47 Ursae Majoris (também abreviado como 47 UMa ), nomeado como Chalawan, é uma estrela anã amarela similar ao Sol situada na constelação de Ursa Major.
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(υ) | A Bayesian analysis of 47 Ursae Majoris radial velocity data confirms and refines the properties of two previously reported planets with periods of 1079 and 2325 d. The analysis also provides orbital constraints on an additional long-period planet with a period of ∼10 000 d. …
Orbital speed | (m) | Joined the Solar ⦠47 Ursae Majoris c (sometimes abbreviated 47 Uma c) is an extrasolar planet approximately 46 light-years from Earth in the constellation of Ursa Major.The planet was discovered located in a long-period around the star 47 Ursae Majoris.Its orbit lasts 6.55 years and … Also known as 47 Ursae Majoris, Rowan is a non-portal star in the Praezorian Sector and nominally part of the Pollux Corridor. The analysis also provides orbital constraints on an additional long period planet with a period ∼ 10000 days. Gl 407, HR 4277, BD +41°2147, HD 95128, LTT 12934, GCTP 2556.00, SAO 43557, FK5 1282, GC 15087, HIP 53721. The planet was discovered located in a long-period orbit (38 ⦠caption = An artist's impression of 47 Ursae Majoris b.Planetbox star star = 47 Ursae Majoris constell = Ursa Major Ursa Major Thank you for helping build the largest language community on the internet. 47 Ursae Majoris b was discovered in 1996 and has a mass at least 2.63 times that of Jupiter.
Declination | 6 March 2010 | 47 Ursae Majoris c is an extrasolar planet orbiting the Sun-like star 47 Ursae Majoris, making one orbital revolution every 2,594 days. | 1.172 ± 0.111 R☉ |
The star can be found southeast of Omega UMa, southwest of Psi UMa , northeast of 46 UMa, and northwest of 55 UMa (see another chart with 47 UMa labeled ). 47 Ursae Majoris (abbreviated 47 UMa), also named Chalawan (Thai: ชาละวัน, pronounced [t͡ɕʰāː.lā.wān]), is a yellow dwarf star approximately 46 light-years from Earth in the constellation of Ursa Major.As of 2011, three extrasolar planets (designated 47 Ursae Majoris b, c and d; the first two later named Taphao Thong and Taphao Kaew) are believed to orbit the star. | Age | [11], Los analises fechos darréu nun punxeron confirmar la esistencia del segundu planeta, y suxurióse que'l conxuntu de datos utilizaos nel so descubrimientu fallaben. The planet was discovered located in a long-period orbit (38 years) around the star 47 Ursae Majoris. De Stär huet e Planéitesystem, dat nobewisen aus dräi Exoplanéite besteet. De Stär δ Ursa Majoris dréit den Numm Megrez, arabesch fir âWuerzelâ, woumat de âSchwanzusazâ gemengt ass. & FISCHER D. MNRAS, 403, 731 paper arxiv. 47 Ursae MajorisUAS: Chalawan 47 Ursae Majoris (abbreviated 47 UMa), formally named Chalawan /ËtÊÉËlÉwÉn/, is a yellow dwarf star approximately 46 light-years from Earth in the constellation of Ursa Major.The star is located fairly close to the Solar System ay a distance of 45.913 light-years. Con una masa similar a la masa solar, 47 Ursae Majoris ye llixeramente más rica en metales que'l Sol, cuntando con alredor del 110% de la bayura solar en fierro. The evidence of this planet was found by Bayesian Kepler periodogram in March 2010. Template:Planetbox begin Template:Planetbox star Template:Planetbox orbit Template:Planetbox character Template:Planetbox discovery Template:Planetbox reference Template:Planetbox end 47 Ursae Majoris d (sometimes abbreviated 47 Uma d) is an extrasolar planet approximately 46 light-years away in the constellation of Ursa Major. De Sarkophag oder d'Doudelued ass d'Këscht vum Won. It is the longest-period planet detected by Doppler spectroscopy. És actualment el planeta més ⦠Visita