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Featured in a radio segment airing Tuesday March 26th, Dr. Virginie Faramaz teaches an introductory astronomy class at the Tohono O'odham Community College, bringing University of Arizona curriculum to students from Tribal nations across the country

Steward Observatory Professor Teaches Indigenous College Students About the Stars

Steward Observatory Professor Teaches Indigenous College Students About the Stars

Before Dr. Virginie Faramaz arrived at Steward Observatory as an assistant research professor, she had earned her PhD in exoplanetary system dynamics"trying to predict planets from the shape of comet belts"and she had completed two postdocs: one in Chile, and another at the Jet Propulsion Lab." She became faculty at University of Arizona during the pandemic, and she is currently interested in how planetary systems within the habitable zone of stars retrieve organic materials and water from beyond what she calls the "ice line." Her work will help researchers choose exoplanets to observe that are likeliest to harbor life."

But alongside her interest in faraway planets and the hunt for clues of life beyond Earth, Faramaz arrived in Tucson with the hope of teaching. This year, that dream came true: she was invited to lead an online course for the San Carlos Apache College (SCAC) in conjunction with the Tohono O'odham Community College (TOCC), following in the footsteps of Steward Observatory's Peter Milne, who taught introductory astronomy in this setting last year. Stepping beyond her research and into the virtual classroom, Faramaz now teaches about the solar system to indigenous students from as far away as Nebraska.

Faramaz believes that her introductory course in astronomy sets students up for skills that reach far beyond astronomy, from critical thinking to physics. "We touch on a little bit of everything," she says. This is what initially drew her to astronomy as a student, too: she double-majored in physics and chemistry, and when she went on to pursue her master"s degree, she discovered that astronomy spanned all her interests. If her TOCC students "come away with some general knowledge of the universe, and some sense of wonder, and some sense of how science works, and if they have a little bit of critical thinking "that's what I hope they will get out of the class."

This semester, Faramaz is learning as much from her students as they are learning from her. For example, Apache students in her class taught her that wintertime is traditionally the only time when stories about the night sky can be told"so in the early months of the semester, before winter turned to spring, Faramaz asked the class to share myths about the cosmos with each other. Some shared stories from as far away as Greece and the Yakama Nation. One student described how the Yomi people describe the universe as being made up of nine layers. Another student taught the class how the Big Dipper is called "the hook," describing the Tohono O'odham tool used during the local saguaro harvest to pluck fruit from the tops of tall cacti.

Between sharing stories about constellations and learning about quantum physics and spectral lines, the wonder of astronomy permeates Faramaz" class. "The immensity of space and the universe is so mind blowing," she says. "I hope it will give them the impulse to push further with their education."

On March 26th, Faramaz talks with the Tohono O'odham Community College radio station about her introductory astronomy class. The show airs locally on 3/26/2024 between 2 pm and 4 pm MST:

 

KWAK LP 102.5 (San Xavier Community)

KOHF LP 101.1 FM (Florence)

KOHN 91.9 FM (Sells)

KOHH 90.7 FM (San Lucy)

Jackie Champagne

A Steward Postdoc Tells Cosmic Stories for Kids

This fall, Dr. Jaclyn Champagne, our JASPER postdoc researcher at Steward Observatory, wrote a compelling piece for The Conversation about the environments where colossal black holes form (Powerful black holes might grow up in bustling galactic neighborhoods). The story was so popular that Astronomy Magazine re-published it, and The Conversation asked Dr. Champagne if she might be able to write a story for children about her research area. The result: a kid-friendly article that explores why some black holes are bigger than others. Read it here, and be sure to share it with the curious young readers in your life!

 

New images taken with the James Webb Space Telescope reveal intricate, never-before-seen structures and features hidden in visible light. The insights will help astronomers better understand the history of the Milky Way.

Click here to read more.

In a new paper authored by former UArizona Astronomy Major David Setton and Steward Observatory Associate Professor of Astronomy Gurtina Besla, a 100,000-light-year bow shock on the edge of the Milky Way may change our understanding of how the circumgalactic medium evolves.

Click here to read more.

At the University of Arizona, a pioneering group of astronomers is part of an international team that built the most sophisticated mid-infrared instrument in the world and launched it aboard a NASA telescope now a million miles from earth in search of distant galaxies, young stars, and new planets. This week, the Royal Astronomical Society (RAS) of the United Kingdom celebrated the accomplishments of that group, announcing that the prestigious Group Achievement Award has been awarded to the international Mid InfraRed Instrument (MIRI) team in honour of their work on the James Webb Space Telescope (JWST).          

                                                                                            

Developed over the course of two decades, JWST is the most powerful telescope ever launched into space. The spectacular images and scientific data coming from JWST have electrified astronomy and the public by redefining our understanding of the cosmos through new insights into the atmospheres of planets beyond our Solar System and new data on star and galaxy formation.

