supported by the National Natural Science Foundation of China (42241116 and U1831132);supported by the Macao Science and Technology Development Fund (No. SKL-LPS(MUST)-20212023);the 2022 Project of Xinjiang Uygur Autonomous Region of China for Heaven Lake Talent Program;supported by the Chinese Academy of Sciences Foundation of the young scholars of western (2020-XBQNXZ-019);supported by a DAR grant in planetology from the French Space Agency (CNES).
Most asteroids and comets are formed in the early stages of the solar system and therefore contain a wealth of information about their birth.The asteroid exploration mission planned in the coming years by China will l...
the Centre for Innovation and Transfer of Natural Sciences and Engineering Knowledge, University of Rzeszów, Poland
The paper presents a model of the thermodynamic evolution of the comet nucleus surface.In the proposed approach,we focus on the analysis of the formation of pits visible on the surface of the cometary nucleus.These pi...
The paper presents three processes related to the dynamics of cometary particles.The following thermodynamic mechanisms were taken into account:quiet sublimation,emission of cometary matter via jet and migration of pa...
the support the author received from the Centre for Innovation and Transfer of Natural Sciences and Engineering Knowledge,University of Rzeszow,Poland。
This paper presents a new approach to analyzing the change of cometary brightness.In our considerations,we assume that astronomical silicates(dust agglomerates)and gas are present in the coma.This assumption is a cons...
the National Natural Science Foundation of China(U1831132 and 41874010);Innovation Group of Natural Fund of Hubei Province(2018CFA087);supported by a DAR fund in planetology from the French Space Agency(CNES)。
In China’s asteroid mission to be launched around 2025,(7968)133 P/Elst-Pizarro(hereafter 133 P)will be the second target,after a visit to asteroid(469219)Kamo’oalewa.This paper describes a simulation of precise orb...
the author received from the Centre for Innovation and Transfer of Natural Sciences and Engineering Knowledge,University of Rzeszow,Poland。
We analyze the thermodynamic model of changes in comet brightness focusing on the exceptional case which is comet 29 P/Schwassmann-Wachmann(hereafter 29 P/SW).This object demonstrates quasiregular flares that occur in...
supported by the program of the light in China’s Western Region (LCWR, Grant No. 2015XBQN-A-02);the National Natural Science Foundation of China (Grant No. 11661161016);the 13th Five-year Informatization Plan of Chinese Academy of Sciences (Grant No. XXH13503–03–107);the Youth Innovation Promotion Association CAS (Grant No. 2018080);the Talent Importing Program offered by the government of Xinjiang Uygur Autonomous Region
In this work, we report the observations of the long-period comet C/2015 O1 performed on2018 January 29–30 and April 13 with the Nanshan 1-meter wide-field telescope operated by Xinjiang Astronomical Observatory. We ...