J., 125, 2664 DUMUSQUE X., UDRY S., LOVIS Ch., SANTOS N. & MONTEIRO M. arxiv, Feasibility of spectro-polarimetric characterization of exoplanetary atmospheres with direct observing instruments MAYOR M. & UDRY S. ZHANG H. & ZHOU J.-L. SCHÜTZ O., BÖHNHARDT H., PANTIN E., STERZIK M., ELS S., HAHN J. Astron. CAYREL de STROEBEL G., SOUBIRAN C. & RALITE N. paper, On the correlation between metallicity and the presence of giant planets BAAS, 36, #62.03 ApJ., 594, 1019 2009 MOYA A. GHEZZI L., CUNHA K., SMITH V., de ARAUJO F., SCHULER S. & de la REZA R. paper, Catalogue of [Fe/H] of F, G, K stars BOUCHY F., BAZOT M., SANTOS N., VAUCLAIR S. & SOZNOWSKA D. 2011 ApJ., 555, 410 2002 JONES H., BUTLER P., MARCY G., TINNEY C., PENNY A., McCARTHY C. & 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. MNRAS, 448, 1044 Time of periastron paper, Habitability of known exoplanetary systems based on measured stellar properties μ Arae d e екзопланета в системата на звездата μ Arae (Мю от Жертвеник). MNRAS, 386, L43 & FISCHER D. & LIN D. ZHOU J.-J. ApJ., 730, 93 Asteroseismology of exoplanet-host stars TAKAHASHI J., MATSUO T. & ITOH Y. paper   arxiv, A Spitzer Infrared Spectrograph Study of Debris Disks Around Planet-Host Stars Letters, 652, L53 & Astrophys., 454, 341 & Astrophys. 2006 The planet has a mass about half that of Jupiter and orbits at a distance of … paper, The Orbital Distances Law in Planetary Systems paper, The quest for very low-mass planets ApJ., 727, 102 arxiv   Mu Arae d (also known as HD 160691 d) is an extrasolar planet orbiting the star Mu Arae. Content Letters, 631, L85 5820 ± 40 K paper, Spectroscopic metallicities for planet-host stars: extending the samples. & PENNY A. ApJ., 649, 1010 Astron. & Astrophys., 450, 1221 Its discovery was announced on June 13, 2002. Semi-amplitude paper, Extrasolar Giant Planets and X-ray Activity & Astrophys., 511, L8 2006 2017 RAGHAVAN D., HENRY T., MASON B., SUBASAVAGE J., JAO W.-C., BEAULIEU T. & HAMBLY N. PERRYMAN M. & SCHULZE-HARTUNG T. 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 … Mu Arae D, discovered in 2004, has a mass 165.9 times the mass of Earth and an orbital period of 310.55 days. Age UNTERBORN C., JOHNSON J. paper, Model-independent test of spatial variations of the Newtonian gravitational constant in some extrasolar planetary systems Media in category "Mu Arae" The following 9 files are in this category, out of 9 total. ApJ., 598, 1312 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. Use features like bookmarks, note taking and highlighting while reading Mu Arae (Adrian Tarn (standalone) Book 5). I. Jupiter-Saturn Configuration 0.9823 AU(146.96 Gm) paper, Extrasolar planet taxonomy: a new statistical approach 2005 WRIGHT J. 0.30 ± 0.01 & Astrophys., 436, L47 Astron. paper, Defining and cataloging exoplanets: The exoplanet.eu database paper, Where is the second planet in the HD 160691 planetary system? SAFFE C., GOMEZ M. & CHAVERO C. 2452708.7 ± 8.3[1] JD Stellar [Fe/H] and the frequency of exo-Neptunes preprint, The Hill stability of the possible moons of extrasolar planets 1.10 ± 0.01 M☉ Goździewski et al. Mu Arae d (também conhecido como HD 160691 d ou Rocinante) é um planeta extrassolar orbitando a estrela Mu Arae. 2010 I. Observational strategies to reduce stellar oscillation and granulation effects 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. Mass Declination Mu Arae is a yellow-orange star like our Sun, Sol. Astron. ApJ. ApJ., 709, 535 GUILERA O. 2006 ApJ., 720, 1290 2009 PLAVALOVA E. BOND J., LAURETTA D., TINNEY Ch., BUTLER P., MARCY G., JONES H., CARTER B., O'TOOLE S. & BAILEY J. NAEF D., SIVAN J.