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On the maximum amplitude of harmonics of an asteroid lightcurve

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00429291" target="_blank" >RIV/67985815:_____/14:00429291 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1016/j.icarus.2014.03.004" target="_blank" >http://dx.doi.org/10.1016/j.icarus.2014.03.004</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.icarus.2014.03.004" target="_blank" >10.1016/j.icarus.2014.03.004</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    On the maximum amplitude of harmonics of an asteroid lightcurve

  • Original language description

    Most asteroid lightcurves are dominated by the second harmonic of the rotation period, caused by elongated shape. However, if the shape is not very elongate, other harmonics may dominate, leading to ambiguity of which is the true rotation period. We argue from geometry that at low phase angle, harmonics other than the second with amplitude exceeding resp. 0.4 magnitude are nearly impossible, so lightcurves with larger amplitude than that suggest a unique period dominated by the second harmonic, unless the spin is complex, non-principal axis rotation. On the other hand, lightcurves with amplitude less than 0.2?0.3 magnitudes can be dominated by other harmonics, especially the 4th and 6th, so the period may be ambiguous unless odd harmonics can be foundto identify the true rotation period. We present examples of each, low and high amplitude ambiguities.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/GAP209%2F12%2F0229" target="_blank" >GAP209/12/0229: Study of non-gravitational asteroid evolution processes via photometric observations</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2014

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Icarus

  • ISSN

    0019-1035

  • e-ISSN

  • Volume of the periodical

    235

  • Issue of the periodical within the volume

    June

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    5

  • Pages from-to

    55-59

  • UT code for WoS article

    000335291600005

  • EID of the result in the Scopus database