HD 219134 c, also known as HR 8832 c, is a hot, dense, rocky exoplanet orbiting around the K-type star HD 219134 in the constellation of Cassiopeia.Originally thought to be a little less than three times the mass of Earth, it is now known to be over 4 times the mass and 51% larger in radius, suggesting a rocky composition with a higher quantity of iron than Earth. Cependant, sa densité est étrangement faible. HD 219134 f, còn được gọi là HR 8832 f, là một ngoại hành tinh quay quanh sao lùn cam HD 219134 (còn gọi là HR 8832) trong chòm sao Tiên Hậu. HD 219134 b (or HR 8832 b) is one of at least five exoplanets orbiting HD 219134, a main-sequence star in the constellation of exoplanets orbiting HD 219134, a main-sequence star in the constellation of Cassiopeia. It has a minimum mass of 11 Earth Masses, suggesting that it could be a high-mass ocean planet or a Neptune-like ice giant. Chỉ có một bán kính tối thiểu có thể được đưa ra. Nhiệt độ của hành tinh được tính là 411 K (138 °C; 280 °F), tương tự như của Sao Thủy. Ceci est la documentation du modèle {{Palette HD 219134}}.. Syntaxe. HD 219134 c is similar to these planets: HD 219134 d, HD 219134 f, HD 219134 e and more. HD 219134 b est une exoplanète « scintillante » d’une masse qui est presque cinq fois supérieure à celle de la Terre. It has a minimum mass of 11 Earth Masses, suggesting that it could be a high-mass ocean planet or a Neptune-like ice giant. It was subsequently shown to be the same candidate as HD 219134 h from Vogt et al. Please include the reference to the relevant scientific paper in your commit message. +57:10:06). Se situant à 21,3 années-lumière de nous, c'est l'exoplanète tellurique confirmée la plus proche jamais découverte à ce jour. Le système a été remanié en 2016 et ont ajouté de nouvelles planètes, 6 et confirmé agréable, un f, toujours pas de confirmation. HD 219134 b has a size of about 1.6 R ⊕, and a density of 6.4 g/cm 3 and orbits at 21.25 light-years away. Achetez Space NASA Rocky World Planet HD219134b Illustration Art Print Canvas Premium Wall Decor Poster Mural Espace Roche Monde Planète Mur Déco Affiche: Amazon.fr Livraison & retours gratuits possibles (voir conditions) Découverte d’une nouvelle classe d’exoplanètes dont le cœur pourrait être rempli de pierres précieuses. Contingut. Vì nó không được phát hiện là quá cảnh ngôi sao chủ của nó, nên bán kính và khối lượng thực của nó vẫn chưa được biết đến. The planetary system around HD 219134 was discovered independently by teams using HARPS-N and APF, who announced four-planet and six-planet solutions respectively. How do you say HD 219134 d? Architecture of the mixed-mass planetary system around HD 219134, a nearby K dwarf, as characterized by Gillon et al. - SIMBAD4 rel 1.7 - 2020.12.29CET01:41:00 Available data : Basic data • Identifiers • Plot & images • Bibliography • Measurements • External archives • Notes • Annotations . To see these, head over the github or click here to directly go to the git blame output of this system. University Homepage; Research; Explorer home; Research outputs; The HARPS-N Rocky Planet Search. HD 219134 c. Share. Planets similar to or like HD 219134 c. Hot, dense, rocky exoplanet orbiting around the K-type star HR 8832 in the constellation of Cassiopeia. HD 219134 g, also known as HR 8832 g, is an unconfirmed exoplanet orbiting around the K-type star HD 219134 in the constellation of Cassiopeia. It gives a quick overview of the hierarchical architecture. INTRODUCTION 1.1. Ce qui peut provoquer les réactions chimiques à l'origine de l'apparition des pierres précieuses, notamment les rubis et les saphirs, qui sont des oxydes d'aluminium [1]. Không giống như HD 219134 b và HD 219134 c, Kính viễn vọng Không gian Spitzer không quan sát nó và do đó bán kính và mật độ của nó chưa được biết đến. HD 219134 d, também conhecido como HR 8832 d, é um exoplaneta que está orbitando em torno de HR 8832, uma estrela anã laranja que está localizada a 21 anos-luz de distância a partir da Terra, na constelação de Cassiopeia. It has a minimum mass over 16 times that of Earth, indicating that it is likely a Hot Neptune. Để so sánh, Sao Thủy quay quanh Mặt Trời với chu kỳ 88 ngày ở khoảng cách 0,38 AU. The planetary system around HD 219134 was discovered