Searches for Technosignatures: the State of the Profession Jason Wright, Veronica Allen, Julián D
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Adaptive Optics Imaging of Circumstellar Environments
Star Formation at High Angular Resolution IAU Symposium, Vol. 221, 2004 M. G. Burton, R. Jayawardhana & T.L. Bourke, eds. Adaptive Optics Imaging of Circumstellar Environments Daniel Apai, Ilaria Pascucci, Hongchi Wang, Wolfgang Brandner and Thomas Henning Max Planck Institute for Astronomy, Kimiqsiuhl 17., Heidelberg, Germany D-69117 Carol Grady NOAO/STIS, Goddard Space Flight Center, Code 681, NASA/GSFC, Greenbelt, MD 20771, USA Dan Potter Steward Observatory, University of Arizona, 933 N. Cherry Avenue, Tucson, AZ 85721, USA Abstract. We present results from our high-resolution, high-contrast imaging campaign targeting the circumstellar environments of young, nearby stars of different masses. The observations have been conducted using the ALFA/CA 3.5m and NACO UT4/VLT adaptive optics systems. In order to enhance the contrast we applied the methods PSF-subtraction and polarimetric differential imaging (PDI). The observations of young stars yielded the identification of numerous new companion candidates, the most interesting one being rv 0.5" from FU Ori. We also obtained high-resolution near-infrared imaging of the circumstellar envelope of SU Aur and AB Aur. Our PDI of the TW Hya circumstellar disk traced back the disk emission as close as 0.1" ~ 6 AU from the star, the closest yet. Our results demonstrate the potential of the adaptive optics systems in achieving high-resolution and high-contrast imaging and thus in the study of circumstellar disks, envelopes and companions. 1. Introduction Young, nearby stars are our prime source of information to study the circum- stellar disk structure and evolution. They are also the ideal targets for adaptive optics (AO) observations, as they are usually bright enough to provide excellent wavefront reference. -
CURRICULUM VITAE for DANIEL APAI Research Interests: Extrasolar Planets; Planet Formation; Planetary Atmospheres; Astrobiology; Space Telescope Architectures
CURRICULUM VITAE FOR DANIEL APAI Research Interests: Extrasolar Planets; Planet formation; Planetary atmospheres; Astrobiology; Space telescope architectures Professional Appointments 2017 – Associate Professor, Depts. of Astronomy and Planetary Sciences, Univ. of Arizona 2011 – 2017 Assistant Professor, Depts. of Astronomy and Planetary Sciences, Univ. Arizona 2008 – 2011 Assistant Astronomer, Space Telescope Science Institute Education 2004 PhD, University of Heidelberg and Max Planck Institute of Astronomy 2000 MSc in Physics, University of Szeged Recent International Service: Chair, HST–TESS Advisory Committee, Space Telescope Science Institute Science Advisory Committee member, Giant Magellan Telescope Executive Committee member, NASA Exoplanet Program Analysis Group (EXOPAG) Steering Committee member, NASA Nexus for Exoplanet System Science (NExSS) Chair, Exoplanet Science Questions for Direct Imaging Missions, SAG15/EXOPAG Member, Hubble Space Telescope Financial Review Committee Major Approved Programs as Principal Investigator 9 Hubble Space Telescope + 4 Spitzer Space Telescope programs, including: - Extrasolar Storms: Spitzer Exploration Science Program (1,144 Spitzer hour, 24 HST orbits) - Cloud Atlas: Hubble Space Telescope (112 orbits), 12+ refereed papers Earths in Other Solar Systems: $5.7M program (R&A), 45-member team, 140 refereed papers Nautilus: A large-aperture space telescope for a biosignature survey based on diffractive optics, Co-PI of $1.1M Gordon & Betty Moore Foundation grant Advising/Mentoring: Postdoc. Researchers -
Peter Plavchan
Peter Plavchan Assistant Professor of Astronomy Associate Director, George Mason Observatory PI, EarthFinder NASA Mission Concept Study PI, Astrophysics of Exoplanets Instrumentation Lab Co-PI, MINERVA-Australis Department of Physics & Astronomy Office: (703) 903-5893 George Mason University Cell: (626) 234-1628 Planetary Hall 263 Fax: (703) 993-1269 4400 University Dr, MS 3F3 [email protected] Fairfax, VA 22030 http://exo.gmu.edu twitter:@PlavchanPeter Education University of California, Los Angeles, Los Angeles, CA 2001-2006 MS, PhD in Physics California Institute of Technology, Pasadena, CA 1996-2001 BS in Physics, with honor Awards & Honors College of