Question: The probe sent to the planet with Ausonia Mensa by nationals of the country with Goa launched on what?

full_context: Document 1: Samurai: Historian H. Paul Varley notes the description of Japan given by Jesuit leader St. Francis Xavier (1506–1552): "There is no nation in the world which fears death less." Xavier further describes the honour and manners of the people: "I fancy that there are no people in the world more punctilious about their honour than the Japanese, for they will not put up with a single insult or even a word spoken in anger." Xavier spent the years 1549–1551 converting Japanese to Christianity. He also observed: "The Japanese are much braver and more warlike than the people of China, Korea, Ternate and all of the other nations around the Philippines."
Document 2: Mars Orbiter Mission: The Mars Orbiter Mission (MOM), also called Mangalyaan (``Mars - craft '', from Sanskrit: मंगल mangala,`` Mars'' and यान yāna, ``craft, vehicle ''), is a space probe orbiting Mars since 24 September 2014. It was launched on 5 November 2013 by the Indian Space Research Organisation (ISRO). It is India's first interplanetary mission and ISRO has also become the fourth space agency to reach Mars, after the Soviet space program, NASA, and the European Space Agency. It is the first Asian nation to reach Mars orbit, and the first nation in the world to do so in its first attempt.
Document 3: Samurai: 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"). Anjiro was not an intellectual, but he impressed Xavier because he took careful notes of everything he said in church. 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. They were hard workers and respectful of authority. 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.
Document 4: Ausonia Montes: Ausonia Montes is a mountain in the Mare Tyrrhenum quadrangle of Mars, at 25.42° south latitude and 99.04° east longitude. It is across and was named after an albedo feature name.
Document 5: Echus Chasma: Echus Chasma is a chasma in the Lunae Planum high plateau north of the Valles Marineris canyon system of Mars. It is in the Coprates quadrangle. Clay has been found within it, meaning that water once sat there for a time. It may have been one of the many lakes that have been advanced for the Martian past. Research from 2010 suggests that Mars also had lakes along parts of the equator which is where Echus Chasma lies. 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. 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. 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. In this study, channels were discovered that connected lake basins near Ares Vallis. When one lake filled up, its waters overflowed the banks and carved the channels to a lower area where another lake would form. These dry lakes would be targets to look for evidence (biosignatures) of past life.
Document 6: Printing in Goa: Many factors contributed to the necessity of the initiation of printing in the subcontinent, the primary being evangelization and the Jesuits were solely responsible for this. Francis Xavier is known to have been teaching the Bible in Tharangambadi (Tranquebar), Tamil Nadu around 1542. Also, when the Viceroy of Goa, on behalf of King Joao III of Portugal, opened schools for Indians, Francis Xavier pressured Portugal to make printing presses available to India, Ethiopia and Japan. Meanwhile, the Emperor of Abyssinia (now Ethiopia) also requested Portugal to send a press along with missionaries. Consequently, the first batch of Jesuit missionaries, along with the printing press, left for Ethiopia on March 29, 1556, on a Spanish ship. The Patriarch designate of Abyssinia, Joao Nunes Barreto, as well as a team of technicians accompanied the press.
Document 7: Ausonia Mensa: Ausonia Mensa is a mensa in the Hellas quadrangle of Mars, located at 30.3° S and 262.3° W. It is 103 km across and was named after an albedo feature name. The term "Mensa" is used for a flat-topped prominence with cliff-like edges. Ausonia Mensa has many small channels. Some features look like alluvial fans. These channels add to the mass of evidence that water once flowed on Mars. Images of curved channels have been seen in images from Mars spacecraft dating back to the early seventies with the Mariner 9 orbiter.
Document 8: Mars 7: Mars 7 was launched by a Proton-K carrier rocket with a Blok D upper stage, flying from Baikonur Cosmodrome Site 81/24. The launch occurred at 17:00:17 UTC on 9 August 1973, with the first three stages placing the spacecraft and upper stage into a low Earth parking orbit before the Blok D fired to propel Mars 7 into heliocentric orbit bound for Mars. The spacecraft performed a course correction on 16 August 1973.
