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Searchlites Vol SearchLites Vol. 22 No. 4, Autumn 2016 The Quarterly Newsletter of The SETI League, Inc. Offices: 433 Liberty Street Don't Stop the Presses Little Ferry NJ By H. Paul Shuch, Executive Director Emeritus 07643 USA Phone: Every decade or so, the SETI community is treated to a tantalizing (201) 641-1770 (though inconclusive) hint that the existence proof we seek may indeed Facsimile: (201) 641-1771 be within our grasp. Invariably, the popular press seizes upon incom- Email: plete information to increase circulation by prematurely announcing [email protected] Web: our success. In the 1960s, the discovery at CalTech of quasar CTA- www.setileague.org 102 was heralded as proof of extraterrestrial intelligence, until cooler President heads prevailed and the true nature of the source was uncovered. In Richard Factor the 1970s, the Ohio State University “Wow!” signal was similarly ex- Registered Agent: aggerated. In The SETI League’s early days, the EQ Pegasi hoax (fol- Anthony Agnello lowed shortly by the Pearl Harbor Hoax) achieved their fifteen minutes Secretary/Treasurer: A. Heather Wood of fame. Now, we’re at it again with wild speculations about a single presumed detection associated with the star HD 164595. Executive Director Emeritus: H. Paul Shuch, Ph.D. The facts as I understand them are fairly straightforward. About a Trustee: year and a half ago, our Russian colleagues used the RATAN-600 tran- Martin Schreiber, CPA sit radio telescope to conduct a routine RF survey of the regions of the sky surrounding promising Kepler exoplanet locations. Using an ex- Advisory Board: Anthony Agnello tremely broadband receiver at a wavelength of 2.7 cm, their data re- Greg Bear vealed an extremely brief RF peak somewhere between 10.6 and 11.6 Paul Davies, Ph.D. Robert S. Dixon, Ph.D. GHz. No spectral analysis was possible, so no Doppler velocity in- Frank D. Drake, Ph.D. formation could be inferred. The detection never repeated, nor was it Claudio Maccone, Ph.D. Clifford Stoll, Ph.D. duplicated at any other facility. End of story. Last month, publicizing a paper to be presented at the upcoming In- SearchLites, ISSN 1096-5599, ternational Astronautical Congress in Guadalajara, an email to mem- is the Quarterly Newsletter of The SETI League, Inc., a bers of the IAA SETI Committee referred to this possible detection. membership-supported, non- And, before we could say “X-files,” the media was all over it with re- profit [501(c)(3)], educational and scientific corporation, dedi- ports of extraterrestrials discovered just 94 light years away. cated to the electromagnetic So, here is what I know: some sort of X-band radiation entered the Search for Extra-Terrestrial Intelligence. SETI League, Dr. telescope while it was scanning in the general direction of a known SETI, and the above logo are all registered service marks of The exoplanet. That doesn’t mean the signal came from intelligence, or SETI League, Inc. Entire con- even necessarily from that planet; it merely entered the telescope. We tents copyright © 2016 by The SETI League, Inc. Permission get hits like this all the time, and usually trace them to satellite inter- is hereby granted for re- ference, or terrestrial RFI, or nearby microwave ovens or police Dop- production in whole or in part, provided credit is given. All pler radars. They are not SETI detections until either they repeat, or opinions expressed are those they are independently verified as such. No matter what conference of the individual contributors. agendas, article preprints, or the press may tell you. Page 1 SearchLites Volume 22, Number 4 -- Autumn 2016 Guest Editorial roughly U.S. $5 million in investment “interest” in a year—half the current Arecibo budget--which could be used as a creative “match” to attract long-term donors, Arecibo Observatory: corporate “underwriters,” and green/science foundations Translating Ripples in Spacetime into the worldwide. Fabric of a Networked Sustainable Fu- Positioned with an aggressive grant-generating pol- icy with an institutional overhead of 40% and U.S. $12 ture for an Iconic Radio Telescope million in grants (cf. Arecibo’s current NSF/NASA sup- port levels) would yield nearly U.S. $5 million. In short, by William F. Vartorella, Ph.D., C.B.C. an endowment + grants’ institutional overhead + asteroid KJ4ORX, Camden, South Carolina and comet detection and Arecibo Observatory becomes Arecibo, in a very real sense, has spawned a science self-sustaining. And, to take one example, the grants and as revolutionary as Galileo’s first observations with a “contract support” do not strictly have to focus on eso- rudimentary telescope. True to its purpose, it has sensed teric radio astronomy. As an emerging NGO, Arecibo “ripples in spacetime,” those mysterious, posited gravita- could determine access, partners, and help set the agenda tional waves--the Holy Grail of Einstein’s followers-- for broader global imperatives for radio telescopes. Lest that Albert Einstein