G. Apostolovska, Z. Donchev, A. Kostov, V. Ivanova, G. Borisov, B. Bilkina
{"title":"Photometry and shape modeling of Mars crosser asteroid (1011) Laodamia","authors":"G. Apostolovska, Z. Donchev, A. Kostov, V. Ivanova, G. Borisov, B. Bilkina","doi":"10.2298/SAJ1489079A","DOIUrl":null,"url":null,"abstract":"An analysis of photometric observations of Mars crosser asteroid 1011 \n Laodamia conducted at Bulgarian National Astronomical Observatory Rozhen over \n a twelve year interval (2002, 2003, 2004, 2006, 2007, 2008, 2011, 2012 and \n 2013) is made. Based on the obtained lightcurves the spin vector, sense of \n rotation, and preliminary shape model of (1011) Laodamia have been determined \n using the lightcurve inversion method. The aim of this investigation is to \n increase the set of asteroids with known spin and shape parameters and to \n contribute in improving the model in combination with other techniques and \n sparse data produced by photometric asteroid surveys such as Pan-STARRS or \n GAIA.","PeriodicalId":48878,"journal":{"name":"Serbian Astronomical Journal","volume":null,"pages":null},"PeriodicalIF":0.8000,"publicationDate":"2014-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Serbian Astronomical Journal","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.2298/SAJ1489079A","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 1
Abstract
An analysis of photometric observations of Mars crosser asteroid 1011
Laodamia conducted at Bulgarian National Astronomical Observatory Rozhen over
a twelve year interval (2002, 2003, 2004, 2006, 2007, 2008, 2011, 2012 and
2013) is made. Based on the obtained lightcurves the spin vector, sense of
rotation, and preliminary shape model of (1011) Laodamia have been determined
using the lightcurve inversion method. The aim of this investigation is to
increase the set of asteroids with known spin and shape parameters and to
contribute in improving the model in combination with other techniques and
sparse data produced by photometric asteroid surveys such as Pan-STARRS or
GAIA.
期刊介绍：
Serbian Astronomical Journal publishes original observations and researches in all branches of astronomy. The journal publishes:
Invited Reviews - review article on some up-to-date topic in astronomy, astrophysics and related fields (written upon invitation only),
Original Scientific Papers - article in which are presented previously unpublished author''s own scientific results,
Preliminary Reports - original scientific paper, but shorter in length and of preliminary nature,
Professional Papers - articles offering experience useful for the improvement of professional practice i.e. article describing methods and techniques, software, presenting observational data, etc.
In some cases the journal may publish other contributions, such as In Memoriam notes, Obituaries, Book Reviews, as well as Editorials, Addenda, Errata, Corrigenda, Retraction notes, etc.
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