Titan makes up 95% of the mass of all 82 satellites of Saturn. Titan's diameter is 5152 km, which means that it is larger than the Moon by 50%, and it is also significantly larger than Mercury. On the satellite, a subsurface ocean is possible, the theory of the presence of which has already been advanced earlier by some scientists. It is located under a layer of ice and consists of 10% ammonia, which is a natural antifreeze for it and does not allow the ocean to freeze. On the one hand, the ocean contains a huge amount of salt, which makes the likelihood of life in it hardly possible. But on the other hand, since chemical processes constantly occur on Titan, forming molecules of complex hydrocarbon substances, this can lead to the emergence...
Gas giant satellites are generally believed to form in circumplanetary disks (CPDs): a gas disk cont...
International audienceCassini's VIMS and the RADAR have been investigating Titan's surface since 200...
International audienceThe Cassini-Huygens instruments revealed that Titan, Saturn's largest moon, ha...
This paper aims at considering the issues of regression modeling of the surface of Saturn's moon Tit...
Saturn's moon, Titan is a geomorphologically active planetary object, and its surface is influenced ...
Titan, Saturn's largest satellite, is subject to solid body tides exerted by Saturn on the timescale...
International audienceThe investigation of Titans surface chemical composition is of great importanc...
We investigate Titan's low- and mid-latitude surface using spectro-imaging near-infrared data from C...
International audienceThe Cassini-Huygens mission that explored the Saturn system during the period ...
International audienceOur understanding of Titan, Saturn's largest satellite, has recently been cons...
Saturn's largest natural satellite, Titan, is an icy moon expected to harbour a liquid sub-surface w...
Abstract Our understanding of Titan, Saturn’s largest satellite, has recently been consid-erably enh...
Gas giant satellites are generally believed to form in circumplanetary disks (CPDs): a gas disk cont...
International audienceCassini's VIMS and the RADAR have been investigating Titan's surface since 200...
International audienceThe Cassini-Huygens instruments revealed that Titan, Saturn's largest moon, ha...
This paper aims at considering the issues of regression modeling of the surface of Saturn's moon Tit...
Saturn's moon, Titan is a geomorphologically active planetary object, and its surface is influenced ...
Titan, Saturn's largest satellite, is subject to solid body tides exerted by Saturn on the timescale...
International audienceThe investigation of Titans surface chemical composition is of great importanc...
We investigate Titan's low- and mid-latitude surface using spectro-imaging near-infrared data from C...
International audienceThe Cassini-Huygens mission that explored the Saturn system during the period ...
International audienceOur understanding of Titan, Saturn's largest satellite, has recently been cons...
Saturn's largest natural satellite, Titan, is an icy moon expected to harbour a liquid sub-surface w...
Abstract Our understanding of Titan, Saturn’s largest satellite, has recently been consid-erably enh...
Gas giant satellites are generally believed to form in circumplanetary disks (CPDs): a gas disk cont...
International audienceCassini's VIMS and the RADAR have been investigating Titan's surface since 200...
International audienceThe Cassini-Huygens instruments revealed that Titan, Saturn's largest moon, ha...