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On the detection of the Wilkes Land impact crater

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F18%3A00499614" target="_blank" >RIV/67985815:_____/18:00499614 - isvavai.cz</a>

  • Alternative codes found

    RIV/68407700:21110/18:00326920 RIV/61989100:27350/18:10239174 RIV/00025615:_____/18:N0000032

  • Result on the web

    <a href="http://dx.doi.org/10.1186/s40623-018-0904-7" target="_blank" >http://dx.doi.org/10.1186/s40623-018-0904-7</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1186/s40623-018-0904-7" target="_blank" >10.1186/s40623-018-0904-7</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    On the detection of the Wilkes Land impact crater

  • Original language description

    The definitive existence of a giant impact crater, two times larger than the Chixulub crater in the Yucatan peninsula, from an extraterrestrial origin, 1.6 km beneath Wilkes Land, East Antarctica, remain controversial. Here, we use the latest high-resolution gravito-topographic geopotential (SatGravRET 2014) model over Antarctica to offer a plausible confirmation of its existence. SatGravRET 2014 has a spatial resolution between 1 and 10 km at most places and included contemporary space gravimetry and gradiometry data from GRACE and GOCE, and other data including Bedmap 2 bedrock topography. We computed the gravity disturbances, the Marussi tensor of the second derivatives of the disturbing potential, the gravity invariants and their specific ratio, the strike angles and the virtual deformations to quantify the detailed geophysical features for the Wilkes Land anomaly. This set of the gravitational parameters revealed enhanced and more detailed geophysical features on the Wilkes Land Crater than previously possible only with the traditional gravity anomalies. Our findings support prior studies stating that in the Wilkes Land there is a huge impact crater/basin with detectable gravity mascon which is mostly consistent with the characteristics of an impact crater.

  • 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

    10511 - Environmental sciences (social aspects to be 5.7)

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2018

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Earth, Planets and Space

  • ISSN

    1880-5981

  • e-ISSN

  • Volume of the periodical

    70

  • Issue of the periodical within the volume

    August

  • Country of publishing house

    DE - GERMANY

  • Number of pages

    12

  • Pages from-to

  • UT code for WoS article

    000441939500001

  • EID of the result in the Scopus database

    2-s2.0-85052228405