Science & Technology

BNL LECTURE: ZHANGBU XU

By Daniel Dunaief

Gregory Breit and John Wheeler were right in the 1930s and Werner Heisenberg and Hans Heinrich Euler in 1936 and John Toll in the 1950s were also right.

Breit, who was born in Russia and came to the United States in 1915, and Wheeler, who was the first American involved in the theoretical development of the atomic bomb, wrote a paper that offered theoretical ideas about how to produce mass from energy.

Breit and Wheeler suggested that colliding light particles could create pairs of electrons and their antimatter opposites, known as positrons. This idea was an extension of one of Albert Einstein’s most famous equations, E=mc2, converting pure energy into matter in its simplest form.

Zhangbu Xu in front of the time-of-flight detector, which is important for identifying the electrons and positrons the STAR Collaboration measured. Photo from BNL

Working at the Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Laboratory, a team of scientists in the STAR Collaboration has provided experimental proof that the ideas of some of these earlier physicists were correct.

“To create the conditions which the theory predicted, even that process is quite exhausting, but actually quite exciting,” said Zhangbu Xu, a senior scientist at BNL in the physics department.

The researchers published their results recently in Physics Review Letters, which provides a connection to Breit and Wheeler, who published their original work in a predecessor periodical called Physics Review.

While Breit and Wheeler wrote that the probability of two gamma rays colliding was “hopeless,” they suggested that accelerated heavy ions could be an alternative, which is exactly what the researchers at RHIC did.

The STAR team, for Solenoidal Tracker at RHIC, also proved another theory proposed decades ago by physicists Heisenberg, who also described the Heisenberg Uncertainty Principle, and Hans Heinrich Euler in 1936 and John Toll, who would later become the second president at Stony Brook University, in the 1950s.

These physicists predicted that a powerful magnetic field could polarize a vacuum of empty space. This polarized vacuum should deflect the paths of photons depending on photon polarization.

Researchers had never seen this polarization-dependent deflection, called birefringence, in a vacuum on Earth until this set of experiments.

Creating mass from energy

Xu and others started with a gold ion. Without its electrons, the 79 protons in the gold ion have a positive charge, which, when projected at high speeds, triggers a magnetic field that spirals around the particle as it travels.

Once the ion reaches a high enough speed, the strength of the magnetic field equals the strength of the perpendicular electric field. This creates a photon that hovers around the ion.

The speeds necessary for this experiment is even closer to the speed of light, at 99.995%, than ivory soap is to being pure, at 99.44%.

When the ions move past each other without colliding, the photon fields interact. The researchers studied the angular distribution patterns of each electron and its partner positron.

“We also measured all the energy, mass distribution, and quantum numbers of the system,” Daniel Brandenburg, a Goldhaber Fellow at BNL who analyzed the STAR data, said in a statement.

Even in 1934, Xu said, the researchers realized the cross section for the photons to interact was so small that it was almost impossible to create conditions necessary for such an experiment.

“Only in the last 10 years, with the new angular distribution of e-plus [positrons] and e-minus [electrons] can we say, ‘Hey, this is from the photon/ photon creation,’” Xu said.

Bending light in a vacuum

Heisenberg and Euler in 1936 and Toll in the 1950’s theorized that a powerful magnetic field could polarize a vacuum, which should deflect the paths of photons. Toll calculated in theory how the light scatters off strong magnetic fields and how that connects to the creation of the electron and positron pair, Xu explained. “That is exactly what we did almost 70 years later,” he said.

This is the first experiment on Earth that demonstrates experimentally that polarization affects the interactions of light with the magnetic field in a vacuum.

Xu explained that one of the reasons this principle hasn’t been observed often is that the effect is small without a “huge magnetic field. That’s why it was predicted many decades ago, but we didn’t observe it.”

Scientists who were a part of this work appreciated the connection to theories their famous and successful predecessors had proposed decades earlier.

“Both of these findings build on predictions made by some of the great physicists in the early 20th century,” Frank Geurts, a professor at Rice University, said in a statement. 

The work on bending light through a vacuum is a relatively new part of the research effort.

Three years ago, the scientists realized they could study this, which was a surprising moment, Xu said.

“Many of our collaborators (myself included) did not know what vacuum birefringence was a few years ago,” he said. “This is why scientific discovery is exciting. You don’t know what nature has prepared for you. Sometimes you stumble on something exciting. Sometimes, there is a null set (empty hand) in your endeavor.

Xu lives in East Setauket. His son Kevin is earning his bachelor’s degree at the University of Pennsylvania, where he is studying science and engineering. His daughter Isabel is a junior at Ward Melville High School.

As for the recent work, Xu, who earned his PhD and completed two years of postdoctoral research at Yale before coming to BNL, said he is pleased with the results.

“I’ve been working on this project for 20 years,” he said. “I have witnessed and participated in quite a few exciting discoveries RHIC has produced. These are very high on my list.”