independently by teams using HARPS-N and APF, who announced four-planet and six-planet solutions respectively. The detection of the HD 219134 c transit increases the probability that planets d and f also transit. As a bright (V = 5.57), nearby (d = 6.55 pc) K-type main-sequence dwarf of naked-eye visibility, it has long been of interest as a potential planet-bearing star. More references to the scientific publications and comments can be found in the commit messages. HD 219134 h, planet, semi-major axis: 3.06 ±0.05 AU. Wikipedia. The planetary system around HD 219134 was discovered independently by teams using HARPS-N and APF, who announced four-planet and six-planet solutions respectively. Full table display Database search. You can also view all commits contributing to this file on github. Tools. HD 219134 b (or HR 8832 b) is one of at least five exoplanets orbiting HD 219134, a main-sequence star in the constellation of Cassiopeia. Ngoại hành tinh này ban đầu được thiết bị HARPS-N tại Kính viễn vọng quốc gia Galileo của Ý phát hiện bằng phương pháp vận tốc xuyên tâm. This small cold gas planet is named after the deity Thee Hy, the bringer of fear. Juli 2015 d'Entdeckung vum HD 219134 b an deenen dräi weidere Planéiten HR 8832 publizéiert. But in six other systems (HD 219134 and Kepler-48, 87, 89, 167, 289) the habitable zone looks empty. In the HARPS-N solution, this planet was designated HD 219134 e and was assigned a shorter-period, more eccentric orbit. Full table display Database search. HD 219134 c is similar to these planets: HD 219134 d, HD 219134 f, HD 219134 e and more. Explore the Archive Interactive Table Search and File Upload HD 219134 d, planet, semi-major axis: 0.237 ±0.003 AU. Thank you for helping build the largest language community on the internet. All information on this page has been directly generated from this XML file. - SIMBAD4 rel 1.7 - 2020.07.28CEST18:09:02 Available data : Basic data • Identifiers • Plot & images • Bibliography • Measurements • External archives • Notes • Annotations . HD 219134 b has a size of about 1.6 R ⊕, and a density of 6.4 g/cm 3 and orbits at 21.25 light-years away. Topic. HD 219134 g, also known as HR 8832 g, is an unconfirmed [citation needed] exoplanet orbiting around the K-type star HD 219134 in the constellation of Cassiopeia. Elle aussi, tourne orbite presque circulaire. Imatges; Articles Relacionats; Enllaços Relacionats; Grups; Imatges. Unlike HD 219134 b it has not been observed by the Spitzer telescope and thus its HD 219134 b is a super-Earth, an exoplanet with a radius and mass bigger than Earth, but smaller than that of the ice giants Neptune and Uranus. HD 219134 g, planet, semi-major axis: 0.3753 ±0.0004 AU. 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. Caractéristiques. Nó có khối lượng tối thiểu hơn 16 lần so với Trái Đất, cho thấy nó có khả năng là Sao Hải Vương nóng. Il s'agit d'une super-Terre dont le rayon et la masse sont respectivement 1,6 et 4,5 fois plus grand que ceux de la Terre. Its mass is 16.17 Earths, it takes 46.9 days to complete one orbit of its star, and is 0.237 AU from its star. Để so sánh, Mặt Trời có nhiệt độ 5.778 K và 4,55 tỷ năm tuổi.[2][3]. Its mass is 16.17 Earths, it takes 46.9 days to complete one orbit of its star, and is 0.237 AU from its star. Wikipedia. migration through a radially structured disk. Topic. If you prefer to download the dataset as an ASCII tables, you might find the oec_tables repository useful. Its discovery was announced in … This table lists all people who have contributed to the Open Exoplanet Catalogue. Carregar la teva Imatge DSS Images Other Images Articles Relacionats . Spitzer observations allowed the discoverers to detect the transit of the innermost planet in front of the star making HD 219134 b the nearest known transiting planet to date. This table lists all planets in the system HD 219134. (2015), and the latter name is now used for this planet. It has a minimum mass of 11 Earth Masses, suggesting that it could be a high-mass ocean planet or a Neptune-like ice giant. Explore the Archive Interactive Table Search and File Upload You can also download the entire catalogue over at github. HD 219134 b ass dee bis elo sonnenoste Exoplanéit, dee mat der Transitmethod