the Unjournal Club (a take-off from the journal clubs found in many science grad student programs).  This runs at the top of the 2nd hour of the regular meetings after the main speaker has finished.  The plan is to help break the boundaries between members and share our interests in astronomy.  Here I am asking you to volunteer to give an “unjournal” club session!  For example I gave a talk last month on the Mars Perseverance rover finding a possible biosignature fossil on Mars based on a recent paper in Nature.  But the unjournal club talks don’t need to be scholarly, journal-like topics at all, they only need to engage members with what you care about in astronomy.  If you aren’t there in person you can still do a talk via Zoom which works great with PowerPoint slides or simple text or photos.  To get on the schedule for an upcoming meeting (e.g., Nov 11), please contact me or program chair Victor Davis.

Announcement:  Electronically Assisted Astronomy (EAA) Is Now Part of the AAAP Astroimaging Group.  Members interested in EAA activities (“astrovideo”) are invited to join the AAAP Astroimaging Group.  This includes smart telescopes such as the ZWO SeeStar and Unistellar telescopes.  Meetings going forward will include discussions of equipment and software for EAA as well as astrophotography. Please contact Michael Dimario at astroimagers@princetonastronomy.org and Gene Allen at secretary@princetonastronomy.org to sign up or share ideas for the meetings.  The next session is  planned for Dec 30. 
Brilliant Star Forming Regions in the Autumn Sky.  I’ve been observing some of the deep sky objects well-positioned in the northern sky over the past few weeks of good weather.  Using narrow-band filters in astrophotography allows us to see through some of the light pollution and get images of some remarkable nebulae in the northern region around the constellation Cepheus. The image below of the NGC 7822 (H-II region) in Cepheus was taken with a 12.5-in reflector telescope using a dual H-alpha and Oxygen-3 narrow band filter with color camera, The intense red color in the image comes from hydrogen-alpha emission from interstellar clouds of ionized hydrogen gas.  The pillar-like condensed gas cloud structures in NGC 7822 are formed by stellar winds radiating from massive new stars embedded within the nebula. The radiation ionizes the gas and forms compressed, high density regions of both gas and dust to generate the pillars and darker globules, in turn contributing to more new stars being born.    

Nebula NGC 7822 in the Constellation Perseus.  The pillar like columns are high density regions being compressed by the stellar winds of newly born stars.  Image from NJ by Rex Parker using a 12.5 inch reflector telescope with dual-narrow band filter and ZWO ASI2400MC camera.

Posted in November 2025, Sidereal Times | Tagged , , | Leave a comment

From The Program Chair

by Victor Davis

The Universe in a Computer

The November, 2025 meeting of the AAAP will take place in Peyton Hall on the campus of Princeton University on Tuesday, November 11th at 7:30 PM. As usual, the meeting is open to AAAP members and the public. Participants can join the meeting in-person at Peyton Hall or log in to the Zoom session as early as 7:00 pm to chat informally before the meeting begins. 

The evening’s guest speaker, Romain Teyssier will describe his work using supercomputers to model the dynamics of the Universe, and the success and shortcomings in our current model, Lambda Cold Dark Matter in reproducing the properties and behavior that we see. 

Options for Attending the Meeting

You may choose to attend the meeting in person or participate via Zoom or YouTube as we’ve been doing for the past few years. (See How to Participate below for details). Due to security concerns, if you log in before the host has set up internet connectivity in Peyton Hall, you may need to wait in the Waiting Room for a few minutes until the host is prepared to admit you into the meeting. You’ll need to unmute yourself to make comments or ask questions. It’s polite, though not required, for you to enable your camera so other participants can see you. The meeting will be recorded and edited for posting to our club’s YouTube channel.

Join us for our “meet the speaker” dinner

Prof. Teyssier will be joining us for our traditional “meet the speaker” dinner at Winberie’s before the meeting.  Our reservation is for 5:45 pm Tuesday, November 11th. Please contact the Program Chair if you plan to attend. 

Here’s the anticipated agenda for November 11th, 2025’s monthly meeting of the AAAP:

Meeting Event~TimeParticipant Can Self-Unmute?
Pre-meeting informal chatting7:00 – 7:30Yes
Director Rex Parker’s remarks7:30 – 7:40Yes
Program Chair Victor Davis’ speaker introduction7:40 – 7:42Yes
Guest speaker:
Romain Teyssier
Professor of Astrophysical Sciences and Applied and Computational Mathematics
Princeton University
“The Universe in a Computer”
7:42 – 8:40No
Q&A Session8:40 – 8:55Yes
5-minute break8:55 – 9:00Yes
Business Meeting9:00 – 9:55Yes                               
Director Rex Parker’s remarks/Informal chatting9:55 -10:00Yes

(Times are approximate)

Getting to Peyton Hall
The parking lots across the street (Ivy Lane) from Peyton Hall are now construction sites, unavailable for parking. We’ve been advised by the administration of the astrophysics department that we should park in the new enclosed parking garage off Fitzrandolph street and walk around the stadium and athletic fields. Here’s a map of the campus and walking routes from the parking garage to Peyton Hall. The map shows the recently completed East Garage. Not shown is an access road Sweet Gum that connects from Faculty Road to an entrance at the lower left corner of the garage. Stadium Road connects from Fitzrandolph Road to another entrance at the opposite corner (and higher level) of the garage. It’s about a 10-15 minute walk from the parking garage to Peyton Hall.




Featured Speaker:
Romain Teyssier
Professor of Astrophysical Sciences and Applied and Computational Mathematics
Princeton University
teyssier@princeton.edu

The Universe in a Computer

Our current model of the Universe, known as the Lambda Cold Dark Matter (^CDM) model, is so successful at describing the distribution of galaxies in the Universe that we actually see that we can use large galaxy surveys as high-precision experiments to determine the fundamental constants of nature. Modeling the dynamics of dark matter, dark energy, and baryons requires large computer simulations to reproduce the many observed properties of galaxies. Prof. Teyssier will also discuss the limits of our current knowledge from the Big Bang to present day galaxies such as the Milky Way and the recent cracks in the ^CDM model as revealed by recent observations.

