2020 Science Gap List
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The Discovery of Exoplanets
L'Univers, S´eminairePoincar´eXX (2015) 113 { 137 S´eminairePoincar´e New Worlds Ahead: The Discovery of Exoplanets Arnaud Cassan Universit´ePierre et Marie Curie Institut d'Astrophysique de Paris 98bis boulevard Arago 75014 Paris, France Abstract. Exoplanets are planets orbiting stars other than the Sun. In 1995, the discovery of the first exoplanet orbiting a solar-type star paved the way to an exoplanet detection rush, which revealed an astonishing diversity of possible worlds. These detections led us to completely renew planet formation and evolu- tion theories. Several detection techniques have revealed a wealth of surprising properties characterizing exoplanets that are not found in our own planetary system. After two decades of exoplanet search, these new worlds are found to be ubiquitous throughout the Milky Way. A positive sign that life has developed elsewhere than on Earth? 1 The Solar system paradigm: the end of certainties Looking at the Solar system, striking facts appear clearly: all seven planets orbit in the same plane (the ecliptic), all have almost circular orbits, the Sun rotation is perpendicular to this plane, and the direction of the Sun rotation is the same as the planets revolution around the Sun. These observations gave birth to the Solar nebula theory, which was proposed by Kant and Laplace more that two hundred years ago, but, although correct, it has been for decades the subject of many debates. In this theory, the Solar system was formed by the collapse of an approximately spheric giant interstellar cloud of gas and dust, which eventually flattened in the plane perpendicular to its initial rotation axis. -
Modeling Super-Earth Atmospheres in Preparation for Upcoming Extremely Large Telescopes
Modeling Super-Earth Atmospheres In Preparation for Upcoming Extremely Large Telescopes Maggie Thompson1 Jonathan Fortney1, Andy Skemer1, Tyler Robinson2, Theodora Karalidi1, Steph Sallum1 1University of California, Santa Cruz, CA; 2Northern Arizona University, Flagstaff, AZ ExoPAG 19 January 6, 2019 Seattle, Washington Image Credit: NASA Ames/JPL-Caltech/T. Pyle Roadmap Research Goals & Current Atmosphere Modeling Selecting Super-Earths for State of Super-Earth Tool (Past & Present) Follow-Up Observations Detection Preliminary Assessment of Future Observatories for Conclusions & Upcoming Instruments’ Super-Earths Future Work Capabilities for Super-Earths M. Thompson — ExoPAG 19 01/06/19 Research Goals • Extend previous modeling tool to simulate super-Earth planet atmospheres around M, K and G stars • Apply modified code to explore the parameter space of actual and synthetic super-Earths to select most suitable set of confirmed exoplanets for follow-up observations with JWST and next-generation ground-based telescopes • Inform the design of advanced instruments such as the Planetary Systems Imager (PSI), a proposed second-generation instrument for TMT/GMT M. Thompson — ExoPAG 19 01/06/19 Current State of Super-Earth Detections (1) Neptune Mass Range of Interest Earth Data from NASA Exoplanet Archive M. Thompson — ExoPAG 19 01/06/19 Current State of Super-Earth Detections (2) A Approximate Habitable Zone Host Star Spectral Type F G K M Data from NASA Exoplanet Archive M. Thompson — ExoPAG 19 01/06/19 Atmosphere Modeling Tool Evolution of Atmosphere Model • Solar System Planets & Moons ~ 1980’s (e.g., McKay et al. 1989) • Brown Dwarfs ~ 2000’s (e.g., Burrows et al. 2001) • Hot Jupiters & Other Giant Exoplanets ~ 2000’s (e.g., Fortney et al. -
PEAS: the PLANET AS EXOPLANET ANALOG SPECTROGRAPH. E. C. Martin1 and A
