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VLA and ALMA study Jupiter and Io


Element from a VLA picture of Jupiter made in conjunction with observations by the Juno spacecraft in orbit round that planet. Credit score: Moeckel, et al., Invoice Saxton, NRAO/AUI/NSF

Whereas the Nationwide Science Basis’s Karl G. Jansky Very Massive Array (VLA) and the Atacama Massive Millimeter/submillimeter Array (ALMA) steadily reveal vital new details about objects far past our personal Milky Way Galaxy—at distances of many hundreds of thousands or billions of light-years—additionally they are very important instruments for unraveling a lot nearer mysteries, proper right here in our personal solar system.


A pair of latest papers illustrate how these telescopes are serving to planetary scientists perceive the workings of the solar system’s largest planet, Jupiter, and its innermost moon Io.

Jupiter’s ambiance is advanced and dynamic, and adjustments quickly. To check the enormous planet’s ambiance at totally different depths, scientists mixed observations made with devices aboard NASA’s Juno spacecraft, in orbit round Jupiter, with observations with the VLA. They collected knowledge in regards to the distribution of the hint gasoline ammonia at totally different ranges within the ambiance to assist decide the vertical construction of the ambiance.

These observations wanted to be sufficiently detailed to mix Juno’s lengthy wavelength observations with the VLA’s high-frequency decision to grasp vertical transport within the ambiance. The spatial decision of the ground-based VLA observations was similar to that of the instrument aboard the spacecraft orbiting the planet. These observations produced the highest-resolution radio picture but manufactured from Jupiter. This method helps the scientists advance their understanding of Jupiter’s deep ambiance.

Io, whose inside continuously is heated by robust gravitational tidal forces, is essentially the most volcanically-active physique in our solar system. The moon has a tenuous ambiance primarily composed of Sulfur Dioxide (SO2), which comes from eruptions of its many volcanoes and sublimation of its SO2 floor frost.

Scientists have used ALMA to review the hint gases of Sodium Chloride (NaCl—table salt) and Potassium Chloride (KCl) within the atmosphere. They discovered that these compounds are largely confined in extent and are at excessive temperatures, indicating that they, too, are expelled by volcanoes.

In addition they discovered that they’re in numerous areas from the place the SO2 is emitted, which means that there could also be variations within the subsurface magma or within the eruptive processes between the volcanoes that emit SO2 and those who emit NaCl and KCl.

Each works are revealed on the arXiv preprint server.

Extra info:
Chris Moeckel et al, Ammonia Abundance Derived from Juno MWR and VLA Observations of Jupiter, arXiv (2022). DOI: 10.48550/arxiv.2209.03513

Erin Redwing et al, NaCl & KCl in Io’s Environment, arXiv (2022). DOI: 10.48550/arxiv.2209.12974

Journal info:
arXiv

Quotation:
VLA and ALMA examine Jupiter and Io (2022, December 13)
retrieved 13 December 2022
from https://phys.org/information/2022-12-vla-alma-jupiter-io.html

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