Sallie L. Baliunas | |
---|---|
Born | New York City, United States | February 23, 1953
Nationality | American |
Alma mater | Villanova University, Harvard University |
Awards | Bok Prize (1988), Newton Lacy Pierce Prize in Astronomy (1988) |
Scientific career | |
Fields | Astrophysics |
Institutions | Mount Wilson Observatory, Center for Astrophysics | Harvard & Smithsonian |
Thesis | Optical and ultraviolet studies of stellar chromospheres of Lambda Andromedae and other late-type stars (1980) |
Doctoral advisor | Andrea Dupree |
Sallie Louise Baliunas (born February 23, 1953) [1] is a retired astrophysicist. She formerly worked at the Center for Astrophysics | Harvard & Smithsonian and was the Deputy Director of the Mount Wilson Observatory from 1991 to 2003.
Baliunas was born and grew up in New York City and its suburbs. She attended public schools in the New York City area and high school in New Jersey. [2] She received a BS in astrophysics from Villanova University in 1974, [3] and an AM and a PhD in astrophysics from Harvard University in 1975 and 1980. [2] [4] [5] Her doctoral thesis was titled, Optical and ultraviolet studies of stellar chromospheres of Lambda Andromedae and other late-type stars. [6]
Baliunas was a research associate of the Harvard College Observatory in 1980 and became an astrophysicist in the Smithsonian Astrophysical Observatory at the Center for Astrophysics | Harvard & Smithsonian in 1989. [4]
Baliunas was also a visiting scholar at Dartmouth College, an adjunct professor at Tennessee State University, and was deputy director of the Mount Wilson Observatory from 1991 to 2003. [4] [7]
She has been a member of the American Astronomical Society, American Geophysical Union, American Physical Society, Astronomical Society of the Pacific, International Astronomical Union, and Sigma XI. [4]
She served on both the scientific advisory board [4] and the board of directors of the Marshall Institute, [8] a now defunct conservative think tank.
Baliunas's main focus was initially on astrophysical research. [9] She studied visible and ultraviolet spectroscopy of stars; structure, variations, and activity in cool stars; evolution of stellar angular momentum; solar variability and global change; adaptive optics; exoplanets of Sun-like stars. She has published little in recent years, with only two refereed astronomy papers since 2010.
In 1992, Baliunas was third author on a Nature paper [10] that used observed variations in sun-like stars as an analogue of possible past variations in the Sun. The paper says that
By 1995, she had entered the global warming controversy. In January of that year the Marshall Institute think tank published a review she had written for them, "Are Human Activities Causing Global Warming?" disputing the IPCC Second Assessment Report and arguing that "predictions of an anthropogenic global warming have been greatly exaggerated, and that the human contribution to global warming over the course of the 21st century will be less than one degree Celsius and probably only a few tenths of a degree." She concluded with the view that "even if fears of anthropogenic global warming were realized – a concern which finds no support in the scientific data – there is no significant penalty for waiting at least two decades before taking corrective action to reduce global CO2 emissions." [11] The work of Willie Soon and Baliunas, suggesting that solar variability is more strongly correlated with variations in air temperature than any other factor, even carbon dioxide levels, has been widely publicized by lobby groups including the Marshall Institute [12] and Tech Central Station, [13] and mentioned in the popular press. [14] Baliunas and Soon became well known for climate change denial, and in 1997 she won the Petr Beckmann Award for her "devastating critique of the global warming hoax." [15]
In regard to there being a connection between CO2 rise and climate change, she said in a 2001 essay with Willie Soon:
The claim that atmospheric data showed no warming trend was incorrect, as the published satellite and balloon data at that time already showed a warming trend (see satellite temperature record). In later statements Baliunas acknowledged the measured warming in the satellite and balloon records, though she disputed that the observed warming reflected human influence. [17]
Baliunas contends that findings of human influence on climate change are motivated by financial considerations: "If scientists and researchers were coming out releasing reports that global warming has little to do with man, and most to do with just how the planet works, there wouldn't be as much money to study it." [18] [19] She does not address the countervailing financial considerations of the energy companies that fund some of her collaborators, including Willie Soon who received over $1 million from petroleum and coal interests since 2001. [20]
