Astrophysics

Interview with interviews Michael Oppenheimer, Professor of Geosciences and International Affairs and the High Meadows Environmental Institute at Princeton University. Oppenheimer describes the three-way nature of his work at Princeton, between the School of Public and International Affairs and the Science, Technology, and Environmental Policy program. He describes the possibilities for climate change policy in the transition from Presidents Trump to Biden, and he discusses the moral dimension to climate change diplomacy and what the “Global North” owes the “Global South.” Oppenheimer recounts his childhood in Queens, the opportunities that allowed him to enroll at MIT at age 16, and his decision to focus on chemistry and to become involved in political activity in the 1960s. He explains his decision to go to the University of Chicago for graduate school, where he studied under the direction of Steve Berry on low-temperature spectroscopy of alkali halides. Oppenheimer describes his postdoctoral research at what would soon become the Center for Astrophysics at Harvard to work on astrophysics from an atomic and molecular perspective and on the chemistry of comets. He explains how the acidification issue in the Adirondack Lakes serves as an entrée to his interests in environmental policy and how this led to his work for the Environmental Defense Fund. Oppenheimer describes his work on the linearity question and why it is relevant for understanding carbon emissions and his advocacy work on the Clean Air Act. He explains the early science that concluded that even a few degrees of warming would be globally catastrophic, and the early signs that the Republican party would serve generally to block legislation to mitigate climate change. Oppenheimer discusses his involvement with international climate negotiations and policy with the IPCC and the issue of contrarianism in global warming debates. He contrasts the simplicity of the greenhouse effect with the complexity of understanding climate change, and he explains his decision to move to Princeton within the context of what he thought the Kyoto Protocol had achieved. Oppenheimer reflects on how climate change has increased in the public consciousness, and at the end of the interview, he considers early missed opportunities for more change in climate policy, and where he sees reason for both optimism and pessimism as the world faces future threats relating to climate change.

This is an interview with Edward Weiler, who served as chief scientist of the Hubble Space Telescope from 1979 to 1998, as NASA Associate Administrator for science activities from 1998 to 2004 and again from 2008 to 2011, and as director of the Goddard Space Flight Center from 2004 to 2008. The interview focuses primarily on his work relating to Hubble and the James Webb Space Telescope. Subjects addressed include his work developing international collaboration, and he explains the value of his strong working relationship with David Southwood of the European Space Agency. Weiler details his involvement with the correction of the spherical aberration afflicting Hubble’s primary mirror. He highlights NASA Administrator Dan Goldin’s role in establishing the scope of the Webb telescope, and he offers his views on the project’s troubles and the 2010 review chaired by John Casani that diagnosed sources of its cost growth and schedule slippage. Weiler also recounts his motivations for retiring from NASA in 2011, his activities since then, and he expresses his perspective on matters such as human space flight, lunar exploration, and the value of international partnerships in space science.

Interview with Tony Tyson, Distinguished Research Professor at UC Davis in the Department of Physics and Astronomy. The interview begins with Tyson sharing stories from his childhood in southern California and his early interest in ham radio. He discusses his undergraduate studies at Stanford and his introduction to low-temperature physics. Tyson describes his graduate studies at University of Wisconsin and a fellowship at University of Chicago. He explains his thesis experiment on phase transitions and discusses having both Dave Douglas and Chandrasekhar as advisors. Tyson recalls being recruited by Bell Labs and talks about his initial work there on gravitational radiation. He describes branching out into cosmology and astrophysics and recounts his time in John Wheeler’s gravity group at the Institute for Advanced Study. Tyson reflects on the impact of CCDs and his role in their development for astronomy. Tyson also discusses the evolution of the LSST project, of which he is the founding director. Topics include site selection, funding and fundraising, and the renaming of the project for Vera Rubin. The interview concludes with Tyson sharing his hopes for the future of the field and his excitement for the new discoveries that will inevitably come from the LSST. 

Interview with James Gunn, American astronomer and Emeritus Eugene Higgins Professor of Astronomy at Princeton University. Gunn discusses his graduate work at Caltech where he worked with Guido Munch. He describes his graduate thesis on the correlation function of galaxies and recalls his growing interest in cosmology at the time. Gunn traces the development of dark matter research during the 1970s and 1980s, reflecting on the important contributions of his peers as well as his own. He discusses his other research interests such as Omega matter and virial discrepancy. Gunn also describes his role in the growth of the cosmology department at Caltech. 

Interview with Matt Mountain, President of the Association of Universities for Research in Astronomy (AURA), and Telescope Scientist & Science Working Group member for the James Webb Space Telescope (JWST). Mountain recounts growing up in the UK and his early interest in science. He reflects on his time at Imperial College London, where his interest in astronomy suited his background in physics and his work on the infrared. He describes drifting away from theoretical physics and moving towards building instruments, later building one of the first infrared spectrographs for his PhD dissertation. He recounts his recruitment to the Royal Observatory Edinburgh by the Astronomer Royal Malcolm Longair, where he would help build CGS4 for the UKIRT telescope. Mountain recalls working with Tim Hawarden on his idea of passive cooling, which would later be used JWST. He describes being appointed as the project scientist for the Gemini project, leading to his move to the U.S. He explains having to learn and understand the US political system in relation to science, particularly the way astronomy is funded. He credits his time in Edinburgh with teaching him the importance of effective communication between engineers and scientists, which would prove crucial for his role as Gemini director and later projects. Mountain discusses his later role as director of the Space Telescope Science Institute and the early conversations on a next generation space telescope. He details his role as telescope scientist for the Webb telescope and his perspective on international space science partnerships. He reflects on the budget concerns and schedule delays surrounding the Webb telescope and the later working conditions during the Covid-19 pandemic. Towards the end of the interview, Mountain discusses some of the science from JWST, his current role at AURA, and the future of astronomy.

