About Astronomers a Listing by Andrew Fraknoi (Fromm Institute, U
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Blockbusters: Films and the Books About Them Display Maggie Mason Smith Clemson University, [email protected]
Clemson University TigerPrints Presentations University Libraries 5-2017 Blockbusters: Films and the Books About Them Display Maggie Mason Smith Clemson University, [email protected] Follow this and additional works at: https://tigerprints.clemson.edu/lib_pres Part of the Library and Information Science Commons Recommended Citation Mason Smith, Maggie, "Blockbusters: Films and the Books About Them Display" (2017). Presentations. 105. https://tigerprints.clemson.edu/lib_pres/105 This Display is brought to you for free and open access by the University Libraries at TigerPrints. It has been accepted for inclusion in Presentations by an authorized administrator of TigerPrints. For more information, please contact [email protected]. Blockbusters: Films and the Books About Them Display May 2017 Blockbusters: Films and the Books About Them Display Photograph taken by Micki Reid, Cooper Library Public Information Coordinator Display Description The Summer Blockbuster Season has started! Along with some great films, our new display features books about the making of blockbusters and their cultural impact as well as books on famous blockbuster directors Spielberg, Lucas, and Cameron. Come by Cooper throughout the month of May to check out the Star Wars series and Star Wars Propaganda; Jaws and Just When you thought it was Safe: A Jaws Companion; The Dark Knight trilogy and Hunting the Dark Knight; plus much more! *Blockbusters on display were chosen based on AMC’s list of Top 100 Blockbusters and Box Office Mojo’s list of All Time Domestic Grosses. - Posted on Clemson University Libraries’ Blog, May 2nd 2017 Films on Display • The Amazing Spider-Man. Dir. Marc Webb. Perf. Andrew Garfield, Emma Stone, Rhys Ifans. -
Gruber Foundation Formed at Yale Yale Joins Sloan Digital Sky Survey
Yale University Astronomy Department Newsletter Vol. 3 Fall 2011 No. 1 Yale joins Sloan Digital Sky Survey III Yale is now a fully participating member of the Sloan Digital Sky Survey III (SDSS-III) Collaboration. Although Yale was not a member during the first two phases of SDSS, the suc- cess of SDSS and the excitement of Yale astronomers about the projects and data of SDSS-III led Yale to join now. Based on citations in refereed articles and meeting abstracts, SDSS has been rated as the telescope project with the biggest sci- entific impact in history, beating out even the Hubble Space Telescope and the Keck Telescopes (c.f. Madrid, Juan P. and Macchetto, Duccio 2009arXiv0901.4552M). The previous incarnations of SDSS have imaged 13,000 square degrees, corresponding to about a third of the en- tire sky. SDSS-III is taking spectra of interesting objects that were found in these images, through a program of four sur- veys that cover three scientific themes. The Baryon Oscil- lation Spectroscopic Survey (BOSS) studies dark energy and the geometry of space. (SEE SDSS-III, p. 4) SDSS-III Data Release 8 image from January 2011 Gruber Foundation formed at Yale with prizes and fellowships in astronomy and cosmology In May of 2011, Patricia and Peter Gruber officially formed the Gruber Founda- tion at Yale University, dedicated to the advancement of science, support of young scientists, global justice, and women’s rights. The Gruber Foundation at Yale will succeed The Peter and Patricia Gruber Foundation, originally estab- lished in 1993, and carry on its philanthropic mission, including its prestigious annual science prizes. -
Throughout the Universe, Galaxies Are Rushing Away from Us – and from Each Other – at Tremendously High Speeds
