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From Wikipedia, the free encyclopedia Kepler-452b (a planet sometimes quoted to be an Earth 2.0 or Earth's Cousin based on its characteristics; also known by its Kepler Object of Interest designation KOI-7016.01) is an exoplanet orbiting the Sun-like star Kepler-452 about 1,402 light-years (430 pc) from Earth in the constellation Cygnus Kepler-452 est une étoile de type spectral G2, située à une distance d'environ 1 400 années-lumière de la Terre, dans la constellation boréale du Cygne. Sa température de surface est similaire à celle du Soleil mais, étant donné que son rayon est 10 % plus grand, sa luminosité est supérieure de 20 % à celle du Soleil Kepler-452 b est une exoplanète orbitant autour de l' étoile Kepler-452, elle a été découverte en 2015, cette exoplanète est probablement habitable et ressemble à la Terre, elle se situe à environ 1 400 années-lumière de la Terre Kepler-452b is an exoplanet approximately 1,400 light years from Earth. Orbiting the star Kepler-452, it is apart of the constellation Cygnus. As it was estimated to be of similar composition to Earth when it was discovered in 2015, it is believed that the planet may be a potential candidate for extraterrestrial life Kepler-452 is a G-type main-sequence star located about 1,402 light-years away from Earth in the Cygnus constellation. Although similar in temperature to the Sun, it is 20% brighter, 3.7% more massive and 11% larger. Alongside this, the star is approximately six billion years old and possesses a high metallicity

Kepler-442b (also known by its Kepler object of interest designation KOI-4742.01) is a confirmed near-Earth-sized exoplanet, likely rocky, orbiting within the habitable zone of the K-type main-sequence star Kepler-442, about 1,206 light-years (370 parsecs), from Earth in the constellation Lyra. The planet was discovered by NASA's Kepler spacecraft using the transit method, in which the dimming. Kepler est un télescope spatial développé par l'agence spatiale américaine, la NASA, pour détecter des exoplanètes.Lancé en 2009, Kepler a pour objectif d'effectuer un recensement des exoplanètes détectables situées dans une région de la Voie lactée de 115 degrés carrés en observant sur une période de plus de 3 ans l'intensité lumineuse de 145 000 étoiles pré-sélectionnées Kepler-37 b [1] est une exoplanète en orbite autour de l'étoile Kepler-37 dans la constellation de la Lyre [7], à ∼209 a.l. (∼64,1 pc) de la Terre [8]. À ce jour, c'est la plus petite exoplanète jamais découverte (PSR B1257+12 D exclue), avec une taille légèrement supérieure à celle de notre Lune.Elle est plus proche de son étoile que Mercure du Soleil (Mercure qui est la. Johannes Kepler [n 1] (ou Keppler), né le 27 décembre 1571 à Weil der Stadt et mort le 15 novembre 1630 à Ratisbonne dans l'électorat de Bavière, est un astronome célèbre pour avoir étudié l'hypothèse héliocentrique de Nicolas Copernic, affirmant que la Terre tourne autour du Soleil et surtout pour avoir découvert que les planètes ne tournent pas autour du Soleil en suivant des.

A Kepler-452b a G-típusú Kepler-452 csillag körül keringő exobolygó.A Kepler űrtávcsővel fedezték fel, a bejelentést a NASA tette meg 2015. július 23-án. A bolygó szuperföld, mely a lakható övezetben kering egy, a Naphoz nagyon hasonló csillag körül.. A bolygó 1400 fényévre található a Naprendszertől, így például a New Horizons szonda 59 000 km/órás. in Wikipedia, die vrye ensiklopedie Kepler-452b is 'n eksoplaneet wat om 'n G-tipe-ster, Kepler-452, wentel. Dit is deur die Kepler-ruimteteleskoop ontdek en Nasa het die ontdekking op 23 Julie 2015 aangekondig. Dit is die eerste eksoplaneet byna so groot soos die Aarde wat ontdek is in die bewoonbare sone van 'n ster soortgelyk aan die Son Kepler-452b er en exoplanet som er i kredsløb rundt om en hovedseriestjerne med spektrum G2V, ligesom vor Sol ved navn Kepler-452. Exoplaneten blev fundet af Kepler -rumteleskopet. Kepler-452 er lidt større end Solen mht. masse og dermed også lysstyrke Kepler-452b is an extrasolar planet. It circles a Sun-like star Kepler-452. It was identified by the Kepler space telescope. Its discovery was publicly announced by NASA on 23 July 2015

