Juno is a PI-led mission to Jupiter, the second mission in NASA's New Frontiers Program.
The 3625-kg spacecraft spins at 2 rpm and is powered by three 9-meter-long solar arrays …

Astrophysical fluid bodies that orbit close to one another induce tidal distortions and flows
that are subject to dissipative processes. The spin and orbital motions undergo a coupled …

A spherical harmonic model of the magnetic field of Jupiter is obtained from vector magnetic
field observations acquired by the Juno spacecraft during 32 of its first 33 polar orbits. These …

On 27 August 2016, the Juno spacecraft acquired science observations of Jupiter, passing
less than 5000 kilometers above the equatorial cloud tops. Images of Jupiter's poles show a …

Jupiter's atmosphere is rotating differentially, with zones and belts rotating at speeds that
differ by up to 100 metres per second. Whether this is also true of the gas giant's interior has …

Sub-Neptune exoplanets are commonly hypothesized to consist of a silicate-rich magma
ocean topped by a hydrogen-rich atmosphere. Previous work studying the outgassing of …

Dark matter (DM) can be captured in celestial bodies after scattering and losing sufficient
energy to become gravitationally bound. We derive a general framework that describes the …

Gravity and magnetic field data obtained by the Juno mission show that Jupiter's strong
zonal winds extend a few thousand kilometers into the interior, but are quenched above the …

Nonannihilating dark matter particles, owing to their interactions with ordinary baryonic
matter, can efficiently accumulate inside celestial objects. For heavy mass, they gravitate …

We present the results of the first Charged-Particle Transport Coefficient Code Comparison
Workshop, which was held in Albuquerque, NM October 4–6, 2016. In this first workshop …