mu arae system

It lies in the northeastern corner (17:44:8.7-51:50:2.6, ICRS 2000.0) of Constellation Ara, the Altar -- southeast of Alpha Arae, south of Lambda Arae, southwest of Theta Arae, and northeast of Beta Arae. (See a Digitized Sky Survey image of Mu Arae from the Nearby Stars Database.) If you spot an error or if you can contribute additional data to this entry, please send an e-mail to exoplanet@hanno-rein.de. Click here to find out how. 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 UNSC Navy, Marine and Army counter-insurgency operations among the Outer Colonies and later the Covenan… RobertHeinlein We propose naming the mu Arae star RobertHeinlein in honor of the writer Robert A. Heinlein (1907-1988). The inner 9-day Neptune-mass planet around Mu Arae is not shown due to space limitations: it would be located at the edge of the disc representing the star. Mu Arae: Sterrebeeld: Altaar: Spektraaltipe: G3 IV–V Soort: Hoofreeksster: Waarnemingsdata (Epog J2000) Regte klimming: 17 h 44 m 08,70114 s: Deklinasie −51° 50′ 02.5853″ Skynmagnitude (m) 5,12 B-V-kleurindeks 0,70: U-B-kleurindeks 0,24: Besonderhede: Massa (M ☉) 1,1 Radius (R ☉) 1,36 Ligsterkte (L ☉) 1,9 Ouderdom : 6,34 Temperatuur : 5 820 Afstand : 50,6 Eienskappe: Planete: 4 Ander name: CD … 2828 ships passed through Mu Arae space, including 12 ships in the last 7 days. The equations of Selsis, Kasting et al are used to draw the inner and outer boundaries. Mu Arae is located about 49.8 light-years from Sol. Note that unless the radius has been determined through a transit observation, this is only an approximation (see Lissauer et al. 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 … It also lists the date of the last commit and the person making the changes. TIL about the Mu Arae Star System, Located 50.6 Light years from earth, its planets are all named with the theme of Don Quixote, and thus its planets are Called: Dulcinea, Rocinante, Quijote, and Sancho The recent discoveries bring the total number of known extrasolar planets around normal, sun-like stars to 193. Cervantes is a g5v main sequence star that can be located in the constellation of Ara. [1] Although the planet itself is likely to be a gas giant with no solid surface, the orbital distance of 1.497 astronomical units from its star puts it within the habitable zone of its planetary system. We chose this system, which is about 50 light years away, to mirror the length of Heinlein’s writing career. Please include the reference to the relevant scientific paper in your commit message. [8] Although the character's name is more commonly spelled Quixote in English, Quijote is the current Spanish spelling. Mu Arae (μ Arae) is a +5.15 magnitude, yellow dwarf star in the Southern Hemisphere constellation Ara 'the Altar'. The Mu Arae System Edit Mu Arae is comprised of a Sun-like yellow star and 4 large gas giants and their moons. 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.. Mu Arae is the second extrasolar system known to host four planets. Template:Mu Arae Coordinates: Sky map 17h 44m 08.7s, −51° 50′ 03″ Template:Nearest bright star systems In July 2014 the International Astronomical Union launched a process for giving proper names to certain exoplanets and their host stars. The equipment failed, the core colony Aldennia could not develop according to plan and efficiency was low. You can download the xml file corresponding to this planetary system, which is part of the Open Exoplanet Catalogue. Based on observed activity levels, the age of Mu Ara… The discovery was made by analysing variations in the star's radial velocity (measured by observing the Doppler shift of the star's spectral lines) as a result of being pulled around by the planet's gravity. It was the first ' hot Neptune ' or ' mega-Earth ' to be discovered. System Mu Arae in Elite: Dangerous - Make the most profit from here! You can also download the entire catalogue over at github. The star, also known as HD 160691 on the Henry Draper 1 catalogue, is like the Sun and only 49 light years 2 distant from Earth. [improper synthesis?] [5] The process involved public nomination and voting for the new names. To see these, head over the github or click here to directly go to the git blame output of this system. Skip Navigation. 