Double Stars at the U.S. Naval Observatory
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Arxiv:0809.1275V2
How eccentric orbital solutions can hide planetary systems in 2:1 resonant orbits Guillem Anglada-Escud´e1, Mercedes L´opez-Morales1,2, John E. Chambers1 [email protected], [email protected], [email protected] ABSTRACT The Doppler technique measures the reflex radial motion of a star induced by the presence of companions and is the most successful method to detect ex- oplanets. If several planets are present, their signals will appear combined in the radial motion of the star, leading to potential misinterpretations of the data. Specifically, two planets in 2:1 resonant orbits can mimic the signal of a sin- gle planet in an eccentric orbit. We quantify the implications of this statistical degeneracy for a representative sample of the reported single exoplanets with available datasets, finding that 1) around 35% percent of the published eccentric one-planet solutions are statistically indistinguishible from planetary systems in 2:1 orbital resonance, 2) another 40% cannot be statistically distinguished from a circular orbital solution and 3) planets with masses comparable to Earth could be hidden in known orbital solutions of eccentric super-Earths and Neptune mass planets. Subject headings: Exoplanets – Orbital dynamics – Planet detection – Doppler method arXiv:0809.1275v2 [astro-ph] 25 Nov 2009 Introduction Most of the +300 exoplanets found to date have been discovered using the Doppler tech- nique, which measures the reflex motion of the host star induced by the planets (Mayor & Queloz 1995; Marcy & Butler 1996). The diverse characteristics of these exoplanets are somewhat surprising. Many of them are similar in mass to Jupiter, but orbit much closer to their 1Carnegie Institution of Washington, Department of Terrestrial Magnetism, 5241 Broad Branch Rd. -
Thursday, December 22Nd Swap Meet & Potluck Get-Together Next First
Io – December 2011 p.1 IO - December 2011 Issue 2011-12 PO Box 7264 Eugene Astronomical Society Annual Club Dues $25 Springfield, OR 97475 President: Sam Pitts - 688-7330 www.eugeneastro.org Secretary: Jerry Oltion - 343-4758 Additional Board members: EAS is a proud member of: Jacob Strandlien, Tony Dandurand, John Loper. Next Meeting: Thursday, December 22nd Swap Meet & Potluck Get-Together Our December meeting will be a chance to visit and share a potluck dinner with fellow amateur astronomers, plus swap extra gear for new and exciting equipment from somebody else’s stash. Bring some food to share and any astronomy gear you’d like to sell, trade, or give away. We will have on hand some of the gear that was donated to the club this summer, including mirrors, lenses, blanks, telescope parts, and even entire telescopes. Come check out the bargains and visit with your fellow amateur astronomers in a relaxed evening before Christmas. We also encourage people to bring any new gear or projects they would like to show the rest of the club. The meeting is at 7:00 on December 22nd at EWEB’s Community Room, 500 E. 4th in Eugene. Next First Quarter Fridays: December 2nd and 30th Our November star party was clouded out, along with a good deal of the month afterward. If that sounds familiar, that’s because it is: I changed the date in the previous sentence from October to November and left the rest of the sentence intact. Yes, our autumn weather is predictable. Here’s hoping for a lucky break in the weather for our two December star parties. -
Boceto Revista Astronomica