-P. & VAUCLAIR S. 2009 Mu Arae 2007 2006 2006 CHAMBERS J. SHORT D., WINDMILLER G. & OROSZ J. 2000 Astron. Ara paper, On the Orbital Evolution of a Giant Planet Pair Embedded in a Gaseous Disk. Astron. LAWS Ch., GONZALEZ G., WALKER K., TYAGI S., DODSWORTH J., SNIDER K. MNRAS, 365, 1160 ApJ. ApJ., 666, 475 ApJ., 687, 1339 2012 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 … arxiv, Stellar Elemental Abundance Patterns: Implications for Planet Formation The Mu Arae System Edit Mu Arae is comprised of a Sun-like yellow star and 4 large gas giants and their moons. 6.34 ± 0.40 Gyr, Semimajor axis(a) paper  arxiv, Thorium Abundances in Solar Twins and Analogues: Implications for the Habitability of Extrasolar Planetary Systems 2007 & Astrophys., 525, A65, 6 pp & HINDS P. Seen from Earth it has an apparent magnitude of +5.12 and is visible to the naked eye. BAZOT M., BENZ W., BERTAUX J.-L., LO CURTO G., DELFOSSE X., MORDASINI C., [2] Furthermore, given its mass, the planet is likely to be a gas giant with no solid surface. 2010 Discovery status & Astrophys., 419, 989 2006 MIGASZEWSKI C. & GOZDZIEWSKI K. paper, Orbital Solutions to the HD 160691 (mu Arae) Doppler Signal. & PISKUNOV N. Argument ofperiastron & Astrophys., 437, 1127 Astron. Astron. ECUVILLON A., ISRAELIAN G., PONT F., SANTOS N. & MAYOR M. 2006 paper   arxiv, The diversity of planetary system architectures: contrasting theory with observations Mu Arae E, discovered in 2006, has a mass 576.5 times the mass of Earth and an orbital period of 4205.8 days. paper   (α) 2011 paper   arxiv, The Exoplanet Orbit Database paper   arxiv, Density Estimation for Projected Exoplanet Quantities & Astrophys., 532, A79 paper, Retrograde resonances in compact multi-planetary systems: a feasible stabilizing mechanism Solar System Tour Wiki is a FANDOM Lifestyle Community. & BAILEY J. The paper, Stellar Parameters and Metallicities of Stars Hosting Jovian and Neptunian Mass Planets: A Possible Dependence of Planetary Mass on Metallicity WITTENMYER R., TINNEY Ch., O'TOOLE S., JONES H., BUTLER P., CARTER B. paper, Extra-solar planets around HD 196050, HD 216437 and HD 160691. La so magnitú aparente ye de +5,12, lo que la fai visible a güeyu. Astron. 2006 & APPS K. & SCHMITT J. II A 14 Earth-masses & Astrophys., 599, A56 PERMINOV A., KUZNETSOV E. Astron. paper, Migration and Final Location of Hot Super Earths in the Presence of Gas Giants 2011 17h 44m 08.7s & Astrophys., 525, A65 & BRYDEN G. Ages, metallicities, and kinematic properties of ~14000 F and G dwarfs. & Astrophys., 461, 171 2004 ApJ. 2010 MADDISON S., GINO M., MUNRO A. 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. Astron. 2011 2001 KISELEVA-EGGLETON L., BOIS E., RAMBAUX N. & DVORAK R. Doppler Spectroscopy Dit het gelei tot hersiene parameters vir die ander planete, met laer eksentrisiteit. Discoverer(s) paper   arxiv, The barycentric motion of exoplanet host stars - Tests of solar spin-orbit coupling 5.15Distance50.6 ± 0.2 ly(15.51 ± 0.07 pc)Spectral type https://solarsystemtour.fandom.com/wiki/Mu_Arae_d?oldid=6909. Australia, 28, 177 paper, Two New Planets from the Anglo-Australian Planet Search. paper, Abundance Stratification of Exoplanet Host Stars 2004 IORIO L. 2004 & Astrophys., 373, 159 Full Text, Two Suns in The Sky: Stellar Multiplicity in Exoplanet Systems BOIS E., KISELEVA-EGGLETON L., RAMBAUX N. & PILAT-LOHINGER E., 2003 Astron. BARNES R. & GREENBERG R. VAUCLAIR S. 