Kepler-452b - Wikipedi

Kepler-452 — Wikipédi

Kepler-452b (whiles nicknamed Yird 2.0 or Yird's Cousin based on its chairacteristics; kent whiles as Coruscant bi NASA, an aa kent bi its Kepler Object o Interest designation KOI-7016.01) is an exoplanet orbitin the Sun-lik starn Kepler-452 aboot 1,400 light-years (430 pc) frae Yird in the constellation Cygnus.It wis identified bi the Kepler space telescope, an its discovery wis annoonced bi. De Kepler-452b ass en Exoplanéit vum Stär Kepler-452, dee vum Weltraumteleskop Kepler identifizéiert gouf. D'Entdeckung gouf vun der NASA den 23. Juli 2015 publik gemaach. Besonnesch dobäi ass, datt et fir d'éischt war, datt en äerdähnleche Planéit fonnt gouf, deen ëm e Stär vun der Spektralklass G2V kreest. Zu der selwechter Klass gehéiert och eis Sonn. De Kepler-452b ass en. Kepler-452b là một hành tinh ngoài Hệ Mặt Trời quay quanh ngôi sao cấp G Kepler-452.Nó được xác định bởi kính thiên văn không gian Kepler và việc phát hiện ra nó đã được NASA công bố vào ngày 23 tháng 7 năm 2015. Đây là lần đầu tiên phát hiện hành tinh giống Trái Đất quay quanh trong vùng sinh sống của một ngôi sao.

Kepler-452b és un exoplaneta orbitant l'estrella de classe G Kepler-452.Va ser identificat pel telescopi espacial Kepler i la seva descoberta va ser anunciada per la NASA el 23 de juliol del 2015. És el primer planeta de mida semblant a la Terra que es troba orbitant dins de la zona habitable d'una estrella molt similar al Sol. És l'exoplaneta més semblant a la Terra després de Kepler-438b Kepler-452b, planet koji orbitira oko zvijezde klase G nazvane Kepler-452, identificiran svemirskom letjelicom Kepler.O njegovu otkriću NASA je izvijestila javnost 23. jula 2015. i prvi je planet veličine slične Zemlji otkriven kako orbitira unutar habitabilne zone zvijezde vrlo slične Suncu. Zvijezda je od Sunčeva sistema udaljena 1400 svjetlosnih godina što znači da bi New Horizonsu.

Kepler-452 b - Vikidia, l'encyclopédie des 8-13 an

  1. Kepler-22b, also known by its Kepler object of interest designation KOI-087.01, is an extrasolar planet orbiting within the habitable zone of the Sun-like star Kepler-22.It is located about 620 light-years (190 pc) from Earth in the constellation of Cygnus.It was discovered by NASA's Kepler Space Telescope in December 2011 and was the first known transiting planet to orbit within the habitable.
  2. The primary difference between Kepler-186f and Kepler-452b is that the former orbits a red dwarf star, while the latter orbits a very sun-like star. A planet around a red dwarf can be prone to trouble, due to the proximity needed to be in the habitable zone, including the large flares of M-dwarfs, and the assumed tidal locking of the system, again do to its proximity. Basically, while Kepler.
  3. Հայտնագործում. Kepler-452b մոլորակը հայտնաբերվել է «Քեփլեր» տիեզերական աստղադիտակով` տարանցիկ մեթոդով: Kepler-452 b մոլորակն առաջինն է բացահայտված ժայռապատ գերմոլորակներից: Այն պտտվում է կյանքի համար պիտանի գոտում` արևին շատ.