El eclipse de Luna del 15 de abril de 2014 - fotografía por Alejandro Blain Año 86 Número 281 Mayo 2014 Asociación Argentina Amigos de la Astronomía Editorial Telescopio Remoto 4 Hace unas semanas estaba de docente con un grupo de estudiantes Artemio Luis Fava en Quiroga y sin internet cuando me llamó Inés (que había vuelto de CASLEO) para contarme la noticia: un grupo de investigadores había Tierra a la vista... 5 detectado el modo B de polarización… lo que confirmaba las predicciones Iván David Castillo de la teoría inflacionaria del Big Bang. Dicho de otro modo ¡el Big Bang está confirmado! Y por primera vez en mucho tiempo sentí que somos MAVEN - NASA 7 polvo de estrellas. María Agostina Gangemi Si bien mi exclamación no es del todo cierta (más que haberse confirmado el Big Bang, se ha ganado seguridad en el modelo y es posible Damas del cielo 11 explicar hasta más atrás en el tiempo), creo que es el hecho científico más María Marta Do Santos importante que haya ocurrido durante mi vida y agradezco a todos los que ayudaron a poder plasmarlo en esta revista. Contamos con un interesante En el CASLEO de campaña 17 artículo del Dr. Bengochea acompañado de una historieta de PHD Inés Simone Comics de los doctores Jorge Cham y Jon Kaufman (perteneciente al grupo de investigación de BICEP2). No dejen de visitar www.phdcomics. Zoología galáctica 19 com , www.caifa.com.ar ni www.facebook.com/ParalajeCientifico Mgter. Ezequiel Koile Más cerca de nosotros, en el planeta rojo, mientras el Curiosity sigue La inflación cósmica 22 caminando en la superficie (un poco rengo y reculando) se le aproximan Dr. -
1903Aj 23 . . . 22K 22 the Asteojsomic Al
22 THE ASTEOJSOMIC AL JOUENAL. Nos- 531-532 22K . Taking into account the smallness of the weights in- concerned. Through the use of these tables the positions . volved, the individual differences which make up the and motions of many stars not included in the present 23 groups in the preceding table agree^very well. catalogue can be brought into systematic harmony with it, and apparently without materially less accuracy for the in- dividual stars than could be reached by special compu- Tables of Systematic Correction for N2 and A. tations for these stars in conformity with the system of B. 1903AJ The results of the foregoing comparisons. have been This is especially true of the star-places computed by utilized to form tables of systematic corrections for ISr2, An, Dr. Auwers in the catalogues, Ai and As. As will be seen Ai and As. In right-ascension no distinction is necessary by reference to the catalogue the positions and motions of between the various catalogues published by Dr. Auwers, south polar stars taken from N2 agree better with the beginning with the Fundamental-G at alo g ; but in decli- results of this investigation than do those taken from As, nation the distinction between the northern, intermediate, which, in turn, are quoted from the Cape Catalogue for and southern catalogues must be preserved, so far as is 1890. SYSTEMATIC COBEECTIOEB : CEDEE OF DECLINATIONS. Eight-Ascensions ; Cokrections, ¿las and 100z//xtf. Declinations; Corrections, Æs and IOOzZ/x^. B — ISa B —A B —N2 B —An B —Ai âas 100 â[is âas 100 âgô âSs 100 -
Meteor Csillagászati Évkönyv 2015
Ár: 3000 Ft 015 2 csillagászati évkönyv r meteor o e csillagászati évkönyv t e m 2015 ISSN 0866 - 2851 9 7 7 0 8 6 6 2 8 5 0 0 2 METEOR CSILLAGÁSZATI ÉVKÖNYV 2015 METEOR CSILLAGÁSZATI ÉVKÖNYV 2015 MCSE – 2014. SZEPTEMBER–NOVEMBER METEOR CSILLAGÁSZATI ÉVKÖNYV 2015 MCSE – 2014. SZEPTEMBER–NOVEMBER meteor csillagászati évkönyv 2015 Szerkesztette: Benkõ József Mizser Attila Magyar Csillagászati Egyesület www.mcse.hu Budapest, 2014 METEOR CSILLAGÁSZATI ÉVKÖNYV 2015 MCSE – 2014. SZEPTEMBER–NOVEMBER Az évkönyv kalendárium részének összeállításában közremûködött: Bagó Balázs Görgei Zoltán Kaposvári Zoltán Kiss Áron Keve Kovács József Molnár Péter Sárneczky Krisztián Sánta Gábor Szabadi Péter Szabó M. Gyula Szabó Sándor Szöllôsi Attila A kalendárium csillagtérképei az Ursa Minor szoftverrel készültek. www.ursaminor.hu Szakmailag ellenôrizte: Szabados László A kiadvány a Magyar Tudományos Akadémia támogatásával készült. További támogatóink mindazok, akik az SZJA 1%-ával támogatják a Magyar Csillagászati Egyesületet. Adószámunk: 19009162-2-43 Felelôs kiadó: Mizser Attila Nyomdai elôkészítés: Kármán Stúdió, www.karman.hu Nyomtatás, kötészet: OOK-Press Kft., www.ookpress.hu Felelôs vezetô: Szathmáry Attila Terjedelem: 23 ív fekete-fehér + 8 oldal színes melléklet 2014. november ISSN 0866-2851 METEOR CSILLAGÁSZATI ÉVKÖNYV 2015 MCSE – 2014. SZEPTEMBER–NOVEMBER Tartalom Bevezetô ................................................... 