From left, postdoctoral researcher Yunjun Zhao and Brookhaven Lab biochemist Chang-Jun Liu in a greenhouse with poplar trees. Photo from BNL

By Daniel Dunaief

Plants not only make our food, produce the oxygen we breathe, and provide key ingredients in medicines, but they could also contribute chemicals that might otherwise require fossil fuels to produce.

Scientists have known since 1955 that poplar trees produce small amounts of a product called p-hydroxybenzoic acid that they attach to the lignin in their cell walls. What they didn’t know, however, was how they were attached.

After years of cloning genes and, more recently, using the gene editing tool CRISPR, Chang-Jun Liu, a plant biochemist at Brookhaven National Laboratory, and collaborators in Japan discovered the gene that codes for an enzyme that catalyzes the attachment of pBA to the lignin.

Up to now, companies have produced pBA by using fossil fuels as raw materials and for the energy required to generate enough heat and pressure for the catalytic reactions.

This discovery, which Liu published in the journal Nature Plants, could provide a more eco-friendly way to produce a chemical involved in the manufacture of toothpaste, shampoos, commercial moisturizers, shaving gels, and spray tanning solutions, among other products.

The global market value of p-hydroxybenzoic acid was $59 million in 2020 and is expected to climb to $80 million in the next five years.

“We wanted to identify the enzyme that is responsible for attaching pBA into lignin and reconstitute this pathway and promote its storage in the cell wall,” Liu said. Ideally, he’d like to combine the pathways that produce the donor molecule containing pBA with their enzyme to promote pBA storage in cell walls.

Once Liu found the gene responsible for that enzyme, he did what scientists typically do to check on the importance of a genetic sequence: first, he knocked it out and second, he overexpressed it.

By knocking out the genetic sequence, he found that poplar trees stopped producing pBA. Overexpressing the gene, on the other hand, not only increased the amount of this chemical by about 48 percent, but also raised the strength of the lignin and, consequently, the durability of the cell wall.

Aside from the benefit of increasing the natural production of the chemical, changing the amount of pBA could have implications for the environment and industry. Less durable lignin, which has a lower amount of pBA, could be useful in producing pulp, paper and biofuel, making it easier to access the biomass of the wood.

More durable lignin could be useful in the timber industry, while also enabling the plant to remove more carbon, mostly in the form of carbon dioxide, from the air.

“If we can engineer the plant to produce more of this carbon-dense compound, … particularly in the root, we can fix more carbon into the underground fraction, which will absorb more carbon from the air to promote carbon sequestration,” Liu said.

A long process

The work that led to identifying the gene that codes for the enzyme that attaches pBA to lignin took about 15 years.

Liu knew this enzyme worked to attach pBA, among other chemicals, in a test tube, but the journey to prove its importance in the poplar trees took considerable work.

Liu cloned 20 genes that are expressed in woody tissues and encoded enzymes called acyltransferases. While expressing these enzymes, he mixed them with an isotope-labeled carbon, which allowed him to check to see whether the enzyme contributed to the process of attaching pBA to lignin.

He tried using RNA interference to knock down the targeted gene, but that didn’t work.

The breakthrough that established the importance of this gene came when Liu used CRISPR. 

Next steps

Scientists aren’t sure of the specific steps or even why plants produce pBA in the first place.

Plants produce pBA through the shikimate pathway, but the exact routes leading to pBA formation are still undiscovered. 

As for why plants produce pBA, one hypothesis is that the plant uses a higher amount as a defense mechanism, making its lignin harder to remove for an insect. It could also provide resistance to mechanical stress caused by wind or snow.

“We do not have solid evidence to prove that,” he said, but “we need to explore that further.”

Liu also hopes to take a synthetic biology approach to build a more effective pathway by using the enzyme to make the plant a partner in producing pBA and in capturing and storing organic carbon.

The biochemist hopes to find a commercial partner who might be interested in exploring the development of a process that occurs naturally in poplar trees.

The environmental impact of increasing pBA in plants on the ecology of the areas in which these poplar trees might grow is unclear.

“We do not know at this moment whether this will benefit or be harmful to the soil microbial community,” he said. “In some cases, it can help the plant absorb more nutrients. It potentially can also kill other microbial life.”

For the plant, it’s unclear what the effect of higher pBA might be. The enzyme Liu identified moves pBA from inside the cell to the cell where, which would likely mitigate any toxicity because that is dead material. 

“We expect the increase of cell wall-bound pBA should promote the trees’ ability in withstanding environmental changes,” he explained.

Altering the cell’s metabolic processes by rebuilding a new pathway that produces high amounts of pBA could negatively affect a tree’s normal growth. Liu would need to conduct more experiments to explore this possible effect.

A resident of Rocky Point, Liu lives with his wife Yang Chen, who is a special education teacher assistant at Rocky Point Middle School. Their son Allen is in his third year at Purdue University, while Bryant is in his second year at the University of Southern California. The family enjoys skiing and hiking trips.

