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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. -
Stars and Their Spectra: an Introduction to the Spectral Sequence Second Edition James B
Cambridge University Press 978-0-521-89954-3 - Stars and Their Spectra: An Introduction to the Spectral Sequence Second Edition James B. Kaler Index More information Star index Stars are arranged by the Latin genitive of their constellation of residence, with other star names interspersed alphabetically. Within a constellation, Bayer Greek letters are given first, followed by Roman letters, Flamsteed numbers, variable stars arranged in traditional order (see Section 1.11), and then other names that take on genitive form. Stellar spectra are indicated by an asterisk. The best-known proper names have priority over their Greek-letter names. Spectra of the Sun and of nebulae are included as well. Abell 21 nucleus, see a Aurigae, see Capella Abell 78 nucleus, 327* ε Aurigae, 178, 186 Achernar, 9, 243, 264, 274 z Aurigae, 177, 186 Acrux, see Alpha Crucis Z Aurigae, 186, 269* Adhara, see Epsilon Canis Majoris AB Aurigae, 255 Albireo, 26 Alcor, 26, 177, 241, 243, 272* Barnard’s Star, 129–130, 131 Aldebaran, 9, 27, 80*, 163, 165 Betelgeuse, 2, 9, 16, 18, 20, 73, 74*, 79, Algol, 20, 26, 176–177, 271*, 333, 366 80*, 88, 104–105, 106*, 110*, 113, Altair, 9, 236, 241, 250 115, 118, 122, 187, 216, 264 a Andromedae, 273, 273* image of, 114 b Andromedae, 164 BDþ284211, 285* g Andromedae, 26 Bl 253* u Andromedae A, 218* a Boo¨tis, see Arcturus u Andromedae B, 109* g Boo¨tis, 243 Z Andromedae, 337 Z Boo¨tis, 185 Antares, 10, 73, 104–105, 113, 115, 118, l Boo¨tis, 254, 280, 314 122, 174* s Boo¨tis, 218* 53 Aquarii A, 195 53 Aquarii B, 195 T Camelopardalis, -
Astronomy 2009 Index
Astronomy Magazine 2009 Index Subject Index 1RXS J160929.1-210524 (star), 1:24 4C 60.07 (galaxy pair), 2:24 6dFGS (Six Degree Field Galaxy Survey), 8:18 21-centimeter (neutral hydrogen) tomography, 12:10 93 Minerva (asteroid), 12:18 2008 TC3 (asteroid), 1:24 2009 FH (asteroid), 7:19 A Abell 21 (Medusa Nebula), 3:70 Abell 1656 (Coma galaxy cluster), 3:8–9, 6:16 Allen Telescope Array (ATA) radio telescope, 12:10 ALMA (Atacama Large Millimeter/sub-millimeter Array), 4:21, 9:19 Alpha (α) Canis Majoris (Sirius) (star), 2:68, 10:77 Alpha (α) Orionis (star). See Betelgeuse (Alpha [α] Orionis) (star) Alpha Centauri (star), 2:78 amateur astronomy, 10:18, 11:48–53, 12:19, 56 Andromeda Galaxy (M31) merging with Milky Way, 3:51 midpoint between Milky Way Galaxy and, 1:62–63 ultraviolet images of, 12:22 Antarctic Neumayer Station III, 6:19 Anthe (moon of Saturn), 1:21 Aperture Spherical Telescope (FAST), 4:24 APEX (Atacama Pathfinder Experiment) radio telescope, 3:19 Apollo missions, 8:19 AR11005 (sunspot group), 11:79 Arches Cluster, 10:22 Ares launch system, 1:37, 3:19, 9:19 Ariane 5 rocket, 4:21 Arianespace SA, 4:21 Armstrong, Neil A., 2:20 Arp 147 (galaxy pair), 2:20 Arp 194 (galaxy group), 8:21 art, cosmology-inspired, 5:10 ASPERA (Astroparticle European Research Area), 1:26 asteroids. See also names of specific asteroids binary, 1:32–33 close approach to Earth, 6:22, 7:19 collision with Jupiter, 11:20 collisions with Earth, 1:24 composition of, 10:55 discovery of, 5:21 effect of environment on surface of, 8:22 measuring distant, 6:23 moons orbiting, -
February 2019 BRAS Newsletter
Monthly Meeting February 11th at 7PM at HRPO (Monthly meetings are on 2nd Mondays, Highland Road Park Observatory). Speaker: Chris Desselles on Astrophotography What's In This Issue? President’s Message Secretary's Summary Outreach Report Astrophotography Group Asteroid and Comet News Light Pollution Committee Report Recent BRAS Forum Entries Messages from the HRPO Science Academy International Astronomy Day Friday Night Lecture Series Globe at Night Adult Astronomy Courses Nano Days Observing Notes – Canis Major – The Great Dog & Mythology Like this newsletter? See PAST ISSUES online back to 2009 Visit us on Facebook – Baton Rouge Astronomical Society Newsletter of the Baton Rouge Astronomical Society February 2019 © 2019 President’s Message The highlight of January was the Total Lunar Eclipse 20/21 January 2019. There was a great turn out at HRPO, and it was a lot of fun. If any of the members wish to volunteer at HRPO, please speak to Chris Kersey, BRAS Liaison for BREC, to fill out the paperwork. MONTHLY SPEAKERS: One of the club’s needs is speakers for our monthly meetings if you are willing to give a talk or know of a great speaker let us know. UPCOMING BRAS MEETINGS: Light Pollution Committee - HRPO, Wednesday, February 6, 6:15 P.M. Business Meeting – HRPO, Wednesday, February 6, 7 P.M. Monthly Meeting – HRPO, Monday, February 11, 7 P.M. VOLUNTEERS: While BRAS members are not required to volunteer, if we do grow our volunteer core in 2019 we can do more fun activities without wearing out our great volunteers. Volunteering is an excellent opportunity to share what you know while increasing your skills. -