la páxina d'alderique del proyeutu pa collaborar y facer entrugues o suxerencies. It would complete this orbit within about 431 days or less than 1.2 years. It has a mass of at least 1.64 times that of Jupiter. Monthly Notices of the Royal Astronomical Society, https://solarsystemtour.fandom.com/wiki/47_Ursae_Majoris_d?oldid=6293. EZ Ursae Majoris Radius. Chalawan is a Main Sequence Star type star. As of 2008, it has been confirmed that two extrasolar planets orbit the star. Because of this, 47 Ursae Majoris was listed as one of top 100 target stars for NASA's former Terrestrial Planet Finder mission. 47 Ursae Majoris Chalawan Taurus ... /ËmjuËfráµ»d/ Ursa Major ο Ursae Majoris A Muscida /ËmjuËsáµ»dÉ/ Delphinus 18 Delphini Musica /ËmjuËzáµ»kÉ/ Perseus HAT-P-29 Muspelheim* // Cancer ξ Cancri A Nahn /ËnÉËn/ Dorado WASP-62 Naledi* // Puppis Solar System Tour Wiki is a FANDOM Lifestyle Community. 47 Ursae Majoris (disingkat 47 UMa), umumnya disebut Chalawan / ˈ tʃ ɑː l ə w ə n /, adalah sebuah bintang katai kuning yang berjarak sekitar 46 tahun cahaya dari Bumi di konstelasi Ursa Major.Per 2011, tiga planet ekstrasurya (yang dinamakan 47 Ursae Majoris b, c dan d; dua yang pertama kemudian dinamai Taphao Thong dan Taphao Kaew) dipercayai mengelilingi bintang tersebut. [1] En 2002 conocióse que 47 Ursae Majoris cuntaba con dos planetes estrasolares orbitando al so alredor. The planet is currently the innermost known planet in its planetary system. 47 Ursae Majoris |
Saltar a navegación Saltar a la gueta. Discovery . | Argument ofperiastron | The discovery of a second planet in the 47 Ursae Majoris system, 47 UMa c, was announced in 2002 and subsequently confirmed by other groups. [5], En 2001, midÃes astrométricas preliminares realizaes pol satélite Hipparcos apurrieron datos sobre la órbita de 47 Ursae Majoris b, afirmando qu'esti tenÃa un enclÃn de 63,1º. En 2002 conocióse que 47 Ursae Majoris cuntaba con dos planetes estrasolares orbitando al so alredor. (e) | Gregory and Fischer |
La última edición d'esta páxina foi el 24 och 2020, a les 14:50. El modelu que meyor afacer a los datos empÃricos indica que ye posible que'l planeta tenga un periodu de 7.856 dÃes y qu'esti asitiáu a 7,73 UA. Contràriament a la major part dels planetes extrasolars coneguts, la seva excentricitat orbital és baixa. [9] SicasÃ, analises posteriores demostraron que les midÃes d'Hipparcos nun son lo suficientemente precises como pa determinar les órbites de dichos planetes, y con éses l'enclÃn y la masa real siguen siendo desconocÃes. 47 Ursae Majoris d (sometimes abbreviated 47 Uma d) is an extrasolar planet approximately 46 light-years away in the constellation of Ursa Major. It orbits at a distance of about 1.73 billion km (c.1.076 billion miles) once every 38.33 years, which is equivalent to being between Saturn and Uranus in our system. 47 Ursae Majoris (often abbreviated 47 UMa) is a solar analog, yellow dwarf star approximately 46 light-years [1] away from Earth in theconstellation of Ursa Major.As of 2011, it has been confirmed that three Jupiter-like extrasolar planets orbit the star. 47 Ursae Majoris d (sometimes abbreviated 47 Uma d) is an extrasolar planet approximately 46 light-years away in the constellation of Ursa Major. El planeta tien siquier 2,63 vegaes la masa de Xúpiter y tarda 1.089 dÃes en completar el so xiru alredor de la so estrella. A Bayesian analysis of 47 Ursae Majoris (47 UMa) radial velocity data confirms and refines the properties of two previously reported planets with periods of 1079 and 2325 days. El so periodu de rotación, d'unos 24 dÃes, ye tamién similar al del Sol. With a spectral type of G1V, it is also slightly hotter than the Sun, at around 5,882 K. 47 Ursae Majoris has anabsolute magnitude of +4.29, implying it has a visual luminosity around 60% greater than the Sun. 47 Ursae Majoris has a similar mass to that of our Sun. El descubrimientu realizóse usando'l mesmu métodu de velocidá radial usáu pa detectar al primer planeta. [3] Con una magnitú aparente de +5,03, ye visible a simple vista en bones condiciones. | 5.03 |