The work to confirm the link between the gene and the production of pBA involved numerous post doctoral researchers.

Liu appreciates the effort of his research team over the years. “I’m very happy that we were finally able to resolve this issue,” he said.

Charles and Helen Reichert Planetarium

The Reichert Planetarium at the Suffolk County Vanderbilt Museum, 180 Little Neck Road, Centerport presents an exciting new program for young astronomers from Monday, Aug. 23 to Thursday, Autg. 26. Enroll your kids in the Junior Astronomer Workshops for four days filled with stellar activities, crafts, games, and Planetarium shows – presented by the Vanderbilt’s talented astronomy educators.

Erin Bennett, lead Planetarium educator, said, “Junior astronomers will learn about astronomy topics that include the Solar System, how to use a telescope, and how to identify constellations they can see from their own backyard. This program focuses on hands-on learning activities and crafts supplemented by interactive presentations in the Planetarium theater.”

Each session is from 9 a.m. to 1 p.m. Each day includes a show in the Planetarium, an educational activity or game, a craft, and a break for lunch. Lunch will not be provided. Junior Astronomers are expected to bring a bag lunch, which will be refrigerated. Registration is open for students between 8 and 12 years old. Cost: $145 for non-members; $125 for members. Space is limited, early registration is encouraged.

Anyone who is not vaccinated must wear a face mask. There will be time set aside for campers to eat lunch and take a mask break.

For any questions, please email erin.bennett@vanderbiltmuseum.org.

 

Attendees at a conference at CSHL, an in-person tradition started in 1933. These conferences were suspended from 1943 to 1945 during WWII and were virtual during the pandemic in 2020 and for most of 2021. Photo by Miriam Chuai/CSHL

By Daniel Dunaief

For scientists, meetings and conferences aren’t just a chance to catch up on the latest research, gossip and see old friends: they can also provide an intellectual spark that enhances their careers and leads to new collaborations.

Amid the pandemic, almost all of those in-person conferences stopped, including the annual courses and meetings that Cold Spring Harbor Laboratory hosts. The internationally renowned lab has run meetings since 1933, with a few years off between 1943 and 1945 during World War II.

CSHL’s David Stewart. Photo by Gina Motisi/CSHL

While scientists made progress on everything from basic to translational research, including in laboratories that pivoted towards work on the SARS-CoV-2 virus, which causes COVID-19, they missed out on the kinds of opportunities that come from in-person interactions.

Assuming COVID infection rates are low enough this fall, CSHL is hoping to restart in-person conferences and courses, with the first conference that will address fifty years of the enzyme reverse transcriptase scheduled for Oct. 20th through the 23rd. That event was originally scheduled for October of 2020.

One of the planned guest speakers for that conference, David Baltimore, who discovered the enzyme that enables RNA to transfer information to DNA and is involved in retroviruses like HIV, won the Nobel Prize.

“I am hoping that there will be significant participation by many eminent scientists, so that is in itself somewhat [of] a ceremonial start,” wrote David Stewart, Executive Director of meetings and courses at Cold Spring Harbor Laboratory.

To attend any of the seven in-person meetings on the calendar before the end of the year, participants need to have vaccinations from either Pfizer, Moderna, Johnson & Johnson or AstraZeneca.

Attendees will have to complete an online form and bring a vaccination card or certificate. Scientists who don’t provide that information “will not be admitted and will not get a key to their room or be able to attend the event,” Stewart said.

CSHL also plans to maintain the thorough and deep cleaning procedures the lab developed. 

Stewart hopes that 75 to 80 percent or more of the talks presented will be live, with a virtual audience that could be larger than the in-person attendance.

“It is important to have a critical mass of presenters and audience in-person, but there’s no real limit on how large the virtual audience could be,” he explained.

Typically, the courses attract participants from over 50 countries. Even this year, especially with travel restrictions for some countries still in place, Stewart expects that the majority of participants will travel from locations within the United States.

The Executive Director explained that CSHL was planning to introduce a carbon offset program for all travel to conferences and courses that the facility reimburses starting in 2020. After evaluating several options, they plan to purchase carbon offsets from Cool Effect and will encourage participants paying their own way to do the same or through a similar program.

The courses, meanwhile, will begin on October 4th, with macromolecular crystallography and programming for biology. CSHL hopes to run six of these courses before the end of the year, including a scientific writing retreat.

“We are looking to 100 percent enrollment for our courses, so likely this year that will largely be domestic,” Stewart explained.

The courses, which normally have 16 participants, may have 12 students, as the lab tries to run these training opportunities safely without masks or social distancing.

From March of 2020 through the end of last year, the lab had planned 25 meetings and 25 courses. As the pandemic spread, the lab pivoted to virtual meetings. “I felt like a car salesman trying to sell virtual conferences,” Stewart recalled. For the most part, the lab was able to keep to its original schedule of conferences, albeit through a virtual format.