Exoplanets in our Backyard 2020 (LPI Contrib. No. 2195) 3006.pdf PEAS: THE PLANET AS EXOPLANET ANALOG SPECTROGRAPH. E. C. Martin1 and A. J. Skemer1, 1Department of Astronomy & Astrophysics, University of California, Santa Cruz, CA ([email protected]) Introduction: Exoplanets are abundant in our Galaxy • Produce 2D surface maps of Venus, Mars, Jupi- and yet characterizing them remains a technical chal- ter, Saturn, Uranus, Neptune lenGe. Solar System planets provide an opportunity to • Produce fiducial measurements that will be used test the practical limitations of exoplanet observations to plan instruments for future exoplanet mis- with hiGh siGnal-to-noise data, and ancillary data (such sions, such as HabEx/LUVOIR and TMT. as 2D maps and in situ measurements) that we cannot Long term: access for exoplanets. However, data on Solar System • Time-series observations of Solar System plan- planets differ from exoplanets in that Solar System ets to explore variability and weather patterns planets are spatially resolved while exoplanets are all on planets unresolved point-sources. • Comparison to historical data (e.g. [4]) There have been several recent efforts to validate techniques for interpreting exoplanet observations by • Study planetary seismoloGy (oscillation modes) binning images of Solar System planets to a single of Solar System planets pixel: For example, Cowan et al. [1] used images from the EPOXI mission to study Earth’s Globally averaGed PEAS Instrument Design Planetary light collect- properties as it rotated; MayorGa et al. [2] used data ed by the telescope will be split into a spectroGraph from the Cassini spacecraft’s fly-by of Jupiter to ob- system and an imaGinG system for simultaneous obser- serve Globally averaGed reflected liGht phase curves; vations. -
Arxiv:2007.10995V1
Draft version July 23, 2020 Typeset using LATEX twocolumn style in AASTeX63 Transits of Known Planets Orbiting a Naked-Eye Star Stephen R. Kane,1 Selc¸uk Yalc¸ınkaya,2 Hugh P. Osborn,3,4,5 Paul A. Dalba,1, ∗ Louise D. Nielsen,6 Andrew Vanderburg,7, † Teo Mocnikˇ ,1 Natalie R. Hinkel,8 Colby Ostberg,1 Ekrem Murat Esmer,9 Stephane´ Udry,6 Tara Fetherolf,1 Ozg¨ ur¨ Bas¸turk¨ ,9 George R. Ricker,4 Roland Vanderspek,4 David W. Latham,10 Sara Seager,4,11,12 Joshua N. Winn,13 Jon M. Jenkins,14 Romain Allart,6 Jeremy Bailey,15 Jacob L. Bean,16 Francois Bouchy,6 R. Paul Butler,17 Tiago L. Campante,18,19 Brad D. Carter,20 Tansu Daylan,4, ‡ Magali Deleuil,3 Rodrigo F. Diaz,21 Xavier Dumusque,6 David Ehrenreich,6 Jonathan Horner,20 Andrew W. Howard,22 Howard Isaacson,23,20 Hugh R.A. Jones,24 Martti H. Kristiansen,25,26 Christophe Lovis,6 Geoffrey W. Marcy,23 Maxime Marmier,6 Simon J. O’Toole,27,28 Francesco Pepe,6 Darin Ragozzine,29 Damien Segransan,´ 6 C.G. Tinney,30 Margaret C. Turnbull,31 Robert A. Wittenmyer,20 Duncan J. Wright,20 and Jason T. Wright32 1Department of Earth and Planetary Sciences, University of California, Riverside, CA 92521, USA 2Ankara University, Graduate School of Natural and Applied Sciences, Department of Astronomy and Space Sciences, Tandogan, TR-06100, Turkey 3Aix-Marseille Universit, CNRS, CNES, Laboratoire d’Astrophysique de Marseille, France 4Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA 5NCCR/PlanetS, Centre for Space & Habitability, University of Bern, Bern, Switzerland 6Observatoire de Gen`eve, Universit´ede Gen`eve, 51 ch. -
The Exoplanet Revolution
FEATURES THE EXOPLANET REVOLUTION l Yamila Miguel – Leiden Observatory, Leiden, The Netherlands – DOI: https://doi.org/10.1051/epn/2019506 Hot Jupiters, super-Earths, lava-worlds and the search for life beyond our solar system: the exoplanet revolution started almost 30 years ago and is now taking off. re there other planets like the Earth out discovered the astonishing number of 4000 exoplanets, there? This is probably one of the oldest and counting. Every new discovery shows an amazing questions of humanity. For centuries and diversity that impacts in the perception and understand- Auntil the 90s, we only knew of the existence ing of our own solar system. of 8 planets. But today we live in a privileged time. For the first time in history we know that there are other How to find exoplanets? planets orbiting distant stars. Finding exoplanets is an extremely difficult task. These