| Distance | 45.9 ly(14.06 pc) |
| Spectral type | D'alcuerdu a les afirmaciones del equipu de descubridores, el planeta tarda en redol a 2,594 dÃes en completar la so órbita. (α) | 47 Ursae Majoris b (viết tắt 47 UMA b), chính thức đặt tên Taphao Thong / t ə ˌ p aʊ ˈ t ɒ ŋ /, là một hành tinh ngoài hệ mặt trời khoảng 46 năm ánh sáng từ Trái Đất trong chòm sao Đại Hùng.Hành tinh này được phát hiện nằm trong một chu kì quỹ đạo quanh ngôi sao 47 Ursae Majoris… Right ascension | The orbit of 47UMa d is currently quite uncertain; both it and that of 47 UMa c may be circular. Fischer, G.W. | És lleugerament més rica en metalls que el Sol, amb un 110% de l'abundància solar de ferro. 47 Ursae Majoris b orbita a una distància de 2,10 UA la seva estrella, tardant 1.078 dies o 2,95 anys en completar una revolució. Discovery site | 47 Ursae Majoris b is an extrasolar planet approximately 46 light-years away in the constellation of Ursa Major. G1V |
A fecha de 2008, unviáronse dos mensaxes METI a 47 Ursae Majoris. It lies in the southcentral part (10:59:28.0+40:25:48.9, ICRS 2000.0) of Constellation Ursa Major , the Great Bear. As of 2011, it is the outermost of three known planets in its planetary system. . El 6 de marzu de 2010 confirmóse la esistencia del tercer planeta 47 Ursae Majoris d. 47 Ursae Majoris alcuéntrase ente los cien estrelles oxetivu de la NASA pa la so misión Terrestrial Planet Finder.[2]. | Discovery date | 47 Ursae Majoris d (Dekoranta) (eujovian) Solar Dominion Inner Sphere worlds, colonised by the Akirates, a heterodox offshoot of the powerful Stevens clade. Alderique:47 Ursae Majoris. ~82.4 mas |
| Template:Country data United States |
Three planetary candidates detected with ELODIE, http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2004A%26A...414..351N&db_key=AST&nosetcookie=1, Long-Period Objects in the Estrasolar Planetary Systems 47 Ursae Majoris and 14 Herculis, http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2007ApJ...654..625W&db_key=AST&nosetcookie=1, A Bayesian periodogram finds evidence for three planets in 47 Ursae Majoris, Prospects for Habitable "Earths" in Known Exoplanetary Systems, http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2005ApJ...622.1091J&db_key=AST&nosetcookie=1, The Search for other Earths: limits on the giant planet orbits that allow habitable terrestrial planets to form, http://www.cplire.ru/rus/ra&sr/VAK-2004.html, Enciclopedia de los planetes estrasolares: 47 Ursae Majoris, https://ast.wikipedia.org/w/index.php?title=47_Ursae_Majoris&oldid=3067773, Wikipedia:ArtÃculos bonos na Wikipedia en portugués, Wikipedia:ArtÃculos bonos na Wikipedia n'inglés, Wikipedia:ArtÃculos bonos na Wikipedia en catalán, Wikipedia:ArtÃculos bonos na Wikipedia en castellanu, Llicencia Creative Commons Reconocimientu/CompartirIgual 3.0. Instead extensive orbital settlements extend throughout the system, and bubblehab colonies have … Contents[show] Name 47 Ursae Majoris d Also called, 47 Uma b Discovery date March 6, 2010 Discoverers P.C. âBeenâ vum Bier. | Constellation | Because of this, 47 Ursae Majoris was listed as one of top 100 target stars for NASA's former Terrestrial Planet Finder mission. Chalawan is a Main Sequence Star type star. Solar-type stars with planetary companions: 51 Pegasi and 47 Ursae Majoris Temperature | Discovery . Dentro do sistema, é o planeta mais próximo da estrela que se conhece. [Fe/H] | 110+132−160[1]° |
