009 Z-1 Z-2 Z-3 Z-5 Z-8 Z-9 014 015 007 003 008 002 004 010 013 005

Total Page：16

File Type：pdf, Size：1020Kb

009 Z-1 Z-2 Z-3 Z-5 Z-8 Z-9 014 015 007 003 008 002 004 010 013 005

Z-6 8 BASSEN RIFT DESSICA • 7 • XENDI SABU • ANKAA ROMULAN NEUTRAL ZONE • INFERNA MAXIA ZETA • TRILLUS PRIME • 70 VIRGINIS • • MU HERCULIS 6 FELLEBIA • • 70 OPHIUCHI BENZAR • SIGMA BOOTIS • SEGINUS • THETA SCULPTORIS • YALDALLA • • CHI HERCULIS ARCTURUS • 5 ALTAIR • BORAKA • FORMALHAUT • CALDER • • VEGA Z-5 Z-1 009 2 007 002 0044 • TYRA GLIESE 783 • PORRIMA • DRAYLAX • • TENEEBIA • NEETHIA 3 • LALANDE 25372 BARNARD’S STAR • KALEB • DENOBULA TRIAXA • ALPHA CENTAURI • 9 • LAMBDA BOOTIS BETA COMAE BERENICES • • TELLAR • BABEL SOL • ZAVIJAVA • PYRITHIA • 1 DRAKEN • PREE’NOS • UFP • Wolf 359 SIGMA DRACONIS • • KAFERIA (TAU CETI) CHI DRACONIS • VAN MAANEN’S STAR • • P ERIDANI 11 • GROOMBRIDGE 34 BARRADAS • DENEB • 10 • SIRUS AXANAR • ALKAID • 61 URSAE MAJORIS’ • • NEHRU • ANDORIA COR CAROLI • • TERRA NOVA P’JEM • 01413 CETI • 003 005 Z-8 Z-2 • ALDUS 010 VULCAN • • AZATI PRIME • MIZAR • MU CASSIOPEIAE J’RAL • XYRILLIA • DELTA LEONIS • • EPSILON SCULPTORIS • EALPHA FORNACIS THE DRACO VALE • PELIAR ZEL ROSS 47 • • AKAALI • LORILLIA • ALPHA V • TAU 1 ERIDANI • TEMECKLIA • CALDIK 47 URSAE MAJORIS • AGOSORIA NEBULA • MAB-BU • DENEVA • TRILL 12 • 36 URSAE MAJORIS ORION • 11 LEONIS MINORIS • • KOBLIAD • DRAYLON • VALAKIS • KLAESTRON • GALADOR • CHI CETI A RIGEL • • BETA RIGEL FARIUS • GALADOR CORRIDOR • IOTA PERSEI • CORIDAN TRIALAS • • THETA URSAE MAJORIS • POLLUX NAUSICAA • Z-9 Z-3 015KOTAKI • 008 006 013 • TESNIA KRESSARI • • PI 1 URSAE MAJORIS VEREX • KALANDRA • ARACNID NEBULA HANOLAN • NEW FRANCE • SIGMA CETI • • TELLUN • ESKA • TOROTH • MERAK THE TRIANGLE • CAPELLA • ALPHA TRIANGULI • MANZAR • SOLARION • DAKALA ARGOLIS CLUSTER EVORA • • RISA FEDERATION TRADE ROUTE • TOHVUN ORION TRADE ROUTE DENOBULAN TRADE Z-11ROUTE Z-10 Z-4 011 012 Z-7 LIMIT OF SUBSPACE NETWORK 1 STARBASE CASTOR • SULIBAN • SUBSPACE RELAY MAP OF KNOWN SPACE / UFP STARFLEET STELLAR CARTOGRAPHY SERVICE / 2166 ALPHA QUADRANT BETA QUADRANT BRIAR PATCH.