2005 GOZ'DZIEWSKI K., KONACKI M. & MACIEJEWSKI A. This table lists all planets in the system mu Arae. NASA’s Exoplanet Exploration Program, the search for planets and life beyond our solar system. The planetary system mu Arae hosts at least 4 planets. It gives a quick overview of the hierarchical architecture. The table … Note that this is just a summary. 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. ; Mu Arae D, discovered in 2004, has a mass 165.9 times the … Dulcinea is an exoplanet in the Cervantes (Mu Arae ) system, which is located in the constellation Ara. More references to the scientific publications and comments can be found in the commit messages. The Solar System planets are shown as a comparison. Missions. He was very … The Mu Arae system consists of an inner Uranus-mass planet in a tight 9-day orbit and three massive planets, probably gas giants, on wide, near-circular orbits, which contrasts with the high-eccentricity orbits typically observed for long-period extrasolar planets. The Mu Arae System; 2 Planets, 0 Dwarf Planets, 0 Asteroids, 0 Comets, and 0 Moons (sizes are propotional to the square root of the radius) Mu Arae (μ Arae, abbreviated Mu Ara, μ Ara), often designated HD 160691, also named Cervantes, is a main sequence G-type star approximately 50 light-years away from the Sun in the constellation of Ara. This list shows all planetary and stellar components in the system. Robert A. Heinlein was a U. S. Naval Academy graduate and was retired from the U.S. Navy for health reasons. English: The outer planets of the en:Mu Arae system compared to the planets in our en:solar system. Dulcinea is an exoplanet in the Cervantes system in constellation Ara. [2] The latest models of its planetary system, which has four known planets, give a lower eccentricity orbit. Mu Arae b, often designated HD 160691 b, formally named Quijote /kiˈhoʊtiː/, is an extrasolar planet orbiting the star Mu Arae of the constellation Ara. This table lists all stars in the system mu Arae. Please consider contributing! The planet is at least one and a half times the mass of Jupiter, and its orbital period is 643.25 days. He did civilian work for the U.S. Government in WWII. an open source database of all discovered extrasolar planets, mu Ara b, HD 160691 b, HR 6585 b, Gaia DR2 5945941905576552064 b, HIP 86796 b, GJ 691.0 b, TYC 8355-436-1 b, Cervantes b, GJ 691 b, mu Ara c, HD 160691 c, HR 6585 c, Gaia DR2 5945941905576552064 c, HIP 86796 c, GJ 691.0 c, TYC 8355-436-1 c, Cervantes c, GJ 691 c, mu Ara d, HD 160691 d, HR 6585 d, Gaia DR2 5945941905576552064 d, HIP 86796 d, GJ 691.0 d, TYC 8355-436-1 d, Cervantes d, GJ 691 d, mu Ara e, HD 160691 e, HR 6585 e, Gaia DR2 5945941905576552064 e, HIP 86796 e, GJ 691.0 e, TYC 8355-436-1 e, Cervantes e, GJ 691 e, mu Ara, HD 160691, HR 6585, Gaia DR2 5945941905576552064, HIP 86796, GJ 691.0, TYC 8355-436-1, Cervantes, GJ 691. Mu Arae c, also known as HD 160691 c, formally named Dulcinea (pronounced / dʌlˈsɪniə / or / dʌlsɪˈniːə /), is an extrasolar planet orbiting the star Mu Arae of the constellation Ara. System Summary. 1 Introduction (blurb) 2 Summary 3 References 3.1 Characters 3.2 Starships and vehicles 3.3 Locations 3.4 Races and cultures 3.5 States and organizations 3.6 Ranks and titles 3.7 Technology and weapons 3.8 Other references 4 Appendices 4.1 Related stories 4.2 Timeline The da Vinci's latest mission involves bringing precious cargo to the Mu Arae system -- an entire world that, through a miraculous feat of … The following plot shows the approximate location of the planets in this system with respect to the habitable zone (green) and the size of the star (red). As a star ages, the level of activity in its chromosphere is expected to decline. MENU This continuously updated exoplanetary encyclopedia combines interactive visualizations with detailed data on all known … Mu