7 Kalendárium ............................................... 13 Cikkek Kiss László: A változócsillagászat újdonságai .................... 227 Tóth Imre: Az üstökösök megismerésének mérföldkövei ........... 242 Petrovay Kristóf: Az éghajlatváltozás és a Nap ................... 265 Kovács József: A kozmológiai állandótól a sötét energiáig – 100 éves az általános relativitáselmélet ...................... 280 Szabados László: A jó „öreg” Hubble-ûrtávcsô ................... 296 Kolláth Zoltán: A fényszennyezésrôl a Fény Nemzetközi Évében 311 Beszámolók Mizser Attila: A Magyar Csillagászati Egyesület 2013. -
Extrasolar Planets and Their Host Stars
Kaspar von Braun & Tabetha S. Boyajian Extrasolar Planets and Their Host Stars July 25, 2017 arXiv:1707.07405v1 [astro-ph.EP] 24 Jul 2017 Springer Preface In astronomy or indeed any collaborative environment, it pays to figure out with whom one can work well. From existing projects or simply conversations, research ideas appear, are developed, take shape, sometimes take a detour into some un- expected directions, often need to be refocused, are sometimes divided up and/or distributed among collaborators, and are (hopefully) published. After a number of these cycles repeat, something bigger may be born, all of which one then tries to simultaneously fit into one’s head for what feels like a challenging amount of time. That was certainly the case a long time ago when writing a PhD dissertation. Since then, there have been postdoctoral fellowships and appointments, permanent and adjunct positions, and former, current, and future collaborators. And yet, con- versations spawn research ideas, which take many different turns and may divide up into a multitude of approaches or related or perhaps unrelated subjects. Again, one had better figure out with whom one likes to work. And again, in the process of writing this Brief, one needs create something bigger by focusing the relevant pieces of work into one (hopefully) coherent manuscript. It is an honor, a privi- lege, an amazing experience, and simply a lot of fun to be and have been working with all the people who have had an influence on our work and thereby on this book. To quote the late and great Jim Croce: ”If you dig it, do it. -
Außerirdischen Verhält
Claus Pias Kalküle der Hoffnung Wer suchet, der findet nicht, wer aber nicht suchet, der wird gefunden. Franz Kafka Alienation Im September des Jahres 1971 veranstaltete eine Gruppe renommierter Wissenschaftler eine Tagung darüber, was wohl die Bedingungen der Entwicklung von Intelligenz auf anderen Planeten sein mögen. Einig war man sich vor allem darüber, daß die Lebensformen sehr klein sein müßten und daß sie keine Individualität oder Persönlichkeit besitzen dürften. Ein entscheidender Schritt in der Evolution, der später mit großer Wahrscheinlichkeit zum Aufbau technischer Zivilisation und zu beeindruckenden Ingenieursleistungen führen würde, wäre sicherlich die Fähigkeit der direkten elektrischen Kommunikation von Nervensystem zu Nervensystem. Denn erst so ergäbe sich die Chance einer komplexen sozialen Organisation und entstünden die unverzichtbaren Netzwerke und Muster kollektiver Intelligenz. Und daß man darüber nicht lange diskutieren muß, erschien als eine Evidenz der Ökonomie, die doch überall dort im Universum gelten sollte, wo intelligentes Leben schon entstanden ist oder noch entstehen wird. Denn wie schlecht beraten wäre die Evolution, würde sie einzelne Individuen produzieren, deren erlerntes Wissen mit jedem Todesfall unweigerlich verlorenginge? Jede kulturelle Stabilität und Nachhaltigkeit beruhe schließlich auf Redundanz und der Sicherung der Kommunikation… So oder so ähnlich steht es in den Mitschriften einer Tagung vom September des Jahres 1971, auf der sich renommierte Wissenschaftler mit den Bedingungen für die Entwicklung von Intelligenz auf anderen Planeten beschäftigten.1 Die seltsame Verdopplung gehört zur besonderen Logik jener Veranstaltung, deren Diskussionen immer wieder mit den gleichen stereotypen Sätzen anfangen: „I could visualize…“, „Let us consider…“, „Let us assume…“, „Let us imagine…“, „Suppose that…“ oder einfach nur: „What if…“. -
