Jodrell Bank Discovery Centre Constellation Spotting Guide
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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. -
Get Outside What to Look for in the Summer Sky Your Hosts of the Summer Sky Are Three Bright Stars — Vega, Altair and Deneb
Get Outside What to Look for in the Summer Sky Your hosts of the summer sky are three bright stars — Vega, Altair and Deneb. Together they make up the Summer Triangle. Look for the triangle in the east on a June evening, moving NORTH to overhead as the season progresses. Polaris The Big Dipper Deneb Cygnus Vega Lyra Hercules Arcturus EaST West Summer Triangle Altair Aquila Sagittarius Antares Turn the map so Scorpius the direction you are facing is at the Teapot the bottom. south facebook.com/KidsCanBooks @KidsCanPress GET OUTSIDE Text © 2013 Jane Drake & Ann Love Illustrations © 2013 Heather Collins www.kidscanpress.com Get Outside Vega The Keystone The brightest star in the Between Vega and Arcturus, Summer Triangle, Vega is look for four stars in a wedge or The summer bluish white. It is in the keystone shape. This is the body solstice constellation Lyra, the Harp. of Hercules, the Strongman. His feet are to the north and Every day from late Altair his arms to the south, making December to June, the The second-brightest star in his figure kneel Sun rises and sets a little the triangle, Altair is white. upside down farther north along the Altair is in the constellation in the sky. horizon. But about June Aquila, the Eagle. 21, the Sun seems to stop Keystone moving north. It rises in Deneb the northeast and sets in The dimmest star of the the northwest, seemingly Summer Triangle, Deneb would in the same spots for be the brightest if it were not so Hercules several days. -
Neutron Stars
Chandra X-Ray Observatory X-Ray Astronomy Field Guide Neutron Stars Ordinary matter, or the stuff we and everything around us is made of, consists largely of empty space. Even a rock is mostly empty space. This is because matter is made of atoms. An atom is a cloud of electrons orbiting around a nucleus composed of protons and neutrons. The nucleus contains more than 99.9 percent of the mass of an atom, yet it has a diameter of only 1/100,000 that of the electron cloud. The electrons themselves take up little space, but the pattern of their orbit defines the size of the atom, which is therefore 99.9999999999999% Chandra Image of Vela Pulsar open space! (NASA/PSU/G.Pavlov et al. What we perceive as painfully solid when we bump against a rock is really a hurly-burly of electrons moving through empty space so fast that we can't see—or feel—the emptiness. What would matter look like if it weren't empty, if we could crush the electron cloud down to the size of the nucleus? Suppose we could generate a force strong enough to crush all the emptiness out of a rock roughly the size of a football stadium. The rock would be squeezed down to the size of a grain of sand and would still weigh 4 million tons! Such extreme forces occur in nature when the central part of a massive star collapses to form a neutron star. The atoms are crushed completely, and the electrons are jammed inside the protons to form a star composed almost entirely of neutrons. -
Survey of Britain's Most Powerful Radial Engine : an Example Of
JULY 5TH, 1945 FLIGHT Survey of Britain's Most Powerful Radial Engine : An Example of . r l^OgiCal Layout to Achieve Compactness with Power T has been eommbn knowledge far some time past that •power figure of 3,500, the b.h.p. /litre of both Hercules the Bristol Aeroplane Co., Ltd., have been engaged with Centaurus is 46.5, although we know that the latter engine the production of a larger and improved model in the is somewhat better than this, as may be rough!y indicated age of radial, air-cooled, sleeve-valve engines with which by the figures for b.h.p./sq. in. of piston area, these ey have for so long enhanced their reputation. This being respectively:. Hercules 4.93. and Centaurus better mmon knowledge—the result of unofficial "leaks"— than 5.34. • f ibraced the facts that the new engine was an 18-cylinder : Cooling Arrangements lit of over 2,000 h.p. and was called the Centaurug.. ther than this nothing much was generally known until As an indication of refinement in the design of the cowl- nctioned reference, to the engine was made with the ing, if. we take as a datum the frontal area of the Hercules lease of the Short Shetland flying boat (Flight, May 17th, at 2,122 sq. in. and give it the value of unity, then the 145), when it was revealed that the Centaurus was of Centaurus frontal area of 2,402 sq. in. gives a comparative 'er 2,500 h.p. ratio of 1.13:1, which is well below the relative h.p..ratio Even now we are not permitted to give any indication of 1.385 :1, itself a conservative figure. -