In addition to the scheduled meetings, CSHL decided to add meetings to discuss the latest scientific information related to COVID research. 

Stewart approached Hung Fan, a retired virologist at the University of California at Irvine, to help put together these COVID exchanges. Those meetings occurred in June, July, August, October, and January. The sixth one recently concluded.

The meetings addressed “everything around the science of the virus,” Stewart said, which included the biology, the origin, the genomics, the immune response, vaccines, therapeutics and diagnostics, among other scientific issues.

“There was a lot of excellent work being done around SARS-CoV-2,” Stewart said. “We were trying to identify that early on. It was helpful to have people who knew the field well.”

Fan said he combed through preprints like the CSHL-based bioRxiv and related medRxiv every day for important updates on the disease.

Fan described the scientific focus and effort of the research community as being akin to the Manhattan Project which built the atomic bomb during World War II, where “everybody said, ‘We have a common enemy and we want to apply all our capabilities to combating that.”

While Fan is pleased with the productive and valuable exchanges that occurred amid the virtual conferences, he recognized the benefit of sharing a room and a drink with scientific colleagues.

“A lot of the productive interactions at meetings take place in a social setting, at the bar, over dinner” and in other unstructured gatherings, he said. “People are relaxed and can share their scientific thoughts.”

After presentations, Fan described how researchers discuss the work presented and compare that to their own efforts. It’s easier to talk with people in person “as opposed to making a formalized approach through letters and emails.”

Stock photo

By Elof Axel Carlson

Elof Axel Carlson

The IQ or intelligence quotient was introduced early in the 20th century to measure learning abilities in school children. It spread from Germany to the United States where it was enthusiastically adopted in K-12 schools.  

I took the test four times. The first score I got, 116, was in first or second grade. The second score, about 3 years later, was 130. The third test in junior high school (PS210) was 149. The last score was in my freshman orientation week at NYU and it was 160. How do I know my scores? I was a teacher’s pet throughout my education and in high school, one of my volunteer activities was filing the report cards of students after teacher’s made their entries. 

In the process of filing I looked at my own record card (and my friends) and saw my scores for K-12. I saw my NYU score while being counseled in the Freshman week follow up. My test scores for various aptitude tests were on the sheet of paper my counselor was reading. She said I was talented but very insecure.  

The IQ score is usually interpreted in 30-point intervals with normal 100 (86-115); bright 130 (116- 145); and genius (146 and up) for the more intelligent students. 

A more damning score exists for categories of students classified as slow learners, with a terminology no longer used, morons 70 ( 56-85); imbeciles 40 (26-55); and idiots (25 and below). Those with less than normal IQ scores are sometimes classified collectively as retarded, feebleminded, or regarded or euphemistically as exceptional children.  

High IQ was widely admired and accepted as the basis for success in  school and in life. Lewis Terman’s Genetic Studies of Genius used the IQ test about 1910 to identify 1000 gifted children in California (mean IQ = 140). They were followed at Stanford University for more than 50 years.  They became college educated successful lawyers, MDs, professors, CEOs and other middle-class professionals with numerous publications and comfortable incomes.  

In contrast George and Muriel Goertzel’s Cradles of Eminence used a different approach. They selected 300 Americans who lived in the 20th century who had two or more books written about them. Their mean IQ was 127. Instead of comfortable middle-class upbringings that were characteristic of Terman’s high IQ children, the Goertzel’s biographies revealed about two-thirds had troubled homes growing up with a parent who was a business failure, psychotic, idiosyncratic, alcoholic, or physically handicapped. 

The Goertzel’s argued that IQ was insufficient for eminence. Eminence required what they called “a neural itch” that stimulated children to focus more intensely on their work, to exercise their imagination and creativity, and to generate the energy to complete tasks and compensate (sublimate in Freudian terminology) for the stress they encountered growing up. 

Not a single one of the 1000 Terman high IQ children ended up with a biography written about him or her. If being the subject of a biography is a measure of eminence, IQ is a poor predictor. IQ is more aptly an academic quotient and not an intelligence quotient. It measures the ability to take tests not the capacity to be innovative or driven to greatness.  

Elof Axel Carlson is a distinguished teaching professor emeritus in the Department of Biochemistry and Cell Biology at Stony Brook University.

A group of gelada monkeys in Ethiopia. Photo from Jacob Feder

By Daniel Dunaief

Timing can mean the difference between life and death for young geladas (an Old World monkey species). Geladas whose fathers remain leaders of a social group for as much as a year or more have a better chance of survival than those whose fathers are displaced by new males under a year after they’re born. 

New males who enter a social group can, and often do, kill the young of other males, giving the new male leaders a chance to impregnate the female members of their social group who might otherwise be unable to conceive.

Jacob Feder

 

The odds of a new male leader killing a young gelada are about 60 percent at birth, compared to closer to 15 percent at around a year of age, according to researchers at Stony Brook University (SBU).

