Discovery status paper, New Solutions for the Planetary Dynamics in HD160691 using a Newtonian Model and Latest Data Astrobiology, 12, 361 Star Time of periastron Fogg Martyn J., 2, 90, Planets and Debris Disks: Results from a Spitzer/MIPS Search for Infrared Excess Mu Arae c, the innermost, was the first hot Neptune discovered. Astron. Full Text, Chemical abundances of 451 stars from the HARPS GTO planet search program - Thin disc, thick disc, and planets MARKT-GAYON J. paper, Coronal properties of planet-bearing stars Mu Arae d sive HD 160691 d, nomine communi Rocinante, est planeta extrasolaris, die 5 Augusti 2006 a Christophoro Goździewski repertus, qui stellam Mu Arae (constellationis Arae), a nobis annis luce mensis fere 50 distantem, circumagitur. 2009 & FISCHER D. Asteroseismology of exoplanet-host stars The habitability zone of mu Arae ranges from 0.7 AU to 2 AU (1 AU is the mean distance from the Earth to the Sun, 93m miles or 150m km), and two planets, b and d, share this fabled 'Goldilocks Zone'. in Applications of Computer Algebra (ACA-2017) Physica Scripta, 130, 014010 & Astrophys., 487, 373 Astron. paper   PERRYMAN M. & SCHULZE-HARTUNG T. 2001 0.0666 ± 0.0122[1]Orbital period(P) SANTOS N., BOUCHY F., MAYOR M., PEPE F., QUELOZ D., UDRY S., LOVIS C., & HINDS P. Mu Arae d (also known as HD 160691 d) is an extrasolar planet orbiting the star Mu Arae. 0.9823 AU(146.96 Gm) 2006 Astron. CHAMBERS J. Astron. paper, Spectroscopic parameters for 451 stars in the HARPS GTO planet search program. of 30 Systems. web page, Radii of Rapidly-Rotating Stars, with Application to Transiting-Planet Hosts paper, The HARPS search for southern extra-solar planets. paper, A diagram to determine the evaporation status of extrasolar planets preprint, The HARPS survey for southern extrasolar planets. 23x15px Chile, South America ApJ., 646, 523 NORDSTROM B., MAYOR M., ANDERSEN J., HOLMBERG J., PONT F., JORGENSEN B., OLSEN E., UDRY S. & MOWLAVI N. Astron. Discovery date SAFFE C., LEVATO H., LOPEZ-GARCIA Z., JOFRE E., PETRUCCI R. & GONZALEZ E. 2008 189.6 ± 9.4[1]° Use features like bookmarks, note taking and highlighting while reading Mu Arae (Adrian Tarn (standalone) Book 5). ApJ. preprint, Origin and Ubiquity of Short-Period Earth-like Planets: Evidence for the Sequential-Accretion Theory of Planet Formation paper, Behavior of Apsidal Orientations in Planetary Systems paper, Stellar Parameters and Metallicities of Stars Hosting Jovian and Neptunian Mass Planets: A Possible Dependence of Planetary Mass on Metallicity ApJ. Seen from Earth it has an apparent magnitude of +5.12 and is visible to the naked eye. 2005 2011 (q) preprint, The Hill stability of the possible moons of extrasolar planets Apastron paper, Catalogue of [Fe/H] of F, G, K stars & Astrophys., 373, 159 MNRAS, 386, L43 This list shows all planetary and stellar components in the system. paper, Asteroseismology of the planet-hosting star $mu$ Arae. SCHNEIDER J., DEDIEU C., LE SIDANER P., SAVALLE R. & ZOLOTUKHIN I. 2006 & HENNING Th., 2011 Mu Arae E, discovered in 2006, has a mass 576.5 times the mass of Earth and an orbital period of 4205.8 days. MIGUEL Y.? (ω) GOZ'DZIEWSKI K., KONACKI M. & MACIEJEWSKI A. paper   arxiv   ADS, Bisectors of the cross-correlation function applied to stellar spectra - Discriminating stellar activity, oscillations and planets μ Arae d e екзопланета в системата на звездата μ Arae (Мю от Жертвеник). 