Rosetta space mission to Comet 67P/Churyumov−Gerasimenko
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 att...
Збережено в:
| Опубліковано в: : | Кинематика и физика небесных тел |
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| Дата: | 2005 |
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| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
Головна астрономічна обсерваторія НАН України
2005
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| Онлайн доступ: | https://nasplib.isofts.kiev.ua/handle/123456789/79698 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Цитувати: | 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. |
Репозитарії
Digital Library of Periodicals of National Academy of Sciences of Ukraine| Резюме: | 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.
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| ISSN: | 0233-7665 |