Question: What did Goa's country launch to send the mangalyaan to the planet where Chasma Boreale was found?

<P0-S0> The Mars Orbiter Mission probe lifted - off from the First Launch Pad at Satish Dhawan Space Centre (Sriharikota Range SHAR), Andhra Pradesh, using a Polar Satellite Launch Vehicle (PSLV) rocket C25 at 09: 08 UTC on 5 November 2013. <P0-S1> The launch window was approximately 20 days long and started on 28 October 2013. <P0-S2> The MOM probe spent about a month in Earth orbit, where it made a series of seven apogee - raising orbital manoeuvres before trans - Mars injection on 30 November 2013 (UTC). <P0-S3> After a 298 - day transit to Mars, it was successfully inserted into Mars orbit on 24 September 2014. <SEP> <P1-S0> mars 2m no.522 was launched at 10:33:00 utc on 2 april 1969 atop a proton-k 8k78k carrier rocket with a blok d upper stage, flying from baikonur cosmodrome site 81/24. <P1-S1> one of the first stage engines caught fire almost immediately at liftoff. <P1-S2> the remaining engines managed to compensate for about 30 seconds of flight, but the thrust section fire eventually resulted in loss of control. <P1-S3> the proton pitched over and began flying horizontally before ground controllers sent a manual shutoff command. <P1-S4> the vehicle nosedived into the ground just outside the launch complex 41 seconds after launch. <P1-S5> subsequent examination found that a missing drain plug allowed nitrogen tetroxide to leak out and start a fire. <SEP> <P2-S0> In December 1547, Francis was in Malacca (Malaysia) waiting to return to Goa (India) when he met a low-ranked samurai named Anjiro (possibly spelled "Yajiro"). <P2-S1> Anjiro was not an intellectual, but he impressed Xavier because he took careful notes of everything he said in church. <P2-S2> Xavier made the decision to go to Japan in part because this low-ranking samurai convinced him in Portuguese that the Japanese people were highly educated and eager to learn. <P2-S3> They were hard workers and respectful of authority. <P2-S4> In their laws and customs they were led by reason, and, should the Christian faith convince them of its truth, they would accept it en masse. <SEP> <P3-S0> echus chasma is a chasma in the lunae planum high plateau north of the valles marineris canyon system of mars. <P3-S1> it is in the coprates quadrangle. <P3-S2> clay has been found within it, meaning that water once sat there for a time. <P3-S3> it may have been one of the many lakes that have been advanced for the martian past. <P3-S4> research from 2010 suggests that mars also had lakes along parts of the equator which is where echus chasma lies. <P3-S5> although earlier research had showed that mars had a warm and wet early history that has long since dried up, these lakes existed in the hesperian epoch, a much later period. <P3-S6> using detailed images from nasa's mars reconnaissance orbiter, the researchers speculate that there may have been increased volcanic activity, meteorite impacts or shifts in mars' orbit during this period to warm mars' atmosphere enough to melt the abundant ice present in the ground. <P3-S7> volcanoes would have released gases that thickened the atmosphere for a temporary period, trapping more sunlight and making it warm enough for liquid water to exist. <P3-S8> in this study, channels were discovered that connected lake basins near ares vallis. <P3-S9> when one lake filled up, its waters overflowed the banks and carved the channels to a lower area where another lake would form. <P3-S10> these dry lakes would be targets to look for evidence (biosignatures) of past life. <SEP> <P4-S0> Chasma Boreale is a large canyon in Mars's north polar ice cap in the Mare Boreum quadrangle of Mars at 83° north latitude and 47.1° west longitude. <P4-S1> It is about long and was named after a classical albedo feature name. <P4-S2> The canyon's sides reveal layered features within the ice cap that result from seasonal melting and deposition of ice, together with dust deposits from Martian dust storms. <P4-S3> Information about the past climate of Mars may eventually be revealed in these layers, just as tree ring patterns and ice core data do on Earth. <P4-S4> Both polar caps also display grooved features, probably caused by wind flow patterns. <P4-S5> The grooves are also influenced by the amount of dust. <P4-S6> The more dust, the darker the surface. <P4-S7> The darker the surface, the more melting as dark surfaces absorb more energy.