Facebook Instagram Twitter RSS Feed PodBean Back to top on side

Shape model of the asteroid (2501) Lohja from long-term photometric observations

In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no. 2
M. Husárik
Detaily:
Rok, strany: 2018, 319 - 328
Kľúčové slová:
asteroids, rotation, photometry, shapes
O článku:
We present lightcurves, shapes, and a 3D convex spin-axis model for the main-belt asteroid (2501) Lohja. The models were obtained with the lightcurve inversion process using combined dense photometric data from the apparitions between years 2006 and 2017. The analysis found a sidereal period of 3.80835 hours, and a possible ecliptic pole solution (J2000.0), the prograde sense of rotation and main ratios of the ellipsoidal model.
Ako citovať:
ISO 690:
Husárik, M. 2018. Shape model of the asteroid (2501) Lohja from long-term photometric observations. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no.2, pp. 319-328. 1335-1842.

APA:
Husárik, M. (2018). Shape model of the asteroid (2501) Lohja from long-term photometric observations. Contributions of the Astronomical Observatory Skalnaté Pleso, 48(2), 319-328. 1335-1842.