Science Excellence in Mentoring award nomination 2019 College of Natural and Applied Sciences Research Award, MSU 2017 NASA Group Achievement Award 2017 Citation: For the development and tests at Mauna Kea observatories of a near-infrared Laser Frequency Comb as a wavelength standard for the detection and characterization of exoplanets. NASA Honor Achievement Award, NASA Exoplanet Archive Team 2014 Citation: For outstanding achievement in the rapid and on-budget launch of the NASA Exoplanet Archive NASA Honor Achievement Award, Spitzer Science In-Reach Team 2010 Citation: For outstanding support of Spitzer IRAC Warm Instrument Characterization and significant contributions to NASA and JPL commitments to education of the global community. UCLA Physics Division Fellowship 2001-2006 Kobe International School of Planetary Sciences Fellowship 2005 Astronomy Department Outstanding Teaching -
Hubble Space Telescope Primer for Cycle 18
January 2010 Hubble Space Telescope Primer for Cycle 18 An Introduction to HST for Phase I Proposers Space Telescope Science Institute 3700 San Martin Drive Baltimore, Maryland 21218 [email protected] Operated by the Association of Universities for Research in Astronomy, Inc., for the National Aeronautics and Space Administration How to Get Started If you are interested in submitting an HST proposal, then proceed as follows: • Visit the Cycle 18 Announcement Web page: http://www.stsci.edu/hst/proposing/docs/cycle18announce Then continue by following the procedure outlined in the Phase I Roadmap available at: http://apst.stsci.edu/apt/external/help/roadmap1.html More technical documentation, such as that provided in the Instrument Handbooks, can be accessed from: http://www.stsci.edu/hst/HST_overview/documents Where to Get Help • Visit STScI’s Web site at: http://www.stsci.edu • Contact the STScI Help Desk. Either send e-mail to [email protected] or call 1-800-544-8125; from outside the United States and Canada, call [1] 410-338-1082. The HST Primer for Cycle 18 was edited by Francesca R. Boffi, with the technical assistance of Susan Rose and the contributions of many others from STScI, in particular Alessandra Aloisi, Daniel Apai, Todd Boroson, Brett Blacker, Stefano Casertano, Ron Downes, Rodger Doxsey, David Golimowski, Al Holm, Helmut Jenkner, Jason Kalirai, Tony Keyes, Anton Koekemoer, Jerry Kriss, Matt Lallo, Karen Levay, John MacKenty, Jennifer Mack, Aparna Maybhate, Ed Nelan, Sami-Matias Niemi, Cheryl Pavlovsky, Karla Peterson, Larry Petro, Charles Proffitt, Neill Reid, Merle Reinhart, Ken Sembach, Paula Sessa, Nancy Silbermann, Linda Smith, Dave Soderblom, Denise Taylor, Nolan Walborn, Alan Welty, Bill Workman and Jim Younger. -
EOS Newsletter May 2019
PROJECT EOS May 24, 2019 EARTHS IN OTHER SOLAR SYSTEMS Recent Publications On the Mass Function, Multiplicity, and Origins of Wide-Orbit Giant Planets ………………………………. Unlocking CO Depletion in PROJECT EOS Protoplanetary Disks II. Primordial C/H Predictions Inside the CO Snowline ……………………………….. Laboratory evidence for co- condensed oxygen- and carbon-rich meteoritic is part of NASA’s Nexus for stardust from nova outbursts Earths in Other Solar Systems Exoplanetary System Science program, which carries out ……………………………….. coordinated research toward to the goal of searching for and + Line Ratios Reveal N2H determining the frequency of habitable extrasolar planets with Emission Originates above the atmospheric biosignatures in the Solar neighborhood. Midplane in TW Hydrae Our interdisciplinary EOS team includes astrophysicists, ……………………………….. planetary scientists, cosmochemists, material scientists, No Clear, Direct Evidence for chemists and physicists. Multiple Protoplanets The Principal Investigator of EOS is Daniel Apai (University of Orbiting LkCa 15: LkCa 15 Arizona). The project’s lead institutions are The University of bcd are Likely Inner Disk Arizona‘s Steward Observatory and Lunar and Planetary Signals Laboratory. ……………………………….. The EOS Institutional Consortium consists of the Steward The Exoplanet Population Observatory and the Lunar and Planetary Laboratory of the Observation Simulator. II - University of Arizona, the National Optical Astronomy Population Synthesis in the Observatory, the Department of Geophysical Sciences at the Era of Kepler University of Chicago, the Planetary Science Institute, and the Catholic University of Chile. For a complete list of publications, please visit the EOS Library on the SAO/NASA Astrophysics Data System. eos-nexus.org !1 PROJECT EOS May 24, 2019 On the Mass Function, Multiplicity, and Origins of Wide-Orbit Giant Planets Kevin Wagner, Dániel Apai, Kaitlin M. -
