Umeå University's logo

umu.sePublications
System disruptions
We are currently experiencing disruptions on the search portals due to high traffic. We are working to resolve the issue, you may temporarily encounter an error message.
Change search
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • apa-6th-edition.csl
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf
The comet interceptor mission
Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, United Kingdom; The Centre for Planetary Sciences at UCL/Birkbeck, London, United Kingdom.
Umeå University, Faculty of Science and Technology, Department of Physics.ORCID iD: 0000-0001-5379-1158
Department of Astrophysical Sciences, Princeton University, Princeton, United States.
Number of Authors: 2342024 (English)In: Space Science Reviews, ISSN 0038-6308, E-ISSN 1572-9672, Vol. 220, article id 9Article, review/survey (Refereed) Published
Abstract [en]

Here we describe the novel, multi-point Comet Interceptor mission. It is dedicated to theexploration of a little-processed long-period comet, possibly entering the inner Solar System for the first time, or to encounter an interstellar object originating at another star. Theobjectives of the mission are to address the following questions: What are the surface composition, shape, morphology, and structure of the target object? What is the composition ofthe gas and dust in the coma, its connection to the nucleus, and the nature of its interactionwith the solar wind? The mission was proposed to the European Space Agency in 2018, andformally adopted by the agency in June 2022, for launch in 2029 together with the Arielmission. Comet Interceptor will take advantage of the opportunity presented by ESA’s FClass call for fast, flexible, low-cost missions to which it was proposed. The call requireda launch to a halo orbit around the Sun-Earth L2 point. The mission can take advantage ofthis placement to wait for the discovery of a suitable comet reachable with its minimum ΔV capability of 600 ms−1. Comet Interceptor will be unique in encountering and studying, at anominal closest approach distance of 1000 km, a comet that represents a near-pristine sample of material from the formation of the Solar System. It will also add a capability that noprevious cometary mission has had, which is to deploy two sub-probes – B1, provided by theJapanese space agency, JAXA, and B2 – that will follow different trajectories through thecoma. While the main probe passes at a nominal 1000 km distance, probes B1 and B2 willfollow different chords through the coma at distances of 850 km and 400 km, respectively.The result will be unique, simultaneous, spatially resolved information of the 3-dimensionalproperties of the target comet and its interaction with the space environment. We presentthe mission’s science background leading to these objectives, as well as an overview of thescientific instruments, mission design, and schedule.

Place, publisher, year, edition, pages
Springer Nature, 2024. Vol. 220, article id 9
Keywords [en]
Comets, Spacecraft, Instruments – spaceborne and space research
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:umu:diva-220716DOI: 10.1007/s11214-023-01035-0Scopus ID: 2-s2.0-85183417097OAI: oai:DiVA.org:umu-220716DiVA, id: diva2:1836571
Funder
The European Space Agency (ESA), 4000136673/21/NL/IB/igThe European Space Agency (ESA), 3-17164/21/NL/GP/pbeSwedish National Space Board, 108/18Swedish National Space Board, 2021-00047EU, Horizon 2020, 802699EU, Horizon Europe, 101079231EU, Horizon Europe, 10051045EU, European Research CouncilAvailable from: 2024-02-09 Created: 2024-02-09 Last updated: 2024-02-09Bibliographically approved

Open Access in DiVA

fulltext(10769 kB)70 downloads
File information
File name FULLTEXT01.pdfFile size 10769 kBChecksum SHA-512
89421c89ed8ee3be5bfdad0fae3f2d6a8df5b868f8d7f3a77a0de07acbce855e767725f62a015215fb9e994120303c0249ad810bc2149731a22021b5f6ed966f
Type fulltextMimetype application/pdf

Other links

Publisher's full textScopus

Authority records

Gunell, Herbert

Search in DiVA

By author/editor
Gunell, Herbert
By organisation
Department of Physics
In the same journal
Space Science Reviews
Astronomy, Astrophysics and Cosmology

Search outside of DiVA

GoogleGoogle Scholar
Total: 71 downloads
The number of downloads is the sum of all downloads of full texts. It may include eg previous versions that are now no longer available

doi
urn-nbn

Altmetric score

doi
urn-nbn
Total: 349 hits
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • apa-6th-edition.csl
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf