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Speaker: Katherine Laliotis

Speaker: Katherine Laliotis, Cosmologist, KIPAC

Illuminating the Universe Through Weak Gravitational Lensing

Free and open to the public. Free Parking in nearby lots.

NASA’s Roman Space Telescope project has successfully integrated essential components, enhancing its capability to study astronomical phenomena like dark matter and exoplanets. The project remains on track for completion in 2026, with a launch planned by May 2027. Credit: NASA’s Goddard Space Flight Center

Question: How can we learn about matter that we can’t see? Answer: By looking at how the invisible matter’s gravity affects the matter we can seeThis is gravitational lensing, an exciting and active field of cosmology research through which we hope to answer fundamental questions about the universe like the nature of dark matter and dark energy.  In this talk, I’ll focus on weak gravitational lensing: how it works, what It can tell us about the universe, and the prospects for up-and-coming weak lensing surveys with the Rubin Observatory and Roman Space Telescope.

Katherine Laliotis is a senior graduate student from Ohio State University, visiting KIPAC long-term. She specializes in observational cosmology, using observations of the universe to try and answer fundamental questions like “What is the universe made of?” and “How did the universe evolve?” Katherine’s research focuses on understanding and accounting for sources of systematic error for upcoming weak gravitational lensing surveys with the Nancy Grace Roman Space Telescope and the Vera Rubin Observatory. She also spends time thinking about how to maximize synergies between the two observatories, bringing together two different datasets to construct a uniquely broad joint survey. Katherine is passionate about connecting science to the public through outreach, education, and writing. She is a freelance science writer, covering topics at the intersection of science and society in magazines like Scientific American and Undark.

We propose a mission concept for a space observatory with a large-aperture (50-meter) unsegmented primary mirror suitable for a variety of astronomical applications. The mirror would be created in space via a novel approach based on fluidic shaping in microgravity, which has already been successfully demonstrated in a laboratory neutral buoyancy environment, in parabolic microgravity flights, and aboard the International Space Station (ISS). Theoretically scale-invariant, this technique has produced optical components with superb, sub-nanometer (RMS) surface quality. 

Volunteers Needed for CSM’s Annual Family Science Day – September 27

Since the College of San Mateo has always supported the Society for events, we in turn show our support by assisting with their events. The Society contributes to CSM’s Annual Family Science Day, Saturday, September 27 by holding a variety of activities and assisting with the reception. This is a unique opportunity for solar events, as the activities take place during the day.

Event Schedule and Volunteer Shifts:
• Part 1: 1pm–5pm (volunteers needed from noon) – Daytime volunteers will assist with solar activities, such as “Make a Planisphere” and building a Solar System Model, as well as staffing our membership table. Drinks and snacks are provided for volunteers during this shift.
• Part 2: 7pm–11pm (evening volunteers needed for reception setup) – Evening volunteers will help set up for the reception, which will follow the keynote presentation by Dr. Pascal Lee.
This year’s keynote speaker is Dr. Pascal Lee, a planetary scientist at the SETI Institute and co-founder/chairman of the Mars Institute, and a regular presenter to the Society. He will deliver his talk, “From the Moon to Mars,” which was previously presented to the Society on March 7. If you missed March’s meeting, this is an excellent opportunity to catch it.

After the reception, CSM will open its rooftop observatory for stargazing and live music.

Why Volunteer?
• Your support helps make Family Science Day a memorable experience for all attendees!
• Gain hands-on experience, expand your network, and contribute to a vibrant community event.

If you are interested in volunteering or would like more information, please contact Marion Weiler (mgwe@pacbell.net) if interested in volunteering or for more information.

New Faces on the SMCAS Board

There are some new faces on the SMCAS Board and we are very excited to introduce them. One has jumped into the Society with both feet by not only becoming a new member but a board member, too. Please welcome Kimberly Alger to the Society as one of our newest Board Members at Large. Kimberly has been attending Star Parties for the past few months and become a board member because it sounded like a fun way to get more involved in the club. Her parents introduced her to astronomy by taking her to meteor showers and the Space Center in Houston. There she saw retired rockets from the Apollo era and looked through a solar telescope for the first time when Venus transited across the sun.  Currently she’s a middle school teacher who loves talking math and science with her students.


Another new face to the board but not to Star Parties is Stephen Kwong. Though he’s been attending Star Parties since 2022, Steve didn’t become an official member until this year and is also jumping with both feet into the Society by being a Board Member at Large. Stephen became a board member because he’s passionate about stargazing and wants to help spread the joy of stargazing to our communities.