EOS Newsletter MARCH 2020
PROJECT EOS March 15, 2020 EARTHS IN OTHER SOLAR SYSTEMS Recent Publications ACCESS: A Visual toNear-infrared Spectrum of the Hot Jupiter WASP-43b with Evidence of H2O, but No Evidence of Na or K ………………………………. Identifying Exo-Earth Candidates in Direct Imaging Data through PROJECT EOS Bayesian Classification ………………………………. Nautilus: A Very Large-Aperture, Ultralight Space Telescope for Exoplanet Exploration, Time- domain Astrophysics, and Faint Objects ………………………………. EPOS: Exoplanet Population Earths in Other Solar Systems is part of NASA’s Nexus for Observation Simulator Exoplanetary System Science program, which carries out ……………………………….. coordinated research toward to the goal of searching for and ACCESS: the Arizona-CfA- determining the frequency of habitable extrasolar planets with Catolica-Carnegie Exoplanet atmospheric biosignatures in the Solar neighborhood. Spectroscopy Survey Our interdisciplinary EOS team includes astrophysicists, ……………………………….. Exoplanet Population Synthesis in planetary scientists, cosmochemists, material scientists, the Era of Large Exoplanets chemists and physicists. Surveys The Principal Investigator of EOS is Daniel Apai (University of ……………………………….. Arizona). The project’s lead institutions are The University of The Sun-like Stars Opportunity ……………………………….. Arizona‘s Steward Observatory and Lunar and Planetary Life Beyond the Solar System: Laboratory. Remotely Detectable The EOS Institutional Consortium consists of the Steward Biosignatures Observatory and the Lunar and Planetary Laboratory of the ……………………………….. Planet formation and migration University of Arizona, the National Optical Astronomy near the silicate sublimation front Observatory, the Department of Geophysical Sciences at the in protoplanetary disks University of Chicago, the Planetary Science Institute, and the ……………………………….. Catholic University of Chile. Search for L5 Earth Trojans with For a complete list of publications, please visit the DECam EOS Library on the SAO/NASA Astrophysics Data System. -
Searching for Intelligent Life in Alien Skies Harry Thomas December 2020 Dr. Sarah Johnson
Atmospheric Technosignatures: Searching for Intelligent Life in Alien Skies Harry Thomas December 2020 Dr. Sarah Johnson (STIA 227: Environmental Geoscience) Introduction In 1950, the famed physicist Enrico Fermi was out to lunch with colleagues when he asked, “Do you ever wonder where everybody is?” The Fermi Paradox has come to describe the disparity between the abundance of star systems, with a multitude of planets that might harbor 1 life, and the lack of detectable alien civilizations. This question, rooted in a deeper existential curiosity about our place in the cosmos, has fueled researchers to search for signs of alien intelligence. So far, none have been detected. Since 1992, over 4000 planets have been found orbiting stars outside of the solar system. Some of these planets, known as exoplanets, are similar to Earth in terms of their composition 2 and the amount of radiation they receive from their host star. The search for extraterrestrial intelligence has largely revolved around the search for alien radio transmissions, but there is a growing contingent of scientists who argue that we should be searching for other indicators of alien civilizations. Some of the most promising of these indicators, better known as technosignatures, can be found in the skies and orbits of exoplanets. Technosignatures Technosignature is a broad term that can be applied to anything that indicates the presence of a technologically developed civilization. Its list of engendering technologies runs the gamut from ones that are well within the grasp of human technological reality to ones that stretch the limits of imagination; both the burning of chemical fuels and Dyson Spheres, massive arrays of solar collectors that enclose an entire star to capture as much of its energy as possible, are fair 3 game for technosignatures. -
Characterizing Planets with Direct Imaging
