A possible direct exposure of the Earth to the cold dense interstellar medium 2-3 Myr ago.

Solar physics

Journal

Nature astronomy
ISSN: 2397-3366
Titre abrégé: Nat Astron
Pays: England
ID NLM: 101738506

Informations de publication

Date de publication:
2024
Historique:
received: 13 07 2022
accepted: 25 04 2024
medline: 23 8 2024
pubmed: 23 8 2024
entrez: 23 8 2024
Statut: ppublish

Résumé

Cold, dense clouds in the interstellar medium of our Galaxy are 4-5 orders of magnitude denser than their diffuse counterparts. Our Solar System has most likely encountered at least one of these dense clouds during its lifetime. However, evidence for such an encounter has not been studied in detail yet. Here we derive the velocity field of the Local Ribbon of Cold Clouds (LRCC) by modelling the 21 cm data from the HI4PI survey, finding that the Solar System may have passed through the LRCC in the constellation Lynx 2-3 million years ago. Using a state-of-the-art simulation of the heliosphere, we show that during the passage, the heliosphere shrinks to a scale of 0.22 au, smaller than the Earth's orbit around the Sun. This would have put the Earth in direct contact with the dense interstellar medium for a period of time and exposed it to a neutral hydrogen density above 3,000 cm

Identifiants

pubmed: 39175532
doi: 10.1038/s41550-024-02279-8
pii: 2279
pmc: PMC11335566
doi:

Types de publication

Journal Article

Langues

eng

Pagination

983-990

Informations de copyright

© This is a U.S. Government work and not under copyright protection in the US; foreign copyright protection may apply 2024.

Déclaration de conflit d'intérêts

Competing interestsThe authors declare no competing interests.

Auteurs

Merav Opher (M)

Radcliffe Institute for Advanced Study at Harvard University, Cambridge, MA USA.
Astronomy Department, Boston University, Boston, MA USA.

Abraham Loeb (A)

Astronomy Department, Harvard University, Cambridge, MA USA.

J E G Peek (JEG)

Space Telescope Science Institute, Baltimore, MD USA.
Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD USA.

Classifications MeSH