In 2003, Baliunas and aerospace engineer Willie Soon published a review paper on historical climatology in Climate Research , which concluded that "the 20th century is probably not the warmest nor a uniquely extreme climatic period of the last millennium." With Soon, Baliunas investigated the correlation between solar variability and temperatures of the Earth's atmosphere. When there are more sunspots, the total solar output increases, and when there are fewer sunspots, it decreases. Soon and Baliunas attribute the Medieval warm period to such an increase in solar output, and believe that decreases in solar output led to the Little Ice Age, a period of cooling from which the earth has been recovering since 1890. [21]
The circumstances of the paper's publication were controversial, prompting concerns about the publishers' peer review process. An editorial revolt within Climate Research followed, with half of the journal's ten editors eventually resigning. The publisher subsequently stated that critics said that the conclusions of the paper "cannot be concluded convincingly from the evidence provided" and that the journal "should have requested appropriate revisions prior to publication." [22]
In 1995, Baliunas testified before the United States House Science Subcommittee on Energy and Environment that CFCs were not responsible for ozone depletion. [23] An article written by Baliunas and Soon in 2000 for the Heartland Institute, a conservative and libertarian public policy think tank, promoted the idea that ozone depletion rather than CO2 emissions could explain atmospheric warming. [24]
Upsilon Andromedae is a binary star located 44 light-years from Earth in the constellation of Andromeda. The system consists of an F-type main-sequence star and a smaller red dwarf.
51 Pegasi, formally named Helvetios, is a Sun-like star located 50.6 light-years from Earth in the constellation of Pegasus. It was the first main-sequence star found to have an exoplanet orbiting it.
The Global Warming Petition Project, also known as the Oregon Petition, is a group which urges the United States government to reject the Kyoto Protocol of 1997 and similar policies. Their petition challenges the scientific consensus on climate change. Though the group claims more than thirty-thousand signatories across various scientific fields, the authenticity and methods of the petitioners as well as the signatories' credentials have been questioned, and the project has been characterized as a disinformation campaign engaged in climate change denial.
Willie Wei-Hock Soon is a Malaysian astrophysicist and aerospace engineer who was long employed as a part-time externally funded researcher at the Solar and Stellar Physics (SSP) Division of the Center for Astrophysics | Harvard & Smithsonian.
36 Ophiuchi is a triple star system 19.5 light-years from Earth. It is in the constellation Ophiuchus.
The George C. Marshall Institute (GMI) was a nonprofit conservative think tank in the United States. It was established in 1984 with a focus on science and public policy issues and had an initial focus in defense policy. Starting in the late 1980s, the institute advocated for views in line with environmental skepticism, most notably climate change denial. The think tank received extensive financial support from the fossil fuel industry.
The Smithsonian Astrophysical Observatory (SAO) is a research institute of the Smithsonian Institution, concentrating on astrophysical studies including galactic and extragalactic astronomy, cosmology, solar, earth and planetary sciences, theory and instrumentation, using observations at wavelengths from the highest energy gamma rays to the radio, along with gravitational waves. Established in Washington, D.C., in 1890, the SAO moved its headquarters in 1955 to Cambridge, Massachusetts, where its research is a collaboration with the Harvard College Observatory (HCO) and the Harvard University Department of Astronomy. In 1973, the Smithsonian and Harvard formalized the collaboration as the Center for Astrophysics | Harvard & Smithsonian (CfA) under a single Director.
The Center for Astrophysics | Harvard & Smithsonian (CfA), previously known as the Harvard–Smithsonian Center for Astrophysics, is an astrophysics research institute jointly operated by the Harvard College Observatory and Smithsonian Astrophysical Observatory. Founded in 1973 and headquartered in Cambridge, Massachusetts, United States, the CfA leads a broad program of research in astronomy, astrophysics, Earth and space sciences, as well as science education. The CfA either leads or participates in the development and operations of more than fifteen ground- and space-based astronomical research observatories across the electromagnetic spectrum, including the forthcoming Giant Magellan Telescope (GMT) and the Chandra X-ray Observatory, one of NASA's Great Observatories.