lació de l'Óssa Major.A 2010, s'ha confirmat que hi orbiten tres planetes extrasolars semblants a Júpiter; per això es va llistar a l'antiga missió Terrestrial Planet Finder de la NASA com un dels 100 objectius principals. Sign in to disable ALL ads. | Mass | 47 Ursae Majoris. Chalawan is not part of the Ursa Major constellation outline but is within the borders of the constellation. L'usu d'esti modelu nesti sistema planetariu dexó afayar que ye 100.000 vegaes más probable tener tres planetes que dos planetes. Discoverer(s) | Confirmed |
10h 59m 28.0s | 2 . If you need the diameter of the star, you just need to multiple the radius by 2. 47 Ursae Majoris เป็นชื่อในระบบแฟลมสตีด (Flamsteed designation) และในการค้นพบดาวเคราะห์ในระบบของดาว 47 Ursae Majoris จึงถูกกำหนดชื่อต่อเนื่องเป็น 47 Ursae Majoris b, c และ d | 9.7+4.1−3.2 AU(~1460 Gm) |
Query : 47 Ursae Majoris : C.D.S. D. N. C. Lin and Shigeru Ida 1997 The Astrophysical Journal 477 781. Orbits of the planets in the 47 Ursae Majoris system. If you need the diameter of the star, you just need to multiple the radius by 2. 47 Ursae Majoris (UMa) is located about 45.9 light-years from Sol. As of 2011, it is the outermost of three known planets in its planetary system. | +40° 25′ 49″ |
The Sun's radius is 695,800km, therefore the star's radius is an estimated 23,575,755.50.km. [14] SerÃa'l planeta de más llargu periodu descubiertu pol métodu de velocidá radial, anque planetes de más llargu plazu namái fueron afayaos por imáxenes direutes y midÃes de tiempu d'un púlsar. | (mV) | (ω) | lació de l' Óssa Major El planeta va ser descobert en un període llarg al voltant de l'estrella 47 Ursae Majoris. Per 2011 - SIMBAD4 rel 1.7 - 2020.06.03CEST10:14:34 Available data : Basic data ⢠Identifiers ⢠Plot & images ⢠Bibliography ⢠Measurements ⢠External archives ⢠Notes ⢠Annotations . In 2001, preliminary astrometric measurements made by the Hipparcos probe suggest the orbit of 47 Ursae Majoris b is inclined at an angle of 63.1° to the plane of the sky. Coordinates: Sky map 10h 59m 28.0s, +40° 25′ 49″ Si estes midÃes confÃrmense, implicarÃa que la masa del planeta serÃa 2,9 vegaes la de Xúpiter. Star | 47 Ursae Majoris d Ngoại hành tinh: Danh sách há» hành tinh: Sao chủ Sao: 47 Ursae Majoris: Chòm sao: Äại Hùng: Xích kinh (α) 10 h 59 m 28.0 s: Xích vÄ© (δ) +40° 25â² 49â³ Cấp sao biá»u kiến (m V) 5,03: Khoảng cách: 45,9 ly (14,06 pc) Phân loại sao: G1V: Khá»i lượng (m) 1,08 M â Bán kính (r) 1,172 ± 0,111 R â Nhiá»t Äá» (T) 5887 ± 3,8 K Esta páxina forma parte del wikiproyeutu Astronomía, un esfuerciu collaborativu col fin d'ameyorar y organizar tolos conteníos rellacionaos con esti tema. SÃa comoquier, los parámetros del segundu planeta siguen siendo desconocÃos.[13]. De tipu espectral G1V,[4]el so temperatura efectivo ye daqué mayor que la del Sol, en redol a 5.855 K.[5] 47 Ursae Majoris tien una magnitú absoluta de +4,29, lo que supón una lluminosidá visual un 60% mayor que la lluminosidá solar. Chalawan Facts. Definitions of Luettelo_eksoplaneetoista_koordinaattien_mukaan, synonyms, antonyms, derivatives of Luettelo_eksoplaneetoista_koordinaattien_mukaan, analogical dictionary of Luettelo_eksoplaneetoista_koordinaattien_mukaan (Finnish) 4,47 267 A2V d: 24 4,54 G4 III-IV Ï: 4,55 437 A3 IV Ï 2: 4 4 Ursae Majoris: 4,59 252 K2 III 83 4,63 549 M2 III Ï: 45 4,66 267 A1 V Ï: 14 4,67 122 Am HR 4132 4,72 112 A7 IV Ï: 8 4,74 287 M3 III 55 4,76 183 A2 V Ï 2: 4,80 67 F7 IV-V e: 18 4,80 118 A5 V 36 4,82 42 ⦠Discovery method | Alcuéntrase al sureste de Ï Ursae Majoris, suroeste de Ï Ursae Majoris y nordeste de 46 Ursae Majoris. 47 Ursae Majoris, often abbreviated as 47 UMa, is a solar twin, yellow dwarf star approximately 46 light-years away from Earth in the constellation of Ursa Major. 0.16+0.09−0.16[1] |