Additionally, pregnant gelada monkeys often spontaneously abort their unborn fetuses once a new male enters the group, as the mother’s hormones cause a miscarriage that enables them to dedicate their resources to the future progeny of the next dominant male.

At the same time, the survival of females depends on becoming a part of a group that is just the right size.

Jacob Feder, a graduate student at SBU, and Amy Lu, Assistant Professor in the Department of Anthropology in the College of Arts and Sciences at Stony Brook, recently published a paper in Proceedings of the Royal Society B that explores the ideal group size that optimizes the longevity of females and the number of their offspring.

The researchers discovered a Goldilocks effect. By studying the behavioral and group data for over 200 wild geladas over the course of 14 years, they determined that a mid-size group with five to seven females has the greatest benefit for their own fitness and for the survival of their offspring.

“There tends to be a trade off” in the dynamics that affect female geladas in different groups, Feder said. Females in the biggest groups face a higher risk of takeovers and takeover-related infanticide, since males are more likely to try to dominate a part of larger social groups where they have greater reproductive opportunities.

By contrast, individuals in the smaller groups may live on the periphery of a multi-group dynamic. These females are less protected against predators.

In their native Ethiopia, geladas are vulnerable to leopards, hyenas, and jackals, among others.

For the females, the survival of their offspring depends on the ability of males to remain in the group long enough.

“The male turnover is one of the major drivers of their reproductive success,” explained Feder.

Researchers have seen new males enter a group and kill infants born from another father. The infants, for their part, don’t often recognize the need to avoid new males, Lu said.

When males enter big groups, females often have to reset their reproduction.

Groups with about nine to 11 females often split into units of four to seven, Feder said. A new male might become the leader for half of the females, leaving the remaining male with the other half. Alternatively, new males may take over each group.

The pregnant females who are part of a group with a new male will spontaneously abort their offspring about 80 percent of the time, as females “cut their losses,” Feder said

About 38 percent of females live in a mid-sized group that is close to optimum size.

Gelada charm

According to Feder and Wu, geladas are a compelling species to research, Feder and Wu said.

Feder found his visits to the East African nation rewarding, especially when he had the opportunity to watch a small female named Crimson.

An important part of daily life for these primates involves grooming, where primates comb through each other’s hair, remove insects and, in many cases, eat them.

Crimson, who was a younger member of the group when Feder started observing geladas, didn’t have much grooming experience with this activity. Instead of running her hands over the body of her grooming partner, she focused on her mouth. Her partner’s wide eyes reflected surprise at the unusual grooming choice.

One of the favorites for Lu was a monkey who has since passed away named Vampire. A part of the V group, Vampire was taller and bigger than most adult females. She displaced male geladas, some of whom were larger than she, almost as often as they displaced her.

“If you go out in the field enough, you know the individuals pretty well,” Lu said. “They all have their own personalities. Some of them walk in a different way and react to situations differently.”

A resident of Centereach, Feder grew up in northern Connecticut, attending Wesleyan University as an undergraduate, where he majored in music and biology. A bass guitar player, Feder said he “dabbles in anything with strings.”

In fourth grade, Feder read a biography of Dian Fossey, which sparked his interest in biology.

While he has yet to combine his musical and science interests with geladas, Feder said these monkeys have a large vocabulary that is almost as big as chimpanzees.

Lu, meanwhile, started studying geladas as a postdoctoral researcher. They’re a great study species that allow scientists to ask compelling questions about reproductive strategies. “At any point, you can follow 20 social groups,” Lu said.

Lu, whose two children are four years old and 16 months old, said she has observed the similarities between human and non-human primate young.

“Babies throw tantrums, whether it is my child or a gelada infant protesting being put on the ground,” she described in an email. Gelada infants use a sad “cooing” sound. Sometimes, the sad cooing sound is real and sometimes “they just get what they want.”

Image from BNL

Every year, the U.S. Department of Energy’s (DOE) Brookhaven National Laboratory opens its gates to thousands of community members for open house events called Summer Sundays. Visitors get to meet the Lab’s scientists and tour a different world-class science facility each week, including the Relativistic Heavy Ion Collider (RHIC), the National Synchrotron Light Source II (NSLS-II), and the Center for Functional Nanomaterials (CFN)—all DOE Office of Science User Facilities.

Following the success of Brookhaven’s virtual Summer Sundays program in 2020 and to continue limiting the spread of COVID-19, the Lab is bringing back its online Summer Sunday program for 2021. Over three Sundays this summer, Brookhaven will host a series of live, virtual events for people of all ages. Each event will feature a guided tour of a Brookhaven Lab facility and live Q&A sessions with a panel of scientists.

Brookhaven Lab plans to return to an in-person public tour format for Summer Sundays 2022, as conditions permit.