Romain Teyssier

Romain Teyssier, PhD, is a Professor of Astrophysical Sciences and Applied and Computational Mathematics at Princeton University, where he teaches astrophysics and computational sciences. He is an expert in cosmology and star and galaxy formation. He is the main author of the RAMSES code, a massively parallel Adaptive Mesh Refinement code for self-gravitating, magnetized, radiative flows. His main research activity is to perform simulations of cosmic structure using supercomputers, in order to understand the origin of astrophysical objects such as stars like our Sun and galaxies such as the Milky Way. He is also modeling the evolution of the Universe in the context of Euclid and LSST.  

Prof. Teyssier graduated from the Ecole Polytechnique in Palaiseau, France, and earned his PhD in Astrophysics from Paris Saclay University. He held a postdoctoral position at Lawrence Livermore National Laboratory in the US, then became a research scientist at the French Alternative Energies and Atomic Energy Commission. He was Professor of Computational Astrophysics at the University of Zurich before coming to Princeton in 2021. 

How to Participate (Links)

Zoom

Amateur Astronomers Association of Princeton is inviting you to a scheduled Zoom meeting.
Time: November 11, 2025 07:00 PM Eastern Time (US and Canada)


Join Zoom Meeting

https://us06web.zoom.us/j/86418065981?pwd=ljpjmRKAyyWzseZeTcOWZJBPB9tPb9.1https://youtube.com/live/hMwWFOdUekk

Click the above icons for Zoom and YouTube

A look ahead at future guest speakers:

DateFeatured SpeakerTopic
December 9
Jiaxuan Li
Graduate Student
Princeton University
jiaxuanl@princeton.edu

Sihao Cheng
Postdoc Member
Institute for Advanced Study
scheng@ias.edu

Eritas Yang
Graduate Student
Princeton University
eritas.yang@princeton.edu
Discovery of Dwarf Planet Candidate in an Extremely Wide Orbit
Dr. Cheng and colleagues discovered in publicly available data from the Dark Energy Camera a dwarf planet candidate, 2017 OF201, currently located at a distance of 90.5 au. Its orbit is extremely wide and extends to the inner Oort cloud, with a semi-major axis of 838 au and a perihelion of 44.9 au precisely determined from 19 observations over seven years. Assuming a typical albedo of 0.15, they estimate a diameter about 700 km, making it the second-largest known object in this dynamical population and a likely dwarf planet.
Thanks to Nick Mellis for suggesting these speakers.
January 13 2026Jamie Rankin
Research Scholar
Princeton University
jsrankin@princeton.edu
Dr. Rankin will talk about her work as Project Manager for the Voyagers’ last gasp; observing the interaction between the solar and interstellar media as these spacecraft (still transmitting data since their launch in 1977!) leave the Sun’s influence. She’ll also speak more broadly about exciting things about how the Sun interacts with the interstellar medium and about the Princeton-led Interstellar Mapping and Acceleration Probe (IMAP) mission launched this past September. 
Dr. Rankin’s role is described in a recent book “The Clock in the Sun” by Pierre Sokolsky.
February 10 2026John Bochanski
Associate Professor and Chair, Department of Computer Science and Physics
Rider University
jbochanski@rider.edu


Dr. Bochanski has been connected to the Legacy Survey of Space and Time Discovery Alliance since his graduate studies more than 15 years ago. Rider University is part of the global effort using the Vera C. Rubin Observatory to map the optical sky. The Rubin observatory (formerly the Large Synoptic Survey Telescope, LSST) will capture more information about our Universe than all other optical telescopes throughout history combined. The observatory released its first images this past June. Prof. Bochanski will discuss the project’s history and discoveries.
Thanks to Nick Mellis for suggesting this speaker.
March 10 2026Robert Vanderbei
Emeritus Professor in the Department of Operations Research and Financial Engineering 
Princeton University
AAAP Assistant Director
rvdb@princeton.edu
Prof.  Bob Vanderbei will talk about stellar dynamics.
April 14 2026Brian Lacki
Astronomer
Berkeley SETI Research Center
astrobrianlacki@gmail.com
September’s guest speaker Edwin Turner voiced his less-than-optimistic view of the prospect for discovering extraterrestrial life. Dr. Lacki, affiliated with Breakthrough Listen, a SETI initiative, recently submitted for publication a catalog of objects he and his team consider to be realistic and valuable observation targets. Dr Lacki will talk about the catalog, “One of Everything: The Breakthrough Listen Exotica Catalog” and opine on the prospects of finding technosignatures and extraterrestrial intelligence.


Thanks to Ira Polans for suggesting this speaker.
May 12 2026John Horgan
Science Writer
horganism3@gmail.com
Mr. Horgan will discuss his controversial 1996 book The End of Science, in which he argues that pure science, defined as “the primordial human quest to understand the universe and our place in it,” may be coming to an end. Horgan claims that science will not achieve insights into nature as profound as evolution by natural selection, the double helix, the Big Bangrelativity theory or quantum mechanics. In the future, he suggests, scientists will refine, extend and apply this pre-existing knowledge but will not achieve any more great “revolutions or revelations.” Shades of Auguste Comte, perhaps?
We expect to have copies of his book(s) for sale for the author to sign at the conclusion of his presentation.
Thanks to Rex Parker for recruiting this speaker.
June 9 2026Jacob Hamer
Assistant Curator
NJ State Museum Planetarium
Jacob.Hamer@sos.nj.gov
As usual, the June meeting will take place in the planetarium at the NJ State Museum in Trenton. There will be no streaming of this live-only sky show and PowerPoint presentation. Topic to be announced.
September 2026Michael DiMario
Chair of AAAP’s Astro-imaging SIG
K2mjd@outlook.com
Dr. DiMario will present a primer on astro-imaging.
October 2026Becka Phillipson
Assistant Professor in Physics
Villanova University
Prof. Phillipson, originally scheduled to be October 2025’s guest speaker, is an unconfirmed prospect to try again in 2026. 

