This page describes an image Comet 67P/Churyumov-Gerasimenko
Image caption:
Comet 67P/Churyumov–Gerasimenko's nucleus is a "dirty snowball" made of a mixture of frozen materials and dust. It is shaped like two large lobes: one 4.1 km × 3.3 km × 1.8 km, the other 2.6 km × 2.3 km × 1.8 km. These lobes are connected by a small bridge. When a cometary nucleus such as this nears the Sun its frozen, icy material is heated, turning into gas. This, combined with the embedded dust, provide the material for the comet's characteristic coma and tail.
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Image credit:
ESA/Rosetta/NAVCAM Credit Link
Related glossary terms:
Comet
, Comet Nucleus
Categories:
Solar System
Image license: Creative Commons Attribution-ShareAlike 3.0 IGO Creative Commons Attribution-ShareAlike 3.0 IGO icons
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Captions in Different Languages:
Image caption: ধূমকেতু ৬৭পি/চুর্যমভ -গেরসিমেনক-এর নিউক্লিয়াস হিমায়িত পদার্থ এবং ধুলোর মিশ্রণে তৈরি একটি "ডার্টি স্নোবল"। এটি দুটি বড় লোবের মতো আকৃতির: একটি ৪.১ কিমি × ৩.৩ কিমি × ১.৮ কিমি, অন্যটি ২.৬ কিমি × ২.৩ কিমি × ১.৮ কিমি। এই লবগুলি একটি ছোট সেতু দ্বারা সংযুক্ত। যখন এর মতো ধূমকেতুর নিউক্লিয়াস সূর্যের কাছাকাছি আসে তখন তার হিমায়িত, বরফযুক্ত উপাদান উত্তপ্ত হয়, গ্যাসে পরিণত হয়। এটি, এমবেডেড ধুলোর সাথে মিলিত, ধূমকেতুর বৈশিষ্ট্যযুক্ত কোমা এবং লেজের জন্য উপাদান সরবরাহ করে।
Image credit: ঈএসএ/রোসেটটা/নাভক্যাম
Related glossary terms: Comet , Comet Nucleus Caption translation status: Not yet approved by a reviewer
Caption translators: Raktim Mukherjee
Image caption: Le noyau de la comète 67P/Tchourioumov-Guérassimenko (ou 67P/Чурюмова — Герасименко en Russe) est une "boule de neige sale" composée d'un mélange de glaces et de poussières. Il a la forme de deux grands lobes : l'un de 4,1 km × 3,3 km × 1,8 km, l'autre de 2,6 km × 2,3 km × 1,8 km. Ces lobes sont reliés par un petit pont. Lorsqu'un noyau cométaire tel que celui-ci s'approche du Soleil, sa matière gelée et glacée est chauffée et se transforme en gaz. Ce gaz, combiné à la poussière qui s'y trouve, constitue la matière de la coma et de la queue, qui sont caractéristiques de la comète.
Image credit: ESA/Rosetta/NAVCAM
Related glossary terms: Comète , Noyau de la comète Caption translation status: Approved by a reviewer
Caption translators: Assia Nechache, Emmanuel Rollinde
Caption reviewers: Nicolas Bott, Mamadou Mahamat Djabbi, Daniel Hestroffer
Image caption: Il nucleo della cometa 67P/Churyumov-Gerasimenko è una "palla di neve sporca" composta da una miscela di materiali ghiacciati e polvere. Ha la forma di due grandi lobi: uno di 4,1 km × 3,3 km × 1,8 km, l'altro di 2,6 km × 2,3 km × 1,8 km. Questi lobi sono collegati da un piccolo ponte. Quando un nucleo cometario come questo si avvicina al Sole, il suo materiale ghiacciato si riscalda, trasformandosi in gas. Questo, insieme alla polvere incorporata, fornisce il materiale per la chioma e la coda, caratteristiche della cometa.
Image credit: ESA/Rosetta/NAVCAM
Related glossary terms: Cometa , Nucleo della cometa Caption translation status: Approved by a reviewer
Caption translators: Giuliana Giobbi
Caption reviewers: Rosa Valiante, Rodolfo Canestrari
Image caption: 67P/Churyumov-Gerasimenko 彗星的彗核是一个由冰冻物质和尘埃混合而成的 "脏雪球"。它的形状像两个大耳叶:一个体积为4.1 千米 × 3.3 千米 × 1.8 千米,另一个为 2.6 千米 × 2.3 千米 × 1.8 千米。这些耳叶由一座小桥连接在一起。当这样的彗星核接近太阳时,它的冰冻物质会被加热,变成气体。这些气体与内部的尘埃共同组成了彗星特有的彗发和彗尾。
Image credit: 欧空局/Rosetta/NAVCAM
Related glossary terms: 彗星 , 彗核 Caption translation status: Not yet approved by a reviewer
Caption translators: Hu Xueying
Image caption: 67P/Churyumov-Gerasimenko 彗星的彗核是一個由冰凍物質和塵埃混合而成的 "臟雪球"。它的形狀像兩個大耳葉:一個體積為4.1 千米 × 3.3 千米 × 1.8 千米,另一個為 2.6 千米 × 2.3 千米 × 1.8 千米。這些耳葉由一座小橋連接在一起。當這樣的彗星核接近太陽時,它的冰凍物質會被加熱,變成氣體。這些氣體與內部的塵埃共同組成了彗星特有的彗發和彗尾。
Image credit: 歐空局/Rosetta/NAVCAM
Related glossary terms: 彗星 , 彗核 Caption translation status: Not yet approved by a reviewer
Caption translators: An automated transliteration from the simplified Chinese translation by - Hu Xueying