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Mapping Robert Storr
Mapping Robert Storr Author Storr, Robert Date 1994 Publisher The Museum of Modern Art: Distributed by H.N. Abrams ISBN 0870701215, 0810961407 Exhibition URL www.moma.org/calendar/exhibitions/436 The Museum of Modern Art's exhibition history— from our founding in 1929 to the present—is available online. It includes exhibition catalogues, primary documents, installation views, and an index of participating artists. MoMA © 2017 The Museum of Modern Art bk 99 £ 05?'^ £ t***>rij tuin .' tTTTTl.l-H7—1 gm*: \KN^ ( Ciji rsjn rr &n^ u *Trr» 4 ^ 4 figS w A £ MoMA Mapping Robert Storr THE MUSEUM OF MODERN ART, NEW YORK DISTRIBUTED BY HARRY N. ABRAMS, INC., NEW YORK (4 refuse Published in conjunction with the exhibition Mappingat The Museum of Modern Art, New York, October 6— tfoti h December 20, 1994, organized by Robert Storr, Curator, Department of Painting and Sculpture The exhibition is supported by AT&TNEW ART/NEW VISIONS. Additional funding is provided by the Contemporary Exhibition Fund of The Museum of Modern Art, established with gifts from Lily Auchincloss, Agnes Gund and Daniel Shapiro, and Mr. and Mrs. Ronald S. Lauder. This publication is supported in part by a grant from The Junior Associates of The Museum of Modern Art. Produced by the Department of Publications The Museum of Modern Art, New York Osa Brown, Director of Publications Edited by Alexandra Bonfante-Warren Designed by Jean Garrett Production by Marc Sapir Printed by Hull Printing Bound by Mueller Trade Bindery Copyright © 1994 by The Museum of Modern Art, New York Certain illustrations are covered by claims to copyright cited in the Photograph Credits. -
Exep Science Plan Appendix (SPA) (This Document)
ExEP Science Plan, Rev A JPL D: 1735632 Release Date: February 15, 2019 Page 1 of 61 Created By: David A. Breda Date Program TDEM System Engineer Exoplanet Exploration Program NASA/Jet Propulsion Laboratory California Institute of Technology Dr. Nick Siegler Date Program Chief Technologist Exoplanet Exploration Program NASA/Jet Propulsion Laboratory California Institute of Technology Concurred By: Dr. Gary Blackwood Date Program Manager Exoplanet Exploration Program NASA/Jet Propulsion Laboratory California Institute of Technology EXOPDr.LANET Douglas Hudgins E XPLORATION PROGRAMDate Program Scientist Exoplanet Exploration Program ScienceScience Plan Mission DirectorateAppendix NASA Headquarters Karl Stapelfeldt, Program Chief Scientist Eric Mamajek, Deputy Program Chief Scientist Exoplanet Exploration Program JPL CL#19-0790 JPL Document No: 1735632 ExEP Science Plan, Rev A JPL D: 1735632 Release Date: February 15, 2019 Page 2 of 61 Approved by: Dr. Gary Blackwood Date Program Manager, Exoplanet Exploration Program Office NASA/Jet Propulsion Laboratory Dr. Douglas Hudgins Date Program Scientist Exoplanet Exploration Program Science Mission Directorate NASA Headquarters Created by: Dr. Karl Stapelfeldt Chief Program Scientist Exoplanet Exploration Program Office NASA/Jet Propulsion Laboratory California Institute of Technology Dr. Eric Mamajek Deputy Program Chief Scientist Exoplanet Exploration Program Office NASA/Jet Propulsion Laboratory California Institute of Technology This research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. © 2018 California Institute of Technology. Government sponsorship acknowledged. Exoplanet Exploration Program JPL CL#19-0790 ExEP Science Plan, Rev A JPL D: 1735632 Release Date: February 15, 2019 Page 3 of 61 Table of Contents 1. -
The Museum of Modern Art
The Museum of Modern Art For Immediate Release May 1995 ARTIST'S CHOICE: ELIZABETH MURRAY June 20 - August 22, 1995 An exhibition conceived and installed by American artist Elizabeth Murray is the fifth in The Museum of Modern Art's series of ARTIST'S CHOICE exhibitions. On view from June 20 to August 22, 1995, ARTIST'S CHOICE: ELIZABETH MURRAY presents more than 100 drawings, paintings, prints, and sculptures by approximately seventy women artists. The exhibition involves works created between 1914 and 1973, including those ranging from early modernists Frida Kahlo and Liubov Popova to contemporary artists Nancy Graves and Dorothea Rockburne. Murray focuses particular attention on artists who made their reputations during the 1950s and 1960s, such as Lee Bontecou, Agnes Martin, Joan Mitchell, when Murray