RocketSTEM Issue #13 - September 2016 | Page 64

The largest of Juno’s six MWR antennas (shown here) takes up a full side of the spacecraft. Credit: NASA In order to avoid the highest levels of radiation coming from Jupiter’s radiation belts, while still getting the spacecraft very close to the planet to allow the science package to complete the assigned tasks, Juno’s scientists have designed the orbits to be highly elliptical. The spacecraft approaches the gas giant from the north, zipping down over the north polar region of the planet coming in as close as 2600 miles, then comes out from the southern polar region and heads out away from the planet before curving back for another pass. While each science orbit lasts 62 62 nearly 14 days, most of the instrument observations are taken while Juno passes closest to Jupiter. These close passes are from pole to pole as Juno is flying a polar orbit, and the closest encounters only last around two hours since Juno is still travelling at a very fast velocity, although the instruments are still collecting data during the approach and departure also. The final phase of the mission is called the Deorbit phase. Designed to send Juno into the atmosphere of Jupiter, this will end up in the destruction of the probe as it was not designed to operate in the extreme environment of Jupiter’s atmosphere. After the science pass on orbit 37, a deorbit burn will occur which will set the lowest point of the next close pass to be below the clouds tops. On February 20, 2018 Juno will have completed its mission. The destruction of the spacecraft in Jupiter’s atmosphere ensures that its orbit would never place it on a collision course with the Jovian moons Europa, Ganymede, or Callisto. Such an impact would violate NASA’s planetary protection requirements. As of this writing, Juno is currently in its first capture orbit, speeding back towards Jupiter, the science instruments are on and while the first orbit is not technically a science orbit, some readings, and certainly some images will be gained during the pass around Jupiter. The first actual science orbit doesn’t begin until the middle of November. In the months ahead, more science and images will come back from Jupiter. What will we discover and what will we see? To learn more about Juno and follow its mission, the following websites are very informative : https://www.missionjuno.swri.edu/ http://www.nasa.gov/mission_pages/ juno/main/index.html To find out where Juno is and “fly along” with the spacecraft, check out NASA’s Eyes on the Solar System program. It’s an internet-based tool that you download to your PC or Mac and use to see many objects in the solar system, including Juno: http://eyes.jpl.nasa.gov/juno Credit: NASA/JPL/Caltech Imager/Spectrometer will be collecting their nest data on that orbit, but the Gravity Science experiment will still be operating during that orbit, but with only the X-Band instrument collecting data, the Ka-Band translator (Kat) is off since it requires the spacecraft to be oriented towards Earth. Then on a GRAV oriented orbit, when the spacecraft is oriented towards Earth, the Kat can download data to Earth in real-time, but the orientation reduces the amount of data collected by other instruments. The design of the orbits should allow Juno to cover the entire planet with its instruments, giving scientists a good picture of all of Jupiter from their various instruments. www.RocketSTEM .org