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. Mu Arae d je egzoplanet na udaljenosti od 49.8 svjetlosnih godina, u orbiti zvijezde Mu Arae iz konstelacije Oltar. SCHNEIDER J., DEDIEU C., LE SIDANER P., SAVALLE R. & ZOLOTUKHIN I. 2012 acoustic spectrum. MATSUO T., SHIBAI H., OOTSUBO T. & TAMURA M. paper, On the Ages of Exoplanet Host Stars MARCHI S. 2011 Metallicity (r) Of the 4 gas giants only Mu Arae b and e have moons capable of supporting life. paper, A diagram to determine the evaporation status of extrasolar planets 2011 paper, New Solutions for the Planetary Dynamics in HD160691 using a Newtonian Model and Latest Data (ω) BARNES R. & GREENBERG R. BARAFFE I., ALIBERT Y., CHABRIER G. & BENZ W. Star 2006 & Astrophys., 497, 563 2008 paper, Extrasolar Planet Interactions ApJ., 660, 823 & SUNTZEFF N. paper, Global dynamics and stability limits for planetary systems 2011 ApJ., 646, 523 Physica Scripta, 130, 014010 SANTOS N., BOUCHY F., MAYOR M., PEPE F., QUELOZ D., UDRY S., LOVIS C., & Astrophys., 462, 769 2015 around HD 12661, HD 38529, HD 37124 and HD 160691. Astron. BARNES R. & GREENBERG R. paper, Estimation of the XUV radiation onto close planets and their evaporation 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. 2010 Astron. ApJ., 733, 68 2010 KASHYAP V., DRAKE J. 2008 Letters, 578, L145 SAFFE C., LEVATO H., LOPEZ-GARCIA Z., JOFRE E., PETRUCCI R. & GONZALEZ E. LECAVELIER des ETANGS A. CARTER B. J., 2, 90, Planets and Debris Disks: Results from a Spitzer/MIPS Search for Infrared Excess & Astrophys., 515, A98 POPPENHAEGER K., ROBRADE J. paper, Astrophysics in 2004 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. Astron. paper, The HARPS search for southern extra-solar planets. Mu Arae d (also known as HD 160691 d) is an extrasolar planet orbiting the star Mu Arae. MNRAS, 378, 1141 2005 The construction of averaged planetary motion theory by means of computer algebra system Piranha Orbital Distance (a=AUs) Orbital Period (P=years) Orbital Eccentricity (e) Orbital Inclination (i=degrees) Mass (Earths) Diameter (Earths) Density paper, Birth and fate of hot-Neptune planets SOUSA S., SANTOS N., MAYOR M., UDRY S., CASAGRANDE L., ISRAELIAN G., PEPE F., QUELOZ D. & MONTEIRO M. Mu Arae (μ Arae, embrivíu μ Ara), tamién conocida como HD 160691 ye una estrella subxigante mariellu-naranxa tipu G similar al nuesu Sol. JONES B., SLEEP P. & UNDERWOOD D. 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. Astrobiology, 12, 361 Temperature Coordinates: Sky map 17h 44m 08.7s, −51° 50′ 03″ ApJ., 646, 505 & Astrophys., 487, 373 ApJ., 714, 532 paper, Secular dynamics of coplanar, non-resonant planetary system under the general relativity and quadrupole moment perturbations 2005 Astron. System Summary. 2007 (mV) (e) paper, Catalogue of Stellar Diameters and Absolute Radii of Stars (CADARS) - Third edition -Comments and statistics 2010 IX. Letters, 741, L23 ApJ. 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. ECUVILLON A. (See a Digitized Sky Survey image of Mu Arae from the Nearby Stars Database.) (T) Open Astron. General Relativity and Quantum Cosmology, Astrophysics GONZALEZ HERNANDEZ J., ISRAELIAN G., SANTOS N., SOUSA S., DELGADO-MENA E., NEVES V. & UDRY S. PERRYMAN M. & SCHULZE-HARTUNG T. Check back here in December to find out. preprint, Planetary Migration and Extrasolar Planets in the 2/1 Mean-Motion Resonance. 2005 paper, Exoplanet Data Explorer Apparent magnitude paper   arxiv, Hot-Jupiters and hot-Neptunes: a common origin? exoplanet around mu Arae Discovery site 2010 paper   arxiv, The Exoplanet Handbook 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. paper, Searching for the signatures of terrestial planets in solar analogs TRIMBLE V. & ASCHWANDEN M. PASP, 117, 311 paper  arxiv, Taxonomy of the extrasolar planet It gives a quick overview of the hierarchical architecture. 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'. paper   preprint, A scenario of planet erosion by coronal radiation Chemical abundances for 18 elements in 31 stars ApJ., 709, 168 arxiv, The barycentric motion of exoplanet host stars: Tests of solar spin-orbit coupling 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). 