nogewise konnt ginn. Sign in to disable ALL ads. Trang này được sửa đổi lần cuối vào ngày 29 tháng 10 năm 2020 lúc 13:32. Note that this is just a summary. It has a minimum mass over 16 times that of Earth, indicating that it is likely a Hot Neptune. BD+56 2966, GJ 892, Gliese 892, HIP 114622, HR 8832, 2MASS J23131692+5710059, PPM 41599, TYC 4006-1866-1, Gaia DR2 2009481748875806976. It resides closer to the star than the inner edge of the system's (empirical) habitable zone, defined by the recent V… We have lots of theories about the evolution of our Solar System. For each of these, I’d love to see dynamical simulations of the long-term stability of hypothetical Earth-mass planets on habitable orbits. It has a mass of 108 Earth Masses, which indicates that the planet is likely a gas giant. 2011b). We often consider super-Earths to be distinct from sub-Neptunes in terms of their volatile fraction. HD 219134 d là có khả năng là một hành tinh băng khổng lồ, với khối lượng tối thiểu là 16,17 khối lượng Trái Đất, tương đương với Sao Hải Vương. HD 219134 g, also known as HR 8832 g, is an unconfirmed exoplanet orbiting around the K-type star HD 219134 in the constellation of Cassiopeia. All five planets are shown at their approximate relative sizes. The entire wiki with photo and video galleries for each article HD 219134 b ass dee bis elo sonnenoste Exoplanéit, dee mat der Transitmethod nogewise konnt ginn. The Solar System planets are shown as a comparison. HD 219134 d, còn được gọi là HR 8832 d, là một ngoại hành tinh quay quanh sao lùn cam HD 219134 (còn gọi là HR 8832) trong chòm sao Tiên Hậu. HD 219134. HD 219134 d, also known as HR 8832 d, is an exoplanet orbiting around the K-type star HR 8832 in the constellation of Cassiopeia.It has a minimum mass over 16 times that of Earth, indicating that it is likely a Hot Neptune.The exoplanet was initially detected by the instrument HARPS-N of the Italian Telescopio Nazionale Galileo via the radial velocity method. Nó có khối lượng tối thiểu hơn 16 lần so với Trái Đất, cho thấy nó có khả năng là Sao Hải Vương nóng. Des astronomes ont confirmé la découverte d’une exoplanète rocheuse, qui est la plus proche en dehors de notre système solaire jamais découverte. HD 219134 d, also known as HR 8832 d, is an exoplanet orbiting around the K-type star HR 8832 in the constellation of Cassiopeia.It has a minimum mass over 16 times that of Earth, indicating that it is likely a Hot Neptune.The exoplanet was initially detected by the instrument HARPS-N of the Italian Telescopio Nazionale Galileo via the radial velocity method. But in six other systems (HD 219134 and Kepler-48, 87, 89, 167, 289) the habitable zone looks empty. HD 219134 g, also known as HR 8832 g, is an unconfirmed exoplanet orbiting around the K-type star HD 219134 in the constellation of Cassiopeia. L’exoplanète HD219134B a été découverte dans la constellation de Cassiopée à environ 21 années-lumière de notre Terre et elle a la particularité d’être recouverte de rubis et de saphirs. (first observation of gravitational waves, announced in 2016), “HD 219134 d Confirmed planet Overview page”, https://vi.wikipedia.org/w/index.php?title=HD_219134_d&oldid=63991282, Giấy phép Creative Commons Ghi công–Chia sẻ tương tự. Utilisateurs en ligne. HD 219134 f, còn được gọi là HR 8832 f, là một ngoại hành tinh quay quanh sao lùn cam HD 219134 (còn gọi là HR 8832) trong chòm sao Tiên Hậu.Nó là một Siêu Trái Đất có khối lượng tối thiểu hơn 7 lần Trái Đất. in nature, and (2) both planets may contain a gas layer, whereas the layer of HD 219134 b must be larger. Frequency of Debris Disks around Solar-Type Stars: First Results from a Spitzer MIPS Survey We have searched for infrared excesses around a well-defined sample of69 FGK main-sequence field stars. Spitzer observations allowed us to detect the transit of the planet in front of the star making HD 219134 b the nearest known transiting planet to date. HD 219134 d, also known as HR 8832 d, is an exoplanet orbiting around the K-type star HR 8832 in the constellation of Cassiopeia. HD 219134 is an orange K-class star (K3V) in the constellation Cassiopeia, and only about half the distance, at 21.25 light years, as TRAPPIST-1 (about 40 light years out). This table lists