Annual Report 2009 ESO
ESO European Organisation for Astronomical Research in the Southern Hemisphere Annual Report 2009 ESO European Organisation for Astronomical Research in the Southern Hemisphere Annual Report 2009 presented to the Council by the Director General Prof. Tim de Zeeuw The European Southern Observatory ESO, the European Southern Observa tory, is the foremost intergovernmental astronomy organisation in Europe. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. Several other countries have expressed an interest in membership. Created in 1962, ESO carries out an am bitious programme focused on the de sign, construction and operation of power ful groundbased observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world View of the La Silla Observatory from the site of the One of the most exciting features of the class observing sites in the Atacama 3.6 metre telescope, which ESO operates together VLT is the option to use it as a giant opti with the New Technology Telescope, and the MPG/ Desert region of Chile: La Silla, Paranal ESO 2.2metre Telescope. La Silla also hosts national cal interferometer (VLT Interferometer or and Chajnantor. ESO’s first site is at telescopes, such as the Swiss 1.2metre Leonhard VLTI). This is done by combining the light La Silla, a 2400 m high mountain 600 km Euler Telescope and the Danish 1.54metre Teles cope. -
The Universe
The Universe Page | 2 INDEX Contents Pg 1) The universe 4 2) History of the universe 6 3) Maps of the universe 7 4) Galaxies 15 5) Stars 18 6) Neutron stars and black holes 21 7) Constellations 23 8) Time travel 27 9) Satellites and rockets 31 10) The Milky Way Galaxy 35 11) The Solar System 37 12) Exoplanets 51 13) The end of the Earth, the Solar System and the Universe 53 Page | 3 The Universe The universe is everything we know that exists like us humans, the planets, the stars, the galaxies etc. The universe has a possibly infinite volume, due to its expansion. (To see how big the universe is, check Maps on Page 7). There are probably at least 100 billion galaxies known to man in the universe, and about 300 sextillion stars. The diameter of the known universe is at least 93 billion light years (1 light year = 9.46×1012 kilometers or 9.46×1015 meters) or 8.80×1026 meters. According to General Theory of Relativity, space expands faster than the speed of light. Due to this rapid expansion, it is not brief whether the size of the universe is finite or infinite. The expansion of the Universe is due to presence of dark energy, which is found to be 73% and dark matter (23%). There is only 4% matter found. However, even though the universe is huge and massive, it has a very small density of 9.9 ×10-30 gm per cubic centimeters (excluding stars, planets and any other celestial body). -
Horizontal Branch – Helium Core-Burning Main Sequence • Ascent of the Asymptotic Giant Branch • Mass Loss • Planetary Nebulae • White Dwarfs
Structure and Evolution of Stars Lecture 17: Post-Main Sequence Evolution of Intermediate Mass Stars ~0.7-2Msun • Exhaustion of core Hydrogen fuel on main sequence • Shell Hydrogen-burning source • Ascent of the red giant branch • Ignition of Helium burning in core - Helium flash • Horizontal Branch – Helium core-burning main sequence • Ascent of the asymptotic giant branch • Mass Loss • Planetary Nebulae • White Dwarfs Structure & Evolution of Stars 1 Post-Main Sequence Evolution • Zero age main sequence (ZAMS) populated according to the initial mass function (IMF). Location on ZAMS depends only on the mass and composition of the star • Energy source from nuclear burning: - p-p chain dominant for stars with M<1.5Msun - CNO cycle dominant at increasingly higher masses • Consider evolution of a ~1Msun star – similar behaviour for mass range ~0.7-2Msun • As core hydrogen burning procedes, mass fractions, X→0 and Y→1 in the core • For stars of mass < 2Msun, the central temperature is not high enough to initiate helium burning and an inert He core of increasing mass grows Structure & Evolution of Stars 2 Sun Mass = 2 × 1030kg Radius = 7 × 108m L = 3.9 × 1026W T = 5800K SOHO image at 304A Structure & Evolution of Stars 3 Structure & Evolution of Stars 4 Post-Main Sequence Evolution: ~1Msun Star • Lifetime from consideration of energy released via fusion of H to 10 He (Lecture 11) and core mass of ~10% of total gives τms≈10 yr • Devoid of energy source the core contracts with ρ and T increasing as gravity winning without a source of energy • T and ρ in shell surrounding the He-core increases and H-burning begins in the shell - shell-burning phase. -
Spectroscopic Time-Series Analysis of R Canis Majoris?,?? H
