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The operational environment and rotational acceleration of asteroid (101955) Bennu from OSIRIS-REx observations

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F19%3A10405366" target="_blank" >RIV/00216208:11320/19:10405366 - isvavai.cz</a>

  • Result on the web

    <a href="https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=GuimuS.O4X" target="_blank" >https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=GuimuS.O4X</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1038/s41467-019-09213-x" target="_blank" >10.1038/s41467-019-09213-x</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    The operational environment and rotational acceleration of asteroid (101955) Bennu from OSIRIS-REx observations

  • Original language description

    During its approach to asteroid (101955) Bennu, NASA&apos;s Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer (OSIRIS-REx) spacecraft surveyed Bennu&apos;s immediate environment, photometric properties, and rotation state. Discovery of a dusty environment, a natural satellite, or unexpected asteroid characteristics would have had consequences for the mission&apos;s safety and observation strategy. Here we show that spacecraft observations during this period were highly sensitive to satellites (sub-meter scale) but reveal none, although later navigational images indicate that further investigation is needed. We constrain average dust production in September 2018 from Bennu&apos;s surface to an upper limit of 150 g s(-1) averaged over 34 min. Bennu&apos;s disk-integrated photometric phase function validates measurements from the pre-encounter astronomical campaign. We demonstrate that Bennu&apos;s rotation rate is accelerating continuously at 3.63 +/- 0.52 x 10(-6) degrees day(-2), likely due to the Yarkovsky-O&apos;Keefe-Radzievskii-Paddack (YORP) effect, with evolutionary implications.

  • 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

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2019

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Nature Communications [online]

  • ISSN

    2041-1723

  • e-ISSN

  • Volume of the periodical

    10

  • Issue of the periodical within the volume

    březen

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    10

  • Pages from-to

    1291

  • UT code for WoS article

    000461558000001

  • EID of the result in the Scopus database

    2-s2.0-85063214884