all links which are relevant to this particular system. Hành tinh này có quỹ đạo tương đối lệch tâm với độ lệch tâm là 0,138. Planets in the system. Il a une masse d'environ trois fois et demie celle de la Terre. HD 219134 c can be rocky. Hành tinh HD 219134 d quay quanh sao lùn màu cam HD 219134, còn được gọi là HR 8832. Nó có nhiệt độ 4.699 K và khoảng 12,5 tỷ năm tuổi trở xuống. Planets b and c are observed in transit, so their radii are known. Connexion. Mot de passe . This table lists all stars in the system HD 219134. Elle orbite autour d’une étoile dans un autre système solaire à environ 21 années-lumière de la Terre. Query : HD 219134 : C.D.S. (2015). Full table display Database search. The planetary system HD 219134 hosts at least 7 planets. 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). ApJ, 821, 74 paper arxiv ADS A Six-Planet System Orbiting HD 219134 6 Users En ligne. Do đó, nó có thể nhìn thấy bằng mắt thường. rotation period for HD 219134 could thus help to confirm the planetary status of, or refute as a false positive, the 22.8 (planet f) and 46.78 day (planet d) RV signals. Nó có 79% bán kính và 80% khối lượng của Mặt Trời với 28% độ sáng mặt trời. HD 219134 (HR 8832; GJ 892; HIP 114622 ) is located high in the northern sky (R.A. = +23:13:17, decl. HD 219134 b has a size of about 1.6 R ⊕, and a density of 6.4 g/cm 3 and orbits at 21.25 light-years away. HD 219134 d: Back : Fictional info ; Suggested name: Thee Hy: Planet type: Small cold gas planet: Orbiting within Pamedeia's orbit, Thee Hy is an inferior planet and never appears to venture far from HD 219134; its maximum angular distance from HD 219134 (elongation) is 31 degrees. HD 219134 d is a super Earth exoplanet that orbits a K-type star. Using NASA's Spitzer Space Telescope, astronomers confirmed the nearest rocky planet outside our Solar system: HD 219134b. Listen to the audio pronunciation of HD 219134 d on pronouncekiwi. Suivez nous. This table lists all planets in the system HD 219134. Please include the corrected xml file and a reference to where the new data is coming from, ideally a scientific paper. HD 219134 d, also known as HR 8832 d, is an exoplanet orbiting around the K-type star HD 219134 in the constellation of Cassiopeia. D'Astronomenteam ëm den Fatemeh Motalebi vom Observatoire Genf huet den 30. Nom d'utilisateur . The equations of Selsis, Kasting et al are used to draw the inner and outer boundaries. 1. HD 219134 b (or HR 8832 b) is one of at least five exoplanets orbiting HD 219134, a main-sequence star in the constellation of Cassiopeia. Note that this is a new feature and not all system parameters might have a reference associated with it yet. Motivation Little is known about compositional and structural diver-sity of super-Earths. Découverte d'une nouvelle classe d'exoplanètes dont le cœur pourrait être rempli de pierres précieuses. migration through a radially structured disk. Using both the radial velocity and transit method, both its mass and radius have been well determined, allowing for accurate modelling of the planet's composition. HD 219134 c. Share. Orbite, température et climat HD 219134 c, also known as HR 8832 c, is a hot, dense, rocky exoplanet orbiting around the K-type star HR 8832 in the constellation of Cassiopeia.Originally thought to be a little less than three times the mass of Earth, it is now known to be over 4 times the mass and 51% larger in radius, suggesting a rocky composition with a higher quantity of iron than Earth. Elle ne peut d’ailleurs pas être vue depuis chez nous à l’œil nu. HD 219134 b has a size of about 1.6 R ⊕, and a density of 6.4 g/cm 3 and orbits at 21.25 light-years away. Độ sáng biểu kiến của ngôi sao, hoặc độ sáng của nó xuất hiện từ Trái Đất là 5. HD 219134 d. Exoplanet orbiting around the K-type star HR 8832 in the constellation of Cassiopeia. The exoplanet was initially detected by the instrument HARPS-N of the Italian Telescopio Nazionale Galileo via the radial velocity method. This is only an estimate, using the star's spectral type and mass. HD 219134 c en orbite autour de l'étoile en 6 jours et demi, à une distance de 0,064 UA. L’exoplanète HD219134 b est située à 21 années-lumière de la … The exoplanet was initially detected by the instrument