Interview with astrophysicist and cosmologist Neta Bahcall, the Eugene Higgins Professor of Astronomy at Princeton University. Bahcall discusses her undergraduate studies in physics and math in Israel before her move to Caltech. She recounts her PhD work with her advisor, William Fowler, as well as collaborations with Maarten Schmidt. Bahcall explains how she was studying nuclear physics at Caltech when she first learned of the virial discrepancy and became interested in galaxy clusters, prompting her to shift her studies toward astronomy. Bahcall describes her work on quasars and the beginnings of her work in cosmology. Throughout the interview, she provides an overview of galaxy cluster research in the 1970s, as well as the beginnings of dark matter research. Bahcall discusses many of her influential papers over the years, on topics such as clusters, large construction, dark matter and omega matter. She describes how her research on clusters relates to cosmology, as well as how her work intersects with radio astronomy. Bahcall reflects on the impact of being a woman in the field, and at the end of the interview, she shares memories from the 1985 IAU meeting on dark matter. 

In this interview, astronomer Peter Jakobsen discusses his involvement with the Hubble and James Webb Space Telescopes during his life-long career at the European Space Agency (ESA). He recounts his early childhood growing up in Cincinnati and later returning to his hometown in Denmark, where he attended the University of Copenhagen. He reflects on his time at the Laboratoire d’Astronomie Spatiale in Marseille during his Master’s degree and his time at Berkeley working in the Space Astrophysics Group led by Stu Bowyer. Jakobsen discusses his job as Project Scientist for the European involvement in the Hubble Space Telescope, the development of ESA’s Faint Object Camera, and the discovery of the spherical aberration. He details his role in the development of COSTAR and Hubble’s repair missions. Jakobsen recalls being skeptical of the initial talks for the Next Generation Space Telescope, but later taking on a key role for the European side of the project. He also recalls the competition between the contractors working on the initial design phase for NIRSpec. Jakobsen gives an account of his last years at ESA and the conditions that led to his retirement from the agency in 2011. He gives his perspective on Webb’s launch and reflects on the budget and schedule delay concerns. He discusses his post-retirement technical work and the guaranteed observing time program for JWST. Towards the end of the interview, Jakobsen describes his current focus with NIRSpec and his reflections on the future of astronomy.

Interview with Kenneth Kellermann, American astronomer at the National Radio Astronomy Observatory. The interview focuses on Kellermann’s role in the early development of very long baseline interferometry (VLBI), beginning in the 1960s. Kellermann goes into detail about the collaborations on VLBI between the American, Australian, and Swedish scientific communities. He also describes the informal exchanges he took part in with Russian scientists. Kellermann discusses the network of scientists from both the US and USSR that worked together on VLBI, and he speaks on his relationship with Iosif Shklovsky. The interview then shifts to Kellermann’s work on the search for extraterrestrial intelligence, beginning with his time in Australia. He talks about various SETI conferences, particularly the First Soviet-American Conference on Communication with Extraterrestrial Intelligence in 1971 in Byurakan. The interview concludes with Kellermann sharing his current thoughts on SETI and how the work has changed over time.

Interview with Peter Donald MacDougall Parker, Professor Emeritus of Physics at Yale. Parker recounts his childhood growing up in New York City and Massachusetts, attending Amherst College, the excitement of being a graduate student at Caltech in the 1960s working on nuclear physics and nuclear astrophysics, his postgraduate position at Brookhaven National Laboratory, and his move to Wright Nuclear Structure Laboratory at Yale University in 1966. Parker recalls over five decades of research, teaching, and service work that includes: experimental nuclear physics and astrophysics work using tandem accelerators, solar neutrino flux, and dark matter search; teaching every single physics course offered at Yale and developing a new course; committee work; the gradual changes in gender demographics in the physics department at Yale. Also prominently mentioned are Willy Fowler, Richard Kavanaugh, Thomas Tombrello, John Bahcall, Ray Davis Jr., Allan Bromley, and his twin brother Robert Parker.

In this interview, astronomer Massimo Stiavelli discusses his involvement with the Hubble and James Webb Space Telescopes. He recounts his early childhood growing up in Italy, higher education at the Scuola Normale Superiore in Pisa, and his interest in elliptical galaxies. He reflects on his time as a postdoctoral researcher at Rutgers University, his time at the European Southern Observatory, and his role deriving signs from the Hubble Space Telescope’s aberrated data. Stiavelli discusses his position with the European Space Agency in Baltimore, along with the initial developments of the Next Generation Space Telescope. He also offers his perception on the Space Telescope Science Institute and the scientists working there. He recalls his early involvement with the NGST’s Science Working Group, his role as Project Scientist, and his perspective on the growing schedule and budget delays that led to Congressional hearings. Stiavelli also recalls the impact of the Covid-19 pandemic on the final stages of Webb’s development, the launch, and its current operation. The interview concludes with an overview of Stiavelli’s views on the future of cosmology and the impact of JWST.