Newpointe-Catalog
NewPointe® Constellation Collections More value from Batesville Constellation Collections 18 Gauge Steel Caskets Leo Collection Leo Brushed Black Silver velvet interior Leo Brushed Black shown with Praying Hands decorative kit. 257178 - half couch Choose from 11 designs. 262411 - full couch See page 15 for your options. • Includes decorative kit option for lid Leo Painted Silver Silver velvet interior 257172 - half couch 262415 - full couch • Includes decorative kit option for lid Leo Brushed Ruby Leo Brushed Blue Leo Painted Sand Leo Painted White Moss Pink velvet interior Light Blue velvet interior Champagne velvet interior Moss Pink velvet interior 257177 - half couch 257179 - half couch 257173 - half couch 257166 - half couch 262410 - full couch 262412 - full couch 262416 - full couch 262414 - full couch • Includes decorative kit option • Includes decorative kit option • Includes decorative kit option • Includes decorative kit option for lid for lid for lid for lid 2 All caskets not available in all locations. Please check to ensure availability in your area. 18 Gauge Steel Caskets Virgo Collection Virgo White/Pink Moss Pink crepe interior| $845 250673 - half couch Virgo White/Pink shown with Roses 254258 - full couch decorative kit and corner decals. Choose from 11 designs. • Includes decorative kit option See page 15 for your options. for lid and corner decals Virgo Blue Light Blue crepe interior 250658 - half couch 254255 - full couch • Includes decorative kit option for lid and corner decals Virgo Silver Virgo White Virgo Copper -
Summer Constellations
Night Sky 101: Summer Constellations The Summer Triangle Photo Credit: Smoky Mountain Astronomical Society The Summer Triangle is made up of three bright stars—Altair, in the constellation Aquila (the eagle), Deneb in Cygnus (the swan), and Vega Lyra (the lyre, or harp). Also called “The Northern Cross” or “The Backbone of the Milky Way,” Cygnus is a horizontal cross of five bright stars. In very dark skies, Cygnus helps viewers find the Milky Way. Albireo, the last star in Cygnus’s tail, is actually made up of two stars (a binary star). The separate stars can be seen with a 30 power telescope. The Ring Nebula, part of the constellation Lyra, can also be seen with this magnification. In Japanese mythology, Vega, the celestial princess and goddess, fell in love Altair. Her father did not approve of Altair, since he was a mortal. They were forbidden from seeing each other. The two lovers were placed in the sky, where they were separated by the Celestial River, repre- sented by the Milky Way. According to the legend, once a year, a bridge of magpies form, rep- resented by Cygnus, to reunite the lovers. Photo credit: Unknown Scorpius Also called Scorpio, Scorpius is one of the 12 Zodiac constellations, which are used in reading horoscopes. Scorpius represents those born during October 23 to November 21. Scorpio is easy to spot in the summer sky. It is made up of a long string bright stars, which are visible in most lights, especially Antares, because of its distinctly red color. Antares is about 850 times bigger than our sun and is a red giant. -
Introduction to Astronomy from Darkness to Blazing Glory
