Calculating Theoretical Habitable Zones Around Main Sequence and Outlying Star Systems
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Educational Directory, 1
DEPARTMENT OF THEINTERIOR BUREAU OF EDUCATION BULLETIN, 1922, No.50, EDUCATIONALDIRECTORY 1922-1923 WASHINGTON GOVERNMENT PRINTING OFFICE 1923 A u ADDITIONAL COPIES OP THIS PUBLICATION MAY BE PROCURED rams THE SUPERINTENDENT OF DOCUMENTS GOVERNMENT PRINTING OFFICE WASHINGTON, AT 115 CENTS PER COPY PURCHASER AGREES NOT TO RESELL 1SR DISTRIBUTE THIS COPT TOR PROT1T.-P1111. RES. S7, APPROVED MAY 11, 1923 IL CONTENTS. I. The United StatesBureau of Education Page: II. Principal State school officers 1 III. County and other local 3 superintendents of schools.- 13 IV. Superintendents of prIblic schools in cities and towns. 46 V. Presidents of universities andcolleges VI. Presidents of junior 67 77 VII. Heads 9f departm nts ofeducation 78 N111 I. Presidentsor deans of schools of theology 87 IX. Presidents or deans of schools of law 90 X. Presidents or deans of schools of tiielicine 92 XI. Presidents or deans of schools of dentistry 94 Presidents or deans of schools of pharmacy.. XII I. Presidents of schools of 94' osteopathy 96 X IV. Presidents or deans of srliools of veterinary medicine 96 XV. Presidents, etc.. of institutionsfor the training of teachers: 1. Presidents of teachers' colleges. 96 II. Principals of normal training schools: 1. Public normal sclu 99 2. Private normal selfols 104 'III. Directors of kindergarten training incolleges, normal schools, and kindergarten training 84110eild 105 XVI. Directors of.summer schools 109 XVII. Librarians of Public and society Librai 126 XVIII. Executive officers of State library 151 X IX. Directors of librafy schools 152 X X. Educational boards and foundations X X I. Church. educational boards and 152 societies. -
Naming the Extrasolar Planets
Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named. -
Arxiv:2105.11583V2 [Astro-Ph.EP] 2 Jul 2021 Keck-HIRES, APF-Levy, and Lick-Hamilton Spectrographs
Draft version July 6, 2021 Typeset using LATEX twocolumn style in AASTeX63 The California Legacy Survey I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades Lee J. Rosenthal,1 Benjamin J. Fulton,1, 2 Lea A. Hirsch,3 Howard T. Isaacson,4 Andrew W. Howard,1 Cayla M. Dedrick,5, 6 Ilya A. Sherstyuk,1 Sarah C. Blunt,1, 7 Erik A. Petigura,8 Heather A. Knutson,9 Aida Behmard,9, 7 Ashley Chontos,10, 7 Justin R. Crepp,11 Ian J. M. Crossfield,12 Paul A. Dalba,13, 14 Debra A. Fischer,15 Gregory W. Henry,16 Stephen R. Kane,13 Molly Kosiarek,17, 7 Geoffrey W. Marcy,1, 7 Ryan A. Rubenzahl,1, 7 Lauren M. Weiss,10 and Jason T. Wright18, 19, 20 1Cahill Center for Astronomy & Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA 2IPAC-NASA Exoplanet Science Institute, Pasadena, CA 91125, USA 3Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA 94305, USA 4Department of Astronomy, University of California Berkeley, Berkeley, CA 94720, USA 5Cahill Center for Astronomy & Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA 6Department of Astronomy & Astrophysics, The Pennsylvania State University, 525 Davey Lab, University Park, PA 16802, USA 7NSF Graduate Research Fellow 8Department of Physics & Astronomy, University of California Los Angeles, Los Angeles, CA 90095, USA 9Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA 10Institute for Astronomy, University of Hawai`i, -
A Basic Requirement for Studying the Heavens Is Determining Where In
Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth's equator) . Each coordinate system is named for its choice of fundamental plane. The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it rotates as the Earth does . The equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but of course it's really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec for short) . It measures the angle of an object above or below the celestial equator. The longitud inal angle is called the right ascension (RA for short). -
Information Bulletin on Variable Stars