CHROMOSPHERIC Ca Ii EMISSION in NEARBY F, G, K, and M STARS1 J
The Astrophysical Journal Supplement Series, 152:261–295, 2004 June A # 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A. CHROMOSPHERIC Ca ii EMISSION IN NEARBY F, G, K, AND M STARS1 J. T. Wright,2 G. W. Marcy,2 R. Paul Butler,3 and S. S. Vogt4 Received 2003 November 11; accepted 2004 February 17 ABSTRACT We present chromospheric Ca ii H and K activity measurements, rotation periods, and ages for 1200 F, G, K, and M type main-sequence stars from 18,000 archival spectra taken at Keck and Lick Observatories as a part of the California and Carnegie Planet Search Project. We have calibrated our chromospheric S-values against the Mount Wilson chromospheric activity data. From these measurements we have calculated median activity levels 0 and derived RHK, stellar ages, and rotation periods from general parameterizations for 1228 stars, 1000 of which have no previously published S-values. We also present precise time series of activity measurements for these stars. Subject headings: stars: activity — stars: chromospheres — stars: rotation On-line material: machine-readable tables 1. INTRODUCTION Duncan et al. (1991) published data from this program in the form of ‘‘season averages’’ of H and K line strengths from The California and Carnegie Planet Search Program has 65,263 observations of 1296 stars (of all luminosity classes) in included observations of 2000 late-type main-sequence stars at high spectral resolution as the core of its ongoing survey of the Northern Hemisphere, and later as detailed analyses of 171,300 observations of 111 stars characterizing the varieties bright, nearby stars to find extrasolar planets through precision and evolution of stellar activity in dwarf stars. -
October 2016 BRAS Newsletter
OctoberOctober 2016 2016 Issue Issue th Next Meeting: Monday, Ocbober 10 at 7PM at HRPO (2nd Mondays, Highland Road Park Observatory) What's In This Issue? President’s Message Secretary's Summary of September Meeting Outreach Report Photo Gallery Light Pollution Committee Report Recent BRAS Events Photo Gallery Recent Forum Entries 20/20 Vision Campaign Messages from the HRPO Observe The Moon Night The August Flood: How Rare Is Rare? The Spooky Spectrum Article: ASTRO SHORT: A Black Hole is Born – And Caught In The Act! Observing Notes: Scutum – The Shield, by John Nagle & Mythology Deep South Star Gaze Registration Form (Pages 18-21, print and mail) Newsletter of the Baton Rouge Astronomical Society October t 2016 President’s Message October, and it is finally getting cooler. Nightfall is coming sooner and lasting longer. The onset of the autumn and winter observing season is here. To celebrate the season, our ever-playful newsletter editor, my lovely wife Michele, has hidden the Witch’s Nebula somewhere in these pages. The first 3 members to find it (independently of course), and report their finding to me ([email protected]), will receive 3 free raffle tickets at the October meeting. Of course you must attend the meeting to participate. As we start trying to get back to some kind of normalcy after the flood, there will be many requests for outreach events. Tis the season to volunteer! The Mini-Maker Faire is coming up on October 8th, and the Stargaze at the Vacheri Library on Tuesday, Oct. 11th. Early registration for the Deep South Star Gaze is almost over. -
Robert Grant Aitken