As always, members’ comments and suggestions are gratefully accepted and much appreciated. Thanks to Ira Polans and Dave Skitt for setting up the online links and connecting the meeting to the world outside Peyton Hall.

victor.davis@verizon.net

program@princetonastronomy.org

(908) 581-1780 cell

Posted in November 2025, Sidereal Times | Tagged , , , | Leave a comment

Minutes of the October 14, 2025 Meeting

by Gene Allen, Secretary

Director Rex Parker opened the meeting in Peyton Hall at 1931 with 25 attending. He reported:

Power has finally been restored to the observatory.

Members who are exploring Electronically Assisted Astronomy, EAA, are now formally invited to participate in the Astroimaging subgroup chaired by Michael DiMario. They have always been welcome but it will now be more plain in the introductory verbiage for their Groups.io forum.

Program Chair Victor Davis introduced our speaker for tonight, Astroimaging Chair Michael DiMario, PhD. His talk was Smooth Moves: Why Strain Wave Mounts Are Taking Over.

Twenty minutes of questions and a break followed the talk.

Rex introduced the Unistellar Project Team, four of our student members who have taken on learning to observe and record astroimages with the donated Unistellar Evscope 2. Presenting were Members Eklavya Doegar, Rujula Kadam, Jason Mak, and Sarvesh Raghupathy. They explained the telescope in some detail, described how they organized themselves, and shared images that they captured as well as ways they hope to participate in AAAP events and outreach. At their request, the Board has agreed to formalize and support a student member subgroup.

Rex made an Unjournal Presentation entitled A rock in my hand, a discovery on Mars describing the similarities between his fossilized shell and rocks recently discovered by the Mars rover Perseverence. Both appear to contain vivianite, a hydrated iron phosphate mineral. One way that vivianite forms on Earth is on decomposing organic matter. In a very detailed paper published in Nature, J. Hurowitz concludes that the discovery warrants consideration as a bio-signature. <https://www.nature.com/articles/s41586-025-09413-0 >

Member Tom Swords described his capture of the transit of Triton and showed the images. Triton is the largest moon of Saturn and the images showed it passing in front of the planet.

Observatory Co-Chair Dave Skitt shared that the observatory will be open, weather permitting, on Halloween. Some spooky fun may be added to the evening.

Merchandise Shop Lead Facilitator Rich Sherman shared that cooler weather gear is being swapped onto the merchandise website.

The meeting was adjourned at 2158.

As of October 12, we have 214 active members. So far in CY2025, renewals number 98 and expirations number 46, giving us a 68% retention rate. We have added 39 new members.

Submitted by Secretary Gene Allen
October 21, 2025

Posted in November 2025, Sidereal Times | Tagged , , | Leave a comment

Translating Faust: Science, Fate, and Free Will

by John Church

As a chemistry major planning to go to graduate school, I took four years of German.  In my final year we read Goethe’s masterpiece “Faust,” based on the legend of a Doctor Faust who sold his soul to the Devil in exchange for worldly pleasures. 

Along the way we read a story by Nobel laureate Hermann Hesse (1877-1962) called “An Evening with Doctor Faust.”  I decided to tune up my rusty German by translating it.  Astronomers will note that this story refers to the accurate prediction of solar eclipses far into the future. It then continues by exploring the idea that we should also be able to predict ordinary events by simply applying the law of cause and effect.  Like eclipses, it would seem that the future of humankind is already fixed in stone and cannot be changed.

Einstein was a determinist when it came to the behavior of atoms.  He opposed quantum theory and once said to his friend the eminent Niels Bohr, “God does not play dice.” Whereupon Bohr famously retorted, “Don’t tell God what to do.”

Hesse was not a fan of mid-1930’s culture.  He became a Swiss citizen in 1923 and steered clear of politics.

An Evening with Doctor Faust

by Hermann Hesse, 1935
Translated by John Church, 2025

Doctor Johann Faust was spending a quiet evening in his dining room together with his friend Doctor Eisenbart. The remains of their repast had been taken away, but an excellent Rhine wine was still fragrant in the heavy gilded goblets upon the table.  Two musicians, a lutist and a flautist, had already departed.

          “I’m now going to carry out my planned experiment,” said Doctor Faust, while taking another deep draught of wine. He was no longer a young man.  This was two or three years before his horrible death.

          “My assistant has fashioned a marvelous device with which one can see and hear many things, both near and far away, not only in the present but in the past and even in the future.  This evening we’re going to explore the future.  As you know, we’ve already enjoyed tales of the past, with heroes, beautiful women, and so on.  But now we can hear things that haven’t actually happened yet, provided that the receiving apparatus has been properly adjusted.”

          Doctor Eisenbart wondered if his good friend had perhaps been hoodwinked by his assistant.

          “I doubt it,” replied Faust. “Anyone who has been properly trained can apply the well-known laws of cause and effect to explore the future.  As with the past, the future cannot be changed, although this can be difficult to see directly. You are aware that astronomers can predict the exact circumstances of a solar eclipse far ahead of time. Correspondingly, if we had the right tools, we should be able to see and hear human things that are yet to come.  My assistant Mephistopheles has made a sort of divining rod for the ear, in which we can discern the sounds that will be heard right here in this very room, hundreds of years from now. We’ve already tried it.  Sometimes we hear nothing, because we’ve found an empty spot in the future.  Occasionally though, we hear a poem in which my own deeds are described.  But enough! Let’s begin.”

          Faust called in his helper, dressed in his usual gray, who set down his small machine with its amplifier and warned the onlookers to remain silent.  Then he turned the device on and it began to hum softly.  Nothing happened for a long time.  Then it suddenly emitted a devilish howl, as if a dragon were being relentlessly pursued through the room.  Doctor Eisenbart turned white as the screams faded off in the distance.

          Silence then followed.  Then there was a man’s voice, apparently coming from far away, in an impressive sermon-like tone.  The listeners could understand portions of it and took down notes, for example:

“— and it proceeds irresistibly, similar to America’s shining example of economic progress, towards its own victorious conclusion and realization — while on the other hand the quality of workers’ lives has reached unprecedented heights — and we can without presumption state that the childhood dreams of an earlier age of paradise through modern production techniques more than — ”

Again there was silence.  The came a new deep and earnest voice that said: “Ladies and gentlemen, please listen to a new poem, a creation of the great Nicholas Unterschwang, who has laid bare the most secret places in the heart of our times: the sense and nonsense of our daily existence.”

