From The Program Chair

by Victor Davis, Program Chair

The Universe in a Computer
The December, 2025 meeting of the AAAP will take place in Peyton Hall on the campus of Princeton University on Tuesday, December 9th 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, Jiaxuan Li, is a fourth-year graduate student pursuing a PhD in astrophysics at Princeton University. Recently, along with Sihao Cheng at the Institute for Advanced Study and fellow Princeton graduate student Eritas Yang, Li and his team discovered a trans-Neptunian object in an unusually wide orbit that challenges the Planet 9 hypothesis.

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
Mr. Li 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, December 9th. 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:

(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.


PhD Candidate in Astrophysics
Princeton University

A Newly-discovered Distant World: The Dwarf Planet Candidate 2017 OF201
Astronomers Jiaxuan Li and Eritas Yang (graduate students at Princeton University’s Department of Astrophysics) and Sihao Chang (Institute for Advanced Study) identified a remarkable new world in the far outer Solar System: a dwarf-planet candidate named 2017 OF201, currently more than 90 times farther from the Sun than Earth. By combining observations spanning the past two decades, the team showed that it follows an enormous, elongated orbit that reaches deep into the inner Oort Cloud. With an estimated diameter of roughly 700 km, it ranks among the largest known objects on such distant orbits and is very likely a dwarf planet. Its extreme trajectory hints at a far larger, still-hidden population of similar bodies that may collectively contain about 1% of Earth’s mass. Intriguingly, its orbit does not share the clustering seen in some other remote objects—a pattern often cited as evidence for a possible “Planet Nine.” Continued searches for distant Solar System bodies will help unveil the true structure and diversity of this unexplored frontier.

Jiaxuan Li
Jiaxuan Li grew up in Dingxi, Gansu Province, a small town in northwestern China. An amateur astronomer since elementary school, Li participated in several international competitions, including the Chinese National Astronomy Olympiad. He earned his undergraduate degree in Astrophysics at Peking University, then came to Princeton to pursue his PhD. He’s interested in a variety of topics in astronomy and astrophysics, mainly on galaxy formation and evolution, low surface brightness astrophysics, sky surveys, machine learning, and instrumentation. His current research examines the formation and evolution of dwarf galaxies through both careful observation and numerical simulations.

How to Participate (Links)
Zoom & YouTube Live
Amateur Astronomers Association of Princeton is inviting you to a scheduled Zoom meeting.
Time: December 9, 2025 07:00 PM Eastern Time (US and Canada)

Join Zoom Meeting
Topic: December 9,2025 AAAP Meeting-Prof. Cheng, Jiaxuan Li, Eritas Yang, Dwarf Planet Candidate
Time: December 9, 2025 07:00 PM Eastern Time (US and Canada)
Meeting ID: 824 8572 5475
Passcode: 136481
Join instructions


https://us06web.zoom.us/j/82485725475?pwd=ikn08sd7Gz4rTLA7LFPIYCQVf2YMib.1 ….https://youtube.com/live/2jYvuRj0oMY
Click the above icons for Zoom and YouTube

AAAP’s library of monthly meetings is available on the club’s YouTube channel. November’s edited meeting featuring a presentation “The Universe in a Computer” by Princeton University astrophysicist Dr. Romain Teyssier can be viewed at https://youtu.be/lqs7znI1nEg

A look ahead at future guest speakers:

Date Featured SpeakerTopic
Jan. 13,
202
6
Jamie 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.
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, 2026Astronomer
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, 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.
Sep. 8, 2026Michael DiMario
Chair of AAAP’s Astro-imaging SIG
K2mjd@outlook.com
Dr. DiMario will present a primer on astro-imaging.
Oct. 13, 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@princetonastronomers.org
(908) 581-1780 cell

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

Observatory Report

by Dave and Jennifer Skitt, Observatory Co-Chairs

Solar Observing on November 29, 2025

Upon hearing of the Grand Re-Opening of the Nature Center in Washington Crossing State Park on Thanksgiving weekend, I wondered what AAAP could do to entice park visitors to view nature in ways above and beyond those offered by the Nature Center.  You see, the Nature Center lies just down the road from our observatory, and their daytime activities were all slated to be indoors.  We could open the Observatory roof and do Solar Observing, of course!

Word went out to our Keyholders to solicit volunteers to staff the observatory while the Nature Center did their thing.  Once we had sufficient coverage for our telescopes, I invited AAAP members and Keyholders-in-Training (KIT’s) to join us.  Then, all we had to do, was hope for clear skies.  Nature provided that for us on Saturday November 29.  And, what an incredibly nice sunny day we had!  