predicted a century ago in his theory we forget, radio telescopes worldwide are at risk—Green of general relativity. Arecibo Observatory, like space Bank, Very Long Baseline Array, Kitt Peak, Parkes Ra- itself, needs to be flexible. This isn’t about NSF’s inves- dio Telescope (Australia). The need here and what tigation of the “environmental impacts of potential Are- would potentially resonate with global donors is a “flag- cibo futures.” To quote Galileo, “All truths are easy to ship initiative” in which Arecibo becomes the iconic understand once they are discovered; the point is to dis- face of radio astronomy, particularly in the “Global cover them.” While NSF’s universe is one of flattened South.” budgets and “red-shifted” funding disappearing over With more than 100 radio telescopes worldwide that some financial horizon, Arecibo’s real challenge is to are or have been used for radio astronomy, these single develop a new disruptive paradigm that addresses what dishes and interferometric arrays are uniquely positioned scholars call the “cost-curve” of telescopes. U.S. $10 for funding, particularly as the “developing South” agi- million—just less than NSF’s and NASA’s combined tates for greater support, access, and prominence in Big annual funding--is roughly the size and challenge of the Science. “Access” is fundable. Unfortunately, Arecibo is Green Bank Radio Telescope’s annual budget in West “prioritized” below other observatories such as Atacama Virginia, another iconic ‘scope seeking money and part- Large Millimeter/Submillimeter Array. This needs to ners. change. Arecibo is on the National Register of Historic Yet the NASA funding to Arecibo at U.S. $3.7 mil- Places and has potential as an UNESCO World Heritage lion is part of the broader Earth defense of detecting po- Site, particularly as its restrictions on AM, FM, and TV tentially Earth-destroying asteroids and comets. More- transmissions within the four-mile access perimeter have over, Arecibo’s extraordinary facilities spearhead upper effectively prevented intrusive development and nega- atmospheric research and the space environment to help tive impact on the flora and fauna of the nearby forests. us understand Climate Change. Ignoring its search for Arecibo, in a very real sense, is a Sentinel, a canary in distant galaxies, signs of extraterrestrial life, and exo- the coalmine of cosmic research and a guardian of local planets, Arecibo serves as a cosmic oasis for some biodiversity. This underscores the potential for grants 20,000 students who visit it annually in debt-strangled and donors and STEM research (and students and eco- Puerto Rico. Its STEM-related programs are hyper- nomic impact of 100,000 tourists per year). critical as Hispanic students are grossly underrepre- NSF has listed five possible outcomes, ranging from sented in the hard sciences. (See, for example, the Puerto continuing current operations to dismantling the tele- Rico Space Grant Consortium.) The conundrum is that scope and returning the site to its natural state. What we decommissioning Arecibo could cost some U.S. $100 advocate (and propose) here is a more creative approach- million—which is roughly a decade’s worth of current - a “thought experiment.” We need to think through the funding for telescope operations. U.S. $100 million is an consequences. NSF seems to take the position that this is achievable fundraising target for an endowment, particu- Schrödinger’s cat: that Arecibo is indeterminately alive larly if Arecibo severs all ties and becomes a free- or dead. Our thinking here is to quantify the event standing global Nongovernmental Organization (NGO). through live donors, what NSF has detailed as finding An endowment of U.S. $100 million would generate “partners.” They are not Dark Matter. Examples abound Page 2 earch ites Volume 22, Number 4 -- Autumn 2016 S L in the visual universe. Some high-profile, historic venues Competition abounds. Yet, employing a decadal such as the Lowell Observatory have taken dramatic analysis, these corporate donors emerge for “Observato- steps to ensure scientific and public access to new in- ries, Planetariums, Physics, Astronomy”—Fireman’s struments (see, the Discovery Channel Telescope-- Fund Insurance Co., Genentech, Inc., Norton Co., Sedg- DCT—a U.S. $53 million “fusion of research and out- wick, James, Inc., Toshiba America Foundation, Phillips reach”). The Vatican’s Advanced Technology Telescope Petroleum Foundation, Allied Signal, ARCO Chemical, (VATT) outside Tucson, Arizona has a strong “Friends” Barnes Aerospace, Beech Aerospace, Boeing, EG&G component (a model that should be followed by all exist- Aerospace, Grimes Aerospace Foundation, Kaman ing `scopes of varying form and function), which appar- Aerospace Corp. Giving Program, Sundstrand Corp. ently is developing, to borrow the words of Don Keel Aerospace Foundation, and Toyota USA (also active in (co-author of Funding Exploration) a cadre of donors STEM), etc.
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