3:30 PM - 3:45 PM
[PCG21-01] Akatsuki returns to Venus
Keywords:Akatsuki, Venus, Exploration
The Akatsuki spacecraft was rotating about the sun with a period of 199 days and was on the trajectory to meet Venus on 22nd of November, 2015 after the orbital maneuvers in November 2011. The date, November 22nd, 2015, was chosen as the shortest encounter timing with consideration of spacecraft's lifetime. Trajectory analysis done later revealed that the orbit around Venus after insertion on 22nd of November, 2015 is unstable. We decided to perform another orbital maneuver in July 2015 to let the spacecraft to meet Venus on 7th of December, 2015 with this date the orbit around Venus would be more stable.
On 7th of December, 2015, the spacecraft approached from outside of Venus orbit and captured by Venus. For the Venus orbit insertion in 2015, termed VOI-R1, four 23 Newton-class thrusters were used as opposed to 500 Newton-class OME used at the 1st VOI in 2010. VOI-R1 burn (1228 seconds) was successfully achieved from 23:51:29 on 6th of December through 00:11:57 on 7th of December (UTC, on-board time).
Akatsuki became the first satellite of a planet in Japan. After VOI-R1, the apoapsis altitude is 0.44 million km with the inclination of 3 degrees. The orbital period is 13 days and 14 hours. The figure shows the VOI-R1 geometry depicted with the Venus center coordinate. For two purposes, to decrease the apoapsis altitude and to avoid long eclipse during the orbiter, we performed a trim maneuver at the first periapsis. The apoapsis altitude is now 0.36 million km with periapsis altitude of 1,000 km - 8,000 km (varying) and the period is 10 days and 12 hours.
Akatsuki will send data over two years to us, and it means that our exploration enters the new era when Japan deliver the continuously changing planet’s data to the whole world.