Introduction to Astronomy From Darkness to Blazing Glory Published by JAS Educational Publications Copyright Pending 2010 JAS Educational Publications All rights reserved. Including the right of reproduction in whole or in part in any form. Second Edition Author: Jeffrey Wright Scott Photographs and Diagrams: Credit NASA, Jet Propulsion Laboratory, USGS, NOAA, Aames Research Center JAS Educational Publications 2601 Oakdale Road, H2 P.O. Box 197 Modesto California 95355 1-888-586-6252 Website: http://.Introastro.com Printing by Minuteman Press, Berkley, California ISBN 978-0-9827200-0-4 1 Introduction to Astronomy From Darkness to Blazing Glory The moon Titan is in the forefront with the moon Tethys behind it. These are two of many of Saturn’s moons Credit: Cassini Imaging Team, ISS, JPL, ESA, NASA 2 Introduction to Astronomy Contents in Brief Chapter 1: Astronomy Basics: Pages 1 – 6 Workbook Pages 1 - 2 Chapter 2: Time: Pages 7 - 10 Workbook Pages 3 - 4 Chapter 3: Solar System Overview: Pages 11 - 14 Workbook Pages 5 - 8 Chapter 4: Our Sun: Pages 15 - 20 Workbook Pages 9 - 16 Chapter 5: The Terrestrial Planets: Page 21 - 39 Workbook Pages 17 - 36 Mercury: Pages 22 - 23 Venus: Pages 24 - 25 Earth: Pages 25 - 34 Mars: Pages 34 - 39 Chapter 6: Outer, Dwarf and Exoplanets Pages: 41-54 Workbook Pages 37 - 48 Jupiter: Pages 41 - 42 Saturn: Pages 42 - 44 Uranus: Pages 44 - 45 Neptune: Pages 45 - 46 Dwarf Planets, Plutoids and Exoplanets: Pages 47 -54 3 Chapter 7: The Moons: Pages: 55 - 66 Workbook Pages 49 - 56 Chapter 8: Rocks and Ice: -
Constellations with Prominent Stars That Can Be Found Near the Meridian at 10 Pm on January 15
ONSTELLATIONS C Altitude Ruler The rotation of the Earth on its axis causes the stars to rise and set each evening. In addition, the orbit of the Earth around the Sun places different regions of the sky in our Horizon night-time view. The PLANISPHERE is an extremely useful tool for finding stars and 10 constellation in the sky, depicting not only what is currently in the sky but it also allows the 20 prediction of the rising and setting times of various celestial objects. 30 THE LAYOUT OF THE PLANISPHERE 40 50 The outer circumference of the dark blue circular disk (which is called the star wheel) you’ll notice that the wheel is divided into the 12 months, and that each month is divided into 60 individual dates. The star wheel rotates about the brass fastener, which represents the 70 North Celestial Pole. The frame of the planisphere has times along the outer edge. 80 Holding the planisphere on the southern corner you'll see "midnight" at the top. Moving Zenith counterclockwise, notice how the hours progress, through 1 AM, 2 AM, and so on through "noon" at the bottom. The hours then proceed through the afternoon and evening (1 PM, 2 PM, etc.) back toward midnight. Once you have the wheel set properly for the correct time and day, the displayed part represents what you see if you stand with the star and planet locator held directly over your head with the brass fastener toward the north. (Notice that the compass directions are also written on the corners of the frame.) Of course, you don't have to actually stand that way to make use of the Star and Planet Locator--this is just a description to help you understand what is displayed. -
Constellation Myths Has Exciting and Sometimes Tragic Guides for Gods and Heroes
TEACHER’S GUIDE TEACHER’S GUIDE TEACHER’S GUIDE Follow-up Activities • www.pantheon.org Encyclopedia Mythica supplies definitions, images, and pronunciation • This collection of constellation myths has exciting and sometimes tragic guides for gods and heroes. events happening at the beginning, middle, and endings of their stories. • www.mythweb.com/encyc/index.html Pretend you are a news reporter called to the scene of one of these Look up your favorite Greek character in this encyclopedia of Greek events. Develop a list of “who,”“what,”“where,”“why” and “how” ques- mythology. tions to ask one of the characters.With a partner, take turns asking and • www.mythman.com recording answers about the tragic or exciting event.Write it up as a A humorous homework help site for students with classical myth “breaking news” story. retellings. • There are many variations and mythological beings in constellation and nature myths. Have students research, compare, and contrast other ver- Suggested Print Resources sions of these tales. Use Bulfinch’s Mythology by Thomas Bulfinch • Andrews,Tamra. Dictionary of Nature Myths: Legends of the Earth, Sea, (Random House, 1998) to discover alternate stories. and Sky. Oxford University Press, Oxford, NY; 2000. • Students can research other stars and planets named after characters in • D’Aulaire, Ingri and Edgar Parin D’Aulaire. Ingri and Edgar Parin Greek mythology. Have them find out why the beautiful Pleiades, the D’Aulaire’s Book of Greek Myths. Doubleday, Garden City, NY; 1962. One CONSTELLATION MYTHS seven daughters of Atlas, are placed as stars in front of the Orion con- of the best-loved classical collections of Greek mythology. -
