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And Space-Based Photometry
Mon. Not. R. Astron. Soc. 000, 1–17 (2002) Printed 5 December 2018 (MN LATEX style file v2.2) Transit analysis of the CoRoT-5, CoRoT-8, CoRoT-12, CoRoT-18, CoRoT-20, and CoRoT-27 systems with combined ground- and space-based photometry St. Raetz1,2,3⋆, A. M. Heras3, M. Fern´andez4, V. Casanova4, C. Marka5 1Institute for Astronomy and Astrophysics T¨ubingen (IAAT), University of T¨ubingen, Sand 1, D-72076 T¨ubingen, Germany 2Freiburg Institute of Advanced Studies (FRIAS), University of Freiburg, Albertstraße 19, D-79104 Freiburg, Germany 3Science Support Office, Directorate of Science, European Space Research and Technology Centre (ESA/ESTEC), Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands 4Instituto de Astrof´ısica de Andaluc´ıa, CSIC, Apdo. 3004, 18080 Granada, Spain 5Instituto Radioastronom´ıa Milim´etrica (IRAM), Avenida Divina Pastora 7, E-18012 Granada, Spain Accepted 2018 November 8. Received: 2018 November 7; in original from 2018 April 6 ABSTRACT We have initiated a dedicated project to follow-up with ground-based photometry the transiting planets discovered by CoRoT in order to refine the orbital elements, constrain their physical parameters and search for additional bodies in the system. From 2012 September to 2016 December we carried out 16 transit observations of six CoRoT planets (CoRoT-5b, CoRoT-8b, CoRoT-12b, CoRoT-18b, CoRoT-20 b, and CoRoT-27b) at three observatories located in Germany and Spain. These observations took place between 5 and 9 yr after the planet’s discovery, which has allowed us to place stringent constraints on the planetary ephemeris. In five cases we obtained light curves with a deviation of the mid-transit time of up to ∼115 min from the predictions. -
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. -
The Midnight Sky: Familiar Notes on the Stars and Planets, Edward Durkin, July 15, 1869 a Good Way to Start – Find North
The expression "dog days" refers to the period from July 3 through Aug. 11 when our brightest night star, SIRIUS (aka the dog star), rises in conjunction* with the sun. Conjunction, in astronomy, is defined as the apparent meeting or passing of two celestial bodies. TAAS Fabulous Fifty A program for those new to astronomy Friday Evening, July 20, 2018, 8:00 pm All TAAS and other new and not so new astronomers are welcome. What is the TAAS Fabulous 50 Program? It is a set of 4 meetings spread across a calendar year in which a beginner to astronomy learns to locate 50 of the most prominent night sky objects visible to the naked eye. These include stars, constellations, asterisms, and Messier objects. Methodology 1. Meeting dates for each season in year 2018 Winter Jan 19 Spring Apr 20 Summer Jul 20 Fall Oct 19 2. Locate the brightest and easiest to observe stars and associated constellations 3. Add new prominent constellations for each season Tonight’s Schedule 8:00 pm – We meet inside for a slide presentation overview of the Summer sky. 8:40 pm – View night sky outside The Midnight Sky: Familiar Notes on the Stars and Planets, Edward Durkin, July 15, 1869 A Good Way to Start – Find North Polaris North Star Polaris is about the 50th brightest star. It appears isolated making it easy to identify. Circumpolar Stars Polaris Horizon Line Albuquerque -- 35° N Circumpolar Stars Capella the Goat Star AS THE WORLD TURNS The Circle of Perpetual Apparition for Albuquerque Deneb 1 URSA MINOR 2 3 2 URSA MAJOR & Vega BIG DIPPER 1 3 Draco 4 Camelopardalis 6 4 Deneb 5 CASSIOPEIA 5 6 Cepheus Capella the Goat Star 2 3 1 Draco Ursa Minor Ursa Major 6 Camelopardalis 4 Cassiopeia 5 Cepheus Clock and Calendar A single map of the stars can show the places of the stars at different hours and months of the year in consequence of the earth’s two primary movements: Daily Clock The rotation of the earth on it's own axis amounts to 360 degrees in 24 hours, or 15 degrees per hour (360/24). -
Educator's Guide: Orion
Legends of the Night Sky Orion Educator’s Guide Grades K - 8 Written By: Dr. Phil Wymer, Ph.D. & Art Klinger Legends of the Night Sky: Orion Educator’s Guide Table of Contents Introduction………………………………………………………………....3 Constellations; General Overview……………………………………..4 Orion…………………………………………………………………………..22 Scorpius……………………………………………………………………….36 Canis Major…………………………………………………………………..45 Canis Minor…………………………………………………………………..52 Lesson Plans………………………………………………………………….56 Coloring Book…………………………………………………………………….….57 Hand Angles……………………………………………………………………….…64 Constellation Research..…………………………………………………….……71 When and Where to View Orion…………………………………….……..…77 Angles For Locating Orion..…………………………………………...