 

For over 50 years, scientists at UArizona have led in infrared astronomy. Infrared light lies beyond the visible light spectrum and lets us detect heat signatures from dim objects, to see through thick clouds of gas and dust that block visible light, or to look for redshifted light from the first stars and galaxies in the early universe. The pioneering infrared research at UArizona began with the work of Gerard Kuiper, Frank Low and Harold Johnson at the Lunar and Planetary Lab around 1965. George Rieke—co-lead of the MIRI project and Regents Professor of Astronomy and Planetary Sciences— joined this team of innovators in 1970. Together, they helped fuel a revolution which, over the course of 50 years, doubled the capability of mid-infrared technology every 10 months: a pace “that makes the growth of computer power look sluggish,” Rieke said.

NASA picked Rieke to collaborate with an international team of scientists to design and build an instrument to provide mid-infrared observations on the world’s largest and most complex space telescope. The revolutionary growth curve of mid-infrared technology has culminated in the 20-year MIRI project, extending the reach of JWST’s other three instruments to the longer mid-infrared wavelengths.  “MIRI has pushed this field to its technical limits,” Rieke says. “It’s going to lay down a heritage that astronomers are going to use for decades. It’s a complete revolution.”

MIRI senses wavelengths from 5 to 28 microns—a range that allows it to detect planets, comets, dust warmed by starlight, and protoplanetary disks. The latter capabilities have been revolutionary in the search for potential planets orbiting stars. Andras Gaspar, Associate Research Professor at Steward Observatory, led a 2023 paper on the debris disk around the star Fomalhaut, 25 light years away. The MIRI images revealed detailed images of nested concentric rings of dust around the star: belts most likely carved by the gravitational forces produced by embedded, unseen planets. The MIRI team has now turned its attention to the debris disk around Vega, a star at a similar distance from earth. As he puzzles through this new data from MIRI, Gaspar says he’s proud to be part of what he considers to be “humanity’s largest and most complex engineering achievement.” Compared with the moon landing, Gaspar says “I think technologically this is more advanced.” 

 

In the time since JWST launched into its million-mile orbit on December 25, 2021, other achievements from the MIRI team include the unveiling of a large number of active galactic nuclei—supermassive black holes at the centers of galaxies—that are buried in thick cosmic dust and hidden from astronomers despite decades of searching. “My very first research project as an undergraduate over ten years ago in China was to search for active galactic nuclei with the Spitzer data,” says Jianwei Lyu, a Steward Observatory Assistant Professor who has led the MIRI survey to detect these black holes. “It is such a wonderful experience to join the MIRI team and pick up the same topic again,” Lyu says. “It is unbelievable to see the huge progress made by JWST and I cannot be fortunate enough."

The MIRI team is large, diverse, and international. UArizona has worked closely with the NASA Jet Propulsion Laboratory (JPL), which had responsibility for the MIRI detectors and their electronics, the software, and the cooler that brings the instrument to a temperature close to absolute zero.  The rest of the instrument was provided by research institutes from ten European nations. Gaspar estimates that the total of astronomers, engineers, technicians, managers, and others involved in launching JWST number in the tens of thousands. Jane Morrison, Associate Staff Scientist at Steward Observatory, reflects on the nature of this team. “As a MIRI test team member, I think back on the various stages of testing MIRI as one of the most exhausting, challenging, rewarding and fun experiences of my career,” she says. “During the decades long testing, team members got married, had children, lost family members, or had other life-changing events. Throughout it all, the MIRI team supported each other through the difficulties of testing such a complicated instrument but also through the difficulties and challenges of life. "

Stacey Alberts, Associate Research Professor at Steward Observatory, who was first hired as a postdoc to work in MIRI instrumentation and science, and now nine years later serves as faculty at UArizona, says “typically science is very open-ended: we don’t have a deadline to figure out how galaxies change. But it's different when we need to launch a telescope.” The push to build and launch MIRI, Alberts says, meant that “we were all going to work together to make that happen.” The highlight to the team’s success—beyond the MIRI data that will continue to transform what we understand about the cosmos—was the flawless launch of JWST in 2021. “JWST is perhaps the most complicated satellite ever launched,” says Rieke, “but everything worked perfectly.” 

The recent award from the Royal Astronomical Society recognizes the entire MIRI team’s impressive achievement in bringing such a lengthy and complex international project to successful fruition, and the scientific results emerging from MIRI that their work has enabled.

 

“Every day I share with my granddaughter the wonder that MIRI and JWST has given us—the brilliant science and images. They are the building blocks of her future,” says Debra Wilson, Arizona MIRI Program Manager. “One thing I tell her: don’t let others say it cannot be done. Believe. Imagine. The improbable is possible.”

Today, as we mark the solstice, the students, staff, and faculty of Steward Observatory and the Department of Astronomy send our warmest greetings to all of you. From our very beginning, we have been transformed by the generosity of those who care about what we do. Lavinia Steward got us started with her generous gift of $60,000 for a telescope of “huge size,” the 36-inch telescope now on Kitt Peak.  Richard F. Caris enabled us to join the Giant Magellan Telescope as a Founding institution through his gift of $20,000,000 in 2015.  As we look to our future, we can not do it without the on-going support from all of you.

