Comet: Difference between revisions
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A '''comet''' is composed of [[ice]], [[gas]] and dust, | A '''comet''' is composed of [[ice]], [[gas]] and dust, and has a highly eccentric, [[elliptical orbit]] around the [[Sun]]. Comets become visible as they approach the Sun and can be much larger than they seem - the tails of some comets are over 1,000,000 km long. Examples include [[Halley's Comet]] and the [[Tago-Sato-Kosaka Comet]]. | ||
In November 2014, the [[European Space Agency]] successfully landed a probe on a [[comet nucleus]], the first time in history that this had been achieved. ''[[Philae (comet lander)|Philae]]'' sent back data for three days as it probed the surface of [[67P/Churyumov–Gerasimenko]]. | In November 2014, the [[European Space Agency]] successfully landed a probe on a [[comet nucleus]], the first time in history that this had been achieved. ''[[Philae (comet lander)|Philae]]'' sent back data for three days as it probed the surface of [[67P/Churyumov–Gerasimenko]]. | ||
Revision as of 14:41, 2 August 2020
A comet is composed of ice, gas and dust, and has a highly eccentric, elliptical orbit around the Sun. Comets become visible as they approach the Sun and can be much larger than they seem - the tails of some comets are over 1,000,000 km long. Examples include Halley's Comet and the Tago-Sato-Kosaka Comet.
In November 2014, the European Space Agency successfully landed a probe on a comet nucleus, the first time in history that this had been achieved. Philae sent back data for three days as it probed the surface of 67P/Churyumov–Gerasimenko.