……….78 Overhead Projector Punch Out of Orion……………………………………82 Where on Earth is: Thrace, Lemnos, and Crete?.............................83 Appendix………………………………………………………………………86 Copyright©2003, Audio Visual Imagineering, Inc. 2 Legends of the Night Sky: Orion Educator’s Guide Introduction It is our belief that “Legends of the Night sky: Orion” is the best multi-grade (K – 8), multi-disciplinary education package on the market today. It consists of a humorous 24-minute show and educator’s package. The Orion Educator’s Guide is designed for Planetarians, Teachers, and parents. The information is researched, organized, and laid out so that the educator need not spend hours coming up with lesson plans or labs. This has already been accomplished by certified educators. The guide is written to alleviate the fear of space and the night sky (that many elementary and middle school teachers have) when it comes to that section of the science lesson plan. It is an excellent tool that allows the parents to be a part of the learning experience. The guide is devised in such a way that there are plenty of visuals to assist the educator and student in finding the Winter constellations. -
The Kinematics of Arp 295 in H-Alpha Emission: an Interacting Galaxy
Revista Mexicana de Astronom´ıa y Astrof´ısica, 00, ??–?? () THE KINEMATICS OF ARP 295 IN Hα EMISSION: AN INTERACTING GALAXY WITH HIGHLY ASYMMETRIC ROTATION Nathan Roche,1 Received November 4, 2018; accepted November 4, 2018 RESUMEN El resumen ser´atraducido al espa˜nol por los editores. We investigate Arp 295, a pair of interacting spirals at z = 0.023, using optical spectroscopy, Hα imaging, and Hα velocity mapping with the Manchester Echelle Spectrograph. Scalelengths are rexp =5.24 for Arp 295a and 2.52 kpc for 295b. A much smaller Im galaxy, Arp 295c, is associated with the larger spiral. Arp 295b is asymmetric with the disk more extended eastwards but with the brightest star-formation regions on its western side. The spectrum of Arp 295b shows strong emission lines with [OII]3727 equivalent width 36A.˚ The total Hα luminosities of Arp 295b and Arp 295c are 4.69 × 1041 and 6.76 × 1040 ergs s−1, corresponding to star-formation −1 rates 3.7 and 0.53 M⊙yr . For Arp 295b, we measure the maximum disk rotation velocity as 252.6 ± 9.9 km s−1 and find the rotation curve is very asymmetric. The east (approaching) side has a higher radial velocity than the west with the maximum difference (at r = 5 arcsec) 88 km s−1 or a factor 1.675. ABSTRACT We investigate Arp 295, a pair of interacting spirals at z =0.023, using optical spectroscopy, Hα imaging, and Hα velocity mapping with the Manchester Echelle Spectrograph. Scalelengths are rexp = 5.24 for Arp 295a and 2.52 kpc for 295b. -
In This Exercise, You Will Learn Some of the Stars That Make up Patterns in the Sky
PHYS 1830 - Perspectives on the Universe Winter 2015 PLANETARIUM EXERCISE In this exercise, you will learn some of the stars that make up patterns in the sky. These are properly known as asterisms. Constellations, on the other hand, are defined as 88 regions or patches of sky that are officially designated by the International Astronomical Union (IAU). Constellations often contain the familiar patterns of stars that are the asterisms, but constellations are usually identified by their Latin name. For example, the asterism of the Big Dipper is contained within the constellation of Ursa Major, the Greater Bear. You will also be introduced to the astronomical coordinate system that is most commonly used to describe positions of objects in the sky: the equatorial coordinate system. Part 1: Sketching You will sketch several asterisms on a single page. Draw a line across the bottom of the page to indicate the position of the horizon. Label this line with the cardinal points. Draw a cross near the top of your sketch to represent the position of the zenith. Label this point. Lightly draw in the position of the meridian and label it. For each sketch, label the time for which the planetarium is set and record your location within the dome. Use circles to mark the relative positions of the stars. The size of the circle should reflect the relative brightness with larger circles indicating brighter stars. Use straight lines to connect the relevant stars to draw the asterism shape. Sketch #1: Big Dipper, Little Dipper, and Cassiopeia Label the asterism/constellation name. -
Winter Constellations Orion