Rho Coronae Borealis is a yellow dwarf star 57.1 light-years away in the constellation of Corona Borealis. The star is thought to be similar to the Sun with nearly the same mass, radius, and luminosity. It is orbited by four known exoplanets.
Delta Trianguli, Latinized from Delta Tri, is a spectroscopic binary star system approximately 35 light-years (11 pc) away in the constellation of Triangulum. The primary star is a yellow dwarf, while the secondary star is thought to be an orange dwarf. It has an apparent magnitude of +4.87 and forms an optical (line-of-sight) triple with Gamma Trianguli and 7 Trianguli.
Iota Andromedae is a single star in the northern constellation of Andromeda. It has the Flamsteed designation 17 Andromedae, while Iota Andromedae is the Bayer designation as Latinized from ι Andromedae. This object is visible to the naked eye at night as a faint, blue-white hued star with an apparent visual magnitude of +4.29. Based upon parallax measurements, it is located approximately 500 light years distant from the Sun.
Beta Comae Berenices is a main sequence dwarf star in the northern constellation of Coma Berenices. It is located at a distance of about 29.95 light-years from Earth. The Greek letter beta (β) usually indicates that the star has the second highest visual magnitude in the constellation. However, with an apparent visual magnitude of 4.3, this star is actually slightly brighter than α Comae Berenices. It can be seen with the naked eye, but may be too dim to be viewed from a built-up urban area.
Upsilon Andromedae c, formally named Samh, is an extrasolar planet orbiting the Sun-like star Upsilon Andromedae A every 241.3 days at an average distance of 0.83 AU. Its discovery in April 1999 by Geoffrey Marcy and R. Paul Butler made this the first multiple-planet system to be discovered around a main-sequence star, and the first multiple-planet system known in a multiple star system. Upsilon Andromedae c is the second-known planet in order of distance from its star.
Upsilon Andromedae d, formally named Majriti, is a super-Jupiter exoplanet orbiting within the habitable zone of the Sun-like star Upsilon Andromedae A, approximately 44 light-years away from Earth in the constellation of Andromeda. Its discovery made it the first multiplanetary system to be discovered around a main-sequence star, and the first such system known in a multiple star system. The exoplanet was found by using the radial velocity method, where periodic Doppler shifts of spectral lines of the host star suggest an orbiting object.
Friends of Science(FoS) is a non-profit advocacy organization based in Calgary, Alberta, Canada. The organization rejects the established scientific consensus that humans are largely responsible for the currently observed global warming. Rather, they propose that "the Sun is the main direct and indirect driver of climate change," not human activity. They argued against the Kyoto Protocol. The society was founded in 2002 and launched its website in October of that year. They are largely funded by the fossil fuel industry.
12 Ophiuchi is a variable star in the constellation Ophiuchus. No companions have yet been detected in orbit around this star, and it remains uncertain whether or not it possesses a dust ring.
Christopher Rhodes de Freitas was a New Zealand climate scientist. He was an associate professor in the School of Environment at the University of Auckland.
Sami Khan Solanki is director of the Max Planck Institute for Solar System Research (MPS), director of the Sun-Heliosphere Department of MPS, a scientific member of the Max Planck Society, and a Chair of the International Max Planck Research School on Physical Processes in the Solar System and Beyond at the Universities of Braunschweig and Göttingen.
The Soon and Baliunas controversy involved the publication in 2003 of a review study written by the aerospace engineer Willie Soon and astronomer Sallie Baliunas in the journal Climate Research. In the review, the authors expressed disagreement with the hockey stick graph and argued that historical temperature changes were related to solar variation rather than greenhouse gas emissions as was the position of the Intergovernmental Panel on Climate Change and other researchers. The publication was quickly taken up by the George W. Bush administration as a basis for amending the first Environmental Protection Agency's Report on the Environment.
Andrea Dupree is a senior astrophysicist at the Center for Astrophysics | Harvard & Smithsonian. She is a Past-President of the American Astronomical Society, and served as the associate director of the Center for Astrophysics | Harvard & Smithsonian. Dupree also served as Head of the Solar, Stellar and Planetary Sciences Division.