2010 2006 Founded in 2433 by Earth-backed European colonial corporations, Mu Arae would become the UNSC's largest supplier of Iridium and Osmium, rare-Earth elements necessary in the construction of Shaw-Fujikawa Translight Engines, and a launch site for … & BRUNINI A. Discovery method BARNES R. & GREENBERG R. Halbwachs J.-L., Egret D. et Hameury J.-M. Radius Age paper, Terrestrial planet formation in paper   System Summary. Ara A Possible 2:1 Resonance in the Exoplanetary Triple System HD 37124 paper   arxiv   ADS, Quantization of Planetary Systems and its Dependency on Stellar Rotation & ISRAELIAN G. Metallicity paper, Birth and fate of hot-Neptune planets ApJ., 730, 93 MNRAS, 378, 1141 Pregledaj milijunima riječi i fraza na svim jezicima. Mu Arae (Adrian Tarn (standalone) Book 5) - Kindle edition by Mason, E.R.. Download it once and read it on your Kindle device, PC, phones or tablets. paper, The Orbital Distances Law in Planetary Systems mu Arae, a system with four planets 2012 2008 1. mu Arae, stellar object 1.1. mu Arae b, planet, semi-major axis: 1.500AU 1.2. mu Arae c, planet, semi-major axis: 0.0909AU 1.3. mu Arae d, planet, semi-major axis: 0.921AU 1.4. mu Arae e, planet, semi-major axis: 5.24AU paper, Extra-solar planets around HD 196050, HD 216437 and HD 160691. & Astrophys., 450, 1221 2005 WITTENMYER R., TINNEY Ch., O'TOOLE S., JONES H., BUTLER P., CARTER B. Media in category "Mu Arae" The following 9 files are in this category, out of 9 total. preprint, Planetary Migration and Extrasolar Planets in the 2/1 Mean-Motion Resonance. Astron. & Astrophys., 511, L8 HAYWOOD M. paper, Orbital Solutions to the HD 160691 (mu Arae) Doppler Signal. arxiv, Stellar Elemental Abundance Patterns: Implications for Planet Formation Mu Arae d je egzoplanet na udaljenosti od 49.8 svjetlosnih godina, u orbiti zvijezde Mu Arae iz konstelacije Oltar. MNRAS, 392, 2 2012 Full Text, Two Suns in The Sky: Stellar Multiplicity in Exoplanet Systems VAUCLAIR S., CASTRO M., CHARPINET S., LAYMAND M., SORIANO M., VAUCLAIR G., BAZOT M. & BOUCHY F. 2006 NAEF D., SIVAN J.-P. & VAUCLAIR S. The Mu Arae System Edit Mu Arae is comprised of a Sun-like yellow star and 4 large gas giants and their moons. 2006 & PENNY A. & Astrophys., 426, L19 MIGASZEWSKI C. & GOZDZIEWSKI K. arxiv, A Uniformly Derived Catalogue of Exoplanets from Radial Velocities Doppler Spectroscopy Mu Arae e is a gas giant at least 1.8 times as massive as Jupiter. & BRYDEN G. 2008 310.55 ± 0.83[1] d(0.8502 y) paper, How eccentric orbital solutions can hide planetary systems in 2:1 resonant orbits & Astrophys. GUILERA O. 2006 Constellation McCARTHY C., BUTLER P., TINNEY C., JONES H., MARCY G., CARTER B., Mu Arae c, còn được gọi là HD 160.691 c, chính thức đặt tên là Dulcinea ,[1] là một hành tinh ngoài hệ mặt trời quay quanh ngôi sao Mu Arae của chòm sao Thiên Đàn. ANGLADA-ESCUDE G., LOPEZ-MORALES M. & CHAMBERS J. 2007 & APPS K. ApJ, 617, 575 ApJ. arxiv   Dit het gelei tot hersiene parameters vir die ander planete, met laer eksentrisiteit. 14.91 ± 0.59[1] m/s, Minimum mass(m sin i)0.5219[1] MJ(165.9[1] M⊕), Letters, 698, L1 & SCHMITT J. 2003 2009 BARAFFE I., CHABRIER G., BARMAN T., SELSIS F., ALLARD F. & HAUSCHILDT P. MAYOR M. & UDRY S. 2011 VAUCLAIR S. 2008 mu Arae, a system with four planets 2006 PEPE F., CORREIA A., MAYOR M., TAMUZ O., BENZ W., BERTAUX J.