 

 

Schedule of events

NSLS-II: Sunday, July 25 at 3:30 p.m. ET

Tune in to get an up-close look at some of the “beamlines” where scientists use ultrabright x-ray light to see the atomic structure of batteries, proteins, and more. Viewers will have the opportunity to pose questions to NSLS-II scientists about each beamline on the tour and all of the research conducted at NSLS-II. Watch on TwitterFacebook, or YouTube.

RHIC: Sunday, August 1 at 3:30 p.m. ET

Join Brookhaven scientists as they explore the physics of particle colliders, including RHIC and the upcoming Electron-Ion Collider (EIC). Get a behind-the-scenes look at RHIC’s operations, then scientists for a Q&A session where they’ll take viewers’ questions about RHIC and the EIC. Watch on TwitterFacebook, or YouTube.

CFN: Sunday, August 8 at 3:30 p.m. ET

Investigate our world at the nanoscale with CFN, where scientists will show viewers the sophisticated microscopes and research tools they use to observe ultrasmall science. Viewers will have the opportunity to pose questions to CFN scientists about each scientific instrument on the tour and all of the research conducted at CFN. Watch on TwitterFacebook, or YouTube.

More details about these events will be announced soon. For the most up-to-date information, follow Brookhaven Lab on Facebook or visit the Summer Sundays website.

How to watch and ask questions

Each of the Lab’s live Summer Sundays events will be streamed to TwitterFacebook, and YouTube. At the time of the event, the live stream will be pinned to the top of Brookhaven’s profile on each platform. You do not need to have a Twitter, Facebook, or Google account to watch the stream.

Viewers are encouraged to submit their questions for the Q&A segment in advance through the Lab’s social media accounts or by sending an email to [email protected]. Live questions will also be accepted during the Q&A through the chat functions on all streaming platforms mentioned above.

Brookhaven National Laboratory is supported by the U.S. Department of Energy’s Office of Science. The Office of Science is the single largest supporter of basic research in the physical sciences in the United States and is working to address some of the most pressing challenges of our time. For more information, visit https://energy.gov/science.

Follow @BrookhavenLab on Twitter or find us on Facebook.

Rebecca Smith at the Sólheimajökull glacier in Iceland, where the scientist did field work during the 2015 Astrobiology Summer School. Photo from Rebecca Smith

By Daniel Dunaief

Rocks may not speak, move or eat, but they can and do tell stories.

Recognizing the value and importance of the ancient narrative rocks on Earth and on other planets provide, NASA sent vehicles to Mars, including the rover Perseverance, which landed on February 18 of this year.

Perseverance brought seven instruments, most of them identified by the acronym-loving teams at NASA, that carry out various investigations, such as searching for clues about a water-rich environment that may have sustained life about 3.5 billion years ago.

Several instrument teams developed and monitor these pieces of equipment, including Joel Hurowitz, Associate Professor in the Department of Geosciences at Stony Brook University and Deputy Principal Investigator on the Planetary Instrument for X-ray Lithochemistry, or PiXL.

In addition to the instrument leads, NASA chose participating scientists who can contribute to several teams, providing scientific support for a host of questions that might arise as the rover explores the terrain of the Red Planet 128 million miles from Earth.

Rebecca Smith, a post-doctoral researcher at Stony Brook in Geosciences Professor Scott McLennan’s lab, is one such participating scientist.

“I get to move around between all these different groups, which is fun,” said Smith, whose appointment will last for three years. While the Mars2020 program takes up about 20 percent of Smith’s time, the remainder is focused on the Mars Science Laboratory mission. Smith is likely to spend almost all of her time on Mars2020 starting this September.

Smith has helped make the science plans for the rover. The scientist and other researchers help select targets for the instruments that will help answer specific science questions. For this work, they collaborate with different science teams. Smith plans to get more involved with specific instrument teams soon, including SuperCam, PiXL and Sherloc.

For Smith’s own research, the scientist has a suite of rock samples that include lacustrine carbonates and hydrothermally altered volcanic rocks. The volcanic rocks formed under conditions that might be analogous to those once present in Jezero crater, where the rover landed and is currently maneuvering. The crater is just north of the Martian equator and has a delta that once long ago contained water and, potentially, life.

On Earth, Smith is using versions of the SuperCam, PiXL, and Sherloc to understand how these rocks would look to different instruments and determine what baseline measurements they need to tell the different types of rocks apart using the instruments aboard the rover.

Smith has studied rocks on Earth located in Hawaii, Iceland and the glaciers in the Three Sisters Volcanic Complex in Oregon.

Many planetary geologists use Earth as an analog to understand geologic processes on other planets. It is still uncertain if the climate of early Mars was warn and wet or cold and icy and wet, Smith explained in an email, adding, “It is possible the minerals we see with the rovers and from orbit can help us answer this question.” 

Most of the work the scientist been involved with is trying to understand how Mars-like volcanic rocks chemically weather under different climates.

Through previous research on Mars, scientists discovered that large regions had poorly crystalline materials. The poorly crystalline nature of the materials makes them difficult to identify using rover-based or orbiter-based instruments.

