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Beetlejuice Handbook for the Recently Deceased Hardcover
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Space Trivia Questions and Answers
Space Trivia Questions From: conversationstartersworld.com/space-trivia-questions 1. What type of galaxy is the most common in the universe? Elliptical galaxies Galaxies are categorized as elliptical, spiral, or irregular. There are at least two trillion galaxies in the universe. Each galaxy is bound by gravity and consists of stars, dust, interstellar gas, and dark matter. They range in size from a few billion stars to one hundred trillion stars. The oldest and most distant observed galaxy is actually 32 billion light years from Earth and is located in the constellation Ursa Major. 2. What is the coldest place in the universe? (Hint: It’s a nebula.) The Boomerang Nebula The Boomerang Nebula is one degree Kelvin which is -458 degrees Fahrenheit or -272.15 degrees Celsius. It is located in the Centaurus constellation and is colder than the background temperature of deep space. 3. The hottest place in the universe is located in which constellation? The constellation Virgo The hottest place in the universe is actually a cloud of gas surrounding a swarm of galaxies that are clustered together in the Virgo constellation. The temperature there reaches 300 million degrees Celsius. The cloud is believed to have been formed as a result of colliding galaxies going at speeds of 2,500 miles per second. 4. How old is the universe in light years? (Plus or minus 1 billion light years.) 13.8 billion light years old Scientists used various methods to estimate its age. These included methods such as measuring the composition of matter and energy density in the universe. -
GEORGE HERBIG and Early Stellar Evolution
GEORGE HERBIG and Early Stellar Evolution Bo Reipurth Institute for Astronomy Special Publications No. 1 George Herbig in 1960 —————————————————————– GEORGE HERBIG and Early Stellar Evolution —————————————————————– Bo Reipurth Institute for Astronomy University of Hawaii at Manoa 640 North Aohoku Place Hilo, HI 96720 USA . Dedicated to Hannelore Herbig c 2016 by Bo Reipurth Version 1.0 – April 19, 2016 Cover Image: The HH 24 complex in the Lynds 1630 cloud in Orion was discov- ered by Herbig and Kuhi in 1963. This near-infrared HST image shows several collimated Herbig-Haro jets emanating from an embedded multiple system of T Tauri stars. Courtesy Space Telescope Science Institute. This book can be referenced as follows: Reipurth, B. 2016, http://ifa.hawaii.edu/SP1 i FOREWORD I first learned about George Herbig’s work when I was a teenager. I grew up in Denmark in the 1950s, a time when Europe was healing the wounds after the ravages of the Second World War. Already at the age of 7 I had fallen in love with astronomy, but information was very hard to come by in those days, so I scraped together what I could, mainly relying on the local library. At some point I was introduced to the magazine Sky and Telescope, and soon invested my pocket money in a subscription. Every month I would sit at our dining room table with a dictionary and work my way through the latest issue. In one issue I read about Herbig-Haro objects, and I was completely mesmerized that these objects could be signposts of the formation of stars, and I dreamt about some day being able to contribute to this field of study. -
Orders of Magnitude (Length) - Wikipedia
03/08/2018 Orders of magnitude (length) - Wikipedia Orders of magnitude (length) The following are examples of orders of magnitude for different lengths. Contents Overview Detailed list Subatomic Atomic to cellular Cellular to human scale Human to astronomical scale Astronomical less than 10 yoctometres 10 yoctometres 100 yoctometres 1 zeptometre 10 zeptometres 100 zeptometres 1 attometre 10 attometres 100 attometres 1 femtometre 10 femtometres 100 femtometres 1 picometre 10 picometres 100 picometres 1 nanometre 10 nanometres 100 nanometres 1 micrometre 10 micrometres 100 micrometres 1 millimetre 1 centimetre 1 decimetre Conversions Wavelengths Human-defined scales and structures Nature Astronomical 1 metre Conversions https://en.wikipedia.org/wiki/Orders_of_magnitude_(length) 1/44 03/08/2018 Orders of magnitude (length) - Wikipedia Human-defined scales and structures Sports Nature Astronomical 1 decametre Conversions Human-defined scales and structures Sports Nature Astronomical 1 hectometre Conversions Human-defined scales and structures Sports Nature Astronomical 1 kilometre Conversions Human-defined scales and structures Geographical Astronomical 10 kilometres Conversions Sports Human-defined scales and structures Geographical Astronomical 100 kilometres Conversions Human-defined scales and structures Geographical Astronomical 1 megametre Conversions Human-defined scales and structures Sports Geographical Astronomical 10 megametres Conversions Human-defined scales and structures Geographical Astronomical 100 megametres 1 gigametre -