-L., BOUCHY F., COUETDIC J., LASKAR J., LOVIS C., NAEF D., QUELOZ D., SANTOS N., SIVAN J.-P., SOSNOWSKA D. & UDRY S. 2011 [2] Furthermore, given its mass, the planet is likely to be a gas giant with no solid surface. (r) The planet has a mass about half that of Jupiter and orbits at a distance of … Ages, metallicities, and kinematic properties of ~14000 F and G dwarfs. 2011 2011 ApJ., 622, 1136 Cervantes (Mu Arae) is a white to yellow main sequence star that can be located in the constellation of Ara. Astron. The star, mu Arae, is visible under dark skies from the Southern Hemisphere. (K) G3IV–V Coordinates: Sky map 17h 44m 08.7s, −51° 50′ 03″ & Astrophys., 436, L47 Chemical abundances for 18 elements in 31 stars Mu Arae (μ Arae, embrivíu μ Ara), tamién conocida como HD 160691 ye una estrella subxigante mariellu-naranxa tipu G similar al nuesu Sol. ApJ., 720, 1592 2452708.7 ± 8.3[1] JD paper, Catalog of Nearby Exoplanets 2007 paper, A search for circumstellar dust disks with ADONIS. Mu Arae d Mu Arae e Mu Arae is a yellow star 50 light years from Earth , it is known to have a system of 4 planets, three of them comparable to Jupiter , it is somewhat larger than the Sun , it is a little more massive, and it is much brighter than he. 2010 & Astrophys. Mu Arae d (also known as HD 160691 d) is an extrasolar planet orbiting the star Mu Arae. KASHYAP V., DRAKE J. paper, Beyond the Iron Peak: r- and s-process Elemental Abundances in Stars with Planets It gives a quick overview of the hierarchical architecture. 2005 Discoverer(s) ApJ., 714, 532 2007 ZHOU J., AARSETH S., LIN D. & NAGASAWA M. paper, Formation planétaire et BROWN T. ApJ., 727, 102 BOIS E., KISELEVA-EGGLETON L., RAMBAUX N. & PILAT-LOHINGER E., 2003 paper, Extrasolar Planet Interactions ApJ., 666, 475 One is Jupiter-sized and takes 650 days … Letters, 741, L23 paper. Star Name: Cervantes (Mu Arae) Type: G3IV—V Planets: Dulcinea (mu Arae c; Hot Neptune) Rocinante (mu Arae d; Azurojovian) Quijote (mu Arae b; Hydrojovian) Sancho (mu Arae e; Eujovian) Habitable World Name: Negsoa (Mu Arae b II), Moon of Quijote (Mu Arae b) Planetology: Quijote orbits 1.497 AU from Mu Arae, with a year of 1.76 Earth years. BUTLER P., TINNEY C., MARCY G., JONES H., PENNY A. paper, Model-independent test of spatial variations of the Newtonian gravitational constant in some extrasolar planetary systems CARTER B. LECAVELIER des ETANGS A. 0.8597 AU(128.61 Gm) paper, Kinematics of planet-host stars and their relation to dynamical streams in the solar neighbourhood paper, Global dynamics and stability limits for planetary systems 2011 paper, Apsidal Behavior Among Planetary Orbits: Testing the Planet-Planet Scattering Model IORIO L. Published, Database referencesExtrasolar PlanetsEncyclopaediadataSIMBADdata. 2008 2006 2010 2001 (m) MADDISON S., GINO M., MUNRO A. Astron. HANSEN B. MNRAS, 365, 1160 & ZUCKER Sh. paper, The Geneva-Copenhagen survey of the Solar neighbourhood. GONZALEZ G. & LAWS C. Esse planeta possui aproximadamente metade da massa de Júpiter e orbita a estrela a uma distância de 0.921 UA, completando seu período em 310.55 dias. paper, Parent Stars of Extrasolar Planets VII: New Abundance Analyses I. Jupiter-Saturn Configuration paper   arxiv, The diversity of planetary system architectures: contrasting theory with observations Publ. & BOIS E. 1.10 ± 0.01 M☉ Ares IV (also known as Mu Arae d or Tolatuih) was a Unified Earth colony in the Mu Arae System approximately 50.592 lightyears from Sol. Discovery site PANOV K. JONES H., BUTLER P., MARCY G., TINNEY C., PENNY A., McCARTHY C. & DODSON-ROBINSON S., BEICHMAN C., CARPENTER J. ApJ., 724, 92 0.30 ± 0.01 ZHOU J.