Night Sky 101: Winter Constellations Orion Orion is possibly the most well-known constellation, apart from The Big and Little Dipper. Easily recognizable by the three bright stars that form the “belt of Orion,” the constellation is, in reality, much larger. The two brightest stars in Orion are called Betelgeuse and Rigel. Betelgeuse has a distinct red tint, which makes it easy to tell them apart. Betelgeuse may soon go completely supernova. Astronomers suspect that this supernova will not affect the Earth, but may cause a double shadow to be cast on the Earth’s surface for up to two weeks. Orion is identified as the hunter by the Greeks. According to the myth, Orion was the son of the god Posiedon and Euryale, queen of the Amazons. Orion inherited his mothers talents and became the greatest hunter in the whole world. However, he boasted about this repeatedly, and was killed by a small scorpion (Scorpius), who stung him on the ankle. Canis Major and Canis Minor According to Greek mythology, Canis Major and Minor represent Orion’s faithful hunting companions. Canis Major appears to be chasing the rabbit constellation, Lepus, in the night sky. Canis Major is home to the sky’s brightest star, Sirius, also called “The Dog Star.” Sirius is a blue star, but appears to be many different colors and has been repeatedly mistaken as a UFO. One of the most unique celestial objects in Canis Major is the colliding spiral galaxies, NGC 2207 and IC 2163. The larger galaxy is in the process of pulling stars and remaining material from the smaller galaxy. -
Startheater 3 Man
AGES 8+ 2009 ® Planetarium Projector with Astronomy Software Instruction Manual Table of Contents Discover the Universe! .......................................................................................................3 Your Own Planetarium ......................................................................................................3 What Is a Constellation? ....................................................................................................3 The Star Sphere ....................................................................................................................4 Assembly and Operation ..................................................................................................4 Installing Batteries .......................................................................................................4 Operating Your Planetarium ....................................................................................5 Setting the Date and Time ........................................................................................6 Care and Maintenance.......................................................................................................6 Meteors and Comets ..........................................................................................................7 The Constellations...............................................................................................................7 The Moving Sky..................................................................................................................10 -
Maui Stargazing Observing List
MAUI STARGAZING OBSERVING LIST FEBRUARY TELESCOPE OBJECTS FEBRUARY LASER POINTER OBJECTS GALAXIES ASTERISMS M 31 (Andromeda) Belt (Orion) M 32 (Andromeda) Big Dipper (Ursa Major (Rising) M 33 Pinwheel (Triangulum) Great Square (Pegasus) M 81 (Ursa Major) Guardians of the Pole (Ursa Minor) M 82 Ursa Major) Milk Dipper (Orion) M 101 (Andromeda) Little Dipper (Ursa Minor) Shield (Orion) MUTLIPLE STAR SYSTEM Sickle (Leo) Castor (Gemini) Sword (Orion) W or M or Chair (Cassiopeia) BRIGHT NEBULAE Winter Circle M 1 Crab (Taurus) Winter Triangle M 42 Orion (Orion) CONSTELLATIONS GLOBULAR STAR CLUSTER Andromeda (Chained Maiden) M 79 (Lepus) Aries (Ram) Auriga (Charioteer) OPEN STAR CLUSTERS Cancer (Crab) Caldwell 41 Hyades (Taurus) (Bare Eye) Canis Major (Big Dog) M 38 Starfish (Auriga) Canis Minor (Little Dog) M 41 Heart of the Dog (Canis Major) Cassiopeia (Queen of Ethiopia) M 44 Beehive (Cancer) Cepheus (King of Ethiopia) M 45 Pleiades (Taurus) Cetus (Whale) NGC 869 Double Cluster (Perseus) Columba (Dove) NGC 884 Double Cluster (Perseus) Eridanus (River) NGC 1976 Trapezuim (Orion) Hydra (Water Snake) rising NGC 7789 Caroline’s Rose (Cassiopeia) Leo (Lion) rising Lepus (Hare) BARE EYE OBJECTS Orion (Hunter) Rising Satellites and Meteor Showers! Pegasus (Flying Horse) Perseus (Hero) FIRST MAGNITUDE STARS Taurus (The Bull) Achernar (Eridanus) Triangulum (Triangle) Aldebaran (Taurus) Ursa Major (Big Bear) Betelgeuse (Orion) Ursa Minor (Little Bear) Bellatrix (Orion) Capella (Auriga the Charioteer) Canopus (Carinae the Keel) Pollux (Gemini) Procyon (Canis Minor) Regulus (Leo) Rigel (Orion) Sirius (Canis Major) . -
September 2020 BRAS Newsletter