Reading Chapter 8: Sec
Reading Chapter 8: Sec. 8.1 (Spectra p. 202-211) Sec. 8.1 Optional: 212-219 Sec. 8.2 H-R Diagram Chapter 9: Not covered Chapter 10: Sec. 10.1 10.2 optional Chapter 10: Sec. 10.3 required Croswell: Chapters 6-9 H-R diagram Stars fall into four categories of stars: 1.main-sequence stars 2. giants 3. supergiants 4. white dwarfs. HRDiagram.anim.mp4 UY Scuti is the largest Star Currently Known Antares, a SUPERGIANT in Scorpius RUY Scuti = 1700 RSUN UY Scuti is the largest Star Currently Known Spectroscopic Parallax ! Spectroscopy allows us to: ! 1. Determine spectral type, hence temperature ! 2. Determine luminosity class (I - VI) (see Sec. 9.5) ! If a star can be placed on the HR diagram, then its absolute magnitude (MV) can be determined. ! By measuring its apparent mag, distance can be determined: ! This method of determining distances is called spectroscopic “parallax” ! Less precise than usual parallax... Stellar Evolution ! As a star ages, it undergoes changes in its Luminosity & Temperature. ! It “moves on the HR Diagram” ! Stars on the Main Sequence (MS) are all fusing Hydrogen. ! When their Hydrogen supply runs out, they leave the MS. ! More massive stars leave first. What powers the Sun? (C&O 10.3) Could it be Chemical Reactions? If so, then how much energy, E, is available? How long could the Sun be powered by chemical reactions? The Sun produces 4 x 1026 Joules/s t = E /LSun Chemical reactions typically release: ~4 eV of energy = 4 * 1.6 x 10-19 J ~ 10-18 J, per atom If every atom in the Sun burns (like coal), then the energy available is: E = n * 10-18 J . -
The Eldorado Star Party 2017 Telescope Observing Club by Bill Flanagan Houston Astronomical Society
The Eldorado Star Party 2017 Telescope Observing Club by Bill Flanagan Houston Astronomical Society Purpose and Rules Welcome to the Annual ESP Telescope Club! The main purpose of this club is to give you an opportunity to observe some of the showpiece objects of the fall season under the pristine skies of Southwest Texas. In addition, we have included a few items on the observing lists that may challenge you to observe some fainter and more obscure objects that present themselves at their very best under the dark skies of the Eldorado Star Party. The rules are simple; just observe the required number of objects listed while you are at the Eldorado Star Party to receive a club badge. Big & Bright The telescope program, “Big & Bright,” is a list of 30 objects. This observing list consists of some objects that are apparently big and/or bright and some objects that are intrinsically big and/or bright. Of course the apparently bright objects will be easy to find and should be fun to observe under the dark sky conditions at the X-Bar Ranch. Observing these bright objects under the dark skies of ESP will permit you to see a lot of detail that is not visible under light polluted skies. Some of the intrinsically big and bright objects may be more challenging because at the extreme distance of these objects they will appear small and dim. Nonetheless the challenge of hunting them down and then pondering how far away and energetic they are can be just as rewarding as observing the brighter, easier objects on the list. -
Arxiv:1709.07265V1 [Astro-Ph.SR] 21 Sep 2017 an Der Sternwarte 16, 14482 Potsdam, Germany E-Mail: [email protected] 2 Smitha Subramanian Et Al
Noname manuscript No. (will be inserted by the editor) Young and Intermediate-age Distance Indicators Smitha Subramanian · Massimo Marengo · Anupam Bhardwaj · Yang Huang · Laura Inno · Akiharu Nakagawa · Jesper Storm Received: date / Accepted: date Abstract Distance measurements beyond geometrical and semi-geometrical meth- ods, rely mainly on standard candles. As the name suggests, these objects have known luminosities by virtue of their intrinsic proprieties and play a major role in our understanding of modern cosmology. The main caveats associated with standard candles are their absolute calibration, contamination of the sample from other sources and systematic uncertainties. The absolute calibration