herself was studying and forming her style. This exhibition and the accompanying video and panel discussion are made possible by a generous grant from The Charles A. Dana Foundation. Organized in collaboration with Kirk Varnedoe, Chief Curator, Department of Painting and Sculpture, the ARTIST'S CHOICE series invites artists to create an exhibition from the Museum's collection according to a personally chosen theme or principle. "I wanted, for myself, to explore what being a woman in the art world has meant," Murray writes in the exhibition brochure. "I wanted to weave together a sense of the genuine and profound contribution women's work has made to the art of our time." - more - 11 West 53 Street, New York, N.Y. 10019-5498 Tel: 212-708-9400 Fax: 212-708-9889 2 Installed in the Museum's third-floor contemporary painting and sculpture galleries, the exhibition is arranged in thematic groupings. -
A Finding Aid to the Lucy R. Lippard Papers, 1930S-2007, Bulk 1960-1990
A Finding Aid to the Lucy R. Lippard Papers, 1930s-2007, bulk 1960s-1990, in the Archives of American Art Stephanie L. Ashley and Catherine S. Gaines Funding for the processing of this collection was provided by the Terra Foundation for American Art 2014 May Archives of American Art 750 9th Street, NW Victor Building, Suite 2200 Washington, D.C. 20001 https://www.aaa.si.edu/services/questions https://www.aaa.si.edu/ Table of Contents Collection Overview ........................................................................................................ 1 Administrative Information .............................................................................................. 1 Biographical / Historical.................................................................................................... 2 Scope and Contents........................................................................................................ 3 Arrangement..................................................................................................................... 4 Names and Subjects ...................................................................................................... 4 Container Listing ............................................................................................................. 6 Series 1: Biographical Material, circa 1960s-circa 1980s........................................ 6 Series 2: Correspondence, 1950s-2006.................................................................. 7 Series 3: Writings, 1930s-1990s........................................................................... -
Science Concept 5: Lunar Volcanism Provides a Window Into the Thermal and Compositional Evolution of the Moon
Science Concept 5: Lunar Volcanism Provides a Window into the Thermal and Compositional Evolution of the Moon Science Concept 5: Lunar volcanism provides a window into the thermal and compositional evolution of the Moon Science Goals: a. Determine the origin and variability of lunar basalts. b. Determine the age of the youngest and oldest mare basalts. c. Determine the compositional range and extent of lunar pyroclastic deposits. d. Determine the flux of lunar volcanism and its evolution through space and time. INTRODUCTION Features of Lunar Volcanism The most prominent volcanic features on the lunar surface are the low albedo mare regions, which cover approximately 17% of the lunar surface (Fig. 5.1). Mare regions are generally considered to be made up of flood basalts, which are the product of highly voluminous basaltic volcanism. On the Moon, such flood basalts typically fill topographically-low impact basins up to 2000 m below the global mean elevation (Wilhelms, 1987). The mare regions are asymmetrically distributed on the lunar surface and cover about 33% of the nearside and only ~3% of the far-side (Wilhelms, 1987). Other volcanic surface features include pyroclastic deposits, domes, and rilles. These features occur on a much smaller scale than the mare flood basalts, but are no less important in understanding lunar volcanism and the internal evolution of the Moon. Table 5.1 outlines different types of volcanic features and their interpreted formational processes. TABLE 5.1 Lunar Volcanic Features Volcanic Feature Interpreted Process -
Exoplanet.Eu Catalog Page 1 # Name Mass Star Name