A Neowise Comet 2020, photo by Ralf Rohner of Skypointer Photography Monthly Meeting September 14th at 7:00 PM, via Jitsi (Monthly meetings are on 2nd Mondays at Highland Road Park Observatory, temporarily during quarantine at meet.jit.si/BRASMeets). GUEST SPEAKER: NASA Michoud Assembly Facility Director, Robert Champion What's In This Issue? President’s Message Secretary's Summary Business Meeting Minutes Outreach Report Asteroid and Comet News Light Pollution Committee Report Globe at Night Member’s Corner –My Quest For A Dark Place, by Chris Carlton Astro-Photos by BRAS Members Messages from the HRPO REMOTE DISCUSSION Solar Viewing Plus Night Mercurian Elongation Spooky Sensation Great Martian Opposition Observing Notes: Aquila – The Eagle Like this newsletter? See PAST ISSUES online back to 2009 Visit us on Facebook – Baton Rouge Astronomical Society Baton Rouge Astronomical Society Newsletter, Night Visions Page 2 of 27 September 2020 President’s Message Welcome to September. You may have noticed that this newsletter is showing up a little bit later than usual, and it’s for good reason: release of the newsletter will now happen after the monthly business meeting so that we can have a chance to keep everybody up to date on the latest information. Sometimes, this will mean the newsletter shows up a couple of days late. But, the upshot is that you’ll now be able to see what we discussed at the recent business meeting and have time to digest it before our general meeting in case you want to give some feedback. Now that we’re on the new format, business meetings (and the oft neglected Light Pollution Committee Meeting), are going to start being open to all members of the club again by simply joining up in the respective chat rooms the Wednesday before the first Monday of the month—which I encourage people to do, especially if you have some ideas you want to see the club put into action. -
Star Wheel Questions Set the Star Wheel for 9Pm on November 1St
Star Wheel Questions Set the star wheel for 9pm on November 1st. the edges of the star window are where the sky meets the ground. This is called the horizon. 1. What constellation is near the northern horizon? (Ursa Major, Bootes) 2. What constellation is near the eastern horizon? (Orion, Eridanus) The center of the star wheel is the top of the sky, over your head. 3. Name two constellations that are near the top of the sky. (Cassiopeia, Cepheus, Andromeda) On the star wheel, bigger stars appear brighter in the sky. 4. Which constellation would be easier to see because it has more bright stars: Cassiopeia or Cepheus? (Cassiopeia) 5. Planets are not shown on the star wheel. Why not? (because they change positions over time) Now set the star wheel for midnight on March 15. 6. Where in the sky would you look to see Canis Major? (near the western horizon) 7. Look toward the east. What constellation is about halfway between the horizon and the top of the sky in the east? (Corona Borealis (best answer) also Hercules, Bootes) The lines connecting the stars give us an idea about which stars belong to a constellation, and offer a pattern for us to look for in the sky. Each star pattern is supposed to represent a person, object or animal. For instance, Leo is supposed to be a lion. You also may have noticed that some constellations are bigger than others. 8. What constellation in the southern sky is the largest? (Hydra) 9. What is a small constellation in the southern sky? (Corvus, Canis Minor) 10. -
Publications of the Astronomical Society of the Pacific 102: 59-76, January 1990
Publications of the Astronomical Society of the Pacific 102: 59-76, January 1990 THE SPECTRUM OF NGC 7027 CHARLES D. KEYES AND L. H. ALLER Department of Astronomy, University of California, Los Angeles, California 90024 AND W. A. FEIBELMAN Laboratory for Astronomy and Solar Physics, NASA-Goddard Space Flight Center, Greenbelt, Maryland 20771 Received 1989 August 10, ABSTRACT NGC 7027 is the brightest planetary nebula (PN) in the sky despite the fact that it is dimmed by 14 db (i.e., about 3.5 magnitudes) of local and interstellar extinction. It is also one of the intrinsically most dense and luminous of PN, although it may have evolved from a progenitor in the 1.5-5 SKq range. Observations secured with the Hamilton echelle spectrograph at Lick Observatory and with the IUE are analyzed to obtain nebular plasma diagnostics and chemical abundances. Much of the 3 nebular plasma seems to have a density Ne ~ 60,000 cm and temperature Te ~ 14,000 K, although 3 the [Ne iv] and [Ar iv] auroral/nebular line ratios suggest a ~ 54,000 cm and Te ^ 16,000 Κ 3 zone, while [S π] suggests a zone at Ne ^ 30,000 cm" , Te ~ 13,000 K. Nebular models based on currently available theoretical stellar fluxes for hot stars (Τ ~ 180,000 Κ to 200,000 K) predict He π X4686 too strong and [Ne v] too weak. It is suggested that the stellar radiation field is greatly enhanced shortward of 130 A because of a dense non-LTE wind. The chemical composition appears to be that of a "normal" carbon-rich object rather than that of a nitrogen-rich object such as NGC 2440, which presumably had a massive progenitor.