Gravity science (Juno)

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The Gravity Science experiment and instrument set aboard the Juno Jupiter orbiter is designed to monitor Jupiter's gravity.{{Cite web|url=http://spaceflight101.com/juno/instrument-overview/|title=Instrument Overview – Juno|website=spaceflight101.com|access-date=2017-01-05}}{{Cite news|url=http://www.space.com/33053-nasa-juno-spacecraft-jupiter-gravity.html|title=Jupiter's Gravity Embraces NASA's Juno Spacecraft|newspaper=Space.com|access-date=2017-01-05}}{{Cite web|url=https://www.missionjuno.swri.edu/media-gallery/instruments|title=Juno's Instruments {{!}} Mission Juno|website=Mission Juno|access-date=2017-01-05}} It maps Jupiter's gravitational field, which will allow the interior of Jupiter to be better understood. It uses special hardware on Juno, and also on Earth, including the high-gain K-band and X-band communication systems of the Deep Space Network as well as Juno{{'}}s Ka-band Translator System (KaTS).{{Cite web|url=http://www.europlanet-eu.org/juno-europe/|title=European Involvement in Juno {{!}} Europlanet Outreach|website=www.europlanet-eu.org|access-date=2017-01-05}} These components work together to detect minute changes in radio frequency (Doppler shift) to measure the spacecraft's velocity over time.{{Cite web | url=http://spaceflight101.com/juno/instrument-overview/ |title = Instrument Overview – Juno}} The KaTS box was funded by the Italian Space Agency and overseen by professor Luciano Iess from University La Sapienza in Rome. KaTS detects signals coming from the DSN on Earth, and then sends replies in a very precise way that allows the velocity of Juno to be determined to within 0.001 millimeters per second. The spacecraft receives a tone signal on the Ka band and then replies using the X-band radio.

As the spacecraft traverses the space near Jupiter, the planet, and even variations in the planets interior, cause a variation in Juno velocity.{{Cite news|url=http://www.sciencefocus.com/article/space/what-will-we-learn-juno-mission|title=What will we learn from the Juno mission?|newspaper=Science Focus|access-date=2017-01-05}} The gravity science experiment measures these velocity changes using a combination of hardware on Earth and the spacecraft, which allows the effect of gravity to be measured, and thereby mass variations in Jupiter's interior.

Communication signals:

• Deep Space Network 25 sends a tone signal at 32.5 GHz (Ka-Band)
• Juno KaTS sends tone signal at 35 GHz (X-Band)

Juno launched in 2011 and arrived at Jupiter orbit in July 2016.{{Cite news|url=https://www.nasa.gov/mission_pages/juno/spacecraft/index.html|title=Juno Spacecraft and Instruments|last=Greicius|first=Tony|date=2015-03-13|newspaper=NASA|access-date=2017-01-04|archive-date=2017-05-09|archive-url=https://web.archive.org/web/20170509053559/https://www.nasa.gov/mission_pages/juno/spacecraft/index.html|url-status=dead}}

The GS was planned out to be used on orbits 4, orbit 9, and orbits 10 through 32.{{Cite web|url=https://www.missionjuno.swri.edu/orbit?show=hs_orbit_story_gravity-science-orbits|title=Gravity Science Orbits|website=Mission Juno|access-date=2017-02-07}} When GS operates it must point its antenna at Earth, and is not operated simultaneously with the Microwave Radiometer instrument on Juno. The parameters of the GS experiment were adjusted to account for a 53-day orbit the Juno spacecraft ended up being in.{{Cite book|last1=Buccino|first1=D.|last2=Kahan|first2=D.|last3=Yang|first3=O.|last4=Oudrhiri|first4=K.|title=2018 IEEE Aerospace Conference |chapter=Initial operations experience and results from the Juno gravity experiment |date=March 2018|pages=1–8|doi=10.1109/AERO.2018.8396438|isbn=978-1-5386-2014-4|s2cid=49540278 }}

The GS experiment uses Deep Space Network's DSS-25 antenna which is equipped with simultaneous dual X- and Ka-band transmitters and receivers, as well as the spacecraft which also has X and Ka-band radio systems.