                              He holds the chimney in his hand,
With fins on both of his cheeks;
While consulting the barometer,
He climbs a ladder without rungs.

                             He ascends the long ladder
With clouds in his coat lining.
At length he becomes afraid,
And is overcome with vacillation.

Faust was able to write down most of this poem.  Eisenbart also took copious notes.

          The sleepy voice of an older woman now became audible.  She said: “Boring program!  As if they invented the radio just for this! Ah, here’s a little music.”

Then came a wild and exceedingly rhythmic music, now blaring, now languishing, a completely unknown, strange, indecent, evil music emitted from howling, squeaking, and cackling wind instruments, vibrating with gongs, interrupted with singing and the screaming of lyrics in an unknown language.  

At intervals there was this message in rhymed verse: “Everyone will admire your hair if you use Goo-Goo regularly!”

Once again came those screaming, howling tones, those dragon-like wails full of fear and anger, louder and louder.

As the laughing assistant brought his machine to a standstill, the two learned gentlemen blinked strangely at one another with embarrassment and shame, as if they had been witnessing an indecent performance. They looked at their notes and pointed at one another.

“What do you make of it?”  asked Faust.

Doctor Eisenbart took a drink from his goblet.  He looked at the floor and remained quiet and reflective for a long time.  Finally he said, “It’s horrible!  There can be no doubt that from this fragment we have just heard, that mankind is insane!  These are our sons, the great-grandchildren of our great-grandchildren, who were saying such dubious, sad, confusing things, emitting such terribly arousing screams, singing such incomprehensibly idiotic songs.  Our descendants, friend Faust, will end in madness.”

          “I’m not completely convinced of that,” said Faust.  “Your prediction is not at all improbable, but it is perhaps more pessimistic than necessary.  If here, in this one little place on Earth, we hear such wild, despairing, indecent and doubtful noises, that doesn’t necessarily mean that all of mankind will have gone crazy.  It’s possible that in a few hundred years a madhouse will stand here, and all that’s happened is that we’ve stumbled upon a sample of it.  It’s also possible that we’ve heard a company of drunkards giving way to their fancies.  Think about a carnival and all the noise that that makes!  Very similar, in my opinion.   But what really puzzles me is all those other sounds, those screams, that couldn’t possibly have come from human voices or musical instruments.  They are absolutely devilish! Only demons could do this.”

          He turned to Mephistopheles. “Do you know anything about this? Can you tell us something about these sounds?”

          “We have,” said his assistant, “actually heard demonic sounds. The Earth has already been half taken over by the Devil.  Eventually he will own it all and it will be a province of Hell itself.  Gentlemen, you’ve expressed great negativity about what you’ve heard.  It’s remarkable and fitting that music and poetry will still exist in Hell.  Belial is in charge of this department.  I think he’s doing a great job!”

Posted in November 2025, Sidereal Times | Tagged , , , , | Leave a comment

Are Velocity calculations from Spectral Measurements creating the Hubble Tension and Dark Energy theories?

by William H. Davis jr.

Astronomers collect and use spectral shift data to estimate the velocity of objects or photon emitters (E) beyond Earth. This spectral data is one of the most important and often the only tool used to evaluate the universe beyond the maximum distance for precise triangulation. Spectral patterns indicate the frequency (fe) of the photons radiated from the emitter (E). It is an invariant independent variable but subject to the effects of Special Relativity (SR). The patterns are based on the local spectral patterns observed as a set of known frequency emission lines known for a particular element. Hydrogen is typically abundant in stars so the Balmer series, a group of emissions from hydrogen is used. The electrons changing energy levels emit particular frequencies of light at each level jump. For objects without hydrogen the patterns for other elements can be used.

The following will be covered:

  1. Develop a simple energy balance to estimate velocity using Plank’s Equation, E=hf.
  2. The relativistic Doppler equation solution will be shown and compared to the linear model solutions.
  3. Correcting the local velocity to the observers frame.
  4. Examine the present use of Doppler and compare to the simple energy balance and SR solutions.
  5. Discuss the use of z (change of wave length) claiming to be ≅ v/c.

Simple energy balance method calculating velocity from the frequency ratio

Frequency is linearly and directly proportional to energy, as per Plank’s Equation, E=hf. Frequency shift f | is directly proportional to the observed velocity of E. The observer can determine the ± shift by observation. The shift observed is unaffected regardless of the motions of the observer or the emitter. There is no choice. There are two separate equations for shift one for red and one for blue.  The sign of v, a vector will be – for redshift, –energy and + for blueshift +energy. The velocity and  fe are independent variables. The observed frequency fo is a dependent variable based on the velocity and fe
fo=(fe ±Δf or Δv).

  • Redshift (R) is ( fo < fe ) : fe fe =1 is the starting point at zero velocity.
    The red shift range of fo is ( fe → o) resulting in fo being a % of fe

 Δ f fe = fo fe – 1 ≅-v/c Test: Inverse action v↑ fo ↓ with the range of 1.

  • Blueshift (B) is ( fo < fe ) : fo/ fo =1 is the starting point at zero velocity.

Δf fo = 1- fe ⁄ fo  ≅ +v/c:  Test: Direct action v↑ fo ↑ range of fo  is 1. Total energy available is fe with no external energy input. When, fe → 0, then fomax  = 2 fe .

Note: the switch or change of reference in the denominators and the sign change between the two equations. The red and blue frequency ratios above are fractions <1, bound between 1 and zero or 1 and 2 and have a range of 1. These ratios are equated to ±v/c with a constant of 1 because the range of each side of the equations is 1 or100% of the range. Both equations are linear and ≅ v/c. V cannot equal or exceed c.

The shift determination eliminates the need to choose between the observer or emitter moving to determine ≈velocity. Shift determines the equation or model.

Correcting for SR eliminates the need to choose shift or condition making all points of references equal.