Copy Link

Recommended publications

Mathématiques Et Espace
Atelier disciplinaire AD 5 Mathématiques et Espace Anne-Cécile DHERS, Education Nationale (mathématiques) Peggy THILLET, Education Nationale (mathématiques) Yann BARSAMIAN, Education Nationale (mathématiques) Olivier BONNETON, Sciences - U (mathématiques) Cahier d'activités Activité 1 : L'HORIZON TERRESTRE ET SPATIAL Activité 2 : DENOMBREMENT D'ETOILES DANS LE CIEL ET L'UNIVERS Activité 3 : D'HIPPARCOS A BENFORD Activité 4 : OBSERVATION STATISTIQUE DES CRATERES LUNAIRES Activité 5 : DIAMETRE DES CRATERES D'IMPACT Activité 6 : LOI DE TITIUS-BODE Activité 7 : MODELISER UNE CONSTELLATION EN 3D Crédits photo : NASA / CNES L'HORIZON TERRESTRE ET SPATIAL (3 ème / 2 nde ) __________________________________________________ OBJECTIF : Détermination de la ligne d'horizon à une altitude donnée. COMPETENCES : ● Utilisation du théorème de Pythagore ● Utilisation de Google Earth pour évaluer des distances à vol d'oiseau ● Recherche personnelle de données REALISATION : Il s'agit ici de mettre en application le théorème de Pythagore mais avec une vision terrestre dans un premier temps suite à un questionnement de l'élève puis dans un second temps de réutiliser la même démarche dans le cadre spatial de la visibilité d'un satellite. Fiche élève ____________________________________________________________________________ 1. Victor Hugo a écrit dans Les Châtiments : "Les horizons aux horizons succèdent […] : on avance toujours, on n’arrive jamais ". Face à la mer, vous voyez l'horizon à perte de vue. Mais "est-ce loin, l'horizon ?". D'après toi, jusqu'à quelle distance peux-tu voir si le temps est clair ? Réponse 1 : " Sans instrument, je peux voir jusqu'à .................. km " Réponse 2 : " Avec une paire de jumelles, je peux voir jusqu'à ............... km " 2. Nous allons maintenant calculer à l'aide du théorème de Pythagore la ligne d'horizon pour une hauteur H donnée.
[Show full text]
Where Are the Distant Worlds? Star Maps
W here Are the Distant Worlds? Star Maps Abo ut the Activity Whe re are the distant worlds in the night sky? Use a star map to find constellations and to identify stars with extrasolar planets. (Northern Hemisphere only, naked eye) Topics Covered • How to find Constellations • Where we have found planets around other stars Participants Adults, teens, families with children 8 years and up If a school/youth group, 10 years and older 1 to 4 participants per map Materials Needed Location and Timing • Current month's Star Map for the Use this activity at a star party on a public (included) dark, clear night. Timing depends only • At least one set Planetary on how long you want to observe. Postcards with Key (included) • A small (red) flashlight • (Optional) Print list of Visible Stars with Planets (included) Included in This Packet Page Detailed Activity Description 2 Helpful Hints 4 Background Information 5 Planetary Postcards 7 Key Planetary Postcards 9 Star Maps 20 Visible Stars With Planets 33 © 2008 Astronomical Society of the Pacific www.astrosociety.org Copies for educational purposes are permitted. Additional astronomy activities can be found here: http://nightsky.jpl.nasa.gov Detailed Activity Description Leader’s Role Participants’ Roles (Anticipated) Introduction: To Ask: Who has heard that scientists have found planets around stars other than our own Sun? How many of these stars might you think have been found? Anyone ever see a star that has planets around it? (our own Sun, some may know of other stars) We can’t see the planets around other stars, but we can see the star.