I arrived around 0930 and made a brief stop by the renovated Nature Center to introduce myself and our event to the new naturalist, Joe Moore.  We both promised to direct visitors to each others activities.

In total, we had six telescope set-ups in the field along with the observatory scopes.  Our scopes were white light solar only and the field scopes had both white light and hydrogen-alpha capabilities.  Later in the day, we pointed a few scopes toward at Venus and the Moon, for a change of scenery.

Five KIT’s appeared and I went through the set up and safety protocol for solar observing with our telescopes.  The KIT’s were a big help in kicking things off in the morning.  Two of them earned their keys to the observatory as they had completed their training.

While I was too busy to get a final head count (or photos), I estimate we had 35-40 visitors of all ages.  In the crowd were a few Park volunteer employees and the executive director of the Washington Crossing Park Association.  Also present were a local mom and dad and their daughter, who is currently studying Engineering at UC Berkley and working on a NASA planetary mission set to launch in 2030.  They said they have visited our observatory off and on since their daughter was a little girl.  Wow!

It was a busy day for all of us; there was never a dull moment.  My wife, Jennifer, helped us close out the day, directing people to telescopes, answering questions and handing out brochures.  Jennifer’s arrival provided Bill Murray and I a few moments to hang the Gene Ramsey memorial plague.  While completing the task, we spoke well of Gene, remembering his contributions to the club and our personal lives. 

As the Sun cast longer shadows and 1600 drew near, Jennifer and I took a walk up to the Nature Center.  Jennifer spoke of bugs and flying squirrels (ask me about that sometime) and I talked of future club interaction with Joe and the Nature Center staff.  Everyone agreed resumption of Nature Center operations was a good thing.  Needless to say, Jennifer and I were deeply satisfied with the days activities.  

Many, many thanks to all who came out to make it happen and observe the Sun.

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

From The Astrophotography Group

by Michael DiMario, Astrophotography Chair

Bubble Nebula NGC7635 taken by Michael DiMario
Telescope:       Celestron C9.25 Edge HD at FL 1645mm f7.0
Mount:             Losmandy GM811G
Exposures:       229 subframes @ 300 sec each over 5 nights for 19 hours of integration; ASI2600MC-P; Optolong L-Ultimate filter
Processing software: Pixinsight
Location, Bortle, and Date: Doylestown, PA; Bortle 6; August 22-30, 2025
Description and Story: The Bubble Nebula NGC7635 is a rich ionized hydrogen region (HII) in the constellation Cassiopeia. The “bubble” shape was created from the stellar wind created by the intensely hot central star (SAO 20575) and is within a giant, glowing molecular cloud. The Bubble itself is about 10 light-years in diameter.

Great Carina Nebula NGC3372 taken by Michael DiMario
Telescope:       Takahashi FSQ85EDX FL 455mm f5.3
Mount:             Losmandy GM811G
Exposures:       27 subs @ 30 sec each; ASI2600MC-P; Antilla Triband filter
Processing software: Pixinsight
Location, Bortle, and Date: Big Cypress, FL; Bortle 2; March 31, 2024
Description and Story: Great Carina Nebula is located in the southern sky constellation Carina located in the Carina–Sagittarius Arm of the Milky Way galaxy. The nebula is approximately 8,500 light-years from Earth. The nebula is one of the largest diffuse nebulae in Earth’s sky whereby it is four times as large as and brighter than the Orion Nebula.

This image taken in 2024, was reprocessed in Pixinsight. This evening’s session began with a 6-foot alligator very near my observing spot. Fortunately, it moved quickly back to the water. As darkness enveloped, the Everglades continued to be challenging with passing clouds, very large mosquitoes seemingly the size and whirring of humming birds, and python hunters with their large floodlights. The area of sky where the Great Carina Nebula was located was clear and was not my observing plan that night. However, NGC3372 was an opportunity to be taken that night as it was visible given its very low altitude. It was challenging as it was approximately 1-5 deg above the southern horizon, over far off trees and a field of many astronomers’ red lights. Imaging at this low of an altitude is equivalent to looking through approximately 11-26 atmospheres as opposed to 1 atmosphere at zenith.

