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Investigating Internal Magnetic Field Sources on the Moon and Mars

Descrizione del progetto

Comprendere come funziona la dinamo terrestre

Per miliardi di anni, il campo magnetico globale della Terra è dovuto a una dinamo all’interno del ferro per la maggior parte fuso nell’interno del pianeta. Come funziona il meccanismo della dinamo terrestre? La risposta a questa domanda richiede una comprensione di come funziona una dinamo planetaria. Il progetto SIGMA, finanziato dall’UE, studierà i campi magnetici della crosta di altri corpi planetari (Mercurio, Luna e Marte) dove potrebbero aver operato diverse dinamo. Ad esempio, Marte ha un grande magnetismo residuo di un’antica dinamo e gli scienziati ritengono che anche la Luna un tempo avesse un campo magnetico, basandosi su evidenze di rocce lunari magnetizzate. SIGMA utilizzerà una nuova metodologia di indagine e la generazione di modelli avanzati. I risultati saranno preziosi per il campo dell’esplorazione planetaria.

Obiettivo

The Earth possesses an internal magnetic field produced by convection movements occurring in the outer liquid metallic core of the planet, called dynamo. In order to understand how the Earth dynamo mechanisms work, it is required to understand how a planetary dynamo operates as a whole, from its birth to its demise. For this purpose, our inner Solar System provides a natural laboratory.
Today, amongst all our companion telluric planets, only Mercury possesses a core magnetic field. Venus has no observable internal magnetic field, which is enigmatic. Crustal magnetic fields are observed at the surface of Mars and the Moon, which is indicative that these bodies likely had a dynamo in their history, but is no longer active. More importantly, these crustal fields hold fundamental information about the ancient core field, such as its morphology, intensity and temporal variation.
By studying the crustal magnetic fields of other planetary bodies, such as Mercury, the Moon or Mars, where different dynamos might have operated, the dynamo processes themselves can be better understood. The SIGMA project targets to unveil crucial unanswered questions of the Earth global magnetic field evolution through an investigation of different planetary crustal anomalies using a novel methodology of surveys (developed by the host) and the generation of advanced models (expertise of the fellow candidate). The results will have an innovative impact in the imminent planetary exploration, where the candidate would be positioned as a senior and independent researcher with a profile comprising theoretical and experimental pioneering techniques.

Coordinatore

INSTITUTO NACIONAL DE TECNICA AEROESPACIAL ESTEBAN TERRADAS
Contribution nette de l'UE
€ 160 932,48
Indirizzo
CR TORREJON AJALVIR KM 4 2
28850 Torrejon De Ardoz Madrid
Spagna

Mostra sulla mappa

Regione
Comunidad de Madrid Comunidad de Madrid Madrid
Tipo di attività
Research Organisations
Collegamenti
Costo totale
€ 160 932,48