“The fact that they could have formed in the presence of water makes them important to understand,” Smith explained.

Part of the work Smith is doing is to understand if poorly crystalline material formed by water have specific properties that relate to the environment or climate in which they formed.

Smith said the bigger picture question of the work the teams are doing is, “was there life on Mars? If not, why not? We think that Mars, for the first billion years or so, was pretty similar to Earth around the same time and Earth developed life.”

Indeed, Earth had liquid water on its surface, which provided a habitat for microbial life about 3.5 billion years ago.

The ancient rock record on Mars provides a better-preserved history because the Red Planet doesn’t have plate tectonics.

“Based on what we know about Earth, if life ever developed on early Mars, it would likely have been microbial,” Smith wrote.

Other goals of Mars2020 include characterizing the climate and the geology. Both goals focus on looking for evidence of ancient habitable environments and characterizing those to understand a host of details, such as the pH of the water, the temperature and details about how long the water was on the surface.

Part of the reason NASA put out a call for participating scientists is to “bridge instrument data” from different pieces of equipment, Smith explained.

“I love the collaborative nature of working on a team like this,” Smith offered. “Everybody is interested in getting the most important information and doing the best job that we can.”

Smith enjoys the opportunity to study potentially conflicting signals in rocks to determine what they indicate about the past.“Geology is just so complex. It’s a big puzzle. Forces have been acting over a very long period of time and forces change over time. We are trying to tease apart what happened and when.”

While Smith works at Stony Brook, the post-doctoral scientist returned to California during the pandemic to live closer to her family. After finishing the current research program, Smith plans to remain open to various options, including teaching.

Smith appreciates the opportunity to work on the Mars 2020 mission, adding, “I’m really grateful for that during this past year in particular.”

Photo by Julianne Mosher

Famed scientist, inventor and entrepreneur Nikola Tesla would have been 165 this year, and the best way to celebrate his life and legacy was to party at his old lab in Shoreham. 

On Saturday, July 10, hundreds of people gathered at the Tesla Science Center at Wardenclyffe for the Tesla Birthday Expo and Birthday Night Show.

The events featured a number of educational exhibits including many of the local STEAM — science, technology, engineering, arts and math — exhibits, robotic clubs, Tesla coils, Tesla car showcase, amateur radio, battlebots, Maker Space trailer, local artisans and an interactive STEAM bus from New York Institute of Technology. The daytime event was coupled with a lively nighttime celebration featuring the band ArcAttack.

“What an amazing day to celebrate one of this world’s most acclaimed scientist and inventor,” said county Legislator Sarah Anker (D-Mount Sinai). “Thanks to the many TSCW volunteers, local and international community support, and the many partnerships with government, Nikola Tesla’s legacy will continue to inspire and encourage our future scientists.”

The Tesla Science Center at Wardenclyffe, located in Shoreham, is Nikola Tesla’s last remaining laboratory. Known as a man before his time, he was deemed a genius while researching alternating current systems. He believed that energy didn’t have to be a rich man’s luxury. Energy could be available to all and powered naturally. He thought he could power the whole Northeastern seaboard from Niagara Falls. 

An inventor with hundreds of patents, he was involved in the invention of the radio, remote control and more.

In 1901 Tesla acquired the Wardenclyffe property in Shoreham to test his theories of being able to wirelessly transmit electrical messages, funded by J.P. Morgan. A huge 187-foot tower was designed and constructed for the purpose.

In 1903 creditors confiscated his heavier equipment, and in 1917 the tower was demolished. The concrete feet used to hold the structure can still be seen on the property today. 

Tesla was eventually cut off, causing him to lose control of the site. The property became a film processing company in the early ’30s, where harsh chemicals were dumped into the ground. The contaminated property was sold again and became shuttered in 1987. 

A decades-long cleanup ensued, and the property was put back up for sale. 

The community — locally, nationally and even internationally — came together to fundraise to eventually buy the property in 2013, preserve it and make it a real historic site. 

According to Doug Borge, chief operating officer at TSCW, “At our annual Tesla Birthday events, we not only celebrate Nikola Tesla’s contributions, but also his living legacy that we each build upon through science and innovation.”

The mission of Tesla’s last remaining lab is to develop the site into a transformative global science center that embraces his bold spirit of invention, provides innovative learning experiences, fosters the advancement of new technologies and preserves his legacy in the Tesla Museum.

The group imagines a world where people appreciate Tesla’s contributions, are inspired by his scientific audacity and engage in the future betterment of humanity.

“Today is a perfect example of where we are as an organization,” Borge said. “We’re a community hub for people that love science technology, that are associated with Nikola Tesla and to be a resource for people to leverage, learn and become their own version of Tesla.”

In general, technology and interactivity at this year’s Tesla Birthday Expo were more engaging and popular than ever, he added. New and expanded STEAM exhibits allowed attendees to get hands-on with Tesla inventions and technology. 