“It’s really rewarding to me when I witness the joys of others viewing astronomical objects for the first time through a telescope!”

As with others, his interest in astronomy was sparked by his kids. When his youngest son was in kindergarten, they saw Saturn and Jupiter through a telescope during the Great Conjunction of 2020. From then on, he was hooked.


Another new face to the board but very familiar to the Society is Chanan Greenberg. Most know Chanan and depending on how long you’ve been a member, you might remember him serving on the board as vice president between 2007 and 2013. Chanan became a board member, both then and now, to be more active in the club’s public outreach and support club activities. You might also recall that during that time, Chanan moved from San Mateo to the South Bay but is still continues to be a very dedicated and active member. It was Chanan’s grandfather that introduced him to astronomy with a pair of binoculars and a 60mm refractor. His first viewing of the moon hooked him. However, it wasn’t until many years later that his wife encouraged him to pursue astronomy as a hobby, just before the birth of his daughter.


Chanan also shared that before he became vice president, they had tradition of going to Denny’s after Star Parties and hanging out and talking more about astronomy topics. Many members helped and inspired him to then pursue astrophotography. To see more of his images go to www.greenhawkobservatory.com.


Lastly, the Board has appointed a Youth Board Member since a young member was interested in serving but wasn’t old enough to serve. We’re fortunate that Kaelyn Chutczer agreed to the appointment and is another new face at the board meetings. Kaelyn wanted to be a board member in hopes of getting more students interested in astronomy. She knows there are a lot of other teenagers who would appreciate the opportunity to learn more about science. Her father, Marc Chutczer, a five-year member, introduced her to the Society. She’s been going to Star Parties for as long as she can remember! She started attending the monthly meetings about a year ago. Kaelyn shared that ever since her father got a telescope, she’s been able to understand the science in astronomy much more than when she was a child. In addition, at her school, Kaelyn is in two choirs and a political speech and debate club.

“I’m very excited to get to work with the board this year!”

Speaker: Katherine Laliotis

Speaker: Katherine Laliotis, Cosmologist, KIPAC

Illuminating the Universe Through Weak Gravitational Lensing

Free and open to the public. Free Parking in nearby lots.

NASA’s Roman Space Telescope project has successfully integrated essential components, enhancing its capability to study astronomical phenomena like dark matter and exoplanets. The project remains on track for completion in 2026, with a launch planned by May 2027. Credit: NASA’s Goddard Space Flight Center

Question: How can we learn about matter that we can’t see? Answer: By looking at how the invisible matter’s gravity affects the matter we can seeThis is gravitational lensing, an exciting and active field of cosmology research through which we hope to answer fundamental questions about the universe like the nature of dark matter and dark energy.  In this talk, I’ll focus on weak gravitational lensing: how it works, what It can tell us about the universe, and the prospects for up-and-coming weak lensing surveys with the Rubin Observatory and Roman Space Telescope.

Katherine Laliotis is a senior graduate student from Ohio State University, visiting KIPAC long-term. She specializes in observational cosmology, using observations of the universe to try and answer fundamental questions like “What is the universe made of?” and “How did the universe evolve?” Katherine’s research focuses on understanding and accounting for sources of systematic error for upcoming weak gravitational lensing surveys with the Nancy Grace Roman Space Telescope and the Vera Rubin Observatory. She also spends time thinking about how to maximize synergies between the two observatories, bringing together two different datasets to construct a uniquely broad joint survey. Katherine is passionate about connecting science to the public through outreach, education, and writing. She is a freelance science writer, covering topics at the intersection of science and society in magazines like Scientific American and Undark.

We propose a mission concept for a space observatory with a large-aperture (50-meter) unsegmented primary mirror suitable for a variety of astronomical applications. The mirror would be created in space via a novel approach based on fluidic shaping in microgravity, which has already been successfully demonstrated in a laboratory neutral buoyancy environment, in parabolic microgravity flights, and aboard the International Space Station (ISS). Theoretically scale-invariant, this technique has produced optical components with superb, sub-nanometer (RMS) surface quality. 

