Mission type | Science |
---|---|
Operator | NASA / Applied Physics Laboratory / University of Arizona |
Website | https://ivo.lpl.arizona.edu/ |
Mission duration | 5-year transit to Jupiter 47-month primary mission at Jupiter |
Spacecraft properties | |
Manufacturer | Applied Physics Laboratory |
Launch mass | <2000 kg |
Dry mass | <800 kg |
Start of mission | |
Launch date | January 2029 (proposed)[1] |
Rocket | TBD |
Launch site | Cape Canaveral |
Jupiter orbiter | |
Orbits | 10 |
Flyby of Io | |
Io Volcano Observer (IVO) is a proposed low-cost mission to explore Jupiter's moon Io to understand tidal heating as a fundamental planetary process.[1] The main science goals are to understand (A) how and where tidal heat is generated inside Io, (B) how tidal heat is transported to the surface, and (C) how Io is evolving. These results are expected to have direct implications for the thermal history of Europa and Ganymede as well as provide insights into other tidally heated worlds such as Titan and Enceladus. The IVO data may also improve our understanding of magma oceans and thus the early evolution of the Earth and Moon.
IVO is similar to the Io Orbiter concept suggested for the New Frontiers Program by the 2013–2022 U. S. National Research Council Planetary Science Decadal Survey.[2] The mission was proposed to NASA's Discovery Program by the University of Arizona and Johns Hopkins University's Applied Physics Laboratory in 2010, 2015, and 2019.[3][4][5] IVO was also proposed to NASA's Discovery & Scout Mission Capability Expansion (DSMCE) in 2007 and awarded a concept-study in 2009.[6][7]
In 2020, IVO was selected along with three other Discovery proposals for further study, with one or two expected to be selected to fly.[8] In all cases the Principal Investigator has been Alfred McEwen. However, IVO and Trident were passed over in the Discovery 15 and 16 selection phase in favor of DAVINCI+ and VERITAS, both missions to Venus.[9]