This past year has been full of extraordinary achievements for which we are tremendously thankful. Our astronomers discovered the most distant galaxy ever observed by humans and identified spectacular evidence of unseen planets circling a nearby star. Steward Observatory helped document the brightest gamma ray burst ever seen and Richard F. Caris Mirror Lab began casting the seventh (and last required) primary mirror segment for the Giant Magellan Telecope (GMT). Together with our sister departments LPL and Planetary Sciences, Steward Observatory and Astronomy ranked #1 in the NSF HERD rankings (research dollars expended) for a remarkable 35th consecutive year.

Our outreach and education programs continue to grow and excel. We currently have the largest number of undergraduate majors (over 400) and PhD students (51) that we have ever had. Our retention and graduate rates have been increased each of the past four years. Our students are grateful for the scholarship and research assistance provided by the Friends of Steward.

U.S NSF McMurdo Station Research Base, Antarctica. (GMT+13)

Lift off for GUSTO from the launch pad at Ross Ice Shelf near McMurdo, Antarctica.

University of Arizona professor Christopher Walker, principal investigator of the GUSTO scientific ballon mission, reports from the U.S National Science Foundation's McMurdo Station Research Base, Antarctica that  GUSTO’s integrated gondola and payload is currently ascending at flight altitude of approximately 120,000 feet and instrument calibrations are underway to study the interstellar space – the matter between the stars – using far infrared detectors. The mission is a joint effort between the University of Arizona, NASA and APL. Congratulations to the GUSTO team!

More information about this mission can be found on NASA's websiteUsing GPS data you can find where GUSTO is located right now here.  

The discovery of phosphorus in a molecular cloud at the edge of the Milky Way galaxy challenges current views of how the element originates and extends the galactic habitable zone.

"But to make phosphorus, you need some kind of violent event," explained Lucy Ziurys, Regents Professor of chemistry and biochemistry and astronomy and astronomer at Steward Observatory. "It is thought that phosphorus is created in supernova explosions, and for that, you need a star that has at least 20 times the mass of the sun." Learn more

University doctoral students used two radio telescopes, including the Arizona Radio Observatory 12-meter radio telescope on Kitt Peak, to make the discovery.

The GUSTO Payload

GUSTO Balloon Mission awaiting launch on December 22 or 27, 2023 from McMurdo station, Antarctica

The GUSTO mission—led by UArizona professor Christopher Walker—comes the latest news from team member Brian Duffy:

Their equipment compatibility test is Wednesday 20 December.

The Flight Readiness Review (FRR) is scheduled for 22 December.

After that, they will launch on the first day they have launch conditions compatible with our mission.

Chris Walker is estimating launch on 27 December! Learn more

The Verge: NASA’s GUSTO balloon telescope will map part of the Milky Way. The first to be funded as part of the Explorers Program, GUSTO will spend at least 55 days floating above Antarctica.

A new paper out in Nature highlights a discovery made with the NIRCam instrument on NASA’s James Webb Space Telescope (JWST): the telltale fingerprint of methane on a planet 950 trillion miles away. JWST observed the exoplanet WASP-80 b as it passed in front of and behind its host star, revealing spectra indicative of an atmosphere containing methane gas and water vapor. While water vapor has been detected in over a dozen planets to date, until recently methane – a molecule found in abundance in the atmospheres of Jupiter, Saturn, Uranus, and Neptune within our solar system – has remained elusive in the atmospheres of transiting exoplanets when studied with space-based spectroscopy. 

Methane, a molecule that is composed of a carbon atom surrounded by four hydrogen atoms, is an important molecule in atmospheres in the Solar System worlds and extrasolar planets. This discovery opens doors for understanding the chemical processes behind the birth the evolution of planets, and allows us to compare what we know about planets in our own solar system with exoplanets in other parts of the universe. 

This new study was made possible with the NIRCam instrument on JWST and its team of engineers, technicians and scientists who developed the camera, who were led by Marcia Rieke at the University of Arizona—making NIRCam one of the finest examples of female-led space science. NIRCam senses near infrared wavelengths longer than the human eye can see. The instrument has the extreme sensitivity in the near infrared necessary to search for the distinctive fingerprint of methane in planet atmospheres, even those that are more than 950 trillion miles away like WASP-80 b. 

UArizona Assistant Research Professor Everett Schlawin, in collaboration with the MANATEE team, modeled the atmosphere of the planet before JWST was launched to predict that methane would be detectable with NIRCam. Sure enough, the planet showed strong absorptions of light by methane in the atmosphere of the planet. Schlawin also performed one of two independent analyses to tease out the small planet signature from the vastly brighter host star to study the terminator of the planet (between its day and night) as well as the dayside (facing the star). The two independent analyses showed, to high confidence, that methane is present in this atmosphere, even though disequilibrium processes can destroy the molecule. This new detection opens the pathway to study planets below 1340 F/730 C, figuring out what they are made of and what kind of chemistry is governing their gaseous atmospheres.

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