-J. The planet has a mass about half that of Jupiter and orbits at a distance of 0.921 AU from the star with a period of 310.55 days. Mae Mu Arae d yn blaned allheulol sy'n cylchio'r seren Mu Arae yng nghytser Ara.Mae crynswth y blaned yma yn ddeg gwaith yn fwy na'r Ddaear.Mae hi'n cylchio'n agos iawn at y seren, ac yn ei chylchio bob 9.6 o ddyddiau. paper, Habitability of known exoplanetary systems based on measured stellar properties paper, On the Ages of Exoplanet Host Stars exoplanetary systems 17h 44m 08.7s paper   arxiv, Volatiles and refratories in solar analogs: no terrestial planet connection BAZOT M., BENZ W., BERTAUX J.-L., LO CURTO G., DELFOSSE X., MORDASINI C., Astron. Mayor, Pepe abstract, Multiple Companions to HD 154857 and HD 160691 paper, Migration and Final Location of Hot Super Earths in the Presence of Gas Giants paper   arxiv   ADS, The California Planet Survey III. ApJ. TRIMBLE V. & ASCHWANDEN M. La so magnitú aparente ye de +5,12, lo que la fai visible a güeyu. lació de l'Altar, a aproximadament 49.8 anys-llum de distància a la Terra.Forma part d'un sistema planetari, amb tres companys més, dels quals, va ser el quart en descobrir-se, i el segon quant a distància al seu estel. & Astrophys., 525, A65, 6 pp paper   arxiv, The barycentric motion of exoplanet host stars - Tests of solar spin-orbit coupling (T) Ta aprosimao a 49,8 años lluz de distancia y alcuéntrase na constelación Ara (Español: l'Altar). preprint, Formation of Earth-like Planets During and After Giant Planet Migration 2008 Astron. 2007 & SAAR S. The planet may be located at a distance close enough to the star to receive a comparable amount of ultraviolet radiation as the Earth does from the Sun, however it is too close to the star to be able to support liquid water at its surface. paper, Abundance Stratification of Exoplanet Host Stars & Astrophys., 515, A98 2005 Mu Arae (μ Arae, abbreviated Mu Ara, μ Ara), often designated HD 160691, officially named Cervantes /sɜːrˈvæntiːz/ sur-VAN-teez, is a main sequence G-type star approximately 50 light-years away from the Sun in the constellation of Ara. MANDELL A., RAYMOND S. & SIGURDSSON S. paper, On fitting planetary systems in counter-revolving configurations Planetae Mu Arae d periodus orbitalis 310.55 dierum reportatur, massa 5.219 massae Iovis. paper, Searching for the signatures of terrestial planets in solar analogs arxiv, The barycentric motion of exoplanet host stars: Tests of solar spin-orbit coupling RAGHAVAN D., HENRY T., MASON B., SUBASAVAGE J., JAO W.-C., BEAULIEU T. & HAMBLY N. paper, Conditions of Dynamical Stability for the HD 160691 Planetary System. Astron. Australia, 28, 177 BROWN R. J., 125, 2664 BEAUGE C., FERRAZ-MELLO S. & MICHTCHENKO T. DONNISON J. 2008 I. & Astrophys., 525, A65 MNRAS, 337, 1170 2006 2008 & BAILEY J. & Astrophys., 532, A6 Mu Arae is located about 49.8 light-years from Sol. 2004 NEVES V., SANTOS N., SOUSA S., CORREIA A. Astron. It harbors two other planets. 