Stability of Planets in Binary Star Systems
StabilityStability ofof PlanetsPlanets inin BinaryBinary StarStar SystemsSystems Ákos Bazsó in collaboration with: E. Pilat-Lohinger, D. Bancelin, B. Funk ADG Group Outline Exoplanets in multiple star systems Secular perturbation theory Application: tight binary systems Summary + Outlook About NFN sub-project SP8 “Binary Star Systems and Habitability” Stand-alone project “Exoplanets: Architecture, Evolution and Habitability” Basic dynamical types S-type motion (“satellite”) around one star P-type motion (“planetary”) around both stars Image: R. Schwarz Exoplanets in multiple star systems Observations: (Schwarz 2014, Binary Catalogue) ● 55 binary star systems with 81 planets ● 43 S-type + 12 P-type systems ● 10 multiple star systems with 10 planets Example: γ Cep (Hatzes et al. 2003) ● RV measurements since 1981 ● Indication for a “planet” (Campbell et al. 1988) ● Binary period ~57 yrs, planet period ~2.5 yrs Multiplicity of stars ~45% of solar like stars (F6 – K3) with d < 25 pc in multiple star systems (Raghavan et al. 2010) Known exoplanet host stars: single double triple+ source 77% 20% 3% Raghavan et al. (2006) 83% 15% 2% Mugrauer & Neuhäuser (2009) 88% 10% 2% Roell et al. (2012) Exoplanet catalogues The Extrasolar Planets Encyclopaedia http://exoplanet.eu Exoplanet Orbit Database http://exoplanets.org Open Exoplanet Catalogue http://www.openexoplanetcatalogue.com The Planetary Habitability Laboratory http://phl.upr.edu/home NASA Exoplanet Archive http://exoplanetarchive.ipac.caltech.edu Binary Catalogue of Exoplanets http://www.univie.ac.at/adg/schwarz/multiple.html Habitable Zone Gallery http://www.hzgallery.org Binary Catalogue Binary Catalogue of Exoplanets http://www.univie.ac.at/adg/schwarz/multiple.html Dynamical stability Stability limit for S-type planets Rabl & Dvorak (1988), Holman & Wiegert (1999), Pilat-Lohinger & Dvorak (2002) Parameters (a , e , μ) bin bin Outer limit at roughly max. -
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. -
Platform-Independent Mobile Robot Communication
Philipp A. Baer Platform-Independent Development of Robot Communication Software kassel university press This work has been accepted by the faculty of Electrical Engineering and Computer Science of the University of Kassel as a thesis for acquiring the academic degree of Doktor der Ingenieurwissenschaften (Dr.-Ing.). Advisers: Prof. Dr. Kurt Geihs Prof. Dr. Gerhard K. Kraetzschmar Additional Doctoral Committee Members: Prof. Dr. Albert Zündorf Prof. Dr. Klaus David Defense day: 04th December 2008 Bibliographic information published by Deutsche Nationalbibliothek The Deutsche Nationalbibliothek lists this publication in the Deutsche Nationalbibliografie; detailed bibliographic data is available in the Internet at http://dnb.d-nb.de. Zugl.: Kassel, Univ., Diss. 2008 ISBN print: 978-3-89958-644-2 ISBN online: 978-3-89958-645-9 URN: urn:nbn:de:0002-6453 © 2008, kassel university press GmbH, Kassel www.upress.uni-kassel.de Printed by: Unidruckerei, University of Kassel Printed in Germany Für Mutti und Mama. Mutti, du bleibst unvergessen. * 29. September 1923 = 14. Oktober 2008 Contents List of Figuresv List of Tables vii Abstract ix I Introduction1 1 Introduction3 1.1 Motivation.........................................4 1.1.1 Software Structure................................5 1.1.2 Development Methodology...........................5 1.1.3 Communication.................................6 1.1.4 Configuration and Monitoring.........................6 1.2 Problem Analysis.....................................7 1.2.1 Development Methodology...........................7 1.2.2 Communication Infrastructure........................8 1.2.3 Resource Discovery...............................8 1.3 Solution Approach....................................9 1.4 Major Results........................................ 11 1.5 Overview.......................................... 12 2 Foundations 13 2.1 Autonomous Mobile Robots............................... 13 2.1.1 Hardware Architecture............................. 14 2.1.2 Robot Software.................................