exoplanet.eu_catalog # name mass star_name star_distance star_mass OGLE-2016-BLG-1469L b 13.6 OGLE-2016-BLG-1469L 4500.0 0.048 11 Com b 19.4 11 Com 110.6 2.7 11 Oph b 21 11 Oph 145.0 0.0162 11 UMi b 10.5 11 UMi 119.5 1.8 14 And b 5.33 14 And 76.4 2.2 14 Her b 4.64 14 Her 18.1 0.9 16 Cyg B b 1.68 16 Cyg B 21.4 1.01 18 Del b 10.3 18 Del 73.1 2.3 1RXS 1609 b 14 1RXS1609 145.0 0.73 1SWASP J1407 b 20 1SWASP J1407 133.0 0.9 24 Sex b 1.99 24 Sex 74.8 1.54 24 Sex c 0.86 24 Sex 74.8 1.54 2M 0103-55 (AB) b 13 2M 0103-55 (AB) 47.2 0.4 2M 0122-24 b 20 2M 0122-24 36.0 0.4 2M 0219-39 b 13.9 2M 0219-39 39.4 0.11 2M 0441+23 b 7.5 2M 0441+23 140.0 0.02 2M 0746+20 b 30 2M 0746+20 12.2 0.12 2M 1207-39 24 2M 1207-39 52.4 0.025 2M 1207-39 b 4 2M 1207-39 52.4 0.025 2M 1938+46 b 1.9 2M 1938+46 0.6 2M 2140+16 b 20 2M 2140+16 25.0 0.08 2M 2206-20 b 30 2M 2206-20 26.7 0.13 2M 2236+4751 b 12.5 2M 2236+4751 63.0 0.6 2M J2126-81 b 13.3 TYC 9486-927-1 24.8 0.4 2MASS J11193254 AB 3.7 2MASS J11193254 AB 2MASS J1450-7841 A 40 2MASS J1450-7841 A 75.0 0.04 2MASS J1450-7841 B 40 2MASS J1450-7841 B 75.0 0.04 2MASS J2250+2325 b 30 2MASS J2250+2325 41.5 30 Ari B b 9.88 30 Ari B 39.4 1.22 38 Vir b 4.51 38 Vir 1.18 4 Uma b 7.1 4 Uma 78.5 1.234 42 Dra b 3.88 42 Dra 97.3 0.98 47 Uma b 2.53 47 Uma 14.0 1.03 47 Uma c 0.54 47 Uma 14.0 1.03 47 Uma d 1.64 47 Uma 14.0 1.03 51 Eri b 9.1 51 Eri 29.4 1.75 51 Peg b 0.47 51 Peg 14.7 1.11 55 Cnc b 0.84 55 Cnc 12.3 0.905 55 Cnc c 0.1784 55 Cnc 12.3 0.905 55 Cnc d 3.86 55 Cnc 12.3 0.905 55 Cnc e 0.02547 55 Cnc 12.3 0.905 55 Cnc f 0.1479 55 -
Cartographic Perspectives Information Society 1
Number 53, Winterjournal 2006 of the Northcartographic American Cartographic perspectives Information Society 1 cartographic perspectives Number 53, Winter 2006 in this issue Letter from the Editor INTRODUCTION Art and Mapping: An Introduction 4 Denis Cosgrove Dear Members of NACIS, FEATURED ARTICLES Welcome to CP53, the first issue of Map Art 5 Cartographic Perspectives in 2006. I Denis Wood plan to be brief with my column as there is plenty to read on the fol- Interpreting Map Art with a Perspective Learned from 15 lowing pages. This is an important J.M. Blaut issue on Art and Cartography that Dalia Varanka was spearheaded about a year ago by Denis Wood and John Krygier. Art-Machines, Body-Ovens and Map-Recipes: Entries for a 24 It’s importance lies in the fact that Psychogeographic Dictionary nothing like this has ever been kanarinka published in an academic journal. Ever. To punctuate it’s importance, Jake Barton’s Performance Maps: An Essay 41 let me share a view of one of the John Krygier reviewers of this volume: CARTOGRAPHIC TECHNIQUES …publish these articles. Nothing Cartographic Design on Maine’s Appalachian Trail 51 more, nothing less. Publish them. Michael Hermann and Eugene Carpentier III They are exciting. They are interest- ing: they stimulate thought! …They CARTOGRAPHIC COLLECTIONS are the first essays I’ve read (other Illinois Historical Aerial Photography Digital Archive Keeps 56 than exhibition catalogs) that actu- Growing ally try — and succeed — to come to Arlyn Booth and Tom Huber terms with the intersections of maps and art, that replace the old formula REVIEWS of maps in/as art, art in/as maps by Historical Atlas of Central America 58 Reviewed by Mary L. -
18Th EANA Conference European Astrobiology Network Association
18th EANA Conference European Astrobiology Network Association Abstract book 24-28 September 2018 Freie Universität Berlin, Germany Sponsors: Detectability of biosignatures in martian sedimentary systems A. H. Stevens1, A. McDonald2, and C. S. Cockell1 (1) UK Centre for Astrobiology, University of Edinburgh, UK ([email protected]) (2) Bioimaging Facility, School of Engineering, University of Edinburgh, UK Presentation: Tuesday 12:45-13:00 Session: Traces of life, biosignatures, life detection Abstract: Some of the most promising potential sampling sites for astrobiology are the numerous sedimentary areas on Mars such as those explored by MSL. As sedimentary systems have a high relative likelihood to have been habitable in the past and are known on Earth to preserve biosignatures well, the remains of martian sedimentary systems are an attractive target for exploration, for example by sample return caching rovers [1]. To learn how best to look for evidence of life in these environments, we must carefully understand their context. While recent measurements have raised the