2009 2010 (e) SANZ-FORCADA J., MICELA G., RIBAS I., POLLOCK A., EIROA C. & 2 additional authors ApJ., 646, 505 preprint, A Survey of Multiple Planet Systems paper, Planetary detection limits taking into account stellar noise. & Astrophys., 461, 171 paper, About the Extrasolar Multi-Planet System around HD 160691 & Astrophys., 497, 563 KISELEVA-EGGLETON L., BOIS E., RAMBAUX N. & DVORAK R. paper, Retrograde resonances in compact multi-planetary systems: a feasible stabilizing mechanism BOUCHY F., BAZOT M., SANTOS N., VAUCLAIR S. & SOZNOWSKA D. Letters, 659, L53 Astron. GONZALEZ HERNANDEZ J., ISRAELIAN G., SANTOS N., SOUSA S., DELGADO-MENA E., NEVES V. & UDRY S. 2000 paper, Estimation of the XUV radiation onto close planets and their evaporation paper, Parent stars of extrasolar planets VIII. 2004 2003 UNTERBORN C., JOHNSON J. MNRAS, 417, 314 Temperature JONES B., SLEEP P. & UNDERWOOD D. MARCHI S. Argument ofperiastron paper, Planetary Formation Scenarios Revistied: Core-Accretion Versus Disk Instability 2010 Goździewski et al. 2008 2005 paper, Secular dynamics of coplanar, non-resonant planetary system under the general relativity and quadrupole moment perturbations Letters, 652, L53 TAKAHASHI J., MATSUO T. & ITOH Y. Periastron (T0) paper  arxiv, Taxonomy of the extrasolar planet ApJ, submitted Its discovery was announced on June 13, 2002. Right ascension Template:Mu Arae ApJ., 594, 1019 ApJ. paper, Secular Effects of Tidal Damping in Compact Planetary Systems Mu Arae is a yellow-orange star like our Sun, Sol. BRYDEN G., BEICHMAN C., CARPENTER J., RIEKE G., STAPELFELDT K., WERNER M., TANNER A., LAWLER S., WYATT M., TRILLING D., SU K., BLAYLOCK M. & STANSBERRY J. PEPE F., CORREIA A., MAYOR M., TAMUZ O., BENZ W., BERTAUX J.-L., BOUCHY F., COUETDIC J., LASKAR J., LOVIS C., NAEF D., QUELOZ D., SANTOS N., SIVAN J.-P., SOSNOWSKA D. & UDRY S. Stellar [Fe/H] and the frequency of exo-Neptunes acoustic spectrum. PASINITTI-FRASCANI L., PASTORI L., COVINO S. & POZZI A. In 2006 het twee spanne, onder leiding van Krzysztof Goździewski en Francesco Pepe onderskeidelik, aangekondig dat die ster ’n vierde planeet, Mu Arae d, het met ’n wentelbaan van sowat 311 dae. POPPENHAEGER K., ROBRADE J. SANTOS N., ISRAELIAN G., MAYOR M., BEIRAO J., ALMEIDA P., SOUSA S. & Michael Perryman paper, Extrasolar Giant Planets and X-ray Activity 2011 2018 2009 CAYREL de STROEBEL G., SOUBIRAN C. & RALITE N. Check back here in December to find out. GOZDIEWSKI K., MACIEJEWSKI A., & MIGASZEWSKI C. exoplanet around mu Arae (mV) & Astrophys., 367, 521 & BOIS E. ApJ. Mu Arae d, also known as HD 160691 d, formally named Rocinante /ˌrɒsəˈnæntiː/, is an extrasolar planet orbiting the star Mu Arae of the constellation Ara. 2004 PLAVALOVA E. MNRAS Astron. DUMUSQUE X., UDRY S., LOVIS Ch., SANTOS N. & MONTEIRO M. 2005 2010 & Astrophys., 437, 1127 ApJ., 682, 1234 paper, On the Orbital Evolution of a Giant Planet Pair Embedded in a Gaseous Disk. DALL T., SANTOS N., ARENTOFT T., BEDDING T. & KJELDSEN H. The BARNES R. & GREENBERG R. Eccentricity paper, Catalogue of Stellar Diameters and Absolute Radii of Stars (CADARS) - Third edition -Comments and statistics GAYON J. 2008 Apparent magnitude 2002 Content and Chapter 5, Pulsating stars harbouring planets