Comparative analysis of the absolute magnitudes of asteroids with MPC, Pan-STARRS, and PTF datasets
VG Shevchenko
At present, the main database of asteroid absolute magnitudes is the Minor Planet
Center (MPC). The MPC receives asteroid magnitudes from many observatories in
different spectral bands of different photometric systems, but calculates absolute …
Center (MPC). The MPC receives asteroid magnitudes from many observatories in
different spectral bands of different photometric systems, but calculates absolute …
GM Gartrelle, PS Hardersen, MRM Izawa, MC Nowinski - Icarus, 2020
D-type asteroids are a prime example of the many dark, low-albedo asteroids which
do not reflect sufficient light to reveal detectable mineral absorptions. While D-type
asteroids are relatively rare in the inner solar system and the main asteroid belt, they …
do not reflect sufficient light to reveal detectable mineral absorptions. While D-type
asteroids are relatively rare in the inner solar system and the main asteroid belt, they …
VG Shevchenko
1. Results For our dataset, we used first the data of the asteroid magnitude-phase
dependences collected at the Institute of Astronomy of VN Karazin Kharkiv National
University [5, 10–12]. We also used observational data of asteroids from our other …
dependences collected at the Institute of Astronomy of VN Karazin Kharkiv National
University [5, 10–12]. We also used observational data of asteroids from our other …



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