[Show full text]
Download the Search for New Planets
“VITAL ARTICLES ON SCIENCE/CREATION” September 1999 Impact #315 THE SEARCH FOR NEW PLANETS by Don DeYoung, Ph.D.* The nine solar system planets, from Mercury to Pluto, have been much-studied targets of the space age. In general, a planet is any massive object which orbits a star, in our case, the Sun. Some have questioned the status of Pluto, mainly because of its small size, but it remains a full-fledged planet. There is little evidence for additional solar planets beyond Pluto. Instead, attention has turned to extrasolar planets which may circle other stars. Intense competition has arisen among astronomers to detect such objects. Success insures media attention, journal publication, and continued research funding. The Interest in Planets Just one word explains the intense interest in new planets—life. Many scientists are convinced that we are not alone in space. Since life evolved on Earth, it must likewise have happened elsewhere, either on planets or their moons. The naïve assumption is that life will arise if we “just add water”: Earth-like planet + water → spontaneous life This equation is falsified by over a century of biological research showing the deep complexity of life. Scarcely is there a fact more certain than that matter does not spring into life on its own. Drake Equation Astronomer Frank Drake pioneered the Search for ExtraTerrestrial Intelligence project, or SETI, in the 1960s. He also attempted to calculate the total number of planets with life. The Drake Equation in simplified form is: Total livable Probability of Planets with planets x evolution = evolved life *Don DeYoung, Ph.D., is an Adjunct Professor of Physics at ICR.
[Show full text]
Naming the Extrasolar Planets
Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, Königstuhl 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.
[Show full text]
400 Years of Women in Science Review by Andrew W
National Capital Astronomers, Inc. Phone: 301/565-3709 Volume 56, Number I September, 1997 ISSN 0898-7548 A biography Alan P. Boss is a staff member at the Carnegie Institution of Washington's Department of Terrestrial Magnetism Abstract highly eccentric orbits are a clue to their (DTM) in northwest Washington, D.C. Searches for extrasolar planets and origin as stars rather than as planets. Boss received his Ph.D. in physics from brown dwarfs have a long and dismal Giant planets must form in the relatively the University of California, Santa Bar- history. HowevAr r"-of discoveries cool, outer regions of protoplanetary bara, in 1979. He spent two years as a have . the advent of an era of disks, which is why the discovery of postdoctoral fellow at NASA's Ames ~ ..----tfi'SCovery of extrasolar planetary sys- several giant planets with circular orbits Reseach Center in California before tems. The newly discovered objects ap- very close to their central stars was a joining the staff ofDTM in 1981. Boss's pear to be a mixture of gas giant planets, shock to theorists. These discoveries research focuses on using three dimen- similar to Jupiter, and brown dwarf have forced theorists to accept the fact sional hydrodynamics codes to model stars, elusive objects that have long been that some planets must migrate inwards the formation of stars and planetary sys- hypothesized to exist but never seen from their place of birth toward their tems. He has been helping NASA plan before. Brown dwarf stars are interme- central star. This inward migration ap- its search for extrasolar planets ever diate in mass between giant planets and pears to have been negligible for our since 1988, and continues to be acti ve in the lowest mass stars that can burn hy- solar system, however.
[Show full text]
Arxiv:0809.1275V2
How eccentric orbital solutions can hide planetary systems in 2:1 resonant orbits Guillem Anglada-Escudé1, Mercedes López-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.
[Show full text]
Today in Astronomy 106: Exoplanets
Today in Astronomy 106: exoplanets The successful search for extrasolar planets Prospects for determining the fraction of stars with planets, and the number of habitable planets per planetary system (fp and ne). T. Pyle, SSC/JPL/Caltech/NASA. 26 May 2011 Astronomy 106, Summer 2011 1 Observing exoplanets Stars are vastly brighter and more massive than planets, and most stars are far enough away that the planets are lost in the glare. So astronomers have had to be more clever and employ the motion of the orbiting planet. The methods they use (exoplanets detected thereby): Astrometry (0): tiny wobble in star’s motion across the sky. Radial velocity (399): tiny wobble in star’s motion along the line of sight by Doppler shift. Timing (9): tiny delay or advance in arrival of pulses from regularly-pulsating stars. Gravitational microlensing (10): brightening of very distant star as it passes behind a planet. 26 May 2011 Astronomy 106, Summer 2011 2 Observing exoplanets (continued) Transits (69): periodic eclipsing of star by planet, or vice versa. Very small effect, about like that of a bug flying in front of the headlight of a car 10 miles away. Imaging (11 but 6 are most likely to be faint stars): taking a picture of the planet, usually by blotting out the star. Of these by far the most useful so far has been the combination of radial-velocity and transit detection. Astrometry and gravitational microlensing of sufficient precision to detect lots of planets would need dedicated, specialized observatories in space. Imaging lots of planets will require 30-meter-diameter telescopes for visible and infrared wavelengths.