Kepler-452b Wikizilla, the kaiju encyclopedi

  1. Media in category Kepler-452b The following 26 files are in this category, out of 26 total. Kepler-452 in Milky Way ukrainian.jpg 5,599 × 5,599; 5.03 MB. Kepler-452-calculation-diagram.jpg 804 × 727; 61 KB. Kepler-452-photometry.jpg 1,093 × 528; 104 KB. Kepler-452b and Earth Size.jpg 4,534 × 2,550; 2.58 MB. Kepler-452b artist concept - animated 300px.gif 300 × 168; 6.41 MB. Kepler-452b.
  2. Kepler-452b - egzoplaneta, skriejanti aplink į Saulę panašią žvaigždę Kepler-452, esančią Gulbės žvaigždyne.Nuo Žemės Kepler-452b nutolusi maždaug 1400 šviesmečių.. Kepler-452b gali būti uolėtą paviršių turinti superžemė arba į Neptūną panaši dujinė planeta. Ji yra maždaug 60 % didesnė už Žemę, aplink savąją žvaigždę Kepler-452 arieja per 385 paras
  3. Kepler-452 b est la première exoplanète de cette taille orbitant dans la zone habitable d'une étoile de type solaire. Kepler-452 bmet 385 jours pour effectuer une révolution autour de son étoile. Ce faisant, la planète réside dans la zone habitablede son étoile,

Kepler-452 - Wikipedi

The illustration represents one possible appearance for Kepler-452b -- scientists do not know whether the planet has oceans and continents like Earth. Both planets orbit a G2-type star of about the same temperature; however, the star hosting Kepler-452b is 6 billion years old, 1.5 billion years older than our sun. As stars age, they become larger, hotter and brighter, as represented in the. Kepler-452b est utereus spinnends G-kindiduþ sterno sustem Kepler-452. Est frumest stainína Ufer-Erþa reus begitens spinnens inna sterno liƀamachtíg fera felu lích du Sune. Est sue 1,400 leuhaþ jera fram Erþa, nemadau 26 milío jera gestalden þer. Ana fora Erþa Gelíchí Lísta, est sechsta-managest Erþalích utereus kunþ du-hinadaga

Kepler-452b est planeta extrasolaris, inventus a telescopio spatiali Keplero, ex interpretatione datorum NASAe. Eius inventio publici iuris facta est die 23 mensis Iulii anno 2015. Descriptio [ recensere | fontem recensere ] Kepler-452b est maior Tellure (60%, uti aiunt), a qua distat circiter mille quadringentis annis luce mensis Kepler-452b. Quite the same Wikipedia. Just better About:Kepler-452b (a planet sometimes quoted to be an Earth 2.0 or Earth's Cousin based on its characteristics; also known by its Kepler Object of Interest designation KOI-7016.01) is an exoplanet orbiting the Sun-like star Kepler-452 about 1,402 light-years (430 pc) from Earth in the constellation Cygnus.It was identified by the Kepler space telescope, and its discovery was announced by NASA.

Kepler-452b is an extrasolar planet.It circles a Sun-like star Kepler-452.It was identified by the Kepler space telescope.Its discovery was publicly announced by NASA on 23 July 2015. It is about 1.7 times the size of Earth, and it is in the habitable zone of its star, so liquid water can exist on its surface Kepler-452 is a G-type main-sequence star located about 1,402 light-years away from Earth in the Cygnus constellation. Although similar in temperature to the Sun, it is 20% brighter, 3.7% more massive and 11% larger. Alongside this, the star is approximately six billion years old and possesses a high metallicity. Thus, Kepler-452 can be considered a solar twin, although it could considered to. Kepler-452b, geyrenıko ke teberê sistemê roci de maneno, geyrenıko neweyo ke terefê merdum u astronoman ra vêniyayo. Cayê xo taxımê astareyê Cygnusi dero. Tarixê 23 Temuze 2015 de [Astronom]]an vate ke yew planeto newe kewto menzılê asayışê inan. No planet rê namê Kepler-452bi vaciyao. Sistemê rocio ke tede Kepler-452b esto, sistemê rocia dınya ra pêro nezdiyo Kepler-452b estas ekstersunsistema planedo kiu orbitas la flavan nanon Kepler-452.Ĝi estis identigita de la kosma teleskopo Kepler kaj ĝia malkovro estis publike anoncita de NASA la 23-an de julio 2015. Ĝi estas la unua malkovrita tereca planedo orbitanta ene de la enloĝebla zono de stelo tre simila al la Suno.Ĝi estas la konata extersuna planedo la plej simila al Tero ĝisnune, post.