Special Relativity Clock Correction

Frequency is cycles per second. The principles of special relativity apply. Velocity creates a clock differences between fo and fe that results in some error for the velocity calculations if SR is not considered. When motion is involved, fo and fe have different clock rates. When the clock differences are corrected by the Lorentz transformation of the red and blue equations which results in two identical equations. The SR equation equates the vectors –v/c for redshift and +v/c for blueshift as the natural state or direction. This equation is in many references but the application is not mentioned.

 Red and Blue models corrected or transformed as:       
         

Plots of the linear and transformed models (blue top, red bottom)

Note: The solution is for ve , the local or apparent velocity. Conversion to v0 produces the actual velocity compared to the observer. The clock of the emitter in motion is always slower than the observer’s clock. The actual velocity is always less than the local or apparent velocity.

Actual velocity v0 versus apparent velocity ve

The present use of Doppler to determine velocity from the frequency ratio

Option (1) Text book model based is on the observer moving and the emitter stationary with redshift
(-v21): We know the earth is moving. When a model states it is based on a certain state or reference that is what it normally means! For some reason this model is not used?

This option is identical to the redshift equation (R) above and meets all the parameters for redshift. It is not presently used?

Option (2): Text book redshift model: Observer stationary and Emitter in motion = +v?21, is the present model being used when we know the Earth is a moving platform > 106 miles/hr and do not know the status of E? 

This is not consistent with redshift but is with blueshift λ⤍(1→.5)range. If v=0→ fo= 1 or fo. The red direction was established at in Equation (R) and the transformed model. This equation is +v? The + velocity vector represents + blue direction not red. No matter what the state of the observer is, the observed shift cannot change. The different solutions are not compatible with SR (No preferred reference). The observer will see redshift as fo < fe in all cases the same as a SR solution.

Solving for v/c, fo and fe switch places. The denominator is fo compared to fe as per Textbook option (1).  This equation is based on fo which is a different reference base than (1).
It is a blueshift model ( fo > fe ) , which is a bound relationship with v/c based on fo rather than fe .

 Solve for v/c:


Option 2 blueshift frequency:

Using the equation for the opposite shift inverts frequency to a wave calculation (z). This produces a hyperbolic curvature which exceeds c. This is discussed in the next section about z.

The use of z The definition of z is the fractional wave length change Δλ /λ(e or o) caused by motion of an emitter.  The textbook choice of: + redshift z is based on the stationary observer

z=(λ0e)/λe→λoe-1≅v/c ?

Since, λo→∞ this equation is not equal to ≅v/c and cannot be directly solved for v. If used for redshift it is hyperbolic curve to ∞. Distance and or velocity cannot be determined without a proper conversion. The z being used is not ≅ v/c. It only appears to be ≈ numerically accurate with the opposite sign at lower velocities but is mathematically incorrect. There is no solution using λ ratios to determine velocity in redshift because λo→∞ is in the numerator of the equation. The present calculation of z is a multiple of λo and not a fraction. The numerator is greater than the denominator.

Comparison of the unbound Doppler and z with the bound redshift solution

Summary:
We have failed to integrate Special Relativity into astrophysics modeling which creates an issue with choice and accuracy. We have made incorrect choices using Doppler, which creates a hyperbolic solution for v. This results in models that violate the speed limit c. The assumed velocities of emitters have not been corrected to the observer’s frame. Some are replacing v with z in calculations. All of the errors are cumulative in the same direction, thus contribute to an illusion of a rapid expansion. The result is the Dark Energy theory (force with a string) to reconcile the observations. We need to get all of our determinations of velocity and distance as accurate as possible because we are projecting our models beyond the data. Keep in mind we can only do estimates ±. The error of measurement, distance and going back in time has a huge impact on the accuracy of our calculations.

Next month I will discuss issues with using standard candles to estimate distance.





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The case for multi-messenger astronomy

by S. Prasad Ganti

In the beginning, there was only visible light astronomy which meant viewing distant objects in space using our naked eye or with the help of an optical telescope. Gradually things changed and we started doing astronomy by capturing radiation from other parts of the electromagnetic spectrum, i.e. radio waves, infra red waves, x-rays. ultra violet waves and gamma rays. Astronomy has become richer as a result. We are able to map our universe in much greater detail since. 

Understandably earlier observations were done using naked eyes only. Our ancestors were able to view the dark skies as there was no light pollution. The only instruments they had were their eyes. With the invention of the telescope about four hundred years ago, our vision got extended. Telescopes became powerful. But still the observations were restricted to using our eyes. With the invention of photography, plates started replacing the eyes. Plates could be analyzed much after the images were captured. And by many more people than just the observer who captured the images. This was the state of art until about a hundred years ago.    

With that state of art, Edwin Hubble found out about other galaxies like Andromeda, as distinct from our Milky way and came up with an approximate distance. He analyzed the photographic plates captured using the 100 inch telescope at Mount Wilson. We have come a long way since then, by branching out to other parts of the electromagnetic spectrum. Other than visible light, radio waves from distant objects can penetrate the Earth’s atmosphere and be received on the ground. This was discovered accidentally by a radio engineer Karl Jansky at AT&T. Radio communication was in vogue at that time and Jansky’s job was to trace other sources of radio “noise” coming in the way of intended communication. Although initially ignored, decades later, Jansky’s discovery led to Radio astronomy. With radio antennas, instead of optical lenses, forming the basis of radio telescopes.    

A combination of radio and  optical telescopes provided us with a more vivid  picture of our universe. Still there were patches of sky which looked totally dark. As if the voids meant absence of any significant objects. Sounding rockets started launches into space beginning  in the 1950s. One such rocket contained sensors to detect X-rays. It found the first X-ray source titled CYG X-1 coming from the Cygnus constellation.   

In physics, any body which is hotter than absolute zero, emits radiation. Including our Earth and we ourselves. It is called black body radiation. Hotter bodies emit higher energy waves like Gamma rays, X-rays, visible light etc. Being much cooler, we emit infrared rays. Night vision glasses are built on capturing these infrared rays to see in the dark. Since we have all kinds of objects with different temperatures in our universe, we have different types of radiation to “see”.  Our sun emits most of its  radiation in the form of visible light. And our eyes evolved to be sensitive to visible light. Hence our bias towards visible light. 