[Show full text]
Binocular Double Star Logbook
Astronomical League Binocular Double Star Club Logbook 1 Table of Contents Alpha Cassiopeiae 3 14 Canis Minoris Sh 251 (Oph) Psi 1 Piscium* F Hydrae Psi 1 & 2 Draconis* 37 Ceti Iota Cancri* 10 Σ2273 (Dra) Phi Cassiopeiae 27 Hydrae 40 & 41 Draconis* 93 (Rho) & 94 Piscium Tau 1 Hydrae 67 Ophiuchi 17 Chi Ceti 35 & 36 (Zeta) Leonis 39 Draconis 56 Andromedae 4 42 Leonis Minoris Epsilon 1 & 2 Lyrae* (U) 14 Arietis Σ1474 (Hya) Zeta 1 & 2 Lyrae* 59 Andromedae Alpha Ursae Majoris 11 Beta Lyrae* 15 Trianguli Delta Leonis Delta 1 & 2 Lyrae 33 Arietis 83 Leonis Theta Serpentis* 18 19 Tauri Tau Leonis 15 Aquilae 21 & 22 Tauri 5 93 Leonis OΣΣ178 (Aql) Eta Tauri 65 Ursae Majoris 28 Aquilae Phi Tauri 67 Ursae Majoris 12 6 (Alpha) & 8 Vul 62 Tauri 12 Comae Berenices Beta Cygni* Kappa 1 & 2 Tauri 17 Comae Berenices Epsilon Sagittae 19 Theta 1 & 2 Tauri 5 (Kappa) & 6 Draconis 54 Sagittarii 57 Persei 6 32 Camelopardalis* 16 Cygni 88 Tauri Σ1740 (Vir) 57 Aquilae Sigma 1 & 2 Tauri 79 (Zeta) & 80 Ursae Maj* 13 15 Sagittae Tau Tauri 70 Virginis Theta Sagittae 62 Eridani Iota Bootis* O1 (30 & 31) Cyg* 20 Beta Camelopardalis Σ1850 (Boo) 29 Cygni 11 & 12 Camelopardalis 7 Alpha Librae* Alpha 1 & 2 Capricorni* Delta Orionis* Delta Bootis* Beta 1 & 2 Capricorni* 42 & 45 Orionis Mu 1 & 2 Bootis* 14 75 Draconis Theta 2 Orionis* Omega 1 & 2 Scorpii Rho Capricorni Gamma Leporis* Kappa Herculis Omicron Capricorni 21 35 Camelopardalis ?? Nu Scorpii S 752 (Delphinus) 5 Lyncis 8 Nu 1 & 2 Coronae Borealis 48 Cygni Nu Geminorum Rho Ophiuchi 61 Cygni* 20 Geminorum 16 & 17 Draconis* 15 5 (Gamma) & 6 Equulei Zeta Geminorum 36 & 37 Herculis 79 Cygni h 3945 (CMa) Mu 1 & 2 Scorpii Mu Cygni 22 19 Lyncis* Zeta 1 & 2 Scorpii Epsilon Pegasi* Eta Canis Majoris 9 Σ133 (Her) Pi 1 & 2 Pegasi Δ 47 (CMa) 36 Ophiuchi* 33 Pegasi 64 & 65 Geminorum Nu 1 & 2 Draconis* 16 35 Pegasi Knt 4 (Pup) 53 Ophiuchi Delta Cephei* (U) The 28 stars with asterisks are also required for the regular AL Double Star Club.