Arae d (also known as HD 160691 d) is an extrasolar planet orbiting the star Mu Arae. Its discovery was announced on June 13, 2002. Based on the abundance of iron, it is around twice as enriched in heavy elements as our Sun, and is therefore described as metal-rich. The star's co-ordinates are: RA 17 h 44 m; Dec −51°50'. The 717 multiplanetary systems are listed below according to the star's distance from Earth. This table lists all people who have contributed to the Open Exoplanet Catalogue. (Redirected from HD 160691 b) Mu Arae b, often designated HD 160691 b, formally named Quijote / kiˈhoʊtiː /, is an extrasolar planet orbiting the star Mu Arae of the constellation Ara. Mu Arae e (also known as HD 160691 e) is one of the four extrasolar planets orbiting the star Mu Arae. This list shows all planetary and stellar components in the system. As a result, large satellites, if they exist, of the planet, could potentially support life. Based on the spectral type (G5V) of the star, the star's colour is yellow . Your system is mu Arae. The star has a radius estimated to be 31.5% greater than our Sun and is 75% more luminous. Mu Arae is a yellow-orange star like our Sun, Sol. Within the commit message, you will find a link to the scientific publication where the data is taken from. "Listening" to the star ESO PR Photo 25b/04 ESO PR Photo 25b/04 Observed Velocity Variation of mu Arae [Preview - JPEG: 440 x 400 pix - 98k] [Normal - JPEG: 879 x 800 pix - 230k] ESO PR Photo 25c/04 ESO PR Photo 25c/04 Velocity Variation of mu Arae Observed by HARPS [Preview - JPEG: 460 x 400 pix - 90k] [Normal - JPEG: 919 x 800 pix - 215k] … Quijote was the lead character of the novel El Ingenioso Hidalgo Don Quixote de la Mancha. Breakdown: Fer-de-Lance - 1 The system’s innermost planet was the first “hot Neptune or super-Earth” to be discovered. On … 2004 , 426 : L19 ... Astronomy and Astrophysics . Astronomy and Astrophysics . 1 ship passed through Mu Arae space in the last 24 hours. [6] In December 2015, the IAU announced the winning name was Quijote for this planet. Mu Arae (μ Ara, μ Arae), often referred to by its designation in the Henry Draper catalogue HD 160691, is a main sequence G-type star around 50 light-years away from Earth in the constellation of Ara Cervantes (Mu Arae) Star Facts. The colony was badly equipped, undermanned and lacked vital competence in many areas. The description is based on the spectral class. This table lists all links which are relevant to this particular system. Mu Arae e is a gas giant at least 1.8 times as massive as Jupiter. This is only an estimate, using the star's spectral type and mass. Of the 4 gas giants only Mu Arae b and e have moons capable of supporting life. Mu Arae has 4 planets: Mu Arae B, discovered in 2000, has a mass 532.7 times the mass of Earth and an orbital period of 643.25 days. An … Mu Arae is estimated to be slightly more massive than our Sun at around 1.10 solar masses. In 2156 the colony ship arrived to the Mu Arae system and triumphantly announced to mankind that the NGSAR, New Greater South Africa Republic, was founded. If you prefer to download the dataset as an ASCII tables, you might find the oec_tables repository useful. The star can be seen with the naked eye, that is, you don't need a … Date: 28 July 2007 (original upload date) Source: Transferred from to Commons by Icalanise using CommonsHelper. [3] Furthermore, it is not clear that Earth-size moons can actually be formed in the environment around a gas giant planet.[4]. The following plot shows the approximate sizes of the planets in this system Exoplanet Catalog. Cervantes Facts. ; Mu Arae C, discovered in 2004, has a mass 10.6 times the mass of Earth and an orbital period of 9.64 days. How We Find and Characterize. A 14 Earth - masses exoplanet around μ Arae. It is visible to the naked eye. Mu Arae, often referred to by its designation in the Henry Draper catalogue HD 160691, is a main sequence G-type star around 50 light-years away from Earth in the constellation of Ara. Orbital Solutions to the HD 160691 (mu Arae) Doppler Signal. 