OCEANUS Observatorymulti-Spacecraft Capture Flagship Exploring Mission the a Concepttmospheric to Explorenature Ofuranus Uranus and and Saturn Saturn

OCEANUS Observatorymulti-Spacecraft Capture Flagship Exploring Mission the a Concepttmospheric to Explorenature Ofuranus Uranus and and Saturn Saturn

OCEANUS ObservatoryMulti-Spacecraft Capture Flagship Exploring Mission the A Concepttmospheric to ExploreNature ofUranus Uranus and and Saturn Saturn A conceptual Uranus and Saturn flagship mission design developed by the Astronautical engineering students of Purdue University. Uranus belongs to a class of planets Exoplanets Commonality by Size called ice giants. “Ice” in this context refers to volatile materials that are solid at the low temperatures of the outer Solar System (e.g. , water, ammonia, and methane). Earth-size Super Humankind’s last close encounter Earth-size with the Ice Giants was when NASA's Voyager 2 spacecraft made its Uranus-size closest approach on January 24, 1986 Jupiter-size In the 30 years since Voyager, we have studied exoplanets via the Kepler space observatory. Based on exoplanet observations we believe ice giant-sized planets are the most common type of planet, yet we have never studied one in Super great detail. Thus, a mission to Uranus is one of the highest Jupiter-size priority missions as per the Planetary Science Decadal Survey The Ice Giants The Ice Science Overview OCEANUS major science goals: Validate planetary formation models Explore unusual magnetosphere of Uranus Study unknown atmospheric conditions Determine the origin of Rings and Satellites Determine the interior structure To carry out these objectives, OCEANUS carries a complement of 9 dedicated scientific instruments, as well as two probes which will descend into Saturn’s and Uranus’ atmospheres. Saturn Probe Opportunity Along the route to Uranus, OCEANUS passes by Saturn and performs a gravity assist, which is an opportunity to deploy a probe. A probed has never been deployed into Saturn, so OCEANUS mission provides a unique opportunity to study Saturn’s atmosphere in detail. Mission Trajectory 1/8/2040 OCEANUS is launched from Earth. 1/14/2032 130 days before the Saturn flyby, the first probe is released. OCEANUS performs a gravity 1 assist at Saturn, placing the 7/3/2028 orbiter on a trajectory to Uranus. 130 days before the Uranus arrival, the second probe is released. OCEANUS arrives at Uranus and captures into a 20 day science orbit. Uranus Orbiter (shown with probes) OCEANUS OCEANUS Spacecraft Shared probe design Why “OCEANUS”? In Greek mythology, Oceanus was the firstborn son of Gaia and Ouranos. He was revered by the Ancient Greeks as the divine symbol of the Ocean, or the waters beyond the Mediterranean Sea. In the Roman names, “Ouranos” is Uranus, and “Gaia” is the goddess associated with the Earth, and remembering Kronos (Saturn) is the brother of Oceanus, it became natural to name our mission OCEANUS. Probe Operations Similar for both Saturn and Uranus 1. Probe Entry 2. Maximum Heating 4. Front Shield 3. Pilot Chute Separation Deploys Saturn Back Cover Probe Release Uranus 5. Begin Science Probe Collection 1 bar level for 1 bar level for Saturn Uranus.

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