COMMISSIONS AND OF THE I A U INFORMATION BULLETIN ON VARIABLE STARS Nos November July EDITORS L SZABADOS K OLAH TECHNICAL EDITOR A HOLL TYPESETTING K ORI ADMINISTRATION Zs KOVARI EDITORIAL BOARD L A BALONA M BREGER E BUDDING M deGROOT E GUINAN D S HALL P HARMANEC M JERZYKIEWICZ K C LEUNG M RODONO N N SAMUS J SMAK C STERKEN Chair H BUDAPEST XI I Box HUNGARY URL httpwwwkonkolyhuIBVSIBVShtml HU ISSN COPYRIGHT NOTICE IBVS is published on b ehalf of the th and nd Commissions of the IAU by the Konkoly Observatory Budap est Hungary Individual issues could b e downloaded for scientic and educational purp oses free of charge Bibliographic information of the recent issues could b e entered to indexing sys tems No IBVS issues may b e stored in a public retrieval system in any form or by any means electronic or otherwise without the prior written p ermission of the publishers Prior written p ermission of the publishers is required for entering IBVS issues to an electronic indexing or bibliographic system to o CONTENTS C STERKEN A JONES B VOS I ZEGELAAR AM van GENDEREN M de GROOT On the Cyclicity of the S Dor Phases in AG Carinae ::::::::::::::::::::::::::::::::::::::::::::::::::: : J BOROVICKA L SAROUNOVA The Period and Lightcurve of NSV ::::::::::::::::::::::::::::::::::::::::::::::::::: :::::::::::::: W LILLER AF JONES A New Very Long Period Variable Star in Norma ::::::::::::::::::::::::::::::::::::::::::::::::::: :::::::::::::::: EA KARITSKAYA VP GORANSKIJ Unusual Fading of V Cygni Cyg X in Early November ::::::::::::::::::::::::::::::::::::::: -
Una Aproximación Física Al Universo Local De Nebadon
4 1 0 2 local Nebadon de Santiago RodríguezSantiago Hernández Una aproximación física al universo (160.1) 14:5.11 La curiosidad — el espíritu de investigación, el estímulo del descubrimiento, el impulso a la exploración — forma parte de la dotación innata y divina de las criaturas evolutivas del espacio. Tabla de contenido 1.-Descripción científica de nuestro entorno cósmico. ............................................................................. 3 1.1 Lo que nuestros ojos ven. ................................................................................................................ 3 1.2 Lo que la ciencia establece ............................................................................................................... 4 2.-Descripción del LU de nuestro entorno cósmico. ................................................................................ 10 2.1 Universo Maestro ........................................................................................................................... 10 2.2 Gran Universo. Nivel Espacial Superunivesal ................................................................................. 13 2.3 Orvonton. El Séptimo Superuniverso. ............................................................................................ 14 2.4 En el interior de Orvonton. En la Vía Láctea. ................................................................................. 18 2.5 En el interior de Orvonton. Splandon el 5º Sector Mayor ............................................................ 19 -
Mètodes De Detecció I Anàlisi D'exoplanetes
MÈTODES DE DETECCIÓ I ANÀLISI D’EXOPLANETES Rubén Soussé Villa 2n de Batxillerat Tutora: Dolors Romero IES XXV Olimpíada 13/1/2011 Mètodes de detecció i anàlisi d’exoplanetes . Índex - Introducció ............................................................................................. 5 [ Marc Teòric ] 1. L’Univers ............................................................................................... 6 1.1 Les estrelles .................................................................................. 6 1.1.1 Vida de les estrelles .............................................................. 7 1.1.2 Classes espectrals .................................................................9 1.1.3 Magnitud ........................................................................... 9 1.2 Sistemes planetaris: El Sistema Solar .............................................. 10 1.2.1 Formació ......................................................................... 11 1.2.2 Planetes .......................................................................... 13 2. Planetes extrasolars ............................................................................ 19 2.1 Denominació .............................................................................. 19 2.2 Història dels exoplanetes .............................................................. 20 2.3 Mètodes per detectar-los i saber-ne les característiques ..................... 26 2.3.1 Oscil·lació Doppler ........................................................... 27 2.3.2 Trànsits -
