A planetary smashup billions of years ago may be to blame for Jupiter’s weirdly puffy core.
Recent measurements of Jupiter’s gravitational field indicate that, rather than a dense pit of rock and ice, Jupiter’s core is a haze of heavy elements possibly spanning half the planet’s radius (SN: 6/24/17, p. 14). That observation, made by NASA’s Juno spacecraft that started orbiting Jupiter in 2016, flies in the face of current planet formation models (SN: 6/25/16, p. 16). Those models suggest that Jupiter would have formed from a dense kernel that accumulated a thick envelope of gas.
New computer simulations now show that a collision between Jupiter and another large planetary body could have shattered Jupiter’s original compact core into the scattered collection of heavy elements seen today. Understanding the origins of Jupiter’s internal structure may give insight into the processes that shape other gas giants in our solar system and around other stars, researchers report in the Aug. 15 Nature.
“This impact may have happened when the solar system was very, very young, and in a chaotic phase when there were lots of objects roaming around,” says Andrea Isella, an astronomer at Rice University in Houston. As the biggest planetary body in its neighborhood, Jupiter was liable to gravitationally attract other objects wandering the solar system, he says.