Pumpkin Spice and Cosmic Delights

Greetings to the Society, 

Back to Pizza and the Planetarium

As summer winds down and pumpkin-flavored everything creeps back onto shelves, our society is gearing up for a lively fall season. Our general meetings return on September 5 — always a chance to reconnect, swap stories about what we’ve seen in the night sky, share some pizza, and catch up on upcoming events. Following the social portion, we’ll welcome Dr. Bart De Pontieu, Solar Physicist, who will present Unraveling the Mysteries of the Sun’s Atmosphere. It promises to be a fascinating dive into our star’s secrets

Sharing the Sky

September and October also bring opportunities for us to share the night sky with the wider community. On September 27, we’ll take part in Family Science Day at the College of San Mateo. Then, on October 25, we’ll team up with Stanford’s KIPAC STEM Community Day. These events are wonderful chances to spark wonder in kids and families — and maybe even be mistaken for a wizard while pointing out Saturn’s rings.

Celestial Highlights

And the skies are giving us plenty to talk about:

  • All SeptemberInterstellar Comet 3I/ATLAS is passing through, a rare visitor from beyond our solar system. Catch it with a telescope before it disappears behind the Sun in late October.
  • September 21Saturn at opposition, shining at its brightest.
  • September 23Neptune at opposition, faint but rewarding in a telescope.
  • Early OctoberComet C/2025 K1 ATLAS reaches peak brightness and may be visible with binoculars — worth scanning the skies!
  • October 22–23 – The Orionid meteor shower peaks, with excellent viewing under dark skies.
  • October 29 – Elusive Mercury shines in the evening sky at greatest elongation.

Spacefaring News

Meanwhile, space exploration is keeping pace. NASA’s ESCAPADE mission to Mars launches on September 29, hitching a ride on Blue Origin’s New Glenn rocket — their first interplanetary venture. NASA’s IMAP probe will soon begin studying space weather, and the Pandora mission aims to peer into the atmospheres of distant exoplanets.

Closing Thoughts

So whether you join us at a meeting, at a community event, or under the stars, I hope this season brings you awe, inspiration, and maybe a meteor or two for good luck.

Clear skies,

Michael Cooke

President, San Mateo County Astronomical Society

My Favorite Astronomer: Galileo

Galileo di Vincenzo Bonaiuti de’ Galilei is one of the most famous astronomers in the world. He’s often considered to be the father of modern science since he made major contributions to the fields of physics, mathematics and philosophy. He is the central figure of the Scientific Revolution of the seventeenth century.


As many, the story I learned about Galileo was when how he challenged the Catholic Church and their teachings about the solar system. They believed the Earth was the center of the Solar System and he was crucified for going against the teachings of the church and became a martyr for science. This belief was further cemented when I heard the first lines of a song called “Galileo” by the Indigo Girls:

“Galileo’s head was on the block,
the crime was lookin’ up the truth.”

It wasn’t until many years later that I learned that he wasn’t killed by the church and lived to be 77 years old. However, when he died, he was under house arrest.

Galileo was born February 15, 1564 in Pisa, Italy. His father, Vincenzo, was a court musician and authored some music theories while his mother, Giulia Ammannati, was a descendant of cloth merchants. When it was time him to go a university, he enrolled in the University of Pisa in 1580 to earn a medical degree. He never earned it and actually studied mathematics. From 1589 to 1610, Galileo was chair of mathematics at the universities of Pisa and then Padua. In the latter years, he began investigating hydrostatics and the strength of materials and continued his studies on motion that leads to the discovery of the parabolic path of projectiles.

All his projects came to halt in 1609 when he took a new spyglass and improved the magnification on the lens and pointed it at the sky. He eventually was able to increase the magnification by 30 times. From here, most know the history of his discoveries, such as the large moons Jupiter, often referred to as Galileo’s moons, Io, Europa, Ganymede, Callisto. He also was the first to see the Rings of Saturn! (Although with the strength of his magnification, he couldn’t actually see the rings, which is why he described them “handle” or “ears”.) He was also the first to see that the Moon wasn’t a smooth sphere; that there were hills and craters on the surface. He even saw sunspots and rushed to put his observations in a pamphlet in 1610 called, “Sidereus Nuncius,” which is Latin and translates to “Starry Messenger.” Between being able to show prominent leaders his observations and having mathematicians verify them, such as, Johannes Kepler, who wrote a letter in support of his pamphlet, the pamphlet catapulted Galileo onto the world stage. With its success, Galileo is appointed as the “Chief Mathematician of the University of Pisa and Philosopher and Mathematician to the Grand Duke of Tuscany” for life.

Empowered by his successes, in 1613, Galileo wrote “Letters on Sunspots,” where he expresses support for heliocentrism, the sun being in the center of the solar system. In 1616, Galileo wrote his theory about the tides in which he argues that it is proof that the Earth moves. A month later, on the orders of the Pope Paul V, Cardinal Bellarmine goes to Galileo’s residence to warn him not to defend the Copernican theory. It would about a decade later when Galileo get the attention of the Church.


