национального университета имени Тараса Шевченко 2 Главная астрономическая обсерватория НАН Украины 3 Межрегиональная академия управления персоналом В результате двухлетних наблюдений авторы выделили класс сумеречных болидов. В отличие от ночных наблюдений светящихся метеорных следов, которые можно наблюдать не более десяти секунд, сумеречные следы наблюдаются от нескольких минут до двух часов. В работе рассмотрено синхронное наблюдение вечернего сумеречного болида в небе над Киевом 25.06.2014 Дашкиевым Г.Н. и Стекловым А.Ф. Базовое расстояние между точками фотографирования составило 8,55 км. Исходя из предположения, что взрыв крупных метеороидов в атмосфере планеты и вспышка блеска происходит на высоте их максимального торможения в интервале значительно меньше высоты однородной атмосферы, следует, что тепловой взрыв метеороида произошел на высоте существенно больше 15 км. Причем высвечивание и распад, возможно, кометного вещества началось на высоте более 25 км. Тело не долетело до поверхности Земли и распалось на мелкодисперсные частицы. Предварительные оценки начальной массы данного фрагмента до входа в атмосферу составляют от 2 до 10 тонн. А на обеих фотографиях виден только дисперсный след от распавшихся фрагментов кометного ядра.
This paper presents theoretical developments of some issues in the physics of space intrusions. We report the discovery of a new effect -variations in brightness and "wobbling" in the meteor trail. The frequency of the variations of brightness (f c ) and wobbling (f m ) that can be measured is important information parameters that allow us to obtain estimates all the characteristics of the meteor if its height and speed are known. Basic two-side intrusion observations automatically determine both the height and speed of the intrusion. We offer a new "tuning technique" that allows determining the meteor characteristics during one-side observations. The essence of a new technique is to fine-tune the initial parameters of the simulation model of intrusion until the calculated and measured frequencies f c , f m coincide. We found that rotation plays an important role in the dynamics of meteors; in particular, they can burst in due to centrifugal forces that exceed the strength of the material. In the case of one-side observations, we construct a grid of intrusion models using the Impact 4A software program on the plane of the primary "mass-speed" meteoroid. As a result of modelling, we find the height at which the frequency ratio f c /f m coincides with the value found from measurements for exploding meteoroid. The paper describes the characteristics of the space intrusion of a meteor in Kyiv on August 12, 2019, 22:52:57 UT. The amplitude of the brightness fluctuations was found about 0.1 magnitudes, the amplitude of the wobbling of about 4 arc seconds. Using the Impact 4A software program the preatmospheric velocity was evaluated ∼ 40 km/sec; the mass of the meteoroid was evaluated approximately 0.45 kg. This meteoroid reached maximum light at 82.2 km and ablated partially. We find estimates of a residual mass of about 10 grams and a residual speed of about 20 km/s. We found that the radius of the helical path of the meteor at this height is about 1.5 meters. The meteoroid reached a critical value of the speed of rotation on the surface. At this moment, a meteoroid exploded and destroyed.
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