| Orbital period | (P) | Apastron | [3] Referenser Noter Its mass is 1.64 Jupiters, it takes 38.4 years to complete one orbit of its star, and is 11.6 AU ⦠Chalawan Facts. Definitions of 47 Ursae Majoris d, synonyms, antonyms, derivatives of 47 Ursae Majoris d, analogical dictionary of 47 Ursae Majoris d (English) t trá»i khoảng 46 nÄm ánh sáng từ Trái Äất trong chòm sao Äại Hùng.Hành tinh này Äược phát hiá»n nằm trong má»t chu kì quỹ Äạo quanh ngôi sao 47 Ursae Majoris⦠47 Ursae Majoris (tamién embrivíu como 47 UMa) ye una estrella nana mariella similar al Sol asitiada na constelación del sietestrellu. Microlensing Events from Measurements of the Deflection × 47 Ursae Majoris By Written in the Sand. The planet was discovered located in a long-period orbit (38 years) around the star 47 Ursae Majoris. 47 Ursae Majoris; The red dot shows the location of 47 Ursae Majoris in Ursa Major. Template:Nearest bright star systems. D'alcuerdu a la so actividá cromosférica, la estrella puede tener en redol a 6.000 millones d'años d'antigüedá, anque modelos d'evolución estelar suxuren una antigüedá cimera, d'unos 8.700 millones d'años. Joined the Solar Dominion in 2866 AT. Discovery status | Time of periastron | Data at NED - NASA/IPAC Extragalactic Database : 47 Ursae Majoris. (q) | El descubrimientu prodúxose reparando'l cambéu na velocidá radial de la estrella, cuando se percibió la gravedá d'un planeta al so alredor. A terrestrial planet orbiting 47 Ursae Majoris at around the first inner tenth of the orbital distance of the calculated habitable zone would have an average orbital distance just under 1.13 AU, between the orbits of Earth and Mars in the Solar System. 47 Ursae Majoris b is an extrasolar planet orbiting the Sun-like star 47 Ursae Majoris. Take your favorite fandoms with you and never miss a beat. 47 Ursae Majoris d (sometimes abbreviated 47 Uma d) is an extrasolar planet approximately 46 light-years away in the constellation of Ursa Major. Calling 47 UMa. Chalawan is not part of the Ursa Major constellation outline but ⦠47 Ursae MajorisUAS: Chalawan 47 Ursae Majoris (abbreviated 47 UMa), formally named Chalawan /ˈtʃɑːləwən/, is a yellow dwarf star approximately 46 light-years from Earth in the constellation of Ursa Major.The star is located fairly close to the Solar System ay a distance of 45.913 light-years. The Hill stability of the possible moons of extrasolar planets 2010 DONNISON J. MNRAS, 406, 1918 paper. ชื่อ. [17], Coordenaes: 10h 59m 27.974s, 40° 25â² 48.922â³, Wittenmyer, R. A., Endl, M., Cochran, W. D. (2007). The Minzera have so far allowed humans to settle there without resistance. [6], Como'l Sol, 47 Ursae Majoris alcuéntrase na secuencia principal, convirtiendo hidróxenu en heliu nel so nucleu per aciu fusión nuclear. Chalawan (47 Ursae Majoris) Star Facts. Apparent magnitude | Origem: Wikipédia, a enciclopédia livre. 47 Ursae Majoris d (sometimes abbreviated 47 Uma d) is an extrasolar planet approximately 46 light-years away in the constellation of Ursa Major. Star: Chalawan, 47 Ursae Majoris Type: G1V Luminosity: 1.6 x Sol Distance from Sol: 45.91 ly Colonised 1977 AT Planets: 47 Ursae Majoris b (Taphao Thong) (hydrojovian)47 Ursae Majoris c (Taphao Kaew) ()47 Ursae Majoris d (Dekoranta) (eujovian)Solar Dominion Inner Sphere worlds, colonised by the Akirates, a heterodox offshoot of the powerful Stevens clade. The G0 V star 47 UMa exhibits very low amplitude radial velocity variations having a period of 2.98 yr, a velocity amplitude of K = 45.5 m s-1, and small eccentricity.The residuals scatter by 11 m s-1 from a Keplerian fit to the 34 velocity measurements obtained during 8 yr. It has a mass of at least 1.64 times that of Jupiter. Alcuéntrase al sureste de Ï Ursae Majoris, suroeste de Ï Ursae Majoris y nordeste de 46 Ursae Majoris. [1] Den ligger på ett avstånd av ungefär 375 ljusår. The planet was discovered located in a long-period orbit (38 years) around the star 47 Ursae Majoris. 11.6+2.1−2.9[1] AU(~1730 Gm) |
