Photometry and shape modeling of Mars crosser asteroid (1011) Laodamia | Zendy

G. Apostolovska | Zendy; Z. Donchev | Zendy; A. Kostov | Zendy; V. Ivanova | Zendy; G. Borisov | Zendy; B. Bilkina | Zendy

AI Assistant Blog Pricing

Home ZAIA Blog

Open Access

Photometry and shape modeling of Mars crosser asteroid (1011) Laodamia

Author(s) -

G. Apostolovska,

Z. Donchev,

A. Kostov,

V. Ivanova,

G. Borisov,

B. Bilkina

Publication year - 2014

Publication title -

serbian astronomical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 0.196

H-Index - 16

eISSN - 1820-9289

pISSN - 1450-698X

DOI - 10.2298/saj1489079a

Subject(s) - asteroid , physics , photometry (optics) , observatory , astronomy , mars exploration program , light curve , astrophysics , stars

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

The content you want is available to Zendy users.

Already have an account? Click here to sign in.

Having issues? You can contact us here

Accelerating Research