In addition to different frequencies (and types) of radiation emitted by different objects in space, the frequency of the radiation can change enroute. As the source objects are moving away from us, the radiation gets red shifted (something like the siren of a moving ambulance changing its pitch as it approaches us or moves away from us), which means it gets stretched and longer wavelengths result. A moving object emitting  X-rays can get red shifted to visible light as it is perceived by us.     

There is a lot of interstellar dust between us and some of the source objects. The dust is composed of small grains made of carbon (soot) or silicon (sand), about the same size as visible light. It can absorb, reflect or scatter the visible light. It either blocks us from seeing the object totally or we can see it in a different frequency. 

All these phenomena result in us getting different wavelengths of radiation. Our atmosphere blocks most of those frequencies except for visible light and radio waves. The only way to observe those blocked wavelengths is by placing those telescopes in space. Chandra X-ray telescope and James Webb infrared telescopes are two such instruments which cannot be replaced by any earth based instrument.       

There are different kinds of messengers coming towards us in various forms. By combining the images from all these different types of telescopes, we get a complete mosaic of our universe. No more dark patches.

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Snippets

compiled by Arlene & David Kaplan

-NYT

George F. Smoot, Who Showed How the Cosmos Began, Is Dead at 80 George F. Smoot, an American physicist and Nobel laureate who helped elucidate the story of cosmic creation, providing evidence of what he called the primordial seeds that grew into galaxies and galaxy clusters, died on Sept. 18 at his home in Paris….more

-NYT
-NYT

Take a Look at Rare Photos of Red Lightning in New Zealand About 150 miles southwest of Christchurch, New Zealand, far away from the light pollution in urban centers, three photographers planned to capture the Milky Way galaxy over the clay cliffs outside Ōmārama on the night of Oct. 11….more

-NYT

An Army of Robot Telescopes in Texas Makes the Stars Feel Closer Than Ever During the day, this patch of land in sparsely populated Central Texas is not remarkable. Eleven buildings, nearly identical, look like bland, oversize backyard sheds. Several large R.V.s are parked nearby. Not long ago, cows grazed here….more

-CBS

Astronomers discover most powerful “odd radio circle” twins ever detected Deep in outer space, astronomers have discovered another “odd radio circle” — the latest in a short list of mysterious rings that surround distant galaxies — and researchers say this one is particularly peculiar. “Odd radio circles,” or ORCs, are enormous and unexplained phenomena that can only be detected using radio telescopes…..more

-CBS

SpaceX launches 11th test flight of giant Super Heavy-Starship rocket SpaceX launched its Super Heavy-Starship rocket on Monday for the 11th time, marking another successful test flight that built upon previous launches. Elon Musk, SpaceX founder and CEO, briefly made an appearance on the company’s livestream ahead of the launch, saying it was the first time that he was going to be outside to watch the rocket. ….more

-CBS

Interstellar comet passing by Mars seen in rare images A rare interstellar comet — only the third ever confirmed to enter our solar system — was photographed last week, closely approaching Mars, the European Space Agency said Tuesday. The images taken on Friday by two Mars orbiters show a bright, fuzzy white dot of the comet, also known as 3I/ATLAS,…more

-CBS

Mysterious “rogue planet” spotted gobbling 6 billion tons of gas and dust a second A mysterious “rogue planet” has been observed gobbling 6 billion tons of gas and dust a second — an unprecedented rate that blurs the line between planets and stars, astronomers said Thursday. Unlike Earth and other planets in our solar system, which orbit the sun, rogue planets float freely through the universe untethered to a star…..more

-CBS

Unprecedented views of largest star-forming region in our galaxy captured by Webb telescope NASA’s powerful James Webb Space telescope has revealed a colorful spread of stars and cosmic dust in the Milky Way’s most active star-forming region. The telescope was studying Sagittarius B2, a massive molecular cloud, NASA said in a news release…more

-CBS

Space weather satellites blast off to collect information on solar storms A cluster of space weather satellites blasted off Wednesday morning to cast fresh eyes on solar storms that can produce stunning auroras but also scramble communications and threaten astronauts in flight. The three satellites soared from Kennedy Space Center shortly after sunrise on the same SpaceX rocket….more

Space.com

You won’t see intertsellar comet 3l/ATLAS zoom closest to the sun on Oct. 30 – but these spacecraft will The interstellar comet 3I/ATLAS is just a day away from perihelion, which is its closest point to the sun and the time around which it is expected to be most active. Although 3I/ATLAS is currently hidden from view from Earth, flying behind the sun, spacecraft elsewhere in the solar system still have the comet in their sights…more

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From The Director

by Rex Parker, PhD
director@princetonastronomy.org

October 14, 2025 Meeting on Campus.  I look forward to seeing you for our monthly meeting Oct 14 at Peyton Hall of Astrophysics.  Our guest speaker will be Becka Phillipson, Asst Prof in Physics at Villanova University. Her expertise includes black hole and neutron star studies, active galactic nuclei, and time domain astronomy (that is, observable changes in astronomical position, brightness, and structure during human-centric time periods). Dr. Phillipson uses machine learning and artificial intelligence to pursue these areas, making Oct 14 a great opportunity for us to get closer to the cutting edge of astrophysics, and better understand where and how AI is being used. We will also stream the meeting via Zoom as usual, but it’s better to attend in person at Peyton Hall if you can.  Please see Victor’s article in this issue for more information.

“Unjournal Club” at the meeting, Oct 14.  If you have been wondering what the new generation of “smart telescopes” is all about, you can have an insider’s look at Peyton Hall after the break on Oct 14. The Unjournal Club (aka, the 10min member talk) will be given by the Unistellar Project Team, the student members who have been exploring astronomy with the club’s Unistellar EVScope2.  The students have put together a short presentation describing how they used and shared this powerful yet portable advanced telescope over the summer.  The scope will be on display for us to marvel at.  You will want to be present at the meeting for this!