The first planet orbiting a star similar to the Sun was planets shine mostly due to the reflection of the stellar . Artist’s impression discovered in 1995 -only 24 years ago- and it started light in their atmospheres and their light is incredibly of COROT-7b. a revolution in Astronomy. Today astronomers have weak compared to that of their host stars. For this reason, © ESO/L. Calçada EPN 50/5&6 41 FEATURES THE Exoplanet REVolution observing exoplanets directly is extremely difficult and allows astronomers to calculate the planet’s density, astronomers had to develop indirect techniques that infer important to start assessing planetary compositions the presence of the planet. and diversity. Two of the most successful techniques to discov- er exoplanets are the "Transits" and "Radial Veloci- The Exoplanet Zoo ties" techniques. -
Pre-Vetted False Positives for TESS
Swarthmore College Works Physics & Astronomy Faculty Works Physics & Astronomy 11-1-2018 The KELT Follow-Up Network And Transit False-Positive Catalog: Pre-Vetted False Positives For TESS K. A. Collins K. I. Collins FJ.ollow Pepper this and additional works at: https://works.swarthmore.edu/fac-physics J. Labadie-Bar Part of the Astrtz ophysics and Astronomy Commons Let us know how access to these works benefits ouy K. G. Stassun See next page for additional authors Recommended Citation K. A. Collins, K. I. Collins, J. Pepper, J. Labadie-Bartz, K. G. Stassun, B. S. Gaudi, D. Bayliss, J. Bento, K. D. Colón, D. Feliz, D. James, M. C. Johnson, R. B. Kuhn, M. B. Lund, M. T. Penny, J. E. Rodriguez, R. J. Siverd, D. J. Stevens, X. Yao, G. Zhou, M. Akshay, G. F. Aldi, C. Ashcraft, S. Awiphan, Ö. Baştürk, D. Baker, T. G. Beatty, P. Benni, P. Berlind, G. B. Berriman, Z. Berta-Thompson, A. Bieryla, V. Bozza, S. C. Novati, M. L. Calkins, J. M. Cann, D. R. Ciardi, W. D. Cochran, David H. Cohen, D. Conti, J. R. Crepp, I. A. Curtis, G. D'Ago, K. A. Diazeguigure, C. D. Dressing, F. Dubois, E. Ellington, T. G. Ellis, G. A. Esquerdo, P. Evans, A. Friedli, A. Fukui, B. J. Fulton, E. J. Gonzales, J. C. Good, J. Gregorio, T. Gumusayak, D. A. Hancock, C. K. Harada, R. Hart, E. G. Hintz, H. Jang-Condell, E. J. Jeffery, Eric L.N. Jensen, E. Jofré, M. D. Joner, A. Kar, D. H. Kasper, B. Keten, J. -
Exploring Exoplanet Populations with NASA's Kepler Mission
SPECIAL FEATURE: PERSPECTIVE PERSPECTIVE SPECIAL FEATURE: Exploring exoplanet populations with NASA’s Kepler Mission Natalie M. Batalha1 National Aeronautics and Space Administration Ames Research Center, Moffett Field, 94035 CA Edited by Adam S. Burrows, Princeton University, Princeton, NJ, and accepted by the Editorial Board June 3, 2014 (received for review January 15, 2014) The Kepler Mission is exploring the diversity of planets and planetary systems. Its legacy will be a catalog of discoveries sufficient for computing planet occurrence rates as a function of size, orbital period, star type, and insolation flux.The mission has made significant progress toward achieving that goal. Over 3,500 transiting exoplanets have been identified from the analysis of the first 3 y of data, 100 planets of which are in the habitable zone. The catalog has a high reliability rate (85–90% averaged over the period/radius plane), which is improving as follow-up observations continue. Dynamical (e.g., velocimetry and transit timing) and statistical methods have confirmed and characterized hundreds of planets over a large range of sizes and compositions for both single- and multiple-star systems. Population studies suggest that planets abound in our galaxy and that small planets are particularly frequent. Here, I report on the progress Kepler has made measuring the prevalence of exoplanets orbiting within one astronomical unit of their host stars in support of the National Aeronautics and Space Admin- istration’s long-term goal of finding habitable environments beyond the solar system. planet detection | transit photometry Searching for evidence of life beyond Earth is the Sun would produce an 84-ppm signal Translating Kepler’s discovery catalog into one of the primary goals of science agencies lasting ∼13 h. -