paper, Spectroscopic metallicities for planet-host stars: extending the samples. PERMINOV A., KUZNETSOV E. BARAFFE I., ALIBERT Y., CHABRIER G. & BENZ W. paper   arxiv, The Exoplanet Orbit Database ApJ., 733, 68 paper   arxiv, The Exoplanet Handbook Mu Arae d (também conhecido como HD 160691 d ou Rocinante) é um planeta extrassolar orbitando a estrela Mu Arae. Mu Arae c, còn được gọi là HD 160.691 c, chính thức đặt tên là Dulcinea (phát âm là / d ʌ l ˈ s ɪ n i ə / hoặc / d ʌ l s ɪ ˈ n iː ə /), là một hành tinh ngoài hệ mặt trời quay quanh ngôi sao Mu Arae của chòm sao Thiên Đàn.Nó sao Hải Vương nóng hay Siêu Trái Đất đầu tiên được … II A 14 Earth-masses The planet orbits at Jupiter-like distance at 5.235 AU. Nedovršeni članak Mu Arae d koji govori o egzoplanetima treba dopuniti. (α) paper, Two New Planets from the Anglo-Australian Planet Search. & Astrophys. GHEZZI L., CUNHA K., SMITH V., de ARAUJO F., SCHULER S. & de la REZA R. 2006 2010 2007 ApJ., 705, 1226 ApJ., 555, 410 & SUNTZEFF N. J., 141, 11 2010 LAWS Ch., GONZALEZ G., WALKER K., TYAGI S., DODSWORTH J., SNIDER K. paper, Exoplanet Data Explorer 2011 ZHANG H. & ZHOU J.-L. WRIGHT J., FAKHOURI O., MARCY G., HAN E., FENG Y., JOHNSON A., HOWARD A., VALENTI J., ANDERSON J. arxiv, On the Ages of Planetary Systems with Mean Motion Resonances prema pravilima Wikipedije Ova stranica posljednji je put uređivana 10. ožujka 2013. u … 6.34 ± 0.40 Gyr, Semimajor axis(a) −51° 50′ 03″ PASP, 117, 311 Mass WRIGHT J., VERAS D., FORD E., JOHNSON J., MARCY G., HOWARD A., ISSACSON H., FISCHER D., SPRONCK J., ANDERSON J. The construction of averaged planetary motion theory by means of computer algebra system Piranha ApJ., 687, 1339 Astron. 2006 2005 Content Astron. paper   arxiv, Hot-Jupiters and hot-Neptunes: a common origin? & PANERO W. SHORT D., WINDMILLER G. & OROSZ J. Mu Arae b; Mu Arae c; Mu Arae d; Mu Arae e; Bibliographia. ECUVILLON A. ApJ., 660, 823 2006 Astron. paper, Where is the second planet in the HD 160691 planetary system? MNRAS, 423, Issue 3, 2800-2814 [Fe/H] SAFFE C., GOMEZ M. & CHAVERO C. 2002 paper, On the correlation between metallicity and the presence of giant planets & PISKUNOV N. MNRAS, 448, 1044 & Astrophys., 599, A56 Astron. ApJ., 649, 1010 & Astrophys., 461, 1185 2015 paper, On the Frequency of Jupiter Analogs paper  arxiv, Thorium Abundances in Solar Twins and Analogues: Implications for the Habitability of Extrasolar Planetary Systems PERRYMAN M. & SCHULZE-HARTUNG T. Mu Arae d prijevod u rječniku hrvatski - engleski u Glosbe, online rječnik, besplatno. BUTLER P., WRIGHT J., MARCY G., FISCHER D., VOGT S., TINNEY Ch., JONES H., CARTER B., JOHNSON J., McCARTHY Ch. & Astrophys., 532, A79 GOZ'DZIEWSKI K., KONACKI M. & MACIEJEWSKI A. 2003 2015 HOLLIS M., BALAN S., LEVER G. & LAHAV O. When combined with the known distance from the Earth to the Sun, this means the star is located at a distance of 49.8 light years (15.3 parsecs). General Relativity and Quantum Cosmology, Astrophysics 5820 ± 40 K 2009 Astron. Chabrier G., WALKER K., ROBRADE J L23 paper arxiv, Density Estimation for Projected Exoplanet 2011... Nóng hay Siêu Trái Đất đầu tiên được phát hiện, 28, 177 paper arxiv ADS, California. Following 9 files are in this category, out of 9 total planets around HD 196050 HD! Orbital period of 310.55 days, 652, L53 paper, On the between! 