Here’s some more background on the Unistellar scope.The club acquired through generous donation last spring a Unistellar EVScope2.  You may be familiar with the SeeStar smart scopes from ZWO, which several members now own and enjoy.  The Unistellar is similar in concept and function but unique in design.  It is mirror-based (114mm Newtonian reflector), so this larger aperture gathers more photons than other refractor lens-based smart scopes on the market.  The EVScope2 features a high sensitivity Sony CMOS sensor (STARVIS technology).  This particular model also features a Nikon electronic eyepiece, along with integrated mobile app to view emerging images on a smart phone or tablet.  Up to 10 persons can simultaneously observe via local Wifi without an external internet connection.  The scope quickly and automatically aligns itself and tracks without polar alignment.  With its carbon tripod it is highly portable, lightweight, and simple to set up, making the deep sky accessible despite light pollution.

Proposal for a Youth/Student Group in AAAP.  We have an opportunity to support the development of a youth group within AAAP.  Some of the student members in AAAP who led the Unistellar observing project this summer (described above) have proposed an ongoing youth sub-group within AAAP.  They would be students in high school or above, be dues-paying members (usually with their parents), and would be engaged in learning and sharing astronomy and astro technology with other students and adults.  They would help with AAAP outreach programs and develop contacts within schools and libraries in the area. The Board endorses this proposal and will establish some guidelines and appoint an advisor(s), under which the group can operate through the auspices of AAAP.  This will be discussed at the Oct 14 meeting, when you will get a chance to meet a few of our energetic young amateur astronomers.  I hope you will be present at Peyton for this discussion. 

Announcement:  EAA Is Now Part of the AAAP Astroimaging Group.  The AAAP-exclusive astrophotography interest group is being expanded to include EAA activities (EAA is electronically assisted astronomy), or what I like to call astrovideo.  Further, the Group.io website dedicated to AAAP astroimagers will now support equipment and software discussions of EAA as well as astrophotography and EAA. Please contact Michael Dimario at astroimagers@princetonastronomy.org and Gene Allen at secretary@princetonastronomy.org to sign up or share ideas.

New Findings in the Search for Biosignatures of Extraterrestrial Life.  In AAAP as elsewhere in astronomy, exoplanet research and the possibility for biosignatures of extraterrestrial life are hot topics.  The idea of water-rich “Hycean” exoplanets and the suggestion of biosignature gases in exoplanet K218b are being debated (discussed in my article in May 2025 Sidereal Times). A new paper suggests that the hypothesis of deep water oceans on these worlds is likely wrong (Sept 18, Astrophysical Journal Letters;  link to the free article:  https://iopscience.iop.org/article/10.3847/2041-8213/adff73).  The current paper challenges the ideas of how large planets with water-rich atmospheres can form, with implications for interpreting recent exoplanet spectral data from JWST. 

Closer to home, NASA released a head-turning report from a new analysis of photographic images from a Mars rock collected by Perseverance rover in 2024. The specimen from an ancient dry riverbed in Jezero Crater could be a type of fossil revealing chemical evidence of ancient microbial life.  The study was published in the Sept 10 issue of Nature, with lead author from the SUNY Dept of Geosciences (link: Redox-driven mineral and organic associations in Jezero Crater, Mars | Nature). The specimen, nicknamed “Cheyava Falls,” shows contrasting spots consistent with ancient microbial redox activity (oxidation-reduction reactions), based on mineral features found in known fossils on earth.  Of course, other non-biological explanations exist and NASA stressed that these are not confirmed fossils.  Most importantly, the findings support the need to fund and execute a Mars rock sample return mission as originally planned and now being reevaluated by NASA.  

A Possible Fossil Biosignature on Mars? NASA’s Perseverance Mars rover found and imaged this rock nicknamed Cheyava Falls. The irregular mm-sized spots in the red matrix in the image are being interpreted as possible redox biochemical reaction products from microbial life, perhaps billions of years ago. Credit:  NASA

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From The Program Chair

by Victor Davis, Program Chair

He Who Lives in Harmony with Himself Lives in Harmony with the Universe
Marcus Aurelius

Smooth Moves: Why Strain Wave Mounts are Taking Over
The October, 2025 meeting of the AAAP will take place in Peyton Hall on the campus of Princeton University on Tuesday, October 14th at 7:30 PM. As usual, the meeting is open to AAAP members and the public. Participants can join the meeting in-person at Peyton Hall or log in to the Zoom session as early as 7:00 pm to chat informally before the meeting begins.

The evening’s guest speaker, Michael DiMario, chairs this club’s Astroimaging-EAA Group. Due to a misunderstanding regarding meeting dates, Dr. DiMario will step in to take over for Becka Phillipson, who will be rescheduled for a future meeting

Also, Eklavya Doegar and her fellow members of the Unistellar Student Group will show images they acquired with the newly donated “smart” telescope and discuss their experiences using it.

Options for Attending the Meeting
You may choose to attend the meeting in person or participate via Zoom or YouTube as we’ve been doing for the past few years. (See How to Participate below for details). Due to security concerns, if you log in before the host has set up internet connectivity in Peyton Hall, you may need to wait in the Waiting Room for a few minutes until the host is prepared to admit you into the meeting. You’ll need to unmute yourself to make comments or ask questions. It’s polite, though not required, for you to enable your camera so other participants can see you. The meeting will be recorded and edited for posting to our club’s YouTube channel.

No “meet the speaker dinner”
Dr. DiMario has expressed his preference to forego the traditional pre-meeting dinner at Winberie’s.

Here’s the anticipated agenda for October 14, 2025’s monthly meeting of the AAAP:

(Times are approximate)

Getting to Peyton Hall
The parking lots across the street (Ivy Lane) from Peyton Hall are now construction sites, unavailable for parking. We’ve been advised by the administration of the astrophysics department that we should park in the new enclosed parking garage off Fitzrandolph street and walk around the stadium and athletic fields. Here’s a map of the campus and walking routes from the parking garage to Peyton Hall. The map shows the recently completed East Garage. Not shown is an access road Sweet Gum that connects from Faculty Road to an entrance at the lower left corner of the garage. Stadium Road connects from Fitzrandolph Road to another entrance at the opposite corner (and higher level) of the garage. It’s about a 10-15 minute walk from the parking garage to Peyton Hall.