| | Al contrariu que la mayorÃa de planetes estrasolares conocÃos, 47 Ursae Majoris b tien una órbita con bien poca escentricidá. 47 Ursae Majoris d is a gas giant exoplanet that orbits a G-type star. 47 Ursae Majoris Den 47 Ursae Majoris, (ofgekierzt: 47 UMa) oder Chalawan ass e Gielen Zwerg d'selwecht wéi eis Sonn. III. 47 Ursae Majoris c (sometimes abbreviated 47 Uma c) is an extrasolar planet approximately 46 light-years from Earth in the constellation of Ursa Major.The planet was discovered located in a long-period around the star 47 Ursae Majoris.Its orbit lasts 6.55 years and ⦠[15] SicasÃ, la presencia d'un planeta xigante a 2,5 UA de la estrella, podrÃa interferir na formación d'un planeta na zona central, y amenorgáu la cantidá d'agua presente nestos planetes centrales mientres el so acrecimientu. 47 Ursae Majoris té una massa similar a la del nostre Sol. Les midÃes fueron realizaes per aciu l'efeutu Doppler nel espectru de la estrella. Properties of Sun-like Stars with Planets: 51 Pegasi, 47 Ursae Majoris, 70 Virginis, and HD 114762 Gregory W. Henry et al. The planet was discovered located in a long- period orbit (38 years) around the star 47 Ursae Majoris . Característiques físiques. 47 Ursae Majoris (tamién embrivÃu como 47 UMa) ye una estrella nana mariella similar al Sol asitiada na constelación del sietestrellu. 47 Ursae Majoris alcuéntrase relativamente cercana al Sistema Solar: d'alcuerdu a midÃes astrométricas realizaes pol satélite Hipparcos, la estrella esibe una paralax de 71,04 milisegundos d'arcu, correspondientes a una distancia de 45,9 años lluz o 14,1 pársecs. 14002+4018−5095[1] d(~38.33 y) |
Esti descubrimientu foi anunciáu por Debra Fischer y PC Gregory. Va ser el primer planeta de període llarg a ser detectat al voltant d'una estrella de seqüència principal.Contràriament a la major part dels planetes extrasolars coneguts, la seva excentricitat orbital és baixa. | Eccentricity | Unlike the majority of known long-period extrasolar planets, the eccentricity of the orbit of 47 Ursae Majoris b is low. 44 Ursae Majoris estimated radius has been calculated as being 33.88 times bigger than the Sun. It is located in a long-period, near-circular orbit and is the innermost known planet in its planetary system. The evidence of this planet was found by Bayesian Kepler periodogramin March ⦠1.08 M☉ |
La última edición d'esta páxina foi el 24 och 2020, a les 14:50. The planet was discovered located in a long-period around the star 47 Ursae Majoris. 47 Ursae Majoris b orbita a una distància de 2,10 UA la seva estrella, tardant 1.078 dies o 2,95 anys en completar una revoluci ó. Va ser el primer planeta de període llarg a ser detectat al voltant d'una estrella de seqüència principal. By using our website and our services, you agree to our use of cookies as described in our Cookie Policy. Esti datu ye similar al de Xúpiter y Saturnu nel Sistema Solar, con un radiu d'órbita cercanu a 5:2 y una proporción de masa aproximao igual. IOPscience. | Temperature | Solar-type stars with planetary companions: 51 Pegasi and 47 Ursae Majoris [7], En 1996, Geoffrey Marcy y R. Paul Butler anunciaron qu'un planeta estrasolar orbitaba alredor de 47 Ursae Majoris. The planet was discovered located in a long-period orbit (38 years) around the star 47 Ursae Majoris. (T) | The Hill stability of the possible moons of extrasolar planets 2010 DONNISON J. MNRAS, 406, 1918 paper. 85 K |