[Show full text]
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,
[Show full text]
Downloads/ Astero2007.Pdf) and by Aerts Et Al (2010)
This work is protected by copyright and other intellectual property rights and duplication or sale of all or part is not permitted, except that material may be duplicated by you for research, private study, criticism/review or educational purposes. Electronic or print copies are for your own personal, non- commercial use and shall not be passed to any other individual. No quotation may be published without proper acknowledgement. For any other use, or to quote extensively from the work, permission must be obtained from the copyright holder/s. i Fundamental Properties of Solar-Type Eclipsing Binary Stars, and Kinematic Biases of Exoplanet Host Stars Richard J. Hutcheon Submitted in accordance with the requirements for the degree of Doctor of Philosophy. Research Institute: School of Environmental and Physical Sciences and Applied Mathematics. University of Keele June 2015 ii iii Abstract This thesis is in three parts: 1) a kinematical study of exoplanet host stars, 2) a study of the detached eclipsing binary V1094 Tau and 3) and observations of other eclipsing binaries. Part I investigates kinematical biases between two methods of detecting exoplanets; the ground based transit and radial velocity methods. Distances of the host stars from each method lie in almost non-overlapping groups. Samples of host stars from each group are selected. They are compared by means of matching comparison samples of stars not known to have exoplanets. The detection methods are found to introduce a negligible bias into the metallicities of the host stars but the ground based transit method introduces a median age bias of about -2 Gyr.
[Show full text]
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.
[Show full text]
3-D Starmap 15.0 All Stars Within 15 Parsecs (50 Light-Years) of Sol
3-D Starmap 15.0 All stars within 15 parsecs (50 light-years) of Sol. Gl 815 2.0:14.9:-1.0 All units are in parsecs. (1 parsec = 3.26 light-years) 1.5 Gl 792 Stars are plotted in cartesian x,y,z coordinates. 3.2:14.7:-0.2 X-Y plane is the plane of the galaxy. Alderamin 2.3 -2.8:14.5:2.4 +x is Coreward, -x is Rimward, NN 4276 -3.9:14.4:0.4 +y is Spinward, -y is Trailing 1.2 Star data is from HYG database. 3.2 Stars circled in green are likely to host 14.0 human-habitable planets, according to 3 Eta Cephei 1.3 -1.9:13.9:2.9 the HabCat database. Gray lines link each star with its two closest neighbors. 2.9 3.0 Green lines link habitable stars with their two Hip 101516 5.7:13.5:-2.3 closest habitable neighbors. NN 4338 B GJ 1228 -4.1:13.4:-4.8 3.0 1.5:13.4:6.2 Gl 878 2.6 GJ 1270 0.4 Links are labeled with their distance in parsecs. -4.6:13.3:0.3 -1.5:13.3:-3.3 3.1 2.6 Gl 794 NN 4109 Winchell Chung: Nyrath the nearly wise 5.5:13.1:-2.3 2.0 7.0:13.1:1.5 http://www.projectrho.com/starmap.html 13.0 Gl 738 2.3 6.5:13.0:3.4 Gl 875.1 1.9 -1.2:12.9:-5.9 2.2 1.5 1.6 2.2 2.7 NN 4073 4.6:12.6:4.5 Gl 14 -6.1:12.5:-5.5 Gl 52 2.6 Gl 806 -28..6:12.4:0.3 1.3:12.4:0.2 4.4 3.8 NN 3069 BD+27°4120 2.6 Gl 813 BD+31°3767 -8.5:12.3:-2.3 2.4:12.3:-4.1 4.9:12.3:-3.55.1:12.3:0.8 BD+57°2735 -4.8:12.2:-0.7 19 Draconis -1.2:12.1:9.0 1.7 12.0 2.1 1.3 Gl 742 26 Draconis NN 4228 3.0 -2.4:11.9:5.6 -0.2:11.9:7.6 4.3:11.6.9:-7.4 1.1 2.5 3.8 1.7 2.4 1.9 35 Gamma Cephei GJ 1243 2.1 2.9 -6.4:11.6:3.6 1.9:11.6:2.1 NN 3117 2.3 NN 4040 2.8 -9.5:11.5:0.6 1.9 2.1 4.1 3.4:11.5:6.4
[Show full text]