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Source: Planetary and space science. 2022. Vol. 210. P. 105378 (1-11)
Type: статьи в журналах
Date: 2022
Description:
Analysing numerical models of the Geminid meteoroid stream for particle masses 0.00003–0.3 g we found evidence of several mean motion resonances: 1:2, 2:5, 3:7, 3:8 and 4:9 with Venus, 2:3 and 5:7 wit
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Source: Monthly notices of the Royal Astronomical Society. 2021. Vol. 507, № 3. P. 4481-4486
Type: статьи в журналах
Date: 2021
Description:
The origin of the Geminid meteoroid stream and its parent body the asteroid (3200) Phaethon is still under discussion. The observed bimodal activity profile of the Geminid shower agrees with a cometar
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Source: Monthly notices of the Royal Astronomical Society. 2016. Vol. 456. P. 78-84
Type: статьи в журналах
Date: 2016
Description:
A pilot numerical model of the Geminid meteoroid stream is presented. This model implies cometary origin of the stream. Ejection of relatively small amount of particles (90 000 test meteoroids with ma
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Source: European Planetary Science Congress 2015 : EPSC abstracts. [S. l.], 2015. Vol. 10. P. 754 [1-2]
Type: статьи в сборниках
Date: 2015
Source: Planetary and space science. 2015. Vol. 118. P. 296-301
Type: статьи в журналах
Date: 2015
Description:
Asteroid (3200) Phaethon is an Apollo asteroid having very small (0.14 au) perihelion distance. We analyze the influence of various perturbing factors on the asteroid motion. Most of them were studied
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