Our Universe Began with a Bang Throughout the Universe, galaxies are rushing away from us – and from each other – at tremendously high speeds. This fact tells us that the Universe is expanding over time. Edwin Hubble (after whom the Hubble Space Telescope was named) first measured the expansion in 1929. Observatories of the Carnegie Institution of Washington Edwin Hubble This posed a big question. If we could run the cosmic movie backward in time, would everything in the Universe be crammed together in a blazing fireball – the starting point of Edwin Hubble & Proceedings of The National Academy of Sciences Hubble’s famous diagram showing the the Big Bang? A lot of scientific distance versus velocity of the galaxies he debate and many new theories observed. The farther away the galaxies, the faster they are moving, showing that the followed Hubble’s discovery. Universe is expanding. Among those in the front lines of the debate were physicists Ralph Alpher and Robert Herman. In 1948 they predicted that an afterglow of this fireball should still exist, though at a much lower temperature than at the time of the Big Bang. Here’s why: As the Universe Fun Fact: expands, the waves of heat About radiation from the Big Bang are 1% of the stretched out, and cool from “snow” you see visible energy to infrared and on broadcast TV then to microwave wavelengths. is caused by the Microwaves are just short- cosmic microwave wavelength radio waves, the same background. form of energy used in microwave ovens. The prediction of an afterglow could be tested! Scientists began building instruments to detect this “cosmic microwave background”, or CMB. -
Download Films / Movies Card Game (PDF)
Back to the Future Blade Runner ET 1985 / sci-fi 1982 / sci-fi 1982 / sci-fi Robert Zemeckis (director) Ridley Scott (director) Steven Spielberg (director) Michael J Fox Harrison Ford Dee Wallace Christopher Lloyd The Godfather Harry Potter and the The Exorcist 1972 / crime thriller Philosopher's Stone 1973 / horror Francis Ford Coppola (director) 2001 / fantasy William Friedkin (director) Maron Brando Chris Columbus (director) Ellen Burstyn Al Pacino Daniel Radcliffe Jaws Raiders of the Lost Ark Goldfinger 1975 / thriller 1981 / action / adventure 1964 / spy thriller Steven Spielberg (director) Steven Spielberg (director) Guy Hamilton (director) Roy Scheider Harrison Ford Sean Connery Robert Shaw Jurassic Park Mad Max The Lion King 1993 / sci-fi 1979 / action 1994 / cartoon / musical Steven Spielberg (director) George Miller (director) Roger Allers / Rob Minkoff Sam Neill Mel Gibson (directors) Laura Dern Joanne Samuel Mission Impossible Pirates of the Caribbean: 1996 / spy / action Pinocchio Dead Man's Chest Brian De Palma (director) 1940 2006 / fantasy adventure Tom Cruise cartoon / musical / fantasy Gore Verbinski (director) Paula Wagner Johnny Depp Apocalypse Now Schindler's List The Matrix 1979 / war film 1993 / historical drama 1999 / sci-fi / action Francis Ford Coppola (director) Steven Spielberg (director) The Wachowskis (directors) Marlon Brando Liam Neeson Keanu Reeves Martin Sheen Ralph Fiennes Carrie-Anne Moss Titanic Crazy Rich Asians The Lord of the Rings: The 1997 / disaster / romance 2018 / romantic comedy Fellowship of the Ring James Cameron (director) Jon M. Chu (director) 2001 / fantasy / adventure Leonardo DiCaprio Constance Wu Peter Jackson (director) Kate Winslet Gemma Chan Elijah Wood Ian McKellen Toy Story The Sound of Music The Dark Knight 1995 1965 / musical / drama 2008 / superhero computer-animated comedy Robert Wise (director) Christopher Nolan (director) John Lasseter (director) Julie Andrews Christian Bale Tom Hanks (voice) Christopher Plummer Michael Caine © ELTbase.com 2019. -
David Kirkby University of California, Irvine, USA 4 August 2020 Expanding Universe
COSMOLOGY IN THE 2020S David Kirkby University of California, Irvine, USA 4 August 2020 Expanding Universe... 2 expansion history a(t |Ωm, ΩDE, …) 3 4 redshift 5 6 0.38Myr opaque universe last scatter 7 inflation opaque universe last scatter gravity waves? 8 CHIME SPT-3G DES 9 TCMB=2.7K, λ~2mm 10 CMB TCMB=2.7K, λ~2mm Galaxies 11 microwave projects: cosmic microwave background (primordial gravity waves, neutrinos, ...) CMB Galaxies optical & NIR projects: galaxy surveys (dark energy, neutrinos, ...) 12 CMB Galaxies telescope location: ground / above atmosphere 13 CMB Atacama desert, Chile CMB ground telescope location: Atacama desert / South Pole 14 Galaxies Galaxy survey instrument: spectrograph / imager 15 Dark Energy Spectroscopic Instrument (DESI) Vera Rubin Observatory 16 Dark Energy Spectroscopic Instrument (DESI) Vera Rubin Observatory 17 EXPANSION HISTORY VS STRUCTURE GROWTH Measurements of our cosmic expansion history constrain the parameters of an expanding homogenous universe: SN LSS , …) expansion historyDE m, Ω a(t |Ω CMB Small inhomogeneities are growing against this backdrop. Measurements of this structure growth provide complementary constraints. 