Characterizing Planets with Direct Imaging Victoria Meadows and the NAI Virtual Planetary Laboratory Team The University of Washington, California Institute of Technology, Jet Propulsion Laboratory, Pennsylvania State University, NASA Goddard Space Flight Center, University of Maryland, NASA Goddard Institute for Space Studies, University of Chicago, Weber State University, Adler Planetarium, NASA Ames Research Center, Stanford University, Rice University, Washington University at Saint Louis, Yale University, Australian Center for Astrobiology, University of Victoria, Laboratoire d’Astrophysique – Bordeaux The NAI’s Virtual Planetary Laboratory Our Challenge Direct Imaging • Must suppress the light from the parent star so that the light from the smaller, fainter planet can be seen - at least 10-9 for Jupiter detection and 10-11 for Earth spectroscopy. • Suppression techniques (e.g. coronography, interferometry) have inner and outer working angles that are ~2λ/D, where D = telescope diameter. • The larger the telescope, or the shorter the wavelength, the closer in to the star we can see. Direct Imaging • Must also resolve planet and star as two separate images • Angular resolution θ = 1.22 λ/D, • Angular resolution improves with larger telescopes, shorter λ Except…for external occulters …where inner working angle is a function of starshade diameter and distance from the telescope Direct Imaging. It’s Hard. Why bother? Doppler Vel. Transit Imaging Eclipse Timing Microlensing Kepler 40 20 Jupiter ] 10 e 4 Neptune Planet Radius [R 1 Earth Radius RelativeEarth to 2013 1 10 100 1000 10000 100000 OrbitalOrbital Period Period [days]in days J. Fortney Direct Imaging. It’s hard. Why bother? Aerosols can severely limit the altitude Depending on observing geometry probed by transit spectra, hiding much of refraction also limits altitudes probed and the atmosphere from study. -
A New Lens for Life-Searching Space Telescopes 5 August 2019
A new lens for life-searching space telescopes 5 August 2019 Apai leads the space science half of the team, while UA professor Tom Milster, of the James C. Wyant College of Optical Sciences, leads the optical design of a replicable space telescope dubbed Nautilus. The researchers intend to deploy a fleet of 35 14-meter-wide spherical telescopes, each individually more powerful than the Hubble Space Telescope. Each unit will contain a meticulously crafted 8.5-meter diameter lens, which will be used for astronomical observations. One use particularly exciting for Apai is analyzing starlight as it filters University of Arizona researchers have designed a fleet through planetary atmospheres, a technique which of 35 powerful space telescopes that will search for the could reveal chemical signatures of life. chemical signatures of life on other worlds. Credit: Nautilus team When combined, the telescope array will be powerful enough to characterize 1,000 extrasolar planets from as far away as 1,000 light years. Even The University of Arizona Richard F. Caris Mirror NASA's most ambitious space telescope missions Laboratory is a world leader in the production of are designed to study a handful of potentially Earth- the world's largest telescope mirrors. In fact, it is like extrasolar planets. currently fabricating mirrors for the largest and most advanced earth-based telescope: The Giant "Such a sample may be too small to truly Magellan Telescope. understand the complexity of exo-earths," according to Apai and Milster's co-authored paper, But there are size constraints, ranging from the which was published July 29 in the Astronomical mirror's own weight, which can distort images, to Journal along with several other authors, including the size of our freeways and underpasses that are Steward Observatory astronomer Glenn Schneider needed to transport finished pieces. -
ASTRONOMY 475/575 – Planetary Astrobiology Spring 2019 Class