mainly de- S. Subramanian Kavli Institute for Astronomy and Astrophysics Peking University, Beijing, China E-mail: [email protected] M. Marengo Iowa State University Department of Physics and Astronomy, Ames, IA, USA E-mail: [email protected] A. Bhardwaj European Southern Observatory 85748, Garching, Germany E-mail: [email protected] Yang Huang Department of Astronomy, Kavli Institute for Astronomy & Astrophysics, Peking University, Beijing, China E-mail: [email protected] L. Inno Max-Planck-Institut f¨urAstronomy 69117, Heidelberg, Germany E-mail: [email protected] A. Nakagawa Kagoshima University, Faculty of Science Korimoto 1-1-35, Kagoshima 890-0065, Japan E-mail: [email protected] J. Storm Leibniz-Institut f¨urAstrophysik Potsdam (AIP) arXiv:1709.07265v1 [astro-ph.SR] 21 Sep 2017 An der Sternwarte 16, 14482 Potsdam, Germany E-mail: [email protected] 2 Smitha Subramanian et al. pends on their chemical composition and age. To understand the impact of these effects on the distance scale, it is essential to develop methods based on differ- ent sample of standard candles. -
Our Star, the SUN DO NOT EDIT--Changes Must Be Made Through “File Info” DO NOT EDIT--Changes Must Be Made Through “File Info” Correctionkey=NL-A Correctionkey=NL-A
DO NOT EDIT--Changes must be made through “File info” CorrectionKey=NL-A Our Star, the SUN DO NOT EDIT--Changes must be made through “File info” DO NOT EDIT--Changes must be made through “File info” CorrectionKey=NL-A CorrectionKey=NL-A Read Preview — Flip through the book. to Look for words that are new, and share them with a partner. Our Star, Learn 1. observatory A room or building housing an astronomical telescope or other the scientific equipment for the study of natural phenomena. 2. pinhole projector A device used to safely view an image of the sun. SUN Skim — Look at the illustrations and photos. What is happening in the story? Credits: 7 ©solarseven/Shutterstock; 10 ©NASA/A. Lutkus/H. Zell. Can you tell what it will be about? Copyright © by Houghton Mifflin Harcourt Publishing Company All rights reserved. No part of this work may be reproduced or transmitted in any form or by any means, electronic or mechanical, including photocopying or recording, or by any information storage or retrieval system, without the prior written permission of the copyright owner unless such copying is expressly permitted by federal copyright law. Requests for permission to make copies of any part of the work should be submitted through our Permissions website at https://customercare.hmhco.com/contactus/Permissions.html or mailed to Houghton Mifflin Harcourt Publishing Company, Attn: Compliance, Contracts, and Licensing, 9400 Southpark Center Loop, Orlando, Florida 32819-8647. Printed in the U.S.A. ISBN 978-0-358-39412-9 Read — Read to learn how scientists 1 2 3 4 5 6 7 8 9 10 XXXX 29 28 27 26 25 24 23 22 21 20 study the sun, our closest star, without 4500000000 damaging their eyes. -
Free My Robux
Free My Robux Free My Robux CLICK HERE TO ACCESS ROBLOX GENERATOR roblox cheat farbe The largest of these types of stars are sometimes called red hypergiants. One of these is 1708 times the size of our Sun (UY Scuti), and is the largest known star in the universe. UY Scuti is about 9,500 light years away from the Earth. Caution! – Beware of Free ROBUX Generators, Roblox Hacks No Survey or Human Verification! There are hundreds of websites online that claim to act as Roblox generators that can openly distribute free ROBUX hacks & gift codes so that Roblox players can charge in to their game, ROBUX-loaded. While this does sound far too good to be true, it ... Below are 48 working coupons for all ro ghoul codes 2021 from reliable websites that we have updated for users to get maximum savings. With ro ghoul codes that we provide, you will get free mask/yen/skin/rc. The codes give 4.5 million rc. Roblox ro ghoul new codes. How to earn robux for free? Link Account. The more games you play, more Robux you can earn. It's simple! Exchange Rublins for Robux. Check this video instruction on how to create game pass. If you still can't get R$ and don't see new transactions, please, contact us. Step 1-Launch a web browser on any device you like and enter ‘nulled.to‘ in the search box and hit the search option.Step 2-Then, scroll down to the bottom of the www.The page that pops up and clicks on ‘Full version’ to view the full version of this web page. -
WELCOME to the SAASTA Astroquiz 2016 ROUND 3
