“Textbook numbers” shift as Juno pins down Jupiter’s true shape

Jupiter shrunk not; the yardstick improved. The largest planet of the solar system has been used decades as a sort of calibration beacon: a “known” giant, whose existence largely goes unnoticed, whose size forms the basis of all interior models to the comparisons of gas worlds at a great distance. That belief was developed based on only a rather limited number of interactions radio experiments during Pioneer and Voyager flyby in the 1970s. There is a new understanding of the radio tracking of Juno that has made it known that Jupiter is somewhat smaller and somewhat more flattened than the long running figures implied, closing the reference values used by scientists throughout the planetary science.

Image Credit to wikipedia.org

It is updated based on radio occultation measurements on 13 flybys, a geometry where the signal of Juno is silenced by Jupiter as observed by the Earth. When the radio beam passes through the upper atmosphere and ionosphere of the planet the path curve becomes bent and the time becomes distorted. Atmospheric structure is coded in those gentle delays, and, with the loss of moment of signal arrival determined, the limb of Jupiter and his figure as a whole. The fast zonal winds on the planet are also explained by the new work and push the gaseous envelope of the planet in an idealized form albeit slightly.

Under the polished method the radius of the poles to the centre measures 41,534 miles (66,842 km), which, however, is 7.5 miles (12 km) in the shorter, and the radius of the equatorial line is 44,421 miles (71,488 km), which, however, is 2.5 miles (4 km) less. Using the same data, the implied full diameters are 88,841 miles (142,976 km) and 83,067 miles (133,684 km) across the equator and the pole to pole, respectively, which agrees with the notion that Jupiter is a bit more “squashed” than the measurements had previously been taken. The modifications are modest on a planet which can engulp a thousand Earths, but they happen just where modern models are the most vulnerable, at the frontier between quantity of gravity, whirling winds, and inward structure.

Those few miles are important since the radius of Jupiter is not simply a few miles—it is a limitation. With any assumed change in radius, the distributions of mass at depth may be suggested by the same gravity field, and the same measurements in the atmosphere may coincide (or not coincide) with interior layers. These few kilometers matter, as one of the authors of the studies, Eli Galanti, described, since small geometric modifications can make interior models fit many data sets simultaneously.

The general heritage of Juno is that the “knowns” of Jupiter continue to become “known better.” The mission has also addressed composition questions that could only be sampled locally in the past by the probes. In another body of findings, Juno in her microwave radiometer experiments, had estimated that at equator, water constitutes approximately 0.25 percent of the atmospheric molecules, and therefore how measurements in one part of the planet may be misleading when the planet is not homogenously mixed. Collectively these pieces of evidence support a useful giant planet lesson: accuracy is gained through numerous observations at a variety of latitudes, depths and viewing configurations.

There is the outward facing payoff as well. The size of Jupiter has traditionally been employed as a standard in interpreting transits and other detached observations of giant exoplanets; a more Jovian standard enables like to be compared with like when distant exoplanets are scaled down to radii, densities, and presumed interiors. The new dimensions, which have been published in Nature Astronomy, do not rephrase what Jupiter is, but are a sharpening of what Jupiter is applied to.

Planetary scientist Yohai Kaspi said that textbooks will have to be updated. Of course the size of Jupiter has not changed, but the measure of it has.

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