HARPS-N of the Italian Telescopio Nazionale Galileo via the radial velocity method. A 12-Year Activity Cycle for the Nearby Planet Host Star HD 219134 2016 JOHNSON M., ENDL M., COCHRAN W., MESCHIARI S., ROBERTSON P. et al. Unlike HD 219134 b and HD 219134 c it has not been observed by the Spitzer Space Telescope and thus its radius and density are unknown. It gives a quick overview of the hierarchical architecture. Its discovery was announced in 2015. This list shows all planetary and stellar components in the system. The entire wiki with photo and video galleries for each article For each of these, I’d love to see dynamical simulations of the long-term stability of hypothetical Earth-mass planets on habitable orbits. Architecture of the system This list shows all planetary and stellar components in the system. Tools. HD 219134 with its four low-mass planets is the first result of the Rocky Planet Search program with HARPS-N on the Telescopio Nazionale Galileo in La Palma. HD 219134 (also known as Gliese 892 or HR 8832) is a main-sequence star in the constellation of Cassiopeia.It is smaller and less luminous than our Sun, with a spectral class of K3V, which makes it an orange-hued star. Riche en calcium, magnésium et silicium et étant très proche de son étoile, HD 219134 b a des températures assez élevées. Trois jours seulement lui suffisent pour en faire le tour, ce qui ne lui permet pas d'être habitable, d'après les astronomes. The planetary system HD 219134 hosts at least 7 planets. 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. HD 219134 d is a super Earth exoplanet that orbits a K-type star. 2017 and Johnson et al. It has a minimum mass of 11 Earth Masses, suggesting that it could be a high-mass ocean planet or a Neptune-like ice giant. Nó có thể bị khóa thủy triều. Explore the Archive Interactive Table Search and File Upload Query : HD 219134 : C.D.S. Juli 2015 d'Entdeckung vum HD 219134 b an deenen dräi weidere Planéiten HR 8832 publizéiert. Nó nhận được khoảng 4,7 lần lượng ánh sáng của Trái Đất nhận từ Mặt Trời. an open source database of all discovered extrasolar planets, https://www.cfa.harvard.edu/pao/HD219134.pdf, http://adsabs.harvard.edu/abs/2016ApJ...821...74J, http://adsabs.harvard.edu/abs/2015ApJ...814...12V, http://adsabs.harvard.edu/abs/2017NatAs...1E..56G, http://adsabs.harvard.edu/abs/2015A%26A...584A..72M, BD+56 2966 b, GJ 892 b, Gliese 892 b, HIP 114622 b, HR 8832 b, 2MASS J23131692+5710059 b, PPM 41599 b, TYC 4006-1866-1 b, Gaia DR2 2009481748875806976 b, BD+56 2966 c, GJ 892 c, Gliese 892 c, HIP 114622 c, HR 8832 c, 2MASS J23131692+5710059 c, PPM 41599 c, TYC 4006-1866-1 c, Gaia DR2 2009481748875806976 c, BD+56 2966 f, GJ 892 f, Gliese 892 f, HIP 114622 f, HR 8832 f, 2MASS J23131692+5710059 f, PPM 41599 f, TYC 4006-1866-1 f, Gaia DR2 2009481748875806976 f, BD+56 2966 d, GJ 892 d, Gliese 892 d, HIP 114622 d, HR 8832 d, 2MASS J23131692+5710059 d, PPM 41599 d, TYC 4006-1866-1 d, Gaia DR2 2009481748875806976 d, BD+56 2966 g, GJ 892 g, Gliese 892 g, HIP 114622 g, HR 8832 g, 2MASS J23131692+5710059 g, PPM 41599 g, TYC 4006-1866-1 g, Gaia DR2 2009481748875806976 g, BD+56 2966 e, GJ 892 e, Gliese 892 e, HIP 114622 e, HR 8832 e, 2MASS J23131692+5710059 e, PPM 41599 e, TYC 4006-1866-1 e, Gaia DR2 2009481748875806976 e, BD+56 2966 h, GJ 892 h, Gliese 892 h, HIP 114622 h, HR 8832 h, 2MASS J23131692+5710059 h, PPM 41599 h, TYC 4006-1866-1 h, Gaia DR2 2009481748875806976 h. The planetary system around HD 219134 was discovered independently by teams using HARPS-N and APF, who announced four-planet and six-planet solutions respectively. D'Astronomenteam ëm den Fatemeh Motalebi vom Observatoire Genf huet den 30. En 2014, il y a eu 715 exoplanètes confirmées d’un coup, elles ont été découvertes par le satellite KEPLER. HD 219134 h, also known as HR 8832 h, is an exoplanet orbiting around the K-type star HR 8832 in the constellation of Cassiopeia. Nó là một Siêu Trái Đất có … ‹ … Please consider contributing! Click here to find out how. Toutefois, HD 219134b orbite trop près de son étoile. HD 219134 d, còn được gọi là HR 8832 d, là một ngoại hành tinh quay quanh sao lùn cam HD 219134 (còn gọi là HR 8832) trong chòm sao Tiên Hậu. Note that if no green band is shown in the plot, then the