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| (Q) | Chalawan is a G0V main sequence star based on the spectral type that was recorded in the Hipparcos star catalogue. El segundu mensaxe, Cosmic Call 2, foi unviáu'l 6 de xunetu de 2003 y va llegar a 47 Ursae Majoris en mayu de 2049. & FISCHER D. MNRAS, 403, 731 paper arxiv. [10], El descubrimientu d'un segundu planeta, denomináu 47 Ursae Majoris c, foi anunciáu por Debra Fischer, Geoffrey Marcy y R. Paul Butler en 2002. Periastron | Metallicity | 2002 • 10 songs. Computer simulations now show, however, that Earth-sized planets are unlikely to form in the so-called "habitable zone" of 47 Ursae Majoris (47 UMa). 47 Ursae Majoris b foi descoberto em 1996 e tem uma massa de pelo menos 2,60 vezes a massa de Júpiter It is the longest-period planet detected by Doppler spectroscopy. Marcy, R.P. «, Llista d'estrelles brilloses más cercanes, http://www.journals.uchicago.edu/doi/abs/10.1086/504701, http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2005A%26A...443..609S&db_key=AST&nosetcookie=1, http://www.journals.uchicago.edu/doi/full/10.1086/310102, Preliminary Astrometric Masses for Proposed Estrasolar Planetary Companions, http://www.journals.uchicago.edu/doi/full/10.1086/318927, Screening the Hipparcos-based astrometric orbits of sub-stellar objects, http://adsabs.harvard.edu/abs/2001A%26A...372..935P, A Second Planet Orbiting 47 Ursae Majoris, http://www.journals.uchicago.edu/doi/full/10.1086/324336, The ELODIE survey for northern extra-solar planets. Dambos fueron tresmitÃos dende'l radar más grande d'Eurasia (el Radar Planetariu de 70 metros d'Eupatoria, n'UcraÃna). 49 Ursae Majoris, eller HD 95310, är en vit stjärna i huvudserien i stjärnbilden Stora björnen.
| Database references |
| Extrasolar PlanetsEncyclopaedia | data |
| SIMBAD | data |
. 47 UMa c discovery paper: "A Second Planet Orbiting 47 Ursae Majoris" D.A.
(T) | 9.0+7.8−3.7 km/s | Déi arabesch Nimmn Merak an Phekda fir d'Stäre β an γ Ursae Majoris bedeiten âLend â bzw. EZ Ursae Majoris estimated radius has been calculated as being 26.43 times bigger than the Sun. 1997 The Astrophysical Journal 474 503. 47 Ursae Majoris; The red dot shows the location of 47 Ursae Majoris in Ursa Major. IOPscience. [12] Ello ye que tales analises establecieron que ye altamente improbable la esistencia d'un planeta con un periodu similar a 2.500 dÃes, pero sà ye posible que tal planeta tuviera un periodu de 6.500 dÃes o cimeru. 47 Ursae Majoris d (sometimes abbreviated 47 Uma d) is an extrasolar planet approximately 46 light-years away in the constellation of Ursa Major. 47 Ursae Majoris FK5: 1282 Gliese-Katalog: GJ 407 Henry-Draper-Katalog: HD 95128 Hipparcos-Katalog: HIP 53721 SAO-Katalog: SAO 43557 Tycho-Katalog: TYC 3009/2703/1 Weider Katalogen: Den 47 Ursae Majoris, (ofgekierzt: 47 UMa) oder Chalawan ass e Gielen Zwerg d'selwecht wéi eis Sonn. | 0.04 |
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B was discovered located in a long- period orbit ( 38 years ) around the star you! Collaborar y facer entrugues o suxerencies and has a similar mass to that of Jupiter would complete this orbit about! Ungefär 375 ljusår exoplanet that orbits a G-type star target stars for NASA 's former Terrestrial planet mission! ( el radar planetariu de 70 metros d'Eupatoria, n'UcraÃna ) settle there without resistance Majoris ''.! J. MNRAS, 406, 1918 paper y tarda 1.089 dÃes en completar el so xiru alredor de la estrella! Doppler spectroscopy a beat do sistema, é o planeta mais próximo da estrela que se conhece dréit...
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