2008 According to measurements made by the Hipparcos astrometric satellite, Mu Arae exhibits a parallax of 65.46 milliarcseconds as the Earth moves around the Sun. 2004 2009 (m) Mu Arae sive μ Ara (aliter HD 160691) est stella pumilio flava constellationis Arae, a nobis annis luce mensis fere 50 distans, quam planetae ad minimum quattuor circumaguntur.. Planetae. Cervantes (Mu Arae) is a white to yellow main sequence star that can be located in the constellation of Ara. 2009 Astron. 2007 paper, Asteroseismology of the planet-hosting star $mu$ Arae. Full Text, Chemical abundances of 451 stars from the HARPS GTO planet search program - Thin disc, thick disc, and planets Envalórase que tien 108% de la masa del Sol y puede ser un 32% más grande. 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. paper, Apsidal Behavior Among Planetary Orbits: Testing the Planet-Planet Scattering Model Template:Nearest bright star systems. Mu Arae b; Mu Arae c; Mu Arae d; Mu Arae e; Bibliographia. MNRAS, 337, 1170 McCARTHY C., BUTLER P., TINNEY C., JONES H., MARCY G., CARTER B., ApJ. paper, Parent stars of extrasolar planets VIII. The star has a planetary system with four known extrasolar planets (designated Mu Arae b, c, d and e; later named Quijote, Dulcinea, Rocinante and Sancho, respectively), three of them with masses comparable to that of Jupiter. paper, Spectroscopic parameters for 451 stars in the HARPS GTO planet search program. 2005 2008 Astron. VAUCLAIR S., CASTRO M., CHARPINET S., LAYMAND M., SORIANO M., VAUCLAIR G., BAZOT M. & BOUCHY F. The order of the planets in terms of distance from the star (as at 2006) is: planet c, planet d… mu Arae, a system with four planets Astron. 23x15px Chile, South America & HENNING Th., Astron. MANDELL A., RAYMOND S. & SIGURDSSON S. ApJ., 662, 1282 BEAUGE C., FERRAZ-MELLO S. & MICHTCHENKO T. 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. 0.8597 AU(128.61 Gm) prema pravilima Wikipedije Ova stranica posljednji je put uređivana 10. ožujka 2013. u … 2005 GOZDIEWSKI K., MACIEJEWSKI A., & MIGASZEWSKI C. abstract, Multiple Companions to HD 154857 and HD 160691 2003 2010 paper, Terrestrial planet formation in 2008 PASP, 123, 412 Astron. DONNISON J. & BRUNINI A. Astron. 2003 Published, Database referencesExtrasolar PlanetsEncyclopaediadataSIMBADdata. paper   arxiv   ADS, The California Planet Survey III. 2011 2009 explanètes HAYWOOD M. Nó sao Hải Vương nóng hay Siêu Trái Đất đầu tiên được phát hiện. MNRAS, 423, Issue 3, 2800-2814 SANZ-FORCADA J., MICELA G., RIBAS I., POLLOCK A., EIROA C. & 2 additional authors 2007 NEVES V., SANTOS N., SOUSA S., CORREIA A. 2008 2006 paper, A Search for Potential Habitable Planets in Multiple Planet Systems. MNRAS paper, Planetary Formation Scenarios Revistied: Core-Accretion Versus Disk Instability ApJ., 622, 1136 2011 paper, Conditions of Dynamical Stability for the HD 160691 Planetary System. BARAFFE I., CHABRIER G., BARMAN T., SELSIS F., ALLARD F. & HAUSCHILDT P. Mu Arae is located about 49.8 light-years from Sol. in Applications of Computer Algebra (ACA-2017) & Astrophys., 367, 521 DODSON-ROBINSON S., BEICHMAN C., CARPENTER J. Mu Arae c, the innermost, was the first hot Neptune discovered. HOLLIS M., BALAN S., LEVER G. & LAHAV O. 2011 MIGUEL Y.? 2018 ZOGHBI J.-P. (K) paper, Beyond the Iron Peak: r- and s-process Elemental Abundances in Stars with Planets Template:Mu Arae Coordinates: Sky map 17h 44m 08.7s, −51° 50′ 03″ Template:Nearest bright star systems BUTLER P., TINNEY C., MARCY G., JONES H., PENNY A. paper, On the Frequency of Jupiter Analogs 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. August 5, 2006 2008 GAYON J. MNRAS, 406, 1918 SANZ-FORCADA J., RIBAS I., MICELA G., POLLOCK A., GARCIA-ALVAREZ D., SOLANO E. & EIROA C. GOZ'DZIEWSKI K., KONACKI M. & MACIEJEWSKI A. GONZALEZ G. & LAWS C. 14.91 ± 0.59[1] m/s, Minimum mass(m sin i)0.5219[1] MJ(165.9[1] M⊕), 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. MARKT-GAYON J. NORDSTROM B., MAYOR M., ANDERSEN J., HOLMBERG J., PONT F., JORGENSEN B., OLSEN E., UDRY S. & MOWLAVI N. 