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dc.contributor.author |
Churyumov, K.I. |
|
dc.date.accessioned |
2015-04-03T19:41:34Z |
|
dc.date.available |
2015-04-03T19:41:34Z |
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dc.date.issued |
2005 |
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dc.identifier.citation |
Rosetta space mission to Comet 67P/Churyumov−Gerasimenko / K.I. Churyumov // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 453-457. — Бібліогр.: 1 назв. — англ. |
uk_UA |
dc.identifier.issn |
0233-7665 |
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dc.identifier.uri |
http://dspace.nbuv.gov.ua/handle/123456789/79698 |
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dc.description.abstract |
On March 2, 2004 Rosetta space mission successfully started from the Kourou cosmodrom to Comet 67P/Churyumov–Gerasimenko. Upon entering orbit around the nucleus observations will be made as the comet becomes more active as it journeys towards the Sun. A lander, named Philae, will be deployed and attempt to make the first ever controlled landing on a comet. On its 10 year journey Rosetta will fly-by two asteroids, namely, 2867 Steins in September 2008 and 21 Lutethia in July 2010. Rosetta will be the first spacecraft to orbit a comet’s nucleus. It will be the first spacecraft to fly alongside a comet as it heads towards the inner Solar System. Rosetta will be the first spacecraft to examine from close proximity how a frozen comet is transformed by the warmth of the Sun. Shortly after its arrival at Comet 67P/Churyumov–Gerasimenko, the Rosetta orbiter will despatch a robotic lander for the first controlled touchdown on a comet nucleus. The Rosetta lander’s instruments will obtain the first images from a comet’s surface and make the first in situ analysis of the relict matter of the Solar System. |
uk_UA |
dc.language.iso |
en |
uk_UA |
dc.publisher |
Головна астрономічна обсерваторія НАН України |
uk_UA |
dc.relation.ispartof |
Кинематика и физика небесных тел |
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dc.subject |
MS5: Dynamics and Physics of Solar System Bodies |
uk_UA |
dc.title |
Rosetta space mission to Comet 67P/Churyumov−Gerasimenko |
uk_UA |
dc.type |
Article |
uk_UA |
dc.status |
published earlier |
uk_UA |
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