Document 9: Seigō Nakano: Nakano sought to bring about a rebirth of Japan through a blend of the samurai ethic, Neo-Confucianism, and populist nationalism modeled on European fascism. He saw Saigō Takamori as epitomizing the 'true spirit' of the Meiji "ishin", and the task of modern Japan to recapture it.
Document 10: Kounotori 5: Kounotori 5 was successfully launched with a H-IIB carrier rocket flying from pad 2 of the Yoshinobu Launch Complex at Tanegashima at 11:50:49 UTC on 19 August 2015. Communication and three-axis attitude controls were established shortly after the launch. Phase Maneuver was performed by 19:25 UTC on August 20, and the first Height Adjustment Maneuver by 17:55 UTC on August 22. The second and third Height Adjustment Maneuver were performed by 03:07 and 06:12 UTC on August 24, respectively.
Document 11: Mars Orbiter Mission: 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. The launch window was approximately 20 days long and started on 28 October 2013. 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). After a 298 - day transit to Mars, it was successfully inserted into Mars orbit on 24 September 2014.
Document 12: Chandrayaan-1: Chandrayaan-1 (, 'Moon craft' ) was the first Indian lunar probe under Chandrayaan program. It was launched by the Indian Space Research Organisation in October 2008, and operated until August 2009. The mission included a lunar orbiter and an impactor. India launched the spacecraft using a PSLV-XL rocket, serial number C11, on 22 October 2008 at 00:52 UTC from Satish Dhawan Space Centre, at Sriharikota about north of Chennai. The mission was a major boost to India's space program, as India researched and developed its own technology in order to explore the Moon. The vehicle was inserted into lunar orbit on 8 November 2008.
Document 13: Capri Mensa: Capri Mensa is a mesa in the Coprates quadrangle of Mars at 14° south latitude and 47.4° west longitude. It is about 275 km long and was named after a classical albedo feature name.
Document 14: Outflow channels: Outflow channels are extremely long, wide swathes of scoured ground on Mars, commonly containing the streamlined remnants of pre-existing topography and other linear erosive features indicating sculpting by fluids moving downslope. Channels extend many hundreds of kilometers in length and are typically greater than one kilometer in width; the largest valley (Kasei Vallis) is around long, greater than wide and exceeds in depth cut into the surrounding plains. These features tend to appear fully sized at fractures in the Martian surface, either from chaos terrains or from canyon systems or other tectonically controlled, deep graben, though there are exceptions. Besides their exceptional size, the channels are also characterized by low sinuosities and high width:depth ratios compared both to other Martian valley features and to terrestrial river channels. Crater counts indicate that most of the channels were cut since the early Hesperian, though the age of the features is variable between different regions of Mars. Some outflow channels in the Amazonis and Elysium Planitiae regions have yielded ages of only tens of million years, extremely young by the standards of Martian topographic features.
Document 15: Samurai: Katō Kiyomasa was one of the most powerful and well-known lords of the Sengoku Era. He commanded most of Japan's major clans during the invasion of Korea (1592–1598). In a handbook he addressed to "all samurai, regardless of rank" he told his followers that a warrior's only duty in life was to "...grasp the long and the short swords and to die". He also ordered his followers to put forth great effort in studying the military classics, especially those related to loyalty and filial piety. He is best known for his quote: "If a man does not investigate into the matter of Bushido daily, it will be difficult for him to die a brave and manly death. Thus it is essential to engrave this business of the warrior into one's mind well."
ground_truth: a Polar Satellite Launch Vehicle (PSLV) rocket C25
sub_queries: Where was Goa? Answer: India
Where is Ausonia Mensa found? Answer: Mars
India 's mangalyaan was sent to the #2 by launching Answer: a Polar Satellite Launch Vehicle (PSLV) rocket C25