A&A 615, A131 (2018) https://doi.org/10.1051/0004-6361/201629914 Astronomy & © ESO 2018 Astrophysics Spectroscopic time-series analysis of R Canis Majoris?;?? H. Lehmann1, V. Tsymbal2, F. Pertermann1, A. Tkachenko3, D. E. Mkrtichian4, and N. A-thano4 1 Thüringer Landessternwarte Tautenburg, Sternwarte 5, 07778 Tautenburg, Germany e-mail: [email protected]; [email protected] 2 Crimean Federal University, Vernadsky av. 4, 295007 Simferopol, Crimea 3 KU Leuven, Instituut voor Sterrenkunde, Celestijnenlaan 200, 3001 Leuven, Belgium e-mail: [email protected] 4 National Astronomical Research Institute of Thailand, 260 Moo 4, T. Donkaev, A. Maerim, Chiang Mai 50180, Thailand Received 17 October 2016 / Accepted 29 March 2018 ABSTRACT R Canis Majoris is the prototype of a small group of Algol-type stars showing short orbital periods and low mass ratios. A previous detection of short-term oscillations in its light curve has not yet been confirmed. We investigate a new time series of high-resolution spectra with the aim to derive improved stellar and system parameters, to search for the possible impact of a third component in the observed spectra, to look for indications of activity in the Algol system, and to search for short-term variations in radial velocities. We disentangled the composite spectra into the spectra of the binary components. Then we analysed the resulting high signal-to- noise spectra of both stars. Using a newly developed program code based on an improved method of least-squares deconvolution, we were able to determine the radial velocities of both components also during primary eclipse. -
President's Message
President’s Message Wow, what a month February has been! LIGO announced, on February 11th, that they had detected and measured gravity waves! What a breakthrough for physics and astrophysics. Dr. Amber Stuver, of LSU and LIGO Livingston, was the speaker at HRPO on Friday, Feb. 19th, during the public talk about this discovery. The guest speaker for the April 11th BRAS meeting will be Dr. Joseph Giaime, LSU professor of Physics and Astronomy, and the LIGO Livingston Observatory head. On December 3, 2015, the European Space Agency (ESA) launched the LISA Pathfinder mission, a space experiment to test and work out the procedures to observe lower frequency gravitational waves (lower than the waves detected by LIGO) emitted by different astronomical sources, such as the merging of super-massive black holes at the center of large galaxies. LISA Pathfinder has started its science mode, testing methods that are to be used in the L3 mission of ESA (a gravitational observatory to measure distortions in the fabric of space-time on the inconceivably tiny scale of a few millionths of a meter over a distance of a million kilometers). April 6th through April 10th is our annual Hodges Gardens Star Party. You can pre-register using the form on the BRAS website. If you have never attended this star party, make plans to attend this one. Clear Skies, and have a good March, John Nagle, BRAS President Canis Major – the Great Dog Position: RA 06 n12.5 to 07 27.5, Dec. -11.03° to -33.25° Named Stars: Sirius (Alpha CMa), “scorching”, “the Dog Star”, mag. -
A Collection of Curricula for the STARLAB Constellation Cylinder
A Collection of Curricula for the STARLAB Constellation Cylinder Including: Constellation Identification by Science First/STARLAB. A Look at the Constellations Cylinder by Joyce Kloncz Stories in the Stars by Gary D. Kratzer ©2008 by Science First/STARLAB, 95 Botsford Place, Buffalo, NY 14216. www.starlab.com. All rights reserved. Curriculum Guide Contents Constellation Identification .......................................3 Cancer (The Crab) ...........................................13 Alphabetical Listing of Constellations ........................3 Centaurus (The Centaur) ...................................14 Northern Celestial Pole Constellations .......................4 Corvus (The Crow) ..........................................14 Cassiopeia .......................................................4 Hydra (The Water Snake) .................................14 Cepheus ...........................................................4 Leo (The Lion) ..................................................15 Draco (The Dragon) ...........................................4 Lupus (The Wolf) ..............................................15 Ursa Major (The Great Bear) ..............................5 Virgo (The Virgin) ............................................15 Ursa Minor (The Little Bear) .................................5 Summer Constellations ..........................................17 Autumn Constellations .............................................6 Aquila (The Eagle) ...........................................17 Andromeda (Andromeda) ..................................6