planet's orbit is far outside the habitable zone. Using both the radial velocity and transit method, both its mass and radius have been well determined, allowing for accurate modelling of the planet's composition. Planets similar to or like HD 219134 c. Hot, dense, rocky exoplanet orbiting around the K-type star HR 8832 in the constellation of Cassiopeia. HD 219134 c, also known as HR 8832 c, is a hot, dense, rocky exoplanet orbiting around the K-type star HD 219134 in the constellation of Cassiopeia. L'exoplanète HD219134 b est située à 21 années-lumière de la … Nó mất khoảng 46,9 ngày để hoàn thành một vòng quỹ đạo ở khoảng cách 0,237 AU. https://www.cfa.harvard.edu/pao/HD219134.pdf four planets discovered by RV, two also with transittime Closes #652 Données d'observation (époque J2000 [1]) Ascension droite: 23 h 13 m 16,976 s [1] Déclinaison +57° 10′ 06,08″ [1] Constellation: Cassiopée: Magnitude apparente: U : 7,460 ± 0,010 [1] B : 6,560 ± 0,007 [1] V : 5,570 ± 0,009 [1] R : 4,76 [1] I : 4,23 [1] H : 3,40 [1] Localisation dans la constellation : Cassiopée. You can download the xml file corresponding to this planetary system, which is part of the Open Exoplanet Catalogue. Within the commit message, you will find a link to the scientific publication where the data is taken from. Transits of the second planet were detected in 2017. The following plot shows the approximate sizes of the planets in this system We have lots of theories about the evolution of our Solar System. Tools. 2016. HD 219134 b is a super-Earth, an exoplanet with a radius and mass bigger than Earth, but smaller than that of the ice giants Neptune and Uranus. Note that unless the radius has been determined through a transit observation, this is only an approximation (see Lissauer et al. It also lists the date of the last commit and the person making the changes. HD 219134 e, planet, semi-major axis: 2.56 +3.41 −0.15 AU. HD 219134 d. Exoplanet orbiting around the K-type star HR 8832 in the constellation of Cassiopeia. This planet was designated HD 219134 d in the HARPS-N announcement. HD 219134 d là hành tinh thứ tư từ ngôi sao của nó. - SIMBAD4 rel 1.7 - 2020.10.04CEST11:39:56 Available data : Basic data • Identifiers • Plot & images • Bibliography • Measurements • External archives • Notes • Annotations . Originally thought to be a little less than three times the mass of Earth, it is now known to be over 4 times the mass and 51% larger in radius, suggesting a rocky composition with a higher quantity of iron than Earth. C.D.S. HD 219134 b (or HR 8832 b) is one of at least five exoplanets orbiting HD 219134, a main-sequence star in the constellation of Cassiopeia. In the left column of the output you can see the commit message corresponding to each parameter. The planet candidate HD 219134 e was discovered by Motalebi et al. Please help making this catalogue better and contribute data or references! HD 219134 d, also known as HR 8832 d, is an exoplanet orbiting around the K-type star HR 8832 in the constellation of Cassiopeia.It has a minimum mass over 16 times that of Earth, indicating that it is likely a Hot Neptune.The exoplanet was initially detected by the instrument HARPS-N of the Italian Telescopio Nazionale Galileo via the radial velocity method. Découverte à ce jour, head over the github or click here to directly to. Découverte d'une nouvelle classe d'exoplanètes dont le cœur pourrait être rempli de pierres précieuses is shown in the HD... All five planets are shown as a comparison this planetary system around HD 219134, a K... The corrected xml file and a reference associated with it yet, 167 289. La Terre new feature and not all system parameters might have a associated! } }.. Syntaxe six-planet system orbiting HD 219134 e and more the Italian Telescopio Galileo... } }.. Syntaxe see the commit message corresponding to this entry, please send e-mail... Thank you for helping build the largest language community on the internet permet pas d'être habitable, d'après les.! Độ 5.778 K và khoảng 12,5 tỷ năm tuổi. [ 2 ] 3... For this planet was designated HD 219134 c is similar to these planets: HD.! Photo and video galleries for each of these, I ’ d love to see these, I d... 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