In 1623, Maffeo Barberini, Galileo’s supporter and friend, was elected Pope Urban VIII. The following year the Pope assured him that he could write about the Copernican theory as long as he treated it as a mathematical hypothesis. As a result, Galileo began to work on a “Dialogue Concerning the Two Chief World Systems.” The “two systems” were the Ptolemaic and Copernican, both of which supported the heliocentrism. It would take Galileo ten years to finish it. He worked with the Inquisition and censors for getting it printed. In 1632, its distribution is prohibited by Pope Urban VIII and a special commission is appointed to examine the book who refers it to the Inquisition. They meet with the Pope and it’s decided to summon Galileo to Rome.


Galileo receives the summons and requests the trial be moved to Florence. His request is denied. The Florentine Inquisitor informs Rome that he had visited Galileo, who was ill, in bed and that three physicians had signed a statement that he was too ill to undertake the journey to Rome. At another meeting again presided over by Pope Urban VIII, himself, the Inquisition rejects Galileo’s request as a ruse and sends him notice that if he does not come to Rome voluntarily, he will be arrested and brought to Rome in chains.


Galileo arrived on February 13, 1633. He is formally interrogated by the Inquisition. He is detained in the building of the Inquisition but in a comfortable apartment. A plea bargain is made where Galileo will plead guilty to lesser charges and will receive a lenient sentence. On April 30, Galileo confesses that he may have made the Copernican case in the “Dialogue” too strong and offers to refute it in his next book. Pope Urban VIII decides that Galileo will be imprisoned for an indefinite period. The sentence is signed by seven of the ten cardinal-inquisitors.
In a formal ceremony at the church of Santa Maria Sopra Minerva, Galileo denies his errors.


He is allowed to be under house arrest at the residence of the Tuscan ambassador and then at the residence of the archbishop of Siena. There he begins putting together his Discourse on Two New Sciences. Eventually he is allowed to return to his villa in Arcetri, near Florence, where he remained under house arrest for the remainder of his life.


It’s now known for the Arcetri Astrophysical Observatory.

My Favorite Astronomer – Edwin Hubble

Edwin Hubble (1889-1953)

Here in 2025, most of us are familiar with the stunning wide-field images from the Hubble Space Telescope, showing hundreds of galaxies scattered across the cosmos. We now understand that the universe contains billions of galaxies, each made up of billions of stars, and that it all began with the Big Bang roughly 13 billion years ago. What’s truly remarkable is that, despite astronomy being practiced for thousands of years, these discoveries were made only within the last century. It’s fascinating to think that in 1915, when Einstein introduced his General Theory of Relativity — a theory still used to describe the structure of the universe — these facts about the cosmos were completely unknown.

One man, Edwin Hubble (1889-1953), kick-started the revolution that led to these discoveries. Hubble was born in Missouri and studied Mathematics and Astronomy at the University of Chicago. He switched fields to get a law degree at Oxford University, before moving back to astronomy, first at Yerkes Observatory in Wisconsin, and later at the Mount Wilson Observatory in California.

Before Hubble’s work, many astronomers believed that the Milky Way galaxy encompassed the entire universe. Nebulae — fuzzy, cloud-like objects in the night sky — were believed to be a part of the Milky Way. What is today called the Andromeda Galaxy (M31) was called the Andromeda Nebula. In the 1920s, using the 100-inch Hooker Telescope at Mount Wilson Observatory in Southern California, Hubble observed Cepheid variable stars in the Andromeda Nebula. By measuring their brightness and applying period-luminosity relationship first developed by Henrietta Leavitt, he calculated their distance and found they were far too distant to be part of the Milky Way. This proved that Andromeda was a separate giant stellar system like the Milky Way, leading to the realization that the universe contains countless galaxies beyond our own. Hubble’s classification of galaxies based on their shapes — elliptical, spiral, irregular — was continued with modifications in later decades.

Hubble’s other groundbreaking contribution came in 1929 when based on meticulous measurements of distances and velocities of numerous galaxies, he concluded that other galaxies are moving away from us and the farther away they are, the faster they recede. The ratio of the speed of the galaxies to their distance was found to be constant (Hubble’s constant, currently estimated at 70 kilometers per second per megaparsec — a megaparsec is equal to 1 million parsecs or approximately 3.26 million light-years). This relationship provided the first observational evidence for an expanding universe and laid the foundation for the Big Bang theory.

