July 1, 2016 – NASA’s Juno spacecraft will make its long anticipated arrival at Jupiter on July 4. Coming face-to-face with the gas giant, Juno will begin to unravel some of the greatest mysteries surrounding our solar system’s largest planet, including the origin of its massive magnetosphere.
Magnetospheres are the result of a collision between a planet’s intrinsic magnetic field and the supersonic solar wind. Jupiter’s magnetosphere — the volume carved out in the solar wind where the planet’s magnetic field dominates –extends up to to 3 million kilometers (nearly 2 million miles) toward the sun and as far as Saturn’s orbit in the other direction. If it were visible in the night sky, Jupiter’s magnetosphere would appear to be about the same size as Earth’s full moon.
Jupiter’s powerful magnetic environment also creates the brightest auroras in the solar system, as charged particles get trapped by the field and rain down into the atmosphere. Juno will directly sample the charged particles and magnetic fields near Jupiter’s poles for the first time, while simultaneously observing the auroras at ultraviolet wavelengths of light. These investigations will greatly improve the understanding of this remarkable phenomenon and of similar magnetic objects, such as young stars that have their own planetary systems.
By studying Jupiter’s magnetosphere, scientists will gain a better understanding about how Jupiter’s magnetic field is generated. They also hope to determine whether the planet has a solid core, which will tell us how Jupiter formed during the earliest days of our solar system.
In order to look inside the planet, the science team equipped Juno with a pair of magnetometers. The magnetometers, which were designed and built by an in-house team of scientists and engineers at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, will allow scientists to map Jupiter’s magnetic field with high accuracy and observe variations in the field over time.
“The best way to think of a magnetometer is like a compass,” said Jack Connerney, deputy principal investigator and head of the magnetometer team at Goddard. “Compasses record the direction of a magnetic field. But magnetometers expand on that capability and record both the direction and magnitude of the magnetic field.”
The magnetometer sensors rest on a boom attached to one of the solar arrays, placing them about 40 feet (12 meters) from the body of the spacecraft. This helps ensure that the rest of the spacecraft does not interfere with the magnetometer.
However, the sensor orientation changes in time with the mechanical distortion of the solar array and boom resulting from the extremely cold temperatures of deep space. This distortion would limit the accuracy of the magnetometer measurements if not measured.
To ensure that the magnetometers retain their high accuracy, the team paired the instruments with a set of four cameras. These cameras measure the distortion of the magnetometer sensors in reference to the stars to determine their orientation.
“This is our first opportunity to do very precise, high-accuracy mapping of the magnetic field of another planet,” Connerney said. “We are going to be able to explore the entire three-dimensional space around Jupiter, wrapping Jupiter in a dense net of magnetic field observations completely covering the sphere.”
One of the mysteries the team hopes to answer is how Jupiter’s magnetic field is generated. Scientists expect to find similarities between Jupiter’s magnetic field and that of Earth.
Magnetic fields are produced by what are known as dynamos — convective motion of electrically conducting fluid inside planets. As a planet rotates, the electrically susceptible liquid swirls around and drives electric currents, inducing a magnetic field. Earth’s magnetic field is generated by liquid iron in the planet’s core.
“But with Jupiter, we don’t know what material is producing the planet’s magnetic field,” said Jared Espley, Juno program scientist for NASA Headquarters, Washington. “What material is present and how deep down it lies is one of the questions Juno is designed to answer.”
The observations made by Juno’s magnetometers will also add to our understanding of Earth’s dynamo, the source of our planet’s magnetic field, which lies deep beneath a magnetized layer of rocks and iron.
Imagine Earth’s crust strewn with refrigerator magnets as you try to peer beneath the surface to observe the dynamo. The magnetization of Earth’s crust will skew your measurements of the magnetic field.
“One of the reasons that the Juno mission is so exciting is because we can map Jupiter’s magnetic field without having to look through the crustal magnetic fields, which behave like a jumble of refrigerator magnets,” Connerney said. “Jupiter has a gaseous envelope about it made of hydrogen and helium that gives us a clear and unobstructed view of the dynamo.”
These observations will also add to the general understanding of how dynamos generate magnetic fields, including here on Earth.
“Any time we understand anything about another planet, we can take that knowledge and apply it to our knowledge about our own planet,” Espley said. “We’ll be looking at Juno’s observations in a big-picture perspective.”
NASA’s Jet Propulsion Laboratory in Pasadena, California, manages the Juno mission for the principal investigator, Scott Bolton, of Southwest Research Institute in San Antonio. Juno is part of NASA’s New Frontiers Program, which is managed at NASA’s Marshall Space Flight Center in Huntsville, Alabama, for NASA’s Science Mission Directorate. Lockheed Martin Space Systems, Denver, built the spacecraft.
CU-Boulder Professor Fran Bagenal of LASP, who co-chairs the Juno Magnetospheric Working Group for NASA and is coordinating many of the science observations for the mission. In addition to Bagenal, LASP Professor Robert Ergun and Research Associate Robert Wilson are part of the Juno science team. Other CU-Boulder Juno participants include undergraduate Kaleb Bodisch, 2015 graduate Logan Dougherty, now a researcher, and graduate students Drake Ranquist and Edward Nerney.