![](\"http:\/\/www.esa.int\/var\/esa\/storage\/images\/esa_multimedia\/images\/2017\/05\/listening_for_cassini\/16928698-2-eng-GB\/Listening_for_Cassini_small.jpg\")
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\nESA\u2019s sensitive tracking antennas at New Norcia, Western Australia, and Malarg\u00fce, Argentina (seen here in 2012), are being called in to help gather crucial science data during Cassini\u2019s last months in orbit, dubbed the Grand Finale.\n<\/p>\n
\nThe mission will end on 15 September, when Cassini plunges into Saturn\u2019s atmosphere, bringing to a close one of the most successful exploration endeavours ever (more information<\/a>).\n<\/p>\n \nThe craft isn\u2019t exiting meekly, however, and its Grand Finale orbits are proving to be immensely valuable. On 26 April, Cassini made the first-ever daring dive between Saturn and its beautiful and enigmatic ring system.\n<\/p>\n \nStarting next week, ESA ground stations will work with NASA\u2019s Deep Space Network<\/a> to record radio signals transmitted by Cassini across 1.6 billion km during 22 communication \u2018passes\u2019.\n<\/p>\n \nThe recorded signals will serve important new scientific purposes with the strong involvement of European teams.\n<\/p>\n \nDuring its final 22 orbits, the Cassini orbiter is approaching Saturn and its ring so close that the tiny wobbles in Cassini\u2019s orbit can be measured to separate the gravitational contribution of the planet and its main rings. From those gravity measurements, allowing radial velocity changes of the spacecraft as tiny as 0.05 mm\/s to be measured, the total mass of Saturn\u2019s ring can be inferred. Scientists will also gain a better understanding of the interior structure of Saturn.\n<\/p>\n \nIn addition, during certain part of the orbits, the radio signal will be transmitted directly through the rings and Saturn\u2019s upper atmosphere, allowing valuable information on their composition and material distribution to be retrieved. \n<\/p>\n \n\u201cWe are just now getting into a new mode of radio science, with much more accurate measurements of gravitational effects compared to previous where the effects of ring density on the radio signals were the main topic of study," says Daniel Firre, the service manager at ESA\u2019s mission control centre in Darmstadt, Germany.\n<\/p>\n \nMore information<\/b>\n<\/p>\n \nhttp:\/\/www.esa.int\/estrack<\/a>\n<\/p>\n \nCatching Cassini’s call<\/a>\n<\/p>\n \nGraphic of Cassini grand finale orbits<\/a><\/p>\n","protected":false},"excerpt":{"rendered":" \nESA’s sensitive tracking antennas at New Norcia, Western Australia, and Malargüe, Argentina (seen here in 2012), are being called in to help gather crucial science data during Cassini’s last months in orbit, dubbed the Grand Finale.\n<\/p>\n \nThe mission will end on 15 September, when Cassini plunges into Saturn’s atmosphere, bringing to a close one of the most successful exploration endeavours ever (more information<\/a>).\n<\/p>\n \nThe craft isn’t exiting meekly, however, and its Grand Finale orbits are proving to be immensely valuable. On 26 April, Cassini made the first-ever daring dive between Saturn and its beautiful and enigmatic ring system.\n<\/p>\n \nStarting next week, ESA ground stations will work with NASA’s Deep Space Network<\/a> to record radio signals transmitted by Cassini across 1.6 billion km during 22 communication ‘passes’.\n<\/p>\n \nThe recorded signals will serve important new scientific purposes with the strong involvement of European teams.\n<\/p>\n \nDuring its final 22 orbits, the Cassini orbiter is approaching Saturn and its ring so close that the tiny wobbles in Cassini’s orbit can be measured to separate the gravitational contribution of the planet and its main rings. From those gravity measurements, allowing radial velocity changes of the spacecraft as tiny as 0.05 mm\/s to be measured, the total mass of Saturn’s ring can be inferred. Scientists will also gain a better understanding of the interior structure of Saturn.\n<\/p>\n \nIn addition, during certain part of the orbits, the radio signal will be transmitted directly through the rings and Saturn’s upper atmosphere, allowing valuable information on their composition and material distribution to be retrieved. \n<\/p>\n \n“We are just now getting into a new mode of radio science, with much more accurate measurements of gravitational effects compared to previous where the effects of ring density on the radio signals were the main topic of study,” says Daniel Firre, the service manager at ESA’s mission control centre in Darmstadt, Germany.\n<\/p>\n \nMore information<\/b>\n<\/p>\n \nhttp:\/\/www.esa.int\/estrack<\/a>\n<\/p>\n<\/p>\n