18 Structure Growth 19 Redshift is not a perfect proxy for distance because of galaxy peculiar motions. Large-scale redshift-space distortions (RSD) trace large-scale matter fluctuations: signal! 20 Angles measured on the sky are also distorted by weak lensing (WL) as light is deflected by the same large-scale matter fluctuations: signal! Large-scale redshift-space distortions (RSD) trace large-scale matter fluctuations: signal! 21 CMB measures initial conditions of structure growth at z~1090: Temperature CMB photons also experience weak lensing! https://wiki.cosmos.esa.int/planck-legacy-archive/index.php/CMB_maps Polarization 22 CMB: INFLATION ERA SIGNATURES https://www.annualreviews.org/doi/abs/10.1146/annurev-astro-081915-023433 lensing E-modes lensing B-modes GW B-modes https://arxiv.org/abs/1907.04473 Lensing B modes already observed. -
Witness (1985 Film)
Witness (1985 film) From Wikipedia, the free encyclopedia Jump to: navigation, search Witness Original poster Directed by Peter Weir Produced by Edward S. Feldman William Kelley Written by Pamela Wallace Earl W. Wallace Harrison Ford Kelly McGillis Jan Rubes Starring Danny Glover Lukas Haas Viggo Mortensen Music by Maurice Jarre Cinematography John Seale Editing by Thom Noble Distributed by Paramount Pictures Release date(s) February 8, 1985 Running time 112 minutes Country United States Language English Budget $12,000,000 (estimated) Gross revenue $68,706,993 (US) [1] Witness is a 1985 American thriller film directed by Peter Weir and starring Harrison Ford and Kelly McGillis. The screenplay by William Kelley, Pamela Wallace, and Earl W. Wallace focuses on a detective protecting a young Amish boy who becomes the target of a ruthless killer after he witnesses a brutal murder in Philadelphia's 30th Street train station. The film was nominated for eight Academy Awards and won two, for Best Original Screenplay and Best Film Editing. It was also nominated for seven BAFTA Awards, winning one for Maurice Jarre's score, and was also nominated for six Golden Globe Awards. William Kelley and Earl W. Wallace won the Writers Guild of America Award for Best Original Screenplay and the 1986 Edgar Award for Best Motion Picture Screenplay presented by the Mystery Writers of America. The film is also notable as the screen debut of future stars Viggo Mortensen and Lukas Haas. The film's script is a frequent model for budding screenwriters, often used to display clear structure in a script. -
A New Universe to Discover: a Guide to Careers in Astronomy
A New Universe to Discover A Guide to Careers in Astronomy Published by The American Astronomical Society What are Astronomy and Astrophysics? Ever since Galileo first turned his new-fangled one-inch “spyglass” on the moon in 1609, the popular image of the astronomer has been someone who peers through a telescope at the night sky. But astronomers virtually never put eye to lens these days. The main source of astronomical data is still photons (particles of light) from space, but the tools used to gather and analyze them are now so sophisticated that it’s no longer necessary (or even possible, in most cases) for a human eye to look through them. But for all the high-tech gadgetry, the 21st-Century astronomer is still trying to answer the same fundamental questions that puzzled Galileo: How does the universe work, and where did it come from? Webster’s dictionary defines “astronomy” as “the science that deals with the material universe beyond the earth’s atmosphere.” This definition is broad enough to include great theoretical physicists like Isaac Newton, Albert Einstein, and Stephen Hawking as well as astronomers like Copernicus, Johanes Kepler, Fred Hoyle, Edwin Hubble, Carl Sagan, Vera Rubin, and Margaret Burbidge. In fact, the words “astronomy” and “astrophysics” are pretty much interchangeable these days. Whatever you call them, astronomers seek the answers to many fascinating and fundamental questions. Among them: *Is there life beyond earth? *How did the sun and the planets form? *How old are the stars? *What exactly are dark matter and dark energy? *How did the Universe begin, and how will it end? Astronomy is a physical (non-biological) science, like physics and chemistry. -