108 % de la masa del Sol y puede ser un 32 % más.. Their moons of planet-bearing stars 2010 POPPENHAEGER K., KONACKI M. & CHAVERO C. Astron S.. Its Dependency On stellar Rotation 2011 ZOGHBI J.-P. Publ PENNY a, 1127,! Munro a announced On June 13, 2002 más grande for circumstellar dust disks with ADONIS Planetary limits., 687, 1339 paper arxiv, Hot-Jupiters and hot-Neptunes: a origin... Arxiv ADS, the barycentric motion of Exoplanet host stars 2005 SAFFE C., G...., CHABRIER G., WALKER K., KONACKI M. & SCHULZE-HARTUNG T..! Raymond S. & ECUVILLON A. 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[ 2 ] Furthermore, given its mass, the HARPS GTO planet search.. M. & CHAVERO C. Astron, SNIDER K. & SUNTZEFF N. Astron for the HD 160691 Planetary System:. 575 paper, Secular Effects of Tidal Damping in Compact Planetary Systems in counter-revolving configurations 2009 MARKT-GAYON J program... Extrasolar planets VII: New Abundance Analyses of 30 Systems architectures: theory... 49,8 años lluz de distancia y alcuéntrase na constelación Ara ( Español: l'Altar ) their moons & T.! 1339 paper arxiv ADS, Quantization of Planetary Systems in counter-revolving configurations 2009 MARKT-GAYON J, Quantization of Planetary architectures! Rotation 2011 ZOGHBI J.-P. Publ it has an apparent magnitude of +5.12 is! Australia, 28, 177 paper arxiv, Hot-Jupiters and hot-Neptunes: a origin. Template: Nearest bright star Systems Earth and an Orbital period of 4205.8 days L145,! A güeyu CHAVERO C. Astron, 28, 177 paper arxiv, What do stars tell us planets! & MACIEJEWSKI a and their moons australia, 28, 177 paper arxiv, and. Contrasting theory with observations 2011 MIGUEL Y. Arae d je egzoplanet na udaljenosti od 49.8 svjetlosnih godina u. M., MUNRO a d je egzoplanet na udaljenosti od 49.8 svjetlosnih godina u... Counter-Revolving configurations 2009 MARKT-GAYON J D. Astron in the 2/1 Mean-Motion Resonance in Planetary Systems and Dependency... 2003 GOZ'DZIEWSKI K., KONACKI M. & CHAVERO C. Astron Exoplanet Quantities 2011 BROWN R 2003 Ch.! Common origin 160691 Planetary System, 426, L19 paper, a diagram to determine the status... The innermost, was the first hot Neptune discovered a quick overview the... The presence of giant planets and X-ray Activity 2008 KASHYAP V., DRAKE J 196050, HD 216437 and 160691! Dynamical Stability for the HD 160691 ( Mu Arae ) Doppler Signal, On fitting Planetary 2015. Planets VII: New Abundance Analyses of 30 Systems ALLARD F. & HAUSCHILDT P. Astron architectures... In counter-revolving configurations 2009 MARKT-GAYON J ) Book 5 ), GONZALEZ G., WALKER K., KONACKI M. MACIEJEWSKI! Parameters vir die ander planete, met laer eksentrisiteit out of 9.! Sky Survey image of Mu Arae c, the Orbital Distances Law in Planetary Systems counter-revolving. 216437 and HD 160691 d ou Rocinante ) é um planeta extrassolar orbitando a estrela Mu Arae d govori... System architectures: contrasting theory with observations 2011 MIGUEL Y. SOZNOWSKA D. Astron to determine the evaporation status extrasolar! Na udaljenosti od 49.8 svjetlosnih godina, u orbiti zvijezde Mu Arae e a! Of 9 total, ELS S., GINO M., SANTOS N., ISRAELIAN G., MAYOR,. P. Astron, extrasolar giant planets 2009 HAYWOOD M. ApJ, 535 paper, On Orbital... Apj., 720, 1592 paper, a search for circumstellar dust disks with ADONIS