upper limit for organic carbon measured in martian sediments [2], our exploration to date shows no evidence for a terrestrial-like biosphere on Mars. We used an analogue of a martian mudstone (Y-Mars[3]) to investigate how best to look for biosignatures in martian sedimentary environments. The mudstone was inoculated with a relevant microbial community and cultured over several months under martian conditions to select for the most Mars-relevant microbes. We sequenced the microbial community over a number of transfers to try and understand what types microbes might be expected to exist in these environments and assess whether they might leave behind any specific biosignatures. -
Simulating (Sub)Millimeter Observations of Exoplanet Atmospheres in Search of Water
University of Groningen Kapteyn Astronomical Institute Simulating (Sub)Millimeter Observations of Exoplanet Atmospheres in Search of Water September 5, 2018 Author: N.O. Oberg Supervisor: Prof. Dr. F.F.S. van der Tak Abstract Context: Spectroscopic characterization of exoplanetary atmospheres is a field still in its in- fancy. The detection of molecular spectral features in the atmosphere of several hot-Jupiters and hot-Neptunes has led to the preliminary identification of atmospheric H2O. The Atacama Large Millimiter/Submillimeter Array is particularly well suited in the search for extraterrestrial water, considering its wavelength coverage, sensitivity, resolving power and spectral resolution. Aims: Our aim is to determine the detectability of various spectroscopic signatures of H2O in the (sub)millimeter by a range of current and future observatories and the suitability of (sub)millimeter astronomy for the detection and characterization of exoplanets. Methods: We have created an atmospheric modeling framework based on the HAPI radiative transfer code. We have generated planetary spectra in the (sub)millimeter regime, covering a wide variety of possible exoplanet properties and atmospheric compositions. We have set limits on the detectability of these spectral features and of the planets themselves with emphasis on ALMA. We estimate the capabilities required to study exoplanet atmospheres directly in the (sub)millimeter by using a custom sensitivity calculator. Results: Even trace abundances of atmospheric water vapor can cause high-contrast spectral ab- sorption features in (sub)millimeter transmission spectra of exoplanets, however stellar (sub) millime- ter brightness is insufficient for transit spectroscopy with modern instruments. Excess stellar (sub) millimeter emission due to activity is unlikely to significantly enhance the detectability of planets in transit except in select pre-main-sequence stars. -
10/17/2015 1 the Origin of the Solar System Chapter 10
10/17/2015 Guidepost As you explore the origins and the materials that make up the solar system, you will discover the answers to several important questions: What are the observed properties of the solar system? Chapter 10 What is the theory for the origin of the solar system that explains the observed properties? The Origin of the Solar System How did Earth and the other planets form? What do astronomers know about other extrasolar planets orbiting other stars? In this and the following six chapters, we will explore in more detail the planets and other objects that make up our solar system, our home in the universe. A Survey of the Solar System Two Kinds of Planets The solar system consists of eight Planets of our solar system can be divided into two very major planets and several other different kinds: objects. Jovian (Jupiter- like) planets: The planets rotate on their axes and Jupiter, Saturn, revolve around the Sun. Uranus, Neptune The planets have elliptical orbits, sometimes inclined to the ecliptic, and all planets revolve in the same directly; only Venus and Uranus rotate in an alternate direction. Nearly all moons also revolve in the Terrestrial (Earthlike) same direction. planets: Mercury, Venus, Earth, Mars Terrestrial Planets Craters on Planets’ Surfaces Craters (like on our Four inner moon’s surface) are planets of the common throughout solar system the solar system. Relatively small in size Not seen on Jovian and mass planets because (Earth is the Surface of Venus they don’t have a largest and Rocky surface can not be seen solid surface. -
Proxima B: the Alien World Next Door - Is Anyone Home?