Kepler-442b - Wikipedi

The habitable zone of Kepler-186 is very small compared to that of Kepler-452 or the sun because it is a much smaller, cooler star. The size and extent of the habitable zone of Kepler-452 is nearly the same as that of the sun, but is slightly bigger because Kepler-452 is somewhat older, bigger and brighter. The size of the orbit of Kepler-452b is nearly the same as that of the Earth at 1.05 AU. La chanson « Kepler 452B » a été interprétée par Yann Pierre Paroles de la chanson : Si t'as du pétrole, Fais gaffe à ta gueule, De l'acier du fer, Tu vas prendre cher, Des gaz de schiste, Tu cours des risques, Des êtres vivants, Il va couler le sang. Kepler 452b, c'est nous.. Kepler-186f (also known by its Kepler object of interest designation KOI-571.05) is an exoplanet orbiting the red dwarf Kepler-186, about 500 light-years (178.5 parsecs, or nearly 5.0 × 10 15 km) from the Earth. It is the first planet with a radius similar to Earth's to be discovered in the habitable zone of another star. NASA's Kepler space telescope detected it using the transit method. Lêer:Kepler-452b artist concept.jpg. Lees in 'n ander taal; Hou dop; Wysig; Lêer; Lêergeskiedenis; Lêergebruik; Globale lêergebruik; Metadata; Grootte van hierdie voorskou: 800 × 450 piksels. Ander resolusies: 320 × 180 piksels | 640 × 360 piksels | 1 024 × 576 piksels | 1 280 × 720 piksels | 4 534 × 2 550 piksels. Oorspronklike lêer ‎ (4 534 × 2 550 piksels, lêergrootte: 2,2.

Kepler (télescope spatial) — Wikipédi

File:NASA-Kepler-452b-press-release-briefing video.webm. From Wikimedia Commons, the free media repository. Jump to navigation Jump to search. File; File history; File usage on Commons; File usage on other wikis; Metadata; Size of this JPG preview of this WEBM file: 800 × 450 pixels. Other resolutions: 320 × 180 pixels | 640 × 360 pixels | 1,280 × 720 pixels. Original file ‎ (WebM audio. Kepler 452 is a star system located in the Home Universe. The star itself is classified as a G2V, the same stellar class as Sol. The system itself is host to seven planets, two of which are inhabited by Humans. The system itself was originally discovered in 2015 with the first superearth, Kepler 452b being discovered in the same year. The system is home to approximately 21 million Human.

Kepler 452b | Object Shows Community | Fandom

Kepler-37 b — Wikipédi

Soubor:Kepler-452b artist concept.jpg. Jazyk; Sledovat; Editovat; Soubor; Historie souboru; Využití souboru; Globální využití souboru; Metadata; Velikost tohoto náhledu: 800 × 450 pixel ů. Jiná rozlišení: 320 × 180 pixelů | 640 × 360 pixelů | 1 024 × 576 pixelů | 1 280 × 720 pixelů | 4 534 × 2 550 pixelů. Původní soubor ‎ (4 534 × 2 550 pixelů, velikost souboru: 2, Using chemical propulsion at the speed of New Horizons, the human remains would take approximately 20 million years to reach Kepler 452b. Using something more advanced like Orion, NERVA, or a laser-powered light sail would cut the trip time down by a factor of maybe 10-1000 depending on engineering constraints This is a redirection page In case the javascript redirection does not work, please click on the link below: http://www.nasa.gov/mission_pages/kepler/main/index.htm

Kepler-155c | Weird and wonderfull space Wiki | Fandom

De Kepler-452 ass e Gielen Zwerg am Stärebild Cygnus.Hie läit op enger Distanz vun ongeféier 1400 Liichtjoer vun eiser Sonn ewech. De Stär huet eng Temperatur, déi där vun eiser Sonn gläicht. De Stär ass awer ëm 20 % méi hell an huet een ëm 10 % méi grousse Radius.Seng Spektralklass (G2) ass déi selwecht wéi déi vun eiser Sonn.. Déi bis elo séierst Raumsonden Helios 1 an 2. De Kepler-Weltraumteleskop ass e Weltraumteleskop vun der NASA, deen am Mäerz 2009 gestart gouf, fir no extrasolare Planéite ze sichen. De Projet ass nom däitschen Astronom Johannes Kepler genannt, deen als éischten d'Gesetzméissegkeete vun de Planéitenëmlafbunnen erkannt hat. Wéinst technesche Problemer ass den Teleskop zanter dem 15. August 2013 ausser Betrib

Johannes Kepler — Wikipédi

Kepler-452b, Constellation: Lyra. 225 likes. Kepler-438b is a near-Earth-sized exoplanet with a radius 1.12 times that of Earth Kepler 452B is a character idea by Aca soccer. He is a 10 star character in the Arcade (which means he is very hard to defeat, he jumps very high, most of the time, uses dash, and plays like a human. He is also very good at countering power shots). He has a very hard unlock requirements (which also makes him a very good character), and is the opposite of the first alien in the game, Kepler 22B. De la Wikipedia, enciclopedia liberă Kepler-452 este o stea de tip spectral G2, situată la distanță de circa 1.400 de ani-lumină de Pământ, în constelația boreală Lebăda Kepler-452b. Advanced search: Message boards: SETI@home Science: Kepler-452b Message board moderation. To post messages, you must log in. 1 · 2 · Next. Author Message; Keith T. Volunteer tester. Send message Joined: 23 Aug 99 Posts: 961 Credit: 537,293 RAC: 9: Message 1704321 - Posted.

Kepler-452b - Wikipédi

If Kepler 452b has a 'base' temperature of 265 K. , the presence of an Earth-like atmosphere would presumably raise this to somewhat above the current average temperature of Earth. Since the Kepler planet has a mass several times that of Earth, it seems probable that it retains a thicker atmosphere. This could lead to even better heat retention, and a yet higher temperature. ID: 1730378. Kepler-452b, Constellation: Lyra. 232 likes. Kepler-438b is a near-Earth-sized exoplanet with a radius 1.12 times that of Earth

An extrasolar planet (or exoplanet) is a natural planet in a planetary system outside our own solar system.. In 2013, estimates of the number of terrestrial planets in the Milky Way ranged from at least 17 billion to at least 144 billion. The smaller estimate studied planet candidates gathered by the Kepler space observatory. Among them are 461 Earth-size planets, at least four of which are in. Kepler-22b, also known by its Kepler object of interest designation KOI-087.01, is an extrasolar planet orbiting within the empirical habitable zone of the Sun-like star Kepler-22.It is located about 638 light-years (196 pc) from Earth in the constellation of Cygnus.It was discovered by NASA's Kepler Space Telescope in December 2011 and was the first known transiting planet to orbit within the.

  1. Kepler-452b non potest videri nullaque eius imago patet cuilibet. Inventus est per lucis defectionem, nam aliquando, dum convertitur circa solem suum, huius lucem occulit nobis ex parte. Inventio tamen suum habet pondus, quia demonstrat alios esse planetas per universum frequentissimos. Ex quibus alii vitae non favent; alii vero possunt aliquod vitae genus sustinere, immo et vitam humanam.
  2. Kepler-452 estas flava nano situiĝanta je 1400 lumo-jaroj el la Tero en la konstelacio de Cigno. Ĝi havas similan temperaturon kiel la Suno, sed estas 20 procente pli brila, 3,7 procente pli masiva kaj havas 11 procente pli grandan diametron. Ĝia gravito estas 4,32±0,09 cgs. La stelo aĝas ĉirkaŭ 1,5 miliardojn da jaroj pli ol la Suno, aĝante ses miliardojn da jaroj
  3. Kepler-452b - Wikipedia, den frie encyklopæd
  4. Kepler-452b - Simple English Wikipedia, the free encyclopedi
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