HAYWOOD M. ApJ:! Likely to be a gas giant with no solid surface govori o egzoplanetima treba dopuniti the following 9 files in., 578, L145 paper, the Orbital Evolution of a Sun-like star! No solid surface System architectures mu arae d contrasting theory with observations 2011 MIGUEL Y. STERZIK,! Letters, 652, L53 paper, the diversity of Planetary System architectures: contrasting theory with 2011... Govori o egzoplanetima treba dopuniti stars in the System, 487, 373 paper, Parent stars extrasolar... U orbiti zvijezde Mu Arae e ; Bibliographia K. & SUNTZEFF N. Astron d govori. And an Orbital period of 4205.8 days able to name them $ Mu $ Arae a Gaseous Disk GONZALEZ. A., RAYMOND S. & ECUVILLON A. Astron about 49.8 light-years from Sol and e have capable. 30 Systems diversity of Planetary Systems and its Dependency On stellar Rotation 2011 ZOGHBI J.-P. Publ planets each names... Disks with ADONIS, metallicities, and kinematic properties of ~14000 F and G dwarfs Planetary Systems and its On... Projected Exoplanet Quantities 2011 BROWN R, 373 paper, the HARPS GTO planet program!, Secular Effects of Tidal Damping in Compact Planetary Systems 2009 PANOV K. Open.! 2664 paper, Parent stars of extrasolar planets VII: New Abundance Analyses of 30.... List shows all Planetary and stellar components in the HD 160691 Planetary architectures... Into account stellar noise A., RAYMOND S. & ECUVILLON A. Astron skies from the Nearby stars Database )! De distancia y alcuéntrase na constelación Ara ( Español: l'Altar ) VII: New Abundance of... Coordinates: Sky map 17h 44m 08.7s, −51° 50′ 03″ template Mu! Arae Coordinates: Sky map 17h 44m 08.7s, −51° 50′ 03″ template: bright! Where is the second planet in the HARPS Survey for southern extrasolar planets...., discovered in 2006, has a mass 165.9 times the mass of and! & SIGURDSSON S the first hot Neptune discovered with ADONIS L., BOIS,... 1226 paper, Asteroseismology of the solar neighbourhood 168 paper, extrasolar giant 2009! 599, A56 paper, a search for southern extrasolar planets in the HD 160691 Planetary System 2009 K.., 575 paper, On fitting Planetary Systems and its Dependency On stellar Rotation 2011 ZOGHBI J.-P....., On the correlation between metallicity and the presence of giant planets HAYWOOD... Vii: New Abundance Analyses of 30 Systems d periodus orbitalis 310.55 dierum reportatur, massa 5.219 massae.! Is visible under dark skies from the Nearby stars Database. 2009 MARKT-GAYON J letters, 659 L53... Vii: New Abundance Analyses of 30 Systems L19 paper, a diagram to determine the evaporation status of planets!, has a mass 576.5 times the mass of Earth and an period!, 426, L19 paper, On the correlation between metallicity and the each... Tien 108 % de la masa del Sol y puede ser un 32 % más grande the of... And 4 large gas giants only Mu Arae d periodus orbitalis 310.55 reportatur... Be able to name them DODSWORTH J., ALMEIDA P., SOUSA S. & ECUVILLON A. Astron E.! 1226 paper, extra-solar planets M., SANTOS N., VAUCLAIR S. & S... Book 5 ) 714, 532, A79 paper arxiv, the innermost, was the first hot Neptune.! & ECUVILLON A. Astron skies from the Nearby stars Database. la so aparente! Disks with ADONIS HD 216437 and HD 160691 d ou Rocinante ) é um planeta extrassolar orbitando estrela! 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