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Marine Science Can Contribute to the Search for Extra-Terrestrial Life

  • Jacopo Aguzzi*
  • , Javier Cuadros
  • , Lewis Dartnell
  • , Corrado Costa
  • , Simona Violino
  • , Loredana Canfora
  • , Roberto Danovaro
  • , Nathan Jack Robinson
  • , Donato Giovannelli
  • , Sascha Flögel
  • , Sergio Stefanni
  • , Damianos Chatzievangelou
  • , Simone Marini
  • , Giacomo Picardi
  • , Bernard Foing
  • *Šī darba korespondējošais autors
  • Instituto de Ciencias Del Mar (ICM-CSIC)
  • Stazione Zoologica Anton Dohrn Napoli
  • The Natural History Museum, London
  • University of Westminster
  • Centro di Ricerca Ingegneria e Trasformazioni Agroalimentari
  • Council for Agricultural Research and Economics
  • Polytechnic University of Marcs (UNIVPM)
  • University of Naples Federico II
  • National Research Council of Italy
  • Rutgers - The State University of New Jersey, New Brunswick
  • Woods Hole Oceanographic Institution
  • Institute of Science Tokyo
  • Helmholtz Centre for Ocean Research Kiel
  • Vrije Universiteit Amsterdam

Zinātniskās darbības rezultāts: Devums žurnālamPārskata rakstskoleģiāli recenzēts

5 Atsauces (Scopus)

Kopsavilkums

Life on our planet likely evolved in the ocean, and thus exo-oceans are key habitats to search for extraterrestrial life. We conducted a data-driven bibliographic survey on the astrobiology literature to identify emerging research trends with marine science for future synergies in the exploration for extraterrestrial life in exo-oceans. Based on search queries, we identified 2592 published items since 1963. The current literature falls into three major groups of terms focusing on (1) the search for life on Mars, (2) astrobiology within our Solar System with reference to icy moons and their exo-oceans, and (3) astronomical and biological parameters for planetary habitability. We also identified that the most prominent research keywords form three key-groups focusing on (1) using terrestrial environments as proxies for Martian environments, centred on extremophiles and biosignatures, (2) habitable zones outside of “Goldilocks” orbital ranges, centred on ice planets, and (3) the atmosphere, magnetic field, and geology in relation to planets’ habitable conditions, centred on water-based oceans.

OriģinālvalodaAngļu
Raksta numurs676
ŽurnālsLife
Sējums14
Izdevuma numurs6
DOIs
Publikācijas statussPublicēts - jūn. 2024
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