2017/08/16 QUESTION 1 WELCOME What is the most abundant gas found to the on Venus' atmosphere? SAASTA A. Carbon Dioxide AstroQuiz 2016 B. Nitrogen ROUND 3 C. Hydrogen D. Oxygen QUESTION 2 QUESTION 3 The most abundant gas found on Earth’s What is the largest known star so far? atmosphere is ________ A. Betelgeuse A. Carbon Dioxide B. UY Scuti B. Nitrogen C. VY Canis majoris C. Hydrogen D. Oxygen D. Sun QUESTION 4 QUESTION 5 Which of the below has a large storm Which of the following is a gas planet on its surface and one of its moons and has at least 27 moons. orbiting the planet backwards? A. Venus A. Venus B. Mercury B. Mercury C. Neptune C. Neptune D. Uranus D. Uranus 1 2017/08/16 QUESTION 6 QUESTION 7 Which of the following is an inner planet Which of the following is an inner planet and has clouds of sulphuric acid. and is usually referred to as morning or evening star? A. Venus A. Venus B. Mercury B. Mercury C. Neptune C. Neptune D. Uranus D. Uranus QUESTION 8 QUESTION 9 Which of the following is true about the The Moon does not have light of its Moon? own but ____ light from the Sun. A. It can be seen at night A. Reflects B. It can be seen during the day B. Refracts C. Sometimes we cannot see it at all C. Deflects D. All of the above D. Diffracts QUESTION 10 QUESTION 11 A meteorite is ______ Which of the following objects is made up of lumps of ice & rock and can take years to go around the Sun. -
The Distance and Size of the Red Hypergiant NML Cygni from VLBA and VLA Astrometry
A&A 544, A42 (2012) Astronomy DOI: 10.1051/0004-6361/201219587 & c ESO 2012 Astrophysics The distance and size of the red hypergiant NML Cygni from VLBA and VLA astrometry B. Zhang1,2,M.J.Reid3,K.M.Menten1,X.W.Zheng4, and A. Brunthaler1,5 1 Max-Plank-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany e-mail: [email protected] 2 Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, 200030 Shanghai, PR China 3 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 4 Department of Astronomy, Nanjing University, 22 Hankou Road, 210093 Nanjing, PR China 5 National Radio Astronomy Observatory, Socorro, NM 87801, USA Received 11 May 2012 / Accepted 4 July 2012 ABSTRACT Context. The red hypergiant NML Cyg has been assumed to be at part of the Cyg OB2 association, although its distance has never been measured directly. A reliable distance is crucial to study the properties of this prominent star. For example, its luminosity, and hence its position on the H-R diagram, is critical information to determine its evolutionary status. In addition, a detection of the radio photosphere would be complementary to other methods of determining the stellar size. Aims. We aim to understand the characteristics of NML Cyg with direct measurements of its absolute position, distance, kinematics, and size. Methods. We observe circumstellar 22 GHz H2O and 43 GHz SiO masers with the Very Long Baseline Array to determine the parallax and proper motion of NML Cyg. We observe continuum emission at 43 GHz from the radio photosphere of NML Cyg with the Very Large Array. -
Astronomy Magazine 2020 Index
Astronomy Magazine 2020 Index SUBJECT A AAVSO (American Association of Variable Star Observers), Spectroscopic Database (AVSpec), 2:15 Abell 21 (Medusa Nebula), 2:56, 59 Abell 85 (galaxy), 4:11 Abell 2384 (galaxy cluster), 9:12 Abell 3574 (galaxy cluster), 6:73 active galactic nuclei (AGNs). See black holes Aerojet Rocketdyne, 9:7 airglow, 6:73 al-Amal spaceprobe, 11:9 Aldebaran (Alpha Tauri) (star), binocular observation of, 1:62 Alnasl (Gamma Sagittarii) (optical double star), 8:68 Alpha Canum Venaticorum (Cor Caroli) (star), 4:66 Alpha Centauri A (star), 7:34–35 Alpha Centauri B (star), 7:34–35 Alpha Centauri (star system), 7:34 Alpha Orionis. See Betelgeuse (Alpha Orionis) Alpha Scorpii (Antares) (star), 7:68, 10:11 Alpha Tauri (Aldebaran) (star), binocular observation of, 1:62 amateur astronomy AAVSO Spectroscopic Database (AVSpec), 2:15 beginner’s guides, 3:66, 12:58 brown dwarfs discovered by citizen scientists, 12:13 discovery and observation of exoplanets, 6:54–57 mindful observation, 11:14 Planetary Society awards, 5:13 satellite tracking, 2:62 women in astronomy clubs, 8:66, 9:64 Amateur Telescope Makers of Boston (ATMoB), 8:66 American Association of Variable Star Observers (AAVSO), Spectroscopic Database (AVSpec), 2:15 Andromeda Galaxy (M31) binocular observations of, 12:60 consumption of dwarf galaxies, 2:11 images of, 3:72, 6:31 satellite galaxies, 11:62 Antares (Alpha Scorpii) (star), 7:68, 10:11 Antennae galaxies (NGC 4038 and NGC 4039), 3:28 Apollo missions commemorative postage stamps, 11:54–55 extravehicular activity