The Mutable Galaxies How Galaxies Enrich with Heavy Elements
GENERAL I ARTICLE The Mutable Galaxies How Galaxies Enrich with Heavy Elements Biman Nath Biman Nath is an Soon after the discovery of the expansion of the astrophysicist at the universe, astronomers hoped to determine the Raman Research parameters of the universe by comparing dis Institute, Bangalore. tant galaxies with nearby ones. Observing dis tant galaxies, however, meant observing them as they were long ago. A crucial assumption in Keywords these studies was that galaxies hardly change, in Galaxies, evolution of stars, the time scale of the expansion of the universe. production of elements. Beatrice Tinsley was one of the first astronomers to point out that galaxies do change. Here we discuss a simplified model of galactic evolution, and show that the comparison of its prediction with observations uncovers clues to how galaxies evolve with time. A cursory look at the starry sky at night is likely to make us think that stars, galaxies and the universe are immutable and changeless. Stars and galaxies do how ever change with time. The beginning of the last century was marked by the discovery of the expansion of the uni verse and also the development of our knowledge of the evolution of stars. Yet, the overall evolution of galaxies, as a result of stellar evolution, was considered too messy, and perhaps even negligible. The study of stars told us that stars shine as a result of thermonuclear reactions inside their cores. These Beatrice Tinsley reactions synthesize heavy elements like carbon, oxy was one of the first gen, nitrogen and so forth, beginning with hydrogen astronomers to and helium (which were created in the first few minutes point out that of the birth of the universe). -
What Happened Before the Big Bang?
Quarks and the Cosmos ICHEP Public Lecture II Seoul, Korea 10 July 2018 Michael S. Turner Kavli Institute for Cosmological Physics University of Chicago 100 years of General Relativity 90 years of Big Bang 50 years of Hot Big Bang 40 years of Quarks & Cosmos deep connections between the very big & the very small 100 years of QM & atoms 50 years of the “Standard Model” The Universe is very big (billions and billions of everything) and often beyond the reach of our minds and instruments Big ideas and powerful instruments have enabled revolutionary progress a very big idea connections between quarks & the cosmos big telescopes on the ground Hawaii Chile and in space: Hubble, Spitzer, Chandra, and Fermi at the South Pole basics of our Universe • 100 billion galaxies • each lit with the light of 100 billion stars • carried away from each other by expanding space from a • big bang beginning 14 billion yrs ago Hubble (1925): nebulae are “island Universes” Universe comprised of billions of galaxies Hubble Deep Field: one ten millionth of the sky, 10,000 galaxies 100 billion galaxies in the observable Universe Universe is expanding and had a beginning … Hubble, 1929 Signature of big bang beginning Einstein: Big Bang = explosion of space with galaxies carried along The big questions circa 1978 just two numbers: H0 and q0 Allan Sandage, Hubble’s “student” H0: expansion rate (slope age) q0: deceleration (“droopiness” destiny) … tens of astronomers working (alone) to figure it all out Microwave echo of the big bang Hot MichaelBig S Turner Bang -
Franchelle Stewart Dorn, M.F.A
FRANCHELLE STEWART DORN, M.F.A. 4216 Scales St. Office: (512) 232-7097 Austin, Texas 78723 Home: (512) 840-0075 _______________________________________________________________________ [email protected] CURRENT POSITION The University of Texas at Austin, Department of Theatre and Dance, Virginia L. Murchison Regents Professor. Teach scene study method loosely based on Stanislavsky technique at the undergraduate levels. Specializing in acting Shakespeare. EDUCATION Yale University School of Drama, New Haven, M.F.A. in Acting, 1975 Finch College, New York City, BA in Theatre Arts, 1972 Ineamus Meliora Honor Society. Concentration in Acting/Theater History. EXPERIENCE • Teacher. Forty-five years teaching acting for the stage at several universities and conservatories. • Actor. Forty-five years