1. Which of the Following Statements Is Incorrect Concerning Sidereal Days and Solar Days?
1. Which of the following statements is incorrect concerning sidereal days and solar days? A. One sidereal day is defined as the time taken for the Earth to make one complete rotation on its axis B. One sidereal day is 3.9 minutes longer than one solar day C. The time difference between one sidereal day and one solar day accounts for the daily slight shift in the position of stars D. The time difference between one sidereal day and one solar day is due to the simultaneous rotation of the Earth about its axis and the revolution of Earth around the Sun 2. The Earth’s aphelion is the position of the Earth on its orbit that is most distant from the Sun. At which time of the year is the Earth furthest from the Sun? A. 3 January B. 21 June C. 3 July D. 21 December 3. Which of the following statements is incorrect regarding solar eclipses? A. During a total solar eclipse, the corona of the Sun becomes visible. B. If the umbra region of the eclipse does not reach the Earth, an annular eclipse will be seen C. A solar eclipse track on Earth runs from the west to the east D. An eclipse that occurred in December 4, 2002 will be seen again in December 14, 2018, in accordance with the Saros cycle 4. The Milankovitch cycles concern about the movement of Earth on its axis and its orbit around the Sun. These cycles include the Earth’s orbit eccentricity, its precession period and its obliquity. -
GTO Keypad Manual, V5.001
ASTRO-PHYSICS GTO KEYPAD Version v5.xxx Please read the manual even if you are familiar with previous keypad versions Flash RAM Updates Keypad Java updates can be accomplished through the Internet. Check our web site www.astro-physics.com/software-updates/ November 11, 2020 ASTRO-PHYSICS KEYPAD MANUAL FOR MACH2GTO Version 5.xxx November 11, 2020 ABOUT THIS MANUAL 4 REQUIREMENTS 5 What Mount Control Box Do I Need? 5 Can I Upgrade My Present Keypad? 5 GTO KEYPAD 6 Layout and Buttons of the Keypad 6 Vacuum Fluorescent Display 6 N-S-E-W Directional Buttons 6 STOP Button 6 <PREV and NEXT> Buttons 7 Number Buttons 7 GOTO Button 7 ± Button 7 MENU / ESC Button 7 RECAL and NEXT> Buttons Pressed Simultaneously 7 ENT Button 7 Retractable Hanger 7 Keypad Protector 8 Keypad Care and Warranty 8 Warranty 8 Keypad Battery for 512K Memory Boards 8 Cleaning Red Keypad Display 8 Temperature Ratings 8 Environmental Recommendation 8 GETTING STARTED – DO THIS AT HOME, IF POSSIBLE 9 Set Up your Mount and Cable Connections 9 Gather Basic Information 9 Enter Your Location, Time and Date 9 Set Up Your Mount in the Field 10 Polar Alignment 10 Mach2GTO Daytime Alignment Routine 10 KEYPAD START UP SEQUENCE FOR NEW SETUPS OR SETUP IN NEW LOCATION 11 Assemble Your Mount 11 Startup Sequence 11 Location 11 Select Existing Location 11 Set Up New Location 11 Date and Time 12 Additional Information 12 KEYPAD START UP SEQUENCE FOR MOUNTS USED AT THE SAME LOCATION WITHOUT A COMPUTER 13 KEYPAD START UP SEQUENCE FOR COMPUTER CONTROLLED MOUNTS 14 1 OBJECTS MENU – HAVE SOME FUN! -
Pivotal Role of Spin in Celestial Body Motion Mechanics: Prelude to a Spinning Universe
Journal of High Energy Physics, Gravitation and Cosmology, 2021, 7, 98-122 https://www.scirp.org/journal/jhepgc ISSN Online: 2380-4335 ISSN Print: 2380-4327 Pivotal Role of Spin in Celestial Body Motion Mechanics: Prelude to a Spinning Universe Puthalath Koroth Raghuprasad Independent Researcher, Odessa, TX, USA How to cite this paper: Raghuprasad, P.K. Abstract (2021) Pivotal Role of Spin in Celestial Body Motion Mechanics: Prelude to a This is the final article in our series dealing with the interplay of spin and Spinning Universe. Journal of High Energy gravity that leads to the generation, and continuation of celestial body mo- Physics, Gravitation and Cosmology, 7, tions in the universe. In our prior studies we focused on such interactions in 98-122. https://doi.org/10.4236/jhepgc.2021.71005 the elementary