When storms carry ammonia gas to the top

Jupiter is easily identifiable from the band-like structures that extend across its surface. These belts are areas of different rotation and quite different properties. But what’s going on underneath them? The Hubble telescope or probes such as Juno primarily show just the exterior layer. To understand the dynamic behavior of Jupiter’s atmosphere, scientists need to look into its depths – something the Atacama Large Millimeter/submillimeter Array (ALMA) makes possible in the radio frequency range.

The atmosphere of the gas giant consists primarily of hydrogen and helium with traces of methane, among other things. In the uppermost cloud layer, however, there is, at first, ammonia ice. Underneath that there is a layer of solid particles made from ammonium hydrosulfide. Even deeper, about 80 kilometers (50 miles) below the uppermost clouds, there is probably a layer of liquid water. Many of Jupiter’s storms unleash their fury in these belts. They are comparable with cyclones and anticyclones here on Earth and are often linked with electrical discharges. In visible light, they are often seen as bright clouds called plumes. Plume eruptions can significantly disrupt a belt’s appearance. They are often visible for months or even years.

In January 2017, amateur astronomers observed just such a plume eruption on Jupiter. Then a research team was able to use ALMA to take a closer look. As the researchers now report in a paper, ALMA helped them to unlock details about the eruption. “Our observations show for the first time that during an eruption, large amounts of ammonia gas are transported upward,” says the astronomer, Imke de Pater of the University of California, Berkeley. “We were also able to confirm the theory that the eruptions are caused by moist convection at the bases of water clouds deep in the atmosphere. They then transport the ammonia all the way to the top, above the normal ammonia cloud deck.”

Here, the bright bands correspond to high temperatures, while the dark bands correspond to lower temperatures. In the visual range, the belts that appear dark here are mostly white, while the belts that appear bright here look brownish in images from telescopes. Image: ALMA (ESO/NAOJ/NRAO), I. de Pater et al.; NRAO/AUI NSF, S. Dagnello
Comparison of an image in the radio spectrum (top, ALMA) and in visible light (Hubble). The eruption in the south is visible in both images. Image: ALMA (ESO/NAOJ/NRAO), I. de Pater et al.; NRAO/AUI NSF, S. Dagnello; NASA/Hubble

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  • BrandonQMorris
  • Brandon Q. Morris es físico y especialista en el espacio. Lleva mucho tiempo preocupado por las cuestiones espaciales, tanto a nivel profesional como privado, y aunque quería ser astronauta, tuvo que quedarse en la Tierra por diversas razones. Le fascina especialmente el "qué pasaría si" y a través de sus libros pretende compartir historias convincentes de ciencia ficción dura que podrían suceder realmente, y que algún día podrían suceder. Morris es autor de varias novelas de ciencia ficción de gran éxito de ventas, como la serie Enceladus.

    Brandon es un orgulloso miembro de la Science Fiction and Fantasy Writers of America y de la Mars Society.