ArcAttack made their first visit to Wardenclyffe and took things to a whole new level with a performance at the night shows featuring Tesla coils, rock music and lightning-producing electric instruments. Volunteers in the audience were “zapped” in a Faraday cage, including TSCW’s executive director Marc Alessi.

“We weren’t sure what to expect in terms of attendance at this year’s Tesla Birthday events, due to the pandemic,” Borge said. “Fortunately, we had a great turnout at both the daytime Tesla Birthday Expo and night show.”

Borge added that “the expo is interesting because you can see the crowds clustering around specific exhibits and interacting with enthusiasm.”  

Some fan favorites were the 3D scan that showed the interior of Tesla’s laboratory as it looks today, the robotics and maker space area, along with the go-carts and robots zipping around. 

“This is such an exciting event for the community to learn about important advances in technology,” said attorney and advocate Laura Ahearn, of Port Jefferson. “I’m really excited about getting to meet community members that come here, and some of the high school students that have built from scratch robotic devices better than anything … when I was in high school, I wish I would have had the opportunities that these young students have because it’s going to help them in their future.”

Borge said within the next few weeks, demolition of the dilapidated, noncontributing factory building suffocating Tesla’s laboratory will begin. Additionally, they plan to break ground on its visitor center that will allow them to pilot exhibits and engage and educate more visitors at Wardenclyffe. 

“These are important next steps in the development of TSCW and a moment that many of our global supporters have been looking forward to since TSCW’s record-breaking crowdfund in 2012, which raised $1.4 million in six weeks from 33,000 donors in 108 countries,” he said. “These funds, along with a matching grant from New York State and contributions from supporters like the Musk Foundation, enabled us to purchase Wardenclyffe in 2013. Fast forward to 2021, and TSCW is now positioned to start renovations after raising $10.2 million and acquiring the necessary plans and permits. It’s important to note that we still need to raise another $9.8 million to finish developing the site.”

County Legislator Kara Hahn (D-Setauket) also made an appearance.

“It’s just really exciting to encourage interest in science and to recognize the history here on Long Island,” she said. “It has such an important impact in so many ways.”

The center will be hosting more events this summer, including the Sound of Science concert on Aug. 28 in collaboration with another nonprofit, Rites of Spring Festival, that will offer a unique immersive musical experience by electronic musicians and contemporary composers.  

Sept. 23 is TSCW’s Third Annual Gala fundraiser for an evening of virtual entertainment, auctions and tech surprises. 

Later in the year, Wardenclyffe will host a Halloween event on Oct. 30, and their annual holiday lighting on Dec. 3. 

Vanderbilt visitors enjoy a trip into space. Photo by Jennifer Vacca

The Suffolk County Vanderbilt Museum in Centerport found a way in the late 1960s to honor William K. Vanderbilt II’s (1878-1944) love of science and exploration – and to create a new revenue source – when it decided to build a planetarium. Last month, the Vanderbilt Reichert Planetarium observed its 50th birthday.

Opened on June 29, 1971, the Planetarium began generating income to support Museum operations. The Planetarium was a testimony to Mr. Vanderbilt’s passionate interest in science and astronomy and his use of celestial navigation in the early 20th century while circumnavigating the globe in his yachts. Most importantly, the Planetarium was and is essential to the Museum’s mission to provide high-quality astronomy and science education.

The Planetarium, which was popular with visitors immediately, became an invaluable teaching tool. By the second decade of this century, however, the facility and its technology were worn and years out of date. In 2012, the Vanderbilt, with substantial help from Suffolk County, undertook a $4-million renovation and complete technological update of the facility, which reopened on March 15, 2013.

The renovation design allows the star projector to retract out of audience sightlines. This feature, along with removable rows of seating, provides flexibility for the William and Mollie Rogers Theater to be used also as a venue for lectures, performing arts, and large-group meetings. Flexible theatre space allows the Museum to expand its audiences, visibility, and regional appeal.

In February 2020, the Vanderbilt received approval from Suffolk County to use Museum endowment funds for significant technological upgrades. The Vanderbilt purchased two advanced systems – laser phosphorus full-dome video projectors that generate sharper imagery and laser-beam projectors to enhance laser-light entertainment shows. Dave Bush, director of the Planetarium, said this state-of-the-art equipment adds dimension and excitement and greatly improves the visual experience.

The Planetarium is an education center with astronomy programs for visiting school groups that align with New York State educational standards. The facility also offers science entertainment programs and laser-light shows. The Observatory recently added a solar telescope for safe viewing of the Sun.

The Planetarium, which has a 60-foot-diameter dome, is one of the largest and most advanced in the United States. More than 85,000 visitors see shows there each year.

In honor of its largest benefactors, the Vanderbilt renamed the facility the Charles and Helen Reichert Planetarium in 2019. Their unprecedented gift is helping to ensure the Planetarium’s future.

Visit www.vanderbiltmuseum.org for upcoming shows and programs.