Perseids 2024 – Installation of FHD meteor cameras in the CEMeNt network by Jakub Koukal | Aug 20, 2024 | Results | 0 | At the beginning of 2024, the CEMeNt network (Central European Meteor Network) entered its...

Washington coast meteorite by Richard Kacerek | Mar 24, 2018 | News | 0 | On Wednesday 7 March 2018 at around 7:10 PM a large number of witnesses along the Washington coast...

2024年1月31日 · This bolide, which flew over the Moravian-Slovak border after two o’clock in the morning on January 9, 2024, was recorded by stations of the CEMeNt network (Central European MetEor NeTwork) as well as stations of the GMN network (Global Meteor Network), whose national component CSMON (Czech and Slovak Meteor Observation Network) operates ...

A study of the 2021 Andromedids is presented based on the Global Meteor Network results. Andromedid orbits were identified during the interval in solar longitude 206° to 278°.

Bright bolide from the weak June Draconids meteor shower by Jakub Koukal | Jun 17, 2024 | Fireballs | 0 | The weak june ro-Drakonid meteor shower (JRD, IAU MDC 0686) was first described in 2018 (P....

2017年11月8日 · However, the emergence of the use of video technology for meteor studies has meant an unprecedented boom of this branch of astronomy since the 1990s, with lots of new meteor data and a huge number of newly discovered meteor showers.

We study the two most important major meteor showers in detail (Perseids and Geminids) and find a very interesting peculiarity in the Geminids; brighter meteors with absolute magnitude M A < –2 decrease in number compared to sporadic meteors and other meteor showers of course, and the beginning height of Geminids is almost the same as

Global Meteor Network could immediately confirm the enhanced activity of this shower. the first two years of the Japanese network. Figure 1 – The radiant of the h Virginids appeared as a rather compact concentration of orbit points on the daily maps of the NASA Meteor shower Portal. The map shows the radiant

2024年6月17日 · The body entered the Earth’s atmosphere at an ideal angle of 49.1°, the speed before entering the atmosphere was 36.62 km/s. It was therefore a medium-speed bolide, the geocentric speed of the meteoroid was 34.75 km/s. The body belonged to the june ro-Draconids meteor shower (IUA MDC 0686 JRD).

2024年8月20日 · The Valašské Meziříčí Observatory has been studying meteor tracks using video technology since 2011 and studying meteor spectra using video technology since 2014. During July 2024, the replacement of existing camera systems for studying meteor orbits at stations of the CEMeNt network with modern CMOS cameras with significantly higher ...