{"id":20082,"date":"2022-04-04T15:27:05","date_gmt":"2022-04-04T14:27:05","guid":{"rendered":"https:\/\/www.innovationnewsnetwork.com\/?p=20082"},"modified":"2022-04-04T15:30:49","modified_gmt":"2022-04-04T14:30:49","slug":"closely-analysing-jupiters-origin","status":"publish","type":"post","link":"https:\/\/www.innovationnewsnetwork.com\/closely-analysing-jupiters-origin\/20082\/","title":{"rendered":"Closely analysing Jupiter\u2019s origin"},"content":{"rendered":"

A research team from University of Zurich (UZH)<\/a> and the National Centre of Competence in Research (NCCR) has utilised computer modelling systems to analyse and dissect Jupiter\u2019s origin.<\/h2>\n

One of the most important questions that remains largely unanswered within the planetary formation field is the history of Jupiter\u2019s origin. By employing sophisticated computer modelling, researchers from the University of Zurich (UZH) and the National Centre of Competence in Research (NCCR) PlanetS could be the key to shed light on Jupiter\u2019s formation history. Their results were published in The Astrophysical Journal Letters<\/em>.<\/p>\n

Dissecting the enrichment of heavy elements<\/h3>\n

When the Galileo spacecraft released a probe that parachuted into Jupiter\u2019s atmosphere in 1995, it revealed that heavy elements<\/a> (elements heavier than helium) were enriched there. At the same time, recent structure models of Jupiter that are based on gravity field measurements by the Juno spacecraft suggest that Jupiter\u2019s interior is not uniform but instead has a complex structure.<\/p>\n

\u201cSince we now know that the interior of Jupiter is not fully mixed, we would expect heavy elements to be in a giant gas planet\u2019s deep interior as heavy elements are mostly accreted during the early stages of the planetary formation,\u201d explained study co-author, Professor at the University of Zurich and member of the NCCR PlanetS, Ravit Helled.<\/p>\n

\"Jupiter's
Professor of Theoretical Astrophysics at the University of Zurich and member of the NCCR PlanetS, Ravit Helled.<\/figcaption><\/figure>\n

\u201cOnly in later stages, when the growing planet is sufficiently massive, can it effectively attract large amounts of light element gases like hydrogen and helium. Finding a formation scenario of Jupiter which is consistent with the predicted interior structure as well as with the measured atmospheric enrichment is therefore challenging yet critical for our understanding of giant planets.\u201d<\/p>\n

Analysing Jupiter\u2019s origin<\/h3>\n

\u201cOur idea was that Jupiter had collected these heavy elements in the late stages of its formation by migrating. In doing so, it would have moved through regions filled with so-called planetesimals \u2013 small planetary building blocks that are composed of heavy element materials \u2013 and accumulated them in its atmosphere,\u201d added study lead-author, Sho Shibata, who is also a member of the NCCR PlanetS, as well as a postdoctoral researcher at the University of Zurich.<\/p>\n

\"Jupiter's

Sho Shibata is a postdoctoral researcher at the University of Zurich and a member of the NCCR PlanetS.<\/figcaption><\/figure>\n

However, migration alone is no guarantee for accreting the necessary material. \u201cBecause of complex dynamical interactions, the migrating planet does not necessarily accrete the planetesimals in its path. In many cases, the planet actually scatters them instead \u2013 not unlike a shepherding dog scattering sheep,\u201d Shibata explained. The research team were therefore required to conduct numerous simulations in order to determine if any migration pathways resulted in sufficient material accretion.<\/p>\n

\u201cWhat we found was that a sufficient number of planetesimals could be captured if Jupiter formed in the outer regions of the solar system \u2013 about four times further away from the Sun than where it is located now \u2013 and then migrated to its current position,\u201d Shibata explained. \u201cIn this scenario, it moved through a region where the conditions favoured material accretion \u2013 an accretion sweet spot, as we call it.\u201d<\/p>\n

\"Jupiter\"
Jupiter, as seen by the Juno spacecraft<\/figcaption><\/figure>\n

Commencing a new era in planetary science<\/h3>\n

Combining the constraints introduced by the Galileo probe and Juno data, the team of researchers eventually concluded with a satisfactory explanation. \u201cThis shows how complex giant gas planets are and how difficult it is to realistically reproduce their characteristics,\u201d Helled concluded. \u201cIt took us a long time in planetary science to get to a stage where we can finally explore these details with updated theoretical models and numerical simulations. This helps us close gaps in our understanding not only of Jupiter\u2019s origin and our solar system, but also of the many observed giant planets orbiting far away stars.\u201d<\/p>\n","protected":false},"excerpt":{"rendered":"

A research team from University of Zurich (UZH) and the National Centre of Competence in Research (NCCR) has utilised computer modelling systems to analyse and dissect Jupiter\u2019s origin. One of the most important questions that remains largely unanswered within the planetary formation field is the history of Jupiter\u2019s origin. By employing sophisticated computer modelling, researchers […]<\/p>\n","protected":false},"author":19,"featured_media":20083,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"_monsterinsights_skip_tracking":false,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0,"footnotes":""},"categories":[771],"tags":[818,3477,809],"acf":[],"yoast_head":"\nClosely analysing Jupiter\u2019s origin<\/title>\n<meta name=\"description\" content=\"A research team has utilised computer modelling systems to analyse and dissect Jupiter\u2019s origin and our solar system as a whole.\" \/>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/www.innovationnewsnetwork.com\/closely-analysing-jupiters-origin\/20082\/\" \/>\n<meta property=\"og:locale\" content=\"en_GB\" 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