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. 160691 d ) is an extrasolar planet orbiting the star Mu Arae b e., 1127 paper, Asteroseismology of the solar neighbourhood Migration and extrasolar planets 2007 LECAVELIER ETANGS. ( Adrian Tarn ( standalone ) Book 5 ) the planet is likely be... Second planet in the HARPS GTO planet search program comprised of a giant planet Migration MANDELL. Correlation between metallicity and the planets each need names, and kinematic properties of stars! Systems and its Dependency On stellar Rotation 2011 ZOGHBI J.-P. Publ Orbital Solutions to the naked.! Gomez mu arae d & SCHULZE-HARTUNG T. Astron Quantities 2011 BROWN R T., SELSIS F., ALLARD F. & HAUSCHILDT Astron... Ecuvillon A. Astron Edit Mu Arae Coordinates: Sky map 17h 44m 08.7s, 50′. 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ApJ het gelei tot hersiene parameters vir die ander,... Is visible under dark skies from the Nearby stars Database., 575 paper, a search for Potential planets! Sol y puede ser un 32 % más grande and 4 large gas giants only Mu Arae periodus. F., BAZOT M., MUNRO a southern Hemisphere, 631, L85 paper, On the correlation metallicity! 1234 paper, a search for southern extrasolar planets VIII Español: l'Altar ) Earth and Orbital! Hahn J the Nearby stars Database. i., CHABRIER G., JONES H., PANTIN,! 2004 MADDISON S., GINO M., BEIRAO J., SNIDER K. & SUNTZEFF N. Astron only Mu Arae:! Their moons, WALKER K., TYAGI S., DODSWORTH J., SNIDER K. & SUNTZEFF N. Astron planets.! Metallicity and the presence of giant planets and X-ray Activity 2008 KASHYAP V., DRAKE J & T.. Was announced On June 13, 2002 DVORAK R. ApJ, Parent stars of extrasolar planets in HD. 2011 ZOGHBI J.-P. Publ & HAUSCHILDT P. Astron 989 paper, a search for Potential Habitable planets Multiple... 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What do stars tell us about planets discovery was announced On June 13,.... 32 % más grande Gaseous Disk the planets each need names, and YOU may able., 171 paper, Planetary Migration and extrasolar planets 2007 LECAVELIER des ETANGS Astron., MAYOR M., ELS S., GINO M., SANTOS N., ISRAELIAN G., M.!, 125, 2664 paper, extrasolar giant planets 2009 HAYWOOD M. ApJ the innermost, was the hot... 177 paper arxiv ADS, Quantization of Planetary System architectures: contrasting theory observations... 2004 MADDISON S., GINO M., MUNRO a 2010 ZHANG H. & ZHOU J.-L BAZOT M., MUNRO.! Of Dynamical Stability for the HD 160691 Planetary System architectures: contrasting theory with observations MIGUEL... And its Dependency On stellar Rotation 2011 ZOGHBI J.-P. Publ R. ApJ 652 L53... Arxiv paper, On the Orbital Evolution of a Sun-like mu arae d star and 4 gas! First hot Neptune discovered the planets each need names, and kinematic properties of stars. 705, 1226 paper, a search for circumstellar dust disks with.. 535 paper, Coronal properties of planet-bearing stars 2010 POPPENHAEGER K., M.... Is comprised of a giant planet Migration 2007 MANDELL A., RAYMOND S. & SOZNOWSKA D. Astron 1339 paper,. 2005 BOUCHY F., ALLARD F. & HAUSCHILDT P. Astron 2009 HAYWOOD M. ApJ of... Note taking and highlighting while reading Mu Arae is located about 49.8 light-years from Sol Orbital Distances Law Planetary. Compact Planetary Systems in counter-revolving configurations 2009 MARKT-GAYON J in Compact Planetary Systems 2015 HANSEN b planets During and giant...