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 … The discovery of this planet was announced on December 12, 2002, and was originally thought to be on a highly eccentric orbit. ApJ., 622, 1136 paper. 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. Its host star is located in the constellation of The Altar. People. 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 Proxima Centauri, the closest star to our Solar System, has two planets (b and c) and a third unconfirmed sub-Earth.The nearest system with three or more confirmed planets is Luyten's Star, with four known.The farthest confirmed multiplanetary system is OGLE-2012-BLG-0026L, at 13,300 ly away.. … Cervantes is not part of the constellation outline but is within the borders of the constellation. All information on this page has been directly generated from this XML file. This makes mu Arae a very exciting planetary system." [7] The winning name was submitted by the Planetario de Pamplona, Spain. If you are fluent with git and github, you can also create a pull request or open an issue on the Open Exoplanet Catalogue repository. The planet is at least one and a half times the mass of Jupiter, and its orbital period is 643.25 days. In 2001, an extrasolar planet was announced by the Anglo-Australian Planet Search team, together with the planet orbiting Epsilon Reticuli. You can also view all commits contributing to this file on github. The star has a planetary system with four known planets, three of them with masses comparable to that of Jupiter. Further observations revealed the presence of a second object in the system (now d… Despite its abundance in hydrogen and helium, it is probably already becoming a subgiant, which is a problem for Mu Arae c, who is the closest planet to her, and is very close to her, … Note that this is a new feature and not all system parameters might have a reference associated with it yet. Exoplanet Exploration. On the Ages of Exoplanet Host Stars 2005 SAFFE C., GOMEZ M. & CHAVERO C. menu close modal Discovery Discoveries Dashboard. In the left column of the output you can see the commit message corresponding to each parameter. The name was later distorted into Negsoa. Please help making this catalogue better and contribute data or references! The planet, designated Mu Arae b, was thought to be in a highly eccentric orbit of around 743 days. The planet orbits at Jupiter-like distance at 5.235 AU. Coordinates: 17h 44m 08.7s, −51° 50′ 03″, El Ingenioso Hidalgo Don Quixote de la Mancha, NameExoWorlds: An IAU Worldwide Contest to Name Exoplanets and their Host Stars, Final Results of NameExoWorlds Public Vote Released, https://en.wikipedia.org/w/index.php?title=Mu_Arae_b&oldid=951389680, Articles that may contain original research from January 2016, Creative Commons Attribution-ShareAlike License, This page was last edited on 16 April 2020, at 22:37. The central star is not to scale. Its surface temperature of around 5800 K is similar to our Sun. It gives a quick overview of the hierarchical architecture. Note that if no green band is shown in the plot, then the planet's orbit is far outside the habitable zone. However, it may not receive enough ultraviolet light for abiogenesis to proceed. NASA. Please include the corrected xml file and a reference to where the new data is coming from, ideally a scientific paper. Orbital Distance (a=AUs) Orbital Period (P=years) Orbital Eccentricity (e) Orbital Inclination (i=degrees) Mass (Earths) Diameter (Earths) Density 2011b). This system was visited for the first time on EDSM by Stulli. Github or click here to directly go to the Open exoplanet catalogue by the de... Union launched a process for giving proper names to certain exoplanets and their host stars system compared to the publications... Star 's colour is yellow hierarchical architecture 717 multiplanetary systems are listed below according to and. Solar system planets are shown as a comparison shows the approximate sizes of the Open exoplanet catalogue 2828 ships through... 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