Another Earth in the Universe
Home / Space/ Special reports Another Earth in the Universe A world similar to the Earth Finally the news we were waiting for, for so long, has arrived. It was only a matter of time. NASA’s Kepler Telescope, has discovered the first Earth-sized extrasolar planet, orbiting in the habitable zone, a region around a star where water in the liquid state can be found. Artist’s concept of Kepler-186f, the exoplanet similar to the Earth discovered with NASA’s Kepler telescope. Credits: Wikipedia The Earth’s “cousin” planet is called Kepler-186f, it is about 500 light years from the Earth, in the constellation of Cygnus. It has been called Kepler-186f because it was discovered with the Kepler telescope, rotating around the star Kepler-186 and is part of a system of five planets (Kepler-186b, Kepler-186c, Kepler-186d, Kepler-186e and Kepler-186f). The Kepler satellite had already discovered various planets orbiting in the habitable zone, however they were all larger, at least 40% larger than the Earth. Image of the planetary system of Kepler-186, which consists of five planets orbiting around the star, Kepler-186. The first four planets have an orbital period of 4,7, 13 and 22 days respectively and are all too hot for life to exist. Kepler-186f has an orbital period of 130 days. Credits: NASA Home / Space/ Special reports The planet system of Kepler-186 instead, consists of five planets; four inner planets, smaller than half our planet, and Kepler-186f, approximately 40% larger than the Earth. -
Exoplanet Community Report
JPL Publication 09‐3 Exoplanet Community Report Edited by: P. R. Lawson, W. A. Traub and S. C. Unwin National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology Pasadena, California March 2009 The work described in this publication was performed at a number of organizations, including the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (NASA). Publication was provided by the Jet Propulsion Laboratory. Compiling and publication support was provided by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not constitute or imply its endorsement by the United States Government, or the Jet Propulsion Laboratory, California Institute of Technology. © 2009. All rights reserved. The exoplanet community’s top priority is that a line of probeclass missions for exoplanets be established, leading to a flagship mission at the earliest opportunity. iii Contents 1 EXECUTIVE SUMMARY.................................................................................................................. 1 1.1 INTRODUCTION...............................................................................................................................................1 1.2 EXOPLANET FORUM 2008: THE PROCESS OF CONSENSUS BEGINS.....................................................2 -
Exoplanet Exploration Collaboration Initiative TP Exoplanets Final Report
EXO Exoplanet Exploration Collaboration Initiative TP Exoplanets Final Report Ca Ca Ca H Ca Fe Fe Fe H Fe Mg Fe Na O2 H O2 The cover shows the transit of an Earth like planet passing in front of a Sun like star. When a planet transits its star in this way, it is possible to see through its thin layer of atmosphere and measure its spectrum. The lines at the bottom of the page show the absorption spectrum of the Earth in front of the Sun, the signature of life as we know it. Seeing our Earth as just one possibly habitable planet among many billions fundamentally changes the perception of our place among the stars. "The 2014 Space Studies Program of the International Space University was hosted by the École de technologie supérieure (ÉTS) and the École des Hautes études commerciales (HEC), Montréal, Québec, Canada." While all care has been taken in the preparation of this report, ISU does not take any responsibility for