Fireworks Galaxy NGC6946 taken by Michael DiMario
Telescope:       Celestron C9.25 Edge HD at FL 2350mm f10.0
Mount:             Losmandy GM811G
Exposures:       86 subframes @ 200 sec each over 2 nights with Antilla Triband filter; 90 subframes @ 200 sec each broadband over 3 nights for 9.8 hours of integration; ASI2600MC-P
Processing software: Pixinsight
Location, Bortle, and Date: Doylestown, PA; Bortle 6; October 3-18, 2025
Description and Story: The Fireworks Galaxy is located between the constellations of Cepheus and Cygnus. Its distance from Earth is about 25.2 million light-years. It is heavily obscured by interstellar matter due to its location close to the galactic plane of the Milky Way. NGC 6946 has also been classified as a double-barred spiral galaxy, with the inner, smaller bar presumably responsible for funneling gas into its center. Due to its large number of star formation, it has been classified as an active starburst galaxy. However, this galaxy derives its name not from its star nursery capability but from the ten supernovae observed since 1917. The number of observed supernovae in this galaxy is ten times the number observed in our Milky Way galaxy, even though the Milky Way has twice as many stars.

Fireworks Galaxy was a challenging project given its small field of view (FOV) and thus imaging at native FL of 2350mm. The tracking of the Losmandy GM811G mount was outstanding. A bright Moon in early October forced the use of the Antilla Triband filter with remaining subframes taken in broadband (no filters) when Moon was absent.

3i/Atlas the Interstellar Comet taken by Daniel Mints
Telescope:       Meade LX200 EMC reduced to 1650mm
Mount:            ZWO AM5N
Exposures:     ZWO533MCPro – 35 subframes @ 60 sec each with Antilla Triband filter
Processing software: Pixinsight/Lightroom
Location, Bortle, and Date: Hillsborough, NJ; Bortle 6; Early Morning, November 18, 2025
Description and Story: Interstellar Comet 2I/Borisov—sometimes called “Atlas of the stars” for the vast journey it represents—made history in 2019 as only the second known visitor from beyond our solar system. Discovered by amateur astronomer Gennadiy Borisov, the comet entered the Sun’s neighborhood at an extraordinary speed and on a sharply hyperbolic path, clear signs that it was not bound to our star. Unlike typical comets shaped by billions of years of orbiting the Sun, 2I/Borisov came from the deep cold between the stars, probably carrying pristine material left over from the formation of a distant, unknown planetary system.

Messier 16 (Eagle Nebula) and Comet C/2025 R2 (SWAN) conjunction taken by Daniel Mints
Telescope:       Samyang 135mm
Mount:            ZWO AM3
Exposures:      ZWO183MMPro – 240 subframes @ 30 sec each (LRGB mono captured)
Processing software: Pixinsight/Lightroom
Location, Bortle, and Date: Rockland, TX; Bortle 1; October 17, 2025
Description and Story: The conjunction of Messier 16 (the Eagle Nebula) and Comet C/2025 R2 (SWAN) creates a stunning celestial scene where two very different cosmic objects briefly share the same patch of sky. The Eagle Nebula, located about 7,000 light-years away in the constellation Serpens, is a vast star-forming region famous for the towering Pillars of Creation. These immense columns of gas and dust are nurseries where new stars ignite, shaping the nebula with intense radiation and sculpting its iconic form. The visual pairing of the fast-moving comet with the distant, majestic Eagle Nebula tells a story of two cosmic journeys: one fleeting and ephemeral, the other spanning millions of years.

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

The Perfect Machine

by S. Prasad Ganti

“The Perfect Machine” is the name of a book written by Ronald Florence. It covers the design, construction and the installation of the 200 inch Hale telescope at the Mount Palomar observatory, close to San Diego in southern California. Recently I had the opportunity to visit Los Angeles and San Diego to be with family and friends. I spent a few hours at the Palomar observatory. Having read the book a few years back, I was thrilled to see the perfect machine. 

The telescope was conceived by George Hale who was known for his research in solar astronomy, and importantly for constructing the 60 inch Yerkes telescope near Chicago and the 100 inch telescope at Mount Wilson near Los Angeles. He also cofounded Caltech. In 1928 Hale secured Rockefeller foundation sponsorship for the 200 inch telescope. It took a couple of decades before the construction could complete, just after the second world war. By that time Hale had passed away. The New York Times suggested that the new telescope be named in his honor. 

The main part of a reflecting  telescope is its mirror. Palomar’s mirror is 200 inches in diameter and was cast in Corning, New York. It is a very painstaking glass making process taking months to get it right. Heating sand in a rotating furnace followed by a very slow cooling process. Contemporary mirrors are not cast as a single piece. Instead they are composed of multiple segments, with each segment controlled by an actuator/motor. This is a scalable design but requires a lot of computing power to precisely move the actuators in tandem so that all the pieces work as one big mirror. Back in those days, such technology did not exist. Hence the need to cast it as one big piece. The cast was sent by a special freight train from New York to Caltech in California. Caltech has a polishing lab where the mirror was polished to very fine tolerances. The polishing work took longer since the work was interrupted by the second world war as Caltech turned to wartime research. 