Through his discoveries, Hubble transformed cosmology from a speculative field into an observational science. His work not only changed our view of the cosmos but also our place within it — demonstrating that Earth and the Milky Way are just small parts of an immense, ever-expanding universe. Edwin Hubble’s legacy continues with the Hubble Space Telescope, which was launched by NASA in 1990. The HST has further expanded our understanding of the universe and over three decades has delivered dozens of iconic images of the universe.

SMCAS Annual Star-B-Que Party: July 19, 6p.m.

The SMCAS Board invites you and your family to our annual Star-B-Que, Saturday, July 19 from 6 p.m. to 11 p.m. at our usual meeting spot, Crestview Park, 1000 Crestview Dr, San Carlos. This is a family friendly event, bring the kids. Feel free to arrive and leave at your convenience. 

Our party will be a potluck; Board members will provide main dishes and this year it will be catered! We are relying on everyone else to bring side dishes or munchies, such as vegetables, chips, salads or desserts and nonalcoholic beverages you would like to share. Please try and label food for anyone that might have food allergies. Utensils will be provided but we encourage you to bring your own non-disposable serving utensils for your dish, to be green. 

Please RSVP with the number of people in your party so the Board can be sure to purchase the appropriate amount of food.

The potluck will close with the final tally of votes, by current membership, for the 2025-26 SMCAS Board Members. Look for voting details via email from Marion Weiler.

Don’t forget, there is a Star Party following so bring your telescope or just stay to look through other members’ scope. Sunset is around 8:30 p.m.

Email the Board at SMCASBD@groups.io with any questions or concerns.

We look forward to seeing your there!

The SMCAS Society is Growing!

The Board is pleasantly surprised to see how busy the Star Parties have been and to see our membership grow. We are very excited to announce that we’re one member away to having 70 people! In other words, we have 69 members. It’s the most members the Society has ever had.

It was very apparent to me at our May 31 Star Party. I tried to arrive earlier than usual (which means before sunset) and was surprised to see people were already lined up at Kevin Simpson’s and Ed Ching’s telescopes to view the moon. Even though the sun hadn’t set yet, it was plainly visible. I was torn between setting up and taking pictures. Since Ed Ching was there with his other Astroscan, I opted for taking pictures and then setting up. After I set up the Astroscan Ed lent to me and the telescope given to me by Frank Graham, Ed and I took turns on focusing on different but close objects. Then later on, when I saw an extremely long line for one of Kevin’s telescopes, I had to go take pictures. 

Ed Ching with his Astroscan.

After taking pictures, I was amazed to see that the entire sidewalk from end-to-end was completely full of telescopes. It hit me that I had never seen so many telescopes, so out of curiosity, I decided to count them. I was shocked and impressed to tell the other Board members that I counted 16 telescopes! Granted, a couple might have been astrophotography set ups, but they still count, right?

I counted 30 adults and children. How many do you count?

When I shared the news with former Society President, Mike Ryan, he asked if anyone had counted the people. It made my mind swirl. Besides it being the most number of telescopes, it was the also the most people I had seen. How could we count people when they are wandering? And in the dark? Perhaps we just need to remember to take pictures and remember to get all of the telescopes. In one of the pics, I counted 30 adults and children around Kevin! 

Again, we’re so excited to see the Society to continue to grow and ask that everyone keep on encouraging membership. With the membership fees, we’re able to get our remarkable presenters for our monthly meetings along with our pizza parties. 

The Board is always open to suggestions and welcome any feedback about what you would like to see the Society do. It’s definitely a group effort! 

Thank you for your continued support.

Mohsen Janatpour’s Proposal

September 3, 2016

Ladies and Gentlemen,

I have known Ken for more than thirty-three years. I have benefited from his knowledge, wisdom, and kindness. He was instrumental in our choices of speakers for Family Science Day, year after year. His solar observations engaged the public and students, enriching our program. The bridge to the Science Building will feel empty without his solar telescope. Over the years, whenever I gave a talk about solar astronomy, I relied on his pictures, and he was always in the audience, attentive to what I had to say. I genuinely miss him.

So, I propose that we create and conduct a solar astronomy workshop in his name every year on Family Science Day. In fact, in the schedule and the program, I propose calling the workshop: “Ken Lum’s Solar Astronomy Workshop.”

I appreciate your input on this. More importantly, on the structure of this workshop.

Thanks, 
Mohsen Janatpour