the accuracy of its content. Electronic copies of the Final Report and the Executive Summary can be downloaded from the ISU Library website at http://isulibrary.isunet.edu/ International Space University Strasbourg Central Campus Parc d’Innovation 1 rue Jean-Dominique Cassini 67400 Illkirch-Graffenstaden Tel +33 (0)3 88 65 54 30 Fax +33 (0)3 88 65 54 47 e-mail: [email protected] website: www.isunet.edu France Unless otherwise credited, figures and images were created by TP Exoplanets. Exoplanets Final Report Page i ACKNOWLEDGEMENTS The International Space University Summer Session Program 2014 and the work on the -
Arxiv:2001.10147V1
Magnetic fields in isolated and interacting white dwarfs Lilia Ferrario1 and Dayal Wickramasinghe2 Mathematical Sciences Institute, The Australian National University, Canberra, ACT 2601, Australia Adela Kawka3 International Centre for Radio Astronomy Research, Curtin University, Perth, WA 6102, Australia Abstract The magnetic white dwarfs (MWDs) are found either isolated or in inter- acting binaries. The isolated MWDs divide into two groups: a high field group (105 − 109 G) comprising some 13 ± 4% of all white dwarfs (WDs), and a low field group (B < 105 G) whose incidence is currently under investigation. The situation may be similar in magnetic binaries because the bright accretion discs in low field systems hide the photosphere of their WDs thus preventing the study of their magnetic fields’ strength and structure. Considerable research has been devoted to the vexed question on the origin of magnetic fields. One hypothesis is that WD magnetic fields are of fossil origin, that is, their progenitors are the magnetic main-sequence Ap/Bp stars and magnetic flux is conserved during their evolution. The other hypothesis is that magnetic fields arise from binary interaction, through differential rotation, during common envelope evolution. If the two stars merge the end product is a single high-field MWD. If close binaries survive and the primary develops a strong field, they may later evolve into the arXiv:2001.10147v1 [astro-ph.SR] 28 Jan 2020 magnetic cataclysmic variables (MCVs). The recently discovered population of hot, carbon-rich WDs exhibiting an incidence of magnetism of up to about 70% and a variability from a few minutes to a couple of days may support the [email protected] [email protected] [email protected] Preprint submitted to Journal of LATEX Templates January 29, 2020 merging binary hypothesis. -
PLANETARY CANDIDATES OBSERVED by Kepler. VIII. a FULLY AUTOMATED CATALOG with MEASURED COMPLETENESS and RELIABILITY BASED on DATA RELEASE 25
Draft version October 13, 2017 Typeset using LATEX twocolumn style in AASTeX61 PLANETARY CANDIDATES OBSERVED BY Kepler. VIII. A FULLY AUTOMATED CATALOG WITH MEASURED COMPLETENESS AND RELIABILITY BASED ON DATA RELEASE 25 Susan E. Thompson,1, 2, 3, ∗ Jeffrey L. Coughlin,2, 1 Kelsey Hoffman,1 Fergal Mullally,1, 2, 4 Jessie L. Christiansen,5 Christopher J. Burke,2, 1, 6 Steve Bryson,2 Natalie Batalha,2 Michael R. Haas,2, y Joseph Catanzarite,1, 2 Jason F. Rowe,7 Geert Barentsen,8 Douglas A. Caldwell,1, 2 Bruce D. Clarke,1, 2 Jon M. Jenkins,2 Jie Li,1 David W. Latham,9 Jack J. Lissauer,2 Savita Mathur,10 Robert L. Morris,1, 2 Shawn E. Seader,11 Jeffrey C. Smith,1, 2 Todd C. Klaus,2 Joseph D. Twicken,1, 2 Jeffrey E. Van Cleve,1 Bill Wohler,1, 2 Rachel Akeson,5 David R. Ciardi,5 William D. Cochran,12 Christopher E. Henze,2 Steve B. Howell,2 Daniel Huber,13, 14, 1, 15 Andrej Prša,16 Solange V. Ramírez,5 Timothy D. Morton,17 Thomas Barclay,18 Jennifer R. Campbell,2, 19 William J. Chaplin,20, 15 David Charbonneau,9 Jørgen Christensen-Dalsgaard,15 Jessie L. Dotson,2 Laurance Doyle,21, 1 Edward W. Dunham,22 Andrea K. Dupree,9 Eric B. Ford,23, 24, 25, 26 John C. Geary,9 Forrest R. Girouard,27, 2 Howard Isaacson,28 Hans Kjeldsen,15 Elisa V. Quintana,18 Darin Ragozzine,29 Avi Shporer,30 Victor Silva Aguirre,15 Jason H. Steffen,31 Martin Still,8 Peter Tenenbaum,1, 2 William F.