The next critical piece in the telescope is the mount. The telescope moves within the mount to point to a specific area in the sky and once locked to an object in the sky, to keep the telescope moving so that the object remains locked even as the earth below is rotating on its axis. It is like chasing a star as it is moving from east to west in the nightly skies. Today’s technology is different from what existed in those days. The current mounts are called alt-azimuth mounts. Such mounts  move in two directions – one up and down vertically, other horizontally firstly to locate a given object and then to move with the object as it moves across the sky. This motion requires a lot of computing power and is the standard mount today on modern telescopes. 

Back in the 1940s, Hale telescope was designed using the equatorial mount. A superstructure called the yoke (a Y or U shaped structure) is permanently aligned parallel to  the axis of earth’s rotation. This fixes one axis of movement. The only manipulation required is to move the mount across the sky as the star moves through the night. This movement is called the right ascension. The telescope itself is mounted between the two arms of the yoke and is free to move in the vertical plane, called the declination. For a long time, I had a tough time imagining what the mount would look like. Pictures did not help me that much. When I saw the real mount, I could realize how it worked. 

The picture given below is courtesy Palomar Observatory/Caltech. The thick tube in the middle of the picture is one arm of the yoke. The angle of this arm with respect to the floor aligns with the earth’s axis of rotation. The black truss structure extending to the top of the observatory is the telescope hung between the two arms of the yoke (the second arm of the yoke is behind the first arm, not visible from this angle). The telescope itself is free to swing up and down between the two arms of the yoke and is controlled by a motor. At the bottom of the truss is the mirror facing the sky. Towards the upper end of the truss are the secondary mirror and the electronics required to capture the images.   

The yoke itself is connected to a horse shoe bearing which is on the right of the yoke. One motor moves the yoke on this bearing to position the telescope to a particular object in the sky. Once set, a second motor moves the yoke to track the object in the sky as the night progresses to dawn. This rotation of the yoke is on the axis which is parallel to earth’s rotation. These three motors are the key controllers of the telescope.        

The following youtube video explains the mount in 2.5 mins while the second video explains the history of Mount Palomar design and construction. Both the videos show the detailed design of the equatorial mount and how it turns. 

The whole structure of the mount and the telescope are housed in an outer cylindrical structure with a dome at the top. The dome has a slit on the top. This slit is open during the night for observations. The whole dome rotates on bearings at the top of the cylindrical structure. This rotation would position the open slit to the part of the sky which needs to be observed. Given below is the picture of the dome which I shot using my iPad pro. The dome is painted white to reflect the sunlight. The temperature inside the observatory needs to be constant so that the telescope remains in alignment all the time. The dark band at the bottom of the dome, but higher than the steps and the front door, indicates the track on which the dome rotates.    

The whole mount, truss and the dome were designed by Russell Porter, who is a polymath considered as one of the founding fathers of amateur astronomy. Porter also contributed to the design of buildings at the Palomar observatory and Caltech campus. He made about 1000 drawings of the telescope and its related instruments and buildings. 

The telescope works in the visible, infrared and ultraviolet ranges. It is a pretty wide range given the technology with which the mirror was built. Fred Zwicky used this telescope to detect supernovae. Maarten Schmidt discovered the first Quasar in 1963. These objects are very bright in the whole universe. But Schmidt’s spectroscopy revealed that the light is so red shifted which indicates that they are billions of light years away, formed during the infant stages of our universe. Now it is postulated that such objects represent supermassive black holes and the accretion disk of gases around them is the bright light we are seeing. Thousands of Quasars have been discovered since. 

The telescope has been fitted with adaptive optics on its secondary mirror  to modernize it. Adaptive optics is used to compensate for the distortions in the atmosphere which make the stars twinkle. The  twinkle looks good in the sky, but makes the observations unsteady. Adaptive optics divides a mirror into smaller segments with each segment controlled separately by an actuator/motor. A reference laser is shot into the skies. The reflected picture of the laser is used to find out how much distortion the atmosphere is causing. Accordingly each actuator is moved differently  to change the shape of the mirror to provide a sharp picture. Adaptive optics is a standard design for all modern telescopes.   

It is a fascinating story of how the telescope was conceived, designed and constructed and the discoveries it made and the efforts to modernize it. My tributes to George Hale and Russell Porter, two of the most important people who built the Mount Palomar observatory. 

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

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

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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

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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!”

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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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