Proxima b: The Alien World Next Door - Is Anyone Home? Edward Guinan Biruni Observatory Dept. Astrophysics & Planetary Science th 40 Anniversary Workshop Villanova University 12 October, 2017 [email protected] Talking Points i. Planet Hunting: Exoplanets ii. Living with a Red Dwarf Program iii. Alpha Cen ABC -nearest Star System iv. Proxima Cen – the red dwarf star v. Proxima b Nearest Exoplanet vi. Can it support Life? vii. Planned Observations / Missions Planet Hunting: Finding Exoplanets A brief summary For citizen science projects: www.planethunters.org Early Thoughts on Extrasolar Planets and Life Thousands of years ago, Greek philosophers speculated… “There are infinite worlds both like and unlike this world of ours...We must believe that in all worlds there are living creatures and planets and other things we see in this world.” Epicurius c. 300 B.C First Planet Detected 51 Pegasi – November 1995 Mayer & Queloz / Marcy & Butler Credit: Charbonneau Many Exoplanets (400+) have been detected by the Spectroscopic Doppler Motion Technique (now can measure motions as low as 1 m/s (3.6 km/h = 2.3 mph)) Exoplanet Transit Eclipses Rp/Rs ~ [Depth of Eclipse] 1/2 Transit Eclipse Depths for Jupiter, Neptune and Earth for the Sun 0.01% (Earth-Sun) 0.15% (Neptune-Sun) 1.2% (Jupiter-Sun) Kepler Mission See: kepler.nasa.gov Has so far discovered 6000+ Confirmed & Candidate Exoplanets The Search for Planets Outside Our Solar System Exoplanet Census May 2017 Exoplanet Census (May-2017) Confirmed exoplanets: 3483+ (Doppler / Transit) 490+ Multi-planet Systems [April 2017] Exoplanet Candidates: 7900+ orbiting 2600+ stars (Mostly from the Kepler Mission) [May 2017] Other unconfirmed (mostly from CoRot)Exoplanets ~186+ Potentially Habitable Exoplanets: 51 (April 2017) Estimated Planets in the Galaxy ~ 50 -100 Billion! Most expected to be hosted by red dwarf stars Nomad (Free-floating planets) ~ 25 - 50 Billion Known planets with life: 1 so far. -
Solo Show by Michael Jones Mckean Proxima Centauri B. Gleise 667 Cc
Solo show by Michael Jones McKean Proxima Centauri b. Gleise 667 Cc. Kepler-442b. Kepler-452b. Wolf 1061c. Kepler-1229b. Kapteyn b. Kelper-62f. Kepler-186f. GJ 273b. TRAPPIST-1e. Du 2 au 26 septembre 2017 / From 2 to 26 September 2017 Vernissage samedi 2 septembre / Opening on Saturday, September 2nd Michael Jones McKean, The Ground, 2017 Galerie Escougnou-Cetraro Galerie Escougnou-Cetraro Michael Jone McKean, no title yet, 2017 (FR) Une tong, une tête, un pot, un scalp, un fossile, un régime de bananes, un ordinateur, une part de pizza, un abat-jour, une branche, une branche morte, un masque, une imprimante-scanner. Cet inventaire à la Prévert ne contient qu’une infime partie des multiples objets qui peuplent l’écologie post-digitale de Michael Jones McKean. Qu’elles prennent la forme de collages (Tau Ceti e, 2015), d’installation à l’échelle de la galerie (The Religion, 2013) ou à celle du bâtiment (The Ground, 2017), les sculptures – puisque c’est le terme que revendique l’auteur – constituent autant de tentatives d’ordonnancement entre le vivant et l’inerte, l’humain et le non-humain, au sein desquelles chaque entité se voit assigner une valeur ontologique équiva- lente. Les œuvres du jeune artiste américain rendent compte d’un réel dont la conscience humaine ne serait plus le seul déterminant, mais qui, dans la lignée des théories de l’assemblage et de l’acteur-réseau, serait un état purement émergent, constamment redéfini par la corrélation des multiples agents qui le peuplent. The Garden, The Comedy, The Folklore, The Yucca Mountain, The Religion : qu’elles décrivent de grandes constructions symboliques et politiques humaines, des réalités géographiques ou temporelles, les sculptures tissent des réseaux denses, non linéaires et non hiérar- chiques, en son sein et au-delà.