Chair of Astroimaging – EAA Group
Amateur Astronomers Association of Princeton

Smooth Moves: Why Strain Wave Mounts are Taking Over

Smooth Moves: Why Strain Wave Mounts are Taking Over
Telescope mounts have come a long way — from bulky worm gears to sleek, high‑precision systems. Strain wave mounts (also called harmonic drives) are transforming how we track the night sky. By using elastic motion instead of traditional gear teeth, these mounts offer extreme precision, near‑zero backlash, and compact designs. This talk will explain strain wave technology, how it works, compare it to traditional worm‑gear mounts, and explore why it’s becoming a game‑changer for amateur astronomy. No engineering background required — just curiosity and a love of the stars.

Michael DiMario, PhD
Michael DiMario has recently retired from Lockheed Martin serving various executive roles and has held executive engineering positions at General Electric Medical and Lucent Technologies/Bell Laboratories. Michael has six patents, a published book on systems engineering, several published book chapters, more than fifty peer reviewed papers. He has been interviewed and quoted in Wired Magazine, GPS World, Sifted, and the Financial Times. In regard to his astronomical pursuits, he chairs the Amateur Astronomers Association of Princeton Astroimaging Group, spends many a night astroimaging, and does considerable astronomical history research. He co-shares the earliest precovery of Pluto on Edward Barnard 1909 photographic glass plates located at Yerkes Observatory.

How to Participate (Links)
Zoom & YouTube Live
Amateur Astronomers Association of Princeton is inviting you to a scheduled Zoom meeting.
Time: October 14, 2025 07:00 PM Eastern Time (US and Canada)

Join Zoom Meeting
Topic: October 2025 AAAP Meeting-Michael DiMario, PhD, Astroimaging Chair, AAAP
Time: October 14, 2025 07:00 PM Eastern Time (US and Canada)


https://us06web.zoom.us/j/83089664878?pwd=AaaS7f2MG3CwruhRo2vtDitxWFN73A.1 ….https://youtube.com/live/SF9U5-vwuwQ
Click the above icons for Zoom and YouTube

Breakthrough Starshot
When last month’s guest speaker, Edwin Turner, visited Peyton Hall several years ago, his topic was the Breakthrough Starshot Initiative. This now-abandoned project was funded by billionaire Yuri Milner. The idea is to launch tiny probes weighing a gram or so attached to reflective sails into orbit and then use high-powered lasers to accelerate them to 20% of the speed of light and direct them to the nearest stars. The history of this project and its quiet demise are described in a recent article in Scientific American magazine. Apparently both billionaires and politicians can be capricious and arbitrary. You can read the article at https://www.scientificamerican.com/article/the-quiet-demise-of-breakthrough-starshot-a-billionaires-interstellar/

A look ahead at future guest speakers:

Date Featured SpeakerTopic
Nov. 11,
2025
Romain Teyssier
Professor of Astrophysical Sciences and Applied and Computational Mathematics
Princeton University
teyssier@princeton.edu
Prof. Teyssier’s main research activity is to perform simulations of cosmic structure using supercomputers in order to understand the origins of stars and galaxies.
Dec. 9, 2025
Sihao Cheng
Postdoc Member
scheng@ias.edu

Jiaxuan Li
Graduate Student
jiaxuanl@princeton.edu

Eritas Yang
Graduate Student
eritas.yang@princeton.edu
Discovery of Dwarf Planet Candidate in an Extremely Wide Orbit
 
Dr. Cheng and colleagues discovered in publicly available data from the Dark Energy Camera a dwarf planet candidate, 2017 OF201, currently located at a distance of 90.5 au. Its orbit is extremely wide and extends to the inner Oort cloud, with a semi-major axis of 838 au and a perihelion of 44.9 au precisely determined from 19 observations over seven years. Assuming a typical albedo of 0.15, they estimate a diameter about 700 km, making it the second-largest known object in this dynamical population and a likely dwarf planet.
 
Thanks to Nick Mellis for suggesting these speakers.
Jan. 12, 2026Not Yet Scheduled
Feb. 12, 2026
John Bochanski
Associate Professor and Chair,
Department of Computer Science and Physics
Rider University
Dr. Bochanski has been connected to the Legacy Survey of Space and Time Discovery Alliance since his graduate studies more than 15 years ago. Rider University is part of the global effort using the Vera C. Rubin Observatory to map the optical sky. The Rubin observatory (formerly the Large Synoptic Survey Telescope, LSST) will capture more information about our Universe than all other optical telescopes throughout history combined. The observatory released its first images this past June. Prof. Bochanski will discuss the project’s history and discoveries.
 
Thanks to Nick Mellis for suggesting this speaker.
Mar. 10, 2026Robert Vanderbei
Emeritus Professor in the Department of Operations Research and Financial Engineering
Princeton University
 
AAAP Assistant Director
rvdb@princeton.edu
Prof.  Bob Vanderbei will talk about stellar dynamics.
Apr. 14, 2026Not Yet Scheduled
May 12, 2026
John Horgan
Science Writer
horganism3@gmail.com
Mr. Horgan will discuss his controversial 1996 book The End of Science, in which he argues that pure science, defined as “the primordial human quest to understand the universe and our place in it,” may be coming to an end. Horgan claims that science will not achieve insights into nature as profound as evolution by natural selection, the double helix, the Big Bangrelativity theory or quantum mechanics. In the future, he suggests, scientists will refine, extend and apply this pre-existing knowledge but will not achieve any more great “revolutions or revelations.” Shades of Auguste Comte, perhaps?
 
We expect to have copies of his book(s) for sale for the author to sign at the conclusion of his presentation.
 
Thanks to Rex Parker for engaging this speaker.
Jun 9, 2026
Jacob Hamer
Assistant Curator
NJ State Museum Planetarium
Jacob.Hamer@sos.nj.gov
As usual, the June meeting will take place in the planetarium at the NJ State Museum in Trenton. There will be no streaming of this live-only sky show and PowerPoint presentation. Topic to be announced.

As always, members’ comments and suggestions are gratefully accepted and much appreciated. Thanks to Ira Polans and Dave Skitt for setting up the online links and connecting the meeting to the world outside Peyton Hall.

victor.davis@verizon.net
program@princetonastronomers.org
(908) 581-1780 cell

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