particles, and in the celestial bodies in the solar system. Fore- most among the findings was that, along with gravity, matter at all levels ex- Received: March 23, 2020 hibits axial spin. We further noted that all freestanding bodies outside our Accepted: December 19, 2020 solar system, including the largest such units, the stars and galaxies also spin Published: December 22, 2020 on their axes. Also, the axial rotation speed of planets in our solar system has Copyright © 2021 by author(s) and a linear positive relationship to their masses, thus hinting at its fundamental Scientific Research Publishing Inc. and autonomous nature. We have reported that this relationship between the This work is licensed under the Creative size of the body and its axial rotation speed extends to the stars and even the Commons Attribution International License (CC BY 4.0). -
The Sizes of the Stars
Chapter 8 The Sizes of the Stars The “Plough” in Ursa Major, photographed by Nik Szymanek Look up into the sky, and you will see the stars as tiny, twinkling points. The twinkling is due entirely to the Earth’s atmosphere; from space (or on the Moon) stars do not twinkle (scintillate) at all, and if you have the chance of seeing stars while you are travelling in a high-flying jet you will find that the twinkling is much less then it is at sea level. But with the naked eye, no star appears as anything but a dot. If you use a star as an obvious disk, you may be assured that there is something wrong. Almost certainly the telescope is out of focus. This being so, it takes an effort of the imagina- tion to appreciate that some of the stars are huge enough to contain the whole orbit of the Earth round the Sun – while admittedly others are so tiny that they could fit com- fortably into the ring road of a small city. For the last the programme of 2005 I was joined by Professors Richard Harrison and Lucy Green to say something about the Sun, the only star close enough to be examined in a great deal, and then by Drs John Mason and Barrie Jones, to discuss the sizes of the various types of stars. P. Moore, The Sky at Night, DOI 10.1007/978-1-4419-6409-0_8, 29 © Springer Science+Business Media, LLC 2010 30 8 The Sizes of the Stars If no stars show obvious disks, then how do we measure their diameters? There are various methods. -
Carnegie Institution Carnegie
C68099_CVR.qxd:CVR 3/29/11 7:58 Page 1 2009-2010 CARNEGIE INSTITUTION FOR 2009-2010 SCIENCE YEAR BOOK 1530 P Street, N.W. Washington DC 20005 Phone: 202.387.6400 Carnegie Institution Fax: 202.387.8092 www.CarnegieScience.edu FOR SCIENCE CARNEGIE INSTITUTION FOR SCIENCE INSTITUTION FOR CARNEGIE YEAR BOOK The paper used in the manufacturing this year book contains 30% post-consumer recycled fiber. By using recycled fiber in place of virgin fiber, the Carnegie Institution preserved 41 trees, saved 126 pounds of waterborne waste, saved 18,504 gallons of water and prevented 4031 pounds of greenhouse gasses. The energy used to print the report was produced by wind power. Designed by Tina Taylor, T2 Design Printed by Monroe Litho ISSN 0069-066X C68099_CVR.qxd:CVR 3/29/11 7:58 Page 2 Department of Embryology 3520 San Martin Dr. / Baltimore, MD 21218 410.246.3001 Geophysical Laboratory 5251 Broad Branch Rd., N.W. / Washington, DC 20015-1305 202.478.8900 Department of Global Ecology 260 Panama St. / Stanford, CA 94305-4101 650.462.1047 The Carnegie Observatories 813 Santa Barbara St. / Pasadena, CA 91101-1292 626.577.1122 Las Campanas Observatory Casilla 601 / La Serena, Chile Department of Plant Biology 260 Panama St. / Stanford, CA 94305-4101 650.325.1521 Department of Terrestrial Magnetism 5241 Broad Branch Rd., N.W. / Washington, DC 20015-1305 202.478.8820 Office of Administration 1530 P St., N.W. / Washington, DC 20005-1910 202.387.6400 www.CarnegieScience.edu 2 009-2010 YEAR BOOK The President’s Report July 1, 2009 - June 30, 2010 CARNEGIE INSTITUTION FOR SCIENCE Former Presidents Former Trustees Daniel C.