ASTRONOMY 475/575 – Planetary Astrobiology Spring 2019 Class meets: T/Th 2:00 pm - 3:15 pm Classroom: Steward Observatory Room 204 Instructors: Dr. Daniel Apai, Dr. Josh Eisner Office: Steward Observatory Rooms N208B and N414 Phone: 621-6534, 626-7645 Email: [email protected] [email protected] Office Hrs: By appointment or whenever the door is open Course Desciption This course will explore the processes related to planet formation, the properties of planets and the planetary conditions required for the emergence of life. We will study the formation of our Solar System and exoplanetary systems, the distribution and properties of exoplanets, and the potential habitability of other planets/moons in our system or extrasolar systems. The course will also review science cases and possible future astrobiology studies, both in situ and via remote sensing, of astrobiologically relevant environments. Toward the end of the semester a few guest lectures will highlight particularly exciting and timely topics. Textbook and Readings There is no required book for this course. For those who would like some additional reading material, we recommend “Planetary Science” by Lissauer and de Pater, and “Earth” by Lunine. Copies should be available in the campus bookstore. Draft lecture notes will be made available on the course website. Some topics are beyond the scope of these sources, and we will draw from journal articles and other sources in these cases. We will also assign several journal ariticles as required reading. Lectures The classes will be devoted to lectures. Professor Eisner will lecture for the first 6 weeks or so, and then Professor Apai will lecture for about 6 weeks. -
Remotely Detectable Biosignatures
Astro2020 Science White Paper Life Beyond the Solar System: Remotely Detectable Biosignatures Thematic Areas: Planetary Systems Star and Planet Formation Formation and Evolution of Compact Objects Cosmology and Fundamental Physics Stars and Stellar Evolution Resolved Stellar Populations and their Environments Galaxy Evolution Multi-Messenger Astronomy and Astrophysics Principal Author: Name: Shawn D. Domagal-Goldman Institution: NASA Goddard Space Flight Center Email: [email protected] Phone: 301-614-6425 Co-leads: Nancy Y. Kiang, NASA Goddard Institute for Space Studies Niki Parenteau, NASA Ames Research Center Co-authors, including co-authors for prior white paper submissions: Daniel Angerhausen, Center for Space and Habitability and Bern University Daniel Apai, Uniersity of Arizona Giada Arney, NASA Goddard Space Flight Center, Vladimir S. Airapetian, NASA Goddard Space Flight Center, American University Natalie M. Batalha, NASA Ames Reseach Center David L. Blank, University of Southern Queensland David C. Catling, University of Washington Charles S. Cockell, UK Centre for Astrobiology and University of Edinburgh Leroy Cronin, University of Glasgow Sebastian O. Danielache Sophia University Priya DasSarma, Institute of Marine and Environmental Technology, University of Maryland - Baltimore Russell Deitrick, University of Washington Anthony Del Genio, NASA Goddard Institute for Space Studies Cecilia Demergasso, Biotechnology Center, Universidad Catolica´ del Norte Kai Finster, Aarhus University Theresa Fisher, Arizona State -
The Search for Life As We (Don't) Know It
THE SEARCH FOR LIFE AS WE (DON’T) KNOW IT Credit: Scientific American , Vol. 298, No. 4 (April 2008), pp. 48-55 [email protected] Janusz J. Petkowski, MIT What is Astrobiology? Astrobiology: interdisciplinary scientific field concerned with the origins, early evolution, distribution, and future of life in the universe. Astrobiology considers the question of whether extraterrestrial life exists, and if it does, how humans can detect it. Where do we even start? Let’s find (habitable) planets first! Modified from Meadows, Barnes AbSciCon 2015 Credit: Sara Seager Transiting Planets Earth radius 6.4 x 103 km Sun radius 6.9 x 105 km Size ratio ~1/100 Area ratio ~1/10000 Animation credit: NASA Credit: Sara Seager Earth is 100 times smaller 300,000 times less massive 10,000,000,000 times fainter ? than the sun Habitable world: a planet that is about Earth size, receives about the same amount of energy from its star that Earth does from the Sun, and has liquid water Credit: Sara Seager Earth/ Planet-star area ratio ~1/100 Atmosphere to star ~1/10,000 Earth/Sun Planet-star area ratio ~1/10,000 Atmosphere to star ~1/50,000,000 Credit: Sara Seager Planet Detection J Exoplanets are diverse with a range of planet size, mass, and orbits N The discovery of Earth twin planets is not yet in reach Not shown is that planet mass E and size give average density and a clue to planet bulk composition 0.01 0.1 Credit: A. Romero-Wolf Credit: Sara Seager Planet Detection Exoplanets are diverse with a range of planet size, mass, and orbits Venus and Earth would look the same to any planet- finding technique Atmosphere studies are key 0.01 0.1 Credit: A.