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An autonomous lunar geophysical experiment package (ALGEP) for future space missions : In response to Call for White Papers for the Voyage 2050 long-term plan in the ESA Science Program

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11310%2F22%3A10462827" target="_blank" >RIV/00216208:11310/22:10462827 - isvavai.cz</a>

  • Result on the web

    <a href="https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=nfmyBQz4Kf" target="_blank" >https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=nfmyBQz4Kf</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1007/s10686-022-09857-6" target="_blank" >10.1007/s10686-022-09857-6</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    An autonomous lunar geophysical experiment package (ALGEP) for future space missions : In response to Call for White Papers for the Voyage 2050 long-term plan in the ESA Science Program

  • Original language description

    Geophysical observations will provide key information about the inner structure of the planets and satellites and understanding the internal structure is a strong constraint on the bulk composition and thermal evolution of these bodies. Thus, geophysical observations are a key to uncovering the origin and evolution of the Moon. In this article, we propose the development of an autonomous lunar geophysical experiment package, composed of a suite of instruments and a central station with standardized interface, which can be installed on various future lunar missions. By fixing the interface between instruments and the central station, it would be possible to easily configure an appropriate experiment package for different missions. We describe here a series of geophysical instruments that may be included as part of the geophysical package: a seismometer, a magnetometer, a heat flow probe, and a laser reflector. These instruments will provide mechanical, thermal, and geodetic parameters of the Moon that are strongly related to the internal structure. We discuss the functionality required for future geophysical observations of the Moon, including the development of the central station that will be used commonly by different payloads.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10505 - Geology

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2022

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Experimental Astronomy

  • ISSN

    0922-6435

  • e-ISSN

    1572-9508

  • Volume of the periodical

    54

  • Issue of the periodical within the volume

    2-3

  • Country of publishing house

    NL - THE KINGDOM OF THE NETHERLANDS

  • Number of pages

    24

  • Pages from-to

    617-640

  • UT code for WoS article

    000794115100001

  • EID of the result in the Scopus database

    2-s2.0-85129809076