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This image was selected as picture of the day on Wikimedia Commons for 25 February 2016. It was captioned as follows: English: Artist's speculative impression of a Hot Jupiter, a type of extrasolar planet discovered with the Hubble Space Telescope. The planet, comparable in mass to Jupiter, is so close to its red dwarf star that it completes an orbit in 10.5 hours. The planet is only 750,000 miles (about 1.207 million kilometres) from the star, 1/130th the distance between Earth and the Sun. Other languages:
Čeština: Umělecká představa exoplanety třídy Hot Jupiter objevené pomocí Hubbleova vesmírného dalekohledu. Planeta o hmotnosti srovnatelné s Jupiterem obíhá tak blízko (přibližně 1 200 milionů km, tedy asi 1/30 vzdálenosti Země od Slunce) kolem hvězdy třídy červený trpaslík, že doba jejího oběhu je pouze 10,5 hodiny. Deutsch: Künstlerische Impression eines Heißen Jupiters, eines Typs von extrasolarem Planet, der mit dem Hubble-Weltraumteleskop entdeckt wurde. Der Planet, der eine dem Jupiter vergleichbare Masse besitzt, ist so nahe an seinem Roten Zwergstern, dass er eine Umlaufzeit von nur 10,5 Stunden hat. Der Planet umrundet den Zentralstern in einer Entfernung von nur ungefähr 1,207 Millionen Kilometern, was etwa 1/130 der Entfernung von Erde und Sonne entspricht. English: Artist's speculative impression of a Hot Jupiter, a type of extrasolar planet discovered with the Hubble Space Telescope. The planet, comparable in mass to Jupiter, is so close to its red dwarf star that it completes an orbit in 10.5 hours. The planet is only 750,000 miles (about 1.207 million kilometres) from the star, 1/130th the distance between Earth and the Sun. Español: Impresión artística de un tipo único de planeta extrasolar descubierto con el telescopio espacial Hubble. El planeta está tan cerca de su estrella madre, que completa una órbita en 10,5 horas terrestres. El planeta se encuentra a una distancia de tan solo 1,2 millones de kilómetros de la estrella, o sea 1/130ª de la distancia entre la Tierra y el Sol. Italiano: Un pianeta gioviano caldo come immaginato da un'artista. Questo è un tipo di pianeta extrasolare scoperto con il telescopio spaziale Hubble di massa simile a quella di Giove in orbita ravvicinata alla sua stella madre. Nederlands: Een artistieke impressie van een hete Jupiter, die door de ruimtetelescoop Hubble is ontdekt. Português: Este é um conceito artístico de um tipo único de planeta extrassolar descoberto com o telescópio espacial Hubble. O planeta está tão próximo da sua estrela-mãe, que completa uma órbita em 10,5 horas terrestres. O exoplaneta orbita sua estrela a uma distância de apenas 1,2 milhões de quilômetros, ou 1/130 a distância entre a Terra e o Sol. Български: Художествено представяне на уникален вид екзопланета наречена "Горещ Юпитер". Планетата с размери на Юпитер е толкова близо до своята звезда червено джудже, че обикаля около нея за едва 10,5 часа. Македонски: Уметничка претстава на планета откриена со вселенскиот телескоп „Хабл“. Планетата е толку блиску до својата ѕвезда што прави круг околу неа за 10,5 часа, односно нејзината година трае помалку од половина земски ден. Оддалечена е само 1,2 милиони километри од неа — растојание 130 пати помало од она на Земјата од Сонцето. Русский: Художественное представление тесной системы из красного карлика и газового гиганта, обращающегося вокруг звезды на расстоянии 1,2 млн км с периодом 10,5 ч Українська: Художнє представлення гарячого юпітера (тип планет поза Сонячною системою), який був відкритий телескопом Габбл. Планета близька за масою до Юпітера та близька до червоного карлика, навколо якого обертається з періодом 10.5 годин. Планета знаходиться від зірки на відстані всього 1.2 млн. кілометрів, що складає 1/130 відстані між Землею та Сонцем. 한국어: 허블 우주 망원경으로 발견된 외계 행성형의 뜨거운 목성을 화가가 추측하여 그린 상상도. 그 질량이 목성에 필적하는 이 행성은 적색 왜성에 너무나 가깝기에 10.5 시간에 1바퀴를 완주한다. 이 행성은 적색 왜성으로부터 120만 7천 km 거리에 있으며, 이는 지구와 태양 사이의 거리의 1/130 에 해당된다. |
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This image was selected as picture of the day on Bengali Wikipedia.
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Summary
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English: This is an artist's impression of a unique type of extrasolar planet discovered with the Hubble Space Telescope. The planet is so close to its star that it completes an orbit in 10.5 hours. The planet is only 750,000 miles (about 1.207 Million kilometres) from the star, or 1/130th the distance between Earth and the Sun.
The Jupiter-sized planet orbits an unnamed red dwarf star that lies in the direction of the Galactic Centre; the exact stellar distance is unknown. Hubble detected the planet in a survey that identified 16 Jupiter-sized planets in short-period, edge-on orbits (as viewed from Earth) that pass in front of their parent stars. Hubble could not see the planets, but measured the dimming of starlight as the planets passed in front of their stars. This illustration presents a purely speculative view of what such a "hot Jupiter" might look like. It could have a powerful magnetic field that traps charged particles from the star. These particles create glowing auroral rings around the planet's magnetic poles. A powerful magnetic flux tube links the planet and star. This enhances stellar activity and triggers powerful flares. A powerful stellar wind creates a bow shock around the planet. The planet's atmosphere seethes at 1,650 degrees Celsius. |
| Date | |
| Source | http://www.spacetelescope.org/images/heic0612c/ |
| Author | NASA, ESA and A. Schaller |
Licensing
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ESA/Hubble images, videos and web texts are released by the ESA under the Creative Commons Attribution 4.0 International license and may on a non-exclusive basis be reproduced without fee provided they are clearly and visibly credited. Detailed conditions are below; see the ESA copyright statement for full information. For images created by NASA or on the hubblesite.org website, or for ESA/Hubble images on the esahubble.org site before 2009, use the {{PD-Hubble}} tag.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
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| current | 17:37, 7 January 2019 | | 5,600 × 4,800 (6.81 MB) | Kesäperuna | 100% JPEG quality from full quality TIFF. |
| 14:58, 4 November 2013 |  | 5,600 × 4,800 (2.27 MB) | Stas1995 | User created page with UploadWizard |
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