professional work on regional stage, on television and in film. Current union member of AEA, AFTRA and SAG. • Producer. Eight years as educational film producer. Own company. • Artistic Director/Executive Vice President. Co-founder and co-designer of the first on-line theatrical company. Own company. (Detailed information on the following pages) 1 TEACHING University of Texas at Austin, Department of Theatre and Dance: Virginia L Murchison Regents Professor, January 2000 – present TD 303S Acting for Non-Majors. An overview of modern American realism. The course utilizes games, improvisations, exercises (vocal and physical), open scenes and published contemporary plays to introduce students to basic acting techniques. TD 313C Acting I. Non-text based process. Exploration of the actor’s instrument – body, voice, imagination. Learn the rudiments of emotion, endowing properties and space, finding objectives, action and obstacles. Learn to follow impulses and interact with a partner. TD 313D Acting II. -
Edwin Hubble (1889-1953) Measured Distance to Andromeda Galaxy (M31) • Noticed Individual Bright Stars in Andromeda
The Resolution: Edwin Hubble (1889-1953) Measured Distance to Andromeda Galaxy (M31) • Noticed individual bright stars in Andromeda • Calculated the distance using the Period-Luminosity Relation for Cepheid Variable Stars The Resolution: Edwin Hubble (1889-1953) Measured Distance to Andromeda Galaxy (M31) • Noticed individual bright stars in Andromeda • Calculated the distance using the Period-Luminosity Relation for Cepheid Variable Stars 1. MEASURED magnitude & Period The Resolution: Edwin Hubble (1889-1953) Measured Distance to Andromeda Galaxy (M31) • Noticed individual bright stars in Andromeda • Calculated the distance using the Period-Luminosity Relation for Cepheid Variable Stars 1. MEASURED magnitude & Period 2. CALCULATED Luminosity The Resolution: Edwin Hubble (1889-1953) Measured Distance to Andromeda Galaxy (M31) • Noticed individual bright stars in Andromeda • Calculated the distance using the Period-Luminosity Relation for Cepheid Variable Stars 1. MEASURED magnitude & Period 2. CALCULATED Luminosity 3. CALCULATED Distance The Resolution: Edwin Hubble (1889-1953) Measured Distance to Andromeda Galaxy (M31) • Noticed individual bright stars in Andromeda • Calculated the distance using the Period-Luminosity Relation for Cepheid Variable Stars 1. MEASURED magnitude & Period 2. CALCULATED Luminosity 3. CALCULATED Distance • Result was MUCH farther than expected... • (2.3 Million Ly - well beyond Milky Way) Henrietta Leavitt & Period-Luminosity Relation Cepheid Variables: Bright stars whose Luminosity (energy output) varies every -
The Universe.Pdf
Standard 1: Students will o understand the scientific Terms to know evidence that supports theories o Big Bang Theory that explain how the universe o Doppler Effect and the solar system developed. o Redshift They will compare Earth to other o Universe objects in the solar system. Standard 1, Objective 1: Describe both the big bang theory of universe formation and the nebular theory of solar system formation and evidence supporting them. Lesson Objectives • Explain the evidence for an expanding universe. • Describe the formation of the universe according to the Big Bang Theory. Introduction The study of the universe is called cosmology. Cosmologists study the structure and changes in the present universe. The universe contains all of the star systems, galaxies, gas and dust, plus all the matter and energy that exist. The universe also includes all of space and time. Evolution of Human Understanding of the Universe What did the ancient Greeks recognize as the universe? In their model, the universe contained Earth at the center, the Sun, the Moon, five planets, and a sphere to which all the stars were attached. This idea held for many centuries until Galileo's telescope allowed people to recognize that Earth is not the center of the universe. They also found out that there are many more stars than were visible to the naked eye. All of those stars were in the Milky Way Galaxy. 13 Timeline of cosmological theories 4th century BCE — Aristotle proposes a Geocentric (Earth-centered) universe in which the Earth is stationary and the cosmos (or universe) revolves around the Earth.