Future evolution of 12P and other Halley-type comets in near-polar orbits
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| Format: | Preprint |
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2025
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| _version_ | 1866917966430339072 |
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| author | Królikowska, M. Kankiewicz, P. Wajer, P. |
| author_facet | Królikowska, M. Kankiewicz, P. Wajer, P. |
| contents | We investigate the future 100 kyr evolution of six selected HTCs to show their basic commonalities and differences in dynamical behaviour. This includes estimating the probability of sungrazing and flipping. We combined three complementary numerical methods to study the dynamical features: the numerical integrations forwards in time, the Lyapunov time estimations, and the Mean Exponential Growth factor of Nearby Orbits (MEGNO). For each comet, we obtain the osculation orbits from the available observations. We then construct swarms of virtual comets as the basis for all dynamical studies. We show that two comets with q<1.3 au achieve the sungrazing state in the future with high probability: 161P with the likelihood of about 80% will be a sungrazing object with q<0.005 au in the next 13 kyr, and 122P with 50% in the next 100 kyr. We found that both these HTCs reach the sungrazing states due to Kozai resonances with other planets than Jupiter; for example, Uranus acts as the agent of Kozai resonance for 161P. We indicate that the high sungrazing probability for both comets is connected with a high likelihood of orbit flipping. The other four HTCs have a slight chance to be sungrazers after 100 kyr (<2.2%); however, three of them can achieve a high flipping probability. We show that the Lyapunov time and MEGNO indicator give a complementary picture of the orbital stability after 10,000 yr. Results allow us to rank comets from the most to least chaotic, where 161P is a particular case with its high probability to disintegrate due to the Kozai mechanism. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2503_17725 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Future evolution of 12P and other Halley-type comets in near-polar orbits Królikowska, M. Kankiewicz, P. Wajer, P. Earth and Planetary Astrophysics 75N04, 70F15 J.2; G.1.10 We investigate the future 100 kyr evolution of six selected HTCs to show their basic commonalities and differences in dynamical behaviour. This includes estimating the probability of sungrazing and flipping. We combined three complementary numerical methods to study the dynamical features: the numerical integrations forwards in time, the Lyapunov time estimations, and the Mean Exponential Growth factor of Nearby Orbits (MEGNO). For each comet, we obtain the osculation orbits from the available observations. We then construct swarms of virtual comets as the basis for all dynamical studies. We show that two comets with q<1.3 au achieve the sungrazing state in the future with high probability: 161P with the likelihood of about 80% will be a sungrazing object with q<0.005 au in the next 13 kyr, and 122P with 50% in the next 100 kyr. We found that both these HTCs reach the sungrazing states due to Kozai resonances with other planets than Jupiter; for example, Uranus acts as the agent of Kozai resonance for 161P. We indicate that the high sungrazing probability for both comets is connected with a high likelihood of orbit flipping. The other four HTCs have a slight chance to be sungrazers after 100 kyr (<2.2%); however, three of them can achieve a high flipping probability. We show that the Lyapunov time and MEGNO indicator give a complementary picture of the orbital stability after 10,000 yr. Results allow us to rank comets from the most to least chaotic, where 161P is a particular case with its high probability to disintegrate due to the Kozai mechanism. |
| title | Future evolution of 12P and other Halley-type comets in near-polar orbits |
| topic | Earth and Planetary Astrophysics 75N04, 70F15 J.2; G.1.10 |
| url | https://arxiv.org/abs/2503.17725 |