NATIONAL ACADEMY OF SCIENCES R O B E R T G R A N T A ITKEN 1864—1951 A Biographical Memoir by W I L L I A M H. V A N D E N B O S Any opinions expressed in this memoir are those of the author(s) and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoir COPYRIGHT 1958 NATIONAL ACADEMY OF SCIENCES WASHINGTON D.C. ROBERT GRANT AITKEN December 31, 1864—October 29, 795/ BY WILLEM H. VAN DEN BOS OBERT GRANT AITKEN was born on December 31, 1864, in Jackson, R.California, and died on October 29,1951, in Berkeley, California. His father, Robert Aitken, came to America from Scotland and his mother, Wilhelmina Depinau, was the daughter of German im- migrants. His early education followed classical rather than scientific lines, as his mother wished him to enter the ministry. In 1880 he entered the Oakland High School and in 1883 Williams College, still with the ministry in view. However, he also took courses in biology and astronomy and did some work in the observatory under Truman Safrord. He graduated in 1887, but as a result of his reading he felt —though he remained a deeply religious man to the end of his days —that he could not become a preacher of the orthodox, doctrinaire theology of the day. He accepted a position as house master in the Hopkins Academy, Oakland. In 1888 Aitken married his high school classmate, Jessie L. Thomas, and accepted a position as head teacher in Livermore Col- lege, where he stayed until 1891, when he was appointed professor of mathematics in the (then) University of the Pacific. -
Astronomical Society of the Pacific 295 Notes From
ASTRONOMICAL SOCIETY OF THE PACIFIC 295 NOTES FROM PACIFIC COAST OBSERVATORIES1 Note on the Diameter of By Frank K. Edmondson The value of the diameter of Antares which is commonly given in textbooks and other places as being equal to 450 solar diameters is based on a parallax of (//0095. This seems to have been obtained by assigning to Antares the mean parallax of the Scorpio-Centaurus Cluster.2 Since both components of the proper motion of Antares agree both in magnitude and direction with nearby cluster stars, and since the radial velocity is also in agreement with cluster stars, such a procedure seems to be quite legitimate. Furthermore, Antares has a seventh magni- tude companion of spectral type Β3 which has the same proper motion as Antares. If Antares did not exist, no one would doubt that the companion is a member of the cluster. The probability that a foreground star would show such agreement of motion by accident is extremely small, and one is thus led to the con- clusion that the probability that Antares belongs to the cluster is very high. The direct determinations of parallax, however, are seri- ously out of agreement with the evidence which has been given. Professor Schlesinger has very kindly sent me the trigonometric and spectroscópic determinations. They are as follows : Observatory Parallax McCormick + 0''025 ± 0'/009 Trigonometric Yale 030 .008 Cape of Good Hope .028 .012 Mount Wilson .014 Spectroscopic Victoria .012 Lockyer .010 The values obtained by the trigonometric method are more ac- cordant among themselves than they have any business to be. -
Double Star Observations Made in 1890 with the 36 Inch
ASTRONOMISCHE NACHRICHTEN. N! 3047-48. Double Star Obserrat'ions made in 1890 with the 36inch Equatorial of the Lick Observatory. By S. 1V. Burn/znnz. 'The double star observations which follow, represent ias proved as serviceable here as elsewhere. It is certainly the principal portion of my work in this direction during :he best arrangement ever invented for use with either ;I the year 1890. Substantially all the work was done be- arge or a small telescope. It would be almost impossible tween April I and December I. On two nights of the :o get along without it in doing this class of work with week the large telescope hds been used by me for micro. .he large equatorial. When the drivingclock is attached, metrical work, when the weather on these nights has been :he movement of the eyepiece, which is nearly thirty feet favorable. A few measures have been made at other times kom the cencre of motion, is so rapid, that it is necessary, with the 12 inch, but nearly all of the measures given :very two or three minutes in some positions of the in- here were made with the great telescope. The character strument, to raise or lower the seat in order to have the of the objects selected for re-measurement was such that Dbserver in a comfortable and convenient position in using it was very desirable to. attain all the accuracy possible the micrometer, and any but a simple device of this kind by employing the more powerful instrument, and many of would be impracticable.